Sample records for active submarine volcanoes

  1. Long-term eruptive activity at a submarine arc volcano.

    PubMed

    Embley, Robert W; Chadwick, William W; Baker, Edward T; Butterfield, David A; Resing, Joseph A; de Ronde, Cornel E J; Tunnicliffe, Verena; Lupton, John E; Juniper, S Kim; Rubin, Kenneth H; Stern, Robert J; Lebon, Geoffrey T; Nakamura, Ko-ichi; Merle, Susan G; Hein, James R; Wiens, Douglas A; Tamura, Yoshihiko

    2006-05-25

    Three-quarters of the Earth's volcanic activity is submarine, located mostly along the mid-ocean ridges, with the remainder along intraoceanic arcs and hotspots at depths varying from greater than 4,000 m to near the sea surface. Most observations and sampling of submarine eruptions have been indirect, made from surface vessels or made after the fact. We describe here direct observations and sampling of an eruption at a submarine arc volcano named NW Rota-1, located 60 km northwest of the island of Rota (Commonwealth of the Northern Mariana Islands). We observed a pulsating plume permeated with droplets of molten sulphur disgorging volcanic ash and lapilli from a 15-m diameter pit in March 2004 and again in October 2005 near the summit of the volcano at a water depth of 555 m (depth in 2004). A turbid layer found on the flanks of the volcano (in 2004) at depths from 700 m to more than 1,400 m was probably formed by mass-wasting events related to the eruption. Long-term eruptive activity has produced an unusual chemical environment and a very unstable benthic habitat exploited by only a few mobile decapod species. Such conditions are perhaps distinctive of active arc and hotspot volcanoes.

  2. Long-term eruptive activity at a submarine arc volcano

    USGS Publications Warehouse

    Embley, R.W.; Chadwick, W.W.; Baker, E.T.; Butterfield, D.A.; Resing, J.A.; de Ronde, Cornel E. J.; Tunnicliffe, V.; Lupton, J.E.; Juniper, S.K.; Rubin, K.H.; Stern, R.J.; Lebon, G.T.; Nakamura, K.-I.; Merle, S.G.; Hein, J.R.; Wiens, D.A.; Tamura, Y.

    2006-01-01

    Three-quarters of the Earth's volcanic activity is submarine, located mostly along the mid-ocean ridges, with the remainder along intraoceanic arcs and hotspots at depths varying from greater than 4,000 m to near the sea surface. Most observations and sampling of submarine eruptions have been indirect, made from surface vessels or made after the fact. We describe here direct observations and sampling of an eruption at a submarine arc volcano named NW Rota-1, located 60 km northwest of the island of Rota (Commonwealth of the Northern Mariana Islands). We observed a pulsating plume permeated with droplets of molten sulphur disgorging volcanic ash and lapilli from a 15-m diameter pit in March 2004 and again in October 2005 near the summit of the volcano at a water depth of 555 m (depth in 2004). A turbid layer found on the flanks of the volcano (in 2004) at depths from 700 m to more than 1,400 m was probably formed by mass-wasting events related to the eruption. Long-term eruptive activity has produced an unusual chemical environment and a very unstable benthic habitat exploited by only a few mobile decapod species. Such conditions are perhaps distinctive of active arc and hotspot volcanoes. ?? 2006 Nature Publishing Group.

  3. The Keelung Submarine volcanoes and gas plumes in the nearshore of northern Taiwan

    NASA Astrophysics Data System (ADS)

    Huang, J. C.; Tsia, C. H.; Hsu, S. K.; Lin, S. S.

    2016-12-01

    Taiwan is located in the collision zone between Philippine Sea Plate and Eurasian Plate. The Philippine Sea Plate subducts northward beneath the Ryukyu arc system while the Eurasian Plate subducts eastward beneath the Luzon arc system. The Taiwan mountain building started at 9 My ago and the most active collision has migrated to middle Taiwan. In consequence, the northern Taiwan has changed its stress pattern from forms a series of thrust faults to normal faults. The stress pattern change has probably induced the post-collisional extension and volcanism in and off northern Taiwan. Under such a tectonic environment, the volcanism and gas plumes are widespread in northern Taiwan and its offshore area. Among the volcanoes of the northern Taiwan volcanic zone, the Tatun Volcano Group is the most obvious one. In this study, we use sub-bottom profiler, EK500 echo sounder, and multibeam echo sounder to study the geophysical structure of a submarine volcano in the nearshore of northern Taiwan. We have analyzed the shallow structures and identified the locations of the gas plumes. The identification of the gas plumes can help us understand the nature of the submarine volcano. Our results show that the gas plumes appear near the Kanchiao Fault and Keelung islet. Some intrusive volcanoes can be observed in the subbottom profiler data. Finally, according to the observations, we found that the Keelung Submarine Volcano is still active. We need the monitor of the active Keelung Submarine Volcano to avoid the volcanic hazard. Additionally, we need to pay attention to the earthquakes related to the Keelung Submarine Volcano.

  4. A Submarine Perspective on Hawaiian Volcanoes

    NASA Astrophysics Data System (ADS)

    Clague, D. A.; Moore, J. G.

    2011-12-01

    Postwar improvements in navigation, sonar-based mapping, and submarine photography enabled the development of bathymetric maps, which revealed submarine morphologic features that could be dredged or explored and sampled with a new generation of manned and unmanned submersibles. The maps revealed debris fields from giant landslides, the great extent of rift zones radiating from volcanic centers, and two previously unknown submarine volcanoes named Mahukona and Loihi, the youngest Hawaiian volcano. About 70 major landslides cover half the flanks of the Hawaiian Ridge out to Midway Island. Some of the landslides attain lengths of 200 km and have volumes exceeding 5,000 km3. More recent higher resolution bathymetry and sidescan data reveal that many submarine eruptions construct circular, flat-topped, monogenetic cones; that large fields of young strongly alkalic lava flows, such as the North Arch and South Arch lava fields, erupt on the seafloor within several hundred km of the islands; and that alkalic lavas erupt during the shield stage on Kilauea and Mauna Loa. The North Arch flow field covers about 24,000 km2, has an estimated volume between about 1000 and 1250 km3, has flows as long as 108 km, and erupted from over 100 vents. The source and melting mechanisms for their production is still debated. The maps also displayed stair-step terraces, mostly constructed of drowned coral reefs, which form during early rapid subsidence of the volcanoes during periods of oscillating sea level. The combination of scuba and underwater photography facilitated the first motion pictures of the mechanism of formation of pillow lava in shallow water offshore Kilauea. The age progression known from the main islands was extended westward along the Hawaiian Ridge past Midway Island, around a bend in the chain and northward along the Emperor Seamounts. Radiometric dating of dredged samples from these submarine volcanoes show that the magma source that built the chain has been active for

  5. Kolumbo submarine volcano (Greece): An active window into the Aegean subduction system.

    PubMed

    Rizzo, Andrea Luca; Caracausi, Antonio; Chavagnac, Valèrie; Nomikou, Paraskevi; Polymenakou, Paraskevi N; Mandalakis, Manolis; Kotoulas, Georgios; Magoulas, Antonios; Castillo, Alain; Lampridou, Danai

    2016-06-17

    Submarine volcanism represents ~80% of the volcanic activity on Earth and is an important source of mantle-derived gases. These gases are of basic importance for the comprehension of mantle characteristics in areas where subaerial volcanism is missing or strongly modified by the presence of crustal/atmospheric components. Though, the study of submarine volcanism remains a challenge due to their hazardousness and sea-depth. Here, we report (3)He/(4)He measurements in CO2-dominated gases discharged at 500 m below sea level from the high-temperature (~220 °C) hydrothermal system of the Kolumbo submarine volcano (Greece), located 7 km northeast off Santorini Island in the central part of the Hellenic Volcanic Arc (HVA). We highlight that the mantle below Kolumbo and Santorini has a (3)He/(4)He signature of at least 7.0 Ra (being Ra the (3)He/(4)He ratio of atmospheric He equal to 1.39×10(-6)), 3 Ra units higher than actually known for gases-rocks from Santorini. This ratio is also the highest measured across the HVA and is indicative of the direct degassing of a Mid-Ocean-Ridge-Basalts (MORB)-like mantle through lithospheric faults. We finally highlight that the degassing of high-temperature fluids with a MORB-like (3)He/(4)He ratio corroborates a vigorous outgassing of mantle-derived volatiles with potential hazard at the Kolumbo submarine volcano.

  6. Kolumbo submarine volcano (Greece): An active window into the Aegean subduction system

    PubMed Central

    Rizzo, Andrea Luca; Caracausi, Antonio; Chavagnac, Valèrie; Nomikou, Paraskevi; Polymenakou, Paraskevi N.; Mandalakis, Manolis; Kotoulas, Georgios; Magoulas, Antonios; Castillo, Alain; Lampridou, Danai

    2016-01-01

    Submarine volcanism represents ~80% of the volcanic activity on Earth and is an important source of mantle-derived gases. These gases are of basic importance for the comprehension of mantle characteristics in areas where subaerial volcanism is missing or strongly modified by the presence of crustal/atmospheric components. Though, the study of submarine volcanism remains a challenge due to their hazardousness and sea-depth. Here, we report 3He/4He measurements in CO2–dominated gases discharged at 500 m below sea level from the high-temperature (~220 °C) hydrothermal system of the Kolumbo submarine volcano (Greece), located 7 km northeast off Santorini Island in the central part of the Hellenic Volcanic Arc (HVA). We highlight that the mantle below Kolumbo and Santorini has a 3He/4He signature of at least 7.0 Ra (being Ra the 3He/4He ratio of atmospheric He equal to 1.39×10−6), 3 Ra units higher than actually known for gases-rocks from Santorini. This ratio is also the highest measured across the HVA and is indicative of the direct degassing of a Mid-Ocean-Ridge-Basalts (MORB)-like mantle through lithospheric faults. We finally highlight that the degassing of high-temperature fluids with a MORB-like 3He/4He ratio corroborates a vigorous outgassing of mantle-derived volatiles with potential hazard at the Kolumbo submarine volcano. PMID:27311383

  7. Numerous Submarine Radial Vents Revealed on Mauna Loa Volcano

    NASA Astrophysics Data System (ADS)

    Wanless, D.; Garcia, M. O.; Rhodes, J. M.; Trusdell, F. A.; Schilling, S.; Weis, D.; Fornari, D.; Vollinger, M.

    2003-12-01

    Among Hawaiian shield volcanoes, Mauna Loa is distinct in having vents outside of its summit and rift zones. These radial vents are located on its northern and western flanks and account for approximately 10% of historic eruptions outside the summit region. Thirty-three subaerial and one submarine vent (active in 1877) were known prior to our work. During a recent Jason2 expedition to the volcano's western flank, nine new submarine radial vents were discovered. Eighty-five samples were collected from these and the 1877 radial vent. Bathymetry and side-scan imagery were acquired using an EM300 multibeam echo sounder. The high resolution data (vertical resolution of approximately 4 m and horizontal resolution of 25 m) allowed us to create the first detailed geologic map of Mauna Loa's western submarine flank. The map was compiled using video and still photography from the Jason2 ROV and geochemical analysis of the samples. The geochemistry includes microprobe glass and XRF whole rock major and trace element data. Eight of the submarine radial vents sampled erupted tholeiitic lavas that are geochemically similar to historical subaerial eruptions on Mauna Loa. However, in contrast to all previously collected Mauna Loa lavas, two of the young vents erupted alkalic basalts. These lavas may have been derived from Mauna Loa, as they have somewhat higher FeO and TiO2 values at a given MgO content than alkalic lavas from neighboring Hualalai volcano, whose vents are located only on rifts 16 km away. Alkalic lavas are indicative of the postshield stage of volcanism and may signal the impending demise of Mauna Loa volcano.

  8. Earthquakes of Loihi submarine volcano and the Hawaiian hot spot.

    USGS Publications Warehouse

    Klein, F.W.

    1982-01-01

    Loihi is an active submarine volcano located 35km S of the island of Hawaii and may eventually grow to be the next and S most island in the Hawaiian chain. The Hawaiian Volcano Observatory recorded two major earthquake swarms located there in 1971-1972 and 1975 which were probably associated with submarine eruptions or intrusions. The swarms were located very close to Loihi's bathymetric summit, except for earthquakes during the second stage of the 1971-1972 swarm, which occurred well onto Loihi's SW flank. The flank earthquakes appear to have been triggered by the preceding activity and possible rifting along Loihi's long axis, similar to the rift-flank relationship at Kilauea volcano. Other changes accompanied the shift in locations from Loihi's summit to its flank, including a shift from burst to continuous seismicity, a rise in maximum magnitude, a change from small earthquake clusters to a larger elongated zone, a drop in b value, and a presumed shift from concentrated volcanic stresses to a more diffuse tectonic stress on Loihi's flank. - Author

  9. The missing link between submarine volcano and promising geothermal potential in Jinshan, Northern Taiwan

    NASA Astrophysics Data System (ADS)

    Wang, S. C.; Hutchings, L.; Chang, C. C.; Lee, C. S.

    2017-12-01

    The Tatun volcanic group (TVG) and the Keelung submarine volcano (KSV) are active volcanoes and surrounding three nuclear plant sites in north Taiwan. The famous Jinshan-Wanli hot springs locates between TVG and KSV, moreover, the geochemical anomalies of acidic boiling springs on the seacoast infer that the origin is from magmatic fluids, sea water and meteoric water mixture, strongly implying that mantle fluids ascends into the shallow crust. The evidence for a magma chamber, submarine volcano, and boiling springs have a close spatial relationship. Based on UNECE specifications to Geothermal Energy Resources (2016), the Jinshan-Wanli geothermal area could be classified as Known Geothermal Energy Source for geothermal direct use and Potential Geothermal Energy Source for conventional geothermal system. High resolution reservoir exploration and modeling in Jinshan-Wanli geothermal area is developing for drilling risk mitigation. The geothermal team of National Taiwan Ocean University and local experts are cooperating for further exploration drilling and geothermal source evaluation. Keywords: geothermal resource evaluation, Jinshan-Wanli geothermal area, submarine volcano

  10. Submarine geology and geomorphology of active Sub-Antarctic volcanoes: Heard and McDonald Islands

    NASA Astrophysics Data System (ADS)

    Watson, S. J.; Coffin, M. F.; Whittaker, J. M.; Lucieer, V.; Fox, J. M.; Carey, R.; Arculus, R. J.; Bowie, A. R.; Chase, Z.; Robertson, R.; Martin, T.; Cooke, F.

    2016-12-01

    Heard and McDonald Islands (HIMI) are World Heritage listed sub-Antarctic active volcanic islands in the Southern Indian Ocean. Built atop the Kerguelen Plateau by Neogene-Quaternary volcanism, HIMI represent subaerial exposures of the second largest submarine Large Igneous Province globally. Onshore, processes influencing island evolution include glaciers, weathering, volcanism, vertical tectonics and mass-wasting (Duncan et al. 2016). Waters surrounding HIMI are largely uncharted, due to their remote location. Hence, the extent to which these same processes shape the submarine environment around HIMI has not been investigated. In early 2016, we conducted marine geophysical and geologic surveys around HIMI aboard RV Investigator (IN2016_V01). Results show that volcanic and sedimentary features prominently trend east-west, likely a result of erosion by the eastward flowing Antarctic Circumpolar Current and tidal currents. However, spatial patterns of submarine volcanism and sediment distribution differ substantially between the islands. >70 sea knolls surround McDonald Island suggesting substantial submarine volcanism. Geophysical data reveals hard volcanic seafloor around McDonald Island, whereas Heard Island is characterised by sedimentary sequences tens of meters or more thick and iceberg scours - indicative of glacial processes. Differences in submarine geomorphology are likely due to the active glaciation of Heard Island and differing rock types (Heard: alkali basalt, McDonald: phonolite), and dominant products (clastics vs. lava). Variations may also reflect different magmatic plumbing systems beneath the two active volcanoes (Heard produces larger volumes of more focused lava, whilst McDonald extrudes smaller volumes of more evolved lavas from multiple vents across the edifice). Using geophysical data, corroborated with new and existing geologic data, we present the first geomorphic map revealing the processes that shape the submarine environment around HIMI.

  11. Structural evolution of deep-water submarine intraplate volcanoes / Azores

    NASA Astrophysics Data System (ADS)

    Stakemann, Josefine; Huebscher, Christian; Beier, Christoph; Hildenbrand, Anthony; Nomikou, Paraskevi; Terrinha, Pedro; Weiß, Benedikt

    2017-04-01

    We present multibeam and high-resolution reflection seismic data which elucidate the architecture of three submarine intraplate volcanoes located in the southern Azores Archipelago. Data have been collected during RV Meteor cruise M113 in 2015. Four GI-Guns served as the seismic source. The digital streamer comprised 144 channels distributed over a length of 600 m. The three cones are situated in a depth down to 2300 m with heights varying between 200 m and 243 m, an average diameter of 1360 m and an average slope angle of ca. 22°. All three circular cones are surrounded by a circular channel. These features, previously named "fried eggs" were previously interpreted as impact crater (Dias et al., 2009). A comparison with nearby submarine volcanoes close to São Miguel island (Weiß et al., 2015), however, strongly suggests a volcanic origin. The seismic data indicate that the volcanic cones formed on top of a ca. 100 m thick pelagic succession covering the igneous basement. Magma ascent deformed the volcanic basement, displaced the pelagic sediments and a first eruption phase formed a small, seismically transparent volcanic cone. Further eruptions created a volcanic cone with rather transparent reflections within the inferior region changing to strong reflection amplitudes with a chaotic pattern in the superior area. Compared to the igneous basement internal reflection amplitudes are mainly weak. The seismic transparency and slope angle exclude the presence of effusive rocks, since lavas usually create strong impedance contrasts. A comparison of the seismic characteristics with those from submarine Kolumbo volcano (Hübscher et al., 2015) suggests volcaniclastic lithologies from explosive eruptions. The circular channel around the volcanic cone shows the characteristics of a moat channel created by bottom currents. References: Dias, F.C., Lourenco, N., Lobo, A., Santos de Campos, A., Pinto de Abreu, M., 2009. "Fried Egg": An Oceanic Impact Crater in the Mid

  12. Submarine radial vents on Mauna Loa Volcano, Hawai'i

    USGS Publications Warehouse

    Wanless, V. Dorsey; Garcia, M.O.; Trusdell, F.A.; Rhodes, J.M.; Norman, M.D.; Weis, Dominique; Fornari, D.J.; Kurz, M.D.; Guillou, Herve

    2006-01-01

    A 2002 multibeam sonar survey of Mauna Loa's western flank revealed ten submarine radial vents and three submarine lava flows. Only one submarine radial vent was known previously. The ages of these vents are constrained by eyewitness accounts, geologic relationships, Mn-Fe coatings, and geochemical stratigraphy; they range from 128 years B.P. to possibly 47 ka. Eight of the radial vents produced degassed lavas despite eruption in water depths sufficient to inhibit sulfur degassing. These vents formed truncated cones and short lava flows. Two vents produced undegassed lavas that created “irregular” cones and longer lava flows. Compositionally and isotopically, the submarine radial vent lavas are typical of Mauna Loa lavas, except two cones that erupted alkalic lavas. He-Sr isotopes for the radial vent lavas follow Mauna Loa's evolutionary trend. The compositional and isotopic heterogeneity of these lavas indicates most had distinct parental magmas. Bathymetry and acoustic backscatter results, along with photography and sampling during four JASON2 dives, are used to produce a detailed geologic map to evaluate Mauna Loa's submarine geologic history. The new map shows that the 1877 submarine eruption was much larger than previously thought, resulting in a 10% increase for recent volcanism. Furthermore, although alkalic lavas were found at two radial vents, there is no systematic increase in alkalinity among these or other Mauna Loa lavas as expected for a dying volcano. These results refute an interpretation that Mauna Loa's volcanism is waning. The submarine radial vents and flows cover 29 km2 of seafloor and comprise a total volume of ∼2×109 m3 of lava, reinforcing the idea that submarine lava eruptions are important in the growth of oceanic island volcanoes even after they emerged above sea level.

  13. Near-specular acoustic scattering from a buried submarine mud volcano.

    PubMed

    Gerig, Anthony L; Holland, Charles W

    2007-12-01

    Submarine mud volcanoes are objects that form on the seafloor due to the emission of gas and fluidized sediment from the Earth's interior. They vary widely in size, can be exposed or buried, and are of interest to the underwater acoustics community as potential sources of active sonar clutter. Coincident seismic reflection data and low frequency bistatic scattering data were gathered from one such buried mud volcano located in the Straits of Sicily. The bistatic data were generated using a pulsed piston source and a 64-element horizontal array, both towed over the top of the volcano. The purpose of this work was to appropriately model low frequency scattering from the volcano using the bistatic returns, seismic bathymetry, and knowledge of the general geoacoustic properties of the area's seabed to guide understanding and model development. Ray theory, with some approximations, was used to model acoustic propagation through overlying layers. Due to the volcano's size, scattering was modeled using geometric acoustics and a simple representation of volcano shape. Modeled bistatic data compared relatively well with experimental data, although some features remain unexplained. Results of an inversion for the volcano's reflection coefficient indicate that it may be acoustically softer than expected.

  14. H2O Contents of Submarine and Subaerial Silicic Pyroclasts from Oomurodashi Volcano, Northern Izu-Bonin Arc

    NASA Astrophysics Data System (ADS)

    McIntosh, I. M.; Tani, K.; Nichols, A. R.

    2014-12-01

    Oomurodashi volcano is an active shallow submarine silicic volcano in the northern Izu-Bonin Arc, located ~20 km south of the inhabited active volcanic island of Izu-Oshima. Oomurodashi has a large (~20km diameter) flat-topped summit located at 100 - 150 metres below sea level (mbsl), with a small central crater, Oomuro Hole, located at ~200 mbsl. Surveys conducted during cruise NT12-19 of R/V Natsushima in 2012 using the remotely-operated vehicle (ROV) Hyper-Dolphin revealed that Oomuro Hole contains numerous active hydrothermal vents and that the summit of Oomurodashi is covered by extensive fresh rhyolitic lava and pumice clasts with little biogenetic or manganese cover, suggesting recent eruption(s) from Oomuro Hole. Given the shallow depth of the volcano summit, such eruptions are likely to have generated subaerial eruption columns. A ~10ka pumiceous subaerial tephra layer on the neighbouring island of Izu-Oshima has a similar chemical composition to the submarine Oomurodashi rocks collected during the NT12-19 cruise and is thought to have originated from Oomurodashi. Here we present FTIR measurements of the H2O contents of rhyolitic pumice from both the submarine deposits sampled during ROV dives and the subaerial tephra deposit on Izu-Oshima, in order to assess magma degassing and eruption processes occurring during shallow submarine eruptions.

  15. Submarine radial vents on Mauna Loa Volcano, Hawaìi

    NASA Astrophysics Data System (ADS)

    Wanless, V. Dorsey; Garcia, M. O.; Trusdell, F. A.; Rhodes, J. M.; Norman, M. D.; Weis, Dominique; Fornari, D. J.; Kurz, M. D.; Guillou, Hervé

    2006-05-01

    A 2002 multibeam sonar survey of Mauna Loa's western flank revealed ten submarine radial vents and three submarine lava flows. Only one submarine radial vent was known previously. The ages of these vents are constrained by eyewitness accounts, geologic relationships, Mn-Fe coatings, and geochemical stratigraphy; they range from 128 years B.P. to possibly 47 ka. Eight of the radial vents produced degassed lavas despite eruption in water depths sufficient to inhibit sulfur degassing. These vents formed truncated cones and short lava flows. Two vents produced undegassed lavas that created "irregular" cones and longer lava flows. Compositionally and isotopically, the submarine radial vent lavas are typical of Mauna Loa lavas, except two cones that erupted alkalic lavas. He-Sr isotopes for the radial vent lavas follow Mauna Loa's evolutionary trend. The compositional and isotopic heterogeneity of these lavas indicates most had distinct parental magmas. Bathymetry and acoustic backscatter results, along with photography and sampling during four JASON2 dives, are used to produce a detailed geologic map to evaluate Mauna Loa's submarine geologic history. The new map shows that the 1877 submarine eruption was much larger than previously thought, resulting in a 10% increase for recent volcanism. Furthermore, although alkalic lavas were found at two radial vents, there is no systematic increase in alkalinity among these or other Mauna Loa lavas as expected for a dying volcano. These results refute an interpretation that Mauna Loa's volcanism is waning. The submarine radial vents and flows cover 29 km2 of seafloor and comprise a total volume of ˜2 × 109 m3 of lava, reinforcing the idea that submarine lava eruptions are important in the growth of oceanic island volcanoes even after they emerged above sea level.

  16. Chemical Fluxes from a Recently Erupted Submarine Volcano on the Mariana Arc

    NASA Astrophysics Data System (ADS)

    Buck, N. J.; Resing, J. A.; Lupton, J. E.; Larson, B. I.; Walker, S. L.; Baker, E. T.

    2016-12-01

    While hydrothermal circulation is paramount to the geochemical budget for a wide array of elements, relatively few flux estimates exist in the literature. To date most studies have concentrated on constraining global and vent-field scale inputs originating from ocean spreading ridges. The goal of this study is to directly measure the chemical flux from an active submarine volcano injecting hydrothermal fluids into the surface ocean. Ahyi Seamount, a submarine intraoceanic arc volcano located in the Northern Mariana Islands, has a summit depth <100 m and erupted in May 2014. In November 2014 a hydrothermal plume originating from Ahyi was sampled aboard the R/V Roger Revelle during the Submarine Ring of Fire 2014 Ironman Expedition. Shipboard hull mounted Acoustic Doppler Current Profile data was collected to provide current vector measurements to be used in combination with continuous and discrete CTD data. Towed CTD sections were conducted perpendicular to the current direction - a sampling strategy that optimizes chemical flux estimate calculations by reducing complexities introduced by temporal variability in the speed and direction of plume dispersion. The Ahyi plume had a significant optical backscatter signal accompanied by evidence of reduced chemical species and a lowered pH. It was sampled for He isotopes, CH4, H2, H2S, total CO2, nutrients, TSM and total and dissolved Fe and Mn. Laboratory analyses found enriched concentrations of H2, 3He, CO2 and Fe, consistent with a recent eruption. Preliminary flux calculations estimate a Fe input of 16 mmol s-1. This indicates shallow submarine arc volcanoes are capable of supplying appreciable quantities of Fe into the surface ocean. Further laboratory analyses and calculations to characterize and constrain the fluxes of other chemical constituents are underway.

  17. A large submarine sand-rubble flow on kilauea volcano, hawaii

    USGS Publications Warehouse

    Fornari, D.J.; Moore, J.G.; Calk, L.

    1979-01-01

    Papa'u seamount on the south submarine slope of Kilauea volcano is a large landslide about 19 km long, 6 km wide, and up to 1 km thick with a volume of about 39 km3. Dredge hauls, remote camera photographs, and submersible observations indicate that it is composed primarily of unconsolidated angular glassy basalt sand with scattered basalt blocks up to 1 m in size; no lava flows were seen. Sulfur contents of basalt glass from several places on the sand-rubble flow and nearby areas are low (< 240 ppm), indicating that the clastic basaltic material was all erupted on land. The Papa'u sandrubble flow was emplaced during a single flow event fed from a large near-shore bank of clastic basaltic material which in turn was formed as lava flows from the summit area of Kilauea volcano disintegrated when they entered the sea. The current eruptive output of the volcano suggests that the material in the submarine sand-rubble flow represents about 6000 years of accumulation, and that the flow event occurred several thousand years ago. ?? 1979.

  18. Mapping the sound field of an erupting submarine volcano using an acoustic glider.

    PubMed

    Matsumoto, Haru; Haxel, Joseph H; Dziak, Robert P; Bohnenstiehl, Delwayne R; Embley, Robert W

    2011-03-01

    An underwater glider with an acoustic data logger flew toward a recently discovered erupting submarine volcano in the northern Lau basin. With the volcano providing a wide-band sound source, recordings from the two-day survey produced a two-dimensional sound level map spanning 1 km (depth) × 40 km(distance). The observed sound field shows depth- and range-dependence, with the first-order spatial pattern being consistent with the predictions of a range-dependent propagation model. The results allow constraining the acoustic source level of the volcanic activity and suggest that the glider provides an effective platform for monitoring natural and anthropogenic ocean sounds. © 2011 Acoustical Society of America

  19. Argon-40: Excess in submarine pillow basalts from Kilauea Volcano, Hawaii

    USGS Publications Warehouse

    Brent, Dalrymple G.; Moore, J.G.

    1968-01-01

    Submarine pillow basalts from Kilauea Volcano contain excess radiogenic argon-40 and give anomalously high potassium-argon ages. Glassy rims of pillows show a systematic increase in radiogenic argon-40 with depth, and a pillow from a depth of 2590 meters shows a decrease in radiogenic argon-40 inward from the pillow rim. The data indicate that the amount of excess radiogenic argon-40 is a direct function of both hydrostatic pressure and rate of cooling, and that many submarine basalts are not suitable for potassium-argon dating.

  20. Argon-40: excess in submarine pillow basalts from kilauea volcano, hawaii.

    PubMed

    Dalrymple, G B; Moore, J G

    1968-09-13

    Submarine pillow basalts from Kilauea Volcano contain excess radiogenic argon-40 and give anomalously high potassium-argon ages. Glassy rims of pillows show a systematic increase in radiogenic argon-40 with depth, and a pillow from a depth of 2590 meters shows a decrease in radiogenic argon40 inward from the pillow rim. The data indicate that the amount of excess radiogenic argon-40 is a direct function of both hydrostatic pressure and rate of cooling, and that many submarine basalts are not suitable for potassium-argon dating.

  1. Submarine geology of the Hilina slump and morpho-structural evolution of Kilauea volcano, Hawaii

    NASA Astrophysics Data System (ADS)

    Smith, John R.; Malahoff, Alexander; Shor, Alexander N.

    1999-12-01

    Marine geophysical data, including SEA BEAM bathymetry, HAWAII MR1 sidescan, and seismic reflection profiles, along with recent robot submersible observations and samples, were acquired over the offshore continuation of the mobile Kilauea volcano south flank. This slope comprises the three active hot spot volcanoes Mauna Loa, Kilauea, and Loihi seamount and is the locus of the Hawaiian hot spot. The south flank is the site of frequent low-intensity seismicity as well as episodic large-magnitude earthquakes. Its sub-aerial portion creeps seaward at a rate of approximately 10 cm/year. The Hilina slump is the only large submarine landslide in the Hawaiian Archipelago thought to be active, and this study is one of the first to more highly resolve submarine slide features there. The slump is classified into four distinct zones from nearshore to the island's base. Estimates of size based on these data indicate a slumped area of 2100 km 2 and a volume of 10,000-12,000 km 3, equivalent to about 10% of the entire island edifice. The overall picture gained from these data sets is one of mass wasting of the neovolcanic terrain as it builds upward and seaward, though reinforcement by young and pre-Hawaii seamounts adjacent to the pedestal is apparent. Extensive lava delta deposits are formed by hyaloclastites and detritus from recent lava flows into the sea. These deposits dominate the upper submarine slope offshore of Kilauea, with pillow breccia revealed at mid-depths. Along the lower flanks, massive outcrops of volcanically derived sedimentary rocks were found underlying Kilauea, thus necessitating a rethinking of previous models of volcanic island development. The morphologic and structural evolutionary model for Kilauea volcano and the Hilina slump proposed here attempts to incorporate this revelation. A hazard assessment for the Hilina slump is presented where it is suggested that displacement of the south flank to date has been restrained by a still developing northeast

  2. Environmental monitoring of El Hierro Island submarine volcano, by combining low and high resolution satellite imagery

    NASA Astrophysics Data System (ADS)

    Eugenio, F.; Martin, J.; Marcello, J.; Fraile-Nuez, E.

    2014-06-01

    El Hierro Island, located at the Canary Islands Archipelago in the Atlantic coast of North Africa, has been rocked by thousands of tremors and earthquakes since July 2011. Finally, an underwater volcanic eruption started 300 m below sea level on October 10, 2011. Since then, regular multidisciplinary monitoring has been carried out in order to quantify the environmental impacts caused by the submarine eruption. Thanks to this natural tracer release, multisensorial satellite imagery obtained from MODIS and MERIS sensors have been processed to monitor the volcano activity and to provide information on the concentration of biological, chemical and physical marine parameters. Specifically, low resolution satellite estimations of optimal diffuse attenuation coefficient (Kd) and chlorophyll-a (Chl-a) concentration under these abnormal conditions have been assessed. These remote sensing data have played a fundamental role during field campaigns guiding the oceanographic vessel to the appropriate sampling areas. In addition, to analyze El Hierro submarine volcano area, WorldView-2 high resolution satellite spectral bands were atmospherically and deglinted processed prior to obtain a high-resolution optimal diffuse attenuation coefficient model. This novel algorithm was developed using a matchup data set with MERIS and MODIS data, in situ transmittances measurements and a seawater radiative transfer model. Multisensor and multitemporal imagery processed from satellite remote sensing sensors have demonstrated to be a powerful tool for monitoring the submarine volcanic activities, such as discolored seawater, floating material and volcanic plume, having shown the capabilities to improve the understanding of submarine volcanic processes.

  3. Cyclic thermal behavior associated to the degassing process at El Hierro submarine volcano, Canary Islands.

    NASA Astrophysics Data System (ADS)

    Fraile-Nuez, E.; Santana-Casiano, J. M.; González-Dávila, M.

    2016-12-01

    One year after the ceasing of magmatic activity in the shallow submarine volcano of the island of El Hierro, significant physical-chemical anomalies produced by the degassing process as: (i) thermal anomalies increase of +0.44 °C, (ii) pH decrease of -0.034 units, (iii) total dissolved inorganic carbon, CT increase by +43.5 µmol kg-1 and (iv) total alkalinity, AT by +12.81 µmol kg-1 were still present in the area. These evidences highlight the potential role of the shallow degassing processes as a natural ecosystem-scale experiments for the study of significant effects of global change stressors on marine environments. Additionally, thermal time series obtained from a temporal yo-yo CTD study, in isopycnal components, over one of the most active points of the submarine volcano have been analyzed in order to investigate the behavior of the system. Signal processing of the thermal time series highlights a strong cyclic temperature period of 125-150 min at 99.9% confidence, due to characteristic time-scales revealed in the periodogram. These long cycles might reflect dynamics occurring within the shallow magma supply system below the island of El Hierro.

  4. Submarine geology of Hana Ridge and Haleakala Volcano's northeast flank, Maui

    USGS Publications Warehouse

    Eakins, Barry W.; Robinson, Joel E.

    2006-01-01

    We present a morphostructural analysis of the submarine portions of Haleakala Volcano and environs, based upon a 4-year program of geophysical surveys and submersible explorations of the underwater flanks of Hawaiian volcanoes that was conducted by numerous academic and governmental research organizations in Japan and the U.S. and funded primarily by the Japan Agency for Marine–Earth Science and Technology. A resulting reconnaissance geologic map features the 135-km-long Hana Ridge, the 3000 km2 Hana slump on the volcano's northeast flank, and island-surrounding terraces that are the submerged parts of volcanic shields. Hana Ridge below 2000 m water depth exhibits the lobate morphology typical of the subaqueously erupted parts of Hawaiian rift zones, with some important distinctions: namely, subparallel crestlines, which we propose result from the down-rift migration of offsets in the dike intrusion zone, and an amphitheater at its distal toe, where a submarine landslide has embayed the ridge tip. Deformation of Haleakala's northeast flank is limited to that part identified as the Hana slump, which lies downslope from the volcano's submerged shield, indicating that flank mobility is also limited in plan, inconsistent with hypothesized volcanic spreading driven by rift-zone dilation. The leading edge of the slump has transverse basins and ridges that resemble the thrust ramps of accretionary prisms, and we present a model to describe the slump's development that emphasizes the role of coastally generated fragmental basalt on gravitational instability of Haleakala's northeast flank and that may be broadly applicable to other ocean-island slumps.

  5. Looking for Larvae Above an Erupting Submarine Volcano, NW Rota-1, Mariana Arc

    NASA Astrophysics Data System (ADS)

    Beaulieu, S.; Hanson, M.; Tunnicliffe, V.; Chadwick, W. W., Jr.; Breuer, E. R.

    2016-02-01

    In 2009 the first marine protected areas for deep-sea hydrothermal vents in U.S. waters were established as part of the Volcanic Unit of the Marianas Trench Marine National Monument. In this region, hydrothermal vents are located along the Mariana Arc and back-arc spreading center. In particular hydrothermal vents are located near the summit of NW Rota-1, an active submarine volcano on the Mariana Arc which was erupting between 2003 and 2010 and ceased as of 2014. NW Rota-1 experienced a massive landslide in late 2009, decimating the habitat on the southern side of the volcano. This project looked at zooplankton tow samples taken from the water column above NW Rota-1 in 2010, searching for larvae which have the potential to recolonize the sea floor after such a major disturbance. Samples were sorted in entirety into coarse taxa, and then larvae were removed for DNA barcoding. Overall zooplankton composition was dominated by copepods, ostracods, and chaetognaths, the majority of which are pelagic organisms. Comparatively few larvae of benthic invertebrates were found, but shrimp, gastropod, barnacle, and polychaete larvae did appear in low numbers in the samples. Species-level identification obtained via genetic barcoding will allow for these larvae to be matched to species known to inhabit the benthic communities at NW Rota-1. Identified larvae will give insight into the organisms which can re-colonize the seafloor vent communities after a disturbance such as the 2009 landslide. Communities at hydrothermal vents at other submarine volcanoes in the Monument may act as sources for these larvae, but connectivity in this region of complex topography is unknown. As the microinvertebrate biodiversity in the Monument has yet to be fully characterized, our project also provides an opportunity to better describe both the zooplankton and benthic community composition in this area of the Monument.

  6. The active submarine NW termination of the South Aegean Active Volcanic Arc: The Submarine Pausanias Volcanic Field

    NASA Astrophysics Data System (ADS)

    Foutrakis, Panagiotis M.; Anastasakis, George

    2018-05-01

    Methana peninsula shows the longest recorded volcanic history at the western end of the South Aegean Active Volcanic Arc, including volcanic products from the Upper Pliocene to recent times. The volcanic rocks comprise widespread dacite domes and andesite lava flows from several small volcanic centers and are only imprecisely dated. In this paper, the integrated analysis of swath bathymetry, side scan sonar data, and high resolution seismic reflection profiles correlated with core samples, has allowed detailed mapping, characterization and precise chronological identification of the Pausanias submarine volcanic field activity offshore northern Methana. Six volcanic cones or domes are recognized, typically 1-3 km in diameter, some elongated NE-SW and some with a small central crater. On their flanks, the acoustically reflective volcanic rocks pass laterally into incoherent transparent seismic facies interpreted as volcaniclastic deposits, possibly including hyaloclastites, that interfinger with the regional basin sediments. A sea-bottom hummocky field, is interpreted as volcanic avalanche and appears to be the submarine continuation of the volcaniclastic apron of northern Methana peninsula. A robust chronostratigraphic framework has been established, based on the recognition of shoreline progradational units and their connection with Quaternary eustatic sea level cycles. Relative dating of the different phases of submarine volcanic activity during the Upper Quaternary has been achieved by correlating the imaged volcaniclastic flows, interlayered within the chronostratigraphically dated sediments. Dating by stratigraphic position, relative to 2D imaged eustatic sea level clinoform wedges appears to be more precise than radiometric methods on land. Three main submarine Volcanic Events (VE) are recognized: VE3 at 450 ka, a less precisely dated interval at 200-130 ka (VE2), and VE1 at 14 ka. Based on chronostratigraphic constraints, subsidence rates of 0.16 (±0.008) m

  7. Degassing history of water, sulfur, and carbon in submarine lavas from Kilauea Volcano, Hawaii

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

    Dixon, J.E.; Stolper, E.M.; Clague, D.A.

    1991-05-01

    Major, minor, and dissolved volatile element concentrations were measured in tholeiitic glasses from the submarine portion (Puna Ridge) of the east rift zone of Kilauea Volcano, Hawaii. Dissolved H{sub 2}O and S concentrations display a wide range relative to nonvolatile incompatible elements at all depths. This range cannot be readily explained by fractional crystallization, degassing of H{sub 2}O and S during eruption on the seafloor, or source region heterogeneities. Dissolved CO{sub 2} concentrations, in contrast, show a positive correlation with eruption depth and typically agree within error with the solubility at that depth. The authors propose that most magmas alongmore » the Puna Ridge result from (1) mixing of a relatively volatile-rich, undegassed component with magmas that experienced low pressure (perhaps subaerial) degassing during which substantial H{sub 2}O, S, and CO{sub 2} were lost, followed by (2) fractional crystallization of olivine, clinopyroxene, and plagioclase from this mixture to generate a residual liquid; and (3) further degassing, principally of CO{sub 2} for samples erupted deeper than 1,000 m, during eruption on the seafloor. They predict that average Kilauean primary magmas with 16% MgO contain {approximately}0.47 wt % H{sub 2}0, {approximately}900 ppm S, and have {delta}D values of {approximately}{minus}30 to {minus}40%. The model predicts that submarine lavas from wholly submarine volcanoes (i.e., Loihi), for which there is no opportunity to generate the degassed end member by low pressure degassing, will be enriched in volatiles relative to those from volcanoes whose summits have breached the sea surface (i.e., Kilauea and Mauna Loa).« less

  8. Exploring the "Sharkcano": Biogeochemical observations of the Kavachi submarine volcano (Solomon Islands) using simple, cost-effective methods.

    NASA Astrophysics Data System (ADS)

    Phillips, B. T.; Albert, S.; Carey, S.; DeCiccio, A.; Dunbabin, M.; Flinders, A. F.; Grinham, A. R.; Henning, B.; Howell, C.; Kelley, K. A.; Scott, J. J.

    2015-12-01

    Kavachi is a highly active undersea volcano located in the Western Province of the Solomon Islands, known for its frequent phreatomagmatic eruptions and ephemeral island-forming activity. The remote location of Kavachi and its explosive behavior has restricted scientific exploration of the volcano, limiting observations to surface imagery and peripheral water-column data. An expedition to Kavachi in January 2015 was timed with a rare lull in volcanic activity, allowing for observation of the inside of Kavachi's caldera and its flanks. Here we present medium-resolution bathymetry of the main peak paired with benthic imagery, petrologic analysis of samples from the caldera rim, measurements of gas flux over the main peak, and hydrothermal plume structure data. A second peak was discovered to the Southwest of the main cone and displayed evidence of diffuse-flow venting. Populations of gelatinous animals, small fish, and sharks were observed inside the active crater, raising new questions about the ecology of active submarine volcanoes. Most equipment used in this study was lightweight, relatively low-cost, and deployed using small boats; these methods may offer developing nations an economic means to explore deep-sea environments within their own territorial waters.

