Sample records for zone dike intrusion

  1. The 12 September 1999 Upper East Rift Zone dike intrusion at Kilauea Volcano, Hawaii

    USGS Publications Warehouse

    Cervelli, Peter; Segall, P.; Amelung, F.; Garbeil, H.; Meertens, C.; Owen, S.; Miklius, Asta; Lisowski, M.

    2002-01-01

    Deformation associated with an earthquake swarm on 12 September 1999 in the Upper East Rift Zone of Kilauea Volcano was recorded by continuous GPS receivers and by borehole tiltmeters. Analyses of campaign GPS, leveling data, and interferometric synthetic aperture radar (InSAR) data from the ERS-2 satellite also reveal significant deformation from the swarm. We interpret the swarm as resulting from a dike intrusion and model the deformation field using a constant pressure dike source. Nonlinear inversion was used to find the model that best fits the data. The optimal dike is located beneath and slightly to the west of Mauna Ulu, dips steeply toward the south, and strikes nearly east-west. It is approximately 3 by 2 km across and was driven by a pressure of ??? 15 MPa. The total volume of the dike was 3.3 x 106 m3. Tilt data indicate a west to east propagation direction. Lack of premonitory inflation of Kilauea's summit suggests a passive intrusion; that is, the immediate cause of the intrusion was probably tensile failure in the shallow crust of the Upper East Rift Zone brought about by persistent deep rifting and by continued seaward sliding of Kilauea's south flank.

  2. Dike intrusions during rifting episodes obey scaling relationships similar to earthquakes.

    PubMed

    Passarelli, L; Rivalta, E; Shuler, A

    2014-01-28

    As continental rifts evolve towards mid-ocean ridges, strain is accommodated by repeated episodes of faulting and magmatism. Discrete rifting episodes have been observed along two subaerial divergent plate boundaries, the Krafla segment of the Northern Volcanic Rift Zone in Iceland and the Manda-Hararo segment of the Red Sea Rift in Ethiopia. In both cases, the initial and largest dike intrusion was followed by a series of smaller intrusions. By performing a statistical analysis of these rifting episodes, we demonstrate that dike intrusions obey scaling relationships similar to earthquakes. We find that the dimensions of dike intrusions obey a power law analogous to the Gutenberg-Richter relation, and the long-term release of geodetic moment is governed by a relationship consistent with the Omori law. Due to the effects of magma supply, the timing of secondary dike intrusions differs from that of the aftershocks. This work provides evidence of self-similarity in the rifting process.

  3. Dike intrusions during rifting episodes obey scaling relationships similar to earthquakes

    PubMed Central

    L., Passarelli; E., Rivalta; A., Shuler

    2014-01-01

    As continental rifts evolve towards mid-ocean ridges, strain is accommodated by repeated episodes of faulting and magmatism. Discrete rifting episodes have been observed along two subaerial divergent plate boundaries, the Krafla segment of the Northern Volcanic Rift Zone in Iceland and the Manda-Hararo segment of the Red Sea Rift in Ethiopia. In both cases, the initial and largest dike intrusion was followed by a series of smaller intrusions. By performing a statistical analysis of these rifting episodes, we demonstrate that dike intrusions obey scaling relationships similar to earthquakes. We find that the dimensions of dike intrusions obey a power law analogous to the Gutenberg-Richter relation, and the long-term release of geodetic moment is governed by a relationship consistent with the Omori law. Due to the effects of magma supply, the timing of secondary dike intrusions differs from that of the aftershocks. This work provides evidence of self-similarity in the rifting process. PMID:24469260

  4. Gravity and the mechanics of dike intrusion

    NASA Astrophysics Data System (ADS)

    Townsend, M.

    2017-12-01

    Dikes are a diverse yet ubiquitous feature of terrestrial volcanic and magmatic settings, ranging in size from decimeter-thick aplite dikes in silicic plutons, to meters-thick dikes at basaltic shield volcanoes and rift zones, to 100-meter-thick "giant" dikes in swarms that can exceed over 2000 km in length. Dike profiles may be planar or curved, elliptical or teardrop-shaped, and blunt or tapered at the tips. The variety of size, shape, composition, and intrusion environment is in contrast with the ubiquitous observation that dikes tend to be vertically inclined, emanate from central reservoirs, and propagate laterally for distances that are 10 to over 100 times their height. In this talk, I will briefly review the geological and geophysical observations of dike geometry and propagation directions. These data motivate a 2D mechanical model for vertical dikes in which the primary loading is due to gravity. Using this model, I will explore fundamental relationships between density structure within the magma and surrounding crust, driving pressure, topographic and tectonic loading, and the size, shape, and depth at which dikes become vertically stable such that subsequent propagation is lateral. Modeling results highlight a dual effect of gravity, as both a source of diversity in stable dike geometries and as a robust mechanism for trapping dikes in the subsurface.

  5. Hazard Models From Periodic Dike Intrusions at Kı¯lauea Volcano, Hawai`i

    NASA Astrophysics Data System (ADS)

    Montgomery-Brown, E. K.; Miklius, A.

    2016-12-01

    The persistence and regular recurrence intervals of dike intrusions in the East Rift Zone (ERZ) of Kı¯lauea Volcano lead to the possibility of constructing a time-dependent intrusion hazard model. Dike intrusions are commonly observed in Kı¯lauea Volcano's ERZ and can occur repeatedly in regions that correlate with seismic segments (sections of rift seismicity with persistent definitive lateral boundaries) proposed by Wright and Klein (USGS PP1806, 2014). Five such ERZ intrusions have occurred since 1983 with inferred locations downrift of the bend in Kı¯lauea's ERZ, with the first (1983) being the start of the ongoing ERZ eruption. The ERZ intrusions occur on one of two segments that are spatially coincident with seismic segments: Makaopuhi (1993 and 2007) and Nāpau (1983, 1997, and 2011). During each intrusion, the amount of inferred dike opening was between 2 and 3 meters. The times between ERZ intrusions for same-segment pairs are all close to 14 years: 14.07 (1983-1997), 14.09 (1997-2011), and 13.95 (1993-2007) years, with the Nāpau segment becoming active about 3.5 years after the Makaopuhi segment in each case. Four additional upper ERZ intrusions are also considered here. Dikes in the upper ERZ have much smaller opening ( 10 cm), and have shorter recurrence intervals of 8 years with more variability. The amount of modeled dike opening during each of these events roughly corresponds to the amount of seaward south flank motion and deep rift opening accumulated in the time between events. Additionally, the recurrence interval of 14 years appears to be unaffected by the magma surge of 2003-2007, suggesting that flank motion, rather than magma supply, could be a controlling factor in the timing and periodicity of intrusions. Flank control over the timing of magma intrusions runs counter to the historical research suggesting that dike intrusions at Kı¯lauea are driven by magma overpressure. This relatively free sliding may have resulted from decreased

  6. Father's Day dike intrusion and eruption reveals interaction between magmatic and tectonic processes at Kilauea Volcano, Hawaii

    NASA Astrophysics Data System (ADS)

    Foster, J. H.; Brooks, B. A.; Sandwell, D. T.; Poland, M.; Miklius, A.; Myer, D.; Okubo, P. G.; Patrick, M.; Wolfe, C.

    2007-12-01

    The June 17-19, 2007, Father's Day dike intrusion and eruption at Kilauea volcano brought to an end a seven- year period of steady state lava effusion at the Pu'u 'O'o vent. The event was observed by an unprecedented number of geophysical instruments, with temporary arrays of GPS and tiltmeters augmenting the continuous monitoring network. Envisat and ALOS SAR scenes were also acquired during this event and provide further information on the surface deformation as the event progressed. Fortuitously, the Envisat acquisition was during a pause in the middle of the sequence, while the ALOS PALSAR scene was acquired at the end of the sequence, allowing us to model each phase separately. Analysis of these data sets indicates that, in addition to three phases of the dike intrusion, a slow earthquake also occurred on the south flank of Kilauea. The slow earthquake apparently began near the end of the second phase of the dike intrusion. It was still underway the following day, when the third phase of the intrusion began and culminated in a small eruption. This suggests the possibility that the slow earthquake was triggered by the initial diking, and then in turn influenced the progression of the intrusion. Two of the largest previous slow earthquakes also hint at a connection between slow earthquakes and eruptive activity on Kilauea. The range of observations of the Father's Day events provides us with a unique opportunity to investigate the complex interactions between the tectonic processes of the south flank and magmatic processes within the summit and rift zones.

  7. Transient deformation following the 30 January 1997 dike intrusion at Kīlauea volcano, Hawai'i

    NASA Astrophysics Data System (ADS)

    Desmarais, Emily K.; Segall, Paul

    2007-02-01

    On 30 January 1997 an intrusion on Kīlauea volcano opened a new fissure within the East Rift Zone (ERZ) at Nāpau Crater, 3 km uprift from the ongoing eruptions at Pu’u ’Ō’ō. The fissure eruption lasted 22 h and opened a 5.1 km long, nearly vertical dike 1.9 m, extending from the surface to a depth of 2.4 km (Owen et al. 2000b). During the eruption, the lava pond at Pu’u ’Ō’ō drained, and eruptions ceased there. Pu’u ’Ō’ō eventually refilled in late February and eruptions resumed there on 28 March 1997. Continuous GPS data show a large transient following the 30 January 1997 dike intrusion. After lengthening 40 cm during the initial eruption, the baseline between two stations spanning the ERZ lengthened an additional 10 cm over the following 6 months. A coastal station KAEP also exhibited transient deformation, as it continued to move southward (5 cm) over the same 6-month period. The baseline between two stations spanning Kīlauea’s summit caldera contracted sharply during the eruption, but gradually recovered to slightly longer than its previous length 2 months after the intrusion. We use the extended network inversion filter (McGuire and Segall 2003) to invert continuous GPS data for volume change of a spherical pressure source under Kīlauea’s summit, opening distribution on a nearly vertical dike in the ERZ and potential slip on a decollement 9 km beneath the south flank. Following the 30 January intrusion, rift extension continued below the initial dike intrusion for the duration of the transient. Decollement slip, regardless of its assumed depth, is not required to fit the data. The modeled transient summit reinflation and rift opening patterns under Nāpau crater coincide with changes in observed behavior of Pu’u ’Ō’ō’s lava pond. Rift opening accelerated while Pu’u ’Ō’ō eruptions paused and began to decelerate after the lava pond reappeared nearly a month after the Nāpau eruption. The transient deformation is

  8. Intrusion of granitic magma into the continental crust facilitated by magma pulsing and dike-diapir interactions: Numerical simulations

    NASA Astrophysics Data System (ADS)

    Cao, Wenrong; Kaus, Boris J. P.; Paterson, Scott

    2016-06-01

    We conducted a 2-D thermomechanical modeling study of intrusion of granitic magma into the continental crust to explore the roles of multiple pulsing and dike-diapir interactions in the presence of visco-elasto-plastic rheology. Multiple pulsing is simulated by replenishing source regions with new pulses of magma at a certain temporal frequency. Parameterized "pseudo-dike zones" above magma pulses are included. Simulation results show that both diking and pulsing are crucial factors facilitating the magma ascent and emplacement. Multiple pulses keep the magmatic system from freezing and facilitate the initiation of pseudo-dike zones, which in turn heat the host rock roof, lower its viscosity, and create pathways for later ascending pulses of magma. Without diking, magma cannot penetrate the highly viscous upper crust. Without multiple pulsing, a single magma body solidifies quickly and it cannot ascent over a long distance. Our results shed light on the incremental growth of magma chambers, recycling of continental crust, and evolution of a continental arc such as the Sierra Nevada arc in California.

  9. Influence of Topographic Unloading on Magma Intrusions: Modelling Dike Propagation Under Calderas

    NASA Astrophysics Data System (ADS)

    Gaete Rojas, A. B.; Kavanagh, J.; Walter, T. R.

    2017-12-01

    Dikes are common igneous bodies involved in the transport of magma through the crust to feed volcanic eruptions. Dike emplacement in the presence of topographic depressions, as produced by unloading in volcanic systems with calderas, is enigmatic. Field observations of post-caldera volcanism suggest the emplacement of dikes often occurs as cone sheets and/or ring/radial dikes. However, the extrapolation of the surface expression of these laminar intrusions to depth to infer their sub-surface geometry is often based on limited information. As a result, key questions remain regarding the propagation dynamics of dikes beneath calderas, including the physical processes that influence the development of an intrusive cone sheet rather than a circumferential, steep-sided ring dike that could breach the surface. Scaled laboratory modeling allows us to study the development of cone sheets and ring dikes in 3D in the presence of a surface depression, tracking the evolution of the dynamic processes of their formation.Here, we analyze the evolution of dikes propagating in an elastic medium in the presence of a stress perturbation due to unloading. We performed experiments using a 30 × 40 × 40 cm3tank filled with 2.5 wt.% solidified gelatine with a cylindrical surface depression to produce a crustal analogue with caldera-like topography. Magma-filled hydrofractures were creating by injecting dyed water as the magma analogue. The intrusion evolution was monitored using 3 cameras, with an overhead laser scanner measuring the progressive surface uplift and polarized light tracking the evolution of the stress field. We find that the formation of a cone sheet or a ring dike is a consequence of the caldera size and its stress field, with small calderas favouring ring dike formation. The offset of the injection point relative to the centre of the caldera is also assessed. Cone sheets are formed as the dike is strongly deflected, and the dike propagation front transitions into

  10. Geodetic evidence for en echelon dike emplacement and concurrent slow slip during the June 2007 intrusion and eruption at Kīlauea volcano, Hawaii

    USGS Publications Warehouse

    Montgomery-Brown, E. K.; Sinnett, D.K.; Poland, M.; Segall, P.; Orr, T.; Zebker, H.; Miklius, Asta

    2010-01-01

    A series of complex events at Kīlauea Volcano, Hawaii, 17 June to 19 June 2007, began with an intrusion in the upper east rift zone (ERZ) and culminated with a small eruption (1500 m3). Surface deformation due to the intrusion was recorded in unprecedented detail by Global Positioning System (GPS) and tilt networks as well as interferometric synthetic aperture radar (InSAR) data acquired by the ENVISAT and ALOS satellites. A joint nonlinear inversion of GPS, tilt, and InSAR data yields a deflationary source beneath the summit caldera and an ENE-striking uniform-opening dislocation with ~2 m opening, a dip of ∼80° to the south, and extending from the surface to ~2 km depth. This simple model reasonably fits the overall pattern of deformation but significantly misfits data near the western end of an inferred dike-like source. Three more complex dike models are tested that allow for distributed opening including (1) a dike that follows the surface trace of the active rift zone, (2) a dike that follows the symmetry axis of InSAR deformation, and (3) two en echelon dike segments beneath mapped surface cracks and newly formed steaming areas. The en echelon dike model best fits near-field GPS and tilt data. Maximum opening of 2.4 m occurred on the eastern segment beneath the eruptive vent. Although this model represents the best fit to the ERZ data, it still fails to explain data from a coastal tiltmeter and GPS sites on Kīlauea's southwestern flank. The southwest flank GPS sites and the coastal tiltmeter exhibit deformation consistent with observations of previous slow slip events beneath Kīlauea's south flank, but inconsistent with observations of previous intrusions. Slow slip events at Kīlauea and elsewhere are thought to occur in a transition zone between locked and stably sliding zones of a fault. An inversion including slip on a basal decollement improves fit to these data and suggests a maximum of ~15 cm of seaward fault motion, comparable to previous slow

  11. Volcanic tremor and frequency gliding during dike intrusions at Kı¯lauea—A tale of three eruptions

    NASA Astrophysics Data System (ADS)

    Unglert, K.; Jellinek, A. M.

    2015-02-01

    To characterize syneruptive/intrusive deviations from background volcanic tremor at Kı¯lauea, Hawai`i, we analyze the spatial and temporal properties of broadband tremor during dike intrusions into the East Rift Zone (ERZ) in 2007 and 2011, as well as during explosive eruptive activity at Kı¯lauea's summit in 2008. Background tremor was similar for each event, and the 2008 explosions did not affect its properties. In contrast, the intrusions were accompanied by departures from this background in the form of two phases of seismicity that were separated in space and time. In both 2007 and 2011, Phase I was characterized by a quick succession of discrete events, which were most intense at the onset of intrusion near the presumed locations of the dikes intruding into the ERZ. Phase II, marked by continuous broadband tremor around the summit, followed 10-14 h later. In 2007, Phase II tremor was accompanied by a monotonic downward shift (glide) of spectral peaks between ˜0.6 and 1.5 Hz over at least 15 h. During Phase II in 2011, a gradual upward and subsequent symmetric downward glide between ˜0.6 and 6.6 Hz occurred over 5-10 h, respectively. The spectra during both phases differed from the background and 2008, as well as from each other, indicating different physical mechanisms. Phase I in 2007 and 2011 is probably related to the mechanics of dike intrusion. Phase II tremor may be characteristic for evolving magma-bubble dynamics related to the geometry of the plumbing system and the style of magma flow.

  12. Dike zones on Venus

    NASA Technical Reports Server (NTRS)

    Markov, M. S.; Sukhanov, A. L.

    1987-01-01

    Venusian dike zone structures were identified from Venera 15 and 16 radar images. These include: a zone of subparallel rows centered at 30 deg N, 7 deg E; a system of intersecting bands centered at 67 deg N, 284 deg E; polygonal systems in lavas covering the structural base uplift centered at 47 deg N, 200 deg E; a system of light bands in the region of the ring structure centered at 43 deg N, 13 deg E; and a dike band centered at 27 deg N, 36 deg E.

  13. Dike Intrusion Process of 2000 Miyakejima - Kozujima Event estimated from GPS measurements in Kozujima - Niijima Islands, central Japan

    NASA Astrophysics Data System (ADS)

    Murase, M.; Nakao, S.; Kato, T.; Tabei, T.; Kimata, F.; Fujii, N.

    2003-12-01

    Kozujima - Niijima Islands of Izu Volcano Islands are located about 180 km southeast of Tokyo, Japan. Although the last volcano eruptions in Kozujima and Niijima volcanoes are recorded more than 1000 year before, the ground deformation of 2-3 cm is detected at Kozujima - Niijima Islands by GPS measurements since 1996. On June 26, 2000, earthquake swarm and large ground deformation more than 20 cm are observed at Miyakejima volcano located 40 km east-southeastward of Kozu Island, and volcano eruption are continued since July 7. Remarkable earthquake swarm including five earthquakes more than M5 is stretching to Kozushima Island from Miyakejima Island. From the rapid ground deformation detected by continuous GPS measurements at Miyakejima Island on June 26, magma intrusion models of two or three dikes are discussed in the south and west part of Miyakejima volcano by Irwan et al.(2003) and Ueda et al.(2003). They also estimate dike intrusions are propagated from southern part of Miyakejima volcano to western part, and finally dike intrusion is stretching to 20 km distance toward Kozujima Island. From the ground deformation detected by GPS daily solution of Nation-wide dense GPS network (GEONET), some dike intrusion models are discussed. Ito et al.(2002) estimate the huge dike intrusion with length of about 20 km and volume of 1 km3 in the sea area between the Miyake Island and Kozu Island. (And) Nishimura et al.(2001) introduce not only dike but also aseismic creep source to explain the deformation in Shikinejima. Yamaoka et al.(2002) discuss the dike and spherical deflation source under the dike, because of no evidence supported large aseismic creep. They indicate a dike and spherical deflation source model is as good as dike and creep source model. In case of dike and creep, magma supply is only from the chamber under the Miyakejima volcano. In dike and spherical deflation source model, magma supply is from under Miyakejima volcano and under the dike. Furuya et al

  14. Surface fracturing and graben subsidence during the 2014 Bárdarbunga dike intrusion in Iceland

    NASA Astrophysics Data System (ADS)

    Rut Hjartardóttir, Ásta; Einarsson, Páll; Tumi Gudmundsson, Magnús; Högnadóttir, Thordís

    2015-04-01

    A dike propagated laterally away from the Bárdarbunga central volcano in August 2014. The dike propagated about 48 km towards the northeast and north-northeast, mostly beneath the Vatnajökull glacier. However, the farthest 8 km of the dike were located north of the glacier, where the ice-free area allowed surface fractures and graben subsidence to be observed. This dike intrusion was accompanied by eruptions, the most prominent ones occurring within the graben at the distal end of the dike. In this study, photographs taken from airplanes were rectified by using the ArcGIS software. This was done in order to map the fractures and eruptive fissures which were formed or reactivated during this dike intrusion, and to show the temporal evolution of the fracture pattern. Ground deformation across the graben was measured from an airplane with a radar altimeter and kinematic GPS. The propagation of the dike was shown by laterally propagating earthquakes and by ground deformation recorded by GPS geodetic network. Three days after the dike had propagated north of the Vatnajökull glacier, new and reactivated fractures were detected in this area, above the dike. The fractures delineated two grabens in direct continuation of each other. The southern graben extended 5 km northwards from the glacier boundary, and was 700-1000 m wide. Before the eruptions, the northern graben was seen ~6.6-7.5 km north of the glacier, and was only 250-450 m wide. Two days later, on the 29th of August, a four-hour long eruption took place on a 600 m long eruptive fissure 6 km north of the glacier. Then, the narrow northern graben was seen extending about 1-1.6 km farther to the south than before the eruption, with the new eruptive fissure in the middle of it. The eruption resumed again two days later, extending the same eruptive fissure towards the south and north, to a total of ~1900 m length. This eruption is still ongoing (in January 2014). On the 5th of September, three short (~100 to 250 m

  15. Dike/Drift Interactions

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    E. Gaffiney

    2004-11-23

    This report presents and documents the model components and analyses that represent potential processes associated with propagation of a magma-filled crack (dike) migrating upward toward the surface, intersection of the dike with repository drifts, flow of magma in the drifts, and post-magma emplacement effects on repository performance. The processes that describe upward migration of a dike and magma flow down the drift are referred to as the dike intrusion submodel. The post-magma emplacement processes are referred to as the post-intrusion submodel. Collectively, these submodels are referred to as a conceptual model for dike/drift interaction. The model components and analyses ofmore » the dike/drift interaction conceptual model provide the technical basis for assessing the potential impacts of an igneous intrusion on repository performance, including those features, events, and processes (FEPs) related to dike/drift interaction (Section 6.1).« less

  16. Rapid dike intrusion into Sakurajima volcano on August 15, 2015, as detected by multi-parameter ground deformation observations

    NASA Astrophysics Data System (ADS)

    Hotta, Kohei; Iguchi, Masato; Tameguri, Takeshi

    2016-04-01

    We present observations of ground deformation at Sakurajima in August 2015 and model the deformation using a combination of GNSS, tilt and strain data in order to interpret a rapid deformation event on August 15, 2015. The pattern of horizontal displacement during the period from August 14 to 16, 2015, shows a WNW-ESE extension, which suggests the opening of a dike. Using a genetic algorithm, we obtained the position, dip, strike length, width and opening of a dislocation source based on the combined data. A nearly vertical dike with a NNE-SSW strike was found at a depth of 1.0 km below sea level beneath the Showa crater. The length and width are 2.3 and 0.6 km, respectively, and a dike opening of 1.97 m yields a volume increase of 2.7 × 106 m3. 887 volcano-tectonic (VT) earthquakes beside the dike suggest that the rapid opening of the dike caused an accumulation of strain in the surrounding rocks, and the VT earthquakes were generated to release this strain. Half of the total amount of deformation was concentrated between 10:27 and 11:54 on August 15. It is estimated that the magma intrusion rate was 1 × 106 m3/h during this period. This is 200 times larger than the magma intrusion rate prior to one of the biggest eruptions at the summit crater of Minami-dake on July 24, 2012, and 2200 times larger than the average magma intrusion rate during the period from October 2011 to March 2012. The previous Mogi-type ground deformation is considered to be a process of magma accumulation in preexisting spherical reservoirs. Conversely, the August 2015 event was a dike intrusion and occurred in a different location to the preexisting reservoirs. The direction of the opening of the dike coincides with the T-axes and direction of faults creating a graben structure.

  17. On the physical links between the dynamics of the Izu Islands 2000 dike intrusions and the statistics of the induced seismicity

    NASA Astrophysics Data System (ADS)

    Passarelli, Luigi; Rivalta, Eleonora; Simone, Cesca; Aoki, Yosuke

    2014-05-01

    The emplacement of magma-filled dikes often induce abundant seismicity in the surrounding host rocks. Most of the earthquakes are thought to occur close to the propagating tip (or edges, in 3D) of the dike, where stresses are concentrated. The resulting seismicity often appears as a swarm, controlled mainly by dike-induced stresses and stressing rate and by other factors, such as the background stressing rate, tectonic setting, regional stresses and tectonic history. The spatial distribution and focal mechanisms of the seismicity bear information on the interaction of the dike stress field and the tectonic setting of the area. The seismicity accompanying the intrusion of a dike is usually characterized by weak events, for which it is difficult to calculate the focal mechanisms. Therefore, only for a few well-recorded dike intrusions a catalog of focal mechanisms, allowing to perform a robust statistical analysis, is available. The 2000 dike intrusion at Miyakejima is in this sense an outstanding case, as about 18000 seismic events were recorded in a time span of three months. This seismic swarm was one of the most energetic ever recorded with five M>6 earthquakes. For this swarm a catalog of 1500 focal mechanisms is avalable (NIED, Japan). We perform a clustering analysis of the focal mechanism solutions, in order to infer the most frequent focal mechanism features prior to the intrusion (pre-diking period) and during the co-diking period. As previously suggested, we find that the dike stress field modified substantially the pre-existing seismicity pattern, by shadowing some non-optimally oriented strike-slip structures and increasing seismic rate on optimally oriented strike-slip tectonic structures. Alongside, during the co-diking period a large number of normal and oblique-normal faulting were observed. These events cannot be explained within the tectonics of the intrusion area. We suggest they are directly generated by the intense stress field induced at the

  18. Pre-eruption deformation caused by dike intrusion beneath Kizimen volcano, Kamchatka, Russia, observed by InSAR

    USGS Publications Warehouse

    Ji, Lingyun; Lu, Zhong; Dzurisin, Daniel; Senyukov, Sergey

    2013-01-01

    Interferometric synthetic aperture radar (InSAR) images reveal a pre-eruption deformation signal at Kizimen volcano, Kamchatka, Russia, where an ongoing eruption began in mid-November, 2010. The previous eruption of this basaltic andesite-to-dacite stratovolcano occurred in 1927–1928. InSAR images from both ascending and descending orbital passes of Envisat and ALOS PALSAR satellites show as much as 6 cm of line-of-sight shortening from September 2008 to September 2010 in a broad area centered at Kizimen. About 20 cm of opening of a nearly vertical dike provides an adequate fit to the surface deformation pattern. The model dike is approximately 14 km long, 10 km high, centered 13 km beneath Kizimen, and strikes NE–SW. Time-series analysis of multi-temporal interferograms indicates that (1) intrusion started sometime between late 2008 and July 2009, (2) continued at a nearly constant rate, and (3) resulted in a volume expansion of 3.2 × 107 m3 by September 2010, i.e., about two months before the onset of the 2010 eruption. Earthquakes located above the tip of the dike accompanied the intrusion. Eventually, magma pressure in the dike exceeded the confining strength of the host rock, triggering the 2010 eruption. Our results provide insight into the intrusion process that preceded an explosive eruption at a Pacific Rim stratovolcano following nearly a century of quiescence, and therefore have implications for monitoring and hazards assessment at similar volcanoes elsewhere.

  19. Relating Seismicity to Dike Emplacement, and the Conundrum of Dyke-Parallel Faulting

    NASA Astrophysics Data System (ADS)

    Dering, G.; Micklethwaite, S.; Cruden, A. R.; Barnes, S. J.; Fiorentini, M. L.

    2016-12-01

    Seismic monitoring shows that faulting and fracturing precede and accompany magma emplacement on timescales of hours and days. One outstanding problem is that the precision of earthquake hypocentre locations is typically limited to tens or hundreds of meters and cannot resolve whether the hypocentres relate to strain of wall rock fragments within the dikes, in a process zone around the intrusion or peripherally in the country rock. We examine a swarm of 19 dolerite dikes, near Albany, Western Australia using an unmanned aerial vehicle and Structure-from-Motion photogrammetry to obtain accurate, high resolution 3D reconstructions of outcrop and to digitally extract structural data. We find rare overprinting relationships indicate dike emplacement and faulting was coeval and that the number of faults/fractures increase into the dike swarm (2.2 ± 0.7 more fractures, per unit length in host rocks intruded by dikes relative to the background value). The faults are cataclasite-bearing and parallel to the dikes but intriguingly dike emplacement appears to have been accommodated by mode 1 extension. We further provide the first evidence that dike-parallel shear failure occurs in a damage zone associated with the dike swarm. These results support seismological observations of dike-parallel shear failure associated with some intrusion events, which contradict Mohr-Coulomb theory and numerical modelling of dike propagation in brittle-elastic rock, where shear failure is predicted to occur on faults oriented approximately 30° to the dyke plane. We suggest the dike swarm occupies a network of joints and fractures formed prior to swarm emplacement but then reactivated ahead of propagating dikes and remaining active during the early stages of emplacement.

  20. Lunar floor-fractured craters: Modes of dike and sill emplacement and implications of gas production and intrusion cooling on surface morphology and structure

    NASA Astrophysics Data System (ADS)

    Wilson, Lionel; Head, James W.

    2018-05-01

    Lunar floor-fractured craters (FFCs) represent the surface manifestation of a class of shallow crustal intrusions in which magma-filled cracks (dikes) rising to the surface from great depth encounter contrasts in host rock lithology (breccia lens, rigid solidified melt sheet) and intrude laterally to form a sill, laccolith or bysmalith, thereby uplifting and deforming the crater floor. Recent developments in the knowledge of lunar crustal thickness and density structure have enabled important revisions to models of the generation, ascent and eruption of magma, and new knowledge about the presence and behavior of magmatic volatiles has provided additional perspectives on shallow intrusion processes in FFCs. We use these new data to assess the processes that occur during dike and sill emplacement with particular emphasis on tracking the fate and migration of volatiles and their relation to candidate venting processes. FFCs result when dikes are capable of intruding close to the surface, but fail to erupt because of the substructure of their host impact craters, and instead intrude laterally after encountering a boundary where an increase in ductility (base of breccia lens) or rigidity (base of solidified melt sheet) occurs. Magma in dikes approaching the lunar surface experiences increasingly lower overburden pressures: this enhances CO gas formation and brings the magma into the realm of the low pressure release of H2O and sulfur compounds, both factors adding volatiles to those already collected in the rising low-pressure part of the dike tip. High magma rise velocity is driven by the positive buoyancy of the magma in the part of the dike remaining in the mantle. The dike tip overshoots the interface and the consequent excess pressure at the interface drives the horizontal flow of magma to form the intrusion and raise the crater floor. If sill intrusion were controlled by the physical properties at the base of the melt sheet, dikes would be required to approach to

  1. Geothermal evolution of an intruded dike in the rift zone of Kilauea volcano, Hawaii from VLF and self-potential measurements

    NASA Astrophysics Data System (ADS)

    Davis, Paul M.

    2015-09-01

    Self-potential (SP) and VLF measurements were made in 1973, 1975, 1995, 1997 and 2012 across a basaltic dike that intruded into the Koae fault zone of Kilauea volcano, Hawaii in May 1973. The SP anomaly remained strong throughout. In 2012 it was at about 60% of the strength it had in 1973. In contrast, the VLF anomaly, though diminished, was still observable in 1995/1997, but by 2012 it had disappeared. A hydrothermal dike model, with parameters calibrated by modeling the solidification of Kilauea Iki lava lake, is used to calculate temperatures and conductivity variation. Following Jaeger's (1957) method, we find that the time in years for a dike of width W (m) to solidify is 0.0075W2. Thus, a 1 m dike solidifies within the first few days, and after 39 years is only tens of degrees above ambient. Given the orders of magnitude difference between the conductivities of wet and dry basalt, we infer, that after solidification, the VLF anomalies were caused by induction in a localized veil of wet, hot basalt enveloping the dike, that was generated initially by condensation of steam, and subsequently by condensation of evaporated water as temperatures reduced. The conductivity anomaly persisted until the mid-nineties. By 2012, temperatures and condensation were too small for a VLF signal. The persistent SP anomaly is attributed to localized fluid disruption, with evaporation mainly at the water table and in the vadose zone. Streaming potentials are associated with evaporative circulation in the vadose zone. Next to the dike a positive potential is generated by upward flow of moisture-laden air, with a smaller negative potential on its flanks from downward infiltrating rainwater. The analysis indicates that the combination of SP and VLF measurements can characterize the evolving geothermal regime of intrusions above the water table.

  2. Conduits and dike distribution analysis in San Rafael Swell, Utah

    NASA Astrophysics Data System (ADS)

    Kiyosugi, K.; Connor, C.; Wetmore, P. H.; Ferwerda, B. P.; Germa, A.

    2011-12-01

    Volcanic fields generally consist of scattered monogenetic volcanoes, such as cinder cones and maars. The temporal and spatial distribution of monogenetic volcanoes and probability of future activity within volcanic fields is studied with the goals of understanding the origins of these volcano groups, and forecasting potential future volcanic hazards. The subsurface magmatic plumbing systems associated with volcanic fields, however, are rarely observed or studied. Therefore, we investigated a highly eroded and exposed magmatic plumbing system on the San Rafael Swell (UT) that consists of dikes, volcano conduits and sills. San Rafael Swell is part of the Colorado Plateau and is located east of the Rocky Mountain seismic belt and the Basin and Range. The overburden thickness at the time of mafic magma intrusion (Pliocene; ca. 4 Ma) into Jurassic sandstone is estimated to be ~800 m based on paleotopographical reconstructions. Based on a geologic map by P. Delaney and colleagues, and new field research, a total of 63 conduits are mapped in this former volcanic field. The conduits each reveal features of root zone and / or lower diatremes, including rapid dike expansion, peperite and brecciated intrusive and host rocks. Recrystallized baked zone of host rock is also observed around many conduits. Most conduits are basaltic or shonkinitic with thickness of >10 m and associated with feeder dikes intruded along N-S trend joints in the host rock, whereas two conduits are syenitic and suggesting development from underlying cognate sills. Conduit distribution, which is analyzed by a kernel function method with elliptical bandwidth, illustrates a N-S elongate higher conduit density area regardless of the azimuth of closely distributed conduits alignment (nearest neighbor distance <200 m). In addition, dike density was calculated as total dike length in unit area (km/km^2). Conduit and sill distribution is concordant with the high dike density area. Especially, the distribution

  3. Constraints on dike propagation from continuous GPS measurements

    NASA Astrophysics Data System (ADS)

    Segall, Paul; Cervelli, Peter; Owen, Susan; Lisowski, Mike; Miklius, Asta

    2001-09-01

    The January 1997 East Rift Zone eruption on Kilauea volcano, Hawaii, occurred within a network of continuous Global Positioning System (GPS) receivers. The GPS measurements reveal the temporal history of deformation during dike intrusion, beginning ˜8 hours prior to the onset of the eruption. The dike volume as a function of time, estimated from the GPS data using elastic Green's functions for a homogeneous half-space, shows that only two thirds of the final dike volume accumulated prior to the eruption and the rate of volume change decreased with time. These observations are inconsistent with simple models of dike propagation, which predict accelerating dike volume up to the time of the eruption and little or no change thereafter. Deflationary tilt changes at Kilauea summit mirror the inferred dike volume history, suggesting that the rate of dike propagation is limited by flow of magma into the dike. A simple, lumped parameter model of a coupled dike magma chamber system shows that the tendency for a dike to end in an eruption (rather than intrusion) is favored by high initial dike pressures, compressional stress states, large, compressible magma reservoirs, and highly conductive conduits linking the dike and source reservoirs. Comparison of model predictions to the observed dike volume history, the ratio of erupted to intruded magma, and the deflationary history of the summit magma chamber suggest that most of the magma supplied to the growing dike came from sources near to the eruption through highly conductive conduits. Interpretation is complicated by the presence of multiple source reservoirs, magma vesiculation and cooling, as well as spatial variations in dike-normal stress. Reinflation of the summit magma chamber following the eruption was measured by GPS and accompanied a rise in the level of the Pu'u O'o lava lake. For a spheroidal chamber these data imply a summit magma chamber volume of ˜20 km3, consistent with recent estimates from seismic

  4. Constraints on dike propagation from continuous GPS measurements

    USGS Publications Warehouse

    Segall, P.; Cervelli, Peter; Owen, S.; Lisowski, M.; Miklius, Asta

    2001-01-01

    The January 1997 East Rift Zone eruption on Kilauea volcano, Hawaii, occurred within a network of continuous Global Positioning System (GPS) receivers. The GPS measurements reveal the temporal history of deformation during dike intrusion, beginning ??? 8 hours prior to the onset of the eruption. The dike volume as a function of time, estimated from the GPS data using elastic Green's functions for a homogeneous half-space, shows that only two thirds of the final dike volume accumulated prior to the eruption and the rate of volume change decreased with time. These observations are inconsistent with simple models of dike propagation, which predict accelerating dike volume up to the time of the eruption and little or no change thereafter. Deflationary tilt changes at Kilauea summit mirror the inferred dike volume history, suggesting that the rate of dike propagation is limited by flow of magma into the dike. A simple, lumped parameter model of a coupled dike magma chamber system shows that the tendency for a dike to end in an eruption (rather than intrusion) is favored by high initial dike pressures, compressional stress states, large, compressible magma reservoirs, and highly conductive conduits linking the dike and source reservoirs. Comparison of model predictions to the observed dike volume history, the ratio of erupted to intruded magma, and the deflationary history of the summit magma chamber suggest that most of the magma supplied to the growing dike came from sources near to the eruption through highly conductive conduits. Interpretation is complicated by the presence of multiple source reservoirs, magma vesiculation and cooling, as well as spatial variations in dike-normal stress. Reinflation of the summit magma chamber following the eruption was measured by GPS and accompanied a rise in the level of the Pu'u O'o lava lake. For a spheroidal chamber these data imply a summit magma chamber volume of ??? 20 km3, consistent with recent estimates from seismic

  5. Volcanotectonic earthquakes induced by propagating dikes

    NASA Astrophysics Data System (ADS)

    Gudmundsson, Agust

    2016-04-01

    Volcanotectonic earthquakes are of high frequency and mostly generated by slip on faults. During chamber expansion/contraction earthquakes are distribution in the chamber roof. Following magma-chamber rupture and dike injection, however, earthquakes tend to concentrate around the dike and follow its propagation path, resulting in an earthquake swarm characterised by a number of earthquakes of similar magnitudes. I distinguish between two basic processes by which propagating dikes induce earthquakes. One is due to stress concentration in the process zone at the tip of the dike, the other relates to stresses induced in the walls and surrounding rocks on either side of the dike. As to the first process, some earthquakes generated at the dike tip are related to pure extension fracturing as the tip advances and the dike-path forms. Formation of pure extension fractures normally induces non-double couple earthquakes. There is also shear fracturing in the process zone, however, particularly normal faulting, which produces double-couple earthquakes. The second process relates primarily to slip on existing fractures in the host rock induced by the driving pressure of the propagating dike. Such pressures easily reach 5-20 MPa and induce compressive and shear stresses in the adjacent host rock, which already contains numerous fractures (mainly joints) of different attitudes. In piles of lava flows or sedimentary beds the original joints are primarily vertical and horizontal. Similarly, the contacts between the layers/beds are originally horizontal. As the layers/beds become buried, the joints and contacts become gradually tilted so that the joints and contacts become oblique to the horizontal compressive stress induced by a driving pressure of the (vertical) dike. Also, most of the hexagonal (or pentagonal) columnar joints in the lava flows are, from the beginning, oblique to an intrusive sheet of any attitude. Consequently, the joints and contacts function as potential shear

  6. Modeling Thermal Pressurization Around Shallow Dikes Using Temperature-Dependent Hydraulic Properties: Implications for Deformation Around Intrusions

    NASA Astrophysics Data System (ADS)

    Townsend, Meredith R.

    2018-01-01

    Pressurization and flow of groundwater around igneous intrusions depend in part on the hydraulic diffusivity of the host rocks and processes that enhance diffusivity, such as fracturing, or decrease diffusivity, such as mineral precipitation during chemical alteration. Characterizing and quantifying the coupled effects of alteration, pore pressurization, and deformation have significant implications for deformation around intrusions, geothermal energy, contact metamorphism, and heat transfer at mid-ocean ridges. Fractures around dikes at Ship Rock, New Mexico, indicate that pore pressures in the host rocks exceeded hydrostatic conditions by at least 15 MPa following dike emplacement. Hydraulic measurements and petrographic analysis indicate that mineral precipitation clogged the pores of the host rock, reducing porosity from 0.25 to <0.10 and reducing permeability by 5 orders of magnitude. Field data from Ship Rock are used to motivate and constrain numerical models for thermal pore fluid pressurization adjacent to a meter-scale dike, using temperature-dependent hydraulic properties in the host rock as a proxy for porosity loss by mineral precipitation during chemical alteration. Reduction in permeability by chemical alteration has a negligible effect on pressurization. However, reduction in porosity by mineral precipitation increases fluid pressure by constricting pore volume and is identified as a potentially significant source of pressure. A scaling relationship is derived to determine when porosity loss becomes important; if permeability is low enough, pressurization by porosity loss outweighs pressurization by thermal expansion of fluids.

  7. Quantification of the intrusion process at Kīlauea volcano, Hawai'i

    NASA Astrophysics Data System (ADS)

    Wright, Thomas L.; Marsh, Bruce

    2016-12-01

    The characteristic size of two types of intrusions identified beneath Kīlauea's East Rift zone are uniquely estimated by combining time constraints from fractional crystallization and the rates of magma solidification during cooling. Some intrusions were rapidly emplaced as dikes, but stalled before reaching the surface, and cooled and crystallized to feed later fractionated eruptions. More specifically, using the observed time interval between initial emplacement and eruption of fractionated lava, whose degree of fractionation is estimated from petrologic mixing calculations, the extent of solidification or cooling needed to produce this amount of fractionation can be directly inferred. And from the known erupted volumes the spatial extent or size of this fractionated volume can be analytically related to the full size of the source body itself. Two examples yield dike widths of 82 and 68 m. Other intrusions remain close to the east rift magma transport path and are observed to last for decades or longer as viable magma bodies that may participate in feeding later eruptions. The thickness of semi-permanent reservoirs near the East Rift Zone magma transport path can be estimated by assuming a resupply rate that is sufficiently frequent to restrict cooling to < 10 °C. It is inferred that both types of intrusions likely began as dike offshoots from the East Rift Zone magma transport path, but the frequently resupplied bodies may have later been converted to sills or laccoliths of heights estimated at 43-62 m. Our modeled intrusions contrast with models of rapidly emplaced thinner dikes feeding shallow intrusions, which are accompanied by intense rift earthquake swarms and are often associated with eruptions. These calculations show that long-term heating of the wallrock of the magma transport paths serves to slow conduit cooling, which may be partly responsible for sustaining long East Rift Zone eruptions. Adjacent to the vertical transport path beneath K

  8. Coupled heat and silica transport associated with dike intrusion into sedimentary rock: effects on isotherm location and permeability evolution

    NASA Astrophysics Data System (ADS)

    Dutrow, Barbara L.; Travis, Bryan J.; Gable, Carl W.; Henry, Darrell J.

    2001-11-01

    An 11-meter-wide alkalic monchiquite dike recovered from the subsurface of Louisiana has produced a metasomatic aureole in the adjacent interbedded carbonate mudstones and siltstones. The asymmetric contact aureole, which extends nearly 6 m above and 4 m below the intrusion, contains the metamorphic minerals, diopside, pectolite, fluor-apophyllite, fluorite, and garnet. A series of coupled heat and mass transport calculations was undertaken to provide thermal constraints for the aureole, in the absence of robust geothermometric assemblages, and insights into accompanying mass transport associated with the sedimentary rock-dike system. Calculations were completed for systems with homogeneous, anisotropic, and layered permeability, κ. Transport, dissolution, and precipitation of silica were also incorporated into calculations. All systems modeled indicate that the thermal pulse waned in ∼3 yr with a return to background temperatures in ∼10 yr. Heat and fluid transport produce maximum temperature isotherms that are distinctly different in spatial extent and lateral variability for each numerical system. The homogeneous κ case produced isotherms that pinch and swell vertically above the dike and have large lateral variations, in contrast to the anisotropic κ case that produced a single large plume above the dike. The layered system κ case produced the most spatially extensive thermal aureole, unlike that recorded in the rocks. Addition of dissolved silica to the flow system significantly impacts the calculated transport of heat and fluid, primarily due to density changes that affect upwelling dynamics. Although precipitation and dissolution of SiO2 can affect flow through the feedback to permeability, κ changes were found to be minor for these system conditions. Where κ decreased, flow was refocused into higher κ zones, thus mitigating the κ differences over time. This negative feedback tends to defocus flow and provides a mechanism for lateral migration of

  9. Dike intrusions into bituminous coal, Illinois Basin: H, C, N, O isotopic responses to rapid and brief heating

    USGS Publications Warehouse

    Schimmelmann, A.; Mastalerz, Maria; Gao, L.; Sauer, P.E.; Topalov, K.

    2009-01-01

    Unlike long-term heating in subsiding sedimentary basins, the near-instantaneous thermal maturation of sedimentary organic matter near magmatic intrusions is comparable to artificial thermal maturation in the laboratory in terms of short duration and limited extent. This study investigates chemical and H, C, N, O isotopic changes in high volatile bituminous coal near two Illinois dike contacts and compares observed patterns and trends with data from other published studies and from artificial maturation experiments. Our study pioneers in quantifying isotopically exchangeable hydrogen and measuring the D/H (i.e., 2H/1H) ratio of isotopically non-exchangeable organic hydrogen in kerogen near magmatic contacts. Thermal stress in coal caused a reduction of isotopically exchangeable hydrogen in kerogen from 5% to 6% in unaltered coal to 2-3% at contacts, mostly due to elimination of functional groups (e.g., {single bond}OH, {single bond}COOH, {single bond}NH2). In contrast to all previously published data on D/H in thermally matured organic matter, the more mature kerogen near the two dike contacts is D-depleted, which is attributed to (i) thermal elimination of D-enriched functional groups, and (ii) thermal drying of hydrologically isolated coal prior to the onset of cracking reactions, thereby precluding D-transfer from relatively D-enriched water into kerogen. Maxima in organic nitrogen concentration and in the atomic N/C ratio of kerogen at a distance of ???2.5 to ???3.5 m from the thicker dike indicate that reactive N-compounds had been pyrolytically liberated at high temperature closer to the contact, migrated through the coal seam, and recombined with coal kerogen in a zone of lower temperature. The same principle extends to organic carbon, because a strong ??13Ckerogen vs. ??15Nkerogen correlation across 5.5 m of coal adjacent to the thicker dike indicates that coal was functioning as a flow-through reactor along a dynamic thermal gradient facilitating back

  10. Dike propagation energy balance from deformation modeling and seismic release

    NASA Astrophysics Data System (ADS)

    Bonaccorso, Alessandro; Aoki, Yosuke; Rivalta, Eleonora

    2017-06-01

    Magma is transported in the crust mainly by dike intrusions. In volcanic areas, dikes can ascend toward the free surface and also move by lateral propagation, eventually feeding flank eruptions. Understanding dike mechanics is a key to forecasting the expected propagation and associated hazard. Several studies have been conducted on dike mechanisms and propagation; however, a less in-depth investigated aspect is the relation between measured dike-induced deformation and the seismicity released during its propagation. We individuated a simple x that can be used as a proxy of the expected mechanical energy released by a propagating dike and is related to its average thickness. For several intrusions around the world (Afar, Japan, and Mount Etna), we correlate such mechanical energy to the seismic moment released by the induced earthquakes. We obtain an empirical law that quantifies the expected seismic energy released before arrest. The proposed approach may be helpful to predict the total seismic moment that will be released by an intrusion and thus to control the energy status during its propagation and the time of dike arrest.Plain Language Summary<span class="hlt">Dike</span> propagation is a dominant mechanism for magma ascent, transport, and eruptions. Besides being an intriguing physical process, it has critical hazard implications. After the magma <span class="hlt">intrusion</span> starts, it is difficult to predict when and where a specific horizontal <span class="hlt">dike</span> is going to halt and what its final length will be. In our study, we singled an equation that can be used as a proxy of the expected mechanical energy to be released by the opening <span class="hlt">dike</span>. We related this expected energy to the seismic moment of several eruptive <span class="hlt">intrusions</span> around the world (Afar region, Japanese volcanoes, and Mount Etna). The proposed novel approach is helpful to estimate the total seismic moment to be released, therefore allowing potentially predicting when the <span class="hlt">dike</span> will end its propagation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26PSL.434...64M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26PSL.434...64M"><span>On the mechanisms governing <span class="hlt">dike</span> arrest: Insight from the 2000 Miyakejima <span class="hlt">dike</span> injection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maccaferri, F.; Rivalta, E.; Passarelli, L.; Aoki, Y.</p> <p>2016-01-01</p> <p>Magma stored beneath volcanoes is sometimes transported out of the magma chambers by means of laterally propagating <span class="hlt">dikes</span>, which can lead to fissure eruptions if they intersect the Earth's surface. The driving force for lateral <span class="hlt">dike</span> propagation can be a lateral tectonic stress gradient, the stress gradient due to the topographic loads, the overpressure of the magma chamber, or a combination of those forces. The 2000 <span class="hlt">dike</span> <span class="hlt">intrusion</span> at Miyakejima volcano, Izu arc, Japan, propagated laterally for about 30 km and stopped in correspondence of a strike-slip system, sub-perpendicular to the <span class="hlt">dike</span> plane. Then the <span class="hlt">dike</span> continued to inflate, without further propagation. Abundant seismicity was produced, including five M > 6 earthquakes, one of which occurred on the pre-existing fault system close to the tip of the <span class="hlt">dike</span>, at approximately the time of arrest. It has been proposed that the main cause for the <span class="hlt">dike</span> arrest was the fault-induced stress. Here we use a boundary element numerical approach to study the interplay between a propagating <span class="hlt">dike</span> and a pre-stressed strike-slip fault and check the relative role played by <span class="hlt">dike</span>-fault interaction and topographic loading in arresting the Miyakejima <span class="hlt">dike</span>. We calibrate the model parameters according to previous estimates of <span class="hlt">dike</span> opening and fault displacement based on crustal deformation observations. By computing the energy released during the propagation, our model indicates whether the <span class="hlt">dike</span> will stop at a given location. We find that the stress gradient induced by the topography is needed for an opening distribution along the <span class="hlt">dike</span> consistent with the observed seismicity, but it cannot explain its arrest at the prescribed location. On the other hand, the interaction of <span class="hlt">dike</span> with the fault explains the arrest but not the opening distribution. The joint effect of the topographic load and the stress interaction with strike-slip fault is consistent with the observations, provided the pre-existing fault system is pre-loaded with a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://onlinelibrary.wiley.com/doi/10.1002/grl.50633/abstract','USGSPUBS'); return false;" href="http://onlinelibrary.wiley.com/doi/10.1002/grl.50633/abstract"><span><span class="hlt">Intrusive</span> <span class="hlt">dike</span> complexes, cumulate cores, and the extrusive growth of Hawaiian volcanoes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Flinders, Ashton F.; Ito, Garrett; Garcia, Michael O.; Sinton, John M.; Kauahikaua, Jim; Taylor, Brian</p> <p>2013-01-01</p> <p>The Hawaiian Islands are the most geologically studied hot-spot islands in the world yet surprisingly, the only large-scale compilation of marine and land gravity data is more than 45 years old. Early surveys served as reconnaissance studies only, and detailed analyses of the crustal-density structure have been limited. Here we present a new chain-wide gravity compilation that incorporates historical island surveys, recently published work on the islands of Hawai‘i, Kaua‘i, and Ni‘ihau, and >122,000 km of newly compiled marine gravity data. Positive residual gravity anomalies reflect dense <span class="hlt">intrusive</span> bodies, allowing us to locate current and former volcanic centers, major rift <span class="hlt">zones</span>, and a previously suggested volcano on Ka‘ena Ridge. By inverting the residual gravity data, we generate a 3-D view of the dense, <span class="hlt">intrusive</span> complexes and olivine-rich cumulate cores within individual volcanoes and rift <span class="hlt">zones</span>. We find that the Hāna and Ka‘ena ridges are underlain by particularly high-density <span class="hlt">intrusive</span> material (>2.85 g/cm3) not observed beneath other Hawaiian rift <span class="hlt">zones</span>. Contrary to previous estimates, volcanoes along the chain are shown to be composed of a small proportion of <span class="hlt">intrusive</span> material (<30% by volume), implying that the islands are predominately built extrusively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034169','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034169"><span>Spatiotemporal evolution of <span class="hlt">dike</span> opening and décollement slip at Kīlauea Volcano, Hawai'i</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Montgomery-Brown, E. K.; Sinnett, D.K.; Larson, K.M.; Poland, Michael P.; Segall, P.; Miklius, Asta</p> <p>2011-01-01</p> <p>Rapid changes in ground tilt and GPS positions on Kīlauea Volcano, Hawai'i, are interpreted as resulting from a shallow, two-segment <span class="hlt">dike</span> <span class="hlt">intrusion</span> into the east rift <span class="hlt">zone</span> that began at 1217 UTC (0217 HST) on 17 June 2007 and lasted almost 3 days. As a result of the <span class="hlt">intrusion</span>, a very small volume of basalt (about 1500 m3) erupted on 19 June. Northward tilt at a coastal tiltmeter, subsidence of south flank GPS sites, southeastward displacements at southwestern flank GPS sites, and a swarm of flank earthquakes suggest that a slow slip event occurred on the décollement beneath Kīlauea's south flank concurrent with the rift <span class="hlt">intrusion</span>. We use 4 min GPS positions that include estimates of time-dependent tropospheric gradients and ground tilt data to study the spatial and temporal relationships between the two inferred shallow, steeply dipping <span class="hlt">dike</span> segments extending from the surface to about 2 km depth and décollement slip at 8 km depth. We invert for the temporal evolution of distributed <span class="hlt">dike</span> opening and décollement slip in independent inversions at each time step using a nonnegative least squares algorithm. On the basis of these inversions, the <span class="hlt">intrusion</span> occurred in two stages that correspond spatially and temporally with concentrated rift <span class="hlt">zone</span> seismicity. The <span class="hlt">dike</span> opening began on the western of the two segments before jumping to the eastern segment, where the majority of opening accumulated. <span class="hlt">Dike</span> opening preceded the start of décollement slip at an 84% confidence level; the latter is indicated by the onset of northward tilt of a coastal tiltmeter. Displacements at southwest flank GPS sites began about 18 h later and are interpreted as resulting from slow slip on the southwestern flank. Additional constraints on the evolution of the <span class="hlt">intrusion</span> and décollement slip come from inversion of an Envisat interferogram that spans the <span class="hlt">intrusion</span> until 0822 UTC on 18 June 2007, combined with GPS and tilt data. This inversion shows that up to 0822 UTC on 18 June, d</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/18451','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/18451"><span>Work <span class="hlt">zone</span> <span class="hlt">intrusion</span> alarm effectiveness.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2010-09-01</p> <p>16. Abstract : The New Jersey Department of Transportation (NJDOT) commissioned a study to evaluate how : effective a work <span class="hlt">zone</span> safety device known as the SonoBlaster! Work <span class="hlt">Zone</span> <span class="hlt">Intrusion</span> Alarm would be : in protecting maintenance workers fro...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035898','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035898"><span>The May 2005 eruption of Fernandina volcano, Galápagos: The first circumferential <span class="hlt">dike</span> <span class="hlt">intrusion</span> observed by GPS and InSAR</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Chadwick, W.W.; Jonsson, Sigurjon; Geist, Dennis J.; Poland, M.; Johnson, Daniel J.; Batt, S.; Harpp, Karen S.; Ruiz, A.</p> <p>2011-01-01</p> <p>The May 2005 eruption of Fernandina volcano, Galápagos, occurred along circumferential fissures parallel to the caldera rim and fed lava flows down the steep southwestern slope of the volcano for several weeks. This was the first circumferential <span class="hlt">dike</span> <span class="hlt">intrusion</span> ever observed by both InSAR and GPS measurements and thus provides an opportunity to determine the subsurface geometry of these enigmatic structures that are common on Galápagos volcanoes but are rare elsewhere. Pre- and post- eruption ground deformation between 2002 and 2006 can be modeled by the inflation of two separate magma reservoirs beneath the caldera: a shallow sill at ~1 km depth and a deeper point-source at ~5 km depth, and we infer that this system also existed at the time of the 2005 eruption. The co-eruption deformation is dominated by uplift near the 2005 eruptive fissures, superimposed on a broad subsidence centered on the caldera. Modeling of the co-eruption deformation was performed by including various combinations of planar dislocations to simulate the 2005 circumferential <span class="hlt">dike</span> <span class="hlt">intrusion</span>. We found that a single planar <span class="hlt">dike</span> could not match both the InSAR and GPS data. Our best-fit model includes three planar <span class="hlt">dikes</span> connected along hinge lines to simulate a curved concave shell that is steeply dipping (~45–60°) toward the caldera at the surface and more gently dipping (~12–14°) at depth where it connects to the horizontal sub-caldera sill. The shallow sill is underlain by the deep point source. The geometry of this modeled magmatic system is consistent with the petrology of Fernandina lavas, which suggest that circumferential eruptions tap the shallowest parts of the system, whereas radial eruptions are fed from deeper levels. The recent history of eruptions at Fernandina is also consistent with the idea that circumferential and radial <span class="hlt">intrusions</span> are sometimes in a stress-feedback relationship and alternate in time with one another.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033239','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033239"><span>Changes in optical properties, chemistry, and micropore and mesopore characteristics of bituminous coal at the contact with <span class="hlt">dikes</span> in the Illinois Basin</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mastalerz, Maria; Drobniak, A.; Schimmelmann, A.</p> <p>2009-01-01</p> <p>Changes in high-volatile bituminous coal (Pennsylvanian) near contacts with two volcanic <span class="hlt">intrusions</span> in Illinois were investigated with respect to optical properties, coal chemistry, and coal pore structure. Vitrinite reflectance (Ro) increases from 0.62% to 5.03% within a distance of 5.5??m from the larger <span class="hlt">dike</span>, and from 0.63% to 3.71% within 3.3??m from the small <span class="hlt">dike</span>. Elemental chemistry of the coal shows distinct reductions in hydrogen and nitrogen content close to the <span class="hlt">intrusions</span>. No trend was observed for total sulfur content, but decreases in sulfate content towards the <span class="hlt">dikes</span> indicate thermochemical sulfate reduction (TSR). Contact-metamorphism has a dramatic effect on coal porosity, and microporosity in particular. Around the large <span class="hlt">dike</span>, the micropore volume, after a slight initial increase, progressively decreases from 0.0417??cm3/g in coal situated 4.7??m from the <span class="hlt">intrusive</span> contact to 0.0126??cm3/g at the contact. Strongly decreasing mesopore and micropore volumes in the altered <span class="hlt">zone</span>, together with frequent cleat and fracture filling by calcite, indicate deteriorating conditions for both coalbed gas sorption and gas transmissibility. ?? 2008 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035274','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035274"><span><span class="hlt">Dike</span> orientations in the late jurassic independence <span class="hlt">dike</span> swarm and implications for vertical-axis tectonic rotations in eastern California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hopson, R.F.; Hillhouse, J.W.; Howard, K.A.</p> <p>2008-01-01</p> <p>Analysis of the strikes of 3841 <span class="hlt">dikes</span> in 47 domains in the 500-km-long Late Jurassic Independence <span class="hlt">dike</span> swarm indicates a distribution that is skewed clockwise from the dominant northwest strike. Independence <span class="hlt">dike</span> swarm azimuths tend to cluster near 325?? ?? 30??, consistent with initial subparallel <span class="hlt">intrusion</span> along much of the swarm. <span class="hlt">Dike</span> azimuths in a quarter of the domains vary widely from the dominant trend. In domains in the essentially unrotated Sierra Nevada block, mean <span class="hlt">dike</span> azimuths range mostly between 300?? and 320??, with the exception of Mount Goddard (247??). Mean <span class="hlt">dike</span> azimuths in domains in the Basin and Range Province in the Argus, Inyo, and White Mountains areas range from 291?? to 354?? the mean is 004?? in the El Paso Mountains. In the Mojave Desert, mean <span class="hlt">dike</span> azimuths range from 318?? to 023??, and in the eastern Transverse Ranges, they range from 316?? to 051??. Restoration for late Cenozoic vertical-axis rotations, suggested by paleodeclinations determined from published studies from nearby Miocene and younger rocks, shifts <span class="hlt">dike</span> azimuths into better agreement with azimuths measured in the tectonically stable Sierra Nevada. This confirms that vertical-axis tectonic rotations explain some of the dispersion in orientation, especially in the Mojave Desert and eastern Transverse Ranges, and that the <span class="hlt">dike</span> orientations can be a useful if imperfect guide to tectonic rotations where paleomagnetic data do not exist. Large deviations from the main trend of the swarm may reflect (1) clockwise rotations for which there is no paleomagnetic evidence available, (2) <span class="hlt">dike</span> <span class="hlt">intrusions</span> of other ages, (3) crack filling at angles oblique or perpendicular to the main swarm, (4) pre-Miocene rotations, or (5) unrecognized domain boundaries between <span class="hlt">dike</span> localities and sites with paleomagnetic determinations. ?? 2008 The Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020980','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020980"><span>Fluid inclusion and vitrinite-reflectance geothermometry compared to heat-flow models of maximum paleotemperature next to <span class="hlt">dikes</span>, western onshore Gippsland Basin, Australia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barker, C.E.; Bone, Y.; Lewan, M.D.</p> <p>1999-01-01</p> <p>Nine basalt <span class="hlt">dikes</span>, ranging from 6 cm to 40 m thick, intruding the Upper Jurassic-Lower Cretaceous Strzelecki Group, western onshore Gippsland Basin, were used to study maximum temperatures (Tmax) reached next to <span class="hlt">dikes</span>. Tmax was estimated from fluid inclusion and vitrinitereflectance geothermometry and compared to temperatures calculated using heat-flow models of contact metamorphism. Thermal history reconstruction suggests that at the time of <span class="hlt">dike</span> <span class="hlt">intrusion</span> the host rock was at a temperature of 100-135??C. Fracture-bound fluid inclusions in the host rocks next to thin <span class="hlt">dikes</span> ( 1.5, using a normalized distance ratio used for comparing measurements between <span class="hlt">dikes</span> regardless of their thickness. In contrast, the pattern seen next to the thin <span class="hlt">dikes</span> is a relatively narrow <span class="hlt">zone</span> of elevated Rv-r. Heat-flow modeling, along with whole rock elemental and isotopic data, suggests that the extended <span class="hlt">zone</span> of elevated Rv-r is caused by a convection cell with local recharge of the hydrothermal fluids. The narrow <span class="hlt">zone</span> of elevated Rv-r found next to thin <span class="hlt">dikes</span> is attributed to the rise of the less dense, heated fluids at the <span class="hlt">dike</span> contact causing a flow of cooler groundwater towards the <span class="hlt">dike</span> and thereby limiting its heating effects. The lack of extended heating effects suggests that next to thin <span class="hlt">dikes</span> an incipient convection system may form in which the heated fluid starts to travel upward along the <span class="hlt">dike</span> but cooling occurs before a complete convection cell can form. Close to the <span class="hlt">dike</span> contact at X/D 1.5. ?? 1998 Elsevier Science B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70193352','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70193352"><span>Geochemistry and mineralogy of the Dotson <span class="hlt">Zone</span> HREE deposit in the Bokan Mountain peralkaline igneous complex, southeastern Alaska, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Taylor, Cliff D.; Lowers, Heather; Adams, David; Robinson, R. James</p> <p>2017-01-01</p> <p>The Bokan Mountain igneous complex (BMIC) is a typical example of a peralkaline <span class="hlt">intrusive</span> system that has evolved to the point of developing late stage HFSE- and REE-rich silicic pegmatites and <span class="hlt">dikes</span>. The Dotson <span class="hlt">Zone</span> comprises a series of felsic <span class="hlt">dikes</span> that extend from the southeast margin of the composite pluton and may represent an important resource of critical HREEs. Petrographically, the primary igneous mineral assemblage is altered by late-igneous and hydrothermal fluids resulting in redistribution and enrichment of REEs. An area of flexure in the southeastern end of the Dotson <span class="hlt">Zone</span> was the primary locus of enrichment as shown by the pervasive alteration and consistently high REE+Y values. We favor a model in which the <span class="hlt">dikes</span> were emplaced concurrently with the marginal <span class="hlt">intrusions</span>, and then altered during emplacement of the inner, main <span class="hlt">intrusion</span> in a relatively rapid series of overlapping <span class="hlt">intrusive</span> and late magmatic fluid-high temperature hydrothermal events as the complex cooled. A much later sodic <span class="hlt">intrusive</span> event focused on the BMIC may have resulted in additional silica-Na-Zr-rich alteration in proximity to the pluton.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/35396','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/35396"><span>Work <span class="hlt">Zone</span> <span class="hlt">Intrusion</span> Report Interface Design</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2018-02-02</p> <p>While necessary for roadways, work <span class="hlt">zones</span> present a safety risk to crew. Half of road workers deaths between 2005 and 2010 were due to collisions with motorists intruding on the work <span class="hlt">zone</span>. Therefore, addressing <span class="hlt">intrusions</span> is an important step for ensu...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_2 --> <div id="page_3" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="41"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/18351','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/18351"><span><span class="hlt">Zone</span> of <span class="hlt">intrusion</span> study.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2010-10-15</p> <p>The Midwest Roadside Safety Facility (MwRSF) performed an analysis using LS-DYNA simulation to investigate the <span class="hlt">zone</span> of <span class="hlt">intrusion</span> (ZOI) of an NCHRP Report No. 350 2000p pickup truck when impacting a 40-in. high F-shape parapet. : The ZOI for the 40-in...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940020107','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940020107"><span>The transition from diapirism to <span class="hlt">dike</span> <span class="hlt">intrusion</span>: Implications for planetary volcanism</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubin, Allan M.</p> <p>1994-01-01</p> <p>Magma transport processes influence the rate of magma transport and how far the magma travels before it freezes, the degree to which the magma communicates chemically with the host rock, the morphology of volcanic landforms on planetary surfaces, the interplay between magmatism and regional tectonics, and even the direction the magma moves. The primary question motivating this research is: How does magma rheology influence the mechanisms by which it is transported through planetary lithospheres? It is widely recognized that on Earth basaltic <span class="hlt">intrusions</span> typically take the form of narrow <span class="hlt">dikes</span>, while granites are typically found in more equidimensional plutons. Several explanations for this observation were offered over the last 50 years. While basalts and rhyolites vary somewhat in temperature and density, the major difference is the 2 to 8 orders of magnitude contrast in viscosity. The significant ductile strains associated with many granitic plutons has led to the statement that the occurrence of granites in diapirs rather than <span class="hlt">dikes</span> results from the fact that there is insufficient viscosity contrast between the magma and wall rock for the granite to intrude narrow cracks. A second explanation states that granites are so viscous that they cannot propagate far before freezing. Despite the length of time these explanations have been around, there has been relatively little effort to investigate them quantitatively. My goal has been to evaluate these explanations through a series of well-posed numerical models. These models can be tested by the decades of field data collected by structural geologists that have yet to be integrated into any coherent theory, and the results should have important implications for volcanism on the terrestrial planets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMNH53A1731B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMNH53A1731B"><span>Deformation signals from InSAR time series analysis related to the 2007 and 2011 east rift <span class="hlt">zone</span> <span class="hlt">intrusions</span> at Kilauea Volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baker, S.; Amelung, F.</p> <p>2011-12-01</p> <p>Located on the Big Island of Hawaii, Kilauea volcano is one of the most active volcanoes on Earth with continuous eruptive activity since 1983. The eruptive activity is predominately from the Pu'u O'o vent within the east rift <span class="hlt">zone</span>, but periodic <span class="hlt">intrusions</span> occur in the upper east rift <span class="hlt">zone</span> between the summit and Pu'u O'o. These <span class="hlt">intrusions</span> occur as <span class="hlt">dikes</span> typically accompanied by fissure openings and eruptions of small volumes of lava. Interferometric synthetic aperture radar (InSAR) provides surface displacement measurements showing how the ground moves before, during, and after these <span class="hlt">intrusions</span>. Given the recent increase in the number of active or planned SAR satellites and the more frequent repeat-pass times, InSAR is proving to be a valuable monitoring tool for volcanic hazards. Using data from Radarsat-1, Envisat, ALOS, and TerraSAR-X satellites, we generate line-of-sight InSAR time series using the small baseline subset (SBAS) which provides dense spatial and temporal coverage at Kilauea covering the 17 June 2007 and 5 March 2011 <span class="hlt">intrusions</span>. For these two events, the summit caldera area switches from deflation to inflation months to years before both <span class="hlt">intrusions</span>, and just prior to the <span class="hlt">intrusions</span> we observe increased rates of inflation accompanied by elevated seismic activity in the upper east rift <span class="hlt">zone</span>. Observations of the <span class="hlt">intrusion</span> relate surface displacement and the response of the summit caldera area provide insight into the shallow magmatic system and the connectivity of the system. By combining InSAR time series with other geophysical data sets (such as seismic or GPS), we obtain more details about the associated hazard and a better understanding of the time-dependent relationship between what we are measuring and the controlling processes at the volcano.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JSAES..77...70S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JSAES..77...70S"><span>Mafic subvolcanic <span class="hlt">intrusions</span> and their petrologic relation with the volcanism in the south hinge Torres Syncline, Paraná-Etendeka Igneous Province, southern Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sarmento, Carla Cecília Treib; Sommer, Carlos Augusto; Lima, Evandro Fernandes</p> <p>2017-08-01</p> <p> coast, with the same direction as the Namibia coast <span class="hlt">dike</span> swarm. This suggests that these <span class="hlt">dikes</span> were part of the triple junction system related to the opening of the South Atlantic Ocean. The preferred directions of the <span class="hlt">intrusive</span> <span class="hlt">dikes</span> in the lava flows are similar to the directions of the Ponta Grossa and Rio Grande Arcs and the Torres Syncline. They may have been a part of, or been caused by one or more geotectonic cycles that originated these structures. The emplacement process of the asymmetric <span class="hlt">dikes</span> suggests they were enclosed under the hydraulic fracture model, since they do not follow a pre-existing fracture filling pattern. The emplacement of the sills conforms to the weakness <span class="hlt">zones</span> of the sedimentary units. Regarding the <span class="hlt">intrusive</span> <span class="hlt">dikes</span> in the flows, divided by lithofacies associations, also taking into account the geochemical and petrographic similarities, it is observed that these <span class="hlt">dikes</span> are part of a supply system of the basic lava flows, stratigraphically positioned above the host lava flows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V44A..04W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V44A..04W"><span>Quantification of the <span class="hlt">Intrusion</span> Process at Kïlauea Volcano, Hawai'I</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wright, T. L.; Marsh, B. D.</p> <p>2014-12-01</p> <p>Knowing the time between initial <span class="hlt">intrusion</span> and later eruption of a given volume of differentiated magma is key to evaluating the connections among magma transport and emplacement, solidification and differentiation, and melt extraction and eruption. Cooling rates for two Kïlauea lava lakes as well as known parent composition and residence times for <span class="hlt">intrusions</span> that resulted in fractionated lavas later erupted on the East Rift <span class="hlt">Zone</span> in 1955 (34 years) and 1977 (22 years) allow <span class="hlt">intrusion</span> dimensions to be calculated. We model <span class="hlt">intrusions</span> beneath Kïlauea's East Rift <span class="hlt">Zone</span> near their point of separation from the magma transport path at ~ 5 km depth using Jaeger's (1957) method calibrated against Alae and Makaopuhi lava lakes with wallrock temperatures above the curie point at 450-550°C. Minimum thicknesses of 50-70 meters are found for <span class="hlt">intrusions</span> that fed the two fractionated lavas, as well as for long-lived magma bodies identified from geodetic monitoring during many East Rift eruptions. These <span class="hlt">intrusions</span> began as <span class="hlt">dikes</span>, but probably became sills or laccolithic bodies that remained near the transport path. Short-lived <span class="hlt">intrusions</span> also arrested near the magma transport path, but that retain a <span class="hlt">dike</span> geometry, are hypothesized to serve as a trigger for the small but discrete increments of seaward movement on Kïlauea's south flank that characterize slow-slip earthquakes. Two additional thoughts arise from the quantitative modeling of magma cooling. First, long-term heating of the wallrock surrounding the horizontal East Rift <span class="hlt">Zone</span> transport path slows the rate of cooling within the conduit, possibly contributing to the longevity of the East Rift eruption that began in 1983. Second, the combined effects of heating of the wall rock and ever-increasing magma supply rate from the mantle may have forced breakdown and widening of the vertical transport conduit, which could explain the 5-15-km deep long-period earthquake swarms beneath Kīlauea's summit between 1987 and 1992.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V43B3145W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V43B3145W"><span><span class="hlt">Dike</span> Propagation Mechanisms from Seismicity Accompanying the 2014 Bárðarbunga-Holuhraun Fissure Eruption, Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Woods, J.; Ágústsdóttir, T.; Greenfield, T. S.; Green, R. G.; White, R. S.; Brandsdottir, B.</p> <p>2015-12-01</p> <p>We present data from our dense seismic network which captured in unprecedented detail the micro-seismicity associated with the 2014 <span class="hlt">dike</span> <span class="hlt">intrusion</span> from the subglacial Bárðarbunga volcano in central Iceland. Over 30,000 automatically located earthquakes delineate a complex 46 km <span class="hlt">dike</span> propagation during the days preceding the onset of effusive magmatism at the Holuhraun lava field on 29 August 2014. Approximately 1.5 km3 of lava was erupted, making this the largest eruption in Iceland for over 200 years.Micro-seismicity tracks the lateral migration of the <span class="hlt">dike</span>, with a concentration of earthquakes in the advancing tip where stresses are greatest, and trailing <span class="hlt">zones</span> of lesser or no seismicity behind. Onset of an initial 4 hour fissure eruption was accompanied simultaneously by a backward retreat in seismic activity, followed by a gradual re-advance prior to the onset of a second, sustained fissure eruption in the same location on 31 August. Rock fracture mechanisms are determined from fault plane solutions of these seismic events. At the tip of the advancing <span class="hlt">dike</span>, left-lateral strike-slip faulting parallel to the propagation is dominant, utilising pre-existing lineations and releasing stress accumulated in the brittle layer from rift <span class="hlt">zone</span> extension. Behind the <span class="hlt">dike</span> tip, both right-lateral and left-lateral strike-slip earthquakes are found, marking failure of solidifying magma plugs within the <span class="hlt">dike</span> conduit. Contrary to many models of <span class="hlt">dike</span> propagation, both normal faulting and failure at high angles to the <span class="hlt">dike</span> are rare. Furthermore, a distinct lack of seismicity is observed in the 3-4 km region beneath the surface rupture. This suggests that opening is occuring aseismically, with earthquakes focused at the base of the <span class="hlt">dike</span> near the brittle-ductile boundary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V43B3144A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V43B3144A"><span>Detailed Segmentation and Episodic Propagation of the 2014 Bárðarbunga <span class="hlt">Dike</span> <span class="hlt">Intrusion</span> and Seismicity Accompanying the Sustained Holuhraun Eruption, Central Icleand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ágústsdóttir, T.; Woods, J.; Greenfield, T. S.; Green, R. G.; White, R. S.; Brandsdottir, B.</p> <p>2015-12-01</p> <p>An intense swarm of seismicity on 16 August 2014 marked the <span class="hlt">intrusion</span> of a large <span class="hlt">dike</span> from the subglacial Bárðarbunga volcano, central Iceland. Melt propagated laterally from the central volcano at the brittle-ductile boundary at ~6 km b.s.l. and created over 30,000 earthquakes along a 46 km path heading NE from Bárðarbunga. On 31 August a fissure eruption began at Holuhraun and the seismicity rate within the <span class="hlt">dike</span> dropped instantaneously to a much lower level suggesting that once a pathway to the surface had formed, magma was able to flow freely and largely aseismically. Melt was fed from the subsiding Bárðarbunga volcano to Holuhraun for 6 months, until the eruption ceased on 27 February 2015. We discuss the relationship between bursts of seismicity in the feeder volcano and periods of rapid <span class="hlt">dike</span> propagation. We use a dense seismic network and relative earthquake relocations to map in detail the segmentation of the <span class="hlt">dike</span> on all scales. New <span class="hlt">dike</span> segments were initiated with a rapid advance of the <span class="hlt">dike</span> tip at typically 1 km/h, separated by pauses of up to 78 h. During the stalled periods the magma pressure built until it was sufficient to fracture a new segment, which then propagated rapidly forward. Large segments became seismically quiet once a new segment had intruded beyond it as extensional stresses had been relieved and melt was able to flow freely. Each rapid propagation phase was accompanied by a drop in the seismicity rate directly behind the <span class="hlt">dike</span> tip, most likely due to a stress shadow being formed behind the <span class="hlt">dike</span> tip. Moment tensor solutions show that the dominant failure mechanism is left-lateral strike slip faulting at the leading edge, orientated parallel to the <span class="hlt">dike</span>, with a combination of right-lateral, left-lateral and normal faulting behind the <span class="hlt">dike</span> tip, contradicting many widely used models. Much of the seismicity behind the tip may represent fracture of frozen melt as the <span class="hlt">dike</span> inflated and propagated forward</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V51E2737L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V51E2737L"><span>Three-Dimensional Analysis of <span class="hlt">dike</span>/fault interaction at Mono Basin (California) using the Finite Element Method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>La Marra, D.; Battaglia, M.</p> <p>2013-12-01</p> <p>Mono Basin is a north-trending graben that extends from the northern edge of Long Valley caldera towards the Bodie Hills and is bounded by the Cowtrack Mountains on the east and the Sierra Nevada on the west. The Mono-Inyo Craters volcanic chain forms a north-trending <span class="hlt">zone</span> of volcanic vents extending from the west moat of the Long Valley caldera to Mono Lake. The Hartley Springs fault transects the southern Mono Craters-Inyo Domes area between the western part of the Long Valley caldera and June Lake. Stratigraphic data suggest that a series of strong earthquakes occurred during the North Mono-Inyo eruption sequence of ~1350 A.D. The spatial and temporal proximity between Hartley Springs Fault motion and the North Mono-Inyo eruption sequence suggests a possible relation between seismic events and eruptions. We investigate the interactions between slip along the Hartley Springs fault and <span class="hlt">dike</span> <span class="hlt">intrusion</span> beneath the Mono-Inyo craters using a three-dimensional finite element model of the Mono Basin. We employ a realistic representation of the Basin that includes topography, vertical and lateral heterogeneities of the crust, contact relations between fault planes, and a physical model of the pressure required to propagate the <span class="hlt">dike</span>. We estimate (a) the distribution of Coulomb stress changes to study the influence of <span class="hlt">dike</span> <span class="hlt">intrusion</span> on Hartley Springs fault, and (b) the local stress and volumetric dilatation changes to understand how fault slip may influence the propagation of a <span class="hlt">dike</span> towards the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720004690','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720004690"><span>Ethiopian Tertiary <span class="hlt">dike</span> swarms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mohr, P. A.</p> <p>1971-01-01</p> <p>Mapping of the Ethiopian rift and Afar margins revealed the existence of Tertiary <span class="hlt">dike</span> swarms. The structural relations of these swarms and the fed lava pile to monoclinal warping of the margins partly reflect a style of continental margin tectonics found in other parts of the world. In Ethiopia, however, conjugate <span class="hlt">dike</span> trends appear to be unusually strongly developed. Relation of <span class="hlt">dikes</span> to subsequent margin faulting is ambiguous, and there are instances where the two phenomena are spatially separate and of differing trends. There is no evidence for lateral migration with time of <span class="hlt">dike</span> injection toward the rift <span class="hlt">zone</span>. No separate impingement of Red Sea, Gulf of Aden, and African rift system stress fields on the Ethiopian region can be demonstrated from the Tertiary <span class="hlt">dike</span> swarms. Rather, a single, regional paleostress field existed, suggestive of a focus beneath the central Ethiopian plateau. This stress field was dominated by tension: there is no cogent evidence for shearing along the rift margins. A gentle compression along the rift floor is indicated. A peculiar sympathy of <span class="hlt">dike</span> hade directions at given localities is evident.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.V31D..08G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.V31D..08G"><span>Basaltic <span class="hlt">Dike</span> Propagation at Yucca Mountain, Nevada, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gaffney, E. S.; Damjanac, B.; Warpinski, N. R.</p> <p>2004-12-01</p> <p>We describe simulations of the propagation of basaltic <span class="hlt">dikes</span> using a 2-dimensional, incompressible hydrofracture code including the effects of the free surface with specific application to potential interactions of rising magma with a nuclear waste repository at Yucca Mountain, Nevada. As the leading edge of the <span class="hlt">dike</span> approaches the free surface, confinement at the crack tip is reduced and the tip accelerates relative to the magma front. In the absence of either excess confining stress or excess gas pressure in the tip cavity, this leads to an increase of crack-tip velocity by more than an order of magnitude. By casting the results in nondimensional form, they can be applied to a wide variety of <span class="hlt">intrusive</span> situations. When applied to an alkali basalt <span class="hlt">intrusion</span> at the proposed high-level nuclear waste repository at Yucca Mountain, the results provide for a description of the subsurface phenomena. For magma rising at 1 m/s and <span class="hlt">dikes</span> wider than about 0.5 m, the tip of the fissure would already have breached the surface by the time magma arrived at the nominal 300-m repository depth. An approximation of the effect of magma expansion on <span class="hlt">dike</span> propagation is used to show that removing the restriction of an incompressible magma would result in even greater crack-tip acceleration as the <span class="hlt">dike</span> approached the surface. A second analysis with a distinct element code indicates that a <span class="hlt">dike</span> could penetrate the repository even during the first 2000 years after closure during which time heating from radioactive decay of waste would raise the minimum horizontal compressive stress above the vertical stress for about 80 m above and below the repository horizon. Rather than sill formation, the analysis indicates that increased pressure and <span class="hlt">dike</span> width below the repository cause the crack tip to penetrate the horizon, but much more slowly than under in situ stress conditions. The analysis did not address the effects of either anisotropic joints or heat loss on this result.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70001085','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70001085"><span>The stress state near Spanish Peaks, colorado determined from a <span class="hlt">dike</span> pattern</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Muller, O.H.; Pollard, D.D.</p> <p>1977-01-01</p> <p>The radial pattern of syenite and syenodiorite <span class="hlt">dikes</span> of the Spanish Peaks region is analysed using theories of elasticity and <span class="hlt">dike</span> emplacement. The three basic components of Ode??'s model for the <span class="hlt">dike</span> pattern (a pressurized, circular hole; a rigid, planar boundary; and uniform regional stresses) are adopted, but modified to free the regional stresses from the constraint of being orthogonal to the rigid boundary. <span class="hlt">Dike</span> areal density, the White Peaks <span class="hlt">intrusion</span>, the strike of the upturned Mesozoic strata, and the contact between these strata and the intensely folded and faulted Paleozoic rocks are used to brient the rigid boundary along a north-south line. The line of <span class="hlt">dike</span> terminations locates the rigid boundary about 8 km west of West Peak. The location of a circular plug, Goemmer Butte, is chosen as a point of isotropic stress. A map correlating the location of isotropic stress points with regional stress parameters is derived from the theory and used to determine a regional stress orientation (N82E) and a normalized stress magnitude. The stress trajectory map constructed using these parameters mimics the <span class="hlt">dike</span> pattern exceptionally well. The model indicates that the regional principal stress difference was less than 0.05 times the driving pressure in the West Peak <span class="hlt">intrusion</span>. The regional stress difference probably did not exced 5 MN/m2. ?? 1977 Birkha??user Verlag.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JVGR..129..237L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JVGR..129..237L"><span>Internal structure of Puna Ridge: evolution of the submarine East Rift <span class="hlt">Zone</span> of Kilauea Volcano, Hawai ̀i</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leslie, Stephen C.; Moore, Gregory F.; Morgan, Julia K.</p> <p>2004-01-01</p> <p>Multichannel seismic reflection, sonobuoy, gravity and magnetics data collected over the submarine length of the 75 km long Puna Ridge, Hawai ̀i, resolve the internal structure of the active rift <span class="hlt">zone</span>. Laterally continuous reflections are imaged deep beneath the axis of the East Rift <span class="hlt">Zone</span> (ERZ) of Kilauea Volcano. We interpret these reflections as a layer of abyssal sediments lying beneath the volcanic edifice of Kilauea. Early arrival times or 'pull-up' of sediment reflections on time sections imply a region of high P-wave velocity ( Vp) along the submarine ERZ. Refraction measurements along the axis of the ridge yield Vp values of 2.7-4.85 km/s within the upper 1 km of the volcanic pile and 6.5-7 km/s deeper within the edifice. Few coherent reflections are observed on seismic reflection sections within the high-velocity area, suggesting steeply dipping <span class="hlt">dikes</span> and/or chaotic and fractured volcanic materials. Southeastward dipping reflections beneath the NW flank of Puna Ridge are interpreted as the buried flank of the older Hilo Ridge, indicating that these two ridges overlap at depth. Gravity measurements define a high-density anomaly coincident with the high-velocity region and support the existence of a complex of <span class="hlt">intrusive</span> <span class="hlt">dikes</span> associated with the ERZ. Gravity modeling shows that the <span class="hlt">intrusive</span> core of the ERZ is offset to the southeast of the topographic axis of the rift <span class="hlt">zone</span>, and that the surface of the core dips more steeply to the northwest than to the southeast, suggesting that the <span class="hlt">dike</span> complex has been progressively displaced to the southeast by subsequent <span class="hlt">intrusions</span>. The gravity signature of the <span class="hlt">dike</span> complex decreases in width down-rift, and is absent in the distal portion of the rift <span class="hlt">zone</span>. Based on these observations, and analysis of Puna Ridge bathymetry, we define three morphological and structural regimes of the submarine ERZ, that correlate to down-rift changes in rift <span class="hlt">zone</span> dynamics and partitioning of <span class="hlt">intrusive</span> materials. We propose that these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V51C..06H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V51C..06H"><span>The propagation direction of mafic radial <span class="hlt">dikes</span> inferred from flow-direction analysis of an exposed radial <span class="hlt">dike</span> sequence, Summer Coon Volcano, Colorado, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harp, A.; Valentine, G.</p> <p>2016-12-01</p> <p>Mafic eruptions along the flanks of stratovolcanoes pose significant hazards to life and property due to the uncertainty linked to new vent locations and their potentially close proximity to inhabited areas. Flank eruptions are often fed by radial <span class="hlt">dikes</span> with magma supplied either laterally from the central conduit or vertically from a deeper storage location. The highly eroded Oligocene age Summer Coon stratovolcano, Colorado reveals over 700 mafic <span class="hlt">dikes</span> surrounding a series of <span class="hlt">intrusive</span> stocks (inferred conduit). The exposure provides an opportunity to study radial <span class="hlt">dike</span> propagation directions and their relationship with the conduit in the lower portions of a volcanic edifice. Detailed geologic mapping and a geophysical survey revealed that little or no direct connection exists between the mafic radial <span class="hlt">dikes</span> and the inferred conduit at the current level of exposure. Oriented samples collected from the chilled margins of 29 mafic <span class="hlt">dikes</span> were analyzed for flow fabrics and emplacement directions. Among them, 20 <span class="hlt">dikes</span> show flow angles greater than 30 degrees from horizontal, and a single <span class="hlt">dike</span> had flow fabrics oriented at approximately 20 degrees. Of the <span class="hlt">dikes</span> with steeper fabrics nine <span class="hlt">dikes</span> were emplaced up and toward the volcano's center between 30-75 degrees from horizontal, and 11 <span class="hlt">dikes</span> emplaced up and away from the volcano's center between 35-60 degrees. The two groups of <span class="hlt">dikes</span> likely responded to the stress field within the edifice, where steepest-emplaced had relatively high magma overpressure and were focused toward the volcano's summit, while <span class="hlt">dikes</span> with lower overpressures propagated out toward the flanks. At Summer Coon, the lack of connection between mafic <span class="hlt">dikes</span> and the inferred conduit and presence of only one sub-horizontally emplaced <span class="hlt">dike</span> implies the stresses within lower edifice impeded lateral <span class="hlt">dike</span> nucleation and propagation while promoting and influencing the emplacement direction of upward propagating <span class="hlt">dikes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRB..123..264C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRB..123..264C"><span>Seismic Amplitude Ratio Analysis of the 2014-2015 Bár∂arbunga-Holuhraun <span class="hlt">Dike</span> Propagation and Eruption</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caudron, Corentin; White, Robert S.; Green, Robert G.; Woods, Jennifer; Ágústsdóttir, Thorbjörg; Donaldson, Clare; Greenfield, Tim; Rivalta, Eleonora; Brandsdóttir, Bryndís.</p> <p>2018-01-01</p> <p>Magma is transported in brittle rock through <span class="hlt">dikes</span> and sills. This movement may be accompanied by the release of seismic energy that can be tracked from the Earth's surface. Locating <span class="hlt">dikes</span> and deciphering their dynamics is therefore of prime importance in understanding and potentially forecasting volcanic eruptions. The Seismic Amplitude Ratio Analysis (SARA) method aims to track melt propagation using the amplitudes recorded across a seismic network without picking the arrival times of individual earthquake phases. This study validates this methodology by comparing SARA locations (filtered between 2 and 16 Hz) with the earthquake locations (same frequency band) recorded during the 2014-2015 Bár∂arbunga-Holuhraun <span class="hlt">dike</span> <span class="hlt">intrusion</span> and eruption in Iceland. Integrating both approaches also provides the opportunity to investigate the spatiotemporal characteristics of magma migration during the <span class="hlt">dike</span> <span class="hlt">intrusion</span> and ensuing eruption. During the <span class="hlt">intrusion</span> SARA locations correspond remarkably well to the locations of earthquakes. Several exceptions are, however, observed. (1) A low-frequency signal was possibly associated with a subglacial eruption on 23 August. (2) A systematic retreat of the seismicity was also observed to the back of each active segment during stalled phases and was associated with a larger spatial extent of the seismic energy source. This behavior may be controlled by the <span class="hlt">dike</span>'s shape and/or by <span class="hlt">dike</span> inflation. (3) During the eruption SARA locations consistently focused at the eruptive site. (4) Tremor-rich signal close to ice cauldrons occurred on 3 September. This study demonstrates the power of the SARA methodology, provided robust site amplification; Quality Factors and seismic velocities are available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/32574','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/32574"><span>Work <span class="hlt">zone</span> <span class="hlt">intrusion</span> alert technologies : assessment and practical guidance : final report.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>2017-06-01</p> <p>A work <span class="hlt">zone</span> <span class="hlt">intrusion</span> alert technology is a type of safety system that is used in a roadway work <span class="hlt">zone</span> to alert field workers and secure time for them to escape when errant vehicles intrude into the work <span class="hlt">zone</span>. Although such technologies have potential...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.8077G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.8077G"><span>The Freyenstein Shear <span class="hlt">Zone</span> - Implications for exhumation of the South Bohemian Batholith (Moldanubian Superunit, Strudengau, Austria)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Griesmeier, Gerit; Iglseder, Christoph; Konstantin, Petrakakis</p> <p>2016-04-01</p> <p>The Moldanubian superunit is part of the internal <span class="hlt">zone</span> of the Variscan Orogen in Europe and borders on the Saxothuringian and Sudetes <span class="hlt">zones</span> in the north. In the south, it is blanketed by the Alpine foreland molasse. Tectonically it is subdivided into the Moldanubian Nappes (MN), the South Bohemian Batholith (SBB) and the Bavarian Nappes. This work describes the ~ 500 m thick Freyenstein shear <span class="hlt">zone</span>, which is located at the southern border of the Bohemian Massif north and south of the Danube near Freyenstein (Strudengau, Lower Austria). The area is built up by granites of Weinsberg-type, which are interlayered by numerous <span class="hlt">dikes</span> and paragneisses of the Ostrong nappe system. These <span class="hlt">dikes</span> include medium grained granites and finegrained granites (Mauthausen-type granites), which form huge <span class="hlt">intrusions</span>. In addition, smaller <span class="hlt">intrusions</span> of dark, finegrained diorites und aplitic <span class="hlt">dikes</span> are observed. These rocks are affected by the Freyenstein shear <span class="hlt">zone</span> und ductily deformed. Highly deformed pegmatoides containing white mica crystals up to one cm cut through the deformed rocks and form the last <span class="hlt">dike</span> generation. The Freyenstein shear <span class="hlt">zone</span> is a NE-SW striking shear <span class="hlt">zone</span> at the eastern edge of the SBB. The mylonitic foliation is dipping to the SE with angles around 60°. Shear-sense criteria like clast geometries, SĆ structures as well as microstructures show normal faulting top to S/SW with steep (ca. 50°) angles. The Freyenstein shear <span class="hlt">zone</span> records a polyphase history of deformation and crystallization: In a first phase, mylonitized mineral assemblages in deformed granitoides can be observed, which consist of pre- to syntectonic muscovite-porphyroclasts and biotite as well as dynamically recrystallized potassium feldspar, plagioclase and quartz. The muscovite porphyroclasts often form mica fishes and show top to S/SW directed shear-sense. The lack of syntectonic chlorite crystals points to metamorphic conditions of lower amphibolite-facies > than 450° C. In a later stage fluid</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V31C0520P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V31C0520P"><span>Under-Pressured and Avoiding Interaction: How Magmatic Storage Regions Can Deflect <span class="hlt">Dikes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pansino, S.; Taisne, B.</p> <p>2017-12-01</p> <p>It has been shown through numerical techniques that ascending <span class="hlt">dikes</span> can be attracted to a pressurized magma storage region. This is due to the state of stresses around such a region, in which the minimum compressive stress is tangential to reservoir boundary and <span class="hlt">dikes</span> thereby prefer to propagate radially. We show that the reverse scenario has a reverse effect. A storage region that has under-pressurized, perhaps due to an eruption, rotates the stresses in the crust to deflect <span class="hlt">dikes</span> away; this inhibits interaction with the reservoir and favors other behaviors like <span class="hlt">intrusion</span> or monogenetic eruptions. We demonstrate through analogue experiments the ability for a <span class="hlt">dike</span> to avoid a magmatic reservoir, which depends in part on the internal pressure as well as on the initial <span class="hlt">dike</span> orientation. We show that <span class="hlt">dikes</span> have the potential to change orientation, curling and twisting to avoid the pressure sink, or to propagate preferentially at their sides, allowing them to slide away laterally.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033216','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033216"><span>Paleomagnetism of Proterozoic mafic <span class="hlt">dikes</span> from the Tobacco Root Mountains, southwest Montana</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Harlan, S.S.; Geissman, J. Wm; Snee, L.W.</p> <p>2008-01-01</p> <p>Paleomagnetic data from Proterozoic mafic <span class="hlt">dikes</span> in southwestern Montana provides evidence for two distinct episodes of subparallel <span class="hlt">dike</span> emplacement at ca. 1450 and 780 Ma. Published geochemical data from <span class="hlt">dikes</span> in the southern Tobacco Root Mountains has identified three distinct compositional groups, termed groups A, B, and C. Geochronological data from the group A <span class="hlt">dikes</span> yielded a Sm-Nd age of 1448 ?? 49 Ma. Emplacement of these <span class="hlt">dikes</span> is thought to reflect mafic magmatism associated with extension accompanying development of the adjacent Mesoproterozoic Belt Basin. Paleomagnetic results from these <span class="hlt">dikes</span> and a group C <span class="hlt">dike</span> yield antipodal magnetizations with a group-mean direction of D = 225.0??, I = 61.8?? (k = 27.9, ??95 = 7.7??, N = 14 independent means/24 sites). The average paleomagnetic pole (8.7??N, 216.1??E, A95 = 10.3??) is considered to be primary on the basis of positive baked contact tests and similarity to poles of ca. 1.45-1.4 Ga from <span class="hlt">intrusions</span> elsewhere in North America, but is discordant with respect to poles from age equivalent sedimentary rocks of the Meosoproterozoic Belt Supergroup. 40Ar/39Ar dates from geochemical group B <span class="hlt">dikes</span> are consistent with published U-Pb dates that demonstrate <span class="hlt">dike</span> emplacement at 780 Ma as part of the regional Gunbarrel magmatic event. Hornblende concentrates from the group B <span class="hlt">dikes</span> yield 40Ar/39Ar apparent ages of 778-772 Ma, whereas biotite from a baked contact <span class="hlt">zone</span> yielded a plateau date of 788 Ma. Paleomagnetic results from the group B <span class="hlt">dikes</span> yield a mean direction of D = 301.5??, I = -17.1?? (k = 65.7, ??95 = 4.0??, N = 12 independent means/23 sites) with a paleomagnetic pole at 14.6??N, 127.0??E (A95 = 3.2??). The combination of geochronologic data, results of a baked contact test, and spatial agreement of the paleomagnetic poles with poles of similar age elsewhere in North America indicates that this is also a primary magnetization associated with <span class="hlt">dike</span> emplacement. Paleomagnetic data from some of the Tobacco Root</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020343','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020343"><span>Influence of an igneous <span class="hlt">intrusion</span> on the inorganic geochemistry of a bituminous coal from Pitkin County, Colorado</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Finkelman, R.B.; Bostick, N.H.; Dulong, F.T.; Senftle, F.E.; Thorpe, A.N.</p> <p>1998-01-01</p> <p>Although the effects of igneous <span class="hlt">dikes</span> on the organic matter in coal have been observed at many localities there is virtually no information on the effects of the <span class="hlt">intrusions</span> of the inorganic constituents in the coal. Such a study may help to elucidate the behavior of trace elements during in situ gasification of coal and may provide insights into the resources potential for coal and coke affected by the <span class="hlt">intrusion</span>. To determine the effects of an igneous <span class="hlt">intrusion</span> on the inorganic chemistry of a coal we used a series of 11 samples of coal and natural coke that had been collected at intervals from 3 to 106 cm from a <span class="hlt">dike</span> that intruded the bituminous Dutch Creek coal in Pitkin, CO. The samples were chemically analyzed for 66 elements. SEM-EDX and X-ray diffraction analysis were performed on selected samples. Volatile elements such as F, Cl, Hg, and Se are not depleted in the samples (coke and coal) nearest the <span class="hlt">dike</span> that were exposed to the highest temperatures. Their presence in these samples is likely due to secondary enrichment following volatilization of the elements inherent in the coal. Equilibration with ground water may account for the uniform distribution of Na, B, and Cl. High concentrations of Ca, Mg, Fe, Mn, Sr, and CO2 in the coke region are attributed to the reaction of CO and CO2 generated during the coking of the coal with fluids from the <span class="hlt">intrusion</span>, resulting in the precipitation of carbonates. Similarly, precipitation of sulfide minerals in the coke <span class="hlt">zone</span> may account for the relatively high concentrations of Ag, Hg, Cu, Zn, and Fe. Most elements are concentrated at the juncture of the fluidized coke and the thermally metamorphosed coal. Many of the elements enriched in this region (for example, Ga, Ge, Mo, Rb, U, La, Ce, Al, K, and Si) may have been adsorbed on either the clays or the organic matter or on both.Although the effects of igneous <span class="hlt">dikes</span> on the organic matter in coal have been observed at many localities there is virtually no information on the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JVGR..150..213M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JVGR..150..213M"><span>Time dependent model of magma <span class="hlt">intrusion</span> in and around Miyake and Kozu Islands, Central Japan in June August, 2000</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murase, Masayuki; Irwan, Meilano; Kariya, Shinichi; Tabei, Takao; Okuda, Takashi; Miyajima, Rikio; Oikawa, Jun; Watanabe, Hidefumi; Kato, Teruyuki; Nakao, Shigeru; Ukawa, Motoo; Fujita, Eisuke; Okayama, Muneo; Kimata, Fumiaki; Fujii, Naoyuki</p> <p>2006-02-01</p> <p>A time-dependent model of magma <span class="hlt">intrusion</span> is presented for the Miyake-Kozu Island area in central Japan based on global positioning system (GPS) measurements at 28 sites recorded between June 27 and August 27, 2000. A model derived from a precise hypocenter distribution map indicates the presence of three <span class="hlt">dikes</span> between Miyake and Kozu Islands. Other <span class="hlt">dike</span> <span class="hlt">intrusion</span> models, including a <span class="hlt">dike</span> with aseismic creep and a <span class="hlt">dike</span> associated with a deep deflation source are also discussed. The optimal parameters for each model are estimated using a genetic algorithm (GA) approach. Using Akaike's information criteria (AIC), the three-<span class="hlt">dike</span> model is shown to provide the best solution for the observed deformation. Volume changes in spherical inflation and deflation sources, as well as three <span class="hlt">dikes</span>, are calculated for seven discretized periods after GA optimization of the <span class="hlt">dike</span> geometry. The optimization suggests a concentration of <span class="hlt">dike</span> expansion near Miyake Island in the period from June 27 to July 1 associated with large deflation at a depth of about 7 km below Miyake volcano, indicating magma supply from depth below Miyake Island. In the period from July 9 to August 10, a huge <span class="hlt">dike</span> <span class="hlt">intrusion</span> near Kozu Island is inferred, accompanied by expansion of the lower parts of a central <span class="hlt">dike</span>, suggesting magma supply from depth in the region between Miyake and Kozu Islands.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_3 --> <div id="page_4" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="61"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29326978','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29326978"><span>Seismic signature of active <span class="hlt">intrusions</span> in mountain chains.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Di Luccio, Francesca; Chiodini, Giovanni; Caliro, Stefano; Cardellini, Carlo; Convertito, Vincenzo; Pino, Nicola Alessandro; Tolomei, Cristiano; Ventura, Guido</p> <p>2018-01-01</p> <p><span class="hlt">Intrusions</span> are a ubiquitous component of mountain chains and testify to the emplacement of magma at depth. Understanding the emplacement and growth mechanisms of <span class="hlt">intrusions</span>, such as diapiric or <span class="hlt">dike</span>-like ascent, is critical to constrain the evolution and structure of the crust. Petrological and geological data allow us to reconstruct magma pathways and long-term magma differentiation and assembly processes. However, our ability to detect and reconstruct the short-term dynamics related to active <span class="hlt">intrusive</span> episodes in mountain chains is embryonic, lacking recognized geophysical signals. We analyze an anomalously deep seismic sequence (maximum magnitude 5) characterized by low-frequency bursts of earthquakes that occurred in 2013 in the Apennine chain in Italy. We provide seismic evidences of fluid involvement in the earthquake nucleation process and identify a thermal anomaly in aquifers where CO 2 of magmatic origin dissolves. We show that the <span class="hlt">intrusion</span> of <span class="hlt">dike</span>-like bodies in mountain chains may trigger earthquakes with magnitudes that may be relevant to seismic hazard assessment. These findings provide a new perspective on the emplacement mechanisms of <span class="hlt">intrusive</span> bodies and the interpretation of the seismicity in mountain chains.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5756663','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5756663"><span>Seismic signature of active <span class="hlt">intrusions</span> in mountain chains</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Di Luccio, Francesca; Chiodini, Giovanni; Caliro, Stefano; Cardellini, Carlo; Convertito, Vincenzo; Pino, Nicola Alessandro; Tolomei, Cristiano; Ventura, Guido</p> <p>2018-01-01</p> <p><span class="hlt">Intrusions</span> are a ubiquitous component of mountain chains and testify to the emplacement of magma at depth. Understanding the emplacement and growth mechanisms of <span class="hlt">intrusions</span>, such as diapiric or <span class="hlt">dike</span>-like ascent, is critical to constrain the evolution and structure of the crust. Petrological and geological data allow us to reconstruct magma pathways and long-term magma differentiation and assembly processes. However, our ability to detect and reconstruct the short-term dynamics related to active <span class="hlt">intrusive</span> episodes in mountain chains is embryonic, lacking recognized geophysical signals. We analyze an anomalously deep seismic sequence (maximum magnitude 5) characterized by low-frequency bursts of earthquakes that occurred in 2013 in the Apennine chain in Italy. We provide seismic evidences of fluid involvement in the earthquake nucleation process and identify a thermal anomaly in aquifers where CO2 of magmatic origin dissolves. We show that the <span class="hlt">intrusion</span> of <span class="hlt">dike</span>-like bodies in mountain chains may trigger earthquakes with magnitudes that may be relevant to seismic hazard assessment. These findings provide a new perspective on the emplacement mechanisms of <span class="hlt">intrusive</span> bodies and the interpretation of the seismicity in mountain chains. PMID:29326978</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189102','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189102"><span>What lies beneath: geophysical mapping of a concealed Precambrian <span class="hlt">intrusive</span> complex along the Iowa–Minnesota border</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Drenth, Benjamin J.; Anderson, Raymond R.; Schulz, Klaus J.; Feinberg, Joshua M.; Chandler, Val W.; Cannon, William F.</p> <p>2015-01-01</p> <p> much of the NEIIC is composed of such complexes, and broadly speaking, may be a discontinuous group of several <span class="hlt">intrusive</span> bodies. Most units are cut by suspected northwest-trending faults imaged as magnetic lineaments, and one produces apparent sinistral fault separation of a <span class="hlt">dike</span> in the eastern part of the survey area. The location, trend, and apparent sinistral sense of motion are consistent with the suspected faults being part of the Belle Plaine fault <span class="hlt">zone</span>, a complex transform fault <span class="hlt">zone</span> within the Midcontinent rift system that is here proposed to correspond with a major structural discontinuity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.G51A0064M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.G51A0064M"><span>Time Dependent Model of Magma <span class="hlt">Intrusion</span> in and around Miyake and Kozu Islands, Central Japan in June-August, 2000</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Murase, M.; Irwan, M.; Kariya, S.; Tabei, T.; Okuda, T.; Miyajima, R.; Kimata, F.; Fujii, N.</p> <p>2004-12-01</p> <p>We discuss a time dependent model of magma <span class="hlt">intrusion</span> in and around Miyake and Kozu Islands, Central Japan from GPS measurements at 28 sites in Miyake Island, Kozu Island and their surrounding islands in the period from June 27 to August 27, 2000. A <span class="hlt">dike</span> complex model of three sheets is assumed between Miyake and Kozu Islands, suggested from the precise hypocenter distribution map (Sakai et al., 2003). Other <span class="hlt">dike</span> <span class="hlt">intrusion</span> models, a <span class="hlt">dike</span> with an aseismic creep model (Nishimura et al.,2001; Furuya et al.,2003) and a <span class="hlt">dike</span> with a deep deflation source model (Yamaoka et al., submitted) , are also discussed. Akaike's Information Criteria (AIC) value of optimal parameters of a <span class="hlt">dike</span> complex model indicates lower than that of other two models. After fixing the geometry of three <span class="hlt">dikes</span> using a genetic algorithm (GA), the amounts of <span class="hlt">dike</span> openings of top, inside, and bottom of each <span class="hlt">dike</span> are estimated by GA for seven time periods. In the period from June 27 to July 8, <span class="hlt">dike</span> opening is concentrated in the <span class="hlt">dike</span> near Miyake Island, and a large deflation is also estimated at a depth of 5 km of Miyake Volcano. It suggests that magma is supplied from the depths of Miyake Island. In next period until August 10, a huge <span class="hlt">dike</span> <span class="hlt">intrusion</span> is characterized in the <span class="hlt">dike</span> near Kozu Island and the lower parts of <span class="hlt">dike</span> in central and near Miyake Island. This suggests that magma is supplied from depth between Miyake and Kozu Islands. In the period of August 10 to 27, a huge deflation is estimated at a depth of 10 km under Miyake Volcano, and <span class="hlt">dike</span> opening is limited</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033565','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033565"><span>A model for radial <span class="hlt">dike</span> emplacement in composite cones based on observations from Summer Coon volcano, Colorado, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Poland, Michael P.; Moats, W.P.; Fink, J.H.</p> <p>2008-01-01</p> <p>We mapped the geometry of 13 silicic <span class="hlt">dikes</span> at Summer Coon, an eroded Oligocene stratovolcano in southern Colorado, to investigate various characteristics of radial <span class="hlt">dike</span> emplacement in composite volcanoes. Exposed <span class="hlt">dikes</span> are up to about 7 km in length and have numerous offset segments along their upper peripheries. Surprisingly, most <span class="hlt">dikes</span> at Summer Coon increase in thickness with distance from the center of the volcano. Magma pressure in a <span class="hlt">dike</span> is expected to lessen away from the pressurized source region, which would encourage a blade-like <span class="hlt">dike</span> to decrease in thickness with distance from the center of the volcano. We attribute the observed thickness pattern as evidence of a driving pressure gradient, which is caused by decreasing host rock shear modulus and horizontal stress, both due to decreasing emplacement depths beneath the sloping flanks of the volcano. Based on data from Summer Coon, we propose that radial <span class="hlt">dikes</span> originate at depth below the summit of a host volcano and follow steeply inclined paths towards the surface. Near the interface between volcanic cone and basement, which may represent a neutral buoyancy surface or stress barrier, magma is transported subhorizontally and radially away from the center of the volcano in blade-like <span class="hlt">dikes</span>. The <span class="hlt">dikes</span> thicken with increasing radial distance, and offset segments and fingers form along the upper peripheries of the <span class="hlt">intrusions</span>. Eruptions may occur anywhere along the length of the <span class="hlt">dikes</span>, but the erupted volume will generally be greater for <span class="hlt">dike</span>-fed eruptions far from the center of the host volcano owing to the increase in driving pressure with distance from the source. Observed eruptive volumes, vent locations, and vent-area <span class="hlt">intrusions</span> from inferred post-glacial <span class="hlt">dike</span>-fed eruptions at Mount Adams, Washington, USA, support the proposed model. Hazards associated with radial <span class="hlt">dike</span> emplacement are therefore greater for longer <span class="hlt">dikes</span> that propagate to the outer flanks of a volcano. ?? Springer-Verlag 2007.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V33C2383W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V33C2383W"><span>Constraints on the Geometries and Compositions of Subvolcanic Conduits from <span class="hlt">Intrusions</span> of the San Rafael Swell, Utah</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wetmore, P. H.; Connor, C.; Wilson, J.</p> <p>2010-12-01</p> <p>Conduit models incorporate varying degrees of complexity (or parsimony) and account for the transport properties of magmas, steady-state or transient behavior, and conduit geometry (e.g., 1- to 1.5 D, variable width and erodable conduit walls). Improvement of these models is important if we are to work toward deployment of eruption models at active volcanoes, link these models to geophysical observations (seismic, deformation, gravity) and eventually forecast eruption magnitude. One conclusion of a recent comparison of many conduit models (Sahagian, 2005 JVGR) is that next generation models need to better account for interaction of the erupting mixture with surrounding wall rocks (accounting for melting, solidification, and erosion) and better account for the effects of conduit shape on flows. In an effort to address these issues our research group has completed mapping of a suite of subvolcanic <span class="hlt">intrusions</span> (<span class="hlt">dikes</span>, sills, and conduits) from the west-central San Rafael Swell of central Utah. The results of this study demonstrate that vertical flow of melt through crust in this system of <span class="hlt">intrusion</span> was dominated by <span class="hlt">dikes</span>. Conduits form, in nearly all cases, as a result of localized flow along <span class="hlt">dikes</span>. The conduits are commonly comprised of three distinct lithologic units: brecciated host rock (without any <span class="hlt">intrusive</span> material), brecciated host rock mixed with brecciated and mechanically contaminated <span class="hlt">intrusive</span>, and relatively clean (i.e. containing less than ~10% accidental material) <span class="hlt">intrusive</span>. Contacts between all three of these units are typically discreet and traceable for several tens of meters. In some examples clasts within the unmixed breccia unit exhibit a strong alignment of clasts dipping into the core of the conduit. These observations suggests an evolutionary history that involves an early phase of brecciation and mixing, followed by confined flow with a fluidized mixed unit and an essentially uninvolved outer <span class="hlt">zone</span> (i.e. the breccia). The final phase likely</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGP51A0786H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGP51A0786H"><span>Tectonic implications of a paleomagnetic direction obtained from a Miocene <span class="hlt">dike</span> swarm in central Honshu, Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoshi, H.; Sugisaki, Y.</p> <p>2017-12-01</p> <p>Central Honshu of Japan is an ideal field for the study of crustal deformation related to arc-arc collision. In this study we obtained rock magnetic and paleomagnetic results from early Miocene igneous rocks in central Honshu in order to examine rotational deformation caused by the collision of the Izu-Bonin-Mariana (IBM) arc with central Honshu. In Takane of the Hida region, gabbro <span class="hlt">intrusions</span> and older sedimentary rocks are intruded by numerous andesitic <span class="hlt">dikes</span> that comprise a parallel <span class="hlt">dike</span> swarm. The <span class="hlt">dikes</span> formed under two different normal-faulting paleostress conditions, which were suggested using a method of clustering <span class="hlt">dike</span> orientations. Cross-cutting relationships indicate that the two paleostress conditions existed during the same period. More than 240 oriented cores were taken at 38 sites in two localities for magnetic study. The andesites and gabbros generally have magnetite, and some andesites also contain pyrrhotite. The magnetite records easterly deflected remanent magnetization directions of dual polarities that pass the reversals test. Positive baked contact tests at two sites demonstrate that the easterly deflected direction is a thermoremanent magnetization acquired at the time of <span class="hlt">intrusion</span>. The overall in situ (i.e., in geographic coordinates) mean direction for andesitic <span class="hlt">dikes</span> is judged to be highly reliable, although there are two possible scenarios for explaining the easterly deflection: (1) clockwise rotation and (2) tilting to the northwest. We prefer the former scenario and conclude that 45° clockwise rotation occurred in Takane with respect to the North China Block of the Asian continent. This rotation must represent the clockwise rotation of entire Southwest Japan during the opening period of the Japan Sea. Very little difference is observed between the amount of the easterly deflection in Takane and those in the Tokai and Hokuriku regions, indicating no significant relative rotation. Thus, the crust beneath Takane has not suffered rotation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.V14A..01L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.V14A..01L"><span>Layered <span class="hlt">intrusion</span> formation by top down thermal migration <span class="hlt">zone</span> refining (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lundstrom, C.</p> <p>2009-12-01</p> <p>The formation of layered mafic <span class="hlt">intrusions</span> by crystallization from cooling magmas represents the textbook example of igneous differentiation, often attributed to fractional crystallization through gravitational settling. Yet in detail, such interpretations have significant problems such that it remains unclear how these important features form. Put in the Earth perspective that no km scale blob of >50% melt has ever been imaged geophysically and that geochronological studies repeatedly indicate age inconsistencies with “big tank” magma chambers, it may be questioned if km scale magma chambers have ever existed. I will present the case for forming layered <span class="hlt">intrusions</span> by a top down process whereby arriving basaltic magma reaches a permeability barrier, begins to underplate and forms the <span class="hlt">intrusion</span> incrementally by sill injection with the body growing downward at ~1 mm/yr rate or less. A temperature gradient <span class="hlt">zone</span> occurs in the overlying previously emplaced sills, leading to chemical components migrating by diffusion. As long as the rate of diffusion can keep up with rate of sill addition, the body will differentiate along a path similar to a liquid line of descent. In this talk, I will integrate data from 3 areas: 1) laboratory experiments examining the behavior of partially molten silicates in a temperature gradient (thermal migration); 2) numerical modeling of the moving temperature gradient <span class="hlt">zone</span> process using IRIDIUM (Boudreau, 2003); 3) measurements of Fe isotope ratios and geochronology from the Sonju Lake <span class="hlt">Intrusion</span> in the Duluth Complex. This model provides the ability to form km scale <span class="hlt">intrusions</span> by a seismically invisible means, can explain million year offsets in chronology, and has implications for reef development and PGE concentration. Most importantly, this model of top down layered <span class="hlt">intrusion</span> formation, following a similar recent proposal for granitoid formation (Lundstrom, 2009), represents a testable hypothesis: because temperature gradient driven</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51D0510S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51D0510S"><span>Igneous Sheet <span class="hlt">Intrusions</span> as a Record of Paleostress States</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stephens, T. L.; Walker, R. J.; Healy, D.; Bubeck, A.; England, R. W.; McCaffrey, K. J. W.</p> <p>2017-12-01</p> <p>The architecture of igneous sheet <span class="hlt">intrusion</span> networks provides useful constraints on paleostress during emplacement. Several models for sill emplacement have used the close spatial relationships between sills and <span class="hlt">dikes</span> in layered (sedimentary) host rocks to propose that <span class="hlt">dike</span>-sill transitions are driven by layering. Such models require a stress rotation - from horizontal extension for <span class="hlt">dikes</span>, to horizontal compression for sills - which is assumed to reflect a near-hydrostatic stress state, facilitating the dilation and <span class="hlt">intrusion</span> of pre-existing structures (e.g. faults, joints, and bedding). Here, we present case examples of sills for which layering is not the main control on emplacement: Isle of Mull (UK), Faroe Islands (European Atlantic margin) and the San Rafael Subvolcanic Field (Utah, USA). In each case, <span class="hlt">dikes</span> cut, or are cut by, sills; indicating that <span class="hlt">dikes</span> were not the feeders to sills in the same section. The sills consist of linked, flat and shallowly-dipping segments that always show near-vertical opening directions. Sills cut bedding and formation contacts with consistent low-angle dips, and cut or abut against vertical faults, fractures, and tectonic foliations. From this, we infer that magma pressure during emplacement did not exceed the horizontal stress. To constrain the stress state during emplacement we present a novel approach that combines analysis of local and overall sill geometry data with mechanical models for slip tendency, dilation tendency, and fracture susceptibility. We also present a new depth-independent mechanical model, which estimates paleostress ratio and driving fluid pressure ratio using the opening angles of dilated fluid-filled fractures. Our results show that the studied sills record previously unrecognised local fluctuations in the far-field stress state, during magmatic supply. Sills, therefore, present an important tool for determining paleostress in areas where few brittle deformation structures (e.g. faults), other than</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V53A1139S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V53A1139S"><span>Source Models of the June 17th, 2007 Kilauea <span class="hlt">Intrusion</span>: Monte Carlo Optimization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sinnett, D. K.; Montgomery-Brown, E. D.; Segall, P.; Miklius, A.; Poland, M.; Yun, S.; Zebker, H.</p> <p>2007-12-01</p> <p>Father's Day, 17 June 2007, marked the beginning of the 56th episode of the ongoing eruption of Kilauea volcano, Hawaii. The episode culminated in a short-lived eruption approximately 6 km west of Pu\\`{}u \\`{}O\\`{}o and 13 km southeast of Kilauea summit. The interruption of magma supply to, and withdrawal from, the reservoir beneath Pu\\`{}u \\`{}O\\`{}o caused cessation of activity and ~100 m of crater floor subsidence there. The continuous and campaign GPS, electronic tiltmeter, and seismic networks, as well as InSAR captured the episode in fine detail. Visual inspection of the data show subsidence at Kilauea summit and Pu\\`{}u \\`{}O\\`{}o, which fed the inflating <span class="hlt">dike</span>. We began by modeling the <span class="hlt">intrusion</span> with a Mogi source beneath Kilauea summit and a dislocation with uniform opening beneath the east rift <span class="hlt">zone</span> embedded in an isotropic, homogenous, elastic, half space. We invert for the 12 source parameters (length, width, depth, dip, strike, horizontal position, and opening of the <span class="hlt">dike</span>, and position, depth, and volume change of the Mogi source) using Monte Carlo optimization. The inversion used three component displacement data from 23 continuous and campaign GPS stations, diurnally and tidally filtered tilt from 6 stations, and an ENVISAT InSAR interferogram spanning 04/12/07 to 06/21/07 decimated using a quadtree algorithm. The optimum model included ~-4.1 * 106 m3 of volume loss from a reservoir 3 km beneath the summit, and a total <span class="hlt">dike</span> volume of ~19*106 m3 (~4.84 km length x 2.45 km width x 1.6 m opening at 2.4 km depth). The discrepancy between summit volume loss and total <span class="hlt">dike</span> volume suggests that other sources must have fed the <span class="hlt">dike</span>. A crude estimate of volume loss from Pu\\`{}u \\`{}O\\`{}o is 8.5*106 m3 accounting for ~ 66% of the volume of the <span class="hlt">dike</span>. The eruption site lies inside the eastern edge of the model, and ~0.5 km to the south of the best fit <span class="hlt">dike</span> top. The best fit <span class="hlt">dike</span> top parallels the northern margin of an area of ground cracking near</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030111250&hterms=swarm&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dswarm','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030111250&hterms=swarm&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dswarm"><span>Magma Reservoirs Feeding Giant Radiating <span class="hlt">Dike</span> Swarms: Insights from Venus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Grosfils, E. B.; Ernst, R. E.</p> <p>2003-01-01</p> <p>Evidence of lateral <span class="hlt">dike</span> propagation from shallow magma reservoirs is quite common on the terrestrial planets, and examination of the giant radiating <span class="hlt">dike</span> swarm population on Venus continues to provide new insight into the way these complex magmatic systems form and evolve. For example, it is becoming clear that many swarms are an amalgamation of multiple discrete phases of <span class="hlt">dike</span> <span class="hlt">intrusion</span>. This is not surprising in and of itself, as on Earth there is clear evidence that formation of both magma reservoirs and individual giant radiating <span class="hlt">dikes</span> often involves periodic magma injection. Similarly, giant radiating swarms on Earth can contain temporally discrete subswarms defined on the basis of geometry, crosscutting relationships, and geochemical or paleomagnetic signatures. The Venus data are important, however, because erosion, sedimentation, plate tectonic disruption, etc. on Earth have destroyed most giant radiating <span class="hlt">dike</span> swarm's source regions, and thus we remain uncertain about the geometry and temporal evolution of the magma sources from which the <span class="hlt">dikes</span> are fed. Are the reservoirs which feed the <span class="hlt">dikes</span> large or small, and what are the implications for how the <span class="hlt">dikes</span> themselves form? Does each subswarm originate from a single, periodically reactivated reservoir, or do subswarms emerge from multiple discrete geographic foci? If the latter, are these discrete foci located at the margins of a single large magma body, or do multiple smaller reservoirs define the character of the magmatic center as a whole? Similarly, does the locus of magmatic activity change with time, or are all the foci active simultaneously? Careful study of giant radiating <span class="hlt">dike</span> swarms on Venus is yielding the data necessary to address these questions and constrain future modeling efforts. Here, using giant radiating <span class="hlt">dike</span> swarms from the Nemesis Tessera (V14) and Carson (V43) quadrangles as examples, we illustrate some of the <span class="hlt">dike</span> swarm focal region diversity observed on Venus and briefly explore some</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tecto..36.3298E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tecto..36.3298E"><span>Crustal Structure of Active Deformation <span class="hlt">Zones</span> in Africa: Implications for Global Crustal Processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ebinger, C. J.; Keir, D.; Bastow, I. D.; Whaler, K.; Hammond, J. O. S.; Ayele, A.; Miller, M. S.; Tiberi, C.; Hautot, S.</p> <p>2017-12-01</p> <p>The Cenozoic East African rift (EAR), Cameroon Volcanic Line (CVL), and Atlas Mountains formed on the slow-moving African continent, which last experienced orogeny during the Pan-African. We synthesize primarily geophysical data to evaluate the role of magmatism in shaping Africa's crust. In young magmatic rift <span class="hlt">zones</span>, melt and volatiles migrate from the asthenosphere to gas-rich magma reservoirs at the Moho, altering crustal composition and reducing strength. Within the southernmost Eastern rift, the crust comprises 20% new magmatic material ponded in the lower crust and intruded as sills and <span class="hlt">dikes</span> at shallower depths. In the Main Ethiopian Rift, <span class="hlt">intrusions</span> comprise 30% of the crust below axial <span class="hlt">zones</span> of <span class="hlt">dike</span>-dominated extension. In the incipient rupture <span class="hlt">zones</span> of the Afar rift, magma <span class="hlt">intrusions</span> fed from crustal magma chambers beneath segment centers create new columns of mafic crust, as along slow-spreading ridges. Our comparisons suggest that transitional crust, including seaward dipping sequences, is created as progressively smaller screens of continental crust are heated and weakened by magma <span class="hlt">intrusion</span> into 15-20 km thick crust. In the 30 Ma Recent CVL, which lacks a hot spot age progression, extensional forces are small, inhibiting the creation and rise of magma into the crust. In the Atlas orogen, localized magmatism follows the strike of the Atlas Mountains from the Canary Islands hot spot toward the Alboran Sea. CVL and Atlas magmatism has had minimal impact on crustal structure. Our syntheses show that magma and volatiles are migrating from the asthenosphere through the plates, modifying rheology, and contributing significantly to global carbon and water fluxes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JVGR..254...80J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JVGR..254...80J"><span>A hybrid composite <span class="hlt">dike</span> suite from the northern Arabian Nubian Shield, southwest Jordan: Implications for magma mixing and partial melting of granite by mafic magma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jarrar, Ghaleb H.; Yaseen, Najel; Theye, Thomas</p> <p>2013-03-01</p> <p>The Arabian Nubian Shield is an exemplary juvenile continental crust of Neoproterozoic age (1000-542 Ma). The post-collisional rift-related stage (~ 610 to 542 Ma) of its formation is characterized among others by the <span class="hlt">intrusion</span> of several generations of simple and composite <span class="hlt">dikes</span>. This study documents a suite of hybrid composite <span class="hlt">dikes</span> and a natural example of partial melting of granite by a mafic magma from the northernmost extremity of Arabian Nubian Shield in southwest Jordan. The petrogenesis of this suite is discussed on the basis of field, petrographic, geochemical, and Rb/Sr isotopic data. These <span class="hlt">dikes</span> give spectacular examples of the interaction between basaltic magma and the granitic basement. This interaction ranges from brecciation, partial melting of the host alkali feldspar granite to complete assimilation of the granitic material. Field structures range from <span class="hlt">intrusive</span> breccia (angular partially melted granitic fragments in a mafic groundmass) to the formation of hybrid composite <span class="hlt">dikes</span> that are up to 14 m in thickness. The rims of these <span class="hlt">dikes</span> are trachyandesite (latite) with alkali feldspar ovoids (up to 1 cm in diameter); while the central cores are trachydacite to dacite and again with alkali feldspar ovoids and xenoliths from the <span class="hlt">dike</span> rims. The granitic xenoliths in the <span class="hlt">intrusive</span> breccia have been subjected to at least 33% partial melting. A seven-point Rb/Sr isochron from one of these composite <span class="hlt">dikes</span> yields an age of 561 ± 33 Ma and an initial 87Sr/86Sr ratio of 0.70326 ± 0.0003 (2σ) and MSWD of 0.62. Geochemical modeling using major, trace, rare earth elements and isotopes suggests the generation of the hybrid composite <span class="hlt">dike</span> suite through the assimilation of 30% to 60% granitic crustal material by a basaltic magma, while the latter was undergoing fractional crystallization at different levels in the continental crust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V23A0681H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V23A0681H"><span>Petrologic Consequences of the Magmatic Death of a Continental Arc: Vanda <span class="hlt">Dike</span> Swarm, Dry Valleys, Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harpp, K. S.; Christensen, B. C.; Geist, D. J.; Garcia, M. O.</p> <p>2005-12-01</p> <p>The Dry Valleys of southern Victoria Land, Antarctica, are notable for the presence of the Vanda <span class="hlt">dikes</span>, prominent NE-trending swarms that crosscut a sequence of granitoid plutons. These older plutons are regional in extent and comprise 3 Cambro-Ordovician groups, including: a) calc-alkaline granitoids formed at an active plate margin during the Ross Orogeny (c. 505 Ma); b) adakitic granitoids, likely marking the conclusion of Ross Orogeny subduction-related activity (c. 490 Ma); and c) younger monzonitic plutons, probably generated in an intraplate extensional setting (Cox et al., 2000). The Vanda <span class="hlt">dikes</span> crosscut the younger plutons, possibly between c. 490 and 477 Ma (Allibone et al., 1993; Encarnacion and Grunow, 1996). <span class="hlt">Dikes</span> from the east wall of Bull Pass and the south wall of the Wright Valley range from 0.5-25 m wide with nearly vertical dips, are usually several km long, and, in the center of the swarms, occur with a frequency of ~18 <span class="hlt">dikes</span>/km. Most have chilled margins and are surrounded by brittle fractures, indicative of shallow <span class="hlt">intrusion</span> into cold country rock. <span class="hlt">Dike</span> compositions are bimodal, most defining a trend at the boundary between the high-K calc-alkaline and shoshonite series in SiO2-K2O space; some Wright Valley <span class="hlt">dikes</span> have slightly lower K2O and are calc-alkaline. Granite porphyry <span class="hlt">dikes</span> are relatively homogeneous (69-73 wt.% SiO2), whereas the mafic <span class="hlt">dikes</span> exhibit a wider range of compositions (49-57 wt.% SiO2). The felsic and mafic <span class="hlt">dikes</span> have distinct trace element abundances but similar normalized distribution patterns, including fractionated heavy rare earth elements and negative Eu and high field-strength element anomalies. Average Sr/Y ratios of both the felsic and mafic <span class="hlt">dikes</span> cluster around 20, well below a typical adakite signature. Major and trace element variations suggest that the felsic <span class="hlt">dikes</span> may be differentiates of the mafic magmas. Field relations further indicate that the felsic lavas may represent, on average, a later phase of <span class="hlt">dike</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70177883','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70177883"><span>Monogenetic volcanoes fed by interconnected <span class="hlt">dikes</span> and sills in the Hopi Buttes volcanic field, Navajo Nation, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Muirhead, James D.; Van Eaton, Alexa R.; Re, Giuseppe; White, James D. L.; Ort, Michael H.</p> <p>2016-01-01</p> <p>Although monogenetic volcanic fields pose hazards to major cities worldwide, their shallow magma feeders (<500 m depth) are rarely exposed and, therefore, poorly understood. Here, we investigate exposures of <span class="hlt">dikes</span> and sills in the Hopi Buttes volcanic field, Arizona, to shed light on the nature of its magma feeder system. Shallow exposures reveal a transition <span class="hlt">zone</span> between <span class="hlt">intrusion</span> and eruption within 350 m of the syn-eruptive surface. Using a combination of field- and satellite-based observations, we have identified three types of shallow magma systems: (1) <span class="hlt">dike</span>-dominated, (2) sill-dominated, and (3) interconnected <span class="hlt">dike</span>-sill networks. Analysis of vent alignments using the pyroclastic massifs and other eruptive centers (e.g., maar-diatremes) shows a NW-SE trend, parallel to that of <span class="hlt">dikes</span> in the region. We therefore infer that <span class="hlt">dikes</span> fed many of the eruptions. <span class="hlt">Dikes</span> are also observed in places transforming to transgressive (ramping) sills. Estimates of the observable volume of <span class="hlt">dikes</span> (maximum volume of 1.90 × 106 m3) and sills (minimum volume of 8.47 × 105 m3) in this study reveal that sills at Hopi Buttes make up at least 30 % of the shallow intruded volume (∼2.75 × 106 m3 total) within 350 m of the paeosurface. We have also identified saucer-shaped sills, which are not traditionally associated with monogenetic volcanic fields. Our study demonstrates that shallow feeders in monogenetic fields can form geometrically complex networks, particularly those intruding poorly consolidated sedimentary rocks. We conclude that the Hopi Buttes eruptions were primarily fed by NW-SE-striking <span class="hlt">dikes</span>. However, saucer-shaped sills also played an important role in modulating eruptions by transporting magma toward and away from eruptive conduits. Sill development could have been accompanied by surface uplifts on the order of decimeters. We infer that the characteristic feeder systems described here for the Hopi Buttes may underlie monogenetic fields elsewhere</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoJI.205.1244A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoJI.205.1244A"><span>Seafloor spreading event in western Gulf of Aden during the November 2010-March 2011 period captured by regional seismic networks: evidence for <span class="hlt">diking</span> events and interactions with a nascent transform <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ahmed, Abdulhakim; Doubre, Cécile; Leroy, Sylvie; Kassim, Mohamed; Keir, Derek; Abayazid, Ahmadine; Julie, Perrot; Laurence, Audin; Vergne, Jérome; Alexandre, Nercessian; Jacques, Eric; Khanbari, Khaled; Sholan, Jamal; Rolandone, Frédérique; Al-Ganad, Ismael</p> <p>2016-05-01</p> <p>In November 2010, intense seismic activity including 29 events with a magnitude above 5.0, started in the western part of the Gulf of Aden, where the structure of the oceanic spreading ridge is characterized by a series of N115°-trending slow-spreading segments set within an EW-trending rift. Using signals recorded by permanent and temporary networks in Djibouti and Yemen, we located 1122 earthquakes, with a magnitude ranging from 2.1 to 5.6 from 2010 November 1 to 2011 March 31. By looking in detail at the space-time distribution of the overall seismicity, and both the frequency and the moment tensor of large earthquakes, we re-examine the chronology of this episode. In addition, we also interpret the origin of the activity using high-resolution bathymetric data, as well as from observations of seafloor cable damage caused by high temperatures and lava flows. The analysis allows us to identify distinct active areas. First, we interpret that this episode is mainly related to a <span class="hlt">diking</span> event along a specific ridge segment, located at E044°. In light of previous <span class="hlt">diking</span> episodes in nearby subaerial rift segments, for which field constraints and both seismic and geodetic data exist, we interpret the space-time evolution of the seismicity of the first few days. Migration of earthquakes suggests initial magma ascent below the segment centre. This is followed by a southeastward <span class="hlt">dike</span> propagation below the rift immediately followed by a northwestward <span class="hlt">dike</span> propagation below the rift ending below the northern ridge wall. The cumulative seismic moment associated with this sequence reaches 9.1 × 1017 Nm, and taking into account a very low seismic versus geodetic moment, we estimate a horizontal opening of ˜0.58-2.9 m. The seismic activity that followed occurred through several bursts of earthquakes aligned along the segment axis, which are interpreted as short <span class="hlt">dike</span> <span class="hlt">intrusions</span> implying fast replenishment of the crustal magma reservoir feeding the <span class="hlt">dikes</span>. Over the whole period</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V53A3068M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V53A3068M"><span>Modeling of February 1993 <span class="hlt">Intrusion</span> Seen by JERS-1 Satellite, Kilauea Volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moore, S.; Wauthier, C.; Fukushima, Y.; Poland, M. P.</p> <p>2016-12-01</p> <p>Interferometric Synthetic Aperture Radar (InSAR) is a valuable means of remotely assessing deformation on the surface of the earth. At Kilauea Volcano, Hawai'i many InSAR deformation maps (interferograms) have been studied in recent years to monitor deformation on the volcano. In February 1993, a <span class="hlt">diking</span> event occurred that could be one of the first <span class="hlt">intrusions</span> seen by InSAR satellites at Kilauea. This event has not received much attention due to little geodetic data spanning the event. Between October 1992 and March 1993, SAR images from the JERS-1 satellite captured 30 centimeters of surface deformation occurring along the East Rift <span class="hlt">Zone</span> (ERZ) near Makaopuhi crater. Seismic activity was similar to other <span class="hlt">intrusions</span> with more than 5,000 shallow (<5 km) earthquakes occurred in the area between the summit caldera and Makaopuhi crater from February 7-9, 1993 [Okubo & Nakata, 2003]. We used simple analytical half-space solutions (e.g., Mogi [1958], Okada [1992)]), as well as a more complex and mechanically robust numerical approach (3D-MBEM [Cayol and Cornet, 1997]) to model deformation sources active between October 1992 and March 1993. Non-linear inversions of the JERS-1 Interferogram show that the most likely source to account for the February 1993 observed deformation is a subvertical rectangular <span class="hlt">dike</span> with an opening of 1.5 m reaching depths of 1.5 to 3 km.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Icar..248..424J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Icar..248..424J"><span>Lunar floor-fractured craters as magmatic <span class="hlt">intrusions</span>: Geometry, modes of emplacement, associated tectonic and volcanic features, and implications for gravity anomalies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jozwiak, Lauren M.; Head, James W.; Wilson, Lionel</p> <p>2015-03-01</p> <p>Lunar floor-fractured craters are a class of 170 lunar craters with anomalously shallow, fractured floors. Two end-member processes have been proposed for the floor formation: viscous relaxation, and subcrater magmatic <span class="hlt">intrusion</span> and sill formation. Recent morphometric analysis with new Lunar Reconnaissance Orbiter Laser Altimeter (LOLA) and image (LROC) data supports an origin related to shallow magmatic <span class="hlt">intrusion</span> and uplift. We find that the distribution and characteristics of the FFC population correlates strongly with crustal thickness and the predicted frequency distribution of overpressurization values of magmatic <span class="hlt">dikes</span>. For a typical nearside lunar crustal thickness, <span class="hlt">dikes</span> with high overpressurization values favor surface effusive eruptions, medium values favor <span class="hlt">intrusion</span> and sill formation, and low values favor formation of solidified <span class="hlt">dikes</span> concentrated lower in the crust. We develop a model for this process, make predictions for the morphologic, morphometric, volcanic, and geophysical consequences of the process and then compare these predictions with the population of observed floor-fractured craters. In our model, the process of magmatic <span class="hlt">intrusion</span> and sill formation begins when a <span class="hlt">dike</span> propagates vertically towards the surface; as the <span class="hlt">dike</span> encounters the underdense brecciated region beneath the crater, the magmatic driving pressure is insufficient to continue vertical propagation, but pressure in the stalled <span class="hlt">dike</span> exceeds the local lithostatic pressure. The <span class="hlt">dike</span> then begins to propagate laterally forming a sill which does not propagate past the crater floor region because increased overburden pressure from the crater wall and rim crest pinch off the <span class="hlt">dike</span> at this boundary; the sill then continues to inflate, further raising and fracturing the brittle crater floor. When the <span class="hlt">intrusion</span> diameter to <span class="hlt">intrusion</span> depth ratio is smaller than a critical value, the <span class="hlt">intrusion</span> assumes a laccolith shape with a domed central region. When the ratio exceeds a critical value</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989CoMP..101...12M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989CoMP..101...12M"><span>Anomalous isotopic compositions of Sr, Ar and O in the Mesozoic diabase <span class="hlt">dikes</span> of Liberia, West Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mauche, Renée; Faure, Gunter; Jones, Lois M.; Hoefs, Jochen</p> <p>1989-01-01</p> <p>The Mesozoic diabase <span class="hlt">dikes</span> of Liberia are tholeiites whose 87Sr/86Sr and 87Rb/86Sr ratios scatter widely on the Rb-Sr isochron diagram. The problem is attributed to differences in the initial 87Sr/86Sr ratios of these rocks which range from 0.70311 to 0.70792, assuming a uniform age of 186 Ma for the <span class="hlt">dikes</span> and using λ(87Rb)=1.42 × 10-11y-1. The range of values is similar to that observed in the Mesozoic basalt flows and <span class="hlt">dikes</span> of other Gondwana continents. New whole-rock K-Ar dates confirm previous conclusions that the diabase <span class="hlt">dikes</span> in the Liberian and Pan-African age provinces of Liberia absorbed extraneous 40Ar after <span class="hlt">intrusion</span>. Only the <span class="hlt">dikes</span> in the Paynesville Sandstone have K-Ar dates that range from 117 Ma to 201 Ma and may not contain extraneous 40Ar. However, <span class="hlt">dikes</span> from all three age provinces of Liberia have elevated initial 87Sr/86Sr ratios. These results indicate that contamination with radiogenic 87Sr occurred primarily before <span class="hlt">intrusion</span> of the magma whereas the addition of extraneous 40Ar occurred after emplacement and reflects the age and mineral composition of the country rock. The δ 18O values of the Liberian diabase range from +5.6/% to +9.10/% and correlate positively with initial 87Sr/86Sr ratios. The data can be modeled by fractional crystallization and simultaneous assimilation of crustal rocks by the magma. However, samples containing amphibole and biotite replacing pyroxene deviate from the Sr-O isotope trajectories of the model and appear to have been depleted in 18O and enriched in 87Sr by interactions with groundwater at high temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.703...98T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.703...98T"><span>Mechanical models for <span class="hlt">dikes</span>: A third school of thought</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Townsend, Meredith R.; Pollard, David D.; Smith, Richard P.</p> <p>2017-04-01</p> <p>Geological and geophysical data from continental volcanic centers and giant radial swarms, and from oceanic shield volcanoes and rift <span class="hlt">zones</span>, indicate that <span class="hlt">dikes</span> propagate laterally for distances that can be 10 to over 100 times their height. What traps <span class="hlt">dikes</span> within the shallow lithosphere and promotes these highly eccentric shapes? Gravity-induced stress gradients in the surrounding rock and pressure gradients in the magma are the primary loading mechanisms; pressure gradients due to magma flow are secondary to insignificant, because the flow direction is dominantly horizontal. This configuration of vertical, blade-shaped <span class="hlt">dikes</span> with horizontal <span class="hlt">dike</span> propagation and magma flow is fundamentally different from the two <span class="hlt">dike</span> model configurations described in a recent review paper as two schools of thought for mechanical models of <span class="hlt">dikes</span>. In School I, a <span class="hlt">dike</span> is disconnected from its source and ascends under the influence of buoyancy. In School II, a <span class="hlt">dike</span> is connected to a magma reservoir and is driven upward by magma flux from the source. We review the geological and geophysical data supporting the vertical <span class="hlt">dike</span> - horizontal flow/propagation configuration and suggest the abundance and veracity of these data in many different geological settings, and the modeling results that address this physical process, warrant adding this as a third school of thought. A new analytical solution for the boundary-value problem of a homogeneous, isotropic, and linear elastic solid with a vertical, fluid-filled crack is used to investigate the effects of gravitationally induced stress and pressure gradients on the aperture distribution, <span class="hlt">dike</span>-tip stress intensity, and stable height. Model results indicate that in a homogeneous crust, <span class="hlt">dikes</span> can achieve stable heights greater than a kilometer only if the host rock fracture toughness KIC 100 MPa · m1/2. However, density stratification of the crust is an effective mechanism for trapping kilometer-scale <span class="hlt">dikes</span> even if the host rock is very weak</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008Litho.106..365L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008Litho.106..365L"><span>U Pb zircon age, geochemical and Sr Nd Pb Hf isotopic constraints on age and origin of alkaline <span class="hlt">intrusions</span> and associated mafic <span class="hlt">dikes</span> from Sulu orogenic belt, Eastern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Shen; Hu, Ruizhong; Gao, Shan; Feng, Caixia; Qi, Youqiang; Wang, Tao; Feng, Guangying; Coulson, Ian M.</p> <p>2008-12-01</p> <p>Post-orogenic alkaline <span class="hlt">intrusions</span> and associated mafic <span class="hlt">dikes</span> from the Sulu orogenic belt of eastern China consist of quartz monzonites, A-type granites and associated mafic <span class="hlt">dikes</span>. We report here U-Pb zircon ages, geochemical data and Sr-Nd-Pb-Hf isotopic data for these rocks. The SHRIMP U-Pb zircon analyses yield consistent ages ranging from 120.3 ± 2.1 Ma to 126.9 ± 1.9 Ma for five samples from the felsic rocks, and two crystallization ages of 119.0 ± 1.7 Ma and 120.2 ± 1.9 Ma for the mafic <span class="hlt">dikes</span>. The felsic rocks and mafic <span class="hlt">dikes</span> are characterized by high ( 87Sr/ 86Sr) i ranging from 0.7079 to 0.7089, low ɛNd( t) values from - 15.3 to - 19.2, 206Pb/ 204Pb = 16.54-17.25, 207Pb/ 204Pb = 15.38-15.63, 208Pb/ 204Pb = 37.15-38.45, and relatively uniform ɛHf( t) values of between - 21.6 ± 0.6 and - 23.7 ± 1.0, for the magmatic zircons. The results suggest that they were derived from a common enriched lithospheric mantle source that was metasomatized by foundered lower crustal eclogitic materials before magma generation. Geochemical and isotopic characteristics imply that the primary magma to these rocks originated through partial melting of ancient lithospheric mantle that was variably hybridized by melts derived from foundered lower crustal eclogite. The mafic <span class="hlt">dikes</span> may have been generated by subsequent fractionation of clinopyroxene, whereas the felsic rocks resulted from fractionation of potassium feldspar, plagioclase and ilmenite or rutile. Both were not affected by crustal contamination. Combined with previous studies, these findings provide new evidence that the intense lithospheric thinning beneath the Sulu belt of eastern China occurred between 119 and 127 Ma, and that this was caused by the removal of the lower lithosphere (mantle and lower crust).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1960/0096/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1960/0096/report.pdf"><span>Petrography and petrology of Smoky Butte <span class="hlt">intrusives</span>, Garfield County, Montana</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Matson, Robert E.</p> <p>1960-01-01</p> <p>The Smoky Butte <span class="hlt">intrusives</span> are located in T. 18 N., R. 36 E. Garfield County, Montana on the extreme eastern edge of the petrographic province of Central Montana. They consist of <span class="hlt">dikes</span> and plugs arranged in linear, en-echelon pattern with a northeast trend and intrude the Tullock member (Paleocene age) of the Fort Union formation. Extrusive rocks are absent. The rocks are potassium-rich volcanic types showing a disequilibrium mineral assemblage consisting of sanidine, leucite, biotite, olivine, pyroxene, magnetite plus. ilmenite, apatite, calcite, quartz, and a yellowish to dark greenish glassy groundmass. Two chemical analyses of Smoky Butte rocks show high magnesium, potassium, titanium, and phosphorous and low aluminum and sodium content. The two norm calculations show that the rocks are oversaturated with 1.3 and 3.1 per-cent excess silica. Because of the peculiar nature of the Smoky Butte rocks, descriptive names have been applied to them. They are divided into six different types. Three periods of <span class="hlt">intrusion</span> are proposed for Smoky Butte quarry where three rock types crop out. Other evidence for multiple injection occurs in several multiple <span class="hlt">dikes</span>. The upper contact of the <span class="hlt">intrusion</span> is visible on a few plugs and <span class="hlt">dikes</span>. Smoky Butte rocks show some similarities to the undersaturated potassium-rich rocks of the Highwood and Bearpaw Mountains of Montana, the rocks of the Leucite Hills of Wyoming, and the oversaturated rocks of the West Kimberly District of Australia.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFMGP22A0263P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFMGP22A0263P"><span>Characterization of Clastic <span class="hlt">Dikes</span> Using Controlled Source Audio Magnetotellurics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Persichetti, J. A.; Alumbaugh, D.</p> <p>2001-12-01</p> <p>A site consisting of 3D geology on the Hanford Reservation in Hanford, Washington, has been surveyed using Controlled Source Audio Magnetotellurics (CSAMT) to determine the method's ability to detect clastic <span class="hlt">dikes</span>. The <span class="hlt">dikes</span> are fine-grained, soft-sediment <span class="hlt">intrusions</span>, formed by the buoyant rise of buried, unconsolidated, water rich mud into overlying unconsolidated sediment. The <span class="hlt">dikes</span> are of major importance because they may act as natural barriers inhibiting the spread of contaminants, or as conduits, allowing the contaminants to be quickly wicked away from the contaminant storage tanks that may be located in close vicinity of the <span class="hlt">dikes</span>. The field setup consisted of a 33 meter by 63 meter receiver grid with 3 meter spacing in all directions with the transmitter positioned 71.5 meters from the center of the receiver grid. A total of 12 frequencies were collected from 1.1kHz to 66.2kHz. The CSAMT data is being analyzed using a 2D CSAMT RRI code (Lu, Unsworth and Booker, 1999) and a 2D MT RRI code (Smith and Booker, 1991). Of interest is examining how well the 2D codes are able to map 3D geology, the level of resolution that is obtained, and how important it is to include the 3D source in the solution. The ultimate goal is to determine the applicability of using CSAMT for mapping these types of features at the Hanford Reservation site.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1815409M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1815409M"><span><span class="hlt">Dikes</span> under Pressure - Monitoring the Vulnerability of <span class="hlt">Dikes</span> by Means of SAR Interferometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marzahn, Philip; Seidel, Moritz; Ludwig, Ralf</p> <p>2016-04-01</p> <p><span class="hlt">Dikes</span> are the main man made structures in flood protection systems for the protection of humans and economic values. Usually <span class="hlt">dikes</span> are built with a sandy core and clay or concrete layer covering the core. Thus, <span class="hlt">dikes</span> are prone to a vertical shrinkage due to soil physical processes such as reduction of pore space and gravity increasing the risk of a crevasse during floods. In addition, this vulnerability is amplified by a sea level rise due to climate change. To guarantee the stability of <span class="hlt">dikes</span>, a labourer intensive program is carried out by national authorities monitoring the <span class="hlt">dikes</span> by visual inspection. In the presented study, a quantitative approach is presented using SAR Interferometry for the monitoring of the stability of <span class="hlt">dikes</span> from space. In particular, the vertical movement of <span class="hlt">dikes</span> due to shrinkage is monitored using persistent scatterer interferometry. Therefore three different types of <span class="hlt">dikes</span> have been investigated: a sea coast <span class="hlt">dike</span> with a concrete cover, a sea coast <span class="hlt">dike</span> with short grass cover and a smaller river <span class="hlt">dike</span> with grass cover. All <span class="hlt">dikes</span> are located in Germany. Results show the potential of the monitoring technique as well as spatial differences in the stability of <span class="hlt">dikes</span> with subsidence rates in parts of a <span class="hlt">dike</span> up to 7 mm/a.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V43G2947A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V43G2947A"><span>Overview of Hole GT3A: The sheeted <span class="hlt">dike</span>/gabbro transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abe, N.; Harris, M.; Michibayashi, K.; de Obeso, J. C.; Kelemen, P. B.; Takazawa, E.; Teagle, D. A. H.; Coggon, J. A.; Matter, J. M.; Phase I Science Party, T. O. D. P.</p> <p>2017-12-01</p> <p> the relative timing of <span class="hlt">dike</span> and gabbro <span class="hlt">intrusion</span>, and identify that the Upper Gabbro Sequence intrudes into <span class="hlt">dikes</span>, whereas the Lower Gabbro Sequence is intruded by <span class="hlt">dikes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/wi0215.photos.171825p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/wi0215.photos.171825p/"><span>106. DAM EARTH <span class="hlt">DIKE</span> SUBMERSIBLE DAMS & <span class="hlt">DIKE</span> ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>106. DAM - EARTH <span class="hlt">DIKE</span> - SUBMERSIBLE DAMS & <span class="hlt">DIKE</span> CONN. AT MOVABLE DAM (ML-8-52/2-FS) March 1940 - Upper Mississippi River 9-Foot Channel, Lock & Dam No. 8, On Mississippi River near Houston County, MN, Genoa, Vernon County, WI</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1202/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1202/report.pdf"><span>Deformation of host rocks and flow of magma during growth of minette <span class="hlt">dikes</span> and breccia-bearing <span class="hlt">intrusions</span> near Ship Rock, New Mexico</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Delaney, Paul T.; Pollard, David D.</p> <p>1981-01-01</p> <p>We have studied a small group of minette <span class="hlt">dikes</span> and plugs that crop out within a flat-lying sequence of siltstone and shale near Ship Rock, a prominent volcanic throat of tuff breccia in northwestern New Mexico. Seven <span class="hlt">dikes</span> form a radial pattern about Ship Rock we describe in detail the northeastern <span class="hlt">dike</span>, which has an outcrop length of about 2,900 m, an average thickness of 2.3 m, and a maximum thickness of 7.2 m. The <span class="hlt">dike</span> is composed of 35 discrete segments arranged in echelon; orientation. of <span class="hlt">dike</span> segments ranges systematically from N. 52? E. to N. 66? E. A prominent joint set strikes parallel to the segments and is localized within several tens of meters of the <span class="hlt">dike</span>. Regional joint patterns display no obvious relation to <span class="hlt">dike</span> orientation. Small offsets of segment contacts, as well as wedge-shaped bodies of crumpled host rock within segments mark the sites of coalescence of smaller segments during <span class="hlt">dike</span> growth. Bulges in the <span class="hlt">dike</span> contact, which represent a nondilational component of growth, indicate that wall rocks were brecciated and eroded during the flow of magma. Breccias make up about 9 percent of the 7,176-m 2 area of the <span class="hlt">dike</span>, are concentrated in its southwest half, and are commonly associated with its thickest parts. We also describe three subcircular plugs; each plug is smaller than 30 m in diameter, is laterally associated with a <span class="hlt">dike</span>, and contains abundant breccias. Field evidence indicates that these plugs grew from the <span class="hlt">dikes</span> by brecciation and erosion of wallrocks and that the bulges in the contact of the northeastern <span class="hlt">dike</span> represent an initial stage of this process. From continuum-mechanical models of host-rock deformation, we conclude that <span class="hlt">dike</span> propagation was the dominant mechanism for creating conduits for magma ascent where the host rock was brittle and elastic. At a given driving pressure, <span class="hlt">dikes</span> dilate to accept greater volumes of magma than plugs, and for a given dilation, less work is done on the host rocks. In addition, the pressure required</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019498','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019498"><span>Physical processes of shallow mafic <span class="hlt">dike</span> emplacement near the San Rafael Swell, Utah</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Delaney, P.T.; Gartner, A.E.</p> <p>1997-01-01</p> <p> the dominant N75??E direction of <span class="hlt">dike</span> opening was not strongly favored. Across the center of the swarm, about 10 to 15 <span class="hlt">dikes</span> overlap and produce 15-20 m of dilation. Many are in sufficient proximity that later <span class="hlt">dikes</span> should be thinner than earlier ones if neither the magma pressures nor regional stresses were changing during the emplacement interval. However, <span class="hlt">dike</span> thicknesses vary systematically neither along the length of the swarm nor in proportion to the number of neighboring <span class="hlt">dikes</span>. It appears that crustal extension during the maginatic interval relieved compressive stresses localized by <span class="hlt">intrusion</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ExG....48..177S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ExG....48..177S"><span>3D numerical modelling of negative apparent conductivity anomalies in loop-loop electromagnetic measurements: a case study at a dacite <span class="hlt">intrusion</span> in Sugisawa, Akita Prefecture, Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Selepeng, Ame Thato; Sakanaka, Shin'ya; Nishitani, Tadashi</p> <p>2017-04-01</p> <p>Under certain geological conditions, low induction number electromagnetic (LIN-EM) instruments are known to produce negative apparent conductivity (σa) responses. This is particularly the case when the shallow subsurface is characterised by highly conductive bodies, however little attention has been given to this issue in the research literature. To analyse negative σa anomalies and their causative structures, we make use of a 3D integral equation forward modelling technique based on a 3D weighting function. We present 3D numerical modelling results over a volcanic tuff body intruded by several dacite <span class="hlt">dikes</span>, in Sugisawa, Akita Prefecture, Japan. Apparent conductivity data were acquired using a Geonics EM-34-3 system in the horizontal magnetic dipole (HMD) and vertical magnetic dipole (VMD) operating modes. Our 3D model resolved the horizontal and vertical extent of the dacite <span class="hlt">dikes</span> and also delineated a high conductive <span class="hlt">zone</span> between the volcanic tuff and the <span class="hlt">intrusive</span> dacite <span class="hlt">dikes</span>. This <span class="hlt">zone</span> is the causative structure for negative σa responses in the VMD data, and is interpreted to be an alteration <span class="hlt">zone</span>. Interestingly, the negative σa response was absent when the instrument alignment azimuth was changed, implying an anisotropic effect on the EM signature in the study area. The true conductivity model achieved by 3D forward modelling is shown to compare favourably with the DC resistivity data acquired in the same area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1030186','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1030186"><span>Vapor <span class="hlt">Intrusion</span> Estimation Tool for Unsaturated <span class="hlt">Zone</span> Contaminant Sources. User’s Guide</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-08-30</p> <p>324449 Page Intentionally Left Blank iii Executive Summary Soil vapor extraction (SVE) is a prevalent remediation approach for volatile contaminants...strength and location, vadose <span class="hlt">zone</span> transport, and a model for estimating movement of soil -gas vapor contamination into buildings. The tool may be...framework for estimating the impact of a vadose <span class="hlt">zone</span> contaminant source on soil gas concentrations and vapor <span class="hlt">intrusion</span> into a building</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JGRB..11010201P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JGRB..11010201P"><span>Modeling magma flow and cooling in <span class="hlt">dikes</span>: Implications for emplacement of Columbia River flood basalts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petcovic, Heather L.; Dufek, Josef D.</p> <p>2005-10-01</p> <p>The Columbia River flood basalts include some of the world's largest individual lava flows, most of which were fed by the Chief Joseph <span class="hlt">dike</span> swarm. The majority of <span class="hlt">dikes</span> are chilled against their wall rock; however, rare <span class="hlt">dikes</span> caused their wall rock to undergo partial melting. These partial melt <span class="hlt">zones</span> record the thermal history of magma flow and cooling in the <span class="hlt">dike</span> and, consequently, the emplacement history of the flow it fed. Here, we examine two-dimensional thermal models of basalt injection, flow, and cooling in a 10-m-thick <span class="hlt">dike</span> constrained by the field example of the Maxwell Lake <span class="hlt">dike</span>, a likely feeder to the large-volume Wapshilla Ridge unit of the Grande Ronde Basalt. Two types of models were developed: static conduction simulations and advective transport simulations. Static conduction simulation results confirm that instantaneous injection and stagnation of a single <span class="hlt">dike</span> did not produce wall rock melt. Repeated injection generated wall rock melt <span class="hlt">zones</span> comparable to those observed, yet the regular texture across the <span class="hlt">dike</span> and its wall rock is inconsistent with repeated brittle injection. Instead, advective flow in the <span class="hlt">dike</span> for 3-4 years best reproduced the field example. Using this result, we estimate that maximum eruption rates for Wapshilla Ridge flows ranged from 3 to 5 km3 d-1. Local eruption rates were likely lower (minimum 0.1-0.8 km3 d-1), as advective modeling results suggest that other fissure segments as yet unidentified fed the same flow. Consequently, the Maxwell Lake <span class="hlt">dike</span> probably represents an upper crustal (˜2 km) exposure of a long-lived point source within the Columbia River flood basalts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Litho.277..241W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Litho.277..241W"><span>New insights into the origin of ladder <span class="hlt">dikes</span>: Implications for punctuated growth and crystal accumulation in the Cathedral Peak granodiorite</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wiebe, R. A.; Jellinek, A. M.; Hodge, K. F.</p> <p>2017-04-01</p> <p>Ladder <span class="hlt">dikes</span> are steep tabular bodies, typically a meter or less thick, composed of moderately dipping, concave upward, alternating dark (i.e. schlieren) and light bands oriented roughly perpendicular to the ladder <span class="hlt">dike</span> margins. These structures occur widely but sparsely in granitic rocks and are found prominently in the Cathedral Peak granodiorite (CPG) of the Tuolumne <span class="hlt">Intrusive</span> suite. Previous studies have interpreted that ladder <span class="hlt">dikes</span> form as a result of processes including the downward flow of crystal mush in cracks within strong crystal mush or by upward flow in steep tubes that migrate within a strong crystal mush. Our new observations indicate that ladder <span class="hlt">dikes</span> formed by downward flow of crystal mush in troughs or valleys, in a manner potentially comparable to trough bands in mafic layered <span class="hlt">intrusions</span>. Extensions of the schlieren outward and upward away from the ladder <span class="hlt">dike</span> margins into the host granite demonstrate that the host granite was deposited as mounds on both sides at the same time as the ladder <span class="hlt">dikes</span>. Ladder <span class="hlt">dikes</span>, therefore, record lateral flows of crystal mush on a magma chamber floor. Vertical exposures suggest these flows are on the order of ten meters thick. Some steep exposures on granite domes indicate multiple ladder <span class="hlt">dikes</span> (and flows) over a stratigraphic height of 80-100 m. Later (stratigraphically higher) flows commonly deform and erode the top of an earlier flow, and granitic material rich in K-feldspar megacrysts has locally engulfed large blocks of ladder <span class="hlt">dikes</span>, demonstrating that the megacrysts were also transported in flows. Flows in the CPG are directed away from the center of the pluton toward the western and eastern margins and apparently spread along a strong crystal mush floor and into a rheologically complex CPG magma. Whereas established dynamical models for spreading (single phase) gravity currents with simple and complex rheologies explain the elongate geometry, spacing and orientation of the tabular bodies, the origin and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.3707D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.3707D"><span>A laser profilometry technique for monitoring fluvial <span class="hlt">dike</span> breaching in laboratory experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dewals, Benjamin; Rifai, Ismail; Erpicum, Sébastien; Archambeau, Pierre; Violeau, Damien; Pirotton, Michel; El kadi Abderrezzak, Kamal</p> <p>2017-04-01</p> <p>A challenging aspect for experimental modelling of fluvial <span class="hlt">dike</span> breaching is the continuous monitoring of the transient breach geometry. In dam breaching cases induced by flow overtopping over the whole breach crest (plane erosion), a side view through a glass wall is sufficient to monitor the breach formation. This approach can be extended for 3D dam breach tests (spatial erosion) if the glass wall is located along the breach centreline. In contrast, using a side view does not apply for monitoring fluvial <span class="hlt">dike</span> breaching, because the breach is not symmetric in this case. We present a non-<span class="hlt">intrusive</span>, high resolution technique to record the breach development in experimental models of fluvial <span class="hlt">dikes</span> by means of a laser profilometry (Rifai et al. 2016). Most methods used for monitoring dam and <span class="hlt">dike</span> breaching involve the projection of a pattern (fringes, grid) on the dam or <span class="hlt">dike</span> body and the analysis of its deformation on images recorded during the breaching (e.g., Pickert et al. 2011, Frank and Hager 2014). A major limitation of these methods stems from reflection on the water surface, particularly in the vicinity of the breach where the free surface is irregular and rippled. This issue was addressed by Spinewine et al. (2004), who used a single laser sheet so that reflections on the water surface were strongly limited and did not hamper the accurate processing of each image. We have developed a similar laser profilometry technique tailored for laboratory experiments on fluvial <span class="hlt">dike</span> breaching. The setup is simple and relatively low cost. It consists of a digital video camera (resolution of 1920 × 1080 pixels at 60 frames per second) and a swiping red diode 30 mW laser that enables the projection of a laser sheet over the <span class="hlt">dike</span> body. The 2D image coordinates of each deformed laser profile incident on the <span class="hlt">dike</span> are transformed into 3D object coordinates using the Direct Linear Transformation (DLT) algorithm. All 3D object coordinates computed over a swiping cycle of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1214914A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1214914A"><span>Ductile deformation history in Laibid metamorphic rocks, Sanandaj-Sirjan <span class="hlt">Zone</span>, Iran</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aflaki, Mahtab; Mohajjel, Mohammad</p> <p>2010-05-01</p> <p>Sanandaj-Sirjan <span class="hlt">zone</span>, in northeast of Zagros suture <span class="hlt">zone</span>, is the metamorphic belt of the Zagros orogen which is metamorphosed during Late Mesozoic, as the active margin of the Neotethys subduction system. Since Late Cretaceous, oblique collision between Afro-Arabian continent and Central Iran micro continent resulted in dextral transpression and Poly-phase deformations of this <span class="hlt">zone</span>. Laibid area, northwest of Esfahan province, is situated in complexly deformed sub <span class="hlt">zone</span> of the Sanandaj-Sirjan <span class="hlt">zone</span> in which structurally exposed Permian metamorphosed rocks are separated from the younger Triassic-Jurassic metamorphic rocks by faulted boundaries. Cretaceous unites do not exist in the study area, but in southern most parts un-metamorphosed Early Cretaceous rocks rest on Jurassic metamorphic units over an angular unconformity. Field observations reveal the existence of 3 folding patterns, folded <span class="hlt">dikes</span>, semi-ductile to ductile shear <span class="hlt">zones</span> and also sin-tectonic granite <span class="hlt">intrusion</span>. Hassan-Robat Alkali-porphyritic-granite is exposed in the eastern part of the area with the possible ages between post-Early Cretaceous to pre-Eocene. In this research, the focus is on ductile structures and their deformation history in the Laibid area. Structural analysis of the folds reveals three deformation stages of a progressive deformation in this area. These folding patterns observed in all pre-Cretaceous metamorphosed unites, but not in Cretaceous rocks. The first stage includes tight to isoclinal folds, S0 || S1, with the aspect ratio changes respectively from tall and short. Although their axial plane and fold axis orientations change due to other two folding stages, but they mostly have moderately dipping to the NE axial plane and moderately plunging fold axis to NW or SE. In the eastern part of the area the trend of F1 foliation changes around the Hassan-Robat granite. The second folding stage includes open to close asymmetric folds which have broad aspect ratio. This folding stage</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017241','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017241"><span>A-type granite and the Red Sea opening</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Coleman, R.G.; DeBari, S.; Peterman, Z.