  9. Numerical tsunami hazard assessment of the submarine volcano Kick 'em Jenny in high resolution are

    NASA Astrophysics Data System (ADS)

    Dondin, Frédéric; Dorville, Jean-Francois Marc; Robertson, Richard E. A.

    2016-04-01

    Landslide-generated tsunami are infrequent phenomena that can be potentially highly hazardous for population located in the near-field domain of the source. The Lesser Antilles volcanic arc is a curved 800 km chain of volcanic islands. At least 53 flank collapse episodes have been recognized along the arc. Several of these collapses have been associated with underwater voluminous deposits (volume > 1 km3). Due to their momentum these events were likely capable of generating regional tsunami. However no clear field evidence of tsunami associated with these voluminous events have been reported but the occurrence of such an episode nowadays would certainly have catastrophic consequences. Kick 'em Jenny (KeJ) is the only active submarine volcano of the Lesser Antilles Arc (LAA), with a current edifice volume estimated to 1.5 km3. It is the southernmost edifice of the LAA with recognized associated volcanic landslide deposits. The volcano appears to have undergone three episodes of flank failure. Numerical simulations of one of these episodes associated with a collapse volume of ca. 4.4 km3 and considering a single pulse collapse revealed that this episode would have produced a regional tsunami with amplitude of 30 m. In the present study we applied a detailed hazard assessment on KeJ submarine volcano (KeJ) form its collapse to its waves impact on high resolution coastal area of selected island of the LAA in order to highlight needs to improve alert system and risk mitigation. We present the assessment process of tsunami hazard related to shoreline surface elevation (i.e. run-up) and flood dynamic (i.e. duration, height, speed...) at the coast of LAA island in the case of a potential flank collapse scenario at KeJ. After quantification of potential initial volumes of collapse material using relative slope instability analysis (RSIA, VolcanoFit 2.0 & SSAP 4.5) based on seven geomechanical models, the tsunami source have been simulate by St-Venant equations-based code

  10. Looking for Larvae Above an Erupting Submarine Volcano, NW Rota-1, Mariana Arc

    NASA Astrophysics Data System (ADS)

    Hanson, M.; Beaulieu, S.; Tunnicliffe, V.; Chadwick, W.; Breuer, E. R.

    2015-12-01

    In 2009 the first marine protected areas for deep-sea hydrothermal vents in U.S. waters were established as part of the Volcanic Unit of the Marianas Trench Marine National Monument. In this region, hydrothermal vents are located along the Mariana Arc and back-arc spreading center. In particular hydrothermal vents are located near the summit of NW Rota-1, an active submarine volcano on the Mariana Arc which was erupting between 2003 through 2010 and ceased as of 2014. In late 2009, NW Rota-1 experienced a massive landslide decimating the habitat on the southern side of the volcano. This presented an enormous natural disturbance to the community. This project looked at zooplankton tow samples taken from the water column above NW Rota-1 in 2010, searching specifically for larvae which have the potential to recolonize the sea floor after such a major disturbance. We focused on samples for which profiles with a MAPR sensor indicated hydrothermal plumes in the water column. Samples were sorted in entirety into coarse taxa, and then larvae were removed for DNA barcoding. Overall zooplankton composition was dominated by copepods, ostracods, and chaetognaths, the majority of which are pelagic organisms. Comparatively few larvae of benthic invertebrates were found, but shrimp, gastropod, barnacle, and polychaete larvae did appear in low numbers in the samples. Species-level identification obtained via genetic barcoding will allow for these larvae to be matched to species known to inhabit the benthic communities at NW Rota-1. Identified larvae will give insight into the organisms which can re-colonize the seafloor vent communities after a disturbance such as the 2009 landslide. Communities at hydrothermal vents at other submarine volcanoes in the Monument also can act as sources for these planktonic, recolonizing larvae. As the microinvertebrate biodiversity in the Monument has yet to be fully characterized, our project also provides an opportunity to better describe both

  11. The Kolumbo submarine volcano of Santorini island is a large pool of bacterial strains with antimicrobial activity.

    PubMed

    Bourbouli, Maria; Katsifas, Efstathios A; Papathanassiou, Evangelos; Karagouni, Amalia D

    2015-05-01

    Microbes in hydrothermal vents with their unique secondary metabolism may represent an untapped potential source of new natural products. In this study, samples were collected from the hydrothermal field of Kolumbo submarine volcano in the Aegean Sea, in order to isolate bacteria with antimicrobial activity. Eight hundred and thirty-two aerobic heterotrophic bacteria were isolated and then differentiated through BOX-PCR analysis at the strain level into 230 genomic fingerprints, which were screened against 13 different type strains (pathogenic and nonpathogenic) of Gram-positive, Gram-negative bacteria and fungi. Forty-two out of 176 bioactive-producing genotypes (76 %) exhibited antimicrobial activity against at least four different type strains and were selected for 16S rDNA sequencing and screening for nonribosomal peptide (NRPS) and polyketide (PKS) synthases genes. The isolates were assigned to genus Bacillus and Proteobacteria, and 20 strains harbored either NRPS, PKS type I or both genes. This is the first report on the diversity of culturable mesophilic bacteria associated with antimicrobial activity from Kolumbo area; the extremely high proportion of antimicrobial-producing strains suggested that this unique environment may represent a potential reservoir of novel bioactive compounds.

  12. Significant discharge of CO2 from hydrothermalism associated with the submarine volcano of El Hierro Island

    NASA Astrophysics Data System (ADS)

    Santana-Casiano, J. M.; Fraile-Nuez, E.; González-Dávila, M.; Baker, E. T.; Resing, J. A.; Walker, S. L.

    2016-05-01

    The residual hydrothermalism associated with submarine volcanoes, following an eruption event, plays an important role in the supply of CO2 to the ocean. The emitted CO2 increases the acidity of seawater. The submarine volcano of El Hierro, in its degasification stage, provided an excellent opportunity to study the effect of volcanic CO2 on the seawater carbonate system, the global carbon flux, and local ocean acidification. A detailed survey of the volcanic edifice was carried out using seven CTD-pH-ORP tow-yo studies, localizing the redox and acidic changes, which were used to obtain surface maps of anomalies. In order to investigate the temporal variability of the system, two CTD-pH-ORP yo-yo studies were conducted that included discrete sampling for carbonate system parameters. Meridional tow-yos were used to calculate the amount of volcanic CO2 added to the water column for each surveyed section. The inputs of CO2 along multiple sections combined with measurements of oceanic currents produced an estimated volcanic CO2 flux = 6.0 105 ± 1.1 105 kg d-1 which is ~0.1% of global volcanic CO2 flux. Finally, the CO2 emitted by El Hierro increases the acidity above the volcano by ~20%.

  13. Significant discharge of CO2 from hydrothermalism associated with the submarine volcano of El Hierro Island.

    PubMed

    Santana-Casiano, J M; Fraile-Nuez, E; González-Dávila, M; Baker, E T; Resing, J A; Walker, S L

    2016-05-09

    The residual hydrothermalism associated with submarine volcanoes, following an eruption event, plays an important role in the supply of CO2 to the ocean. The emitted CO2 increases the acidity of seawater. The submarine volcano of El Hierro, in its degasification stage, provided an excellent opportunity to study the effect of volcanic CO2 on the seawater carbonate system, the global carbon flux, and local ocean acidification. A detailed survey of the volcanic edifice was carried out using seven CTD-pH-ORP tow-yo studies, localizing the redox and acidic changes, which were used to obtain surface maps of anomalies. In order to investigate the temporal variability of the system, two CTD-pH-ORP yo-yo studies were conducted that included discrete sampling for carbonate system parameters. Meridional tow-yos were used to calculate the amount of volcanic CO2 added to the water column for each surveyed section. The inputs of CO2 along multiple sections combined with measurements of oceanic currents produced an estimated volcanic CO2 flux = 6.0 10(5) ± 1.1 10(5 )kg d(-1) which is ~0.1% of global volcanic CO2 flux. Finally, the CO2 emitted by El Hierro increases the acidity above the volcano by ~20%.

  14. Significant discharge of CO2 from hydrothermalism associated with the submarine volcano of El Hierro Island

    PubMed Central

    Santana-Casiano, J. M.; Fraile-Nuez, E.; González-Dávila, M.; Baker, E. T.; Resing, J. A.; Walker, S. L.

    2016-01-01

    The residual hydrothermalism associated with submarine volcanoes, following an eruption event, plays an important role in the supply of CO2 to the ocean. The emitted CO2 increases the acidity of seawater. The submarine volcano of El Hierro, in its degasification stage, provided an excellent opportunity to study the effect of volcanic CO2 on the seawater carbonate system, the global carbon flux, and local ocean acidification. A detailed survey of the volcanic edifice was carried out using seven CTD-pH-ORP tow-yo studies, localizing the redox and acidic changes, which were used to obtain surface maps of anomalies. In order to investigate the temporal variability of the system, two CTD-pH-ORP yo-yo studies were conducted that included discrete sampling for carbonate system parameters. Meridional tow-yos were used to calculate the amount of volcanic CO2 added to the water column for each surveyed section. The inputs of CO2 along multiple sections combined with measurements of oceanic currents produced an estimated volcanic CO2 flux = 6.0 105 ± 1.1 105 kg d−1 which is ~0.1% of global volcanic CO2 flux. Finally, the CO2 emitted by El Hierro increases the acidity above the volcano by ~20%. PMID:27157062

  15. Breathing modes of Kolumbo submarine volcano (Santorini, Greece).

    PubMed

    Bakalis, Evangelos; Mertzimekis, Theo J; Nomikou, Paraskevi; Zerbetto, Francesco

    2017-04-13

    Submarine volcanoes, such as Kolumbo (Santorini, Greece) are natural laboratories for fostering multidisciplinary studies. Their investigation requires the most innovative marine technology together with advanced data analysis. Conductivity and temperature of seawater were recorded directly above Kolumbo's hydrothermal vent system. The respective time series have been analyzed in terms of non-equilibrium techniques. The energy dissipation of the volcanic activity is monitored by the temperature variations of seawater. The venting dynamics of chemical products is monitored by water conductivity. The analysis of the time series in terms of stochastic processes delivers scaling exponents with turning points between consecutive regimes for both conductivity and temperature. Changes of conductivity are shown to behave as a universal multifractal and their variance is subdiffusive as the scaling exponents indicate. Temperature is constant over volcanic rest periods and a universal multifractal behavior describes its changes in line with a subdiffusive character otherwise. The universal multifractal description illustrates the presence of non-conservative conductivity and temperature fields showing that the system never retains a real equilibrium state. The existence of a repeated pattern of the combined effect of both seawater and volcanic activity is predicted. The findings can shed light on the dynamics of chemical products emitted from the vents and point to the presence of underlying mechanisms that govern potentially hazardous, underwater volcanic environments.

  16. Breathing modes of Kolumbo submarine volcano (Santorini, Greece)

    NASA Astrophysics Data System (ADS)

    Bakalis, Evangelos; Mertzimekis, Theo J.; Nomikou, Paraskevi; Zerbetto, Francesco

    2017-04-01

    Submarine volcanoes, such as Kolumbo (Santorini, Greece) are natural laboratories for fostering multidisciplinary studies. Their investigation requires the most innovative marine technology together with advanced data analysis. Conductivity and temperature of seawater were recorded directly above Kolumbo’s hydrothermal vent system. The respective time series have been analyzed in terms of non-equilibrium techniques. The energy dissipation of the volcanic activity is monitored by the temperature variations of seawater. The venting dynamics of chemical products is monitored by water conductivity. The analysis of the time series in terms of stochastic processes delivers scaling exponents with turning points between consecutive regimes for both conductivity and temperature. Changes of conductivity are shown to behave as a universal multifractal and their variance is subdiffusive as the scaling exponents indicate. Temperature is constant over volcanic rest periods and a universal multifractal behavior describes its changes in line with a subdiffusive character otherwise. The universal multifractal description illustrates the presence of non-conservative conductivity and temperature fields showing that the system never retains a real equilibrium state. The existence of a repeated pattern of the combined effect of both seawater and volcanic activity is predicted. The findings can shed light on the dynamics of chemical products emitted from the vents and point to the presence of underlying mechanisms that govern potentially hazardous, underwater volcanic environments.

  17. Hydrothermal Venting at Hinepuia Submarine Volcano, Kermadec Arc: Understanding Magmatic-Hydrothermal Fluid Chemistry

    NASA Astrophysics Data System (ADS)

    Stucker, Valerie K.; Walker, Sharon L.; de Ronde, Cornel E. J.; Caratori Tontini, Fabio; Tsuchida, Shinji

    2017-10-01

    The Hinepuia volcanic center is made up of two distinct edifices aligned northwest to southeast, with an active cone complex in the SE. Hinepuia is one of several active volcanoes in the northern segment of the Kermadec arc. Regional magnetic data show no evidence for large-scale hydrothermal alteration at Hinepuia, yet plume data confirm present-day hydrothermal discharge, suggesting that the hydrothermal system may be too young to have altered the host rocks with respect to measurable changes in magnetic signal. Gravity data are consistent with crustal thinning and shallow mantle under the volcanic center. Following the discovery of hydrothermal plumes over Hinepuia, the submersible Shinkai 6500 was used to explore the SE cone and sample hydrothermal fluids. The chemistry of hydrothermal fluids from submarine arc and backarc volcanoes is typically dominated by water-rock interactions and/or magmatic degassing. Chemical analyses of vent fluids show that Hinepuia does not quite fit either traditional model. Moreover, the Hinepuia samples fall between those typically ascribed to both end-member fluid types when plotted on a K-Mg-SO4 ternary diagram. Due to evidence of strong degassing, abundant native sulfur deposition, and H2S presence, the vent sampled at Hinepuia is ultimately classified as a magmatic-hydrothermal system with a water-rock influence. This vent is releasing water vapor and magmatic volatiles with a notable lack of salinity due to subcritical boiling and phase separation. Magmatic-hydrothermal fluid chemistry appears to be controlled by a combination of gas flux, phase separation processes, and volcano evolution and/or distance from the magma source.

  18. New insights into hydrothermal vent processes in the unique shallow-submarine arc-volcano, Kolumbo (Santorini), Greece

    PubMed Central

    Kilias, Stephanos P.; Nomikou, Paraskevi; Papanikolaou, Dimitrios; Polymenakou, Paraskevi N.; Godelitsas, Athanasios; Argyraki, Ariadne; Carey, Steven; Gamaletsos, Platon; Mertzimekis, Theo J.; Stathopoulou, Eleni; Goettlicher, Joerg; Steininger, Ralph; Betzelou, Konstantina; Livanos, Isidoros; Christakis, Christos; Bell, Katherine Croff; Scoullos, Michael

    2013-01-01

    We report on integrated geomorphological, mineralogical, geochemical and biological investigations of the hydrothermal vent field located on the floor of the density-stratified acidic (pH ~ 5) crater of the Kolumbo shallow-submarine arc-volcano, near Santorini. Kolumbo features rare geodynamic setting at convergent boundaries, where arc-volcanism and seafloor hydrothermal activity are occurring in thinned continental crust. Special focus is given to unique enrichments of polymetallic spires in Sb and Tl (±Hg, As, Au, Ag, Zn) indicating a new hybrid seafloor analogue of epithermal-to-volcanic-hosted-massive-sulphide deposits. Iron microbial-mat analyses reveal dominating ferrihydrite-type phases, and high-proportion of microbial sequences akin to "Nitrosopumilus maritimus", a mesophilic Thaumarchaeota strain capable of chemoautotrophic growth on hydrothermal ammonia and CO2. Our findings highlight that acidic shallow-submarine hydrothermal vents nourish marine ecosystems in which nitrifying Archaea are important and suggest ferrihydrite-type Fe3+-(hydrated)-oxyhydroxides in associated low-temperature iron mats are formed by anaerobic Fe2+-oxidation, dependent on microbially produced nitrate. PMID:23939372

  19. Internal structure of Puna Ridge: evolution of the submarine East Rift Zone of Kilauea Volcano, Hawai ̀i

    NASA Astrophysics Data System (ADS)

    Leslie, Stephen C.; Moore, Gregory F.; Morgan, Julia K.

    2004-01-01

    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 zone. Laterally continuous reflections are imaged deep beneath the axis of the East Rift Zone (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 dikes 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 intrusive dikes associated with the ERZ. Gravity modeling shows that the intrusive core of the ERZ is offset to the southeast of the topographic axis of the rift zone, and that the surface of the core dips more steeply to the northwest than to the southeast, suggesting that the dike complex has been progressively displaced to the southeast by subsequent intrusions. The gravity signature of the dike complex decreases in width down-rift, and is absent in the distal portion of the rift zone. 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 zone dynamics and partitioning of intrusive materials. We propose that these

  20. North Kona slump: Submarine flank failure during the early(?) tholeiitic shield stage of Hualalai Volcano

    USGS Publications Warehouse

    Lipman, P.W.; Coombs, M.L.

    2006-01-01

    The North Kona slump is an elliptical region, about 20 by 60 km (1000-km2 area), of multiple, geometrically intricate benches and scarps, mostly at water depths of 2000–4500 m, on the west flank of Hualalai Volcano. Two dives up steep scarps in the slump area were made in September 2001, using the ROV Kaiko of the Japan Marine Science and Technology Center (JAMSTEC), as part of a collaborative Japan–USA project to improve understanding of the submarine flanks of Hawaiian volcanoes. Both dives, at water depths of 2700–4000 m, encountered pillow lavas draping the scarp-and-bench slopes. Intact to only slightly broken pillow lobes and cylinders that are downward elongate dominate on the steepest mid-sections of scarps, while more equant and spherical pillow shapes are common near the tops and bases of scarps and locally protrude through cover of muddy sediment on bench flats. Notably absent are subaerially erupted Hualalai lava flows, interbedded hyaloclastite pillow breccia, and/or coastal sandy sediment that might have accumulated downslope from an active coastline. The general structure of the North Kona flank is interpreted as an intricate assemblage of downdropped lenticular blocks, bounded by steeply dipping normal faults. The undisturbed pillow-lava drape indicates that slumping occurred during shield-stage tholeiitic volcanism. All analyzed samples of the pillow-lava drape are tholeiite, similar to published analyses from the submarine northwest rift zone of Hualālai. Relatively low sulfur (330–600 ppm) and water (0.18–0.47 wt.%) contents of glass rinds suggest that the eruptive sources were in shallow water, perhaps 500–1000-m depth. In contrast, saturation pressures calculated from carbon dioxide concentrations (100–190 ppm) indicate deeper equilibration, at or near sample sites at water depths of − 3900 to − 2800 m. Either vents close to the sample sites erupted mixtures of undegassed and degassed magmas, or volatiles were resorbed from

  1. 30 years in the life of an active submarine volcano: The evolution of Kick-`em-Jenny and implications for hazard in the southern Caribbean

    NASA Astrophysics Data System (ADS)

    Allen, R. W.; Berry, C.; Henstock, T.; Collier, J.; Dondin, F. J. Y.; Latchman, J. L.; Robertson, R. E. A.

    2017-12-01

    Effective monitoring is an essential part of the process of identifying and mitigating volcanic hazards. In the submarine environment this task is made all the more difficult with observations typically limited to land-based seismic networks and infrequent shipboard surveys. Since announcing itself to the world in 1939, the Kick-`em-Jenny (KeJ) volcano, 8km off of the north coast of Grenada, has been the source of 13 episodes of T-phase recordings. These distinctive seismic signals, often coincident with heightened seismicity, have been interpreted as extrusive eruptions with a mean recurrence interval of 5-6 years. Visual confirmation of these episodes is rare and many would be unknown without the seismic evidence. By conducting new bathymetric surveys in 2016 and 2017 and reprocessing 3 further legacy data sets spanning more than 30 years and several such events we are able to present a clearer picture of the development of KeJ through time. The final bathymetric grids produced have a cell size of just 5m and, for the more modern surveys, a vertical accuracy on the order of 1m. These grids easily demonstrate the correlation between T-phase episodes and morphological changes at the volcano's edifice. In the time-period of observation we document a clear construction deficit at KeJ with only 5.75x106m3 of material added through constructive volcanism, while 5 times this amount is lost through landslides and volcanic dome collapse. The peak depth of KeJ now sits at 196m b.s.l., the lowest recorded since 1966. Limited recent magma production means that KeJ may be susceptible to larger eruptions with longer repeat times than those covered in our study. These larger eruptions would pose a more significant local hazard than the small scale volcanic events observed in recent decades. We conclude that T-phase recordings are likely to have a more varied origin than previously discussed, and are unlikely to be solely the result of extrusive submarine eruptions. This

  2. Characteristics of Offshore Hawai';i Island Seismicity and Velocity Structure, including Lo';ihi Submarine Volcano

    NASA Astrophysics Data System (ADS)

    Merz, D. K.; Caplan-Auerbach, J.; Thurber, C. H.

    2013-12-01

    the regional velocity model (HG50; Klein, 1989) in the shallow lithosphere above 16 km depth. This is likely a result of thick deposits of volcaniclastic sediments and fractured pillow basalts that blanket the southern submarine flank of Mauna Loa, upon which Lo';ihi is currently superimposing (Morgan et al., 2003). A broad, low-velocity anomaly was observed from 20-40 km deep beneath the area of Pahala, and is indicative of the central plume conduit that supplies magma to the active volcanoes. A localized high-velocity body is observed 4-6 km deep beneath Lo';ihi's summit, extending 10 km to the North and South. Oriented approximately parallel to Lo';ihi's active rift zones, this high-velocity body is suggestive of intrusion in the upper crust, similar to Kilauea's high-velocity rift zones.

  3. Hawaii's volcanoes revealed

    USGS Publications Warehouse

    Eakins, Barry W.; Robinson, Joel E.; Kanamatsu, Toshiya; Naka, Jiro; Smith, John R.; Takahashi, Eiichi; Clague, David A.

    2003-01-01

    Hawaiian volcanoes typically evolve in four stages as volcanism waxes and wanes: (1) early alkalic, when volcanism originates on the deep sea floor; (2) shield, when roughly 95 percent of a volcano's volume is emplaced; (3) post-shield alkalic, when small-volume eruptions build scattered cones that thinly cap the shield-stage lavas; and (4) rejuvenated, when lavas of distinct chemistry erupt following a lengthy period of erosion and volcanic quiescence. During the early alkalic and shield stages, two or more elongate rift zones may develop as flanks of the volcano separate. Mantle-derived magma rises through a vertical conduit and is temporarily stored in a shallow summit reservoir from which magma may erupt within the summit region or be injected laterally into the rift zones. The ongoing activity at Kilauea's Pu?u ?O?o cone that began in January 1983 is one such rift-zone eruption. The rift zones commonly extend deep underwater, producing submarine eruptions of bulbous pillow lava. Once a volcano has grown above sea level, subaerial eruptions produce lava flows of jagged, clinkery ?a?a or smooth, ropy pahoehoe. If the flows reach the ocean they are rapidly quenched by seawater and shatter, producing a steep blanket of unstable volcanic sediment that mantles the upper submarine slopes. Above sea level then, the volcanoes develop the classic shield profile of gentle lava-flow slopes, whereas below sea level slopes are substantially steeper. While the volcanoes grow rapidly during the shield stage, they may also collapse catastrophically, generating giant landslides and tsunami, or fail more gradually, forming slumps. Deformation and seismicity along Kilauea's south flank indicate that slumping is occurring there today. Loading of the underlying Pacific Plate by the growing volcanic edifices causes subsidence, forming deep basins at the base of the volcanoes. Once volcanism wanes and lava flows no longer reach the ocean, the volcano continues to submerge, while

  4. Magma plumbing system and seismicity of an active mid-ocean ridge volcano.

    PubMed

    Schmid, Florian; Schlindwein, Vera; Koulakov, Ivan; Plötz, Aline; Scholz, John-Robert

    2017-02-20

    At mid-ocean ridges volcanism generally decreases with spreading rate but surprisingly massive volcanic centres occur at the slowest spreading ridges. These volcanoes can host unexpectedly strong earthquakes and vigorous, explosive submarine eruptions. Our understanding of the geodynamic processes forming these volcanic centres is still incomplete due to a lack of geophysical data and the difficulty to capture their rare phases of magmatic activity. We present a local earthquake tomographic image of the magma plumbing system beneath the Segment 8 volcano at the ultraslow-spreading Southwest Indian Ridge. The tomography shows a confined domain of partial melt under the volcano. We infer that from there melt is horizontally transported to a neighbouring ridge segment at 35 km distance where microearthquake swarms and intrusion tremor occur that suggest ongoing magmatic activity. Teleseismic earthquakes around the Segment 8 volcano, prior to our study, indicate that the current magmatic spreading episode may already have lasted over a decade and hence its temporal extent greatly exceeds the frequent short-lived spreading episodes at faster opening mid-ocean ridges.

  5. Bubble Plumes at NW Rota-1 Submarine Volcano, Mariana Arc: Visualization and Analysis of Multibeam Water Column Data

    NASA Astrophysics Data System (ADS)

    Merle, S. G.; Chadwick, W. W.; Embley, R. W.; Doucet, M.

    2012-12-01

    During a March 2010 expedition to NW Rota-1 submarine volcano in the Mariana arc a new EM122 multibeam sonar system on the R/V Kilo Moana was used to repeatedly image bubble plumes in the water column over the volcano. The EM122 (12 kHz) system collects seafloor bathymetry and backscatter data, as well as acoustic return water column data. Previous expeditions to NW Rota-1 have included seafloor mapping / CTD tow-yo surveys and remotely operated vehicle (ROV) dives in 2004, 2005, 2006 and 2009. Much of the focus has been on the one main eruptive vent, Brimstone, located on the south side of the summit at a depth of ~440m, which has been persistently active during all ROV visits. Extensive degassing of CO2 bubbles have been observed by the ROV during frequent eruptive bursts from the vent. Between expeditions in April 2009 and March 2010 a major eruption and landslide occurred at NW Rota-1. ROV dives in 2010 revealed that after the landslide the eruptive vent had been reorganized from a single site to a line of vents. Brimstone vent was still active, but 4 other new eruptive vents had also emerged in a NW/SE line below the summit extending ~100 m from the westernmost to easternmost vents. During the ROV dives, the eruptive vents were observed to turn on and off from day to day and hour to hour. Throughout the 2010 expedition numerous passes were made over the volcano summit to image the bubble plumes above the eruptive vents in the water column, in order to capture the variability of the plumes over time and to relate them to the eruptive output of the volcano. The mid-water sonar data set totals >95 hours of observations over a 12-day period. Generally, the ship drove repeatedly over the eruptive vents at a range of ship speeds (0.5-4 knots) and headings. In addition, some mid-water data was collected during three ROV dives when the ship was stationary over the vents. We used the FMMidwater software program (part of QPS Fledermaus) to visualize and analyze the data

  6. New Perspectives on the Structure and Morphology of the Submarine Flanks of Galápagos Volcanoes- Fernandina and Isabela

    NASA Astrophysics Data System (ADS)

    Fornari, D. J.; Kurz, M. D.; Geist, D. J.; Johnson, P. D.; Peckman, U. G.; Scheirer, D.

    2001-12-01

    The submarine flanks of oceanic volcanoes are dynamic environments that reflect the history of volcanic construction and mass-wasting. The submarine slopes of the Galápagos had only been investigated during two modern research cruises - the 1990 PLUME 2 cruise and during the 2000 AHA-Nemo cruise. These data provide the backdrop for a recent sonar mapping and dredging cruise, carried out in Aug-Sept., 2001 on board R/V Revelle, over the southwestern and western edge of the Galápagos platform. The survey included detailed MR1 side-scan sonar imagery (gridded at 8 m pixel resolution) and EM120 multibeam bathymetry (gridded at 100 m pixel resolution), which provided the basis for detailed dredging and towed camera investigations of the submarine flanks of Fernandina and Isabela. The principal geologic provinces delineated by the MR1 sonar imagery include submarine rift zones, major landslides between the rifts, and inferred young lava flows at 3000-3500 m depth located 10-20 km west of the islands. Prominent submarine terraces extend for tens of kilometers along the platform edge south of Isabela and west of Floreana, and in the bight between Fernandina and Cerro Azul volcanoes. The depth range for the terraces is variable between 2000-3300 m. Galápagos submarine rift zones are characterized by mottled backscatter reflectivity seen elsewhere on seamounts, Hawaiian submarine rifts, and the mid-ocean ridge, and are interpreted as constructional submarine volcanic terrain comprising pillow and lobate lava. Extensive spatial variability in acoustic contrast is visible in the MR1 sonar data and is interpreted as complex inter-fingering of submarine eruptive units. These areas of presumably young, high reflectivity flows are located away from the submarine rifts and appear to overlie sediment. These flows cover distances as great as ~10-15 km and are located 10-20 km from the nearest coastline. These large submarine flows may relate to large subaerial events such as the

  7. Submarine Pyroclastic Flow Deposits; July 2003 Dome Collapse Event of the Soufrière Hills Volcano, Montserrat, West Indies

    NASA Astrophysics Data System (ADS)

    Trofimovs, J.; Sparks, S.; Talling, P.

    2006-12-01

    What happens when pyroclastic flows enter the ocean? To date, the subject of submarine pyroclastic flow behaviour has been controversial. Ambiguity arises from inconclusive evidence of a subaqueous depositional environment in ancient successions, to difficulty in sampling the in situ products of modern eruptions. A research voyage of the RRS James Clark Ross (9-18 May 2005) sampled 52 sites offshore from the volcanic island of Montserrat. The Soufrière Hills volcano, Montserrat, has been active since 1995 with eruptive behaviour dominated by andesite lava dome growth and collapse. Over 90% of the pyroclastic material produced has been deposited into the ocean. In July 2003 the Soufrière Hills volcano produced the largest historically documented dome collapse event. 210 x 106 m3 of pyroclastic material avalanched down the Tar River Valley, southeast Montserrat, to be deposited into the ocean. Bathymetric imaging and coring of offshore pyroclastic deposits, with a specific focus on the July 2003 units, reveals that the pyroclastic flows mix rapidly and violently with the water as they enter the ocean. Mixing takes place between the shore and 500 m depth where the deposition of basal coarse-grained parts of the flow initiates on slopes of 15° or less. The coarse components (pebbles to boulders) are deposited proximally from dense basal slurries to form steep sided, near linear ridges that amalgamate to form a kilometer-scale submarine fan. These proximal deposits contain <1% of ash-grade material. The finer components (dominantly ash-grade) are mixed into the overlying water column to form turbidity currents that flow distances >40 km from source. The total volume of pyroclastic material deposited within the submarine environment during this event exceeds 170 x 106 m3, with 65% deposited in proximal lobes and 35% deposited as distal turbidites. This broadly correlates with the block and ash components respectively, of the source subaerial pyroclastic flow. However

  8. Evolution of submarine eruptive activity during the 2011-2012 El Hierro event as documented by hydroacoustic images and remotely operated vehicle observations

    NASA Astrophysics Data System (ADS)

    Somoza, L.; González, F. J.; Barker, S. J.; Madureira, P.; Medialdea, T.; de Ignacio, C.; Lourenço, N.; León, R.; Vázquez, J. T.; Palomino, D.