</p> <p>1992-01-01</p> <p>Miocene-Oligocene A-type granite intrudes the eastern side of the Red Sea margin within the <span class="hlt">zone</span> of extension from Jiddah, Saudi Arabia south to Yemen. The <span class="hlt">intrusions</span> developed in the early stages of continental extension as Arabia began to move slowly away from Africa (around 30-20 Ma). Within the narrow <span class="hlt">zone</span> of extension silicic magmas formed <span class="hlt">dikes</span>, sills, small plutons and extrusive equivalents. In the Jabal Tirf area of Saudi Arabia these rocks occur in an elongate <span class="hlt">zone</span> consisting of late Precambrian basement to the east, which is gradually invaded by mafic <span class="hlt">dikes</span>. The number of <span class="hlt">dikes</span> increases westward until an igneous complex is produced parallel to the present Red Sea axis. The Jabal Tirf igneous complex consists of diabase and rhyolite-granophyre sills (20-24 Ma). Although these are intrusine <span class="hlt">intrusive</span> rocks their textures indicate shallow depths of <span class="hlt">intrusion</span> (< 1 km). To the south, in the Yemen, contemporaneous with alkali basaltic eruptions (26-30 Ma) and later silicic eruptions, small plutons, <span class="hlt">dikes</span>, and stocks of alkali granite invaded thick (1500 m) volcanic series, at various levels and times. Erosion within the uplifted margin of Yemen suggests that the maximum depth of <span class="hlt">intrusion</span> was less than 1-2 km. Granophyric <span class="hlt">intrusions</span> (20-30 Ma) within mafic <span class="hlt">dike</span> swarms similar to the Jabal Tirf complex are present along the western edge of the Yemen volcanic plateau, marking a north-south <span class="hlt">zone</span> of continental extension. The alkali granites of Yemen consist primarily of perthitic feldspar and quartz with some minor alkali amphiboles and acmite. These granites represent water-poor, hypersolvus magmas generated from parent alkali basalt magmas. The granophyric, two-feldspar granites associated with the mafic <span class="hlt">dike</span> swarms and layered gabbros formed by fractional crystallization from tholeiitic basalt parent developed in the early stages of extension. Initial 87Sr/86Sr ratios of these rocks and their bulk chemistry indicate that production of peralkaline and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.G51A0073W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.G51A0073W"><span>Bi-directional volcano-earthquake interaction at Mauna Loa Volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walter, T. R.; Amelung, F.</p> <p>2004-12-01</p> <p>At Mauna Loa volcano, Hawaii, large-magnitude earthquakes occur mostly at the west flank (Kona area), at the southeast flank (Hilea area), and at the east flank (Kaoiki area). Eruptions at Mauna Loa occur mostly at the summit region and along fissures at the southwest rift <span class="hlt">zone</span> (SWRZ), or at the northeast rift <span class="hlt">zone</span> (NERZ). Although historic earthquakes and eruptions at these <span class="hlt">zones</span> appear to correlate in space and time, the mechanisms and implications of an eruption-earthquake interaction was not cleared. Our analysis of available factual data reveals the highly statistical significance of eruption-earthquake pairs, with a random probability of 5-to-15 percent. We clarify this correlation with the help of elastic stress-field models, where (i) we simulate earthquakes and calculate the resulting normal stress change at volcanic active <span class="hlt">zones</span> of Mauna Loa, and (ii) we simulate <span class="hlt">intrusions</span> in Mauna Loa and calculate the Coulomb stress change at the active fault <span class="hlt">zones</span>. Our models suggest that Hilea earthquakes encourage <span class="hlt">dike</span> <span class="hlt">intrusion</span> in the SWRZ, Kona earthquakes encourage <span class="hlt">dike</span> <span class="hlt">intrusion</span> at the summit and in the SWRZ, and Kaoiki earthquakes encourage <span class="hlt">dike</span> <span class="hlt">intrusion</span> in the NERZ. Moreover, a <span class="hlt">dike</span> in the SWRZ encourages earthquakes in the Hilea and Kona areas. A <span class="hlt">dike</span> in the NERZ may encourage and discourage earthquakes in the Hilea and Kaoiki areas. The modeled stress change patterns coincide remarkably with the patterns of several historic eruption-earthquake pairs, clarifying the mechanisms of bi-directional volcano-earthquake interaction for Mauna Loa. The results imply that at Mauna Loa volcanic activity influences the timing and location of earthquakes, and that earthquakes influence the timing, location and the volume of eruptions. In combination with near real-time geodetic and seismic monitoring, these findings may improve volcano-tectonic risk assessment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.V21H..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.V21H..05M"><span>Rift <span class="hlt">Zone</span> Abandonment and Reconfiguration in Hawaii: Evidence from Mauna Loa’s Ninole Rift <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morgan, J. K.; Park, J.; Zelt, C. A.</p> <p>2009-12-01</p> <p>Large oceanic volcanoes commonly develop elongate rift <span class="hlt">zones</span> that disperse viscous magmas to the distal reaches of the edifice. <span class="hlt">Intrusion</span> and <span class="hlt">dike</span> propagation occur under tension perpendicular to the rift <span class="hlt">zone</span>, controlled by topography, magmatic pressures, and deformation of the edifice. However, as volcanoes grow and interact, the controlling stress fields can change, potentially altering the orientations and activities of rift <span class="hlt">zones</span>. This phenomenon is probably common, and can produce complex internal structures that influence the evolution of a volcano and its neighbors. However, little direct evidence for such rift <span class="hlt">zone</span> reconfiguration exists, primarily due to poor preservation or recognition of earlier volcanic configurations. A new onshore-offshore 3-D seismic velocity model for the Island of Hawaii, derived from a joint tomographic inversion of an offshore airgun shot - onshore receiver geometry and earthquake sources beneath the island, demonstrates a complicated history of rift <span class="hlt">zone</span> reconfiguration on Mauna Loa volcano, Hawaii, including wholesale rift <span class="hlt">zone</span> abandonment. Mauna Loa’s southeast flank contains a massive high velocity <span class="hlt">intrusive</span> complex, now buried beneath flows derived from Mauna Loa’s active southwest rift <span class="hlt">zone</span> (SWRZ). Introduced here as the Ninole Rift <span class="hlt">Zone</span>, this feature extends more than 60 km south of Mauna Loa’s summit, spans a depth range of ~2-14 km below sea level, and is the probable source of the 100-200 ka Ninole volcanics in several prominent erosional hills. A lack of high velocities beneath the upper SWRZ and its separate <span class="hlt">zone</span> of high velocities on the submarine flank, indicate that the younger rift <span class="hlt">zone</span> was built upon a pre-existing edifice that emanated from the Ninole rift <span class="hlt">zone</span>. The ancient Ninole rift <span class="hlt">zone</span> may stabilize Mauna Loa’s southeast flank, focusing recent volcanic activity and deformation onto the unbuttressed west flank. The upper portion of the Ninole rift <span class="hlt">zone</span> appears to have migrated westward over time</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70046825','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70046825"><span>Evolution of <span class="hlt">dike</span> opening during the March 2011 Kamoamoa fissure eruption, Kīlauea Volcano, Hawai`i</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lundgren, Paul; Poland, Michael; Miklius, Asta; Orr, Tim R.; Yun, Sang-Ho; Fielding, Eric; Liu, Zhen; Tanaka, Akiko; Szeliga, Walter; Hensley, Scott; Owen, Susan</p> <p>2013-01-01</p> <p>The 5–9 March 2011 Kamoamoa fissure eruption along the east rift <span class="hlt">zone</span> of Kīlauea Volcano, Hawai`i, followed months of pronounced inflation at Kīlauea summit. We examine <span class="hlt">dike</span> opening during and after the eruption using a comprehensive interferometric synthetic aperture radar (InSAR) data set in combination with continuous GPS data. We solve for distributed <span class="hlt">dike</span> displacements using a whole Kīlauea model with dilating rift <span class="hlt">zones</span> and possibly a deep décollement. Modeled surface <span class="hlt">dike</span> opening increased from nearly 1.5 m to over 2.8 m from the first day to the end of the eruption, in agreement with field observations of surface fracturing. Surface <span class="hlt">dike</span> opening ceased following the eruption, but subsurface opening in the <span class="hlt">dike</span> continued into May 2011. <span class="hlt">Dike</span> volumes increased from 15, to 16, to 21 million cubic meters (MCM) after the first day, eruption end, and 2 months following, respectively. <span class="hlt">Dike</span> shape is distinctive, with a main limb plunging from the surface to 2–3 km depth in the up-rift direction toward Kīlauea's summit, and a lesser projection extending in the down-rift direction toward Pu`u `Ō`ō at 2 km depth. Volume losses beneath Kīlauea summit (1.7 MCM) and Pu`u `Ō`ō (5.6 MCM) crater, relative to <span class="hlt">dike</span> plus erupted volume (18.3 MCM), yield a <span class="hlt">dike</span> to source volume ratio of 2.5 that is in the range expected for compressible magma without requiring additional sources. Inflation of Kīlauea's summit in the months before the March 2011 eruption suggests that the Kamoamoa eruption resulted from overpressure of the volcano's magmatic system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRB..118..897L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRB..118..897L"><span>Evolution of <span class="hlt">dike</span> opening during the March 2011 Kamoamoa fissure eruption, Kīlauea Volcano, Hawai`i</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lundgren, Paul; Poland, Michael; Miklius, Asta; Orr, Tim; Yun, Sang-Ho; Fielding, Eric; Liu, Zhen; Tanaka, Akiko; Szeliga, Walter; Hensley, Scott; Owen, Susan</p> <p>2013-03-01</p> <p>5-9 March 2011 Kamoamoa fissure eruption along the east rift <span class="hlt">zone</span> of Kīlauea Volcano, Hawai`i, followed months of pronounced inflation at Kīlauea summit. We examine <span class="hlt">dike</span> opening during and after the eruption using a comprehensive interferometric synthetic aperture radar (InSAR) data set in combination with continuous GPS data. We solve for distributed <span class="hlt">dike</span> displacements using a whole Kīlauea model with dilating rift <span class="hlt">zones</span> and possibly a deep décollement. Modeled surface <span class="hlt">dike</span> opening increased from nearly 1.5 m to over 2.8 m from the first day to the end of the eruption, in agreement with field observations of surface fracturing. Surface <span class="hlt">dike</span> opening ceased following the eruption, but subsurface opening in the <span class="hlt">dike</span> continued into May 2011. <span class="hlt">Dike</span> volumes increased from 15, to 16, to 21 million cubic meters (MCM) after the first day, eruption end, and 2 months following, respectively. <span class="hlt">Dike</span> shape is distinctive, with a main limb plunging from the surface to 2-3 km depth in the up-rift direction toward Kīlauea's summit, and a lesser projection extending in the down-rift direction toward Pu`u `Ō`ō at 2 km depth. Volume losses beneath Kīlauea summit (1.7 MCM) and Pu`u `Ō`ō (5.6 MCM) crater, relative to <span class="hlt">dike</span> plus erupted volume (18.3 MCM), yield a <span class="hlt">dike</span> to source volume ratio of 2.5 that is in the range expected for compressible magma without requiring additional sources. Inflation of Kīlauea's summit in the months before the March 2011 eruption suggests that the Kamoamoa eruption resulted from overpressure of the volcano's magmatic system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Litho.212...16T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Litho.212...16T"><span>Petrogenesis of the Ni-Cu-PGE sulfide-bearing Tamarack <span class="hlt">Intrusive</span> Complex, Midcontinent Rift System, Minnesota</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Taranovic, Valentina; Ripley, Edward M.; Li, Chusi; Rossell, Dean</p> <p>2015-01-01</p> <p>The Tamarack <span class="hlt">Intrusive</span> Complex (TIC, 1105.6 ± 1.2 Ma) in NE Minnesota, was emplaced during the early stages of the development of the Midcontinent Rift System (MRS, "Early Stage": 1110-1106 Ma). Country rocks of the TIC are those of the Paleoproterozoic Thomson Formation, part of the Animikie Group including sulfide-bearing metasedimentary black shale. The magmatic system is composed of at least two principal mafic-ultramafic <span class="hlt">intrusive</span> sequences: the sulfide-barren Bowl <span class="hlt">Intrusion</span> in the south and the "<span class="hlt">dike</span>" area <span class="hlt">intrusions</span> in the north which host Ni-Cu-Platinum Group Elements (PGE) mineralization with up to 2.33% Ni, 1.24% Cu, 0.34 g/t Pt, 0.23 g/t Pd and 0.18 g/t Au. Two distinct <span class="hlt">intrusive</span> units in the "<span class="hlt">dike</span>" area are the CGO (coarse-grained olivine-bearing) <span class="hlt">Intrusion</span>, a sub-vertical <span class="hlt">dike</span>-like body, and the overlying sub-horizontal FGO (fine-grained olivine-bearing) <span class="hlt">Intrusion</span>. Both <span class="hlt">intrusions</span> comprise peridotite, feldspathic peridotite, feldspathic pyroxenite, melatroctolite and melagabbro. Massive sulfides are volumetrically minor and mainly occur as lenses emplaced into the country rocks associated with both <span class="hlt">intrusions</span>. Semi-massive (net-textured) sulfides are distributed at the core of the CGO <span class="hlt">Intrusion</span>, surrounded by a halo of the disseminated sulfides. Disseminated sulfides also occur in lenses along the base of the FGO <span class="hlt">Intrusion</span>. Olivine compositions in the CGO <span class="hlt">Intrusion</span> are between Fo89 and Fo82 and in the FGO <span class="hlt">Intrusion</span> from Fo84 to Fo82. TIC <span class="hlt">intrusions</span> have more primitive olivine compositions than that of olivine in the sheet-like <span class="hlt">intrusions</span> in the Duluth Complex (below Fo70), as well as olivine from the smaller, conduit-related, Eagle and East Eagle <span class="hlt">Intrusions</span> in Northern Michigan (Fo86 to Fo75). The FeO/MgO ratios of the CGO and FGO <span class="hlt">Intrusion</span> parental magmas, inferred from olivine compositions, are similar to those of picritic basalts erupted during the early stages of the MRS formation. Trace element ratios differ slightly from other <span class="hlt">intrusions</span> in the</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020843','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020843"><span>Change in the magnetic properties of bituminous coal intruded by an igneous <span class="hlt">dike</span>, Dutch Creek Mine, Pitkin County, Colorado</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Thorpe, A.N.; Senftle, F.E.; Finkelman, R.B.; Dulong, F.T.; Bostick, N.H.</p> <p>1998-01-01</p> <p>Magnetization measurements have been made on natural coke-coal samples collected at various distances from a felsic porphyry <span class="hlt">dike</span> in a coal seam in Dutch Creek Mine, Colorado to help characterize the nature and distribution of the iron-bearing phases. The magnetization passes through a maximum at the coke-to-coal transition about 31 cm from the <span class="hlt">dike</span> contact. The magnetic measurements support the geochemical data indicating that magmatic fluids along with a high-temperature gas pulse moved into the coal bed. Interaction of the magmatic fluids with the coal diminished the reducing power of the thermal gas pulse from the <span class="hlt">dike</span> to a point about 24 cm into the coal. The hot reducing gas penetrated further and produced a high temperature (~400-525??C) <span class="hlt">zone</span> (at about 31 cm) just ahead of the magmatic fluids. Metallic iron found in this <span class="hlt">zone</span> is the principal cause of the observed high magnetization. Beyond this <span class="hlt">zone</span>, the temperature was too low to alter the coal significantly.Magnetization measurements have been made on natural coke-coal samples collected at various distances from a felsic porphyry <span class="hlt">dike</span> in a coal seam in Dutch Creek Mine, Colorado to help characterize the nature and distribution of the iron-bearing phases. The magnetization passes through a maximum at the coke-to-coal transition about 31 cm from the <span class="hlt">dike</span> contact. The magnetic measurements support the geochemical data indicating that magmatic fluids along with a high-temperature gas pulse moved into the coal bed. Interaction of the magmatic fluids with the coal diminished the reducing power of the thermal gas pulse from the <span class="hlt">dike</span> to a point about 24 cm into the coal. The hot reducing gas penetrated further and produced a high temperature (approximately 400-525 ??C) <span class="hlt">zone</span> (at about 31 cm) just ahead of the magmatic fluids. Metallic iron found in this <span class="hlt">zone</span> is the principal cause of the observed high magnetization. Beyond this <span class="hlt">zone</span>, the temperature was too low to alter the coal significantly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.9878M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.9878M"><span>Age dependent variation of magnetic fabric on <span class="hlt">dike</span> swarms from Maio Island (Cape Verde)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moreira, Mário; Madeira, José; Mata, João.; Represas, Patrícia</p> <p>2010-05-01</p> <p>Maio is one of the oldest and most eroded islands of Cape Verde Archipelago. It comprises three major geological units: (1) an old raised sea-floor sequence of MORB covered by Jurassic(?)-Cretaceous deep marine sediments; (2) an <span class="hlt">intrusive</span> 'Central Igneous Complex' (CIC), forming a dome-like structure in the older rocks; and (3) a sequence of initially submarine, then subaerial, extrusive volcanic formations and sediments. Based on the trend distribution of 290 <span class="hlt">dikes</span>, we performed magnetic sampling on 26 basic and one carbonatite <span class="hlt">dikes</span>. Anisotropy of magnetic susceptibility (AMS) was measured to infer geometries of magmatic flow. <span class="hlt">Dikes</span> were sampled in both chilled margins were larger shear acting on particles embedded in the magmatic flow is expected. Sampling involved 11 <span class="hlt">dikes</span> (N=195) intruding MORB pillows from the Upper Jurassic 'Batalha Formation' (Bt fm); 6 <span class="hlt">dikes</span> (N=95) intruding the Lower Cretaceous 'Carquejo Formation' (Cq fm), and 10 <span class="hlt">dikes</span> (N=129) intruding the submarine sequence of the Neogene 'Casas Velhas Formation' (CV fm). The studied hypabissal rocks are usually porphyritic, with phenocrysts of clinopyroxene and/or olivine set on an aphanitic groundmass. <span class="hlt">Dikes</span> intruding CV fm trend N-S to NE-SW and plunge to SW. In Bt fm, <span class="hlt">dikes</span> make ≈ 99% of the outcrops, span all directions and include frequent low dip sills. <span class="hlt">Dikes</span> intruding Cq fm are shallow (mostly parallel to the limestone strata), dip 30o- 40o to the E, and trend N-S to NE-SW. Bulk susceptibility of the 26 basic <span class="hlt">dikes</span> presents an average value of k = 47 ± 26 (×10-3) SI. The carbonatite <span class="hlt">dike</span> intruding Bt fm has lower susceptibility: k = 4.6 ± 1.2 (×10-3) SI. More than 80% of the <span class="hlt">dikes</span> show normal and triaxial magnetic fabric. Anisotropy is usually low, with P' < 1.08, but in CV fm <span class="hlt">dikes</span> the anisotropy is higher and grows (up to P' ≈ 1.5) towards the centre of the volcano. Dominant magnetic fabric in CV fm is planar but in <span class="hlt">dikes</span> from Cq fm and Bt fm it varies between oblate and prolate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS1013a2185A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS1013a2185A"><span>Geoelectric imaging for saline water <span class="hlt">intrusion</span> in Geopark <span class="hlt">zone</span> of Ciletuh Bay, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ardi, N. D.; Iryanti, M.; Asmoro, C. P.; Yusuf, A.; Sundana, A. N. A.; Safura, H. Y.; Fitri, M.; Anggraeni, M.; Kurniawan, R.; Afrianti, R.; Sumarni</p> <p>2018-05-01</p> <p>Saline water <span class="hlt">intrusion</span> in estuary is an urgent ecological encounter across the world. The Ciletuh Bay, located in the southern Sukabumi district, is an area with high cultivated potential becoming one of the most important geology tourism <span class="hlt">zones</span> in Indonesia. However, salt water <span class="hlt">intrusion</span> along the creek is a natural spectacle that disturbs the economic growth of the whole region. This research was intended at plotting the subsurface level of saltwater interventions into aquifers at the northern part of Ciletuh creek, Indonesia. The study implemented geoelectric imaging methods. 37 imaging datum were acquired using Wenner array configuration. The saline water were identified across the study area. The result of two dimensional cross-sectional resistivity shows that there is an indication of sea content in our measured soil, i.e. the smallest resistivity value is 0.579 Ωm found at a depth of 12.4 m to 19.8 m at a track length of 35 m to 60 m is categorized in the clayey which shows low groundwater quality. However, when compared with the results of direct observation of groundwater from the wells of residents, the water obtained is brackish water. A water chemistry test is conducted to ascertain the initial results of this method so that a potential sea <span class="hlt">intrusion</span> potential map can be interpreted more clearly. This can consequently help as an extrapolative model to define depth to saline water at any site within the saline water <span class="hlt">zone</span> in the study area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988JGR....9314773W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988JGR....9314773W"><span>Three Hawaiian calderas: An origin through loading by shallow <span class="hlt">intrusions</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walker, George P. L.</p> <p>1988-12-01</p> <p>The calderas of Kilauea and Mauna Loa are highly dynamic structures, and in the <200-year historic period have varied in volume by a factor of 2, and gained or lost 1 km3 per century. The deeply eroded caldera of the extinct Koolau Volcano in Oahu is wider than active Hawaiian calderas, and its lavas have a strong centripetal dip and funnel structure not evident at Kilauea or Mauna Loa. The differences can be attributed to the different erosion depths, and the time integrated subsidence profile of Kilauea is also a stepped funnel (having its apex at Halemaumau). Koolau caldera is the focus of an extraordinarily intense <span class="hlt">dike</span> complex, and an intriguing feature is the great diminution in <span class="hlt">dike</span> concentration into the caldera. It is thought that <span class="hlt">dike</span> injection in any part of the complex generally continued until it reached 50% to 65%. In outer parts of the caldera, the complex was maintained at or rebuilt to this value despite subsidence. In the center of the caldera (where the positive Bouguer anomaly is centered), subsidence evidently greatly outpaced the capacity of <span class="hlt">dike</span> injections to rebuild the complex. Assuming the same <span class="hlt">dike</span> injection rate as Kilauea and Mauna Loa yields a volumetric subsidence rate in Koolau caldera exceeding 1 km3 per century. Hawaiian calderas are much more dynamic than calderas of silicic volcanoes, shaped by frequent small events instead of a few great ones. The temporal and volumetric correspondence of historical subsidence events with eruptions is poor, and this and the high subsidence rates argue for a caldera-forming mechanism that consumes the subsided rocks. It is suggested that subsidence is caused by the great localized excess load of <span class="hlt">intrusive</span> rocks, carrying the center of the volcano into the thermally weakened lithosphere above the Hawaiian hot spot. It is envisaged that under steady state conditions the magma chamber rises, as the injection of <span class="hlt">intrusions</span> causes the level of neutral buoyancy (at which the chamber is located) to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.6692U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.6692U"><span>Propagation and arrest of <span class="hlt">dikes</span> under topography: Models applied to the 2014 Bardarbunga (Iceland) rifting event</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Urbani, S.; Acocella, V.; Rivalta, E.; Corbi, F.</p> <p>2017-07-01</p> <p><span class="hlt">Dikes</span> along rift <span class="hlt">zones</span> propagate laterally downslope for tens of kilometers, often becoming arrested before topographic reliefs. We use analogue and numerical models to test the conditions controlling the lateral propagation and arrest of <span class="hlt">dikes</span>, exploring the presence of a slope in connection with buoyancy and rigidity layering. A gentle downslope assists lateral propagation when combined with an effective barrier to magma ascent, e.g., gelatin stiffness contrasts, while antibuoyancy alone may be insufficient to prevent upward propagation. We also observe that experimental <span class="hlt">dikes</span> become arrested when reaching a plain before opposite reliefs. Our numerical models show that below the plain the stress field induced by topography hinders further <span class="hlt">dike</span> propagation. We suggest that lateral <span class="hlt">dike</span> propagation requires an efficient barrier (rigidity) to upward propagation, assisting antibuoyancy, and a lateral pressure gradient perpendicular to the least compressive stress axis, while <span class="hlt">dike</span> arrest may be induced by external reliefs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770028469&hterms=swarm&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dswarm','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770028469&hterms=swarm&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dswarm"><span>The Sagatu Ridge <span class="hlt">dike</span> swarm, Ethiopian rift margin. [tectonic evolution</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mohr, P. A.; Potter, E. C.</p> <p>1976-01-01</p> <p>A swarm of <span class="hlt">dikes</span> forms the core of the Sagatu Ridge, a 70-km-long topographic feature elevated to more than 4000 m above sea level and 1500 m above the level of the Eastern (Somalian) plateau. The ridge trends NNE and lies about 50 km east of the northeasterly trending rift-valley margin. <span class="hlt">Intrusion</span> of the <span class="hlt">dikes</span> and buildup of the flood-lava pile, largely hawaiitic but with trachyte preponderant in the final stages, occurred during the late Pliocene-early Pleistocene and may have been contemporaneous with downwarping of the protorift trough to the west. The ensuing faulting that formed the present rift margin, however, bypassed the ridge. The peculiar situation and orientation of the Sagatu Ridge, and its temporary existence as a line of crustal extension and voluminous magmatism, are considered related to a powerful structural control by a major line of Precambrian crustal weakness, well exposed further south. Transverse rift structures of unknown type appear to have limited the development of the ridge to the north and south.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BVol...76..807V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BVol...76..807V"><span>Unconventional maar diatreme and associated <span class="hlt">intrusions</span> in the soft sediment-hosted Mardoux structure (Gergovie, France)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Valentine, Greg A.; van Wyk de Vries, Benjamin</p> <p>2014-03-01</p> <p>A Miocene age volcanic-hypabyssal structure comprising volcaniclastic deposits and mafic <span class="hlt">intrusions</span> is exposed with vertical relief of ˜110 m on the side of Gergovie Plateau (Auvergne, France). Three main volcaniclastic facies are: (1) Fluidal tuff breccia composed of juvenile basalt and sediment clasts with dominantly fluidal shapes, with several combinations of basalt and sediment within individual clasts. (2) Thickly bedded lapilli tuff composed of varying proportions of fine-grained sediment derived from Oligocene-Miocene lacustrine marls and mudstones and basaltic lapilli, blocks, and bombs. (3) Planar-bedded tuff forming thin beds of fine to coarse ash-size sedimentary material and basalt clasts. <span class="hlt">Intrusive</span> bodies in the thickly bedded lapilli tuff range from irregularly shaped and anastomosing <span class="hlt">dikes</span> and sills of meters to tens of meters in length, to a main feeder <span class="hlt">dike</span> that is up to ˜20 m wide, and that flares into a spoon-shaped sill at ˜100 m in diameter and 10-20 m thick in the eastern part of the structure. Volcaniclastic deposits and structural features suggest that ascending magma entrained soft, saturated sediment host material into the feeder <span class="hlt">dike</span> and erupted fluidal magma and wet sediment via weak, Strombolian-like explosions. Host sediment and erupted material subsided to replace the extracted sediments, producing the growth subsidence structure that is similar to upper diatreme facies in typical maar diatremes but lacks evidence for explosive disruption of diatreme fill. Irregularly shaped small <span class="hlt">intrusions</span> extended from the main feeder <span class="hlt">dike</span> into the diatreme, and many were disaggregated due to shifting and subsidence of diatreme fill and recycled via eruption. The Mardoux structure is an "unconventional" maar diatreme in that it was produced mainly by weak explosive activity rather than by violent phreatomagmatic explosions and is an example of complex coupling between soft sediment and ascending magma.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUSM.T43D..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUSM.T43D..02H"><span>40Ar/39Ar dates from alkaline <span class="hlt">intrusions</span> of the northern Crazy Mountains, south-central Montana</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harlan, S. S.</p> <p>2005-05-01</p> <p>The Crazy Mountains basin of south-central Montana is a complex foreland basin that formed during the interaction of thin-skinned, decollement-style folds of the Montana thrust belt and the basement-involved folds and thrust faults of the Rocky Mountain foreland province. Near the depositional center of the basin, synorogenic strata of the Paleocene Fort Union Formation have been intruded and locally thermally metamorphosed by strongly alkaline to subalkaline Tertiary <span class="hlt">intrusive</span> rocks. The subalkaline rocks are found mostly in the southern Crazy Mountains and form stocks (Big Timber stock, Loco Mountain stock), radiating <span class="hlt">dikes</span> and sills. With the exception of the Ibex Mountain sill (?), the alkaline rocks are restricted to the northern Crazy Mountains. New 40Ar/39Ar dates are reported from the strongly alkaline rocks, including the Comb Creek stock and <span class="hlt">dike</span> swarm, the Ibex Mountain sill(?), and sills from the Robinson anticline <span class="hlt">intrusive</span> complex. The alkaline rocks of the Robinson anticline <span class="hlt">intrusive</span> complex are exposed in the easternmost folds of the Cordilleran fold and thrust belt, but despite their arcuate and apparently folded map geometry they have been shown to post-date folding. Hornblende from a trachyte sill in the Robinson anticline <span class="hlt">intrusive</span> complex yielded a relatively simple age spectrum with a weighted mean of 50.61 ± 0.14 Ma (2σ), which probably records the age of sill emplacement. Nepheline syenite and mafic nepheline syenites of the Comb Creek stock and a <span class="hlt">dike</span> from its radial <span class="hlt">dike</span> swarm, two sills from the Robinson antlicline <span class="hlt">intrusive</span> complex, and the Ibex Mountains sill(?) gave biotite plateau dates ranging from 50.03 to 50.22 Ma, with 2σ errors of ± 0.11 to 0.19 Ma. Because these dates are from fairly small, hypabyssal <span class="hlt">intrusions</span>, they must have cooled quickly and thus these dates closely approximate the emplacement age of the <span class="hlt">intrusions</span>. These data indicate that the strongly alkaline <span class="hlt">intrusions</span> were emplaced during a fairly restricted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1133/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1133/report.pdf"><span>Clastic <span class="hlt">dikes</span> of Heart Mountain fault breccia, northwestern Wyoming, and their significance</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pierce, W.G.</p> <p>1979-01-01</p> <p>Structural features in northwestern Wyoming indicate that the Heart Mountain fault movement was an extremely rapid, cataclysmic event that created a large volume of carbonate fault breccia derived entirely from the lower part of the upper plate. After fault movement had ceased, much of the carbonate fault breccia, here called calcibreccia, lay loose on the resulting surface of tectonic denudation. Before this unconsolidated calcibreccia could be removed by erosion, it was buried beneath a cover of Tertiary volcanic rocks: the Wapiti Formation, composed of volcanic breccia, poorly sorted volcanic breccia mudflows, and lava flows, and clearly shown in many places by inter lensing and intermixing of the calcibreccia with basal volcanic rocks. As the weight of volcanic overburden increased, the unstable water-saturated calcibreccia became mobile and semifluid and was injected upward as <span class="hlt">dikes</span> into the overlying volcanic rocks and to a lesser extent into rocks of the upper plate. In some places the lowermost part of the volcanic overburden appears to have flowed with the calcibreccia to form <span class="hlt">dike</span> like bodies of mixed volcanic rock and calcibreccia. One calcibreccia <span class="hlt">dike</span> even contains carbonized wood, presumably incorporated into unconsolidated calcibreccia on the surface of tectonic denudation and covered by volcanic rocks before moving upward with the <span class="hlt">dike</span>. Angular xenoliths of Precambrian rocks, enclosed in another calcibreccia <span class="hlt">dike</span> and in an adjoining dikelike mass of volcanic rock as well, are believed to have been torn from the walls of a vent and incorporated into the basal part of the Wapiti Formation overlying the clastic carbonate rock on the fault surface. Subsequently, some of these xenoliths were incorporated into the calcibreccia during the process of <span class="hlt">dike</span> <span class="hlt">intrusion</span>. Throughout the Heart Mountain fault area, the basal part of the upper-plate blocks or masses are brecciated, irrespective of the size of the blocks, more intensely at the base and in places</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033591','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033591"><span>Textural, mineralogical and stable isotope studies of hydrothermal alteration in the main sulfide <span class="hlt">zone</span> of the Great Dyke, Zimbabwe and the precious metals <span class="hlt">zone</span> of the Sonju Lake <span class="hlt">Intrusion</span>, Minnesota, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Li, C.; Ripley, E.M.; Oberthur, T.; Miller, J.D.; Joslin, G.D.</p> <p>2008-01-01</p> <p>Stratigraphic offsets in the peak concentrations of platinum-group elements (PGE) and base-metal sulfides in the main sulfide <span class="hlt">zone</span> of the Great Dyke and the precious metals <span class="hlt">zone</span> of the Sonju Lake <span class="hlt">Intrusion</span> have, in part, been attributed to the interaction between magmatic PGE-bearing base-metal sulfide assemblages and hydrothermal fluids. In this paper, we provide mineralogical and textural evidence that indicates alteration of base-metal sulfides and mobilization of metals and S during hydrothermal alteration in both mineralized <span class="hlt">intrusions</span>. Stable isotopic data suggest that the fluids involved in the alteration were of magmatic origin in the Great Dyke but that a meteoric water component was involved in the alteration of the Sonju Lake <span class="hlt">Intrusion</span>. The strong spatial association of platinum-group minerals, principally Pt and Pd sulfides, arsenides, and tellurides, with base-metal sulfide assemblages in the main sulfide <span class="hlt">zone</span> of the Great Dyke is consistent with residual enrichment of Pt and Pd during hydrothermal alteration. However, such an interpretation is more tenuous for the precious metals <span class="hlt">zone</span> of the Sonju Lake <span class="hlt">Intrusion</span> where important Pt and Pd arsenides and antimonides occur as inclusions within individual plagioclase crystals and within alteration assemblages that are free of base-metal sulfides. Our observations suggest that Pt and Pd tellurides, antimonides, and arsenides may form during both magmatic crystallization and subsolidus hydrothermal alteration. Experimental studies of magmatic crystallization and hydrothermal transport/deposition in systems involving arsenides, tellurides, antimonides, and base metal sulfides are needed to better understand the relative importance of magmatic and hydrothermal processes in controlling the distribution of PGE in mineralized layered <span class="hlt">intrusions</span> of this type. ?? Springer-Verlag 2007.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940016200&hterms=Hawaii+Kilauea+volcano&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DHawaii%2BKilauea%2Bvolcano','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940016200&hterms=Hawaii+Kilauea+volcano&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DHawaii%2BKilauea%2Bvolcano"><span>Thermal and rheological controls on magma migration in <span class="hlt">dikes</span>: Examples from the east rift <span class="hlt">zone</span> of Kilauea volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parfitt, E. A.; Wilson, L.; Pinkerton, H.</p> <p>1993-01-01</p> <p>Long-lived eruptions from basaltic volcanoes involving episodic or steady activity indicate that a delicate balance has been struck between the rate of magma cooling in the <span class="hlt">dike</span> system feeding the vent and the rate of magma supply to the <span class="hlt">dike</span> system from a reservoir. We describe some key factors, involving the relationships between magma temperature, magma rheology, and <span class="hlt">dike</span> geometry that control the nature of such eruptions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021588','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021588"><span>An ancient depleted mantle sample from a 42-Ma <span class="hlt">dike</span> in Montana: Constraints on persistence of the lithosphere during Eocene Magmatism</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dudas, F.O.; Harlan, S.S.</p> <p>1999-01-01</p> <p>Recent models for the Cenozoic tectonic evolution of the western margin of North America propose that delamination of ancient lithosphere accompanied asthenospheric upwelling, magmatism, and uplift subsequent to Laramide deformation. On the basis of the age of an alkaline <span class="hlt">dike</span> in south-central Montana, thermometry of mantle xenoliths from the <span class="hlt">dike</span>, and Sr, Nd, and Pb isotopic compositions of the <span class="hlt">dike</span> and a xenocryst, we show that refractory lithosphere, derived from ancient, depleted mantle, remained in place under the Wyoming Craton as late as 42 Ma. The Haymond School <span class="hlt">Dike</span>, a camptonite, yields a 40Ar/39Ar plateau date of 41.97 ?? 0.19 Ma (2??). Paleomagnetic data are consistent with this date and indicate <span class="hlt">intrusion</span> during chron C19r. The <span class="hlt">dike</span> has Sr, Nd, and Pb isotopic compositions similar to those of other Eocene alkaline rocks from central Montana. A clinopyroxene megacryst from the <span class="hlt">dike</span> has ??42 = 17, and 87Sr/86Sr = 0.70288, indicating that it derives from ancient, depleted mantle isotopically distinct from the source of the host camptonite. Thermometry of xenoliths from the <span class="hlt">dike</span> shows pyroxene populations that formed at 880?? and 1200??C. Combining thermometry with previous estimates of the regional Eocene geotherm inferred from xenoliths in kimberlites, and with the Al-in-orthopyroxene barometer, we infer that lithospheric mantle remained intact to depths of 110-150 km as late as 42 Ma. Eocene magmatism was not accompanied by complete removal of ancient lithosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026861','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026861"><span>Multi-stage origin of the Coast Range ophiolite, California: Implications for the life cycle of supra-subduction <span class="hlt">zone</span> ophiolites</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shervais, J.W.; Kimbrough, D.L.; Renne, P.; Hanan, B.B.; Murchey, B.; Snow, C.A.; Zoglman, Schuman M.M.; Beaman, J.</p> <p>2004-01-01</p> <p>The Coast Range ophiolite of California is one of the most extensive ophiolite terranes in North America, extending over 700 km from the northernmost Sacramento Valley to the southern Transverse Ranges in central California. This ophiolite, and other ophiolite remnants with similar mid-Jurassic ages, represent a major but short-lived episode of oceanic crust formation that affected much of western North America. The history of this ophiolite is important for models of the tectonic evolution of western North America during the Mesozoic, and a range of conflicting interpretations have arisen. Current petrologic, geochemical, stratigraphic, and radiometric age data all favor the interpretation that the Coast Range ophiolite formed to a large extent by rapid extension in the forearc region of a nascent subduction <span class="hlt">zone</span>. Closer inspection of these data, however, along with detailed studies of field relationships at several locales, show that formation of the ophiolite was more complex, and requires several stages of formation. Our work shows that exposures of the Coast Range ophiolite preserve evidence for four stages of magmatic development. The first three stages represent formation of the ophiolite above a nascent subduction <span class="hlt">zone</span>. Rocks associated with the first stage include ophiolite layered gabbros, a sheeted complex, and volcanic rocks vith arc tholeiitic or (roore rarely) low-K calc-alkaline affinities. The second stage is characterized by <span class="hlt">intrusive</span> wehrlite-clinopyroxenite complexes, <span class="hlt">intrusive</span> gabbros, Cr-rich diorites, and volcanic rocks with high-Ca boninitic or tholeiitic ankaramite affinities. The third stage includes diorite and quartz diorite plutons, felsic <span class="hlt">dike</span> and sill complexes, and calc-alkaline volcanic rocks. The first three stages of ophiolite formation were terminated by the <span class="hlt">intrusion</span> of mid-ocean ridge basalt <span class="hlt">dikes</span>, and the eruption of mid-ocean ridge basalt or ocean-island basalt volcanic suites. We interpret this final magmatic event (MORB</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGP43B0982V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGP43B0982V"><span>Paleomagnetism and Geochronology of the Precambrian <span class="hlt">Dikes</span> in NE Fennoscandia, Kola Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Veselovskiy, R. V.; Samsonov, A.; Stepanova, A.</p> <p>2017-12-01</p> <p>Paleomagnetism of Proterozoic <span class="hlt">dikes</span> of Scandinavia, Karelia, and southern part of the Kola Peninsula is extensively explored in many studies (Veikkolainen et al., 2014). In particular, the paleomagnetism of <span class="hlt">intrusive</span> formations in the southern part of the Kola Peninsula is thoroughly scrutinized in the study authored by Alexey Khramov and his colleagues (Khramov et al., 1997). However, information about the systematic paleomagnetic studies of the Archaean and Proterozoic <span class="hlt">dikes</span> of the Central Kola block and, especially, Murmansk block are absent. Based on the results of preliminary paleomagnetic investigation of 57 Precambrian <span class="hlt">dikes</span> of the Kola Peninsula, in 31 of them a stable monopolar component of natural remanent magnetization is revealed. The peculiarities of distribution of this magnetization component within the Kola Peninsula and the rock magnetic characteristics of the <span class="hlt">dikes</span> in which this component is isolated suggest its secondary nature and relate the mechanism and formation time to the remagnetization processes which took place in the northwest of Fennoscandia about 1.8 Ga during the Svecofennian orogeny. The corresponding geomagnetic pole of Fennoscandia is located in the immediate vicinity of the known Paleoproterozoic (1.9-1.7 Ga) poles of Baltica (Khramov et al., 1997; Veikkolainen et al., 2014). We also present the new geochronological Ar/Ar, Sm-Nd, Rb-Sr and U-Pb data which allow to determine the age of remagnetization as 1.86 Ga. The studies were supported by the Russian Science Foundation (project no. 16-17-10260), partially supported by the Russian Federation Government (project no. 14.Z50.31.0017) and Russian Foundation for Basic Research (project no. 17-05-01121a).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.V43I..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.V43I..04H"><span>Evidence of Tectonic Rotations and Magmatic Flow Within the Sheeted <span class="hlt">Dike</span> Complex of Super-Fast Spread Crust Exposed at the Pito Deep Rift</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horst, A. J.; Varga, R. J.; Gee, J. S.; Karson, J. A.</p> <p>2008-12-01</p> <p>Escarpments bounding the Pito Deep Rift expose cross-sections into ~3 Ma oceanic crust accreted at a super-fast spreading (>140 mm/yr) segment of the East Pacific Rise (EPR). <span class="hlt">Dikes</span> within the sheeted <span class="hlt">dike</span> complex persistently strike NE, parallel to local abyssal hill lineaments and magnetic anomaly stripes, and dip SE, outward and away from the EPR. During the Pito Deep 2005 Cruise, both ALVIN and JASON II used the Geocompass to fully orient a total of 69 samples [63 basaltic <span class="hlt">dikes</span>, 6 massive gabbros] collected in situ. Paleomagnetic analyses of these oriented samples provide a quantitative constraint of kinematics of structural rotations of <span class="hlt">dikes</span>. Magnetic remanence of <span class="hlt">dike</span> samples indicates a dominant normal polarity with almost all directions rotated clockwise from the expected direction. The most geologically plausible model to account for these dispersions using these data coupled with the general orientation of the <span class="hlt">dikes</span> incorporates two different structural rotations: 1) A horizontal-axis rotation that occurred near the EPR axis, related to sub-axial subsidence, and 2) A clockwise vertical-axis rotation, associated with the rotation of the Easter microplate consistent with current models. Additionally, the anisotropy of magnetic susceptibility (AMS) of <span class="hlt">dike</span> samples indicates rock fabric and magmatic flow direction within <span class="hlt">dikes</span>. In most samples, two of three AMS eigenvectors lie near the <span class="hlt">dike</span> plane orientations. Generally, Kmin lies perpendicular to <span class="hlt">dike</span> planes, while Kmax is often shallow within the <span class="hlt">dike</span> planes, indicating dominantly subhorizontal magma flow. Steep Kmax in a few samples indicates vertical flow directions that suggest either primary flow or gravitational back-flow during waning stages of <span class="hlt">dike</span> <span class="hlt">intrusion</span>. These results provide the first direct evidence for primarily horizontal magma flow in sheeted <span class="hlt">dikes</span> of super-fast spread oceanic crust. Results for Pito Deep Rift and previous results for Hess Deep Rift reveal outward dipping <span class="hlt">dikes</span> that are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T31B1812A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T31B1812A"><span>Unique Tremor observed coincident with the major emplacement phase of the September 2005 <span class="hlt">dike</span> in Afar, Ethiopia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ayele, A.; Keir, D.; Wright, T. J.; Ebinger, C. J.; Stuart, G. W.; Neuberg, J.</p> <p>2009-12-01</p> <p>The advent of digital and broadband seismic stations helped to capture the complex dynamics of earthquakes and volcanic sources processes ranging from high frequency microfractures to ultra long period transient signals. The September 2005 <span class="hlt">dike</span> in the Afar depression of Ethiopia demonstrated to be one of the rare events of its kind to demonstrate the complex interaction of ambient tectonic stress, volcanic processes and <span class="hlt">dike</span> <span class="hlt">intrusions</span>. Unusually long period tremor in the range 18-20 seconds is observed by seismic stations located from ~ 350-700 km distance on 25 September, 2006 at about 14:00:00 GMT. This tremor sustain for about 30 minutes at FURI station. This time is coincident with the major emplacement phase of the <span class="hlt">dike</span> beneath the Ado Ale Volcanic Complex (AVC before the small felsic eruption at Da’Ure in the afternoon of September 26, 2005. This tremor sustain for about 30 minutes at FURI station. The preliminary interpretation of this observation is postulated to be a highly pressurized magma source/reservoir breaking into the channel and its interaction with its deformable rock walls.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1954/0014/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1954/0014/report.pdf"><span>Fusion of arkosic sand by <span class="hlt">intrusive</span> andesite</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bailey, Roy A.</p> <p>1954-01-01</p> <p>An andesite <span class="hlt">dike</span> in the Valles Mountains of northern New Mexico has intruded and partly fused arkosic sediments for a distance of 50 feet from its contacts. The <span class="hlt">dike</span> is semi-circular in form, has a maximum width of about 100 feet, and is about 500 feet long. Small associated arcuate <span class="hlt">dikes</span> are arranged in spiral fashion around the main <span class="hlt">dike</span>, suggesting that they were intruded along shear fractures similar to those described by Burbank (1941). The fused rocks surrounding the andesite <span class="hlt">dike</span> are of three general types: 1) partly fused arkosic sand, 2) fused clay, and 3) hybrid rocks. The fused arkosic sand consists of relict detrital grains of quartz, orthoclose, and plagioclase, imbedded in colorless glass containing microlites of tridymite, cordierite, and magnetite. The relict quartz grains are corroded and embayed by glass; the orthoclase is sanidinized and partly fused; and the plagioclase is inverted to the high temperature form and is partly fused. The fused clay, which was originally a mixture of montmorillonite and hydromica, consists primarily of cordierite but also contains needle-like crystals of sillimanite (?) or mullite (?). The hybrid rocks originated in part by intermixing of fused arkosic sediments and andesitic liquid and in part by diffusion of mafic constituents through the fused sediments. They are rich in cordierite and magnetite and also contain hypersthene, augite, and plagioclase. The composition of pigeonite in the andesite indicates that the temperature of the andesite at the time of <span class="hlt">intrusion</span> probably did not exceed 1200?C. Samples of arkosic sand were fused in the presence of water in a Morey bomb at 1050?C. Stability relations of certain minerals in the fused sand suggest that fusion may have taken place at a lower temperature, however, and the fluxing action of volatiles from the andesite are thought to have made this possible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUSM.V14A..06C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUSM.V14A..06C"><span>Future Volcanism at Yucca Mountain - Statistical Insights from the Non-Detection of Basalt <span class="hlt">Intrusions</span> in the Potential Repository</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coleman, N.; Abramson, L.</p> <p>2004-05-01</p> <p> upper-bound probability of 2E-7/yr (95% conf. level) for an igneous <span class="hlt">intrusion</span> over the next 1E4 yrs. If we assume one undiscovered <span class="hlt">dike</span> exists, the upper-bound probability would rise to 4E-7/yr. Higher probabilities may be possible if conditions that fostered Plio-Quaternary volcanism became enhanced over time. To the contrary, basalts of the past 11 Ma in Crater Flat have erupted in four episodes that together show a declining trend in erupted magma volume (DOE, TBD13, 2003). Smith et al (GSA Today, 2002) suggest there may be a common magma source for volcanism in Crater Flat and the Lunar Crater volcanic field, and that recurrence rates for YM could be underestimated. Their interpretation is highly speculative given the 130-km (80-mi) distance between these <span class="hlt">zones</span>. A claim that crustal extension at YM is anomalously large, possibly favoring renewed volcanism (Wernicke et al, Science, 1999), was contradicted by later work (Savage et al, JGR, 2000). Spatial-temporal models that predict future <span class="hlt">intrusion</span> probabilities of >2E-7/yr may be overly conservative and unrealistic. Along with currently planned site characterization activities, realistic models could be developed by considering the non-detection of basaltic <span class="hlt">dikes</span> in the potential repository footprint. (The views expressed are the authors' and do not reflect any final judgment or determination by the Advisory Committee on Nuclear Waste or the Nuclear Regulatory Commission regarding the matters addressed or the acceptability of a license application for a geologic repository at Yucca Mt.)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010CoMP..160..683F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010CoMP..160..683F"><span>Hydrous partial melting in the sheeted <span class="hlt">dike</span> complex at fast spreading ridges: experimental and natural observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>France, Lydéric; Koepke, Juergen; Ildefonse, Benoit; Cichy, Sarah B.; Deschamps, Fabien</p> <p>2010-11-01</p> <p>In ophiolites and in present-day oceanic crust formed at fast spreading ridges, oceanic plagiogranites are commonly observed at, or close to the base of the sheeted <span class="hlt">dike</span> complex. They can be produced either by differentiation of mafic melts, or by hydrous partial melting of the hydrothermally altered sheeted <span class="hlt">dikes</span>. In addition, the hydrothermally altered base of the sheeted <span class="hlt">dike</span> complex, which is often infiltrated by plagiogranitic veins, is usually recrystallized into granoblastic <span class="hlt">dikes</span> that are commonly interpreted as a result of prograde granulitic metamorphism. To test the anatectic origin of oceanic plagiogranites, we performed melting experiments on a natural hydrothermally altered <span class="hlt">dike</span>, under conditions that match those prevailing at the base of the sheeted <span class="hlt">dike</span> complex. All generated melts are water saturated, transitional between tholeiitic and calc-alkaline, and match the compositions of oceanic plagiogranites observed close to the base of the sheeted <span class="hlt">dike</span> complex. Newly crystallized clinopyroxene and plagioclase have compositions that are characteristic of the same minerals in granoblastic <span class="hlt">dikes</span>. Published silicic melt compositions obtained in classical MORB fractionation experiments also broadly match the compositions of oceanic plagiogranites; however, the compositions of the coexisting experimental minerals significantly deviate from those of the granoblastic <span class="hlt">dikes</span>. Our results demonstrate that hydrous partial melting is a likely common process in the root <span class="hlt">zone</span> of the sheeted <span class="hlt">dike</span> complex, starting at temperatures exceeding 850°C. The newly formed melt can either crystallize to form oceanic plagiogranites or may be recycled within the melt lens resulting in hybridized and contaminated MORB melts. It represents the main MORB crustal contamination process. The residue after the partial melting event is represented by the granoblastic <span class="hlt">dikes</span>. Our results support a model with a dynamic melt lens that has the potential to trigger hydrous partial melting</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V53A3071L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V53A3071L"><span>Inflation and Collapse of the Wai'anae Volcano (Oahu,Hawaii, USA):Insights from Magnetic Fabric Studies of <span class="hlt">Dikes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lau, J. K. S.; Herrero-Bervera, E.; Moreira, M. A. D. A.</p> <p>2016-12-01</p> <p>The Waianae Volcano is the older of two shield volcanoes that make up the island of Oahu. Previous age determinations suggest that the subaerial portion of the edifice erupted between approximately 3.7 and 2.7 Ma. The eroded Waianae Volcano had a well-developed caldera centered near the back of its two most prominent valleys and two major rift <span class="hlt">zones</span>: a prominent north-west rift <span class="hlt">zone</span>, well-defined by a complex of sub-parallel <span class="hlt">dikes</span> trending approximately N52W, and a more diffuse south rift <span class="hlt">zone</span> trending between S20W to due South. In order to investigate the volcanic evolution, the plumbing and the triggering mechanisms of the catastrophic mass wasting that had occurred in the volcano, we have undertaken an AMS study of 7 <span class="hlt">dikes</span> from the volcano. The width of the <span class="hlt">dikes</span> ranged between 0.5 to 4 m. Low-field susceptibility versus temperature (k-T) and SIRM experiments were able to identify magnetite at 575 0C and at about 250-300 0C, corresponding to titanomagnetite.. Magnetic fabric studies of the <span class="hlt">dikes</span> along a NW-SE section across the present southwestern part of the Waianae volcano have been conducted. The flow direction was studied using the imbrication angle between the <span class="hlt">dike</span> walls and the magnetic foliation. The flow direction has been obtained in the 7 studied <span class="hlt">dikes</span>. For the majority of the cases, the maximum axis, K1, appears to be perpendicular to the flow direction, and in some cases, with a permutation with respect to the intermediate axis, K2, or even with respect to the minimum axis, K3. In addition, in one of the sites studied, the minimum axis, K3, is very close to the flow direction. In all cases, the magma flowed along a direction with a moderate plunge. For six of the <span class="hlt">dikes</span>, the interpreted flow was from the internal part of the volcano towards the volcano border, and corresponds probably to the inflation phase of the volcano. In two cases (<span class="hlt">dikes</span> located on the northwestern side of the volcano), the flow is slightly downwards, possibly related to the</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tecto..37..705G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tecto..37..705G"><span><span class="hlt">Intrusion</span> of Magmatic Bodies Into the Continental Crust: 3-D Numerical Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gorczyk, Weronika; Vogt, Katharina</p> <p>2018-03-01</p> <p>Magma <span class="hlt">intrusion</span> is a major material transfer process in the Earth's continental crust. Yet the mechanical behavior of the intruding magma and its host are a matter of debate. In this study we present a series of numerical thermomechanical simulations on magma emplacement in 3-D. Our results demonstrate the response of the continental crust to magma <span class="hlt">intrusion</span>. We observe change in <span class="hlt">intrusion</span> geometries between <span class="hlt">dikes</span>, cone sheets, sills, plutons, ponds, funnels, finger-shaped and stock-like <span class="hlt">intrusions</span>, and injection time. The rheology and temperature of the host are the main controlling factors in the transition between these different modes of <span class="hlt">intrusion</span>. Viscous deformation in the warm and deep crust favors host rock displacement and plutons at the crust-mantle boundary forming deep-seated plutons or magma ponds in the lower to middle crust. Brittle deformation in the cool and shallow crust induces cone-shaped fractures in the host rock and enables emplacement of finger- or stock-like <span class="hlt">intrusions</span> at shallow or intermediate depth. Here the passage of magmatic and hydrothermal fluids from the <span class="hlt">intrusion</span> through the fracture pattern may result in the formation of ore deposits. A combination of viscous and brittle deformation forms funnel-shaped <span class="hlt">intrusions</span> in the middle crust. <span class="hlt">Intrusion</span> of low-density magma may more over result in T-shaped <span class="hlt">intrusions</span> in cross section with magma sheets at the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019277','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019277"><span>Inflation of Long Valley caldera, California, Basin and Range strain, and possible Mono Craters <span class="hlt">dike</span> opening from 1990-94 GPS surveys</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Marshall, G.A.; Langbein, J.; Stein, R.S.; Lisowski, M.; Svarc, J.</p> <p>1997-01-01</p> <p>Five years of annual Global Positioning System (GPS) surveys of a network centered on Long Valley, California, constrain displacement rates for these stations relative to a central station in the network. These observations are consistent with recent models of resurgent dome inflation in Long Valley (Langbein et al., 1995) and have sufficient signal to detect the presence of Basin and Range strain in the Long Valley region. The data also allow for the possibility of <span class="hlt">dike</span> inflation beneath the Mono Craters; <span class="hlt">dike</span> <span class="hlt">intrusion</span> is consistent with the Mono Craters' recent geologic history of ash eruptions, with seismic tomography, leveling data, and geologic studies of these volcanic domes and flows. Copyright 1997 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.T43A1978B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.T43A1978B"><span>Strain distribution across magmatic margins during the breakup stage: Seismicity patterns in the Afar rift <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brown, C.; Ebinger, C. J.; Belachew, M.; Gregg, T.; Keir, D.; Ayele, A.; Aronovitz, A.; Campbell, E.</p> <p>2008-12-01</p> <p>Fault patterns record the strain history along passive continental margins, but geochronological constraints are, in general, too sparse to evaluate these patterns in 3D. The Afar depression in Ethiopia provides a unique setting to evaluate the time and space relations between faulting and magmatism across an incipient passive margin that formed above a mantle plume. The margin comprises a high elevation flood basalt province with thick, underplated continental crust, a narrow fault-line escarpment underlain by stretched and intruded crust, and a broad <span class="hlt">zone</span> of highly intruded, mafic crust lying near sealevel. We analyze fault and seismicity patterns across and along the length of the Afar rift <span class="hlt">zone</span> to determine the spatial distribution of strain during the final stages of continental breakup, and its relation to active magmatism and <span class="hlt">dike</span> <span class="hlt">intrusions</span>. Seismicity data include historic data and 2005-2007 data from the collaborative US-UK-Ethiopia Afar Geodynamics Project that includes the 2005-present Dabbahu rift episode. Earthquake epicenters cluster within discrete, 50 km-long magmatic segments that lack any fault linkage. Swarms also cluster along the fault-line scarp between the unstretched and highly stretched Afar rift <span class="hlt">zone</span>; these earthquakes may signal release of stresses generated by large lateral density contrasts. We compare Coulomb static stress models with focal mechanisms and fault kinematics to discriminate between segmented magma <span class="hlt">intrusion</span> and crank- arm models for the central Afar rift <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033092','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033092"><span>Origin of the Lyme Dome and implications for the timing of multiple Alleghanian deformational and <span class="hlt">intrusive</span> events in southern Connecticut</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Walsh, G.J.; Aleinikoff, J.N.; Wintsch, R.P.</p> <p>2007-01-01</p> <p>Geologic mapping, structural analysis, and geochronology in the area of the Lyme dome, southern Connecticut provides constraints on the origin of the rocks in the core of the dome, the absolute timing of the principal deformational and thermal events attributed to Alleghanian orogenesis, and the processes that generated the dome. Detrital zircon geochronology in combination with ages on <span class="hlt">intrusive</span> rocks brackets the deposition of quartzite in the core of the dome sometime between ca. 925 and 620 Ma. Granite and granodiorite intruded the Neoproteorozic metasedimentary rocks in the core of the dome at ca. 620 to 610 Ma. Four major early Permian events associated with the Alleghanian orogeny affected the rocks in the Lyme dome area. Syn-tectonic migmatization and widespread penetrative deformation (D1, ca. 300 - 290 Ma) included emplacement of alaskite at 290 ?? 4 Ma during regional foliation development and aluminosilicate-orthoclase metamorphic conditions. Rocks of the Avalon terrane may have wedged between Gander cover rocks and Gander basement in the core of the Lyme during D1. Limited structural evidence for diapiric uplift of the Lyme dome indicates that diapirism started late in D1 and was completed by D2 (ca. 290 - 280 Ma) when horizontal WNW contractional stresses dominated over vertical stresses. Second sillimanite metamorphism continued and syn-tectonic D2 granite pegmatite (288 ?? 4 Ma) and the Joshua Rock Granite Gniess (284 ?? 3 Ma) intruded at this time. North-northwest extension during D3 (ca. 280 - 275 Ma) led to granitic pegmatite <span class="hlt">intrusion</span> along S3 cleavage planes and in extensional <span class="hlt">zones</span> in boudin necks during hydraulic failure and decompression melting. <span class="hlt">Intrusion</span> of a Westerly Granite <span class="hlt">dike</span> at 275 ?? 4 Ma suggests that D3 extension was active, and perhaps concluding, by ca. 275 Ma. Late randomly oriented but gently dipping pegmatite <span class="hlt">dikes</span> record a final stage of <span class="hlt">intrusion</span> during D4 (ca. 275 - 260 Ma), and a switch from NNW extension to vertical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004JGRB..109.2410O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004JGRB..109.2410O"><span>Creep, <span class="hlt">dike</span> <span class="hlt">intrusion</span>, and magma chamber deflation model for the 2000 Miyake eruption and the Izu islands earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ozawa, S.; Miyazaki, S.; Nishimura, T.; Murakami, M.; Kaidzu, M.; Imakiire, T.; Ji, X.</p> <p>2004-02-01</p> <p>Analysis of Global Positioning System data shows shrinkage of Miyake Island and the widening between Nijima and Kozu Islands during the period of the Miyake island volcanic activity and the ensuing Izu islands earthquakes in 2000. The estimated time evolution of a model consisting of a <span class="hlt">dike</span>, creeping faults, and a Mogi source suggests that a crack opening on Miyake Island occurred immediately after the start of the seismic activities on 26 June and ended within several days at the west coast of Miyake Island. After the seabed eruption on 27 June, magma migrated from Miyake Island to Kozu and Nijima Islands within several days. The estimated volume of intruded magma totals around 1.2 × 109 m3. Associated with the magma <span class="hlt">intrusion</span> between Miyake and Kozu Islands, left-lateral and right-lateral creep motions occurred in regions off the west coast of Miyake Island and near Kozu Island. The accumulated moment energy is equivalent to an earthquake of Mw 6.6 and 6.6 for right-lateral and left-lateral creeping faults, respectively. The estimated magma chamber continued deflation beneath the southwestern part of Miyake Island from 26 June, totaling around 0.12 × 109 m3 in volume change, in addition to the collapse volume of 0.6 × 109 m3 at the summit of Mount Oyama on Miyake Island. The volume change on Miyake Island can be compensated by the migrated magma toward Kozu Island from the deflation source beneath Miyake Island. The deflation speed of the magma chamber beneath Miyake Island decreased and increased before and after the eruption of 14-15 July and 18 August, suggesting a change in balance of mass influx and draining out rate of the magma chamber.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036672','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036672"><span>Episodic <span class="hlt">intrusion</span>, internal differentiation, and hydrothermal alteration of the miocene tatoosh <span class="hlt">intrusive</span> suite south of Mount Rainier, Washington</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>du Bray, E.A.; Bacon, C.R.; John, D.A.; Wooden, J.L.; Mazdab, F.K.</p> <p>2011-01-01</p> <p>The Miocene Tatoosh <span class="hlt">intrusive</span> suite south of Mount Rainier is composed of three broadly granodioritic plutons that are manifestations of ancestral Cascades arc magmatism. Tatoosh <span class="hlt">intrusive</span> suite plutons have individually diagnostic characteristics, including texture, mineralogy, and geochemistry, and apparently lack internal contacts. New ion-microprobe U-Pb zircon ages indicate crystallization of the Stevens pluton ca. 19.2 Ma, Reflection-Pyramid pluton ca. 18.5 Ma, and Nisqually pluton ca. 17.5 Ma. The Stevens pluton includes rare, statistically distinct ca. 20.1 Ma zircon antecrysts. Wide-ranging zircon rare earth element (REE), Hf, U, and Th concentrations suggest late crystallization from variably evolved residual liquids. Zircon Eu/Eu*-Hf covariation is distinct for each of the Reflection-Pyramid, Nisqually, and Stevens plutons. Although most Tatoosh <span class="hlt">intrusive</span> suite rocks have been affected by weak hydrothermal alteration, and sparse mineralized veins cut some of these rocks, significant base or precious metal mineralization is absent. At the time of shallow emplacement, each of these magma bodies was largely homogeneous in bulk composition and petrographic features, but, prior to final solidification, each of the Tatoosh <span class="hlt">intrusive</span> suite plutons developed internal compositional variation. Geochemical and petrographic trends within each pluton are most consistent with differential loss of residual melt, possibly represented by late aplite <span class="hlt">dikes</span> or erupted as rhyolite, from crystal-rich magma. Crystal-rich magma that formed each pluton evidently accumulated in reservoirs below the present level of exposure and then intruded to a shallow depth. Assembled by episodic <span class="hlt">intrusion</span>, the Tatoosh <span class="hlt">intrusive</span> suite may be representative of midsized composite plutonic complexes beneath arc volcanoes. ?? 2011 Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22803455','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22803455"><span>[Estimation of spur <span class="hlt">dike</span>-affected fish habitat area].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ray-Shyan, Wu; Yan-Ru, Chen; Yi-Liang, Ge</p> <p>2012-04-01</p> <p>Based on the HEC-RAS and River 2D modes, and taking 5% change rate of weighted usable area (WUA) as the threshold to define the spur <span class="hlt">dike</span>- affected area of target fish species Acrossocheilus paradoxus in Fazi River in Taiwan, this paper studied the affected area of the fish habitat by spur <span class="hlt">dike</span>, and, in combining with the references about the installations of spur <span class="hlt">dikes</span> in Taiwan in recent 10 years, analyzed the relative importance of related affecting factors such as <span class="hlt">dike</span> height, <span class="hlt">dike</span> length (water block rate), average slope gradient of river way, single or double spur <span class="hlt">dike</span>, and flow discharge. In spite of the length of the <span class="hlt">dike</span>, the affected area in downstream was farther, and was about 2-6 times as large as that in upstream. The ratio of the affected area in downstream / upstream decreased with increasing slope gradient, but increased with increasing <span class="hlt">dike</span> length and flow discharge. When the discharge was approximate to 10 years return periods, the ratio of the affected area would be close to a constant of 2. Building double spur <span class="hlt">dike</span> would produce a better WUA than building single spur <span class="hlt">dike</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH11A0090M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH11A0090M"><span>The Experiences and Challenges in Drilling into Semi molten or Molten <span class="hlt">Intrusive</span> in Menengai Geothermal Field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mortensen, A. K.; Mibei, G. K.</p> <p>2017-12-01</p> <p>Drilling in Menengai has experienced various challenges related to drilling operations and the resource itself i.e. quality discharge fluids vis a vis gas content. The main reason for these challenges is related to the nature of rocks encountered at depths. <span class="hlt">Intrusives</span> encountered within Menengai geothermal field have been group into three based on their geological characteristics i.e. S1, S2 and S3.Detailed geology and mineralogical characterization have not been done on these <span class="hlt">intrusive</span> types. However, based on physical appearances, S1 is considered as a diorite <span class="hlt">dike</span>, S2 is syenite while S3 is molten rock material. This paper summarizes the experiences in drilling into semi molten or molten <span class="hlt">intrusive</span> (S3).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008GGG.....9.5O07H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008GGG.....9.5O07H"><span>Role of upwelling hydrothermal fluids in the development of alteration patterns at fast spreading ridges: Evidence from the sheeted <span class="hlt">dike</span> complex at Pito Deep</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heft, Kerri L.; Gillis, Kathryn M.; Pollock, Megan A.; Karson, Jeffery A.; Klein, Emily M.</p> <p>2008-05-01</p> <p>Alteration of sheeted <span class="hlt">dikes</span> exposed along submarine escarpments at the Pito Deep Rift (NE edge of the Easter microplate) provides constraints on the crustal component of axial hydrothermal systems at fast spreading mid-ocean ridges. Samples from vertical transects through the upper crust constrain the temporal and spatial scales of hydrothermal fluid flow and fluid-rock reaction. The <span class="hlt">dikes</span> are relatively fresh (average extent of alteration is 27%), with the extent of alteration ranging from 0 to >80%. Alteration is heterogeneous on scales of tens to hundreds of meters and displays few systematic spatial trends. Background alteration is amphibole-dominated, with chlorite-rich <span class="hlt">dikes</span> sporadically distributed throughout the <span class="hlt">dike</span> complex, indicating that peak temperatures ranged from <300°C to >450°C and did not vary systematically with depth. <span class="hlt">Dikes</span> locally show substantial metal mobility, with Zn and Cu depletion and Mn enrichment. Amphibole and chlorite fill fractures throughout the <span class="hlt">dike</span> complex, whereas quartz-filled fractures and faults are only locally present. Regional variability in alteration characteristics is found on a scale of <1-2 km, illustrating the diversity of fluid-rock interaction that can be expected in fast spreading crust. We propose that much of the alteration in sheeted <span class="hlt">dike</span> complexes develops within broad, hot upwelling <span class="hlt">zones</span>, as the inferred conditions of alteration cannot be achieved in downwelling <span class="hlt">zones</span>, particularly in the shallow <span class="hlt">dikes</span>. Migration of circulating cells along rides axes and local evolution of fluid compositions produce sections of the upper crust with a distinctive character of alteration, on a scale of <1-2 km and <5-20 ka.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.479..108X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.479..108X"><span>Disequilibrium growth of olivine in mafic magmas revealed by phosphorus <span class="hlt">zoning</span> patterns of olivine from mafic-ultramafic <span class="hlt">intrusions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xing, Chang-Ming; Wang, Christina Yan; Tan, Wei</p> <p>2017-12-01</p> <p>Olivine from mafic-ultramafic <span class="hlt">intrusions</span> rarely displays growth <span class="hlt">zoning</span> in major and some minor elements, such as Fe, Mg and Ni, due to fast diffusion of these elements at high temperatures. These elements in olivine are thus not useful in deciphering magma chamber processes, such as magma convection, multiple injection and mixing. High-resolution X-ray elemental intensity mapping reveals distinct P <span class="hlt">zoning</span> patterns of olivine from two mafic-ultramafic <span class="hlt">intrusions</span> in SW China. Polyhedral olivine grains from lherzolite and dunite of the Abulangdang <span class="hlt">intrusion</span> show P-rich dendrites similar to those observed in volcanic rocks. Rounded olivine grains from net-textured Fe-Ti oxide ores of the Baima layered <span class="hlt">intrusion</span> have irregular P-rich patches/bands crosscut and interlocked by P-poor olivine domains. P-rich patches/bands contain 250 to 612 ppm P, much higher than P-poor olivine domains with 123 to 230 ppm P. In electron backscattered diffraction (EBSD) maps, P-rich patches/bands within a single olivine grain have the same crystallographic orientation, indicating that they were remnants of the same crystal. Thus, both P-rich patches/bands and P-poor olivine domains in the same grain show a disequilibrium texture and clearly record two-stage growth. The P-rich patches/bands are likely the remnants of a polyhedral olivine crystal that formed in the first stage, whereas the P-poor olivine domains containing rounded Ti-rich magnetite and Fe-rich melt inclusions may have formed from an Fe-rich ambient melt in the second stage. The complex P <span class="hlt">zoning</span> of olivine can be attributed to the dissolution of early polyhedral olivine and re-precipitation from the Fe-rich ambient melt. The early polyhedral olivine was in chemical disequilibrium with the ambient melt that may have been developed by silicate liquid immiscibility in a crystal mush. Our study implies that olivine crystals in igneous cumulates with an equilibrium appearance may have experienced disequilibrium growth processes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1041/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1041/report.pdf"><span><span class="hlt">Intrusive</span> rocks northeast of Steamboat Springs, Park Range, Colorado, with a section on geochronology</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Snyder, George L.; Hedge, Carl E.</p> <p>1978-01-01</p> <p>Major Precambrian and minor Tertiary <span class="hlt">intrusive</span> rocks northeast of Steamboat Springs in the Park Range between 40?30' and 40?45' N. lat. are described and compared with related rocks elsewhere in Colorado and Wyoming. The Precambrian <span class="hlt">intrusives</span> were emplaced in a sequence of high-grade interlayered felsic gneisses, amphibolites, and pelitic schists of sedimentary and volcanic origin. These rocks are cut by a major northeast-trending Precambrian shear <span class="hlt">zone</span> where mainly left lateral movement of 1/ 2 to 1 mile is certain. Cumulative movement of many miles is possible. The Precambrian <span class="hlt">intrusives</span> consist of a batholith, the Mount Ethel pluton, a smaller Buffalo Pass pluton, and small <span class="hlt">dikes</span> or lenses of fine-grained porphyry, pegmatites, and ultramafics. The Mount Ethel pluton is an oval shaped body 7 miles wide by about 40 miles long (shown by geophysical data to extend beneath younger sediments in North Park). Outer batholithic contacts are sharp and dip steeply outward at about 85?. Five mappable internal variants consist, in order of decreasing age, of granodiorite, quartz monzonite porphyry of Rocky Peak, quartz monzonite of Roxy Ann Lake, granite and quartz monzonite, and. leucogranite. Internal contacts between these plutonic variants are sharp, and evidence of liquid-solid relationships abounds; despite this, all rocks except the granodiorite contribute to an Rb-Sr whole-rock isochron indicating emplacement about 1.4 b.y. (billion years) ago. The most important variants volumetrically are: the quartz monzonite porphyry of Rocky Peak, which forms an irregular 2-mile-thick carapace or mapped band around the west edge of the pluton and is lithologically similar to nearby Sherman Granite, and the quartz monzonite of Roxy Ann Lake, which forms most of the rest of the pluton and is lithologically similar to Silver Plume Granite. An apparent Sherman -Silver Plume dichotomy with similar rock types and similar relative ages is noted throughout Colorado plutons of that age</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011Tectp.500...65M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011Tectp.500...65M"><span>Growth of plutons by incremental emplacement of sheets in crystal-rich host: Evidence from Miocene <span class="hlt">intrusions</span> of the Colorado River region, Nevada, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, Calvin F.; Furbish, David J.; Walker, Barry A.; Claiborne, Lily L.; Koteas, G. Christopher; Bleick, Heather A.; Miller, Jonathan S.</p> <p>2011-03-01</p> <p>Growing evidence supports the notion that plutons are constructed incrementally, commonly over long periods of time, yet field evidence for the multiple injections that seem to be required is commonly sparse or absent. Timescales of up to several million years, among other arguments, indicate that the dominant volume does not remain largely molten, yet if growing plutons are constructed from rapidly solidifying increments it is unlikely that <span class="hlt">intrusive</span> contacts would escape notice. A model wherein magma increments are emplaced into melt-bearing but crystal-rich host, rather than either solid or crystal-poor material, provides a plausible explanation for this apparent conundrum. A partially solidified <span class="hlt">intrusion</span> undoubtedly comprises <span class="hlt">zones</span> with contrasting melt fraction and therefore strength. Depending on whether these <span class="hlt">zones</span> behave elastically or ductilely in response to <span class="hlt">dike</span> emplacement, intruding magma may spread to form sheets by either of two mechanisms. If the melt-bearing host is elastic on the relevant timescale, magma spreads rather than continuing to propagate upward, where it encounters a <span class="hlt">zone</span> of higher rigidity (higher crystal fraction). Similarly, if the <span class="hlt">dike</span> at first ascends through rigid, melt-poor material and then encounters a <span class="hlt">zone</span> that is weak enough (poor enough in crystals) to respond ductilely, the ascending material will also spread because the <span class="hlt">dike</span> tip ceases to propagate as in rigid material. We propose that ascending magma is thus in essence trapped, by either mechanism, within relatively crystal-poor <span class="hlt">zones</span>. Contacts will commonly be obscure from the start because the contrast between intruding material (crystal-poorer magma) and host (crystal-richer material) is subtle, and they may be obscured even further by subsequent destabilization of the crystal-melt framework. Field evidence and zircon <span class="hlt">zoning</span> stratigraphy in plutons of the Colorado River region of southern Nevada support the hypothesis that emplacement of magma replenishments into a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.V43D2880M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.V43D2880M"><span>Mushy magma processes in the Tuolumne <span class="hlt">intrusive</span> complex, Sierra Nevada, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Memeti, V.; Paterson, S. R.</p> <p>2012-12-01</p> <p> whole rock data. 4) Single mineral geochemistry suggests that this increased heterogeneity in the interior of the complex is likely caused by the presence of mixed mineral populations that acquired their compositional <span class="hlt">zoning</span> in magmas different than the one they most recently crystallized in. 5) Mixed mineral populations have also been found in places of local magma mixing (e.g., tubes and troughs), and 6) oscillatory trace element <span class="hlt">zoning</span> in K-feldspar phenocrysts most likely represents magma replenishment. All of these phenomena suggest a fairly dynamic environment of magma replenishment, magmatic erosion and extensive mixing at the locus of chamber growth. Magma replenishment subsided after episodic flare-ups and the magma mush dominantly underwent fractional crystallization and magmatic fabric formation during waning stages, when it was capable of preserving the evidence at map to crystal scale, lacking any later overprint by mixing. Fractionation related evidence is apparent in the presence of 1) map to outcrop scale leucogranite lenses and <span class="hlt">dikes</span> in all major Tuolumne units (including the Johnson Peak granite itself), 2) the concentric compositional zonation of magmatic lobes (e.g., southern Half Dome lobe), 3) local crystal accumulations and widespread schlieren, and 4) fractionation related single mineral element <span class="hlt">zoning</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JSAES..32..183C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JSAES..32..183C"><span>Reassessment of the volume of the Las Aguilas mafic-ultramafic <span class="hlt">intrusives</span>, San Luis, Argentina, based on an alternative geophysical model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Claudia, Zaffarana; Silvana, Geuna; Stella, Poma; Alberto, Patiño Douce</p> <p>2011-10-01</p> <p>In the Sierra de San Luis, Central Argentina, a belt of small and discontinuous lenses of mafic-ultramafic rocks intrude a polydeformed basement and are thought to be the cause of a local increase of the metamorphic grade from amphibolite to granulite facies conditions. This assumption was especially based on forward modelling of a huge gravity anomaly centered over the Sierra de San Luis, which lead some workers to think that a vast volume of mafic-ultramafic rocks lay in shallow levels. Here, we propose an alternative model to explain this anomaly, in which the mafic-ultramafic <span class="hlt">intrusion</span> is not the ultimate source. Therefore, there is no need to propose a bigger size than that observed in outcrops for the mafic-ultramafic bodies. The thermal effect of the emplacement of mafic-ultramafic sills and <span class="hlt">dikes</span> on the host rocks was estimated applying a simple analytical solution (error function) for heating of a semi-infinite half space (the country rocks) in contact with a hotter sheet of finite thickness (the mafic-ultramafic <span class="hlt">intrusion</span>). Results indicate that the effect of the <span class="hlt">intrusion</span> of these hot mafic magmas is local, because beyond a few hundred meters from the contact <span class="hlt">zone</span> temperatures never exceed 600 °C, and a few km from the <span class="hlt">intrusion</span> they barely increase 50 °C relative to the initial temperature. These results, together with the preservation of primary igneous characteristics (such as rhythmic layering) being overprinted by metamorphic textural changes, indicate that the <span class="hlt">intrusion</span> occurred before regional deformation. It is suggested that the thermal anomaly in the Pringles Metamorphic Complex could have been mainly caused by factors inherent to their geodynamic setting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950054759&hterms=granite&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dgranite','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950054759&hterms=granite&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dgranite"><span>Getting granite <span class="hlt">dikes</span> out of the source region</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubin, Allan M.</p> <p>1995-01-01</p> <p>Whether a <span class="hlt">dike</span> can propagate far from a magma reservoir depends upon the competition between the rate at which propagation widens the <span class="hlt">dike</span> and the rate at which freezing constricts the aperture available for magma flow. Various formulations are developed for a viscous fluid at temperature T(sub m) intruding a growing crack in an elastic solid. The initial solid temperature equals T(sub m) at the source and decreases linearly with distance from the source. If T(sub m) is the unique freezing temperature of the fluid, <span class="hlt">dike</span> growth is initially self-similar and an essentially exact solution is obtained; if T(sub m) is above the solidus temperature, the solution is approximate but is designed to overestimate the distance the <span class="hlt">dike</span> may propagate. The ability of a <span class="hlt">dike</span> to survive thermally depends primarily upon a single parameter that is a measure of the ratio of the <span class="hlt">dike</span> frozen margin thickness to elastic thickness. Perhaps more intuitively, one may define a minimum distance from the essentially solid reservoir wall to the point at which the host rock temperature drops below the solidus, necessary for <span class="hlt">dikes</span> to propagate far into subsolidus rock. It is concluded that for reasonable material properties and source conditions, most basalt <span class="hlt">dikes</span> will have little difficulty leaving the source region, but most rhyolite <span class="hlt">dikes</span> will be halted by freezing soon after the magma encounters rock at temperatures below the magma solidus. While these results can explain why granitic <span class="hlt">dikes</span> are common near granitic plutons but rare elsewhere, the potentially large variation in magmatic systems makes it premature to rule out the possibility that most granites are transported through the crust in <span class="hlt">dikes</span>. Nonetheless, these results highlight difficulties with such proposals and suggest that it may also be premature to rule out the possibility that most granite plutons ascend as more equidimensional bodies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030945','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030945"><span>Bald Mountain gold mining district, Nevada: A Jurassic reduced <span class="hlt">intrusion</span>-related gold system</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nutt, C.J.; Hofstra, A.H.</p> <p>2007-01-01</p> <p>The Bald Mountain mining district has produced about 2 million ounces (Moz) of An. Geologic mapping, field relationships, geochemical data, petrographic observations, fluid inclusion characteristics, and Pb, S, O, and H isotope data indicate that An mineralization was associated with a reduced Jurassic <span class="hlt">intrusion</span>. Gold deposits are localized within and surrounding a Jurassic (159 Ma) quartz monzonite porphyry pluton and <span class="hlt">dike</span> complex that intrudes Cambrian to Mississippian carbonate and clastic rocks. The pluton, associated <span class="hlt">dikes</span>, and An mineralization were controlled by a crustal-scale northwest-trending structure named the Bida trend. Gold deposits are localized by fracture networks in the pluton and the contact metamorphic aureole, <span class="hlt">dike</span> margins, high-angle faults, and certain strata or shale-limestone contacts in sedimentary rocks. Gold mineralization was accompanied by silicification and phyllic alteration, ??argillic alteration at shallow levels. Although An is typically present throughout, the system exhibits a classic concentric geochemical zonation pattern with Mo, W, Bi, and Cu near the center, Ag, Pb, and Zn at intermediate distances, and As and Sb peripheral to the <span class="hlt">intrusion</span>. Near the center of the system, micron-sized native An occurs with base metal sulfides and sulfosalts. In peripheral deposits and in later stages of mineralization, Au is typically submicron in size and resides in pyrite or arsenopyrite. Electron microprobe and laser ablation ICP-MS analyses show that arsenopyrite, pyrite, and Bi sulfide minerals contain 10s to 1,000s of ppm Au. Ore-forming fluids were aqueous and carbonic at deep levels and episodically hypersaline at shallow levels due to boiling. The isotopic compositions of H and O in quartz and sericite and S and Pb in sulfides are indicative of magmatic ore fluids with sedimentary sulfur. Together, the evidence suggests that Au was introduced by reduced S-bearing magmatic fluids derived from a reduced <span class="hlt">intrusion</span>. The reduced</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=STS054-152-016&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3D5S','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=STS054-152-016&hterms=5S&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3D5S"><span>Great <span class="hlt">Dike</span> of Zimbabwe, Zimbabwae, Africa</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1993-01-01</p> <p>The Great <span class="hlt">Dike</span> of Zimbabwe (17.5S, 31.5E) bisects the entire length of Zimbabwae in southern Africa and is one of the prominent visual features easily recognized from low orbit. The volcanic rocks which make up the <span class="hlt">dike</span> are about 1.2 billion years old and are rich in chromite and platinum which are mined from it. The straight line of the <span class="hlt">dike</span> is offset in places by faults which are often occupied by streams flowing through the fractures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030700','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030700"><span>Contact <span class="hlt">zone</span> permeability at <span class="hlt">intrusion</span> boundaries: New results from hydraulic testing and geophysical logging in the Newark Rift Basin, New York, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Matter, J.M.; Goldberg, D.S.; Morin, R.H.; Stute, M.</p> <p>2006-01-01</p> <p>Hydraulic tests and geophysical logging performed in the Palisades sill and the underlying sedimentary rocks in the NE part of the Newark Rift Basin, New York, USA, confirm that the particular transmissive <span class="hlt">zones</span> are localized within the dolerite-sedimentary rock contact <span class="hlt">zone</span> and within a narrow interval below this contact <span class="hlt">zone</span> that is characterized by the occurrence of small layers of chilled dolerite. Transmissivity values determined from fluid injection, aquifer testing, and flowmeter measurements generally fall in the range of 8.1E-08 to 9.95E-06 m2/s and correspond to various scales of investigation. The analysis of acoustic and optical BHTV images reveals two primary fracture sets within the dolerite and the sedimentary rocks - subhorizontal fractures, intersected by subvertical ones. Despite being highly fractured either with subhorizontal, subvertical or both fracture populations, the dolerite above and the sedimentary rocks below the contact <span class="hlt">zone</span> and the <span class="hlt">zone</span> with the layers of chilled dolerite are significantly less conductive. The distribution of the particular conductive intervals is not a function of the two dominant fracture populations or their density but rather of the <span class="hlt">intrusion</span> path of the sill. The <span class="hlt">intrusion</span> caused thermal fracturing and cracking of both formations, resulting in higher permeability along the contact <span class="hlt">zone</span>. ?? Springer-Verlag 2005.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T43D..04O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T43D..04O"><span>State-of-stress in magmatic rift <span class="hlt">zones</span>: Predicting the role of surface and subsurface topography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oliva, S. J. C.; Ebinger, C.; Rivalta, E.; Williams, C. A.</p> <p>2017-12-01</p> <p>Continental rift <span class="hlt">zones</span> are segmented along their length by large fault systems that form in response to extensional stresses. Volcanoes and crustal magma chambers cause fundamental changes to the density structure, load the plates, and alter the state-of-stress within the crust, which then dictates fracture orientation. In this study, we develop geodynamic models scaled to a < 7 My rift sector in the Eastern rift, East Africa where geophysical imaging provides tight constraints on subsurface structure, petrologic and thermodynamic studies constrain material densities, and seismicity and structural analyses constrain active and time-averaged kinematics. This area is an ideal test area because a 60º stress rotation is observed in time-averaged fault and magma <span class="hlt">intrusion</span>, and in local seismicity, and because this was the site of a large volume <span class="hlt">dike</span> <span class="hlt">intrusion</span> and seismic sequence in 2007. We use physics-based 2D and 3D models (analytical and finite elements) constrained by data from active rift <span class="hlt">zones</span> to quantify the effects of loading on state-of-stress. By modeling varying geometric arrangements, and density contrasts of topographic and subsurface loads, and with reasonable regional extensional forces, the resulting state-of-stress reveals the favored orientation for new <span class="hlt">intrusions</span>. Although our models are generalized, they allow us to evaluate whether a magmatic system (surface and subsurface) can explain the observed stress rotation, and enable new <span class="hlt">intrusions</span>, new faults, or fault reactivation with orientations oblique to the main border faults. Our results will improve our understanding of the different factors at play in these extensional regimes, as well as contribute to a better assessment of the hazards in the area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990Tecto...9..811D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990Tecto...9..811D"><span>Tectonic evolution of the Troodos Ophiolite within the Tethyan Framework</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dilek, Yildirim; Thy, Peter; Moores, Eldridge M.; Ramsden, Todd W.</p> <p>1990-08-01</p> <p>A new tectonic model reconciles conflicting structural and geochemical evidence for the origin of the Troodos ophiolite, a well-preserved remnant of Neotethyan oceanic crust. Grabens and normal faults within the sheeted <span class="hlt">dike</span> complex and the extrusive sequence of the Troodos ophiolite resemble those of oceanic spreading centers. Diverse <span class="hlt">intrusive</span> and tectonic contact relationships between the sheeted <span class="hlt">dike</span> complex and the underlying plutonic sequence indicate multiple and episodic <span class="hlt">intrusion</span> of magma and along- and across-strike variation in volcanic and tectonic activity during development of oceanic crust. Coupled with the existence of the Arakapas transform fault to the south, these structural and <span class="hlt">intrusive</span> relationships suggest origin at an intersection between a spreading center and a transform fault. The arclike chemistry of sheeted <span class="hlt">dikes</span> and related extrusive rocks and the inferred highly depleted and hydrous nature of the mantle source of the late stage <span class="hlt">intrusive</span> and extrusive rocks argue, however, for generation of part of the ophiolite within a subduction <span class="hlt">zone</span> environment. Regional reconstructions suggest that the Mesozoic Neotethys may have evolved as a marginal basin both to the Afro-Arabian continent and the Paleotethyan ocean over an active or recently active south dipping subduction <span class="hlt">zone</span>. The Troodos ophiolite and other eastern Mediterranean ophiolites, whose magma compositions were affected by the subducted Paleotethyan slab, may have formed along east-west trending spreading centers separated by north-south trending transform faults within this marginal basin. A rapid change in relative plate motion in late Cretaceous time between Eurasia and Afro-Arabia created a regional compressive regime that may have resulted in plate boundary reorganizations within the Neotethyan realm and in initiation of north dipping subduction <span class="hlt">zone(s</span>) beneath the Troodos and other ophiolites in the region. The apparent forearc setting of the Troodos ophiolite is a</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035720','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035720"><span>Growth of plutons by incremental emplacement of sheets in crystal-rich host: Evidence from Miocene <span class="hlt">intrusions</span> of the Colorado River region, Nevada, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Miller, C.F.; Furbish, D.J.; Walker, B.A.; Claiborne, L.L.; Koteas, G.C.; Bleick, H.A.; Miller, J.S.</p> <p>2011-01-01</p> <p>Growing evidence supports the notion that plutons are constructed incrementally, commonly over long periods of time, yet field evidence for the multiple injections that seem to be required is commonly sparse or absent. Timescales of up to several million years, among other arguments, indicate that the dominant volume does not remain largely molten, yet if growing plutons are constructed from rapidly solidifying increments it is unlikely that <span class="hlt">intrusive</span> contacts would escape notice. A model wherein magma increments are emplaced into melt-bearing but crystal-rich host, rather than either solid or crystal-poor material, provides a plausible explanation for this apparent conundrum. A partially solidified <span class="hlt">intrusion</span> undoubtedly comprises <span class="hlt">zones</span> with contrasting melt fraction and therefore strength. Depending on whether these <span class="hlt">zones</span> behave elastically or ductilely in response to <span class="hlt">dike</span> emplacement, intruding magma may spread to form sheets by either of two mechanisms. If the melt-bearing host is elastic on the relevant timescale, magma spreads rather than continuing to propagate upward, where it encounters a <span class="hlt">zone</span> of higher rigidity (higher crystal fraction). Similarly, if the <span class="hlt">dike</span> at first ascends through rigid, melt-poor material and then encounters a <span class="hlt">zone</span> that is weak enough (poor enough in crystals) to respond ductilely, the ascending material will also spread because the <span class="hlt">dike</span> tip ceases to propagate as in rigid material. We propose that ascending magma is thus in essence trapped, by either mechanism, within relatively crystal-poor <span class="hlt">zones</span>. Contacts will commonly be obscure from the start because the contrast between intruding material (crystal-poorer magma) and host (crystal-richer material) is subtle, and they may be obscured even further by subsequent destabilization of the crystal-melt framework. Field evidence and zircon <span class="hlt">zoning</span> stratigraphy in plutons of the Colorado River region of southern Nevada support the hypothesis that emplacement of magma replenishments into a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wsp/2217/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wsp/2217/report.pdf"><span>Evaluation of Major <span class="hlt">Dike</span>-Impounded Ground-Water Reservoirs, Island of Oahu</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Takasaki, Kiyoshi J.; Mink, John Francis</p> <p>1985-01-01</p> <p>Ground-water reservoirs impounded by volcanic <span class="hlt">dikes</span> receive a substantial part of the total recharge to ground water on the island of Oahu because they generally underlie the rainiest areas. These reservoirs accumulate the infiltration from rainfall, store it temporarily, and steadily leak it to abutting basal reservoirs or to streams cutting into them. The <span class="hlt">dike</span> reservoirs have high hydraulic heads and are mostly isolated from saline water. The most important and productive of the <span class="hlt">dike</span>-impounded reservoirs are in an area of about 135 square miles in the main fissure <span class="hlt">zone</span> of the Koolau volcano where the top of the <span class="hlt">dike</span>-impounded water reaches an altitude of at least 1,000 feet. Water is impounded and stored both above and below sea level. The water stored above sea level in the 135 square mile area has been roughly estimated at 560 billion gallons. In comparison, the water stored above sea level in reservoirs underlying a <span class="hlt">dike</span>-intruded area of about 53 square miles in the Waianae Range has been roughly estimated at 100 billion gallons. Storage below sea level is indeterminable, owing to uncertainties about the ability of the rock to store water as <span class="hlt">dike</span> density increases and porosity decreases. Tunnels, by breaching <span class="hlt">dike</span> controls, have reduced the water stored above sea level by at least 50 billion gallons in the Koolau Range and by 5 1/2 billion gallons in the Waianae Range, only a small part of the total water stored. Total leakage from storage in the Koolau Range has been estimated at about 280 Mgal/d (million gallons per day). This estimated leakage from the <span class="hlt">dike</span>-impounded reservoirs makes up a significant part of the ground-water yield of the Koolau Range, which has been estimated to range from 450 to 580 Mgal/d. The largest unused surface leakage is in the Kaneohe, Kahana, and Punaluu areas, and the largest unused underflow occurs in the Waialee, Hauula-Laie, Punaluu, and Kahana areas. The unused underflow leakage is small in areas near and east of Waialae, but</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70156134','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70156134"><span>Mapping the 3-D extent of the Northern Lobe of the Bushveld layered mafic <span class="hlt">intrusion</span> from geophysical data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Finn, Carol A.; Bedrosian, Paul A.; Cole, Janine; Khoza, Tshepo David; Webb, Susan J.</p> <p>2015-01-01</p> <p>Geophysical models image the 3D geometry of the mafic portion of the Bushveld Complex north of the Thabazimbi-Murchison Lineament (TML), critical for understanding the origin of the world's largest layered mafic <span class="hlt">intrusion</span> and platinum group element deposits. The combination of the gravity and magnetic data with recent seismic, MT, borehole and rock property measurements powerfully constrains the models. The <span class="hlt">intrusion</span> north of the TML is generally shallowly buried (generally <1500 m) with a modeled area of ∼160 km × ∼125 km. The modeled thicknesses are not well constrained but vary from ∼<1000 to >12,000 m, averaging ∼4000 m. A feeder, suggested by a large modeled thickness (>10,000 m) and funnel shape, for Lower <span class="hlt">Zone</span> magmas could have originated near the intersection of NS and NE trending TML faults under Mokopane. The TML has been thought to be the feeder <span class="hlt">zone</span> for the entire Bushveld Complex but the identification of local feeders and/or <span class="hlt">dikes</span> in the TML in the models is complicated by uncertainties on the syn- and post-Bushveld deformation history. However, modeled moderately thick high density material near the intersection of faults within the central and western TML may represent feeders for parts of the Bushveld Complex if deformation was minimal. The correspondence of flat, high resistivity and density regions reflect the sill-like geometry of the Bushveld Complex without evidence for feeders north of Mokopane. Magnetotelluric models indicate that the Transvaal sedimentary basin underlies much of the Bushveld Complex north of the TML, further than previously thought and important because the degree of reaction and assimilation of the Transvaal rocks with the mafic magmas resulted in a variety of mineralization <span class="hlt">zones</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930030857&hterms=Saunders&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D30%26Ntt%3DSaunders%252C%2BM','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930030857&hterms=Saunders&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D30%26Ntt%3DSaunders%252C%2BM"><span><span class="hlt">Dike</span> emplacement on Venus and on earth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mckenzie, Dan; Mckenzie, James M.; Saunders, R. S.</p> <p>1992-01-01</p> <p>Attention is given to long linear features visible in SAR images of the surface of Venus. They are shallow graben a few kilometers across. Calculations show that <span class="hlt">dike</span> emplacement can account for such features if the top of the <span class="hlt">dikes</span> is a few kilometers below the surface of the planet. The <span class="hlt">dikes</span> are often curved near their probable sources, and the magnitude of the regional stress field estimated from this curvature is about 3 MPa, or similar to that of earth. On both Venus and earth, <span class="hlt">dikes</span> often form intersecting patterns. Two-dimensional calculations show that this behavior can occur only if the stress field changes with time. Transport of melt over distances as large as 2000 km in <span class="hlt">dikes</span> whose width is 30 m or more occurs in some continental shields on earth and can also account for linear features on Venus that extend for comparable distances. Such transport is possible because the viscosity and thermal conductivity of both the melt and the wall rock are small.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V33B3132S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V33B3132S"><span>Exploring Cumulates in Small, Shallow Parts of a Large Mafic Magma System to Provide Baseline Models for Crystallization in Larger <span class="hlt">Intrusions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Srogi, L.; Willis, K. V.; Lutz, T. M.; Plank, T. A.; Pollock, M.; Connolly, B.; Wood, A. M.</p> <p>2016-12-01</p> <p>Small, shallow portions of large magmatic systems cool more rapidly and potentially have less subsolidus overprinting than large mafic <span class="hlt">intrusions</span>, but it is unclear whether they are small-scale analogs for the same crystallization processes. The Morgantown-Jacksonwald magmatic system (MJS), western Newark Basin, Pennsylvania, is part of the 201-Ma Central Atlantic Magmatic Province (CAMP) formed during Pangean rifting. The MJS consists of several interconnected <span class="hlt">intrusions</span> exposed in cross-section from the Jacksonwald basalt at the paleosurface to 6 km depth (<0.2 GPa). Mg-rich orthopyroxene (opx) phenocrysts form crystal accumulations in some <span class="hlt">dikes</span> and in basal and roof <span class="hlt">zones</span> of sills in the MJS, in many CAMP <span class="hlt">intrusions</span>, and in younger Ferrar dolerites, Antarctica. Some samples with opx phenocrysts have dm-scale modal layering. Despite ubiquitous occurrence, the opx is little-studied and our work tests most previous authors' assumption that opx was brought in from deeper <span class="hlt">intrusions</span>. Opx cores with Mg/(Mg+Fe) of 80-77% yield mid-crustal pressures of 0.4-0.6 GPa (using method of Putirka, 2008). LA-ICPMS was used to obtain trace element concentrations in mm-size phenocrysts in a chill margin within 0.5m of the basal contact and cm-size phenocrysts from cumulate about 10m above. REE concentrations are similar in both samples: LREE-depleted cores (normalized La/Sm = 0.05-0.1); variably LREE-enriched rims; some negative Eu anomalies. REE patterns calculated for liquids in equilibrium with opx using published Kd values are roughly parallel to but significantly higher than REE in host chill margin diabase. CSDs of opx and matrix plagioclase from several samples within 10m of the basal contact will be used to evaluate models of crystal growth vs. mechanical sorting. Modes and mineral compositions are not consistent with MELTS fractionation models: opx crystallizes in place of pigeonite; pyroxenes are <span class="hlt">zoned</span> in Ca not Fe-Mg; late-crystallizing quartz and K-feldspar are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011Miner..42..121S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011Miner..42..121S"><span>An overview of the association between lamprophyric <span class="hlt">intrusions</span> and rare-metal mineralization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Štemprok, Miroslav; Seifert, Thomas</p> <p>2011-01-01</p> <p>Granite-related rare metal districts in orogenic settings are occasionally associated with lamprophyre <span class="hlt">dikes</span>. We recorded 63 occurrences of lamprophyres in bimodal <span class="hlt">dike</span> suites of about 200 granite bodies related to rare metal deposits. Most lamprophyres occur in Paleozoic and Mesozoic metallogenic provinces in the northern hemisphere. Lamprophyres which are associated with rare metal deposits are calc-alkaline (kersantites, minettes, spessartites) or more rarely alkaline lamprophyres (camptonites, monchiquites) which occur in the roof <span class="hlt">zone</span> of complex granitic bodies as pre-granitic, intra-granitic, intra-ore or post-ore <span class="hlt">dikes</span>. Most lamprophyres are spatially associated with dominant felsic <span class="hlt">dikes</span> and/or with mafic <span class="hlt">dikes</span> represented by diorites or diabases. Diorites and lamprophyres occasionally exhibit transitional compositions from one to another. Lamprophyres share common geochemical characteristics of highly evolved granitoids such as enrichment in K and F, increased abundances of Li, Rb, and Cs and enrichment in some HFSE (e.g. Zr, U, Th, Mo, Sn, W). Lamprophyres in rare metal districts testify to accessibility of the upper crust to mantle products at the time of rare metal mineralization and possible influence of mantle melts or mantle-derived fluids in the differentiation of granitic melts in the lower crust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.5156V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.5156V"><span>Analysis of flood hazard under consideration of <span class="hlt">dike</span> breaches</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vorogushyn, S.; Apel, H.; Lindenschmidt, K.-E.; Merz, B.</p> <p>2009-04-01</p> <p>The study focuses on the development and application of a new modelling system which allows a comprehensive flood hazard assessment along <span class="hlt">diked</span> river reaches under consideration of <span class="hlt">dike</span> failures. The proposed Inundation Hazard Assessment Model (IHAM) represents a hybrid probabilistic-deterministic model. It comprises three models interactively coupled at runtime. These are: (1) 1D unsteady hydrodynamic model of river channel and floodplain flow between <span class="hlt">dikes</span>, (2) probabilistic <span class="hlt">dike</span> breach model which determines possible <span class="hlt">dike</span> breach locations, breach widths and breach outflow discharges, and (3) 2D raster-based diffusion wave storage cell model of the hinterland areas behind the <span class="hlt">dikes</span>. Due to the unsteady nature of the 1D and 2D coupled models, the dependence between hydraulic load at various locations along the reach is explicitly considered. The probabilistic <span class="hlt">dike</span> breach model describes <span class="hlt">dike</span> failures due to three failure mechanisms: overtopping, piping and slope instability caused by the seepage flow through the <span class="hlt">dike</span> core (micro-instability). <span class="hlt">Dike</span> failures for each mechanism are simulated based on fragility functions. The probability of breach is conditioned by the uncertainty in geometrical and geotechnical <span class="hlt">dike</span> parameters. The 2D storage cell model driven by the breach outflow boundary conditions computes an extended spectrum of flood intensity indicators such as water depth, flow velocity, impulse, inundation duration and rate of water rise. IHAM is embedded in a Monte Carlo simulation in order to account for the natural variability of the flood generation processes reflected in the form of input hydrographs and for the randomness of <span class="hlt">dike</span> failures given by breach locations, times and widths. The scenario calculations for the developed synthetic input hydrographs for the main river and tributary were carried out for floods with return periods of T = 100; 200; 500; 1000 a. Based on the modelling results, probabilistic <span class="hlt">dike</span> hazard maps could be generated that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BVol...80...16H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BVol...80...16H"><span>Emplacement controls for the basaltic-andesitic radial <span class="hlt">dikes</span> of Summer Coon volcano and implications for flank vents at stratovolcanoes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harp, A. G.; Valentine, G. A.</p> <p>2018-02-01</p> <p>Mafic flank eruptions are common events that pose a serious hazard to the communities and infrastructure often encroaching on the slopes of stratovolcanoes. Flank vent locations are dictated by the propagation path of their feeder <span class="hlt">dikes</span>. The <span class="hlt">dikes</span> are commonly thought to propagate either laterally from the central conduit or vertically from a deeper source. However, these interpretations are often based on indirect measurements, such as surface deformation and seismicity at active systems, and several studies at eroded volcanoes indicate the propagation paths may be more complex. We investigated the Oligocene age Summer Coon volcano (Colorado, USA), where erosion has exposed over 700 basaltic-andesitic radial <span class="hlt">dikes</span>, to constrain the propagation directions, geometries, and spatial distributions of mafic <span class="hlt">dikes</span> within a stratovolcano. The mean fabric angle of aligned plagioclase crystals was measured in oriented samples from the margins of 77 <span class="hlt">dikes</span>. Of the 41 <span class="hlt">dikes</span> with statistically significant flow fabrics, 85% had fabric angles that were inclined—plunging both inward and outward relative to the center of the volcano. After comparing fabric angles to those reported in other studies, we infer that, while most of the <span class="hlt">dikes</span> with outward-plunging fabrics descended toward the flanks from a source within the edifice and near its axis, <span class="hlt">dikes</span> with inward-plunging fabrics ascended through the edifice and toward the flanks from a deeper source. A possible control for the inclination of ascending <span class="hlt">dikes</span> was the ratio between magma overpressure and the normal stress in the host rock. While higher ratios led to high-angle propagation, lower ratios resulted in inclined emplacement. <span class="hlt">Dikes</span> crop out in higher frequencies within a <span class="hlt">zone</span> surrounding the volcano axis at 2500 m radial distance from the center and may be the result of ascending <span class="hlt">dikes</span>, emplaced at similar propagation angles, intersecting the current level of exposure at common distances from the volcano axis. The process</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027827','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027827"><span>Sub-seafloor acoustic characterization of seamounts near the Ogasawara Fracture <span class="hlt">Zone</span> in the western Pacific using chirp (3-7 kHz) subbottom profiles</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lee, T.-G.; Hein, J.R.; Lee, Kenneth; Moon, J.-W.; Ko, Y.-T.</p> <p>2005-01-01</p> <p>A detailed analysis of chirp (3-7 kHz) subbottom profiles and bathymetry was performed on data collected from seamounts near the Ogasawara Fracture <span class="hlt">Zone</span> (OFZ) in the western Pacific. The OFZ, which is a 150 km wide rift <span class="hlt">zone</span> showing 600 km of right-lateral movement in a NW-SE direction, is unique among the fracture <span class="hlt">zones</span> of the Pacific in that it includes many old seamounts (e.g., Magellan Seamounts and seamounts on Dutton Ridge). Sub-seafloor acoustic echoes on the seamounts are classified into nine specific types based on the nature and continuity of the echoes, subbottom structure, and morphology of the seafloor: (1) distinct echoes (types I-1, I-2, I-3), (2) indistinct echoes (types II-1, II-2, II-3), and (3) hyperbolic echoes (types III-1, III-2, III-3). Type I-2 pelagic sediments, characterized by thin and intermittent coverage, were probably deposited in topographically sheltered areas when bottom currents were strong, whereas type I-1 pelagic sediments accumulated during continuous and widespread sedimentation. Development of seamount flank rift <span class="hlt">zones</span> in the OFZ may have been influenced by preexisting structures in the transform fracture <span class="hlt">zone</span> at the time of volcanism, whereas those on Ita Mai Tai seamount in the Pigafetta Basin originated solely by edifice-building processes. Flank rift <span class="hlt">zones</span> that formed by <span class="hlt">dike</span> <span class="hlt">intrusions</span> and eruptions played an important role in mass wasting. Mass-wasting processes included block faulting or block slides around the summit margin, sliding/slumping, debris flows, and turbidites, which may have been triggered by faulting, volcanism, <span class="hlt">dike</span> injection, and weathering during various stages in the evolution of the seamounts. ?? 2005 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025625','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025625"><span>Late Neoproterozoic felsite (602.3 +/- 2 Ma) and associated metadiabase <span class="hlt">dikes</span> in the Reading Prong, Pennsylvania, and rifting of Laurentia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Smith, R.C.</p> <p>2003-01-01</p> <p>Felsite <span class="hlt">dikes</span> in the Rittenhouse Gap iron mine district of the Reading Prong, eastern Pennsylvania, have a close geochemical affinity with the peralkaline Battle Mountain Member of the Robertson River Igneous Suite (RRIS), northern Virginia. These newly recognized Rittenhouse Gap Felsite <span class="hlt">dikes</span> of the Swabia Creek Igneous Suite (SCIS) of eastern Pennsylvania plot as within-plate, A-type, A1 granites on various discriminant diagrams, but are quite distinct from late Neoproterozoic Catoctin Metarhyolite of Pennsylvania which has lower Ga/Al and Nb, but higher Eu. Newly recognized metadiabase <span class="hlt">dikes</span>, also found in the Rittenhouse Gap district and proposed as Tunnel Mine Metadiabase of the SCIS, classify as alkali within-plate or continental initial rifting alkali tholeiites. They are quite distinct chemically and mineralogically from Catoctin Metabasalt flows and equivalent metadiabase <span class="hlt">dikes</span> in Pennsylvania, which have lower Nb. Sr and Nd isotopic data indicate that the Tunnel Mine Metadiabase and Rittenhouse Gap Felsite are of mantle origin, but that the latter also includes a crustal component. The SCIS bimodal volcanics in Pennsylvania suggest a previously unrecognized rift environment in Pennsylvania at 602 Ma, somewhat predating the recognized, latest Neoproterozoic Catoctin event in Pennsylvania. As such, they fill in both temporal and geographic gaps for the rifting of Laurentia in Pennsylvania. It is proposed that the SCIS melt developed from a remnant ember of the northeastward trace of the older Mount Rogers-RRIS hotspot as Laurentia rotated clockwise. However, release and <span class="hlt">intrusion</span> of the SCIS may have been related to younger Catoctin event crustal thinning that slightly predated the mafic <span class="hlt">dike</span> phase of the Catoctin as Laurentia later migrated northward over a second hotspot. Eventually, the mafic phase associated with this second hotspot sufficiently attenuated the crust to allow introduction of Catoctin volcanics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020128','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020128"><span>Paleomagnetism of the Miocene <span class="hlt">intrusive</span> suite of Kidd Creek: Timing of deformation in the Cascade arc, southern Washington</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hagstrum, J.T.; Swanson, D.A.; Snee, L.W.</p> <p>1998-01-01</p> <p>Paleomagnetic study of the <span class="hlt">intrusive</span> suite of Kidd Creek in the southern Washington Cascades (23 sites in <span class="hlt">dikes</span> and sills) was undertaken to help determine if these rocks are comagmatic and whether they postdate regional folding of the volcanic arc. Fission track and 40Ar-39Ar age determinations indicate an age of ???12.7 Ma (middle Miocene) for these rocks. The similarity of normal-polarity characteristic directions for most samples corroborate the available geochemical data indicating that these rocks are most likely comagmatic. Reversed-polarity directions for samples from four sites, however, show that emplacement of Kidd Creek <span class="hlt">intrusions</span> spanned at least one reversal of the geomagnetic field. The paleomagnetic directions for the <span class="hlt">dikes</span> and sills fail a fold test at the 99% confidence level indicating that the Kidd Creek rocks postdate regional folding. The mean in situ direction also indicates that the Kidd Creek and older rocks have been rotated 22?? ?? 6?? clockwise about a vertical or near-vertical axis from the expected Miocene direction. Compression and regional folding of the Cascade arc in southern Washington therefore had ended by ???12 Ma prior to the onset of deformation resulting in rotation of these rocks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1214302J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1214302J"><span>High-resolution seismic measurements at loamy <span class="hlt">dikes</span> for monitoring high-water influences</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jaksch, Katrin; Giese, Rüdiger</p> <p>2010-05-01</p> <p>For the risk management of high-water events it is important to know how secure river <span class="hlt">dikes</span> are. Even the structures of <span class="hlt">dikes</span> are often unknown. Methods for the exploration of existing <span class="hlt">dikes</span> and of their underground, for an evaluation of failure potential and strengthening requirements are needed. In the presented work, the potential of a high-resolution seismics to monitor the moisture penetration of <span class="hlt">dikes</span> during flood periods was analyzed. To identify the extent of moisture penetration and to determine the structures of a loamy <span class="hlt">dike</span> body would enable to determine the probability of a <span class="hlt">dike</span> failure. <span class="hlt">Dikes</span> made of loam show a different behavior of moisture penetration under high-water influence. The distribution and penetration of water is moderate compared to sandy <span class="hlt">dikes</span> and resist longer high-water events. The water expands slowly in the <span class="hlt">dike</span> body in all directions known as fingering. It should be analyzed how the moisture penetration from a <span class="hlt">dike</span> can be displayed with seismic methods. The aim was to identify on the basis of seismic measurements the areas of moisture penetration within a <span class="hlt">dike</span> during a flood and out of it to determine the probability of collapse of the <span class="hlt">dike</span>. For that purpose the structures in the <span class="hlt">dike</span> body should be determined in reference to the materials and his soil parameters like water content and porosity. A test facility was built for <span class="hlt">dikes</span> including a regulation for the water level. This allowed the simulation of flood scenarios at <span class="hlt">dikes</span>. Two <span class="hlt">dikes</span> with different loam content were built in order to determine the failure mechanism of <span class="hlt">dikes</span>. With a width of 8 meters at the basis they had nearly the dimension of river <span class="hlt">dikes</span>. Seismic instrumentation was installed on both <span class="hlt">dike</span> models. The seismic survey consists of three parallel receiver lines on the <span class="hlt">dike</span> which recorded seismic signals emitted along the same lines, resulting in a 3D-seismic data set. The receivers were 3-component-geophones fixed in spikes, at the flooded side of the <span class="hlt">dike</span> were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.3337T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.3337T"><span>Interpreting inverse magnetic fabric in <span class="hlt">dikes</span> from Eastern Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Trippanera, Daniele; Urbani, Stefano; Porreca, Massimiliano; Acocella, Valerio; Kissel, Catherine; Sagnotti, Leonardo; Winkler, Aldo</p> <p>2017-04-01</p> <p>Since the 70's magnetic fabric analysis has been used to infer magma emplacement in <span class="hlt">dikes</span>. However, the interpretation of magmatic flow orientation in <span class="hlt">dikes</span> is often complicated by the occurrence of anomalous (i.e. inverse) magnetic fabric. This latter may either reflect the presence of single-domain (SD) grains or result from peculiar orientation mechanisms of magnetic minerals in magmas of different viscosities. Tertiary <span class="hlt">dike</span> swarms of extinct volcanic systems in Eastern Iceland represent the ideal case study to clarify the origin of anomalous magnetic fabric. Here we present the results of a multidisciplinary study on <span class="hlt">dikes</span> belonging to the Alftafjordur volcanic system (Eastern Iceland), including a: (1) structural field study in order to identify kinematic and thermal indicators of <span class="hlt">dikes</span>; (2) anisotropy of low-field magnetic susceptibility (AMS) analysis, to investigate the magnetic fabric and reconstruct the flow direction of 25 <span class="hlt">dikes</span>; (3) first order reversal curve (FORC) diagrams and thermomagnetic properties of selected <span class="hlt">dikes</span> to define the magnetic mineralogy; (4) petrofabric and image analyses at different microscopic scales to investigate the origin of the magnetic fabric and compare the AMS results with mineral texture. Our results show that half of the <span class="hlt">dikes</span> show a well defined inverse magnetic fabrics (k max orthogonal to the <span class="hlt">dike</span> margins) and anomalous high anisotropy degrees. Only 7 <span class="hlt">dikes</span> have a normal magnetic fabric and other 6 <span class="hlt">dikes</span> have an intermediate magnetic fabric. No clear prevalence of SD grains, which could explain the inverse magnetic fabric, was observed. On the contrary, petrofabric and thermomagnetic analysis reveal the presence of low Ti-content coarse magnetite and high Ti-content elongated magnetite grains as the main contributors to most of the observed magnetic fabrics. In particular, the orientation of the elongated high Ti-content magnetite grains, though usually scattered, is partly comparable with that of the maximum and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Icar..283..176H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..283..176H"><span>Generation, ascent and eruption of magma on the Moon: New insights into source depths, magma supply, <span class="hlt">intrusions</span> and effusive/explosive eruptions (Part 2: Predicted emplacement processes and observations)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Head, James W.; Wilson, Lionel</p> <p>2017-02-01</p> <p>We utilize a theoretical analysis of the generation, ascent, <span class="hlt">intrusion</span> and eruption of basaltic magma on the Moon to develop new insights into magma source depths, supply processes, transport and emplacement mechanisms via <span class="hlt">dike</span> <span class="hlt">intrusions</span>, and effusive and explosive eruptions. We make predictions about the <span class="hlt">intrusion</span> and eruption processes and compare these with the range of observed styles of mare volcanism, and related features and deposits. Density contrasts between the bulk mantle and regions with a greater abundance of heat sources will cause larger heated regions to rise as buoyant melt-rich diapirs that generate partial melts that can undergo collection into magma source regions; diapirs rise to the base of the anorthositic crustal density trap (when the crust is thicker than the elastic lithosphere) or, later in history, to the base of the lithospheric rheological trap (when the thickening lithosphere exceeds the thickness of the crust). Residual diapiric buoyancy, and continued production and arrival of diapiric material, enhances melt volume and overpressurizes the source regions, producing sufficient stress to cause brittle deformation of the elastic part of the overlying lithosphere; a magma-filled crack initiates and propagates toward the surface as a convex upward, blade-shaped <span class="hlt">dike</span>. The volume of magma released in a single event is likely to lie in the range 102 km3 to 103 km3, corresponding to <span class="hlt">dikes</span> with widths of 40-100 m and both vertical and horizontal extents of 60-100 km, favoring eruption on the lunar nearside. Shallower magma sources produce <span class="hlt">dikes</span> that are continuous from the source region to the surface, but deeper sources will propagate <span class="hlt">dikes</span> that detach from the source region and ascend as discrete penny-shaped structures. As the Moon cools with time, the lithosphere thickens, source regions become less abundant, and rheological traps become increasingly deep; the state of stress in the lithosphere becomes increasingly contractional</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V12A..