    2017-08-01

    Submarine volcanic eruptions are frequent and important events, yet they are rarely observed. Here we relate bathymetric and hydroacoustic images from the 2011 to 2012 El Hierro eruption with surface observations and deposits imaged and sampled by ROV. As a result of the shallow submarine eruption, a new volcano named Tagoro grew from 375 to 89 m depth. The eruption consisted of two main phases of edifice construction intercalated with collapse events. Hydroacoustic images show that the eruptions ranged from explosive to effusive with variable plume types and resulting deposits, even over short time intervals. At the base of the edifice, ROV observations show large accumulations of lava balloons changing in size and type downslope, coinciding with the area where floating lava balloon fallout was observed. Peaks in eruption intensity during explosive phases generated vigorous bubbling at the surface, extensive ash, vesicular lapilli and formed high-density currents, which together with periods of edifice gravitational collapse, produced extensive deep volcaniclastic aprons. Secondary cones developed in the last stages and show evidence for effusive activity with lava ponds and lava flows that cover deposits of stacked lava balloons. Chaotic masses of heterometric boulders around the summit of the principal cone are related to progressive sealing of the vent with decreasing or variable magma supply. Hornitos represent the final eruptive activity with hydrothermal alteration and bacterial mats at the summit. Our study documents the distinct evolution of a submarine volcano and highlights the range of deposit types that may form and be rapidly destroyed in such eruptions.Plain Language SummaryToday and through most of geological history, the greatest number and volume of volcanic eruptions on Earth have occurred underwater. However, in comparison to subaerial eruption, little is known about <span class="hlt">submarine</span> eruptive processes as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSME31B..08R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSME31B..08R"><span>­­­­High-Resolution Mapping of Kick`em Jenny <span class="hlt">Submarine</span> <span class="hlt">Volcano</span> and Associated Landslides</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ruchala, T. L.; Carey, S.; Hart, L.; Chen, M.; Scott, C.; Tominaga, M.; Dondin, F. J. Y.; Fujii, M.</p> <p>2016-02-01</p> <p>To understand the physical and geological processes that drive the volcanism and control the morphology of Kick`em Jenny (KEJ) <span class="hlt">volcano</span>, the only <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> in the in the Lesser Antilles volcanic arc, we conducted near-source, high-resolution mapping of KEJ and its subsurface using the Remotely Operated Vehicle (ROV) Hercules during cruise NA054 of the E/V Nautilus (Sept.-Oct. 2014). Shipboard bathymetric data (EM302 system) and slope analysis maps were used to decipher the detailed seafloor morphology surrounding KEJ. Multiple generations of <span class="hlt">submarine</span> landslides and canyons were observed, suggesting the area has been hosting dynamic sediment transport systems at multiple scales over time. Some of them might have been associated by past eruptions. Clear contacts between partially lithified carbonate sediments and volcanic formations were identified from ROV videos at the middle of the landslide slope face. Detailed observations of facies on these exposures provide constraints on the time intervals between landslide events along the western slope of KEJ. ROV video imagery also identified outcrops of columnar basalts located in the middle of the landslide deposits. These are similar in appearance to those observed in the KEJ crater during previous ROV dives, indicating a possible travel distance of volcanic materials from the crater region along landslide path. High-resolution photo mosaics, bathymetry, and magnetic data acquired by ROV Hercules were used to investigate geological processes and the possible volcanic source of landslide material within the KEJ crater. Mapping in the northwestern part of the crater floor revealed distinctive regions, including (i) microbial mats, (ii) <span class="hlt">active</span> hydrothermal vent sites; (iii) landforms curved by channelized bottom current where seafloor is outcropped; and (iv) coarse scree the distribution of which may correlate with the distance from the crater rim. Near-bottom magnetic profiles show coherent magnetic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3390001','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3390001"><span>The <span class="hlt">submarine</span> <span class="hlt">volcano</span> eruption at the island of El Hierro: physical-chemical perturbation and biological response</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Fraile-Nuez, E.; González-Dávila, M.; Santana-Casiano, J. M.; Arístegui, J.; Alonso-González, I. J.; Hernández-León, S.; Blanco, M. J.; Rodríguez-Santana, A.; Hernández-Guerra, A.; Gelado-Caballero, M. D.; Eugenio, F.; Marcello, J.; de Armas, D.; Domínguez-Yanes, J. F.; Montero, M. F.; Laetsch, D. R.; Vélez-Belchí, P.; Ramos, A.; Ariza, A. V.; Comas-Rodríguez, I.; Benítez-Barrios, V. M.</p> <p>2012-01-01</p> <p>On October 10 2011 an underwater eruption gave rise to a novel shallow <span class="hlt">submarine</span> <span class="hlt">volcano</span> south of the island of El Hierro, Canary Islands, Spain. During the eruption large quantities of mantle-derived gases, solutes and heat were released into the surrounding waters. In order to monitor the impact of the eruption on the marine ecosystem, periodic multidisciplinary cruises were carried out. Here, we present an initial report of the extreme physical-chemical perturbations caused by this event, comprising thermal changes, water acidification, deoxygenation and metal-enrichment, which resulted in significant alterations to the <span class="hlt">activity</span> and composition of local plankton communities. Our findings highlight the potential role of this eruptive process as a natural ecosystem-scale experiment for the study of extreme effects of global change stressors on marine environments. PMID:22768379</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27103730','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27103730"><span>Draft Genome Sequence of Methanoculleus sediminis S3FaT, a Hydrogenotrophic Methanogen Isolated from a <span class="hlt">Submarine</span> Mud <span class="hlt">Volcano</span> in Taiwan.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Sheng-Chung; Chen, Mei-Fei; Weng, Chieh-Yin; Lai, Mei-Chin; Wu, Sue-Yao</p> <p>2016-04-21</p> <p>Here, we announce the genome sequence of ITALIC! Methanoculleus sediminisS3Fa(T)(DSM 29354(T)), a strict anaerobic methanoarchaeon, which was isolated from sediments near the <span class="hlt">submarine</span> mud <span class="hlt">volcano</span> MV4 located offshore in southwestern Taiwan. The 2.49-Mb genome consists of 2,459 predicted genes, 3 rRNAs, 48 tRNAs, and 1 ncRNA. The sequence of this novel strain may provide more information for species delineation and the roles that this strain plays in the unique marine mud <span class="hlt">volcano</span> habitat. Copyright © 2016 Chen et al.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap3_Clague.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap3_Clague.pdf"><span>Growth and degradation of Hawaiian <span class="hlt">volcanoes</span>: Chapter 3 in Characteristics of Hawaiian <span class="hlt">volcanoes</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>Clague, David A.; Sherrod, David R.; Poland, Michael P.; Takahashi, T. Jane; Landowski, Claire M.</p> <p>2014-01-01</p> <p>Large Hawaiian <span class="hlt">volcanoes</span> can persist as islands through the rapid subsidence by building upward rapidly enough. But in the long run, subsidence, coupled with surface erosion, erases any volcanic remnant above sea level in about 15 m.y. One consequence of subsidence, in concert with eustatic changes in sea level, is the drowning of coral reefs that drape the <span class="hlt">submarine</span> flanks of the <span class="hlt">actively</span> subsiding <span class="hlt">volcanoes</span>. At least six reefs northwest of the Island of Hawai‘i form a stairstep configuration, the oldest being deepest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS21A1955D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS21A1955D"><span>Flank Collapse Assessment At Kick-'em-Jenny <span class="hlt">Submarine</span> <span class="hlt">Volcano</span> (Lesser Antilles): A Combined Approach Using Modelling and Experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dondin, F. J. Y.; Heap, M. J.; Robertson, R. E. A.; Dorville, J. F. M.; Carey, S.</p> <p>2016-12-01</p> <p>In the Lesser Antilles over 52 volcanic landslide episodes have been identified. These episodes serve as a testament to the hazard posed by volcanic landslides to a region composed of many islands that are small independent countries with vulnerable local economies. This study presents a relative slope stability analysis (RIA) to investigate the stability condition of the only <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> of the Lesser Antilles Arc: Kick-'em-Jenny <span class="hlt">Submarine</span> <span class="hlt">Volcano</span> (KeJ). Thus we hope to provide better constraint on the landslide source geometry to help mitigate volcanic landslide hazards at a KeJ. KeJ is located ca. 8 km north of Grenada island. KeJ lies within a collapse scar from a prehistorical flank collapse. This collapse was associated with a voluminous landslide deposit of about 4.4km3 with a 14 km runout. Numerial simulations showed that this event could generate a regional tsunami. We aim to quantify potential initial volumes of collapsed material using a RIA. The RIA evaluates the critical potential failure surface associated with factor of safety (Fs) inferior to unity and compares them to areas of deficit/surplus of mass/volume obtained from the comparison of an high resolution digital elevation model of the edifice with an ideal 3D surface. We use freeware programs <span class="hlt">Volcano</span>Fit 2.0 and SSAP 4.7. and produce a 3D representation of the stability map. We report, for the first time, results of a Limit Equilibrium Method performed using geomechanical parameters retrieved from rock mechanics tests performed on two rock basaltic-andesite rock samples collected from within the crater of the <span class="hlt">volcano</span> during the 1-18 November 2013 NA039 E/V Nautilus cruise. We performed triaxial and uniaxial deformation tests to obtain values of strength at the top and bottom of the edifice. We further characterized the permeability and P-wave velocity of the samples collected. The chosen internal structure for the model is composed of three bodies: (i) a body composed of basaltic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMNH23B1876D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMNH23B1876D"><span>Numerical Tsunami Hazard Assessment of the Only <span class="hlt">Active</span> Lesser Antilles Arc <span class="hlt">Submarine</span> <span class="hlt">Volcano</span>: Kick 'em Jenny.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dondin, F. J. Y.; Dorville, J. F. M.; Robertson, R. E. A.</p> <p>2015-12-01</p> <p>The Lesser Antilles Volcanic Arc has potentially been hit by prehistorical regional tsunamis generated by voluminous volcanic landslides (volume > 1 km3) among the 53 events recognized so far. No field evidence of these tsunamis are found in the vincity of the sources. Such a scenario taking place nowadays would trigger hazardous tsunami waves bearing potentially catastrophic consequences for the closest islands and regional offshore oil platforms.Here we applied a complete hazard assessment method on the only <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> of the arc Kick 'em Jenny (KeJ). KeJ is the southernmost edifice with recognized associated volcanic landslide deposits. From the three identified landslide episodes one is associated with a collapse volume ca. 4.4 km3. Numerical simulations considering a single pulse collapse revealed that this episode would have produced a regional tsunami. An edifice current volume estimate is ca. 1.5 km3.Previous study exists in relationship to assessment of regional tsunami hazard related to shoreline surface elevation (run-up) in the case of a potential flank collapse scenario at KeJ. However this assessment was based on inferred volume of collapse material. We aim to firstly quantify potential initial volumes of collapse material using relative slope instability analysis (RSIA); secondly to assess first order run-ups and maximum inland inundation distance for Barbados and Trinidad and Tobago, i.e. two important economic centers of the Lesser Antilles. In this framework we present for seven geomechanical models tested in the RSIA step maps of critical failure surface associated with factor of stability (Fs) for twelve sectors of 30° each; then we introduce maps of expected potential run-ups (run-up × the probability of failure at a sector) at the shoreline.The RSIA evaluates critical potential failure surface associated with Fs <1 as compared to areas of deficit/surplus of mass/volume identified on the volcanic edifice using (<span class="hlt">Volcano</span>Fit 2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41C1984J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41C1984J"><span>From <span class="hlt">Submarine</span> <span class="hlt">Volcanoes</span> to Modern Atolls: New Insights from the Mozambique Channel (SW Indian Ocean)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jorry, S.; Courgeon, S.; Camoin, G.; BouDagher-Fadel, M.; Jouet, G.; Poli, E.</p> <p>2016-12-01</p> <p>Although the long-term evolution of isolated shallow-water carbonate platforms leading to guyot and atoll formation has been the subject of numerous studies during the last decades, their driving processes are still the subject of <span class="hlt">active</span> debates. The Mozambique Channel (SW Indian Ocean) is characterized by several modern carbonate platforms, ranging from 11°S to 21°S in latitudes. These platforms are characterized by reef margins mostly developed on windward sides with internal parts blanketed by sand dunes and numerous reef pinnacles, or by Darwin-type atolls with enclosed lagoons. Dredge sampling, underwater observations and geophysical acquisitions carried out during recent oceanographic cruises (PTOLEMEE and PAMELA-MOZ1) along slopes and basins adjacent to modern platforms led to the discovery of flat-top seamounts corresponding to shallow-water carbonate platforms which grew on top of <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>. Microfacies and datings (biostratigraphy analysis coupled with Strontium isotopic stratigraphy) indicate that those carbonate platforms, characterized by fauna assemblages dominated by corals, Halimeda and red algaes, and larger benthic foraminifera, developed in tropical settings from Early Miocene to Late Miocene/Early Pliocene times. <span class="hlt">Submarine</span> volcanism, karstification and pedogenesis evidences on top of the drowned edifices demonstrate that tectonic deformation, rejuvenated volcanic <span class="hlt">activity</span> and subaerial exposure occurred after and potentially during the Neogene platform aggradation. Growth of modern platforms on top of submerged carbonate terraces is explained by topographic irregularities inherited from volcanism, tectonic and/or subaerial exposure conditions which could have produced favorable substratum for carbonates which grew during the Plio-Quaternary, up to reach modern sea-level. This research is co-funded by TOTAL and IFREMER as part of the PAMELA (Passive Margin Exploration Laboratories) scientific project.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001EOSTr..82...67D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001EOSTr..82...67D"><span>“Edifice Rex” Sulfide Recovery Project: Analysis of <span class="hlt">submarine</span> hydrothermal, microbial habitat</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delaney, John R.; Kelley, Deborah S.; Mathez, Edmond A.; Yoerger, Dana R.; Baross, John; Schrenk, Matt O.; Tivey, Margaret K.; Kaye, Jonathan; Robigou, Veronique</p> <p></p> <p>Recent scientific developments place inquiries about <span class="hlt">submarine</span> volcanic systems in a broad planetary context. Among these is the discovery that <span class="hlt">submarine</span> eruptions are intimately linked with massive effusions of microbes and their products from below the sea floor [Holden et al., 1998]. This material includes microbes that only grow at temperatures tens of degrees higher than the temperatures of the vent fluids from which they were sampled. Such results lend support for the existence of a potentially extensive, but currently unexplored sub-sea floor microbial biosphere associated with <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> [Deming and Baross, 1993; Delaney et al., 1998; Summit and Baross, 1998].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S44B..08D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S44B..08D"><span>Insights on volcanic behaviour from the 2015 July 23-24 T-phase signals generated by eruptions at Kick-'em-Jenny <span class="hlt">Submarine</span> <span class="hlt">Volcano</span>, Grenada, Lesser Antilles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dondin, F. J. Y.; Latchman, J. L.; Robertson, R. E. A.; Lynch, L.; Stewart, R.; Smith, P.; Ramsingh, C.; Nath, N.; Ramsingh, H.; Ash, C.</p> <p>2015-12-01</p> <p>Kick-'em-Jenny <span class="hlt">volcano</span> (KeJ) is the only known <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> in the Lesser Antilles Arc. Since 1939, the year it revealed itself, and until the <span class="hlt">volcano</span>-seismic unrest of 2015 July 11-25 , the <span class="hlt">volcano</span> has erupted 12 times. Only two eruptions breached the surface: 1939, 1974. The <span class="hlt">volcano</span> has an average eruption cycle of about 10-11 years. Excluding the Montserrat, Soufrière Hills, KeJ is the most <span class="hlt">active</span> <span class="hlt">volcano</span> in the Lesser Antilles arc. The University of the West Indies, Seismic Research Centre (SRC) has been monitoring KeJ since 1953. On July 23 and 24 at 1:42 am and 0:02 am local time, respectively, the SRC recorded T-phase signals , considered to have been generated by KeJ. Both signals were recorded at seismic stations in and north of Grenada: SRC seismic stations as well as the French <span class="hlt">volcano</span> observatories in Guadeloupe and Martinique, Montserrat <span class="hlt">Volcano</span> Observatory, and the Puerto Rico Seismic Network. These distant recordings, along with the experience of similar observations in previous eruptions, allowed the SRC to confirm that two explosive eruptions occurred in this episode at KeJ. Up to two days after the second eruption, when aerial surveillance was done, there was no evidence of <span class="hlt">activity</span> at the surface. During the instrumental era, eruptions of the KeJ have been identified from T-phases recorded at seismic stations from Trinidad, in the south, to Puerto Rico, in the north. In the 2015 July eruption episode, the seismic station in Trinidad did not record T-phases associated with the KeJ eruptions. In this study we compare the T-phase signals of 2015 July with those recorded in KeJ eruptions up to 1974 to explore possible causative features for the T-phase recording pattern in KeJ eruptions. In particular, we investigate the potential role played by the Sound Fixing and Ranging (SOFAR) layer in influencing the absence of the T-phase on the Trinidad seismic station during this eruption.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022059','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022059"><span>In search of ancestral Kilauea <span class="hlt">volcano</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>Lipman, P.W.; Sisson, T.W.; Ui, T.; Naka, J.</p> <p>2000-01-01</p> <p>Submersible observations and samples show that the lower south flank of Hawaii, offshore from Kilauea <span class="hlt">volcano</span> and the <span class="hlt">active</span> Hilina slump system, consists entirely of compositionally diverse volcaniclastic rocks; pillow lavas are confined to shallow slopes. <span class="hlt">Submarine</span>-erupted basalt clasts have strongly variable alkalic and transitional basalt compositions (to 41% SiO2, 10.8% alkalies), contrasting with present-day Kilauea tholeiites. The volcaniclastic rocks provide a unique record of ancestral alkalic growth of an archetypal hotspot <span class="hlt">volcano</span>, including transition to its tholeiitic shield stage, and associated slope-failure events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011NatGe...4..799R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011NatGe...4..799R"><span><span class="hlt">Active</span> <span class="hlt">submarine</span> eruption of boninite in the northeastern Lau Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Resing, Joseph A.; Rubin, Kenneth H.; Embley, Robert W.; Lupton, John E.; Baker, Edward T.; Dziak, Robert P.; Baumberger, Tamara; Lilley, Marvin D.; Huber, Julie A.; Shank, Timothy M.; Butterfield, David A.; Clague, David A.; Keller, Nicole S.; Merle, Susan G.; Buck, Nathaniel J.; Michael, Peter J.; Soule, Adam; Caress, David W.; Walker, Sharon L.; Davis, Richard; Cowen, James P.; Reysenbach, Anna-Louise; Thomas, Hans</p> <p>2011-11-01</p> <p>Subduction of oceanic crust and the formation of volcanic arcs above the subduction zone are important components in Earth's geological and geochemical cycles. Subduction consumes and recycles material from the oceanic plates, releasing fluids and gases that enhance magmatic <span class="hlt">activity</span>, feed hydrothermal systems, generate ore deposits and nurture chemosynthetic biological communities. Among the first lavas to erupt at the surface from a nascent subduction zone are a type classified as boninites. These lavas contain information about the early stages of subduction, yet because most subduction systems on Earth are old and well-established, boninite lavas have previously only been observed in the ancient geological record. Here we observe and sample an <span class="hlt">active</span> boninite eruption occurring at 1,200m depth at the West Mata <span class="hlt">submarine</span> <span class="hlt">volcano</span> in the northeast Lau Basin, southwest Pacific Ocean. We find that large volumes of H2O, CO2 and sulphur are emitted, which we suggest are derived from the subducting slab. These volatiles drive explosive eruptions that fragment rocks and generate abundant incandescent magma-skinned bubbles and pillow lavas. The eruption has been ongoing for at least 2.5 years and we conclude that this boninite eruption is a multi-year, low-mass-transfer-rate eruption. Thus the Lau Basin may provide an important site for the long-term study of <span class="hlt">submarine</span> volcanic eruptions related to the early stages of subduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS53C1226C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS53C1226C"><span>Comparison with Offshore and Onshore Mud <span class="hlt">Volcanoes</span> in the Southwestern Taiwan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Y. H.; Su, C. C.; Chen, T. T.; Liu, C. S.; Paull, C. K.; Caress, D. W.; Gwiazda, R.; Lundsten, E. M.; Hsu, H. H.</p> <p>2017-12-01</p> <p>The offshore area southwest (SW) of Taiwan is on the convergent boundary between the Eurasian and Philippine Sea plates. The plate convergence manifests in this unique geological setting as a fold-and-thrust-belt. Multi-channel seismic profiles, and bathymetry and gravity anomaly data collected from Taiwan offshore to the SW show the presence of a large amount of mud <span class="hlt">volcanoes</span> and diapirs with NE-SW orientations. In the absence of comprehensive sampling and detailed geochemistry data from <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span>, the relation between onshore and offshore mud <span class="hlt">volcanoes</span> remains ambiguous. During two MBARI and IONTU joint cruises conducted in 2017 we collected high-resolution multibeam bathymetry data (1-m-resolution) and chirp sub-bottom profiles with an autonomous underwater vehicle (AUV) from <span class="hlt">submarine</span> Mud <span class="hlt">Volcano</span> III (MV3), and obtained precisely located samples and video observations with a remotely operated vehicle (ROV). MV3 is an <span class="hlt">active</span> <span class="hlt">submarine</span> mud <span class="hlt">volcano</span> at 465 m water depth offshore SW Taiwan. This cone-shape mud <span class="hlt">volcano</span> is almost 780 m wide, 150 m high, with 8° slopes, and a 30 m wide mound on the top. Several linear features are observed in the southwest of the mound, and these features are interpreted as a series of marks caused by rolling rocks that erupted from the top of MV3. We collected three rocks and push cores from MV3 and its top with the ROV, in order to compare their chemical and mineralogical composition to that of samples collected from mud <span class="hlt">volcanoes</span> along the Chishan fault. The surface and X-radiography imaging, 210Pb chronology, grain size and X-ray diffractometer analyses were conducted to compare geochemical and sedimentary properties of offshore and onshore mud <span class="hlt">volcanoes</span>. The results indicate that the offshore and onshore mud <span class="hlt">volcanoes</span> have similar characteristics. We suggest that offshore and onshore mud <span class="hlt">volcanoes</span> of SW Taiwan are no different in the source of their materials and their mechanism of creation and evolution.</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('http://adsabs.harvard.edu/abs/2012EGUGA..1411980A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1411980A"><span>Deployment of a seismic array for <span class="hlt">volcano</span> monitoring during the ongoing <span class="hlt">submarine</span> eruption at El Hierro, Canary Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abella, R.; Almendros, J.; Carmona, E.; Martin, R.</p> <p>2012-04-01</p> <p>On 17 July 2011 there was an important increase of the seismic <span class="hlt">activity</span> at El Hierro (Canary Islands, Spain). This increase was detected by the <span class="hlt">Volcano</span> Monitoring Network (Spanish national seismic network) run by the Instituto Geográfico Nacional (IGN). As a consequence, the IGN immediately deployed a dense, complete monitoring network that included seismometers, GPS stations, geochemical equipment, magnetometers, and gravity meters. During the first three months of <span class="hlt">activity</span>, the seismic network recorded over ten thousand <span class="hlt">volcano</span>-tectonic earthquakes, with a maximum magnitude of 4.6. On 10 October 2011 an intense volcanic tremor started. It was a monochromatic signal, with variable amplitude and frequency content centered at about 1-2 Hz. The tremor onset was correlated with the initial stages of the <span class="hlt">submarine</span> eruption that occurred from a vent located south of El Hierro island, near the village of La Restinga. At that point the IGN, in collaboration with the Instituto Andaluz de Geofísica, deployed a seismic array intended for volcanic tremor monitoring and analysis. The seismic array is located about 7 km NW of the <span class="hlt">submarine</span> vent. It has a 12-channel, 24-bit data acquisition system sampling each channel at 100 sps. The array is composed by 1 three-component and 9 vertical-component seismometers, distributed in a flat area with an aperture of 360 m. The data provided by the seismic array are going to be processed using two different approaches: (1) near-real-time, to produce information that can be useful in the management of the volcanic crisis; and (2) detailed investigations, to study the volcanic tremor characteristics and relate them to the eruption dynamics. At this stage we are mostly dedicated to produce fast, near-real-time estimates. Preliminary results have been obtained using the maximum average cross-correlation method. They indicate that the tremor wavefronts are highly coherent among array stations and propagate across the seismic array with an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018LPICo2085.6039R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018LPICo2085.6039R"><span>Explosive Deep Sea Volcanism Produces Composite <span class="hlt">Volcanoes</span> (Stratocones) with Predominantly Diffuse Flow Hydrothermal Ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rubin, K. H.; Chadwick, W. C.; Embley, R. W.; Butterfield, D. A.</p> <p>2018-05-01</p> <p>Newly-discovered extensive explosive deep sea volcanism produces distinct stratovolcano structures and physical rock characteristics, and host primarily diffuse flow hydrothermal <span class="hlt">activity</span>, unlike focused flow systems at effusive <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17051217','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17051217"><span>Novel microbial communities of the Haakon Mosby mud <span class="hlt">volcano</span> and their role as a methane sink.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Niemann, Helge; Lösekann, Tina; de Beer, Dirk; Elvert, Marcus; Nadalig, Thierry; Knittel, Katrin; Amann, Rudolf; Sauter, Eberhard J; Schlüter, Michael; Klages, Michael; Foucher, Jean Paul; Boetius, Antje</p> <p>2006-10-19</p> <p>Mud volcanism is an important natural source of the greenhouse gas methane to the hydrosphere and atmosphere. Recent investigations show that the number of <span class="hlt">active</span> <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span> might be much higher than anticipated (for example, see refs 3-5), and that gas emitted from deep-sea seeps might reach the upper mixed ocean. Unfortunately, global methane emission from <span class="hlt">active</span> <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span> cannot be quantified because their number and gas release are unknown. It is also unclear how efficiently methane-oxidizing microorganisms remove methane. Here we investigate the methane-emitting Haakon Mosby Mud <span class="hlt">Volcano</span> (HMMV, Barents Sea, 72 degrees N, 14 degrees 44' E; 1,250 m water depth) to provide quantitative estimates of the in situ composition, distribution and <span class="hlt">activity</span> of methanotrophs in relation to gas emission. The HMMV hosts three key communities: aerobic methanotrophic bacteria (Methylococcales), anaerobic methanotrophic archaea (ANME-2) thriving below siboglinid tubeworms, and a previously undescribed clade of archaea (ANME-3) associated with bacterial mats. We found that the upward flow of sulphate- and oxygen-free mud <span class="hlt">volcano</span> fluids restricts the availability of these electron acceptors for methane oxidation, and hence the habitat range of methanotrophs. This mechanism limits the capacity of the microbial methane filter at <span class="hlt">active</span> marine mud <span class="hlt">volcanoes</span> to <40% of the total flux.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21382146','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21382146"><span>Methanogenic diversity and <span class="hlt">activity</span> in hypersaline sediments of the centre of the Napoli mud <span class="hlt">volcano</span>, Eastern Mediterranean Sea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lazar, Cassandre Sara; Parkes, R John; Cragg, Barry A; L'Haridon, Stéphane; Toffin, Laurent</p> <p>2011-08-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> are a significant source of methane to the atmosphere. The Napoli mud <span class="hlt">volcano</span>, situated in the brine-impacted Olimpi Area of the Eastern Mediterranean Sea, emits mainly biogenic methane particularly at the centre of the mud <span class="hlt">volcano</span>. Temperature gradients support the suggestion that Napoli is a cold mud <span class="hlt">volcano</span> with moderate fluid flow rates. Biogeochemical and molecular genetic analyses were carried out to assess the methanogenic <span class="hlt">activity</span> rates, pathways and diversity in the hypersaline sediments of the centre of the Napoli mud <span class="hlt">volcano</span>. Methylotrophic methanogenesis was the only significant methanogenic pathway in the shallow sediments (0-40 cm) but was also measured throughout the sediment core, confirming that methylotrophic methanogens could be well adapted to hypersaline environments. Hydrogenotrophic methanogenesis was the dominant pathway below 50 cm; however, low rates of acetoclastic methanogenesis were also present, even in sediment layers with the highest salinity, showing that these methanogens can thrive in this extreme environment. PCR-DGGE and methyl coenzyme M reductase gene libraries detected sequences affiliated with anaerobic methanotrophs (mainly ANME-1) as well as Methanococcoides methanogens. Results show that the hypersaline conditions in the centre of the Napoli mud <span class="hlt">volcano</span> influence <span class="hlt">active</span> biogenic methane fluxes and methanogenic/methylotrophic diversity. © 2011 Society for Applied Microbiology and Blackwell Publishing Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993vpp..book.....F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993vpp..book.....F"><span><span class="hlt">Volcanoes</span>. A planetary perspective.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Francis, P.</p> <p></p> <p>In this book, the author gives an account of the familiar violent aspects of <span class="hlt">volcanoes</span> and the various forms that eruptions can take. He explores why <span class="hlt">volcanoes</span> exist at all, why <span class="hlt">volcanoes</span> occur where they do, and how examples of major historical eruptions can be interpreted in terms of physical processes. Throughout he attempts to place volcanism in a planetary perspective, exploring the pre-eminent role of <span class="hlt">submarine</span> volcanism on Earth and the stunning range of volcanic phenomena revealed by spacecraft exploration of the solar system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014DSRI...93..156C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014DSRI...93..156C"><span>Cold seeps associated with a <span class="hlt">submarine</span> debris avalanche deposit at Kick'em Jenny <span class="hlt">volcano</span>, Grenada (Lesser Antilles)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carey, Steven; Ballard, Robert; Bell, Katherine L. C.; Bell, Richard J.; Connally, Patrick; Dondin, Frederic; Fuller, Sarah; Gobin, Judith; Miloslavich, Patricia; Phillips, Brennan; Roman, Chris; Seibel, Brad; Siu, Nam; Smart, Clara</p> <p>2014-11-01</p> <p>Remotely operated vehicle (ROV) exploration at the distal margins of a debris avalanche deposit from Kick'em Jenny <span class="hlt">submarine</span> <span class="hlt">volcano</span> in Grenada has revealed areas of cold seeps with chemosynthetic-based ecosystems. The seeps occur on steep slopes of deformed, unconsolidated hemipelagic sediments in water depths between 1952 and 2042 m. Two main areas consist of anastomosing systems of fluid flow that have incised local sediments by several tens of centimeters. No temperature anomalies were observed in the vent areas and no <span class="hlt">active</span> flow was visually observed, suggesting that the venting may be waning. An Eh sensor deployed on a miniature autonomous plume recorder (MAPR) recorded a positive signal and the presence of live organisms indicates at least some venting is still occurring. The chemosynthetic-based ecosystem included giant mussels (Bathymodiolus sp.) with commensal polychaetes (Branchipolynoe sp.) and cocculinid epibionts, other bivalves, Siboglinida (vestimentiferan) tubeworms, other polychaetes, and shrimp, as well as associated heterotrophs, including gastropods, anemones, crabs, fish, octopods, brittle stars, and holothurians. The origin of the seeps may be related to fluid overpressure generated during the collapse of an ancestral Kick'em Jenny <span class="hlt">volcano</span>. We suggest that deformation and burial of hemipelagic sediment at the front and base of the advancing debris avalanche led to fluid venting at the distal margin. Such deformation may be a common feature of marine avalanches in a variety of geological environments especially along continental margins, raising the possibility of creating large numbers of ephemeral seep-based ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.V22A0567R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.V22A0567R"><span>A Geochemical Study of Magmatic Processes and Evolution along the <span class="hlt">Submarine</span> Southwest Rift zone of Mauna Loa <span class="hlt">Volcano</span>, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rhodes, J. M.; Garcia, M. O.; Weis, D.; Trusdell, F. A.; Vollinger, M. J.</p> <p>2003-12-01</p> <p>Mauna Loa's southwest rift zone (SWR) extends for 102 km from its summit caldera, at an elevation of 4,170 m above sea level, to <span class="hlt">submarine</span> depths of over 4,500 m. About 65% of the rift zone is subaerial and 35% <span class="hlt">submarine</span>. Recent sampling with the Jason II submersible of the `mile-high' (1800 m) Ka Lae <span class="hlt">submarine</span> landslide scarp and the deepest section of the rift zone, in conjunction with previous submersible and dredge-haul collecting, provides petrological and geochemical understanding of rift zone processes, as well as a record of Mauna Loa's eruptive history extending back about 400 ka. The major and trace element trends of the <span class="hlt">submarine</span> lavas are remarkably similar to those of historical and young prehistoric lavas (<31 ka) erupted along the subaerial SWR. We take this to imply that magma-forming processes have remained relatively constant over much of the <span class="hlt">volcano</span>'s recorded eruptive history. However, the distribution of samples along these trends has varied, and is correlated with elevation. There are very few picrites (>12% MgO) among the subaerial lavas, and compositions tend to cluster around 6.8-8.0% MgO. In contrast, picritic lavas are extremely abundant in the <span class="hlt">submarine</span> samples, increasing in frequency with depth, especially below 1200 m. These observations support earlier interpretations that the <span class="hlt">submarine</span> lavas are derived directly from deeper levels in the magma column, and that magmas from a shallow, steady-state, magma reservoir are of uncommon at these depths. Isotopic ratios of Pb and Sr in the <span class="hlt">submarine</span> lavas, in conjunction with Nb/Y and Zr/Nb ratios, extend from values that are identical with subaerial historical Mauna Loa lavas to lavas with markedly lower 87Sr/86Sr and higher 206Pb/204Pb isotopic ratios. As yet, we see no correlation with depth or age, but the implications are that, in the past, the plume source of Mauna Loa magmas was more variable than in the last 31 ka, and contained a greater proportion of the Kea component. *Team members</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41C1971R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41C1971R"><span>Characterizing Volcanic Processes using Near-bottom, High Resolution Magnetic Mapping of the Caldera and Inner Crater of the Kick'em Jenny <span class="hlt">Submarine</span> <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ruchala, T. L.; Chen, M.; Tominaga, M.; Carey, S.</p> <p>2016-12-01</p> <p>Kick'em Jenny (KEJ) is an <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> located in the Lesser Antilles subduction zone, 7.5 km north of the Caribbean island Grenada. KEJ, known as one of the most explosive <span class="hlt">volcanoes</span> in Caribbean, erupted 12 times since 1939 with recent eruptions in 2001 and possibly in 2015. Multiple generations of <span class="hlt">submarine</span> landslides and canyons have been observed in which some of them can be attributed to past eruptions. The structure of KEJ can be characterized as a 1300 m high conical profile with its summit crater located around 180 m in depth. <span class="hlt">Active</span> hydrothermal venting and dominantly CO2 composition gas seepage take place inside this 250m diameter crater, with the most <span class="hlt">activity</span> occurring primarily within a small ( 70 x 110 m) depression zone (inner crater). In order to characterize the subsurface structure and decipher the processes of this volcanic system, the Nautilus NA054 expedition in 2014 deployed the underwater Remotely Operated Vehicle (ROV) Hercules to conduct near-bottom geological observations and magnetometry surveys transecting KEJ's caldera. Raw magnetic data was corrected for vehicle induced magnetic noise, then merged with ROV to ship navigation at 1 HZ. To extract crustal magnetic signatures, the reduced magnetic data was further corrected for external variations such as the International Geomagnetic Reference Field and diurnal variations using data from the nearby San Juan Observatory. We produced a preliminary magnetic anomaly map of KEJ's caldera for subsequent inversion and forward modeling to delineate in situ magnetic source distribution in understanding volcanic processes. We integrated the magnetic characterization of the KEJ craters with shipboard multibeam, ROV visual descriptions, and photomosaics. Initial observations show the distribution of short wavelength scale highly magnetized source centered at the north western part of the inner crater. Although locations of gas seeps are ubiquitous over the inner crater area along ROV</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V11E..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V11E..03C"><span>Hydrothermal Venting at Kick'Em Jenny <span class="hlt">Submarine</span> <span class="hlt">Volcano</span> (West Indies)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carey, S.; Croff Bell, K. L.; Dondin, F. J. Y.; Roman, C.; Smart, C.; Lilley, M. D.; Lupton, J. E.; Ballard, R. D.</p> <p>2014-12-01</p> <p>Kick'em Jenny is a frequently-erupting, shallow <span class="hlt">submarine</span> <span class="hlt">volcano</span> located ~8 km off the northwest coast of Grenada in the West Indies. The last eruption took place in 2001 but did not breach the sea surface. Focused and diffuse hydrothermal venting is taking place mainly within a small (~100 x 100 m) depression within the 300 m diameter crater of the <span class="hlt">volcano</span> at depths of about 265 meters. Near the center of the depression clear fluids are being discharged from a focused mound-like vent at a maximum temperature of 180o C with the simultaneous discharge of numerous bubble streams. The gas consists of 93-96% CO2 with trace amounts of methane and hydrogen. A sulfur component likely contributes 1-4% of the gas total. Gas flux measurements on individual bubble streams ranged from 10 to 100 kg of CO2 per day. Diffuse venting with temperatures 5 to 35o C above ambient occurs throughout the depression and over large areas of the main crater. These zones are extensively colonized by reddish-yellow bacterial mats with the production of loose Fe-oxyhydroxides largely as a surface coating and in some cases, as fragile spires up to several meters in height. A high-resolution photo mosaic of the crater depression was constructed using the remotely operated vehicle Hercules on cruise NA039 of the E/V Nautilus. The image revealed prominent fluid flow patterns descending the sides of the depression towards the base. We speculate that the negatively buoyant fluid flow may be the result of second boiling of hydrothermal fluids at Kick'em Jenny generating a dense saline component that does not rise despite its elevated temperature. Increased density may also be the result of high dissolved CO2 content of the fluids, although we were not able to measure this directly. The low amount of sulphide mineralization on the crater floor suggests that deposition may be occurring mostly subsurface, in accord with models of second boiling mineralization from other hydrothermal vent systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFMED13E0757W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFMED13E0757W"><span>Dive and Explore: An Interactive Web Visualization that Simulates Making an ROV Dive to an <span class="hlt">Active</span> <span class="hlt">Submarine</span> <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weiland, C.; Chadwick, W. W.</p> <p>2004-12-01</p> <p>Several years ago we created an exciting and engaging multimedia exhibit for the Hatfield Marine Science Center that lets visitors simulate making a dive to the seafloor with the remotely operated vehicle (ROV) named ROPOS. The exhibit immerses the user in an interactive experience that is naturally fun but also educational. The public display is located at the Hatfield Marine Science Visitor Center in Newport, Oregon. We are now completing a revision to the project that will make this engaging virtual exploration accessible to a much larger audience. With minor modifications we will be able to put the exhibit onto the world wide web so that any person with internet access can view and learn about exciting volcanic and hydrothermal <span class="hlt">activity</span> at Axial Seamount on the Juan de Fuca Ridge. The modifications address some cosmetic and logistic ISSUES confronted in the museum environment, but will mainly involve compressing video clips so they can be delivered more efficiently over the internet. The web version, like the museum version, will allow users to choose from 1 of 3 different dives sites in the caldera of Axial <span class="hlt">Volcano</span>. The dives are based on real seafloor settings at Axial seamount, an <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> on the Juan de Fuca Ridge (NE Pacific) that is also the location of a seafloor observatory called NeMO. Once a dive is chosen, then the user watches ROPOS being deployed and then arrives into a 3-D computer-generated seafloor environment that is based on the real world but is easier to visualize and navigate. Once on the bottom, the user is placed within a 360 degree panorama and can look in all directions by manipulating the computer mouse. By clicking on markers embedded in the scene, the user can then either move to other panorama locations via movies that travel through the 3-D virtual environment, or they can play video clips from actual ROPOS dives specifically related to that scene. Audio accompanying the video clips informs the user where they are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.V43F2328J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.V43F2328J"><span>40Ar/39Ar geochronology of <span class="hlt">submarine</span> Mauna Loa <span class="hlt">volcano</span>, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jicha, B.; Rhodes, J. M.; Singer, B. S.; Vollinger, M. J.; Garcia, M. O.</p> <p>2009-12-01</p> <p>A major impediment to our understanding of the nature and structure of the Hawaiian plume, and evaluating the competing plume models has been a lack of thick stratigraphic sections from which to obtain long temporal records of magmatic history. The Hawaii Scientific Drilling Project (HSDP) made a significant advance towards solving this problem by documenting the long-term magmatic evolution of Mauna Kea <span class="hlt">volcano</span> on the Kea side of the plume. To evaluate comparable long-term magmatic history on the Loa side of the plume we collected a stratigraphically controlled sample suite using Jason and Pisces dives from three vertical transects of the 1.6 km high Kae Lae landslide scarp cut into Mauna Loa’s <span class="hlt">submarine</span> southwest rift zone (SWR). We have undertaken an 40Ar/39Ar investigation of Mauna Loa’s growth history to integrate new geochronologic constraints with geochemical, and isotopic data, illuminating temporal trends within the Hawaiian plume. Obtaining precise 40Ar/39Ar ages from tholeiitic lavas younger than 500 ka containing only 0.2-0.6 wt.% K2O is challenging due to the extremely low radiogenic 40Ar contents. Furnace incremental heating experiments of groundmass separated from 15 <span class="hlt">submarine</span> lavas have yielded four new age determinations (a 27% success rate). These four lavas give concordant age spectra with plateau and isochron ages that agree with stratigraphy. We also analyzed two previously-dated subaerial Mauna Kea tholeiites from the HSDP-2 drill core, to assess inter-laboratory reproducibility and calibrate our results to those obtained for the core. Two experiments on sample SR413-4.0 and one experiment from SR781-21.2 gave weighted mean plateau ages of 364 ± 95 ka and 473 ± 109, respectively, which are indistinguishable from the published 40Ar/39Ar ages of 390 ± 70 ka and 482 ± 67. Although Sharp and Renne (2005) preferred isochron ages for the <span class="hlt">submarine</span> Mauna Kea tholeiites recovered from HSDP, we find that <span class="hlt">submarine</span> Mauna Loa lavas contain</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1815570D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1815570D"><span>Flank Collapse Assessment At Kick-'em-Jenny <span class="hlt">Submarine</span> <span class="hlt">Volcano</span> (Lesser Antilles): A Combined Approach Using Modelling and Experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dondin, Frédéric; Heap, Michael; Robert, Richard E. A.; Dorville, Jean-Francois M.; Carey, Steven</p> <p>2016-04-01</p> <p>Volcanic landslides - the result of volcanic flank failure - are highly hazardous mass movements due to their high mobility, the wide area they can impact, and their potential to generate tsunamis. In the Lesser Antilles at least 53 episodes of flank collapse have been identified, with many of them associated with voluminous (Vdeposit exceeding 1 km3) <span class="hlt">submarine</span> volcanic landslide deposits. The existence of such voluminous deposits highlights the hazard of potentially devastating tsunami waves to the populated islands of the Lesser Antilles. To help understand and mitigate such hazards, we applied a relative stability assessment method to the only <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> of the Lesser Antilles island arc: Kick-'em-Jenny (KeJ). KeJ - located 8 km north of the island of Grenada - is the southernmost edifice in the arc with recognized associated volcanic landslide deposits. From the three identified landslide prehistoric episodes, one is associated with a collapse volume of about 4.4 km3. Numerical simulations considering a single pulse collapse revealed that this episode would have produced a regional tsunami. A volume estimate of the present day edifice is about 1.5 km3. We aim to quantify potential initial volumes of collapsed material using relative instability analysis (RIA). The RIA evaluates the critical potential failure surface associated with factor of safety (Fs) inferior to 1 and compares them to areas of deficit/surplus of mass/volume obtained from the comparison of an high resolution digital elevation model of the edifice with an ideal 3D surface named Volcanoid. To do so we use freeware programs <span class="hlt">Volcano</span>Fit 2.0 and SSAP 4.5. We report, for the first time, results of a Limit Equilibrium Method (Janbu's rigorous method) as a slope stability computation analysis performed using geomechanical parameters retrieved from rock mechanics tests performed on two rock basaltic-andesite rock samples collected from within the crater of the <span class="hlt">volcano</span> during the 1</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V31E..01C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V31E..01C"><span>Vertical Motions of Oceanic <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clague, D. A.; Moore, J. G.