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V12A..04S"><span>Aligning petrology with geophysics: the Father's Day <span class="hlt">intrusion</span> and eruption, Kīlauea Volcano, Hawai`i</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salem, L. C.; Edmonds, M.; Maclennan, J.; Houghton, B. F.; Poland, M. P.</p> <p>2016-12-01</p> <p>The Father's Day 2007 eruption at Kīlauea Volcano, Hawai`i, is an unprecedented opportunity to align geochemical techniques with the exceptionally detailed volcano monitoring data collected by the Hawaiian Volcano Observatory (HVO). Increased CO2 emissions were measured during a period of inflation at the summit of Kilauea in 2003-2007, suggesting that the rate of magma supply to the summit had increased [Poland et al., 2012]. The June 2007 Father's Day eruption in the East Rift <span class="hlt">Zone</span> (ERZ) occurred at the peak of the summit inflation. It offers the potential to sample magmas that have ascended on short timescales prior to 2007 from the lower crust, and perhaps mantle, with limited fractionation in the summit reservoir. The bulk rock composition of the lavas erupted are certainly consistent with this idea, with >8.5 wt% MgO compared to a typical 7.0-7.5 wt% for contemporaneous Pu`u`O`o ERZ lavas. However, our analysis of the major and trace element chemistry of olivine-hosted melt inclusions shows that the melts are in fact relatively evolved, with Mg# <53, compared to up to 63 for some high fountaining eruptions, e.g. Kīlauea Iki. The magma evidently entrained a crystal cargo of more primitive olivines, compositionally typical of summit eruption magma (with 81-84 mol% Fo). The melt inclusion chemistry shows homogenized and narrowly distributed trace element ratios, medium/low CO2 abundances and high concentrations of sulfur (unlike typical ERZ magmas). However, the chemistry is unlike melts that have partially bypassed the summit reservoir, e.g. those erupted at Kīlauea Iki, Mauna Ulu. We suggest that the Father's Day magma had been resident in the magma reservoir prior to the 2003-2007 inflation, and was evacuated from the reservoir into the ERZ in response to the increased rate of <span class="hlt">intrusion</span> of magma from depth. Dissolved volatile contents along profiles in embayments ("open" melt inclusions) were measured and compared to diffusion models to predict timescales</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH33B0258E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH33B0258E"><span>Experimental investigation of fluvial <span class="hlt">dike</span> breaching due to flow overtopping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>El Kadi Abderrezzak, K.; Rifai, I.; Erpicum, S.; Archambeau, P.; Violeau, D.; Pirotton, M.; Dewals, B.</p> <p>2017-12-01</p> <p>The failure of fluvial <span class="hlt">dikes</span> (levees) often leads to devastating floods that cause loss of life and damages to public infrastructure. Overtopping flows have been recognized as one of the most frequent cause of <span class="hlt">dike</span> erosion and breaching. Fluvial <span class="hlt">dike</span> breaching is different from frontal <span class="hlt">dike</span> (embankments) breaching, because of specific geometry and boundary conditions. The current knowledge on the physical processes underpinning fluvial <span class="hlt">dike</span> failure due to overtopping remains limited. In addition, there is a lack of a continuous monitoring of the 3D breach formation, limiting the analysis of the key mechanisms governing the breach development and the validation of conceptual or physically-based models. Laboratory tests on breach growth in homogeneous, non-cohesive sandy fluvial <span class="hlt">dikes</span> due to flow overtopping have been performed. Two experimental setups have been constructed, permitting the investigation of various hydraulic and geometric parameters. Each experimental setup includes a main channel, separated from a floodplain by a <span class="hlt">dike</span>. A rectangular initial notch is cut in the crest to initiate <span class="hlt">dike</span> breaching. The breach development is monitored continuously using a specific developed laser profilometry technique. The observations have shown that the breach develops in two stages: first the breach deepens and widens with the breach centerline being gradually shifted toward the downstream side of the main channel. This behavior underlines the influence of the flow momentum component parallel to the <span class="hlt">dike</span> crest. Second, the <span class="hlt">dike</span> geometry upstream of the breach stops evolving and the breach widening continues only toward the downstream side of the main channel. The breach evolution has been found strongly affected by the flow conditions (i.e. inflow discharge in the main channel, downstream boundary condition) and floodplain confinement. The findings of this work shed light on key mechanisms of fluvial <span class="hlt">dike</span> breaching, which differ substantially from those of dam</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011391','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011391"><span>Modeling of self-potential anomalies near vertical <span class="hlt">dikes</span>.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fitterman, D.V.</p> <p>1983-01-01</p> <p>The self-potential (SP) Green's function for an outcropping vertical <span class="hlt">dike</span> is derived from solutions for the dc resistivity problem for the same geometry. The Green's functions are numerically integrated over rectangular source regions on the contacts between the <span class="hlt">dike</span> and the surrounding material to obtain the SP anomaly. The analysis is valid for thermoelectrical source mechanisms. Two types of anomalies can be produced by this geometry. When the two source planes are polarized in opposite directions, a monopolar anomaly is produced. This corresponds to the thermoelectrical properties of the <span class="hlt">dike</span> being in contrast with the surrounding material. When the thermoelectric coefficients change monotonically across the <span class="hlt">dike</span>, a dipolar anomaly is produced. In either case positive and negative anomalies are possible, and the greatest variation in potential will occur in the most resistive regions. -Author</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gq/1766/pdf/gq1766_pamphlet.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gq/1766/pdf/gq1766_pamphlet.pdf"><span>Geologic map of the Lead Mountain 15’ quadrangle, San Bernardino County, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Howard, Keith A.; Jagiello, Keith J.; Fitzgibbon, Todd T.; John, Barbara E.</p> <p>2013-01-01</p> <p>The Lead Mountain 15’ quadrangle in the Mojave Desert contains a record of Jurassic, Cretaceous, Tertiary, and Quaternary magmatism. Small amounts of Mesoproterozoic(?) augen gneiss and Paleozoic and Mesozoic(?) metasedimentary rocks are preserved in small patches; they are intruded by voluminous Jurassic plutons of quartz diorite to granite composition and by Late Cretaceous granite of the Cadiz Valley batholith. Jurassic <span class="hlt">intrusive</span> rocks include part of the Bullion Mountain <span class="hlt">Intrusive</span> Suite and also younger <span class="hlt">dikes</span> inferred to be part of the Jurassic Independence <span class="hlt">dike</span> swarm. A contact-metamorphosed aureole 2 km wide in the Jurassic plutonic rocks fringes the Cadiz Valley batholith. Early Miocene dacitic magmatism produced a dense swarm of <span class="hlt">dikes</span> in the eastern Bullion Mountains and the volcanic-<span class="hlt">intrusive</span> remnant of a volcano at Lead Mountain. Tilting of the <span class="hlt">dike</span> swarm from inferred vertical orientations may have resulted from Miocene tectonic extension. Conglomerate of Pliocene and (or) Miocene age is also tilted. Younger volcanism is recorded by Pliocene basalt of the Deadman Lake volcanic field, basalt of Lead Mountain (approximately 0.36 Ma), and the even younger basalt of Amboy. Quaternary sedimentation built alluvial fans and filled playas in the map area. Faulting in the dextral eastern California shear <span class="hlt">zone</span> produced several northwest-striking faults in the quadrangle, some of them active into the Pleistocene and some that may have many kilometers of right-lateral offset.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880021110&hterms=volcano+eruption+hawaii&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dvolcano%2Beruption%2Bhawaii','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880021110&hterms=volcano+eruption+hawaii&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dvolcano%2Beruption%2Bhawaii"><span>Rifts of deeply eroded Hawaiian basaltic shields: A structural analog for large Martian volcanoes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Knight, Michael D.; Walker, G. P. L.; Mouginis-Mark, P. J.; Rowland, Scott K.</p> <p>1988-01-01</p> <p>Recently derived morphologic evidence suggests that <span class="hlt">intrusive</span> events have not only influenced the growth of young shield volcanoes on Mars but also the distribution of volatiles surrounding these volcanoes: in addition to rift <span class="hlt">zones</span> and flank eruptions on Arsia Mons and Pavonis Mons, melt water channels were identified to the northwest of Hecates Tholus, to the south of Hadriaca Patera, and to the SE of Olympus Mons. Melt water release could be the surface expression of tectonic deformation of the region or, potentially, <span class="hlt">intrusive</span> events associated with <span class="hlt">dike</span> emplacement from each of these volcanoes. In this study the structural properties of Hawaiian shield volcanoes were studied where subaerial erosion has removed a sufficient amount of the surface to enable a direct investigation of the internal structure of the volcanoes. The field investigation of <span class="hlt">dike</span> morphology and magma flow characteristics for several volcanoes in Hawaii is reported. A comprehensive investigation was made of the Koolau <span class="hlt">dike</span> complex that passes through the summit caldera. A study of two other dissected Hawaiian volcanoes, namely Waianae and East Molokai, was commenced. The goal is not only to understand the emplacement process and magma flow within these terrestrial <span class="hlt">dikes</span>, but also to explore the possible role that <span class="hlt">intrusive</span> events may have played in volcano growth and the distribution of melt water release on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSAES..83...68M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSAES..83...68M"><span>Mississippian lamprophyre <span class="hlt">dikes</span> in western Sierras Pampeanas, Argentina: Evidence of transtensional tectonics along the SW margin of Gondwana</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martina, Federico; Canelo, Horacio N.; Dávila, Federico M.; de Hollanda, María Helena M.; Teixeira, Wilson</p> <p>2018-04-01</p> <p>In the Famatina range, Sierras Pampeanas of Argentina (SW Gondwana), subvertical calc-alkaline lamprophyric <span class="hlt">dike</span> swarms crop out through >300 km. The <span class="hlt">dikes</span> cut Ordovician units with a prominent NW-SE trending and are covered by continental sedimentary successions of Pennsylvanian to Permian age. The <span class="hlt">dikes</span> show a strong structural control associated with Riedel fault systems. Detailed field analysis suggested a ∼N-S opening direction oblique to the attitude of <span class="hlt">dike</span> walls and a left-lateral transtensional tectonics during the emplacement. 40Ar/39Ar geochronology of a lamprophyric sample defined a crystallization age (plateau; whole rock) of 357.1 ± 7.1 Ma (MSWD = 2.3). Coetaneous ductile <span class="hlt">zones</span> with dominant strike-slip motion, documented along western Argentina for >600 km, suggest a regional event in SW Gondwana during the Mississippian. We propose that this deformation was the result of the counterclockwise fast rotation of Gondwana between 365 and 345 Ma, when the Famatina range and western Argentina occupied a sub-polar position. A transform margin along SW Gondwana better explains our (and others) data rather than a subduction margin. This scenario is also consistent with the occurrence of A-type granites and normal-fault basins within the foreland as well as bimodal volcanics.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/circ/1978/0772b/report.pdf#page=70','USGSPUBS'); return false;" href="https://pubs.usgs.gov/circ/1978/0772b/report.pdf#page=70"><span>New ages on <span class="hlt">intrusive</span> rocks and altered <span class="hlt">zones</span> in the Alaska Peninsula: A section in The United States Geological Survey in Alaska: Accomplishments during 1977</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wilson, Frederic H.; Detterman, Robert L.; Silberman, Miles L.</p> <p>1978-01-01</p> <p>Preliminary potassium-argon dating of <span class="hlt">intrusive</span> rocks and altered <span class="hlt">zones</span> in the Chignik and Sutwik Island quadrangles of the Alaska Peninsula seems to indicate at least three and possibly four Tertiary ages of alteration and mineralization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21043263','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21043263"><span>Linking river, floodplain, and vadose <span class="hlt">zone</span> hydrology to improve restoration of a coastal river affected by saltwater <span class="hlt">intrusion</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kaplan, D; Muñoz-Carpena, R; Wan, Y; Hedgepeth, M; Zheng, F; Roberts, R; Rossmanith, R</p> <p>2010-01-01</p> <p>Floodplain forests provide unique ecological structure and function, which are often degraded or lost when watershed hydrology is modified. Restoration of damaged ecosystems requires an understanding of surface water, groundwater, and vadose (unsaturated) <span class="hlt">zone</span> hydrology in the floodplain. Soil moisture and porewater salinity are of particular importance for seed germination and seedling survival in systems affected by saltwater <span class="hlt">intrusion</span> but are difficult to monitor and often overlooked. This study contributes to the understanding of floodplain hydrology in one of the last bald cypress [Taxodium distichum (L.) Rich.] floodplain swamps in southeast Florida. We investigated soil moisture and porewater salinity dynamics in the floodplain of the Loxahatchee River, where reduced freshwater flow has led to saltwater <span class="hlt">intrusion</span> and a transition to salt-tolerant, mangrove-dominated communities. Twenty-four dielectric probes measuring soil moisture and porewater salinity every 30 min were installed along two transects-one in an upstream, freshwater location and one in a downstream tidal area. Complemented by surface water, groundwater, and meteorological data, these unique 4-yr datasets quantified the spatial variability and temporal dynamics of vadose <span class="hlt">zone</span> hydrology. Results showed that soil moisture can be closely predicted based on river stage and topographic elevation (overall Nash-Sutcliffe coefficient of efficiency = 0.83). Porewater salinity rarely exceeded tolerance thresholds (0.3125 S m(-1)) for bald cypress upstream but did so in some downstream areas. This provided an explanation for observed vegetation changes that both surface water and groundwater salinity failed to explain. The results offer a methodological and analytical framework for floodplain monitoring in locations where restoration success depends on vadose <span class="hlt">zone</span> hydrology and provide relationships for evaluating proposed restoration and management scenarios for the Loxahatchee River.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PhPro..25..452L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhPro..25..452L"><span>Spatial-temporal Change of Sanshui district's <span class="hlt">Dike</span>-pond from 1979-2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Jiaxing; Chen, Jianfei; Wang, Xiaoxuan</p> <p></p> <p><span class="hlt">Dike</span>-pond is a representative style of ecological agriculture in the PRD(Pearl River Delta). Since 1992, Guangdong quicken its pace of reform and opening-up to the outside world. A mass of factories had been built in the PRD. The <span class="hlt">dike</span>-ponds have come across some influential changes in the recent 30 years. To detect and study on the changes of <span class="hlt">dike</span>-ponds, the Remote Sensing and Geography Information System skill was applied in this paper. This article selected Sanshui district as an example and used Landsat TM 1979, 1990, 2000 and SPOT 2009 satellite image as the major data sources. With the help of ITTVIS company newly released software-ENVI EX, object-oriented approach has been used to extract the <span class="hlt">dike</span>-pond land from each image. The result indicates that the area of <span class="hlt">dike</span>-pond gained rapidly growth from 1979 to 2000, but decrease critically during 2000-2009. When using Change Detection Analysis to compute each period's change statistics, the result shown that the increased <span class="hlt">dike</span>-pond area were mainly from vegetation covered land and other bare land. Then we found out that the mean centre of Sanshui district's <span class="hlt">dike</span>-pond was moving from northwest to southeast during 1979-2009. Therefore, it comes to the conclusion that Sanshui district's <span class="hlt">dike</span>-pond increased across the southeast of Sanshui district from 1979 to 2009. Last but not least, some suggestions have been put forward to keep the <span class="hlt">dike</span>-pond land area from decreasing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap5_Poland.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap5_Poland.pdf"><span>Magma supply, storage, and transport at shield-stage Hawaiian volcanoes: Chapter 5 in Characteristics of Hawaiian volcanoes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Poland, Michael P.; Miklius, Asta; Montgomery-Brown, Emily K.; Poland, Michael P.; Takahashi, T. Jane; Landowski, Claire M.</p> <p>2014-01-01</p> <p>Magma supply to Hawaiian volcanoes has varied over millions of years but is presently at a high level. Supply to Kīlauea’s shallow magmatic system averages about 0.1 km3/yr and fluctuates on timescales of months to years due to changes in pressure within the summit reservoir system, as well as in the volume of melt supplied by the source hot spot. Magma plumbing systems beneath Kīlauea and Mauna Loa are complex and are best constrained at Kīlauea. Multiple regions of magma storage characterize Kīlauea’s summit, and two pairs of rift <span class="hlt">zones</span>, one providing a shallow magma pathway and the other forming a structural boundary within the volcano, radiate from the summit to carry magma to <span class="hlt">intrusion</span>/eruption sites located nearby or tens of kilometers from the caldera. Whether or not magma is present within the deep rift <span class="hlt">zone</span>, which extends beneath the structural rift <span class="hlt">zones</span> at ~3-km depth to the base of the volcano at ~9-km depth, remains an open question, but we suggest that most magma entering Kīlauea must pass through the summit reservoir system before entering the rift <span class="hlt">zones</span>. Mauna Loa’s summit magma storage system includes at least two interconnected reservoirs, with one centered beneath the south margin of the caldera and the other elongated along the axis of the caldera. Transport of magma within shield-stage Hawaiian volcanoes occurs through <span class="hlt">dikes</span> that can evolve into long-lived pipe-like pathways. The ratio of eruptive to noneruptive <span class="hlt">dikes</span> is large in Hawai‘i, compared to other basaltic volcanoes (in Iceland, for example), because Hawaiian <span class="hlt">dikes</span> tend to be intruded with high driving pressures. Passive <span class="hlt">dike</span> <span class="hlt">intrusions</span> also occur, motivated at Kīlauea by rift opening in response to seaward slip of the volcano’s south flank.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006E%26PSL.245..389P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006E%26PSL.245..389P"><span>Geometric and kinematic features of the <span class="hlt">dike</span> complex at Mt. Somma, Vesuvio (Italy)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Porreca, M.; Acocella, V.; Massimi, E.; Mattei, M.; Funiciello, R.; De Benedetti, A. A.</p> <p>2006-05-01</p> <p><span class="hlt">Dikes</span> provide important information on the structure, state of stress and activity of a volcano. Mt. Somma borders part of the Vesuvio cone (Italy), displaying ˜ 100 <span class="hlt">dikes</span> emplaced between ˜ 18 and 30 ka. Field, AMS (anisotropy of magnetic susceptibility) and thin section analyses are used to characterize their geometry and kinematics (direction and sense of flow). The <span class="hlt">dikes</span> mostly have a NNW-SSE to NE-SW strike. Approximately 57% are radial to the older Somma edifice, ˜ 27% are oblique and ˜ 16% tangential. Among the latter two groups, ˜ 32% are outward dipping and ˜ 11% inward dipping. The <span class="hlt">dike</span> thickness varies between 0.2 and 3 m, with a mean value of 1.17 m. The kinematics of 19 <span class="hlt">dikes</span> is determined through a combination of field (8 <span class="hlt">dikes</span>), AMS (16 <span class="hlt">dikes</span>) and thin section analyses (15 <span class="hlt">dikes</span>). Thirteen <span class="hlt">dikes</span> have a vertical upward flow, whereas six have an oblique-subhorizontal flow, suggesting a lateral propagation from the summit or eccentric vents of the former Somma edifice. These propagation paths differ from those deducible from the recent activity, as all the seven major fissure eruptions between 1631 and 1944 were related to the lateral propagation of radial <span class="hlt">dikes</span>. We propose that these different behaviours in <span class="hlt">dike</span> propagation may be mainly related to the opening conditions of the summit conduit. The laterally propagating <span class="hlt">dikes</span> in 1631-1944 formed with an open conduit. Conversely, the vertically propagating <span class="hlt">dikes</span> may have formed, between 18 and 30 ka, with a closed conduit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.G42A..04A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.G42A..04A"><span>Geodetic measurements and numerical models of the Afar rifting sequence 2005-2010</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ali, T.; Feigl, K.; Calais, E.; Hamling, I. J.; Wright, T. J.</p> <p>2012-12-01</p> <p>Rifting episodes are characterized by magma migration and <span class="hlt">dike</span> <span class="hlt">intrusions</span> that perturb the stress field within the surrounding lithosphere, inducing viscous flow in the lower crust and upper mantle that leads to observable, transient surface deformation. The Manda Hararo-Dabbahu rifting episode that occurred in the Afar depression between 2005 and 2010 is the first such episode to unfold fully in the era of satellite geodesy, thus providing a unique opportunity to probe the rheology of lithosphere at a divergent plate boundary. GPS and SAR measurements over the region since 2005 show accelerated surface deformation rates during post-<span class="hlt">diking</span> intervals [Wright et al., Nature Geosci., 2012]. Using these observations in combination with a numerical model, we estimate model parameters that best explain the deformation signal. Our model accounts for three distinct processes: (i) secular plate spreading between Nubian and Arabian plates, (ii) time dependent post-rifting viscoelastic relaxation following the 14 <span class="hlt">dike</span> <span class="hlt">intrusions</span> that occurred between 2005 and 2010, including the 60 km long mega <span class="hlt">dike</span> <span class="hlt">intrusion</span> of September 2005, and (iii) magma accumulation within crustal reservoirs that feed the <span class="hlt">dikes</span>. To model the time dependent deformation field, we use the open-source unstructured finite element code, Defmod [Ali, 2011, http://defmod.googlecode.com/]. Using a gradient-based iterative scheme [Ali and Feigl, Geochem. Geophys. Geosyst., 2012], we optimize the fit between observed and modeled deformation to estimate parameters in the model, including the locking depth of the rift <span class="hlt">zone</span>, geometry and depth of magma reservoirs and rheological properties of lower crust and upper mantle, along with their formal uncertainties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Icar..283..146W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..283..146W"><span>Generation, ascent and eruption of magma on the Moon: New insights into source depths, magma supply, <span class="hlt">intrusions</span> and effusive/explosive eruptions (Part 1: Theory)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Lionel; Head, James W.</p> <p>2017-02-01</p> <p> <span class="hlt">zones</span> deeper within the mantle. Thus magma accumulations at the base of the crust would have been able to intrude <span class="hlt">dikes</span> part-way through the crust, but not able to feed eruptions to the surface; in order to be erupted, magma must have been extracted from deeper mantle sources, consistent with petrologic evidence. Buoyant <span class="hlt">dikes</span> growing upward from deep mantle sources of partial melt can disconnect from their source regions and travel through the mantle as isolated bodies of melt that encounter and penetrate the crust-mantle density boundary. They adjust their lengths and internal pressure excesses so that the stress intensity at the lower tip is zero. The potential total vertical extent of the resulting melt body depends on the vertical extent of the source region from which it grew. For small source extents, the upper tip of the resulting <span class="hlt">dike</span> crossing the crust-mantle boundary cannot reach the surface anywhere on the Moon and therefore can only form a <span class="hlt">dike</span> <span class="hlt">intrusion</span>; for larger source extents, the <span class="hlt">dike</span> can reach the surface and erupt on the nearside but still cannot reach the surface on the farside; for even larger source extents, eruptions could occur on both the nearside and the farside. The paucity of farside eruptions therefore implies a restricted range of vertical extents of partial melt source region sizes, between ∼16 and ∼36 km. When eruptions can occur, the available pressure in excess of what is needed to support a static magma column to the surface gives the pressure gradient driving magma flow. The resulting typical turbulent magma rise speeds are ∼10 to a few tens of m s-1, <span class="hlt">dike</span> widths are of order 100 m, and eruption rates from 1 to 10 km long fissure vents are of order 105 to 106 m3 s-1. Volume fluxes in lunar eruptions derived from lava flow thicknesses and surface slopes or rille lengths and depths are found to be of order 105 to 106 m3 s-1 for volume-limited lava flows and >104 to 105 m3 s-1 for sinuous rilles, with <span class="hlt">dikes</span> widths of ∼50 m. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012Tectp.526..133Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012Tectp.526..133Z"><span>Modelling of deformation around magmatic <span class="hlt">intrusions</span> with application to gold-related structures in the Yilgarn Craton, Western Australia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Y.; Karrech, A.; Schaubs, P. M.; Regenauer-Lieb, K.; Poulet, T.; Cleverley, J. S.</p> <p>2012-03-01</p> <p>This study simulates rock deformation around high temperature granite <span class="hlt">intrusions</span> and explores how gold bearing shear <span class="hlt">zones</span> near <span class="hlt">intrusions</span> were developed in the Yilgarn, using a new continuum damage mechanics algorithm that considers the temperature and time dependent elastic-visco-plastic constitutive behaviour of crustal materials. The results demonstrate that strain rates have the most significant effects on structural patterns for both extensional and compressional cases. Smaller strain rates promote the formation of narrow high-strain shear <span class="hlt">zones</span> and strong strain localisation along the flank or shoulder areas of the <span class="hlt">intrusion</span> and cold granite dome. Wider diffuse shear <span class="hlt">zones</span> are developed under higher strain rates due to strain hardening. The cooling of the <span class="hlt">intrusion</span> to background temperatures occurred over a much shorter time interval when compared to the duration of deformation and shear <span class="hlt">zones</span> development. Strong strain localisation near the <span class="hlt">intrusion</span> and shear <span class="hlt">zone</span> development in the crust occurred under both extensional and compressional conditions. There is always clear strain localisation around the shoulders of the <span class="hlt">intrusion</span> and the flanks of the "cold" granitic dome in early deformation stages. In the models containing a pre-existing fault, strain localisation near the <span class="hlt">intrusion</span> became asymmetric with much stronger localisation and the development of a damage <span class="hlt">zone</span> at the shoulder adjacent to the reactivated fault. At higher deformation stages, the models produced a range of structural patterns including graben and half graben basin (extension), "pop-up" wedge structures (compression), tilted fault blocks and switch of shear movement from reverse to normal on shear <span class="hlt">zones</span>. The model explains in part why a number of gold deposits (e.g. Wallaby and Paddington deposits) in the Yilgarn were formed near the flank of granite-cored domes and deep "tapping" faults, and shows that the new modelling approach is capable of realistically simulating high strain</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V43G2955F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V43G2955F"><span>Oman Drilling Project GT3 site survey: dynamics at the roof of an oceanic magma chamber</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>France, L.; Nicollet, C.; Debret, B.; Lombard, M.; Berthod, C.; Ildefonse, B.; Koepke, J.</p> <p>2017-12-01</p> <p>Oman Drilling Project (OmanDP) aims at bringing new constraints on oceanic crust accretion and evolution by drilling Holes in the whole ophiolite section (mantle and crust). Among those, operations at GT3 in the Sumail massif drilled 400 m to sample the <span class="hlt">dike</span> - gabbro transition that corresponds to the top (gabbros) and roof (<span class="hlt">dikes</span>) of the axial magma chamber, an interface where hydrothermal and magmatic system interacts. Previous studies based on oceanic crust formed at present day fast-spreading ridges and preserved in ophiolites have highlighted that this interface is a dynamic horizon where the axial melt lens that top the main magma chamber can intrude, reheat, and partially assimilate previously hydrothermally altered roof rocks. Here we present the preliminary results obtained in GT3 area that have allowed the community to choose the drilling site. We provide a geological and structural map of the area, together with new petrographic and chemical constraints on the dynamics of the <span class="hlt">dike</span> - gabbro transition. Our new results allow us to quantify the dynamic processes, and to propose that 1/ the <span class="hlt">intrusive</span> contact of the varitextured gabbro within the <span class="hlt">dikes</span> highlights the <span class="hlt">intrusion</span> of the melt lens top in the <span class="hlt">dike</span> rooting <span class="hlt">zone</span>, 2/ both <span class="hlt">dikes</span> and previously crystallized gabbros are reheated, and recrystallized by underlying melt lens dynamics (up to 1050°C, largely above the hydrous solidus temperature of altered <span class="hlt">dikes</span> and gabbros), 3/ the reheating range can be > 200°C, 4/ the melt lens depth variations for a given ridge position is > 200m, 5/ the reheating stage and associated recrystallization within the <span class="hlt">dikes</span> occurred under hydrous conditions, 6/ the reheating stage is recorded at the root <span class="hlt">zone</span> of the sheeted <span class="hlt">dike</span> complex by one of the highest stable conductive thermal gradient ever recorded on Earth ( 3°C/m), 7/ local chemical variations in recrystallized <span class="hlt">dikes</span> and gabbros are highlighted and used to quantify crystallization and anatectic processes, and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912236J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912236J"><span>Constraining <span class="hlt">dike</span> emplacement conditions from virtual outcrop modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jørgen Kjøll, Hans; Andersen, Torgeir; Tegner, Christian</p> <p>2017-04-01</p> <p>In the Late Neoproterozoic, the paleocontinents of Baltica and Laurentia rifted apart and sea-floor spreading into the Ordovician formed the Iapetus Ocean. The Iapetus later closed and the two continents collided forming the Caledonian orogen. Rocks related to the break-up and subsequent opening of the Iapetus, now reside as partly well-preserved tectonic lenses in thrust nappes within the Scandinavian Caledonides. The break-up architecture can be separated in two distinct domains, one hyperextended magma-poor segment in the SW, and one magma-rich part that comprise the Baltoscandian <span class="hlt">Dike</span> Swarm (BDS), the main subject of this study. The magma-rich segment is exposed from c. Røros in the south, through Sweden and into Northern Norway, a distance of more than 900 kilometers. The magmatism of the BDS has been dated to c. 580-610 Ma and is now interpreted to represent a break-up related large igneous province (LIP). The BDS is generally well exposed in freshly glaciated outcrops and mountain cliffs. It intrudes proximal to distal marine, argillaceous, meta-sandstones and carbonates that locally display well-preserved extensional features, such as normal faults at both high and low angle. Partial melting of host rocks is observed at several localities, indicating relatively high temperatures during <span class="hlt">dike</span> emplacement. Temperature estimates by previous workers indicate high-T (850°C) conditions during the break-up from the northernmost part of the <span class="hlt">dike</span> swarm. Emplacement depths have not yet been accurately constrained, although some anomalous high pressure for an extensional environment (≈9Kbar) is indicated in the Corrovarre area. The spectacular exposure of the <span class="hlt">dike</span> swarm provides the opportunity to evaluate the conditions during emplacement from <span class="hlt">dike</span> geometries and morphologies. The several hundred meters high vertical cliff walls give excellent opportunities to assess the <span class="hlt">dike</span> geometries over a range of host lithologies and across several km of stratigraphy (up to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005EP%26S...57..925S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005EP%26S...57..925S"><span>Izu detachment hypothesis: A proposal of a unified cause for the Miyake-Kozu event and the Tokai slow event</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seno, Tetsuzo</p> <p>2005-10-01</p> <p>Based on the fact that interseismic deformation of collision <span class="hlt">zones</span> is generally described by slip along a detachment at depth, I attempt to interpret the deformation of the Izu collision <span class="hlt">zone</span> in terms of a detachment model. The systematic deviation of the GPS velocities of the Izu Peninsula (Nov. 1998-June 2000) from the Philippine Sea-Eurasian relative plate motions is fitted by the slip on the detachment at a depth of 15-20 km with a rate of 3 cm/yr. On June 26, 2000, seismo-magmatic activity that started near Miyakejima expanded NW by 20 km close to Kozushima in association with <span class="hlt">dike</span> <span class="hlt">intrusion</span> over a few months. The horizontal movements associated with this event, however, spread over wide areas in central Honshu. Simple <span class="hlt">dike</span> <span class="hlt">intrusion</span> models cannot explain these movements. To explain these, I hypothesize that a 20 cm of rapid slip occurred on the detachment at the time of this event. The abnormal crustal movements in the Tokai-central Honshu-Kanto region then started after the event. I propose that they represent delayed diffusive transfer of the slip on the detachment over surrounding low viscosity layers, such as nearby rupture <span class="hlt">zones</span> of great earthquakes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011423','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011423"><span>Surface deformation in volcanic rift <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pollard, D.D.; Delaney, P.T.; Duffield, W.A.; Endo, E.T.; Okamura, A.T.</p> <p>1983-01-01</p> <p>The principal conduits for magma transport within rift <span class="hlt">zones</span> of basaltic volcanoes are steeply dipping <span class="hlt">dikes</span>, some of which feed fissure eruptions. Elastic displacements accompanying a single <span class="hlt">dike</span> emplacement elevate the flanks of the rift relative to a central depression. Concomitant normal faulting may transform the depression into a graben thus accentuating the topographic features of the rift. If eruption occurs the characteristic ridge-trough-ridge displacement profile changes to a single ridge, centered at the fissure, and the erupted lava alters the local topography. A well-developed rift <span class="hlt">zone</span> owes its structure and topography to the integrated effects of many magmatic rifting events. To investigate this process we compute the elastic displacements and stresses in a homogeneous, two-dimensional half-space driven by a pressurized crack that may breach the surface. A derivative graphical method permits one to estimate the three geometric parameters of the <span class="hlt">dike</span> (height, inclination, and depth-to-center) and the mechanical parameter (driving pressure/rock stiffness) from a smoothly varying displacement profile. Direct comparison of measured and theoretical profiles may be used to estimate these parameters even if inelastic deformation, notably normal faulting, creates discontinuities in the profile. Geological structures (open cracks, normal faults, buckles, and thrust faults) form because of stresses induced by <span class="hlt">dike</span> emplacement and fissure eruption. Theoretical stress states associated with dilation of a pressurized crack are used to interpret the distribution and orientation of these structures and their role in rift formation. ?? 1983.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006GeoRL..33.8301A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006GeoRL..33.8301A"><span>Propagation of <span class="hlt">dikes</span> at Vesuvio (Italy) and the effect of Mt. Somma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Acocella, V.; Porreca, M.; Neri, M.; Massimi, E.; Mattei, M.</p> <p>2006-04-01</p> <p><span class="hlt">Dikes</span> provide crucial information on how magma propagates within volcanoes. Somma-Vesuvio (Italy) consists of the active Vesuvio cone, partly bordered by the older Mt. Somma edifice. Historical chronicles on the fissure eruptions in 1694-1944 are matched with an analytical solution to define the propagation path of the related <span class="hlt">dikes</span> and to study any control of the Mt. Somma relief. The fissures always consisted of the downslope migration of vents from an open summit conduit, indicating lateral propagation as the predominant mechanism for shallow <span class="hlt">dike</span> emplacement. No fissure emplaced beyond Mt. Somma, suggesting that its buttressing hinders the propagation of the radial <span class="hlt">dikes</span>. An analytical solution is defined to describe the mechanism of formation of the laterally propagating <span class="hlt">dikes</span> and to evaluate the effect of topography. The application to Somma-Vesuvio suggests that, under ordinary excess magmatic pressures, the <span class="hlt">dikes</span> should not propagate laterally at depths >240-480 m below the surface, as the increased lithostatic pressure requires magmatic pressures higher than average. This implies that, when the conduit is open, the lateral emplacement of <span class="hlt">dikes</span> is expectable on the S, W and E slopes. The lack of fissures N of Mt. Somma is explained by its buttressing, which hinders <span class="hlt">dike</span> propagation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6396C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6396C"><span>Automatic Monitoring System Design and Failure Probability Analysis for River <span class="hlt">Dikes</span> on Steep Channel</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chang, Yin-Lung; Lin, Yi-Jun; Tung, Yeou-Koung</p> <p>2017-04-01</p> <p>The purposes of this study includes: (1) design an automatic monitoring system for river <span class="hlt">dike</span>; and (2) develop a framework which enables the determination of <span class="hlt">dike</span> failure probabilities for various failure modes during a rainstorm. The historical <span class="hlt">dike</span> failure data collected in this study indicate that most <span class="hlt">dikes</span> in Taiwan collapsed under the 20-years return period discharge, which means the probability of <span class="hlt">dike</span> failure is much higher than that of overtopping. We installed the <span class="hlt">dike</span> monitoring system on the Chiu-She <span class="hlt">Dike</span> which located on the middle stream of Dajia River, Taiwan. The system includes: (1) vertical distributed pore water pressure sensors in front of and behind the <span class="hlt">dike</span>; (2) Time Domain Reflectometry (TDR) to measure the displacement of <span class="hlt">dike</span>; (3) wireless floating device to measure the scouring depth at the toe of <span class="hlt">dike</span>; and (4) water level gauge. The monitoring system recorded the variation of pore pressure inside the Chiu-She <span class="hlt">Dike</span> and the scouring depth during Typhoon Megi. The recorded data showed that the highest groundwater level insides the <span class="hlt">dike</span> occurred 15 hours after the peak discharge. We developed a framework which accounts for the uncertainties from return period discharge, Manning's n, scouring depth, soil cohesion, and friction angle and enables the determination of <span class="hlt">dike</span> failure probabilities for various failure modes such as overtopping, surface erosion, mass failure, toe sliding and overturning. The framework was applied to Chiu-She, Feng-Chou, and Ke-Chuang <span class="hlt">Dikes</span> on Dajia River. The results indicate that the toe sliding or overturning has the highest probability than other failure modes. Furthermore, the overall failure probability (integrate different failure modes) reaches 50% under 10-years return period flood which agrees with the historical failure data for the study reaches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019632','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019632"><span>Metamorphic and structural evidence for significant vertical displacement along the Ross Lake fault <span class="hlt">zone</span>, a major orogen-parallel shear <span class="hlt">zone</span> in the Cordillera of western North America</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Baldwin, J.A.; Whitney, D.L.; Hurlow, H.A.</p> <p>1997-01-01</p> <p> of the RLFZ that now separates the two structural blocks. High-angle faults in the study area are dextral-reverse mylonitic shear <span class="hlt">zones</span> that experienced later brittle normal slip. Vertical motion on these shear <span class="hlt">zones</span> before <span class="hlt">intrusion</span> of Skymo gabbro can account for metamorphic discontinuities indicated by P-T results. The terranes have also been internally deformed by nonintersecting but coeval dextral and sinistral shear <span class="hlt">zones</span> that formed after the terranes were brought together in the RLFZ and intruded by Eocene <span class="hlt">dikes</span>. These results show that the RLFZ has accommodated significant vertical displacement but perhaps no more than tens of kilometers of early Tertiary lateral movement. Structural evidence for earlier, large-magnitude strike-slip displacement is not preserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T43H..04E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T43H..04E"><span>Crustal Strain Patterns in Magmatic and Amagmatic Early Stage Rifts: Border Faults, Magma <span class="hlt">Intrusion</span>, and Volatiles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ebinger, C. J.; Keir, D.; Roecker, S. W.; Tiberi, C.; Aman, M.; Weinstein, A.; Lambert, C.; Drooff, C.; Oliva, S. J. C.; Peterson, K.; Bourke, J. R.; Rodzianko, A.; Gallacher, R. J.; Lavayssiere, A.; Shillington, D. J.; Khalfan, M.; Mulibo, G. D.; Ferdinand-Wambura, R.; Palardy, A.; Albaric, J.; Gautier, S.; Muirhead, J.; Lee, H.</p> <p>2015-12-01</p> <p>Rift initiation in thick, strong continental lithosphere challenges current models of continental lithospheric deformation, in part owing to gaps in our knowledge of strain patterns in the lower crust. New geophysical, geochemical, and structural data sets from youthful magmatic (Magadi-Natron, Kivu), weakly magmatic (Malawi, Manyara), and amagmatic (Tanganyika) sectors of the cratonic East African rift system provide new insights into the distribution of brittle strain, magma <span class="hlt">intrusion</span> and storage, and time-averaged deformation. We compare and contrast time-space relations, seismogenic layer thickness variations, and fault kinematics using earthquakes recorded on local arrays and teleseisms in sectors of the Western and Eastern rifts, including the Natron-Manyara basins that developed in Archaean lithosphere. Lower crustal seismicity occurs in both the Western and Eastern rifts, including sectors on and off craton, and those with and without central rift volcanoes. In amagmatic sectors, lower crustal strain is accommodated by slip along relatively steep border faults, with oblique-slip faults linking opposing border faults that penetrate to different crustal levels. In magmatic sectors, seismicity spans surface to lower crust beneath both border faults and eruptive centers, with earthquake swarms around magma bodies. Our focal mechanisms and Global CMTs from a 2007 fault-<span class="hlt">dike</span> episode show a local rotation from ~E-W extension to NE-SE extension in this linkage <span class="hlt">zone</span>, consistent with time-averaged strain recorded in vent and eruptive chain alignments. These patterns suggest that strain localization via widespread magma <span class="hlt">intrusion</span> can occur during the first 5 My of rifting in originally thick lithosphere. Lower crustal seismicity in magmatic sectors may be caused by high gas pressures and volatile migration from active metasomatism and magma degassing, consistent with high CO2 flux along fault <span class="hlt">zones</span>, and widespread metasomatism of xenoliths. Volatile release and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23223393','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23223393"><span>Ancient igneous <span class="hlt">intrusions</span> and early expansion of the Moon revealed by GRAIL gravity gradiometry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Andrews-Hanna, Jeffrey C; Asmar, Sami W; Head, James W; Kiefer, Walter S; Konopliv, Alexander S; Lemoine, Frank G; Matsuyama, Isamu; Mazarico, Erwan; McGovern, Patrick J; Melosh, H Jay; Neumann, Gregory A; Nimmo, Francis; Phillips, Roger J; Smith, David E; Solomon, Sean C; Taylor, G Jeffrey; Wieczorek, Mark A; Williams, James G; Zuber, Maria T</p> <p>2013-02-08</p> <p>The earliest history of the Moon is poorly preserved in the surface geologic record due to the high flux of impactors, but aspects of that history may be preserved in subsurface structures. Application of gravity gradiometry to observations by the Gravity Recovery and Interior Laboratory (GRAIL) mission results in the identification of a population of linear gravity anomalies with lengths of hundreds of kilometers. Inversion of the gravity anomalies indicates elongated positive-density anomalies that are interpreted to be ancient vertical tabular <span class="hlt">intrusions</span> or <span class="hlt">dikes</span> formed by magmatism in combination with extension of the lithosphere. Crosscutting relationships support a pre-Nectarian to Nectarian age, preceding the end of the heavy bombardment of the Moon. The distribution, orientation, and dimensions of the <span class="hlt">intrusions</span> indicate a globally isotropic extensional stress state arising from an increase in the Moon's radius by 0.6 to 4.9 kilometers early in lunar history, consistent with predictions of thermal models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.1428S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1428S"><span>Sedimentation and contamination patterns of <span class="hlt">dike</span> systems along the Rhône River (France)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seignemartin, Gabrielle; Tena, Alvaro; Piégay, Hervé; Roux, Gwenaelle; Winiarski, Thierry</p> <p>2017-04-01</p> <p>Humans have historically modified the Rhône River, especially in the last centuries. In the 19th century, the river was systematically embanked for flood protection purposes, and works continued along the 20th century with <span class="hlt">dike</span> system engineering work for navigation. The Rhône was canalised and its historical course by-passed by a series of hydroelectric dams. Besides, industrial activity polluted the river. For example, high levels of PCB's were attributed to the inputs of the heavily industrialized <span class="hlt">zone</span> downstream from Lyon. During floods, these contaminants, associated with the suspended sediment, were trapped by the engineering works and the floodplain. Currently, a master plan to reactivate the river dynamics in the alluvial margins by removing the groyne-fields and <span class="hlt">dikes</span> in the by-passed sections is being implemented. Within this context, this work aims to assess historical dynamics of sediment and associated contaminants in the floodplain (e.g. trace metal elements), notably in the <span class="hlt">dike</span> system, in order to evaluate the contamination risk related to bank protection removal. With this objective, a transversal methodology has been applied coupling GIS diachronic analysis (old maps, bathymetric data, Orthophotos, LIDAR, etc.) to understand the historical floodplain evolution, sediment survey to obtain sediment thickness (metal rod and Ground Penetrating Radar), and sediment sampling (manual auger and core sampling) to obtain the metal element concentrations (X-Ray Fluorescence and Inductively Coupled Plasma Mass Spectrometry). By this way, metal element patterns were defined and used as contamination tracing indicators to apprehend the contamination history but also as geochemical background indicators to define the sediment source influence. We found that sediment temporal patterns are directly related with the by-pass construction year. Spatially, fine sediment deposition predominates in the <span class="hlt">dike</span> systems, being lower in the floodplain already disconnected in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GGG....14..712S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GGG....14..712S"><span>Formation of thick stratiform Fe-Ti oxide layers in layered <span class="hlt">intrusion</span> and frequent replenishment of fractionated mafic magma: Evidence from the Panzhihua <span class="hlt">intrusion</span>, SW China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Song, Xie-Yan; Qi, Hua-Wen; Hu, Rui-Zhong; Chen, Lie-Meng; Yu, Song-Yue; Zhang, Jia-Fei</p> <p>2013-03-01</p> <p>Panzhihua <span class="hlt">intrusion</span> is one of the largest layered <span class="hlt">intrusions</span> that hosts huge stratiform Fe-Ti oxide layers in the central part of the Emeishan large igneous province, SW China. Up to 60 m thick stratiform massive Fe-Ti oxide layers containing 85 modal% of magnetite and ilmenite and overlying magnetite gabbro compose cyclic units of the Lower <span class="hlt">Zone</span> of the <span class="hlt">intrusion</span>. The cyclic units of the Middle <span class="hlt">Zone</span> consist of magnetite gabbro and overlying gabbro. In these cyclic units, contents of Fe2O3(t), TiO2 and Cr and Fe3+/Ti4+ ratio of the rocks decrease upward, Cr content of magnetite and forsterite percentage of olivine decrease as well. The Upper <span class="hlt">Zone</span> consists of apatite gabbro characterized by enrichment of incompatible elements (e.g., 12-18 ppm La, 20-28 ppm Y) and increasing of Fe3+/Ti4+ ratio (from 1.3 to 2.3) upward. These features indicate that the Panzhihua <span class="hlt">intrusion</span> was repeatedly recharged by more primitive magma and evolved magmas had been extracted. Calculations using MELTS indicate that extensive fractionation of olivine and clinopyroxene in deep level resulted in increasing Fe and Ti contents in the magma. When these Fe-Ti-enriched magmas were emplaced along the base of the Panzhihua <span class="hlt">intrusion</span>, Fe-Ti oxides became an early crystallization phase, leading to a residual magma of lower density. We propose that the unusually thick stratiform Fe-Ti oxide layers resulted from coupling of gravity settling and sorting of the crystallized Fe-Ti oxides from Fe-Ti-enriched magmas and frequent magma replenishment along the floor of the magma chamber.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V23B4790K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V23B4790K"><span>Coupling fluid dynamics and host-rock deformation associated with magma <span class="hlt">intrusion</span> in the crust: Insights from analogue experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kavanagh, J. L.; Dennis, D. J.</p> <p>2014-12-01</p> <p>Models of magma ascent in the crust tend to either consider the dynamics of fluid flow within <span class="hlt">intrusions</span> or the associated host-rock deformation. However, these processes are coupled in nature, and so to develop a more complete understanding of magma ascent dynamics in the crust both need to be taken into account. We present a series of gelatine analogue experiments that use both Particle Image Velocimentry (PIV) and Digital Image Correlation (DIC) techniques to characterise the dynamics of fluid flow within <span class="hlt">intrusions</span> and to quantify the associated deformation of the intruded media. Experiments are prepared by filling a 40x40x30 cm3 clear-Perspex tank with a low-concentration gelatine mixture (2-5 wt%) scaled to be of comparable stiffness to crustal strata. Fluorescent seeding particles are added to the gelatine mixture during its preparation and to the magma analogue prior to injection. Two Dantec CCD cameras are positioned outside the tank and a vertical high-power laser sheet positioned along the centre line is triggered to illuminate the seeding particles with short intense pulses. Dyed water (the magma analogue) injected into the solid gelatine from below causes a vertically propagating penny-shaped crack (<span class="hlt">dike</span>) to form. Incremental and cumulative displacement vectors are calculated by cross-correlation between successive images at a defined time interval. Spatial derivatives map the fluid flow within the <span class="hlt">intrusion</span> and associated strain and stress evolution of the host, both during <span class="hlt">dike</span> propagation and on to eruption. As the gelatine deforms elastically at the experimental conditions, strain calculations correlate with stress. Models which couple fluid dynamics and host deformation make an important step towards improving our understanding of the dynamics of magma transport through the crust and to help constrain the tendency for eruption.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017StGM...39...17D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017StGM...39...17D"><span>New Experiences in <span class="hlt">Dike</span> Construction with Soil-Ash Composites and Fine-Grained Dredged Materials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duszyński, Remigiusz; Duszyńska, Angelika; Cantré, Stefan</p> <p>2017-12-01</p> <p>The supporting structure inside a coastal <span class="hlt">dike</span> is often made of dredged non-uniform sand with good compaction properties. Due to the shortage of natural construction material for both coastal and river <span class="hlt">dikes</span> and the surplus of different processed materials, new experiments were made with sand-ash mixtures and fine-grained dredged materials to replace both <span class="hlt">dike</span> core and <span class="hlt">dike</span> cover materials resulting in economical, environmentally friendly and sustainable <span class="hlt">dikes</span>. Ash from EC Gdańsk and dredged sand from the Vistula river were mixed to form an engineering material used for <span class="hlt">dike</span> construction. The optimum sand-ash composites were applied at a field test site to build a large-scale research <span class="hlt">dike</span>. Fine-grained dredged materials from Germany were chosen to be applied in a second full-scale research <span class="hlt">dike</span> in Rostock. All materials were investigated according to the standards for soil mechanical analysis. This includes basic soil properties, mechanical characteristics, such as grain-size distribution, compaction parameters, compressibility, shear strength, and water permeability. In the field, the infiltration of water into the <span class="hlt">dike</span> body as well as the erosion resistance of the cover material against overflowing water was determined. Results of both laboratory and field testing are discussed in this paper. In conclusion, the mixing of bottom ash with mineral soil, such as relatively uniform dredged sand, fairly improves the geotechnical parameters of the composite, compared to the constituents. Depending on the composite, the materials may be suitable to build a <span class="hlt">dike</span> core or an erosion-resistant <span class="hlt">dike</span> cover.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JHyd..538..304R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JHyd..538..304R"><span>Experimental saltwater <span class="hlt">intrusion</span> in coastal aquifers using automated image analysis: Applications to homogeneous aquifers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robinson, G.; Ahmed, Ashraf A.; Hamill, G. A.</p> <p>2016-07-01</p> <p>This paper presents the applications of a novel methodology to quantify saltwater <span class="hlt">intrusion</span> parameters in laboratory-scale experiments. The methodology uses an automated image analysis procedure, minimising manual inputs and the subsequent systematic errors that can be introduced. This allowed the quantification of the width of the mixing <span class="hlt">zone</span> which is difficult to measure in experimental methods that are based on visual observations. Glass beads of different grain sizes were tested for both steady-state and transient conditions. The transient results showed good correlation between experimental and numerical <span class="hlt">intrusion</span> rates. The experimental <span class="hlt">intrusion</span> rates revealed that the saltwater wedge reached a steady state condition sooner while receding than advancing. The hydrodynamics of the experimental mixing <span class="hlt">zone</span> exhibited similar traits; a greater increase in the width of the mixing <span class="hlt">zone</span> was observed in the receding saltwater wedge, which indicates faster fluid velocities and higher dispersion. The angle of <span class="hlt">intrusion</span> analysis revealed the formation of a volume of diluted saltwater at the toe position when the saltwater wedge is prompted to recede. In addition, results of different physical repeats of the experiment produced an average coefficient of variation less than 0.18 of the measured toe length and width of the mixing <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MinDe..51..343W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MinDe..51..343W"><span>Platinum mineralization in the Kapalagulu <span class="hlt">Intrusion</span>, western Tanzania</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilhelmij, Harry R.; Cabri, Louis J.</p> <p>2016-03-01</p> <p>Low-grade copper and nickel mineralization was found near the eastern shore of Lake Tanganyika at Kungwe Bay in the early part of the twentieth century. The mineralization occurs in harzburgite at the base of a layered gabbro complex known as the Kapalagulu <span class="hlt">Intrusion</span>, emplaced between the Paleoproterozoic Ubendian basement and overlying Neoproterozoic Itiaso Group metasediments. Several mining and exploration companies continued the geophysical and drilling exploration for base metals throughout the last century culminating in the discovery of high-grade platinum-group element (PGE) mineralization associated with chromitite and sulfide-bearing harzburgite within the southeastern extension of the Kapalagulu <span class="hlt">Intrusion</span> (known as the Lubalisi <span class="hlt">Zone</span>) that is covered by a layer of nickel-rich laterite regolith. The poorly layered southeastern harzburgite forms part of the >1500 m-thick Lower Ultramafic Sequence and resembles a <span class="hlt">dike</span>-like body that flares upwards into a succession of well-layered gabbroic rocks of the Upper Mafic Sequence. No PGE mineralization has been found in the layered gabbro; all the mineralization is associated with the chromite- and sulfide-rich harzburgite of the Lower Ultramafic Sequence and the laterite regolith overlying the mineralized harzburgite. The Lubalisi <span class="hlt">Zone</span> harzburgite is underlain by basal dunite and overlain by an interval of layered harzburgite and troctolite and this ultramafic sequence is folded into a syncline that plunges towards the northwest that has been modified by major dolerite-filled faults orientated subparallel to the fold axial surface. Extensive deep drilling in the Lubalisi <span class="hlt">Zone</span> of the Kapalagulu <span class="hlt">Intrusion</span> shows that the folded harzburgite can be subdivided into a lower feldspathic harzburgite, a harzburgite containing chromitite seams and intervals of sulfide and chromite mineralization known as the Main Chromite Sulfide Succession (MCSS), an overlying sulfide-rich harzburgite, and an upper feldspathic harzburgite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T31C1842D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T31C1842D"><span>Structure and Geochemistry of the Continental-Oceanic Crust Boundary of the Red Sea and the Rifted Margin of Western Arabia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dilek, Y.; Furnes, H.; Schoenberg, R.</p> <p>2009-12-01</p> <p>The continental-oceanic crust boundary and an incipient oceanic crust of the Red Sea opening are exposed within the Arabian plate along a narrow <span class="hlt">zone</span> of the Tihama Asir coastal plain in SW Saudi Arabia. <span class="hlt">Dike</span> swarms, layered gabbros, granophyres and basalts of the 22 Ma Tihama Asir (TA) continental margin ophiolite represent products of magmatic differentiation formed during the initial stages of rifting between the African and Arabian plates. Nearly 4-km-wide <span class="hlt">zone</span> of NW-trending sheeted <span class="hlt">dikes</span> are the first products of mafic magmatism associated with incipient oceanic crust formation following the initial continental breakup. Gabbro <span class="hlt">intrusions</span> are composed of cpx-ol-gabbro, cpx-gabbro, and norite/troctolite, and are crosscut by fine-grained basaltic <span class="hlt">dikes</span>. Granophyre bodies intrude the sheeted <span class="hlt">dike</span> swarms and are locally <span class="hlt">intrusive</span> into the gabbros. Regional Bouger gravity anomalies suggest that the Miocene mafic crust represented by the TA complex extends westward beneath the coastal plain sedimentary rocks and the main trough of the Red Sea. The TA complex marks an incipient Red Sea oceanic crust that was accreted to the NE side of the newly formed continental rift in the earliest stages of seafloor spreading. Its basaltic to trachyandesitic lavas and <span class="hlt">dikes</span> straddle the subalkaline-mildly alkaline boundary. Incompatible trace element relationships (e.g. Zr-Ti, Zr-P) indicate two distinct populations. The REE concentrations show an overall enrichment compared to N-MORB; light REEs are enriched over the heavy ones ((La/Yb)n > 1), pointing to an E-MORB influence. Nd-isotope data show ɛNd values ranging from +4 to +8, supporting an E-MORB melt source. The relatively large variations in ɛNd values also suggest various degrees of involvement of continental crust during ascent and emplacement, or by mixing of another mantle source.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/pa2635.photos.356809p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/pa2635.photos.356809p/"><span>2. VIEW EAST ALONG <span class="hlt">DIKE</span> TOWARDS HYDROELECTRIC GENERATING FACILITY. FORMER ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>2. VIEW EAST ALONG <span class="hlt">DIKE</span> TOWARDS HYDROELECTRIC GENERATING FACILITY. FORMER TRANSFORMER BUILDING AND SERVICE SHED SEEN TO LEFT BELOW <span class="hlt">DIKE</span> - Middle Creek Hydroelectric Dam, On Middle Creek, West of U.S. Route 15, 3 miles South of Selinsgrove, Selinsgrove, Snyder County, PA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JAfES.102...70S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JAfES.102...70S"><span>Fracturing of doleritic <span class="hlt">intrusions</span> and associated contact <span class="hlt">zones</span>: Implications for fluid flow in volcanic basins</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Senger, Kim; Buckley, Simon J.; Chevallier, Luc; Fagereng, Åke; Galland, Olivier; Kurz, Tobias H.; Ogata, Kei; Planke, Sverre; Tveranger, Jan</p> <p>2015-02-01</p> <p>Igneous <span class="hlt">intrusions</span> act as both carriers and barriers to subsurface fluid flow and are therefore expected to significantly influence the distribution and migration of groundwater and hydrocarbons in volcanic basins. Given the low matrix permeability of igneous rocks, the effective permeability in- and around <span class="hlt">intrusions</span> is intimately linked to the characteristics of their associated fracture networks. Natural fracturing is caused by numerous processes including magma cooling, thermal contraction, magma emplacement and mechanical disturbance of the host rock. Fracturing may be locally enhanced along <span class="hlt">intrusion</span>-host rock interfaces, at dyke-sill junctions, or at the base of curving sills, thereby potentially enhancing permeability associated with these features. In order to improve our understanding of fractures associated with <span class="hlt">intrusive</span> bodies emplaced in sedimentary host rocks, we have investigated a series of outcrops from the Karoo Basin of the Eastern Cape province of South Africa, where the siliciclastic Burgersdorp Formation has been intruded by various <span class="hlt">intrusions</span> (thin dykes, mid-sized sheet <span class="hlt">intrusions</span> and thick sills) belonging to the Karoo dolerite. We present a quantified analysis of fracturing in- and around these igneous <span class="hlt">intrusions</span> based on five outcrops at three individual study sites, utilizing a combination of field data, high-resolution lidar virtual outcrop models and image processing. Our results show a significant difference between the three sites in terms of fracture orientation. The observed differences can be attributed to contrasting <span class="hlt">intrusion</span> geometries, outcrop geometry (for lidar data) and tectonic setting. Two main fracture sets were identified in the dolerite at two of the sites, oriented parallel and perpendicular to the contact respectively. Fracture spacing was consistent between the three sites, and exhibits a higher degree of variation in the dolerites compared to the host rock. At one of the study sites, fracture frequency in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1414101H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1414101H"><span>Assessment of Environmental Radiation Impacts Related to Granites, <span class="hlt">Dikes</span> and Stream Sediments of Sharm El-Sheikh Area, South Sinai, Egypt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heikal, M.; Ghoneim, M.; El Galy, M.; El Dousky, B.; Sherif, M.</p> <p>2012-04-01</p> <p>Sharm El Sheikh area represents one of the most touristic resort allover the world. This area is surrounded by such exposures of Precambrian granites and <span class="hlt">dike</span> swarms as well as Miocene-Pliocene sedimentary rocks that imply more or less radionuclides U, Th, Ra and K. The radioactivity imposed within the Precambrian rocks has carefully focalized on both field and lab using up-to-date equipments and instruments. In order to evaluate the radiological hazard of the natural radioactivity, the radium equivalent activity (Raeq), gamma activity concentration index (Iγ), external hazard index (Hex) internal hazard index (Hin) and annual effective dose rate (AEDR) have been calculated and compared with the internationally approved values. The permissible values for each index revealed that all exposures of granite and mafic <span class="hlt">dikes</span> have values below safety limits of radiation. The stream sediments within the major wadis are also safe and available for the population and agricultural purposes and/or as construction materials. On the other hand, the felsic <span class="hlt">dikes</span> that occur far from Sharm El Sheikh town exceed the permissible radiation limits indicating their environmental hazards impacts. It was recommended to restrict land use in a buffer <span class="hlt">zone</span> adjacent to the felsic <span class="hlt">dikes</span> of very limited distributions. A planned major town extension of Sharm El Sheikh area has to be stopped around and within these <span class="hlt">dikes</span> sites, but alternative future residential areas could be delineated to the northwest of the town. An intensive coordination with the Ministry of Environmental Affairs of Egypt, the town planners and other affected authorities guarantees must take into considerations the outstanding integration of the recommendations of our study into future town and regional land use planning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JGRB..111.5204W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JGRB..111.5204W"><span>Volcano-earthquake interaction at Mauna Loa volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walter, Thomas R.; Amelung, Falk</p> <p>2006-05-01</p> <p>The activity at Mauna Loa volcano, Hawaii, is characterized by eruptive fissures that propagate into the Southwest Rift <span class="hlt">Zone</span> (SWRZ) or into the Northeast Rift <span class="hlt">Zone</span> (NERZ) and by large earthquakes at the basal decollement fault. In this paper we examine the historic eruption and earthquake catalogues, and we test the hypothesis that the events are interconnected in time and space. Earthquakes in the Kaoiki area occur in sequence with eruptions from the NERZ, and earthquakes in the Kona and Hilea areas occur in sequence with eruptions from the SWRZ. Using three-dimensional numerical models, we demonstrate that elastic stress transfer can explain the observed volcano-earthquake interaction. We examine stress changes due to typical <span class="hlt">intrusions</span> and earthquakes. We find that <span class="hlt">intrusions</span> change the Coulomb failure stress along the decollement fault so that NERZ <span class="hlt">intrusions</span> encourage Kaoiki earthquakes and SWRZ <span class="hlt">intrusions</span> encourage Kona and Hilea earthquakes. On the other hand, earthquakes decompress the magma chamber and unclamp part of the Mauna Loa rift <span class="hlt">zone</span>, i.e., Kaoiki earthquakes encourage NERZ <span class="hlt">intrusions</span>, whereas Kona and Hilea earthquakes encourage SWRZ <span class="hlt">intrusions</span>. We discuss how changes of the static stress field affect the occurrence of earthquakes as well as the occurrence, location, and volume of <span class="hlt">dikes</span> and of associated eruptions and also the lava composition and fumarolic activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012269','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012269"><span>Petrology, composition, and age of <span class="hlt">intrusive</span> rocks associated with the Quartz Hill molybdenite deposit, southeastern Alaska.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hudson, T.; Smith, James G.; Elliott, R.L.</p> <p>1979-01-01</p> <p>A large porphyry molybdenum deposit (Quartz Hill deposit) was recently discovered in the heart of the Coast Range batholithic complex about 70 km E of Ketchikan, SE Alaska. <span class="hlt">Intrusive</span> rocks associated with the mineral deposit form two composite epizonal to hypabyssal stocks and many <span class="hlt">dikes</span> in country rocks. All observed metallization and alteration is within the Quartz Hill stock. Molybdenite forms fracture coatings and occurs in veins with quartz. Alteration is widespread and includes development of secondary quartz, pyrite, K-feldspar, biotite, white mica, chlorite, and zeolite. Field relations indicate that the stocks were emplaced after regional uplift and erosion of the Coast Range batholithic complex, and K-Ar data show that <span class="hlt">intrusion</span> and alteration took place in late Oligocene time, about 27 to 30 Ma ago. Data from the Ketchikan quadrangle indicate that porphyry molybdenum metallization in the Coast Range batholithic complex is associated with regionally extensive but spotty, middle Tertiary or younger, felsic magmatism. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAESc.141..112L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAESc.141..112L"><span>Petrogenesis of the Dalongkai ultramafic-mafic <span class="hlt">intrusion</span> and its tectonic implication for the Paleotethyan evolution along the Ailaoshan tectonic <span class="hlt">zone</span> (SW China)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Huichuan; Wang, Yuejun; Zi, Jian-Wei</p> <p>2017-06-01</p> <p>Layered ultramafic-mafic <span class="hlt">intrusions</span> are usually formed in an arc/back-arc or intra-plate tectonic environment, or genetically related to a mantle plume. In this paper, we report on an ultramafic-mafic <span class="hlt">intrusion</span>, the Dalongkai <span class="hlt">intrusion</span> in the Ailaoshan tectonic <span class="hlt">zone</span> (SW China), whose occurrence is closely associated with arc/back-arc magmatic rocks. The Dalongkai <span class="hlt">intrusion</span> is composed of plagioclase-lherzolite, hornblende-peridotite, lherzolite and wehrlite at the bottom, cumulate plagioclase-pyroxenite at the middle part, changing to fine-grained gabbro towards the upper part of the <span class="hlt">intrusion</span>, forming layering structure. Zircons from the plagioclase-pyroxenites and gabbros yielded U-Pb ages of 272.1 ± 1.7 Ma and 266.4 ± 5.8 Ma, respectively. The plagioclase-pyroxenites show cumulate textures, and are characterized by high MgO (25.0-28.0 wt.%; mg# = 80.6-82.3), Cr (1606-2089 ppm) and Ni (893-1203 ppm) contents, interpreted as early cumulate phases. By contrast, the gabbros have relatively lower mg# values (56.3-62.7), and Cr (157-218 ppm) and Ni (73-114 ppm) concentrations, and may represent frozen liquids. The plagioclase-pyroxenites and gabbros share similar chondrite-normalized REE patterns and primitive mantle-normalized trace element profiles which are analogous to those of typical back-arc basin basalts. The εNd(t) values for both rock types range from +2.20 to +4.22. These geochemical and isotopic signatures suggest that the Dalongkai ultramafic-mafic rocks originated from a MORB-like mantle source metasomatized by subduction-related, sediment-derived fluids. Our data, together with other geological evidence, indicate that the emplacement of the Dalongkai ultramafic-mafic <span class="hlt">intrusion</span> most likely occurred in a back-arc extensional setting associated with subduction of the Ailaoshan Paleotethyan branch ocean during the Middle Permian, thus ruling out the previously speculated linkage to the Emeishan mantle plume, or to an intra-continental rift.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.springerlink.com/content/b16q171628wp85t2','USGSPUBS'); return false;" href="http://www.springerlink.com/content/b16q171628wp85t2"><span>Saltwater <span class="hlt">intrusion</span> in coastal regions of North America</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barlow, Paul M.; Reichard, Eric G.</p> <p>2010-01-01</p> <p>Saltwater has intruded into many of the coastal aquifers of the United States, Mexico, and Canada, but the extent of saltwater <span class="hlt">intrusion</span> varies widely among localities and hydrogeologic settings. In many instances, the area contaminated by saltwater is limited to small parts of an aquifer and to specific wells and has had little or no effect on overall groundwater supplies; in other instances, saltwater contamination is of regional extent and has resulted in the closure of many groundwater supply wells. The variability of hydrogeologic settings, three-dimensional distribution of saline water, and history of groundwater withdrawals and freshwater drainage has resulted in a variety of modes of saltwater <span class="hlt">intrusion</span> into coastal aquifers. These include lateral <span class="hlt">intrusion</span> from the ocean; upward <span class="hlt">intrusion</span> from deeper, more saline <span class="hlt">zones</span> of a groundwater system; and downward <span class="hlt">intrusion</span> from coastal waters. Saltwater contamination also has occurred along open boreholes and within abandoned, improperly constructed, or corroded wells that provide pathways for vertical migration across interconnected aquifers. Communities within the coastal regions of North America are taking actions to manage and prevent saltwater <span class="hlt">intrusion</span> to ensure a sustainable source of groundwater for the future. These actions can be grouped broadly into scientific monitoring and assessment, engineering techniques, and regulatory approaches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1919230B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1919230B"><span>Reactive transport modeling of ferroan dolomitization by seawater interaction with mafic igneous <span class="hlt">dikes</span> and carbonate host rock at the Latemar platform, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blomme, Katreine; Fowler, Sarah Jane; Bachaud, Pierre</p> <p>2017-04-01</p> <p> share these benefits (e.g. [6]). Predicted alteration mineral assemblages are consistent with observations on <span class="hlt">dikes</span> and with ferroan and non-ferroan dolomite genesis. The simulation results also show that fluid dolomitizing potential (Mg/Ca and Fe/Mg) increases during dissolution of igneous solid solution minerals. Enrichment in fluid Fe concentration is sufficient to stabilize ferroan replacement dolomite. Consistent with field observations, ferroan dolomite forms closest to <span class="hlt">dikes</span> due to the abundance of Fe associated with the <span class="hlt">dikes</span>. This leads to depletion of Fe in fluid flowing away from <span class="hlt">dikes</span> and formation of non-ferroan replacement dolomite further afield. References S.K. Carmichael, J.M. Ferry, W.F. McDonough, Formation of replacement dolomite in the Latemar carbonate buildup, Dolomites, Northern Italy: Part 1. Field relations, mineralogy and geochemistry, Am. J. Sci. 308 (2008) 851-884. J.M. Ferry, B.H. Passey, C. Vasconcelos, J.M. Eiler, Formation of dolomite at 40 - 80 °C in the Latemar carbonate buildup, Dolomites, Italy, from clumped isotope thermometry, Geology. 39 (2011) 571-574. C. Jacquemyn, M. Huysmans, D. Hunt, G. Casini, R. Swennen, Multi-scale three-dimensional distribution of fracture- and igneous <span class="hlt">intrusion</span>- controlled hydrothermal dolomite from digital outcrop model, Latemar platform, Dolomites, northern Italy, Am. Assoc. Pet. Geol. Bull. 99 (2015) 957-984. C. Jacquemyn, H. El Desouky, D. Hunt, G. Casini, R. Swennen, Dolomitization of the Latemar platform: Fluid flow and dolomite evolution, Mar. Pet. Geol. 55 (2014) 43-67. L. Trenty, A. Michel, E. Tillier, Y. Le Gallo, A Sequential Splitting Strategy for CO2 Storage Modelling, in: ECMOR X - 10th Eur. Conf. Math. Oil Recover., 2006. T. Gabellone, F. Whitaker, Secular variations in seawater chemistry controlling dolomitisation in shallow reflux systems: Insights from reactive transport modelling, Sedimentology. 63 (2016) 1233-1259.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGP51A0777B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGP51A0777B"><span>Relation between Fabric Anisotropy of Host-Rock vis-à-vis Far-Field Stress, and the Emplacement Of Pegmatite <span class="hlt">Dikes</span> - an example from the Dharwar Craton (South India)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bhatt, S.; Rana, V.; Mamtani, M. A.</p> <p>2017-12-01</p> <p><span class="hlt">Dikes</span> are known to control magma transport within the lithosphere. They (<span class="hlt">dikes</span>) usually form by the fracturing of host rock and propagate orthogonal to the minimum principal stress direction and/or may follow the pre-existing anisotropy depending on the magnitude of fluid pressure and the tensile strength of the host rock. Pegmatite veins/<span class="hlt">dikes</span> are often associated with hydraulic fracturing and high magmatic fluid pressure, which is attributed to volatile rich hydrous melt. The Koppal Pluton (KP) is a syenite body that lies to the East of the Chitradurga Shear <span class="hlt">Zone</span>, which separates the Dharwar Craton into East and West Dharwar Craton. The KP is visually isotropic and profusely permeated by pegmatite <span class="hlt">dikes</span>. Orientation data of the pegmatite <span class="hlt">dikes</span> (n=357) were collected for geometric and paleostress analysis. The orientation of anisotropy with respect to the maximum principal stress and fluid pressure dictates whether a new fracture will form or a pre-existing anisotropy will be reactivated/dilated. To understand the relationship between the pre-existing anisotropy and orientation of pegmatite <span class="hlt">dikes</span>, anisotropy of magnetic susceptibility (AMS) analysis was performed on the samples of KP. AMS analysis reveals NNE-SSW oriented magnetic fabric ascribed to regional D3 deformational event (NW-SE compression). Mean orientation of the magnetic fabric (NNE-SSW) is oblique to the mean orientation of the pegmatite <span class="hlt">dikes</span> (NNW-SSE). It is envisaged that pegmatite <span class="hlt">dikes</span> emplaced syntectonically as mode-I crack during regional D3 deformation event (pure shear dominated transpression) and developed oblique to the magnetic fabric of the pluton. The present study leads to a better understanding about the influence and interaction of principle stress, magmatic fluid pressure, and host-rock anisotropy on the ascent and emplacement of pegmatite <span class="hlt">dikes</span> that intrude the visually isotropic KP. Acknowledgments: SB acknowledges INSPIRE Fellowship Programme (Award no: IF131138) of DST (New</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2016/1169/ofr20161169.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2016/1169/ofr20161169.pdf"><span>Environmental and eelgrass response to <span class="hlt">dike</span> removal: Nisqually River Delta (2010–14)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Takesue, Renee K.</p> <p>2016-10-03</p> <p>Restoration of tidal flows to formerly <span class="hlt">diked</span> marshland can alter land-to-sea fluxes and patterns of accumulation of terrestrial sediment and organic matter, and these tidal flows can also affect existing nearshore habitats. <span class="hlt">Dikes</span> were removed from 308 hectares (ha) of the Nisqually National Wildlife Refuge on the Nisqually River Delta in south Puget Sound, Washington, in fall 2009 to improve habitat for wildlife, such as juvenile salmon. Ecologically important intertidal and subtidal eelgrass (Zostera marina) beds grow on the north and west margins of the delta. The goal of this study was to understand long-term changes in eelgrass habitat and their relation to <span class="hlt">dike</span> removal. Sediment and eelgrass properties were monitored annually in May from 2010 to 2014 at two sites on the west side of the Nisqually River Delta along McAllister Creek, a spring-fed creek near two restored tidal channels. In May 2014, the mean canopy height of eelgrass was the same as in previous years in an 8-ha bed extending to the Nisqually River Delta front, but mean canopy height was 20 percent lower in a 0.3-ha eelgrass bed closer to the restored marsh when compared to mean canopy height of eelgrass in May 2010, 6 months after <span class="hlt">dike</span> removal was completed. Over 5 years, the amount of eelgrass leaf area per square meter (m2) in the 8-ha bed increased slightly, and surface-sediment grain size became finer. In contrast, in the 0.3-ha bed, eelgrass leaf area per m2 decreased by 45 percent, and surface sediment coarsened. Other potential stressors, including sediment pore water reduction-oxidation potential (redox) and hydrogen sulfide (H2S) concentration in the eelgrass rhizosphere, or root <span class="hlt">zone</span>, were below levels that negatively affect eelgrass growth and therefore did not appear to be environmental stressors on plants. Eelgrass biomass partitioning, though less favorable in the 8-ha eelgrass bed compared to the 0.3-ha one, was well above the critical above-ground to below-ground biomass ratio of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhDT.......195M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhDT.......195M"><span>Time dependent deformation of Kilauea Volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montgomery-Brown, Emily Kvietka Desmarais</p> <p></p> <p> to a decollement structure 8 km under the south flank, and the locations of the microearthquakes suggest that both occur on the same structure. In 2007, Episode 56 of the Pu'u 'O'o-Kupianaha eruption occurred. This episode was exciting both because it was the largest <span class="hlt">intrusion</span> in the last decade, and because it occurred concurrently with a flank slow-slip event. The <span class="hlt">intrusion</span> started on Father's day (June 17th), 2007 with increased seismicity and abrupt tilts at the summit and rift <span class="hlt">zones</span>. Quasi-static models of the total deformation determined from GPS, tilt, and InSAR indicate that the <span class="hlt">intrusion</span> occurred on two en echelon <span class="hlt">dike</span> segments in the upper East Rift <span class="hlt">Zone</span> along with deformation consistent with slow-slip in the same areas of previous events. The ˜ 2 m maximum opening occurred on the eastern segment near Makaopui crater. Unlike previous <span class="hlt">intrusions</span> in 1997, 1999, and 2000, the <span class="hlt">dike</span> model was not sufficient to explain deformation on the western flank. Additionally, a coastal tiltmeter installed in anticipation of a slow-slip event recorded tilts consistent with those observed during the 2005 slow-slip event. These observations led to the conclusion that a concurrent slow-slip event occurred. Geodetic models indicate a similar amount of decollement slip occurred as in previous slow-slip events. Sub-daily GPS positions were used to study the spatio-temporal distribution of the <span class="hlt">dike</span> <span class="hlt">intrusion</span>. The time-dependent <span class="hlt">intrusion</span> model shows that the <span class="hlt">intrusion</span> began on the western en echelon segment before jumping to the eastern segment, which accumulated the majority of the 2 m of opening. Sub-daily GPS positions limit the number of stations available since there are very few continuous stations north of the East Rift <span class="hlt">Zone</span>, where coverage is critical for separating the <span class="hlt">intrusion</span> from the slow-slip. However, an ENVISAT interferogram at 08:22 on June 18, 2007 provides additional spatial coverage of deformation up to that point. Combining this image with the GPS and tilt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V44C..04M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V44C..04M"><span>Evolution of Volcano-Plutonic Centers in the Northern Colorado River Extensional Corridor, Nevada-Arizona: Protracted Cycles of Replenishment, Mush Accumulation, Fractionation, and Melt Extraction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, C. F.; Miller, J. S.; Claiborne, L. L.; Walker, B. A.; Faulds, J. E.; Wooden, J. L.</p> <p>2007-12-01</p> <p>Three major magmatic systems were simultaneously active during early development of the northern Colorado River extensional corridor. These systems, centered on Spirit Mountain batholith, Searchlight pluton, and Aztec Wash and Nelson plutons, include hypabyssal <span class="hlt">intrusions</span> as well as coarser, deeper-seated rocks emplaced at depths of 5-13 km. Erupted products of Searchlight are clearly exposed; connections between the other systems and extensive coeval volcanic sequences, while very likely, remain unverified. <span class="hlt">Intrusion</span> at each center began at 17-18 Ma and terminated with a <span class="hlt">dike</span> swarm at ca. 15.5 Ma. <span class="hlt">Dikes</span>, sills, and evidence for mingling document the frequent replenishment suggested by longevity of the centers. Quenched magmas in pillows, <span class="hlt">dikes</span>, and chilled margins indicate that input included trachybasalt (49- 52 wt pct SiO2), trachydacite (quartz monzonite; 62-65 wt pct SiO2), and low-Si rhyolite (granite; ca. 73 wt pct SiO2); similar magmas formed a large part of the regional volcanic sequence. Some of the basalt may represent juvenile magma from enriched mantle, but Sr and Nd isotopic data indicate that all other input magmas are hybrids with both juvenile and ancient crustal components. Although local mixing is evident from field and geochemical evidence, the system-wide hybridization occurred at deeper crustal levels prior to emplacement into the upper crust. Whole-rock elemental compositions, field relations, crystal-size distributions and textures within the volcanic rocks and co-genetic <span class="hlt">intrusions</span> indicate repeated cycles of magma emplacement and extraction of fractionated melt from cumulate mush. Cumulates are enriched in Sr and Ba and have positive Eu anomalies relative to input magmas. The melt-rich extracts have high-silica rhyolite compositions. They are exposed in plutons as small <span class="hlt">dikes</span> and large subhorizontal sheets and roof <span class="hlt">zones</span> comprising fine-grained, commonly vesicle-rich aplitic granite, and they erupted from the Searchlight center and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPhCS.720a2052M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPhCS.720a2052M"><span>Theoretical prediction of gold vein location in deposits originated by a wall magma <span class="hlt">intrusion</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martin, Pablo; Maass-Artigas, Fernando; Cortés-Vega, Luis</p> <p>2016-05-01</p> <p>The isotherm time-evolution resulting from the <span class="hlt">intrusion</span> of a hot <span class="hlt">dike</span> in a cold rock is analized considering the general case of nonvertical walls. This is applied to the theoretical prediction of the gold veins location due to isothermal evolution. As in previous treatments earth surface effects are considered and the gold veins are determined by the envelope of the isotherms. The locations of the gold veins in the Callao mines of Venezuela are now well predicted. The new treatment is now more elaborated and complex that in the case of vertical walls, performed in previous papers, but it is more adequated to the real cases as the one in El Callao, where the wall is not vertical.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1979/0844/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1979/0844/report.pdf"><span>Geology and porphyry copper-type alteration-mineralization of igneous rocks at the Christmas Mine, Gila County, Arizona</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Koski, Randolph A.</p> <p>1979-01-01</p> <p>The Christmas copper deposit, located in southern Gila County, Arizona, is part of the major porphyry copper province of southwestern North America. Although Christmas is known for skarn deposits in Paleozoic carbonate rocks, ore-grade porphyry-type copper mineralization also occurs in a composite granodioritic <span class="hlt">intrusive</span> complex and adjacent mafic volcanic country rocks. This study considers the nature, distribution, and genesis of alteration-mineralization in the igneous rock environment at Christmas. At the southeast end of the Dripping Spring Mountains, the Pennsylvanian Naco Limestone is unconformably overlain by the Cretaceous Williamson Canyon Volcanics, a westward-thinning sequence of basaltic volcanic breccia and lava flows, and subordinate clastic sedimentary rocks. Paleozoic and Mesozoic strata are intruded by Laramide-age <span class="hlt">dikes</span>, sills, and small stocks of hornblende andesite porphyry and hornblende rhyodacite porphyry, and the mineralized Christmas <span class="hlt">intrusive</span> complex. Rocks of the elongate Christmas stock, intruded along an east-northeast-trending fracture <span class="hlt">zone</span>, are grouped into early, veined quartz diorite (Dark Phase), biotite granodiorite porphyry (Light Phase), and granodiorite; and late, unveined dacite porphyry and granodiorite porphyry. Biotite rhyodacite porphyry <span class="hlt">dikes</span> extending east and west from the vicinity of the stock are probably coeval with biotite granodiorite porphyry. Accumulated normal displacement of approximately 1 km along the northwest-trending Christmas-Joker fault system has juxtaposed contrasting levels (lower, <span class="hlt">intrusive</span>-carbonate rock environment and upper, <span class="hlt">intrusive</span>-volcanic rock environment) within the porphyry copper system. K-Ar age determinations and whole-rock chemical analyses of the major <span class="hlt">intrusive</span> rock types indicate that Laramide calc-alkaline magmatism and ore deposition at Christmas evolved over an extended period from within the Late Cretaceous (~75-80 m.y. ago) to early Paleocene (~63-61 m.y. ago). The sequence of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=273960','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=273960"><span>Flow near a model spur <span class="hlt">dike</span> with a fixed scoured bed</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Three-dimensional flow velocities were measured using an acoustic Doppler velocimeter at a closely spaced grid over a fixed scoured bed with a submerged spur <span class="hlt">dike</span>. Three-dimensional flow velocities were measured at 3484 positions around the trapezoidal shaped submerged model spur <span class="hlt">dike</span> over a fixed ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OptLT.103..346S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptLT.103..346S"><span>Distributed optical fiber-based monitoring approach of spatial seepage behavior in <span class="hlt">dike</span> engineering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Su, Huaizhi; Ou, Bin; Yang, Lifu; Wen, Zhiping</p> <p>2018-07-01</p> <p>The failure caused by seepage is the most common one in <span class="hlt">dike</span> engineering. As to the characteristics of seepage in <span class="hlt">dike</span>, such as longitudinal extension engineering, the randomness, strong concealment and small initial quantity order, by means of distributed fiber temperature sensor system (DTS), adopting an improved optical fiber layer layout scheme, the location of initial interpolation point of the saturation line is obtained. With the barycentric Lagrange interpolation collocation method (BLICM), the infiltrated surface of <span class="hlt">dike</span> full-section is generated. Combined with linear optical fiber monitoring seepage method, BLICM is applied in an engineering case, which shows that a real-time seepage monitoring technique is presented in full-section of <span class="hlt">dike</span> based on the combination method.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Tecto..35.1177H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Tecto..35.1177H"><span>Mechanical anisotropy control on strain localization in upper mantle shear <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Herwegh, Marco; Mercolli, Ivan; Linckens, Jolien; Müntener, Othmar</p> <p>2016-05-01</p> <p>Mantle rocks at oceanic spreading centers reveal dramatic rheological changes from partially molten to solid-state ductile to brittle deformation with progressive cooling. Using the crustal-scale Wadi al Wasit mantle shear <span class="hlt">zone</span> (SZ, Semail ophiolite, Oman), we monitor such changes based on quantitative field and microstructural investigations combined with petrological and geochemical analyses. The spatial distribution of magmatic <span class="hlt">dikes</span> and high strain <span class="hlt">zones</span> gives important information on the location of magmatic and tectonic activity. In the SZ, <span class="hlt">dikes</span> derived from primitive melts (websterites) are distributed over the entire SZ but are more abundant in the center; <span class="hlt">dikes</span> from more evolved, plagioclase saturated melts (gabbronorites) are restricted to the SZ center. Accordingly, harzburgite deformation fabrics show a transition from protomylonite (1100°C), mylonite (900-800°C) to ultramylonite (<700°C) and a serpentine foliation (<500°C) from the SZ rim to the center. The spatial correlation between solid-state deformation fabrics and magmatic features indicates progressive strain localization in the SZ on the cooling path. Three stages can be discriminated: (i) Cycles of melt injection (dunite channels and websterite <span class="hlt">dikes</span>) and solid-state deformation (protomylonites-mylonites; 1100-900°C), (ii) dominant solid-state deformation in harzburgite mylonites (900-800°C) with some last melt injections (gabbronorites) and ultramylonites (<700°C), and (iii) infiltration of seawater inducing a serpentine foliation (<500°C) followed by cataclasis during obduction. The change of these processes in space and time indicates that early <span class="hlt">dike</span>-related ridge-parallel deformation controls the onset of the entire strain localization history promoting nucleation sites for different strain weakening processes as a consequence of changing physicochemical conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.8299B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.8299B"><span>How integrating 3D LiDAR data in the <span class="hlt">dike</span> surveillance protocol: The French case</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bretar, F.; Mériaux, P.; Fauchard, C.</p> <p>2012-04-01</p> <p>The recent and dramatic floods of the last years in Europe (e.g. Rhône river major flood, December 2003, Windstorm Xynthia, February 2010, in France) and in the United-States (Hurricane Katrina, August 2005) showed the vulnerability of flood or coastal defence systems. The first key point for avoiding these dramatic damages and the high cost of a failure and its consequences lies in the appropriate conception and construction of the <span class="hlt">dikes</span>, but above all in the relevance of the surveillance protocol. Many factors introduce weaknesses in the fluvial or maritime <span class="hlt">dikes</span>. Most of them are old embankment structures. For instance, some of the French Loire River <span class="hlt">dikes</span> were built several centuries ago. They may have been rebuilt, modified, heightened several times, with some materials that do not necessarily match the original conception of the structure. In other respects, tree roots or animal burrows could modify the structure of the <span class="hlt">dike</span> and reduce the watertightness or mechanical properties. The French government has built a national database, "BarDigues", since 1999 to inventory and characterize <span class="hlt">dikes</span>. Today, there are approx. 9000 km of <span class="hlt">dikes</span> protecting 1.5 to 2 millions of people. In the meantime, a GIS application, called « <span class="hlt">Dike</span> SIRS » [Maurel P., 2004] , provides an operational and accurate tool to several great stakeholders in charge of managing more than 100 km of <span class="hlt">dikes</span>. Today, the <span class="hlt">dike</span> surveillance and diagnosis protocol consists in identifying the weaknesses of the structure and providing the degree of safety by making a preliminary study (historical research, geological and morphodynamic study, topography), geophysical study (e.g. electromagnetic methods and electrical resistivity tomography) and at last geotechnical study (e.g. drillings and stability modelling) at the very local scale when necessary [Mériaux P. & Royet P, 2007] . Considering the stretch of hundreds of kilometres, rapid, cost-effective and reliable techniques for surveying the <span class="hlt">dike</span> must be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1220/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1220/report.pdf"><span><span class="hlt">Intrusive</span> rocks of the Holden and Lucerne quadrangles, Washington; the relation of depth <span class="hlt">zones</span>, composition, textures, and emplacement of plutons</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cater, Fred W.</p> <p>1982-01-01</p> <p> serpentine. These occur either as included irregular masses in later <span class="hlt">intrusives</span> or as tectonically emplaced lenses in metamorphic rocks. Also of uncertain age but probably much younger, perhaps as young as Eocene, are larger masses of hornblendite and hornblende periodotite that grade into hornblende gabbro. These are exposed on the surface and in the underground workings of the Holden mine. Oldest of the granitoid <span class="hlt">intrusives</span> are the narrow, nearly concordant Dumbell Mountain plutons, having a radiometric age of about 220 m.y. They consist of gneissic hornblende-quartz diorite and quartz diorite gneiss. Most contacts consist of lit-par-lit <span class="hlt">zones</span>, but some are gradational or more rarely sharp. The plutons are typically catazonal. Closely resembling the Dumbell Mountain plutons in outcrop appearance, but differing considerably in composition, are the Bearcat Ridge plutons. These consist of gneissic quartz diorite and granodiorite. The Bearcat Ridge plutons are not in contact with older dated plutons, but because their textural and structural characteristics so closely resemble those of the Dumbell Mountain plutons, they are considered to be the same age. Their composition, however, is suggestive of a much younger age. Cutting the Dumbell Mountain plutons is the Leroy Creek pluton, consisting of gneissic biotite-quartz diorite and trondjhemite. The gneissic foliation in the Leroy Creek is characterized by a strong and pervasive swirling. Cutting both the Dumbell Mountain and Leroy Creek plutons are the almost dikelike Seven-fingered Jack plutons. These range in composition from gabbro to quartz diorite; associated with them are contact complexes of highly varied rocks characterized by gabbro and coarse-grained hornblendite. Most of the rocks are gneissic, but some are massive and structureless. Radiometric ages by various methods range from 100 to 193 m.y. <span class="hlt">Dikes</span>, sills, small stocks, and irregular clots of leucocratic quartz diorite and granodiorite are abundant in t</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=258852&keyword=Microsoft+AND+Excel&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=258852&keyword=Microsoft+AND+Excel&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>An Approach for Developing Site-Specific Lateral and Vertical Inclusion <span class="hlt">Zones</span> within which Structures Should be Evaluated for Petroleum Vapor <span class="hlt">Intrusion</span> due to Releases of Motor Fuel from Underground Storage Tanks</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Buildings may be at risk from Petroleum Vapor <span class="hlt">Intrusion</span> (PVI) when they overlie petroleum hydrocarbon contamination in the unsaturated <span class="hlt">zone</span> or dissolved in groundwater. The U.S. EPA Office of Underground Storage Tanks (OUST) is preparing Guidance for Addressing Petroleum Vapor I...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..341...84K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..341...84K"><span>Fluidization of host sediments and its impacts on peperites-forming processes, the Cretaceous Buan Volcanics, Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kwon, Chang Woo; Gihm, Yong Sik</p> <p>2017-07-01</p> <p>In the Cretaceous Buan Volcanics (SW Korea), blocky and fluidal peperites are developed in a bed of poorly sorted, massive pumiceous lapilli tuff (hot sediments) as a result of the vertical to subvertical <span class="hlt">intrusion</span> of the trachyandesitic <span class="hlt">dikes</span> into the bed. Blocky peperites are composed of polyhedral or platy juvenile clasts with a jigsaw-crack texture. Fluidal peperites are characterized by fluidal or globular juvenile clasts with irregular or ragged margins. The blocky peperites are ubiquitous in the host sediments, whereas the fluidal peperites only occur in fine-grained <span class="hlt">zone</span> (well sorted fine to very fine ash) that are aligned parallel to the <span class="hlt">dike</span> margin. The development of the fine-grained <span class="hlt">zone</span> within the poorly sorted host sediments is interpreted to form by grain size segregation caused by upward moving pore water (fluidization) that has resulted from heat transfer from intruding magma toward the waterlogged host sediments during <span class="hlt">intrusion</span>. With the release of pore water and the selective entrainment of fine-grained ash, the fine-grained <span class="hlt">zone</span> formed within the host sediments. Subsequent interactions between the fine-grained <span class="hlt">zone</span> and the intruding magma resulted in ductile deformation of the magma, which generated fluidal peperites. Outside the fine-grained <span class="hlt">zone</span>, because of the relative deficiency of both pore water and fine-grained ash, intruding magma fragmented in a brittle manner, resulting in the formation of blocky peperites. The results of this study suggest that redistribution of constituent particles (ash) and interstitial fluids during fluidization resulted in heterogeneous physical conditions of the host sediments, which influenced peperite-forming processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019695','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019695"><span>Biogeochemical effects of seawater restoration to <span class="hlt">diked</span> salt marshes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Portnoy, J.W.; Giblin, A.E.</p> <p>1997-01-01</p> <p>We conducted greenhouse microcosm experiments to examine the biogeochemical effects of restoring seawater to historically <span class="hlt">diked</span> Cape Cod salt marshes. Peat cores from both seasonally flooded and drained <span class="hlt">diked</span> marshes were waterlogged with seawater, and porewater chemistry was subsequently monitored for 21 mo. The addition of seawater to highly organic, seasonally flooded peat caused the death of freshwater wetland plants, 6-8 cm of sediment subsidence, and increased N and P mineralization. Also, sulfides and alkalinity increased 10-fold, suggesting accelerated decomposition by sulfate reduction. Addition of seawater to the low-organic-content acidic peat from the drained marsh increased porewater pH, alkalinity, PO4-P, and Fe(II), which we attribute to the reestablishment of SO4 and Fe(III) mineral reduction. Increased cation exchange contributed to 6-fold increases in dissolved Fe(II) and Al and 60-fold increases in NH4-N within 6 mo of sail-nation. Seawater reintroductions to seasonally flooded <span class="hlt">diked</span> marshes will cause porewater sulfides to increase, likely reducing the success of revegetation efforts. Sulfide toxicity is of less concern in resalinated drained peats because of the abundance of Fe(II) to precipitate sulfides, and of NH4-N to offset sulfide inhibition of N uptake. Restoration of either seasonally flooded or drained <span class="hlt">diked</span> marshes could stimulate potentially large nutrient and Fe(II) releases, which could in turn increase primary production and lower oxygen in receiving waters. These findings suggest that tidal restoration be gradual and carefully monitored.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/2007/250/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/2007/250/"><span>Modal Composition and Age of <span class="hlt">Intrusions</span> in North-Central and Northeast Nevada</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>du Bray, Edward A.; Crafford, A. Elizabeth Jones</p> <p>2007-01-01</p> <p>Introduction Data presented in this report characterize igneous <span class="hlt">intrusions</span> of north-central and northeast Nevada and were compiled as part of the Metallogeny of the Great Basin project conducted by the U.S. Geological Survey (USGS) between 2001 and 2007. The compilation pertains to the area bounded by lats 38.5 and 42 N., long 118.5 W., and the Nevada-Utah border (fig. 1). The area contains numerous large plutons and smaller stocks but also contains equally numerous smaller, shallowly emplaced <span class="hlt">intrusions</span>, including <span class="hlt">dikes</span>, sills, and endogenous dome complexes. Igneous <span class="hlt">intrusions</span> (hereafter, <span class="hlt">intrusions</span>) of multiple ages are major constituents of the geologic framework of north-central and northeast Nevada (Stewart and Carlson, 1978). Mesozoic and Cenozoic <span class="hlt">intrusions</span> are particularly numerous and considered to be related to subduction along the west edge of the North American plate during this time. Henry and Ressel (2000) and Ressel and others (2000) have highlighted the association between magmatism and ore deposits along the Carlin trend. Similarly, Theodore (2000) has demonstrated the association between <span class="hlt">intrusions</span> and ore deposits in the Battle Mountain area. Decades of geologic investigations in north-central and northeast Nevada (hereafter, the study area) demonstrate that most hydrothermal ore deposits are spatially, and probably temporally and genetically, associated with <span class="hlt">intrusions</span>. Because of these associations, studies of many individual <span class="hlt">intrusions</span> have been conducted, including those by a large number of Master's and Doctoral thesis students (particularly University of Nevada at Reno students and associated faculty), economic geologists working on behalf of exploration and mining companies, and USGS earth scientists. Although the volume of study area <span class="hlt">intrusions</span> is large and many are associated with ore deposits, no synthesis of available data that characterize these rocks has been assembled. Compilations that have been produced for <span class="hlt">intrusions</span> in Nevada</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021576','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021576"><span>Cooling rates and crystallization dynamics of shallow level pegmatite-aplite <span class="hlt">dikes</span>, San Diego County, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Webber, Karen L.; Simmons, William B.; Falster, Alexander U.; Foord, Eugene E.</p> <p>1999-01-01</p> <p>Pegmatites of the Pala and Mesa Grande Pegmatite Districts, San Diego County, California are typically thin, sheet-like composite pegmatite-aplite <span class="hlt">dikes</span>. Aplitic portions of many <span class="hlt">dikes</span> display pronounced mineralogical layering referred to as "line rock," characterized by fine-grained, garnet-rich bands alternating with albite- and quartz-rich bands. Thermal modeling was performed for four <span class="hlt">dikes</span> in San Diego County including the 1 m thick Himalaya <span class="hlt">dike</span>, the 2 m thick Mission <span class="hlt">dike</span>, the 8 m thick George Ashley <span class="hlt">dike</span>, and the 25 m thick Stewart <span class="hlt">dike</span>. Calculations were based on conductive cooling equations accounting for latent heat of crystallization, a melt emplacement temperature of 650 °C into 150 °C fractured, gabbroic country rock at a depth of 5 km, and an estimated 3 wt% initial H2O content in the melt. Cooling to -5 cm/s. Crystal size distribution (CSD) studies of garnet from layered aplites suggest growth rates of about 10-6 cm/s. These results indicate that the <span class="hlt">dikes</span> cooled and crystallized rapidly, with variable nucleation rates but high overall crystal-growth rates. Initial high nucleation rates coincident with emplacement and strong undercooling can account for the millimeter-size aplite grains. Lower nucleation rates coupled with high growth rates can explain the decimeter-size minerals in the hanging walls, cores, and miarolitic cavities of the pegmatites. The presence of tourmaline and/or lepidolite throughout these <span class="hlt">dikes</span> suggests that although the melts were initially H2O-undersaturated, high melt concentrations of incompatible (or fluxing) components such as B, F, and Li (±H2O), aided in the development of large pegmatitic crystals that grew rapidly in the short times suggested by the conductive cooling models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA147440','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA147440"><span>Environmental and Water Quality Operational Studies. Environmental Guidelines for <span class="hlt">Dike</span> Fields.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1984-09-01</p> <p>public release; distribution unlimited. I. DISTRIBUTION STATEMENT (of the abstract entered In Block 20, If different from Report) IS. SUPPLEMENTARY NOTES...necessary and identify by block number) Aquatic biology--Environmental aspects. (LC) <span class="hlt">Dikes</span> (Engineering)--Design and construction--Environmental...w ad Idenwify by block number) ’The environmental guidelines for <span class="hlt">dike</span> fields-contained within this report consist of environmental objectives, design</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.1245K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.1245K"><span>Igneous layering in the peralkaline <span class="hlt">intrusions</span> ,Kola Peninsula :leading role of gravitational differentiation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kogarko, L. N..</p> <p>2012-04-01</p> <p>In the center of Kola Peninsula there are two large layered <span class="hlt">intrusions</span> of agpaitic nepheline syenites - Khibina and Lovozero. . The Khibina alkaline massif (Kola Peninsula,Russia) hosts the world's largest and economically most important apatite deposit. The Khibina massif is a complex multiphase body built up from a number of ring-like and conical <span class="hlt">intrusions</span>. The apatite bearing <span class="hlt">intrusion</span> is ring-like and is represented by a layered body of ijolitic composition with a thickness of about 1 - 2 km. The upper <span class="hlt">zone</span> is represented by different types of apatite ores. These rocks consist of 60-90% euhedral very small (tenths of mm)apatite crystals. The lower <span class="hlt">zone</span> has mostly ijolitic composition. The lower <span class="hlt">zone</span> grades into underlying massive urtite consisting of 75-90% large (several mm) euhedral nepheline. Our experimental studies of systems with apatite demonstrated the near-eutectic nature of the apatite-bearing <span class="hlt">intrusion</span>, resulting in practically simultaneous crystallization of nepheline, apatite and pyroxene. The mathematical model of the formation of the layered apatite-bearing <span class="hlt">intrusion</span> based on the processes of sedimentation under the conditions of steady state convection taking account of crystal sizes is proposed. Under the conditions of steady-state convection large crystals of nepheline continuously had been settling forming massive underlying urtite whereas smaller crystals of pyroxenes, nepheline and apatite had been stirred in the convecting melt. During the cooling the intensity of convection decreased causing a settling of smaller crystals of nepheline and pyroxene and later very small crystalls of apatite in the upper part of alkaline magma chamber. The Lovozero massif, the largest of the Globe layered peralkaline <span class="hlt">intrusion</span>, comprises super-large rare-metal (Nb, Ta, REE) deposit. The main ore mineral is loparite (Na, Ce, Ca)2 (Ti, Nb)2O6 which was mined during many years. The composition of cumulus loparite changed systematically upward through the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H51A1169A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H51A1169A"><span>Three Dimensional Vapor <span class="hlt">Intrusion</span> Modeling: Model Validation and Uncertainty Analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Akbariyeh, S.; Patterson, B.; Rakoczy, A.; Li, Y.</p> <p>2013-12-01</p> <p>Volatile organic chemicals (VOCs), such as chlorinated solvents and petroleum hydrocarbons, are prevalent groundwater contaminants due to their improper disposal and accidental spillage. In addition to contaminating groundwater, VOCs may partition into the overlying vadose <span class="hlt">zone</span> and enter buildings through gaps and cracks in foundation slabs or basement walls, a process termed vapor <span class="hlt">intrusion</span>. Vapor <span class="hlt">intrusion</span> of VOCs has been recognized as a detrimental source for human exposures to potential carcinogenic or toxic compounds. The simulation of vapor <span class="hlt">intrusion</span> from a subsurface source has been the focus of many studies to better understand the process and guide field investigation. While multiple analytical and numerical models were developed to simulate the vapor <span class="hlt">intrusion</span> process, detailed validation of these models against well controlled experiments is still lacking, due to the complexity and uncertainties associated with site characterization and soil gas flux and indoor air concentration measurement. In this work, we present an effort to validate a three-dimensional vapor <span class="hlt">intrusion</span> model based on a well-controlled experimental quantification of the vapor <span class="hlt">intrusion</span> pathways into a slab-on-ground building under varying environmental conditions. Finally, a probabilistic approach based on Monte Carlo simulations is implemented to determine the probability distribution of indoor air concentration based on the most uncertain input parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/wi0215.photos.171826p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/wi0215.photos.171826p/"><span>107. DAM EARTH <span class="hlt">DIKE</span> SUBMERSIBLE DAMS PLANS ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>107. DAM - EARTH <span class="hlt">DIKE</span> - SUBMERSIBLE DAMS - PLANS & SECTIONS (ML-8-52/3-FS) March 1940 - Upper Mississippi River 9-Foot Channel, Lock & Dam No. 8, On Mississippi River near Houston County, MN, Genoa, Vernon County, WI</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.3698R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.3698R"><span>Fluvial <span class="hlt">dike</span> breaching due to overtopping: how different is it from dam breaching?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rifai, Ismail; Erpicum, Sébastien; Archambeau, Pierre; Violeau, Damien; Pirotton, Michel; El kadi Abderrezzak, Kamal; Dewals, Benjamin</p> <p>2017-04-01</p> <p>During floods in large rivers, casualties and extent of damage are often aggravated by breach formation across fluvial <span class="hlt">dikes</span>. The most frequent cause of breaching is flow overtopping. Predicting the breach geometry and associated outflow hydrograph is of critical importance for estimating the inundation characteristics in the floodplain and the resulting flood risk. Because fluvial <span class="hlt">dikes</span> are built along a main channel that conveys flowing water, fluvial <span class="hlt">dike</span> breaching differs from dam breaching, in which the embankment is built across the channel downstream of a reservoir. While a vast body of studies exists on dam breaching configuration (e.g., Schmocker et al. 2012, 2014, Müller et al. 2016), little is known on specific aspects of fluvial <span class="hlt">dike</span> breaching. We performed laboratory experiments that highlight the specific erosion processes governing fluvial <span class="hlt">dike</span> breaching (Rifai et al. 2017a). The experimental setup includes a 10 m long and 1 m wide main channel, separated from a floodplain by a 0.3 m high <span class="hlt">dike</span> of trapezoidal cross-section. The <span class="hlt">dike</span> material was homogeneous and made of uniform sand. A rectangular initial notch was cut in the crest to initiate 3D breaching. The breach development was monitored continuously using a self-developed laser profilometry technique (Rifai et al. 2016). The observations reveal that the breach develops in two stages. First, a combined breach deepening and widening occur, together with a gradual shift of the breach centreline toward the downstream side of the main channel. Later, the breach widening continues only toward the downstream side of the main channel, highlighting a significant influence of flow momentum in the main channel. Moreover, the breach cross-section is tilted toward the downstream end of the main channel, which is a signature of an asymmetric velocity distribution through the breach (Rifai et al. 2017b). When the inflow discharge in the main channel is increased, the breach development becomes much faster (e</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.T23B1411H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.T23B1411H"><span>Models of Deformation of Uppermost Oceanic Lithosphere: Comparison of Crustal Flexure in the Blönduós Area, Northern Iceland, and Structure of East Pacific Rise Crust at Hess Deep</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horst, A. J.; Karson, J. A.; Varga, R. J.; Gee, J. S.</p> <p>2007-12-01</p> <p>Models of the internal structure of oceanic crust have been constructed from studies of ophiolites and from more recent observations of tectonic windows into the upper crust. Spreading rate and/or magma supply are the central variables that control ridge processes and the ultimate architecture of ocean crust. In addition to ophiolites, Iceland also provides an important analog to study mid-ocean ridge processes and structure. Flexure <span class="hlt">zones</span> in Iceland characterize the structure of Tertiary-Recent lava flows, and are areas wherein lavas dip regionally inward toward the axis of one of several ~N/S-trending rift <span class="hlt">zones</span>. These rift <span class="hlt">zones</span> are interpreted to represent fossil spreading centers which were abandoned during a series of eastward-directed ridge jumps. In the Hildará area, north-central Iceland, the eastern side of a regional flexure is characterized by westward-dipping lavas, approximately 6-8 Ma, which are cut by east-dipping normal faults and <span class="hlt">dikes</span>. The upper-crustal structure within this flexure <span class="hlt">zone</span> from slow spread (~20 mm/yr) crust exhibits remarkable similarities to the structure of the upper crust created at a fast-spreading (110 mm/yr) segment of the East Pacific Rise (EPR) observed at Hess Deep. In this modern ocean setting, ~1 Ma crust is characterized by west-dipping lavas above consistently east-dipping (away from the EPR) <span class="hlt">dikes</span> and <span class="hlt">dike</span>-subparallel fault <span class="hlt">zones</span>. In both locations, paleomagnetic and structural data indicate that west-dipping lavas and east-dipping <span class="hlt">dikes</span> result from tectonic rotations. In addition, cross-cutting <span class="hlt">dike</span> relationships demonstrate that <span class="hlt">dike</span> <span class="hlt">intrusion</span> occurred both during and after normal fault- related tilting. These data indicate that fault-controlled tilting was initiated within the narrow neovolcanic <span class="hlt">zone</span> of the ridge and is not associated with off-axis processes. Lavas at magmatically robust ridges commonly flow away from elevated ridge-crests. Measurement of anisotropy of magnetic susceptibility (AMS) of the lavas</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021101','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021101"><span>More than one way to stretch: A tectonic model for extension along the plume track of the Yellowstone hotspot and adjacent Basin and Range Province</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Parsons, T.; Thompson, G.A.; Smith, R.P.</p> <p>1998-01-01</p> <p>The eastern Snake River Plain of southern Idaho poses a paradoxical problem because it is nearly aseismic and unfaulted although it appears to be actively extending in a SW-NE direction continuously with the adjacent block-faulted Basin and Range Province. The plain represents the 100-km-wide track of the Yellowstone hotspot during the last ???16-17 m.y., and its crust has been heavily intruded by mafic magma, some of which has erupted to the surface as extensive basalt flows. Outside the plain's distinct topographic boundaries is a transition <span class="hlt">zone</span> 30-100 km wide that has variable expression of normal faulting and magmatic activity as compared with the surrounding Basin and Range Province. Many models for the evolution of the Snake River Plain have as an integral component the suggestion that the crust of the plain became strong enough through basaltic <span class="hlt">intrusion</span> to resist extensional deformation. However, both the boundaries of the plain and its transition <span class="hlt">zone</span> lack any evidence of <span class="hlt">zones</span> of strike slip or other accommodation that would allow the plain to remain intact while the Basin and Range Province extended around it; instead, the plain is coupled to its surroundings and extending with them. We estimate strain rates for the northern Basin and Range Province from various lines of evidence and show that these strains would far exceed the elastic limit of any rocks coupled to the Basin and Range; thus, if the plain is extending along with its surroundings, as the geologic evidence indicates, it must be doing so by a nearly aseismic process. Evidence of the process is provided by volcanic rift <span class="hlt">zones</span>, indicators of subsurface <span class="hlt">dikes</span>, which trend across the plain perpendicular to its axis. We suggest that variable magmatic strain accommodation, by emplacement and inflation of <span class="hlt">dikes</span> perpendicular to the least principal stress in the elastic crust, allows the crust of the plain to extend nearly aseismically. <span class="hlt">Dike</span> injection releases accumulated elastic strain but</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GeCoA.102...65R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GeCoA.102...65R"><span>Geochemical evidence of mantle reservoir evolution during progressive rifting along the western Afar margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rooney, Tyrone O.; Mohr, Paul; Dosso, Laure; Hall, Chris</p> <p>2013-02-01</p> <p>The Afar triple junction, where the Red Sea, Gulf of Aden and African Rift System extension <span class="hlt">zones</span> converge, is a pivotal domain for the study of continental-to-oceanic rift evolution. The western margin of Afar forms the southernmost sector of the western margin of the Red Sea rift where that margin enters the Ethiopian flood basalt province. Tectonism and volcanism at the triple junction had commenced by ˜31 Ma with crustal fissuring, <span class="hlt">diking</span> and voluminous eruption of the Ethiopian-Yemen flood basalt pile. The <span class="hlt">dikes</span> which fed the Oligocene-Quaternary lava sequence covering the western Afar rift margin provide an opportunity to probe the geochemical reservoirs associated with the evolution of a still active continental margin. 40Ar/39Ar geochronology reveals that the western Afar margin <span class="hlt">dikes</span> span the entire history of rift evolution from the initial Oligocene flood basalt event to the development of focused <span class="hlt">zones</span> of <span class="hlt">intrusion</span> in rift marginal basins. Major element, trace element and isotopic (Sr-Nd-Pb-Hf) data demonstrate temporal geochemical heterogeneities resulting from variable contributions from the Afar plume, depleted asthenospheric mantle, and African lithosphere. The various <span class="hlt">dikes</span> erupted between 31 Ma and 22 Ma all share isotopic signatures attesting to a contribution from the Afar plume, indicating this initial period in the evolution of the Afar margin was one of magma-assisted weakening of the lithosphere. From 22 Ma to 12 Ma, however, diffuse <span class="hlt">diking</span> during continued evolution of the rift margin facilitated ascent of magmas in which depleted mantle and lithospheric sources predominated, though contributions from the Afar plume persisted. After 10 Ma, magmatic <span class="hlt">intrusion</span> migrated eastwards towards the Afar rift floor, with an increasing fraction of the magmas derived from depleted mantle with less of a lithospheric signature. The <span class="hlt">dikes</span> of the western Afar margin reveal that magma generation processes during the evolution of this continental rift margin</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H41F1505S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H41F1505S"><span>Effects of <span class="hlt">Dike</span> Fields on Channel Characteristics of the Lower Missiszippi River</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Simon, A.; Biedenharn, D. S.; Danis, N.; Little, C. D.</p> <p>2017-12-01</p> <p><span class="hlt">Dike</span> systems along the Lower Mississippi River have been functioning as intended through the mid-1990s. Measures of main-channel depth, which are primary metrics to evaluate the effectiveness of the <span class="hlt">dike</span> fields show significant increases at both +0 and +35 Low Water Reference Plane (LWRP). Median values for the two conditions (+0 and +35 LWRP) show increases of 19.0 and 28.8%, respectively. Main-channel depths at +0 LWRP were in the 25- to 26-ft range, indicating that main-channel depths in the <span class="hlt">dike</span>-system reaches have been maintained well above the minimum 9-ft value required. Increases in average boundary shear stress of about 8 and 18% for the whole channel and main channel at +35 LWRP, respectively, reflect increases in sediment-transport capacity. The effectiveness of the <span class="hlt">dike</span> systems in reducing the need for maintenance dredging is supported by the inverse relation between the amount of dredging and the cumulative length of constructed <span class="hlt">dikes</span>. Maintenance dredging peaked in the late 1960s at about 60 million cubic yards (yd3) in the Memphis and Vicksburg Districts and decreased to about 4 million yd3 by 2003, a reduction of about 93%. Cases where total conveyance has decreased appear to result from longer-termed, broad adjustment processes related to other factors including the historical cutoff program along the Lower Mississippi River.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V34A..02O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V34A..02O"><span>Trends in <span class="hlt">intrusive</span> and eruptive activity during Kilauea's long-lived east rift <span class="hlt">zone</span> eruption</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Orr, T. R.; Patrick, M. R.; Heliker, C.</p> <p>2011-12-01</p> <p>Kilauea Volcano's Pu`u `O`o eruption, continuing for nearly three decades, offers a unique opportunity to study trends in eruptive behavior. One such trend, that of uprift <span class="hlt">intrusion</span> ± eruption, accompanied by crater floor collapse and eruptive hiatus, has been repeated several times at Pu`u `O`o. This includes the February 7, 1993, <span class="hlt">intrusion</span>; the January 29, 1997, <span class="hlt">intrusion</span> and eruption; the September 12, 1999, <span class="hlt">intrusion</span>; and the June 17, 2007, <span class="hlt">intrusion</span> and eruption. Activity resumed within Pu`u `O`o following each of these events, and crater refilling culminated eventually in the outbreak of lava from new vents on the flank of the Pu`u `O`o cone. The pattern was repeated again in 2011, when a brief fissure eruption uprift from Pu`u `O`o started on March 5. The Pu`u `O`o crater floor dropped about 115 m in response to the eruption, which ceased on March 9. After a short hiatus, lava reappeared in Pu`u `O`o on March 26, and the crater began to fill slowly thereafter by overflow from a central lava lake. Starting in late June 2011, however, the crater floor began to uplift in a wholesale fashion, suggesting an increase in the pressure beneath the Pu`u `O`o edifice. By late July, the lava within the crater had reached its highest level since early 2004, and lava had begun to overflow from the southwestern side of the crater. On August 3, the west side of the Pu`u `O`o cone was abruptly thrust upward as a sill was injected beneath that portion of the cone. Within minutes, lava began to erupt from a crack on the west flank of Pu`u `O`o, completing the pattern of <span class="hlt">intrusion</span>, crater collapse, refilling, and breakout. During a long-lived eruption, maintaining a detailed observational and geophysical record is essential for recognizing patterns that may emerge. Recognizing such a pattern allowed Hawaiian Volcano Observatory scientists to prepare a response well in advance of the August 3, 2011 event, and provides guidance for responding to future eruption crises at Pu`u `O</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830019049','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830019049"><span>The Ponta Grossa Arch: A proposal for ts configuration and evolution from the interpretation of remote sensing data. M.S. Thesis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parada, N. D. J. (Principal Investigator); Dealmeida, T. I. R.</p> <p>1983-01-01</p> <p>Visual analysis of MSS imagery was used to construct a map of <span class="hlt">dikes</span> in a wide area of the Ponta Grossa Arch both in the Parana Basin and its basement. Analysis of the map by photographic methods defined the <span class="hlt">zone</span> of highest density of the <span class="hlt">dikes</span>, and some aspects of the longitudinal and transverse heterogeneities, as well as localized the apex of the Arch. Borders of the Arch were also suggested. Field investigations confirmed the position of the apex of the flexure on Palezoic sediments and pre-lava Mesozoic sediments. Controversial aspects of the relative absence of <span class="hlt">dikes</span> in certain units or lithologies and the composition of <span class="hlt">intrusions</span> surrounding the city of Castro were observed. The apparent synchronism between the activity of the Parana Basin and the Arch is discussed as well as the frequent inverse characteristics of vertical movements. The similarity of rocks in Brazil and Africa is also considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016871','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016871"><span>Deep magma body beneath the summit and rift <span class="hlt">zones</span> of Kilauea Volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Delaney, P.T.; Fiske, R.S.; Miklius, Asta; Okamura, A.T.; Sako, M.K.</p> <p>1990-01-01</p> <p>A magnitude 7.2 earthquake in 1975 caused the south flank of Kilauea Volcano, Hawaii, to move seaward in response to slippage along a deep fault. Since then, a large part of the volcano's edifice has been adjusting to this perturbation. The summit of Kilauea extended at a rate of 0.26 meter per year until 1983, the south flank uplifted more than 0.5 meter, and the axes of both the volcano's rift <span class="hlt">zones</span> extended and subsided; the summit continues to subside. These ground-surface motions have been remarkably steady and much more widespread than those caused by either recurrent inflation and deflation of the summit magma chamber or the episodic propagation of <span class="hlt">dikes</span> into the rift <span class="hlt">zones</span>. Kilauea's magmatic system is, therefore, probably deeper and more extensive than previously thought; the summit and both rift <span class="hlt">zones</span> may be underlain by a thick, near vertical <span class="hlt">dike</span>-like magma system at a depth of 3 to 9 kilometers.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17843792','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17843792"><span>Deep magma body beneath the summit and rift <span class="hlt">zones</span> of kilauea volcano, hawaii.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Delaney, P T; Fiske, R S; Miklius, A; Okamura, A T; Sako, M K</p> <p>1990-03-16</p> <p>A magnitude 7.2 earthquake in 1975 caused the south flank of Kilauea Volcano, Hawaii, to move seaward in response to slippage along a deep fault. Since then, a large part of the volcano's edifice has been adjusting to this perturbation. The summit of Kilauea extended at a rate of 0.26 meter per year until 1983, the south flank uplifted more than 0.5 meter, and the axes of both the volcano's rift <span class="hlt">zones</span> extended and subsided; the summit continues to subside. These ground-surface motions have been remarkably steady and much more widespread than those caused by either recurrent inflation and deflation of the summit magma chamber or the episodic propagation of <span class="hlt">dikes</span> into the rift <span class="hlt">zones</span>. Kilauea's magmatic system is, therefore, probably deeper and more extensive than previously thought; the summit and both rift <span class="hlt">zones</span> may be underlain by a thick, near vertical <span class="hlt">dike</span>-like magma system at a depth of 3 to 9 kilometers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930072214&hterms=Scottish&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DScottish','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930072214&hterms=Scottish&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DScottish"><span>Buffered and unbuffered <span class="hlt">dike</span> emplacement on Earth and Venus - Implications for magma reservoir size, depth, and rate of magma replenishment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parfitt, E. A.; Head, J. W., III</p> <p>1993-01-01</p> <p>Models of the emplacement of lateral <span class="hlt">dikes</span> from magma chambers under constant (buffered) driving pressure conditions and declining (unbuffered) driving pressure conditions indicate that the two pressure scenarios lead to distinctly different styles of <span class="hlt">dike</span> emplacement. In the unbuffered case, the lengths and widths of laterally emplaced <span class="hlt">dikes</span> will be severely limited and the <span class="hlt">dike</span> lengths will be highly dependent on chamber size; this dependence suggests that average <span class="hlt">dike</span> length can be used to infer the dimensions of the source magma reservoir. On Earth, the characteristics of many mafic-<span class="hlt">dike</span> swarms suggest that they were emplaced in buffered conditions (e.g., the Mackenzie <span class="hlt">dike</span> swarm in Canada and some <span class="hlt">dikes</span> within the Scottish Tertiary). On Venus, the distinctive radial fractures and graben surrounding circular to oval features and edifices on many size scales and extending for hundreds to over a thousand km are candidates for <span class="hlt">dike</span> emplacement in buffered conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V53A1743F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V53A1743F"><span>Stratigraphy, Hydrothermal Alteration and Evolution of the Mangakino Geothermal System, Taupo Volcanic <span class="hlt">Zone</span>, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fagan, C. J.; Wilson, C. J.; Spinks, K. D.; Browne, P. R.; Simmons, S. F.</p> <p>2006-12-01</p> <p>A major part of the ca. 1.6 Myr history of the Taupo Volcanic <span class="hlt">Zone</span> (TVZ) is represented by buried and hydrothermally altered rocks penetrated by geothermal exploration wells. The geothermal field at Mangakino is sited in the oldest TVZ caldera on the western edge of the TVZ. Four exploration wells into the field reveal a thick sequence of flat-lying ignimbrites. Basement Mesozoic greywacke metasediments were not reached by the deepest well, MA2 (3192 m), implying the presence of a thick caldera infill. Ignimbrites exposed at the surface nearby have distinct mineralogies and crystal contents, which enable correlation with down-hole lithologies. Five ignimbrites are identified in the wells: the 0.32 Ma Whakamaru, 0.93 Ma Marshall, 1.0 Ma Rocky Hill, 1.18 Ma Ahuroa and 1.25 Ma Ongatiti ignimbrites, two of which are >800m thick. The Whakamaru and Marshall units are separated by a thick sequence of lacustrine and volcaniclastic deposits related to infilling of the Mangakino caldera. The ignimbrite sequence is continuous between all wells, with no fault offset, and only well MA3 intersects two rhyolite <span class="hlt">intrusions</span> at 1190 m and 1850 m that are thought to be feeder <span class="hlt">dikes</span> to post-0.32 Ma rhyolite domes to the east of Mangakino. Alteration assemblages include epidote and wairakite in MA2 below 2200 m. Adularia occurs in MA2 and MA3 where it replaces, wholly or in part, primary andesine. Adularia is also locally replaced by illite, indicating a shift in hydrothermal conditions. Other minerals present are chlorite, quartz, calcite, titanite and pyrite. Secondary quartz and calcite veins are seen in thin section, with a first appearance in the lacustrine sediments at 550 m in both MA2 and MA3. Fluid inclusions in secondary calcite show high temperatures (300 and 315 °C) while inclusions in primary quartz show ca. 165 °C (the current temperature at the sampled depth), recording current conditions. The modern maximum temperature is 250 °C at 3000 m in MA2. Evidence for two</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20391178','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20391178"><span><span class="hlt">Intrusive</span> images and <span class="hlt">intrusive</span> thoughts as different phenomena: two experimental studies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hagenaars, Muriel A; Brewin, Chris R; van Minnen, Agnes; Holmes, Emily A; Hoogduin, Kees A L</p> <p>2010-01-01</p> <p>According to the dual representation theory of PTSD, <span class="hlt">intrusive</span> trauma images and <span class="hlt">intrusive</span> verbal thoughts are produced by separate memory systems. In a previous article it was shown that after watching an aversive film, participants in non-movement conditions reported more <span class="hlt">intrusive</span> images than participants in a free-to-move control condition (Hagenaars, Van Minnen, Holmes, Brewin, & Hoogduin, 2008). The present study investigates whether the experimental conditions of the Hagenaars et al. study had a different effect on <span class="hlt">intrusive</span> thoughts than on <span class="hlt">intrusive</span> images. Experiment 2 further investigated the image-thoughts distinction by manipulating stimulus valence (trauma film versus neutral film) and assessing the subsequent development of <span class="hlt">intrusive</span> images and thoughts. In addition, both experiments studied the impact of peri-traumatic emotions on subsequent <span class="hlt">intrusive</span> images and thoughts frequency across conditions. Results showed that experimental manipulations (non-movement and trauma film) caused higher levels of <span class="hlt">intrusive</span> images relative to control conditions (free movement and neutral film) but they did not affect <span class="hlt">intrusive</span> thoughts. Peri-traumatic anxiety and horror were associated with subsequent higher levels of <span class="hlt">intrusive</span> images, but not <span class="hlt">intrusive</span> thoughts. Correlations were inconclusive for anger and sadness. The results suggest <span class="hlt">intrusive</span> images and thoughts can be manipulated independently and as such can be considered different phenomena.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70147948','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70147948"><span>Fish assemblages at engineered and natural channel structures in the lower Missouri river: implications for modified <span class="hlt">dike</span> structures</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Schloesser, J.T.; Paukert, Craig P.; Doyle, W.J.; Hill, T.; Steffensen, K.D.; Travnichek, Vincent H.</p> <p>2012-01-01</p> <p>Large rivers throughout the world have been modified by using <span class="hlt">dike</span> structures to divert water flows to deepwater habitats to maintain navigation channels. These modifications have been implicated in the decline in habitat diversity and native fishes. However, <span class="hlt">dike</span> structures have been modified in the Missouri River USA to increase habitat diversity to aid in the recovery of native fishes. We compared species occupancy and fish community composition at natural sandbars and at notched and un-notched rock <span class="hlt">dikes</span> along the lower Missouri River to determine if notching <span class="hlt">dikes</span> increases species diversity or occupancy of native fishes. Fish were collected using gill nets, trammel nets, otter trawls, and mini fyke nets throughout the lower 1212 river km of the Missouri River USA from 2003 to 2006. Few differences in species richness and diversity were evident among engineered <span class="hlt">dike</span> structures and natural sandbars. Notching a <span class="hlt">dike</span> structure had no effect on proportional abundance of fluvial dependents, fluvial specialists, and macrohabitat generalists. Occupancy at notched <span class="hlt">dikes</span> increased for two species but did not differ for 17 other species (81%). Our results suggest that <span class="hlt">dike</span> structures may provide suitable habitats for fluvial species compared with channel sand bars, but <span class="hlt">dike</span> notching did not increase abundance or occupancy of most Missouri River fishes. Published in 2011 by John Wiley & Sons, Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030814','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030814"><span>The Sonju Lake layered <span class="hlt">intrusion</span>, northeast Minnesota: Internal structure and emplacement history inferred from magnetic fabrics</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Maes, S.M.; Tikoff, B.; Ferre, E.C.; Brown, P.E.; Miller, J.D.</p> <p>2007-01-01</p> <p>The Sonju Lake <span class="hlt">intrusion</span> (SLI), in northeastern Minnesota, is a layered mafic complex of Keweenawan age (1096.1 ?? 0.8 Ma) related to the Midcontinent rift. The cumulate paragenesis of the <span class="hlt">intrusion</span> is recognized as broadly similar to the Skaergaard <span class="hlt">intrusion</span>, a classic example of closed-system differentiation of a tholeiitic mafic magma. The SLI represents nearly closed-system differentiation through bottom-up fractional crystallization. Geochemical studies have identified the presence of a stratabound, 50-100 m thick <span class="hlt">zone</span> anomalously enriched in Au + PGE. Similar to the PGE reefs of the Skaergaard <span class="hlt">intrusion</span>, this PGE-enriched <span class="hlt">zone</span> is hosted within oxide gabbro cumulates, about two-third of the way up from the base of the <span class="hlt">intrusion</span>. We present a petrofabric study using the anisotropy of magnetic susceptibility (AMS) to investigate the emplacement and flow patterns within the Sonju Lake <span class="hlt">intrusion</span>. Petrographic and electron microprobe studies, combined with AMS and hysteresis measurements indicate the primary source of the magnetic signal is pseudo-single domain (PSD) magnetite or titanomagnetite. Low field AMS was measured at 32 sites within the Sonju Lake <span class="hlt">intrusion</span>, which provided information about primary igneous fabrics. The magnetic fabrics in the layered series of the Sonju Lake <span class="hlt">intrusion</span> are consistent with sub-horizontal to inclined emplacement of the <span class="hlt">intrusion</span> and show evidence that the cumulate layers were deposited in a dynamic environment. Well-aligned magnetic lineations, consistently plunging shallowly toward the southwest, indicate the source of the magma is a vertical sill-like feeder, presumably located beneath the Finland granite. The Finland granite acted as a density trap for the Sonju Lake magmas, forcing lateral flow of magma to the northeast. The strongly oblate magnetic shape fabrics indicate the shallowly dipping planar fabrics were enhanced by compaction of the crystal mush. ?? 2007 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.9240Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.9240Z"><span>Kontay <span class="hlt">intrusion</span> (Polar Siberia)- an example of strong magmatic differentiation in the single magmatic body</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zaitsev, Victor</p> <p>2016-04-01</p> <p>Kontay <span class="hlt">intrusion</span> is located in the north-west part of Maimecha-Kotuy province, (part of Siberian Large Igneous Province) in the northern part of the Siberian Platform. <span class="hlt">Intrusion</span> is fully overlaid and practically not studied before. Geophysical data evident that <span class="hlt">intrusion</span> has form of laccolite with diameter ˜7.5 km and thickness ˜ 2.5 km [1]. Initially lower part of <span class="hlt">intrusion</span> was described as "gabbro-anortozite and anortositic gabbro" and higher part - as "leucocratic granophyric anortosites" [2]. Complex mineralo-petrological-geochemical study allow to divide <span class="hlt">intrusion</span> section on three <span class="hlt">zones</span>: Lower <span class="hlt">zone</span> (below 1100 m) - layered sequence of leucocratic and melanocratic of biotite- and ortopyroxene-bearing gabbro, with minor alkaline feldspar, Middle <span class="hlt">zone</span> (1100-700m) - biotite- and K-feldspar bearing gabbro and monzonotes, interstitial space often contain micrographical structures. Biotite corroded clinopyroxene and form interstitial crystals and Upper <span class="hlt">zone</span> (700-214 m) - petrographically monotone porthyric quartz-monzonites and granosyenites with rare phenocrysts of plagioclase, magnetite, clinopyroxene and biotite. The main secondary minerals are albite, amphibole (edenite-feroedenite), secondary biotite, chlorite, and F,Al-bearing titanite. Rocks of the all parts fall in the same trends on the binary petrochemical diagrams, they belong to the High-K calc-alkaline seria. They are clearly more alkaline then <span class="hlt">intrusions</span> of Norilsk district and less alkaline then alkaline-ultramafic <span class="hlt">intrusions</span> of Maymecha-Kotuy province. Volcanic rocks of Norilsk and Maymecha-Kotuy area was subdivided for four geochemical types, mainly by the Ti-content, Th/U, Gd/Yb and Sm/Yb ratio: Low-Ti-1 (predominated), Low-Ti-2 (well -developed in Norilsk region), Moderate-Ti (developed only in the lower part of volcanic formation in Norilsk region), High-Ti (rare in Norilsk region, but widely spread in Mailecha-Kotuy area) [3]. Kontay <span class="hlt">intrusion</span> rocks belong to Moderate-Ti group. The closest</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://sofia.usgs.gov/publications/wri/77-33/','USGSPUBS'); return false;" href="http://sofia.usgs.gov/publications/wri/77-33/"><span>Saline-water <span class="hlt">intrusion</span> related to well construction in Lee County, Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Boggess, Durward Hoye; Missimer, T.M.; O'Donnell, T. H.</p> <p>1977-01-01</p> <p>Ground water is the principle source of water supply in Lee County, Florida where an estimated 30,000 wells have been drilled since 1990. These wells ranges in depth from about 10 to 1,240 feet and tap the water table aquifer or one or more of the artesian water-bearing units or <span class="hlt">zones</span> in the Tamiami Formation, the upper part of the Hawthorn Formation, the lower part of the Hawthorn Formation and the Tampa Limestone and the Suwannee Limestone. Before 1968, nearly all wells were constructed with galvanized or black iron pipe. Many of these wells are sources of saline-water <span class="hlt">intrusion</span> into freshwater-bearing <span class="hlt">zones</span>. The water-bearing <span class="hlt">zones</span> in the lower part of the Hawthorn Formation, Tampa Limestone, and Suwannee Limestone are artesian-they have higher water levels and usually contain water with a higher concentration of dissolved solids than do the aquifers occurring at shallower depths. The water from these deeper aquifers generally range in dissolved solids concentration from about 1,500 to 2,400 mg/L, and in chloride from about 500 to 1,00 mg/L. A maximum chloride concentration of 15,200 mg/L has been determined. Few of the 3,00 wells estimated to have been drilled to these <span class="hlt">zones</span> contain sufficient casing to prevent upward flow into overlaying water-bearing <span class="hlt">zones</span>. Because of water-level differentials, upward movement and lateral <span class="hlt">intrusion</span> of saline water occurs principally into the upper part of the Hawthorn Formation where the chloride concentrations in water unaffected by saline-water <span class="hlt">intrusion</span> ranges from about 80 to 150 mg/L. Where <span class="hlt">intrusion</span> from deep artesian <span class="hlt">zones</span> has occurred, the chloride concentration in water from the upper part of the Hawthorn Formation ranges from about 300 to more than 2,100 mg/L Surface discharges of the saline water from wells tapping the lower part of the Hawthorn Formation and the Suwannee Limestone also had affected the water-table aquifer which normally contains water with 10 to 50 mg/L of chloride. In one area, the chloride</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V43E0569Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V43E0569Y"><span>Paleoproterozoic mafic <span class="hlt">dike</span> swarms of the Dunhuang Block: record of initial breakup of the Columbia suppercontinent?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ye, X. T.; Zhang, C. L.</p> <p>2017-12-01</p> <p>Mafic <span class="hlt">dike</span> swarms have been described as igneous record related to the breakup and dispersal of continental masses. Studying their origin and distribution are thus important for the understanding of the regional magmatic-tectonic evolution during the late Paleoproterozoic and possible relationship between the Dunhuang Block and the Columbia supercontinent. Here detail petrolography, zircon U-Pb age, and geochemistry are presented of the mafic <span class="hlt">dikes</span> in the Dunhuang Block. The mafic <span class="hlt">dikes</span> are tabular, E-W trending, mainly consist of the diabase and diabasic gabbro. Fine-grained gabbroic rocks are seen in the center of some of the thick <span class="hlt">dikes</span>. These rocks are massive, showing ophitic texture with tholeiitic affinity and dominated by basaltic compositions. Zircon SHRIMP U-Pb dating of these dykes yields emplacement age of 1867 ± 8 Ma. According to their geochemical features, the mafic <span class="hlt">dikes</span> are subdivided into three groups (G1, G2, and G3). G1 <span class="hlt">dikes</span> have low SiO2 (47.80-48.82%), high MgO (6.00-8.44%), Cr (92-170 ppm), and Ni (46-106 ppm), indicating that they were not significantly affected by fractional crystallization or crustal assimilations. This result is consistent with their insignificant Nb-Ta troughs on the incompatible elements spider diagrams. Compared to G1 <span class="hlt">dikes</span>, G2 <span class="hlt">dikes</span> show higher SiO2 (49.18-49.76%), lower MgO (4.92-5.23%), Cr (35-44 ppm), and Ni (72-82 ppm). They show moderate Nb-Ta depletion on the primitive mantle normalized spider diagrams. Compared with G1 and G2 <span class="hlt">dikes</span>, G3 <span class="hlt">dikes</span> exhibit lowest SiO2 (46.05-49.76%) and MgO (4.07-4.37%) and highest TiO2 (3.38-3.50%), P2O5 (1.81-1.94%), and total alkalis (5.04-5.73%). In addition, G3 <span class="hlt">dikes</span> have higher total REE abundances and extremely depleted in Nb-Ta with Nb/La ratios from 0.25 to 0.27. Although these mafic <span class="hlt">dikes</span> show different REE and trace element patterns, the element signatures (Nb/La, Th/La, Ce/Nb, Th/Nb, and (Zr/Nb)N ratios) are similar to those of the intraplate basalts, while different</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..118a2021S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..118a2021S"><span>Ratio of Major Ions in Groundwater to Determine Saltwater <span class="hlt">Intrusion</span> in Coastal Areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sudaryanto; Naily, Wilda</p> <p>2018-02-01</p> <p>Saltwater or seawater <span class="hlt">intrusion</span> into groundwater aquifers occurs mostly in big cities and developing coastal cities. Coastal hydrology is associated with complex and highly dynamic environmental characteristics of interactions between groundwater, surface water, and water from the estuary. The rise of sea levels and excessive use of groundwater for clean water source trigger saltwater <span class="hlt">intrusion</span>. Identification of saltwater <span class="hlt">intrusion</span> into groundwater can be done by groundwater sampling and major ion analysis. The major ions dissolved in water are Ca, Mg, Na, K, Cl, HCO3, and SO4; the major ion ratios are Cl/Br, Ca/Mg, Ca/ (HCO3 and SO4), and Na/Cl. By knowing whether groundwater quality has been or has not been influenced by saltwater, groundwater <span class="hlt">zones</span> can be determined in every coastal area. In addition, by analyzing and reviewing some concepts about the <span class="hlt">intrusion</span> or contamination of saltwater into groundwater, there will be sufficient results for the identification of saltwater <span class="hlt">intrusion</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.T21D2203M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.T21D2203M"><span>Neogene Fault and Feeder <span class="hlt">Dike</span> Patterns in the Western Ross Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Magee, W. R.; Wilson, T. J.</p> <p>2010-12-01</p> <p>In Antarctica, where much of the continent is covered by water and ice, geophysical data from the Antarctic submarine continental shelf is a fundamental part of reconstructing geological history. Multibeam sonar from the western Ross Sea has revealed elongate volcanic edifices and fields of elongate submarine hills on the seafloor. Origin of the submarine hills as carbonate mounds and drumlins have been proposed. The hills are up to ~8000m long and ~3500m wide, and rise 50-100m above the seafloor. Morphometric analysis of the hills shows they are elongate, with axial ratios ranging from 1.2:1 to 2:1, and some hills are linked to form elongate ridges. Seismic profiles show significant pull-ups directly below the hills, consistent with narrow, higher-density magmatic bodies; thus we favor an origin as volcanic seamounts above subsurface feeder <span class="hlt">dikes</span>. If this volcanic hypothesis is correct, feeder <span class="hlt">dikes</span> below the hills and elongate volcanic ridges may document magmatically-forced extension within the Terror Rift. The seamount field forms part of a regional en echelon array of volcanic ridges extending NNW from Beaufort Island toward Drygalski Ice Tongue. The ridges and elongate seamount cluster trend NNE, subparallel to mapped fault trends in this sector of the Terror Rift. This geometry is compatible with right-lateral transtension along this <span class="hlt">zone</span>, as previously proposed for the Terror Rift as a whole. Volcanic islands and dredged volcanic ridges within the en echelon array are dated at ~7-4 Ma, implying Neogene deformation. We are completing a detailed analysis of orientation patterns and cross-cutting relations between faults and volcanic hills and their feeder systems to test this model for Neogene rift kinematics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70044480','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70044480"><span>A model for Iapetan rifting of Laurentia based on Neoproterozoic <span class="hlt">dikes</span> and related rocks</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Burton, William C.; Southworth, Scott</p> <p>2010-01-01</p> <p>Geologic evidence of the Neoproterozoic rifting of Laurentia during breakup of Rodinia is recorded in basement massifs of the cratonic margin by <span class="hlt">dike</span> swarms, volcanic and plutonic rocks, and rift-related clastic sedimentary sequences. The spatial and temporal distribution of these geologic features varies both within and between the massifs but preserves evidence concerning the timing and nature of rifting. The most salient features include: (1) a rift-related magmatic event recorded in the French Broad massif and the southern and central Shenandoah massif that is distinctly older than that recorded in the northern Shenandoah massif and northward; (2) felsic volcanic centers at the north ends of both French Broad and Shenandoah massifs accompanied by <span class="hlt">dike</span> swarms; (3) differences in volume between massifs of cover-sequence volcanic rocks and rift-related clastic rocks; and (4) WNW orientation of the Grenville <span class="hlt">dike</span> swarm in contrast to the predominately NE orientation of other Neoproterozoic <span class="hlt">dikes</span>. Previously proposed rifting mechanisms to explain these features include rift-transform and plume–triple-junction systems. The rift-transform system best explains features 1, 2, and 3, listed here, and we propose that it represents the dominant rifting mechanism for most of the Laurentian margin. To explain feature 4, as well as magmatic ages and geochemical trends in the Northern Appalachians, we propose that a plume–triple-junction system evolved into the rift-transform system. A ca. 600 Ma mantle plume centered east of the Sutton Mountains generated the radial <span class="hlt">dike</span> swarm of the Adirondack massif and the Grenville <span class="hlt">dike</span> swarm, and a collocated triple junction generated the northern part of the rift-transform system. An eastern branch of this system produced the Long Range <span class="hlt">dike</span> swarm in Newfoundland, and a subsequent western branch produced the ca. 554 Ma Tibbit Hill volcanics and the ca. 550 Ma rift-related magmatism of Newfoundland.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018HESS...22.1875T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018HESS...22.1875T"><span>Assessing impacts of <span class="hlt">dike</span> construction on the flood dynamics of the Mekong Delta</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tran, Dung Duc; van Halsema, Gerardo; Hellegers, Petra J. G. J.; Phi Hoang, Long; Quang Tran, Tho; Kummu, Matti; Ludwig, Fulco</p> <p>2018-03-01</p> <p>Recent flood dynamics of the Mekong Delta have raised concerns about an increased flood risk downstream in the Vietnamese Mekong Delta. Accelerated high <span class="hlt">dike</span> building on the floodplains of the upper delta to allow triple cropping of rice has been linked to higher river water levels in the downstream city of Can Tho. This paper assesses the hydraulic impacts of upstream <span class="hlt">dike</span> construction on the flood hazard downstream in the Vietnamese Mekong Delta. We combined the existing one-dimensional (1-D) Mekong Delta hydrodynamic model with a quasi-two-dimensional (2-D) approach. First we calibrated and validated the model using flood data from 2011 and 2013. We then applied the model to explore the downstream water dynamics under various scenarios of high <span class="hlt">dike</span> construction in An Giang Province and the Long Xuyen Quadrangle. Calculations of water balances allowed us to trace the propagation and distribution of flood volumes over the delta under the different scenarios. Model results indicate that extensive construction of high <span class="hlt">dikes</span> on the upstream floodplains has had limited effect on peak river water levels downstream in Can Tho. Instead, the model shows that the impacts of <span class="hlt">dike</span> construction, in terms of peak river water levels, are concentrated and amplified in the upstream reaches of the delta. According to our water balance analysis, river water levels in Can Tho have remained relatively stable, as greater volumes of floodwater have been diverted away from the Long Xuyen Quadrangle than the retention volume lost due to <span class="hlt">dike</span> construction. Our findings expand on previous work on the impacts of water control infrastructure on flood risk and floodwater regimes across the delta.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991Sci...252..276H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991Sci...252..276H"><span>Venus volcanism - Initial analysis from Magellan data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Head, J. W.; Campbell, D. B.; Elachi, C.; Guest, J. E.; McKenzie, D. P.; Saunders, R. S.; Schaber, G. G.; Schubert, G.</p> <p>1991-04-01</p> <p>Magellan images confirm that volcanism is widespread and has been fundamentally important in the formation and evolution of the crust of Venus. High-resolution imaging data reveal evidence for <span class="hlt">intrusion</span> (<span class="hlt">dike</span> formation and cryptodomes) and extrusion (a wide range of lava flows). Also observed are thousands of small shield volcanoes, larger edifices up to several hundred kilometers in diameter, massive outpourings of lavas, and local pyroclastic deposits. Although most features are consistent with basaltic compositions, a number of large pancake-like domes are morphologically similar to rhyolite-dacite domes on earth. Flows and sinuous channels with lengths of many hundreds of kilometers suggest that extremely high effusion rates or very fluid magmas (perhaps komantiites) may be present. Volcanism is evident in various tectonic settings (coronae, linear extensional and compressional <span class="hlt">zones</span>, mountain belts, upland rises, highland plateaus, and tesserae). Volcanic resurfacing rates appear to be low (less than 2 cu km/yr) but the significance of <span class="hlt">dike</span> formation and <span class="hlt">intrusions</span>, and the mode of crustal formation and loss remain to be established.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016722','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016722"><span>Venus volcanism: Initial analysis from Magellan data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Head, J.W.; Campbell, D.B.; Elachi, C.; Guest, J.E.; Mckenzie, D.P.; Saunders, R.S.; Schaber, G.G.; Schubert, G.</p> <p>1991-01-01</p> <p>Magellan images confirm that volcanism is widespread and has been fundamentally important in the formation and evolution of the crust of Venus. High-resolution imaging data reveal evidence for <span class="hlt">intrusion</span> (<span class="hlt">dike</span> formation and cryptodomes) and extrusion (a wide range of lava flows). Also observed are thousands of small shield volcanoes, larger edifices up to several hundred kilometers in diameter, massive outpourings of lavas, and local pyroclastic deposits. Although most features are consistent with basaltic compositions, a number of large pancake-like domes are morphologically similar to rhyolite-dacite domes on Earth. Flows and sinuous channels with lengths of many hundreds of kilometers suggest that extremely high effusion rates or very fluid magmas (perhaps komatiites) may be present. Volcanism is evident in various tectonic settings (coronae, linear extensional and compressional <span class="hlt">zones</span>, mountain belts, upland rises, highland plateaus, and tesserae). Volcanic resurfacing rates appear to be low (less than 2 km3/yr) but the significance of <span class="hlt">dike</span> formation and <span class="hlt">intrusions</span>, and the mode of crustal formation and loss remain to be established.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880005496','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880005496"><span>Petrogenesis of basalts from the Archean Matachewan <span class="hlt">Dike</span> Swarm Superior Province of Canada</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nelson, Dennis O.</p> <p>1987-01-01</p> <p>The Matachewan <span class="hlt">Dike</span> swarm of eastern Ontario comprises Archean age basalts that were emplaced in the greenstone, granite-greenstone, and metasedimentary terrains of the Superior Province of Canada. The basalts are Fe-rich tholeiites, characterized by the near ubiquitos presence of large, compositionally uniform, calcic plagioclase. Major and trace element whole-rock compositions, along with microprobe analyses of constituent phases, from a group of <span class="hlt">dikes</span> from the eastern portion of the province, were evaluated to constrain petrological processes that operated during the formation and evolution of the magmas. Three compositional groupings, were identified within the <span class="hlt">dikes</span>. One group has compositional characteristics similar to modern abyssal tholeiites and is termed morb-type. A second group, enriched in incompatible elements and light-REE enriched, is referred to as the enriched group. The third more populated group has intermediate characteristics and is termed the main group. The observation of both morb-type and enriched compositions within a single <span class="hlt">dike</span> strongly argues for the contemporaneous existence of magmas derived through different processes. Mixing calculations suggest that two possibilities exist. The least evolved basalts lie on a mixing line between the morb-type and enriched group, suggesting mixing of magmas derived from heterogeneous mantle. Mixing of magmas derived from a depleted mantle with heterogeneous Archean crust can duplicate certain aspects of the Matachewan <span class="hlt">dike</span> composition array.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....7780G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....7780G"><span><span class="hlt">Dike</span> emplacement and the birth of the Yellowstone hotspot, western USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Glen, J. M.; Ponce, D. A.; Nomade, S.; John, D. A.</p> <p>2003-04-01</p> <p>The birth of the Yellowstone hotspot in middle Miocene time was marked by extensive flood basalt volcanism. Prominent aeromagnetic anomalies (referred to collectively as the Northern Nevada rifts), extending hundreds of kilometers across Nevada, are thought to represent <span class="hlt">dike</span> swarms injected at the time of flood volcanism. Until now, however, <span class="hlt">dikes</span> from only one of these anomalies (eastern) have been documented, sampled, and dated (40Ar/ 39Ar ages range from 15.4 +/-0.2 to 16.7 +/-0.5Ma; John et al., 2000, ages recalculated using the FCS standard age of 28.02 +/-0.28Ma). We present new paleomagnetic data and an 40Ar/ 39Ar age of 16.6 +/-0.3Ma for a mafic <span class="hlt">dike</span> suggesting that all the anomalies likely originate from the same mid-Miocene fracturing event. The magnetic anomalies, together with the trends of <span class="hlt">dike</span> swarms, faults, and fold axes produce a radiating pattern that converges on a point near the Oregon-Idaho boarder. We speculate that this pattern formed by stresses imposed by the impact of the Yellowstone hotspot. Glen and Ponce (2002) propose a simple stress model to account for this fracture pattern that consists of a point source of stress at the base of the crust and a regional stress field aligned with the presumed middle Miocene stress direction. Overlapping point and regional stresses result in stress trajectories that form a radiating pattern near the point source (i.e., hotspot). Far from the influence of the point stress, however, stress trajectories verge towards the NNW-trending regional stress direction (i.e., plate boundary stresses), similar to the pattern of <span class="hlt">dike</span> swarm traces. Glen and Ponce, 2002, Geology, 30, 7, 647-650 John et al., 2000, Geol. Soc. Nev. Sym. Proc., May 15-18, 2000, 127-154</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSM.V24A..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSM.V24A..02S"><span>Basaltic Diatreme To Root <span class="hlt">Zone</span> Volcanic Processes In Tuzo Kimberlite Pipe (Gahcho Kué Kimberlite Field, NWT, Canada)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seghedi, I.; Kurszlaukis, S.; Maicher, D.</p> <p>2009-05-01</p> <p>Tuzo pipe is infilled by a series of coherent and fragmental kimberlite facies types typical for a diatreme to root <span class="hlt">zone</span> transition level. Coherent or transitional coherent kimberlite facies dominate at depth, but also occur at shallow levels, either as <span class="hlt">dikes</span> or as individual or agglutinated coherent kimberlite clasts (CKC). Several fragmental kimberlite varieties fill the central and shallow portions of the pipe. The definition, geometry and extent of the geological units are complex and are controlled by vertical elements. Specific for Tuzo is: (1) high abundance of locally derived xenoliths (granitoids and minor diabase) between and within the kimberlite phases, varying in size from sub-millimeter to several tens of meters, frequent in a belt-like domain between 120-200 m depth in the pipe; (2) the general presence of CKC, represented by round-subround, irregular to amoeboid-shaped clasts with a macrocrystic or aphanitic texture, mainly derived from fragmentation of erupting magma and less commonly from previously solidified kimberlite, as well as recycled pyroclasts. In addition, some CKC are interpreted to be intersections of a complex <span class="hlt">dike</span> network. This diversity attests formation by various volcanic processes, extending from <span class="hlt">intrusive</span> to explosive; (3) the presence of bedded polymict wall- rock and kimberlite breccia occurring mostly in deep levels of the pipe below 345 m depth. The gradational contact relationships of these deposits with the surrounding kimberlite rocks and their location suggest that they formed in situ. The emplacement of Tuzo pipe involved repetitive volcanic explosions alternating with periods of relative quiescence causing at least partial consolidation of some facies. The volume deficit in the diatreme-root <span class="hlt">zone</span> after each eruption was compensated by gravitational collapse of overlying diatreme tephra and pre-fragmented wall-rock xenoliths. Highly explosive phases were alternating with weak explosions or <span class="hlt">intrusive</span> phases, suggesting</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T13E2675L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T13E2675L"><span>A Jurassic Shock-Aftershock Earthquake Sequence Recorded by Small Clastic Pipes and <span class="hlt">Dikes</span> within Dune Cross-Strata, Zion National Park, Utah</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loope, D. B.; Zlotnik, V. A.; Kettler, R. M.; Pederson, D. T.</p> <p>2012-12-01</p> <p> dune lee slope through a pipe, the erupted sand dried and was buried by climbing wind-ripple strata as the large dune continued to advance downwind. The mapped cluster recording eight distinct seismic events lies within thin-laminated sediment that was deposited by wind ripples during 1 m (~ 1 year) of southeastward dune migration. We conclude that the small pipes and <span class="hlt">dikes</span> of our study sites are products of numerous >MM 5 earthquakes, some of which recurred at intervals of less than 2 months. We interpret one small cluster of pipes and <span class="hlt">dikes</span> with well-defined upward terminations as a distinct shock-aftershock sequence. Because the largest modern earthquakes can produce surface liquefaction only up to about 175 km from their epicenters, the Jurassic epicenters must have been well within that distance. The tendency of modern plate boundaries to produce high-frequency aftershocks suggests that the epicenter for this Jurassic sequence lay to the southwest, within the plate boundary <span class="hlt">zone</span> (not within continental rocks to the east). As eolian dunes steadily migrate over interdune surfaces underlain by water-saturated dune cross-strata, the thin, distinct laminae produced by the wind ripples that occupy dune toes can faithfully record high-frequency seismic events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015131','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015131"><span>Petrologic constraints on rift-<span class="hlt">zone</span> processes - Results from episode 1 of the Puu Oo eruption of Kilauea volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Garcia, M.O.; Ho, R.A.; Rhodes, J.M.; Wolfe, E.W.</p> <p>1989-01-01</p> <p>The Puu Oo eruption in the middle of Kilauea volcano's east rift <span class="hlt">zone</span> provides an excellent opportunity to utilize petrologic constraints to interpret rift-<span class="hlt">zone</span> processes. Emplacement of a <span class="hlt">dike</span> began 24 hours before the start of the eruption on 3 January 1983. Seismic and geodetic evidence indicates that the <span class="hlt">dike</span> collided with a magma body in the rift <span class="hlt">zone</span>. Most of the lava produced during the initial episode of the Puu Oo eruption is of hybrid composition, with petrographic and geochemical evidence of mixing magmas of highly evllved and more mafic compositions. Some olivine and plagioclase grains in the hybrid lavas show reverse <span class="hlt">zoning</span>. Whole-rock compositional variations are linear even for normally compatible elements like Ni and Cr. Leastsquares mixing calculations yield good residuals for major and trace element analyses for magma mixing. Crystal fractionation calculations yield unsatisfactory residuals. The highly evolved magma is similar in composition to the lava from the 1977 eruption and, at one point, vents for these two eruptions are only 200 m apart. Possibly both the 1977 lava and the highly evolved component of the episode 1 Puu Oo lava were derived from a common body of rift-<span class="hlt">zone</span>-stored magma. The more mafic mixing component may be represented by the most mafic lava from the January 1983 eruption; it shows no evidence of magma mixing. The <span class="hlt">dike</span> that was intruded just prior to the start of the Puu Oo eruption may have acted as a hydraulic plunger causing mixing of the two rift-<span class="hlt">zone</span>-stored magmas. ?? 1989 Springer-Verlag.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29477820','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29477820"><span>Assessing sea-level rise impact on saltwater <span class="hlt">intrusion</span> into the root <span class="hlt">zone</span> of a geo-typical area in coastal east-central Florida.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xiao, Han; Wang, Dingbao; Medeiros, Stephen C; Hagen, Scott C; Hall, Carlton R</p> <p>2018-07-15</p> <p>Saltwater <span class="hlt">intrusion</span> (SWI) into root <span class="hlt">zone</span> in low-lying coastal areas can affect the survival and spatial distribution of various vegetation species by altering plant communities and the wildlife habitats they support. In this study, a baseline model was developed based on FEMWATER to simulate the monthly variation of root <span class="hlt">zone</span> salinity of a geo-typical area located at the Cape Canaveral Barrier Island Complex (CCBIC) of coastal east-central Florida (USA) in 2010. Based on the developed and calibrated baseline model, three diagnostic FEMWATER models were developed to predict the extent of SWI into root <span class="hlt">zone</span> by modifying the boundary values representing the rising sea level based on various sea-level rise (SLR) scenarios projected for 2080. The simulation results indicated that the extent of SWI would be insignificant if SLR is either low (23.4cm) or intermediate (59.0cm), but would be significant if SLR is high (119.5cm) in that infiltration/diffusion of overtopping seawater in coastal low-lying areas can greatly increase root <span class="hlt">zone</span> salinity level, since the sand dunes may fail to prevent the landward migration of seawater because the waves of the rising sea level can reach and pass over the crest under high (119.5cm) SLR scenario. Copyright © 2018 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5024158-age-intrusive-relations-lamarck-granodiorite-associated-mafic-plutons-sierra-nevada-california','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5024158-age-intrusive-relations-lamarck-granodiorite-associated-mafic-plutons-sierra-nevada-california"><span>Age and <span class="hlt">intrusive</span> relations of the Lamarck granodiorite and associated mafic plutons, Sierra Nevada, California</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Joye, J.L.; Bachl, C.A.; Miller, J.S.</p> <p></p> <p>The compositionally <span class="hlt">zoned</span> Late Cretaceous Lamarck granodiorite, west of Bishop, hosts numerous mafic <span class="hlt">intrusions</span> ranging from hornblende gabbro to mafic granodiorite. Frost and Mahood (1987) suggested from field relations that the Lamarck and the associated mafic plutons were co-<span class="hlt">intrusive</span>. Contact relations between the Lamarck host and the mafic <span class="hlt">intrusions</span> are variable (sharp to diffuse) and in places suggest commingling. In order to constrain the <span class="hlt">intrusive</span> relationships between the Lamarck and its associated mafic plutons, the authors have analyzed feldspars from the Mt. Gilbert pluton and the Lamarck granodiorite to see if feldspar compositions in the Mt. Gilbert overlap those inmore » the Lamarck host and determined U-Pb zircon ages for the Mt. Gilbert and Lake Sabrina plutons to see if they have the same age as the Lamarck granodiorite. Feldspars from the Lamarck granodiorite are normally <span class="hlt">zoned</span> and range compositionally from An[sub 38--32]; those in the Mt. Gilbert diorite are also normally <span class="hlt">zoned</span> but range compositionally from An[sub 49--41] and do not overlap the Lamarck host. Four to five zircon fractions from each pluton were handpicked and dated using U-Pb methods. The Mt. Gilbert mafic diorite has a concordant age of 92.5 Ma and the Lake Sabrina diorite has a concordant age of 91.5 Ma. Ages for the two plutons overlap within error, but multiple fractions from each suggest that the Lake Sabrina pluton is slightly younger than the Mt. Gilbert pluton. These data and field relationships indicate: (1) plagioclase phenocrysts in the Mt. Gilbert pluton were not derived from the Lamarck granodiorite despite their textural similarity; but (2) the Lamarck granodiorite and its associated mafic plutons are co-<span class="hlt">intrusive</span> as supported by the close agreement of the ages with the crystallization age obtained by Stern and others for the Lamarck granodiorite.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.T51C1546H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.T51C1546H"><span>Magnetic Remanence and Anisotropy of Magnetic Susceptibility of <span class="hlt">Dikes</span> From Super-Fast Spread Crust Exposed At Pito Deep Rift</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horst, A.; Varga, R. J.; Gee, J. S.; Karson, J. A.</p> <p>2006-12-01</p> <p>The tectonic window at the Pito Deep Rift exposes super-fast spread (>140mm/yr) oceanic crust created at the East Pacific Rise (EPR). Observations and investigations of well-exposed cross sections into modern ocean crust, such as Pito Deep, provide essential insights into ridge crest dynamics. Paleomagnetic analysis provides a quantitative means for assessing both magnitude and style of structural rotations of oceanic crust. The Pito Cruise 2005 collected 69 fully oriented samples [67 <span class="hlt">dikes</span>, 2 gabbros] during several ALVIN and JASON II dives. These samples were all oriented in situ using the Geocompass. Along the escarpment of Pito Deep, <span class="hlt">dike</span> orientations have consistant NE strikes and SE dips. These <span class="hlt">dikes</span> are all formed roughly 3 million years ago at the EPR located to the west of their present position. We determined magnetic remanence for a subset of 34 oriented blocks. A majority of <span class="hlt">dikes</span> in this subset have normal polarity and many are clockwise rotated from expected orientations. To assess possible orientation errors during collection, we sampled multiple <span class="hlt">dikes</span> from relatively small areas. On ALVIN dive 4081, for example, we collected 14 samples from a well-exposed, subparallel series of <span class="hlt">dikes</span>. These <span class="hlt">dikes</span> provide stable and consistently oriented remanence directions suggesting that errors in the collection process are small. Remanence data collected to date verify tectonic models that suggest clockwise rotation of the Easter microplate, consistent with current models. In addition to magnetic remanence, we determined the anisotropy of magnetic susceptibility (AMS) of the 34 <span class="hlt">dike</span> samples. AMS studies have proven their utility in a wide range of geological studies and have been shown to determine flow direction within <span class="hlt">dikes</span> in a variety of settings. In most Pito Deep samples, two of three AMS eigenvectors lie close to <span class="hlt">dike</span> plane orientations. Kmin generally lies perpendicular to <span class="hlt">dike</span> planes while, in most samples, Kmax is shallow indicating dominantly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Litho.290...18I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Litho.290...18I"><span>Petrogenesis of an Early Cretaceous lamprophyre <span class="hlt">dike</span> from Kyoto Prefecture, Japan: Implications for the generation of high-Nb basalt magmas in subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Imaoka, Teruyoshi; Kawabata, Hiroshi; Nagashima, Mariko; Nakashima, Kazuo; Kamei, Atsushi; Yagi, Koshi; Itaya, Tetsumaru; Kiji, Michio</p> <p>2017-10-01</p> <p>We studied a 107 Ma vogesite (a kind of lamprophyre with alkali-feldspar > plagioclase, and hornblende ± clinopyroxene ± biotite) <span class="hlt">dike</span> in the Kinki district of the Tamba Belt, Kyoto Prefecture, SW Japan, using petrography, mineralogy, K-Ar ages, and geochemistry to evaluate its petrogenesis and tectonic implications. The <span class="hlt">dike</span> has the very specific geochemical characteristics of a primitive high-Mg basalt, with 48-50 wt.% SiO2 (anhydrous basis), high values of Mg# (67.3-72.4), and high Cr ( 431 ppm), Ni ( 371 ppm), and Co ( 52 ppm) contents. The vogesite is alkaline and ne-normative with high concentrations of large ion lithophile elements (LILEs: Sr = 1270-2200 ppm, Ba = 3910-26,900 ppm), light rare earth elements (LREEs) [(La/Yb)n = 58-62), and high field strength elements (HFSEs: TiO2 = 1.5-1.8 wt.%, Nb = 24-33 ppm, Zr = 171-251 ppm), and the vogesite can be classified as a high-Nb basalt (HNB). The vogesite was formed by the lowest degree of melting of metasomatized mantle in the garnet stability field, and it may also have been formed at higher melting pressures than other Kyoto lamprophyres. The low degree of melting is the primary reason for the high-Nb content of the vogesite, not mantle metasomatism, and a higher degree of melting would have changed the primary magma composition from a HNB to a Nb-enriched basalt (NEB). The vogesite magma was contaminated at an early stage of its development by melts derived from sediments drawn down a subduction <span class="hlt">zone</span>, as indicated by some geochemical indices and the initial Nd isotope ratios. The vogesite exhibits positive correlations between εSr(107 Ma) values (5.4-50.9) and its high Ba and Sr concentrations, and it has a limited range of εNd(107 Ma) values (+ 0.97 to + 2.4). The fact that the vogesite contains centimeter-sized xenoliths of chert, which are composed of polycrystalline quartz, calcite, barite, pyrite, and magnetite, indicates that the barium contamination took place during the ascent of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B22B..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B22B..07S"><span>Environmental Characteristics of Carbonatite and Alkaline <span class="hlt">Intrusion</span>-related Rare Earth Element (REE) Deposits</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seal, R. R., II; Piatak, N. M.</p> <p>2017-12-01</p> <p>Carbonatites and alkaline <span class="hlt">intrusions</span> are important sources of REEs. Environmental risks related to these deposit types have been assessed through literature review and evaluation of the geochemical properties of representative samples of mill tailings and their leachates. The main ore mineral in carbonatite deposits is bastnasite [(Ce,La)(CO3)F], which is found with dolomite and calcite ( 65 %), barite (20 - 25 %), plus a number of minor accessory minerals including sulfides such as galena and pyrite. Generally, alkaline <span class="hlt">intrusion</span>-related REE deposits either occur in layered complexes or with <span class="hlt">dikes</span> and veins cutting alkaline <span class="hlt">intrusions</span>. Such <span class="hlt">intrusions</span> have a more diverse group of REE ore minerals that include fluorcarbonates, oxides, silicates, and phosphates. Ore also can include minor calcite and iron (Fe), lead (Pb), and zinc (Zn) sulfides. The acid-generating potential of both deposit types is low because of a predominance of carbonate minerals in the carbonatite deposits, the presence of feldspars and minor calcite in alkaline <span class="hlt">intrusion</span>-related deposits, and to only minor to trace occurrence of potentially acid-generating sulfide minerals. Both deposit types, however, are produced by igneous and hydrothermal processes that enrich high-field strength, incompatible elements, which typically are excluded from common rock-forming minerals. Elements such as yttrium (Y), niobium Nb), zirconium (Zr), hafnium (Hf), tungsten (W), titanium (Ti), tantalum (Ta), scandium (Sc), thorium (Th), and uranium (U) can be characteristic of these deposits and may be of environmental concern. Most of these elements, including the REEs, but with the exception of U, have low solubilities in water at the near-neutral pH values expected around these deposits. Mill tailings from carbonatite deposits can exceed residential soil and sediment criteria for Pb, and leachates from mill tailings can exceed drinking water guidelines for Pb. The greatest environmental challenges, however, are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V21D0657L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V21D0657L"><span>Volcanoes Behave as Composite Materials: Implications for Modeling Magma Chambers, <span class="hlt">Dikes</span>, and Surface Deformation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leiss, B.; Gudmundsson, A.; Philipp, S. L.</p> <p>2005-12-01</p> <p>By definition, composite volcanoes are composed of numerous alternating material units or layers such as lavas, sediments, and pyroclastics. Commonly, these layers have widely different mechanical properties. In particular, some lava flows and welded pyroclastic flows may be stiff (with a high Young's modulus), whereas others, such as non-welded pyroclastic units and sediments, may be soft (with a low Young's modulus). As a consequence, even if the loading (tectonic stress, magmatic pressure, or displacement) is uniform, the stresses within the composite volcano will vary widely. In this sense, the behavior of composite volcanoes is similar to that of general composite materials. The deformation of the surface of a volcano during an unrest period results from stresses generated by processes and parameters such as fluid pressure in a geothermal field or a magma chamber, a regional tectonic event, and a <span class="hlt">dike</span> injection. Here we present new numerical models on mechanics of magma chambers and <span class="hlt">dikes</span>, and the associated surface deformation of composite volcanoes. The models show that the surface deformation during magma-chamber inflation and deflation depends much on the chamber geometry, the loading conditions, and the mechanical properties of the rock units that constitute the volcano. The models also indicate that the surface deformation induced by a propagating <span class="hlt">dike</span> depends much on the mechanical properties of the layers between the <span class="hlt">dike</span> tip and the surface. In particular, the numerical results show that soft layers and weak contacts between layers may suppress the <span class="hlt">dike</span>-induced tensile stresses and the associated surface deformation. Many <span class="hlt">dikes</span> may therefore become injected and arrested at shallow depths in a volcano while giving rise to little or no surface deformation. Traditional analytical surface-deformation models such as a point source (Mogi model) for a magma-chamber pressure change and a dislocation for a <span class="hlt">dike</span> normally assume the volcano to behave as a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V13F..01I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V13F..01I"><span>Battling through the thermal boundary layer: Deep sampling in ODP Hole 1256D during IODP Expedition 335</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ildefonse, B.; Teagle, D. A.; Blum, P.; IODP Expedition 335 Scientists</p> <p>2011-12-01</p> <p> previous poor core recovery. Including the ~60 m-thick <span class="hlt">zone</span> of granoblastic <span class="hlt">dikes</span> overlying the uppermost gabbro, the <span class="hlt">dike</span>-gabbro transition <span class="hlt">zone</span> at Site 1256 is over 170 m thick, of which more than 100 m are recrystallized granoblastic basalts. This <span class="hlt">zone</span> records a dynamically evolving thermal boundary layer between the principally hydrothermal domain of the upper crust and a deeper <span class="hlt">zone</span> of <span class="hlt">intrusive</span> magmatism. The recovered samples document a sequence of evolving geological conditions and the intimate coupling between temporally and spatially intercalated <span class="hlt">intrusive</span>, hydrothermal, contact-metamorphic, partial melting and retrogressive processes. Despite the operational challenges, we achieved a minor depth advance to 1522 m, but this was insufficient penetration to complete any of the primary objectives. However, Hole 1256D has been thoroughly cleared of junk and drill cuttings that have hampered operations during this and previous Expeditions. At the end of Expedition 335, we briefly resumed coring and stabilized problematic intervals with cement. Hole 1256D is open to its full depth and ready for further deepening in the near future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..344..197W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..344..197W"><span>Surface deformation induced by magmatic processes at Pacaya Volcano, Guatemala revealed by InSAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wnuk, K.; Wauthier, C.</p> <p>2017-09-01</p> <p>Pacaya Volcano, Guatemala is a continuously active, basaltic volcano with an unstable western flank. Despite continuous activity since 1961, a lack of high temporal resolution geodetic surveying has prevented detailed modeling of Pacaya's underlying magmatic plumbing system. A new, temporally dense dataset of Interferometric Synthetic Aperture Radar (InSAR) RADARSAT-2 images, spanning December 2012 to March 2014, show magmatic deformation before and during major eruptions in January and March 2014. Inversion of InSAR surface displacements using simple analytical forward models suggest that three magma bodies are responsible for the observed deformation: (1) a 4 km deep spherical reservoir located northwest of the summit, (2) a 0.4 km deep spherical source located directly west of the summit, and (3) a shallow <span class="hlt">dike</span> below the summit. Periods of heightened volcanic activity are instigated by magma pulses at depth, resulting in rapid inflation of the edifice. We observe an <span class="hlt">intrusion</span> cycle at Pacaya that consists of deflation of one or both magma reservoirs followed by <span class="hlt">dike</span> <span class="hlt">intrusion</span>. <span class="hlt">Intrusion</span> volumes are proportional to reservoir volume loss and do not always result in an eruption. Periods of increased activity culminate with larger <span class="hlt">dike</span>-fed eruptions. Large eruptions are followed by inter-eruptive periods marked by a decrease in crater explosions and a lack of detected deformation. Co-eruptive flank motion appears to have initiated a new stage of volcanic rifting at Pacaya defined by repeated NW-SE oriented <span class="hlt">dike</span> <span class="hlt">intrusions</span>. This creates a positive feedback relationship whereby magmatic forcing from eruptive <span class="hlt">dike</span> <span class="hlt">intrusions</span> induce flank motion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V23C2994N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V23C2994N"><span>Constraints on the Chief Joseph <span class="hlt">Dike</span> Swarm of the Columbia River Flood Basalts from the legacy dataset of William H. Taubeneck</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nasholds, M. W.; Karlstrom, L.; Morriss, M. C.</p> <p>2016-12-01</p> <p>The Chief Joseph <span class="hlt">dike</span> swarm, spanning northeastern OR, southeastern WA, and parts of western ID, is one of the primary <span class="hlt">dike</span> swarms feeding the mid-Miocene Columbia River Basalt Group (CRBG) (e.g. Reidel et al. 2013). William H. Taubeneck (1923-2016) mapped these and other CRBG feeder <span class="hlt">dikes</span> over 40 years, generating an expansive dataset with locations and characteristics of <span class="hlt">dike</span> segments, primarily centered within the Wallowa Mountains, extending as far north as Lewiston, ID, and as far south as Farewell Bend, OR. Taubeneck is credited with originally defining the Chief Joseph swarm, but his data was not made available until his death. Using ArcMap, we are in the process of digitizing, field checking, and making available relevant data from Taubeneck's annotated maps and notebooks. We extract <span class="hlt">dike</span> locations, orientations, thicknesses, and host rock characteristics. We present an overview of the Taubeneck data, relating to Chief Joseph <span class="hlt">dikes</span> in WA, ID, and newer field measurements in the Wallowas, OR. Strikes of the 4410 <span class="hlt">dike</span> segments range from NNW to NNE, with outliers that define smaller clusters with distinct orientations. The <span class="hlt">dikes</span> have primarily near-vertical dips, paleo-depths ranging from 2 km to 0.3 km, and limited observations indicate widths from <5 m to 40 m. A majority of <span class="hlt">dikes</span> are exposed in uplifted granites of the Wallowa batholith and metamorphosed host: 1606 <span class="hlt">dikes</span> occur in quartz diorite, 60 occur in the Hurwal Formation, 139 occur in metavolcanics, while 401 occur in CRBG basalt. The other 2204 <span class="hlt">dikes</span> are not in the Chief Joseph area. There does not seem to be a significant relation between host rock composition and <span class="hlt">dike</span> orientation, although wall rock interactions are more dramatic in non-granitic Tertiary rocks. This dataset may provide further insight into both <span class="hlt">dike</span> emplacement dynamics and the plumbing system of the CRBG.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V33I..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V33I..02M"><span>The Morphological Characteristics and Mechanical Formation of Giant Radial <span class="hlt">Dike</span> Swarms on Venus: An Overview Emphasizing Recent Numerical Modeling Insights</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McGovern, P. J., Jr.; Grosfils, E. B.; Le Corvec, N.; Ernst, R. E.; Galgana, G. A.</p> <p>2017-12-01</p> <p>Over 200 giant radial <span class="hlt">dike</span> swarms have been identified on Venus using Magellan data, yielding insight into morphological characteristics long since erased by erosion and other processes on Earth. Since such radial <span class="hlt">dike</span> systems are typically associated with magma reservoirs, large volcanoes and/or larger-scale plume activity—and because <span class="hlt">dike</span> geometry reflects stress conditions at the time of intrusion—assessing giant radial <span class="hlt">dike</span> formation in the context of swarm morphology can place important constraints upon this fundamental volcanotectonic process. Recent numerical models reveal that, contrary to what is reported in much of the published literature, it is not easy, mechanically, to produce either large or small radial <span class="hlt">dike</span> systems. After extensive numerical examination of reservoir inflation, however, under conditions ranging from a simple halfspace to complex flexural loading, we have thus far identified four scenarios that produce radial <span class="hlt">dike</span> systems. Two of these scenarios yield <span class="hlt">dike</span> systems akin to those often associated with shield and stratocone volcanoes on Earth, while the other two, our focus here, are more consistent with the giant radial <span class="hlt">dike</span> system geometries catalogued on Venus. In this presentation we will (a) review key morphological characteristics of the giant radial systems identified on Venus, (b) briefly illustrate why it is not easy, mechanically, to produce a radial <span class="hlt">dike</span> system, (c) present the two volcanological circumstances we have identified that do allow a giant radial <span class="hlt">dike</span> system to form, and (d) discuss current model limitations and potentially fruitful directions for future research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V11B2770S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V11B2770S"><span>Inherited Fe and Ti electron transition spectroscopic features in altered ultramafic-carbonatite <span class="hlt">intrusives</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shavers, E. J.; Ghulam, A.; Encarnacion, J. P.</p> <p>2016-12-01</p> <p>Spectroscopic reflectance in the visible to short-wave infrared region is an important tool for remote geologic mapping and is applied at scales from satellite to field measurements. Remote geologic mapping is challenging in regions subject to significant surficial weathering. Here we identify absorption features found in altered volcanic pipes and <span class="hlt">dikes</span> in the Avon Volcanic District, Missouri, that are inherited from the original ultramafic and carbonatite lithology. Alteration ranges from small degree hydrothermal alteration to extensive laterization. The absorption features are three broad minima centered near 690, 890, and 1100 nm. Features in this region are recognized to be caused by ferric and ferrous Fe minerals including olivine, carbonates, chlorite, and goethite all of which are found among the Avon pipes and <span class="hlt">dikes</span> that are in various stages of alteration. Iron-related intervalence charge transfer and crystal field perturbations of ions are the principal causes of the spectroscopic features in the visible to near-infrared region yet spectra are also distorted by factors like texture and the presence of opaque minerals known to reduce overall reflectance. In the Avon samples, Fe oxide content can reach >15 wt% leading to prominent absorption features even in the less altered ultramafics with reflectance curve maxima as low as 5%. The exaggerated minima allow the altered <span class="hlt">intrusive</span> rocks to stand out among other weathered lithologies that will often have clay features in the region yet have lower iron concentration. The absorption feature centered near 690 nm is particularly noteworthy. Broad mineral-related absorption features centered at this wavelength are rare but have been linked to Ti3+ in octahedral coordination. The reduced form of Ti is not common in surface lithologies. Titanium-rich andradite has Ti3+ in the octahedral position, is resistant to weathering, is found among the Avon lithologies including ultramafic, carbonatite, and carbonated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014569','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014569"><span>Platinum-group element geochemistry of <span class="hlt">zoned</span> ultramafic <span class="hlt">intrusive</span> suites, Klamath Mountains, California and Oregon.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gray, F.; Page, N.J.; Carlson, C.A.; Wilson, S.A.; Carlson, R.R.</p> <p>1986-01-01</p> <p>Analyses for platinum-group elements of the varied rock suites of three Alaskan-type ultramafic to mafic multi-<span class="hlt">intrusive</span> bodies are reported. Ir and Ru are less than analytical sensitivities of 100 and 20 ppb; Rh is less than or near 1 ppb. Average Pd assays vary among the rocks within <span class="hlt">intrusive</span> complexes and between the three complexes (6.3, 13.7, 36.4 ppb); average Pt assays vary little among the same samples (27.9, 60.9, 34.0 ppb). Statistically adjusted Pt/(Pt + Pd) ratios increase in each suite from gabbro through clinopyroxenite to olivine-rich rocks, possibly owing to Pd fractionation.-G.J.N.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1985/0002/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1985/0002/report.pdf"><span>Composition of coarse-grained magnetite from pegmatite <span class="hlt">dikes</span> related to plutons of quartz monzonite in the Jabal Lababa area, Kingdom of Saudi Arabia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Overstreet, William C.; Mousa, Hassan; Matzko, John J.</p> <p>1985-01-01</p> <p>Crystals of magnetite as large as 30 mm long and 7 mm thick are locally present in quartz-rich <span class="hlt">zones</span> of interior and exterior pegmatite <span class="hlt">dikes</span> related to plutons of quartz monzonite in the Jabal Lababa area. Niobium, tin, and yttrium are strongly enriched in six specimens of magnetite from interior pegmatite <span class="hlt">dikes</span> in a small pluton where these elements form geochemical anomalies in nonmagnetic heavy-mineral concentrates from wadi sediment. Less abundant anomalous elements in the magnetite are molybdenum, lead, and zirconium, which also tend to be present in anomalous amounts in the nonmagnetic concentrates from the niobium-bearing pluton. The most anomalous trace element in the magnetite is zinc, which is at least 10 times as abundant as it is in the quartz monzonite plutons or in the nonmagnetic concentrates. The capacity of magnetite to scavenge molybdenum, zinc, niobium, lead, tin, yttrium, and zirconium suggests the possible utility of magnetite as a geochemical sample medium.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1989Tectp.161...23W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1989Tectp.161...23W"><span><span class="hlt">Dikes</span>, joints, and faults in the upper mantle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilshire, H. G.; Kirby, S. H.</p> <p>1989-04-01</p> <p>Three different types of macroscopic fractures are recognized in upper-mantle and lower-crustal xenoliths in volcanic rocks from around the world: (1) joints that are tensile fractures not occupied by crystallized magma products (2) <span class="hlt">dikes</span> that are tensile fractures occupied by mafic magmas crystallized to pyroxenites, gabbros or hydrous-mineral-rich rocks, (3) faults that are unfilled shear fractures with surface markings indicative of shear displacement. In addition to intra-xenolith fractures, xenoliths commonly have polygonal or faceted shapes that represent fractures exploited during incorporation of the xenoliths into the host magma that brought them to the surface. The various types of fractures are considered to have formed in response to the pressures associated with magmatic fluids and to the ambient tectonic stress field. The presence of fracture sets and crosscutting relations indicate that both magma-filled and unfilled fractures can be contemporaneous and that the local stress field can change with time, leading to repeated episodes of fracture. These observations give insight into the nature of deep fracture processes and the importance of fluid-peridotite interactions in the mantle. We suggest that unfilled fractures were opened by volatile fluids exsolved from ascending magmas to the tops of growing <span class="hlt">dikes</span>. These volatile fluids are important because they are of low viscosity and can rapidly transmit fluid pressure to <span class="hlt">dike</span> and fault tips and because they lower the energy and tectonic stresses required to extend macroscopic cracks and to allow sliding on pre-existing fractures. Mantle seismicity at depths of 20-65 km beneath active volcanic centers in Hawaii corresponds to the depth interval where CO 2-rich fluids are expected to be liberated from ascending basaltic magmas, suggesting that such fluids play an important role in facilitating earthquake instabilities in the presence of tectonic stresses. Other phenomena related to the fractures include</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V54B..03O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V54B..03O"><span>Percolation of isotopically heterogeneous interstitial melts in the crystal mush of the Rum layered <span class="hlt">intrusion</span>, NW Scotland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Driscoll, B.; Hepworth, L. N.; Daly, J. S.; Gertisser, R.; Emeleus, C. H.</p> <p>2017-12-01</p> <p>The cumulate stratigraphy of layered <span class="hlt">intrusions</span> offers a means of interrogating the replenishment and solidification histories of mafic magma chambers. Cumulates comprise cumulus minerals, which accumulate to form a silicate framework, and intercumulus minerals, which represent melt crystallised within the crystal mush. This fundamental textural distinction lies at the heart of cumulus theory and underpins some of the classic models of crystal-liquid differentiation that are based on layered <span class="hlt">intrusions</span>. In order to shed further light on the importance of postcumulus processes in layered <span class="hlt">intrusions</span>, and to demonstrate that crystal mushes may behave as open-systems during the crystallisation of cumulates, we investigated mineral-scale textural and geochemical heterogeneity in Unit 10 of the 60 Ma Rum layered <span class="hlt">intrusion</span>. Numerous ( 1 mm thick) Cr-spinel seams occur throughout the 65 m Unit 10 peridotite stratigraphy. Unusually, intercumulus plagioclase and clinopyroxene crystals in the peridotite several centimetres above and below these seams exhibit complex optical and major element <span class="hlt">zoning</span>. Sampling of individual intra-crystal <span class="hlt">zones</span> in these phases was carried out using a New Wave Micromill, for analysis of their 87Sr/86Sr compositions to be measured on unspiked samples by TIMS. Both minerals reveal intra-crystalline isotopic heterogeneity. The maximum range (with 2σ uncertainties) of 87Sr/86Sr in the Unit 10 plagioclase is 0.704026±17-0.704591±8 and in clinopyroxene is 0.703533±23-0.704517±17. Within a single, oscillatory-<span class="hlt">zoned</span> plagioclase, three discrete <span class="hlt">zones</span> yield 87Sr/86Sr values of 0.704337±20, 0.704095±20 and 0.704052±11. A complex patchily-<span class="hlt">zoned</span> clinopyroxene yields a 87Sr/86Sr range of 0.703533±23-0.703894±23. The new data demonstrate that multiple generations of isotopically distinct melts percolated through the Unit 10 crystal mush, suggesting solidification from cumulates that underwent repeated cycles of resorption and recrystallisation at the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7067L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7067L"><span>Successive reactive liquid flow episodes in a layered <span class="hlt">intrusion</span> (Unit 9, Rum Eastern Layered <span class="hlt">Intrusion</span>, Scotland)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leuthold, Julien; Blundy, Jon; Holness, Marian</p> <p>2014-05-01</p> <p> moving upwards and laterally through the cumulate pile. The Rum layered <span class="hlt">intrusion</span> is an open <span class="hlt">intrusive</span> complex, composed of individual partially molten <span class="hlt">zones</span>, evolving independently. The Rum layered <span class="hlt">intrusion</span> offers a direct overview of processes taking place in shallow intra-plate and ridge magma chambers. <span class="hlt">Intrusion</span> of hot magma into a pre-existing cumulate pile results in the modification both the incoming liquid and the host-rock cumulates. Our study highlights the necessity of considering this type of process when modelling the geochemistry of lavas erupted from magma chambers subject to repeated replenishment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ISPAr49B3..227H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ISPAr49B3..227H"><span>Morphological Changes Along a <span class="hlt">Dike</span> Landside Slope Sampled by 4d High Resolution Terrestrial Laser Scanning</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Herrero-Huertaa, Mónica; Lindenbergh, Roderik; Ponsioen, Luc; van Damme, Myron</p> <p>2016-06-01</p> <p>Emergence of light detection and ranging (LiDAR) technology provides new tools for geomorphologic studies improving spatial and temporal resolution of data sampling hydrogeological instability phenomena. Specifically, terrestrial laser scanning (TLS) collects high resolution 3D point clouds allowing more accurate monitoring of erosion rates and processes, and thus, quantify the geomorphologic change on vertical landforms like <span class="hlt">dike</span> landside slopes. Even so, TLS captures observations rapidly and automatically but unselectively. In this research, we demonstrate the potential of TLS for morphological change detection, profile creation and time series analysis in an emergency simulation for characterizing and monitoring slope movements in a <span class="hlt">dike</span>. The experiment was performed near Schellebelle (Belgium) in November 2015, using a Leica Scan Station C10. Wave overtopping and overflow over a <span class="hlt">dike</span> were simulated whereby the loading conditions were incrementally increased and 14 successful scans were performed. The aim of the present study is to analyse short-term morphological dynamic processes and the spatial distribution of erosion and deposition areas along a <span class="hlt">dike</span> landside slope. As a result, we are able to quantify the eroded material coming from the impact on the terrain induced by wave overtopping which caused the <span class="hlt">dike</span> failure in a few minutes in normal storm scenarios (Q = 25 l/s/m) as 1.24 m3. As this shows that the amount of erosion is measurable using close range techniques; the amount and rate of erosion could be monitored to predict <span class="hlt">dike</span> collapse in emergency situation. The results confirm the feasibility of the proposed methodology, providing scalability to a comprehensive analysis over a large extension of a <span class="hlt">dike</span> (tens of meters).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V53A..07A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V53A..07A"><span>Rare Mineralogy in Alkaline Ultramafic Rocks, Western Kentucky Fluorspar District</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anderson, W.</p> <p>2017-12-01</p> <p>The alkaline ultramafic <span class="hlt">intrusive</span> <span class="hlt">dike</span> complex in the Western Kentucky Fluorspar District contains unusual mineralogy that was derived from mantle magma sources. Lamprophyre and peridotite petrologic types occur in the district where altered fractionated peridotites are enriched in Rare Earth Elements (REE) and some lamprophyre facies are depleted in incompatible elements. Unusual minerals in <span class="hlt">dikes</span>, determined by petrography and X-ray diffraction, include schorlomite and andradite titanium garnets, astrophyllite, spodumene, niobium rutile, wüstite, fluoro-tetraferriphlogopite, villiaumite, molybdenite, and fluocerite, a REE-bearing fluoride fluorescent mineral. Mixing of MVT sphalerite ore fluids accompanies a mid-stage igneous alteration and <span class="hlt">intrusion</span> event consistent with paragenetic studies. The presence of lithium in the spodumene and fluoro-tetraferriphlogopite suggests a lithium phase in the mineral fluids, and the presence of enriched REE in <span class="hlt">dikes</span> and fluorite mineralization suggest a metasomatic event. Several of these rare minerals have never been described in the fluorspar district, and their occurrence suggests deep mantle metasomatism. Several REE-bearing fluoride minerals occur in the <span class="hlt">dikes</span> and in other worldwide occurrences, they are usually associated with nepheline syenite and carbonatite differentiates. There is an early and late stage fluoride mineralization, which accompanied <span class="hlt">dike</span> <span class="hlt">intrusion</span> and was also analyzed for REE content. One fluorite group is enriched in LREE and another in MREE, which suggests a bimodal or periodic fluorite emplacement. Whole-rock elemental analysis was chondrite normalized and indicates that some of the <span class="hlt">dikes</span> are slightly enriched in light REE and show a classic fractionation enrichment. Variations in major-element content; high titanium, niobium, and zirconium values; and high La/Yb, Zr/Y, Zr/Hf, and Nb/Ta ratios suggest metasomatized lithospheric-asthenospheric mantle-sourced <span class="hlt">intrusions</span>. The high La/Yb ratios in some</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JHyDy.tmp....1R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JHyDy.tmp....1R"><span>The coupling between hydrodynamic and purification efficiencies of ecological porous spur-<span class="hlt">dike</span> in field drainage ditch</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rao, Lei; Wang, Pei-fang; Dai, Qing-song; Wang, Chao</p> <p>2018-05-01</p> <p>In this study, a series of ecological porous spur-<span class="hlt">dikes</span> are arranged in an experiment channel to simulate a real field drainage ditch. The inside and outside flow fields of spur-<span class="hlt">dikes</span> are determined by numerical simulations and experimental methods. An Ammonia-Nitrogen (NH3-N) degradation evaluation model is built to calculate the pollution removal rate by coupling with the inner flow field of the porous spur-<span class="hlt">dikes</span>. The variations of the total pollutant removal rate in the channel are discussed in terms of different porosities and gap distances between spur-<span class="hlt">dikes</span> and inlet flow velocities. It is indicated that a reasonable parameter matching of the porosity and the gap distance with the flow velocity of the ditch can bring about a satisfactory purification efficiency with a small delivery quantity of ecological porous materials.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.T12C..07B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.T12C..07B"><span>Quasi-Periodic Slow Earthquakes and Their Association With Magmatic Activity at Kilauea Volcano, Hawai`i</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brooks, B. A.; Foster, J. H.; Sandwell, D.; Poland, M.; Myer, D.; Wolfe, C.; Patrick, M.</p> <p>2007-12-01</p> <p>Since 1998 the mobile south flank of Kilauea volcano, Hawai`i, has been the site of multiple slow earthquake (SE) events recorded principally with continuous GPS. One spatially coincident family of these SEs exhibited a high degree of periodicity (774 +/- 7 days) from 1998 to 2005 suggesting the next SE would be in mid-March, 2007. In fact, no anomalous deformation occurred there until the June 17 Father's day <span class="hlt">dike</span> <span class="hlt">intrusion</span> that caused up to 1m of opening along Kilauea's east rift <span class="hlt">zone</span>. We analyzed deformation related to the Father's day event using GPS, tilt, ALOS and Envisat interferometry, microseismicity, and elastic dislocation modeling. Our analysis reveals significant motions of far-field sites that cannot be explained by <span class="hlt">dike</span>-related deformation and that are very similar to previous SE displacements of the same sites, strongly suggesting that a SE occurred. Inclusion of this event in the overall time series yields SE repeat times of 798 +/- 50 days, apparently maintaining the quasi- periodicity of the Kilauea events. Furthermore, the timing of <span class="hlt">dike</span>- and SE-related deformation and stress modeling suggest the Father's day <span class="hlt">dike</span> triggered the slow earthquake. We explore the connection between magmatism and SEs at Kilauea and find a potential correlation between SE-timing and eruptive activity since 2000. This suggests the possibility that a mechanistic understanding of Kilauea SEs may require consideration of magmatic processes in addition to fault <span class="hlt">zone</span> processes.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V51C2675B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V51C2675B"><span>Crystal accumulation and compositional trends in a calc-alkaline batholith: implications for correlation of plutonic and volcanic rocks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barnes, C. G.; Coint, N.</p> <p>2013-12-01</p> <p>The Wooley Creek batholith is a tilted, calc-alkaline <span class="hlt">intrusive</span> complex in the Klamath Mountain province, California, that can be divided into two main <span class="hlt">zones</span>: lower (~159.2 × 0.2 Ma) and upper (~158.2 × 0.3 Ma), separated by a central transition <span class="hlt">zone</span>. The lower <span class="hlt">zone</span> consists of multiple <span class="hlt">intrusive</span> units of gabbro through tonalite, with minor mafic synplutonic <span class="hlt">dikes</span> and <span class="hlt">intrusive</span> melagabbro and pyroxenite. Major and trace element data plot in two groups: a mafic group that encompasses pyroxenite to diorite, and a tonalitic group. For each group, Mg/Fe in augite was used to determine the approximate composition of equilibrium melt and then major element mass balance was used to calculate proportions of cumulate phases and melt. For the mafic group, no single parental magma can be identified, which is consistent with assembly via many magma batches. However, the most mafic rocks were derived from basaltic andesite magmas and represent 30 to 100% cumulate augite + opx × plagioclase × olivine. Interstitial melt in the tonalitic group was dacitic, and mass balance indicates from 30 to 80% cumulate pyroxenes + plagioclase × accessory apatite and Fe-Ti oxides. The parental magma was probably silicic andesite. The upper <span class="hlt">zone</span> varies gradationally from structurally low quartz diorite to uppermost granite. Upper <span class="hlt">zone</span> magmas ';leaked' to form dacitic to rhyodacitic ';roof <span class="hlt">dikes</span>'. Previous work (Coint et al., Geosphere, in press) showed that the upper <span class="hlt">zone</span> formed from an approximately homogeneous magma body and that compositional variation was related to upward percolation of melt. Mass balance supports this interpretation and indicates that (1) the parental magmas were andesitic, (2) structurally low rocks are 15 to 65 % cumulate hornblende + plagioclase × pyroxene, and (3) high-level granite and granodiorite are the fractionated products of this accumulation. These results show that the upper <span class="hlt">zone</span> is a good example of fractional crystallization within a moderate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T43A0667C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T43A0667C"><span>Timing of Multiple Stages of Granitic Magmatisms: Constraints on Shearing along the Ailao Shan-Red River Shear <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, W.; Liu, J.; Fan, W.; Feng, J.; DAO, H.; Yan, J.</p> <p>2017-12-01</p> <p>The Ailao Shan-Red River (ASRR) shear <span class="hlt">zone</span> is a large scale shear <span class="hlt">zone</span> resulted from collision between India and Euro-Asia Plates in Cenozoic. Magmatisms related to the shear <span class="hlt">zone</span> evolution took place before, during or after shearing process that contributes to pre-, syn- and post- granitic emplacement. Combined structure, fabric and geochronology analyses of granitic rocks within sheared Proterozoic country rocks along the ASRR shear <span class="hlt">zone</span> offer important clues on timing of shearing activity and constraining on transformation of types of the shearing. Zircon U-Pb dating results indicate that the granitic <span class="hlt">intrusions</span> within the ASRR shear <span class="hlt">zone</span> are broadly grouped into two stages: Permo-Triassic (256.0±6.0 Ma, 244.0±7.6 Ma and 234.0±9.3 Ma) and Cenozoic (27.1±1.5 Ma, 26.34±0.62 Ma and 25.10±0.61 Ma). The Permo-Triassic <span class="hlt">intrusions</span> show evidences for intensive mylonitization. The older Cenozoic granitic rocks were also strongly sheared, but the younger Cenozoic granites were weakly sheared and they cut across early <span class="hlt">intrusions</span> (e.g. the Permo-Triassic and older Cenozoic <span class="hlt">intrusions</span>). Petrographic microscope observations suggest that the Permo-Triassic granitic <span class="hlt">intrusions</span> show prominent superimposition of high temperature mylonization by low temperature mylonization. Quartz c-axis fabrics of the granites demonstrate that there are multiple maxima due to the superimposition. The older Cenozoic granitic <span class="hlt">intrusion</span> of 27.1±1.5 Ma shows weak mylonization and possess four symmetrical point maxima in their quartz c-axis fabrics. The EBSD data indicate that the <span class="hlt">intrusion</span> experienced pure shearing. <span class="hlt">Intrusions</span> of 26.34±0.62 Ma and 25.10±0.61 Ma show evidences for very weak mylonization. The quartz c-axis patterns of the rocks dominantly resulted from low temperature deformation by simple shearing. It is concluded, in summary, that: (1) Permo-Triassic granitic <span class="hlt">intrusions</span> experienced superimposed shearing of high and low temperatures; (2) Evidences for both early pure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..4310738S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..4310738S"><span>Evidence for Moho-lower crustal transition depth <span class="hlt">diking</span> and rifting of the Sierra Nevada microplate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, Kenneth D.; Kent, Graham M.; Seggern, David P.; Driscoll, Neal W.; Eisses, Amy</p> <p>2016-10-01</p> <p>Lithospheric rifting most often initiates in continental extensional settings where "breaking of a plate" may or may not progress to sea floor spreading. Generally, the strength of the lithosphere is greater than the tectonic forces required for rupture (i.e., the "tectonic force paradox"), and it has been proposed that rifting requires basaltic magmatism (e.g., <span class="hlt">dike</span> emplacement) to reduce the strength and cause failure, except for the case of a thin lithosphere (<30 km thick). Here we isolate two very similar and unprecedented observations of Moho-lower crustal transition <span class="hlt">dike</span> or fluid injection earthquake swarms under southern Sierra Valley (SV: 2011-2012) and North Lake Tahoe (LT: 2003-2004), California. These planar distributions of seismicity can be interpreted to define the end points, and cover 25% of the length, of an implied 56 km long structure, each striking N45°W and dipping 50°NE. A single event at 30 km depth that locates on the implied dipping feature between the two swarms is further evidence for a single Moho-transition depth structure. We propose that basaltic or fluid emplacement at or near Moho depths weakens the upper mantle lid, facilitating lithospheric rupture of the Sierra Microplate. Similar to the LT sequence, the SV event is also associated with increased upper crustal seismicity. An 27 October 2011, Mw 4.7 earthquake occurred directly above the deep SV sequence at the base of the upper crustal seismogenic <span class="hlt">zone</span> ( 15 km depth).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015E%26PSL.431..140K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015E%26PSL.431..140K"><span>Deep <span class="hlt">intrusions</span>, lateral magma transport and related uplift at ocean island volcanoes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Klügel, Andreas; Longpré, Marc-Antoine; García-Cañada, Laura; Stix, John</p> <p>2015-12-01</p> <p>Oceanic intraplate volcanoes grow by accumulation of erupted material as well as by coeval or discrete magmatic <span class="hlt">intrusions</span>. Dykes and other <span class="hlt">intrusive</span> bodies within volcanic edifices are comparatively well studied, but <span class="hlt">intrusive</span> processes deep beneath the volcanoes remain elusive. Although there is geological evidence for deep magmatic <span class="hlt">intrusions</span> contributing to volcano growth through uplift, this has rarely been demonstrated by real-time monitoring. Here we use geophysical and petrological data from El Hierro, Canary Islands, to show that <span class="hlt">intrusions</span> from the mantle and subhorizontal transport of magma within the oceanic crust result in rapid endogenous island growth. Seismicity and ground deformation associated with a submarine eruption in 2011-2012 reveal deep subhorizontal <span class="hlt">intrusive</span> sheets (sills), which have caused island-scale uplift of tens of centimetres. The pre-eruptive <span class="hlt">intrusions</span> migrated 15-20 km laterally within the lower oceanic crust, opening pathways that were subsequently used by the erupted magmas to ascend from the mantle to the surface. During six post-eruptive episodes between 2012 and 2014, further sill <span class="hlt">intrusions</span> into the lower crust and upper mantle have caused magma to migrate up to 20 km laterally, resulting in magma accumulation exceeding that of the pre-eruptive phase. A comparison of geobarometric data for the 2011-2012 El Hierro eruption with data for other Atlantic intraplate volcanoes shows similar bimodal pressure distributions, suggesting that eruptive phases are commonly accompanied by deep <span class="hlt">intrusions</span> of sills and lateral magma transport. These processes add significant material to the oceanic crust, cause uplift, and are thus fundamentally important for the growth and evolution of volcanic islands. We suggest that the development of such a magma accumulation <span class="hlt">zone</span> in the lower oceanic crust begins early during volcano evolution, and is a consequence of increasing size and complexity of the mantle reservoir system, and potentially</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002CoMP..142..564J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002CoMP..142..564J"><span>Petrology of iron-rich magmatic segregations associated with strongly peraluminous trondhjemite in the Cornucopia stock, northeastern Oregon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnson, K.; Barnes, C. G.; Browning, J. M.; Karlsson, H. R.</p> <p></p> <p>The Middle Cretaceous Cornucopia stock in the Blue Mountains of northeastern Oregon is a small composite <span class="hlt">intrusion</span> consisting of hornblende biotite tonalite, biotite trondhjemite, and three cordierite two mica trondhjemite units. Unusual magnetite + biotite-rich tonalitic rocks are associated with the Crater Lake cordierite trondhjemite, the youngest of the <span class="hlt">intrusions</span>. Oxide-rich tonalites are characterized by high Fe ( 47-68 wt% total Fe as FeO), low SiO2 (<36 wt%), and enrichments in HFSE and REE (La(N)=361-903). Oxide-rich tonalites appear in a variety of forms, including composite <span class="hlt">dikes</span> and sheets, in which they are associated with leucocratic tonalite. Leucotonalite is lower in SiO2 (60-72 wt%) than Crater Lake trondhjemite, and generally has ΣREE contents and Eu anomalies intermediate between the oxide-rich tonalite and Crater Lake compositions. Oxide-rich tonalites crosscut, and are crosscut by, shear <span class="hlt">zones</span> in the host trondhjemite, indicating their emplacement late in the pluton's crystallization history. Granitic <span class="hlt">dikes</span> crosscut the composite <span class="hlt">dikes</span> in all localities. Geochemical considerations and sedimentary-like structures, such as load casts and bedding of magnetite-rich assemblages in the composite <span class="hlt">dikes</span> and sheets, are suggestive of crystal settling from an Fe-rich parental magma. The Fe-rich liquid parental to the oxide-rich tonalite-leucotonalite pairs formed by extensive, in-situ, plagioclase + quartz-dominated crystallization of strongly peraluminous trondhjemite. Early magnetite saturation in the trondhjemite was suppressed, either because the parental trondhjemitic magma had a lower initial total Fe content or because it had a lower ferric-ferrous ratio, possibly reflecting a lower oxygen fugacity. Accumulation of magnetite from Fe-rich residual magma is a viable mechanism for the concentration of iron, and the subsequent formation of Fe-rich rocks, in calcic siliceous <span class="hlt">intrusions</span>. Apparently, Fe-enrichment can occur locally in calcic magmas, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001CoMP..142..564J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001CoMP..142..564J"><span>Petrology of iron-rich magmatic segregations associated with strongly peraluminous trondhjemite in the Cornucopia stock, northeastern Oregon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnson, K.; Barnes, C. G.; Browning, J. M.; Karlsson, H. R.</p> <p>2001-11-01</p> <p>The Middle Cretaceous Cornucopia stock in the Blue Mountains of northeastern Oregon is a small composite <span class="hlt">intrusion</span> consisting of hornblende biotite tonalite, biotite trondhjemite, and three cordierite two mica trondhjemite units. Unusual magnetite + biotite-rich tonalitic rocks are associated with the Crater Lake cordierite trondhjemite, the youngest of the <span class="hlt">intrusions</span>. Oxide-rich tonalites are characterized by high Fe ( 47-68 wt% total Fe as FeO), low SiO2 (<36 wt%), and enrichments in HFSE and REE (La(N)=361-903). Oxide-rich tonalites appear in a variety of forms, including composite <span class="hlt">dikes</span> and sheets, in which they are associated with leucocratic tonalite. Leucotonalite is lower in SiO2 (60-72 wt%) than Crater Lake trondhjemite, and generally has ΣREE contents and Eu anomalies intermediate between the oxide-rich tonalite and Crater Lake compositions. Oxide-rich tonalites crosscut, and are crosscut by, shear <span class="hlt">zones</span> in the host trondhjemite, indicating their emplacement late in the pluton's crystallization history. Granitic <span class="hlt">dikes</span> crosscut the composite <span class="hlt">dikes</span> in all localities. Geochemical considerations and sedimentary-like structures, such as load casts and bedding of magnetite-rich assemblages in the composite <span class="hlt">dikes</span> and sheets, are suggestive of crystal settling from an Fe-rich parental magma. The Fe-rich liquid parental to the oxide-rich tonalite-leucotonalite pairs formed by extensive, in-situ, plagioclase + quartz-dominated crystallization of strongly peraluminous trondhjemite. Early magnetite saturation in the trondhjemite was suppressed, either because the parental trondhjemitic magma had a lower initial total Fe content or because it had a lower ferric-ferrous ratio, possibly reflecting a lower oxygen fugacity. Accumulation of magnetite from Fe-rich residual magma is a viable mechanism for the concentration of iron, and the subsequent formation of Fe-rich rocks, in calcic siliceous <span class="hlt">intrusions</span>. Apparently, Fe-enrichment can occur locally in calcic magmas, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18755967','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18755967"><span>Magmatically triggered slow slip at Kilauea Volcano, Hawaii.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brooks, Benjamin A; Foster, James; Sandwell, David; Wolfe, Cecily J; Okubo, Paul; Poland, Michael; Myer, David</p> <p>2008-08-29</p> <p>We demonstrate that a recent <span class="hlt">dike</span> <span class="hlt">intrusion</span> probably triggered a slow fault-slip event (SSE) on Kilauea volcano's mobile south flank. Our analysis combined models of Advanced Land Observing Satellite interferometric <span class="hlt">dike-intrusion</span> displacement maps with continuous Global Positioning System (GPS) displacement vectors to show that deformation nearly identical to four previous SSEs at Kilauea occurred at far-field sites shortly after the <span class="hlt">intrusion</span>. We model stress changes because of both secular deformation and the <span class="hlt">intrusion</span> and find that both would increase the Coulomb failure stress on possible SSE slip surfaces by roughly the same amount. These results, in concert with the observation that none of the previous SSEs at Kilauea was directly preceded by <span class="hlt">intrusions</span> but rather occurred during times of normal background deformation, suggest that both extrinsic (<span class="hlt">intrusion</span>-triggering) and intrinsic (secular fault creep) fault processes can lead to SSEs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V12B..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V12B..07M"><span>Hiding the Evidence: Growth of plutons by incremental emplacement of sheets in crystal mush</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, C. F.; Furbish, D. J.; Claiborne, L. L.; Walker, B. A.; Bleick, H. A.; Steinwinder, T. R.; Koteas, G. C.</p> <p>2006-12-01</p> <p>Growing evidence supports the notion that plutons are constructed incrementally, commonly over long periods of time, yet field evidence for the multiple injections that seem to be required is commonly sparse or absent (e.g. Glazner et al. 2004). Timescales of up to several million years, among other arguments, indicate that the dominant volume does not remain largely molten, yet if growing plutons are constructed from rapidly solidifying increments it is unlikely that <span class="hlt">intrusive</span> contacts would escape notice. A model wherein magma increments are emplaced into crystal mush rather than either solid or crystal-poor material provides a plausible explanation for this apparent conundrum. A partially solidified <span class="hlt">intrusion</span> undoubtedly comprises <span class="hlt">zones</span> with contrasting melt fraction and therefore strength. The emplacement of <span class="hlt">dikes</span> that intrude such a strength-<span class="hlt">zoned</span> <span class="hlt">intrusion</span> will be guided by the contrasts in the same way that <span class="hlt">dikes</span> intruding solid media: magma spreads rather than continuing to propagate upward where it encounters a <span class="hlt">zone</span> of higher rigidity (e.g. experiments by Kavanagh et al. 2006). We propose that ascending magma is in essence trapped by low-strength <span class="hlt">zones</span> in plutonic mushes that are relatively melt-rich. In many cases, such <span class="hlt">zones</span> may be subhorizontal and thus sill-like in geometry, but shapes and orientations could be highly variable, depending on the prior history of the composite <span class="hlt">intrusion</span>. Contacts will commonly be obscure from the start because the contrast between intruding material (crystal-poorer magma) and host (crystal-richer mush) is subtle, and it may be obscured even further by subsequent destabilization of the mush. Field evidence and zircon <span class="hlt">zoning</span> stratigraphy in plutons of the Colorado River region of southern Nevada support the hypothesis that emplacement of magma replenishments into a mush host is important in pluton construction. Except for highly fractionated <span class="hlt">dikes</span> and sills, the dominant granite unit of the Spirit Mountain batholith</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V53F..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V53F..02S"><span><span class="hlt">Intrusion</span> Triggering of Explosive Eruptions: Lessons Learned from EYJAFJALLAJÖKULL 2010 Eruptions and Crustal Deformation Studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sigmundsson, F.; Hreinsdottir, S.; Hooper, A. J.; Arnadottir, T.; Pedersen, R.; Roberts, M. J.; Oskarsson, N.; Auriac, A.; Decriem, J.; Einarsson, P.; Geirsson, H.; Hensch, M.; Ofeigsson, B. G.; Sturkell, E. C.; Sveinbjornsson, H.; Feigl, K.</p> <p>2010-12-01</p> <p>Gradual inflation of magma chambers often precedes eruptions at highly active volcanoes. During eruptions, rapid deflation occurs as magma flows out and pressure is reduced. Less is known about the deformation style at moderately active volcanoes, such as Eyjafjallajökull, Iceland, where an explosive summit eruption of trachyandesite beginning on 14 April 2010 caused exceptional disruption to air traffic. This eruption was preceded by an effusive flank eruption of olivine basalt from 20 March - 12 April 2010. Geodetic and seismic observations revealed the growth of an <span class="hlt">intrusive</span> complex in the roots of the volcano during three months prior to eruptions. After initial horizontal growth, modelling indicates both horizontal and sub-vertical growth in three weeks prior the first eruption. The behaviour is attributed to subsurface variations in crustal stress and strength originating from complicated volcano foundations. A low-density layer may capture magma allowing pressure to build before an <span class="hlt">intrusion</span> can ascend towards higher levels. The <span class="hlt">intrusive</span> complex was formed by olivine basalt as erupted on the volcano flank 20 March - 12 April; the <span class="hlt">intrusive</span> growth halted at the onset of this eruption. Deformation associated with the eruption onset was minor as the <span class="hlt">dike</span> had reached close to the surface in the days before. Isolated eruptive vents opening on long-dormant volcanoes may represent magma leaking upwards from extensive pre-eruptive <span class="hlt">intrusions</span> formed at depth. A deflation source activated during the summit eruption of trachyandesite is distinct from, and adjacent to, all documented sources of inflation in the volcano roots. Olivine basalt magma which recharged the volcano appears to have triggered the summit eruption, although the exact mode of triggering is uncertain. Scenarios include stress triggering or propagation of olivine basalt into more evolved magma. The trachyandesite includes crystals that can be remnants of minor recent <span class="hlt">intrusion</span> of olivine basalt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013MinDe..48..687M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013MinDe..48..687M"><span>The role of <span class="hlt">intrusions</span> in the formation of Irish-type mineralisation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McCusker, Jim; Reed, Christopher</p> <p>2013-08-01</p> <p>The Stonepark Prospect is located in County Limerick, south-central Ireland. Multiple <span class="hlt">zones</span> of Zn-Pb mineralisation have been identified at Stonepark and these are approximately 5 km west of the Pallas Green Prospect. At Stonepark, the sulphide bodies are hosted within the Waulsortian Limestone and closely resemble other Irish-type deposits. The mineralisation is composed of pyrite-marcasite, sphalerite and galena with gangue Fe-dolomite and calcite cements. A key difference at Stonepark is the presence of Chadian-aged volcanic rocks (Knockroe Volcanics) that intrude into and overlie the Waulsortian Limestone. Subsequent hydrothermal brecciation of the Waulsortian Limestone and Knockroe <span class="hlt">intrusions</span> resulted in the formation of tabular polymict breccia bodies containing mixed carbonate and clasts of <span class="hlt">intrusive</span> rocks. These have then been overprinted by massive sulphide mineralisation. Further syn-mineralisation brecciation has overprinted the earlier breccias. Drilling has demonstrated a spatial relationship between the volume of <span class="hlt">intrusive</span> rocks (dykes and polymict breccias) and Zn-Pb mineralisation. This association suggests that the <span class="hlt">intrusive</span> rocks provided a mechanism for the introduction of the mineralising fluids into the breccia bodies. This is significant as to date no large controlling fault has been identified, as is seen at other Irish-type deposits. Further work is required to understand the alteration process of the <span class="hlt">intrusive</span> rocks and how this may relate to the mineralising process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.tandfonline.com/doi/abs/10.1080/00028487.2014.911207','USGSPUBS'); return false;" href="http://www.tandfonline.com/doi/abs/10.1080/00028487.2014.911207"><span>Fish assemblages, connectivity, and habitat rehabilitation in a <span class="hlt">diked</span> Great Lakes coastal wetland complex</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kowalski, Kurt P.; Wiley, Michael J.; Wilcox, Douglas A.</p> <p>2014-01-01</p> <p>Fish and plant assemblages in the highly modified Crane Creek coastal wetland complex of Lake Erie were sampled to characterize their spatial and seasonal patterns and to examine the implications of the hydrologic connection of <span class="hlt">diked</span> wetland units to Lake Erie. Fyke netting captured 52 species and an abundance of fish in the Lake Erie–connected wetlands, but fewer than half of those species and much lower numbers and total masses of fish were captured in <span class="hlt">diked</span> wetland units. Although all wetland units were immediately adjacent to Lake Erie, there were also pronounced differences in water quality and wetland vegetation between the hydrologically isolated and lake-connected wetlands. Large seasonal variations in fish assemblage composition and biomass were observed in connected wetland units but not in disconnected units. Reestablishment of hydrologic connectivity in <span class="hlt">diked</span> wetland units would allow coastal Lake Erie fish to use these vegetated habitats seasonally, although connectivity does appear to pose some risks, such as the expansion of invasive plants and localized reductions in water quality. Periodic isolation and drawdown of the <span class="hlt">diked</span> units could still be used to mimic intermediate levels of disturbance and manage invasive wetland vegetation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2004/1409/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2004/1409/report.pdf"><span>Assessment of Shallow-Water Habitat Availability in Modified <span class="hlt">Dike</span> Structures, Lower Missouri River, 2004</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jacobson, Robert B.; Elliott, Caroline M.; Johnson, Harold E.</p> <p>2004-01-01</p> <p>This study documented the effects of wing-<span class="hlt">dike</span> notching on the availabilit of shallow water habitat in the Lower Missouri River. Five wing <span class="hlt">dikes</span> were surveyed in late May 2004 after they were notched in early May as part of shallow-water habitat (SWH) rehabilitation activities undertaken by the U.S. Army Corps of Engineers. Surveys included high-resolution hydroacoustic depth, velocity, and substrate mapping. Relations of bottom elevations within the wing <span class="hlt">dike</span> fields to index discharges and water-surface elevations indicate that little habitat meeting the SWH definition was created immediately following notching. This result is not unexpected, as significant geomorphic adjustment may require large flow events. Depth, velocity, and substrate measurements in the post-rehabilitation time period provide baseline data for monitoring ongoing changes. Differences in elevation and substrate were noted at all sites. Most <span class="hlt">dike</span> fields showed substantial aggradation and replacement of mud substrate with sandier sediment, although the changes did not result in increased availability of SWH at the index discharge. It is not known how much of the elevation and substrate changes can be attributed directly to notching and how much would result from normal sediment transport variation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003JGRB..108.2097S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003JGRB..108.2097S"><span>Episodic <span class="hlt">dike</span> swarms inferred from near-bottom magnetic anomaly maps at the southern East Pacific Rise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shah, Anjana K.; Cormier, Marie-Helene; Ryan, William B. F.; Jin, Wen; Sinton, John; Bergmanis, Eric; Carlut, Julie; Bradley, Al; Yoerger, Dana</p> <p>2003-02-01</p> <p>Near-bottom, high-resolution magnetic field data gathered at the southern East Pacific Rise near 17°28'S, 18°14'S, and 18°37'S, using the autonomous underwater vehicle Autonomous Benthic Explorer (ABE) echo various geologic structures, including void space within lobate caverns, recent pillow mounds, and hydrothermal vent activity. This study is focused on a magnetic field low extending several kilometers along axis, coincident with a trough created by the draining of a lava lake during a highly effusive fissure eruption at 17°28'S. Similar lows are observed at three other drained lava lake troughs, including one which is at least 1800 years old, residing 400 m away from the present-day axis. We attribute these lows to the presence of shallow <span class="hlt">dike</span> swarms. The degree to which other geologic features may contribute to the lows is constrained using geologic, geophysical, and geochemical observations and forward modeling. Compositional analyses of Alvin samples at 17°28'S do not support Fe or Ti variations as a primary source. Hypotheses requiring hydrothermal alteration and porosity variations are both inconsistent with geologic observations and near-bottom gravity data analysis from similar areas. Previous mappings between paleointensity variations and the observed magnetic field over distances of several kilometers from the axis suggest that such variations do not create the field low. The dominant source of the magnetization low is most likely the presence of a 100-200 m wide region of shallow <span class="hlt">dikes</span> which are poorly magnetized relative to extrusives, or a region heated above magnetic blocking or Curie temperatures by <span class="hlt">intrusions</span> during the most recent eruption (though the latter interpretation cannot explain the low at the fossil trough). In the first case, this extrusive thinning implies a change in eruptive behavior over the last 750-1500 years given the local spreading rate. For the latter case, thermal models suggest the anomaly had to have been created by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1857i0004B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1857i0004B"><span>Wave run-up of a possible Anak-Krakatau tsunami on planned and optimized Jakarta Sea <span class="hlt">Dike</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Badriana, M. R.; Bachtiar, H.; Adytia, D.; Sembiring, L.; Andonowati, van Groesen, E.</p> <p>2017-07-01</p> <p>The infrastructural plans in the Jakarta Bay to reduce risks of flooding in Jakarta city comprise a large Sea <span class="hlt">Dike</span> that encloses a retention lake. Part of the planned <span class="hlt">dike</span> has the shape of the iconic Garuda bird. This paper shows that if in the future an explosion of Anak Krakatau will occur with strength 1/4th of the original Karkatau 1883 explosion, wave crests of 11m and troughs of 6m may collide against the bird's head. As an alternative example, a more optimized design of the <span class="hlt">dike</span> is constructed that reduces the maximal wave effects considerably.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/wa0488.photos.370695p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/wa0488.photos.370695p/"><span>1. View of north tower, facing northwest from <span class="hlt">dike</span> on ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>1. View of north tower, facing northwest from <span class="hlt">dike</span> on north bank of the Columbia River. - Pasco-Kennewick Transmission Line, Columbia River Crossing Towers, Columbia Drive & Gum Street, Kennewick, Benton County, WA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V51H..08S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V51H..08S"><span>Setting of the Father's Day Eruption at Kilauea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Swanson, D. A.</p> <p>2007-12-01</p> <p> the <span class="hlt">zone</span>. The Koa`e fault system joins the east rift <span class="hlt">zone</span> at the curve. The complex structural setting likely affects the frequency of magmatic activity in the segment. All of the eruptive and <span class="hlt">intrusive</span> activity results in storage of isolated magma bodies. Not surprisingly, petrologists find evidence that summit magma mixes with stored, fractionated magma. The area near Makaopuhi Crater and Kane Nui o Hamo is a particular focus, inferred since the mid-1960s to harbor a shallow magma reservoir. All of the eruptions and <span class="hlt">intrusions</span> are accompanied by sharp deflation and shallow seismicity at the summit and shallow seismicity and uplift along the <span class="hlt">intrusion</span> or eruptive fissures. Most often, no seismicity occurs between the summit and the area of <span class="hlt">intrusion</span> or eruption. Within that area, seismicity commonly migrates downrift but occasionally uprift. Similarly, crack opening generally progresses downrift, with a few exceptions. Cracks generally trend about 65 degrees and can be either left- or right-stepping. Cracks open along azimuths of 155-175, with local exceptions. There is no structural difference between eruptive cracks (fissures) and non- eruptive cracks. Single eruptive fissures rarely exceed 200 m in length, instead stepping within en echelon <span class="hlt">zones</span> above a presumably linear <span class="hlt">dike</span>. Since the late 1960s, widening has been measured across the active area during eruptions and <span class="hlt">intrusions</span>, first by EDM and then by satellite-based systems. The opening is nearly symmetrical within the rift <span class="hlt">zone</span>, but farther out the north flank barely responds whereas the south flank moves seaward. Available leveling data show uplift on either side of the <span class="hlt">dike</span> and subsidence along the crest. Examples of deformation in the 1960s and 1970s will be presented, and bibliographic references to past activity will be available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V53C3116W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V53C3116W"><span>Temporal Evolution of Surface Deformation and Magma Sources at Pacaya Volcano, Guatemala Revealed by InSAR</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wnuk, K.; Wauthier, C.</p> <p>2016-12-01</p> <p>Pacaya Volcano, Guatemala is a persistently active volcano whose western flank is unstable. Despite continuous activity since 1961, a lack of high temporal resolution geodetic surveying has prevented detailed modeling of Pacaya's underlying magmatic plumbing system. A new, temporally dense dataset of Interferometric Synthetic Aperture Radar (InSAR) RADARSAT-2 images, spanning December 2012 to March 2014, shows magmatic deformation before and during major eruptions in January and March 2014. Inverse modeling of InSAR surface displacements suggest that three magma bodies are responsible for observed deformation: (1) a 3.7 km deep spherical reservoir located northwest of the summit, (2) a 0.4 km deep spherical source located directly west of the summit, and (3) a shallow <span class="hlt">dike</span> below the summit that provides the primary transport pathway for erupted materials. Periods of heightened activity are brought on by magma pulses at depth, which result in rapid inflation of the edifice. We observe an <span class="hlt">intrusion</span> cycle at Pacaya that consists of deflation of one or both magma reservoirs followed by <span class="hlt">dike</span> <span class="hlt">intrusion</span>. <span class="hlt">Intrusion</span> volumes are proportional to reservoir volume loss, and do not always result in an eruption. Periods of increased activity culminate with larger <span class="hlt">dike</span> fed eruptions. Large eruptions are followed by inter eruptive periods marked by a decrease in crater explosions and a lack of deformation. A full understanding of magmatic processes at Pacaya is required to assess potential impacts on other aspects of the volcano such as the unstable western flank. Co-eruptive flank motion appears to have initiated a new stage of volcanic rifting at Pacaya defined by repeated NW-SE <span class="hlt">dike</span> <span class="hlt">intrusions</span>. This creates a positive feedback relationship whereby magmatic forcing from eruptive <span class="hlt">dike</span> <span class="hlt">intrusions</span> induces flank motion</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813550M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813550M"><span>Drone based structural mapping at Holuhraun indicates fault reactivation and complexity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mueller, Daniel; Walter, Thomas R.; Steinke, Bastian; Witt, Tanja; Schoepa, Anne; Duerig, Tobi; Gudmundsson, Magnus T.</p> <p>2016-04-01</p> <p>Accompanied by an intense seismic swarm in August 2014, a <span class="hlt">dike</span> laterally formed, starting under Icelands Vatnajökull glacier, propagating over a distance of more than 45 km within only two weeks, leading to the largest eruption by volume since the 1783-84 Laki eruption. Along its propagation path, the <span class="hlt">dike</span> caused intense surface displacements up to meters. Based on seismicity, GPS and InSAR, the propagation has already been analysed and described as segmented lateral <span class="hlt">dike</span> growth. We now focus on few smaller regions of the <span class="hlt">dike</span>. We consider the Terrasar-X tandem digital elevation map and aerial photos and find localized <span class="hlt">zones</span> where structural fissures formed and curved. At these localized, regions we performed a field campaign in summer 2015, applying the close range remote sensing techniques Structure from Motion (SfM) and Terrestrial Laser Scanning (TLS). Over 4 TLS scan were collected, along with over 5,000 aerial images. Point clouds from SfM and TLS are merged and compared, and local structural lineaments analysed. As a result, we obtained an unprecedentedly high-resolution digital elevation map. With this map, we analyse the structural expression of the fissure eruption at the surface and improve understanding on the conditions that influenced the magma propagation path. We elaborate scenarios that lead to complexities of the surface structures and the link to the underlying <span class="hlt">dike</span> <span class="hlt">intrusion</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911762G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911762G"><span>Effects of fluidization of the host sediment on peperite textures: A field example from the Cretaceous Buan Volcanics, SW Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gihm, Yong Sik; Kwon, Chang Woo</p> <p>2017-04-01</p> <p>In the Cretaceous Buan Volcanics (SW Korea), blocky and fluidal peperites are hosted in a massive pumiceous lapilli tuff intruded by intermediate <span class="hlt">dikes</span>. Blocky peperites, the most abundant species, are characterized by polyhedral or platy juvenile clasts and a jigsaw-crack texture. Fluidal peperites occur only along <span class="hlt">dike</span> margins, where the host sediments are composed of well sorted, fine to very fine ash (fine-grained <span class="hlt">zone</span>), and are characterized by fluidal or globular juvenile clasts with irregular or ragged margins. The fine-grained <span class="hlt">zone</span> is interpreted to form by grain size segregation caused by upward moving pore water (fluidization) that has resulted from heat transfer from intruding magma toward waterlogged host sediments during <span class="hlt">intrusion</span>. With the release of pore water and the selective entrainment of fine-grained ash, fine-grained <span class="hlt">zones</span> formed within the host sediments. Subsequent interactions between the fine-grained <span class="hlt">zone</span> and the intruding magma resulted in ductile deformation of the magma before fragmentation, which generated fluidal peperites. Outside the fine-grained <span class="hlt">zone</span>, intruding magma fragmented in a brittle manner because of the relative deficiency of both pore water and fine-grained ash, resulting in the formation of blocky peperites. The results of this study suggest that redistribution of constituent particles (ash) and interstitial fluids during fluidization resulted in heterogeneous physical conditions of the host sediments, which influenced peperite-forming processes, as reflected by the different peperite textures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..350....7C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..350....7C"><span>Resonance oscillations of the Soufrière Hills Volcano (Montserrat, W.I.) magmatic system induced by forced magma flow from the reservoir into the upper plumbing <span class="hlt">dike</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Chin-Wu; Huang, Hsin-Fu; Hautmann, Stefanie; Sacks, I. Selwyn; Linde, Alan T.; Taira, Taka'aki</p> <p>2018-01-01</p> <p>Short-period deformation cycles are a common phenomenon at active volcanoes and are often attributed to the instability of magma flow in the upper plumbing system caused by fluctuations in magma viscosity related to cooling, degassing, and crystallization. Here we present 20-min periodic oscillations in ground deformation based on high-precision continuous borehole strain data that were associated with the 2003 massive dome-collapse at the Soufrière Hills Volcano, Montserrat (West Indies). These high-frequency oscillations lasted 80 min and were preceded by a 4-hour episode of rapid expansion of the shallow magma reservoir. Strain amplitude ratios indicate that the deformational changes were generated by pressure variations in the shallow magma reservoir and - with reversed polarity - the adjacent plumbing <span class="hlt">dike</span>. The unusually short period of the oscillations cannot be explained with thermally induced variations in magma properties. We investigate the underlying mechanism of the oscillations via a numerical model of forced magma flow through a reservoir-<span class="hlt">dike</span> system accounting for time-dependent dilation/contraction of the <span class="hlt">dike</span> due to a viscous response in the surrounding host rock. Our results suggest that the cyclic pressure variations are modulated by the dynamical interplay between rapid expansion of the magma chamber and the incapacity of the narrow <span class="hlt">dike</span> to take up fast enough the magma volumes supplied by the reservoir. Our results allow us to place first order constraints on the viscosity of crustal host rocks and consequently its fractional melt content. Hence, we present for the first time crustal-scale in situ measurements of rheological properties of mush <span class="hlt">zones</span> surrounding magmatic systems.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/ca1662.photos.011939p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ca1662.photos.011939p/"><span>1. OIL HOUSE FOUNDATIONS, <span class="hlt">DIKE</span>, AND PORTION OF SOUTH FRONT ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>1. OIL HOUSE FOUNDATIONS, <span class="hlt">DIKE</span>, AND PORTION OF SOUTH FRONT OF MAIN ASSEMBLY PLANT. VIEW TO WEST. - Ford Motor Company Long Beach Assembly Plant, Oil House, 700 Henry Ford Avenue, Long Beach, Los Angeles County, CA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/pa2635.photos.356810p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/pa2635.photos.356810p/"><span>3. VIEW NORTH FROM TOP OF <span class="hlt">DIKE</span>, WITH FORMER TRANSFORMER ...</span></a></p> <p><a target="_blank" href="http://www.loc.gov/pictures/collection/hh/">Library of Congress Historic Buildings Survey, Historic Engineering Record, Historic Landscapes Survey</a></p> <p></p> <p></p> <p>3. VIEW NORTH FROM TOP OF <span class="hlt">DIKE</span>, WITH FORMER TRANSFORMER BUILDING AND SERVICE SHED - Middle Creek Hydroelectric Dam, On Middle Creek, West of U.S. Route 15, 3 miles South of Selinsgrove, Selinsgrove, Snyder County, PA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70026284','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70026284"><span>Structural localization and origin of compartmentalized fluid flow, Comstock lode, Virginia City, Nevada</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Berger, B.R.; Tingley, J.V.; Drew, L.J.</p> <p>2003-01-01</p> <p>Bonanza-grade orebodies in epithermal-style mineral deposits characteristically occur as discrete <span class="hlt">zones</span> within spatially more extensive fault and/or fracture systems. Empirically, the segregation of such systems into compartments of higher and lower permeability appears to be a key process necessary for high-grade ore formation and, most commonly, it is such concentrations of metals that make an epithermal vein district world class. In the world-class silver- and gold-producing Comstock mining district, Nevada, several lines of evidence lead to the conclusion that the Comstock lode is localized in an extensional stepover between right-lateral fault <span class="hlt">zones</span>. This evidence includes fault geometries, kinematic indicators of slip, the hydraulic connectivity of faults as demonstrated by veins and <span class="hlt">dikes</span> along faults, and the opening of a normal-fault-bounded, asymmetric basin between two parallel and overlapping northwest-striking, lateral- to lateral-oblique-slip fault <span class="hlt">zones</span>. During basin opening, thick, generally subeconomic, banded quartz-adularia veins were deposited in the normal fault <span class="hlt">zone</span>, the Comstock fault, and along one of the bounding lateral fault <span class="hlt">zones</span>, the Silver City fault. As deformation continued, the <span class="hlt">intrusion</span> of <span class="hlt">dikes</span> and small plugs into the hanging wall of the Comstock fault <span class="hlt">zone</span> may have impeded the ability of the stepover to accommodate displacement on the bounding strike-slip faults through extension within the stepover. A transient period of transpressional deformation of the Comstock fault <span class="hlt">zone</span> ensued, and the early-stage veins were deformed through boudinaging and hydraulic fragmentation, fault-motion inversion, and high- and low-angle axial rotations of segments of the fault planes and some fault-bounded wedges. This deformation led to the formation of spatially restricted compartments of high vertical permeability and hydraulic connectivity and low lateral hydraulic connectivity. Bonanza orebodies were formed in the compartmentalized <span class="hlt">zones</span> of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035069','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035069"><span>Nonexplosive and explosive magma/wet-sediment interaction during emplacement of Eocene <span class="hlt">intrusions</span> into Cretaceous to Eocene strata, Trans-Pecos igneous province, West Texas</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Befus, K.S.; Hanson, R.E.; Miggins, D.P.; Breyer, J.A.; Busbey, A.B.</p> <p>2009-01-01</p> <p>Eocene <span class="hlt">intrusion</span> of alkaline basaltic to trachyandesitic magmas into unlithified, Upper Cretaceous (Maastrichtian) to Eocene fluvial strata in part of the Trans-Pecos igneous province in West Texas produced an array of features recording both nonexplosive and explosive magma/wet-sediment interaction. <span class="hlt">Intrusive</span> complexes with 40Ar/39Ar dates of ~ 47-46??Ma consist of coherent basalt, peperite, and disrupted sediment. Two of the complexes cutting Cretaceous strata contain masses of conglomerate derived from Eocene fluvial deposits that, at the onset of <span class="hlt">intrusive</span> activity, would have been > 400-500??m above the present level of exposure. These <span class="hlt">intrusive</span> complexes are inferred to be remnants of diatremes that fed maar volcanoes during an early stage of magmatism in this part of the Trans-Pecos province. Disrupted Cretaceous strata along diatreme margins record collapse of conduit walls during and after subsurface phreatomagmatic explosions. Eocene conglomerate slumped downward from higher levels during vent excavation. Coherent to pillowed basaltic <span class="hlt">intrusions</span> emplaced at the close of explosive activity formed peperite within the conglomerate, within disrupted Cretaceous strata in the conduit walls, and within inferred remnants of the phreatomagmatic slurry that filled the vents during explosive volcanism. A younger series of <span class="hlt">intrusions</span> with 40Ar/39Ar dates of ~ 42??Ma underwent nonexplosive interaction with Upper Cretaceous to Paleocene mud and sand. <span class="hlt">Dikes</span> and sills show fluidal, billowed, quenched margins against the host strata, recording development of surface instabilities between magma and groundwater-rich sediment. Accentuation of billowed margins resulted in propagation of <span class="hlt">intrusive</span> pillows into the adjacent sediment. More intense disruption and mingling of quenched magma with sediment locally produced fluidal and blocky peperite, but sufficient volumes of pore fluid were not heated rapidly enough to generate phreatomagmatic explosions. This work suggests that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000JMS....23..285K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000JMS....23..285K"><span>On the parameterization of interleaving and turbulent mixing using CTD data from the Azores Frontal <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuzmina, N. P.