</p> <p>2006-12-01</p> <p>Oceanic <span class="hlt">volcanoes</span> offer abundant evidence of changes in their elevations through time. Their large-scale motions begin with a period of rapid subsidence lasting hundreds of thousands of years caused by isostatic compensation of the added mass of the <span class="hlt">volcano</span> on the ocean lithosphere. The response is within thousands of years and lasts as long as the <span class="hlt">active</span> <span class="hlt">volcano</span> keeps adding mass on the ocean floor. Downward flexure caused by volcanic loading creates troughs around the growing <span class="hlt">volcanoes</span> that eventually fill with sediment. Seismic surveys show that the overall depression of the old ocean floor beneath Hawaiian <span class="hlt">volcanoes</span> such as Mauna Loa is about 10 km. This gross subsidence means that the drowned shorelines only record a small part of the total subsidence the islands experienced. In Hawaii, this history is recorded by long-term tide-gauge data, the depth in drill holes of subaerial lava flows and soil horizons, former shorelines presently located below sea level. Offshore Hawaii, a series of at least 7 drowned reefs and terraces record subsidence of about 1325 m during the last half million years. Older sequences of drowned reefs and terraces define the early rapid phase of subsidence of Maui, Molokai, Lanai, Oahu, Kauai, and Niihau. Volcanic islands, such as Maui, tip down toward the next younger <span class="hlt">volcano</span> as it begins rapid growth and subsidence. Such tipping results in drowned reefs on Haleakala as deep as 2400 m where they are tipped towards Hawaii. Flat-topped <span class="hlt">volcanoes</span> on <span class="hlt">submarine</span> rift zones also record this tipping towards the next younger <span class="hlt">volcano</span>. This early rapid subsidence phase is followed by a period of slow subsidence lasting for millions of years caused by thermal contraction of the aging ocean lithosphere beneath the <span class="hlt">volcano</span>. The well-known evolution along the Hawaiian chain from high to low volcanic island, to coral island, and to guyot is due to this process. This history of rapid and then slow subsidence is interrupted by a period of minor uplift</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002GMS...128..193S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002GMS...128..193S"><span><span class="hlt">Submarine</span> alkalic through tholeiitic shield-stage development of Kīlauea <span class="hlt">volcano</span>, 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>Sisson, Thomas W.; Lipman, Peter W.; Naka, Jiro</p> <p></p> <p>The <span class="hlt">submarine</span> Hilina region exposes a succession of magma compositions spanning the juvenile "Lō'ihi" through tholeiitic shield stages of Kīlauea <span class="hlt">volcano</span>. Early products, preserved as glass grains and clasts in volcaniclastic rocks of the 3000 m deep Hilina bench, include nephelinite, basanite, phonotephrite, hawaiite, alkali basalt, transitional basalt, and rare alkali-poor Mauna Loa-like tholeiite. Transitional basalt pillow lavas overlie the volcaniclastic section and record an early phase of subsequent subalkaline magmatism. Rare degassed tholeiitic pillow lava and talus above the volcaniclastic section are products of subaerial shield volcanism. Major and trace element variations of clasts and pillow lavas point to a factor of 2-2.5 increase in degree of melting from juvenile alkalic to modern tholeiitic Kīlauea. Progressive changes in element ratios that distinguish Hawaiian shield <span class="hlt">volcanoes</span>, without commensurate changes in elements fractionated by partial melting, also signal increased contributions from Mauna Loa-type source regions as Kīlauea matured from its juvenile alkalic to its tholeiitic shield stage. Ancestral Kīlauea basanites and nephelinites were not primitive magmas but might have evolved from plume-derived alkali picritic parents by lithospheric-level crystallization differentiation, or solidification and remelting, involving pyroxene and garnet, similar to the subcrustal differentiation origin of hawaiites [Frey et al., 1990]. Low magmatic productivity early in Kīlauea's history sustained a poorly integrated trans-lithospheric conduit system in which magmas stalled and differentiated, producing evolved hawaiites, nephelinites, and basanites. This contrasts with shield-stage Kīlauea where high magmatic productivity flushes the conduit system and delivers primitive magmas to shallow levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012419','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012419"><span><span class="hlt">Submarine</span> volcanic features west of Kealakekua Bay, 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>Fornari, D.J.; Lockwood, J.P.; Lipman, P.W.; Rawson, M.; Malahoff, A.</p> <p>1980-01-01</p> <p>Visual observations of <span class="hlt">submarine</span> volcanic vents were made from the submersible vehicle DSV "Sea Cliff" in water depths between 1310 and 690 m, west of Kealakekua Bay, Hawaii. Glass-rich, shelly <span class="hlt">submarine</span> lavas surround circular 1- to 3-m-diameter volcanic vents between 1050 and 690 m depth in an area west-northwest of the southernpoint (Keei Pt.) of Kealakekua Bay. Eye-witness accounts indicate that this area was the site of a <span class="hlt">submarine</span> eruption on February 24, 1877. Chemical analyses of lavas from these possible seafloor vent areas indicate that the eruptive products are very similar in composition to volcanic rocks produced by historic eruptions of Mauna Loa <span class="hlt">volcano</span>. ?? 1980.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4105617','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4105617"><span>The <span class="hlt">Submarine</span> <span class="hlt">Volcano</span> Eruption off El Hierro Island: Effects on the Scattering Migrant Biota and the Evolution of the Pelagic Communities</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ariza, Alejandro; Kaartvedt, Stein; Røstad, Anders; Garijo, Juan Carlos; Arístegui, Javier; Fraile-Nuez, Eugenio; Hernández-León, Santiago</p> <p>2014-01-01</p> <p>The <span class="hlt">submarine</span> <span class="hlt">volcano</span> eruption off El Hierro Island (Canary Islands) on 10 October 2011 promoted dramatic perturbation of the water column leading to changes in the distribution of pelagic fauna. To study the response of the scattering biota, we combined acoustic data with hydrographic profiles and concurrent sea surface turbidity indexes from satellite imagery. We also monitored changes in the plankton and nekton communities through the eruptive and post-eruptive phases. Decrease of oxygen, acidification, rising temperature and deposition of chemicals in shallow waters resulted in a reduction of epipelagic stocks and a disruption of diel vertical migration (nocturnal ascent) of mesopelagic organisms. Furthermore, decreased light levels at depth caused by extinction in the volcanic plume resulted in a significant shallowing of the deep acoustic scattering layer. Once the eruption ceased, the distribution and abundances of the pelagic biota returned to baseline levels. There was no evidence of a <span class="hlt">volcano</span>-induced bloom in the plankton community. PMID:25047077</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25047077','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25047077"><span>The <span class="hlt">submarine</span> <span class="hlt">volcano</span> eruption off El Hierro Island: effects on the scattering migrant biota and the evolution of the pelagic communities.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ariza, Alejandro; Kaartvedt, Stein; Røstad, Anders; Garijo, Juan Carlos; Arístegui, Javier; Fraile-Nuez, Eugenio; Hernández-León, Santiago</p> <p>2014-01-01</p> <p>The <span class="hlt">submarine</span> <span class="hlt">volcano</span> eruption off El Hierro Island (Canary Islands) on 10 October 2011 promoted dramatic perturbation of the water column leading to changes in the distribution of pelagic fauna. To study the response of the scattering biota, we combined acoustic data with hydrographic profiles and concurrent sea surface turbidity indexes from satellite imagery. We also monitored changes in the plankton and nekton communities through the eruptive and post-eruptive phases. Decrease of oxygen, acidification, rising temperature and deposition of chemicals in shallow waters resulted in a reduction of epipelagic stocks and a disruption of diel vertical migration (nocturnal ascent) of mesopelagic organisms. Furthermore, decreased light levels at depth caused by extinction in the volcanic plume resulted in a significant shallowing of the deep acoustic scattering layer. Once the eruption ceased, the distribution and abundances of the pelagic biota returned to baseline levels. There was no evidence of a <span class="hlt">volcano</span>-induced bloom in the plankton community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20533949','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20533949"><span>Bacterial diversity in Fe-rich hydrothermal sediments at two South Tonga Arc <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Forget, N L; Murdock, S A; Juniper, S K</p> <p>2010-12-01</p> <p>Seafloor iron oxide deposits are a common feature of <span class="hlt">submarine</span> hydrothermal systems. Morphological study of these deposits has led investigators to suggest a microbiological role in their formation, through the oxidation of reduced Fe in hydrothermal fluids. Fe-oxidizing bacteria, including the recently described Zetaproteobacteria, have been isolated from a few of these deposits but generally little is known about the microbial diversity associated with this habitat. In this study, we characterized bacterial diversity in two Fe oxide samples collected on the seafloor of <span class="hlt">Volcanoes</span> 1 and 19 on the South Tonga Arc. We were particularly interested in confirming the presence of Zetaproteobacteria at these two sites and in documenting the diversity of groups other than Fe oxidizers. Our results (small subunit rRNA gene sequence data) showed a surprisingly high bacterial diversity, with 150 operational taxonomic units belonging to 19 distinct taxonomic groups. Both samples were dominated by Zetaproteobacteria Fe oxidizers. This group was most abundant at <span class="hlt">Volcano</span> 1, where sediments were richer in Fe and contained more crystalline forms of Fe oxides. Other groups of bacteria found at these two sites include known S- and a few N-metabolizing bacteria, all ubiquitous in marine environments. The low similarity of our clones with the GenBank database suggests that new species and perhaps new families were recovered. The results of this study suggest that Fe-rich hydrothermal sediments, while dominated by Fe oxidizers, can be exploited by a variety of autotrophic and heterotrophic micro-organisms. © 2010 Blackwell Publishing Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MarGR.tmp...29C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MarGR.tmp...29C"><span>Multi-stage formation of La Fossa Caldera (Vulcano Island, Italy) from an integrated subaerial and <span class="hlt">submarine</span> analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Casalbore, D.; Romagnoli, C.; Bosman, A.; De Astis, G.; Lucchi, F.; Tranne, C. A.; Chiocci, F. L.</p> <p>2018-06-01</p> <p> remnants of intra-caldera volcanic <span class="hlt">activity</span> are still evident. <span class="hlt">Submarine</span> morphological features associated to the entrance of subaerial lava flow units into the sea are presented, particularly related to the construction of the La Fossa Cone and Vulcanello. More generally, this study demonstrates the utility of integrated marine and subaerial studies to unravel the <span class="hlt">volcano</span>-tectonic evolution of <span class="hlt">active</span> insular <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70182514','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70182514"><span>Growth and collapse of Waianae <span class="hlt">volcano</span>, Hawaii, as revealed by exploration of its <span class="hlt">submarine</span> flanks</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Coombs, Michelle L.; Clague, David A.; Moore, Gregory F.; Cousens, Brian L.</p> <p>2004-01-01</p> <p>Wai‘anae <span class="hlt">Volcano</span> comprises the western half of O‘ahu Island, but until recently little was known about the <span class="hlt">submarine</span> portion of this <span class="hlt">volcano</span>. Seven new submersible dives, conducted in 2001 and 2002, and multibeam bathymetry offshore of Wai‘anae provide evidence pertaining to the overall growth of the <span class="hlt">volcano</span>'s edifice as well as the timing of collapses that formed the Wai‘anae slump complex. A prominent slope break at ∼1400 mbsl marks the paleoshoreline of Wai‘anae at the end of its shield-building stage and wraps around Ka‘ena Ridge, suggesting that this may have been an extension of Wai‘anae's northwest rift zone. Subaerially erupted tholeiitic lavas were collected from a small shield along the crest of Ka‘ena Ridge. The length of Wai‘anae's south rift zone is poorly constrained but reaches at least 65 km on the basis of recovered tholeiite pillows at this distance from the <span class="hlt">volcano</span>'s center. Wai‘anae's growth was marked by multiple collapse and deformation events during and after its shield stage, resulting in the compound mass wasting features on the <span class="hlt">volcano</span>'s southwest flank (Wai‘anae slump complex). The slump complex, one of the largest in Hawai‘i, covering an area of ∼5500 km2, is composed of several distinct sections on the basis of morphology and the lithologies of recovered samples. Two dives ascended the outer bench of the slump complex and collected predominantly low-S tholeiites that correlate with subaerial lavas erupted early during the <span class="hlt">volcano</span>'s shield stage, from 3.9 to 3.5 Ma. Pillow lavas from the outer bench have Pb, Sr, and Nd isotopic values that overlap with previously published subaerial Wai‘anae lavas. On the basis of the compositions of the recovered samples, the main body of the slump complex, as represented by the outer bench, probably formed during and shortly after the early shield stage. To the southwest of the outer bench lies a broad debris field on the seafloor, interpreted to have formed by 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_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/2012JGRB..117.9204J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRB..117.9204J"><span>40Ar/39Ar geochronology of <span class="hlt">submarine</span> Mauna Loa <span class="hlt">volcano</span>, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jicha, Brian R.; Rhodes, J. Michael; Singer, Brad S.; Garcia, Michael O.</p> <p>2012-09-01</p> <p>New geochronologic constraints refine the growth history of Mauna Loa <span class="hlt">volcano</span> and enhance interpretations of the petrologic, geochemical, and isotopic evolution of Hawaiian magmatism. We report results of 40Ar/39Ar incremental heating experiments on low-K, tholeiitic lavas from the 1.6 km high Kahuku landslide scarp cutting Mauna Loa's <span class="hlt">submarine</span> southwest rift zone, and from lavas in a deeper section of the rift. Obtaining precise40Ar/39Ar ages from young, tholeiitic lavas containing only 0.2-0.3 wt.% K2O is challenging due to their extremely low radiogenic 40Ar contents. Analyses of groundmass from 45 lavas yield 14 new age determinations (31% success rate) with plateau and isochron ages that agree with stratigraphic constraints. Lavas collected from a 1250 m thick section in the landslide scarp headwall were all erupted around 470 ± 10 ka, implying an extraordinary period of accumulation of ˜25 mm/yr, possibly correlating with the peak of the shield-building stage. This rate is three times higher than the estimated vertical lava accumulation rate for shield-building at Mauna Kea (8.6 ± 3.1 mm/yr) based on results from the Hawaii Scientific Drilling Project. Between ˜470 and 273 ka, the lava accumulation rate along the southwest rift zone decreased dramatically to ˜1 mm/yr. We propose that the marked reduction in lava accumulation rate does not mark the onset of post-shield volcanism as previously suggested, but rather indicates the upward migration of the magma system as Mauna Loa evolved from a <span class="hlt">submarine</span> stage of growth to one that is predominantly subaerial, thereby cutting off supply to the distal rift zone. Prior to ˜250 ka, lavas with Loihi-like isotopic signatures were erupted along with lavas having typical Mauna Loa values, implying greater heterogeneity in the plume source earlier in Mauna Loa's growth. In addition to refining accumulation rates and the isotopic evolution of the lavas erupted along the southwest rift zone, our new40Ar/39Ar results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....8058W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....8058W"><span>Highlights from the 2002 JASON2 marine expedition to Mauna Loa <span class="hlt">Volcano</span>, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weis, D.; Submarine Mauna Loa Science Team</p> <p>2003-04-01</p> <p>The new JASON2 ROV was used for 12 dives to explore and sample the <span class="hlt">submarine</span> flanks of Mauna Loa, the world’s largest <span class="hlt">active</span> <span class="hlt">volcano</span>. JASON2 collected 215 visually (using video and still camera) and spatially well-documented rock and sediment samples totaling 1130 kg from the volcano’s southwest rift zone and western flank. The goals of the expedition were to investigate the nature and history of the Hawaiian mantle plume as revealed in a 1.6 km thick, <span class="hlt">submarine</span> landslide scarp, to examine volcanic processes along the 37 km long, <span class="hlt">submarine</span> portion of the southwest rift zone, which has 4.5 km of relief, and to sample the newly discovered <span class="hlt">submarine</span> radial vents. In addition, detailed bathymetric data was collected for an area of 2000 km2 using an EM300 system, which has a pixel resolution of 30 m allowing for identification of small (horizontal) scale volcanic and tectonic features. These surveys provide the first detailed examination of the volcano’s <span class="hlt">submarine</span> rift zone and western flank. They revealed 11 new radial vents, many of which appear to be young based on examination by JASON2. Radial vents are uncommon on Hawaiian <span class="hlt">volcanoes</span> and represent only 2 of the 39 historical Mauna Loa eruptions. Picritic basalts are remarkably abundant in the rift zone section, which may record 400,000 years of eruptive <span class="hlt">activity</span> representing about one half of the volcano’s total lifetime. This time period is comparable to that sampled by phase 2 of the Hawaiian Scientific Drilling Project. The initial bathymetric and geologic results from this cruise will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ESASP.677E.108B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ESASP.677E.108B"><span>Glob<span class="hlt">Volcano</span>: Earth Observation Services for Global Monitroing of <span class="hlt">Active</span> <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Borgstrom, S.; Bianchi, M.; Bronson, W.; Tampellini, M. L.; Ratti, R.; Seifert, F. M.; Komorowski, J. C.; Kaminski, E.; Peltier, A.; Van der Voet, P.</p> <p>2010-03-01</p> <p>The Glob<span class="hlt">Volcano</span> project (2007-2010) is part of the Data User Element (DUE) programme of the European Space Agency (ESA).The objective of the project is to demonstrate EO-based (Earth Observation) services able to support the <span class="hlt">Volcano</span> Observatories and other mandate users (Civil Protection, <span class="hlt">volcano</span> scientific community) in their monitoring <span class="hlt">activities</span>.The set of offered EO based information products is the following:- Deformation Mapping- Surface Thermal Anomalies- Volcanic Gas Emission- Volcanic Ash TrackingThe Deformation Mapping service is performed exploiting either PSInSARTM or Conventional DInSAR (EarthView® InSAR). The processing approach is selected according to the availability of SAR data and users' requests.The information services are assessed in close cooperation with the user organizations for different types of <span class="hlt">volcano</span>, from various geographical areas in various climatic zones. Users are directly and <span class="hlt">actively</span> involved in the validation of the Earth Observation products, by comparing them with ground data available at each site.In a first phase, the Glob<span class="hlt">Volcano</span> Information System was designed, implemented and validated, involving a limited number of test areas and respective user organizations (Colima in Mexico, Merapi in Indonesia, Soufrière Hills in Montserrat Island, Piton de la Fournaise in La Reunion Island, Karthala in Comore Islands, Stromboli and <span class="hlt">Volcano</span> in Italy). In particular Deformation Mapping results obtained for Piton de la Fournaise were compared with deformation rates measured by the <span class="hlt">volcano</span> observatory using GPS stations and tiltmeters. IPGP (Institut de Physique du Globe de Paris) is responsible for the validation <span class="hlt">activities</span>.The second phase of the project (currently on-going) concerns the service provision on pre-operational basis. Fifteen volcanic sites located in four continents are monitored and as many user organizations are involved and cooperating with the project team.In addition to the proprietary tools mentioned before, in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V14A..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V14A..06G"><span>Emissions of Fe(II) and its kinetic of oxidation at Tagoro <span class="hlt">submarine</span> <span class="hlt">volcano</span>, El Hierro (Canary Islands)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>González-Dávila, M.; Santana-González, C.; Santana-Casiano, J. M.</p> <p>2017-12-01</p> <p>The eruptive process that took place in October 2011 in the <span class="hlt">submarine</span> <span class="hlt">volcano</span> Tagoro off the Island of El Hierro (Canary Island) and the subsequent degasification stage, five months later, have increased the concentration of TdFe(II) (Total dissolved iron(II)) in the waters nearest to the volcanic edifice. In order to detect any variation in concentrations of TdFe(II) due to hydrothermal emissions, three cruises were carried out two years after the eruptive process in October 2013, March 2014, May 2015, March 2016 and November 2016. The results from these cruises confirmed important positive anomalies in TdFe(II), which coincided with negatives anomalies in pHF,is (pH in free scale, at in situ conditions) located in the proximity of the main cone. Maximum values in TdFe(II) both at the surface, associated to chlorophyll a maximum, and at the sea bottom, were also observed, showing the important influence of organic complexation and particle re-suspension processes. Temporal variability studies were carried out over periods ranging from hours to days in the stations located over the main and two secondary cones in the volcanic edifice with positive anomalies in TdFe(II) concentrations and negative anomalies in pHF,is values. Observations showed an important variability in both pHF,is and TdFe(II) concentrations, which indicated the volcanic area was affected by a degasification process that remained in the <span class="hlt">volcano</span> after the eruptive phase had ceased. Fe(II) oxidation kinetic studies were also undertaken in order to analyze the effects of the seawater properties in the proximities of the <span class="hlt">volcano</span> on the oxidation rate constants and t1/2 (half-life time) of ferrous iron. The increased TdFe(II) concentrations and the low associated pHF,is values acted as an important fertilization event in the seawater around the Tagoro <span class="hlt">volcano</span> at the Island of El Hierro providing optimal conditions for the regeneration of the area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998Geo....26..439S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998Geo....26..439S"><span>Boron-rich mud <span class="hlt">volcanoes</span> of the Black Sea region: Modern analogues to ancient sea-floor tourmalinites associated with Sullivan-type Pb-Zn deposits?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Slack, John F.; Turner, Robert J. W.; Ware, Paul L. G.</p> <p>1998-05-01</p> <p>Large <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span> in the abyssal part of the Black Sea south of the Crimean Peninsula are similar in many respects to synsedimentary mud <span class="hlt">volcanoes</span> in the Mesoproterozoic Belt-Purcell basin. One of the Belt-Purcell mud <span class="hlt">volcanoes</span> directly underlies the giant Sullivan Pb-Zn-Ag deposit in southeastern British Columbia. Footwall rocks to the Sullivan deposit comprise variably tourmalinized siltstone, conglomerate, and related fragmental rock; local thin pyrrhotite-rich and spessartine-quartz beds are interpreted as Fe and Fe-Mn exhalites, respectively. Analogous Fe- and Mn-rich sediments occur near the abyssal Black Sea mud <span class="hlt">volcanoes</span>. Massive pyrite crusts and associated carbonate chimneys discovered in relatively shallow waters (˜200 m depth) west of the Crimean Peninsula indicate an <span class="hlt">active</span> sea-floor hydrothermal system. Subaerial mud <span class="hlt">volcanoes</span> on the Kerch and Taman Peninsulas (˜100 km north of the abyssal mud <span class="hlt">volcanoes</span>) contain saline thermal waters that locally have very high B contents (to 915 mg/L). These data suggest that tourmalinites might be forming in or near <span class="hlt">submarine</span> Black Sea mud <span class="hlt">volcanoes</span>, where potential may also exist for Sullivan-type Pb-Zn mineralization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020337','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020337"><span>Boron-rich mud <span class="hlt">volcanoes</span> of the Black Sea region: modern analogues to ancient sea-floor tourmalinites associated with Sullivan-type Pb-Zn 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>Slack, J.F.; Turner, R.J.W.; Ware, P.L.G.</p> <p>1998-01-01</p> <p>Large <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span> in the abyssal part of the Black Sea south of the Crimean Peninsula are similar in many respects to synsedimentary mud <span class="hlt">volcanoes</span> in the Mesoproterozoic Belt-Purcell basin. One of the Belt-Purcell mud <span class="hlt">volcanoes</span> directly underlies the giant Sullivan Pb-Zn-Ag deposit in southeastern British Columbia. Footwall rocks to the Sullivan deposit comprise variably tourmalinized siltstone, conglomerate, and related fragmental rock; local thin pyrrhotite-rich and spessartine-quartz beds are interpreted as Fe and Fe-Mn exhalites, respectively. Analogous Fe- and Mn-rich sediments occur near the abyssal Black Sea mud <span class="hlt">volcanoes</span>. Massive pyrite crusts and associated carbonate chimneys discovered in relatively shallow waters (~200 m depth) west of the Crimean Peninsula indicate an <span class="hlt">active</span> sea-floor-hydrothermal system. Subaerial mud <span class="hlt">volcanoes</span> on the Kerch and Taman Peninsulas (~100 km north of the abyssal mud <span class="hlt">volcanoes</span>) contain saline thermal waters that locally have very high B contents (to 915 mg/L). These data suggest that tourmalinites might be forming in or near <span class="hlt">submarine</span> Black Sea mud <span class="hlt">volcanoes</span>, where potential may also exist for Sullivan-type Pb-Zn mineralization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CoMP..173...40K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CoMP..173...40K"><span>Constraints on the source of Cu in a <span class="hlt">submarine</span> magmatic-hydrothermal system, Brothers <span class="hlt">volcano</span>, Kermadec island arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Keith, Manuel; Haase, Karsten M.; Klemd, Reiner; Smith, Daniel J.; Schwarz-Schampera, Ulrich; Bach, Wolfgang</p> <p>2018-05-01</p> <p>Most magmatic-hydrothermal Cu deposits are genetically linked to arc magmas. However, most continental or oceanic arc magmas are barren, and hence new methods have to be developed to distinguish between barren and mineralised arc systems. Source composition, melting conditions, the timing of S saturation and an initial chalcophile element-enrichment represent important parameters that control the potential of a subduction setting to host an economically valuable deposit. Brothers <span class="hlt">volcano</span> in the Kermadec island arc is one of the best-studied examples of arc-related <span class="hlt">submarine</span> magmatic-hydrothermal <span class="hlt">activity</span>. This study, for the first time, compares the chemical and mineralogical composition of the Brothers seafloor massive sulphides and the associated dacitic to rhyolitic lavas that host the hydrothermal system. Incompatible trace element ratios, such as La/Sm and Ce/Pb, indicate that the basaltic melts from L'Esperance <span class="hlt">volcano</span> may represent a parental analogue to the more evolved Brothers lavas. Copper-rich magmatic sulphides (Cu > 2 wt%) identified in fresh volcanic glass and phenocryst phases, such as clinopyroxene, plagioclase and Fe-Ti oxide suggest that the surrounding lavas that host the Brothers hydrothermal system represent a potential Cu source for the sulphide ores at the seafloor. Thermodynamic calculations reveal that the Brothers melts reached volatile saturation during their evolution. Melt inclusion data and the occurrence of sulphides along vesicle margins indicate that an exsolving volatile phase extracted Cu from the silicate melt and probably contributed it to the overlying hydrothermal system. Hence, the formation of the Cu-rich seafloor massive sulphides (up to 35.6 wt%) is probably due to the contribution of Cu from a bimodal source including wall rock leaching and magmatic degassing, in a mineralisation style that is hybrid between Cyprus-type volcanic-hosted massive sulphide and subaerial epithermal-porphyry deposits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940029486','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940029486"><span>Mount Rainier <span class="hlt">active</span> cascade <span class="hlt">volcano</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1994-01-01</p> <p>Mount Rainier is one of about two dozen <span class="hlt">active</span> or recently <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Cascade Range, an arc of <span class="hlt">volcanoes</span> in the northwestern United States and Canada. The <span class="hlt">volcano</span> is located about 35 kilometers southeast of the Seattle-Tacoma metropolitan area, which has a population of more than 2.5 million. This metropolitan area is the high technology industrial center of the Pacific Northwest and one of the commercial aircraft manufacturing centers of the United States. The rivers draining the <span class="hlt">volcano</span> empty into Puget Sound, which has two major shipping ports, and into the Columbia River, a major shipping lane and home to approximately a million people in southwestern Washington and northwestern Oregon. Mount Rainier is an <span class="hlt">active</span> <span class="hlt">volcano</span>. It last erupted approximately 150 years ago, and numerous large floods and debris flows have been generated on its slopes during this century. More than 100,000 people live on the extensive mudflow deposits that have filled the rivers and valleys draining the <span class="hlt">volcano</span> during the past 10,000 years. A major volcanic eruption or debris flow could kill thousands of residents and cripple the economy of the Pacific Northwest. Despite the potential for such danger, Mount Rainier has received little study. Most of the geologic work on Mount Rainier was done more than two decades ago. Fundamental topics such as the development, history, and stability of the <span class="hlt">volcano</span> are poorly understood.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T53A4659H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T53A4659H"><span>The preliminary results of new <span class="hlt">submarine</span> caldera on the west of Kume-jima island, Central Ryukyu Arc, Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harigane, Y.; Ishizuka, O.; Shimoda, G.; Sato, T.</p> <p>2014-12-01</p> <p>The Ryukyu Arc occurs between the islands of Kyushu and Taiwan with approximately 1200 km in the full length. This volcanic arc is caused by subduction of the Philippine Sea plate beneath the Eurasia Plate along the Ryukyu trench, and is composed of forearc islands, chains of arc <span class="hlt">volcanoes</span>, and a back-arc rift called Okinawa Trough. The Ryukyu Arc is commonly divided into three segments (northern, central and southern) that bounded by the Tokara Strait and the Kerama Gap, respectively (e.g., Konishi 1965; Kato et al., 1982). Sato et al. (2014) mentioned that there is no <span class="hlt">active</span> subaerial <span class="hlt">volcano</span> in the southwest of Iotori-shima in the Central Ryukyu Arc whereas the Northern Ryukyu Arc (i.e., the Tokara Islands) has <span class="hlt">active</span> frontal arc <span class="hlt">volcanoes</span>. Therefore, the existence of <span class="hlt">volcanoes</span> and volcanotectonic history of <span class="hlt">active</span> volcanic front in the southwestern part of the Central Ryukyu Arc are still ambiguous. Detailed geophysical and geological survey was mainly conducted using R/V Kaiyou-maru No.7 during GK12 cruise operated by the Geological Survey of Japan/National Institute of Advanced Industrial Science and Technology, Japan. As a result, we have found a new <span class="hlt">submarine</span> volcanic caldera on the west of Kume-jima island, where located the southwestern part of Central Ryukyu Arc. Here, we present (1) the bathymetrical feature of this new <span class="hlt">submarine</span> caldera for the first time and (2) the microstructural and petrological observations of volcanic rocks (20 volcanic samples in 13 dredge sites) sampled from the small volcanic cones of this caldera <span class="hlt">volcano</span>. The dredged samples from the caldera consist of mainly rhyolite pumice with minor andesites, Mn oxides-crust and hydrothermally altered rocks. Andesite has plagioclase, olivine and pyroxene phenocrysts. Key words: volcanic rock, caldera, arc volcanism, <span class="hlt">active</span> volcanic front, Kume-jima island, Ryukyu Arc</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V23B0608N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V23B0608N"><span>Liquid and Emulsified Sulfur in <span class="hlt">Submarine</span> Solfatara Fields of two Northern Mariana Arc <span class="hlt">Volcanoes</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nakamura, K.; Embley, R. W.; Chadwick, W. W.; Butterfield, D. A.; Takano, B.; Resing, J. A.; de Ronde, C. E.; Lilley, M. D.; Lupton, J. E.; Merle, S. G.; Inagaki, F.</p> <p>2006-12-01</p> <p>Because elemental sulfur melting point is ca 100 deg C (depend on allotropes and heating rate, S8 triple point temperature: 115 deg C), the evidence of liquid sulfur has been known for many subaerial crater lakes and small ponds in geothermal regions throughout the world. But the milky nature of water (sulfur-in- water emulsion in limited water mass) prohibited the direct observation of on-going processes at the bottom of these subaerial lakes. In the passive degassing environment at the summit craters of Daikoku and Nikko Seamounts of the northern Mariana Arc, the continuous flushing of sulfur emulsion by seawater allowed us to observe on- going <span class="hlt">submarine</span> solfatara processes and associated chemistry through dives with ROVs during the NT05-18 cruise (JAMSTEC R/V Natsushima and ROV hyper-Dolphin) and the <span class="hlt">Submarine</span> Ring of Fire 2006 cruise (R/V Melville and ROV JASON II). A higher viscosity for liquid elemental sulfur relative to that of seawater, as well as a limited stability of sulfur emulsion (aqueous sulfur sol) at high temperatures in electrolyte solution (seawater), ensures limited mobility of liquid sulfur in the conduits of hydrothermal vents. The subseafloor boiling depth of hydrothermal fluid limits the locus of any liquid sulfur reservoir. It was observed in an exposed liquid sulfur pond that the penetration of gas bubbles (mostly CO2) created sulfur emulsion while collapsing liquid sulfur film between seawater and gas bubbles. Liquid sulfur pits, encrusted sulfur, liquid sulfur fountain structure, sulfur stalactites and stalagmites, mini-pillow lava-like sulfur flows, accretionary sulfur lapilli and sulfur deltas were also observed at the summits of two <span class="hlt">volcanoes</span>. Note: Solfatara: Italian. A type of fumarole, the gases of which are characteristically sulfurous. In 'Glossary of geology.'</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BVol...79....5D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BVol...79....5D"><span>Flank instability assessment at Kick-'em-Jenny <span class="hlt">submarine</span> <span class="hlt">volcano</span> (Grenada, Lesser Antilles): a multidisciplinary approach using experiments and modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dondin, F. J.-Y.; Heap, M. J.; Robertson, R. E. A.; Dorville, J.-F. M.; Carey, S.</p> <p>2017-01-01</p> <p>Kick-'em-Jenny (KeJ)—located ca. 8 km north of the island of Grenada—is the only <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> of the Lesser Antilles Volcanic Arc. Previous investigations of KeJ revealed that it lies within a collapse scar inherited from a past flank instability episode. To assess the likelihood of future collapse, we employ here a combined laboratory and modeling approach. Lavas collected using a remotely operated vehicle (ROV) provided samples to perform the first rock physical property measurements for the materials comprising the KeJ edifice. Uniaxial and triaxial deformation experiments showed that the dominant failure mode within the edifice host rock is brittle. Edifice fractures (such as those at Champagne Vent) will therefore assist the outgassing of the nearby magma-filled conduit, favoring effusive behavior. These laboratory data were then used as input parameters in models of slope stability. First, relative slope stability analysis revealed that the SW to N sector of the <span class="hlt">volcano</span> displays a deficit of mass/volume with respect to a volcanoid (ideal 3D surface). Slope stability analysis using a limit equilibrium method (LEM) showed that KeJ is currently stable, since all values of stability factor or factor of safety (Fs) are greater than unity. The lowest values of Fs were found for the SW-NW sector of the <span class="hlt">volcano</span> (the sector displaying a mass/volume deficit). Although currently stable, KeJ may become unstable in the future. Instability (severe reductions in Fs) could result, for example, from overpressurization due to the growth of a cryptodome. Our modeling has shown that instability-induced flank collapse will most likely initiate from the SW-NW sector of KeJ, therefore mobilizing a volume of at least ca. 0.7 km3. The mobilization of ca. 0.7 km3 of material is certainly capable of generating a tsunami that poses a significant hazard to the southern islands of the West Indies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70009840','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70009840"><span><span class="hlt">Submarine</span> basalt from the Revillagigedo Islands region, 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>Moore, J.G.</p> <p>1970-01-01</p> <p>Ocean-floor dredging and <span class="hlt">submarine</span> photography in the Revillagigedo region off the west coast of Mexico reveal that the dominant exposed rock of the <span class="hlt">submarine</span> part of the large island-forming <span class="hlt">volcanoes</span> (Roca Partida and San Benedicto) is a uniform alkali pillow basalt; more siliceous rocks are exposed on the upper, subaerial parts of the <span class="hlt">volcanoes</span>. Basalts dredged from smaller seamounts along the Clarion fracture zone south of the Revillagigedo Islands are tholeiitic pillow basalts. Pillows of alkali basalts are more vesicular than Hawaiian tholeiitic pillows collected from the same depths. This difference probably reflects a higher original volatile content of the alkali basalts. Manganese-iron oxide nodules common in several dredge hauls generally contain nucleii of rhyolitic pumice or basalt pillow fragments. The pumice floated to its present site from subaerial eruptions, became waterlogged and sank, and was then coated with manganese-iron oxides. The thickness of palagonite rinds on the glassy pillow fragments is proportional to the thickness of manganese-iron oxide layers, and both are a measure of the age of the nodule. Both oldest basalts (10-100 m.y.) and youngest (less than 1 m.y.) are along the Clarion fracture zone, whereas basalts from Roca Partida and San Benedicto <span class="hlt">volcanoes</span> are of intermediate age. ?? 1970.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS34A..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS34A..07C"><span>Repeat AUV Mapping and ROV Observations of <span class="hlt">Active</span> Mud <span class="hlt">Volcanos</span> on the Canadian Beaufort Sea Continental Slope</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caress, D. W.; Paull, C. K.; Dallimore, S.; Lundsten, E. M.; Anderson, K.; Gwiazda, R.; Melling, H.; Lundsten, L.; Graves, D.; Thomas, H. J.; Cote, M.</p> <p>2017-12-01</p> <p>Two <span class="hlt">active</span> <span class="hlt">submarine</span> mud <span class="hlt">volcano</span> sites located at 420 and 740 m depths on the margin of the Canadian Beaufort Sea were mapped in 2013 and again in 2016 using the same survey line pattern allowing detection of change over three years. The surveys were conducted using MBARI's mapping AUVs which fields a 200 kHz or 400 kHz multibeam sonar, a 1-6 kHz chirp sub-bottom profiler, and a 110 kHz chirp sidescan from a 50 m altitude. The resulting bathymetry has 1 m lateral resolution and 0.1 m vertical precision and sidescan mosaics have 1 m lateral resolution. Vertical changes of ≥0.2 m are observable by differencing repeat surveys. These features were also visited with MBARI's miniROV, which was outfitted for these dives with a manipulator mounted temperature probe. The 420 m mud <span class="hlt">volcano</span> is nearly circular, 1100 m across, flat-topped, and superimposed on the pre-existing smooth slope. The central plateau has low relief <3 m consisting of concentric rings and ovoid mounds that appear to reflect distinct eruptions at shifting locations. The 740 m site contains 3 mud <span class="hlt">volcanoes</span>, most prominently a 630 m wide, 30 m high flat-topped plateau with about 4 m of relief similar to the 420 m feature plus a 5 m high cone on the southern rim. North of this plateau is a smooth-textured conically shaped feature also standing about 30 m above the floor of the subsidence structure. Sidescan mosaics reveal significant changes in backscatter patterns at both mud <span class="hlt">volcano</span> sites between surveys. Comparison of bathymetry also reveals new flows of up to 1.8 m thickness at both sites, as well as subtle spreading of the flat plateaus rims. An <span class="hlt">active</span> mudflow was encountered during a miniROV dive on a high backscatter target at the 740 m site. This tongue of mud was observed to be slowly flowing downslope. The ROV temperature probe inserted 2 cm into the flow measured 23°C, compared to ambient water (-0.4°C), indicating the rapid ascent of the mud from considerable subsurface depths. Bubbles</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS31D2054J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS31D2054J"><span>Hydrothermal Rock-Fluid Interactions in 15-year-old <span class="hlt">Submarine</span> Basaltic Tuff at Surtsey <span class="hlt">Volcano</span>, Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jackson, M. D.; Couper, S.; Li, Y.; Stan, C. V.; Tamura, N.; Stefansson, A.; Moore, J. G.; Wenk, H. R.</p> <p>2016-12-01</p> <p>Basaltic tephra at Surtsey <span class="hlt">volcano</span>, produced by 1963-1967 eruptions in the offshore SE Icelandic rift zone, record the complex interplay of factors that determine rates of palagonitization and crystallization of authigenic minerals in seafloor basalts worldwide. We investigate how formation of nanocrystalline clay mineral in fresh sideromelane glass influenced crystallization of mineral cements in <span class="hlt">submarine</span> tuff from a 181 m core drilled in 1979. Synchrotron-based microdiffraction and microfluorescence maps (2x5 µm X-ray beam spot size) at beamline 12.3.2, Advanced Light Source, SEM-EDS compositional analyses, and fluid geochemical models compare processes in lapilli-sized glass fragments, vitric cementing matrix, and fine ash accretions. In lapilli at 137.9 m (100°C), nanocrystalline clay mineral in gel-palagonite has asymetric 14.9-12.6 Å (001) reflections, with Fe and Ti enrichment relative to Si, Al and Ca, compared with adjacent sideromelane. Neighboring fibro-palagonite has symmetric (001) and greater Fe and Ti enrichment. Al-tobermorite, a rare calcium-silicate-hydrate, crystallized in nearby vesicles. The 11.30-11.49 Å (002) interlayer and Ca/(Si+Al) ratio of 0.9-1.0 record release of Si, Al, and Ca in a chemical system relatively isolated from <span class="hlt">submarine</span> hydrothermal fluid flow. In vitric matrix relatively open to fluid flow, however, phillipsite zeolite cement predominates. Al-tobermorite formed at 88.45 m (130°C) and 102.6 m (140°C), but is associated with fibro-palagonite and analcite, reflecting more rapid palagonitization, and changing cation solubility and pH at higher temperature. Tubular palagonite microstructures show nanocrystalline clay mineral with (001) preferred orientations that wrap around relict microchannels, produced perhaps through biogenic <span class="hlt">activity</span>. Nanocrystalline clay mineral d-spacings suggest similarities with nontronite, but zeolite in palagonite diffraction patterns and 6-9 wt% MgO suggest a polycrystalline composite with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28676800','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28676800"><span>Atribacteria from the Subseafloor Sedimentary Biosphere Disperse to the Hydrosphere through <span class="hlt">Submarine</span> Mud <span class="hlt">Volcanoes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hoshino, Tatsuhiko; Toki, Tomohiro; Ijiri, Akira; Morono, Yuki; Machiyama, Hideaki; Ashi, Juichiro; Okamura, Kei; Inagaki, Fumio</p> <p>2017-01-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> (SMVs) are formed by muddy sediments and breccias extruded to the seafloor from a source in the deep subseafloor and are characterized by the discharge of methane and other hydrocarbon gasses and deep-sourced fluids into the overlying seawater. Although SMVs act as a natural pipeline connecting the Earth's surface and subsurface biospheres, the dispersal of deep-biosphere microorganisms and their ecological roles remain largely unknown. In this study, we investigated the microbial communities in sediment and overlying seawater at two SMVs located on the Ryukyu Trench off Tanegashima Island, southern Japan. The microbial communities in mud <span class="hlt">volcano</span> sediments were generally distinct from those in the overlying seawaters and in the well-stratified Pacific margin sediments collected at the Peru Margin, the Juan de Fuca Ridge flank off Oregon, and offshore of Shimokita Peninsula, northeastern Japan. Nevertheless, in-depth analysis of different taxonomic groups at the sub-species level revealed that the taxon affiliated with Atribacteria , heterotrophic anaerobic bacteria that typically occur in organic-rich anoxic subseafloor sediments, were commonly found not only in SMV sediments but also in the overlying seawater. We designed a new oligonucleotide probe for detecting Atribacteria using the catalyzed reporter deposition-fluorescence in situ hybridization (CARD-FISH). CARD-FISH, digital PCR and sequencing analysis of 16S rRNA genes consistently showed that Atribacteria are abundant in the methane plumes of the two SMVs (0.58 and 1.5 × 10 4 cells/mL, respectively) but not in surrounding waters, suggesting that microbial cells in subseafloor sediments are dispersed as "deep-biosphere seeds" into the ocean. These findings may have important implications for the microbial transmigration between the deep subseafloor biosphere and the hydrosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5476839','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5476839"><span>Atribacteria from the Subseafloor Sedimentary Biosphere Disperse to the Hydrosphere through <span class="hlt">Submarine</span> Mud <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hoshino, Tatsuhiko; Toki, Tomohiro; Ijiri, Akira; Morono, Yuki; Machiyama, Hideaki; Ashi, Juichiro; Okamura, Kei; Inagaki, Fumio</p> <p>2017-01-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> (SMVs) are formed by muddy sediments and breccias extruded to the seafloor from a source in the deep subseafloor and are characterized by the discharge of methane and other hydrocarbon gasses and deep-sourced fluids into the overlying seawater. Although SMVs act as a natural pipeline connecting the Earth’s surface and subsurface biospheres, the dispersal of deep-biosphere microorganisms and their ecological roles remain largely unknown. In this study, we investigated the microbial communities in sediment and overlying seawater at two SMVs located on the Ryukyu Trench off Tanegashima Island, southern Japan. The microbial communities in mud <span class="hlt">volcano</span> sediments were generally distinct from those in the overlying seawaters and in the well-stratified Pacific margin sediments collected at the Peru Margin, the Juan de Fuca Ridge flank off Oregon, and offshore of Shimokita Peninsula, northeastern Japan. Nevertheless, in-depth analysis of different taxonomic groups at the sub-species level revealed that the taxon affiliated with Atribacteria, heterotrophic anaerobic bacteria that typically occur in organic-rich anoxic subseafloor sediments, were commonly found not only in SMV sediments but also in the overlying seawater. We designed a new oligonucleotide probe for detecting Atribacteria using the catalyzed reporter deposition-fluorescence in situ hybridization (CARD-FISH). CARD-FISH, digital PCR and sequencing analysis of 16S rRNA genes consistently showed that Atribacteria are abundant in the methane plumes of the two SMVs (0.58 and 1.5 × 104 cells/mL, respectively) but not in surrounding waters, suggesting that microbial cells in subseafloor sediments are dispersed as “deep-biosphere seeds” into the ocean. These findings may have important implications for the microbial transmigration between the deep subseafloor biosphere and the hydrosphere. PMID:28676800</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA18245.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA18245.html"><span>Ubinas <span class="hlt">Volcano</span> <span class="hlt">Activity</span> in Peruvian Andes</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2014-05-01</p> <p>On April 28, 2014, NASA Terra spacecraft spotted signs of <span class="hlt">activity</span> at Ubinas <span class="hlt">volcano</span> in the Peruvian Andes. The appearance of a new lava dome in March 2014 and frequent ash emissions are signs of increasing <span class="hlt">activity</span> at this <span class="hlt">volcano</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024561','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024561"><span>The proximal part of the giant <span class="hlt">submarine</span> Wailau landslide, Molokai, 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>Clague, D.A.; Moore, J.G.</p> <p>2002-01-01</p> <p>The main break-in-slope on the northern <span class="hlt">submarine</span> flank of Molokai at -1500 to -1250 m is a shoreline feature that has been only modestly modified by the Wailau landslide. <span class="hlt">Submarine</span> canyons above the break-in-slope, including one meandering stream, were subaerially carved. Where such canyons cross the break-in-slope, plunge pools may form by erosion from bedload sediment carried down the canyons. West Molokai <span class="hlt">Volcano</span> continued infrequent volcanic <span class="hlt">activity</span> that formed a series of small coastal sea cliffs, now submerged, as the island subsided. Lavas exposed at the break-in-slope are subaerially erupted and emplaced tholeiitic shield lavas. <span class="hlt">Submarine</span> rejuvenated-stage volcanic cones formed after the landslide took place and following at least 400-500 m of subsidence after the main break-in-slope had formed. The sea cliff on east Molokai is not the headwall of the landslide, nor did it form entirely by erosion. It may mark the location of a listric fault similar to the Hilina faults on present-day Kilauea <span class="hlt">Volcano</span>. The Wailau landslide occurred about 1.5 Ma and the Kalaupapa Peninsula most likely formed 330??5 ka. Molokai is presently stable relative to sea level and has subsided no more than 30 m in the last 330 ka. At their peak, West and East Molokai stood 1.6 and 3 km above sea level. High rainfall causes high surface runoff and formation of canyons, and increases groundwater pressure that during dike intrusions may lead to flank failure. <span class="hlt">Active</span> shield or postshield volcanism (with dikes injected along rift zones) and high rainfall appear to be two components needed to trigger the deep-seated giant Hawaiian landslides. ?? 2002 Elsevier Science B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025521','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025521"><span>Ups and downs on spreading flanks of ocean-island <span class="hlt">volcanoes</span>: evidence from Mauna Loa and Kīlauea</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lipman, Peter W.; Eakins, Barry W.; Yokose, Hisayoshi</p> <p>2003-01-01</p> <p><span class="hlt">Submarine</span>-flank deposits of Hawaiian <span class="hlt">volcanoes</span> are widely recognized to have formed largely by gravitationally driven <span class="hlt">volcano</span> spreading and associated landsliding. Observations from submersibles show that prominent benches at middepths on flanks of Mauna Loa and Kilauea consist of volcaniclastic debris derived by landsliding from nearby shallow <span class="hlt">submarine</span> and subaerial flanks of the same edifice. Massive slide breccias from the mature subaerial tholeiitic shield of Mauna Loa underlie the frontal scarp of its South Kona bench. In contrast, coarse volcaniclastic sediments derived largely from <span class="hlt">submarine</span>-erupted preshield alkalic and transitional basalts of ancestral Kilauea underlie its Hilina bench. Both midslope benches record the same general processes of slope failure, followed by modest compression during continued <span class="hlt">volcano</span> spreading, even though they record development during different stages of edifice growth. The dive results suggest that volcaniclastic rocks at the north end of the Kona bench, interpreted by others as distal sediments from older <span class="hlt">volcanoes</span> that were offscraped, uplifted, and accreted to the island by far-traveled thrusts, alternatively are a largely coherent stratigraphic assemblage deposited in a basin behind the South Kona bench.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17225386','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17225386"><span>Acoustic scattering from mud <span class="hlt">volcanoes</span> and carbonate mounds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Holland, Charles W; Weber, Thomas C; Etiope, Giuseppe</p> <p>2006-12-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> occur in many parts of the world's oceans and form an aperture for gas and fluidized mud emission from within the earth's crust. Their characteristics are of considerable interest to the geology, geophysics, geochemistry, and underwater acoustics communities. For the latter, mud <span class="hlt">volcanoes</span> are of interest in part because they pose a potential source of clutter for <span class="hlt">active</span> sonar. Close-range (single-interaction) scattering measurements from a mud <span class="hlt">volcano</span> in the Straits of Sicily show scattering 10-15 dB above the background. Three hypotheses were examined concerning the scattering mechanism: (1) gas entrained in sediment at/near mud <span class="hlt">volcano</span>, (2) gas bubbles and/or particulates (emitted) in the water column, (3) the carbonate bio-construction covering the mud <span class="hlt">volcano</span> edifice. The experimental evidence, including visual, acoustic, and nonacoustic sensors, rules out the second hypothesis (at least during the observation time) and suggests that, for this particular mud <span class="hlt">volcano</span> the dominant mechanism is associated with carbonate chimneys on the mud <span class="hlt">volcano</span>. In terms of scattering levels, target strengths of 4-14 dB were observed from 800 to 3600 Hz for a monostatic geometry with grazing angles of 3-5 degrees. Similar target strengths were measured for vertically bistatic paths with incident and scattered grazing angles of 3-5 degrees and 33-50 degrees, respectively.</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('http://hdl.handle.net/2060/20100033209','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100033209"><span>Mud <span class="hlt">Volcanoes</span> - Analogs to Martian Cones and Domes (by the Thousands!)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Allen, Carlton C.; Oehler, Dorothy</p> <p>2010-01-01</p> <p>Mud <span class="hlt">volcanoes</span> are mounds formed by low temperature slurries of gas, liquid, sediments and rock that erupt to the surface from depths of meters to kilometers. They are common on Earth, with estimates of thousands onshore and tens of thousands offshore. Mud <span class="hlt">volcanoes</span> occur in basins with rapidly-deposited accumulations of fine-grained sediments. Such settings are ideal for concentration and preservation of organic materials, and mud <span class="hlt">volcanoes</span> typically occur in sedimentary basins that are rich in organic biosignatures. Domes and cones, cited as possible mud <span class="hlt">volcanoes</span> by previous authors, are common on the northern plains of Mars. Our analysis of selected regions in southern Acidalia Planitia has revealed over 18,000 such features, and we estimate that more than 40,000 occur across the area. These domes and cones strongly resemble terrestrial mud <span class="hlt">volcanoes</span> in size, shape, morphology, associated flow structures and geologic setting. Geologic and mineralogic arguments rule out alternative formation mechanisms involving lava, ice and impacts. We are studying terrestrial mud <span class="hlt">volcanoes</span> from onshore and <span class="hlt">submarine</span> locations. The largest concentration of onshore features is in Azerbaijan, near the western edge of the Caspian Sea. These features are typically hundreds of meters to several kilometers in diameter, and tens to hundreds of meters in height. Satellite images show spatial densities of 20 to 40 eruptive centers per 1000 square km. Many of the features remain <span class="hlt">active</span>, and fresh mud flows as long as several kilometers are common. A large field of <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span> is located in the Gulf of Cadiz, off the Atlantic coasts of Morocco and Spain. High-resolution sonar bathymetry reveals numerous km-scale mud <span class="hlt">volcanoes</span>, hundreds of meters in height. Seismic profiles demonstrate that the mud erupts from depths of several hundred meters. These <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span> are the closest morphologic analogs yet found to the features in Acidalia Planitia. We are also conducting</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991E%26PSL.107..318C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991E%26PSL.107..318C"><span>Gas-rich <span class="hlt">submarine</span> exhalations during the 1989 eruption of Macdonald Seamount</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>C´e, J.-L.; Stoffers, P.; McMurtry, G.; Richnow, H.; Puteanus, D.; Sedwick, P.</p> <p>1991-11-01</p> <p>In January 1989 we observed <span class="hlt">submarine</span> eruptions on the summit of Macdonald <span class="hlt">volcano</span> during a French-German diving programme with the IFREMER submersible Cyana. Gas-streaming of large amounts of CH 4, CO 2 and SO 2 from summit vents, inferred from water column anomalies and observed by submersible, was accompanied on the sea surface by steam bursts, turbulence, red-glowing gases, and black bubbles comprising volcanic ash, sulphur and sulphides. Chloride depletion of water sampled on the floor of an <span class="hlt">actively</span> degassing summit crater suggests either boiling and phase separation or additions of magmatic water vapour. Submersible observations, in-situ sampling and shipboard geophysical and hydrographic measurements show that the hydrothermal system of this hotspot <span class="hlt">volcano</span> is distinguished by the influence of magmatic gases released from its shallow summit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GGG....17.1000C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GGG....17.1000C"><span>Hydrothermal venting and mineralization in the crater of Kick'em Jenny <span class="hlt">submarine</span> <span class="hlt">volcano</span>, Grenada (Lesser Antilles)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carey, Steven; Olsen, Rene; Bell, Katherine L. C.; Ballard, Robert; Dondin, Frederic; Roman, Chris; Smart, Clara; Lilley, Marvin; Lupton, John; Seibel, Brad; Cornell, Winton; Moyer, Craig</p> <p>2016-03-01</p> <p>Kick'em Jenny is a frequently erupting, shallow <span class="hlt">submarine</span> <span class="hlt">volcano</span> located 7.5 km off the northern coast of Grenada in the Lesser Antilles subduction zone. Focused and diffuse hydrothermal venting is taking place mainly within a small (˜70 × 110 m) depression within the 300 m diameter crater of the <span class="hlt">volcano</span> at depths of about 265 m. Much of the crater is blanketed with a layer of fine-grained tephra that has undergone hydrothermal alteration. Clear fluids and gas are being discharged near the center of the depression from mound-like vents at a maximum temperature of 180°C. The gas consists of 93-96% CO2 with trace amounts of methane and hydrogen. Gas flux measurements of individual bubble streams range from 10 to 100 kg of CO2 per day. Diffuse venting with temperatures 5-35°C above ambient occurs throughout the depression and over large areas of the main crater. These zones are colonized by reddish-yellow bacteria with the production of Fe-oxyhydroxides as surface coatings, fragile spires up to several meters in height, and elongated mounds up to tens of centimeters thick. A high-resolution photomosaic of the inner crater depression shows fluid flow patterns descending the sides of the depression toward the crater floor. We suggest that the negatively buoyant fluid flow is the result of phase separation of hydrothermal fluids at Kick'em Jenny generating a dense saline component that does not rise despite its elevated temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016446','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016446"><span>Large landslides from oceanic <span class="hlt">volcanoes</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>Holcomb, R.T.; Searle, R.C.</p> <p>1991-01-01</p> <p>Large landslides are ubiquitous around the <span class="hlt">submarine</span> flanks of Hawaiian <span class="hlt">volcanoes</span>, and GLORIA has also revealed large landslides offshore from Tristan da Cunha and El Hierro. On both of the latter islands, steep flanks formerly attributed to tilting or marine erosion have been reinterpreted as landslide headwalls mantled by younger lava flows. These landslides occur in a wide range of settings and probably represent only a small sample from a large population. They may explain the large volumes of archipelagic aprons and the stellate shapes of many oceanic <span class="hlt">volcanoes</span>. Large landslides and associated tsunamis pose hazards to many islands. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003JAESc..21..515W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003JAESc..21..515W"><span>Three <span class="hlt">active</span> <span class="hlt">volcanoes</span> in China and their hazards</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wei, H.; Sparks, R. S. J.; Liu, R.; Fan, Q.; Wang, Y.; Hong, H.; Zhang, H.; Chen, H.; Jiang, C.; Dong, J.; Zheng, Y.; Pan, Y.</p> <p>2003-02-01</p> <p>The <span class="hlt">active</span> <span class="hlt">volcanoes</span> in China are located in the Changbaishan area, Jingbo Lake, Wudalianchi, Tengchong and Yutian. Several of these <span class="hlt">volcanoes</span> have historical records of eruption and geochronological evidence of Holocene <span class="hlt">activity</span>. Tianchi <span class="hlt">Volcano</span> is a well-preserved Cenozoic polygenetic central <span class="hlt">volcano</span>, and, due to its recent history of powerful explosive eruptions of felsic magmas, with over 100,000 people living on its flanks is a high-risk <span class="hlt">volcano</span>. Explosive eruptions at 4000 and 1000 years BP involved plinian and ignimbrite phases. The Millennium eruption (1000 years BP) involved at least 20-30 km 3 of magma and was large enough to have a global impact. There are 14 Cenozoic monogenetic scoria cones and associated lavas with high-K basalt composition in the Wudalianchi volcanic field. The Laoheishan and Huoshaoshan cones and related lavas were formed in 1720-1721 and 1776 AD. There are three Holocene <span class="hlt">volcanoes</span>, Dayingshan, Maanshan, and Heikongshan, among the 68 Quaternary <span class="hlt">volcanoes</span> in the Tengchong volcanic province. Three of these <span class="hlt">volcanoes</span> are identified as <span class="hlt">active</span>, based on geothermal <span class="hlt">activity</span>, geophysical evidence for magma, and dating of young volcanic rocks. Future eruptions of these Chinese <span class="hlt">volcanoes</span> pose a significant threat to hundreds of thousands of people and are likely to cause substantial economic losses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70179216','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70179216"><span>The changing shapes of <span class="hlt">active</span> <span class="hlt">volcanoes</span>: History, evolution, and future challenges for <span class="hlt">volcano</span> geodesy</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.; Hamburger, Michael W.; Newman, Andrew V.</p> <p>2006-01-01</p> <p>At the very heart of volcanology lies the search for the 'plumbing systems' that form the inner workings of Earth’s <span class="hlt">active</span> <span class="hlt">volcanoes</span>. By their very nature, however, the magmatic reservoirs and conduits that underlie these <span class="hlt">active</span> volcanic systems are elusive; mostly they are observable only through circumstantial evidence, using indirect, and often ambiguous, surficial measurements. Of course, we can infer much about these systems from geologic investigation of materials brought to the surface by eruptions and of the exposed roots of ancient <span class="hlt">volcanoes</span>. But how can we study the magmatic processes that are occurring beneath Earth’s <span class="hlt">active</span> <span class="hlt">volcanoes</span>? What are the geometry, scale, physical, and chemical characteristics of magma reservoirs? Can we infer the dynamics of magma transport? Can we use this information to better forecast the future behavior of <span class="hlt">volcanoes</span>? These questions comprise some of the most fundamental, recurring themes of modern research in volcanology. The field of <span class="hlt">volcano</span> geodesy is uniquely situated to provide critical observational constraints on these problems. For the past decade, armed with a new array of technological innovations, equipped with powerful computers, and prepared with new analytical tools, <span class="hlt">volcano</span> geodesists have been poised to make significant advances in our fundamental understanding of the behavior of <span class="hlt">active</span> volcanic systems. The purpose of this volume is to highlight some of these recent advances, particularly in the collection and interpretation of geodetic data from <span class="hlt">actively</span> deforming <span class="hlt">volcanoes</span>. The 18 papers that follow report on new geodetic data that offer valuable insights into eruptive <span class="hlt">activity</span> and magma transport; they present new models and modeling strategies that have the potential to greatly increase understanding of magmatic, hydrothermal, and <span class="hlt">volcano</span>-tectonic processes; and they describe innovative techniques for collecting geodetic measurements from remote, poorly accessible, or hazardous <span class="hlt">volcanoes</span>. To provide</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PApGe.172.3189F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PApGe.172.3189F"><span>An Overview of Geodetic <span class="hlt">Volcano</span> Research in the Canary Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernández, José; González, Pablo J.; Camacho, Antonio G.; Prieto, Juan F.; Brú, Guadalupe</p> <p>2015-11-01</p> <p>The Canary Islands are mostly characterized by diffuse and scattered volcanism affecting a large area, with only one <span class="hlt">active</span> stratovolcano, the Teide-Pico Viejo complex (Tenerife). More than 2 million people live and work in the 7,447 km2 of the archipelago, resulting in an average population density three times greater than the rest of Spain. This fact, together with the growth of exposure during the past 40 years, increases volcanic risk with respect previous eruptions, as witnessed during the recent 2011-2012 El Hierro <span class="hlt">submarine</span> eruption. Therefore, in addition to purely scientific reasons there are economic and population-security reasons for developing and maintaining an efficient <span class="hlt">volcano</span> monitoring system. In this scenario geodetic monitoring represents an important part of the monitoring system. We describe <span class="hlt">volcano</span> geodetic monitoring research carried out in the Canary Islands and the results obtained. We consider for each epoch the two main existing constraints: the level of volcanic <span class="hlt">activity</span> in the archipelago, and the limitations of the techniques available at the time. Theoretical and observational aspects are considered, as well as the implications for operational <span class="hlt">volcano</span> surveillance. Current challenges of and future perspectives in geodetic <span class="hlt">volcano</span> monitoring in the Canaries are also presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995GMS....92..289K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995GMS....92..289K"><span>Isotopic evolution of Mauna Loa <span class="hlt">Volcano</span>: A view from the <span class="hlt">submarine</span> southwest rift zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kurz, Mark D.; Kenna, T. C.; Kammer, D. P.; Rhodes, J. Michael; Garcia, Michael O.</p> <p></p> <p>New isotopic and trace element measurements on lavas from the <span class="hlt">submarine</span> southwest rift zone (SWR) of Mauna Loa continue the temporal trends of subaerial Mauna Loa flows, extending the known compositional range for this <span class="hlt">volcano</span>, and suggesting that many of the SWR lavas are older than any exposed on land. He and Nd isotopic compositions are similar to those in the oldest subaerial Mauna Loa lavas (Kahuku and Ninole Basalts), while 87Sr/86Sr ratios are slightly lower (as low as .7036) and Pb isotopes are higher (206Pb'204Pb up to 18.30). The coherence of all the isotopes suggests that helium behaves as an incompatible element, and that helium isotopic variations in the Hawaiian lavas are produced by melting and mantle processes, rather than magma chamber or metasomatic processes unique to the gaseous elements. The variations of He, Sr, and Nd are most pronounced in lavas of approximately 10 ka age range [Kurz and Kammer, 1991], but the largest Pb isotopic variation occurs earlier. These variations are interpreted as resulting from the diminishing contribution from the upwelling mantle plume material as the shield building ends at Mauna Loa. The order of reduction in the plume isotopic signature is inferred to be Pb (at >100 ka), He (at ˜14 ka), Sr (at ˜9 ka), and Nd (at ˜8 ka); the different timing may relate to silicate/melt partition coefficients, with most incompatible elements removed first, and also to concentration variations within the plume. Zr/Nb, Sr/Nb, and fractionation-corrected Nb concentrations, correlate with the isotopes and are significantly higher in some of the <span class="hlt">submarine</span> SWR lavas, suggesting temporal variability on time scales similar to the Pb isotopes (i.e. ˜ 100 ka). Historical lavas define trace element and isotopic trends that are distinct from the longer term (10 to 100 ka) variations, suggesting that different processes cause the short term variability. The temporal evolution of Mauna Loa, and particularly the new data from the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023152','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023152"><span>Lava bubble-wall fragments formed by <span class="hlt">submarine</span> hydrovolcanic explosions on Lo'ihi Seamount and Kilauea <span class="hlt">Volcano</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>Clague, D.A.; Davis, A.S.; Bischoff, J.L.; Dixon, J.E.; Geyer, R.</p> <p>2000-01-01</p> <p>Glassy bubble-wall fragments, morphologically similar to littoral limu o Pele, have been found in volcanic sands erupted on Lo'ihi Seamount and along the <span class="hlt">submarine</span> east rift zone of Kilauea <span class="hlt">Volcano</span>. The limu o Pele fragments are undegassed with respect to H2O and S and formed by mild steam explosions. Angular glass sand fragments apparently form at similar, and greater, depths by cooling-contraction granulation. The limu o Pele fragments from Lo'ihi Seamount are dominantly tholeiitic basalt containing 6.25-7.25% MgO. None of the limu o Pele samples from Lo'ihi Seamount contains less than 5.57% MgO, suggesting that higher viscosity magmas do not form lava bubbles. The dissolved CO2 and H2O contents of 7 of the limu o Pele fragments indicate eruption at 1200??300 m depth (120??30 bar). These pressures exceed that generally thought to limit steam explosions. We conclude that hydrovolcanic eruptions are possible, with appropriate pre-mixing conditions, at pressures as great as 120 bar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.V21A2763E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.V21A2763E"><span>Experimental Insights on Natural Lava-Ice/Snow Interactions and Their Implications for Glaciovolcanic and <span class="hlt">Submarine</span> Eruptions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, B. R.; Karson, J.; Wysocki, R.; Lev, E.; Bindeman, I. N.; Kueppers, U.</p> <p>2012-12-01</p> <p>Lava-ice-snow interactions have recently gained global attention through the eruptions of ice-covered <span class="hlt">volcanoes</span>, particularly from Eyjafjallajokull in south-central Iceland, with dramatic effects on local communities and global air travel. However, as with most <span class="hlt">submarine</span> eruptions, direct observations of lava-ice/snow interactions are rare. Only a few hundred potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span> are presently ice-covered, these <span class="hlt">volcanoes</span> are generally in remote places, and their associated hazards make close observation and measurements dangerous. Here we report the results of the first large-scale experiments designed to provide new constraints on natural interactions between lava and ice/snow. The experiments comprised controlled effusion of tens of kilograms of melted basalt on top of ice/snow, and provide insights about observations from natural lava-ice-snow interactions including new constraints for: 1) rapid lava advance along the ice-lava interface; 2) rapid downwards melting of lava flows through ice; 3) lava flow exploitation of pre-existing discontinuities to travel laterally beneath and within ice; and 4) formation of abundant limu o Pele and non-explosive vapor transport from the base to the top of the lava flow with minor O isotope exchange. The experiments are consistent with observations from eruptions showing that lava is more efficient at melting ice when emplaced on top of the ice as opposed to beneath the ice, as well as the efficacy of tephra cover for slowing melting. The experimental extrusion rates are as within the range of those for <span class="hlt">submarine</span> eruptions as well, and reproduce some features seen in <span class="hlt">submarine</span> eruptions including voluminous production of gas rich cavities within initially anhydrous lavas and limu on lava surfaces. Our initial results raise questions about the possibility of secondary ingestion of water by <span class="hlt">submarine</span> and glaciovolcanic lava flows, and the origins of apparent primary gas cavities in those flows. Basaltic melt moving down</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS53C1712F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS53C1712F"><span>The <span class="hlt">submarine</span> <span class="hlt">volcano</span> eruption at the island of El Hierro: physical-chemical perturbation and biological response</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fraile-Nuez, E.; Santana-Casiano, J.; Gonzalez-Davila, M.</p> <p>2013-12-01</p> <p>On October 10 2011 an underwater eruption gave rise to a novel shallow <span class="hlt">submarine</span> <span class="hlt">volcano</span> south of the island of El Hierro, Canary Islands, Spain. During the eruption large quantities of mantle-derived gases, solutes and heat were released into the surrounding waters. In order to monitor the impact of the eruption on the marine ecosystem, periodic multidisciplinary cruises were carried out. Here, we present an initial report of the extreme physical-chemical perturbations caused by this event, comprising thermal changes, water acidification, deoxygenation and metal-enrichment, which resulted in significant alterations to the <span class="hlt">activity</span> and composition of local plankton communities. Our findings highlight the potential role of this eruptive process as a natural ecosystem-scale experiment for the study of extreme effects of global change stressors on marine environments. (A) Natural color composite from the MEdium Resolution Imaging Spectrometer (MERIS) instrument aboard ENVISAT Satellite (European Space Agency), (November 9, 2011 at 14:45 UTC). Remote sensing data have been used to monitor the evolution of the volcanic emissions, playing a fundamental role during field cruises in guiding the Spanish government oceanographic vessel to the appropriate sampling areas. The inset map shows the position of Canary Islands west of Africa and the study area (solid white box). (B) Location of the stations carried out from November 2011 to February 2012 at El Hierro. Black lines denote transects A-B and C-D.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.T13B2193W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.T13B2193W"><span>Transport of Fine Ash Through the Water Column at Erupting <span class="hlt">Volcanoes</span> - Monowai Cone, Kermadec-Tonga Arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walker, S. L.; Baker, E. T.; Leybourne, M. I.; de Ronde, C. E.; Greene, R.; Faure, K.; Chadwick, W.; Dziak, R. P.; Lupton, J. E.; Lebon, G.</p> <p>2010-12-01</p> <p>Monowai cone is a large, <span class="hlt">active</span>, basaltic stratovolcano, part of the <span class="hlt">submarine</span> Monowai volcanic center (MVC) located at ~26°S on the Kermadec-Tonga arc. At other <span class="hlt">actively</span> erupting <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>, magma extrusions and hydrothermal vents have been located only near the summit of the edifice, generating plumes enriched with hydrothermal components and magmatic gasses that disperse into the ocean environment at, or shallower than, the summit depth. Plumes found deeper than summit depths are dominated by fresh volcaniclastic ash particles, devoid of hydrothermal tracers, emplaced episodically by down-slope gravity flows, and transport fine ash to 10’s of km from the <span class="hlt">active</span> eruptions. A water column survey of the MVC in 2004 mapped intensely hydrothermal-magmatic plumes over the shallow (~130 m) summit of Monowai cone and widespread plumes around its flanks. Due to the more complex multiple parasitic cone and caldera structure of MVC, we analyzed the dissolved and particulate components of the flank plumes for evidence of additional sources. Although hydrothermal plumes exist within the adjacent caldera, none of the parasitic cones on Monowai cone or elsewhere within the MVC were hydrothermally or volcanically <span class="hlt">active</span>. The combination of an intensely enriched summit plume, sulfur particles and bubbles at the sea surface, and ash-dominated flank plumes indicate Monowai cone was <span class="hlt">actively</span> erupting at the time of the 2004 survey. Monowai cone is thus the fourth erupting <span class="hlt">submarine</span> <span class="hlt">volcano</span> we have encountered, and all have had deep ash plumes distributed around their flanks [the others are: Kavachi (Solomon Island arc), NW Rota-1 (Mariana arc) and W Mata (NE Lau basin)]. These deep ash plumes are a syneruptive phenomenon, but it is unknown how they are related to eruptive style and output, or to the cycles of construction and collapse that occur on the slopes of <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>. Repeat multibeam bathymetric surveys have documented two large-scale sector collapse</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GGG....19..356L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GGG....19..356L"><span>Mud Volcanism in a Canyon: Morphodynamic Evolution of the <span class="hlt">Active</span> Venere Mud <span class="hlt">Volcano</span> and Its Interplay With Squillace Canyon, Central Mediterranean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loher, Markus; Ceramicola, Silvia; Wintersteller, Paul; Meinecke, Gerrit; Sahling, Heiko; Bohrmann, Gerhard</p> <p>2018-02-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> develop through the extrusion of methane-rich fluids and sediments onto the seafloor. The morphology of a mud <span class="hlt">volcano</span> can record its extrusive history and processes of erosion and deformation affecting it. The study of offshore mud <span class="hlt">volcano</span> dynamics is limited because only few have been mapped at resolutions that reveal their detailed surface structures. More importantly, rates and volumes of extruded sediment and methane are poorly constrained. The 100 m high twin cones of Venere mud <span class="hlt">volcano</span> are situated at ˜1,600 m water depth within Squillace Canyon along the Ionian Calabrian margin, Mediterranean Sea. Seafloor bathymetry and backscatter data obtained by a ship-based system and an autonomous underwater vehicle (AUV) allow mapping of mudflow deposits of the mud <span class="hlt">volcano</span> and bedforms in the surrounding canyon. Repeated surveying by AUV document <span class="hlt">active</span> mud movement at the western summit in between 2014 and 2016. Through sediment coring and tephrochronology, ages of buried mudflow deposits are determined based on the sedimentation rate and the thickness of overlying hemipelagic sediments. An average extrusion rate of 27,000 m3/yr over the last ˜882 years is estimated. These results support a three-stage evolutionary model of Venere mud <span class="hlt">volcano</span> since ˜4,000 years ago. It includes the onset of quiescence at the eastern cone (after ˜2,200 years ago), erosive events in Squillace Canyon (prior to ˜882 years ago), and mudflows from the eastern cone (since ˜882 years). This study reveals new interactions between a mud <span class="hlt">volcano</span> and a canyon in the deep sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V31A3066B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V31A3066B"><span>CO2 and H2O Contents of Melt Inclusions from the 1891 Basaltic Balloon Eruption of Foerstner <span class="hlt">Submarine</span> <span class="hlt">Volcano</span>, Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Balcanoff, J. R.; Carey, S.; Kelley, K. A.; Boesenberg, J. S.</p> <p>2016-12-01</p> <p>Eruptions that produce basaltic balloon products are an uncommon eruption style only observed in five cases during historical times. Basaltic balloon products form in gas rich shallow <span class="hlt">submarine</span> eruptions, which produce large hollow clasts with sufficient buoyancy to float on seawater. Foerstner <span class="hlt">submarine</span> <span class="hlt">volcano</span>, off the coast of Pantelleria (Italy), erupted with this style in 1891 and is the only eruption where the vent site (250 m water depth) has been studied and sampled in detail with remotely operated vehicles (ROVs). Here, we report Fournier Transform Infrared Spectroscopy (FTIR) and electron microprobe (EMP) analyses of major elements and dissolved volatiles in melt inclusions from olivine and plagioclase phenocrysts picked from highly vesicular clasts recovered from the seafloor. The trachybasaltic melt is enriched in alkalis with notably high phosphorus (1.82-2.38 wt%), and melt inclusions show elevated H2O concentrations of 0.17 to 1.2 wt.% and highly elevated CO2 concentrations of 928 to 1864 ppm. Coexisting matrix glass is completely degassed with respect to carbon dioxide but has variable water contents up to 0.19 %. The maximum carbon dioxide value implies saturation at 1.5 kb, or 4.5 km below the <span class="hlt">volcano</span>. Trends in the CO2 and H2O data are most compatible with calculated open system degassing behavior. This is consistent with a proposed balloon formation mechanism involving a hybrid strombolian eruption style with the potential accumulation of gas-rich pockets below the vent as gas bubbles moved upwards independent of the low viscosity basaltic melt. Discharge of the gas-rich pockets led to the discharge of meter-sized slugs of magma with large internal vesicles (several tens of centimeters). A subset of these clasts had bulk densities that were lower than seawater, allowing them to rise to the sea surface where they either exploded or became water saturated and sank back to the seafloor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V33A1174X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V33A1174X"><span>Penguin Bank: A Loa-Trend Hawaiian <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, G.; Blichert-Toft, J.; Clague, D. A.; Cousens, B.; Frey, F. A.; Moore, J. G.</p> <p>2007-12-01</p> <p>Hawaiian <span class="hlt">volcanoes</span> along the Hawaiian Ridge from Molokai Island in the northwest to the Big Island in the southeast, define two parallel trends of <span class="hlt">volcanoes</span> known as the Loa and Kea spatial trends. In general, lavas erupted along these two trends have distinctive geochemical characteristics that have been used to define the spatial distribution of geochemical heterogeneities in the Hawaiian plume (e.g., Abouchami et al., 2005). These geochemical differences are well established for the <span class="hlt">volcanoes</span> forming the Big Island. The longevity of the Loa- Kea geochemical differences can be assessed by studying East and West Molokai <span class="hlt">volcanoes</span> and Penguin Bank which form a volcanic ridge perpendicular to the Loa and Kea spatial trends. Previously we showed that East Molokai <span class="hlt">volcano</span> (~1.5 Ma) is exclusively Kea-like and that West Molokai <span class="hlt">volcano</span> (~1.8 Ma) includes lavas that are both Loa- and Kea-like (Xu et al., 2005 and 2007).The <span class="hlt">submarine</span> Penguin Bank (~2.2 Ma), probably an independent <span class="hlt">volcano</span> constructed west of West Molokai <span class="hlt">volcano</span>, should be dominantly Loa-like if the systematic Loa and Kea geochemical differences were present at ~2.2 Ma. We have studied 20 samples from Penguin Bank including both <span class="hlt">submarine</span> and subaerially-erupted lavas recovered by dive and dredging. All lavas are tholeiitic basalt representing shield-stage lavas. Trace element ratios, such as Sr/Nb and Zr/Nb, and isotopic ratios of Sr and Nd clearly are Loa-like. On an ɛNd-ɛHf plot, Penguin Bank lavas fall within the field defined by Mauna Loa lavas. Pb isotopic data lie near the Loa-Kea boundary line defined by Abouchami et al. (2005). In conclusion, we find that from NE to SW, i.e., perpendicular to the Loa and Kea spatial trend, there is a shift from Kea-like East Molokai lavas to Loa-like Penguin Bank lavas with the intermediate West Molokai <span class="hlt">volcano</span> having lavas with both Loa- and Kea-like geochemical features. Therefore, the Loa and Kea geochemical dichotomy exhibited by Big Island <span class="hlt">volcanoes</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027546','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027546"><span>Hawaiian <span class="hlt">submarine</span> manganese-iron oxide crusts - A dating tool?</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.; Clague, D.A.</p> <p>2004-01-01</p> <p>Black manganese-iron oxide crusts form on most exposed rock on the ocean floor. Such crusts are well developed on the steep lava slopes of the Hawaiian Ridge and have been sampled during dredging and submersible dives. The crusts also occur on fragments detached from bedrock by mass wasting, on submerged coral reefs, and on poorly lithified sedimentary rocks. The thickness of the crusts was measured on samples collected since 1965 on the Hawaiian Ridge from 140 dive or dredge localities. Fifty-nine (42%) of the sites were collected in 2001 by remotely operated vehicles (ROVs). The thinner crusts on many samples apparently result from post-depositional breakage, landsliding, and intermittent burial of outcrops by sediment. The maximum crust thickness was selected from each dredge or dive site to best represent crusts on the original rock surface at that site. The measurements show an irregular progressive thickening of the crusts toward the northwest-i.e., progressive thickening toward the older volcanic features with increasing distance from the Hawaiian hotspot. Comparison of the maximum crust thickness with radiometric ages of related subaerial features supports previous studies that indicate a crust-growth rate of about 2.5 mm/m.y. The thickness information not only allows a comparison of the relative exposure ages of two or more features offshore from different <span class="hlt">volcanoes</span>, but also provides specific age estimates of volcanic and landslide deposits. The data indicate that some of the landslide blocks within the south Kona landslide are the oldest exposed rock on Mauna Loa, Kilauea, or Loihi <span class="hlt">volcanoes</span>. Crusts on the floors of <span class="hlt">submarine</span> canyons off Kohala and East Molokai <span class="hlt">volcanoes</span> indicate that these canyons are no longer serving as channelways for downslope, sediment-laden currents. Mahukona <span class="hlt">volcano</span> was approximately synchronous with Hilo Ridge, both being younger than Hana Ridge. The Nuuanu landslide is considerably older than the Wailau landslide. The Waianae</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFMED42B0182W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFMED42B0182W"><span>The NeMO Explorer Web Site: Interactive Exploration of a Recent <span class="hlt">Submarine</span> Eruption and Hydrothermal Vents, Axial <span class="hlt">Volcano</span>, Juan de Fuca Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weiland, C.; Chadwick, W. W.; Embley, R. W.</p> <p>2001-12-01</p> <p>To help visualize the <span class="hlt">submarine</span> volcanic landscape at NOAA's New Millennium Observatory (NeMO), we have created the NeMO Explorer web site: http://www.pmel.noaa.gov/vents/nemo/explorer.html. This web site takes visitors a mile down beneath the ocean surface to explore Axial Seamount, an <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> 300 miles off the Oregon coast. We use virtual reality to put visitors in a photorealistic 3-D model of the seafloor that lets them view hydrothermal vents and fresh lava flows as if they were really on the seafloor. At each of six virtual sites there is an animated tour and a 360o panorama in which users can view the volcanic landscape and see biological communities within a spatially accurate context. From the six sites there are hyperlinks to 50 video clips taken by a remotely operated vehicle. Each virtual site concentrates on a different topic, including the dynamics of the 1998 eruption at Axial <span class="hlt">volcano</span> (Rumbleometer), high-temperature hydrothermal vents (CASM and ASHES), diffuse hydrothermal venting (Marker33), subsurface microbial blooms (The Pit), and the boundary between old and new lavas (Castle vent). In addition to exploring the region geographically, visitors can also explore the web site via geological concepts. The concepts gallery lets you quickly find information about mid-ocean ridges, hydrothermal vents, vent fauna, lava morphology, and more. Of particular interest is an animation of the January 1998 eruption, which shows the rapid inflation (by over 3 m) and draining of the sheet flow. For more info see Fox et al., Nature, v.412, p.727, 2001. This project was funded by NOAA's High Performance Computing and Communication (HPCC) and Vents Programs. Our goal is to present a representative portion of the vast collection of NOAA's multimedia imagery to the public in a way that is easy to use and understand. These data are particularly challenging to present because of their high data rates and low contextual information. The 3-D models create</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29067531','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29067531"><span>Microbial community differentiation between <span class="hlt">active</span> and inactive sulfide chimneys of the Kolumbo <span class="hlt">submarine</span> <span class="hlt">volcano</span>, Hellenic Volcanic Arc.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Christakis, Christos A; Polymenakou, Paraskevi N; Mandalakis, Manolis; Nomikou, Paraskevi; Kristoffersen, Jon Bent; Lampridou, Danai; Kotoulas, Georgios; Magoulas, Antonios</p> <p>2018-01-01</p> <p>Over the last decades, there has been growing interest about the ecological role of hydrothermal sulfide chimneys, their microbial diversity and associated biotechnological potential. Here, we performed dual-index Illumina sequencing of bacterial and archaeal communities on <span class="hlt">active</span> and inactive sulfide chimneys collected from the Kolumbo hydrothermal field, situated on a geodynamic convergent setting. A total of 15,701 OTUs (operational taxonomic units) were assigned to 56 bacterial and 3 archaeal phyla, 133 bacterial and 16 archaeal classes. <span class="hlt">Active</span> chimney communities were dominated by OTUs related to thermophilic members of Epsilonproteobacteria, Aquificae and Deltaproteobacteria. Inactive chimney communities were dominated by an OTU closely related to the archaeon Nitrosopumilus sp., and by members of Gammaproteobacteria, Deltaproteobacteria, Planctomycetes and Bacteroidetes. These lineages are closely related to phylotypes typically involved in iron, sulfur, nitrogen, hydrogen and methane cycling. Overall, the inactive sulfide chimneys presented highly diverse and uniform microbial communities, in contrast to the <span class="hlt">active</span> chimney communities, which were dominated by chemolithoautotrophic and thermophilic lineages. This study represents one of the most comprehensive investigations of microbial diversity in <span class="hlt">submarine</span> chimneys and elucidates how the dissipation of hydrothermal <span class="hlt">activity</span> affects the structure of microbial consortia in these extreme ecological niches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1215724T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1215724T"><span>Glob<span class="hlt">Volcano</span> pre-operational services for global monitoring <span class="hlt">active</span> <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tampellini, Lucia; Ratti, Raffaella; Borgström, Sven; Seifert, Frank Martin; Peltier, Aline; Kaminski, Edouard; Bianchi, Marco; Branson, Wendy; Ferrucci, Fabrizio; Hirn, Barbara; van der Voet, Paul; van Geffen, J.</p> <p>2010-05-01</p> <p>The Glob<span class="hlt">Volcano</span> project (2007-2010) is part of the Data User Element programme of the European Space Agency (ESA). The project aims at demonstrating Earth Observation (EO) based integrated services to support the <span class="hlt">Volcano</span> Observatories and other mandate users (e.g. Civil Protection) in their monitoring <span class="hlt">activities</span>. The information services are assessed in close cooperation with the user organizations for different types of <span class="hlt">volcano</span>, from various geographical areas in various climatic zones. In a first phase, a complete information system has been designed, implemented and validated, involving a limited number of test areas and respective user organizations. In the currently on-going second phase, Glob<span class="hlt">Volcano</span> is delivering pre-operational services over 15 volcanic sites located in three continents and as many user organizations are involved and cooperating with the project team. The set of Glob<span class="hlt">Volcano</span> offered EO based information products is composed as follows: Deformation Mapping DInSAR (Differential Synthetic Aperture Radar Interferometry) has been used to study a wide range of surface displacements related to different phenomena (e.g. seismic faults, <span class="hlt">volcanoes</span>, landslides) at a spatial resolution of less than 100 m and cm-level precision. Permanent Scatterers SAR Interferometry method (PSInSARTM) has been introduced by Politecnico of Milano as an advanced InSAR technique capable of measuring millimetre scale displacements of individual radar targets on the ground by using multi-temporal data-sets, estimating and removing the atmospheric components. Other techniques (e.g. CTM) have followed similar strategies and have shown promising results in different scenarios. Different processing approaches have been adopted, according to data availability, characteristic of the area and dynamic characteristics of the <span class="hlt">volcano</span>. Conventional DInSAR: Colima (Mexico), Nyiragongo (Congo), Pico (Azores), Areanal (Costa Rica) PSInSARTM: Piton de la Fournaise (La Reunion Island</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036539','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036539"><span>Early growth of Kohala <span class="hlt">volcano</span> and formation of long Hawaiian rift zones</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lipman, Peter W.; Calvert, Andrew T.</p> <p>2011-01-01</p> <p>Transitional-composition pillow basalts from the toe of the Hilo Ridge, collected from outcrop by submersible, have yielded the oldest ages known from the Island of Hawaii: 1138 ± 34 to 1159 ± 33 ka. Hilo Ridge has long been interpreted as a <span class="hlt">submarine</span> rift zone of Mauna Kea, but the new ages validate proposals that it is the distal east rift zone of Kohala, the oldest subaerial <span class="hlt">volcano</span> on the island. These ages constrain the inception of tholeiitic volcanism at Kohala, provide the first measured duration of tholeiitic shield building (≥870 k.y.) for any Hawaiian <span class="hlt">volcano</span>, and show that this 125-km-long rift zone developed to near-total length during early growth of Kohala. Long eastern-trending rift zones of Hawaiian <span class="hlt">volcanoes</span> may follow fractures in oceanic crust <span class="hlt">activated</span> by arching of the Hawaiian Swell in front of the propagating hotspot.</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('https://www.ncbi.nlm.nih.gov/pubmed/25384354','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25384354"><span>Eruption of a deep-sea mud <span class="hlt">volcano</span> triggers rapid sediment movement.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Feseker, Tomas; Boetius, Antje; Wenzhöfer, Frank; Blandin, Jerome; Olu, Karine; Yoerger, Dana R; Camilli, Richard; German, Christopher R; de Beer, Dirk</p> <p>2014-11-11</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> are important sources of methane to the water column. However, the temporal variability of their mud and methane emissions is unknown. Methane emissions were previously proposed to result from a dynamic equilibrium between upward migration and consumption at the seabed by methane-consuming microbes. Here we show non-steady-state situations of vigorous mud movement that are revealed through variations in fluid flow, seabed temperature and seafloor bathymetry. Time series data for pressure, temperature, pH and seafloor photography were collected over 431 days using a benthic observatory at the <span class="hlt">active</span> Håkon Mosby Mud <span class="hlt">Volcano</span>. We documented 25 pulses of hot subsurface fluids, accompanied by eruptions that changed the landscape of the mud <span class="hlt">volcano</span>. Four major events triggered rapid sediment uplift of more than a metre in height, substantial lateral flow of muds at average velocities of 0.4 m per day, and significant emissions of methane and CO₂ from the seafloor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4242465','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4242465"><span>Eruption of a deep-sea mud <span class="hlt">volcano</span> triggers rapid sediment movement</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Feseker, Tomas; Boetius, Antje; Wenzhöfer, Frank; Blandin, Jerome; Olu, Karine; Yoerger, Dana R.; Camilli, Richard; German, Christopher R.; de Beer, Dirk</p> <p>2014-01-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> are important sources of methane to the water column. However, the temporal variability of their mud and methane emissions is unknown. Methane emissions were previously proposed to result from a dynamic equilibrium between upward migration and consumption at the seabed by methane-consuming microbes. Here we show non-steady-state situations of vigorous mud movement that are revealed through variations in fluid flow, seabed temperature and seafloor bathymetry. Time series data for pressure, temperature, pH and seafloor photography were collected over 431 days using a benthic observatory at the <span class="hlt">active</span> Håkon Mosby Mud <span class="hlt">Volcano</span>. We documented 25 pulses of hot subsurface fluids, accompanied by eruptions that changed the landscape of the mud <span class="hlt">volcano</span>. Four major events triggered rapid sediment uplift of more than a metre in height, substantial lateral flow of muds at average velocities of 0.4 m per day, and significant emissions of methane and CO2 from the seafloor. PMID:25384354</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060035732&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060035732&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dactive%2Bvolcanoes"><span><span class="hlt">Active</span> Deformation of Etna <span class="hlt">Volcano</span> Combing IFSAR and GPS data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lundgren, Paul</p> <p>1997-01-01</p> <p>The surface deformation of an <span class="hlt">active</span> <span class="hlt">volcano</span> is an important indicator of its eruptive state and its hazard potential. Mount Etna <span class="hlt">volcano</span> in Sicily is a very <span class="hlt">active</span> <span class="hlt">volcano</span> with well documented eruption episodes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUSM.V43C..04L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUSM.V43C..04L"><span>Examination of the constructional processes of <span class="hlt">submarine</span> Cerro Azul and the Galapagos Platform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lambert, M. K.; Harpp, K. S.; Geist, D. J.; Fornari, D. J.; Kurz, M. D.; Koleszar, A. M.; Rollins, N. A.