</p> <p>2000-01-01</p> <p>CTD-data obtained in the Azores Frontal <span class="hlt">Zone</span> using a towed undulating vehicle are analyzed to study the relationship between characteristics of <span class="hlt">intrusions</span> and mean parameters of the thermohaline field. A self-similar dependence between <span class="hlt">intrusion</span> intensity and hydrological parameters is obtained. The most well-founded interpretation of the empirical dependence is as follows: (a) the main source supporting <span class="hlt">intrusive</span> layering is the salt finger convection; (b) the abrupt decrease of <span class="hlt">intrusion</span> intensity with the reduction of geostrophic Richardson number obtained from the analysis is explained by the beginning of turbulence when salt fingers do not work any longer, so the "driving force" for <span class="hlt">intrusive</span> motion disappears. These results are consistent with the conclusions of the paper [Kuzmina N.P., Rodionov V.B., 1992. About the influence of baroclinicity upon generation of the thermohaline <span class="hlt">intrusions</span> in the oceanic frontal <span class="hlt">zones</span>. Izvestiya Akad. Nauk SSSR, Atmosperic and Oceanic Physics 28 (10-11), 1077-1086]. These conclusions imply that there are three main mechanisms of <span class="hlt">intrusive</span> layering at oceanic fronts, namely the 2D baroclinic instability of geostrophic flow, the vertical shear instability and the thermohaline instability where the driving source of <span class="hlt">intrusive</span> motion is double diffusive convection. The baroclinic and thermohaline instabilities can generate <span class="hlt">intrusions</span> of large vertical scale, while vertical shear instability usually gives rise to thin turbulent layers. Turbulence in these thin layers can prevent salt finger convection and thus destroy the energy source of the <span class="hlt">intrusive</span> motion conditioned by thermoclinicity. Therefore, the baroclinicity plays two parts in the processes of the <span class="hlt">intrusive</span> layering: (1) it prevents double-diffusion interleaving by means of turbulence, and (2) it generates <span class="hlt">intrusions</span> due to the 2D baroclinic instability of geostrophic current. Using features of thermohaline interleaving as a specific tracer of turbulent mixing, we have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014352','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014352"><span>FORTRAN 77 programs for conductive cooling of <span class="hlt">dikes</span> with temperature-dependent thermal properties and heat of crystallization</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Delaney, P.T.</p> <p>1988-01-01</p> <p>Temperature histories obtained from transient heat-conduction theory are applicable to most <span class="hlt">dikes</span> despite potential complicating effects related to magma flow during emplacement, groundwater circulation, and metamorphic reaction during cooling. Here. machine-independent FORTRAN 77 programs are presented to calculate temperatures in and around <span class="hlt">dikes</span> as they cool conductively. Analytical solutions can treat thermal-property contrasts between the <span class="hlt">dike</span> and host rocks, but cannot address the release of magmatic heat of crystallization after the early stages of cooling or the appreciable temperature dependence of thermal conductivity and diffusivity displayed by most rock types. Numerical solutions can incorporate these additional factors. The heat of crystallization can raise the initial temperature at the <span class="hlt">dike</span> contact, ??c1, about 100??C above that which would be estimated if it were neglected, and can decrease the rate at which the front of solidified magma moves to the <span class="hlt">dike</span> center by a factor of as much as three. Thermal conductivity and diffusivity of rocks increase with decreasing temperature and, at low temperatures, these properties increase more if the rocks are saturated with water. Models that treat these temperature dependencies yield estimates of ??c1 that are as much as 75??C beneath those which would be predicted if they were neglected. ?? 1988.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017946','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017946"><span>Thermal budget of the lower east rift <span class="hlt">zone</span>, Kilauea Volcano</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Delaney, Paul T.; Duffield, Wendell A.; Sass, John H.; Kauahikaua, James P.; ,</p> <p>1993-01-01</p> <p>The lower east rift <span class="hlt">zone</span> of Kilauea has been the site of repeated fissure eruptions fed by <span class="hlt">dikes</span> that traverse the depths of interest to geothermal explorations. We find that a hot-rock-and-magma system of low permeability extending along the rift <span class="hlt">zone</span> at depths below about 4 km and replenished with magma at a rate that is small in comparison to the modern eruption rate Kilauea can supply heat to an overlying hydrothermal aquifer sufficient to maintain temperatures of about 250??C if the characteristic permeability to 4-km depth is about 10-15m2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014Ocgy...54..557K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014Ocgy...54..557K"><span>Application of interleaving models for the description of <span class="hlt">intrusive</span> layering at the fronts of deep polar water in the Eurasian Basin (Arctic)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuzmina, N. P.; Zhurbas, N. V.; Emelianov, M. V.; Pyzhevich, M. L.</p> <p>2014-09-01</p> <p>Interleaving models of pure thermohaline and baroclinic frontal <span class="hlt">zones</span> are applied to describe <span class="hlt">intrusions</span> at the fronts found in the upper part of the Deep Polar Water (DPW) when the stratification was absolutely stable. It is assumed that differential mixing is the main mechanism of the <span class="hlt">intrusion</span> formation. Important parameters of the interleaving such as the growth rate, vertical scale, and slope of the most unstable modes relative to the horizontal plane are calculated. It was found that the interleaving model for a pure thermohaline front satisfactory describes the important <span class="hlt">intrusion</span> parameters observed at the frontal <span class="hlt">zone</span>. In the case of a baroclinic front, satisfactory agreement over all the interleaving parameters is observed between the model calculations and observations provided that the vertical momentum diffusivity significantly exceeds the corresponding coefficient of mass diffusivity. Under specific (reasonable) constraints of the vertical momentum diffusivity, the most unstable mode has a vertical scale approximately two-three times smaller than the vertical scale of the observed <span class="hlt">intrusions</span>. A thorough discussion of the results is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V11C..07H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V11C..07H"><span>Subduction-modified oceanic crust in the sources of continental picrite <span class="hlt">dikes</span> from the Karoo LIP?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heinonen, J. S.; Carlson, R. W.; Riley, T. R.; Luttinen, A. V.; Horan, M. F.</p> <p>2013-12-01</p> <p>The Ahlmannryggen mountain range in East Antarctica hosts unusual LILE-depleted, but Fe- and Ti-enriched ultramafic <span class="hlt">dikes</span> (Group 3) that belong to the Jurassic (~180 Ma) Karoo continental flood basalt (CFB) province. Their high initial ɛNd (+5 to +9) indicates their origin within the sublithospheric mantle beneath the Gondwana supercontinent. Using the new Pb and Os isotopic data and previously published geochemical and mineral chemical data, we try to constrain their mantle sources. The <span class="hlt">dikes</span> that lack evidence of crustal contamination exhibit very radiogenic ɛNd (+8.6 to +9.0), relatively radiogenic 206Pb/204Pb (18.2-18.4) and 87Sr/86Sr (0.7035-0.7037), and unradiogenic 187Os/188Os (0.124-0.125) at 180 Ma. These isotopic compositions are unlike those typical of MORBs, excluding depleted mantle as the sole source contributor. The Pb isotopic composition of the <span class="hlt">dikes</span> plots close to the 4.43 Ga geochron and hence is compatible with derivation from an early-depleted reservoir (EDR), recently suggested to be a major source component in CFBs. However, the high ɛNd of the <span class="hlt">dikes</span> exceeds the ɛNd estimated for EDR (+4.9 to +8.5 at 180 Ma) and the relative Nb, Fe, and Ti enrichment (pyroxenite fingerprint) of the <span class="hlt">dikes</span> is not readily ascribed to EDR source. Based on our isotopic and trace element modeling, we regard that the mantle source of the picrite <span class="hlt">dikes</span> contained seawater-altered and subduction-modified MORB with a recycling age of 0.8 Ga. Such a source component would explain the unusual combination of elevated initial 87Sr/86Sr, ɛNd, and 206Pb/204Pb, relative depletion in fluid-mobile LILE, U, Th, Pb, and LREE, and relative enrichment in Nb, Fe, Ti, and other HFSE. Behavior of Re and Os in subduction environments is not well constrained, but loss of Re from recycled MORB, as observed in some subduction-associated eclogites and blueschists, and predominant contribution of Os from depleted peridotite matrix could have produced the observed low 187Os/188Os</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999CoMP..137..115V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999CoMP..137..115V"><span>Metamorphic charnockite in contact aureoles around <span class="hlt">intrusive</span> enderbite from Natal, South Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van den Kerkhof, Alfons M.; Grantham, Geoffrey H.</p> <p></p> <p>In the Port Edward area of southern Kwa-Zulu Natal, South Africa, charnockitic aureoles up to 10m in width in the normally garnetiferous Nicholson's Point Granite, are developed adjacent to <span class="hlt">intrusive</span> contacts with the Port Edward Enderbite and anhydrous pegmatitic veins. Mineralogical differences between the country rock and charnockitic aureole suggest that the dehydration reaction Bt+Qtz-->Opx+Kfs+H2O and the reaction of Grt+Qtz-->Opx+Pl were responsible for the charnockitization. The compositions of fluid inclusions show systematic variation with: (1) the Port Edward Enderbite being dominated by CO2 and N2 fluid inclusions; (2) the non-charnockitized granite by saline aqueous inclusions with 18-23 EqWt% NaCl; (3) the charnockitic aureoles by low-salinity and pure water inclusions (<7 EqWt% NaCl); (4) the pegmatites by aqueous inclusions of various salinity with minor CO2. As a result of the thermal event the homogenization temperatures of the inclusions in charnockite show a much larger range (up to 390°C) compared to the fluid inclusions in granite (mostly <250°C). Contrary to fluid-controlled charnockitization (brines, CO2) which may have taken place along shear <span class="hlt">zones</span> away from the <span class="hlt">intrusive</span> body, the present ``proximal'' charnockitized granite formed directly at the contact with enderbite. The inclusions indicate contact metamorphism induced by the <span class="hlt">intrusion</span> of ``dry'' enderbitic magma into ``wet'' granite resulting in local dehydration. This was confirmed by cathodoluminescence microscopy showing textures indicative for the local reduction of structural water in the charnockite quartz. Two-pyroxene thermometry on the Port Edward Enderbite suggests <span class="hlt">intrusion</span> at temperatures of 1000-1050°C into country rock with temperature of <700°C. The temperature of aureole formation must have been between 700°C (breakdown of pyrite to form pyrrhotite) and 1000°C. Charnockitization was probably controlled largely by heat related to anhydrous <span class="hlt">intrusions</span> causing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/ust/petroleum-vapor-intrusion','PESTICIDES'); return false;" href="https://www.epa.gov/ust/petroleum-vapor-intrusion"><span>Petroleum Vapor <span class="hlt">Intrusion</span></span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>One type of vapor <span class="hlt">intrusion</span> is PVI, in which vapors from petroleum hydrocarbons such as gasoline, diesel, or jet fuel enter a building. <span class="hlt">Intrusion</span> of contaminant vapors into indoor spaces is of concern.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70004950','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70004950"><span>An evaluation of the relative quality of <span class="hlt">dike</span> pools for benthic macroinvertebrates in the Lower Missouri River, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Poulton, B.C.; Allert, A.L.</p> <p>2012-01-01</p> <p>A habitat-based aquatic macroinvertebrate study was initiated in the Lower Missouri River to evaluate relative quality and biological condition of <span class="hlt">dike</span> pool habitats. Water-quality and sediment-quality parameters and macroinvertebrate assemblage structure were measured from depositional substrates at 18 sites. Sediment porewater was analysed for ammonia, sulphide, pH and oxidation-reduction potential. Whole sediments were analysed for particle-size distribution, organic carbon and contaminants. Field water-quality parameters were measured at subsurface and at the sediment-water interface. Pool area adjacent and downstream from each <span class="hlt">dike</span> was estimated from aerial photography. Macroinvertebrate biotic condition scores were determined by integrating the following indicator response metrics: % of Ephemeroptera (mayflies), % of Oligochaeta worms, Shannon Diversity Index and total taxa richness. Regression models were developed for predicting macroinvertebrate scores based on individual water-quality and sediment-quality variables and a water/sediment-quality score that integrated all variables. Macroinvertebrate scores generated significant determination coefficients with <span class="hlt">dike</span> pool area (R2=0.56), oxidation–reduction potential (R2=0.81) and water/sediment-quality score (R2=0.71). Dissolved oxygen saturation, oxidation-reduction potential and total ammonia in sediment porewater were most important in explaining variation in macroinvertebrate scores. The best two-variable regression models included <span class="hlt">dike</span> pool size + the water/sediment-quality score (R2=0.84) and <span class="hlt">dike</span> pool size + oxidation-reduction potential (R2=0.93). Results indicate that <span class="hlt">dike</span> pool size and chemistry of sediments and overlying water can be used to evaluate <span class="hlt">dike</span> pool quality and identify environmental conditions necessary for optimizing diversity and productivity of important aquatic macroinvertebrates. A combination of these variables could be utilized for measuring the success of habitat enhancement</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22454568','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22454568"><span><span class="hlt">Intrusion</span>-aware alert validation algorithm for cooperative distributed <span class="hlt">intrusion</span> detection schemes of wireless sensor networks.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shaikh, Riaz Ahmed; Jameel, Hassan; d'Auriol, Brian J; Lee, Heejo; Lee, Sungyoung; Song, Young-Jae</p> <p>2009-01-01</p> <p>Existing anomaly and <span class="hlt">intrusion</span> detection schemes of wireless sensor networks have mainly focused on the detection of <span class="hlt">intrusions</span>. Once the <span class="hlt">intrusion</span> is detected, an alerts or claims will be generated. However, any unidentified malicious nodes in the network could send faulty anomaly and <span class="hlt">intrusion</span> claims about the legitimate nodes to the other nodes. Verifying the validity of such claims is a critical and challenging issue that is not considered in the existing cooperative-based distributed anomaly and <span class="hlt">intrusion</span> detection schemes of wireless sensor networks. In this paper, we propose a validation algorithm that addresses this problem. This algorithm utilizes the concept of <span class="hlt">intrusion</span>-aware reliability that helps to provide adequate reliability at a modest communication cost. In this paper, we also provide a security resiliency analysis of the proposed <span class="hlt">intrusion</span>-aware alert validation algorithm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MarGR..37..113G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MarGR..37..113G"><span>Identification of saline water <span class="hlt">intrusion</span> in part of Cauvery deltaic region, Tamil Nadu, Southern India: using GIS and VES methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gnanachandrasamy, G.; Ramkumar, T.; Venkatramanan, S.; Chung, S. Y.; Vasudevan, S.</p> <p>2016-06-01</p> <p>We use electrical resistivity data arrayed in a 2715 km2 region with 30 locations to identify the saline water <span class="hlt">intrusion</span> <span class="hlt">zone</span> in part of Cauvery deltaic region, offshore Eastern India. From this dataset we are able to derive information on groundwater quality, thickness of aquifer <span class="hlt">zone</span>, structural and stratigraphic conditions relevant to groundwater conditions, and permeability of aquifer systems. A total of 30 vertical electrode soundings (VES) were carried out by Schlumberger electrode arrangement to indicate complete lithology of this region using curve matching techniques. The electrical soundings exhibited that H and HK type curves were suitable for 16 shallow locations, and QH, KQ, K, KH, QQ, and HA curves were fit for other location. Low resistivity values suggested that saline water <span class="hlt">intrusion</span> occurred in this region. According to final GIS map, most of the region was severely affected by seawater <span class="hlt">intrusion</span> due to the use of over-exploitation of groundwater.The deteriorated groundwater resources in this coastal region should raise environmental and health concerns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70029745','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029745"><span>Duration of a large Mafic <span class="hlt">intrusion</span> and heat transfer in the lower crust: A SHRIMP U-Pb zircon Study in the Ivrea-Verbano <span class="hlt">Zone</span> (Western Alps, Italy)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Peressini, G.; Quick, J.E.; Sinigoi, S.; Hofmann, A.W.; Fanning, M.</p> <p>2007-01-01</p> <p>The Ivrea-Verbano <span class="hlt">Zone</span> in the western Italian Alps contains one of the world's classic examples of ponding of mantle-derived, mafic magma in the deep crust. Within it, a voluminous, composite mafic pluton, the Mafic Complex, intruded lower-crustal, high-grade paragneiss of the Kinzigite Formation during Permian-Carboniferous time, and is now exposed in cross-section as a result of Alpine uplift. The age of the <span class="hlt">intrusion</span> is still debated because the results of geochronological studies in the last three decades on different rock types and with various dating techniques range from 250 to about 300 Ma. Sensitive high-resolution ion microprobe (SHRIMP) U-Pb zircon age determinations on 12 samples from several locations within the Mafic Complex were performed to better constrain the age of the igneous event. The results indicate a long history of magma emplacement and cooling, which reconciles the spread in previously published ages. The main <span class="hlt">intrusive</span> phase took place at 288 ?? 4 Ma, causing a perturbation of the deep-crustal geotherm, which relaxed to the Sm-Nd closure temperature in garnet-free mafic rocks after about 15-20 Myr of sub-solidus cooling at c. 270 Ma. These results suggest that large, deep crustal plutons, such as those identified geophysically at depths of 10-20 km within extended continental crust (e.g. Yellowstone, Rio Grande Rift, Basin and Range) may have formed rapidly but induced a prolonged thermal perturbation. In addition, the data indicate that a significant thermal event affected the country rock of the Mafic Complex at about 310 Ma. The occurrence of an upper amphibolite- to granulite-facies thermal event in the Kinzigite Formation prior to the main <span class="hlt">intrusive</span> phase of the Mafic Complex has been postulated by several workers, and is corroborated by other geochronological investigations. However, it remains uncertain whether this event (1) was part of a prolonged perturbation of the deep-crustal geotherm, which started long before the onset of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.G44A..03S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.G44A..03S"><span>Deformation interplay at Hawaii Island</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shirzaei, M.; Walter, T. R.</p> <p>2009-12-01</p> <p>Volcanoes are known to be closely related to the tectonic environment, including vent locations and eruptions resulting from faults and earthquakes. Similarly, adjacent volcanoes interact with each other in time and space, as suggested for the Hawaiian volcanoes Kilauea and Mauna Loa. New satellite radar data imply even more complex deformation interplay in Hawaii than previously thought, involving magma chamber pressure changes, <span class="hlt">dike</span> <span class="hlt">intrusions</span>, slow earthquakes and ground subsidence. The affected regions are the Mauna Loa and Kilauea volcano summits, their active rift <span class="hlt">zones</span>, the island’s unstable southeast flank and even the capital city of Hilo. Based on the data acquired by the European satellite ENVISAT, we present in this work a five-year spatio-temporal analysis of the deformation signals recorded between 2003 and 2008. The data suggests that most of the deformation sources are acting in chorus. The magma <span class="hlt">intrusion</span> at the Mauna Loa chamber and the <span class="hlt">intrusion</span> into the Kilauea rift <span class="hlt">dike</span> are correlated in time while also interacting with gravity-driven flank movement events. Some of the events occur silently underneath the Kilauea south flank, such as slow earthquakes that may largely affect all of the active magmatic systems and reverse their sign of correlation. This study of the interplay between multiple deformations and inherently coupled systems provides a better understanding of Hawaiian volcano activity and may lead to new methods for assessing the hazards that arise during volcano-tectonic activities elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816082L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816082L"><span>Deformation history of Mauna Loa (Hawaii) from 2003 to 2014 through InSAR data: understanding the shorter-term processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>La Marra, Daniele; Poland, Michael P.; Acocella, Valerio; Battaglia, Maurizio; Miklius, Asta</p> <p>2016-04-01</p> <p>Geodesy allows detecting the deformation of volcanoes, thus understanding magmatic processes. This becomes particularly efficient when time series are available and volcanoes can be monitored on the mean-term (decades), and not only during a specific event. Here we exploit the SBAS technique, using SAR images from ENVISAT (descending and ascending orbits; 2003 - 2010) and COSMO-SkyMed (descending and ascending orbits; 2012 - 2014), to study a decade of deformation at Mauna Loa (Hawaii). These data are merged time series data from 24 continuously operating GPS stations, which allows us to calibrate the InSAR time series. Our results show a long-term inflation of the volcano from 2003 to 2014, reaching a peak of ~11 cm/yr on the summit area between mid-2004 to mid-2005 and then slowing down. Within this frame, we were able to identify five main periods with approximately linear deformation behavior. The inversion of the deformation data in the first four periods suggests the repeated, though not constant, <span class="hlt">intrusion</span> of one or more <span class="hlt">dikes</span> below the summit caldera and the upper Southwest Rift <span class="hlt">Zone</span>. Moreover, the <span class="hlt">dike</span> <span class="hlt">intrusion</span> coincides with minor acceleration of flank slip. Such a behavior is distinctive and, with the exception of the nearby Kilauea, has not been observed at any other volcano on the mean term. It is proposed that continuous, even though not constant flank instability of the SE flank may promote semi-continuous <span class="hlt">intrusions</span> in a volcano with a ready magma supply.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.P52A..01W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.P52A..01W"><span>Transfer Rates of Magma From Planetary Mantles to the Surface.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, L.; Head, J. W.; Parfitt, E. A.</p> <p>2008-12-01</p> <p>We discuss the speed at which magma can be transferred to a planetary surface from the deep interior. Current literature describes a combination of slow percolation of melt in the mantle where convection-driven pressure-release melting is occurring, concentration of melt by source region deformation, initiation and growth of magma-filled brittle fractures (<span class="hlt">dikes</span>) providing wider pathways for melt movement, additional growth and interconnection of <span class="hlt">dikes</span> with decreasing depth, rise of magma to storage <span class="hlt">zones</span> (reservoirs) located at levels of neutral buoyancy at the base of or within the crust, and transfer from the storage <span class="hlt">zones</span> in <span class="hlt">dikes</span> to feed eruptions or <span class="hlt">intrusions</span>. We do not take issue with these mechanisms but think that their relative importance in various circumstances is poorly appreciated. On Earth, preservation of diamonds in kimberlites implies very rapid (hours) transfer of melts from depths of 100-300 km, and there is strong geochemical evidence that magmas at mid-ocean ridges reach shallow depths faster than is possible by percolation alone. On the Moon, the petrology of pyroclasts involved in dark-mantle-forming eruptions implies rapid (again probably hours) magma transfer from depths of up to 400 km. The ureilite meteorites, samples of the mantle of a disrupted asteroid 200 km in diameter, have compositions only consistent with the rapid (months) extraction of mafic melt from the mantle. All of these examples imply that brittle fractures (<span class="hlt">dikes</span>) can sometimes be initiated at depths where mantle rheology would normally be expected to be plastic rather than elastic, and that melt can be fed into these <span class="hlt">dikes</span> extremely efficiently. Further evidence for this is provided by the giant radial <span class="hlt">dike</span> swarms observed on Earth, Mars and Venus. The <span class="hlt">dikes</span> observed (on Earth) and inferred from the presence of radiating graben systems (Mars) and radiating fracture and graben systems (Venus) are so voluminous that they can only be understood if they are fed from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3312426','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3312426"><span><span class="hlt">Intrusion</span>-Aware Alert Validation Algorithm for Cooperative Distributed <span class="hlt">Intrusion</span> Detection Schemes of Wireless Sensor Networks</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Shaikh, Riaz Ahmed; Jameel, Hassan; d’Auriol, Brian J.; Lee, Heejo; Lee, Sungyoung; Song, Young-Jae</p> <p>2009-01-01</p> <p>Existing anomaly and <span class="hlt">intrusion</span> detection schemes of wireless sensor networks have mainly focused on the detection of <span class="hlt">intrusions</span>. Once the <span class="hlt">intrusion</span> is detected, an alerts or claims will be generated. However, any unidentified malicious nodes in the network could send faulty anomaly and <span class="hlt">intrusion</span> claims about the legitimate nodes to the other nodes. Verifying the validity of such claims is a critical and challenging issue that is not considered in the existing cooperative-based distributed anomaly and <span class="hlt">intrusion</span> detection schemes of wireless sensor networks. In this paper, we propose a validation algorithm that addresses this problem. This algorithm utilizes the concept of <span class="hlt">intrusion</span>-aware reliability that helps to provide adequate reliability at a modest communication cost. In this paper, we also provide a security resiliency analysis of the proposed <span class="hlt">intrusion</span>-aware alert validation algorithm. PMID:22454568</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016764','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016764"><span>Geochemical consequences of flow differentiation in a multiple injection <span class="hlt">dike</span> (Trinity ophiolite, N. California)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brouxel, M.</p> <p>1991-01-01</p> <p>A clinopyroxene-rich <span class="hlt">dike</span> of the Trinity ophiolite sheeted-<span class="hlt">dike</span> complex shows three different magmatic pulses, probably injected in a short period of time (no well developed chilled margin) and important variations of the clinopyroxene and plagioclase percentages between its core (highly porphyritic) and margins (aphyric). This variation, interpreted as related to a flow differentiation phenomenon (mechanical phenocryst redistribution), has important geochemical consequences. It produces increases in the FeO, MgO, CaO, Cr and Ni contents from the margin to the core, together with increases in the clinopyroxene percentage, and decreases in the SiO2, Zr, Y, Nb and REE contents together with a decrease in the percentage of the fine-grained groundmass toward the core of the <span class="hlt">dike</span>. This mineralogical redistribution, which also affects the incompatible trace element ratios because of the difference in plagioclase and clinopyroxene mineral/liquid partition coefficients, illustrate the importance of fractionation processes outside of a magma chamber. ?? 1991.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1565a/pp_1565a.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1565a/pp_1565a.pdf"><span>Late Proterozoic diabase <span class="hlt">dikes</span> of the New Jersey Highlands; a remnant of Iapetan rifting in the north-central Appalachians</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Volkert, R.A.; Puffer, J.H.</p> <p>1995-01-01</p> <p>Diabase <span class="hlt">dikes</span> of widespread occurrence intrude only middle Proterozoic rocks in the New Jersey Highlands. These <span class="hlt">dikes</span> are enriched in TiO2, P2O5, Zr, and light rare earth elements, and have compositions that range from tholeiitic to alkalic. <span class="hlt">Dike</span> descriptions, field relations, petrography, geochemistry, petrogenesis, and tectonic setting are discussed. The data are consistent with emplacement in a rift-related, within-plate environment and suggest a correlation with other occurrences of late Proterozoic Appalachian basaltic magmatism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRB..118.3707H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRB..118.3707H"><span>New constraints on <span class="hlt">dike</span> injection and fault slip during the 1975-1984 Krafla rift crisis, NE Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hollingsworth, J.; Leprince, Sébastien; Ayoub, François; Avouac, Jean-Philippe</p> <p>2013-07-01</p> <p>Correlation of KH9 spy and SPOT5 satellite images, airphotos, digital elevation model differencing, electronic distance measurement, and leveling survey data is used to constrain the deformation resulting from the 1975-1984 Krafla rifting crisis. We find that <span class="hlt">diking</span> typically extends to depths of 5 km, while the <span class="hlt">dike</span> tops range from 0 km in the caldera region to 3 km at the northern end of the rift. Extension is accommodated by <span class="hlt">diking</span> at depth and normal faulting in the shallowest crust. In the southern section of the Krafla rift, surface opening is 80% of the <span class="hlt">dike</span> opening at depth. Over the 70-80 km length of the rift, the average <span class="hlt">dike</span> opening was 4.3-5.4 m. From these estimates, we calculate the total geodetic moment released over the Krafla rift crisis, 4.4-9.0×1019 Nm, which is an order of magnitude higher than the seismic moment released over the same time period, ~5.8×1018 Nm. The total volume of magma added to the upper crust was 1.1-2.1×109m3. This study highlights how optical image correlation using inexpensive declassified spy satellite and airphotos, combined with simple models of crustal deformation, can provide important constraints on the deformation resulting from past earthquake and volcanic events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29791686','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29791686"><span>Extruded upper first molar <span class="hlt">intrusion</span>: Comparison between unilateral and bilateral miniscrew anchorage.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sugii, Mari Miura; Barreto, Bruno de Castro Ferreira; Francisco Vieira-Júnior, Waldemir; Simone, Katia Regina Izola; Bacchi, Ataís; Caldas, Ricardo Armini</p> <p>2018-01-01</p> <p>The aim of his study was to evaluate the stress on tooth and alveolar bone caused by orthodontic <span class="hlt">intrusion</span> forces in a supraerupted upper molar, by using a three-dimensional Finite Element Method (FEM). A superior maxillary segment was modeled in the software SolidWorks 2010 (SolidWorks Corporation, Waltham, MA, USA) containing: cortical and cancellous bone, supraerupted first molar, periodontal tissue and orthodontic components. A finite element model has simulated <span class="hlt">intrusion</span> forces of 4N onto a tooth, directed to different mini-screw locations. Three different <span class="hlt">intrusion</span> mechanics vectors were simulated: anchoring on a buccal mini-implant; anchoring on a palatal mini-implant and the association of both anchorage systems. All analyses were performed considering the minimum principal stress and total deformation. Qualitative analyses exhibited stress distribution by color maps. Quantitative analysis was performed with a specific software for reading and solving numerical equations (ANSYS Workbench 14, Ansys, Canonsburg, Pennsylvania, USA). <span class="hlt">Intrusion</span> forces applied from both sides (buccal and palatal) resulted in a more homogeneous stress distribution; no high peak of stress was detected and it has allowed a vertical resultant movement. Buccal or palatal single-sided forces resulted in concentrated stress <span class="hlt">zones</span> with higher values and tooth tipping to respective force side. Unilateral forces promoted higher stress in root apex and higher dental tipping. The bilateral forces promoted better distribution without evidence of dental tipping. Bilateral <span class="hlt">intrusion</span> technique suggested lower probability of root apex resorption.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JSAES..37..266S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JSAES..37..266S"><span>Early post-collisional Brasiliano magmatism in Botuverá region, Santa Catarina, southern Brazil: Evidence from petrology, geochemistry, isotope geology and geochronology of the diabase and lamprophyre <span class="hlt">dikes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sacks de Campos, Roberto; Philipp, Ruy Paulo; Massonne, Hans-Joachim; Chemale, Farid</p> <p>2012-08-01</p> <p>The post-collisional magmatism related to Brasiliano orogeny represented the final stage of the Dom Feliciano Belt in Rio Grande do Sul and Santa Catarina states, southern Brazil, presenting high-K calc-alkaline to shoshonitic and alkaline chemical signatures. Magmatic episodes related to this early period were found in Botuverá region, Santa Catarina state, represented by diabase and lamprophyre (spessartite-type) <span class="hlt">dikes</span> <span class="hlt">intrusive</span> in metavolcano-sedimentary rocks of the Brusque Metamorphic Complex (CMB). These <span class="hlt">dikes</span> have massive structure and igneous textures ranging from very fine equigranular to porphyritic, and the latter is characterized by the presence of phenocrysts of plagioclase and hornblende. The <span class="hlt">dikes</span> have northeast direction and sharp contacts with the metamorphic rocks, indicating that its position was after the main orogenic regional metamorphism that affected the CMB, interpreted as of collisional nature. The diabase has a basic composition, whereas spessartite lamprophyres are intermediate, with geochemical affinities to the tholeiitic series, with a significant enrichment in light rare-earth elements (LREE) and large ion lithophile elements (LILE) such as Cs, Rb, Ba, K and Sr, and negative anomalies for high-field-strength elements (HFS) such as Nb, Ta, U and T. The concentration of standard trace elements and the Th/Yb and Ta/Yb ratios indicate that these magmas were derived from an enriched mantle source and were strongly contaminated by crust. Except for higher values of K, these features are similar to those found in basaltic volcanic rocks associated with the post-collisional period in south Brazil. The widely dispersed values of ɛND (618), ranging between -13.74 and +5.52, highlights the heterogeneity of the source and reinforces the importance of a crustal component in the generation of these rocks. The extremely low value of ɛNd (618), of -21.67 obtained for spessartite lamprophyres supports the importance of the involvement of crust in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930000949','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930000949"><span>Breccia <span class="hlt">dikes</span> from the Beaverhead Impact structure, southwest Montana</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fiske, P. S.; Hougen, S. B.; Hargraves, R. B.</p> <p>1992-01-01</p> <p>While shatter cones are generally accepted as indicators of meteorite impact, older petrologic features are not widely recognized in the geologic community. Breccia <span class="hlt">dikes</span> are one such feature. They are found in many large impact structures occurring over an area at least as extensively as shatter cones. Breccia <span class="hlt">dikes</span> will survive moderate degrees of metamorphism and tectonism, unlike many other microscopic features (shocked quartz grains, high-pressure polymorphs, etc.) and even large-scale features such as annular or bowl-shaped topographic features. Thus, they are important diagnostic criteria, especially for large, poorly preserved impact structures. The Beaverhead Impact structure is a recently discovered, deeply eroded impact structure in southwestern Montana. The remains of the structure are delineated by the occurrence of shatter cones, found in an area greater than 200 sq km, occurring within the Cabin thrust plate, part of the Cretaceous Sevier fold and thrust system. The distribution of shatter cones is further truncated by Tertiary normal faults. The present remains represent an allochthonous fragment of a larger structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V43A1118Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V43A1118Z"><span>Immiscibility of Fluid Phases at Magmatic-hydrothermal Transition: Formation of Various PGE-sulfide Mineralization for Layered Basic <span class="hlt">Intrusions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhitova, L.; Borisenko, A.; Morgunov, K.; Zhukova, I.</p> <p>2007-12-01</p> <p>Fluid inclusions in quartz of the Merensky Reef (Bushveld Complex, South Africa) and the Chineisky Pluton (Transbaikal Region, Russia) were studied using cryometry, microthermometry, Raman-spectroscopy, LA ICP- MS, scanning electronic microscopy, gas-chromatography and isotopic methods. This allowed us to document some examples of fluid phase separation resulting in formation of different types of PGE-sulfide mineralization for layered basic <span class="hlt">intrusions</span>. The results obtained show at least three generations of fluid separated from boiling residual alumosilicate intercumulus liquid of the Merensky Reef. The earliest fluid phase composed of homogenous high-dense methane and nitrogen gas mixture was identified in primary gas and co-existing anomalous fluid inclusions from symplectitic quartz. The next generation, heterophase fluid, composed of brines containing a free low-dense (mostly of carbon dioxide) gas phase, was observed in primary multiphase and coexisting gas-rich inclusions of miarolitic quartz crystals. The latest generation was also a heterophase fluid (low salinity water-salt solution and free low-dense methane gas phase) found in primary water-salt and syngenetic gas inclusions from peripheral <span class="hlt">zones</span> of miarolitic quartz crystals. For the Chineisky Pluton reduced endocontact magmatogene fluids changed to oxidized low salinity hydrothermal fluids in exocontact <span class="hlt">zone</span>. This resulted in formation of sulfide-PGE enrichment marginal <span class="hlt">zones</span> of <span class="hlt">intrusion</span>. The results obtained give us a possibility to suggest that: 1) Fluid phase separation is a typical feature of magmatogene fluids for layered basic <span class="hlt">intrusions</span>. 2) Reduced fluids can extract and transport substantial PGE and sulfide concentrations. 3) Oxidation of reduced fluids is one of the most important geochemical barriers causing abundant PGE minerals and sulfides precipitation. This in turn results in both formation of PGE reefs or enriched contact <span class="hlt">zones</span> of layered basic <span class="hlt">intrusions</span>. This work was supported by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..135a2009W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..135a2009W"><span>Study of Water Quality Changes due to Offshore <span class="hlt">Dike</span> Development Plan at Semarang Bay</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wibowo, M.; Hakim, B. A.</p> <p>2018-03-01</p> <p>Now, coast of Semarang Gulf is experiencing rapid growth because Semarang as a center economic growth in Central Java. On the other hand, coast of Gulf Semarang also experience a variety of very complex problems, such as tidal flood, land subsidence, as well as coastal damage due to erosion and sedimentation process. To overcome these problems BPPT and other institutions proposed construction of offshore <span class="hlt">dike</span>. Construction of the offshore <span class="hlt">dike</span> is a technology intervention to the marine environment that will certainly affect the hydrodynamic balance in coastal water including water quality in the Gulf of Semarang. Therefore, to determine changes in water quality that will happen is necessary to study the water quality modeling. The study was conducted by using a computational modeling software MIKE-21 Eco Lab Module from DHI. Based on this study result knowed that development offshore <span class="hlt">dike</span> will change water quality in the west and east dam that formed. In west dam the average value of the DO decline 81.56% - 93.32 % and the average value of BOD rise from 22.01 to 31.19% and in the east dam, there is an increase average value DO of 83.19% - 75.80%, while the average value of BOD decrease by 95,04% - 96.01%. To prevent the downward trend in water quality due to the construction of the offshore <span class="hlt">dike</span>, its necessary precautions at the upstream area before entering the Gulf of Semarang.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.721..395R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.721..395R"><span>Magnetic fabrics of the Cretaceous <span class="hlt">dike</span> swarms from São Paulo coastline (SE Brazil): Its relationship with South Atlantic Ocean opening</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raposo, M. Irene B.</p> <p>2017-11-01</p> <p>Magnetic fabric and rock magnetism studies were performed on 91 <span class="hlt">dikes</span> from Cretaceous diabase and lamprophyre <span class="hlt">dike</span> swarms that outcrop side by side on the beaches of NE São Paulo State coastline. The <span class="hlt">dikes</span> crosscut Archean and Proterozoic poly-metamorphic rocks of the Costeiro Complex. Their thicknesses range from a few centimeters to 2 m for lamprophyre and up to about 10 m for the diabase. They trend predominantly N30°-60°E with vertical dip. Magnetic fabrics were determined using anisotropy of low-field magnetic susceptibility (AMS) and anisotropy of anhysteretic remanent magnetization (AARM). Rock-magnetism measurements reveal that magnetite grains in the range of 2-5 μm are the magnetic mineral of both swarms. For most <span class="hlt">dikes</span>, these grains are the carriers of bulk magnetic susceptibility but, surprisingly, are not responsible for the AMS which is carried by Fe-bearing minerals as shown by AARM. The main AMS fabric recognized in the swarms is due to magma flow, in which the Kmax-Kint plane is parallel to the <span class="hlt">dike</span>'s plane, and the magnetic foliation pole (Kmin) is perpendicular to it. The analysis of the Kmax inclination showed that the <span class="hlt">dikes</span> were fed by horizontal to vertical flows. However, for the majority of the <span class="hlt">dikes</span> the AMS and AARM tensors are not coaxial. The AARM lineation (AARMmax) is oriented N30-60W, approximately perpendicular to AMS lineation (Kmax) suggesting that magnetite grains were rotated approximately 90° anticlockwise from the <span class="hlt">dike</span> plane. The AARMmax orientation is similar to the direction of a fault system mainly in the Santos marginal basin which was formed in the Cretaceous rifting during the South Atlantic opening. Therefore the AARM fabric is tectonic in origin, and the comparison of AMS and AARM fabrics suggests that lamprophyre and diabase <span class="hlt">dikes</span> were emplaced in three distinct events in the earliest stages of the South Atlantic opening.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://econgeol.geoscienceworld.org/cgi/content/abstract/106/3/451','USGSPUBS'); return false;" href="http://econgeol.geoscienceworld.org/cgi/content/abstract/106/3/451"><span>Petrogenesis of postcollisional magmatism at Scheelite Dome, Yukon, Canada: Evidence for a lithospheric mantle source for magmas associated with <span class="hlt">intrusion</span>-related gold systems</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mair, John L.; Farmer, G. Lang; Groves, David I.; Hart, Craig J.R.; Goldfarb, Richard J.</p> <p>2011-01-01</p> <p>The type examples for the class of deposits termed <span class="hlt">intrusion</span>-related gold systems occur in the Tombstone-Tungsten belt of Alaska and Yukon, on the eastern side of the Tintina gold province. In this part of the northern Cordillera, extensive mid-Cretaceous postcollisional plutonism took place following the accretion of exotic terranes to the continental margin. The most cratonward of the resulting plutonic belts comprises small isolated <span class="hlt">intrusive</span> centers, with compositionally diverse, dominantly potassic rocks, as exemplified at Scheelite Dome, located in central Yukon. Similar to other spatially and temporally related <span class="hlt">intrusive</span> centers, the Scheelite Dome <span class="hlt">intrusions</span> are genetically associated with <span class="hlt">intrusion</span>-related gold deposits. <span class="hlt">Intrusions</span> have exceptional variability, ranging from volumetrically dominant clinopyroxene-bearing monzogranites, to calc-alkaline minettes and spessartites, with an intervening range of intermediate to felsic stocks and <span class="hlt">dikes</span>, including leucominettes, quartz monzonites, quartz monzodiorites, and granodiorites. All rock types are potassic, are strongly enriched in LILEs and LREEs, and feature high LILE/HFSE ratios. Clinopyroxene is common to all rock types and ranges from salite in felsic rocks to high Mg augite and Cr-rich diopside in lamprophyres. Less common, calcic amphibole ranges from actinolitic hornblende to pargasite. The rocks have strongly radiogenic Sr (initial 87Sr/86Sr from 0.711-0.714) and Pb isotope ratios (206Pb/204Pb from 19.2-19.7), and negative initial εNd values (-8.06 to -11.26). Whole-rock major and trace element, radiogenic isotope, and mineralogical data suggest that the felsic to intermediate rocks were derived from mafic potassic magmas sourced from the lithospheric mantle via fractional crystallization and minor assimilation of metasedimentary crust. Mainly unmodified minettes and spessartites represent the most primitive and final phases emplaced. Metasomatic enrichments in the underlying lithospheric mantle</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024334','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024334"><span>Draped aeromagnetic survey in Transantarctic Mountains over the area of the Butcher Ridge igneous complex showing extent of underlying mafic <span class="hlt">intrusion</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Behrendt, John C.; Damaske, D.; Finn, C.A.; Kyle, P.; Wilson, T.J.</p> <p>2002-01-01</p> <p>A draped aeromagnetic survey over the area surrounding the Butcher Ridge igneous complex (BRIC), Transantarctic Mountains, was acquired in 1997-1998 as part of a larger Transantarctic Mountains Aerogeophysical Research Activity survey. The BRIC is a sill-like hypoabyssal <span class="hlt">intrusion</span> ranging in composition from tholeiitic basalt to rhyolite. An 40Ar/39 Ar age of 174 Ma and the chemical character of the basaltic rocks show the BRIC to be part of the widespread Jurassic Ferrar suite of continental tholeiitic rocks, that extends for 3500 km across Antarctica. The aeromagnetic survey shows a horseshoe-shaped pattern of anomalies reaching amplitudes as great as 1900 nT generally associated with the bedrock topography where it is exposed. It is apparent that the high-amplitude anomaly pattern is more extensive than the 10-km-long exposed outcrop, first crossed by a single 1990 aeromagnetic profile. The highest-amplitude anomalies appear south of the profile acquired in 1990 and extend out of the survey area. The new aeromagnetic data allow determination of the extent of the interpreted Butcher mafic(?) <span class="hlt">intrusion</span> beneath exposures of Beacon sedimentary rock and ice in the area covered, as well as beneath the small BRIC exposure. The magnetic anomalies show a minimum area of 3000 km2, a much greater extent than previously inferred. Magnetic models indicate a minimum thickness of ~1-2 km for a horizontal <span class="hlt">intrusion</span>. However, nonunique models with magnetic layers decreasing in apparent susceptibility with depth are consistent with of a 4- to 8-km-thick layered <span class="hlt">intrusion</span>. These magnetic models indicate progressively deeper erosion of the interpreted mafic-layered body from the south to north. The erosion has removed more magnetic upper layers that mask the magnetic effects of the lower less magnetic layers. The probable minimum volume of the <span class="hlt">intrusion</span> in the area of the survey is ~6000 km3. An alternate, but less likely, interpretation of a series of <span class="hlt">dikes</span> can also fit the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1011511','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1011511"><span>Seepage and Piping through Levees and <span class="hlt">Dikes</span> using 2D and 3D Modeling Codes</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-06-01</p> <p>by the Hydrologic Systems Branch of the Flood and Storm Protection Division (CEERD-HF), U.S. Army Engineer Research and Development Center, Coastal ...ER D C/ CH L TR -1 6- 6 Flood & Coastal Storm Damage Reduction Program Seepage and Piping through Levees and <span class="hlt">Dikes</span> Using 2D and 3D...Flood & Coastal Storm Damage Reduction Program ERDC/CHL TR-16-6 June 2016 Seepage and Piping through Levees and <span class="hlt">Dikes</span> Using 2D and 3D Modeling Codes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoOD..60..172S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoOD..60..172S"><span>Origin of Fe-Ti Oxide Mineralization in the Middle Paleoproterozoic Elet'ozero Syenite-Gabbro <span class="hlt">Intrusive</span> Complex (Northern Karelia, Russia)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharkov, E. V.; Chistyakov, A. V.; Shchiptsov, V. V.; Bogina, M. M.; Frolov, P. V.</p> <p>2018-03-01</p> <p>Magmatic oxide mineralization widely developed in syenite-gabbro <span class="hlt">intrusive</span> complexes is an important Fe and Ti resource. However, its origin is hotly debatable. Some researchers believe that the oxide ores were formed through precipitation of dense Ti-magnetite in an initial ferrogabbroic magma (Bai et al., 2012), whereas others consider them as a product of immiscible splitting of Fe-rich liquid during crystallization of Fe-Ti basaltic magma (Zhou et al., 2013). We consider this problem with a study of the Middle Paleoproterozoic (2086 ± 30 Ma) Elet'ozero Ti-bearing layered <span class="hlt">intrusive</span> complex in northern Karelia (Baltic Shield). The first ore-bearing phase of the complex is mainly made up of diverse ferrogabbros, with subordinate clinopyroxenites and peridotites. Fe-Ti oxides (magnetite, Ti-magnetite, and ilmenite) usually account for 10-15 vol %, reaching 30-70% in ore varieties. The second <span class="hlt">intrusive</span> phase is formed by alkaline and nepheline syenites. Petrographical, mineralogical, and geochemical data indicate that the first phase of the <span class="hlt">intrusion</span> was derived from a moderately alkaline Fe-Ti basaltic melt, while the parental melt of the second phase was close in composition to alkaline trachyte. The orebodies comprise disseminated and massive ores. The disseminated Fe-Ti oxide ores make up lenses and layers conformable to general layering. Massive ores occur in subordinate amounts as layers and lenses, as well as cross-cutting veins. Elevated Nb and Ta contents in Fe-Ti oxides makes it possible to consider them complex ores. It is shown that the Fe-Ti oxide mineralization is related to the formation of a residual (Fe,Ti)-rich liquid, which lasted for the entire solidification history of the first <span class="hlt">intrusive</span> phase. The liquid originated through multiple enrichment of Fe and Ti in the crystallization <span class="hlt">zone</span> of the <span class="hlt">intrusion</span> owing to the following processes: (1) precipitation of silicate minerals in the crystallization <span class="hlt">zone</span> with a corresponding increase in the Fe and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014MinDe..49..279Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014MinDe..49..279Z"><span>Sulfide mineralization associated with arc magmatism in the Qilian Block, western China: zircon U-Pb age and Sr-Nd-Os-S isotope constraints from the Yulonggou and Yaqu gabbroic <span class="hlt">intrusions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Zhao-Wei; Li, Wen-Yuan; Gao, Yong-Bao; Li, Chusi; Ripley, Edward M.; Kamo, Sandra</p> <p>2014-02-01</p> <p>The sulfide-bearing Yulonggou and Yaqu mafic <span class="hlt">intrusions</span> are located in the southern margin of the Qilian Block, Qinghai Province, western China. They are small <span class="hlt">dike</span>-like bodies mainly composed of gabbros and diorites. Disseminated sulfides (pyrrhotite, pentlandite, and chalcopyrite) are present as concordant lenses within the <span class="hlt">intrusions</span>. Precise CA-ID-TIMS zircon U-Pb dating yields the crystallization ages of 443.39 ± 0.42 and 440.74 ± 0.33 Ma for the Yulonggou and Yaqu <span class="hlt">intrusions</span>, respectively. Whole rock samples from both <span class="hlt">intrusions</span> show light rare earth element (REE) enrichments relative to heavy REE and pronounced negative Nb-Ta anomalies relative to Th and La, which are consistent with the products of arc basaltic magmatism. The Yulonggou <span class="hlt">intrusion</span> has negative ɛ Nd values from -5.7 to -7.7 and elevated (87Sr/86Sr) i ratios from 0.711 to 0.714. In contrast, the Yaqu <span class="hlt">intrusion</span> has higher ɛ Nd values from -4.1 to +8.4 and lower (87Sr/86Sr) i ratios from 0.705 to 0.710. The δ34S values of sulfide separates from the Yulonggou and Yaqu deposits vary from 0.8 to 2.4 ‰ and from 2 to 4.3 ‰, respectively. The γ Os values of sulfide separates from the Yulonggou and Yaqu deposits vary between 80 and 123 and between 963 and 1,191, respectively. Higher γ Os values coupled with higher δ34S values for the Yaqu deposit relative to the Yulonggou deposit indicate that external sulfur played a bigger role in sulfide mineralization in the Yaqu <span class="hlt">intrusion</span> than in the Yulonggou <span class="hlt">intrusion</span>. Mixing calculations using Sr-Nd isotope data show that contamination with siliceous crustal materials is more pronounced in the Yulonggou <span class="hlt">intrusion</span> (up to 20 wt%) than in the Yaqu <span class="hlt">intrusion</span> (<15 wt%). The distribution of sulfides in both <span class="hlt">intrusions</span> is consistent with multiple emplacements of sulfide-saturated magmas from depth. The Yulonggou and Yaqu sulfide deposits are not economically valuable under current market condition due to small sizes and low Ni grades, which can be explained</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V11A2508G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V11A2508G"><span>Zircon Messengers Reveal the Age and History of Great Basin Crust, Kern Mountains, Nevada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gottlieb, E. S.; Miller, E. L.; Wooden, J. L.</p> <p>2011-12-01</p> <p>Results of SHRIMP-RG analyses of complexly <span class="hlt">zoned</span> zircons from muscovite-bearing granitic rocks exposed in the Kerns Mountains of East-Central Nevada constrain the timing, duration, and loci of zircon growth within the interior of the U.S. Cordillera during Late Cretaceous through Eocene time. The Kern Mountains are an exhumed block of greenschist to amphibolite facies metamorphosed miogeoclinal rocks that were pervasively intruded by the Late Cretaceous Tungstonia granite pluton and the Eocene Skinner Canyon and Uvada plutons (Best et al., 1974). Euhedral zircons separated from a coarse-grained (2-3 cm) muscovite-bearing phase of the Tungstonia pluton exhibit complex cathodeluminescence (CL) zonation. Sub-angular to sub-rounded cores with highly variable CL are overgrown by oscillatory-<span class="hlt">zoned</span> zircon which in turn is rimmed by dark CL zircon (U>5000 ppm). A weighted mean Pb/U age of 70.2±0.9 Ma (n=20, MSWD=2.5) obtained from the oscillatory-<span class="hlt">zoned</span> zircon coincides with the end of Cretaceous peak metamorphism at shallow crustal levels. Pb/U ages from core <span class="hlt">zones</span> (n=18) predominantly are 0.9-1.4 Ga (n=11; 7 of which <15% discordant) or 2.4-2.7 Ga (n=5; 1 of which <15% discordant), consistent with ages of detrital zircons within the Late Proterozoic McCoy Creek Group exposed in adjacent ranges. A previously undated muscovite-bearing <span class="hlt">dike</span> in Skinner Canyon yielded a texturally complex population of subhedral zircon grains. CL imaging of these grains reveals fragmental, ghost-like cores surrounded by irregularly shaped overgrowth <span class="hlt">zones</span> with diffuse boundaries which are rimmed by oscillatory-<span class="hlt">zoned</span> zircon. Both oscillatory <span class="hlt">zoned</span> and gradational rim areas (n=32) yielded Late Cretaceous to Eocene ages. Twelve spots define the age of <span class="hlt">intrusion</span> at 41.7±0.3 Ma (MSWD=1.8), consistent with the local onset of Eocene magmatism. An older period of zircon growth from ~75-45 Ma, coincident with the proposed duration of the Laramide shallow slab, is defined by zircon with flat to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.S11A1136B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.S11A1136B"><span>To Plume or Not To Plume: SC Mesozoic Diabase <span class="hlt">Dike</span> Orientations, Stress Fields During the Break-up of Pangea, and the Feasibility of a Causal Plume.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beutel, E. K.; Alexander, M.; Kotecha, A.; Edwards, D.</p> <p>2002-12-01</p> <p>New compilations of Mesozoic diabase <span class="hlt">dikes</span> in South Carolina suggest that previously unrecognized N-S and NE-SW <span class="hlt">dike</span> orientations exist throughout the western Charlotte belt, into the Carolina belt and possible into the Laurens Thrust Stack. Previous studies indicated that the majority of <span class="hlt">dikes</span> in South Carolina were solely NW trending. While we found that the majority of <span class="hlt">dikes</span> did trend NW-SE, the number and size of the NE-SW and N-S trending <span class="hlt">dikes</span> indicate that these are not mere fingers off the main NW trending <span class="hlt">dikes</span> and are likely true swarms. Previous studies of Mesozoic diabase <span class="hlt">dikes</span> further north along the Atlantic coast have found evidence that suggests that NW-SE trending <span class="hlt">dikes</span> are the oldest set, the N-S trending set followed, and the NE-SW trending <span class="hlt">dikes</span> were injected last. Based on this relationship, and the stress field that most likely existed in the crust during the injection of each <span class="hlt">dike</span> set, we have constructed a series of evolutionary models for the break-up of Pangea. Our models are based on the assumption that the multiple overlapping swarms negate the possibility of a plume being solely responsible for the break-up or for the <span class="hlt">dikes</span>. These models suggest a complicated history of relative motion between Africa, North America, and South America. Finite element models were run to test the feasibility of these models. Preliminary model results suggest that the extensional stresses necessary for the major <span class="hlt">dike</span> patterns seen in northwestern Africa, northern South America, and the southeastern United States may have occurred when the relative motion of Africa was northeast of North America. Initial model runs suggest that multiple <span class="hlt">dike</span> orientations are best accounted for by a strongly nonlinear rift trend, a temporary aulacogen in Georgia, and/or rift propagation. The affect of events in the Gulf of Mexico is strongly dependent on the location and trend of the rifts and micro-continents modeled.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010fgcn.conf...11R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010fgcn.conf...11R"><span>An Efficient Method for Detecting Misbehaving <span class="hlt">Zone</span> Manager in MANET</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rafsanjani, Marjan Kuchaki; Pakzad, Farzaneh; Asadinia, Sanaz</p> <p></p> <p>In recent years, one of the wireless technologies increased tremendously is mobile ad hoc networks (MANETs) in which mobile nodes organize themselves without the help of any predefined infrastructure. MANETs are highly vulnerable to attack due to the open medium, dynamically changing network topology, cooperative algorithms, lack of centralized monitoring, management point and lack of a clear defense line. In this paper, we report our progress in developing <span class="hlt">intrusion</span> detection (ID) capabilities for MANET. In our proposed scheme, the network with distributed hierarchical architecture is partitioned into <span class="hlt">zones</span>, so that in each of them there is one <span class="hlt">zone</span> manager. The <span class="hlt">zone</span> manager is responsible for monitoring the cluster heads in its <span class="hlt">zone</span> and cluster heads are in charge of monitoring their members. However, the most important problem is how the trustworthiness of the <span class="hlt">zone</span> manager can be recognized. So, we propose a scheme in which "honest neighbors" of <span class="hlt">zone</span> manager specify the validation of their <span class="hlt">zone</span> manager. These honest neighbors prevent false accusations and also allow manager if it is wrongly misbehaving. However, if the manger repeats its misbehavior, then it will lose its management degree. Therefore, our scheme will be improved <span class="hlt">intrusion</span> detection and also provide a more reliable network.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMIN53D..02K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMIN53D..02K"><span>Architecture of near-surface magma transport in the Columbia River Flood Basalts as defined by a career's worth of feeder <span class="hlt">dike</span> mapping: The legacy dataset of William H. Taubeneck</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karlstrom, L.; Morriss, M. C.; Nasholds, M. W.</p> <p>2016-12-01</p> <p>The Miocene Columbia River Flood Basalts (CRFB) are the youngest, best preserved, and most thoroughly studied Large Igneous Province on Earth. The Grande Ronde basalts erupted 150,000 km3in less than 100 kyr ( 72% of the CRFB volume) from a network of feeder <span class="hlt">dikes</span>, the Chief Joseph <span class="hlt">dike</span> swarm, exposed in SE Washington, NE Oregon, and W Idaho, USA. William H. Taubeneck (1923-2016) spent several decades mapping CRFB <span class="hlt">dikes</span>. His extensive, meticulous field work defined the spatial extent and dominant trends in the Chief Joseph <span class="hlt">dike</span> swarm, providing a key constraint for theories of CRFB emplacement and their deep origin. However, these measurements were never published nor made public. We are revitalizing Taubeneck's maps, notebooks, and numerous unpublished geochemical analyses, synthesizing his work with other published and mapped <span class="hlt">dikes</span> and field checking select measurements to ensure accurate interpretation. This dataset should lead to increased understandings of the CRFB shallow plumbing system and flood basalt eruptive dynamics in general. Preliminary analysis of 4,410 mapped CRFB feeder <span class="hlt">dike</span> segments from Taubeneck and other workers reveals systematic trends in both <span class="hlt">dike</span> orientation and lithology of host rock. Average <span class="hlt">dike</span> orientation strikes to the north-northwest across 400 km. Orientations are generally parallel to the cratonic boundary, but appear generally unaffected by a major transition in craton position and also exhibit minor trends with near orthogonal orientations. <span class="hlt">Dike</span> spatial density peaks in Paleozoic to Cenozoic accreted terranes. Exposed <span class="hlt">dikes</span> are concentrated among Jurassic and Cretaceous plutons, which host 53% of mapped <span class="hlt">dikes</span> and accommodate the largest variability in <span class="hlt">dike</span> orientation. Preliminary investigations suggest variations of feeder <span class="hlt">dike</span> thickness with depth in the plumbing system as preserved through exposure in the uplifted Wallowa Mountains, although this is complicated by evidence for <span class="hlt">dikes</span> that accommodated multiple injections and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1899f0006Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1899f0006Z"><span>Mathematical investigation of tsunami-like long waves interaction with submerge <span class="hlt">dike</span> of different thickness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhiltsov, Konstantin; Kostyushin, Kirill; Kagenov, Anuar; Tyryshkin, Ilya</p> <p>2017-11-01</p> <p>This paper presents a mathematical investigation of the interaction of a long tsunami-type wave with a submerge <span class="hlt">dike</span>. The calculations were performed by using the freeware package OpenFOAM. Unsteady two-dimensional Navier-Stokes equations were used for mathematical modeling of incompressible two-phase medium. The Volume of Fluid (VOF) method is used to capture the free surface of a liquid. The effects caused by long wave of defined amplitude motion through a submerged <span class="hlt">dike</span> of varying thickness were discussed in detail. Numerical results show that after wave passing through the barrier, multiple vortex structures were formed behind. Intensity of vortex depended on the size of the barrier. The effectiveness of the submerge barrier was estimated by evaluating the wave reflection and transmission coefficients using the energy integral method. Then, the curves of the dependences of the reflection and transmission coefficients were obtained for the interaction of waves with the <span class="hlt">dike</span>. Finally, it was confirmed that the energy of the wave could be reduced by more than 50% when it passed through the barrier.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009BVol...71..881H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009BVol...71..881H"><span>Endogenous growth in channelized komatiite lava flows: evidence from spinifex-textured sills at Pyke Hill and Serpentine Mountain, Western Abitibi Greenstone Belt, Northeastern Ontario, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Houlé, Michel G.; Préfontaine, Sonia; Fowler, Anthony D.; Gibson, Harold L.</p> <p>2009-10-01</p> <p>Spinifex-textured sills (i.e., veins) characterized by komatiitic magmas that have intruded their own volcanic-piles have long been recognized. For instance, in the early 1970s, Pyke and coworkers, in their classic work at Pyke Hill in Munro Township, noted that not all spinifex-bearing ultramafic rocks formed as lava flows, rather some were clearly emplaced as small <span class="hlt">dikes</span> and sills. Several hypotheses have been proposed to explain spinifex-textured sills: <span class="hlt">intrusion</span> into a cold host, filter pressing, or drainage of residual liquid. However, these do not satisfactorily explain the phenomenon. Field and petrographic observations at Pyke Hill and Serpentine Mountain demonstrate that spinifex-bearing komatiite sills and <span class="hlt">dikes</span> were emplaced during channel inflation processes when new magma was intruded into a cooler, semi-consolidated but permeable cumulate material. Komatiitic liquids were intruded into the olivine cumulate rocks near the boundary between the spinifex and the cumulate <span class="hlt">zones</span> of well-organized to organized komatiite flows. Spinifex-textured sills are generally tabular in morphology, stacked one above another, with curviplanar contacts sub-parallel to stratigraphy. Some sills exhibit complex digitated apophyses. Thinner sills typically have a random olivine spinifex texture similar, though generally composed of coarser crystals, to that of komatiite lava flows. Thicker sills exhibit more complex organization of their constituent crystals characterized by <span class="hlt">zones</span> of random olivine spinifex, overlying <span class="hlt">zones</span> of organized coarse spinifex crystals similar to those found in lava flows. They have striking coarse dendritic spinifex <span class="hlt">zones</span> composed of very large olivine crystals, up to several centimetres long and up to 1 cm wide that are not observed in lava flows. Typically, at the sill margins, the cumulate material of the host flow is composed of euhedral to subhedral olivine crystals that are larger than those distal to the contact. Many of these margin</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T33D0760G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T33D0760G"><span>Geophysical Evidence for Magma <span class="hlt">Intrusion</span> across the Non-Transform Offset between the Famous and North Famous segments of The Mid-Atlantic Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Giusti, M.; Dziak, R. P.; Maia, M.; Perrot, J.; Sukhovich, A.</p> <p>2017-12-01</p> <p>In August of 2010 an unusually large earthquake sequence of >700 events occurred at the Famous and North Famous segments (36.5-37°N) of the Mid-Atlantic Ridge (MAR), recorded by an array of five hydrophones moored on the MAR flanks. The swarm extended spatially >70 km across the two segments. The non-transform offset (NTO) separating the two segements, which is thought to act as strucutural barrier, did not appear to impede or block the earthquake's spatial distribution. Broadband acoustic energy (1-30 Hz) was also observed and accompanied the onset of the swarm, lasting >20 hours. A total of 18 earthquakes from the swarm were detected teleseismically, four had Centroid-Moment Tensor (CMT) solutions derived. The CMT solutions indicated three normal faulting events, and one non-double couple (explosion) event. The spatio-temporal distribution of the seismicity and broadband energy show evidence of two magma <span class="hlt">dike</span> <span class="hlt">intrusions</span> at the North Famous segment, with one <span class="hlt">intrusion</span> crossing the NTO. This is the first evidence for an <span class="hlt">intrusion</span> event detected on the MAR south of the Azores since the 2001 Lucky Strike <span class="hlt">intrusion</span>. Gravimetric data were required to identify whether or not the Famous area is indeed comprised of two segments down to the level of the upper mantle. A high resolution gravity anomaly map of the two segments has been realized, based on a two-dimensional polygons model (Chapman, 1979) and will be compared to gravimetric data originated from SUDACORES experiment (1998, Atalante ship, IFREMER research team). Combined with the earthquake observations, this gravity anomaly map should provide a better understanding the geodynamic processes of this non-transform offset and of the deep magmatic system driving the August 2010 swarm.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014764','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014764"><span>Variation of depth to the brittle-ductile transition due to cooling of a midcrustal <span class="hlt">intrusion</span>.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gettings, M.E.</p> <p>1988-01-01</p> <p>The depth to the brittle-ductile transition in the crust is often defined by the intersection of a shear resistance relation in the brittle upper crust that increases linearly with depth and a power law relation for ductile flow in the lower crust that depends strongly on T. Transient variation of this depth caused by a magmatic <span class="hlt">intrusion</span> at a depth near the regional transition can be modelled by a heat conduction model for a rectangular parallelepiped superimposed on a linear geothermal gradient. When parameters appropriate for the southeastern US are used, a moderate-sized <span class="hlt">intrusion</span> is found to decrease the transition depth by as much as 7 km; significant variations last approx 10 m.y. Since the base of the seismogenic <span class="hlt">zone</span> is identified with the brittle-ductile transition, these results imply that <span class="hlt">intrusions</span> of late Tertiary age or younger could be important sources of clustered seismicity. -A.W.H.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT.......224P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT.......224P"><span>Kinematics of the Snake River Plain and Centennial Shear <span class="hlt">Zone</span>, Idaho, from GPS and earthquatte data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Payne, Suzette J.</p> <p></p> <p>New horizontal Global Positioning System (GPS) velocities at 405 sites using GPS phase data collected from 1994 to 2010 along with earthquakes, faults, and volcanic features reveal how contemporary strain is accommodated in the Northern Basin and Range Province. The 1994-2010 velocity field has observable gradients arising from both rotation and strain. Kinematic interpretations are guided by using a block-model approach and inverting velocities, earthquake slip vector azimuths, and <span class="hlt">dike</span>-opening rates to simultaneously solve for angular velocities of the blocks and uniform horizontal strain rate tensors within selected blocks. The Northern Basin and Range block model has thirteen blocks representing tectonic provinces based on knowledge of geology, seismicity, volcanism, active tectonic faults, and regions with differences in observed velocities. Ten variations of the thirteen blocks are tested to assess the statistical significance of boundaries for tectonic provinces, motions along those boundaries, and estimates of long-term deformation within the provinces. From these tests, a preferred model with seven tectonic provinces is determined by applying a maximum confidence level of ≥99% probability to F-distribution tests between two models to indicate one model with added boundaries has a better fit to the data over a second model. The preferred model is varied to test hypotheses of post-seismic viscoelastic relaxation, significance of <span class="hlt">dikes</span> in accommodating extension, and bookshelf faulting in accommodating shear. Six variations of the preferred model indicate time-varying components due to viscoelastic relaxation from the 1959 Hebgen Lake, Montana and 1983 Borah Peak, Idaho earthquakes have either ceased as of 2002 or are too small to be evident in the observed velocities. Inversions with <span class="hlt">dike</span>-opening models indicate that the previously hypothesized rapid extension by <span class="hlt">dike</span> <span class="hlt">intrusion</span> in volcanic rift <span class="hlt">zones</span> to keep pace with normal faulting is not currently</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMGP21A1132F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMGP21A1132F"><span>Geomagnetic Investigation of Sandstone <span class="hlt">Dikes</span> of the Colorado Front Range, for Determination of Age and Mode of Emplacement</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Freedman, D.; Petronis, M. S.; Siddoway, C. S.</p> <p>2012-12-01</p> <p>In the Colorado Front Range, an array of sandstone <span class="hlt">dikes</span> has intrigued geologists for over a century (Cross 1894,GSAB, 5, 525). Within their crystalline host, the <span class="hlt">dikes</span> reach widths >7m and have a lateral extent of 70km along the Ute Pass Fault (UPF). The essential questions of sediment source, emplacement mode, and age of the <span class="hlt">dikes</span> are unanswered. We present new paleomagnetic, rock magnetic, and anisotropy of magnetic susceptibility (AMS) results used to determine the age and emplacement behavior of the <span class="hlt">dikes</span>. The eleven <span class="hlt">dikes</span> selected for magnetic studies have sharp, planar margins, and share the systematic geometry of the NW striking subvertical <span class="hlt">dike</span> array. They exhibit little or no overprint by brittle fracturing/shear associated with the UPF. Our approach involved the use of paleomagnetic techniques to isolate the characteristic remanent magnetization (ChRM), which we used to limit the age of the <span class="hlt">dikes</span>' magnetization. Anisotropy of magnetic susceptibility (AMS),arising from alignment of detrital magnetite, serves as a proxy for the orientation of flow during <span class="hlt">dike</span> emplacement. U-Pb detrital zircon ages, obtained previously, did not provide a useful constraint on emplacement age because the dominant age matches that of the prevalent host,1.03Ga Pikes Peak Granite. IRM acquisition experiments were performed to identify the principal magnetic phases as a mixture of Fe-Ti oxide phases, likely to be low-Ti magnetite and hematite. The sandstone consists of sub-rounded to rounded sand-sized quartz, angular feldspar (<5%), and detrital magnetite; selected samples have uniform grain size and uniform color arising from hematite cement. Although direct cover relationships are not preserved, a portion of the study sites are proximal to in situ near-horizontal sedimentary cover rocks that offer evidence against large tectonic rotation. Cores were collected using a gas-powered drill with a diamond bit and oriented using a sun compass. Where possible, cores were obtained on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5435964-petrology-aztec-wash-pluton-eldorado-mountains-southern-nevada','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5435964-petrology-aztec-wash-pluton-eldorado-mountains-southern-nevada"><span>Petrology of Aztec Wash pluton, Eldorado Mountains, southern Nevada</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Falkner, C.M.; Miller, C.F.; Wooden, J.L.</p> <p>1993-04-01</p> <p>Aztec Wash pluton, a 50 km[sup 2] <span class="hlt">intrusive</span> complex in the northern Eldorado Mountains, was emplaced ca. 16 Ma (Faulds et al., 1990) during extension within the Colorado River Corridor. The pluton displays extreme compositional variability, ranging from olivine gabbro (ca. 50 wt% SiO[sub 2]) to highly evolved aplite (76% SiO[sub 2]). Most of the <span class="hlt">intrusion</span> is medium grained, homogeneous granite (ca. 72% SiO[sub 2]), but 1/3 is highly heterogeneous and dominated by mafic to intermediate rocks; a 6 [times] 3km, N-S mafic <span class="hlt">zone</span> almost bisects the pluton. Well-displayed magma mingling and late mafic and felsic <span class="hlt">dikes</span> verify the coexistencemore » of mafic and felsic melts. Hornblende barometry indicates that the entire exposed portion of Aztec Wash pluton was emplaced at very shallow depth (« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.487...74C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.487...74C"><span>Magnesium isotopic evidence for chemical disequilibrium among cumulus minerals in layered mafic <span class="hlt">intrusion</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Lie-Meng; Teng, Fang-Zhen; Song, Xie-Yan; Hu, Rui-Zhong; Yu, Song-Yue; Zhu, Dan; Kang, Jian</p> <p>2018-04-01</p> <p>Magnesium isotopic compositions of olivine, clinopyroxene, and ilmenite from the Baima <span class="hlt">intrusion</span>, SW China, for the first time, are investigated to constrain the magnitude and mechanisms of Mg isotope fractionation among cumulus minerals in layered mafic <span class="hlt">intrusions</span> and to evaluate their geological implications. Olivine and clinopyroxene have limited Mg isotope variations, with δ26Mg ranging from -0.33 to +0.05‰ and from -0.29 to -0.13‰, respectively, similar to those of mantle xenolithic peridotites. By contrast, ilmenites display extremely large Mg isotopic variation, with δ26Mg ranging from -0.50 to +1.90‰. The large inter-mineral fractionations of Mg isotopes between ilmenite and silicates may reflect both equilibrium and kinetic processes. A few ilmenites have lighter Mg isotopic compositions than coexisting silicates and contain high MgO contents without compositional <span class="hlt">zoning</span>, indicating equilibrium fractionation. The implication is that the light Mg isotopic compositions of lunar high-Ti basalts may result from an isotopically light source enriched in cumulate ilmenites. On the other hand, most ilmenites have heavy Mg isotopic compositions, coupled with high MgO concentration and chemical <span class="hlt">zoning</span>, which can be quantitatively modeled by kinetic Mg isotope fractionations induced by subsolidus Mg-Fe exchange between ilmenite and ferromagnesian silicates during the cooling of the Baima <span class="hlt">intrusion</span>. The extensive occurrence of kinetic Mg isotope fractionation in ilmenites implies the possibility of widespread compositional disequilibrium among igneous minerals in magma chambers. Consequently, disequilibrium effects need to be considered in studies of basaltic magma evolution, magma chamber processes, and magmatic Fe-Ti oxide ore genesis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1110159F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1110159F"><span>Dynamics of the Axial Melt Lens/<span class="hlt">Dike</span> transition at fast spreading ridges: assimilation and hydrous partial melting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>France, L.; Ildefonse, B.; Koepke, J.</p> <p>2009-04-01</p> <p>Recent detailed field studies performed in the Oman ophiolite on the gabbro/sheeted <span class="hlt">dike</span> transition, compared to corresponding rocks from the EPR drilled by IODP (Site 1256), constrain a general model for the dynamics of the axial melt lens (AML) present at fast spreading ridges (France et al., 2008). This model implies that the AML/<span class="hlt">dike</span> transition is a dynamic interface migrating up- and downward, and that the isotropic gabbro horizon on top of the igneous section represents its fossilization. It is also proposed that upward migrations are associated to reheating of the base of the sheeted <span class="hlt">dike</span> complex and to assimilation processes. Plagiogranitic lithologies are observed close to the truncated base of the <span class="hlt">dikes</span> and are interpreted to represent frozen melts generated by partial melting of previously hydrothermalized sheeted <span class="hlt">dikes</span>. Relicts of previously hydrothermalized lithologies are also observed in the fossil melt lens, and are associated to lithologies that have crystallized under high water activities, with clinopyroxene crystallizing before plagioclase, and An-rich plagioclase. To better understand our field data, we performed hydrous partial melting experiments at shallow pressures (0.1 GPa) under slightly oxidizing conditions (NNO oxygen buffer) and water saturated conditions on hydrothermalized sheeted <span class="hlt">dike</span> sample from the Oman ophiolite. These experiments have been performed between 850°C and 1030°C; two additional experiments in the subsolidus regime were also conducted (750°C and 800°C). Clinopyroxenes formed during incongruent melting at low temperature (<910°C) have compositions that match those from the corresponding natural rocks (reheated base of the sheeted <span class="hlt">dike</span> and relicts of assimilated lithologies). In particular, the characteristic low TiO2 and Al2O3 contents are reproduced. The experimental melts produced at low temperatures correspond to compositions of typical natural plagiogranites. In natural settings, these silicic liquids would be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MinDe.tmp....3R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MinDe.tmp....3R"><span>A genetic link between magnetite mineralization and diorite <span class="hlt">intrusion</span> at the El Romeral iron oxide-apatite deposit, northern Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rojas, Paula A.; Barra, Fernando; Reich, Martin; Deditius, Artur; Simon, Adam; Uribe, Francisco; Romero, Rurik; Rojo, Mario</p> <p>2018-01-01</p> <p>El Romeral is one of the largest iron oxide-apatite (IOA) deposits in the Coastal Cordillera of northern Chile. The Cerro Principal magnetite ore body at El Romeral comprises massive magnetite intergrown with actinolite, with minor apatite, scapolite, and sulfides (pyrite ± chalcopyrite). Several generations of magnetite were identified by using a combination of optical and electron microscopy techniques. The main mineralization event is represented by <span class="hlt">zoned</span> magnetite grains with inclusion-rich cores and inclusion-poor rims, which form the massive magnetite ore body. This main magnetite stage was followed by two late hydrothermal events that are represented by magnetite veinlets that crosscut the massive ore body and by disseminated magnetite in the andesite host rock and in the Romeral diorite. The sulfur stable isotope signature of the late hydrothermal sulfides indicates a magmatic origin for sulfur (δ34S between - 0.8 and 2.9‰), in agreement with previous δ34S data reported for other Chilean IOA and iron oxide-copper-gold deposits. New 40Ar/39Ar dating of actinolite associated with the main magnetite ore stage yielded ages of ca. 128 Ma, concordant within error with a U-Pb zircon age for the Romeral diorite (129.0 ± 0.9 Ma; mean square weighted deviation = 1.9, n = 28). The late hydrothermal magnetite-biotite mineralization is constrained at ca. 118 Ma by 40Ar/39Ar dating of secondary biotite. This potassic alteration is about 10 Ma younger than the main mineralization episode, and it may be related to post-mineralization <span class="hlt">dikes</span> that crosscut and remobilize Fe from the main magnetite ore body. These data reveal a clear genetic association between magnetite ore formation, sulfide mineralization, and the diorite <span class="hlt">intrusion</span> at El Romeral (at 129 Ma), followed by a late and more restricted stage of hydrothermal alteration associated with the emplacement of post-ore <span class="hlt">dikes</span> at ca. 118 Ma. Therefore, this new evidence supports a magmatic-hydrothermal model for the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009mlct.book..133S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009mlct.book..133S"><span>Efficient Mining and Detection of Sequential <span class="hlt">Intrusion</span> Patterns for Network <span class="hlt">Intrusion</span> Detection Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shyu, Mei-Ling; Huang, Zifang; Luo, Hongli</p> <p></p> <p>In recent years, pervasive computing infrastructures have greatly improved the interaction between human and system. As we put more reliance on these computing infrastructures, we also face threats of network <span class="hlt">intrusion</span> and/or any new forms of undesirable IT-based activities. Hence, network security has become an extremely important issue, which is closely connected with homeland security, business transactions, and people's daily life. Accurate and efficient <span class="hlt">intrusion</span> detection technologies are required to safeguard the network systems and the critical information transmitted in the network systems. In this chapter, a novel network <span class="hlt">intrusion</span> detection framework for mining and detecting sequential <span class="hlt">intrusion</span> patterns is proposed. The proposed framework consists of a Collateral Representative Subspace Projection Modeling (C-RSPM) component for supervised classification, and an inter-transactional association rule mining method based on Layer Divided Modeling (LDM) for temporal pattern analysis. Experiments on the KDD99 data set and the traffic data set generated by a private LAN testbed show promising results with high detection rates, low processing time, and low false alarm rates in mining and detecting sequential <span class="hlt">intrusion</span> detections.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T51E2945T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T51E2945T"><span>3D Numerical Models of the Effect of <span class="hlt">Diking</span> on the Faulting Pattern at Incipient Continental Rifts and Steady-State Spreading Centers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tian, X.; Choi, E.; Buck, W. R.</p> <p>2015-12-01</p> <p>The offset of faults and related topographic relief varies hugely at both continental rifts and mid-ocean ridges (MORs). In some areas fault offset is measured in 10s of meters while in places marked by core complexes it is measured in 10s of kilometers. Variation in the magma supply is thought to control much of these differences. Magma supply is most usefully described by the ratio (M) between rates of lithospheric extension accommodated by magmatic <span class="hlt">dike</span> <span class="hlt">intrusion</span> and that occurring via faulting. 2D models with different values of M successfully explain much of the observed cross-sectional structure seen at rifts and ridges. However, magma supply varies along the axis of extension and the interactions between the tectonics and magmatism are inevitably three-dimensional. We investigate the consequences of this along-axis variation in <span class="hlt">diking</span> in terms of faulting patterns and the associated structures using a 3D parallel geodynamic modeling code, SNAC. Many observed 3D structural features are reproduced: e.g., abyssal hill, oceanic core complex (OCC), inward fault jump, mass wasting, hourglass-shaped median valley, corrugation and mullion structure. An estimated average value of M = 0.65 is suggested as a boundary value for separating abyssal hills and OCCs formation. Previous inconsistency in the M range for OCC formation between 2D model results (M = 0.3˜0.5) and field observations (M < 0.3 or M > 0.5) is reconciled by the along-ridge coupling between different faulting regimes. We also propose asynchronous faulting-induced tensile failure as a new possibility for explaining corrugations seen on the surface of core complexes. For continental rifts, we will describe a suite of 2D and 3D model calculations with a range of initial lithospheric structures and values of M. In one set of the 2D models we limit the extensional tectonic force and show how this affects the maximum topographic relief produced across the rift. We are also interested in comparing models in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JGRB..113.4202H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JGRB..113.4202H"><span>Kinematic analysis of fractures in the Great Rift, Idaho: Implications for subsurface <span class="hlt">dike</span> geometry, crustal extension, and magma dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holmes, Adrian A. J.; Rodgers, David W.; Hughes, Scott S.</p> <p>2008-04-01</p> <p>Extension across the southern Great Rift of the Eastern Snake River Plain (ESRP), Idaho, was measured to calculate the dimensions of underlying <span class="hlt">dikes</span> and interpret magmatic and extensional processes. Cumulative rift-perpendicular extension ranges from 0.64 to 4.50 m along the 14 km long Kings Bowl segment, from 1.33 to 4.41 m along the 14 km long New Butte segment, and from 0.74 to 1.57 m along the 4 km long Minidoka segment. Along strike of each segment, extension increases toward coeval vents. Each rift segment is interpreted to be underlain by a subsurface <span class="hlt">dike</span>, whose dimensions are calculated using buoyancy equilibrium and boundary element models. <span class="hlt">Dikes</span> are calculated to have tops that are 950-530 m deep, bottoms that are 23-31 km deep, and widths that taper to zero from a maximum of 2-21 m. Modeling suggests that the Kings Bowl <span class="hlt">dike</span> has a maximum probable width of ˜8 m and a volume of ˜2 km3, about 400 times the volume of its coeval lava flow. <span class="hlt">Dike</span> widths and ages at the southern Great Rift provide evidence for a Holocene ESRP strain rate of about 1 to 3 × 10-16 s-1, which is as much as an order of magnitude slower than strain rates in the adjacent, seismically active Basin and Range province. Eruptive fissures are present where rift width is <1650 m. This corresponds to a depth to <span class="hlt">dike</span> top of <700 m, which we propose was the depth where vesiculation initiated, thus increasing magma pressure and inducing eruption.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..941J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..941J"><span>Comparison of magmatic and amagmatic rift <span class="hlt">zone</span> kinematics using full moment tensor inversions of regional earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jaye Oliva, Sarah; Ebinger, Cynthia; Shillington, Donna; Albaric, Julie; Deschamps, Anne; Keir, Derek; Drooff, Connor</p> <p>2017-04-01</p> <p>Temporary seismic networks deployed in the magmatic Eastern rift and the mostly amagmatic Western rift in East Africa present the opportunity to compare the depth distribution of strain, and fault kinematics in light of rift age and the presence or absence of surface magmatism. The largest events in local earthquake catalogs (ML > 3.5) are modeled using the Dreger and Ford full moment tensor algorithm (Dreger, 2003; Minson & Dreger, 2008) to better constrain source depth and to investigate non-double-couple components. A bandpass filter of 0.02 to 0.10 Hz is applied to the waveforms prior to inversion. Synthetics are based on 1D velocity models derived during seismic analysis and constrained by reflection and tomographic data where available. Results show significant compensated linear vector dipole (CLVD) and isotropic components for earthquakes in magmatic rift <span class="hlt">zones</span>, whereas double-couple mechanisms predominate in weakly magmatic rift sectors. We interpret the isotropic components as evidence for fluid-involved faulting in the Eastern rift where volatile emissions are large, and <span class="hlt">dike</span> <span class="hlt">intrusions</span> well documented. Lower crustal earthquakes are found in both amagmatic and magmatic sectors. These results are discussed in the context of the growing database of complementary geophysical, geochemical, and geological studies in these regions as we seek to understand the role of magmatism and faulting in accommodating strain during early continental rifting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MsT.........35D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MsT.........35D"><span>Geophysical Characterization of a Rare Earth Element Enriched Carbonatite Terrane at Mountain Pass, California Eastern Mojave Desert</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Denton, Kevin M.</p> <p></p> <p>Mountain Pass, California, located in the eastern Mojave Desert, hosts one of the world's richest rare earth element (REE) deposits. The REE-rich rocks occur in a 2.5 km- wide, north-northwest trending <span class="hlt">zone</span> of Mesoproterozoic (1.4-1.42 Ga) stocks and <span class="hlt">dikes</span>, which intrude a larger Paleoproterozoic (1.7 Ga) schist-gneiss terrane that extends 10 km southward from Clark Mountain to the Mescal Range. Several REE-enriched bodies make up the Mountain Pass <span class="hlt">intrusive</span> suite including shonkinite, syenite, and granite comprising an ultrapotassic <span class="hlt">intrusive</span> suite and the Sulphide Queen carbonatite body. Two-dimensional modeling of gravity, magnetic, and electrical resistivity data reveals that the Mountain Pass <span class="hlt">intrusive</span> suite is associated with a local gravity high that is superimposed on a 4-km wide gravity terrace. Rock property data indicate that the Mountain Pass <span class="hlt">intrusive</span> suite is unusually nonmagnetic at the surface (2.0 x 10-3 SI, n = 67). However, aeromagnetic data indicate that these rocks occur along the eastern edge of a prominent north-northwest trending aeromagnetic high of unknown origin. The source of this unknown magnetic anomaly is 2-3 km below the surface and coincides with a body of rock having high electrical conductivity. Electrical resistivity models indicate that this unknown magnetic anomaly is several orders of magnitude more conductive (103 O•m) than the surrounding rock. Combined geophysical data suggest that the carbonatite and its associated ultrapotassic <span class="hlt">intrusive</span> suite were preferentially emplaced along a northwest <span class="hlt">zone</span> of weakness and/or a fault.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V31A2311Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V31A2311Z"><span>Evolution Of An Upper Crustal Plutonic-Volcanic Plumbing System:Insights From High Precision U-Pb Zircon Geochronology Of Intracaldera Tuff And <span class="hlt">Intrusions</span> In Silver Creek Caldera, Arizona, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, T.; Mundil, R.; Miller, C. F.; Miller, J. S.; Paterson, S. R.</p> <p>2010-12-01</p> <p>Study of both plutonic and volcanic regimes in one single magmatic system is a powerful approach towards obtaining a more complete view of the long-term evolution of magma systems. The recently discovered Silver Creek caldera is the source of the voluminous Peach Spring Tuff (PST) (Ferguson, 2008) and presents a unique opportunity to study a field laboratory of a linked plutonic-volcanic system. This relict west-facing half caldera is predominantly filled with trachytic intracaldera tuff with the caldera margin intruded by several petrologically distinct hypabyssal <span class="hlt">intrusions</span>. These include porphyritic granite with granophyric texture, felsic leucogranite, porphyritic monzonite exposed on NE side of the caldera that is <span class="hlt">zoned</span> from more felsic to more mafic, and quartz-phyric <span class="hlt">dikes</span> that intrude the caldera fill. We present preliminary single zircon ages from 4 samples that have been analyzed using the CA-TIMS method after thermal annealing and chemical leaching (Mattinson 2005), including 1 sample from intracaldera tuff and 3 samples from caldera-related <span class="hlt">intrusions</span>. 3-D total U/Pb isochron ages from all four samples fall within a range of 18.32-18.90 Ma with uncertainties between 0.09 and 0.39 Ma, although some of them lack precision and are compromised by elevated common Pb. For example, zircon from the dated porphyritic monzonite yields an age of 18.32±0.42 Ma (MSWD=2.7) where the excess scatter may result from real age dispersion and/or different compositions of the common Pb contribution. The PST had been dated to ~18.5 Ma by 40Ar/39Ar techniques (Nielson et al., 1990). In order to be compared to U/Pb ages the 40Ar/39Ar age must be adjusted for a revised age for the then used flux monitor (MMbh-1) and corrected for the now quantified systematic bias between 40Ar/39Ar and U/Pb ages (Renne et al., 2010), which results in a corrected age of 18.8 Ma. Thus, the ages for our samples match that of the PST within error. Based on current results, the age difference</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019327','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019327"><span>The role of diffusion-controlled oscillatory nucleation in the formation of line rock in pegmatite-aplite <span class="hlt">dikes</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Webber, K.L.; Falster, A.U.; Simmons, W.B.; Foord, E.E.</p> <p>1997-01-01</p> <p>The George Ashley Block (GAB), located in the Pala Pegmatite District, San Diego County, California, is a composite pegmatite-aplite <span class="hlt">dike</span> of 8 m thickness displaying striking mineralogical layering in the aphte portion of the <span class="hlt">dike</span>, referred to as line rock. Rhythmic layering is characterized by garnet-rich bands alternating with albite-quartz-muscovite-rich bands. Cumulus textures are notably absent from the layered portion of the <span class="hlt">dike</span>. Elongated quartz, megacrysts are oriented perpendicular to the garnet-rich layers and poikilitically include garnet, albite, and muscovite. Calculated crystal-free magma viscosity with 3% H2O is 106.2 Pa s and the calculated settling velocity for garnet is 0??51 cm/year. Conductive cooling calculations based on emplacement of a 650??C <span class="hlt">dike</span> into 150?? C fractured gabbroic country rock at 1??5 kbar, and accounting for latent heat of crystallization, demonstrate that the line rock portion of the <span class="hlt">dike</span> cools to 550?? C in about 1 year. Crystal size distribution studies also suggest very rapid nucleation and crystallization. Diffusion-controlled gel crystallization experiments yield textures virtually identical to those observed in the layered aplite, including rhythmic banding, colloform layering, and band discontinuities. Thus, observed textures and calculated magmatic parameters suggest that mineralogical layering in the GAB results from an in situ diffusion-controlled process of oscillatory nucleation and crystallization. We propose that any event that promotes strong undercooling has the potential to initiate rapid heterogeneous nucleation and oscillatory crystal growth, leading to the development of a layer of excluded components in front of the crystallization front, and the formation of line rock.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3404S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3404S"><span>Modeling saltwater <span class="hlt">intrusion</span> in highly heterogeneous coastal aquifers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Safi, Amir; El-Fadel, Mutasem; Doummar, Joanna; Abou Najm, Majdi; Alameddine, Ibrahim</p> <p>2016-04-01</p> <p>In this study, a 3D variable-density flow and solute transport model SEAWAT was used to examine the impact of macroscopic variation in a soil matrix on widening or narrowing the thickness of the saltwater-freshwater mixing <span class="hlt">zone</span>. Located along the Eastern Mediterranean (Beirut), the pilot aquifer consists of karstified limestone of Cretaceous age overlain by Upper Tertiary and Quaternary unconsolidated deposits. The model used the advanced pilot-points parameterization coupled with PEST to characterize spatial heterogeneity. Historically simulated water levels were relied upon to reduce potential numerical instabilities induced by insensitive parameters in transient calibration. The latter demonstrated a high degree of heterogeneity in the middle parts of the aquifer and along western coastlines with specification of a high hydraulic conductivity and low storativity in fault networks. The response of the aquifer to seasonal stresses such as climate cycles, pumping rates and recharge rates was manifested as high fluctuations in potentiometric surface due to potential fast flow pathways along faults. The final distribution of saltwater <span class="hlt">intrusion</span> supports two mechanisms 1) lateral encroachment of recent seawater into the western <span class="hlt">zone</span> of the aquifer which is of most concern due to high horizontal hydraulic conductivity in the wave direction and 2) upconing in the northwest and southwest of the aquifer due to large vertical hydraulic conductivities that tend to exacerbate the vertical movement of salinity. Acknowledgments This study is part of a program on climate change and seawater <span class="hlt">intrusion</span> along the Eastern Mediterranean funded by the International Development Research Center (IDRC) of Canada at the American University of Beirut (AUB). Special thanks are extended to Dr. Charlotte Macalister at IDRC for her support and feedback in implementing this program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.7715J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.7715J"><span>InSAR Observations of the 2009 Harrat Lunayyir (western Saudi Arabia) Dyke <span class="hlt">Intrusion</span> and Post-<span class="hlt">Diking</span> Deformation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jónsson, Sigurjón; Lu, Zhong; Lundgren, Paul</p> <p>2010-05-01</p> <p>Interferometric Satellite Radar (InSAR) observations of one of the volcanic provinces in western Saudi Arabia, Harrat Lunayyir (also known as Harrat Al-Shaqah), provide rich information about the geometry and evolution of a dyke <span class="hlt">intrusion</span> and surface faulting that occurred in the region in April-July 2009. The first sign of activity was the start of a seismic swarm on 24 April that steadily intensified until six magnitude 4.6-5.7 earthquakes struck on 17-20 May. More than 30000 people were evacuated from the area following the activity in mid-May and stayed in the neighboring cities of Yanbu and Medina for several weeks. During the intensive activity in mid-May we sent a request for emergency satellite radar data acquisitions to the European Space Agency and later activated an International Charter to guarantee satellite data collection of the area. We have analyzed a number of Envisat, ALOS, and TerraSAR-X interferograms of the area and the results are outstanding, owing to the stable and vegetation-free surface conditions. Interferograms spanning the main seismic activity in mid-May exhibit strong deformation that extends across a large 40 km × 40 km area, with broad uplift and over a meter of WSW-ENE extension. In addition, the data show clear signs of surface faulting and graben-like subsidence in the middle of the deformed area with the graben subsidence exceeding 50 cm. Modeling of deformation strongly suggests that a near-vertical dyke intruded with a WNW-ESE orientation, parallel to the Red Sea, and that the intruded volume is ~0.13 km3. The dyke <span class="hlt">intrusion</span> appears to have triggered faulting on graben-bounding and inward-dipping normal faults. The shallowest part of the dyke seems to have reached within only 2 km of the surface, right below where the graben is the narrowest and under an area with a number of cinder cones from previous volcanic events. While the day-to-day temporal evolution of the deformation cannot be derived from the InSAR data, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005Litho..83..199H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005Litho..83..199H"><span>A new interpretation of the structure of the Sept Iles <span class="hlt">Intrusive</span> suite, Canada</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Higgins, Michael D.</p> <p>2005-08-01</p> <p> chamber, indicating lateral transport of magma. Chemically distinct syenites in the upper part of the <span class="hlt">intrusion</span> are part of the Point du Criade <span class="hlt">intrusion</span>, a large, late composite sill. Diabase and leucogabbro components show a close link with the SIMI and all the acidic magmas may have originally formed by differentiation of the main magma in cupolas towards the centre of the <span class="hlt">intrusion</span>. A series of late gabbro <span class="hlt">intrusions</span> that cut the SIMI may represent a rejuvenation of magmatism. The Border <span class="hlt">zone</span> is a mass of fine-grained rocks that occurs along the border of the SIMI: it may be another magmatic component, or just the lateral border series of the SIMI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010E%26PSL.299..169P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010E%26PSL.299..169P"><span>Surface morphology of active normal faults in hard rock: Implications for the mechanics of the Asal Rift, Djibouti</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pinzuti, Paul; Mignan, Arnaud; King, Geoffrey C. P.</p> <p>2010-10-01</p> <p>Tectonic-stretching models have been previously proposed to explain the process of continental break-up through the example of the Asal Rift, Djibouti, one of the few places where the early stages of seafloor spreading can be observed. In these models, deformation is distributed starting at the base of a shallow seismogenic <span class="hlt">zone</span>, in which sub-vertical normal faults are responsible for subsidence whereas cracks accommodate extension. Alternative models suggest that extension results from localised magma <span class="hlt">intrusion</span>, with normal faults accommodating extension and subsidence only above the maximum reach of the magma column. In these magmatic rifting models, or so-called magmatic <span class="hlt">intrusion</span> models, normal faults have dips of 45-55° and root into <span class="hlt">dikes</span>. Vertical profiles of normal fault scarps from levelling campaign in the Asal Rift, where normal faults seem sub-vertical at surface level, have been analysed to discuss the creation and evolution of normal faults in massive fractured rocks (basalt lava flows), using mechanical and kinematics concepts. We show that the studied normal fault planes actually have an average dip ranging between 45° and 65° and are characterised by an irregular stepped form. We suggest that these normal fault scarps correspond to sub-vertical en echelon structures, and that, at greater depth, these scarps combine and give birth to dipping normal faults. The results of our analysis are compatible with the magmatic <span class="hlt">intrusion</span> models instead of tectonic-stretching models. The geometry of faulting between the Fieale volcano and Lake Asal in the Asal Rift can be simply related to the depth of <span class="hlt">diking</span>, which in turn can be related to magma supply. This new view supports the magmatic <span class="hlt">intrusion</span> model of early stages of continental breaking.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoJI.tmp..180J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoJI.tmp..180J"><span>Passive monitoring of a sea <span class="hlt">dike</span> during a tidal cycle using sea waves as a seismic noise source</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Joubert, Anaëlle; Feuvre, Mathieu Le; Cote, Philippe</p> <p>2018-05-01</p> <p>Over the past decade, ambient seismic noise has been used successfully to monitor various geological objects with high accuracy. Recently, it has been shown that surface seismic waves propagating within a sea <span class="hlt">dike</span> body can be retrieved from the cross-correlation of ambient seismic noise generated by sea waves. We use sea wave impacts to monitor the response of a sea <span class="hlt">dike</span> during a tidal cycle using empirical Green's functions. These are obtained either by cross-correlation or deconvolution, from signals recorded by sensors installed linearly on the crest of a <span class="hlt">dike</span>. Our analysis is based on delay and spectral amplitude measurements performed on reconstructed surface waves propagating along the array. We show that localized variations of velocity and attenuation are correlated with changes in water level as a probable consequence of water infiltration inside the structure. Sea <span class="hlt">dike</span> monitoring is of critical importance for safety and economic reasons, as internal erosion is generally only detected at late stages by visual observations. The method proposed here may provide a solution for detecting structural weaknesses, monitoring progressive internal erosion, and delineating areas of interest for further geotechnical studies, in view to understanding the erosion mechanisms involved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GeoRL..40.1065K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GeoRL..40.1065K"><span>Aspect ratios and magma overpressures of non-feeder <span class="hlt">dikes</span> observed in the Miyake-jima volcano (Japan), and fracture toughness of its upper part</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kusumoto, Shigekazu; Geshi, Nobuo; Gudmundsson, Agust</p> <p>2013-03-01</p> <p>present a new method for estimating the length and maximum thickness (aperture) of a <span class="hlt">dike</span> from the observed opening at one <span class="hlt">dike</span> tip. We apply the method to 15 arrested non-feeder <span class="hlt">dikes</span> (where the upper tip is known, the lower tip unknown) in the caldera walls of Miyake-jima, Japan, to estimate the length-thickness ratio, as well as the magma overpressure and fracture toughness. The calculated length-thickness ratio ranges from 61 to 246, with an average of 136. The ratios are low because the <span class="hlt">dikes</span> are emplaced close to the surface in comparatively compliant (soft) rocks. Using these ratios and the appropriate elastic constants, the calculated magmatic overpressures of the <span class="hlt">dikes</span> are between 2.3 and 8.9 MPa, and the stress intensity factors between 38 and 117 MPa m1/2. All these values are within the range of typical in situ estimates, supporting the validity of this new method.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T21D2873D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T21D2873D"><span>Quantifying Uncertainty in Inverse Models of Geologic Data from Shear <span class="hlt">Zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davis, J. R.; Titus, S.</p> <p>2016-12-01</p> <p>We use Bayesian Markov chain Monte Carlo simulation to quantify uncertainty in inverse models of geologic data. Although this approach can be applied to many tectonic settings, field areas, and mathematical models, we focus on transpressional shear <span class="hlt">zones</span>. The underlying forward model, either kinematic or dynamic, produces a velocity field, which predicts the <span class="hlt">dikes</span>, foliation-lineations, crystallographic preferred orientation (CPO), shape preferred orientation (SPO), and other geologic data that should arise in the shear <span class="hlt">zone</span>. These predictions are compared to data using modern methods of geometric statistics, including the Watson (for lines such as <span class="hlt">dike</span> poles), isotropic matrix Fisher (for orientations such as foliation-lineations and CPO), and multivariate normal (for log-ellipsoids such as SPO) distributions. The result of the comparison is a likelihood, which is a key ingredient in the Bayesian approach. The other key ingredient is a prior distribution, which reflects the geologist's knowledge of the parameters before seeing the data. For some parameters, such as shear <span class="hlt">zone</span> strike and dip, we identify realistic informative priors. For other parameters, where the geologist has no prior knowledge, we identify useful uninformative priors.We investigate the performance of this approach through numerical experiments on synthetic data sets. A fundamental issue is that many models of deformation exhibit asymptotic behavior (e.g., flow apophyses, fabric attractors) or periodic behavior (e.g., SPO when the clasts are rigid), which causes the likelihood to be too uniform. Based on our experiments, we offer rules of thumb for how many data, of which types, are needed to constrain deformation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015SolE....6..253L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015SolE....6..253L"><span>The rheological behaviour of fracture-filling cherts: example of Barite Valley <span class="hlt">dikes</span>, Barberton Greenstone Belt, South Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ledevin, M.; Arndt, N.; Davaille, A.; Ledevin, R.; Simionovici, A.</p> <p>2015-02-01</p> <p>In the Barberton Greenstone Belt, South Africa, a 100-250 m thick complex of carbonaceous chert <span class="hlt">dikes</span> marks the transition from the Mendon Formation to the Mapepe Formation (3260 Ma). The sub-vertical- to vertical position of the fractures, the abundance of highly shattered <span class="hlt">zones</span> with poorly rotated angular fragments and common jigsaw fit, radial structures, and multiple injection features point to repetitive hydraulic fracturing that released overpressured fluids trapped within the shallow crust. The chemical and isotopic compositions of the chert favour a model whereby seawater-derived fluids circulated at low temperature (< 100-150 °C) within the shallow crust. From the microscopic structure of the chert, the injected material was a slurry of abundant clay-sized, rounded particles of silica, carbonaceous matter and minor clay minerals, all suspended in a siliceous colloidal solution. The <span class="hlt">dike</span> geometry and characteristics of the slurry concur on that the chert was viscoelastic, and most probably thixotropic at the time of injection: the penetration of black chert into extremely fine fractures is evidence for low viscosity at the time of injection and the suspension of large country rock fragments in the chert matrix provides evidence of high viscosity soon thereafter. We explain the rheology by the particulate and colloidal structure of the slurry, and by the characteristic of silica suspensions to form cohesive 3-D networks through gelation. Our results provide valuable information about the compositions, physical characteristics and rheological properties of the fluids that circulated through Archean volcano-sedimentary sequences, which is an additional step to understand conditions on the floor of Archean oceans, the habitat of early life.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70043277','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70043277"><span>Aeromagnetic and gravity investigations of the Coastal Area and Continental Shelf of Liberia, West Africa, and their relation to continental drift</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Behrendt, John C.; Wotorson, Cletus S.</p> <p>1970-01-01</p> <p>An aeromagnetic survey has shown the existence of several basins in which magnetic basement depths are greater than 5 km on the continental shelf off Liberia. Magnetic diabase of 176 to 192 m.y. (Jurassic) in age intruding the Paleozoic (?) rocks and overlain by younger rocks onshore requires the distinction between “magnetic basement” and “basement.” Several lines of evidence suggest that the Paleozoic(?) rocks are less than 1 km thick; this implies that the diabase does not introduce a large error in depth-to-basement estimates. The <span class="hlt">dikes</span> or their extrusive equivalents are traceable, on the basis of the magnetic data, beneath the younger sedimentary rock in the basins to the edge of the continental slope. The magnetic data also delineate a second <span class="hlt">zone</span> of diabase <span class="hlt">dikes</span> 90 km inland, parallel to the coast, which cross the entire country. The <span class="hlt">intrusion</span> of the younger <span class="hlt">dikes</span> probably coincides with rifting at the beginning of the separation of Africa and South America, and the associated magnetic anomaly <span class="hlt">zones</span> appear to be parallel with and continuous into the anomaly bands in the Atlantic. A major northeast-trending break in the magnetic fabric intersects the coast near 9° W. and is associated with Eburnean age rocks (about 2000 m.y.) to the southeast as contrasted with Liberian-age rocks (about 2700 m.y.) to the northwest. Change in magnetic fabric direction inland from northeast to northwest in the coastal area allows recognition of a boundary between the Liberian-age rocks inland and Pan-African-age (about 550 m.y.) rocks in the coastal area northwest of about 9° 20'W. Sets of north-northwest-and west-northwest—trending faults of 1 to 2 km vertical displacement cut the Cretaceous sedimentary rocks onshore and can be traced into the offshore basins. Vertical displacements of several kilometers in the magnetic basement underlying the continental shelf suggest a pattern of block faulting all along the coast and continental shelf. Negative Bouguer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA21266.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA21266.html"><span>Wing <span class="hlt">Dike</span> of Hardened Lava in New Mexico</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-01-25</p> <p>This photograph from northwestern New Mexico shows a ridge roughly 30 feet about 10 meters tall that formed from lava filling an underground fracture then resisting erosion better than the material around it did. The <span class="hlt">dike</span> extends from a volcanic peak (out of view here) called Shiprock in English and Tsé Bit'a'í, meaning "rock with wings," in the Navajo language. It offers an Earth analog for some larger hardened-lava walls on Mars http://photojournal.jpl.nasa.gov/catalog/PIA21266</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7021M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7021M"><span>The Age and Geodynamic Evolution of the Metamorphic sole rocks from Izmir-Ankara-Erzıncan suture <span class="hlt">zone</span> (Northern-Turkey)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Melih Çörtük, Rahmi; Faruk Çelik, Ömer; Özkan, Mutlu; Sherlock, Sarah C.; Marzoli, Andrea; Altıntaş, İsmail Emir; Topuz, Gültekin</p> <p>2016-04-01</p> <p>The İzmir-Ankara-Erzincan suture <span class="hlt">zone</span> in northern Turkey is one of the major tectonic <span class="hlt">zones</span> separating the Pontides to the North from the Anatolide-Tauride block and Kı rşehir Massif to the South. The accretionary complex of the İzmir-Ankara-Erzincan suture <span class="hlt">zone</span>, near Artova, is composed mainly of peridotites with varying degree serpentinization, metamorphic rocks, basalt, sandstones, pelagic and neritic limestones. The metamorphic rocks are represented by amphibolite, garnet micaschit, calc-schist and marble. The metamorphic rocks were interpreted as the metamorphic sole rocks. Because; (i) They are tectonically located beneath the serpentinized peridotites. (ii) Foliation planes of both the amphibolites and mantle tectonites are parallel to each other. (iii) The metamorphic rocks are crosscut by non-metamorphic dolerite <span class="hlt">dikes</span> which exhibite Nb and Ta depletion relative to Th enrichment on the N-MORB normalized multi-element spider diagram. The dolerite <span class="hlt">dikes</span> display flat REE patterns (LaN/YbN=0.85-1.24). These geochemical signatures of the dolerite <span class="hlt">dikes</span> are indicative of subduction component during their occurrences. Geochemical observations of the amphibolites suggest E-MORB- and OIB-like signatures (LaN/SmN= 1.39-3.14) and their protoliths are represented by basalt and alkali basaltic rocks. Amphiboles from the amphibolites are represented by calcic amphiboles (magnesio-hornblende, tchermakite and tremolite) and they yielded 40Ar-39Ar ages between 157.8 ± 3.6 Ma and 139 ± 11 Ma. These cooling ages were interpreted to be the intra-oceanic subduction/thrusting time of the İzmir-Ankara-Erzincan oceanic domain. This study was funded by TÜBİTAK (Project no: 112Y123).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JSG....94..136S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JSG....94..136S"><span>Rift brittle deformation of SE-Brazilian continental margin: Kinematic analysis of onshore structures relative to the transfer and accommodation <span class="hlt">zones</span> of southern Campos Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Savastano, Vítor Lamy Mesiano; Schmitt, Renata da Silva; Araújo, Mário Neto Cavalcanti de; Inocêncio, Leonardo Campos</p> <p>2017-01-01</p> <p>High-resolution drone-supported mapping and traditional field work were used to refine the hierarchy and kinematics of rift-related faults in the basement rocks and Early Cretaceous mafic <span class="hlt">dikes</span> onshore of the Campos Basin, SE-Brazil. Two sets of structures were identified. The most significant fault set is NE-SW oriented with predominantly normal displacement. At mesoscale, this fault set is arranged in a rhombic pattern, interpreted here as a breached relay ramp system. The rhombic pattern is a penetrative fabric from the thin-section to regional scale. The second-order set of structures is an E-W/ESE-WNW system of normal faults with sinistral component. These E-W structures are oriented parallel with regional intrabasinal transfer <span class="hlt">zones</span> associated with the earliest stages of Campos Basin's rift system. The crosscutting relationship between the two fault sets and tholeiitic <span class="hlt">dikes</span> implies that the NE-SW fault set is the older feature, but remained active until the final stages of rifting in this region as the second-order fault set is older than the tholeiitic <span class="hlt">dikes</span>. Paleostresses estimated from fault slip inversion method indicated that extension was originally NW-SE, with formation of the E-W transfer, followed by ESE-WNW oblique opening associated with a relay ramp system and related accommodation <span class="hlt">zones</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V43G2954M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V43G2954M"><span>Metamorphism Near the <span class="hlt">Dike</span>-Gabbro Transition in the Ocean Crust Based on Preliminary Results from Oman Drilling Project Hole GT3A</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Manning, C. E.; Nozaka, T.; Harris, M.; Michibayashi, K.; de Obeso, J. C.; D'Andres, J.; Lefay, R.; Leong, J. A. M.; Zeko, D.; Kelemen, P. B.; Teagle, D. A. H.</p> <p>2017-12-01</p> <p>Oman Drilling Project Hole GT3A intersected 400 m of altered basaltic <span class="hlt">dikes</span>, gabbros, and diorites. The 100% recovery affords an unprecedented opportunity to study metamorphism and hydrothermal alteration near the <span class="hlt">dike</span>-gabbro transition in the ocean crust. Hydrothermal alteration is ubiquitous; all rocks are at least moderately altered, and mean alteration intensity is 54%. The earliest alteration in all rock types is background replacement of igneous minerals, some of which occurred at clinopyroxene amphibolite facies, as indicated by brown-green hornblende, calcic plagioclase, and secondary cpx. In addition, background alteration includes greenschist, subgreenschist, and zeolite facies minerals. More extensive alteration is locally observed in halos around veins, patches, and <span class="hlt">zones</span> related to deformation. Dense networks of hydrothermal veins record a complex history of fluid-rock alteration. During core description, 10,727 individual veins and 371 vein networks were logged in the 400 m of Hole GT3A. The veins displayed a range of textures and connectivities. The total density of veins in Hole GT3A is 26.8 veins m-1. Vein density shows no correlation with depth, but may be higher near <span class="hlt">dike</span> margins and faults. Vein minerals include amphibole, epidote, quartz, chlorite, prehnite, zeolite (chiefly laumontite) and calcite in a range of combinations. Analysis of crosscutting relations leads to classification of 4 main vein types. In order of generally oldest to youngest these are: amphibole, quartz-epidote-chlorite (QEC), zeolite-prehnite (ZP), and calcite. QEC and ZP vein types may contain any combination of minerals except quartz alone; veins filled only by quartz may occur at any relative time. Macroscopic amphibole veins are rare and show no variation with depth. QEC vein densities appear to be higher (>9.3 veins m-1) in the upper 300 m of GT3A, where <span class="hlt">dikes</span> predominate. In contrast, there are 5.5 veins m-1 at 300-400 m, where gabbros and diorites are abundant. ZP</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.agu.org/pubs/crossref/2011/2010WR010043.shtml','USGSPUBS'); return false;" href="http://www.agu.org/pubs/crossref/2011/2010WR010043.shtml"><span>3-D flow and scour near a submerged wing <span class="hlt">dike</span>: ADCP measurements on the Missouri River</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jamieson, E.C.; Rennie, C.D.; Jacobson, R.B.; Townsend, R.D.</p> <p>2011-01-01</p> <p>Detailed mapping of bathymetry and three-dimensional water velocities using a boat-mounted single-beam sonar and acoustic Doppler current profiler (ADCP) was carried out in the vicinity of two submerged wing <span class="hlt">dikes</span> located in the Lower Missouri River near Columbia, Missouri. During high spring flows the wing <span class="hlt">dikes</span> become submerged, creating a unique combination of vertical flow separation and overtopping (plunging) flow conditions, causing large-scale three-dimensional turbulent flow structures to form. On three different days and for a range of discharges, sampling transects at 5 and 20 m spacing were completed, covering the area adjacent to and upstream and downstream from two different wing <span class="hlt">dikes</span>. The objectives of this research are to evaluate whether an ADCP can identify and measure large-scale flow features such as recirculating flow and vortex shedding that develop in the vicinity of a submerged wing <span class="hlt">dike</span>; and whether or not moving-boat (single-transect) data are sufficient for resolving complex three-dimensional flow fields. Results indicate that spatial averaging from multiple nearby single transects may be more representative of an inherently complex (temporally and spatially variable) three-dimensional flow field than repeated single transects. Results also indicate a correspondence between the location of calculated vortex cores (resolved from the interpolated three-dimensional flow field) and the nearby scour holes, providing new insight into the connections between vertically oriented coherent structures and local scour, with the unique perspective of flow and morphology in a large river.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70185074','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70185074"><span>Episodic growth of a Late Cretaceous and Paleogene <span class="hlt">intrusive</span> complex of pegmatitic leucogranite, Ruby Mountains core complex, Nevada, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Howard, Keith A.; Wooden, J.L.; Barnes, C.G.; Premo, W.R.; Snoke, A.W.; Lee, S.-Y.</p> <p>2011-01-01</p> <p>Gneissic pegmatitic leucogranite forms a dominant component (>600 km3) of the midcrustal infrastructure of the Ruby Mountains–East Humboldt Range core complex (Nevada, USA), and was assembled and modified episodically into a batholithic volume by myriad small <span class="hlt">intrusions</span> from ca. 92 to 29 Ma. This injection complex consists of deformed sheets and other bodies emplaced syntectonically into a stratigraphic framework of marble, calc-silicate rocks, quartzite, schist, and other granitoids. Bodies of pegmatitic granite coalesce around host-rock remnants, which preserve relict or ghost stratigraphy, thrusts, and fold nappes. <span class="hlt">Intrusion</span> inflated but did not disrupt the host-rock structure. The pegmatitic granite increases proportionally downward from structurally high positions to the bottoms of 1-km-deep canyons where it constitutes 95%–100% of the rock. Zircon and monazite dated by U-Pb (sensitive high-resolution ion microprobe, SHRIMP) for this rock type cluster diffusely at ages near 92, 82(?), 69, 38, and 29 Ma, and indicate successive or rejuvenated igneous crystallization multiple times over long periods of the Late Cretaceous and the Paleogene. Initial partial melting of unexposed pelites may have generated granite forerunners, which were remobilized several times in partial melting events. Sources for the pegmatitic granite differed isotopically from sources of similar-aged interleaved equigranular granites. Dominant Late Cretaceous and fewer Paleogene ages recorded from some pegmatitic granite samples, and Paleogene-only ages from the two structurally deepest samples, together with varying zircon trace element contents, suggest several disparate ages of final emplacement or remobilization of various small bodies. Folded sills that merge with <span class="hlt">dikes</span> that cut the same folds suggest that there may have been in situ partial remobilization. The pegmatitic granite <span class="hlt">intrusions</span> represent prolonged and recurrent generation, assembly, and partial melting modification of a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol2/pdf/CFR-2010-title10-vol2-sec63-322.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title10-vol2/pdf/CFR-2010-title10-vol2-sec63-322.pdf"><span>10 CFR 63.322 - Human <span class="hlt">intrusion</span> scenario.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 10 Energy 2 2010-01-01 2010-01-01 false Human <span class="hlt">intrusion</span> scenario. 63.322 Section 63.322 Energy... REPOSITORY AT YUCCA MOUNTAIN, NEVADA Postclosure Public Health and Environmental Standards Human <span class="hlt">Intrusion</span> Standard § 63.322 Human <span class="hlt">intrusion</span> scenario. For the purposes of the analysis of human <span class="hlt">intrusion</span>, DOE must...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V43C2396T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V43C2396T"><span>Wall Rock Assimilation and Magma Migration in the Sierra Nevada Batholith: A Study of the Courtright <span class="hlt">Intrusive</span> <span class="hlt">Zone</span>, Central California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Torrez, G.; Putirka, K. D.</p> <p>2010-12-01</p> <p>The Sierra Nevada Batholith is composed of various plutons that interact with each other, and with pre- and syn-batholith metamorphic rocks. In the central part of the Sierra Nevada Batholith, at Courtright Reservoir in California, the younger Mt. Givens Pluton (87-93 Ma; McNulty et al., 2000) intrudes the Dinkey pluton (103 Ma; Bateman et al., 1964), and metasediments (a metamorphic screen) that, in places, separate the two plutons. This Courtright Reservoir <span class="hlt">Intrusive</span> <span class="hlt">zone</span>, as termed by Bateman et al. (1964), provides an ideal setting to examine the dynamics of <span class="hlt">intrusion</span> and assimilation. Whole rock major and trace element compositions of the plutons, their mafic enclaves, and the metasediments, show that all such samples, from both plutons, fall on a single mixing trend. We thus infer that magmas parental to both plutons were roughly similar in composition, and assimilated significant amounts of the same, or very similar metasedimentary wall rocks. We also examined changes in whole rock compositions within the Mt. Givens pluton, as a function of distance from the two rock units with which it is now in contact (the metasediments, and the Dinkey Creek). In the vicinity of the contact between are an abundance of enclaves that are rounded, and appear to have been transported in vertical pipes. Whole rock analysis of the host granitoid material that surrounds these enclaves is clearly more mafic than the granitoid magmas from interior parts of the pluton. These whole rock compositions indicate that the pluton becomes more homogenous moving away from the contact, with a compositional decay occurring over a span of about 50-100 m. There are at least two possible interpretations. The compositional decay may represent a diffusive exchange of mass between an early crystallizing marginal phase of the pluton and the pluton interior. Another (not mutually incompatible) possibility is that the mafic margins represent pipes or tubes (Paterson, 2010), related to some convective</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMNH33A1627K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMNH33A1627K"><span><span class="hlt">Dike</span> Strength Analysis on a Regional Scale Based On a Stochastic Subsoil Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koelewijn, A. R.; Vastenburg, E. W.