</p> <p>2004-05-01</p> <p>One of the primary goals of the 2001 Drift04 cruise was to examine the constructional processes responsible for the Galapagos platform and to investigate the relationship between the platform and the overlying <span class="hlt">volcanoes</span>. Cerro Azul <span class="hlt">volcano</span> is located above the steep escarpment that marks the southwestern limit of the Galapagos platform, at the leading edge of the hotspot. This area is of particular interest in light of a recent seismic tomography experiment by Toomey, Hooft, et al., which suggests that the root of the Galapagos plume is centered between Cerro Azul and adjacent Fernandina Island. During the Drift04 cruise, detailed bathymetric and sidescan sonar studies were carried out across the <span class="hlt">submarine</span> sector of Cerro Azul and 14 dredges were collected from the same area. Major element analyses of the <span class="hlt">submarine</span> lavas indicate that the lavas from the platform edge and the subaerial Cerro Azul lavas constitute a suite of petrologically-related lavas. The dredged glasses of the Drift04 cruise have MgO contents of <7.5% and are indistinguishable from published data on Cerro Azul. Whole rock analyses include a highly primitive sample (20 wt% MgO), which probably contains accumulated olivine. All the <span class="hlt">submarine</span> and subaerial lavas define coherent trends in major element space that are consistent with variable amounts of olivine and olivine+cpx fractionation. Incompatible trace element (ITE) ratios indicate that the mantle source for the <span class="hlt">submarine</span> platform flows is intermediate in composition between the magmas supplying Fernandina and Cerro Azul. Previous researchers have proposed that two mantle endmembers are interacting across the leading edge of the plume, one focused at Fernandina and the other at Floreana Island. The intermediate ITE ratios of the <span class="hlt">submarine</span> and subaerial Cerro Azul lavas are consistent both geographically and compositionally with this hypothesis. Naumann and co-workers concluded that the lavas erupted at Cerro Azul were stored in small</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/fs074-97/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/fs074-97/"><span>Living on <span class="hlt">Active</span> <span class="hlt">Volcanoes</span> - The Island of 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>Heliker, Christina; Stauffer, Peter H.; Hendley, James W.</p> <p>1997-01-01</p> <p>People on the Island of Hawai'i face many hazards that come with living on or near <span class="hlt">active</span> <span class="hlt">volcanoes</span>. These include lava flows, explosive eruptions, volcanic smog, damaging earthquakes, and tsunamis (giant seawaves). As the population of the island grows, the task of reducing the risk from <span class="hlt">volcano</span> hazards becomes increasingly difficult. To help protect lives and property, U.S. Geological Survey (USGS) scientists at the Hawaiian <span class="hlt">Volcano</span> Observatory closely monitor and study Hawai'i's <span class="hlt">volcanoes</span> and issue timely warnings of hazardous <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.6053N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.6053N"><span><span class="hlt">Submarine</span> Volcanic Morphology of Santorini Caldera, Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nomikou, P.; Croff Bell, K.; Carey, S.; Bejelou, K.; Parks, M.; Antoniou, V.</p> <p>2012-04-01</p> <p>Santorini volcanic group form the central part of the modern Aegean volcanic arc, developed within the Hellenic arc and trench system, because of the ongoing subduction of the African plate beneath the European margin throughout Cenozoic. It comprises three distinct volcanic structures occurring along a NE-SW direction: Christianna form the southwestern part of the group, Santorini occupies the middle part and Koloumbo volcanic rift zone extends towards the northeastern part. The geology of the Santorini <span class="hlt">volcano</span> has been described by a large number of researchers with petrological as well as geochronological data. The offshore area of the Santorini volcanic field has only recently been investigated with emphasis mainly inside the Santorini caldera and the <span class="hlt">submarine</span> <span class="hlt">volcano</span> of Kolumbo. In September 2011, cruise NA-014 on the E/V Nautilus carried out new surveys on the <span class="hlt">submarine</span> volcanism of the study area, investigating the seafloor morphology with high-definition video imaging. <span class="hlt">Submarine</span> hydrothermal vents were found on the seafloor of the northern basin of the Santorini caldera with no evidence of high temperature fluid discharges or massive sulphide formations, but only low temperature seeps characterized by meter-high mounds of bacteria-rich sediment. This vent field is located in line with the normal fault system of the Kolumbo rift, and also near the margin of a shallow intrusion that occurs within the sediments of the North Basin. Push cores have been collected and they will provide insights for their geochemical characteristics and their relationship to the <span class="hlt">active</span> vents of the Kolumbo underwater <span class="hlt">volcano</span>. Similar vent mounds occur in the South Basin, at shallow depths around the islets of Nea and Palaia Kameni. ROV exploration at the northern slopes of Nea Kameni revealed a fascinating underwater landscape of lava flows, lava spines and fractured lava blocks that have been formed as a result of 1707-1711 and 1925-1928 AD eruptions. A hummocky topography at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..466P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..466P"><span>Orographic Flow over an <span class="hlt">Active</span> <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poulidis, Alexandros-Panagiotis; Renfrew, Ian; Matthews, Adrian</p> <p>2014-05-01</p> <p>Orographic flows over and around an isolated <span class="hlt">volcano</span> are studied through a series of numerical model experiments. The <span class="hlt">volcano</span> top has a heated surface, so can be thought of as "<span class="hlt">active</span>" but not erupting. A series of simulations with different atmospheric conditions and using both idealised and realistic configurations of the Weather Research and Forecast (WRF) model have been carried out. The study is based on the Soufriere Hills <span class="hlt">volcano</span>, located on the island of Montserrat in the Caribbean. This is a dome-building <span class="hlt">volcano</span>, leading to a sharp increase in the surface skin temperature at the top of the <span class="hlt">volcano</span> - up to tens of degrees higher than ambient values. The majority of the simulations use an idealised topography, in order for the results to have general applicability to similar-sized <span class="hlt">volcanoes</span> located in the tropics. The model is initialised with idealised atmospheric soundings, representative of qualitatively different atmospheric conditions from the rainy season in the tropics. The simulations reveal significant changes to the orographic flow response, depending upon the size of the temperature anomaly and the atmospheric conditions. The flow regime and characteristic features such as gravity waves, orographic clouds and orographic rainfall patterns can all be qualitatively changed by the surface heating anomaly. Orographic rainfall over the <span class="hlt">volcano</span> can be significantly enhanced with increased temperature anomaly. The implications for the eruptive behaviour of the <span class="hlt">volcano</span> and resulting secondary volcanic hazards will also be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V21C2733D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V21C2733D"><span>Acoustic and tephra records of explosive eruptions at West Mata <span class="hlt">submarine</span> <span class="hlt">volcano</span>, NE Lau Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dziak, R. P.; Bohnenstiehl, D. R.; Baker, E. T.; Matsumoto, H.; Caplan-Auerbach, J.; Mack, C. J.; Embley, R. W.; Merle, S. G.; Walker, S. L.; Lau, T. A.</p> <p>2013-12-01</p> <p>West Mata is a 1200 m deep <span class="hlt">submarine</span> <span class="hlt">volcano</span> where explosive boninite eruptions were directly observed in May 2009. Here we present long-term acoustic and tephra records of West Mata explosion <span class="hlt">activity</span> from three deployments of hydrophone and particle sensor moorings beginning on 8 January 2009. These records provide insights into the character of explosive magma degassing occurring at the <span class="hlt">volcano</span>'s summit vent until the decline and eventual cessation of the eruption during late 2010 and early 2011. The detailed acoustic records show three types of volcanic signals, 1) discrete explosions, 2) diffuse explosions, and 3) volcanic tremor. Discrete explosions are short duration, high amplitude broad-band signals caused by rapid gas bubble release. Diffuse signals are likely a result of 'trap-door' explosions where a quench cap of cooled lava forms over the magmatic vent but gas pressure builds underneath the cap. This pressure eventually causes the cap to breach and gas is explosively released until pressure reduces and the cap once again forms. Volcanic tremor is typified by narrow-band, long-duration signals with overtones, as well as narrow-band tones that vary frequency over time between 60-100 Hz. The harmonic tremor is thought to be caused by modulation of rapid, short duration gas explosion pulses and not a magma resonance phenomenon. The variable frequency tones may be caused by focused degassing or hydrothermal fluid flow from a narrow volcanic vent or conduit. High frequency (>30 Hz) tremor-like bands of energy are a result of interference caused by multipath wide-band signals, including sea-surface reflected acoustic phases, that arrive at the hydrophone with small time delays. Acoustic data suggest that eruption velocities for a single explosion range from 4-50 m s-1, although synchronous arrival of explosion signals has complicated our efforts to estimate long-term gas flux. Single explosions exhibit ~4-40 m3 s-1 of total volume flux (gas and rock) but</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25855623','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25855623"><span>Methanoculleus sediminis sp. nov., a methanogen from sediments near a <span class="hlt">submarine</span> mud <span class="hlt">volcano</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Sheng-Chung; Chen, Mei-Fei; Lai, Mei-Chin; Weng, Chieh-Yin; Wu, Sue-Yao; Lin, Saulwood; Yang, Tsanyao F; Chen, Po-Chun</p> <p>2015-07-01</p> <p>A mesophilic, hydrogenotrophic methanogen, strain S3Fa(T), was isolated from sediments collected by Ocean Researcher I cruise ORI-934 in 2010 near the <span class="hlt">submarine</span> mud <span class="hlt">volcano</span> MV4 located at the upper slope of south-west Taiwan. The methanogenic substrates utilized by strain S3Fa(T) were formate and H2/CO2 but not acetate, secondary alcohols, methylamines, methanol or ethanol. Cells of strain S3Fa(T) were non-motile, irregular cocci, 0.5-1.0 μm in diameter. The surface-layer protein showed an Mr of 128,000.The optimum growth conditions were 37 °C, pH 7.1 and 0.17 M NaCl. The DNA G+C content of the genome of strain S3Fa(T) was 62.3 mol%. Phylogenetic analysis revealed that strain S3Fa(T) was most closely related to Methanoculleus marisnigri JR1(T) (99.3% 16S rRNA gene sequence similarity). Genome relatedness between strain S3Fa(T) and Methanoculleus marisnigri JR1(T) was computed using both genome-to-genome distance analysis (GGDA) and average nucleotide identity (ANI) with values of 46.3-55.5% and 93.08%, respectively. Based on morphological, phenotypic, phylogenetic and genomic relatedness data, it is evident that strain S3Fa(T) represents a novel species of the genus Methanoculleus, for which the name Methanoculleus sediminis sp. nov. is proposed. The type strain is S3Fa(T) ( = BCRC AR10044(T) = DSM 29354(T)).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22170423','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22170423"><span>Viral infections stimulate the metabolism and shape prokaryotic assemblages in <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Corinaldesi, Cinzia; Dell'Anno, Antonio; Danovaro, Roberto</p> <p>2012-06-01</p> <p>Mud <span class="hlt">volcanoes</span> are geological structures in the oceans that have key roles in the functioning of the global ecosystem. Information on the dynamics of benthic viruses and their interactions with prokaryotes in mud <span class="hlt">volcano</span> ecosystems is still completely lacking. We investigated the impact of viral infection on the mortality and assemblage structure of benthic prokaryotes of five mud <span class="hlt">volcanoes</span> in the Mediterranean Sea. Mud <span class="hlt">volcano</span> sediments promote high rates of viral production (1.65-7.89 × 10(9) viruses g(-1) d(-1)), viral-induced prokaryotic mortality (VIPM) (33% cells killed per day) and heterotrophic prokaryotic production (3.0-8.3 μgC g(-1) d(-1)) when compared with sediments outside the mud <span class="hlt">volcano</span> area. The viral shunt (that is, the microbial biomass converted into dissolved organic matter as a result of viral infection, and thus diverted away from higher trophic levels) provides 49 mgC m(-2) d(-1), thus fuelling the metabolism of uninfected prokaryotes and contributing to the total C budget. Bacteria are the dominant components of prokaryotic assemblages in surface sediments of mud <span class="hlt">volcanoes</span>, whereas archaea dominate the subsurface sediment layers. Multivariate multiple regression analyses show that prokaryotic assemblage composition is not only dependant on the geochemical features and processes of mud <span class="hlt">volcano</span> ecosystems but also on synergistic interactions between bottom-up (that is, trophic resources) and top-down (that is, VIPM) controlling factors. Overall, these findings highlight the significant role of the viral shunt in sustaining the metabolism of prokaryotes and shaping their assemblage structure in mud <span class="hlt">volcano</span> sediments, and they provide new clues for our understanding of the functioning of cold-seep ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997GeCoA..61.3525R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997GeCoA..61.3525R"><span>Degassing of metals and metalloids from erupting seamount and mid-ocean ridge <span class="hlt">volcanoes</span>: Observations and predictions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rubin, Ken</p> <p>1997-09-01</p> <p>Recently, it has been reported that the element polonium degasses from mid-ocean ridge and seamount <span class="hlt">volcanoes</span> during eruptions. Published and new observations on other volatile metal and metalloid elements can also be interpreted as indicating significant degassing of magmatic vapors during <span class="hlt">submarine</span> eruptions. This process potentially plays an important role in the net transfer of chemical elements from erupting <span class="hlt">volcanoes</span> to seawater in addition to that arising from sea floor hydrothermal systems. In this paper, a framework is constructed for predicting and assessing semiquantitatively the potential magnitude and chemical fingerprints in the water column of metal and metalloid degassing using (1) predictions from a summary of element volatilities during mafic subaerial volcanism worldwide and (2) limited data from <span class="hlt">submarine</span> volcanic effusives. The latter include analyses of polonium and trace metals in near-<span class="hlt">volcano</span> water masses sampled following a <span class="hlt">submarine</span> eruption at Loihi seamount, Hawaii (1000 m bsl) in 1996. The element volatility predictions and observations show good agreement, considering the limited dataset. Some of the highest volatility main group and transition element enrichments in seawater over Loihi are predicted by the degassing mass transfer model I present. When expanded to cover all <span class="hlt">submarine</span> volcanic <span class="hlt">activity</span>, it is predicted that exit fluxes of these elements are up to 10 2-10 3 greater by degassing than by normal MOR hydrothermalism. In contrast, MOR exit fluxes of low volatility alkali and alkaline earth elements are likely 10 2-10 6 greater from hydrothermal inputs. Degassing inputs to the ocean are probably highly episodic, occurring almost entirely during eruptions; these are times of enhanced and abnormal hydrothermalism as well. Although major hydrothermal and degassing events may not be chemically recognizable in real water masses as wholly distinct entities, it is nevertheless possible to predict to what extent each process flavors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V14C..08D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V14C..08D"><span><span class="hlt">Active</span> <span class="hlt">Submarine</span> <span class="hlt">Volcanoes</span> and Electro-Optical Sensor Networks: The Potential of Capturing and Quantifying an Entire Eruptive Sequence at Axial Seamount, Juan de Fuca Ridge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delaney, J. R.; Kelley, D. S.; Proskurowski, G.; Fundis, A. T.; Kawka, O.</p> <p>2011-12-01</p> <p>The NE Pacific Regional Scale Nodes (RSN) component of the NSF Ocean Observatories Initiative is designed to provide unprecedented electrical power and bandwidth to the base and summit of Axial Seamount. The scientific community is engaged in identifying a host of existing and innovative observation and measurement techniques that utilize the high-power and bandwidth infrastructure and its real-time transmission capabilities. The cable, mooring, and sensor arrays will enable the first quantitative documentation of myriad processes leading up to, during, and following a <span class="hlt">submarine</span> volcanic event. Currently planned RSN instrument arrays will provide important and concurrent spatial and temporal constraints on earthquake <span class="hlt">activity</span>, melt migration, hydrothermal venting behavior and chemistry, ambient currents, microbial community structure, high-definition (HD) still images and HD video streaming from the vents, and water-column chemistry in the overlying ocean. Anticipated, but not yet funded, additions will include AUVs and gliders that continually document the spatial-temporal variations in the water column above the <span class="hlt">volcano</span> and the distal zones. When an eruption appears imminent the frequency of sampling will be increased remotely, and the potential of repurposing the tracking capabilities of the mobile sensing platforms will be adapted to the spatial indicators of likely eruption <span class="hlt">activity</span>. As the eruption begins mobile platforms will fully define the geometry, temperature, and chemical-microbial character of the volcanic plume as it rises into the thoroughly documented control volume above the <span class="hlt">volcano</span>. Via the Internet the scientific community will be able to witness and direct adaptive sampling in response to changing conditions of plume formation. A major goal will be to document the eruptive volume and link the eruption duration to the volume of erupted magma. For the first time, it will be possible to begin to quantify the time-integrated output of an underwater</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.488...46D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.488...46D"><span>Lava delta deformation as a proxy for <span class="hlt">submarine</span> slope instability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Di Traglia, Federico; Nolesini, Teresa; Solari, Lorenzo; Ciampalini, Andrea; Frodella, William; Steri, Damiano; Allotta, Benedetto; Rindi, Andrea; Marini, Lorenzo; Monni, Niccolò; Galardi, Emanuele; Casagli, Nicola</p> <p>2018-04-01</p> <p>The instability of lava deltas is a recurrent phenomenon affecting volcanic islands, which can potentially cause secondary events such as littoral explosions (due to interactions between hot lava and seawater) and tsunamis. It has been shown that Interferometric Synthetic Aperture Radar (InSAR) is a powerful technique to forecast the collapse of newly emplaced lava deltas. This work goes further, demonstrating that the monitoring of lava deltas is a successful strategy by which to observe the long-term deformation of subaerial-<span class="hlt">submarine</span> landslide systems on unstable volcanic flanks. In this paper, displacement measurements derived from Synthetic Aperture Radar (SAR) imagery were used to detect lava delta instability at Stromboli <span class="hlt">volcano</span> (Italy). Recent flank eruptions (2002-2003, 2007 and 2014) affected the Sciara del Fuoco (SdF) depression, created a "stacked" lava delta, which overlies a pre-existing scar produced by a <span class="hlt">submarine</span>-subaerial tsunamigenic landslide that occurred on 30 December 2002. Space-borne X-band COSMO-SkyMED (CSK) and C-band SENTINEL-1A (SNT) SAR data collected between February 2010 and October 2016 were processed using the SqueeSAR algorithm. The obtained ground displacement maps revealed the differential ground motion of the lava delta in both CSK and SNT datasets, identifying a stable area (characterized by less than 2 mm/y in both datasets) within the northern sector of the SdF and an unstable area (characterized by velocity fields on the order of 30 mm/y and 160 mm/y in the CSK and SNT datasets, respectively) in the central sector of the SdF. The slope stability of the offshore part of the SdF, as reconstructed based on a recently performed multibeam bathymetric survey, was evaluated using a 3D Limit Equilibrium Method (LEM). In all the simulations, Factor of Safety (F) values between 0.9 and 1.1 always characterized the <span class="hlt">submarine</span> slope between the coastline and -250 m a.s.l. The critical surfaces for all the search volumes corresponded to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28812643','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28812643"><span>A <span class="hlt">submarine</span> volcanic eruption leads to a novel microbial habitat.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Danovaro, Roberto; Canals, Miquel; Tangherlini, Michael; Dell'Anno, Antonio; Gambi, Cristina; Lastras, Galderic; Amblas, David; Sanchez-Vidal, Anna; Frigola, Jaime; Calafat, Antoni M; Pedrosa-Pàmies, Rut; Rivera, Jesus; Rayo, Xavier; Corinaldesi, Cinzia</p> <p>2017-04-24</p> <p><span class="hlt">Submarine</span> volcanic eruptions are major catastrophic events that allow investigation of the colonization mechanisms of newly formed seabed. We explored the seafloor after the eruption of the Tagoro <span class="hlt">submarine</span> <span class="hlt">volcano</span> off El Hierro Island, Canary Archipelago. Near the summit of the volcanic cone, at about 130 m depth, we found massive mats of long, white filaments that we named Venus's hair. Microscopic and molecular analyses revealed that these filaments are made of bacterial trichomes enveloped within a sheath and colonized by epibiotic bacteria. Metagenomic analyses of the filaments identified a new genus and species of the order Thiotrichales, Thiolava veneris. Venus's hair shows an unprecedented array of metabolic pathways, spanning from the exploitation of organic and inorganic carbon released by volcanic degassing to the uptake of sulfur and nitrogen compounds. This unique metabolic plasticity provides key competitive advantages for the colonization of the new habitat created by the <span class="hlt">submarine</span> eruption. A specialized and highly diverse food web thrives on the complex three-dimensional habitat formed by these microorganisms, providing evidence that Venus's hair can drive the restart of biological systems after <span class="hlt">submarine</span> volcanic eruptions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3358031','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3358031"><span>Viral infections stimulate the metabolism and shape prokaryotic assemblages in <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Corinaldesi, Cinzia; Dell'Anno, Antonio; Danovaro, Roberto</p> <p>2012-01-01</p> <p>Mud <span class="hlt">volcanoes</span> are geological structures in the oceans that have key roles in the functioning of the global ecosystem. Information on the dynamics of benthic viruses and their interactions with prokaryotes in mud <span class="hlt">volcano</span> ecosystems is still completely lacking. We investigated the impact of viral infection on the mortality and assemblage structure of benthic prokaryotes of five mud <span class="hlt">volcanoes</span> in the Mediterranean Sea. Mud <span class="hlt">volcano</span> sediments promote high rates of viral production (1.65–7.89 × 109 viruses g−1 d−1), viral-induced prokaryotic mortality (VIPM) (33% cells killed per day) and heterotrophic prokaryotic production (3.0–8.3 μgC g−1 d−1) when compared with sediments outside the mud <span class="hlt">volcano</span> area. The viral shunt (that is, the microbial biomass converted into dissolved organic matter as a result of viral infection, and thus diverted away from higher trophic levels) provides 49 mgC m−2 d−1, thus fuelling the metabolism of uninfected prokaryotes and contributing to the total C budget. Bacteria are the dominant components of prokaryotic assemblages in surface sediments of mud <span class="hlt">volcanoes</span>, whereas archaea dominate the subsurface sediment layers. Multivariate multiple regression analyses show that prokaryotic assemblage composition is not only dependant on the geochemical features and processes of mud <span class="hlt">volcano</span> ecosystems but also on synergistic interactions between bottom-up (that is, trophic resources) and top-down (that is, VIPM) controlling factors. Overall, these findings highlight the significant role of the viral shunt in sustaining the metabolism of prokaryotes and shaping their assemblage structure in mud <span class="hlt">volcano</span> sediments, and they provide new clues for our understanding of the functioning of cold-seep ecosystems. PMID:22170423</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035857','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035857"><span>Postshield stage transitional volcanism on Mahukona <span class="hlt">Volcano</span>, 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>Clague, D.A.; Calvert, A.T.</p> <p>2009-01-01</p> <p>Age spectra from 40Ar/39Ar incremental heating experiments yield ages of 298??25 ka and 310??31 ka for transitional composition lavas from two cones on <span class="hlt">submarine</span> Mahukona <span class="hlt">Volcano</span>, Hawaii. These ages are younger than the inferred end of the tholeiitic shield stage and indicate that the <span class="hlt">volcano</span> had entered the postshield alkalic stage before going extinct. Previously reported elevated helium isotopic ratios of lavas from one of these cones were incorrectly interpreted to indicate eruption during a preshield alkalic stage. Consequently, high helium isotopic ratios are a poor indicator of eruptive stage, as they occur in preshield, shield, and postshield stage lavas. Loihi Seamount and Kilauea are the only known Hawaiian <span class="hlt">volcanoes</span> where the volume of preshield alkalic stage lavas can be estimated. ?? Springer-Verlag 2008.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://ngmdb.usgs.gov/Prodesc/proddesc_68315.htm','USGSPUBS'); return false;" href="http://ngmdb.usgs.gov/Prodesc/proddesc_68315.htm"><span>Geologic Map of the Summit Region of Kilauea <span class="hlt">Volcano</span>, 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>Neal, Christina A.; Lockwood, John P.</p> <p>2003-01-01</p> <p>This report consists of a large map sheet and a pamphlet. The map shows the geology, some photographs, description of map units, and correlation of map units. The pamphlet gives the full text about the geologic map. The area covered by this map includes parts of four U.S. Geological Survey 7.5' topographic quadrangles (Kilauea Crater, <span class="hlt">Volcano</span>, Ka`u Desert, and Makaopuhi). It encompasses the summit, upper rift zones, and Koa`e Fault System of Kilauea <span class="hlt">Volcano</span> and a part of the adjacent, southeast flank of Mauna Loa <span class="hlt">Volcano</span>. The map is dominated by products of eruptions from Kilauea <span class="hlt">Volcano</span>, the southernmost of the five <span class="hlt">volcanoes</span> on the Island of Hawai`i and one of the world's most <span class="hlt">active</span> <span class="hlt">volcanoes</span>. At its summit (1,243 m) is Kilauea Crater, a 3 km-by-5 km collapse caldera that formed, possibly over several centuries, between about 200 and 500 years ago. Radiating away from the summit caldera are two linear zones of intrusion and eruption, the east and the southwest rift zones. Repeated subaerial eruptions from the summit and rift zones have built a gently sloping, elongate shield <span class="hlt">volcano</span> covering approximately 1,500 km2. Much of the <span class="hlt">volcano</span> lies under water; the east rift zone extends 110 km from the summit to a depth of more than 5,000 m below sea level; whereas the southwest rift zone has a more limited <span class="hlt">submarine</span> continuation. South of the summit caldera, mostly north-facing normal faults and open fractures of the Koa`e Fault System extend between the two rift zones. The Koa`e Fault System is interpreted as a tear-away structure that accommodates southward movement of Kilauea's flank in response to distension of the <span class="hlt">volcano</span> perpendicular to the rift zones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1512426J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1512426J"><span>Monitoring El Hierro <span class="hlt">submarine</span> volcanic eruption events with a <span class="hlt">submarine</span> 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>Jurado, Maria Jose; Molino, Erik; Lopez, Carmen</p> <p>2013-04-01</p> <p>A <span class="hlt">submarine</span> volcanic eruption took place near the southernmost emerged land of the El Hierro Island (Canary Islands, Spain), from October 2011 to February 2012. The Instituto Geografico Nacional (IGN) seismic stations network evidenced seismic unrest since July 2012 and was a reference also to follow the evolution of the seismic <span class="hlt">activity</span> associated with the volcanic eruption. From the beginning of the eruption a geophone string was installed less than 2 km away from the new <span class="hlt">volcano</span>, next to La Restinga village shore, to record seismic <span class="hlt">activity</span> related to the volcanic <span class="hlt">activity</span>, continuously and with special interest on high frequency events. The seismic array was endowed with 8, high frequency, 3 component, 250 Hz, geophone cable string with a separation of 6 m between them. The analysis of the dataset using spectral techniques allows the characterization of the different phases of the eruption and the study of its dynamics. The correlation of the data analysis results with the observed sea surface <span class="hlt">activity</span> (ash and lava emission and degassing) and also with the seismic <span class="hlt">activity</span> recorded by the IGN field seismic monitoring system, allows the identification of different stages suggesting the existence of different signal sources during the volcanic eruption and also the posteruptive record of the degassing <span class="hlt">activity</span>. The study shows that the high frequency capability of the geophone array allow the study of important features that cannot be registered by the standard seismic stations. The accumulative spectral amplitude show features related to eruptive changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19114513','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19114513"><span>Molecular comparison of bacterial communities within iron-containing flocculent mats associated with <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> along the Kermadec Arc.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hodges, Tyler W; Olson, Julie B</p> <p>2009-03-01</p> <p>Iron oxide sheaths and filaments are commonly found in hydrothermal environments and have been shown to have a biogenic origin. These structures were seen in the flocculent material associated with two <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> along the Kermadec Arc north of New Zealand. Molecular characterization of the bacterial communities associated with the flocculent samples indicated that no known Fe-oxidizing bacteria dominated the recovered clone libraries. However, clones related to the recently described Fe-oxidizing bacterium Mariprofundus ferrooxydans were obtained from both the iron-containing flocculent (Fe-floc) and sediment samples, and peaks corresponding to Mariprofundus ferrooxydans, as well as the related clones, were observed in several of our terminal restriction fragment length polymorphism profiles. A large group of epsilonproteobacterial sequences, for which there is no cultured representative, dominated clones from the Fe-floc libraries and were less prevalent in the sediment sample. Phylogenetic analyses indicated that several operational taxonomic units appeared to be site specific, and statistical analyses of the clone libraries found that all samples were significantly different from each other. Thus, the bacterial communities in the Fe-floc samples were not more closely related to each other than to the sediment communities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EOSTr..95..157C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EOSTr..95..157C"><span>Discovery of the Largest Historic Silicic <span class="hlt">Submarine</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>Carey, Rebecca J.; Wysoczanski, Richard; Wunderman, Richard; Jutzeler, Martin</p> <p>2014-05-01</p> <p>It was likely twice the size of the renowned Mount St. Helens eruption of 1980 and perhaps more than 10 times bigger than the more recent 2010 Eyjafjallajökull eruption in Iceland. However, unlike those two events, which dominated world news headlines, in 2012 the daylong <span class="hlt">submarine</span> silicic eruption at Havre <span class="hlt">volcano</span> in the Kermadec Arc, New Zealand (Figure 1a; ~800 kilometers north of Auckland, New Zealand), passed without fanfare. In fact, for a while no one even knew it had occurred.</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('http://adsabs.harvard.edu/abs/2009AGUFMNG41A1186S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMNG41A1186S"><span>SmallWorld Behavior of the Worldwide <span class="hlt">Active</span> <span class="hlt">Volcanoes</span> Network: Preliminary Results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spata, A.; Bonforte, A.; Nunnari, G.; Puglisi, G.</p> <p>2009-12-01</p> <p>We propose a preliminary complex networks based approach in order to model and characterize <span class="hlt">volcanoes</span> <span class="hlt">activity</span> correlation observed on a planetary scale over the last two thousand years. Worldwide volcanic <span class="hlt">activity</span> is in fact related to the general plate tectonics that locally drives the faults <span class="hlt">activity</span>, that in turn controls the magma upraise beneath the <span class="hlt">volcanoes</span>. To find correlations among different <span class="hlt">volcanoes</span> could indicate a common underlying mechanism driving their <span class="hlt">activity</span> and could help us interpreting the deeper common dynamics controlling their unrest. All the first evidences found testing the procedure, suggest the suitability of this analysis to investigate global volcanism related to plate tectonics. The first correlations found, in fact, indicate that an underlying common large-scale dynamics seems to drive volcanic <span class="hlt">activity</span> at least around the Pacific plate, where it collides and subduces beneath American, Eurasian and Australian plates. From this still preliminary analysis, also more complex relationships among <span class="hlt">volcanoes</span> lying on different tectonic margins have been found, suggesting some more complex interrelationships between different plates. The understanding of eventually detected correlations could be also used to further implement warning systems, relating the unrest probabilities of a specific <span class="hlt">volcano</span> also to the ongoing <span class="hlt">activity</span> to the correlated ones. Our preliminary results suggest that, as for other many physical and biological systems, an underlying organizing principle of planetary <span class="hlt">volcanoes</span> <span class="hlt">activity</span> might exist and it could be a small-world principle. In fact we found that, from a topological perspective, <span class="hlt">volcanoes</span> correlations are characterized by the typical features of small-world network: a high clustering coefficient and a low characteristic path length. These features confirm that global <span class="hlt">volcanoes</span> <span class="hlt">activity</span> is characterized by both short and long-range correlations. We stress here the fact that numerical simulation carried out in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008EOSTr..89..289I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008EOSTr..89..289I"><span>Imaging an <span class="hlt">Active</span> <span class="hlt">Volcano</span> Edifice at Tenerife Island, Spain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ibáñez, Jesús M.; Rietbrock, Andreas; García-Yeguas, Araceli</p> <p>2008-08-01</p> <p>An <span class="hlt">active</span> seismic experiment to study the internal structure of Teide <span class="hlt">volcano</span> is being carried out on Tenerife, a volcanic island in Spain's Canary Islands archipelago. The main objective of the Tomography at Teide <span class="hlt">Volcano</span> Spain (TOM-TEIDEVS) experiment, begun in January 2007, is to obtain a three-dimensional (3-D) structural image of Teide <span class="hlt">volcano</span> using seismic tomography and seismic reflection/refraction imaging techniques. At present, knowledge of the deeper structure of Teide and Tenerife is very limited, with proposed structural models based mainly on sparse geophysical and geological data. The multinational experiment-involving institutes from Spain, the United Kingdom, Italy, Ireland, and Mexico-will generate a unique high-resolution structural image of the <span class="hlt">active</span> <span class="hlt">volcano</span> edifice and will further our understanding of volcanic processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.V32A..05C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.V32A..05C"><span>Stratigraphic relationships and timing of the 2012 Havre <span class="hlt">submarine</span> silicic volcanic eruption revealed by high resolution bathymetric mapping and observations by underwater vehicles.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carey, R.; Soule, S. A.; Houghton, B. F.; White, J. D. L.; Manga, M.; Wysoczanski, R. J.; Tani, K.; McPhie, J.; Fornari, D. J.; Jutzeler, M.; Caratori Tontini, F.; Ikegami, F.; Jones, M.; Murch, A.; Fauria, K.; Mitchell, S. J.; Cahalan, R. C.; Conway, C.; McKenzie, W.</p> <p>2015-12-01</p> <p>The 2012 deep rhyolitic caldera eruption of Havre <span class="hlt">volcano</span> in the Kermadec arc is the first historic observed <span class="hlt">submarine</span> eruption that produced a pumice raft observed at the ocean's surface. Ship-based bathymetric surveys before and after the eruption permit the intricacies of eruption styles, products and timescales to be quantified. In 2015 we mapped this <span class="hlt">submarine</span> <span class="hlt">volcano</span> in unprecedented detail with two submergence vehicles in tandem, facilitating a wide and comprehensive geological survey and sampling mission. These efforts and observations show highly complex and often simultaneous eruptive behavior from more than 14 vents along two 3 km-long fissures that represent massive ruptures of the caldera walls. This survey also revealed an important role for pre- and inter-eruptive periods of mass wasting processes derived from the intrusion of magma and destablisation of caldera walls. The detailed characterization of the eruption products, and quantification of timescales provides the scientific community with the first glimpse of the nature of <span class="hlt">submarine</span>, intermediate magnitude, deep silicic caldera eruptions and permits unanswered yet first order fundamental questions of <span class="hlt">submarine</span> eruption and transport processes to be addressed in the decades to come.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030816','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030816"><span>Comparative velocity structure of <span class="hlt">active</span> Hawaiian <span class="hlt">volcanoes</span> from 3-D onshore-offshore seismic tomography</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Park, J.; Morgan, J.K.; Zelt, C.A.; Okubo, P.G.; Peters, L.; Benesh, N.</p> <p>2007-01-01</p> <p>We present a 3-D P-wave velocity model of the combined subaerial and <span class="hlt">submarine</span> portions of the southeastern part of the Island of Hawaii, based on first-arrival seismic tomography of marine airgun shots recorded by the onland seismic network. Our model shows that high-velocity materials (6.5-7.0??km/s) lie beneath Kilauea's summit, Koae fault zone, and the upper Southwest Rift Zone (SWRZ) and upper and middle East Rift Zone (ERZ), indicative of magma cumulates within the volcanic edifice. A separate high-velocity body of 6.5-6.9??km/s within Kilauea's lower ERZ and upper Puna Ridge suggests a distinct body of magma cumulates, possibly connected to the summit magma cumulates at depth. The two cumulate bodies within Kilauea's ERZ may have undergone separate ductile flow seaward, influencing the <span class="hlt">submarine</span> morphology of Kilauea's south flank. Low velocities (5.0-6.3??km/s) seaward of Kilauea's Hilina fault zone, and along Mauna Loa's seaward facing Kao'iki fault zone, are attributed to thick piles of volcaniclastic sediments deposited on the <span class="hlt">submarine</span> flanks. Loihi seamount shows high-velocity anomalies beneath the summit and along the rift zones, similar to the interpreted magma cumulates below Mauna Loa and Kilauea <span class="hlt">volcanoes</span>, and a low-velocity anomaly beneath the oceanic crust, probably indicative of melt within the upper mantle. Around Kilauea's <span class="hlt">submarine</span> flank, a high-velocity anomaly beneath the outer bench suggests the presence of an ancient seamount that may obstruct outward spreading of the flank. Mauna Loa's southeast flank is also marked by a large, anomalously high-velocity feature (7.0-7.4??km/s), interpreted to define an inactive, buried volcanic rift zone, which might provide a new explanation for the westward migration of Mauna Loa's current SWRZ and the growth of Kilauea's SWRZ. ?? 2007 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730021547','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730021547"><span>July 1973 ground survey of <span class="hlt">active</span> Central American <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stoiber, R. E. (Principal Investigator); Rose, W. I., Jr.</p> <p>1973-01-01</p> <p>The author has identified the following significant results. Ground survey has shown that thermal anomalies of various sizes associated with volcanic <span class="hlt">activity</span> at several Central American <span class="hlt">volcanoes</span> should be detectable from Skylab. Anomalously hot areas of especially large size (greater than 500 m in diameter) are now found at Santiaguito and Pacaya <span class="hlt">volcanoes</span> in Guatemala and San Cristobal in Nicaragua. Smaller anomalous areas are to be found at least seven other <span class="hlt">volcanoes</span>. This report is completed after ground survey of eleven <span class="hlt">volcanoes</span> and ground-based radiation thermometry mapping at these same points.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.9072B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.9072B"><span>What can we learn about the history of oceanic shield <span class="hlt">volcanoes</span> from deep marine sediments? Example from La Reunion <span class="hlt">volcanoes</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bachelery, Patrick; Babonneau, Nathalie; Jorry, Stephan; Mazuel, Aude</p> <p>2014-05-01</p> <p>The discovery in 2006, during the oceanographic survey FOREVER, of large volcaniclastic sedimentary systems off La Réunion Island (western Indian ocean) revealed a new image of the evolution of oceanic shield <span class="hlt">volcanoes</span> and their dismantling. Marine data obtained from 2006 to 2011 during the oceanographic surveys ERODER 1 to ERODER 4 included bathymetry, acoustic imagery, echosounding profiles, dredging and coring. Six major turbidite systems were mapped and described on the <span class="hlt">submarine</span> flanks of La Reunion volcanic edifice and the surrounding oceanic plate. The interpretation of sediment cores enable us to characterise the processes of gravity-driven sediment transfer from land to deep sea and also to revisit the history of the <span class="hlt">volcanoes</span> of La Réunion Island. Turbidite systems constitute a major component of the transfer of volcanic materials to the abyssal plain (Saint-Ange et al., 2011; 2013; Sisavath et al., 2011; 2012; Babonneau et al., 2013). These systems are superimposed on other dismantling processes (slow deformation such as gravity sliding or spreading, and huge landslides causing debris avalanches). Turbidite systems mainly develop in connection with the hydrographic network of the island, and especially at the mouths of large rivers. They show varying degrees of maturity, with canyons incising the <span class="hlt">submarine</span> slope of the island and feeding depositional areas, channels and lobes extending over 150 km from the coast. The cores collected in turbidite systems show successions of thin and thick turbidites alternating with hemipelagic sedimentation. Sedimentological and stratigraphic analysis of sediment cores yielded a chronology of <span class="hlt">submarine</span> gravity events. First-order information was obtained on the explosive <span class="hlt">activity</span> of these <span class="hlt">volcanoes</span> by identifying tephra layers in the cores (glass shards and pumice). In addition, major events of the volcanic and tectonic history of the island can be identified and dated. In this contribution, we focus most attention on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRB..123.1035L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRB..123.1035L"><span>Understanding the Evolution of an Oceanic Intraplate <span class="hlt">Volcano</span> From Seismic Reflection Data: A New Model for La Réunion, Indian Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lebas, E.; Le Friant, A.; Deplus, C.; de Voogd, B.</p> <p>2018-02-01</p> <p>High-resolution seismic reflection profiles gathered in 2006 on La Réunion <span class="hlt">submarine</span> flanks and surrounding abyssal plain, enabled characterization of the seismostratigraphy architecture of the volcaniclastic apron. Four seismic units are defined beyond the edifice base: (1) a basal unit, interpreted as pelagic sediment predating La Réunion volcanism; (2) a second unit showing low- to medium-amplitude reflections, related to La Réunion emergence including the <span class="hlt">submarine</span> explosive phase; (3) a high-amplitude seismic unit, associated with subaerial volcanic <span class="hlt">activity</span> (i.e., mature island stage); and (4) an acoustically transparent unit, ascribed to erosion that currently affects the volcanic complex. Two prominent horizons delineate the base of the units II and III marking, respectively, the onset of La Réunion seamount explosive <span class="hlt">activity</span> and the Piton des Neiges volcanic <span class="hlt">activity</span>. Related isopach maps demonstrate: (1) the existence of a large proto-Piton des Neiges <span class="hlt">volcano</span> during the first building phase of the volcanic complex, and (2) the central role of the Piton des Neiges <span class="hlt">volcano</span> during the second phase. Shield growth stage of the Piton de la Fournaise <span class="hlt">volcano</span> is also captured in the upper part of the volcaniclastic apron, attesting to its recent contribution. Seismic facies identified in the apron highlight a prevalence of sedimentary and reworking processes since the onset of the volcanism compared to catastrophic flank collapses. We present here a new model of evolution for La Réunion volcanic complex since the onset of the volcanism and argue that a major proto Piton des Neiges-Piton des Neiges volcanic complex controls La Réunion present-day morphology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880033044&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880033044&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes"><span>Using the Landsat Thematic Mapper to detect and monitor <span class="hlt">active</span> <span class="hlt">volcanoes</span> - An example from Lascar <span class="hlt">volcano</span>, northern Chile</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Francis, P. W.; Rothery, D. A.</p> <p>1987-01-01</p> <p>The Landsat Thematic Mapper (TM) offers a means of detecting and monitoring thermal features of <span class="hlt">active</span> <span class="hlt">volcanoes</span>. Using the TM, a prominent thermal anomaly has been discovered on Lascar <span class="hlt">volcano</span>, northern Chile. Data from two short-wavelength infrared channels of the TM show that material within a 300-m-diameter pit crater was at a temperature of at least 380 C on two dates in 1985. The thermal anomaly closely resembles in size and radiant temperature the anomaly over the <span class="hlt">active</span> lava lake at Erta'ale in Ethiopia. An eruption took place at Lascar on Sept. 16, 1986. TM data acquired on Oct. 27, 1986, revealed significant changes within the crater area. Lascar is in a much more <span class="hlt">active</span> state than any other <span class="hlt">volcano</span> in the central Andes, and for this reason it merits further careful monitoring. Studies show that the TM is capable of confidently identifying thermal anomalies less than 100 m in size, at temperatures of above 150 C, and thus it offers a valuable means of monitoring the conditions of <span class="hlt">active</span> or potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span>, particularly those in remote regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMGP33A1089N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMGP33A1089N"><span>Hydrothermal reservoir beneath Taal <span class="hlt">Volcano</span> (Philippines): Implications to volcanic <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nagao, T.; Alanis, P. B.; Yamaya, Y.; Takeuchi, A.; Bornas, M. V.; Cordon, J. M.; Puertollano, J.; Clarito, C. J.; Hashimoto, T.; Mogi, T.; Sasai, Y.</p> <p>2012-12-01</p> <p>Taal <span class="hlt">Volcano</span> is one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Philippines. The first recorded eruption was in 1573. Since then it has erupted 33 times resulting in thousands of casualties and large damages to property. In 1995, it was declared as one of the 15 Decade <span class="hlt">Volcanoes</span>. Beginning in the early 1990s it has experienced several phases of abnormal <span class="hlt">activity</span>, including seismic swarms, episodes of ground deformation, ground fissuring and hydrothermal <span class="hlt">activities</span>, which continues up to the present. However, it has been noted that past historical eruptions of Taal <span class="hlt">Volcano</span> may be divided into 2 distinct cycles, depending on the location of the eruption center, either at Main Crater or at the flanks. Between 1572-1645, eruptions occurred at the Main Crater, in 1707 to 1731, they occurred at the flanks. In 1749, eruptions moved back to the Main Crater until 1911. During the 1965 and until the end of the 1977 eruptions, eruptive <span class="hlt">activity</span> once again shifted to the flanks. As part of the PHIVOLCS-JICA-SATREPS Project magnetotelluric and audio-magnetotelluric surveys were conducted on <span class="hlt">Volcano</span> Island in March 2011 and March 2012. Two-dimensional (2-D) inversion and 3-D forward modeling reveals a prominent and large zone of relatively high resistivity between 1 to 4 kilometers beneath the <span class="hlt">volcano</span> almost directly beneath the Main Crater, surrounded by zones of relatively low resistivity. This anomalous zone of high resistivity is hypothesized to be a large hydrothermal reservoir filled with volcanic fluids. The presence of this large hydrothermal reservoir could be related to past <span class="hlt">activities</span> of Taal <span class="hlt">Volcano</span>. In particular we believe that the catastrophic explosion described during the 1911 eruption was the result of the hydrothermal reservoir collapsing. During the cycle of Main Crater eruptions, this hydrothermal reservoir is depleted, while during a cycle of flank eruptions this reservoir is replenished with hydrothermal fluids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS31E..