</p> <p>2013-12-01</p> <p>About two-third of the Netherlands is protected against flooding by <span class="hlt">dikes</span> and levees. The subsoil can be characterized by fluvial and marine sediments. Maintaining the safety of these <span class="hlt">dikes</span> and levees is of vital importance. Insufficient safety is not permissible, but excessive safety would imply a waste of money and other resources. Therefore safety assessments are carried out on a regular basis. Over the past decades, a practice has grown to calculate a limited number of cross-sections, roughly one every 500 to 1000 meters. For this purpose, a representative cross-section is selected as an estimate of the most vulnerable surface geometry and the subsoil conditions determined from boreholes and cone penetration tests, for which slope stability and piping analyses are carried out. This is a time-consuming procedure which is not only expensive, but also neglects geological knowledge. A method to incorporate geological knowledge of an area, including updating on the basis of additional investigations, has been described in Koelewijn et al. [2011]. In addition, various groups have worked to incorporate geotechnical stability models and detailed Lidar-measurements of the surface into a more efficient and rational calculation process [Knoeff et al. 2011, Lam et al. 2013, van den Ham & Mastbergen, 2013]. Combining this experience with the 3D subsoil model opens possibilities for cost-effective additional soil investigations for those locations where ruling out unfavorable conditions really influences the decisions to be made regarding rejection and improvement, see the figure for examples of different subsoil profiles along a <span class="hlt">dike</span>. The resulting system has been applied for semi-automated calculations of <span class="hlt">dikes</span> in various parts of the Netherlands, totalling over 4000 km by now, and a part of the Mississippi levee system. [van den Ham & Mastbergen, 2013] G.A. van den Ham & D.R. Mastbergen, A semi-probabilistic assessment method for flow slides. AGU Fall meeting, 2013</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T31B1818P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T31B1818P"><span>Surface Morphology of Active Normal Faults in Hard Rock: Implications for the Mechanics of the Asal Rift, Djibouti</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pinzuti, P.; Mignan, A.; King, G. C.</p> <p>2009-12-01</p> <p>Mechanical stretching models have been previously proposed to explain the process of continental break-up through the example of the Asal Rift, Djibouti, one of the few places where the early stages of seafloor spreading can be observed. In these models, deformation is distributed starting at the base of a shallow seismogenic <span class="hlt">zone</span>, in which sub-vertical normal faults are responsible for subsidence whereas cracks accommodate extension. Alternative models suggest that extension results from localized magma injection, with normal faults accommodating extension and subsidence above the maximum reach of the magma column. In these magmatic <span class="hlt">intrusion</span> models, normal faults have dips of 45-55° and root into <span class="hlt">dikes</span>. Using mechanical and kinematics concepts and vertical profiles of normal fault scarps from an Asal Rift campaign, where normal faults are sub-vertical on surface level, we discuss the creation and evolution of normal faults in massive fractured rocks (basalt). We suggest that the observed fault scarps correspond to sub-vertical en echelon structures and that at greater depth, these scarps combine and give birth to dipping normal faults. Finally, the geometry of faulting between the Fieale volcano and Lake Asal in the Asal Rift can be simply related to the depth of <span class="hlt">diking</span>, which in turn can be related to magma supply. This new view supports the magmatic <span class="hlt">intrusion</span> model of early stages of continental breaking.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1916559G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1916559G"><span>Sill <span class="hlt">intrusion</span> in volcanic calderas: implications for vent opening probability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Giudicepietro, Flora; Macedonio, Giovanni; Martini, Marcello; D'Auria, Luca</p> <p>2017-04-01</p> <p>Calderas show peculiar behaviors with remarkable dynamic processes, which do not often culminate in eruptions. Observations and studies conducted in recent decades have shown that the most common cause of unrest in the calderas is due to magma <span class="hlt">intrusion</span>; in particular, the <span class="hlt">intrusion</span> of sills at shallow depths. Monogenic cones, with large areal dispersion, are quite common in the calderas, suggesting that the susceptibility analysis based on geological features, is not strictly suitable for estimating the vent opening probability in calderas. In general, the opening of a new eruptive vent can be regarded as a rock failure process. The stress field in the rocks that surrounds and tops the magmatic reservoirs plays an important role in causing the rock failure and creating the path that magma can follow towards the surface. In this conceptual framework, we approach the problem of getting clues about the probability of vent opening in volcanic calderas through the study of the stress field produced by the <span class="hlt">intrusion</span> of magma, in particular, by the <span class="hlt">intrusion</span> of a sill. We simulate the <span class="hlt">intrusion</span> of a sill free to expand radially, with shape and dimensions which vary with time. The <span class="hlt">intrusion</span> process is controlled by the elastic response of the rock plate above the sill, which bends because of the <span class="hlt">intrusion</span>, and by gravity, that drives the magma towards the <span class="hlt">zones</span> where the thickness of the sill is smaller. We calculated the stress field in the plate rock above the sill. We found that at the bottom of the rock plate above the sill the maximum intensity of tensile stress is concentrated at the front of the sill and spreads radially with it, over time. For this reason, we think that the front of the spreading sill is prone to open for eruptive vents. Even in the central area of the sill the intensity of stress is relatively high, but at the base of the rock plate stress is compressive. Under isothermal conditions, the stress soon reaches its maximum value (time interval</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGP11A0995H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGP11A0995H"><span>Ediacaran paleomagnetic results from feeder <span class="hlt">dikes</span> of the Catoctin Formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hankard, F.; Domeier, M. M.; Bentley, C.; Van Der Voo, R.</p> <p>2011-12-01</p> <p>A paleomagnetic study undertaken sixteen years ago on the Catoctin basalts, feeder <span class="hlt">dikes</span> and sills (Meert et al, 1994) did not bring firm and strong conclusions about the paleoposition of Laurentia during the Ediacaran period. The results were rather complex and sketchy. In effect, three paleomagnetic directions derived from this study were interpreted as follows: one placed Laurentia at high southerly latitude during Catoctin time while the other two were considered as later "remagnetization" events. One remagnetization was hypothesized to have been acquired in the Late Cambrian, when Laurentia was in an equatorial position, whereas a second one was attributed to Taconian mountain-building during the Ordovician period. In order to attempt to unravel the confusing late Precambrian paleogeography, we conducted a detailed paleomagnetic sampling in the Blue Ridge Province of Central Virginia. We focused on the <span class="hlt">dikes</span> that fed the 568-555 Ma volcanism of the Catoctin Formation (Southworth et al, 2009) in the Shenandoah National Park, as well as in several locations outside the park, and along the south shore of the Potomac River (Maryland). These new data should help to define unambiguously which (if any) of the magnetization components is primary for the Catoctin Formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..354..153P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..354..153P"><span><span class="hlt">Intrusive</span> hyaloclastite and peperitic breccias associated to sill and cryptodome emplacement on an Early Paleocene polymagmatic compound cone-dome volcanic complex from El Guanaco mine, Northern Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Páez, G. N.; Permuy Vidal, C.; Galina, M.; López, L.; Jovic, S. M.; Guido, D. M.</p> <p>2018-04-01</p> <p> compositionally variated synvolcanic <span class="hlt">intrusives</span> can be explained either by the presence of a <span class="hlt">zoned</span> magmatic chamber feeding the volcanic complex, or more likely by the influence of the Soledad-Peñafiel Fault <span class="hlt">Zone</span> acting as a preferential pathway for different magma compositions/sources to rise to the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28500488','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28500488"><span>[Analysis of <span class="hlt">intrusion</span> errors in free recall].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Diesfeldt, H F A</p> <p>2017-06-01</p> <p>Extra-list <span class="hlt">intrusion</span> errors during five trials of the eight-word list-learning task of the Amsterdam Dementia Screening Test (ADST) were investigated in 823 consecutive psychogeriatric patients (87.1% suffering from major neurocognitive disorder). Almost half of the participants (45.9%) produced one or more <span class="hlt">intrusion</span> errors on the verbal recall test. Correct responses were lower when subjects made <span class="hlt">intrusion</span> errors, but learning slopes did not differ between subjects who committed <span class="hlt">intrusion</span> errors and those who did not so. Bivariate regression analyses revealed that participants who committed <span class="hlt">intrusion</span> errors were more deficient on measures of eight-word recognition memory, delayed visual recognition and tests of executive control (the Behavioral Dyscontrol Scale and the ADST-Graphical Sequences as measures of response inhibition). Using hierarchical multiple regression, only free recall and delayed visual recognition retained an independent effect in the association with <span class="hlt">intrusion</span> errors, such that deficient scores on tests of episodic memory were sufficient to explain the occurrence of <span class="hlt">intrusion</span> errors. Measures of inhibitory control did not add significantly to the explanation of <span class="hlt">intrusion</span> errors in free recall, which makes insufficient strength of memory traces rather than a primary deficit in inhibition the preferred account for <span class="hlt">intrusion</span> errors in free recall.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA191689','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA191689"><span>Lower Mississippi River Environmental Program. Report 10. Evaluation of Bird and Mammal Utilization of <span class="hlt">Dike</span> Systems Along the Lower Mississippi River.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1987-11-01</p> <p>Salix nigra). and cocklebur (Xanthium strumarium ) occurred in all 10 <span class="hlt">dike</span> systems. False indigo (Amorpha fruticosa). day 6 flower (Commelina diffusa...Xanthium strumarium + + + + + + + + + + Number of species recorded by <span class="hlt">dike</span> system 11 33 56 58 33 50 50 39 52 18 Percent of total number of species</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BVol...80...49H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BVol...80...49H"><span>Erratum: Correction to: Emplacement controls for the basaltic-andesitic radial <span class="hlt">dikes</span> of Summer Coon volcano and implications for flank vents at stratovolcanoes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harp, A. G.; Valentine, G. A.</p> <p>2018-06-01</p> <p>In the article "Emplacement controls for the basaltic-andesitic radial <span class="hlt">dikes</span> of Summer Coon volcano and implications for flank vents at stratovolcanoes", the vertical axis for Fig. 8 a was incorrectly labeled (i.e., the value for <span class="hlt">dikes</span> per km2).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930005131','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930005131"><span>Determining stress states using <span class="hlt">dike</span> swarms: The Lauma Dorsa example</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Grosfils, Eric B.; Head, James W., III</p> <p>1992-01-01</p> <p>Initial examination of the Magellan coverage of Venus has revealed between 150 and 300 large, radially lineated landforms distributed across the planet's surface. Where the lineaments have been examined in detail, the majority fail to exhibit signatures indicative of relief at or above the resolution of the radar; however, when the sense of topographic relief may be ascertained, the lineaments commonly appear as fissures or flat-floored trenches interpreted as graben. Individual lineaments can display graben, fissure, and zero relief behavior along their length, suggesting either that these differences are a function of the resolution of the radar, or that the morphological distinctions are real but somehow genetically linked. In many instances, radial lineaments exhibiting these characteristics are directly associated with surface volcanism, including flanking and terminal flows, superimposed shield domes and pit chains, and central, calderalike topographic lows. These observable characteristics, as well as theoretical studies and comparison with similar terrestrial features, have led to the working hypothesis that many of the radial fracture systems on Venus are the surface manifestation of subsurface <span class="hlt">dikes</span> propagating laterally from a central magma source. If this interpretation is correct, studies of terrestrial <span class="hlt">dikes</span> suggest that the lineament directions, with localized exceptions and barring subsequent deformation, should be perpendicular to the orientation of the least compressive stress at the time of their formation. To test this hypothesis, we briefly examine a radial fracture system (63.7 degrees N, 195 degrees E) located between two deformation belts in Vinmara Planitia, and verify that the lineaments to the east behave in the expected manner. We have also chosen this feature, however, because of its proximity to Lauma Dorsa to the west. On the basis of Venera 15/16 data, both compressional and extensional origins for this deformation belt have been</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.3093M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.3093M"><span>High-resolution seismic imaging of the Kevitsa mafic-ultramafic Cu-Ni-PGE hosted <span class="hlt">intrusion</span>, northern Finland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malehmir, Alireza; Koivisto, Emilia; Wjins, Chris; Tryggvason, Ari; Juhlin, Christopher</p> <p>2014-05-01</p> <p> volume better represents the geology around the mine and in the vicinity of the known deposit, while the 2D seismic profiles were designed to provide information on larger-scale structures in the area. Both the 2D and 3D seismic data were used to create a 3D lithological and structural model of the entire complex. Information on the dimensions of the ore-bearing Kevitsa <span class="hlt">intrusion</span> can be used for more effective exploration in the area. The base of the <span class="hlt">intrusion</span> is particularly clear in the northern and western sectors of the seismic data. Toward the east, the base is mostly defined by disruption of the reflectors internal to the <span class="hlt">intrusion</span>. Recent tests using prestack migration methods on the 3D data show partial improvements in the image, especially at shallow depths. 3D seismic tomography has also been performed and the results indicate low velocity <span class="hlt">zones</span> crossing the open pit that can be interpreted as <span class="hlt">zones</span> of weakness. Future studies will focus on using the tomography results as the input velocity field for prestack depth migration of the 3D data and also improving the 3D geological model of the study area. Acknowledgments: FQM, GTK, HiSeis and Vibrometric</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Geote..52..331K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Geote..52..331K"><span>Late Vendian Complexes in the Structure of Metamorphic Basement of the Fore Range <span class="hlt">Zone</span>, Greater Caucasus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kamzolkin, V. A.; Latyshev, A. V.; Vidyapin, Yu. P.; Somin, M. L.; Smul'skaya, A. I.; Ivanov, S. D.</p> <p>2018-05-01</p> <p>The paper presents new data on the composition, age, and relationships (with host and overlying deposits) of <span class="hlt">intrusive</span> rocks in the basement of the Fore Range <span class="hlt">zone</span> (Greater Caucasus), in the Malaya Laba River Basin. The evolutionary features of <span class="hlt">intrusive</span> units located within the Blyb metamorphic complex are described. It is shown for the first time that the lower levels of this complex are, in a structural sense, outcrops of the Late Vendian basement. The basement is composed of the Balkan Formation and a massif of quartz metadiorites that intrudes it; for the rocks of this massif, ages ranging from 549 ± 7.4 to 574.1 ± 6.7 Ma are obtained for three U-Pb datings by the SHRIMP-II method. The Herzyinan magmatic event is represented by a group of granodiorite <span class="hlt">intrusions</span> penetrating the Blyb complex on a series of faults extending along its boundary with the Main Range <span class="hlt">zone</span>. The obtained estimate for the U-Pb age of one of the <span class="hlt">intrusions</span> (319 ± 3.8 Ma) corresponds to the end of the Serpukhovian stage of the Early Carboniferous.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA443574','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA443574"><span>Machine Learning in <span class="hlt">Intrusion</span> Detection</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2005-07-01</p> <p>machine learning tasks. Anomaly detection provides the core technology for a broad spectrum of security-centric applications. In this dissertation, we examine various aspects of anomaly based <span class="hlt">intrusion</span> detection in computer security. First, we present a new approach to learn program behavior for <span class="hlt">intrusion</span> detection. Text categorization techniques are adopted to convert each process to a vector and calculate the similarity between two program activities. Then the k-nearest neighbor classifier is employed to classify program behavior as normal or <span class="hlt">intrusive</span>. We demonstrate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060029704&hterms=detection+systems&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Ddetection%2Bsystems','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060029704&hterms=detection+systems&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Ddetection%2Bsystems"><span><span class="hlt">Intrusion</span> detection: systems and models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sherif, J. S.; Dearmond, T. G.</p> <p>2002-01-01</p> <p>This paper puts forward a review of state of the art and state of the applicability of <span class="hlt">intrusion</span> detection systems, and models. The paper also presents a classfication of literature pertaining to <span class="hlt">intrusion</span> detection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H33E1213B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H33E1213B"><span>Alternative Methods for Assessing Contaminant Transport from the Vadose <span class="hlt">Zone</span> to Indoor Air</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baylor, K. J.; Lee, A.; Reddy, P.; Plate, M.</p> <p>2010-12-01</p> <p>Vapor <span class="hlt">intrusion</span>, which is the transport of contaminant vapors from groundwater and the vadose <span class="hlt">zone</span> to indoor air, has emerged as a significant human health risk near hazardous waste sites. Volatile organic compounds (VOCs) such as trichloroethylene (TCE) and tetrachloroethylene (PCE) can volatilize from groundwater and from residual sources in the vadose <span class="hlt">zone</span> and enter homes and commercial buildings through cracks in the slab, plumbing conduits, or other preferential pathways. Assessment of the vapor <span class="hlt">intrusion</span> pathway typically requires collection of groundwater, soil gas, and indoor air samples, a process which can be expensive and time-consuming. We evaluated three alternative vapor <span class="hlt">intrusion</span> assessment methods, including 1) use of radon as a surrogate for vapor <span class="hlt">intrusion</span>, 2) use of pressure differential measurements between indoor/outdoor and indoor/subslab to assess the potential for vapor <span class="hlt">intrusion</span>, and 3) use of passive, longer-duration sorbent methods to measure indoor air VOC concentrations. The primary test site, located approximately 30 miles south of San Francisco, was selected due to the presence of TCE (10 - 300 ug/L) in shallow groundwater (5 to 10 feet bgs). At this test site, we found that radon was not a suitable surrogate to asses vapor <span class="hlt">intrusion</span> and that pressure differential measurements are challenging to implement and equipment-intensive. More significantly, we found that the passive, longer-duration sorbent methods are easy to deploy and compared well quantitatively with standard indoor air sampling methods. The sorbent technique is less than half the cost of typical indoor air methods, and also provides a longer duration sample, typically 3 to 14 days rather than 8 to 24 hours for standard methods. The passive sorbent methods can be a reliable, cost-effective, and easy way to sample for TCE, PCE and other VOCs as part of a vapor <span class="hlt">intrusion</span> investigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033154','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033154"><span>Silurian extension in the Upper Connecticut Valley, United States and the origin of middle Paleozoic basins in the Québec embayment</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rankin, D.W.; Coish, R.A.; Tucker, R.D.; Peng, Z.X.; Wilson, S.A.; Rouff, A.A.</p> <p>2007-01-01</p> <p>Pre-Silurian strata of the Bronson Hill arch (BHA) in the Upper Connecticut Valley, NH-VT are host to the latest Ludlow Comerford <span class="hlt">Intrusive</span> Suite consisting, east to west, of a mafic <span class="hlt">dike</span> swarm with sheeted <span class="hlt">dikes</span>, and an <span class="hlt">intrusive</span> complex. The rocks are mostly mafic but with compositions ranging from gabbro to leucocratic tonalite. The suite is truncated on the west by the Monroe fault, a late Acadian thrust that carries rocks of the BHA westward over Silurian-Devonian strata of the Connecticut Valley-Gaspe?? trough (CVGT). <span class="hlt">Dikes</span> intrude folded strata with a pre-<span class="hlt">intrusion</span> metamorphic fabric (Taconian?) but they experienced Acadian deformation. Twenty fractions of zircon and baddeleyite from three sample sites of gabbrodiorite spanning nearly 40 km yield a weighted 207Pb/206Pb age of 419 ?? 1 Ma. Greenschist-facies <span class="hlt">dikes</span>, sampled over a strike distance of 35 km, were tholeiitic basalts formed by partial melting of asthenospheric mantle, with little or no influence from mantle or crustal lithosphere. The <span class="hlt">dike</span> chemistry is similar to mid-ocean ridge, within-plate, and back-arc basin basalts. Parent magmas originated in the asthenosphere and were erupted through severely thinned lithosphere adjacent to the CVGT. Extensive middle Paleozoic basins in the internides of the Appalachian orogen are restricted to the Que??bec embayment of the Laurentian rifted margin, and include the CVGT and the Central Maine trough (CMT), separated from the BHA by a Silurian tectonic hinge. The NE-trending Comerford <span class="hlt">intrusions</span> parallel the CVGT, CMT, and the tectonic hinge, and indicate NW-SE extension. During post-Taconian convergence, the irregular margins of composite Laurentia and Avalon permitted continued collision in Newfoundland (St. Lawrence promontory) and coeval extension in the Que??bec embayment. Extension may be related to hinge retreat of the northwest directed Brunswick subduction complex and rise of the asthenosphere following slab break-off. An alternative hypothesis is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27347649','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27347649"><span>An international perspective on Facebook <span class="hlt">intrusion</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Błachnio, Agata; Przepiorka, Aneta; Benvenuti, Martina; Cannata, Davide; Ciobanu, Adela Magdalena; Senol-Durak, Emre; Durak, Mithat; Giannakos, Michail N; Mazzoni, Elvis; Pappas, Ilias O; Popa, Camelia; Seidman, Gwendolyn; Yu, Shu; Wu, Anise M S; Ben-Ezra, Menachem</p> <p>2016-08-30</p> <p>Facebook has become one of the most popular social networking websites in the world. The main aim of the study was to present an international comparison of Facebook <span class="hlt">intrusion</span> and Internet penetration while examining possible gender differences. The study consisted of 2589 participants from eight countries: China, Greece, Israel, Italy, Poland, Romania, Turkey, USA. Facebook <span class="hlt">intrusion</span> and Internet penetration were taken into consideration. In this study the relationship between Facebook <span class="hlt">intrusion</span> and Internet penetration was demonstrated. Facebook <span class="hlt">intrusion</span> was slightly negatively related to Internet penetration in each country. Copyright © 2016 Elsevier Ireland Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolED...6.1227L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolED...6.1227L"><span>The rheological behavior of fracture-filling cherts: example of Barite Valley <span class="hlt">dikes</span>, Barberton Greenstone Belt, South Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ledevin, M.; Arndt, N.; Simionovici, A.</p> <p>2014-05-01</p> <p>A 100 m-thick complex of near-vertical carbonaceous chert <span class="hlt">dikes</span> marks the transition from the Mendon to Mapepe Formations (3260 Ma) in the Barberton Greenstone Belt, South Africa. Fracturing was intense in this area, as shown by the profusion and width of the <span class="hlt">dikes</span> (ca. 1 m on average) and by the abundance of completely shattered rocks. The <span class="hlt">dike</span>-and-sill organization of the fracture network and the upward narrowing of some of the large veins indicate that at least part of the fluid originated at depth and migrated upward in this hydrothermal plumbing system. Abundant angular fragments of silicified country rock are suspended and uniformly distributed within the larger <span class="hlt">dikes</span>. Jigsaw-fit structures and confined bursting textures indicate that hydraulic fracturing was at the origin of the veins. The confinement of the <span class="hlt">dike</span> system beneath an impact spherule bed suggests that the hydrothermal circulations were triggered by the impact and located at the external margin of a large crater. From the geometry of the <span class="hlt">dikes</span> and the petrography of the cherts, we infer that the fluid that invaded the fractures was thixotropic. On one hand, the injection of black chert into extremely fine fractures is evidence for low viscosity at the time of injection; on the other hand, the lack of closure of larger veins and the suspension of large fragments in a chert matrix provide evidence of high viscosity soon thereafter. The inference is that the viscosity of the injected fluid increased from low to high as the fluid velocity decreased. Such rheological behavior is characteristic of media composed of solid and colloidal particles suspended in a liquid. The presence of abundant clay-sized, rounded particles of silica, carbonaceous matter and clay minerals, the high proportion of siliceous matrix and the capacity of colloidal silica to form cohesive 3-D networks through gelation, account for the viscosity increase and thixotropic behavior of the fluid that filled the veins. Stirring and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JHyd..551..648W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JHyd..551..648W"><span>How significant is the slope of the sea-side boundary for modelling seawater <span class="hlt">intrusion</span> in coastal aquifers?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walther, Marc; Graf, Thomas; Kolditz, Olaf; Liedl, Rudolf; Post, Vincent</p> <p>2017-08-01</p> <p>Application of numerical models is a common method to assess groundwater resources. The versatility of these models allows consideration of different levels of complexity, but the accuracy of the outcomes hinges upon a proper description of the system behaviour. In seawater <span class="hlt">intrusion</span> assessment, the implementation of the sea-side boundary condition is of particular importance. We evaluate the influence of the slope of the sea-side boundary on the simulation results of seawater <span class="hlt">intrusion</span> in a freshwater aquifer by employing a series of slope variations together with a sensitivity analysis by varying additional sensitive parameters (freshwater inflow and longitudinal and transverse dispersivities). Model results reveal a multi-dimensional dependence of the investigated variables with an increasing relevance of the sea-side boundary slope for seawater <span class="hlt">intrusion</span> (decrease of up to 32%), submarine groundwater discharge <span class="hlt">zone</span> (reduction of up to 55%), and turnover times (increase of up to 730%) with increasing freshwater inflow or dispersivity values.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1210247H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1210247H"><span>Investigation of origin for seawater <span class="hlt">intrusion</span> using geophysical well logs and absolute ages of volcanic cores in the eastern part of Jeju Island</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hwang, Seho; Shin, Jehyun</p> <p>2010-05-01</p> <p>Jeju located in the southern extremity of Korea is volcanic island, one of best-known tourist attractions in Korea. Jeju Province operates the monitoring boreholes for the evaluation of groundwater resources in coastal area. Major rock types identified from drill cores are trachybasalt, acicular basalt, scoria, hyalocastite, tuff, unconsolidated U formation, and seoguipo formation and so on. Various conventional geophysical well loggings including radioactive logs (natural gamma log, dual neutron log, and gamma-gamma log), electrical log (or electromagnetic induction log), caliper log, fluid temperature/ conductivity log, and televiewer logs have been conducted to identify basalt sequences and permeable <span class="hlt">zone</span>, and verify seawater <span class="hlt">intrusion</span> in monitoring boreholes. The conductivity logs clearly show the fresh water-saline water boundaries, but we find it hard to identify the permeable <span class="hlt">zones</span> because of the mixed groundwater within the boreholes. Temperature gradient logs are mostly related with lithologic boundaries and permeable <span class="hlt">zones</span> intersected by boreholes of eastern coasts. The wide range of periodic electrical conductivity logging in the deeper depth of monitoring boreholes indicates the possibility of submarine groundwater discharge. However we did not clearly understand the origin of seawater <span class="hlt">intrusion</span> in the eastern coast until now. So we analysis the electrical conductivity profiles, record of sea-level change and 40Ar/39Ar absolute ages of volcanic rock cores from twenty boreholes in east coast. From comparing absolute ages of volcanic rock cores and sea-level of their ages, we find that the almost ages of depth showing high salinity groundwater are about 100 Ka, and from 130Ka to about 180Ka. The former is after the interglacial period and the latter is illinoian. These results indicate that the abrupt raising of sea level after illinoian formed the regional coast, and the <span class="hlt">zone</span> of present seawater <span class="hlt">intrusion</span> also are above the depth of illinoin period. So</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-09-10/pdf/2013-21939.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-09-10/pdf/2013-21939.pdf"><span>78 FR 55216 - Safety <span class="hlt">Zone</span>: Suisun Bay Electromagnetic Scan and Ordnance Recovery, Suisun Bay, Concord, CA</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-09-10</p> <p>...-AA00 Safety <span class="hlt">Zone</span>: Suisun Bay Electromagnetic Scan and Ordnance Recovery, Suisun Bay, Concord, CA AGENCY... (MOTCO) electromagnetic scan and ordnance recovery operations. These safety <span class="hlt">zones</span> are established to... 10, 2013 that they intend to conduct an <span class="hlt">intrusive</span> electromagnetic scan and ordnance recovery...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JSAES..67...11G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JSAES..67...11G"><span>Evidence of Gondwana early rifting process recorded by Resende-Ilha Grande <span class="hlt">Dike</span> Swarm, southern Rio de Janeiro, Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guedes, Eliane; Heilbron, Monica; de Morisson Valeriano, Claudio; de Almeida, Julio César Horta; Szatmari, Peter</p> <p>2016-04-01</p> <p>Continental flood basalts and <span class="hlt">dike</span> swarm have been related to continental breakup process through geological time. The Resende - Ilha Grande <span class="hlt">Dike</span> swarm (RIGDS) located in the southeast Brazil, is related the Gondwana breakup and composed of <span class="hlt">dikes</span>/sills intruded in Precambrian gneiss. The <span class="hlt">dikes</span> have three distinguish orientations: NNW more inland; NS-NNE in the central segment and NE orientation in the coast line, consistent with Precambrian structural lineaments. The swarm comprises high-TiO2 tholeiitic basalts divided into three suites based on REE and Sr and Nd isotope data. The Resende and Volta Redonda suites present higher initial 87Sr/86Sr ratios between 0.7077 and 0.7065, while Angra dos Reis suite presents values of 0.7066 to 0.7057. Geochemical and isotopic data support the sub-continental lithospheric mantle (SCLM) as the main source for the high-TiO2 basalts. The suites heterogeneities are explained by different compositions of SCLM in accreted Precambrian terranes and/or different degree of partial melting and fractional. 40Ar/39Ar data indicate age interval between ca. 156 to 144 Ma for the swarm, older than the average for Gondwana breakup (ca. 130-120 Ma). The age interval places the RIGDS between the Karoo magmatism (181-178 Ma) and the Paraná-Etendeka magmatism (133-134 Ma) and indicates that extensional process affected the supercontinent prior the break-up.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S31B2232B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S31B2232B"><span>Seismogenic structures activated during the pre-eruptive and <span class="hlt">intrusive</span> swarms of Piton de la Fournaise volcano (La Réunion island) between 2008 and 2011</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Battaglia, J.; Brenguier, F.</p> <p>2011-12-01</p> <p>Piton de la Fournaise is a frequently active basaltic volcano with more than 30 fissure eruptions since 1998. These eruptions are always preceded by pre-eruptive swarms of volcano-tectonic earthquakes which accompany <span class="hlt">dike</span> propagation. Occasionally, <span class="hlt">intrusion</span> swarms occur without leading to any eruption. From October 2008 to May 2011, as part of the research project Undervolc, a temporary network of 15 broadband stations has been installed on the volcano to complement the local monitoring network. We examined in detail the 6 <span class="hlt">intrusive</span> and 5 pre-eruptive swarms which occurred during the temporary experiment. All the crises lasted for a few hours and only included shallow events clustered below the summit craters, around and above sea level, showing no signs of deeper magma transfers. These characteristics are common to most swarms observed at Piton de la Fournaise arising questions about the origin of the seismicity which seems to be poorly linked with <span class="hlt">dike</span> propagation. With the aim to identify the main seismogenic structures active during the swarms, we applied precise earthquake detection and classification techniques based on waveform cross-correlation. For each swarm, the onsets of all transients, including small amplitude ones, have been precisely detected at a single station by scanning the continuous data with reference waveforms. The classification of the detected transients indicates the presence of several families of similar earthquakes. The two main families (F01 and F02) include several hundred events. They are systematically activated at the beginning of each pre-eruptive swarm but are inactive during the <span class="hlt">intrusive</span> ones. They group more than 50 percent of the detected events for the corresponding crises. The other clusters are mostly associated with single swarms. To determine the spatial characteristics of the structures corresponding to the main families, we applied precise relocation techniques. Based on the one-station classification, the events</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3505Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3505Z"><span>Application of interleaving models to describe <span class="hlt">intrusive</span> layers in the Deep Polar Water of the Arctic Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhurbas, Nataliya; Kuzmina, Natalia; Lyzhkov, Dmitry; Izvekova, Yulia N.</p> <p>2016-04-01</p> <p>Interleaving models of pure thermohaline and baroclinic frontal <span class="hlt">zones</span> of finite width are applied to describe <span class="hlt">intrusions</span> at the fronts found in the upper part of the Deep Polar Water, the Eurasian basin, under stable-stable thermohaline stratification. It is assumed that differential mixing is the main mechanism of the <span class="hlt">intrusion</span> formation. Different parameterizations of differential mixing (Merrryfield, 2002; Kuzmina et al., 2011) are used in the models. Important parameters of interleaving such as the growth rate, vertical scale, and slope of the most unstable modes are calculated. It is found that the interleaving model of a pure thermohaline front can satisfactory describe the important parameters of <span class="hlt">intrusions</span> observed at a thermohaline, very low baroclinicity front in the Eurasian basin, just in accordance to Merryfield (2002) findings. In the case of baroclinic front, satisfactory agreement over all the interleaving parameters is found between the model calculations and observations provided that the vertical momentum diffusivity significantly exceeds the corresponding mass diffusivity. Under specific (reasonable) constraints of the vertical momentum diffusivity, the most unstable mode has a vertical scale approximately two-three times smaller than the vertical scale of the observed <span class="hlt">intrusions</span>. A thorough discussion of the results is presented. References Kuzmina N., Rudels B., Zhurbas V., Stipa T. On the structure and dynamical features of <span class="hlt">intrusive</span> layering in the Eurasian Basin in the Arctic Ocean. J. Geophys. Res., 2011, 116, C00D11, doi:10.1029/2010JC006920. Merryfield W. J. <span class="hlt">Intrusions</span> in Double-Diffusively Stable Arctic Waters: Evidence for Differential mixing? J. Phys. Oceanogr., 2002, 32, 1452-1439.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V13C2607G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V13C2607G"><span>Geologic Mapping in Nogal Peak Quadrangle: Geochemistry, <span class="hlt">Intrusive</span> Relations and Mineralization in the Sierra Blanca Igneous Complex, New Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goff, F.; Kelley, S. A.; Lawrence, J. R.; Cikowski, C. T.; Krier, D. J.; Goff, C. J.; McLemore, V. T.</p> <p>2011-12-01</p> <p>Nogal Peak quadrangle is located in the northern Sierra Blanca Igneous Complex (SBIC) and contains most of the White Mountain Wilderness (geologic map is available at http://geoinfo.nmt.edu/publications/maps/geologic/ofgm/details.cfml?Volume=134). The geology of the quad consists of a late Eocene to Oligocene volcanic pile (Sierra Blanca Volcanics, mostly alkali basalt to trachyte) intruded by a multitude of <span class="hlt">dikes</span>, plugs and three stocks: Rialto, 31.4 Ma (mostly syenite), Three Rivers, ca. 29 to 27 Ma (quartz syenite intruded by subordinate alkali granite), and Bonito Lake, 26.6 Ma (mostly monzonite). Three Rivers stock is partially surrounded by alkali rhyolites that geochemically resemble the alkali granites. The circular shape of the stock and surrounding rhyolites suggests they form the root of a probable caldera. SBIC rocks have compositions typical of those found within the Rocky Mountain alkaline belt and those associated with continental rift <span class="hlt">zone</span> magmatism. Because the volcanic host rocks are deeply eroded, <span class="hlt">intrusive</span> relations with the stocks are well exposed. Most contacts at stock margins are near vertical. Roof pendants are common near some contacts and stoped blocks up to 700 m long are found within the Three Rivers stock. Contacts, pendants and stoped blocks generally display some combination of hornfelsing, brecciation, fracturing, faulting and mineralization. Sierra Blanca Volcanics display hydrothermal alteration increasing from argillic in the NW sector of the quad to high-temperature porpylitic near stock margins. Retrograde phyllic alteration occurs within breccia pipes and portions of the stocks. Mineral deposits consist of four types: Placer Au, fissure veins (mostly Ag-Pb-Zn±Au), breccia pipes (Au-Mo-Cu), and porphyry Mo-Cu. A singular pipe on the SW margin of Bonito Lake stock contains sapphire-lazulite-alunite. Although Au has been intermittently mined in the quad since 1865, best production of Au originated around the turn of the last</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoRL..42.1758B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoRL..42.1758B"><span>Pressurized magma reservoir within the east rift <span class="hlt">zone</span> of Kīlauea Volcano, Hawai`i: Evidence for relaxed stress changes from the 1975 Kalapana earthquake</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baker, Scott; Amelung, Falk</p> <p>2015-03-01</p> <p>We use 2000-2012 InSAR data from multiple satellites to investigate magma storage in Kīlauea's east rift <span class="hlt">zone</span> (ERZ). The study period includes a surge in magma supply rate and <span class="hlt">intrusion</span>-eruptions in 2007 and 2011. The Kupaianaha area inflated by ~5 cm prior to the 2007 <span class="hlt">intrusion</span> and the Nāpau Crater area by ~10 cm following the 2011 <span class="hlt">intrusion</span>. For the Nāpau Crater area, elastic modeling suggests an inflation source at 5 ± 2 km depth or more below sea level. The reservoir is located in the deeper section of the rift <span class="hlt">zone</span> for which secular magma <span class="hlt">intrusion</span> was inferred for the period following the 1975 Mw7.7 décollement earthquake. Reservoir pressurization suggests that in this section of the ERZ, extensional stress changes due to the earthquake have largely been compensated for and that this section is approaching its pre-1975 state. Reservoir pressurization also puts the molten core model into question for this section of Kīlauea's rift <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033567','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033567"><span>Igneous phenocrystic origin of K-feldspar megacrysts in granitic rocks from the Sierra Nevada batholith</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Moore, J.G.; Sisson, T.W.</p> <p>2008-01-01</p> <p>Study of four K-feldspar megacrystic granitic plutons and related <span class="hlt">dikes</span> in the Sierra Nevada composite batholith indicates that the megacrysts are phenocrysts that grew in contact with granitic melt. Growth to megacrystic sizes was due to repeated replenishment of the magma bodies by fresh granitic melt that maintained temperatures above the solidus for extended time periods and that provided components necessary for K-feldspar growth. These <span class="hlt">intrusions</span> cooled 89-83 Ma, are the youngest in the range, and represent the culminating magmatic phase of the Sierra Nevada batholith. They are the granodiorite of Topaz Lake, the Cathedral Peak Granodiorite, the Mono Creek Granite, the Whitney Granodiorite, the Johnson Granite Porphyry, and the Golden Bear <span class="hlt">Dike</span>. Megacrysts in these igneous bodies attain 4-10 cm in length. All have sawtooth oscillatory <span class="hlt">zoning</span> marked by varying concentration of BaO ranging generally from 3.5 to 0.5 wt%. Some of the more pronounced <span class="hlt">zones</span> begin with resorption and channeling of the underlying <span class="hlt">zone</span>. Layers of mineral inclusions, principally plagioclase, but also biotite, quartz, hornblende, titanite, and accessory minerals, are parallel to the BaO-delineated <span class="hlt">zones</span>, are sorted by size along the boundaries, and have their long axes preferentially aligned parallel to the boundaries. These features indicate that the K-feldspar megacrysts grew while surrounded by melt, allowing the inclusion minerals to periodically attach themselves to the faces of the growing crystals. The temperature of growth of titanite included within the K-feldspar megacrysts is estimated by use of a Zr-in-titanite geothermometer. Megacryst-hosted titanite grains all yield temperatures typical of felsic magmas, mainly 735-760 ??C. Titanite grains in the granodiorite hosts marginal to the megacrysts range to lower growth temperatures, in some instances into the subsolidus. The limited range and igneous values of growth temperatures for megacryst-hosted titanite grains support the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4222060','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4222060"><span>Characterization and Remediation of Chlorinated Volatile Organic Contaminants in the Vadose <span class="hlt">Zone</span>: An Overview of Issues and Approaches</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Brusseau, Mark L.; Carroll, Kenneth C.; Truex, Michael J.; Becker, David J.</p> <p>2014-01-01</p> <p>Contamination of vadose-<span class="hlt">zone</span> systems by chlorinated solvents is widespread, and poses significant potential risk to human health through impacts on groundwater quality and vapor <span class="hlt">intrusion</span>. Soil vapor extraction (SVE) is the presumptive remedy for such contamination, and has been used successfully for innumerable sites. However, SVE operations typically exhibit reduced mass-removal effectiveness at some point due to the impact of poorly accessible contaminant mass and associated mass-transfer limitations. Assessment of SVE performance and closure is currently based on characterizing contaminant mass discharge associated with the vadose-<span class="hlt">zone</span> source, and its impact on groundwater or vapor <span class="hlt">intrusion</span>. These issues are addressed in this overview, with a focus on summarizing recent advances in our understanding of the transport, characterization, and remediation of chlorinated solvents in the vadose <span class="hlt">zone</span>. The evolution of contaminant distribution over time and the associated impacts on remediation efficiency will be discussed, as will the potential impact of persistent sources on groundwater quality and vapor <span class="hlt">intrusion</span>. In addition, alternative methods for site characterization and remediation will be addressed. PMID:25383058</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/1988/4171/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/1988/4171/report.pdf"><span>Potential for saltwater <span class="hlt">intrusion</span> into the Upper Floridan aquifer, Hernando and Manatee counties, Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mahon, G.L.</p> <p>1989-01-01</p> <p>Pumpage from the Upper Floridan aquifer has caused a lowering of the potentiometric surface and has increased potential for saltwater <span class="hlt">intrusion</span> into the aquifer in coastal areas of west-central Florida. Groundwater withdrawals are likely to increase because of expected population growth, especially in coastal areas. To increase the understanding of the potential and mechanics of saltwater <span class="hlt">intrusion</span>, two sites were selected for study. Data were collected at each site from a centrally located deep well, and digital models were developed to simulate groundwater flow and solute transport. The northern site is in Hernando County near the town of Aripeka. The test well in the area was drilled about 1 mile from the coast to a depth of 820 ft. Freshwater was present in the carbonate rock aquifer to a depth of about 500 ft and saltwater occurred from 560 ft to the base of the aquifer at about 750 ft. Between the freshwater and saltwater is the <span class="hlt">zone</span> of transition, also referred to as the freshwater-saltwater interface. The southern site is in Manatee County near the town of Rubonia. Drilling of the test well was completed at 1,260 ft, just below the base of the Upper Floridan aquifer. The transition <span class="hlt">zone</span> in this well occurs between 875 and 975 ft within a highly permeable <span class="hlt">zone</span>. Digital simulations show flow patterns similar to the cyclic flow of seawater and interface theory. Simulations have shown that saltwater contamination of coastal wells would not be noticed as quickly as water-level declines resulting from inland pumpage. (USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015678','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015678"><span>Isotopic variation in the Tuolumne <span class="hlt">Intrusive</span> Suite, central Sierra Nevada, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kistler, R.W.; Chappell, B.W.; Peck, D.L.; Bateman, P.C.</p> <p>1986-01-01</p> <p>Granitoid rocks of the compositionally <span class="hlt">zoned</span> Late Cretaceous Toulumne <span class="hlt">Intrusive</span> Suite in the central Sierra Nevada, California, have initial87Sr/86Sr values (Sri) and143Nd/144Nd values (Ndi) that vary from 0.7057 to 0.7067 and from 0.51239 to 0.51211 respectively. The observed variation of both Sri and Ndi and of chemical composition in rocks of the suite cannot be due to crystal fractionation of magma solely under closed system conditons. The largest variation in chemistry, Ndi, and Sri is present in the outer-most equigranular units of the Tuolumne <span class="hlt">Intrusive</span> Suite. Sri varies positively with SiO2, Na2O, K2O, and Rb concentrations, and negatively with Ndi, Al2O3, Fe2O3, MgO, FeO, CaO, MnO, P2O5, TiO2, and Sr concentrations. This covariation of Sri, Ndi and chemistry can be modeled by a process of simple mixing of basaltic and granitic magmas having weight percent SiO2 of 48.0 and 73.3 respectively. Isotopic characteristic of the mafic magma are Sri=0.7047, Ndi=0.51269 and ??18O=6.0, and of the felsic magma are Sri=0.7068, Ndi=0.51212 and ??18O=8.9. The rocks sampled contain from 50 to 80% of the felsic component. An aplite in the outer equigranular unit of the Tuolumne <span class="hlt">Intrusive</span> Suite apparently was derived by fractional crystallization of plagioclase and hornblende from magma with granudiorite composition that was a product of mixing of the magmas described above. Siliceous magmas derived from the lower crust, having a maximum of 15 percent mantle-derived mafic component, are represented by the inner prophyritic units of the Tuolumne <span class="hlt">Intrusive</span> Suite. ?? 1986 Springer-Verlag.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010fgcn.conf...93J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010fgcn.conf...93J"><span><span class="hlt">Intrusion</span> Detection in Database Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Javidi, Mohammad M.; Sohrabi, Mina; Rafsanjani, Marjan Kuchaki</p> <p></p> <p>Data represent today a valuable asset for organizations and companies and must be protected. Ensuring the security and privacy of data assets is a crucial and very difficult problem in our modern networked world. Despite the necessity of protecting information stored in database systems (DBS), existing security models are insufficient to prevent misuse, especially insider abuse by legitimate users. One mechanism to safeguard the information in these databases is to use an <span class="hlt">intrusion</span> detection system (IDS). The purpose of <span class="hlt">Intrusion</span> detection in database systems is to detect transactions that access data without permission. In this paper several database <span class="hlt">Intrusion</span> detection approaches are evaluated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.jstor.org/stable/44113190','USGSPUBS'); return false;" href="http://www.jstor.org/stable/44113190"><span>Saltwater <span class="hlt">intrusion</span> monitoring in Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prinos, Scott T.</p> <p>2016-01-01</p> <p>Florida's communities are largely dependent on freshwater from groundwater aquifers. Existing saltwater in the aquifers, or seawater that intrudes parts of the aquifers that were fresh, can make the water unusable without additional processing. The quality of Florida's saltwater <span class="hlt">intrusion</span> monitoring networks varies. In Miami-Dade and Broward Counties, for example, there is a well-designed network with recently constructed short open-interval monitoring wells that bracket the saltwater interface in the Biscayne aquifer. Geochemical analyses of water samples from the network help scientists evaluate pathways of saltwater <span class="hlt">intrusion</span> and movement of the saltwater interface. Geophysical measurements, collected in these counties, aid the mapping of the saltwater interface and the design of monitoring networks. In comparison, deficiencies in the Collier County monitoring network include the positioning of monitoring wells, reliance on wells with long open intervals that when sampled might provide questionable results, and the inability of existing analyses to differentiate between multiple pathways of saltwater <span class="hlt">intrusion</span>. A state-wide saltwater <span class="hlt">intrusion</span> monitoring network is being planned; the planned network could improve saltwater <span class="hlt">intrusion</span> monitoring by adopting the applicable strategies of the networks of Miami-Dade and Broward Counties, and by addressing deficiencies such as those described for the Collier County network.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030828','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030828"><span>High-precision U-Pb geochronology in the Minnesota River Valley subprovince and its bearing on the Neoarchean to Paleoproterozoic evolution of the southern Superior Province</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Schmitz, M.D.; Bowring, S.A.; Southwick, D.L.; Boerboom, Terrence; Wirth, K.R.</p> <p>2006-01-01</p> <p>High-precision U-Pb ages have been obtained for high-grade gneisses, late-kinematic to postkinematic granitic plutons, and a crosscutting mafic <span class="hlt">dike</span> of the Archean Minnesota River Valley tectonic subprovince, at the southern ramparts of the Superior craton of North America. The antiquity of the Minnesota River Valley terranes is confirmed by a high-precision U-Pb zircon age of 3422 ?? 2 Ma for a tonalitic phase of the Morton Gneiss. Voluminous, late-kinematic monzogranites of the Benson (Ortonville granite) and Morton (Sacred Heart granite) blocks yield identical crystallization ages of 2603 ?? 1 Ma, illustrating the synchrony and rapidity of deep crustal melting and plutonism throughout the Minnesota River Valley terranes. Postkinematic, 2591 ?? 2 Ma syenogranites and aplitic <span class="hlt">dikes</span> in both blocks effectively constrain the final penetrative deformation of the Minnesota River Valley subprovince. Monazite growth from 2609 to 2595 Ma in granulitic paragneisses of the Benson and Montevideo blocks is interpreted to record prograde to peak granulite facies metamorphic conditions associated with crustal thickening and magmatism. Neoarchean metamorphism and plutonism are interpreted to record the timing of collisional accretion and terminal suturing of the Mesoarchean continental Minnesota River Valley terranes to the southern margin of the Superior Province, along the western Great Lakes tectonic <span class="hlt">zone</span>. Subsequent Paleoproterozoic rifting of this margin is recorded by voluminous basaltic <span class="hlt">dike</span> <span class="hlt">intrusion</span>, expressed in the Minnesota River Valley by major WNW-trending tholeiitic diabase <span class="hlt">dikes</span> dated at 2067 ?? 1 Ma, only slightly younger than the structurally and geochemically similar 2077 ?? 4 Ma Fort Frances (Kenora-Kabetogama) <span class="hlt">dike</span> swarm of northern Minnesota and adjoining Canada. ?? 2006 Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29195195','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29195195"><span>Economic impacts of urban flooding in South Florida: Potential consequences of managing groundwater to prevent salt water <span class="hlt">intrusion</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Czajkowski, Jeffrey; Engel, Vic; Martinez, Chris; Mirchi, Ali; Watkins, David; Sukop, Michael C; Hughes, Joseph D</p> <p>2018-04-15</p> <p>High-value urban <span class="hlt">zones</span> in coastal South Florida are considered particularly vulnerable to salt water <span class="hlt">intrusion</span> into the groundwater-based, public water supplies caused by sea level rise (SLR) in combination with the low topography, existing high water table, and permeable karst substrate. Managers in the region closely regulate water depths in the extensive South Florida canal network to control closely coupled groundwater levels and thereby reduce the risk of saltwater <span class="hlt">intrusion</span> into the karst aquifer. Potential SLR adaptation strategies developed by local managers suggest canal and groundwater levels may have to be increased over time to prevent the increased salt water <span class="hlt">intrusion</span> risk to groundwater resources. However, higher canal and groundwater levels cause the loss of unsaturated <span class="hlt">zone</span> storage and lead to an increased risk of inland flooding when the recharge from rainfall exceeds the capacity of the unsaturated <span class="hlt">zone</span> to absorb it and the water table reaches the surface. Consequently, higher canal and groundwater levels are also associated with increased risk of economic losses, especially during the annual wet seasons. To help water managers and urban planners in this region better understand this trade-off, this study models the relationships between flood insurance claims and groundwater levels in Miami-Dade County. Via regression analyses, we relate the incurred number of monthly flood claims in 16 Miami-Dade County watersheds to monthly groundwater levels over the period from 1996 to 2010. We utilize these estimated statistical relationships to further illustrate various monthly flood loss scenarios that could plausibly result, thereby providing an economic quantification of a "too much water" trade-off. Importantly, this understanding is the first of its kind in South Florida and is exceedingly useful for regional-scale hydro-economic optimization models analyzing trade-offs associated with high water levels. Copyright © 2017 Elsevier B.V. All rights</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018709','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018709"><span>Layered <span class="hlt">intrusions</span> of the Duluth Complex, Minnesota, USA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Miller, J.D.; Ripley, E.M.; ,</p> <p>1996-01-01</p> <p>The Duluth Complex and associated subvolcanic <span class="hlt">intrusions</span> comprise a large (5000 km2) <span class="hlt">intrusive</span> complex in northeastern Minnesota that was emplaced into comagmatic volcanics during the development of the 1.1 Ga Midcontinent rift in North America. In addition to anorthositic and felsic <span class="hlt">intrusions</span>, the Duluth Complex is composed of many individual mafic layered <span class="hlt">intrusions</span> of tholeiitic affinity. The cumulate stratigraphies and cryptic variations of six of the better exposed and better studied <span class="hlt">intrusions</span> are described here to demonstrate the variability in their cumulus mineral paragenesis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29755136','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29755136"><span>Ring faults and ring <span class="hlt">dikes</span> around the Orientale basin on the Moon.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Andrews-Hanna, Jeffrey C; Head, James W; Johnson, Brandon; Keane, James T; Kiefer, Walter S; McGovern, Patrick J; Neumann, Gregory A; Wieczorek, Mark A; Zuber, Maria T</p> <p>2018-08-01</p> <p>The Orientale basin is the youngest and best-preserved multiring impact basin on the Moon, having experienced only modest modification by subsequent impacts and volcanism. Orientale is often treated as the type example of a multiring basin, with three prominent rings outside of the inner depression: the Inner Rook Montes, the Outer Rook Montes, and the Cordillera. Here we use gravity data from NASA's Gravity Recovery and Interior Laboratory (GRAIL) mission to reveal the subsurface structure of Orientale and its ring system. Gradients of the gravity data reveal a continuous ring <span class="hlt">dike</span> intruded into the Outer Rook along the plane of the fault associated with the ring scarp. The volume of this ring <span class="hlt">dike</span> is ~18 times greater than the volume of all extrusive mare deposits associated with the basin. The gravity gradient signature of the Cordillera ring indicates an offset along the fault across a shallow density interface, interpreted to be the base of the low-density ejecta blanket. Both gravity gradients and crustal thickness models indicate that the edge of the central cavity is shifted inward relative to the equivalent Inner Rook ring at the surface. Models of the deep basin structure show inflections along the crust-mantle interface at both the Outer Rook and Cordillera rings, indicating that the basin ring faults extend from the surface to at least the base of the crust. Fault dips range from 13-22° for the Cordillera fault in the northeastern quadrant, to 90° for the Outer Rook in the northwestern quadrant. The fault dips for both outer rings are lowest in the northeast, possibly due to the effects of either the direction of projectile motion or regional gradients in pre-impact crustal thickness. Similar ring <span class="hlt">dikes</span> and ring faults are observed around the majority of lunar basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title49-vol6/pdf/CFR-2010-title49-vol6-sec571-219.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title49-vol6/pdf/CFR-2010-title49-vol6-sec571-219.pdf"><span>49 CFR 571.219 - Standard No. 219; Windshield <span class="hlt">zone</span> <span class="hlt">intrusion</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-10-01</p> <p>... contact with the windshield, shall penetrate the protected <span class="hlt">zone</span> template, affixed according to S6, to a... simultaneously contacts the inner surface of the windshield glazing and the surface of the instrument panel... surface of the windshield. (c) The locus of lines forming a 45° angle with the outer surface of the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028400','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028400"><span>Protolith and metamorphic ages of the Haiyangsuo Complex, eastern China: A non-UHP exotic tectonic slab in the Sulu ultrahigh-pressure terrane</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Liou, J.G.; Tsujimori, T.; Chu, W.; Zhang, R.Y.; Wooden, J.L.</p> <p>2006-01-01</p> <p>The Haiyangsuo Complex in the NE Sulu ultrahigh-pressure (UHP) terrane has discontinuous, coastal exposures of Late Archean gneiss with amphibolitized granulite, amphibolite, Paleoproterozoic metagabbroic <span class="hlt">intrusives</span>, and Cretaceous granitic <span class="hlt">dikes</span> over an area of about 15 km2. The U-Pb SHRIMP dating of zircons indicates that theprotolith age of a garnet-biotite gneiss is >2500 Ma, whereas the granulite-facie metamorphism occurred at around 1800 Ma. A gabbroic <span class="hlt">intrusion</span> was dated at ???1730 Ma, and the formation of amphibolite-facies assemblages in both metagabbro and granulite occurred at ???340-460 Ma. Petrologic and geochronological data indicate that these various rocks show no evidence of Triassic eclogite-facies metamorphism and Neoproterozoic protolith ages that are characteristics of Sulu-Dabie HP-UHP rocks, except Neoproterozoic inherited ages from post-collisional Jurassic granitic <span class="hlt">dikes</span>. Haiyangsuo retrograde granulites with amphibolite-facies assemblages within the gneiss preserve relict garnet formed during granulite-facies metamorphism at ???1.85 Ga. The Paleoproterozoic metamorphic events are almost coeval with gabbroic <span class="hlt">intrusions</span>. The granulite-bearing gneiss unit and gabbro-dominated unit of the Haiyangsuo Complex were intruded by thin granitic <span class="hlt">dikes</span> at about 160 Ma, which is coeval with post-collisional granitic <span class="hlt">intrusions</span> in the Sulu terrane. We suggest that the Haiyangsuo Complex may represent a fragment of the Jiao-Liao-Ji Paleoproterozoic terrane developed at the eastern margin of the Sino-Korean basement, which was juxtaposed with the Sulu terrane prior to Jurassic granitic activity and regional deformation. ?? Springer-Verlag 2006.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1984CoMP...86..386H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1984CoMP...86..386H"><span>A transitional alkalic dolerite <span class="hlt">dike</span> suite of Mesozoic age in Southeastern New England</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hermes, O. Don; Rao, J. M.; Dickenson, M. P.; Pierce, T. A.</p> <p>1984-12-01</p> <p><span class="hlt">Dike</span> rocks from the New England platform of Rhode Island and adjacent Massachusetts consist of premetamorphic and post-metamorphic suites. The older group includes metamorphosed dolerite, minette, and schistose dioritic rocks. Post-metamorphic <span class="hlt">dikes</span> consist of dolerite and sparse monchiquite. The post-metamorphic dolerites are of comparable age to the Eastern North American dolerite suite associated with the Mesozoic basins along the eastern seaboard of North America. However, the southeastern New England dolerites exhibit mineralogy and chemistry more typical of a transitional alkalic suite compared to the more subalkalic tholeiitic dolerites of the Eastern North American suite. Both suites are compatible with a rift tectonic setting, but the more alkalic dolerites may represent a deeper source of small volume melts compared to the Eastern North American dolerites. These more alkaline melts may have concentrated at local centers, or they may be typical of flank dolerites as opposed to the less alkalic varieties that occur within the central axial rift.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1983E%26PSL..66..243R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1983E%26PSL..66..243R"><span>Magma mixing in granitic rocks of the central Sierra Nevada, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reid, John B.; Evans, Owen C.; Fates, Dailey G.</p> <p>1983-12-01</p> <p>The El Capitan alaskite exposed in the North American Wall, Yosemite National Park, was intruded by two sets of mafic <span class="hlt">dikes</span> that interacted thermally and chemically with the host alaskite. Comparisons of petrographic and compositional data for these <span class="hlt">dikes</span> and alaskite with published data for Sierra Nevada plutons lead us to suggest that mafic magmas were important in the generation of the Sierra Nevada batholith. Specifically, we conclude that: (1) <span class="hlt">intrusion</span> of mafic magmas in the lower crust caused partial melting and generation of alaskite (rhyolitic) magmas; (2) interaction between the mafic and felsic magmas lead to the observed linear variation diagrams for major elements; (3) most mafic inclusions in Sierra Nevada plutons represent chilled pillows of mafic magmas, related by fractional crystallization and granitoid assimilation, that dissolve into their felsic host and contaminate it to intermediate (granodioritic) compositions; (4) vesiculation of hydrous mafic magma upon chilling may allow buoyant mafic inclusions and their disaggregation products to collect beneath a pluton's domed ceiling causing the <span class="hlt">zoning</span> (mafic margins-to-felsic core) that these plutons exhibit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70009726','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70009726"><span>InSAR observations of deformation associated with new episodes of volcanism at Kilauea Volcano, Hawai'i, 2007</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Poland, Michael P.</p> <p>2008-01-01</p> <p>In June 2007, the Pu'u 'Ō'ō-Kūpaianaha eruption of Kīlauea Volcano was interrupted when magma intruded the east rift <span class="hlt">zone</span> (ERZ), resulting in a small extrusion of lava near Makaopuhi Crater. Deformation associated with the activity was exceptionally well-documented by ASAR interferometry, which indicates deflation of the summit and uplift and extension of the ERZ. Models of co-<span class="hlt">intrusion</span> interferograms suggest that the <span class="hlt">dike</span> was emplaced in two distinct segments. The modeled volume of the <span class="hlt">dike</span> greatly exceeds that of the deflation source, raising the possibility that magma from the downrift Pu'u 'Ō'ō vent (dominant extrusion site at Kīlauea since 1983) contributed to the eruption near Makaopuhi, or that the magma that fed the eruption from the summit was compressible. A month following the Makaopuhi eruption, an eruptive fissure opened on the east flank of Pu'u 'Ō'ō. Interferograms, processed within 48 hours of the event, were critical in demonstrating that the magma source feeding the eruption was shallow. The eruption probably resulted from overpressure in Pu'u 'Ō'ō's magmatic system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1086408-imaging-high-stage-river-water-intrusion-contaminated-aquifer-along-major-river-corridor-using-time-lapse-surface-electrical-resistivity-tomography','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1086408-imaging-high-stage-river-water-intrusion-contaminated-aquifer-along-major-river-corridor-using-time-lapse-surface-electrical-resistivity-tomography"><span>Imaging high stage river-water <span class="hlt">intrusion</span> into a contaminated aquifer along a major river corridor using 2D time-lapse surface electrical resistivity tomography</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Wallin, Erin L.; Johnson, Timothy C.; Greenwood, William J.</p> <p>2013-03-29</p> <p>The Hanford 300 Area is located adjacent to the Columbia River in south-central Washington State, USA, and was a former site for nuclear fuel processing operations. Waste disposal practices resulted in persistent unsaturated <span class="hlt">zone</span> and groundwater contamination, the primary contaminant of concern being uranium. Uranium behavior at the site is intimately linked with river stage driven groundwater-river water exchange such that understanding the nature of river water <span class="hlt">intrusion</span> into the 300 Area is critical for predicting uranium desorption and transport. In this paper we use time-lapse electrical resistivity tomography (ERT) to image the inland <span class="hlt">intrusion</span> of river during high stagemore » conditions. We demonstrate a modified time-lapse inversion approach, whereby the transient water table elevation is explicitly modeled by removing regularization constraints across the water table boundary. This implementation was critical for producing meaningful imaging results. We inverted approximately 1200 data sets (400 per line over 3 lines) using high performance computing resources to produce a time-lapse sequence of changes in bulk conductivity caused by river water <span class="hlt">intrusion</span> during the 2011 spring runoff cycle over approximately 125 days. The resulting time series for each mesh element was then analyzed using common time series analysis to reveal the timing and location of river water <span class="hlt">intrusion</span> beneath each line. The results reveal non-uniform flows characterized by preferred flow <span class="hlt">zones</span> where river water enters and exits quickly with stage increase and decrease, and low permeability <span class="hlt">zones</span> with broader bulk conductivity ‘break through’ curves and longer river water residence times. The time-lapse ERT inversion approach removes the deleterious effects of changing water table elevation and enables remote and spatial continuous groundwater-river water exchange monitoring using surface based ERT arrays under conditions where groundwater and river water conductivity are in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17904485','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17904485"><span>From <span class="hlt">intrusive</span> to oscillating thoughts.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peirce, Anne Griswold</p> <p>2007-10-01</p> <p>This paper focused on the possibility that <span class="hlt">intrusive</span> thoughts (ITs) are a form of an evolutionary, adaptive, and complex strategy to prepare for and resolve stressful life events through schema formation. <span class="hlt">Intrusive</span> thoughts have been studied in relation to individual conditions, such as traumatic stress disorder and obsessive-compulsive disorder. They have also been documented in the average person experiencing everyday stress. In many descriptions of thought <span class="hlt">intrusion</span>, it is accompanied by thought suppression. Several theories have been put forth to describe ITs, although none provides a satisfactory explanation as to whether ITs are a normal process, a normal process gone astray, or a sign of pathology. There is also no consistent view of the role that thought suppression plays in the process. I propose that thought <span class="hlt">intrusion</span> and thought suppression may be better understood by examining them together as a complex and adaptive mechanism capable of escalating in times of need. The ability of a biological mechanism to scale up in times of need is one hallmark of a complex and adaptive system. Other hallmarks of complexity, including self-similarity across scales, sensitivity to initial conditions, presence of feedback loops, and system oscillation, are also discussed in this article. Finally, I propose that thought <span class="hlt">intrusion</span> and thought suppression are better described together as an oscillatory cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://fl.water.usgs.gov/Abstracts/wri03_4262_shoemaker.html','USGSPUBS'); return false;" href="http://fl.water.usgs.gov/Abstracts/wri03_4262_shoemaker.html"><span>Potential for saltwater <span class="hlt">intrusion</span> into the lower Tamiami aquifer near Bonita Springs, southwestern Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shoemaker, W. Barclay; Edwards, K. Michelle</p> <p>2003-01-01</p> <p>A study was conducted to examine the potential for saltwater <span class="hlt">intrusion</span> into the lower Tamiami aquifer beneath Bonita Springs in southwestern Florida. Field data were collected, and constant- and variable-density ground-water flow simulations were performed that: (1) spatially quantified modern and seasonal stresses, (2) identified potential mechanisms of saltwater <span class="hlt">intrusion</span>, and (3) estimated the potential extent of saltwater <span class="hlt">intrusion</span> for the area of concern. MODFLOW and the inverse modeling routine UCODE were used to spatially quantify modern and seasonal stresses by calibrating a constant-density ground-water flow model to field data collected in 1996. The model was calibrated by assuming hydraulic conductivity parameters were accurate and by estimating unmonitored ground-water pumpage and potential evapotranspiration with UCODE. Uncertainty in these estimated parameters was quantified with 95-percent confidence intervals. These confidence intervals indicate more uncertainty (or less reliability) in the estimates of unmonitored ground-water pumpage than estimates of pan-evaporation multipliers, because of the nature and distribution of observations used during calibration. Comparison of simulated water levels, streamflows, and net recharge with field data suggests the model is a good representation of field conditions. Potential mechanisms of saltwater <span class="hlt">intrusion</span> into the lower Tamiami aquifer include: (1) lateral inland movement of the freshwater-saltwater interface from the southwestern coast of Florida; (2) upward leakage from deeper saline water-bearing <span class="hlt">zones</span> through natural upwelling and upconing, both of which could occur as diffuse upward flow through semiconfining layers, conduit flow through karst features, or pipe flow through leaky artesian wells; (3) downward leakage of saltwater from surface-water channels; and (4) movement of unflushed pockets of relict seawater. Of the many potential mechanisms of saltwater <span class="hlt">intrusion</span>, field data and variable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/vaporintrusion','PESTICIDES'); return false;" href="https://www.epa.gov/vaporintrusion"><span>Vapor <span class="hlt">Intrusion</span></span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>Vapor <span class="hlt">intrusion</span> occurs when there is a migration of volatile chemicals from contaminated groundwater or soil into an overlying building. Volatile chemicals can emit vapors that may migrate through subsurface soils and into indoor air spaces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V51C2689A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V51C2689A"><span>Drilling the Bushveld Complex- the world's largest layered mafic <span class="hlt">intrusion</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ashwal, L. D.; Webb, S. J.; Trumbull, R. B.</p> <p>2013-12-01</p> <p>The fact that surprising new discoveries can be made in layered mafic <span class="hlt">intrusions</span> (e.g., subtle 100-150 m cyclicity in apparently homogeneous cumulates over 1000s of m) means that we are still in the first-order characterization phase of understanding these objects. Accordingly, we have secured funding from ICDP for a planning workshop to be held in Johannesburg in early 2014, aimed at scientific drilling of the Bushveld Complex, the world's largest layered mafic <span class="hlt">intrusion</span>. Science objectives include, but are not limited to: 1. Magma chamber processes & melt evolution. How many melts/magmas/mushes were involved, what were their compositions and how did they interact? What, if anything, is missing from the Complex, and where did it go? Did Bushveld magmatism have an effect upon Earth's atmosphere at 2 Ga? 2. Crust-mantle interactions & origin of Bushveld granitoids. Are Bushveld granites & rhyolites crustal melts, differentiates from the mafic magmas or products of immiscibility? How can the evolved isotopic signatures in the mafic rocks (e.g., epsilon Nd to -8) be understood? 3. Origin of ore deposits. What were the relative roles of gravity settling, magma mixing, immiscibility and hydrothermal fluid transport in producing the PGE, Cr and V deposits? We have identified 3 potential drilling targets representing a total of ~12 km of drill core. Exact locations of drill sites are to be discussed at the workshop. Target A- East-Central Bushveld Complex. We propose 3 overlapping 3 km boreholes that will provide the first roof-to-floor continuous coverage of the Rustenburg Layered Suite. These boreholes will represent a curated, internationally available reference collection of Bushveld material for present and future research. Target B- Southeastern Bushveld Complex. We propose a single borehole of ~2 km depth, collared in Rooiberg felsite, and positioned to intersect the Roof <span class="hlt">Zone</span>, Upper <span class="hlt">Zone</span>, Main <span class="hlt">Zone</span> and floor of the Complex. Amongst other things, this site will</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1892c0009H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1892c0009H"><span>Effect of inflow discharges on the development of matric suction and volumetric water content for <span class="hlt">dike</span> during overtopping tests</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hassan, Marwan A.; Ismail, Mohd A. M.</p> <p>2017-10-01</p> <p>The point of this review is to depict the impact of various inflow discharge rate releases on the instruments of matric suction and volumetric water content during an experimental test of spatial overtopping failure at school of civil engineering in universiti Sains of Malaysia. A dry sand <span class="hlt">dike</span> was conducted inside small flume channel with twelve sensors of tensiometer and Time-Domain Reflectometer (TDR). Instruments are installed in the soil at different locations in downstream and upstream slopes of the <span class="hlt">dike</span> for measuring the response of matric suction and volumetric water content, respectively. Two values of inflow discharge rates of 30 and 40 L/min are utilized as a part of these experiments to simulate the effectiveness of water reservoirs in erosion mechanism. The outcomes demonstrate that the matric suction and volumetric water content are decreased and increased, respectively for both inflow discharges. The higher inflow discharges accelerate the saturation of <span class="hlt">dike</span> soil and the erosion process faster than that for the lower inflow discharges.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/bul/1122e/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/bul/1122e/report.pdf"><span>Geology and Fluorspar Deposits of the Levias-Keystone and <span class="hlt">Dike</span>-Eaton Areas, Crittenden County, Kentucky</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Trace, Robert Denny</p> <p>1962-01-01</p> <p>The fault systems of the Levias-Keystone and <span class="hlt">Dike</span>-Eaton areas, in the Kentucky-Illinois fiuorspar district, are a complex northeastward-trending sys- tem and a simple northwestward-trending system of steeply dipping normal faults, associated in part with a lamprophyre <span class="hlt">dike</span>. Fluorspar mining started in the area about 1900 and, as of 1945, more than 200,000 tons of crude ore probably has been mined; most of the ore was from the Levias-Keystone area. A small quantity of zinc and lead ore also is present in the <span class="hlt">Dike</span>-Eaton area. The deposits are localized along faults that displace fiat-lying or low-dipping limestones, sandstones, and shales of the Meramec and Chester series of Missis- sippian age. Movement along most of the faults was principally vertical, with displacement as much as 600 feet. Some horizontal movement occurred along at least one fault. Geologic mapping of the surface and data from underground workings have revealed 13 faults in an area of four-fifths of a square mile. Only a few of these faults are known to contain economically important deposits of fiuorspar. The most abundant vein minerals are calcite and fiuorite with subordinate quantities of sphalerite, galena, barite, and quartz. Some weathering products of sphalerite and galena are present also. The veins are dominantly calcite that contains fiuorite lenses but in places are mainly fiuorite having lesser quantities of calcite. Sphalerite- and galena-bearing deposits are present in the <span class="hlt">Dike</span>-Eaton area. The ore bodies mainly are the result of fissure filling and replacement of calcite by fiuorite; in addition a small amount of limestone wallrock probably has been replaced. Residual concentrations of high-grade fluorspar in the overburden above faults have yielded some so-called gravel fiuorspar. The position of the veins within the faults may be related to one or more factors such as type of wallrock, change in dip of the fault, and amount of displacement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Tecto..34..571H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Tecto..34..571H"><span>Jurassic rifting at the Eurasian Tethys margin: Geochemical and geochronological constraints from granitoids of North Makran, southeastern Iran</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hunziker, Daniela; Burg, Jean-Pierre; Bouilhol, Pierre; von Quadt, Albrecht</p> <p>2015-03-01</p> <p>This study focuses on an east-west trending belt of granitic to intermediate <span class="hlt">intrusions</span> and their volcanic cover in the northern Dur Kan Complex, a continental slice outcropping to the north of the exposed Makran accretionary wedge in southeastern Iran. Field observations, petrographic descriptions, trace element, and isotope analyses combined with U-Pb zircon geochronology are presented to determine the time frame of magmatism and tectonic setting during the formation of these rocks. Results document three magmatic episodes with different melt sources for (1) granites, (2) a diorite-trondhjemite-plagiogranite sequence, and (3) diabases and lavas. Granites, dated at 170-175 Ma, represent crystallized melt with a strong continental isotopic contribution. The diorite-trondhjemite-plagiogranite sequence is 165-153 Ma old and derives from a mantle magma source with minor continental contribution. East-west trending diabase <span class="hlt">dikes</span> and bodies intruded the granitoids, which were eroded and then covered by Valanginian (140-133 Ma) alkaline lavas and sediments. Alkaline <span class="hlt">dikes</span> and lavas have a mantle isotopic composition. Temporal correlation with plutonites of the Sanandaj-Sirjan <span class="hlt">Zone</span> to the northwest defines a narrow, NW-SE striking and nearly 2000 km long belt of Jurassic <span class="hlt">intrusions</span>. The increasing mantle influence in the magma sources is explained by thinning of continental lithosphere and related mantle upwelling/decompression melting. Accordingly, the formation of the studied igneous rocks is related to the extension of the Iranian continental margin, which ultimately led to the formation of the Tethys-related North Makran Ophiolites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189134','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189134"><span>Bokan Mountain peralkaline granitic complex, Alexander terrane (southeastern Alaska): evidence for Early Jurassic rifting prior to accretion with North America</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dostal, Jaroslav; Karl, Susan M.; Keppie, J. Duncan; Kontak, Daniel J.; Shellnutt, J. Gregory</p> <p>2013-01-01</p> <p>The circular Bokan Mountain complex (BMC) on southern Prince of Wales Island, southernmost Alaska, is a Jurassic peralkaline granitic <span class="hlt">intrusion</span> about 3 km in diameter that crosscuts igneous and metasedimentary rocks of the Alexander terrane. The BMC hosts significant rare metal (rare earth elements, Y, U, Th, Zr, and Nb) mineralization related to the last stage of BMC emplacement. U–Pb (zircon) and 40Ar/39Ar (amphibole and whole-rock) geochronology indicates the following sequence of <span class="hlt">intrusive</span> activity: (i) a Paleozoic basement composed mainly of 469 ± 4 Ma granitic rocks; (ii) <span class="hlt">intrusion</span> of the BMC at 177 ± 1 Ma followed by rapid cooling through ca. 550 °C at 176 ± 1 Ma that was synchronous with mineralization associated with vertical, WNW-trending pegmatites, felsic <span class="hlt">dikes</span>, and aegirine–fluorite veins and late-stage, sinistral shear deformation; and (iii) <span class="hlt">intrusion</span> of crosscutting lamprophyre <span class="hlt">dikes</span> at >150 Ma and again at ca. 105 Ma. The peralkaline nature of the BMC and the WNW trend of associated <span class="hlt">dikes</span> suggest <span class="hlt">intrusion</span> during NE–SW rifting that was followed by NE–SW shortening during the waning stages of BMC emplacement. The 177 Ma BMC was synchronous with other magmatic centres in the Alexander terrane, such as (1) the Dora Bay peralkaline stock and (2) the bimodal Moffatt volcanic suite located ∼30 km north and ∼100 km SE of the BMC, respectively. This regional magmatism is interpreted to represent a regional extensional event that precedes deposition of the Late Jurassic – Cretaceous Gravina sequence that oversteps the Wrangellia and Alexander exotic accreted terranes and the Taku and Yukon–Tanana pericratonic terranes of the Canadian–Alaskan Cordillera.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70046292','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70046292"><span>Bokan Mountain peralkaline granitic complex, Alexander terrane (southeastern Alaska): evidence for Early Jurassic rifting prior to accretion with North America</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dostal, Jaroslav; Karl, Susan M.; Keppie, J. Duncan; Kontak, Daniel J.; Shellnutt, J. Gregory</p> <p>2013-01-01</p> <p>The circular Bokan Mountain complex (BMC) on southern Prince of Wales Island, southernmost Alaska, is a Jurassic peralkaline granitic <span class="hlt">intrusion</span> about 3 km in diameter that crosscuts igneous and metasedimentary rocks of the Alexander terrane. The BMC hosts significant rare metal (rare earth elements, Y, U, Th, Zr, and Nb) mineralization related to the last stage of BMC emplacement. U–Pb (zircon) and 40Ar/39Ar (amphibole and whole-rock) geochronology indicates the following sequence of <span class="hlt">intrusive</span> activity: (i) a Paleozoic basement composed mainly of 469 ± 4 Ma granitic rocks; (ii) <span class="hlt">intrusion</span> of the BMC at 177 ± 1 Ma followed by rapid cooling through ca. 550 °C at 176 ± 1 Ma that was synchronous with mineralization associated with vertical, WNW-trending pegmatites, felsic <span class="hlt">dikes</span>, and aegirine–fluorite veins and late-stage, sinistral shear deformation; and (iii) <span class="hlt">intrusion</span> of crosscutting lamprophyre <span class="hlt">dikes</span> at >150 Ma and again at ca. 105 Ma. The peralkaline nature of the BMC and the WNW trend of associated <span class="hlt">dikes</span> suggest <span class="hlt">intrusion</span> during NE–SW rifting that was followed by NE–SW shortening during the waning stages of BMC emplacement. The 177 Ma BMC was synchronous with other magmatic centres in the Alexander terrane, such as (1) the Dora Bay peralkaline stock and (2) the bimodal Moffatt volcanic suite located ~30 km north and ~100 km SE of the BMC, respectively. This regional magmatism is interpreted to represent a regional extensional event that precedes deposition of the Late Jurassic – Cretaceous Gravina sequence that oversteps the Wrangellia and Alexander exotic accreted terranes and the Taku and Yukon–Tanana pericratonic terranes of the Canadian–Alaskan Cordillera.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H13G1482S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H13G1482S"><span>Hysteretic behavior in seawater <span class="hlt">intrusion</span> in response to discontinuous drought periods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salandin, P.; Darvini, G.</p> <p>2017-12-01</p> <p>The seawater <span class="hlt">intrusion</span> (SWI) represents a relevant problem for communities living in many coastal regions and in small islands, where the amount of fresh water available for human consumption or irrigation purposes depends on the equilibrium between the natural groundwater recharge from precipitations and the surrounding sea. This issue is exacerbated by climate changes, and, as a consequence, the reduction of natural groundwater recharge and the decrease the seaward flows of fresh water rather than sea level rise, as recently demonstrated by Ketabchi et al. (2016), leads to magnify the seawater <span class="hlt">intrusion</span> into coastal aquifers. The temporal fluctuation of the fresh water table level are a natural consequence of the interaction of the aquifer with a water body or due to the seasonal replenishment of the water table. The severe and prolonged drought phenomena as that observed in last years in some areas of the Mediterranean, as over the central western Mediterranean basin, Italy and Spain, where a decreasing trend in total precipitation was detected (Alpert et al., 2002) in addition to the rise in temperature, enlarges the variation of the freshwater flux and can magnify the progression of the saline wedge. In the present study we demonstrate that the presence of varying boundary constraints or forcing factors may lead to hysteretic behavior in saltwater <span class="hlt">intrusion</span>, showing dependence of the saline wedge on historic conditions. Therefore, the dynamic behavior of SWI may depend on both the present and past forcing conditions. To this aim different transient simulations supported by evidences deduced from a physical model are carried out to assess the presence of the hysteretic effects in the SWI phenomenon and to evaluate its influence in the management of the coastal aquifers for both the rational exploitation and the corrected management of water resources. About 70% of the world's population dwells in coastal <span class="hlt">zones</span>. Therefore the optimal exploitation of fresh</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V43B4884H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V43B4884H"><span>Geochronological and Petrological Constraints on the Evolution of the Pan African Ajjaj Shear <span class="hlt">Zone</span>, Saudi Arabia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hassan, M.; Stuewe, K.; Abu-Alam, T. S.; Kloetzli, U. S.; Tiepolo, M.</p> <p>2014-12-01</p> <p>In the active tectonic regions, shear <span class="hlt">zones</span> play an important role to re-configure the structure of the lithosphere. One of the largest shear <span class="hlt">zones</span> on the Earth is the Najd Fault System of the Arabian-Nubian Shield. Literature data record the main active phase of this shear <span class="hlt">zone</span> during the last stages of the Pan-African Orogeny (ca. 630 - 540 Ma). The Najd Fault System is composed of several shear <span class="hlt">zone</span> segments, one of them is the Ajjaj shear <span class="hlt">zone</span>. Determination of the age of variably deformed <span class="hlt">intrusions</span> is expected to give approximated age of deformation in Ajjaj shear <span class="hlt">zone</span>. Six samples of <span class="hlt">intrusive</span> rocks showing variable composition were used to illustrate the time progress and evolution of the Ajjaj shear <span class="hlt">zone</span>. One sample is from a very coarse grained diorite lying within the Ajjaj shear <span class="hlt">zone</span>. It has very weak deformation and produces an intercept U-Pb zircon age of 696 ± 6 Ma. Two samples are from granodiorite-tonalite <span class="hlt">intrusions</span> to the tenant of the Ajjaj shear <span class="hlt">zones</span>. They show conspicuous degree of deformation and define two U-Pb clusters of concordia ages at 747 ± 12 Ma - 668 ± 8 Ma and 742 ± 5 Ma - 702 ± 12 Ma. Three samples are granites from variable plutons along the Ajjaj shear <span class="hlt">zone</span>. Two of them show mylonitic foliation of flattened quartz and platy minerals such as biotite parallel to the main deformation trend of the shear <span class="hlt">zone</span>. They yield U-Pb ages of 601 ± 6 Ma - 584 ± 3 Ma. The third sample is undeformed and has a cross-cut contact relationship with the foliation of the Ajjaj shear <span class="hlt">zone</span>. It yield concordia ages of 581 ± 4 Ma. These data confine the activity of the Ajjaj shear <span class="hlt">zone</span> to a limited period between 605 Ma and 577 Ma. As the activity of the Ajjaj shear <span class="hlt">zone</span> was responsible for the exhumation of the Hamadat metamorphic complex, we also constrained the vertical motions that occurred during the shear <span class="hlt">zone</span> activity using mmetamorphic rocks. It is shown that peak metamorphism occurred around 505 - 700 ºC at two ranges of pressure 8 - 11</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V34A..07L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V34A..07L"><span>Source models for the March 5-9, 2011 Kamoamoa fissure eruption, Kilauea Volcano, Hawai`i, constrained by InSAR and in-situ observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lundgren, P.; Poland, M. P.; Miklius, A.; Yun, S.; Fielding, E. J.; Liu, Z.; Tanaka, A.; Szeliga, W. M.; Hensley, S.</p> <p>2011-12-01</p> <p>On March 5, 2011, the Kamoamoa fissure eruption began along the east rift <span class="hlt">zone</span> (ERZ) of Kilauea Volcano. It followed several months of pronounced inflation at Kilauea's summit and was the first <span class="hlt">dike</span> <span class="hlt">intrusion</span> into the ERZ since June 2007. The eruption began in the late afternoon of March 5, 2011 (Hawaii Standard Time; UTC-10:00 hrs) with rapid deflation beginning at Pu'u 'O'o crater along the ERZ and followed about 30 minutes later at the summit. Magma from both locations fed the <span class="hlt">intrusion</span> and an eruption that included lava fountaining along a set of discontinuous eruptive fissures ~2 km in length located between Napau and Pu'u 'O'o craters. Eruptive activity jumped between fissure segments until it ended on the night of March 9. A rich InSAR data set exists for this eruption from the COSMO-SkyMed (CSK), TerraSAR-X (TSX), ALOS PALSAR, and UAVSAR sensors. CSK data acquired on March 7 and processed that same day provided the earliest, quasi-real-time SAR data for this event. By March 10, after the eruption had ended, we had three CSK acquisitions and one ALOS scene acquired and processed. At present we have the following satellite data (UTC dates): ALOS March 6, 9, 11; CSK March 7, 10, 11; TSX March 11; from a mixture of ascending and descending tracks. UAVSAR airborne SAR data were acquired in early May 2011. Preliminary UAVSAR results are encouraging and complete processing should provide high-resolution data from four viewing directions. SAR data were acquired on all days of the eruption but March 8, allowing us to examine the progression of the <span class="hlt">dike</span> opening beneath the surface with excellent spatial and temporal resolution. We use a combination of unwrapped interferograms, azimuthal pixel offsets, and in-situ data from GPS and electronic tiltmeters to model <span class="hlt">dike</span> opening and summit deflation. GPS data are from the Hawaiian Volcano Observatory (HVO) continuous GPS network augmented by campaign occupations closer to the eruption area. Continuous tilt measurements</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002JSAES..15..409S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002JSAES..15..409S"><span>Timing of mafic magmatism in the Tapajós Province (Brazil) and implications for the evolution of the Amazon Craton: evidence from baddeleyite and zircon U Pb SHRIMP geochronology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santos, João Orestes Schneider; Hartmann, Léo Afraneo; McNaughton, Neal Jesse; Fletcher, Ian Robert</p> <p>2002-09-01</p> <p>The precise timing and possible sources of the mafic rocks in the Amazon craton are critical for reconstruction of the Atlantica supercontinent and correlation of mafic magmatism worldwide. New SHRIMP U-Pb baddeleyite and zircon ages and the reinterpretation of 207 existing dates indicate one orogenic (Ingarana) and four postorogenic (Crepori, Cachoeira Seca, Piranhas, and Periquito) basaltic events in the Tapajós Province, south central Amazon craton. Orogenic gabbro <span class="hlt">dikes</span> that host gold mineralization are 1893 Ma and interpreted as associated with the Ingarana gabbro <span class="hlt">intrusions</span> of the bimodal calk-alkalic Parauari <span class="hlt">intrusive</span> suite. The age of 1893 Ma can be used as a guide to discriminate older and mineralized orogenic <span class="hlt">dikes</span> from younger and nonmineralized Crepori- and Cachoeira Seca-related mafic <span class="hlt">dikes</span>. The baddeleyite U-Pb age of the postorogenic Crepori dolerite (gabbro-dolerite sills and <span class="hlt">dikes</span>) is 1780±9 Ma, ˜150 my older than the ages provided by K-Ar. This value correlates well with the Avanavero tholeiitic <span class="hlt">intrusions</span> in the Roraima group, in the northern part of the craton in Guyana, Venezuela, and Roraima in Brazil. Early Statherian tholeiitic magmatism was widespread not only in the Amazon craton, but also in the La Plata craton of southern South America, where it is known as the giant Piedra Alta swarm of Uruguay and the post-Trans-Amazonian <span class="hlt">dikes</span> of Tandil in Argentina. The Cachoeira Seca troctolite represents laccoliths, Feixes, and São Domingos, whose baddeleyite U-Pb age is 1186±12 Ma, 120-150 my older than the known K-Ar ages. This age is comparable to other Stenian gabbroic rocks with alkalic affinity in the craton, such as the Seringa Formation in NE Amazonas and the basaltic flows of the Nova Floresta formation in Rondônia. Dolerite from the giant Piranhas <span class="hlt">dike</span> swarm in the western Tapajós Province has a Middle Cambrian age (507±4 Ma, baddeleyite) and inherited zircons in the 2238-1229 Ma range. The Piranhas <span class="hlt">dikes</span> fill extensional NNE and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918606G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918606G"><span>Consequences of CO2-rich water <span class="hlt">intrusion</span> into the Critical <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gal, Frédérick; Lions, Julie</p> <p>2017-04-01</p> <p>From a geochemical point of view, the sensitivity of the Critical <span class="hlt">Zone</span> to hazards is not only linked to its proximity to the surface. It may also be linked to - albeit less common - <span class="hlt">intrusion</span> of upward migrating fluids. One of the hazard scenarios to observe these pathways in surface environments is the occurrence of CO2-rich fluid leakage from deeper horizons and especially leakage from reservoir in the case of underground storage such as Carbon Storage applications. Much effort is done to prevent this risk but it necessary to consider the mitigation of this leak to insure safe storage. Numerous active or planned CO2 storage sites belong to large sedimentary basins. In that perspective, a CO2 injection has been performed in a multi-layered - carbonated aquifer (Beauce aquifer) from the Paris basin as this basin has been considered for such applications. The aquifer mineralogy of the targeted site is dominated by calcite (95 to 98%) with traces of quartz and clay minerals. Around 10,000 liters of CO2 were injected at 50 m depth during a series of gaseous pulsed injections for 5 days. After 3 days of incubation in the aquifer, the groundwater was pumped during 5 days allowing the recovery of 140 m3 of backward water. Physico-chemical parameters, major and trace elements concentrations and dissolved CO2 concentrations were monitored to evaluate water-rock interactions occurring within the aquifer and impacts onto water quality. Main changes that were observed during the CO2 release are in good agreement with results from previous experiments performed worldwide. A strong decrease of the pH value (2 units), a rise of the electrical conductivity (2 fold) and changes in the redox conditions (from oxidising to less oxidising) are monitored few hours after the initiation of the pumping. The dissolution of CO2 induces a drop of pH that favours water-rock interaction processes. The kinetic of reactions appears to be dominated by the dissolution of carbonate, mainly calcite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/6274833','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/6274833"><span>A system for distributed <span class="hlt">intrusion</span> detection</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Snapp, S.R.; Brentano, J.; Dias, G.V.</p> <p>1991-01-01</p> <p>The study of providing security in computer networks is a rapidly growing area of interest because the network is the medium over which most attacks or <span class="hlt">intrusions</span> on computer systems are launched. One approach to solving this problem is the <span class="hlt">intrusion</span>-detection concept, whose basic premise is that not only abandoning the existing and huge infrastructure of possibly-insecure computer and network systems is impossible, but also replacing them by totally-secure systems may not be feasible or cost effective. Previous work on <span class="hlt">intrusion</span>-detection systems were performed on stand-alone hosts and on a broadcast local area network (LAN) environment. The focus of ourmore » present research is to extend our network <span class="hlt">intrusion</span>-detection concept from the LAN environment to arbitarily wider areas with the network topology being arbitrary as well. The generalized distributed environment is heterogeneous, i.e., the network nodes can be hosts or servers from different vendors, or some of them could be LAN managers, like our previous work, a network security monitor (NSM), as well. The proposed architecture for this distributed <span class="hlt">intrusion</span>-detection system consists of the following components: a host manager in each host; a LAN manager for monitoring each LAN in the system; and a central manager which is placed at a single secure location and which receives reports from various host and LAN managers to process these reports, correlate them, and detect <span class="hlt">intrusions</span>. 11 refs., 2 figs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gq/1767/gq1767_pamphlet.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gq/1767/gq1767_pamphlet.pdf"><span>Geologic map of the Valley Mountain 15’ quadrangle, San Bernardino and Riverside Counties, California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Howard, Keith A.; Bacheller, John; Fitzgibbon, Todd T.; Powell, Robert E.; Allen, Charlotte M.</p> <p>2013-01-01</p> <p>The Valley Mountain 15’ quadrangle straddles the Pinto Mountain Fault, which bounds the eastern Transverse Ranges in the south against the Mojave Desert province in the north. The Pinto Mountains, part of the eastern Transverse Ranges in the south part of the quadrangle expose a series of Paleoproterozoic gneisses and granite and the Proterozoic quartzite of Pinto Mountain. Early Triassic quartz monzonite intruded the gneisses and was ductiley deformed prior to voluminous Jurassic <span class="hlt">intrusion</span> of diorite, granodiorite, quartz monzonite, and granite plutons. The Jurassic rocks include part of the Bullion Mountains <span class="hlt">Intrusive</span> Suite, which crops out prominently at Valley Mountain and in the Bullion Mountains, as well as in the Pinto Mountains. Jurassic plutons in the southwest part of the quadrangle are deeply denuded from midcrustal emplacement levels in contrast to supracrustal Jurassic limestone and volcanic rocks exposed in the northeast. <span class="hlt">Dikes</span> inferred to be part of the Jurassic Independence <span class="hlt">Dike</span> Swarm intrude the Jurassic plutons and Proterozoic rocks. Late Cretaceous <span class="hlt">intrusion</span> of the Cadiz Valley Batholith in the northeast caused contact metamorphism of adjacent Jurassic plutonic rocks. The Tertiary period saw emplacement of basanitoid basalt at about 23 Ma and deposition of Miocene and (or) Pliocene ridge-capping gravels. An undated east-dipping low-angle normal fault <span class="hlt">zone</span> in the Pinto Mountains drops hanging-wall rocks eastward and may account for part of the contrast in uplift history across the quadrangle. The eastern Transverse Ranges are commonly interpreted as severely rotated clockwise tectonically in the Neogene relative to the Mojave Desert, but similar orientations of Jurassic <span class="hlt">dike</span> swarms suggest that any differential rotation between the two provinces is small in this quadrangle. The late Cenozoic Pinto Mountain Fault and other strike-slip faults cut Quaternary deposits in the quadrangle, with two northwest-striking faults cutting Holocene deposits</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.V51D2071C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.V51D2071C"><span>June 2006 seismic swarm and <span class="hlt">dike</span> injection event beneath the Michoacan-Guanajuato volcanic field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cox, T. F.; Gardine, M.; West, M.</p> <p>2008-12-01</p> <p>A seismic swarm of approximately 700 events, magnitude 2.5-3.5, occurred in June of 2006 approximately 15 km from the summit of the cinder cone Paricutin, in the Michoacan-Guanajuato Volcanic Field in central Mexico. The swarm was detected and located as part of an effort to develop a catalog of regional seismicity using stations fortuitously in place as part of two concurrent IRIS/PASSCAL supported projects- the Mapping of the Rivera Subduction <span class="hlt">Zone</span> (MARS) project run by the University of Texas at Austin and New Mexico State University, and the Colima Volcano Deep Seismic Experiment (CODEX), run by the University of Alaska Fairbanks. Over a two-week period in June 2006, relocated hypocenters clearly show a shallowing trend with time, indicative of a possible <span class="hlt">dike</span> injection event. The rate of injection appears to be 346 m/day. Following the injection, there is a period of earthquakes, which all occurred at approximately 5 km in depth, but which migrated southwards. The waveforms of all of these events show similarities within three major groupings: from May 28 to June 1, June 2 to June 9 (which marks the end of the ascent), and from June 9 to July 2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/11390','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/11390"><span>Water <span class="hlt">Intrusion</span> Problems in Transit Tunnels</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>1986-05-01</p> <p>This report presents the findings of five case studies in which an in-depth analysis was made of tunnel water <span class="hlt">intrusion</span> problems in transit tunnels. Water <span class="hlt">intrusion</span> parameters of transit systems in Atlanta, Boston, Buffalo, New York and Washington, D...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/1040/ds1040.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/1040/ds1040.pdf"><span>Isotopic data for Late Cretaceous <span class="hlt">intrusions</span> and associated altered and mineralized rocks in the Big Belt Mountains, Montana</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>du Bray, Edward A.; Unruh, Daniel M.; Hofstra, Albert H.</p> <p>2017-03-07</p> <p>The quartz monzodiorite of Mount Edith and the concentrically <span class="hlt">zoned</span> <span class="hlt">intrusive</span> suite of Boulder Baldy constitute the principal Late Cretaceous igneous <span class="hlt">intrusions</span> hosted by Mesoproterozoic sedimentary rocks of the Newland Formation in the Big Belt Mountains, Montana. These calc-alkaline plutonic masses are manifestations of subduction-related magmatism that prevailed along the western edge of North America during the Cretaceous. Radiogenic isotope data for neodymium, strontium, and lead indicate that the petrogenesis of the associated magmas involved a combination of (1) sources that were compositionally heterogeneous at the scale of the geographically restricted <span class="hlt">intrusive</span> rocks in the Big Belt Mountains and (2) variable contamination by crustal assimilants also having diverse isotopic compositions. Altered and mineralized rocks temporally, spatially, and genetically related to these <span class="hlt">intrusions</span> manifest at least two isotopically distinct mineralizing events, both of which involve major inputs from spatially associated Late Cretaceous igneous rocks. Alteration and mineralization of rock associated with the <span class="hlt">intrusive</span> suite of Boulder Baldy requires a component characterized by significantly more radiogenic strontium than that characteristic of the associated igneous rocks. However, the source of such a component was not identified in the Big Belt Mountains. Similarly, altered and mineralized rocks associated with the quartz monzodiorite of Mount Edith include a component characterized by significantly more radiogenic strontium and lead, particularly as defined by 207Pb/204Pb values. The source of this component appears to be fluids that equilibrated with proximal Newland Formation rocks. Oxygen isotope data for rocks of the <span class="hlt">intrusive</span> suite of Boulder Baldy are similar to those of subduction-related magmatism that include mantle-derived components; oxygen isotope data for altered and mineralized equivalents are slightly lighter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAESc.158..324C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAESc.158..324C"><span>Petrogenesis of Early Cretaceous dioritic <span class="hlt">dikes</span> in the Shanyang-Zhashui area, South Qinling, central China: Evidence for partial melting of thickened lower continental crust</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Lei; Yan, Zhen; Wang, Zongqi; Wang, Kunming</p> <p>2018-06-01</p> <p>The dioritic <span class="hlt">dikes</span> distributed in the Shanyang-Zhashui area of the South Qinling region play an important role in understanding the deep magmatic processes and tectonic evolution during the orogenic process. The zircon Usbnd Pb ages of the dioritic <span class="hlt">dikes</span> indicate that they were emplaced at ∼144 Ma and therefore postdate the <span class="hlt">dikes</span> that formed in the intracontinental orogenic background after the continental collision between the North China Block (NCB) and the South China Block (SCB). The dioritic <span class="hlt">dikes</span> have SiO2 contents of 56.86-64.93 wt%; K2O contents of 1.65-3.21 wt%; low MgO (1.50-2.66 wt%), Y (14.4-25.5 ppm) and heavy rare earth element (HREE) contents; low Mg# values (39.9-49); high Sr contents (528-4833 ppm); and high Sr/Y ratios (32.8-189). They exhibit highly fractionated REE and flat HREE patterns, strong enrichment in large ion lithophile elements (LILEs; e.g., Rb, Ba, and U) and depletion in high field strength elements (HFSEs) (e.g., Nb), as well as positive Sr and negative Ti anomalies. Furthermore, these dioritic <span class="hlt">dikes</span> exhibit (87Sr/86Sr)i ratios ranging from 0.7048 to 0.7083, εNd(t) values ranging from -3.3 to -1.4, and εHf(t) values ranging from -4.1 to 1.6. The geochemical patterns of the dioritic <span class="hlt">dikes</span> indicate that they possess adakitic characteristics. Moreover, the low MgO contents, Mg# values, Ni contents, Th/Ce ratios, and Srsbnd Ndsbnd Hf isotopic features all indicate that these dioritic <span class="hlt">dikes</span> were generated by the partial melting of thickened mafic lower crust. The high La/Yb and Sr/Y ratios, low Y and Yb contents, absence of significant Eu anomalies, flat HREE patterns, and low Nb/Ta ratios of these rocks suggest that the adakitic melts were derived from the melting of garnet-bearing amphibolite. The geochronologic, elemental and isotopic evidence suggests that the dioritic <span class="hlt">dikes</span> may have formed in a locally extensional environment within an overall N-S compressional setting or during the transition from compressional to extensional</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012438','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012438"><span>Applications of the VLF induction method for studying some volcanic processes of Kilauea volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zablocki, C.J.</p> <p>1978-01-01</p> <p>The very low-frequency (VLF) induction method has found exceptional utility in studying various volcanic processes of Kilauea volcano, Hawaii because: (1) significant anomalies result exclusively from ionically conductive magma or still-hot <span class="hlt">intrusions</span> (> 800??C) and the attendant electrolytically conductive hot groundwater; (2) basalt flows forming the bulk of Kilauea have very high resistivities at shallow depths that result in low geologic noise levels and relatively deep depths of investigation (???100 m); and (3) the azimuths to two of the usable transmitters (NLK and NPM) are aligned favorably with most of the principal geologic features. Measurements of the tilt angle and ellipticity of the polarization ellipse of the magnetic field, using a simple, hand-held receiver, have been used to: (1) delineate the lateral extent of shallow, partially solidified lava lakes, active lava tubes, and recent <span class="hlt">intrusive</span> <span class="hlt">dikes</span>; (2) obtain an indication of the attitude of some recent <span class="hlt">dikes</span>; (3) show that many eruptive fissures cool faster than their <span class="hlt">intrusive</span> counterparts; (4) show that some fumarolic areas are underlain by shallow, highly altered, and conductive <span class="hlt">zones</span>; and (5) provide control information for interpreting data obtained with other electrical techniques. Complementary measurements of scalar apparent resistivity and surface impedance phase, using a new attachment for the VLF receiver, have substantially increased the utility of VLF studies in Kilauea. They provide better lateral resolution of conductors and reduce the ambiguity in interpretation. Notwithstanding recent advances in theoretical modeling techniques, the excellent quality of some of the data warrants extension of interpretive techniques, particularly for quantitatively characterizing the configuration and conductivity of small-dimension bodies. These VLF induction methods should have wide application to studies of active volcanic regions in other parts of the world and could provide some insights into</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatCo...713585C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatCo...713585C"><span>Rapid laccolith <span class="hlt">intrusion</span> driven by explosive volcanic eruption</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Castro, Jonathan M.; Cordonnier, Benoit; Schipper, C. Ian; Tuffen, Hugh; Baumann, Tobias S.; Feisel, Yves</p> <p>2016-11-01</p> <p>Magmatic <span class="hlt">intrusions</span> and volcanic eruptions are intimately related phenomena. Shallow magma <span class="hlt">intrusion</span> builds subsurface reservoirs that are drained by volcanic eruptions. Thus, the long-held view is that <span class="hlt">intrusions</span> must precede and feed eruptions. Here we show that explosive eruptions can also cause magma <span class="hlt">intrusion</span>. We provide an account of a rapidly emplaced laccolith during the 2011 rhyolite eruption of Cordón Caulle, Chile. Remote sensing indicates that an <span class="hlt">intrusion</span> began after eruption onset and caused severe (>200 m) uplift over 1 month. Digital terrain models resolve a laccolith-shaped body ~0.8 km3. Deformation and conduit flow models indicate laccolith depths of only ~20-200 m and overpressures (~1-10 MPa) that likely stemmed from conduit blockage. Our results show that explosive eruptions may rapidly force significant quantities of magma in the crust to build laccoliths. These iconic <span class="hlt">intrusions</span> can thus be interpreted as eruptive features that pose unique and previously unrecognized volcanic hazards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27876800','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27876800"><span>Rapid laccolith <span class="hlt">intrusion</span> driven by explosive volcanic eruption.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Castro, Jonathan M; Cordonnier, Benoit; Schipper, C Ian; Tuffen, Hugh; Baumann, Tobias S; Feisel, Yves</p> <p>2016-11-23</p> <p>Magmatic <span class="hlt">intrusions</span> and volcanic eruptions are intimately related phenomena. Shallow magma <span class="hlt">intrusion</span> builds subsurface reservoirs that are drained by volcanic eruptions. Thus, the long-held view is that <span class="hlt">intrusions</span> must precede and feed eruptions. Here we show that explosive eruptions can also cause magma <span class="hlt">intrusion</span>. We provide an account of a rapidly emplaced laccolith during the 2011 rhyolite eruption of Cordón Caulle, Chile. Remote sensing indicates that an <span class="hlt">intrusion</span> began after eruption onset and caused severe (>200 m) uplift over 1 month. Digital terrain models resolve a laccolith-shaped body ∼0.8 km 3 . Deformation and conduit flow models indicate laccolith depths of only ∼20-200 m and overpressures (∼1-10 MPa) that likely stemmed from conduit blockage. Our results show that explosive eruptions may rapidly force significant quantities of magma in the crust to build laccoliths. These iconic <span class="hlt">intrusions</span> can thus be interpreted as eruptive features that pose unique and previously unrecognized volcanic hazards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991CoMP..108..396M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991CoMP..108..396M"><span><span class="hlt">Intrusion</span> of basaltic magma into a crystallizing granitic magma chamber: The Cordillera del Paine pluton in southern Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Michael, Peter J.</p> <p>1991-10-01</p> <p>The Cordillera del Paine pluton in the southernmost Andes of Chile represents a deeply dissected magma chamber where mafic magma intruded into crystallizing granitic magma. Throughout much of the 10x15 km pluton, there is a sharp and continuous boundary at a remarkably constant elevation of 1,100 m that separates granitic rocks (Cordillera del Paine or CP granite: 69 77% SiO2) which make up the upper levels of the pluton from mafic and comingled rocks (Paine Mafic Complex or PMC: 45 60% SiO2) which dominate the lower exposures of the pluton. Chilled, crenulate, disrupted contacts of mafic rock against granite demonstrate that partly crystallized granite was intruded by mafic magma which solidified prior to complete crystallization of the granitic magma. The boundary at 1,100 m was a large and stable density contrast between the denser, hotter mafic magma and cooler granitic magma. The granitic magma was more solidified near the margins of the chamber when mafic <span class="hlt">intrusion</span> occurred, and the PMC is less disrupted by granites there. Near the pluton margins, the PMC grades upward irregularly from cumulate gabbros to monzodiorites. Mafic magma differentiated largely by fractional crystallization as indicated by the presence of cumulate rocks and by the low levels of compatible elements in most PMC rocks. The compositional gap between the PMC and CP granite indicates that mixing (blending) of granitic magma into the mafic magma was less important, although it is apparent from mineral assemblages in mafic rocks. Granitic magma may have incorporated small amounts of mafic liquid that had evolved to >60% SiO2 by crystallization. Mixing was inhibited by the extent of crystallization of the granite, and by the thermal contrast and the stable density contrast between the magmas. PMC gabbros display disequilibrium mineral assemblages including early formed <span class="hlt">zoned</span> olivine (with orthopyroxene coronas), clinopyroxene, calcic plagioclase and paragasite and later-formed amphibole</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JAESc.113.1117S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JAESc.113.1117S"><span>Variations of trace element concentration of magnetite and ilmenite from the Taihe layered <span class="hlt">intrusion</span>, Emeishan large igneous province, SW China: Implications for magmatic fractionation and origin of Fe-Ti-V oxide ore deposits</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>She, Yu-Wei; Song, Xie-Yan; Yu, Song-Yue; He, Hai-Long</p> <p>2015-12-01</p> <p>In situ LA-ICP-MS trace elemental analysis has been applied to magnetite and ilmenite of the Taihe layered <span class="hlt">intrusion</span>, Emeishan large igneous province, SW China, in order to understand better fractionation processes of magma and origin of Fe-Ti-V oxide ore deposits. The periodic reversals in Mg, Ti, Mn in magnetite and Mg, Sc in ilmenite are found in the Middle <span class="hlt">Zone</span> of the <span class="hlt">intrusion</span> and agree with fractionation trends as recorded by olivine (Fo), plagioclase (An) and clinopyroxene (Mg#) compositions. These suggest the Taihe <span class="hlt">intrusion</span> formed from open magma chamber processes in a magma conduit with multiple replenishments of more primitive magmas. The V and Cr of magnetite are well correlated with V and Cr of clinopyroxene indicating that they became liquidus phases almost simultaneously at an early stage of magma evolution. Ilmenite from the Middle and Upper <span class="hlt">Zones</span> shows variable Cr, Ni, V, Mg, Nb, Ta and Sc contents indicating that ilmenite at some stratigraphic levels crystallized slightly earlier than magnetite and clinopyroxene. The early crystallization of magnetite and ilmenite is the result of the high FeOt and TiO2 contents in the parental magma. The ilmenite crystallization before magnetite in the Middle and Upper <span class="hlt">Zones</span> can be attributed to higher TiO2 content of the magma due to the remelting of pre-existing ilmenite in a middle-level magma chamber. Compared to the coeval high-Ti basalts, the relatively low Zr, Hf, Nb and Ta contents in both magnetite and ilmenite throughout the Taihe <span class="hlt">intrusion</span> indicate that they crystallized from Fe-Ti-(P)-rich silicate magmas. Positive correlations of Ti with Mg, Mn, Sc and Zr of magnetite, and Zr with Sc, Hf and Nb of ilmenite also suggest that magnetite and ilmenite crystallized continuously from the homogeneous silicate magma rather than an immiscible Fe-rich melt. Therefore, frequent replenishments of Fe-Ti-(P)-rich silicate magma and gravitational sorting and settling are crucial for the formation the massive and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51B0449W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51B0449W"><span>Fault-Magma Interactions during Early Continental Rifting: Seismicity of the Magadi-Natron-Manyara basins, Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weinstein, A.; Oliva, S. J.; Ebinger, C.; Aman, M.; Lambert, C.; Roecker, S. W.; Tiberi, C.; Muirhead, J.</p> <p>2017-12-01</p> <p>Although magmatism may occur during the earliest stages of continental rifting, its role in strain accommodation remains weakly constrained by largely 2D studies. We analyze seismicity data from a 13-month, 39-station broadband seismic array to determine the role of magma <span class="hlt">intrusion</span> on state-of-stress and strain localization, and their along-strike variations. Precise earthquake locations using cluster analyses and a new 3D velocity model reveal lower crustal earthquakes along projections of steep border faults that degas CO2. Seismicity forms several disks interpreted as sills at 6-10 km below a monogenetic cone field. The sills overlie a lower crustal magma chamber that may feed eruptions at Oldoinyo Lengai volcano. After determining a new ML scaling relation, we determine a b-value of 0.87 ± 0.03. Focal mechanisms for 66 earthquakes, and a longer time period of relocated earthquakes from global arrays reveal an along-axis stress rotation of 50 o ( N150 oE) in the magmatically active <span class="hlt">zone</span>. Using Kostrov summation of local and teleseismic mechanisms, we find opening directions of N122ºE and N92ºE north and south of the magmatically active <span class="hlt">zone</span>. The stress rotation facilitates strain transfer from border fault systems, the locus of early stage deformation, to the <span class="hlt">zone</span> of magma <span class="hlt">intrusion</span> in the central rift. Our seismic, structural, and geochemistry results indicate that frequent lower crustal earthquakes are promoted by elevated pore pressures from volatile degassing along border faults, and hydraulic fracture around the margins of magma bodies. Earthquakes are largely driven by stress state around inflating magma bodies, and more <span class="hlt">dike</span> <span class="hlt">intrusions</span> with surface faulting, eruptions, and earthquakes are expected.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V11C0350L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V11C0350L"><span>Down and Out at Pacaya Volcano: A Glimpse of Magma Storage and <span class="hlt">Diking</span> as Interpreted From GPS Geodesy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lechner, H. N.; Waite, G. P.; Wauthier, D. C.; Escobar-Wolf, R. P.; Lopez-Hetland, B.</p> <p>2017-12-01</p> <p>Geodetic data from an eight-station GPS network at Pacaya volcano Guatemala allows us to produce a simple analytical model of deformation sources associated with the 2010 eruption and the eruptive period in 2013-2014. Deformation signals for both eruptive time-periods indicate downward vertical and outward horizontal motion at several stations surrounding the volcano. The objective of this research was to better understand the magmatic plumbing system and sources of this deformation. Because this down-and-out displacement is difficult to explain with a single source, we chose a model that includes a combination of a <span class="hlt">dike</span> and spherical source. Our modelling suggests that deformation is dominated the inflation of a shallow <span class="hlt">dike</span> seated high within the volcanic edifice and deflation of a deeper, spherical source below the SW flank of the volcano. The source parameters for the <span class="hlt">dike</span> feature are in good agreement with the observed orientation of recent vent emplacements on the edifice as well the horizontal displacement, while the parameters for a deeper spherical source accommodate the downward vertical motion. This study presents GPS observations at Pacaya dating back to 2009 and provides a glimpse of simple models of possible deformation sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26299620','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26299620"><span>Young women's experiences of <span class="hlt">intrusive</span> behavior in 12 countries.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sheridan, Lorraine; Scott, Adrian J; Roberts, Karl</p> <p>2016-01-01</p> <p>The present study provides international comparisons of young women's (N = 1,734) self-reported experiences of <span class="hlt">intrusive</span> activities enacted by men. Undergraduate psychology students from 12 countries (Armenia, Australia, England, Egypt, Finland, India, Indonesia, Italy, Japan, Portugal, Scotland, and Trinidad) indicated which of 47 <span class="hlt">intrusive</span> activities they had personally experienced. <span class="hlt">Intrusive</span> behavior was not uncommon overall, although large differences were apparent between countries when women's personal experiences of specific <span class="hlt">intrusive</span> activities were compared. Correlations were carried out between self-reported <span class="hlt">intrusive</span> experiences, the Gender Empowerment Measure (GEM), and Hofstede's dimensions of national cultures. The primary associations were between women's experiences of <span class="hlt">intrusive</span> behavior and the level of power they are afforded within the 12 countries. Women from countries with higher GEM scores reported experiencing more <span class="hlt">intrusive</span> activities relating to courtship and requests for sex, while the experiences of women from countries with lower GEM scores related more to monitoring and ownership. <span class="hlt">Intrusive</span> activities, many of them constituent of harassment and stalking, would appear to be widespread and universal, and their incidence and particular form reflect national level gender inequalities. © 2015 Wiley Periodicals, Inc.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA256272','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA256272"><span>Environmental Assessment: Lockport Approach <span class="hlt">Dike</span>, Stage 2 Repairs, Will County, Illinois</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1992-03-01</p> <p>May 1990 with two subsequent events, the most recent in November 1990. In the interest of safety and integrity of project operation , the U.S. Army...and operation . The <span class="hlt">dike</span> is experiencing ongoing erosion to its canal side due to canal level fluctuations and tow prop wash at the various water levels...Impact Statement, Operation and Maintenance of a Nine-Foot Channel in the Illinols Waterway, From the Junction of the Calumet-Sag Channel and the Chicago</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=260083','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=260083"><span>Yield and economics of shallow subsurface drip irrigation (S3DI) and furrow <span class="hlt">diking</span></span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>A shallow subsurface drip irrigation (S3DI) was installed yearly in conjunction with furrow <span class="hlt">diking</span> to document yield and economic benefit of these techniques on peanut (Arachis hypogaea L.), cotton (Gossypium hirsutum L.), and corn (Zea mays L.). This research was conducted for three years from 2005...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S33C2852S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S33C2852S"><span>Coupled Mechanical and Thermal Modeling of Frictional Melt Injection to Constrain Physical Conditions of the Earthquake Source Region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sawyer, W.; Resor, P. G.</p> <p>2016-12-01</p> <p>Pseudotachylyte, a fault rock formed through coseismic frictional melting, provides an important record of coseismic mechanics. In particular, injection veins formed at a high angle to the fault surface have been used to estimate rupture directivity, velocity, pulse length, stress and strength drop, as well as slip weakening distance and wall rock stiffness. These studies, however, have generally treated injection vein formation as a purely elastic process and have assumed that processes of melt generation, transport, and solidification have little influence on the final vein geometry. Using a modified analytical approximation of injection vein formation based on a <span class="hlt">dike</span> <span class="hlt">intrusion</span> model we find that the timescales of quenching and flow propagation are similar for a composite set of injection veins compiled from the Asbestos Mountain Fault, USA (Rowe et al., 2012), Gole Larghe Fault <span class="hlt">Zone</span>, Italy (Griffith et al., 2012) and the Fort Foster Brittle <span class="hlt">Zone</span>. This indicates a complex, dynamic process whose behavior is not fully captured by the current approach. To assess the applicability of the simplifying assumptions of the <span class="hlt">dike</span> model when applied to injection veins we employ a finite-element time-dependent model of injection vein formation. This model couples elastic deformation of the wall rock with the fluid dynamics and heat transfer of the frictional melt. The final geometry of many injection veins is unaffected by the inclusion of these processes. However, some injection veins are found to be flow limited, with a final geometry reflecting cooling of the vein before it reaches an elastic equilibrium with the wall rock. In these cases, numerical results are significantly different from the <span class="hlt">dike</span> model, and two basic assumptions of the <span class="hlt">dike</span> model, self-similar growth and a uniform pressure gradient, are shown to be false. Additionally, we apply the finite-element model to provide two new constraints on the Fort Foster coseismic environment: a lower limit on the initial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010SPIE.7749E..1RS','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010SPIE.7749E..1RS"><span>Research on IPv6 <span class="hlt">intrusion</span> detection system Snort-based</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shen, Zihao; Wang, Hui</p> <p>2010-07-01</p> <p>This paper introduces the common <span class="hlt">intrusion</span> detection technologies, discusses the work flow of Snort <span class="hlt">intrusion</span> detection system, and analyzes IPv6 data packet encapsulation and protocol decoding technology. We propose the expanding Snort architecture to support IPv6 <span class="hlt">intrusion</span> detection in accordance with CIDF standard combined with protocol analysis technology and pattern matching technology, and present its composition. The research indicates that the expanding Snort system can effectively detect various <span class="hlt">intrusion</span> attacks; it is high in detection efficiency and detection accuracy and reduces false alarm and omission report, which effectively solves the problem of IPv6 <span class="hlt">intrusion</span> detection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23998315','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23998315"><span><span class="hlt">Intrusion</span>-based reasoning and depression: cross-sectional and prospective relationships.