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS31E..02M"><span><span class="hlt">Submarine</span> Landslides: A Multidisciplinary Crossroad</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moscardelli, L. G.</p> <p>2014-12-01</p> <p>The study of <span class="hlt">submarine</span> landslides has advanced considerably in the last decade. A multitude of geoscience disciplines, including marine, petroleum and planetary geology, as well as geohazard assessments, are concerned with the study of these units. Oftentimes, researchers working in these fields disseminate their findings within their own communities and a multidisciplinary approach seems to lack. This presentation showcases several case studies in which a broader approach has increased our understanding of <span class="hlt">submarine</span> landslides in a variety of geologic settings. Three-dimensional seismic data from several continental margins (Trinidad, Brazil, Morocco, Canada, GOM), as well as data from outcrop localities are shown to explore geomorphological complexities associated with <span class="hlt">submarine</span> landslides. Discussion associated with the characterization and classification of <span class="hlt">submarine</span> landslides is also part of this work. Topics that will be cover include: 1) how data from conventional oil and gas exploration <span class="hlt">activities</span> can be used to increase our understanding of the dynamic behavior of <span class="hlt">submarine</span> landslides, 2) analogies between terrestrial <span class="hlt">submarine</span> landslides and potential Martian counterparts, 3) impact of <span class="hlt">submarine</span> landslides in margin construction, as well as their economic significance and 4) the importance of quantifying the morphology of <span class="hlt">submarine</span> landslides in a systematic fashion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.sciencedirect.com/science/journal/03770273/150/1','USGSPUBS'); return false;" href="http://www.sciencedirect.com/science/journal/03770273/150/1"><span>Special issue: The changing shapes of <span class="hlt">active</span> <span class="hlt">volcanoes</span>: Recent results and advances in <span class="hlt">volcano</span> geodesy</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.; Newman, Andrew V.</p> <p>2006-01-01</p> <p>The 18 papers herein report on new geodetic data that offer valuable insights into eruptive <span class="hlt">activity</span> and magma transport; they present new models and modeling strategies that have the potential to greatly increase understanding of magmatic, hydrothermal, and <span class="hlt">volcano</span>-tectonic processes; and they describe innovative techniques for collecting geodetic measurements from remote, poorly accessible, or hazardous <span class="hlt">volcanoes</span>. To provide a proper context for these studies, we offer a short review of the evolution of <span class="hlt">volcano</span> geodesy, as well as a case study that highlights recent advances in the field by comparing the geodetic response to recent eruptive episodes at Mount St. Helens. Finally, we point out a few areas that continue to challenge the <span class="hlt">volcano</span> geodesy community, some of which are addressed by the papers that follow and which undoubtedly will be the focus of future research for years to come.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016965','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016965"><span><span class="hlt">Volcano</span> growth and evolution of the island of 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, J.G.; Clague, D.A.</p> <p>1992-01-01</p> <p>The seven <span class="hlt">volcanoes</span> comprising the island of Hawaii and its <span class="hlt">submarine</span> base are, in order of growth, Mahukona, Kohala, Mauna Kea, Hualalai, Mauna Loa, Kilauea, and Loihi. The first four have completed their shield-building stage, and the timing of this event can be determined from the depth of the slope break associated with the end of shield building, calibrated using the ages and depths of a series of dated submerged coral reefs off northwest Hawaii. On each <span class="hlt">volcano</span>, the transition from eruption of tholeiitic to alkalic lava occurs near the end of shield building. The rate of southeastern progression of the end of shield building in the interval from Haleakala to Hualalai is about 13 cm/yr. Based on this rate and an average spacing of <span class="hlt">volcanoes</span> on each loci line of 40-60km, the <span class="hlt">volcanoes</span> required about 600 thousand years to grow from the ocean floor to the time of the end of shield building. They arrive at the ocean surface about midway through this period. -from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.3151C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.3151C"><span>Addressing <span class="hlt">submarine</span> geohazards through scientific drilling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Camerlenghi, A.</p> <p>2009-04-01</p> <p>Natural <span class="hlt">submarine</span> geohazards (earthquakes, volcanic eruptions, landslides, volcanic island flank collapses) are geological phenomena originating at or below the seafloor leading to a situation of risk for off-shore and on-shore structures and the coastal population. Addressing <span class="hlt">submarine</span> geohazards means understanding their spatial and temporal variability, the pre-conditioning factors, their triggers, and the physical processes that control their evolution. Such scientific endeavour is nowadays considered by a large sector of the international scientific community as an obligation in order to contribute to the mitigation of the potentially destructive societal effects of <span class="hlt">submarine</span> geohazards. The study of <span class="hlt">submarine</span> geohazards requires a multi-disciplinary scientific approach: geohazards must be studied through their geological record; <span class="hlt">active</span> processes must be monitored; geohazard evolution must be modelled. Ultimately, the information must be used for the assessment of vulnerability, risk analysis, and development of mitigation strategies. In contrast with the terrestrial environment, the oceanic environment is rather hostile to widespread and fast application of high-resolution remote sensing techniques, accessibility for visual inspection, sampling and installation of monitoring stations. Scientific Drilling through the IODP (including the related pre site-survey investigations, sampling, logging and in situ measurements capability, and as a platform for deployment of long term observatories at the surface and down-hole) can be viewed as the centre of gravity of an international, coordinated, multi-disciplinary scientific approach to address <span class="hlt">submarine</span> geohazards. The IODP Initial Science Plan expiring in 2013 does not address openly geohazards among the program scientific objectives. Hazards are referred to mainly in relation to earthquakes and initiatives towards the understanding of seismogenesis. Notably, the only drilling initiative presently under way is the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1610019R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1610019R"><span>The diversity of mud <span class="hlt">volcanoes</span> in the landscape of Azerbaijan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rashidov, Tofig</p> <p>2014-05-01</p> <p> on surface, often of plane-conical shape, rising for 5 to 400 m and more over the country (for example, mud <span class="hlt">volcano</span> Toragay, 400 m height). The base diameter is from 100 m to 3-4 km and more. Like the magmatic ones, the mud <span class="hlt">volcanoes</span> are crowned with crater of convex-plane or deeply-seated shape. In Azerbaijan there are all types of mud <span class="hlt">volcanoes</span>: <span class="hlt">active</span>, extinct, buried, <span class="hlt">submarine</span>, island, abundantly oil seeping. According to their morphology they are defined into cone-shaped, dome-shaped, ridge-shaped, plateau-shaped. The crater shapes are also various: conical, convex-plane, shield-shaped, deeply-seated, caldera-like. The most complete morphological classification was given in "Atlas of mud <span class="hlt">volcanoes</span> of Azerbaijan" (Yakubov et al., 1971). Recently (Aliyev Ad. et al., 2003) it was proposed a quite new morphological classification of mud <span class="hlt">volcanoes</span> of Azerbaijan. For the first time the mud volcanic manifestations had been defined. <span class="hlt">Volcanoes</span> are ranged according to morphological signs, crater shape and type of <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V23A0590G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V23A0590G"><span>New Insights on <span class="hlt">Submarine</span> Volcanism in the Western Galapagos Archipelago from High Resolution Sonar and Magnetic Surveys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Glass, J. B.; Fornari, D. J.; Tivey, M. A.; Hall, H. F.; Cougan, A. A.; Berkenbosch, H. A.; Holmes, M. L.; White, S. M.; de La Torre, G.</p> <p>2006-12-01</p> <p>We combine high-resolution MR-1 sidescan sonar and EM-300 bathymetric data collected on four cruises (AHA-Nemo2 in 2000 (R/V Melville), DRIFT4 in 2001 (R/V Revelle), TN188 and TN189 in January 2006 (R/V Thompson) to study volcanic platform-building processes on the <span class="hlt">submarine</span> flanks of Fernandina, Isabela, Roca Redonda and Santiago <span class="hlt">volcanoes</span>, in the western Galapagos. Three primary volcanic provinces were identified including: rift zones (16, ranging from 5 to 20 km in length), small <span class="hlt">submarine</span> volcanic cones (<3 km in diameter and several 100 m high) and deep (>3000 m), long (>10 km), large-area <span class="hlt">submarine</span> lava flows. Lengths of the Galapagos rift zones are comparable to western Canary Island rift zones, but significantly shorter than Hawaiian <span class="hlt">submarine</span> rift zones, possibly reflecting lower magma supply. A surface-towed magnetic survey was conducted over the NW Fernandina rift on TN189 and Fourier inversions were performed to correct for topographic effects. Calculated magnetization was highest (up to +32 A/m) over the shallow southwest flank of the rift, coinciding with cone fields and suggesting most recent volcanism has focused at this portion of the rift. Small <span class="hlt">submarine</span> volcanic cones with various morphologies (e.g., pointed, cratered and occasionally breached) are common in the <span class="hlt">submarine</span> western Galapagos both on rift zones and on the island flanks where no rifts are present, such as the northern flank of Santiago Island. Preliminary study of these cones suggests that their morphologies and depth of occurrence may reflect a combination of petrogenetic and eruption processes. Deep, long large-area lava flow fields in regions of low bathymetric relief have been previously identified as a common seafloor feature in the western Galapagos by Geist et al. [in press], and new EM300 data show that a number of the deep lava flows originate from small cones along the mid-lower portion of the NW <span class="hlt">submarine</span> rift of Fernandina. Our high-resolution sonar data suggest that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ready.gov/volcanoes','NIH-MEDLINEPLUS'); return false;" href="https://www.ready.gov/volcanoes"><span><span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://medlineplus.gov/">MedlinePlus</a></p> <p></p> <p></p> <p>... Oregon have the most <span class="hlt">active</span> <span class="hlt">volcanoes</span>, but other states and territories have <span class="hlt">active</span> <span class="hlt">volcanoes</span>, too. A volcanic eruption may involve lava and other debris that can flow up to 100 mph, destroying everything in their ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V22C..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V22C..02D"><span>Cyclic <span class="hlt">Activity</span> of Mud <span class="hlt">Volcanoes</span>: Evidences from Trinidad (SE Caribbean)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deville, E.</p> <p>2007-12-01</p> <p>Fluid and solid transfer in mud <span class="hlt">volcanoes</span> show different phases of <span class="hlt">activity</span>, including catastrophic events followed by periods of relative quiescence characterized by moderate <span class="hlt">activity</span>. This can be notably shown by historical data onshore Trinidad. Several authors have evoked a possible link between the frequencies of eruption of some mud <span class="hlt">volcanoes</span> and seismic <span class="hlt">activity</span>, but in Trinidad there is no direct correlation between mud eruptions and seisms. It appears that each eruptive mud <span class="hlt">volcano</span> has its own period of catastrophic <span class="hlt">activity</span>, and this period is highly variable from one <span class="hlt">volcano</span> to another. The frequency of <span class="hlt">activity</span> of mud <span class="hlt">volcanoes</span> seems essentially controlled by local pressure regime within the sedimentary pile. At the most, a seism can, in some cases, <span class="hlt">activate</span> an eruption close to its term. The dynamics of expulsion of the mud <span class="hlt">volcanoes</span> during the quiescence phases has been studied notably from temperature measurements within the mud conduits. The mud temperature is concurrently controlled by, either, the gas flux (endothermic gas depressurizing induces a cooling effect), or by the mud flux (mud is a vector for convective heat transfer). Complex temperature distribution was observed in large conduits and pools. Indeed, especially in the bigger pools, the temperature distribution characterizes convective cells with an upward displacement of mud above the deep outlet, and ring-shaped rolls associated with the burial of the mud on the flanks of the pools. In simple, tube-like shaped, narrow conduits, the temperature is more regular, but we observed different types of profiles, with either downward increasing or decreasing temperatures. If the upward flow of mud would be regular, we should expect increasing temperatures and progressively decreasing gradient with depth within the conduits. However, the variable measured profiles from one place to another, as well as time-variable measured temperatures within the conduits and especially, at the base of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5114867','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5114867"><span>A distinct source and differentiation history for Kolumbo <span class="hlt">submarine</span> <span class="hlt">volcano</span>, Santorini volcanic field, Aegean arc</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Carey, Steven; Nomikou, Paraskevi; Smet, Ingrid; Godelitsas, Athanasios; Vroon, Pieter</p> <p>2016-01-01</p> <p>Abstract This study reports the first detailed geochemical characterization of Kolumbo <span class="hlt">submarine</span> <span class="hlt">volcano</span> in order to investigate the role of source heterogeneity in controlling geochemical variability within the Santorini volcanic field in the central Aegean arc. Kolumbo, situated 15 km to the northeast of Santorini, last erupted in 1650 AD and is thus closely associated with the Santorini volcanic system in space and time. Samples taken by remotely‐operated vehicle that were analyzed for major element, trace element and Sr‐Nd‐Hf‐Pb isotope composition include the 1650 AD and underlying K2 rhyolitic, enclave‐bearing pumices that are nearly identical in composition (73 wt.% SiO2, 4.2 wt.% K2O). Lava bodies exposed in the crater and enclaves are basalts to andesites (52–60 wt.% SiO2). Biotite and amphibole are common phenocryst phases, in contrast with the typically anhydrous mineral assemblages of Santorini. The strong geochemical signature of amphibole fractionation and the assimilation of lower crustal basement in the petrogenesis of the Kolumbo magmas indicates that Kolumbo and Santorini underwent different crustal differentiation histories and that their crustal magmatic systems are unrelated. Moreover, the Kolumbo samples are derived from a distinct, more enriched mantle source that is characterized by high Nb/Yb (>3) and low 206Pb/204Pb (<18.82) that has not been recognized in the Santorini volcanic products. The strong dissimilarity in both petrogenesis and inferred mantle sources between Kolumbo and Santorini suggests that pronounced source variations can be manifested in arc magmas that are closely associated in space and time within a single volcanic field. PMID:27917071</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27917071','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27917071"><span>A distinct source and differentiation history for Kolumbo <span class="hlt">submarine</span> <span class="hlt">volcano</span>, Santorini volcanic field, Aegean arc.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Klaver, Martijn; Carey, Steven; Nomikou, Paraskevi; Smet, Ingrid; Godelitsas, Athanasios; Vroon, Pieter</p> <p>2016-08-01</p> <p>This study reports the first detailed geochemical characterization of Kolumbo <span class="hlt">submarine</span> <span class="hlt">volcano</span> in order to investigate the role of source heterogeneity in controlling geochemical variability within the Santorini volcanic field in the central Aegean arc. Kolumbo, situated 15 km to the northeast of Santorini, last erupted in 1650 AD and is thus closely associated with the Santorini volcanic system in space and time. Samples taken by remotely-operated vehicle that were analyzed for major element, trace element and Sr-Nd-Hf-Pb isotope composition include the 1650 AD and underlying K2 rhyolitic, enclave-bearing pumices that are nearly identical in composition (73 wt.% SiO 2 , 4.2 wt.% K 2 O). Lava bodies exposed in the crater and enclaves are basalts to andesites (52-60 wt.% SiO 2 ). Biotite and amphibole are common phenocryst phases, in contrast with the typically anhydrous mineral assemblages of Santorini. The strong geochemical signature of amphibole fractionation and the assimilation of lower crustal basement in the petrogenesis of the Kolumbo magmas indicates that Kolumbo and Santorini underwent different crustal differentiation histories and that their crustal magmatic systems are unrelated. Moreover, the Kolumbo samples are derived from a distinct, more enriched mantle source that is characterized by high Nb/Yb (>3) and low 206 Pb/ 204 Pb (<18.82) that has not been recognized in the Santorini volcanic products. The strong dissimilarity in both petrogenesis and inferred mantle sources between Kolumbo and Santorini suggests that pronounced source variations can be manifested in arc magmas that are closely associated in space and time within a single volcanic field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29549332','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29549332"><span>Lack of impact of the El Hierro (Canary Islands) <span class="hlt">submarine</span> volcanic eruption on the local phytoplankton community.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gómez-Letona, M; Arístegui, J; Ramos, A G; Montero, M F; Coca, J</p> <p>2018-03-16</p> <p>The eruption of a <span class="hlt">submarine</span> <span class="hlt">volcano</span> south of El Hierro Island (Canary Islands) in October 2011 led to major physical and chemical changes in the local environment. Large amounts of nutrients were found at specific depths in the water column above the <span class="hlt">volcano</span> associated with suboxic layers resulting from the oxidation of reduced chemical species expelled during the eruptive phase. It has been suggested that the fertilization with these compounds enabled the rapid restoration of the ecosystem in the marine reserve south of the island once the volcanic <span class="hlt">activity</span> ceased, although no biological evidence for this has been provided yet. To test the biological fertilization hypothesis on the pelagic ecosystem, we studied the evolution and variability in chlorophyll a, from in situ and remote sensing data, combined with information on phytoplankton and bacterial community structure during and after the eruptive episode. Remote sensing and in situ data revealed that no phytoplankton bloom took place neither during nor after the eruptive episode. We hypothesize that the fertilization by the <span class="hlt">volcano</span> did not have an effect in the phytoplankton community due to the strong dilution of macro- and micronutrients caused by the efficient renewal of ambient waters in the zone.</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/of/1997/0513/pdf/of1997-0513.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1997/0513/pdf/of1997-0513.pdf"><span><span class="hlt">Volcano</span> hazards at Newberry <span class="hlt">Volcano</span>, 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>Sherrod, David R.; Mastin, Larry G.; Scott, William E.; Schilling, Steven P.</p> <p>1997-01-01</p> <p>Newberry <span class="hlt">volcano</span> is a broad shield <span class="hlt">volcano</span> located in central Oregon. It has been built by thousands of eruptions, beginning about 600,000 years ago. At least 25 vents on the flanks and summit have been <span class="hlt">active</span> during several eruptive episodes of the past 10,000 years. The most recent eruption 1,300 years ago produced the Big Obsidian Flow. Thus, the <span class="hlt">volcano</span>'s long history and recent <span class="hlt">activity</span> indicate that Newberry will erupt in the future. The most-visited part of the <span class="hlt">volcano</span> is Newberry Crater, a volcanic depression or caldera at the summit of the <span class="hlt">volcano</span>. Seven campgrounds, two resorts, six summer homes, and two major lakes (East and Paulina Lakes) are nestled in the caldera. The caldera has been the focus of Newberry's volcanic <span class="hlt">activity</span> for at least the past 10,000 years. Other eruptions during this time have occurred along a rift zone on the <span class="hlt">volcano</span>'s northwest flank and, to a lesser extent, the south flank. Many striking volcanic features lie in Newberry National Volcanic Monument, which is managed by the U.S. Forest Service. The monument includes the caldera and extends along the northwest rift zone to the Deschutes River. About 30 percent of the area within the monument is covered by volcanic products erupted during the past 10,000 years from Newberry <span class="hlt">volcano</span>. Newberry <span class="hlt">volcano</span> is presently quiet. Local earthquake <span class="hlt">activity</span> (seismicity) has been trifling throughout historic time. Subterranean heat is still present, as indicated by hot springs in the caldera and high temperatures encountered during exploratory drilling for geothermal energy. This report describes the kinds of hazardous geologic events that might occur in the future at Newberry <span class="hlt">volcano</span>. A hazard-zonation map is included to show the areas that will most likely be affected by renewed eruptions. In terms of our own lifetimes, volcanic events at Newberry are not of day-to-day concern because they occur so infrequently; however, the consequences of some types of eruptions can be severe. When Newberry</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS13A1707T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS13A1707T"><span>ESR dating of <span class="hlt">submarine</span> hydrothermal <span class="hlt">activities</span> using barite in sulfide deposition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Toyoda, S.; Fujiwara, T.; Ishibashi, J.; Isono, Y.; Uchida, A.; Takamasa, A.; Nakai, S.</p> <p>2012-12-01</p> <p>The temporal change of <span class="hlt">submarine</span> hydrothermal <span class="hlt">activities</span> has been an important issue in the aspect of the evolution of hydrothermal systems which is related with ore formation (Urabe, 1995) and biological systems sustained by the chemical species arising from hydrothermal <span class="hlt">activities</span> (Macdonald et al., 1980). Determining the ages of the hydrothermal deposit will provide essential information on such studies. Dating methods using disequilibrium between radioisotopes such as U-Th method (e.g. You and Bickle, 1998), 226}Ra-{210Pb and 228}Ra-{228Th method (e.g. Noguchi et al., 2011) have been applied to date <span class="hlt">submarine</span> hydrothermal deposits. ESR (electron spin resonance) dating method is commonly applied to fossil teeth, shells, and quartz of Quaternay period where the natural accumulated dose is obtained from the intensities of the ESR signals which are created by natural radiation. The natural dose is divided by the dose rate to the mineral/sample to deduce the age. Okumura et al., (2010) made the first practical application of ESR (electron spin resonance) dating technique to a sample of <span class="hlt">submarine</span> hydrothermal barite (BaSO4) to obtain preliminary ages, where Kasuya et al. (1991) first pointed out that barite can be used for ESR dating. Knowing that ESR dating of barite is promising, in this paper, we will present how we have investigated each factor that contributes ESR dating of barite in <span class="hlt">submarine</span> hydrothermal sulfide deposition. (1) The best ESR condition for measuring the SO3- signal in barite is with the microwave power of 1mW and modulation amplitude of 0.1mT. (2) As results of heating experiments, the signal was found to be stable for the dating age range of several thousands. (3) 226Ra replacing Ba in barite is the source of the radiation. The amount of radioactive elements in sulfide mineral surrounding barite is negligible. (4) The external radiation from the sea water is negligible even in the <span class="hlt">submarine</span> hydrothermal area where the radiation level is much</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA14456.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA14456.html"><span><span class="hlt">Activity</span> at Europe Most <span class="hlt">Active</span> <span class="hlt">Volcano</span> Eyed by NASA Spacecraft</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2016-05-27</p> <p>Mt. Etna, Sicily, Italy, is Europe most <span class="hlt">active</span> <span class="hlt">volcano</span>. In mid-May 2016, Mt. Etna put on a display of lava fountaining, ash clouds and lava flows. Three of the four summit craters were <span class="hlt">active</span>. NASA Terra spacecraft acquired this image on May 26, 2016.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED238672.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED238672.pdf"><span><span class="hlt">Volcanoes</span>.</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>Tilling, Robert I.</p> <p></p> <p>One of a series of general interest publications on science topics, this booklet provides a non-technical introduction to the subject of <span class="hlt">volcanoes</span>. Separate sections examine the nature and workings of <span class="hlt">volcanoes</span>, types of <span class="hlt">volcanoes</span>, volcanic geological structures such as plugs and maars, types of eruptions, volcanic-related <span class="hlt">activity</span> such as geysers…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001954.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001954.html"><span><span class="hlt">Activity</span> at Shiveluch <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>NASA image acquired Sept 7, 2010 Shiveluch (also spelled Sheveluch) is one of the largest and most <span class="hlt">active</span> <span class="hlt">volcanoes</span> on Russia’s Kamchatka Peninsula. It has been spewing ash and steam intermittently—with occasional dome collapses, pyroclastic flows, and lava flows, as well—for the past decade. Shiveluch is a stratovolcano, a steep-sloped formation of alternating layers of hardened lava, ash, and rocks thrown out by earlier eruptions. A lava dome has been growing southwest of the 3,283-meter (10,771-foot) summit. The Advanced Land Imager (ALI) on NASA’s Earth Observing-1 (EO-1) satellite acquired this image on September 7, 2010. Brown and tan debris—perhaps ash falls, perhaps mud from lahars—covers the southern landscape of the <span class="hlt">volcano</span>, while the hills on the northern side remain covered in snow and ice. The Kamchatkan Volcanic Eruption Response Team (KVERT) reported that seismic <span class="hlt">activity</span> at Shiveluch was "above background levels" from September 3-10. Ash plumes rose to an altitude of 6.5 kilometers (21,300 feet) on September 3-4, and gas-and-ash plumes were reported on September 7, when this image was acquired. According to the Smithsonian Institution's <span class="hlt">volcano</span> program, at least 60 large eruptions of Shiveluch have occurred during the current Holocene Epoch of geological history. Intermittent explosive eruptions began in the 1990s, and the largest historical eruptions from Shiveluch occurred in 1854 and 1964. NASA Earth Observatory image created by Jesse Allen and Robert Simmon, using EO-1 ALI data provided courtesy of the NASA EO-1 team. Caption by Mike Carlowicz. Instrument: EO-1 - ALI Credit: NASA Earth Observatory NASA Goddard Space Flight Center contributes to NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s endeavors by providing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Join us on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMNH51C1238C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMNH51C1238C"><span><span class="hlt">Active</span> <span class="hlt">Volcano</span> Monitoring using a Space-based Hyperspectral Imager</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cipar, J. J.; Dunn, R.; Cooley, T.</p> <p>2010-12-01</p> <p><span class="hlt">Active</span> <span class="hlt">volcanoes</span> occur on every continent, often in close proximity to heavily populated areas. While ground-based studies are essential for scientific research and disaster mitigation, remote sensing from space can provide rapid and continuous monitoring of <span class="hlt">active</span> and potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span> [Ramsey and Flynn, 2004]. In this paper, we report on hyperspectral measurements of Kilauea <span class="hlt">volcano</span>, Hawaii. Hyperspectral images obtained by the US Air Force TacSat-3/ARTEMIS sensor [Lockwood et al, 2006] are used to obtain estimates of the surface temperatures for the <span class="hlt">volcano</span>. ARTEMIS measures surface-reflected light in the visible, near-infrared, and short-wave infrared bands (VNIR-SWIR). The SWIR bands are known to be sensitive to thermal radiation [Green, 1996]. For example, images from the NASA Hyperion hyperspectral sensor have shown the extent of wildfires and <span class="hlt">active</span> <span class="hlt">volcanoes</span> [Young, 2009]. We employ the methodology described by Dennison et al, (2006) to obtain an estimate of the temperature of the <span class="hlt">active</span> region of Kilauea. Both day and night-time images were used in the analysis. To improve the estimate, we aggregated neighboring pixels. The <span class="hlt">active</span> rim of the lava lake is clearly discernable in the temperature image, with a measured temperature exceeding 1100o C. The temperature decreases markedly on the exterior of the summit crater. While a long-wave infrared (LWIR) sensor would be ideal for <span class="hlt">volcano</span> monitoring, we have shown that the thermal state of an <span class="hlt">active</span> <span class="hlt">volcano</span> can be monitored using the SWIR channels of a reflective hyperspectral imager. References: Dennison, Philip E., Kraivut Charoensiri, Dar A. Roberts, Seth H. Peterson, and Robert O. Green (2006). Wildfire temperature and land cover modeling using hyperspectral data, Remote Sens. Environ., vol. 100, pp. 212-222. Green, R. O. (1996). Estimation of biomass fire temperature and areal extent from calibrated AVIRIS spectra, in Summaries of the 6th Annual JPL Airborne Earth Science Workshop, Pasadena, CA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015825','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015825"><span>Global data collection and the surveillance of <span class="hlt">active</span> <span class="hlt">volcanoes</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>Ward, P.L.</p> <p>1990-01-01</p> <p>Data relay systems on existing earth-orbiting satellites provide an inexpensive way to collect environmental data from numerous remote sites around the world. This technology could be used effectively for fundamental monitoring of most of the world's <span class="hlt">active</span> <span class="hlt">volcanoes</span>. Such global monitoring would focus attention on the most dangerous <span class="hlt">volcanoes</span> that are likely to significantly impact the geosphere and the biosphere. ?? 1990.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611005D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611005D"><span>Evaluating life-safety risk of fieldwork at New Zealand's <span class="hlt">active</span> <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deligne, Natalia; Jolly, Gill; Taig, Tony; Webb, Terry</p> <p>2014-05-01</p> <p><span class="hlt">Volcano</span> observatories monitor <span class="hlt">active</span> or potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span>. Although the number and scope of remote monitoring instruments and methods continues to grow, in-person field data collection is still required for comprehensive monitoring. Fieldwork anywhere, and especially in mountainous areas, contains an element of risk. However, on <span class="hlt">volcanoes</span> with signs of unrest, there is an additional risk of volcanic <span class="hlt">activity</span> escalating while on site, with potentially lethal consequences. As an employer, a <span class="hlt">volcano</span> observatory is morally and sometimes legally obligated to take reasonable measures to ensure staff safety and to minimise occupational risk. Here we present how GNS Science evaluates life-safety risk for volcanologists engaged in fieldwork on New Zealand <span class="hlt">volcanoes</span> with signs of volcanic unrest. Our method includes several key elements: (1) an expert elicitation for how likely an eruption is within a given time frame, (2) quantification of, based on historical data when possible, given a small, moderate, or large eruption, the likelihood of exposure to near-vent processes, ballistics, or surge at various distances from the vent, and (3) estimate of fatality rate given exposure to these volcanic hazards. The final product quantifies hourly fatality risk at various distances from a volcanic vent; various thresholds of risk (for example, zones with more than 10-5 hourly fatality risk) trigger different levels of required approval to undertake work. Although an element of risk will always be present when conducting fieldwork on potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span>, this is a first step towards providing objective guidance for go/no go decisions for volcanic monitoring.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1998/0582/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1998/0582/report.pdf"><span>Catalog of the historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> of 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>Miller, T.P.; McGimsey, R.G.; Richter, D.H.; Riehle, J.R.; Nye, C.J.; Yount, M.E.; Dumoulin, Julie A.</p> <p>1998-01-01</p> <p>Alaska hosts within its borders over 80 major volcanic centers that have erupted during Holocene time (< 10,000 years). At least 29 of these volcanic centers (table 1) had historical eruptions and 12 additional volcanic centers may have had historical eruptions. Historical in Alaska generally means the period since 1760 when explorers, travelers, and inhabitants kept written records. These 41 volcanic centers have been the source for >265 eruptions reported from Alaska <span class="hlt">volcanoes</span>. With the exception of Wrangell <span class="hlt">volcano</span>, all the centers are in, or near, the Aleutian volcanic arc, which extends 2500 km from Hayes <span class="hlt">volcano</span> 145 km west of Anchorage in the Alaska-Aleutian Range to Buldir Island in the western Aleutian Islands (fig. 1). The volcanic arc, a subduction-related feature associated with underthrusting of the Pacific plate beneath the North American plate is divided between oceanic island arc and continental margin segments, the boundary occurring at about 165° W longitude (fig. 1). An additional 7 volcanic centers in the Aleutian arc (table 2; fig. 1 A) have <span class="hlt">active</span> fumarole fields but no reported historical eruptions.This report discusses the location, physiography and structure, eruptive history, and geology of those <span class="hlt">volcanoes</span> in Alaska that have experienced one or more eruptions that have been recorded in the written history (i.e., in historical time). It is part of the group of catalogs entitled Catalogue of <span class="hlt">Active</span> <span class="hlt">Volcanoes</span> of the World published beginning in 1951 under the auspices of the International Association of Volcanology and Chemistry of the Earth's Interior (IAVCEI). A knowledge of the information contained in such catalogs aids in understanding the type and scale of <span class="hlt">activity</span> that might be expected during a particular eruption, the hazards the eruption may pose, and even the prediction of eruptions. The catalog will thus be of value not only to the inhabitants of Alaska but to government agencies concerned with emergency response, air traffic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007E%26PSL.261..375M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007E%26PSL.261..375M"><span>Triggering and dynamic evolution of the LUSI mud <span class="hlt">volcano</span>, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mazzini, A.; Svensen, H.; Akhmanov, G. G.; Aloisi, G.; Planke, S.; Malthe-Sørenssen, A.; Istadi, B.</p> <p>2007-09-01</p> <p>Mud <span class="hlt">volcanoes</span> are geologically important manifestations of vertical fluid flow and mud eruption in sedimentary basins worldwide. Their formation is predominantly ascribed to release of overpressure from clay- and organic-rich sediments, leading to impressive build-up of mud mountains in <span class="hlt">submarine</span> and subaerial settings. Here we report on a newly born mud <span class="hlt">volcano</span> appearing close to an <span class="hlt">active</span> magmatic complex in a backarc sedimentary basin in Indonesia. The location of the mud <span class="hlt">volcano</span> close to magmatic <span class="hlt">volcanoes</span> results in a high background temperature gradient that triggers mineralogical transformations and geochemical reactions at shallow depth. The eruption of 100 °C mud and gas that started the 29th of May 2006 flooded a large area within the Sidoarjo village in Northeast Java. Thousands of people have so far been evacuated due to the mud flood hazards from the eruption. Since the initial eruption, the flow rate escalated from 5000 to 120,000 m 3/d during the first eleven weeks. Then the erupted volume started to pulsate between almost zero and 120,000 m 3/d in the period August 14 to September 10, whereas it increased dramatically following swarms of earthquakes in September, before reaching almost 180,000 m 3/d in December 2006. Sampling and observations were completed during two fieldwork campaigns on the site. The eruption of boiling water is accompanied by mud, aqueous vapour, CO 2 and CH 4. Based on geochemical and field results, we propose a mechanism where the eruptions started following the 27th of May earthquake due to fracturing and accompanied depressurization of > 100 °C pore fluids from > 1700 m depth. This resulted in the formation of a quasi-hydrothermal system with a geyser-like surface expression and with an <span class="hlt">activity</span> influenced by the regional seismicity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRB..112.8205B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRB..112.8205B"><span><span class="hlt">Volcano</span> flank instability in the Lesser Antilles Arc: Diversity of scale, processes, and temporal recurrence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Boudon, Georges; Le Friant, Anne; Komorowski, Jean-Christophe; Deplus, Christine; Semet, Michel P.</p> <p>2007-08-01</p> <p>The 1997 Boxing Day collapse, a remarkable feature of the ongoing eruption of Soufrière Hills on Montserrat, has prompted new interest in the study of <span class="hlt">volcano</span> stability in the Lesser Antilles. Building on a few cases documented in the literature, we have now identified at least 47 flank collapse events on <span class="hlt">volcanoes</span> of the Caribbean arc where this type of behavior is characteristic and repetitive. About 15 events occurred on <span class="hlt">active</span> <span class="hlt">volcanoes</span> within the last 12,000 years. In the northern part of the arc, flank collapses are repetitive, do not exceed 1 km3 in volume, occur in all directions, and are promoted by intense hydrothermal alteration and well-developed fracturing of the summit part of the edifices. In contrast, infrequent but large sector collapses, with volumes up to tens of km3, are typical of the southern <span class="hlt">volcanoes</span>. They are always directed to the west as a result of the high overall slopes of the islands toward the deep back-arc Grenada Basin. Because Caribbean islands are small, a large part of the resulting debris avalanches have flowed into the sea thus contributing voluminous and sudden inputs of volcaniclastic sediments to the Grenada Basin. Deposits from such <span class="hlt">submarine</span> flows have been identified during the recent AGUADOMAR and CARAVAL oceanographic cruises and traced to their source structures on land. Edifice collapses have a major influence on subsequent volcanic <span class="hlt">activity</span> but also are of high concern because of their tsunamigenic potential.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913517C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913517C"><span>"Mediterranean <span class="hlt">volcanoes</span> vs. chain <span class="hlt">volcanoes</span> in the Carpathians"</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chivarean, Radu</p> <p>2017-04-01</p> <p><span class="hlt">Volcanoes</span> have always represent an attractive subject for students. Europe has a small number of <span class="hlt">volcanoes</span> and Romania has none <span class="hlt">active</span> ones. The curricula is poor in the study of <span class="hlt">volcanoes</span>. We want to make a parallel between the Mediterranean <span class="hlt">active</span> <span class="hlt">volcanoes</span> and the old extinct ones in the Oriental Carpathians. We made an comparison of the two regions in what concerns their genesis, space and time distribution, the specific relief and the impact in the landscape, consequences of their <span class="hlt">activities</span>, etc… The most of the Mediterranean <span class="hlt">volcanoes</span> are in Italy, in the peninsula in Napoli's area - Vezuviu, Campi Flegrei, Puzzoli, volcanic islands in Tirenian Sea - Ischia, Aeolian Islands, Sicily - Etna and Pantelleria Island. Santorini is located in Aegean Sea - Greece. Between Sicily and Tunisia there are 13 underwater <span class="hlt">volcanoes</span>. The island called Vulcano, it has an <span class="hlt">active</span> <span class="hlt">volcano</span>, and it is the origin of the word. Every <span class="hlt">volcano</span> in the world is named after this island, just north of Sicily. Vulcano is the southernmost of the 7 main Aeolian Islands, all volcanic in origin, which together form a small island arc. The cause of the <span class="hlt">volcanoes</span> appears to be a combination of an old subduction event and tectonic fault lines. They can be considered as the origin of the science of volcanology. The volcanism of the Carpathian region is part of the extensive volcanic <span class="hlt">activity</span> in the Mediterranean and surrounding regions. The Carpathian Neogene/Quaternary volcanic arc is naturally subdivided into six geographically distinct segments: Oas, Gutai, Tibles, Calimani, Gurghiu and Harghita. It is located roughly between the Carpathian thrust-and-fold arc to the east and the Transylvanian Basin to the west. It formed as a result of the convergence between two plate fragments, the Transylvanian micro-plate and the Eurasian plate. Volcanic edifices are typical medium-sized andesitic composite <span class="hlt">volcanoes</span>, some of them attaining the caldera stage, complicated by submittal or peripheral domes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPA43C2207T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPA43C2207T"><span>A Broadly-Based Training Program in <span class="hlt">Volcano</span> Hazards Monitoring at the Center for the Study of <span class="hlt">Active</span> <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thomas, D. M.; Bevens, D.</p> <p>2015-12-01</p> <p>The Center for the Study of <span class="hlt">Active</span> <span class="hlt">Volcanoes</span>, in cooperation with the USGS <span class="hlt">Volcano</span> Hazards Program at HVO and CVO, offers a broadly based <span class="hlt">volcano</span> hazards training program targeted toward scientists and technicians from developing nations. The program has been offered for 25 years and provides a hands-on introduction to a broad suite of <span class="hlt">volcano</span> monitoring techniques, rather than detailed training with just one. The course content has evolved over the life of the program as the needs of the trainees have changed: initially emphasizing very basic monitoring techniques (e.g. precise leveling, interpretation of seismic drum records, etc.) but, as the level of sophistication of the trainees has increased, training in more advanced technologies has been added. Currently, topics of primary emphasis have included <span class="hlt">volcano</span> seismology and seismic networks; acquisition and modeling of geodetic data; methods of analysis and monitoring of gas geochemistry; interpretation of volcanic deposits and landforms; training in LAHARZ, GIS mapping of lahar risks; and response to and management of volcanic crises. The course also provides training on public outreach, based on CSAV's Hawaii-specific hazards outreach programs, and <span class="hlt">volcano</span> preparedness and interactions with the media during volcanic crises. It is an intensive eight week course with instruction and field <span class="hlt">activities</span> underway 6 days per week; it is now offered in two locations, Hawaii Island, for six weeks, and the Cascades <span class="hlt">volcanoes</span> of the Pacific Northwest, for two weeks, to enable trainees to experience field conditions in both basaltic and continental volcanic environments. The survival of the program for more than two decades demonstrates that a need for such training exists and there has been interaction and contribution to the program by the research community, however broader engagement with the latter continues to present challenges. Some of the reasons for this will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22628652','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22628652"><span>Linking petrology and seismology at an <span class="hlt">active</span> <span class="hlt">volcano</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saunders, Kate; Blundy, Jon; Dohmen, Ralf; Cashman, Kathy</p> <p>2012-05-25</p> <p>Many <span class="hlt">active</span> <span class="hlt">volcanoes</span> exhibit changes in seismicity, ground deformation, and gas emissions, which in some instances arise from magma movement in the crust before eruption. An enduring challenge in <span class="hlt">volcano</span> monitoring is interpreting signs of unrest in terms of the causal subterranean magmatic processes. We examined over 300 zoned orthopyroxene crystals from the 1980-1986 eruption of Mount St. Helens that record pulsatory intrusions of new magma and volatiles into an existing larger reservoir before the eruption occurred. Diffusion chronometry applied to orthopyroxene crystal rims shows that episodes of magma intrusion correlate temporally with recorded seismicity, providing evidence that some seismic events are related to magma intrusion. These time scales are commensurate with monitoring signals at restless <span class="hlt">volcanoes</span>, thus improving our ability to forecast volcanic eruptions by using petrology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V13I..04R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V13I..04R"><span>Magmatically Greedy Reararc <span class="hlt">Volcanoes</span> of the N. Tofua Segment of the Tonga Arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rubin, K. H.; Embley, R. W.; Arculus, R. J.; Lupton, J. E.</p> <p>2013-12-01</p> <p>Volcanism along the northernmost Tofua Arc is enigmatic because edifices of the arc's volcanic front are mostly, magmatically relatively anemic, despite the very high convergence rate of the Pacific Plate with this section of Tonga Arc. However, just westward of the arc front, in terrain generally thought of as part of the adjacent NE Lau Backarc Basin, lie a series of very <span class="hlt">active</span> <span class="hlt">volcanoes</span> and volcanic features, including the large <span class="hlt">submarine</span> caldera Niuatahi (aka <span class="hlt">volcano</span> 'O'), a large composite dacite lava flow terrain not obviously associated with any particular volcanic edifice, and the Mata <span class="hlt">volcano</span> group, a series of 9 small elongate <span class="hlt">volcanoes</span> in an extensional basin at the extreme NE corner of the Lau Basin. These three volcanic terrains do not sit on arc-perpendicular cross chains. Collectively, these volcanic features appear to be receiving a large proportion of the magma flux from the sub-Tonga/Lau mantle wedge, in effect 'stealing' this magma flux from the arc front. A second occurrence of such magma 'capture' from the arc front occurs in an area just to the south, on southernmost portion of the Fonualei Spreading Center. Erupted compositions at these 'magmatically greedy' <span class="hlt">volcanoes</span> are consistent with high slab-derived fluid input into the wedge (particularly trace element abundances and volatile contents, e.g., see Lupton abstract this session). It is unclear how long-lived a feature this is, but the very presence of such hyperactive and areally-dispersed volcanism behind the arc front implies these <span class="hlt">volcanoes</span> are not in fact part of any focused spreading/rifting in the Lau Backarc Basin, and should be thought of as 'reararc <span class="hlt">volcanoes</span>'. Possible tectonic factors contributing to this unusually productive reararc environment are the high rate of convergence, the cold slab, the highly disorganized extension in the adjacent backarc, and the tear in the subducting plate just north of the Tofua Arc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gip/79/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gip/79/"><span>Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Venezky, Dina Y.; Murray, Tom; Read, Cyrus</p> <p>2008-01-01</p> <p>Steam plume from the 2006 eruption of Augustine <span class="hlt">volcano</span> in Cook Inlet, Alaska. Explosive ash-producing eruptions from Alaska's 40+ historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> pose hazards to aviation, including commercial aircraft flying the busy North Pacific routes between North America and Asia. The Alaska <span class="hlt">Volcano</span> Observatory (AVO) monitors these <span class="hlt">volcanoes</span> to provide forecasts of eruptive <span class="hlt">activity</span>. AVO is a joint program of the U.S. Geological Survey (USGS), the Geophysical Institute of the University of Alaska Fairbanks (UAFGI), and the State of Alaska Division of Geological and Geophysical Surveys (ADGGS). AVO is one of five USGS <span class="hlt">Volcano</span> Hazards Program observatories that monitor U.S. <span class="hlt">volcanoes</span> for science and public safety. Learn more about Augustine <span class="hlt">volcano</span> and AVO at http://www.avo.alaska.edu.