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Berle, David; Moulds, Michelle L</p> <p>2014-01-01</p> <p><span class="hlt">Intrusion</span>-based reasoning refers to the tendency to form interpretations about oneself or a situation based on the occurrence of a negative <span class="hlt">intrusive</span> autobiographical memory. <span class="hlt">Intrusion</span>-based reasoning characterises post-traumatic stress disorder, but has not yet been investigated in depression. We report two studies that aimed to investigate this. In Study 1 both high (n = 42) and low (n = 28) dysphoric participants demonstrated <span class="hlt">intrusion</span>-based reasoning. High-dysphoric individuals engaged in self-referent <span class="hlt">intrusion</span>-based reasoning to a greater extent than did low-dysphoric participants. In Study 2 there were no significant differences in <span class="hlt">intrusion</span>-based reasoning between currently depressed (n = 27) and non-depressed (n = 51) participants, and <span class="hlt">intrusion</span>-based reasoning did not predict depressive symptoms at 6-month follow-up. Interestingly, previously (n = 26) but not currently (n = 27) depressed participants engaged in <span class="hlt">intrusion</span>-based reasoning to a greater extent than never-depressed participants (n = 25), indicating the possibility that <span class="hlt">intrusion</span>-based reasoning may serve as a "scar" from previous episodes. The implications of these findings are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730001644','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730001644"><span>A reconnaissance space sensing investigation of the crustal structure for a strip from the eastern Sierra Nevada to the Colorado Plateau: April 1971</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bechtold, I. C. (Principal Investigator); Liggett, M. A.</p> <p>1972-01-01</p> <p>The author has identified the following significant results. An area of anomalous linear topographic grain and color expressions was recognized in Apollo 9 and ERTS-1 imagery along the Colorado River of northwestern Arizona and southern Nevada. Field reconnaissance and analysis of U-2 photography has shown the anomaly to be a <span class="hlt">zone</span> of north to north-northwest trending <span class="hlt">dike</span> swarms and associated granitic plutons. The <span class="hlt">dikes</span> vary in composition from rhyolite to diabase, with an average composition nearer rhyolite. Shearing and displacement of host rocks along <span class="hlt">dikes</span> suggest <span class="hlt">dike</span> emplacement along active fault <span class="hlt">zones</span>. Post-<span class="hlt">dike</span> deformation has resulted in shearing and complex normal faulting along a similar north-south trend. The epizonal plutonism and volcanism of this north-south belt appears to represent a structurally controlled volcanogenic province which ends abruptly in the vicinity of Lake Mead at a probable eastern extension of the Las Vegas Shear <span class="hlt">Zone</span>. The magnitude and chronology of extensional faulting and plutonism recognized in the north-south <span class="hlt">zone</span>, support the hypothesis that the Las Vegas Shear <span class="hlt">Zone</span> is a transform fault separating two areas of crustal spreading.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17416165','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17416165"><span>An automatically tuning <span class="hlt">intrusion</span> detection system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yu, Zhenwei; Tsai, Jeffrey J P; Weigert, Thomas</p> <p>2007-04-01</p> <p>An <span class="hlt">intrusion</span> detection system (IDS) is a security layer used to detect ongoing <span class="hlt">intrusive</span> activities in information systems. Traditionally, <span class="hlt">intrusion</span> detection relies on extensive knowledge of security experts, in particular, on their familiarity with the computer system to be protected. To reduce this dependence, various data-mining and machine learning techniques have been deployed for <span class="hlt">intrusion</span> detection. An IDS is usually working in a dynamically changing environment, which forces continuous tuning of the <span class="hlt">intrusion</span> detection model, in order to maintain sufficient performance. The manual tuning process required by current systems depends on the system operators in working out the tuning solution and in integrating it into the detection model. In this paper, an automatically tuning IDS (ATIDS) is presented. The proposed system will automatically tune the detection model on-the-fly according to the feedback provided by the system operator when false predictions are encountered. The system is evaluated using the KDDCup'99 <span class="hlt">intrusion</span> detection dataset. Experimental results show that the system achieves up to 35% improvement in terms of misclassification cost when compared with a system lacking the tuning feature. If only 10% false predictions are used to tune the model, the system still achieves about 30% improvement. Moreover, when tuning is not delayed too long, the system can achieve about 20% improvement, with only 1.3% of the false predictions used to tune the model. The results of the experiments show that a practical system can be built based on ATIDS: system operators can focus on verification of predictions with low confidence, as only those predictions determined to be false will be used to tune the detection model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ITEIS.132...14K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ITEIS.132...14K"><span><span class="hlt">Intrusion</span> Detection in Control Systems using Sequence Characteristics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kiuchi, Mai; Onoda, Takashi</p> <p></p> <p><span class="hlt">Intrusion</span> detection is considered effective in control systems. Sequences of the control application behavior observed in the communication, such as the order of the control device to be controlled, are important in control systems. However, most <span class="hlt">intrusion</span> detection systems do not effectively reflect sequences in the application layer into the detection rules. In our previous work, we considered utilizing sequences for <span class="hlt">intrusion</span> detection in control systems, and demonstrated the usefulness of sequences for <span class="hlt">intrusion</span> detection. However, manually writing the detection rules for a large system can be difficult, so using machine learning methods becomes feasible. Also, in the case of control systems, there have been very few observed cyber attacks, so we have very little knowledge of the attack data that should be used to train the <span class="hlt">intrusion</span> detection system. In this paper, we use an approach that combines CRF (Conditional Random Field) considering the sequence of the system, thus able to reflect the characteristics of control system sequences into the <span class="hlt">intrusion</span> detection system, and also does not need the knowledge of attack data to construct the detection rules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5123016','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5123016"><span>Rapid laccolith <span class="hlt">intrusion</span> driven by explosive volcanic eruption</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Castro, Jonathan M.; Cordonnier, Benoit; Schipper, C. Ian; Tuffen, Hugh; Baumann, Tobias S.; Feisel, Yves</p> <p>2016-01-01</p> <p>Magmatic <span class="hlt">intrusions</span> and volcanic eruptions are intimately related phenomena. Shallow magma <span class="hlt">intrusion</span> builds subsurface reservoirs that are drained by volcanic eruptions. Thus, the long-held view is that <span class="hlt">intrusions</span> must precede and feed eruptions. Here we show that explosive eruptions can also cause magma <span class="hlt">intrusion</span>. We provide an account of a rapidly emplaced laccolith during the 2011 rhyolite eruption of Cordón Caulle, Chile. Remote sensing indicates that an <span class="hlt">intrusion</span> began after eruption onset and caused severe (>200 m) uplift over 1 month. Digital terrain models resolve a laccolith-shaped body ∼0.8 km3. Deformation and conduit flow models indicate laccolith depths of only ∼20–200 m and overpressures (∼1–10 MPa) that likely stemmed from conduit blockage. Our results show that explosive eruptions may rapidly force significant quantities of magma in the crust to build laccoliths. These iconic <span class="hlt">intrusions</span> can thus be interpreted as eruptive features that pose unique and previously unrecognized volcanic hazards. PMID:27876800</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018IJEaS.107.1059S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018IJEaS.107.1059S"><span>Petrography, geochemistry, and U-Pb geochronology of pegmatites and aplites associated with the Alvand <span class="hlt">intrusive</span> complex in the Hamedan region, Sanandaj-Sirjan <span class="hlt">zone</span>, Zagros orogen (Iran)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sepahi, Ali Asghar; Salami, Sedigheh; Lentz, David; McFarlane, Christopher; Maanijou, Mohammad</p> <p>2018-04-01</p> <p>The Alvand <span class="hlt">intrusive</span> complex in the Hamedan area in Iran is in the Sanandaj-Sirjan <span class="hlt">zone</span> of the Zagros orogen. It consists of a wide range of plutonic rocks, mainly gabbro, diorite, granodiorite, granite, and leucogranites that were intruded by aplitic and pegmatitic dykes. At least three successive magmatic episodes generated an older gabbro-diorite-tonalite assemblage, followed by a voluminous granodiorite-granite association, which was then followed by minor leucocratic granitoids. Aplitic and pegmatitic dykes and bodies have truncated both plutonic rocks of the Alvand <span class="hlt">intrusive</span> complex and its metamorphic aureole. Chemically they belong to peraluminous LCT (Li-, Cs-, and Ta-bearing) family of pegmatites. Mineralogically, they resemble Muscovite (MS) and Muscovite Rare Element (MSREL) classes of pegmatites. High amounts of some elements, such as Sn (up to 10,000 ppm), Rb (up to 936 ppm), Ba (up to 706 ppm), and LREE (up to 404 ppm) indicate the highly fractionated nature of some of these aplites and pegmatites. U-Pb dating of monazite, zircon, and allanite by LA-ICPMS indicate the following ages: monazite-bearing aplites of Heydareh-e-Poshteshahr and Barfejin areas, southwest of Hamedan, give an age range of 162-172 Ma; zircon in Heydareh-e-Poshteshar gives an average age of 165 Ma and for allanite-bearing pegmatites of Artiman area, north of Tuyserkan, an age of 154.1 ± 3.7 Ma was determined. These overlap with previously reported ages (ca. 167-153 Ma) for the plutonic rocks of the Alvand complex. Therefore, these data reveal that the Jurassic was a period of magmatism in the Hamedan region and adjacent areas in the Sanandaj-Sirjan <span class="hlt">zone</span>, which was situated at the southern edge of the central Iranian micro-plate (southern Eurasian plate) at this time. Our results also suggest that advective heating in a continental arc setting has caused melting of fertile supracrustal lithologies, such as meta-pelites. These partial melts were then emplaced at much higher</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BVol...74..963D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BVol...74..963D"><span>Dykes and structures of the NE rift of Tenerife, Canary Islands: a record of stabilisation and destabilisation of ocean island rift <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delcamp, A.; Troll, V. R.; van Wyk de Vries, B.; Carracedo, J. C.; Petronis, M. S.; Pérez-Torrado, F. J.; Deegan, F. M.</p> <p>2012-07-01</p> <p>Many oceanic island rift <span class="hlt">zones</span> are associated with lateral sector collapses, and several models have been proposed to explain this link. The North-East Rift <span class="hlt">Zone</span> (NERZ) of Tenerife Island, Spain offers an opportunity to explore this relationship, as three successive collapses are located on both sides of the rift. We have carried out a systematic and detailed mapping campaign on the rift <span class="hlt">zone</span>, including analysis of about 400 dykes. We recorded dyke morphology, thickness, composition, internal textural features and orientation to provide a catalogue of the characteristics of rift <span class="hlt">zone</span> dykes. Dykes were intruded along the rift, but also radiate from several nodes along the rift and form en échelon sets along the walls of collapse scars. A striking characteristic of the dykes along the collapse scars is that they dip away from rift or embayment axes and are oblique to the collapse walls. This dyke pattern is consistent with the lateral spreading of the sectors long before the collapse events. The slump sides would create the necessary strike-slip movement to promote en échelon dyke patterns. The spreading flank would probably involve a basal decollement. Lateral flank spreading could have been generated by the intense <span class="hlt">intrusive</span> activity along the rift but sectorial spreading in turn focused <span class="hlt">intrusive</span> activity and allowed the development of deep intra-volcanic <span class="hlt">intrusive</span> complexes. With continued magma supply, spreading caused temporary stabilisation of the rift by reducing slopes and relaxing stress. However, as magmatic <span class="hlt">intrusion</span> persisted, a critical point was reached, beyond which further <span class="hlt">intrusion</span> led to large-scale flank failure and sector collapse. During the early stages of growth, the rift could have been influenced by regional stress/strain fields and by pre-existing oceanic structures, but its later and mature development probably depended largely on the local volcanic and magmatic stress/strain fields that are effectively controlled by the rift <span class="hlt">zone</span> growth</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/foia/vapor-intrusion-characterization-report-revision-10','PESTICIDES'); return false;" href="https://www.epa.gov/foia/vapor-intrusion-characterization-report-revision-10"><span>Vapor <span class="hlt">Intrusion</span> Characterization Report (Revision 1.0)</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>Vapor <span class="hlt">Intrusion</span> Characterization Report (Revision 1) - February 5, 2015: This report, which was approved by the EPA on February 18, 2015, documents the results from implementation of the Final Vapor <span class="hlt">Intrusion</span> Characterization Work Plan.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5042442','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5042442"><span><span class="hlt">Intrusive</span> Memories of Distressing Information: An fMRI Study</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Battaglini, Eva; Liddell, Belinda; Das, Pritha; Malhi, Gin; Felmingham, Kim</p> <p>2016-01-01</p> <p>Although <span class="hlt">intrusive</span> memories are characteristic of many psychological disorders, the neurobiological underpinning of these involuntary recollections are largely unknown. In this study we used functional magentic resonance imaging (fMRI) to identify the neural networks associated with encoding of negative stimuli that are subsequently experienced as <span class="hlt">intrusive</span> memories. Healthy partipants (N = 42) viewed negative and neutral images during a visual/verbal processing task in an fMRI context. Two days later they were assessed on the Impact of Event Scale for occurrence of <span class="hlt">intrusive</span> memories of the encoded images. A sub-group of participants who reported significant <span class="hlt">intrusions</span> (n = 13) demonstrated stronger activation in the amygdala, bilateral ACC and parahippocampal gyrus during verbal encoding relative to a group who reported no <span class="hlt">intrusions</span> (n = 13). Within-group analyses also revealed that the high <span class="hlt">intrusion</span> group showed greater activity in the dorsomedial (dmPFC) and dorsolateral prefrontal cortex (dlPFC), inferior frontal gyrus and occipital regions during negative verbal processing compared to neutral verbal processing. These results do not accord with models of <span class="hlt">intrusions</span> that emphasise visual processing of information at encoding but are consistent with models that highlight the role of inhibitory and suppression processes in the formation of subsequent <span class="hlt">intrusive</span> memories. PMID:27685784</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JSAES..70..324S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JSAES..70..324S"><span>The Ni-Cu-PGE mineralized Brejo Seco mafic-ultramafic layered <span class="hlt">intrusion</span>, Riacho do Pontal Orogen: Onset of Tonian (ca. 900 Ma) continental rifting in Northeast Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salgado, Silas Santos; Ferreira Filho, Cesar Fonseca; Caxito, Fabrício de Andrade; Uhlein, Alexandre; Dantas, Elton Luiz; Stevenson, Ross</p> <p>2016-10-01</p> <p>The Brejo Seco mafic-ultramafic Complex (BSC) occurs at the extreme northwest of the Riacho do Pontal Orogen Internal <span class="hlt">Zone</span>, in the northern margin of the São Francisco Craton in Northeast Brazil. The stratigraphy of this medium size (3.5 km wide and 9 km long) layered <span class="hlt">intrusion</span> consists of four main <span class="hlt">zones</span>, from bottom to top: Lower Mafic <span class="hlt">Zone</span> (LMZ; mainly troctolite), Ultramafic <span class="hlt">Zone</span> (UZ; mainly dunite and minor troctolite); Transitional Mafic <span class="hlt">Zone</span> (TMZ; mainly troctolite) and an Upper Mafic <span class="hlt">Zone</span> (UMZ; gabbro and minor anorthosite, troctolite, and ilmenite magnetitite). Ni-Cu-PGE mineralization occurs at the contact of the UZ with the TMZ, consisting of an up to 50 m thick stratabound <span class="hlt">zone</span> of disseminated magmatic sulfides. An Mg-tholeiitic affinity to the parental magma is indicated by the geochemical fractionation pattern, by the magmatic crystallization sequence and by the elevated Fo content in olivine. A Smsbnd Nd isochron yielded an age of 903 ± 20 Ma, interpreted as the age of crystallization, with initial εNd = 0.8. Evidence of interaction of the BSC parental magma with sialic crust is given by the Rare Earth and trace element patterns, and by slightly negative and overall low values of εNd(900 Ma) in between -0.2 and +3.3. Contrary to early interpretations that it might constitute an ophiolite complex, based mainly on the geochemistry of the host rocks (Morro Branco metavolcanosedimentary complex), here we interpret the BSC as a typical layered mafic-ultramafic <span class="hlt">intrusion</span> in continental crust, related to an extensional regime. The BSC is chrono-correlated to mafic dyke swarms, anorogenic granites and thick bimodal volcanics of similar age and tectonic setting in the São Francisco Craton and surrounding areas. <span class="hlt">Intrusion</span> of the BSC was followed by continued lithospheric thinning, which led to the development of the Paulistana Complex continental rift volcanics around 888 Ma and ultimately to plate separation and the generation of new oceanic crust (Monte</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1047/srp/srp104/of2007-1047srp104.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1047/srp/srp104/of2007-1047srp104.pdf"><span>Multiple shallow level sill <span class="hlt">intrusions</span> coupled with hydromagmatic explosive eruptions marked the initial phase of Ferrar large igneous province magmatism in northern Victoria Land, Antarctica</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Viereck-Goette, L.; Schöner, R.; Bomfleur, B.; Schneider, J.</p> <p>2007-01-01</p> <p>Field data gathered during GANOVEX IX (2005/2006) in Northern Victoria Land, Antarctica, indicate that volcaniclastic deposits of phreatomagmatic eruptions (so-called Exposure Hill Type events) are intercalated with fluvial deposits of Triassic-Jurassic age at two stratigraphic levels. Abundant scoriaceous spatter (locally welded) indicates a hawaiian/strombolian component. Breccia-filled diatremes, from which volcaniclastic deposits were sourced, are rooted in sills which intruded wet sediments. The deposits are thus subaerial expressions of initial Ferrar magmatism involving <span class="hlt">intrusion</span> of multiple shallow-level sills. Due to magma-sediment interaction abundant clastic <span class="hlt">dikes</span> are developed that intrude the sediments and sills. All igneous components in the volcaniclastic deposits are andesitic in composition, as are the chilled margins of the sills. They are more differentiated than the basaltic andesites of the younger effusive section of Kirkpatrick plateau lavas which in northern Victoria Land start with pillow lavas and small volume lava flows from volcanic necks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022013','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022013"><span>Recrystallization and anatexis along the plutonic-volcanic contact of the Turkey Creek caldera, Arizona</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>du Bray, E.A.; Pallister, J.S.</p> <p>1999-01-01</p> <p>Unusual geologic and geochemical relations are preserved along the contact between intracaldera tuff and a resurgent <span class="hlt">intrusion</span> within the 26.9 Ma Turkey Creek caldera of southeast Arizona. Thick intracaldera tuff is weakly argillically altered throughout, except in <span class="hlt">zones</span> within several hundred meters of its contact with the resurgent <span class="hlt">intrusion</span>, where the groundmass of the tuff has been variably converted to granophyre and unaltered sanidine phenocrysts are present. <span class="hlt">Dikes</span> of similarly granophyric material originate at the tuff-resurgent <span class="hlt">intrusion</span> contact and intrude overlying intracaldera megabreccia and tuff. Field relations indicate that the resurgent <span class="hlt">intrusion</span> is a laccolith and that it caused local partial melting of adjacent intracaldera tuff. Geochemical and petrographic relations indicate that small volumes of partially melted intracaldera tuff assimilated and mixed with dacite of the resurgent <span class="hlt">intrusion</span> along their contact, resulting in rocks that have petrographic and compositional characteristics transitional between those of tuff and dacite. Some of this variably contaminated, second-generation magma coalesced, was mobilized, and was intruded into overlying intracaldera rocks. Interpretation of the resurgent <span class="hlt">intrusion</span> in the Turkey Creek and other calderas as intracaldera laccoliths suggests that <span class="hlt">intrusions</span> of this type may be a common, but often unrecognized, feature of calderas. Development of granophyric and anatectic features such as those described here may be equally common in other calderas. The observations and previously undocumented processes described here can be applied to identification and interpretation of similarly enigmatic relations and rocks in other caldera systems. Integration of large-scale field mapping with detailed petrographic and chemical data has resulted in an understanding of otherwise intractable but petrologically important caldera-related features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2012/1010/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2012/1010/"><span>Magmatic ore deposits in layered <span class="hlt">intrusions</span> - Descriptive model for reef-type PGE and contact-type Cu-Ni-PGE deposits</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zientek, Michael L.</p> <p>2012-01-01</p> <p>Layered, ultramafic to mafic <span class="hlt">intrusions</span> are uncommon in the geologic record, but host magmatic ore deposits containing most of the world's economic concentrations of platinum-group elements (PGE) (figs. 1 and 2). These deposits are mined primarily for their platinum, palladium, and rhodium contents (table 1). Magmatic ore deposits are derived from accumulations of crystals of metallic oxides, or immiscible sulfide, or oxide liquids that formed during the cooling and crystallization of magma, typically with mafic to ultramafic compositions. "PGE reefs" are stratabound PGE-enriched lode mineralization in mafic to ultramafic layered <span class="hlt">intrusions</span>. The term "reef" is derived from Australian and South African literature for this style of mineralization and used to refer to (1) the rock layer that is mineralized and has distinctive texture or mineralogy (Naldrett, 2004), or (2) the PGE-enriched sulfide mineralization that occurs within the rock layer. For example, Viljoen (1999) broadly defined the Merensky Reef as "a mineralized <span class="hlt">zone</span> within or closely associated with an unconformity surface in the ultramafic cumulate at the base of the Merensky Cyclic Unit." In this report, we will use the term PGE reef to refer to the PGE-enriched mineralization, not the host rock layer. Within a layered igneous <span class="hlt">intrusion</span>, reef-type mineralization is laterally persistent along strike, extending for the length of the <span class="hlt">intrusion</span>, typically tens to hundreds of kilometers. However, the mineralized interval is thin, generally centimeters to meters thick, relative to the stratigraphic thickness of layers in an <span class="hlt">intrusion</span> that vary from hundreds to thousands of meters. PGE-enriched sulfide mineralization is also found near the contacts or margins of layered mafic to ultramafic <span class="hlt">intrusions</span> (Iljina and Lee, 2005). This contact-type mineralization consists of disseminated to massive concentrations of iron-copper-nickel-PGE-enriched sulfide mineral concentrations in <span class="hlt">zones</span> that can be tens to hundreds</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..122.1876A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..122.1876A"><span>Factors controlling the permeability distribution in fault vein <span class="hlt">zones</span> surrounding granitic <span class="hlt">intrusions</span> (Ore Mountains/Germany)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Achtziger-Zupančič, P.; Loew, S.; Hiller, A.</p> <p>2017-03-01</p> <p>An outstanding legacy data set has been compiled from underground excavations mostly prospected and mined by the former Soviet (German) Stock Company Wismut describing the hydrology of faulted basement rocks in the Ore Mountains (SE Germany). It consists of more than 5000 detailed descriptions of groundwater inflows to about 660 km of tunnels and 57 km of drillings measured during or shortly after excavation. Inflow measurements (recorded between 1E-8 and 4E-2 m3/s) have been converted to fracture transmissivities using a simplified analytical solution. Discarding site specific effects, the median log transmissivity decreases from 1E-7 to 1E-10 m2/s within the studied depth interval of 0-2000 meters below ground surface (mbgs), and the spacing of conductive fracture increases from 0.1 to 2500 m. This general trend is overprinted at three mining sites by a clear reversal of fracture transmissivity which correlates with contact metamorphic aureoles around Variscan granite <span class="hlt">intrusions</span> (327-295 Ma). We hypothesize that this transmissivity increase is caused by processes accompanying granite <span class="hlt">intrusion</span> and contact metamorphism. The thickness of these hydraulically active aureoles is greater in lower-grade metamorphic schist than in higher-grade metamorphic gneisses. Rock mass equivalent continuum conductivities have been estimated by arithmetic averaging of fracture and matrix transmissivities over 100 m intervals and have been converted to permeabilities. The median equivalent continuum permeability decreases with depth according to log(k) = - 1.7 * log(z) - 17.3 (k in m2 and increasing depth z in kilometer being positive). Matrix conductivity controls the bulk conductivity below about 1000 mbgs and is less sensitive to the occurrence of contact metamorphic aureoles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V33A0665W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V33A0665W"><span>Probablistic Analyses of Waste Package Quantities Impacted by Potential Igneous Disruption at Yucca Mountain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wallace, M. G.; Iuzzolina, H.</p> <p>2005-12-01</p> <p>A probabilistic analysis was conducted to estimate ranges for the numbers of waste packages that could be damaged in a potential future igneous event through a repository at Yucca Mountain. The analysis includes disruption from an <span class="hlt">intrusive</span> igneous event and from an extrusive volcanic event. This analysis supports the evaluation of the potential consequences of future igneous activity as part of the total system performance assessment for the license application for the Yucca Mountain Project (YMP). The first scenario, igneous <span class="hlt">intrusion</span>, investigated the case where one or more igneous <span class="hlt">dikes</span> intersect the repository. A swarm of <span class="hlt">dikes</span> was characterized by distributions of length, width, azimuth, and number of <span class="hlt">dikes</span> and the spacings between them. Through the use in part of a latin hypercube simulator and a modified video game engine, mathematical relationships were built between those parameters and the number of waste packages hit. Corresponding cumulative distribution function curves (CDFs) for the number of waste packages hit under several different scenarios were calculated. Variations in <span class="hlt">dike</span> thickness ranges, as well as in repository magma bulkhead positions were examined through sensitivity studies. It was assumed that all waste packages in an emplacement drift would be impacted if that drift was intersected by a <span class="hlt">dike</span>. Over 10,000 individual simulations were performed. Based on these calculations, out of a total of over 11,000 planned waste packages distributed over an area of approximately 5.5 km2 , the median number of waste packages impacted was roughly 1/10 of the total. Individual cases ranged from 0 waste packages to the entire inventory being impacted. The igneous <span class="hlt">intrusion</span> analysis involved an explicit characterization of <span class="hlt">dike</span>-drift intersections, built upon various distributions that reflect the uncertainties associated with the inputs. The second igneous scenario, volcanic eruption (eruptive conduits), considered the effects of conduits formed in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=308904','PESTICIDES'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=308904"><span>Assessment of Mitigation Systems on Vapor <span class="hlt">Intrusion</span> ...</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>Vapor <span class="hlt">intrusion</span> is the migration of subsurface vapors, including radon and volatile organic compounds (VOCs), in soil gas from the subsurface to indoor air. Vapor <span class="hlt">intrusion</span> happens because there are pressure and concentration differentials between indoor air and soil gas. Indoor environments are often negatively pressurized with respect to outdoor air and soil gas (for example, from exhaust fans or the stack effect), and this pressure difference allows soil gas containing subsurface vapors to flow into indoor air through advection. In addition, concentration differentials cause VOCs and radon to migrate from areas of higher to lower concentrations through diffusion, which is another cause of vapor <span class="hlt">intrusion</span>. Current practice for evaluating the vapor <span class="hlt">intrusion</span> pathway involves a multiple line of evidence approach based on direct measurements in groundwater, external soil gas, subslab soil gas, and/or indoor air. No single line of evidence is considered definitive, and direct measurements of vapor <span class="hlt">intrusion</span> can be costly, especially where significant spatial and temporal variability require repeated measurements at multiple locations to accurately assess the chronic risks of long-term exposure to volatile organic compounds (VOCs) like chloroform, perchloroethylene (PCE), and trichloroethylene (TCE).</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S41A2722K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S41A2722K"><span>Shallow active-source imaging of an andesite <span class="hlt">dike</span> in southern New Mexico: comparing Reftek Texan and Fairfield Z-Land recordings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Karplus, M. S.; Kaip, G.; Harder, S. H.; Johnson, K.</p> <p>2016-12-01</p> <p>In October 2015, the Advanced Exploration Seismology class at the University of Texas at El Paso together with additional volunteers acquired a 500-m active-source seismic profile across an andesite <span class="hlt">dike</span> adjacent to the Rio Grande River near Sunland Park, New Mexico. Receivers included 100 RT-125 Reftek Texans with 4.5-Hz geophones, spaced every 5 m, and 47 Fairfield Z-Land nodes incorporating 5-Hz 3C geophones, spaced approximately every 10 m. A 8-gauge, 400 grain seismic gun source was fired every 5-10 m along most of the profile. Several locations at the ends of the profile experienced multiple gun shots, which have been stacked to increase signal-to-noise. We discuss similarities and differences in field methods and data acquired using the Texans compared to the nodes for a shallow active-source experiment. We extend the discussion to other types of active-source experiments using other recently-acquired nodal datasets. We observe changes in velocity between the andesite <span class="hlt">dike</span> and surrounding lithologies, and create a seismic reflection image of the andesite <span class="hlt">dike</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940011734','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940011734"><span>Spatially extensive uniform stress fields on Venus inferred from radial <span class="hlt">dike</span> swarm geometries: The Aphrodite Terra example</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Grosfils, Eric B.; Head, James W.</p> <p>1993-01-01</p> <p>The high resolution and near global coverage of Magellan radar images is facilitating attempts to systematically investigate the stresses that have deformed the venusian crust. Here we continue earlier efforts to utilize approximately 170 large, radially lineated structures interpreted as <span class="hlt">dike</span> swarms to assess the orientation of the regional maximum horizontal compressive stress (MHCS) which existed in their vicinities during emplacement. Examination of swarms near the equator reveals a link to broad scale regional structures, such as Aphrodite Terra, across distances in excess of 1000 km, suggesting the existence of first order stress fields which affect areas of more than 10(exp 6) sq km in a uniform fashion. Focusing further upon the Aphrodite Terra region, the MHCS field in the surrounding lowlands inferred from radial swarms is oriented approximately normal to the slope of the highland topography. This stress configuration appears, at a simple level, to be incompatible with that expected during either upwelling or downwelling construction of the highlands. In addition, the relatively undeformed geometry of the radial structures within the highlands implies that these <span class="hlt">dike</span> swarm features formed more recently than their highly deformed surroundings. We conclude that the differential stresses which existed during emplacement of the <span class="hlt">dike</span> swarms within and adjacent to the Aphrodite Terra highlands are related to the gravitational relaxation of pre-existing topography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.H51C1222M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.H51C1222M"><span>Exploring for geothermal resource in a dormant volcanic system: The Haleakala Southwest Rift <span class="hlt">Zone</span>, Maui, Hawai'i</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martini, B. A.; Lewicki, J. L.; Kennedy, B. M.; Lide, C.; Oppliger, G.; Drakos, P. S.</p> <p>2011-12-01</p> <p>Suites of new geophysical and geochemical surveys provide compelling evidence for geothermal resource at the Haleakala Southwest Rift <span class="hlt">Zone</span> (HSWRZ) on Maui Island, Hawai'i. Ground-based gravity (~400 stations) coupled with heli-borne magnetics (~1500 line kilometers) define both deep and shallow fractures/faults while also delineating potentially widespread subsurface hydrothermal alteration on the lower flanks (below approximately 1800 feet a.s.l.). Multi-level, upward continuation calculations and 2-D gravity and magnetic modeling provide information on source depths, but lack of lithologic information leaves ambiguity in the estimates. Lithology and physical property data from future drilling will improve these interpretations. Additionally, several well-defined gravity lows (possibly vent <span class="hlt">zones</span>) lie coincident with magnetic highs suggesting the presence of <span class="hlt">dike</span> <span class="hlt">intrusions</span> at depth; a potentially young source of heat for a modern geothermal system. Soil CO2 fluxes were measured along transects across geophysically-defined faults and fractures as well as young cinder cones along the HSWRZ; a weak anomalous flux signal was observed at one young cinder cone location. Dissolved inorganic carbon concentrations and δ13C compositions and 3He/4He values measured in several shallow groundwater samples indicate addition of magmatic CO2 and He to the groundwater system. The general lack of observed magmatic surface CO2 signals on the HSWRZ is therefore likely due to a combination of groundwater 'scrubbing' of CO2 and relatively high biogenic surface CO2 fluxes that mask magmatic CO2. Similar surveys at the Puna geothermal field on the Kilauea Lower East Rift <span class="hlt">Zone</span> (KLERZ) also showed a lack of surface CO2 flux signals attributed to a magmatic source, while aqueous geochemistry indicated contribution of magmatic CO2 and He to shallow groundwaters at both Maui and Puna. As magma has been intercepted in geothermal drilling at the Puna field, the lack of measured surface CO2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EPSC...10...59M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EPSC...10...59M"><span>Magmatic <span class="hlt">intrusions</span> in the lunar crust</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Michaut, C.; Thorey, C.</p> <p>2015-10-01</p> <p>The lunar highlands are very old, with ages covering a timespan between 4.5 to 4.2 Gyr, and probably formed by flotation of light plagioclase minerals on top of the lunar magma ocean. The lunar crust provides thus an invaluable evidence of the geological and magmatic processes occurring in the first times of the terrestrial planets history. According to the last estimates from the GRAIL mission, the lunar primary crust is particularly light and relatively thick [1] This low-density crust acted as a barrier for the dense primary mantle melts. This is particularly evident in the fact that subsequent mare basalts erupted primarily within large impact basin: at least part of the crust must have been removed for the magma to reach the surface. However, the trajectory of the magma from the mantle to the surface is unknown. Using a model of magma emplacement below an elastic overlying layer with a flexural wavelength Λ, we characterize the surface deformations induced by the presence of shallow magmatic <span class="hlt">intrusions</span>. We demonstrate that, depending on its size, the <span class="hlt">intrusion</span> can show two different shapes: a bell shape when its radius is smaller than 4 times Λ or a flat top with small bended edges if its radius is larger than 4 times Λ[2]. These characteristic shapes for the <span class="hlt">intrusion</span> result in characteristic deformations at the surface that also depend on the topography of the layer overlying the <span class="hlt">intrusion</span> [3].Using this model we provide evidence of the presence of <span class="hlt">intrusions</span> within the crust of the Moon as surface deformations in the form of low-slope lunar domes and floor-fractured craters. All these geological features have morphologies consistent with models of magma spreading at depth and deforming an overlying elastic layer. Further more,at floor-fractured craters, the deformation is contained within the crater interior, suggesting that the overpressure at the origin of magma ascent and <span class="hlt">intrusion</span> was less than the pressure due to the weight of the crust removed by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70148404','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70148404"><span>Mesozoic magmatism and timing of epigenetic Pb-Zn-Ag mineralization in the western Fortymile mining district, east-central Alaska: Zircon U-Pb geochronology, whole-rock geochemistry, and Pb isotopes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dusel-Bacon, Cynthia; Aleinkoff, J.N.; Day, W.C.; Mortensen, J.K.</p> <p>2015-01-01</p> <p>Epigenetic Pb-Zn-Ag ± Cu prospects in the western Fortymile district are spatially associated with splays of the northeast-trending Kechumstuk sinistral-normal fault <span class="hlt">zone</span> and with ca. 68-66 Ma felsic <span class="hlt">intrusions</span> and <span class="hlt">dikes</span>. The similarity between Pb isotope compositions of feldspars from the Late Cretaceous igneous bodies and sulfides from the epithermal prospects suggests a Late Cretaceous age for most of the mineralization. Fluid flow along the faults undoubtedly played a major role in mineralization. We interpret displacement on the northeast-trending faults to be a far-field effect of dextral translation along Late Cretaceous plate-scale boundaries and faults that were roughly parallel to the subsequently developed Denali and Tintina fault systems, which currently bound the region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4826772','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4826772"><span>Corticostriatal circuitry in regulating diseases characterized by <span class="hlt">intrusive</span> thinking</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kalivas, Benjamin C.; Kalivas, Peter W.</p> <p>2016-01-01</p> <p><span class="hlt">Intrusive</span> thinking triggers clinical symptoms in many neuropsychiatric disorders. Using drug addiction as an exemplar disorder sustained in part by <span class="hlt">intrusive</span> thinking, we explore studies demonstrating that impairments in corticostriatal circuitry strongly contribute to <span class="hlt">intrusive</span> thinking. Neuroimaging studies have long implicated this projection in cue-induced craving to use drugs, and preclinical models show that marked changes are produced at corticostriatal synapses in the nucleus accumbens during a relapse episode. We delineate an accumbens microcircuit that mediates cue-induced drug seeking becoming an <span class="hlt">intrusive</span> event. This microcircuit harbors many potential therapeutic targets. We focus on preclinical and clinical studies, showing that administering N-acetylcysteine restores uptake of synaptic glutamate by astroglial glutamate transporters and thereby inhibits <span class="hlt">intrusive</span> thinking. We posit that because <span class="hlt">intrusive</span> thinking is a shared endophenotype in many disorders, N-acetylcysteine has positive effects in clinical trials for a variety of neuropsychiatric disorders, including drug addiction, gambling, trichotillomania, and depression. PMID:27069381</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27069381','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27069381"><span>Corticostriatal circuitry in regulating diseases characterized by <span class="hlt">intrusive</span> thinking.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kalivas, Benjamin C; Kalivas, Peter W</p> <p>2016-03-01</p> <p><span class="hlt">Intrusive</span> thinking triggers clinical symptoms in many neuropsychiatric disorders. Using drug addiction as an exemplar disorder sustained in part by <span class="hlt">intrusive</span> thinking, we explore studies demonstrating that impairments in corticostriatal circuitry strongly contribute to <span class="hlt">intrusive</span> thinking. Neuroimaging studies have long implicated this projection in cue-induced craving to use drugs, and preclinical models show that marked changes are produced at corticostriatal synapses in the nucleus accumbens during a relapse episode. We delineate an accumbens microcircuit that mediates cue-induced drug seeking becoming an <span class="hlt">intrusive</span> event. This microcircuit harbors many potential therapeutic targets. We focus on preclinical and clinical studies, showing that administering N-acetylcysteine restores uptake of synaptic glutamate by astroglial glutamate transporters and thereby inhibits <span class="hlt">intrusive</span> thinking. We posit that because <span class="hlt">intrusive</span> thinking is a shared endophenotype in many disorders, N-acetylcysteine has positive effects in clinical trials for a variety of neuropsychiatric disorders, including drug addiction, gambling, trichotillomania, and depression.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70182820','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70182820"><span>Controls on <span class="hlt">intrusion</span> of near-trench magmas of the Sanak-Baranof Belt, Alaska, during Paleogene ridge subduction, and consequences for forearc evolution</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kusky, Timothy M.; Bradley, Dwight C.; Donely, D. Thomas; Rowley, David; Haeussler, Peter J.</p> <p>2003-01-01</p> <p>A belt of Paleogene near-trench plutons known as the Sanak-Baranof belt intruded the southern Alaska convergent margin. A compilation of isotopic ages of these plutons shows that they range in age from 61 Ma in the west to ca. 50 Ma in the east. This migrating pulse of magmatism along the continental margin is consistent with North Pacific plate reconstructions that suggests the plutons were generated by migration of a trench-ridge-trench triple junction along the margin. On the Kenai Peninsula the regional lower greenschist metamorphic grade of the turbiditic host rocks, texture of the plutons, contact-metamorphic assemblage, and isotopic and fluid inclusion studies suggest that the plutons were emplaced at pressures of 1.5–3.0 kbars (5.2–10.5 km) into a part of the accretionary wedge with an ambient temperature of 210–300 °C. The presence of kyanite, garnet, and cordierite megacrysts in the plutons indicates that the melts were generated at a depth greater than 20 km and minimum temperature of 650 °C. These megacrysts are probably xenocrystic remnants of a restitic or contact metamorphic phase entrained by the melt during <span class="hlt">intrusion</span>. However, it is also possible that they are primary magmatic phases crystallized from the peraluminous melt.Plutons of the Sanak-Baranof belt serve as time and strain markers separating kinematic regimes that predate and postdate ridge subduction. Pre-ridge subduction structures are interpreted to be related to the interaction between the leading oceanic plate and the Chugach terrane. These include regional thrust faults, NE-striking map-scale folds with associated axial planar foliation, type-1 mélanges, and an arrayof faults within the contact aureole indicating shortening largely accommodated by layer-parallel extension. Syn-ridge subduction features include the plutons, <span class="hlt">dikes</span>, and ductile shear <span class="hlt">zones</span> within contact aureoles with syn-kinematic metamorphic mineral growth and foliation development. Many of the studied plutons</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA530199','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA530199"><span>Herbert Hoover <span class="hlt">Dike</span> (HHD) Phase 1A Groundwater Model</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-07-01</p> <p>ER D C/ CH L TR -1 0- 5 Herbert Hoover <span class="hlt">Dike</span> (HHD) Phase 1A Groundwater Model Co as ta l a nd H yd ra ul ic s La bo ra to ry Hwai...1171 0.0033 1094 0.0101 1159 0.0334 1141 0.0023 Run16 - Run1 L5 7845 0.0224 2360 0.0218 6627 0.1911 5610 0.0114 Run17 - Run1 L5 9768 0.0279 5909...5018 0.0143 Reach 1 Avg. Abs. Diff.* 7845 0.0224 2-1 50 ft from HHD 82590 86894 4304 0.0397 2-2 100 ft from HHD 106002 110644 4643 0.0429 2-3 200</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=90345&Lab=NRMRL&keyword=insulation&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=90345&Lab=NRMRL&keyword=insulation&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>SAMPLING-BASED APPROACH TO INVESTIGATING VAPOR <span class="hlt">INTRUSION</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Vapor <span class="hlt">intrusion</span> is defined as the migration of volatile organic compounds (VOCs) into occupied buildings from contaminated soil or ground water. EPA recently developed guidance to facilitate assessment of vapor <span class="hlt">intrusion</span> at sites regulated by RCRA and CERCLA. The EPA guidance e...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003SPIE.5253..930W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003SPIE.5253..930W"><span>Evidential reasoning research on <span class="hlt">intrusion</span> detection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Xianpei; Xu, Hua; Zheng, Sheng; Cheng, Anyu</p> <p>2003-09-01</p> <p>In this paper, we mainly aim at D-S theory of evidence and the network <span class="hlt">intrusion</span> detection these two fields. It discusses the method how to apply this probable reasoning as an AI technology to the <span class="hlt">Intrusion</span> Detection System (IDS). This paper establishes the application model, describes the new mechanism of reasoning and decision-making and analyses how to implement the model based on the synscan activities detection on the network. The results suggest that if only rational probability values were assigned at the beginning, the engine can, according to the rules of evidence combination and hierarchical reasoning, compute the values of belief and finally inform the administrators of the qualities of the traced activities -- <span class="hlt">intrusions</span>, normal activities or abnormal activities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMEP23C0838R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMEP23C0838R"><span>Assessment of chevron <span class="hlt">dikes</span> for the enhancement of physical-aquatic habitat within the Middle Mississippi River, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Remo, J. W.; Pinter, N.</p> <p>2012-12-01</p> <p>Along the Middle Mississippi River (MMR), rehabilitation of aquatic habitat is being undertaken using river-training structures such as the blunt-nose chevron <span class="hlt">dike</span>. Chevron <span class="hlt">dikes</span> were initially designed to concentrate flow and thus facilitate river navigation, but this new river-training structure is now justified, in part, as a tool for creating aquatic habitat and promoting habitat heterogeneity. The ability of chevrons to create and diversify physical-aquatic habitat has not been verified. In this study, we used 2-D hydrodynamic modeling and reach-scale habitat metrics to assess changes in physical habitat and habitat heterogeneity for pre-chevron and post-chevron along a 2- km reach of the Mississippi River at St. Louis, MO. A historic reference condition (circa 1890) was also modeled to compare physical habitat in a less engineered river channel versus the new physical-habitat patches created by chevron-<span class="hlt">dike</span> enhancement. This modeling approach quantified changes in habitat availability and diversity among selected reference conditions for a wide range of in-channel flows. Depth-velocity habitat classes were used for assessment of change in physical-habitat patches, and spatial statistical tools were employed to evaluate the reach-scale habitat patch diversity. Modeling of post-chevron channel conditions revealed increases in deep to very deep (>3.0 m) areas of slow moving (<0.6 m/s) water downstream of these structures under emergent flow conditions (≤ 1.5 x mean annual flow[MAF]) relative to pre-construction conditions. Chevron construction increased potential over-wintering habitat (deep [>3.0 m], low velocity [<0.6 m/s]) by up to 7.6 ha. The addition of the chevrons to the river channel also created some (0.8-3.8 ha) shallow-water habitat (0-1.5 m depth with a 0-0.6 m/s velocity) for flows ≤2.0 x MAF and contributed to an 8-35% increase in physical-habitat diversity compared to pre-chevron channel conditions. Comparison of the historic reference</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017155','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017155"><span>Volcanic geology and eruption frequency, lower east rift <span class="hlt">zone</span> of Kilauea volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Moore, R.B.</p> <p>1992-01-01</p> <p>Detailed geologic mapping and radiocarbon dating of tholeiitic basalts covering about 275 km2 on the lower east rift <span class="hlt">zone</span> (LERZ) and adjoining flanks of Kilauea volcano, Hawaii, show that at least 112 separate eruptions have occurred during the past 2360 years. Eruptive products include spatter ramparts and cones, a shield, two extensive lithic-rich tuff deposits, aa and pahoehoe flows, and three littoral cones. Areal coverage, number of eruptions and average dormant interval estimates in years for the five age groups assigned are: (I) historic, i.e. A D 1790 and younger: 25%, 5, 42.75; (II) 200-400 years old: 50%, 15, 14.3: (III) 400-750 years old: 20%, 54, 6.6; (IV) 750-1500 years old: 5%, 37, 20.8; (V) 1500-3000 years old: <1%, 1, unknown. At least 4.5-6 km3 of tholeiitic basalt have been erupted from the LERZ during the past 1500 years. Estimated volumes of the exposed products of individual eruptions range from a few tens of cubic meters for older units in small kipukas to as much as 0.4 km3 for the heiheiahulu shield. The average dormant interval has been about 13.6 years during the past 1500 years. The most recent eruption occurred in 1961, and the area may be overdue for its next eruption. However, eruptive activity will not resume on the LERZ until either the <span class="hlt">dike</span> feeding the current eruption on the middle east rift <span class="hlt">zone</span> extends farther down rift, or a new <span class="hlt">dike</span>, unrelated to the current eruption, extends into the LERZ. ?? 1992 Springer-Verlag.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992BVol...54..475M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992BVol...54..475M"><span>Volcanic geology and eruption frequency, lower east rift <span class="hlt">zone</span> of Kilauea volcano, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moore, Richard B.</p> <p>1992-08-01</p> <p>Detailed geologic mapping and radiocarbon dating of tholeiitic basalts covering about 275 km2 on the lower east rift <span class="hlt">zone</span> (LERZ) and adjoining flanks of Kilauea volcano, Hawaii, show that at least 112 separate eruptions have occurred during the past 2360 years. Eruptive products include spatter ramparts and cones, a shield, two extensive lithic-rich tuff deposits, aa and pahoehoe flows, and three littoral cones. Areal coverage, number of eruptions and average dormant interval estimates in years for the five age groups assigned are: (I) historic, i.e. A D 1790 and younger: 25%, 5, 42.75; (II) 200 400 years old: 50%, 15, 14.3: (III) 400 750 years old: 20%, 54, 6.6; (IV) 750 1500 years old: 5%, 37, 20.8; (V) 1500 3000 years old: <1%, 1, unknown. At least 4.5 6 km3 of tholeiitic basalt have been erupted from the LERZ during the past 1500 years. Estimated volumes of the exposed products of individual eruptions range from a few tens of cubic meters for older units in small kipukas to as much as 0.4 km3 for the heiheiahulu shield. The average dormant interval has been about 13.6 years during the past 1500 years. The most recent eruption occurred in 1961, and the area may be overdue for its next eruption. However, eruptive activity will not resume on the LERZ until either the <span class="hlt">dike</span> feeding the current eruption on the middle east rift <span class="hlt">zone</span> extends farther down rift, or a new <span class="hlt">dike</span>, unrelated to the current eruption, extends into the LERZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..122..966R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..122..966R"><span>Postemplacement dynamics of basaltic <span class="hlt">intrusions</span> in the continental crust</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roman, A.; Jaupart, C.</p> <p>2017-02-01</p> <p>Laboratory experiments document the postemplacement behavior of mafic <span class="hlt">intrusions</span> that spread at a density interface and founder as they become denser than their surroundings due to cooling and crystallization. All else being equal, the larger the <span class="hlt">intrusion</span> volume, the farther the <span class="hlt">intrusion</span> can spread and the smaller its aspect ratio is. The final aspect ratio is a function of a single dimensionless number analogous to the Rayleigh number of thermal convection. Once it is denser than its surroundings, the <span class="hlt">intrusion</span> becomes unstable and may founder in two different regimes. At aspect ratios larger than about 0.4, the "teardrop" regime is such that the <span class="hlt">intrusion</span> thickens in a central region, developing the shapes of a funnel and a pendant drop. At lower aspect ratios, another regime is observed, with thickening of the <span class="hlt">intrusion</span> at the leading edge and thinning in a central region. The thick outer ring in turn becomes unstable into a set of teardrops and leads to an irregular horizontal outline. In one variant called the "jellyfish" regime, the thin central region develops a number of downwellings and upwellings in a Rayleigh-Taylor-like pattern. These instabilities may get arrested due to cooling as the <span class="hlt">intrusion</span> and encasing rocks become too strong to deform. One would then be left with a funnel-shaped residual body or a wide irregular one with thick peripheral lobes and a thinner central region. These different patterns can be recognized in upper crustal mafic <span class="hlt">intrusions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol2/pdf/CFR-2013-title10-vol2-sec63-322.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title10-vol2/pdf/CFR-2013-title10-vol2-sec63-322.pdf"><span>10 CFR 63.322 - Human <span class="hlt">intrusion</span> scenario.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-01-01</p> <p>... 10 Energy 2 2013-01-01 2013-01-01 false Human <span class="hlt">intrusion</span> scenario. 63.322 Section 63.322 Energy NUCLEAR REGULATORY COMMISSION (CONTINUED) DISPOSAL OF HIGH-LEVEL RADIOACTIVE WASTES IN A GEOLOGIC REPOSITORY AT YUCCA MOUNTAIN, NEVADA Postclosure Public Health and Environmental Standards Human <span class="hlt">Intrusion</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol2/pdf/CFR-2014-title10-vol2-sec63-322.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title10-vol2/pdf/CFR-2014-title10-vol2-sec63-322.pdf"><span>10 CFR 63.322 - Human <span class="hlt">intrusion</span> scenario.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>... 10 Energy 2 2014-01-01 2014-01-01 false Human <span class="hlt">intrusion</span> scenario. 63.322 Section 63.322 Energy NUCLEAR REGULATORY COMMISSION (CONTINUED) DISPOSAL OF HIGH-LEVEL RADIOACTIVE WASTES IN A GEOLOGIC REPOSITORY AT YUCCA MOUNTAIN, NEVADA Postclosure Public Health and Environmental Standards Human <span class="hlt">Intrusion</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol2/pdf/CFR-2012-title10-vol2-sec63-322.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title10-vol2/pdf/CFR-2012-title10-vol2-sec63-322.pdf"><span>10 CFR 63.322 - Human <span class="hlt">intrusion</span> scenario.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-01-01</p> <p>... 10 Energy 2 2012-01-01 2012-01-01 false Human <span class="hlt">intrusion</span> scenario. 63.322 Section 63.322 Energy NUCLEAR REGULATORY COMMISSION (CONTINUED) DISPOSAL OF HIGH-LEVEL RADIOACTIVE WASTES IN A GEOLOGIC REPOSITORY AT YUCCA MOUNTAIN, NEVADA Postclosure Public Health and Environmental Standards Human <span class="hlt">Intrusion</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol2/pdf/CFR-2011-title10-vol2-sec63-322.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title10-vol2/pdf/CFR-2011-title10-vol2-sec63-322.pdf"><span>10 CFR 63.322 - Human <span class="hlt">intrusion</span> scenario.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-01-01</p> <p>... 10 Energy 2 2011-01-01 2011-01-01 false Human <span class="hlt">intrusion</span> scenario. 63.322 Section 63.322 Energy NUCLEAR REGULATORY COMMISSION (CONTINUED) DISPOSAL OF HIGH-LEVEL RADIOACTIVE WASTES IN A GEOLOGIC REPOSITORY AT YUCCA MOUNTAIN, NEVADA Postclosure Public Health and Environmental Standards Human <span class="hlt">Intrusion</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=219067&keyword=water+AND+vapor&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=219067&keyword=water+AND+vapor&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Vapour <span class="hlt">Intrusion</span> into Buildings - A Literature Review</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>This chapter provides a review of recent research on vapour <span class="hlt">intrusion</span> of volatile organic compounds (VOCs) into buildings. The chapter builds on a report from Tillman and Weaver (2005) which reviewed the literature on vapour <span class="hlt">intrusion</span> through 2005. Firstly, the term ‘vapour intru...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22982907','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22982907"><span>Perceived illness <span class="hlt">intrusions</span> among continuous ambulatory peritoneal dialysis patients.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bapat, Usha; Kedlya, Prashanth G</p> <p>2012-09-01</p> <p>To study the perceived illness <span class="hlt">intrusion</span> of continuous ambulatory peritoneal dialysis (CAPD) patients, to examine their demographics, and to find out the association among demographics, duration of illness as well as illness <span class="hlt">intrusion</span>, 40 chronic kidney disease stage V patients on CAPD during 2006-2007 were studied. Inclusion criteria were patients' above 18 years, willing, stable, and completed at least two months of dialysis. Those with psychiatric co-morbidity were excluded. Sociodemographics were collected using a semi-structured interview schedule. A 14-item illness <span class="hlt">intrusion</span> checklist covering various aspects of life was administered. The subjects had to rate the illness <span class="hlt">intrusion</span> in their daily life and the extent of <span class="hlt">intrusion</span>. The data was analyzed using descriptive statistics and chi square test of association. The mean age of the subjects was 56.05 ± 10.05 years. There was near equal distribution of gender. 82.5% were married, 70.0% belonged to Hindu religion, 45.0% were pre-degree, 25.0% were employed, 37.5% were housewives and 30.0% had retired. 77.5% belonged to the upper socioeconomic strata, 95.0% were from an urban background and 65.0% were from nuclear families. The mean duration of dialysis was 19.0 ± 16.49 months. Fifty-eight percent of the respondents were performing the dialysis exchanges by themselves. More than 95.0%were on three or four exchanges per day. All the 40 subjects reported illness <span class="hlt">intrusion</span> in their daily life. <span class="hlt">Intrusion</span> was perceived to some extent in the following areas: health 47.5%, work 25.0%, finance 37.5%, diet 40.0%, and psychological 50.0%. Illness had not intruded in the areas of relationship with spouse 52.5%, sexual life 30.0%, with friends 92.5%, with family 85.5%, social functions 52.5%, and religious functions 75.0%. Statistically significant association was not noted between illness <span class="hlt">intrusion</span> and other variables. CAPD patients perceived illness <span class="hlt">intrusion</span> to some extent in their daily life. Elderly, educated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V33D3150S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V33D3150S"><span>How to build a mid-crustal <span class="hlt">intrusive</span> suite: geologic mapping, U-Pb geo-/thermochronology, and thermal modeling of the Bergell <span class="hlt">Intrusion</span>, Central Alps</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Samperton, K. M.; Schoene, B.; Annen, C.</p> <p>2015-12-01</p> <p>Insights into the characteristic rates and processes of crustal magmatic systems can best be made through the integration of observational, analytical and modeling perspectives. We present such an approach in reconstructing the emplacement, differentiation and cooling history of the Bergell <span class="hlt">Intrusion</span> (N Italy/SE Switzerland), a normally-<span class="hlt">zoned</span> pluton preserving a ~10 km mid-crustal transect. U-Pb zircon, titanite and allanite geo-/thermochronology of Bergell granitoids provide key empirical constraints for informing numerical simulations of pulse-wise, incremental assembly. Protracted zircon crystallization histories, representing the time between magma zircon saturation and cooling to the solidus, provide a direct petrologic link to forward models of magma emplacement, both of which can be used to derive quantitative magmatic cooling rates for the middle crust. Titanite and allanite dates provide additional constraints on the timing of solidification. Geochronology and modeling are performed in the context of detailed field and structural observations, including those previously interpreted as evidence of upward, pluton-scale melt migration via floor convergence/roof ballooning. Combined Bergell data and modeling demonstrate that pulsed assembly can lead to the formation of substantial melt reservoirs in the middle crust: this finding is largely in contrast to similar models of shallow crustal plutons, highlighting the importance of factors such as ambient country rock temperature in affecting melt residence timescales. This work emphasizes the importance of implementing joint data/modeling studies to <span class="hlt">intrusive</span> rocks across the full range of spatial scales, emplacement levels and tectonic settings observed on Earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V11A0550M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V11A0550M"><span>High precision ages from the Torres del Paine <span class="hlt">Intrusion</span>, Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Michel, J.; Baumgartner, L.; Cosca, M.; Ovtcharova, M.; Putlitz, B.; Schaltegger, U.</p> <p>2006-12-01</p> <p>The upper crustal bimodal Torres del Paine <span class="hlt">Intrusion</span>, southern Chile, consists of the lower Paine-Mafic- Complex and the upper Paine-Granite. Geochronologically this bimodal complex is not well studied except for a few existing data from Halpern (1973) and Sanchez (2006). The aim of this study is to supplement the existing data and to constrain the age relations between the major magmatic pulses by applying high precision U-Pb dating on accessory zircons and 40Ar/39Ar-laser-step-heating-ages on biotites from the Torres del Paine <span class="hlt">Intrusion</span>. The magmatic rocks from mafic complex are fine to medium-grained and vary in composition from quartz- monzonites to granodiorites and gabbros. Coarse-grained olivine gabbros have intruded these rocks in the west. The granitic body is represented by a peraluminous, biotite-orthoclase-granite and a more evolved leucocratic granite in the outer parts towards the host-rock. Field observations suggest a feeder-<span class="hlt">zone</span> for the granite in the west and that the granite postdates the mafic complex. Two granite samples of the outermost margins in the Northeast and South were analyzed. The zircons were dated by precise isotope-dilution U-Pb techniques of chemically abraded single grains. The data are concordant within the analytical error and define weighted mean 206/238U ages of 12.59 ± 0.03 Ma and 12.58 ± 0.01 Ma for the two samples respectively. A 40Ar/39Ar-age for the second sample yield a date of 12.37 ± 0.11 Ma. Three 40Ar/39Ar -ages of biotites were obtained for rocks belonging to the mafic complex. A hbl-bio- granodiorite from the central part, approximately 150 m below the subhorizontal contact with the granite, gives an age of 12.81 ± 0.11 Ma. A hbl-bio-granodiorite and an olivine-gabbro west of the feeder-<span class="hlt">zone</span> date at 12.42 ± 0.14 Ma and 12.49 ± 0.11 Ma, respectively. The obtained older age of 12.81 Ma for the granodiorite in the central part is consistent with structural relationships of brittle fracturing of the mafic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1212440D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1212440D"><span>Granite <span class="hlt">intrusion</span> in a metamorphic core complex: the example of the Mykonos laccolith (Cyclades, Greece)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Denèle, Yoann; Lecomte, Emmanuel; Jolivet, Laurent; Huet, Benjamin; Labrousse, Loïc.; Le Pourhiet, Laetitia; Lacombe, Olivier</p> <p>2010-05-01</p> <p>Numerical and analogical modelling underlined the importance of a pre-existing anomaly of viscosity-density such as a granite or migmatitic body below the brittle-ductile transition as a primary cause of metamorphic core complex (MCC) developpement. While field studies of MCC show a spatial and temporal link between MCC formation and plutonic activity, thermochronological studies show that there is no link between the <span class="hlt">intrusion</span> of granites and the velocity of slip on the detachement plane. The Aegean domain is a good natural laboratory for studying the formation of MCC and syn-tectonic granites. In the northern Cyclades, the Mykonos-Delos-Rhenia MCC is characterised by the <span class="hlt">intrusion</span> of a plurikilometric Late Miocene pluton of I-type granite within a migmatitic gneiss dome. AMS (Anisotropy of magnetic susceptibility) and microstructural studies in the Mykonos granites combined with recent cooling rate data allow us to use the granites as strain marker. The Mykonos granitoïds form a plurikilometric laccolith slightly deeping to the east and presenting an elliptical shape with a N170°E long axis. The laccolith is strongly asymmetrical with an outlying root <span class="hlt">zone</span> in the SW cropping out on Delos and Rhenia islands and a major body mainly developed to the NE and cropping out on Mykonos Island. The laccolith consists of various petrographic facies presenting straight contacts that demonstrate emplacement by successive pulses of more or less differentiated magmas. The laccolith was developed at the interface between the Cycladic Basement and the Blueschists Unit and within the Blueschist Unit. Two events of deformation have been recorded in the granites. The first event is characterized by submagmatic and high to middle temperature protomylonite microstructures developped during or just after the <span class="hlt">intrusion</span>. The second event of deformation characterized by low temperature mylonites and cataclasites close to the major detachment fault corresponds to the localization of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGP43A1231D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGP43A1231D"><span>Geophysical Framework of a Rare Earth Element Enriched Terrane, Mountain Pass, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Denton, K. M.; Ponce, D. A.; Peacock, J.; Miller, D. M.; Miller, J. S.</p> <p>2016-12-01</p> <p>Carbonatite ore deposits continue to be the primary source for rare earth elements (REEs), however large viable REE ore deposits are uncommon. The Mountain Pass carbonatite deposit, located in the eastern Mojave Desert of California, is the largest economic deposit of light REEs in North America. A 1.417 Ga ultrapotassic suite (shonkinite, syenite, and granite) and a 1.375 Ga barite-bastnasite-rich carbonatite (sovite) ore deposit comprise the enclave of REE-enriched outcrops and <span class="hlt">dikes</span> that occupy a narrow ( 3 km) <span class="hlt">zone</span> of 1.7 Ga gneiss extending at least 10-km to the southeast from southern Clark Mountain. Modeling of gravity, magnetic, and magnetotelluric (MT) data reveals subsurface features that form the structural framework of the REE terrane. The carbonatite and ultrapotassic mafic suite is associated with a local gravity high that is superimposed on a 4 km-wide gravity terrace, likely related to less dense granitic gneiss basement. Although physical property data indicate that the <span class="hlt">intrusive</span> suite and carbonatite are essentially and nonmagnetic, aeromagnetic data indicate that these rocks occur along the eastern edge of a prominent north-northwest trending aeromagnetic high. This relationship suggests that they may have been preferentially emplaced along a <span class="hlt">zone</span> of weakness or fault. The source of the magnetic high is 2-3 km below the surface and coincides with a relatively electrically conductive (3 orders of magnitude higher than surrounding rock) feature. MT data indicate that the western edge of the magnetic feature could be connected to a deeper ( 8 km) conductive feature related to possible <span class="hlt">intrusions</span> and/or hydrothermal systems. The lack of a magnetic signature of the REE terrane can be explained by alteration of magnetite, given that the terrane lies within a broader alteration <span class="hlt">zone</span> and observed magnetic low. If so, such an alteration event, capable of remobilizing rare earth elements, likely occurred during or after emplacement of the <span class="hlt">intrusive</span> suite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009LNCS.5755..500Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009LNCS.5755..500Z"><span>A New <span class="hlt">Intrusion</span> Detection Method Based on Antibody Concentration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zeng, Jie; Li, Tao; Li, Guiyang; Li, Haibo</p> <p></p> <p>Antibody is one kind of protein that fights against the harmful antigen in human immune system. In modern medical examination, the health status of a human body can be diagnosed by detecting the <span class="hlt">intrusion</span> intensity of a specific antigen and the concentration indicator of corresponding antibody from human body’s serum. In this paper, inspired by the principle of antigen-antibody reactions, we present a New <span class="hlt">Intrusion</span> Detection Method Based on Antibody Concentration (NIDMBAC) to reduce false alarm rate without affecting detection rate. In our proposed method, the basic definitions of self, nonself, antigen and detector in the <span class="hlt">intrusion</span> detection domain are given. Then, according to the antigen <span class="hlt">intrusion</span> intensity, the change of antibody number is recorded from the process of clone proliferation for detectors based on the antigen classified recognition. Finally, building upon the above works, a probabilistic calculation method for the <span class="hlt">intrusion</span> alarm production, which is based on the correlation between the antigen <span class="hlt">intrusion</span> intensity and the antibody concen-tration, is proposed. Our theoretical analysis and experimental results show that our proposed method has a better performance than traditional methods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS1000a2049J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS1000a2049J"><span>A Survey on Anomaly Based Host <span class="hlt">Intrusion</span> Detection System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jose, Shijoe; Malathi, D.; Reddy, Bharath; Jayaseeli, Dorathi</p> <p>2018-04-01</p> <p>An <span class="hlt">intrusion</span> detection system (IDS) is hardware, software or a combination of two, for monitoring network or system activities to detect malicious signs. In computer security, designing a robust <span class="hlt">intrusion</span> detection system is one of the most fundamental and important problems. The primary function of system is detecting <span class="hlt">intrusion</span> and gives alerts when user tries to <span class="hlt">intrusion</span> on timely manner. In these techniques when IDS find out <span class="hlt">intrusion</span> it will send alert massage to the system administrator. Anomaly detection is an important problem that has been researched within diverse research areas and application domains. This survey tries to provide a structured and comprehensive overview of the research on anomaly detection. From the existing anomaly detection techniques, each technique has relative strengths and weaknesses. The current state of the experiment practice in the field of anomaly-based <span class="hlt">intrusion</span> detection is reviewed and survey recent studies in this. This survey provides a study of existing anomaly detection techniques, and how the techniques used in one area can be applied in another application domain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T51B0447M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T51B0447M"><span>The temporal and spatial distribution of upper crustal faulting and magmatism in the south Lake Turkana rift, East Africa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muirhead, J.; Scholz, C. A.</p> <p>2017-12-01</p> <p>During continental breakup extension is accommodated in the upper crust largely through <span class="hlt">dike</span> <span class="hlt">intrusion</span> and normal faulting. The Eastern branch of the East African Rift arguably represents the premier example of active continental breakup in the presence magma. Constraining how faulting is distributed in both time and space in these regions is challenging, yet can elucidate how extensional strain localizes within basins as rifting progresses to sea-floor spreading. Studies of active rifts, such as the Turkana Rift, reveal important links between faulting and active magmatic processes. We utilized over 1100 km of high-resolution Compressed High Intensity Radar Pulse (CHIRP) 2D seismic reflection data, integrated with a suite of radiocarbon-dated sediment cores (3 in total), to constrain a 17,000 year history of fault activity in south Lake Turkana. Here, a set of N-S-striking intra-rift faults exhibit time-averaged slip-rates as high as 1.6 mm/yr, with the highest slip-rates occurring along faults within 3 km of the rift axis. Results show that strain has localized into a <span class="hlt">zone</span> of intra-rift faults along the rift axis, forming an approximately 20 km-wide graben in central parts of the basin. Subsurface structural mapping and fault throw profile analyses reveal increasing basin subsidence and fault-related strain as this faulted graben approaches a volcanic island in the center of the basin (South Island). The long-axis of this island trends north-south, and it contains a number of elongate cones that support recent emplacement of N-S-striking <span class="hlt">dike</span> <span class="hlt">intrusions</span>, which parallel recently active intra-rift faults. Overall, these observations suggest strain localization into intra-rift faults in the rift center is likely a product of both volcanic loading and the mechanical and thermal effects of <span class="hlt">diking</span> along the rift axis. These results support the establishment of magmatic segmentation in southern Lake Turkana, and highlight the importance of magmatism for focusing upper</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.2583H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.2583H"><span>Disequilibrium dihedral angles in layered <span class="hlt">intrusions</span>: the microstructural record of fractionation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holness, Marian; Namur, Olivier; Cawthorn, Grant</p> <p>2013-04-01</p> <p>The dihedral angle formed at junctions between two plagioclase grains and a grain of augite is only rarely in textural equilibrium in gabbros from km-scale crustal layered <span class="hlt">intrusions</span>. The median of a population of these disequilibrium angles, Θcpp, varies systematically within individual layered <span class="hlt">intrusions</span>, remaining constant over large stretches of stratigraphy with significant increases or decreases associated with the addition or reduction respectively of the number of phases on the liquidus of the bulk magma. The step-wise changes in Θcpp are present in Upper <span class="hlt">Zone</span> of the Bushveld Complex, the Megacyclic Unit I of the Sept Iles <span class="hlt">Intrusion</span>, and the Layered Series of the Skaergaard <span class="hlt">Intrusion</span>. The plagioclase-bearing cumulates of Rum have a bimodal distribution of Θcpp, dependent on whether the cumulus assemblage includes clinopyroxene. The presence of the step-wise changes is independent of the order of arrival of cumulus phases and of the composition of either the cumulus phases or the interstitial liquid inferred to be present in the crystal mush. Step-wise changes in the rate of change in enthalpy with temperature (ΔH) of the cooling and crystallizing magma correspond to the observed variation of Θcpp, with increases of both ΔH and Θcpp associated with the addition of another liquidus phase, and decreases of both associated with the removal of a liquidus phase. The replacement of one phase by another (e.g. olivine ⇔ orthpyroxene) has little effect on ΔH and no discernible effect on Θcpp. An increase of ΔH is manifest by an increase in the fraction of the total enthalpy budget that is the latent heat of crystallization (the fractional latent heat). It also results in an increase in the amount crystallized in each incremental temperature drop (the crystal productivity). An increased fractional latent heat and crystal productivity result in an increased rate of plagioclase growth compared to that of augite during the final stages of solidification</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.H11B0482T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.H11B0482T"><span>The Effect of Freezing on the Dynamics of <span class="hlt">Dike</span> Propagation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tait, S.; Taisne, B.</p> <p>2007-12-01</p> <p>When magma-filled cracks propagate close to the Earth's surface, host rock temperature is well below the magma solidus. Solidification and substantial increase in magma viscosity can occur, are most pronounced near the propagating tip and can slow or arrest the progress of the <span class="hlt">dike</span>. Quantitative analysis is required to predict whether a given <span class="hlt">dike</span> will reach the surface to erupt and the duration of the precursor sequence. This challenging physical problem mixes elasticity, fracture mechanics, heat transfer and fluid flow with strong rheologic gradients due to cooling. We describe the propagation behaviour of such a hydraulic fracture using a laboratory experimental system of a crack fed by a constant flux of paraffin wax from a source reservoir propagating through gelatin below the solidus of the wax. The most novel behaviour is an intermittent regime in which cracks periodically stop advancing due to solidification, then swell at constant length while enhancing the elastic deformation in the surrounding solid before propagation resumes. We present a physical model of this system, based on different balances between driving and resistive forces: the former are elastic stress and liquid buoyancy, the latter are fracture resistance at the tip and viscous resistance. The fracture is represented as a head, behind the propagating tip, connected to the source by a narrow tail. Freezing of liquid close to the tip is assumed to enhance fracture resistance according to a cooling law, and propagation is assumed to occur only when the stress exerted by the liquid is enough to overcome fracture resistance. Our theoretical model reproduces intermittent propagation with precise behaviour depending on the controlling stress balances, and provides a tool to analyse natural systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=257981','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=257981"><span>Furrow <span class="hlt">diking</span> and the economic water use efficiency of irrigated cotton in the southeast United States</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Cotton (Gossypium hirsutum L.) production in the Southeast United States can be limited by periodic drought. Irrigation and furrow <span class="hlt">diking</span> tillage may improve economic yield and water use efficiency of cotton. Timing of rainfall may interfere with the efficiency of irrigation. Field studies were c...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SPIE.8768E..6UC','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SPIE.8768E..6UC"><span>A new <span class="hlt">intrusion</span> prevention model using planning knowledge graph</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cai, Zengyu; Feng, Yuan; Liu, Shuru; Gan, Yong</p> <p>2013-03-01</p> <p>Intelligent plan is a very important research in artificial intelligence, which has applied in network security. This paper proposes a new <span class="hlt">intrusion</span> prevention model base on planning knowledge graph and discuses the system architecture and characteristics of this model. The <span class="hlt">Intrusion</span> Prevention based on plan knowledge graph is completed by plan recognition based on planning knowledge graph, and the <span class="hlt">Intrusion</span> response strategies and actions are completed by the hierarchical task network (HTN) planner in this paper. <span class="hlt">Intrusion</span> prevention system has the advantages of intelligent planning, which has the advantage of the knowledge-sharing, the response focused, learning autonomy and protective ability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA567369','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA567369"><span>Vapor <span class="hlt">Intrusion</span> Assessment and Mitigation 2012</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-03-26</p> <p>1 Geosyntec 0 consultants Vapor <span class="hlt">Intrusion</span> Assessment and Mitigation 2012 Robert Ettinger, M.S., P.E., Todd McAiary, M.Sc., P.Eng., P.G...REPORT DATE 26 MAR 2012 2. REPORT TYPE 3. DATES COVERED 00-00-2012 to 00-00-2012 4. TITLE AND SUBTITLE Vapor <span class="hlt">Intrusion</span> Assessment and...Updates • Typical Assessment Approaches and Common Challenges • Methods to Distinguish Background Sources (McHugh) • Significance • Compound</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830020177','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830020177"><span>Small Gas Turbine Combustor Primary <span class="hlt">Zone</span> Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sullivan, R. E.; Young, E. R.; Miles, G. A.; Williams, J. R.</p> <p>1983-01-01</p> <p>A development process is described which consists of design, fabrication, and preliminary test evaluations of three approaches to internal aerodynamic primary <span class="hlt">zone</span> flow patterns: (1) conventional double vortex swirl stabilization; (2) reverse flow swirl stabilization; and (3) large single vortex flow system. Each concept incorporates special design features aimed at extending the performance capability of the small engine combustor. Since inherent geometry of these combustors result in small combustion <span class="hlt">zone</span> height and high surface area to volume ratio, design features focus on internal aerodynamics, fuel placement, and advanced cooling. The combustors are evaluated on a full scale annular combustor rig. A correlation of the primary <span class="hlt">zone</span> performance with the overall performance is accomplished using three <span class="hlt">intrusion</span> type gas sampling probes located at the exit of the primary <span class="hlt">zone</span> section. Empirical and numerical methods are used for designing and predicting the performance of the three combustor concepts and their subsequent modifications. The calibration of analytical procedures with actual test results permits an updating of the analytical design techniques applicable to small reverse flow annular combustors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V33F0569H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V33F0569H"><span>Noble gas systematics of the Skaergaard <span class="hlt">intrusion</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horton, F.; Farley, K. A.; Taylor, H. P.</p> <p>2017-12-01</p> <p>The noble gas isotopic compositions of olivines from the Skaergaard layered mafic <span class="hlt">intrusion</span> in Greenland reveal that magmas readily exchange noble gases with their environment after emplacement. Although Skaergaard magmas are thought to have derived from the upper mantle, all of the olivine separates we analyzed have 3He/4He ratios less than that of the upper mantle ( 8 Ra, where Ra = 3He/4He of the atmosphere, 1.39 x 10-6). This suggests that crustal and/or atmospheric noble gases have contaminated all Skaergaard magmas to some extent. We obtained the highest 3He/4He ratios ( 2 Ra) from olivines found in the lowermost exposed layers of the <span class="hlt">intrusion</span> away from the margins. Excess radiogenic 4He (indicated by Ra<1) along the margin of the <span class="hlt">intrusion</span> indicates that noble gases from the Archean host-rock were incorporated into the cooling magma chamber, probably via magmatic assimilation. Noble gases in olivines from the upper portions of the <span class="hlt">intrusion</span> have atmospheric isotopic compositions, but higher relative helium abundances than the atmosphere. We suggest that post-crystallization hydrothermal circulation introduced atmosphere-derived noble gases into uppermost layers of the <span class="hlt">intrusion</span>. Such high temperature exchanges of volatiles between plutons and their immediate surroundings may help explain why so few mantle-derived rocks retain mantle-like noble gas signatures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMGP51C1094S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMGP51C1094S"><span>Gravity and magnetic anomalies used to delineate geologic features associated with earthquakes and aftershocks in the central Virginia seismic <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shah, A. K.; Horton, J.; McNamara, D. E.; Spears, D.; Burton, W. C.</p> <p>2013-12-01</p> <p> aftershocks appear to cluster near areas with cross-cutting geologic features such as Jurassic diabase <span class="hlt">dikes</span>. These associations suggest that local variations in rock density and/or rheology may have contributed to modifications of local stress regimes in a manner encouraging localized seismicity associated with the Mw5.8 event and its aftershocks. Such associations are comparable to results of previous studies recognizing correspondences between seismicity and features such as <span class="hlt">intrusive</span> bodies and failed rifts in the New Madrid seismic <span class="hlt">zone</span> and elsewhere. To explore whether similar correspondences may have occurred in the past, we use regional gravity and magnetic data to consider possible relations between historical earthquakes and comparable geologic features elsewhere in the central Virginia seismic <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.8269V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.8269V"><span>Oxygen <span class="hlt">intrusion</span> into anoxic fjords leads to increased methylmercury availability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Veiteberg Braaten, Hans Fredrik; Pakhomova, Svetlana; Yakushev, Evgeniy</p> <p>2013-04-01</p> <p>Mercury (Hg) appears in the oxic surface waters of the oceans at low levels (sub ng/L). Because inorganic Hg can be methylated into the toxic and bioaccumulative specie methylmercury (MeHg) levels can be high at the top of the marine food chain. Even though marine sea food is considered the main risk driver for MeHg exposure to people most research up to date has focused on Hg methylation processes in freshwater systems. This study identifies the mechanisms driving formation of MeHg during oxygen depletion in fjords, and shows how MeHg is made available in the surface water during oxygen <span class="hlt">intrusion</span>. Studies of the biogeochemical structure in the water column of the Norwegian fjord Hunnbunn were performed in 2009, 2011 and 2012. In autumn of 2011 mixing flushing events were observed and lead to both positive and negative effects on the ecosystem state in the fjord. The oxygenated water <span class="hlt">intrusions</span> lead to a decrease of the deep layer concentrations of hydrogen sulfide (H2S), ammonia and phosphate. On the other hand the <span class="hlt">intrusion</span> also raised the H2S boundary from 8 m to a shallower depth of just 4 m. Following the <span class="hlt">intrusion</span> was also observed an increase at shallower depths of nutrients combined with a decrease of pH. Before flushing events were observed concentrations of total Hg (TotHg) increased from 1.3 - 1.7 ng/L in the surface layer of the fjord to concentrations ranging from 5.2 ng/L to 6.4 ng/L in the anoxic <span class="hlt">zone</span>. MeHg increased regularly from 0.04 ng/L in the surface water to a maximum concentration of 5.2 ng/L in the deeper layers. This corresponds to an amount of TotHg present as MeHg ranging from 2.1 % to 99 %. The higher concentrations of MeHg in the deeper layer corresponds to an area where no oxygen is present and concentrations of H2S exceeds 500 µM, suggesting a production of MeHg in the anoxic area as a result of sulphate reducing bacteria activity. After flushing the concentrations of TotHg showed a similar pattern ranging from 0.6 ng/L in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70000346','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70000346"><span>Physical rock properties in and around a conduit <span class="hlt">zone</span> by well-logging in the Unzen Scientific Drilling Project, Japan</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ikeda, R.; Kajiwara, T.; Omura, K.; Hickman, S.</p> <p>2008-01-01</p> <p>The objective of the Unzen Scientific Drilling Project (USDP) is not only to reveal the structure and eruption history of the Unzen volcano but also to clarify the ascent and degassing mechanisms of the magma conduit. Conduit drilling (USDP-4) was conducted in 2004, which targeted the magma conduit for the 1990-95 eruption. The total drilled length of USDP-4 was 1995.75??m. Geophysical well logging, including resistivity, gamma-ray, spontaneous potential, sonic-wave velocity, density, neutron porosity, and Fullbore Formation MicroImager (FMI), was conducted at each drilling stage. Variations in the physical properties of the rocks were revealed by the well-log data, which correlated with not only large-scale formation boundaries but also small-scale changes in lithology. Such variations were evident in the lava <span class="hlt">dike</span>, pyroclastic rocks, and breccias over depth intervals ranging from 1 to 40??m. These data support previous models for structure of the lava conduit, in that they indicate the existence of alternating layers of high-resistivity and high P-wave velocity rocks corresponding to the lava <span class="hlt">dikes</span>, in proximity to narrower <span class="hlt">zones</span> exhibiting high porosity, low resistivity, and low P-wave velocity. These narrow, low-porosity <span class="hlt">zones</span> are presumably higher in permeability than the adjacent rocks and may form preferential conduits for degassing during magma ascent. ?? 2008 Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V11A0359M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V11A0359M"><span>Cup-shaped <span class="hlt">Intrusions</span>, Morphology and Emplacement Mechanism Investigate Through Analogue Modelling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mathieu, L.; van Wyk de Vries, B.</p> <p>2007-12-01</p> <p>We investigate the morphology of large-scale shallow-depth magma <span class="hlt">intrusions</span> and sub-volcanic complexes with analogue models. <span class="hlt">Intrusions</span> of analogue magma are done in a granular material that can contain a ductile layer. The model surface is flat to model the formation of plutonic <span class="hlt">intrusions</span> and it is overlain by a cone when modelling late sub-volcanic complexes. For flat-top models, we obtain cup-shaped <span class="hlt">intrusions</span> fed by dykes. Cup-shaped <span class="hlt">intrusions</span> are inverted-cone like bodies. They are different from saucer-shaped <span class="hlt">intrusions</span> as they possess neither a well developed sill-base, nor an outer rim. However, like saucers, cups are shallow depth <span class="hlt">intrusions</span> that dome the country rocks. They initiate from an advancing dyke and first develop an inverted-cone like morphology. Then, the central thickness increases and thrusts form at the edge of the domed country rocks. At this stage, the <span class="hlt">intrusions</span> progressively involve toward a lopolith shape. By using analogue magma of various viscosities we have been able to constrain key relationships: higher <span class="hlt">intrusion</span> viscosity causes deeper initiation and the deeper they initiate, the larger is the <span class="hlt">intrusion</span> diameter. A natural example of such <span class="hlt">intrusion</span> might by the circles of volcanoes like the Azufre-Lastaria (Peru) that might be overlain be a large-scale cup-shaped <span class="hlt">intrusion</span>. When adding a cone at the surface of the model and, sometimes, a thin ductile layer in the substratum, the morphology of cup-shaped <span class="hlt">intrusions</span> vary. Note that the ductile layer of our models is not thick enough to induce the gravitational spreading of the cone. Generally, cup-shaped <span class="hlt">intrusions</span> are asymmetric in cross section and elliptical in plan view. Their formation creates extension structures in the cone (croissant-shaped rift, straight rift or normal fault) and thrusts in some sectors below the cone. Both types of structures are bordered by strike-slip faults. Cups and saucers share many similarities, but differ probably in the fact that saucers are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JVGR...92..389W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JVGR...92..389W"><span>Effects of shallow basaltic <span class="hlt">intrusion</span> into pyroclastic deposits, Grants Ridge, New Mexico, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>WoldeGabriel, Giday; Keating, Gordon N.; Valentine, Greg A.</p> <p>1999-10-01</p> <p>A localized aureole up to 10 m wide developed around a 150-m-wide, 2.6 Ma basaltic plug at Grants Ridge, New Mexico. The plug intruded into nonwelded, pumice-rich compositionally homogenous tuff and volcaniclastic sediments of similar age (3.3 Ma). Color variation (pinkish to orange), strong local contact welding, brecciation, partial melting, and stoping characterize the host rock within the contact <span class="hlt">zone</span>. Despite the high-temperature basaltic <span class="hlt">intrusion</span>, there is no indication of extensive fluid-driven convective heat transfer and pervasive hydrothermal circulation and alteration of the country rock. The proportion of volcanic glass, loss on ignition (LOI), fluorine, iron, and some trace and rare earth element contents in the host rocks are somewhat depleted at the contact of the <span class="hlt">intrusion</span>. Conversely, the degree of devitrification and the potassium content are higher along the contact. Vapor-phase expulsion of elemental species as complexes of fluoride, chloride, hydroxide, sulfide, and carbon dioxide may have been responsible for the minor depletion of the elements during the devitrification of silicic glass at near-solidus temperature related to the basaltic <span class="hlt">intrusion</span>. The results of finite-difference numerical modeling of the <span class="hlt">intrusion</span> as a dry, conduction-dominated system agree well with geochemical and mineralogical data. Contact welding of the host rocks apparently occurred at temperatures >700°C under a density-driven lateral load of approximately 1 MPa, corresponding to the observed depth below the former ground surface of ˜100 m. Other physical changes in the first 10 m of host rock, represented by partial devitrification and color changes, apparently occurred at temperatures of 500-600°C, which probably persisted for up to 55 years after the emplacement of the basaltic plug. Devitrification is generally enhanced by the presence of aqueous fluids; however, the abundance of volcanic glass within a short distance (˜10 m) from the plug is consistent with</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JOUC...16..991D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JOUC...16..991D"><span>Operational wave now- and forecast in the German Bight as a basis for the assessment of wave-induced hydrodynamic loads on coastal <span class="hlt">dikes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dreier, Norman; Fröhle, Peter</p> <p>2017-12-01</p> <p>The knowledge of the wave-induced hydrodynamic loads on coastal <span class="hlt">dikes</span> including their temporal and spatial resolution on the <span class="hlt">dike</span> in combination with actual water levels is of crucial importance of any risk-based early warning system. As a basis for the assessment of the wave-induced hydrodynamic loads, an operational wave now- and forecast system is set up that consists of i) available field measurements from the federal and local authorities and ii) data from numerical simulation of waves in the German Bight using the SWAN wave model. In this study, results of the hindcast of deep water wave conditions during the winter storm on 5-6 December, 2013 (German name `Xaver') are shown and compared with available measurements. Moreover field measurements of wave run-up from the local authorities at a sea <span class="hlt">dike</span> on the German North Sea Island of Pellworm are presented and compared against calculated wave run-up using the EurOtop (2016) approach.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=self+AND+harming&pg=5&id=EJ754486','ERIC'); return false;" href="https://eric.ed.gov/?q=self+AND+harming&pg=5&id=EJ754486"><span><span class="hlt">Intrusive</span> Memories in Perpetrators of Violent Crime: Emotions and Cognitions</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Evans, Ceri; Ehlers, Anke; Mezey, Gillian; Clark, David M.</p> <p>2007-01-01</p> <p>The authors investigated factors that may determine whether perpetrators of violent crime develop <span class="hlt">intrusive</span> memories of their offense. Of 105 young offenders who were convicted of killing or seriously harming others, 46% reported distressing <span class="hlt">intrusive</span> memories, and 6% had posttraumatic stress disorder. <span class="hlt">Intrusions</span> were associated with lower…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990JGR....9513357S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990JGR....9513357S"><span>Wind-forced salt <span class="hlt">intrusion</span> into a tributary estuary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sanford, Lawrence P.; Boicourt, William C.</p> <p>1990-08-01</p> <p>Moored measurements and hydrographic surveys were carried out during the summers of 1986 and 1987 to examine interaction between the mainstem of the Chesapeake Bay and the Choptank River, an eastern shore tributary estuary. The data show that an important mode of interaction is through wind-forced <span class="hlt">intrusion</span> of saline, hypoxic water from below the pycnocline of the Bay into the lower river. <span class="hlt">Intrusions</span> are driven by lateral tilting of the pycnocline in the Bay, when high salinity water is upwelled on the eastern side of the Bay in response to a southward pulse of wind stress. The resulting internal surges propagate up the relict Choptank entrance channel at a speed of about 20 cm/s and spill onto the broad sill inside the mouth of the river. <span class="hlt">Intrusion</span>-favorable pycnocline tilts in the Bay do not always result in lower layer <span class="hlt">intrusion</span> into the Choptank, but may be blocked or choked in the entrance channel on occasion. The data suggest that wind-forced <span class="hlt">intrusion</span> of salt leads to increased gravitational circulation in the Choptank during the summer months, providing a mechanism through which high frequency energy may be directly translated into lower frequency motion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4283725','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4283725"><span>Heart rate, startle response, and <span class="hlt">intrusive</span> trauma memories</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chou, Chia-Ying; Marca, Roberto La; Steptoe, Andrew; Brewin, Chris R</p> <p>2014-01-01</p> <p>The current study adopted the trauma film paradigm to examine potential moderators affecting heart rate (HR) as an indicator of peritraumatic psychological states and as a predictor of <span class="hlt">intrusive</span> memories. We replicated previous findings that perifilm HR decreases predicted the development of <span class="hlt">intrusive</span> images and further showed this effect to be specific to images rather than thoughts, and to detail rather than gist recognition memory. Moreover, a group of individuals showing both an atypical sudden reduction in HR after a startle stimulus and higher trait dissociation was identified. Only among these individuals was lower perifilm HR found to indicate higher state dissociation, fear, and anxiety, along with reduced vividness of <span class="hlt">intrusions</span>. The current findings emphasize how peritraumatic physiological responses relate to emotional reactions and <span class="hlt">intrusive</span> memory. The moderating role of individual difference in stress defense style was highlighted. PMID:24397333</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16484108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16484108"><span><span class="hlt">Intrusion</span> errors in visuospatial working memory performance.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cornoldi, Cesare; Mammarella, Nicola</p> <p>2006-02-01</p> <p>This study tested the hypothesis that failure in active visuospatial working memory tasks involves a difficulty in avoiding <span class="hlt">intrusions</span> due to information that is already activated. Two experiments are described, in which participants were required to process several series of locations on a 4 x 4 matrix and then to produce only the final location of each series. Results revealed a higher number of errors due to already activated locations (<span class="hlt">intrusions</span>) compared with errors due to new locations (inventions). Moreover, when participants were required to pay extra attention to some irrelevant (non-final) locations by tapping on the table, <span class="hlt">intrusion</span> errors increased. Results are discussed in terms of current models of working memory functioning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014DokES.458.1261S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014DokES.458.1261S"><span>Trondhjemite-granodiorite <span class="hlt">intrusive</span> magmatism of the Losevo lithotectonic <span class="hlt">zone</span> of the Voronezh crystalline massif</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Skryabin, V. Yu.; Terentiev, R. A.</p> <p>2014-10-01</p> <p>The mineralogical-petrographic, petrochemical, and geochemical characteristics of the trondhjemite-granodiorite <span class="hlt">intrusions</span> widespread among the volcanoterrigenous rocks of the eastern part of the Voronezh crystalline massif are studied. The rocks are characterized by cotectic quartz-plagioclase differentiation and differentiated (La/Yb = 31) REE pattern and are enriched in LILE with a decrease in the K/Rb and Zr/Hf ratios and an increase in the Th/U ratio by 1.5-2 times relative to subduction trondhjemites and their volcanic analogs from the modern and young island arcs. These data allow us to conclude that generation of the trondhjemite magma is a result of melting of the rocks of the continental crust during collision. The concordant (SHRIMP) age of trondhjemites is 2047 ± 11 Ma, and the age of zircon cores probably entrapped from the host rocks by the trondhjemitic melt is 2172 ± 17 Ma.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA622509','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA622509"><span>Porting Extremely Lightweight <span class="hlt">Intrusion</span> Detection (ELIDe) to Android</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-10-01</p> <p>ARL-TN-0681 ● OCT 2015 US Army Research Laboratory Porting Extremely Lightweight <span class="hlt">Intrusion</span> Detection (ELIDe) to Android by...Lightweight <span class="hlt">Intrusion</span> Detection (ELIDe) to Android by Ken F Yu and Garret S Payer Computational and Information Sciences Directorate, ARL...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T41C0648L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T41C0648L"><span>Fault <span class="hlt">zone</span> property near Xinfengjiang Reservoir using dense, across-fault seismic array</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, M. H. B.; Yang, H.; Sun, X.</p> <p>2017-12-01</p> <p>Properties of fault <span class="hlt">zones</span> are important to the understanding of earthquake process. Around the fault <span class="hlt">zone</span> is a damaged <span class="hlt">zone</span> which is characterised by a lower seismic velocity. This is detectable as a low velocity <span class="hlt">zone</span> and measure some physical property of the fault <span class="hlt">zone</span>, which is otherwise difficult sample directly. A dense, across-fault array of short period seismometer is deployed on an inactive fault near Xinfengjiang Reservoir. Local events were manually picked. By computing the synthetic arrival time, we were able to constrain the parameters of the fault <span class="hlt">zone</span> Preliminary result shows that the fault <span class="hlt">zone</span> is around 350 m wide with a P and S velocity increase of around 10%. The fault is geologically inferred, and this result suggested that it may be a geological layer. The other possibility is that the higher velocity is caused by a combination of fault <span class="hlt">zone</span> healing and fluid <span class="hlt">intrusion</span>. Whilst the result was not able to tell us the nature of the fault, it demonstrated that this method is able to derive properties from a fault <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1958/0079/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1958/0079/report.pdf"><span>The geology and ore deposits of Upper Mayflower Gulch, Summit County, Colorado</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Randall, John Alexander</p> <p>1958-01-01</p> <p>Upper Mayflower Gulch is on the highly glaciated western side of the Tenmile Range near Kokomo in central Colorado. Somewhat less than $500,000 in silver and gold has been produced from the area since the first mining in the 1880' s. In the mapped area high grade regional metamorphism has produced two varieties of gneiss and a granulite. Total thickness of the rocks is about 5,000 feet. Relict bedding is preserved in compositional banding which strikes north to N. 20 ? E. and dips 70 ? to 80 ? southeast. No significant folding was observed. Normal faulting has occurred since the Precambrian; two major sets of faults are recognizable: (1) a set striking N. 70 ? to 85 ? E. and dipping 75?-85 ? NW; and (2) a set striking N. 70?-50 ? W. and dipping 50?-60 ? SW. Tabular bodies of pegmatite and retrogressively metamorphosed schist along many faults indicate Precambrian movement. The Mayflower fault, a 90 to 300 foot wide <span class="hlt">zone</span> of siltification and shattered rock, strikes about N. 40 ? W. It extends the entire length of the gulch and appears to form the northern terminus for the northeast trending Mosquito Fault. The Mayflower fault shows repeated movement since the Precambrian, totaling about 3,000 feet of apparent dip slip and 640 feet of apparent strike slip. Faulting during the Tertiary includes both additional movement along Precambrian faults and development of shears trending N. to N. 20 ? E. The shears served as channels for the <span class="hlt">intrusion</span> of two varieties of quartz latite porphyry <span class="hlt">dikes</span>. Specular hematite and base-metal sulfide mineralization followed <span class="hlt">intrusion</span> of the porphyry <span class="hlt">dikes</span>; the minerals were deposited in open fault <span class="hlt">zones</span> by high temperature solutions in a low pressure environment. The principal metallic minerals in order of deposition are: hematite, pyrite, chalcopyrite, sphalerite, galena, and rarer argentite. The major mines are the Gold Crest, Payrock, Nova Scotia Boy, and Bird's Nest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018999','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018999"><span>Late Cretaceous remagnetization of Proterozoic mafic <span class="hlt">dikes</span>, southern Highland Mountains, southwestern Montana: A paleomagnetic and 40Ar/39Ar study</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Harlan, S.S.; Geissman, J.W.; Snee, L.W.; Reynolds, R.L.</p> <p>1996-01-01</p> <p>Paleomagnetic results from Early Proterozoic metabasite sills and Middle Proterozoic diabase <span class="hlt">dikes</span> from the southern Highland Mountains of southwestern Montana give well-defined, dual-polarity magnetizations that are statistically identical to those from a small Late Cretaceous pluton that cuts the <span class="hlt">dikes</span>. The concordance of paleomagnetic directions from rocks of three widely separated ages indicates that the Proterozoic rocks were remagnetized, probably during Late Cretaceous time. Paleomagnetic, rock magnetic, and petrographic observations from the metabasite and diabase samples indicate that remanence is carried primarily by low-Ti magnetite. Combining virtual geomagnetic poles from metabasite sills, diabase <span class="hlt">dikes</span>, and the Late Cretaceous pluton, we obtain a paleomagnetic pole at 85.5??N, 310.7??E (K = 19.9, A95 = 9.1??, N = 14 sites) that is similar to a reference pole from the 74 Ma Adel Mountain Volcanics of western Montana. Biotite and hornblende 40Ar/39Ar isotopic dates from host basement geneiss and a hornblende from a remagnetized metabasite sill yield ages of ca. 1800 Ma; these dates probably record cooling of the southern Highland Mountains following high-grade metamorphism at 1.9-1.8 Ga. The gneiss and metabasite age spectra show virtually no evidence of disturbance, indicating that the basement rocks were never heated to temperatures sufficient to cause even partial resetting of their argon systems. Thus, the overprint magnetization of the Highland Mountains rocks is not a thermoremanent magnetization acquired during conductive cooling of nearby Late Cretaceous plutons. Remagnetization of the metabasite sills and diabase <span class="hlt">dikes</span> was probably caused by localized thermochemical and thermoviscous effects during circulation of Late Cretaceous hydrothermal fluids related to epithermal mineralization. The absence of significant disturbance to the 40Ar/39Ar age spectrum from the remagnetized metabasite hornblende indicates that some secondary magnetizations may</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70029364','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029364"><span>Surface deformation associated with the March 1996 earthquake swarm at Akutan Island, Alaska, revealed by C-band ERS and L-band JERS radar interferometry</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lu, Z.; Wicks, C.; Kwoun, O.; Power, J.A.; Dzurisin, D.</p> <p>2005-01-01</p> <p>In March 1996, an intense earthquake swarm beneath Akutan Island, Alaska, was accompanied by extensive ground cracking but no eruption of Akutan volcano. Radar interferograms produced from L-band JERS-1 and C-band ERS-1/2 images show uplift associated with the swarm by as much as 60 cm on the western part of the island. The JERS-1 interferogram has greater coherence, especially in areas with loose surface material or thick vegetation. It also shows subsidence of similar magnitude on the eastern part of the island and displacements along faults reactivated during the swarm. The axis of uplift and subsidence strikes about N70??W, which is roughly parallel to a <span class="hlt">zone</span> of fresh cracks on the northwest flank of the volcano, to normal faults that cut the island and to the inferred maximum compressive stress direction. A common feature of models that fit the deformation is the emplacement of a shallow <span class="hlt">dike</span> along this trend beneath the northwest flank of the volcano. Both before and after the swarm, the northwest flank was uplifted 5-20 mm/year relative to the southwest flank, probably by magma <span class="hlt">intrusion</span>. The <span class="hlt">zone</span> of fresh cracks subsided about 20 mm during 1996-1997 and at lesser rates thereafter, possibly because of cooling and degassing of the <span class="hlt">intrusion</span>. ?? 2005 CASI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21491252','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21491252"><span>The appraisal of <span class="hlt">intrusive</span> thoughts in relation to obsessional-compulsive symptoms.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barrera, Terri L; Norton, Peter J</p> <p>2011-01-01</p> <p>Research has shown that although <span class="hlt">intrusive</span> thoughts occur universally, the majority of individuals do not view <span class="hlt">intrusive</span> thoughts as being problematic (Freeston, Ladouceur, Thibodeau, & Gagnon, 1991; Rachman & de Silva, 1978; Salkovskis & Harrison, 1984). Thus, it is not the presence of <span class="hlt">intrusive</span> thoughts that leads to obsessional problems but rather some other factor that plays a role in the development of abnormal obsessions. According to the cognitive model of obsessive-compulsive disorder (OCD) put forth by Salkovskis (1985), the crucial factor that differentiates between individuals with OCD and those without is the individual's appraisal of the naturally occurring <span class="hlt">intrusive</span> thoughts. This study aimed to test Salkovskis's model by examining the role of cognitive biases (responsibility, thought-action fusion, and thought control) as well as distress in the relationship between <span class="hlt">intrusive</span> thoughts and obsessive-compulsive symptoms in an undergraduate sample of 326 students. An existing measure of <span class="hlt">intrusive</span> thoughts (the Revised Obsessional <span class="hlt">Intrusions</span> Inventory) was modified for this study to include a scale of distress associated with each <span class="hlt">intrusive</span> thought in addition to the current frequency scale. When the Yale-Brown Obsessive-Compulsive Scale was used as the measure of OCD symptoms, a significant interaction effect of frequency and distress of <span class="hlt">intrusive</span> thoughts resulted. Additionally, a significant three-way interaction of Frequency × Distress × Responsibility was found when the Obsessive Compulsive Inventory-Revised was used as the measure of OCD symptoms. These results indicate that the appraisal of <span class="hlt">intrusive</span> thoughts is important in predicting OCD symptoms, thus providing support for Salkovskis's model of OCD.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V23D0668K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V23D0668K"><span>Construction of the Devonian bimodal Gouldsboro pluton via multiple <span class="hlt">intrusion</span>, coastal Maine, USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koteas, C.</p> <p>2006-12-01</p> <p>The Gouldsboro pluton (377 ± 19 ma) (Metzger et al., 1982) of the eastern coastal Maine magmatic province preserves abundant evidence of mechanical interaction between mafic and felsic magmas, as well as the stoping and doming of country rock. Coastal Maine is a unique location where subequal volumes of felsic and mafic material have interacted and are preserved in both plutonic and volcanic complexes. The effects of generation and mobilization of large volumes of magma in the shallow crust are well-preserved. The Gouldsboro pluton provides an excellent perspective from the highest to lowest sections (southwest to northeast) of a hybrid magmatic system. The Gouldsboro magmatic complex is hosted by undated greenstone to the north that is overlain by the 477 ± 18 ma (Metzger, 1977) meta-volcanic/meta-sedimentary Bar Harbor formation. Blocks of both units are discernable as 10 cm to 2 m-diameter blocks within the pluton. The Gouldsboro granite is dominantly a fine to medium grained feldspar- rich leucocratic hornblende granite, although biotite is sometimes present. Miarolitic cavities are common in the highest exposure of the system, especially in the south where the finest grained, most leucocratic granite occurs. Other units include, from lowest to highest in the system, hybrid diorite-gabbro, hybrid granite-granodiorite, granite hosting 30 cm to 3 m-diameter globular basaltic pillows, and a previously unrecognized pyroclastic unit, very similar to the lowermost member of the Cranberry Isle series, a volcanic breccia (Seaman et al., 1999). The pyroclastic unit is intruded by medium grained granite hosting angular fragments of volcanic, mafic plutonic, and country rock. While the contact between gabbro near the base of the pluton and granite in the middle of the pluton is commonly gradational, there are complex <span class="hlt">intrusive</span> breccias in some areas where fine to coarse, angular diorite to gabbro xenoliths are hosted by granodiorite and granite. Enclave-rich <span class="hlt">zones</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1105995','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1105995"><span>Evaluation of Hanford Single-Shell Waste Tanks Suspected of Water <span class="hlt">Intrusion</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Feero, Amie J.; Washenfelder, Dennis J.; Johnson, Jeremy M.</p> <p>2013-11-14</p> <p><span class="hlt">Intrusions</span> evaluations for twelve single-shell tanks were completed in 2013. The evaluations consisted of remote visual inspections, data analysis, and calculations of estimated <span class="hlt">intrusion</span> rates. The observation of an <span class="hlt">intrusion</span> or the preponderance of evidence confirmed that six of the twelve tanks evaluated had <span class="hlt">intrusions</span>. These tanks were tanks 241-A-103, BX-101, BX-103, BX-110, BY-102, and SX-106.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28412538','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28412538"><span>Saharan dust <span class="hlt">intrusions</span> in Spain: Health impacts and associated synoptic conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Díaz, Julio; Linares, Cristina; Carmona, Rocío; Russo, Ana; Ortiz, Cristina; Salvador, Pedro; Trigo, Ricardo Machado</p> <p>2017-07-01</p> <p>A lot of papers have been published about the impact on mortality of Sahara dust <span class="hlt">intrusions</span> in individual cities. However, there is a lack of studies that analyse the impact on a country and scarcer if in addition the analysis takes into account the meteorological conditions that favour these <span class="hlt">intrusions</span>. The main aim is to examine the effect of Saharan dust <span class="hlt">intrusions</span> on daily mortality in different Spanish regions and to characterize the large-scale atmospheric circulation anomalies associated with such dust <span class="hlt">intrusions</span>. For determination of days with Saharan dust <span class="hlt">intrusions</span>, we used information supplied by the Ministry of Agriculture, Food & Environment, it divides Spain into 9 main areas. In each of these regions, a representative province was selected. A time series analysis has been performed to analyse the relationship between daily mortality and PM 10 levels in the period from 01.01.04 to 31.12.09, using Poisson regression and stratifying the analysis by the presence or absence of Saharan dust advections. The proportion of days on which there are Saharan dust <span class="hlt">intrusions</span> rises to 30% of days. The synoptic pattern is characterised by an anticyclonic ridge extending from northern Africa to the Iberian Peninsula. Particulate matter (PM) on days with <span class="hlt">intrusions</span> are associated with daily mortality, something that does not occur on days without <span class="hlt">intrusions</span>, indicating that Saharan dust may be a risk factor for daily mortality. In other cases, what Saharan dust <span class="hlt">intrusions</span> do is to change the PM-related mortality behaviour pattern, going from PM 2.5 . A study such as the one conducted here, in which meteorological analysis of synoptic situations which favour Saharan dust <span class="hlt">intrusions</span>, is combined with the effect on health at a city level, would seem to be crucial when it comes to analysing the differentiated mortality pattern in situations of Saharan dust <span class="hlt">intrusions</span>. Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027179','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027179"><span>Evidence for liquefaction identified in peeled slices of Holocene deposits along the Lower Columbia River, Washington</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Takada, K.; Atwater, B.F.</p> <p>2004-01-01</p> <p>Peels made from 10 geoslices beneath a riverbank at Washington's Hunting Island, 45 km inland from the Pacific coast, aid in identifying sand that liquefied during prehistoric earthquakes of estimated magnitude 8-9 at the Cascadia subduction <span class="hlt">zone</span>. Each slice was obtained by driving sheetpile and a shutter plate to depths of 6-8 m. The resulting sample, as long as 8 m, had a trapezoidal cross section 42-55 cm by 8 cm. The slicing created few artifacts other than bending and smearing at slice edges. Each slice is dominated by well-stratified sand and mud deposited by the tidal Columbia River. Nearly 90% of the sand is distinctly laminated. The sand contains mud beds as thick as 0.5 m and at least 20 m long, and it is capped by a mud bed that contains a buried soil that marks the 1700 Cascadia earthquake of estimated magnitude 9. Every slice intersected sills and <span class="hlt">dikes</span> of fluidized sand, and many slices show folds and faults as well. Sills, which outnumber <span class="hlt">dikes</span>, mostly follow and locally invade the undersides of mud beds. The mud beds probably impeded diffuse upward flow of water expelled from liquefied sand. Trapped beneath mud beds, this water flowed laterally, destroyed bedding by entraining (fluidizing) sand, and locally scoured the overlying mud. Horizontal <span class="hlt">zones</span> of folded sand extend at least 10 or 20 m, and some contain low-angle faults. Many of the folds probably formed while sand was weakened by liquefaction. The low-angle faults may mark the soles of river-bottom slumps or lateral spreads. As many as four great Cascadia earthquakes in the past 2000 yr contributed to the <span class="hlt">intrusions</span>, folds, and faults. This subsurface evidence for fluid escape and deformation casts doubt on maximum accelerations that were previously inferred from local absence of liquefaction features at the ground surface along the Columbia River. The geosliced evidence for liquefaction abounds not only beneath banks riddled with <span class="hlt">dikes</span> but also beneath banks in which <span class="hlt">dikes</span> are absent. Such</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeoOD..56..169F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeoOD..56..169F"><span>Mineral types of hydrothermal alteration <span class="hlt">zones</span> in the Dukat ore field and their relationships to leucogranite and epithermal gold-silver ore, northeastern Russia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Filimonova, L. G.; Trubkin, N. V.; Chugaev, A. V.</p> <p>2014-05-01</p> <p>The paper considers the localization of potassic and propylitic hydrothermal alteration <span class="hlt">zones</span> in the domal volcanic-plutonic structure controlling the position of the Dukat ore field with the eponymous unique epithermal Au-Ag deposit. Comprehensive mineralogical and geochemical data on rocks and minerals in hydrothermal alteration <span class="hlt">zones</span> and associated <span class="hlt">intrusions</span> have shown that quartz-jarosite-sericite, quartz-pyrite-sericite, and quartz-adularia-chlorite alterations were formed with the participation of fluid flows related to a fingerlike projection of a high-K leucogranite porphyry <span class="hlt">intrusion</span> with large phenocrysts. These hydrothermal alterations developed in the rifted graben under conditions of divergent plate boundaries, whereas quartz-clinozoisite-calcite, epidote-chlorite, and garnet-calcite-chlorite alterations were linked to K-Na leucogranite <span class="hlt">intrusive</span> bodies and developed under conditions of convergent plate boundaries reactivated as a result of formation of the marginal Okhotsk-Chukotka volcanic belt. Phase separation and coagulation of specific portions of ascending fluids resulted in the formation and stabilization of small-sized particles of native silver and other ore components, which enabled involvement in flows of secondary geothermal solutions and ore-forming fluids. The Sr, Nd, and Pb isotopic compositions of rocks and minerals from the hydrothermal alteration <span class="hlt">zones</span>, associated <span class="hlt">intrusions</span>, and economic orebodies at the Dukat deposit indicate that their components have been derived from the juvenile continental crust, which was altered in pre-Cretaceous periods of endogenic activity. The components of gangue minerals of potassic and propylitic hydrothertmal alterations and associated <span class="hlt">intrusions</span> have been taken from deep sources differing in 87Sr/86Sr and 143Nd/144Nd at similar U/Pb and Th/Pb ratios. Chalcophile lead in products of hydrothermal activity and melanocratic inclusions in leucogranite has been taken from regions with elevated U/Pb and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11..361C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11..361C"><span>The geographical conditions of intensity of salty waters <span class="hlt">intrusions</span> to coastal lakes on Polish Southern Baltic coast</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cieslinski, R.</p> <p>2009-04-01</p> <p>Lakes situated on the coast of the southern Baltic function in different conditions than those in which typically inland reservoirs occur. They are situated in the contact <span class="hlt">zone</span> of two environments: land and sea. These reservoirs together with their direct catchments form specific hydrographic arrangement, in which the course of physical, chemical and biological processes depends on the fact which of these two environments exerts a stronger influence at a given moment. This is important as the lakes situated in the shore <span class="hlt">zone</span> of the southern Baltic are not exposed to phenomena caused by constant tides, as it is the case in open seas (Ataie-Ashtiani et al., 1999), but only to extreme hydrometeorological conditions, which lead to the formation of the phenomenon of <span class="hlt">intrusions</span> of sea waters and of damming the free outflow of potamic waters (Demirel, 2004; Cieśliński, Drwal, 2005). What should also be remembered are the local hydrographic, hydrological and morphometric conditions. As a result of <span class="hlt">intrusions</span>, in the waters of coastal lakes, apart from inland waters there are also waters of sea origin. The proportions of these genetically distinct waters are variable and differ in individual lakes (Grassi, Netti, 2000; Drwal, Cieśliński, 2007). Despite the difference in the causal factor triggering the phenomenon of salt water <span class="hlt">intrusions</span>, the effect is usually the same as that observed, for instance, in lakes and lagoons of seas with tides (Ishitobi et al., 1999; De Louw, Oude Essink, 2001) and poorly flushed lagoon (Hsing-Juh et al., 2006) or estuaries (Uncles et al., 2002), though the scale of qualitative changes is greater in the case of open seas than in half-closed and closed seas. The status of the research carried out so far enables proposing a hypothesis that chlorides concentrations, as the best indicators for establishing the occurrence of the phenomenon of <span class="hlt">intrusions</span>, depend not only on the meteorological factor but in some of the lakes on various</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/1985/4231/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/1985/4231/report.pdf"><span>Hydrogeologic conditions and saline-water <span class="hlt">intrusion</span>, Cape Coral, Florida, 1978-81</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fitzpatrick, D.J.</p> <p>1986-01-01</p> <p>The upper limestone unit of the intermediate aquifer system, locally called the upper Hawthorn aquifer, is the principal source of freshwater for Cape Coral, Florida. The aquifer has been contaminated with saline water by downward <span class="hlt">intrusion</span> from the surficial aquifer system and by upward <span class="hlt">intrusion</span> from the Floridan aquifer system. Much of the <span class="hlt">intrusion</span> has occurred through open wellbores where steel casings are short or where casings have collapsed because of corrosion. Saline-water contamination of the upper limestone unit due to downward <span class="hlt">intrusion</span> from the surficial aquifer is most severe in the southern and eastern parts of Cape Coral; contamination due to upward <span class="hlt">intrusion</span> has occurred in many areas throughout Cape Coral. <span class="hlt">Intrusion</span> is amplified in areas of heavy water withdrawals and large water-level declines. (USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29908506','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29908506"><span>A framework for performing comparative LCA between repairing flooded houses and construction of <span class="hlt">dikes</span> in non-stationary climate with changing risk of flooding.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hennequin, Thomas; Sørup, Hjalte Jomo Danielsen; Dong, Yan; Arnbjerg-Nielsen, Karsten</p> <p>2018-06-13</p> <p>Sustainable flood management is a basic societal need. In this article, life cycle assessment is used to compare two ways to maintain the state of a coastal urban area in a changing climate with increasing flood risk. On one side, the construction of a <span class="hlt">dike</span>, a hard and proactive scenario, is modelled using a bottom up approach. On the other, the systematic repair of houses flooded by sea surges, a post-disaster measure, is assessed using a Monte Carlo simulation allowing for aleatory uncertainties in predicting future sea level rise and occurrences of extreme events. Two metrics are identified, normalized mean impacts and probability of <span class="hlt">dike</span> being most efficient. The methodology is applied to three case studies in Denmark representing three contrasting areas, Copenhagen, Frederiksværk, and Esbjerg. For all case studies the distribution of the calculated impact of repairing houses is highly right skewed, which in some cases has implications for the comparative LCA. The results show that, in Copenhagen, the scenario of the <span class="hlt">dike</span> is overwhelmingly favorable for the environment, with a 43 times higher impact for repairing houses and only 0% probability of the repairs being favorable. For Frederiksværk and Esbjerg the corresponding numbers are 5 and 0.9 times and 85% and 32%, respectively. Hence constructing a <span class="hlt">dike</span> at this point in time is highly recommended in Copenhagen, preferable in Frederiksværk, and probably not recommendable in Esbjerg. Copyright © 2018 Elsevier B.V. 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