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2927L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2927L"><span>The <span class="hlt">volcano</span>-sedimentary succession of Upper Permian in Wuli area, central Qinghai-Tibetan Plateau: Sedimentology, geochemistry and paleogeography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Shengqian; Jiang, Zaixing; Gao, Yi</p> <p>2017-04-01</p> <p>Detailed observations on cores and thin sections well documented a <span class="hlt">volcano</span>-sedimentary succession from Well TK2, which is located in Wuli area, central Qinghai-Tibetan Plateau. The TK2 <span class="hlt">volcano</span>-sedimentary succession reflects an <span class="hlt">active</span> sedimentary-tectonic setting in the north margin of North Qiangtang-Chamdo terrane in the late Permian epoch. Based on the observation and recognition on lithology and mineralogy, the components of TK2 succession are mainly volcanic and volcaniclastic rocks and four main lithofacies are recognized, including massive volcanic lithofacies (LF1), pyroclastic tuff lithofacies (LF2), tuffaceous sandstone lithofacies (LF3) and mudstone lithofacies (LF4). LF1 is characterized by felsic components, massive structure and porphyrotopic structure with local flow structure, which indicates <span class="hlt">submarine</span> intrusive domes or extrusion-fed lavas that formed by magma ascents via faults or dykes. Meanwhile, its eruption style may reflect a relative high pressure compensation level (PCL) that mainly determined by water depth, which implies a deep-water environment. LF2 is composed of volcanic lapilli or ash and featured with massive structure, parallel bedding and various deformed laminations including convolve structure, slide deformation, ball-and-pillow structure, etc.. LF2 indicates the sedimentation of initial or reworked explosive products not far away from <span class="hlt">volcano</span> centers, reflecting the proximal accumulation of <span class="hlt">volcano</span> eruption-fed clasts or their resedimentation as debris flows. In addition, the <span class="hlt">submarine</span> <span class="hlt">volcano</span> eruptions may induced earthquakes that facilitate the resedimentation of unconsolidated sediments. LF3 contains abundant pyroclastic components and is commonly massive with rip-up mudstone clasts or usually interbedded with LF4. In addition, typical flute casts, scour structures and graded beddings in thin-interbedded layers of sandstone and mudstone are commonly observed, which also represents the sedimentation of debris flows or</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=archimedes+AND+principle&pg=2&id=EJ659984','ERIC'); return false;" href="https://eric.ed.gov/?q=archimedes+AND+principle&pg=2&id=EJ659984"><span>Making a <span class="hlt">Submarine</span>.</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>Cornacchia, Deborah J.</p> <p>2002-01-01</p> <p>Describes Archimedes principle and why a ship sinks when it gets a hole in it. Suggests an <span class="hlt">activity</span> for teaching the concept of density and water displacement through the construction of a simple <span class="hlt">submarine</span>. Includes materials and procedures for this <span class="hlt">activity</span>. (KHR)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V13C2870A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V13C2870A"><span><span class="hlt">Volcanoes</span> Distribution in Linear Segmentation of Mariana Arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andikagumi, H.; Macpherson, C.; McCaffrey, K. J. W.</p> <p>2016-12-01</p> <p>A new method has been developed to describe better <span class="hlt">volcanoes</span> distribution pattern within Mariana Arc. A previous study assumed the distribution of <span class="hlt">volcanoes</span> in the Mariana Arc is described by a small circle distribution which reflects the melting processes in a curved subduction zone. The small circle fit to this dataset used in the study, comprised 12 -mainly subaerial- <span class="hlt">volcanoes</span> from Smithsonian Institute Global Volcanism Program, was reassessed by us to have a root-mean-square misfit of 2.5 km. The same method applied to a more complete dataset from Baker et al. (2008), consisting 37 subaerial and <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>, resulted in an 8.4 km misfit. However, using the Hough Transform method on the larger dataset, lower misfits of great circle segments were achieved (3.1 and 3.0 km) for two possible segments combination. The results indicate that the distribution of <span class="hlt">volcanoes</span> in the Mariana Arc is better described by a great circle pattern, instead of small circle. Variogram and cross-variogram analysis on <span class="hlt">volcano</span> spacing and volume shows that there is spatial correlation between <span class="hlt">volcanoes</span> between 420 and 500 km which corresponds to the maximum segmentation lengths from Hough Transform (320 km). Further analysis of <span class="hlt">volcano</span> spacing by the coefficient of variation (Cv), shows a tendency toward not-random distribution as the Cv values are closer to zero than one. These distributions are inferred to be associated with the development of normal faults at the back arc as their Cv values also tend towards zero. To analyse whether <span class="hlt">volcano</span> spacing is random or not, Cv values were simulated using a Monte Carlo method with random input. Only the southernmost segment has allowed us to reject the null hypothesis that <span class="hlt">volcanoes</span> are randomly spaced at 95% confidence level by 0.007 estimated probability. This result shows infrequent regularity in <span class="hlt">volcano</span> spacing by chance so that controlling factor in lithospheric scale should be analysed with different approach (not from random</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.T42B0938K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.T42B0938K"><span>The Leading Edge of the Galapagos Hotspot: Geochemistry and Geochronology of <span class="hlt">Submarine</span> Glasses Coupled to New Sidescan Sonar Imagery</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kurz, M. D.; Fornari, D. J.; Geist, D. J.; Johnson, P. D.; Curtice, J. M.; Lott, D. E.; Harpp, K.; Saal, A. E.; Peckman, U. G.</p> <p>2001-12-01</p> <p>Fernandina, the western-most <span class="hlt">volcano</span> in the Galapagos archipelago, is at the leading edge of the hotspot with respect to plate motion. Recent mapping of the ocean floor west of Fernandina (on R/V Revelle, using the HMRG towed sidescan sonar MR1, and Simrad EM120 multibeam) provides a dramatic new view of the volcanic constructional processes that have created the islands. The western flank of the <span class="hlt">volcano</span> is characterized by the prominent Northwest, West, and Southwest rift zones, which are constructed of hummocky pillow lavas. Older lava flow terrain is distinguished by weaker acoustic return, whereas extensive younger flows are characterized by strong backscatter patterns with distinctive flow-like margins. MR1 sidescan sonar mapping provides an important new geologic and stratigraphic context for understanding the <span class="hlt">submarine</span> Galapagos platform, particularly from a geochemical perspective. Fernandina lavas have high 3He/4He ratios, up to 29 times atmospheric, and solar-like neon isotopic compositions, characteristics which suggest they are derived from the deep mantle. The high 3He/4He ratios, and rapid eruption rates at Fernandina also indicate that it lies directly above the center of the Galapagos hotspot. In order to place these geochemical data into a chronological framework, we have determined ages for Fernandina <span class="hlt">submarine</span> glasses using the Th-U-He crushing/melting disequilibrium method. Preliminary Th-U-He ages (from the 2000 R/V Melville AHA-Nemo expedition), combined with the new MR1 sonar mapping, shows that the rift zones are characterized by extremely young ages (0 to 30 Ka) while older <span class="hlt">submarine</span> lava flows with lower acoustic backscatter have significantly older ages ( ~ 100 Ka). The geochronological data, and the geological context from the side-scan sonar, provide new evidence for <span class="hlt">volcano</span> growth rates in oceanic hotspot provinces, and will be used to determine the growth rate of the Galapagos platform.</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://hdl.handle.net/2060/19770011592','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770011592"><span>Catalogue of satellite photography of the <span class="hlt">active</span> <span class="hlt">volcanoes</span> of the world</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Heiken, G.</p> <p>1976-01-01</p> <p>A catalogue is presented of <span class="hlt">active</span> <span class="hlt">volcanoes</span> as viewed from Earth-orbiting satellites. The listing was prepared of photographs, which have been screened for quality, selected from the earth resources technology satellite (ERTS) and Skylab, Apollo and Gemini spacecraft. There is photography of nearly every <span class="hlt">active</span> <span class="hlt">volcano</span> in the world; the photographs are particularly useful for regional studies of volcanic fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://ngmdb.usgs.gov/Prodesc/proddesc_82895.htm','USGSPUBS'); return false;" href="http://ngmdb.usgs.gov/Prodesc/proddesc_82895.htm"><span>Database for the Geologic Map of the Summit Region of Kilauea <span class="hlt">Volcano</span>, 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>Dutton, Dillon R.; Ramsey, David W.; Bruggman, Peggy E.; Felger, Tracey J.; Lougee, Ellen; Margriter, Sandy; Showalter, Patrick; Neal, Christina A.; Lockwood, John P.</p> <p>2007-01-01</p> <p>INTRODUCTION The area covered by this map includes parts of four U.S. Geological Survey (USGS) 7.5' topographic quadrangles (Kilauea Crater, <span class="hlt">Volcano</span>, Ka`u Desert, and Makaopuhi). It encompasses the summit, upper rift zones, and Koa`e Fault System of Kilauea <span class="hlt">Volcano</span> and a part of the adjacent, southeast flank of Mauna Loa <span class="hlt">Volcano</span>. The map is dominated by products of eruptions from Kilauea <span class="hlt">Volcano</span>, the southernmost of the five <span class="hlt">volcanoes</span> on the Island of Hawai`i and one of the world's most <span class="hlt">active</span> <span class="hlt">volcanoes</span>. At its summit (1,243 m) is Kilauea Crater, a 3 km-by-5 km collapse caldera that formed, possibly over several centuries, between about 200 and 500 years ago. Radiating away from the summit caldera are two linear zones of intrusion and eruption, the east and the southwest rift zones. Repeated subaerial eruptions from the summit and rift zones have built a gently sloping, elongate shield <span class="hlt">volcano</span> covering approximately 1,500 km2. Much of the <span class="hlt">volcano</span> lies under water: the east rift zone extends 110 km from the summit to a depth of more than 5,000 m below sea level; whereas, the southwest rift zone has a more limited <span class="hlt">submarine</span> continuation. South of the summit caldera, mostly north-facing normal faults and open fractures of the Koa`e Fault System extend between the two rift zones. The Koa`e Fault System is interpreted as a tear-away structure that accommodates southward movement of Kilauea's flank in response to distension of the <span class="hlt">volcano</span> perpendicular to the rift zones. This digital release contains all the information used to produce the geologic map published as USGS Geologic Investigations Series I-2759 (Neal and Lockwood, 2003). The main component of this digital release is a geologic map database prepared using ArcInfo GIS. This release also contains printable files for the geologic map and accompanying descriptive pamphlet from I-2759.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V21E2371O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V21E2371O"><span>Risk-Free <span class="hlt">Volcano</span> Observations Using an Unmanned Autonomous Helicopter: seismic observations near the <span class="hlt">active</span> vent of Sakurajima <span class="hlt">volcano</span>, Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ohminato, T.; Kaneko, T.; Koyama, T.; Yasuda, A.; Watanabe, A.; Takeo, M.; Honda, Y.; Kajiwara, K.; Kanda, W.; Iguchi, M.; Yanagisawa, T.</p> <p>2010-12-01</p> <p>Observations in the vicinity of summit area of <span class="hlt">active</span> <span class="hlt">volcanoes</span> are important not only for understanding physical processes in the volcanic conduit but also for eruption prediction and volcanic hazards mitigation. It is, however, challenging to install observation sensors near <span class="hlt">active</span> vents because of the danger of sudden eruptions. We need safe and efficient ways of installing sensors near the summit of <span class="hlt">active</span> <span class="hlt">volcanoes</span>. We have been developing an <span class="hlt">volcano</span> observation system based on an unmanned autonomous vehicle (UAV) for risk-free <span class="hlt">volcano</span> observations. Our UAV is an unmanned autonomous helicopter manufactured by Yamaha-Motor Co., Ltd. The UAV is 3.6m long and weighs 84kg with maximum payload of 10kg. The UAV can aviate autonomously along a previously programmed path within a meter accuracy using real-time kinematics differential GPS equipment. The maximum flight time and distance from the operator are 90 minutes and 5km, respectively. We have developed various types of <span class="hlt">volcano</span> observation techniques adequate for the UAV, such as aeromagnetic survey, taking infrared and visible images from onboard high-resolution cameras, volcanic ash sampling in the vicinity of <span class="hlt">active</span> vents. Recently, we have developed an earthquake observation module (EOM), which is exclusively designed for the UAV installation in the vicinity of <span class="hlt">active</span> volcanic vent. In order to meet the various requirements for UAV installation, the EOM is very compact, light-weight (5-6kg), and is solar-powered. It is equipped with GPS for timing, a communication device using cellular-phone network, and triaxial accelerometers. Our first application of the EOM installation using the UAV is one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Japan, Sakurajima <span class="hlt">volcano</span>. Since 2006, explosive eruptions have been continuing at the reopened Showa crater at the eastern flank near the summit of Sakurajima. Entering the area within 2 km from the <span class="hlt">active</span> craters is prohibited, and thus there were no observation station in the vicinity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V44A..05V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V44A..05V"><span>Vailulu'u Seamount, Samoa: Life and Death at the Edge of An <span class="hlt">Active</span> <span class="hlt">Submarine</span> <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vailulu'U Research Group, T.</p> <p>2005-12-01</p> <p>Exploration of Vailulu'u seamount (14°13'S; 169°04'W) by manned submersible, ROV, and surface ship revealed a new, 300m tall <span class="hlt">volcano</span> that has grown in the summit crater in less than four years. This shows that Vailulu'u's eruption behavior is at this stage not predictable and continued growth could allow Vailulu'u to breach sea level within decades Several types of hydrothermal vents fill Vailulu'u crater with particulates that reduce visibility to less than a few meters in some regions. Hydrothermal solutions mix with seawater that enters the crater from its breaches to produce distinct biological habitats. Low temperature hydrothermal vents can produce Fe-oxide chimneys or up to one meter-thick microbial mats. Higher temperature vents (85°C) produce low salinity acidic fluids containing buoyant droplets of immiscible CO2. Low temperature hydrothermal vents at Nafanua summit (708m depth) support a thriving population of eels (Dysommia rusosa). The areas around the high temperature vents and the moat and remaining crater around the new <span class="hlt">volcano</span> is almost devoid of any macroscopic life and is littered with fish, and mollusk carcasses that apparently died from exposure to hydrothermal fluid components in deeper crater waters. Acid- tolerant polychaetes adapt to this environment and feed near and on these carcasses. Vailulu'u presents a natural laboratory for the study of how seamounts and their volcanic systems interact with the hydrosphere to produce distinct biological habitats, and how marine life can adapt to these conditions or be trapped in a toxic volcanic system that leads to mass mortality. The Vailulu'u research team: Hubert Staudigel, Samantha Allen, Brad Bailey, Ed Baker, Sandra Brooke, Ryan Delaney, Blake English, Lisa Haucke, Stan Hart, John Helly, Ian Hudson, Matt Jackson, Daniel Jones, Alison Koleszar, Anthony Koppers, Jasper Konter, Laurent Montesi, Adele Pile, Ray Lee, Scott Mcbride, Julie Rumrill, Daniel Staudigel, Brad Tebo, Alexis Templeton</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810029485&hterms=Kilauea+volcano&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DKilauea%2Bvolcano','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810029485&hterms=Kilauea+volcano&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DKilauea%2Bvolcano"><span>Output rate of magma from <span class="hlt">active</span> central <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wadge, G.</p> <p>1980-01-01</p> <p>For part of their historic records, nine of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> on earth have each erupted magma at a nearly constant rate. These output rates are very similar and range from 0.69 to 0.26 cu m/s. The <span class="hlt">volcanoes</span> discussed - Kilauea, Mauna Loa, Fuego, Santiaguito, Nyamuragira, Hekla, Piton de la Fournaise, Vesuvius and Etna - represent almost the whole spectrum of plate tectonic settings of volcanism. A common mechanism of buoyantly rising magma-filled cracks in the upper crust may contribute to the observed restricted range of the rates of output.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29358665','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29358665"><span>Anaerobic methanotrophic communities thrive in deep <span class="hlt">submarine</span> permafrost.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Winkel, Matthias; Mitzscherling, Julia; Overduin, Pier P; Horn, Fabian; Winterfeld, Maria; Rijkers, Ruud; Grigoriev, Mikhail N; Knoblauch, Christian; Mangelsdorf, Kai; Wagner, Dirk; Liebner, Susanne</p> <p>2018-01-22</p> <p>Thawing <span class="hlt">submarine</span> permafrost is a source of methane to the subsurface biosphere. Methane oxidation in <span class="hlt">submarine</span> permafrost sediments has been proposed, but the responsible microorganisms remain uncharacterized. We analyzed archaeal communities and identified distinct anaerobic methanotrophic assemblages of marine and terrestrial origin (ANME-2a/b, ANME-2d) both in frozen and completely thawed <span class="hlt">submarine</span> permafrost sediments. Besides archaea potentially involved in anaerobic oxidation of methane (AOM) we found a large diversity of archaea mainly belonging to Bathyarchaeota, Thaumarchaeota, and Euryarchaeota. Methane concentrations and δ 13 C-methane signatures distinguish horizons of potential AOM coupled either to sulfate reduction in a sulfate-methane transition zone (SMTZ) or to the reduction of other electron acceptors, such as iron, manganese or nitrate. Analysis of functional marker genes (mcrA) and fluorescence in situ hybridization (FISH) corroborate potential <span class="hlt">activity</span> of AOM communities in <span class="hlt">submarine</span> permafrost sediments at low temperatures. Modeled potential AOM consumes 72-100% of <span class="hlt">submarine</span> permafrost methane and up to 1.2 Tg of carbon per year for the total expected area of <span class="hlt">submarine</span> permafrost. This is comparable with AOM habitats such as cold seeps. We thus propose that AOM is <span class="hlt">active</span> where <span class="hlt">submarine</span> permafrost thaws, which should be included in global methane budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA02509.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA02509.html"><span>Galileo Near-Infrared Mapping Spectrometer Detects <span class="hlt">Active</span> Lava Flows at Prometheus <span class="hlt">Volcano</span>, Io</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1999-11-04</p> <p>The <span class="hlt">active</span> <span class="hlt">volcano</span> Prometheus on Jupiter moon Io was imaged by NASA Galileo spacecraft during the close flyby of Io on Oct.10, 1999. The spectrometer can detect <span class="hlt">active</span> <span class="hlt">volcanoes</span> on Io by measuring their heat in the near-infrared wavelengths.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1225/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1225/"><span>Digital Data for <span class="hlt">Volcano</span> Hazards at Newberry <span class="hlt">Volcano</span>, 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>Schilling, S.P.; Doelger, S.; Sherrod, D.R.; Mastin, L.G.; Scott, W.E.</p> <p>2008-01-01</p> <p>Newberry <span class="hlt">volcano</span> is a broad shield <span class="hlt">volcano</span> located in central Oregon, the product of thousands of eruptions, beginning about 600,000 years ago. At least 25 vents on the flanks and summit have been <span class="hlt">active</span> during the past 10,000 years. The most recent eruption 1,300 years ago produced the Big Obsidian Flow. Thus, the <span class="hlt">volcano</span>'s long history and recent <span class="hlt">activity</span> indicate that Newberry will erupt in the future. Newberry Crater, a volcanic depression or caldera has been the focus of Newberry's volcanic <span class="hlt">activity</span> for at least the past 10,000 years. Newberry National Volcanic Monument, which is managed by the U.S. Forest Service, includes the caldera and extends to the Deschutes River. Newberry <span class="hlt">volcano</span> is quiet. Local earthquake <span class="hlt">activity</span> (seismicity) has been trifling throughout historic time. Subterranean heat is still present, as indicated by hot springs in the caldera and high temperatures encountered during exploratory drilling for geothermal energy. The report USGS Open-File Report 97-513 (Sherrod and others, 1997) describes the kinds of hazardous geologic events that might occur in the future at Newberry <span class="hlt">volcano</span>. A hazard-zonation map is included to show the areas that will most likely be affected by renewed eruptions. When Newberry <span class="hlt">volcano</span> becomes restless, the eruptive scenarios described herein can inform planners, emergency response personnel, and citizens about the kinds and sizes of events to expect. The geographic information system (GIS) <span class="hlt">volcano</span> hazard data layers used to produce the Newberry <span class="hlt">volcano</span> hazard map in USGS Open-File Report 97-513 are included in this data set. Scientists at the USGS Cascades <span class="hlt">Volcano</span> Observatory created a GIS data layer to depict zones subject to the effects of an explosive pyroclastic eruption (tephra fallout, pyroclastic flows, and ballistics), lava flows, volcanic gasses, and lahars/floods in Paulina Creek. A separate GIS data layer depicts drill holes on the flanks of Newberry <span class="hlt">Volcano</span> that were used to estimate the probability</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2004/3084/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2004/3084/"><span>The Alaska <span class="hlt">Volcano</span> Observatory - Expanded Monitoring of <span class="hlt">Volcanoes</span> Yields Results</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brantley, Steven R.; McGimsey, Robert G.; Neal, Christina A.</p> <p>2004-01-01</p> <p>Recent explosive eruptions at some of Alaska's 52 historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> have significantly affected air traffic over the North Pacific, as well as Alaska's oil, power, and fishing industries and local communities. Since its founding in the late 1980s, the Alaska <span class="hlt">Volcano</span> Observatory (AVO) has installed new monitoring networks and used satellite data to track <span class="hlt">activity</span> at Alaska's <span class="hlt">volcanoes</span>, providing timely warnings and monitoring of frequent eruptions to the aviation industry and the general public. To minimize impacts from future eruptions, scientists at AVO continue to assess <span class="hlt">volcano</span> hazards and to expand monitoring networks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.V51C2045G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.V51C2045G"><span>An <span class="hlt">active</span> seismic experiment at Tenerife Island (Canary Island, Spain): Imaging an <span class="hlt">active</span> <span class="hlt">volcano</span> edifice</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garcia-Yeguas, A.; Ibañez, J. M.; Rietbrock, A.; Tom-Teidevs, G.</p> <p>2008-12-01</p> <p>An <span class="hlt">active</span> seismic experiment to study the internal structure of Teide <span class="hlt">Volcano</span> was carried out on Tenerife, a volcanic island in Spain's Canary Islands. The main objective of the TOM-TEIDEVS experiment is to obtain a 3-dimensional structural image of Teide <span class="hlt">Volcano</span> using seismic tomography and seismic reflection/refraction imaging techniques. At present, knowledge of the deeper structure of Teide and Tenerife is very limited, with proposed structural models mainly based on sparse geophysical and geological data. This multinational experiment which involves institutes from Spain, Italy, the United Kingdom, Ireland, and Mexico will generate a unique high resolution structural image of the <span class="hlt">active</span> <span class="hlt">volcano</span> edifice and will further our understanding of volcanic processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994JGR....99.9487M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994JGR....99.9487M"><span>Paleomagnetic evidence for high-temperature emplacement of the 1883 subaqueous pyroclastic flows from Krakatau <span class="hlt">Volcano</span>, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mandeville, Charles W.; Carey, Steven; Sigurdsson, Haraldur; King, John</p> <p>1994-05-01</p> <p>The paroxysmal 1883 eruption of Krakatau <span class="hlt">volcano</span> in Indonesia discharge at least 6.5 cu km (dense rock equivalent) of pyroclastic material into the shallow waters of the Sunda Straits within a 15-km radius of the <span class="hlt">volcano</span>. Progressive thermal demagnetization studies of individually oriented pumice clasts from a core sample of the <span class="hlt">submarine</span> pyroclastic deposits show that 41 out of 47 clasts exhibit single-component remanence with mean inclination of -24 deg. The partial thermoremanent magnetization components of both pumice and lithic clasts are well grouped in orientation, indicating that substantial cooling of clasts must have occurred following deposition. Estimated subaqueous emplacement temperature for such clasts is greater than 500 C. Rare two-component lithic fragments exhibit inflection points on vector endpoint diagrams that mark the temperature below which the fragments acquired magnetization of similar orientation. These inflection points range from 350 to 550 C, indicating a minimum subaqueous emplacement temperature of 350 C. Paleomagnetic evidence for high-emplacement temperature supports the hypothesis that proximal 1883 <span class="hlt">submarine</span> pyroclastic deposits resulted from entrance of hot, subaerially generated pyroclastic flows into the sea. Similar deposits have been interpreted from the geologic record, but this is the first documented example of <span class="hlt">submarine</span> pyroclastic flows from a historic eruption. The Kratatau deposits thus serve as an important modern analog for the study of pyroclastic flow/seawater interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002176.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e002176.html"><span>Soufriere Hills <span class="hlt">Volcano</span> Resumes <span class="hlt">Activity</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>A massive eruption of Montserrat’s Soufrière Hills <span class="hlt">Volcano</span> covered large portions of the island in debris. The eruption was triggered by a collapse of Soufrière Hills’ summit lava dome on February 11, 2010. Pyroclastic flows raced down the northern flank of the <span class="hlt">volcano</span>, leveling trees and destroying buildings in the village of Harris, which was abandoned after Soufrière Hills became <span class="hlt">active</span> in 1995. The Montserrat <span class="hlt">Volcano</span> Observatory reported that some flows, about 15 meters (49 feet) thick, reached the sea at Trant’s Bay. These flows extended the island’s coastline up to 650 meters (2,100 feet). These false-color satellite images show the southern half of Montserrat before and after the dome collapse. The top image shows Montserrat on February 21, 2010, just 10 days after the event. For comparison, the bottom image shows the same area on March 17, 2007. Red areas are vegetated, clouds are white, blue/black areas are ocean water, and gray areas are covered by flow deposits. Fresh deposits tend to be lighter than older deposits. On February 21, the drainages leading down from Soufrière Hills, including the White River Valley, the Tar River Valley, and the Belham River Valley, were filled with fresh debris. According to the Montserrat <span class="hlt">Volcano</span> Observatory, pyroclastic flows reached the sea through Aymers Ghaut on January 18, 2010, and flows entered the sea near Plymouth on February 5, 2010. NASA Earth Observatory image by Robert Simmon, using data from the NASA/GSFC/METI/ERSDAC/JAROS, and U.S./Japan ASTER Science Team. Caption by Robert Simmon. To read more go to: earthobservatory.nasa.gov/IOTD/view.php?id=42792 NASA Goddard Space Flight Center is home to the nation's largest organization of combined scientists, engineers and technologists that build spacecraft, instruments and new technology to study the Earth, the sun, our solar system, and the universe. Follow us on Twitter Join us on Facebook</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT........84S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT........84S"><span>Degassing Processes at Persistently <span class="hlt">Active</span> Explosive <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smekens, Jean-Francois</p> <p></p> <p>Among volcanic gases, sulfur dioxide (SO2) is by far the most commonly measured. More than a monitoring proxy for volcanic degassing, SO 2 has the potential to alter climate patterns. Persistently <span class="hlt">active</span> explosive <span class="hlt">volcanoes</span> are characterized by short explosive bursts, which often occur at periodic intervals numerous times per day, spanning years to decades. SO 2 emissions at those <span class="hlt">volcanoes</span> are poorly constrained, in large part because the current satellite monitoring techniques are unable to detect or quantify plumes of low concentration in the troposphere. Eruption plumes also often show high concentrations of ash and/or aerosols, which further inhibit the detection methods. In this work I focus on quantifying volcanic gas emissions at persistently <span class="hlt">active</span> explosive <span class="hlt">volcanoes</span> and their variations over short timescales (minutes to hours), in order to document their contribution to natural SO2 flux as well as investigate the physical processes that control their behavior. In order to make these measurements, I first develop and assemble a UV ground-based instrument, and validate it against an independently measured source of SO2 at a coal-burning power plant in Arizona. I establish a measurement protocol and demonstrate that the instrument measures SO 2 fluxes with < 20 % error. Using the same protocol, I establish a record of the degassing patterns at Semeru <span class="hlt">volcano</span> (Indonesia), a <span class="hlt">volcano</span> that has been producing cycles of repeated explosions with periods of minutes to hours for the past several decades. Semeru produces an average of 21-71 tons of SO2 per day, amounting to a yearly output of 8-26 Mt. Using the Semeru data, along with a 1-D transient numerical model of magma ascent, I test the validity of a model in which a viscous plug at the top of the conduit produces cycles of eruption and gas release. I find that it can be a valid hypothesis to explain the observed patterns of degassing at Semeru. Periodic behavior in such a system occurs for a very narrow range</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2017/5077/sir20175077.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2017/5077/sir20175077.pdf"><span>2014 volcanic <span class="hlt">activity</span> in Alaska: Summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cameron, Cheryl E.; Dixon, James P.; Neal, Christina A.; Waythomas, Christopher F.; Schaefer, Janet R.; McGimsey, Robert G.</p> <p>2017-09-07</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, possible eruptions, volcanic unrest or suspected unrest, and seismic events at 18 volcanic centers in Alaska during 2014. The most notable volcanic <span class="hlt">activity</span> consisted of intermittent ash eruptions from long-<span class="hlt">active</span> Cleveland and Shishaldin <span class="hlt">Volcanoes</span> in the Aleutian Islands, and two eruptive episodes at Pavlof <span class="hlt">Volcano</span> on the Alaska Peninsula. Semisopochnoi and Akutan <span class="hlt">volcanoes</span> had seismic swarms, both likely the result of magmatic intrusion. The AVO also installed seismometers and infrasound instruments at Mount Cleveland during 2014.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JVGR..151...19C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JVGR..151...19C"><span>Growth history of Kilauea inferred from volatile concentrations in <span class="hlt">submarine</span>-collected basalts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coombs, Michelle L.; Sisson, Thomas W.; Lipman, Peter W.</p> <p>2006-03-01</p> <p>Major-element and volatile (H 2O, CO 2, S) compositions of glasses from the <span class="hlt">submarine</span> flanks of Kilauea <span class="hlt">Volcano</span> record its growth from pre-shield into tholeiite shield-stage. Pillow lavas of mildly alkalic basalt at 2600-1900 mbsl on the upper slope of the south flank are an intermediate link between deeper alkalic volcaniclastics and the modern tholeiite shield. Lava clast glasses from the west flank of Papau Seamount are subaerial Mauna Loa-like tholeiite and mark the contact between the two <span class="hlt">volcanoes</span>. H 2O and CO 2 in sandstone and breccia glasses from the Hilina bench, and in alkalic to tholeiitic pillow glasses above and to the east, were measured by FTIR. Volatile saturation pressures equal sampling depths (10 MPa = 1000 m water) for south flank and Puna Ridge pillow lavas, suggesting recovery near eruption depths and/or vapor re-equilibration during down-slope flow. South flank glasses are divisible into low-pressure (CO 2 < 40 ppm, H 2O < 0.5 wt.%, S < 500 ppm), moderate-pressure (CO 2 < 40 ppm, H 2O > 0.5 wt.%, S 1000-1700 ppm), and high-pressure groups (CO 2 > 40 ppm, S > ˜1000 ppm), corresponding to eruption ≥ sea level, at moderate water depths (300-1000 m) or shallower but in disequilibrium, and in deep water (> 1000 m). Saturation pressures range widely in early alkalic to strongly alkalic breccia clast and sandstone glasses, establishing that early Kīlauea's vents spanned much of Mauna Loa's <span class="hlt">submarine</span> flank, with some vents exceeding sea level. Later south flank alkalic pillow lavas expose a sizeable <span class="hlt">submarine</span> edifice that grew concurrent with nearby subaerial alkalic eruptions. The onset of the tholeiitic shield stage is marked by extension of eruptions eastward and into deeper water (to 5500 m) during growth of the Puna Ridge. Subaerial and shallow water eruptions from earliest Kilauea show that it is underlain shallowly by Mauna Loa, implying that Mauna Loa is larger, and Kilauea smaller, than previously recognized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2003/0112/pdf/of03-112.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2003/0112/pdf/of03-112.pdf"><span>Preliminary <span class="hlt">volcano</span>-hazard assessment for Great Sitkin <span class="hlt">Volcano</span>, 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>Waythomas, Christopher F.; Miller, Thomas P.; Nye, Christopher J.</p> <p>2003-01-01</p> <p>Great Sitkin <span class="hlt">Volcano</span> is a composite andesitic stratovolcano on Great Sitkin Island (51°05’ N latitude, 176°25’ W longitude), a small (14 x 16 km), circular volcanic island in the western Aleutian Islands of Alaska. Great Sitkin Island is located about 35 kilometers northeast of the community of Adak on Adak Island and 130 kilometers west of the community of Atka on Atka Island. Great Sitkin <span class="hlt">Volcano</span> is an <span class="hlt">active</span> <span class="hlt">volcano</span> and has erupted at least eight times in the past 250 years (Miller and others, 1998). The most recent eruption in 1974 caused minor ash fall on the flanks of the <span class="hlt">volcano</span> and resulted in the emplacement of a lava dome in the summit crater. The summit of the composite cone of Great Sitkin <span class="hlt">Volcano</span> is 1,740 meters above sea level. The <span class="hlt">active</span> crater is somewhat lower than the summit, and the highest point along its rim is about 1,460 meters above sea level. The crater is about 1,000 meters in diameter and is almost entirely filled by a lava dome emplaced in 1974. An area of <span class="hlt">active</span> fumaroles, hot springs, and bubbling hot mud is present on the south flank of the <span class="hlt">volcano</span> at the head of Big Fox Creek (see the map), and smaller ephemeral fumaroles and steam vents are present in the crater and around the crater rim. The flanking slopes of the <span class="hlt">volcano</span> are gradual to steep and consist of variously weathered and vegetated blocky lava flows that formed during Pleistocene and Holocene eruptions. The modern edifice occupies a caldera structure that truncates an older sequence of lava flows and minor pyroclastic rocks on the east side of the <span class="hlt">volcano</span>. The eastern sector of the <span class="hlt">volcano</span> includes the remains of an ancestral <span class="hlt">volcano</span> that was partially destroyed by a northwest-directed flank collapse. In winter, Great Sitkin <span class="hlt">Volcano</span> is typically completely snow covered. Should explosive pyroclastic eruptions occur at this time, the snow would be a source of water for volcanic mudflows or lahars. In summer, much of the snowpack melts, leaving only a patchy</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014BVol...76..882P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014BVol...76..882P"><span>Evidence from acoustic imaging for <span class="hlt">submarine</span> volcanic <span class="hlt">activity</span> in 2012 off the west coast of El Hierro (Canary Islands, Spain)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pérez, Nemesio M.; Somoza, Luis; Hernández, Pedro A.; de Vallejo, Luis González; León, Ricardo; Sagiya, Takeshi; Biain, Ander; González, Francisco J.; Medialdea, Teresa; Barrancos, José; Ibáñez, Jesús; Sumino, Hirochika; Nogami, Kenji; Romero, Carmen</p> <p>2014-12-01</p> <p>We report precursory geophysical, geodetic, and geochemical signatures of a new <span class="hlt">submarine</span> volcanic <span class="hlt">activity</span> observed off the western coast of El Hierro, Canary Islands. <span class="hlt">Submarine</span> manifestation of this <span class="hlt">activity</span> has been revealed through acoustic imaging of <span class="hlt">submarine</span> plumes detected on the 20-kHz chirp parasound subbottom profiler (TOPAS PS18) mounted aboard the Spanish RV Hespérides on June 28, 2012. Five distinct "filament-shaped" acoustic plumes emanating from the flanks of mounds have been recognized at water depth between 64 and 88 m on a <span class="hlt">submarine</span> platform located NW El Hierro. These plumes were well imaged on TOPAS profiles as "flares" of high acoustic contrast of impedance within the water column. Moreover, visible plumes composed of white rafts floating on the sea surface and sourcing from the location of the <span class="hlt">submarine</span> plumes were reported by aerial photographs on July 3, 2012, 5 days after acoustic plumes were recorded. In addition, several geophysical and geochemical data support the fact that these <span class="hlt">submarine</span> vents were preceded by several precursory signatures: (i) a sharp increase of the seismic energy release and the number of daily earthquakes of magnitude ≥2.5 on June 25, 2012, (ii) significant vertical and horizontal displacements observed at the Canary Islands GPS network (Nagoya University-ITER-GRAFCAN) with uplifts up to 3 cm from June 25 to 26, 2012, (iii) an anomalous increase of the soil gas radon <span class="hlt">activity</span>, from the end of April until the beginning of June reaching peak values of 2.7 kBq/m3 on June 3, 2012, and (iv) observed positive peak in the air-corrected value of 3He/4He ratio monitored in ground waters (8.5 atmospheric 3He/4He ratio ( R A)) at the northwestern El Hierro on June 16, 2012. Combining these <span class="hlt">submarine</span> and subaerial information, we suggest these plumes are the consequence of <span class="hlt">submarine</span> vents exhaling volcanic gas mixed with fine ash as consequence of an event of rapid rise of volatile-rich magma beneath the NW <span class="hlt">submarine</span> ridge</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992Tectp.206..245B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992Tectp.206..245B"><span>Morphostructural study and type of volcanism of <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> over the Pitcairn hot spot in the South Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Binard, Nicolas; Hékinian, Roger; Stoffers, Peter</p> <p>1992-06-01</p> <p>Undersea <span class="hlt">volcanoes</span> found at about 80 km southeast of the island of Pitcairn, are believed to be the manifestation of a hot-spot <span class="hlt">activity</span> located near 129°30'W 25°10'S, along the strike of the Mururoa-Gambier-Pitcairn volcanic alignment. Hydrothermal <span class="hlt">activities</span> and recent volcanic flows were observed on the two largest (20 km in basal diameter) and shallowest (60 m and 450 m depth) <span class="hlt">volcanoes</span>. More than twenty other smaller volcanic edifices ( < 500 m in height) were mapped during a Seabeam survey covering an area of about 8000 km 2. The edifices from the Pitcairn region are conical with a low degree of flatness (summit/basal diameters ratio <0.25), and consist of fresh alkali-enriched lava flows. The other truncated edifices with a high degree of flatness ( > 0.25) made up of ancient MORB-type tholeiitic rocks are inferred to be inherited from the EPR axial regions. The shallow volcanic <span class="hlt">activity</span> which occurred on the two largest edifices are classified as: (1) reactive eruptions, with hydromagmatic <span class="hlt">activities</span>, giving rise to volcanic ejecta, bombs, xenoliths, and ash, and (2) quiet eruptions which formed pillows and/or lobated lavas, and large massive flows. Intrusives (dyke and sill) were observed, cutting through the volcanic ejecta near the summit ( < 500 m depth) of the seamounts. The general structural orientations of the rift zones recognized from the bathymetry of individual <span class="hlt">volcanoes</span> (N160°-180°, N80°, N30° and N120°) are comparable to those observed in the Society and Austral hot-spot regions. These orientations were inferred as corresponding to the structural discontinuities of the ancient oceanic crust, and to the regional stress field of the Pacific plate. Rock samples from the Pitcairn region consist of alkali-basalts, basanites, trachyandesites, and trachytes which are closer in chemical composition to some of the volcanics from the Society rather than to those from the Austral hot-spot regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2015/5110/sir20155110.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2015/5110/sir20155110.pdf"><span>2013 volcanic <span class="hlt">activity</span> in Alaska: summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dixon, James P.; Cameron, Cheryl; McGimsey, Robert G.; Neal, Christina A.; Waythomas, Chris</p> <p>2015-08-14</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, volcanic unrest or suspected unrest, and seismic events at 18 volcanic centers in Alaska during 2013. Beginning with the 2013 AVO Summary of Events, the annual description of the AVO seismograph network and <span class="hlt">activity</span>, once a stand-alone publication, is now part of this report. Because of this change, the annual summary now contains an expanded description of seismic <span class="hlt">activity</span> at Alaskan <span class="hlt">volcanoes</span>. Eruptions occurred at three volcanic centers in 2013: Pavlof <span class="hlt">Volcano</span> in May and June, Mount Veniaminof <span class="hlt">Volcano</span> in June through December, and Cleveland <span class="hlt">Volcano</span> throughout the year. None of these three eruptive events resulted in 24-hour staffing at AVO facilities in Anchorage or Fairbanks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24451461','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24451461"><span>Embedded ARM system for <span class="hlt">volcano</span> monitoring in remote areas: application to the <span class="hlt">active</span> <span class="hlt">volcano</span> on Deception Island (Antarctica).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peci, Luis Miguel; Berrocoso, Manuel; Fernández-Ros, Alberto; García, Alicia; Marrero, José Manuel; Ortiz, Ramón</p> <p>2014-01-02</p> <p>This paper describes the development of a multi-parameter system for monitoring volcanic <span class="hlt">activity</span>. The system permits the remote access and the connection of several modules in a network. An embedded ARM™ processor has been used, allowing a great flexibility in hardware configuration. The use of a complete Linux solution (Debian™) as Operating System permits a quick, easy application development to control sensors and communications. This provides all the capabilities required and great stability with relatively low energy consumption. The cost of the components and applications development is low since they are widely used in different fields. Sensors and commercial modules have been combined with other self-developed modules. The Modular <span class="hlt">Volcano</span> Monitoring System (MVMS) described has been deployed on the <span class="hlt">active</span> Deception Island (Antarctica) <span class="hlt">volcano</span>, within the Spanish Antarctic Program, and has proved successful for monitoring the <span class="hlt">volcano</span>, with proven reliability and efficient operation under extreme conditions. In another context, i.e., the recent volcanic <span class="hlt">activity</span> on El Hierro Island (Canary Islands) in 2011, this technology has been used for the seismic equipment and GPS systems deployed, thus showing its efficiency in the monitoring of a volcanic crisis.</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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3926581','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3926581"><span>Embedded ARM System for <span class="hlt">Volcano</span> Monitoring in Remote Areas: Application to the <span class="hlt">Active</span> <span class="hlt">Volcano</span> on Deception Island (Antarctica)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Peci, Luis Miguel; Berrocoso, Manuel; Fernández-Ros, Alberto; García, Alicia; Marrero, José Manuel; Ortiz, Ramón</p> <p>2014-01-01</p> <p>This paper describes the development of a multi-parameter system for monitoring volcanic <span class="hlt">activity</span>. The system permits the remote access and the connection of several modules in a network. An embedded ARM™™ processor has been used, allowing a great flexibility in hardware configuration. The use of a complete Linux solution (Debian™) as Operating System permits a quick, easy application development to control sensors and communications. This provides all the capabilities required and great stability with relatively low energy consumption. The cost of the components and applications development is low since they are widely used in different fields. Sensors and commercial modules have been combined with other self-developed modules. The Modular <span class="hlt">Volcano</span> Monitoring System (MVMS) described has been deployed on the <span class="hlt">active</span> Deception Island (Antarctica) <span class="hlt">volcano</span>, within the Spanish Antarctic Program, and has proved successful for monitoring the <span class="hlt">volcano</span>, with proven reliability and efficient operation under extreme conditions. In another context, i.e., the recent volcanic <span class="hlt">activity</span> on El Hierro Island (Canary Islands) in 2011, this technology has been used for the seismic equipment and GPS systems deployed, thus showing its efficiency in the monitoring of a volcanic crisis. PMID:24451461</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GRC-2015-CM-0123.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GRC-2015-CM-0123.html"><span>Titan <span class="hlt">Submarine</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2015-06-15</p> <p>What would a <span class="hlt">submarine</span> to explore the liquid methane seas of Saturn's Moon Titan look like? This video shows one <span class="hlt">submarine</span> concept that would explore both the shoreline and the depths of this strange world that has methane rain, rivers and seas! The design was developed for the NASA Innovative Advanced Concepts (NIAC) Program, by NASA Glenn's COMPASS Team, and technologists and scientists from the Applied Physics Lab and <span class="hlt">submarine</span> designers from the Applied Research Lab.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.4788A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.4788A"><span><span class="hlt">Volcano</span>-Tectonic <span class="hlt">Activity</span> at Deception Island <span class="hlt">Volcano</span> Following a Seismic Swarm in the Bransfield Rift (2014-2015)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Almendros, J.; Carmona, E.; Jiménez, V.; Díaz-Moreno, A.; Lorenzo, F.</p> <p>2018-05-01</p> <p>In September 2014 there was a sharp increase in the seismic <span class="hlt">activity</span> of the Bransfield Strait, Antarctica. More than 9,000 earthquakes with magnitudes up to 4.6 located SE of Livingston Island were detected over a period of 8 months. A few months after the series onset, local seismicity at the nearby (˜35 km) Deception Island <span class="hlt">volcano</span> increased, displaying enhanced long-period seismicity and several outbursts of <span class="hlt">volcano</span>-tectonic (VT) earthquakes. Before February 2015, VT earthquakes occurred mainly at 5-20 km SW of Deception Island. In mid-February the numbers and sizes of VT earthquakes escalated, and their locations encompassed the whole volcanic edifice, suggesting a situation of generalized unrest. The <span class="hlt">activity</span> continued in anomalously high levels at least until May 2015. Given the spatial and temporal coincidence, it is unlikely that the Livingston series and the Deception VT swarm were unrelated. We propose that the Livingston series may have produced a triggering effect on Deception Island <span class="hlt">volcano</span>. Dynamic stresses associated to the seismic swarm may have induced overpressure in the unstable volcanic system, leading to a magmatic intrusion that may in turn have triggered the VT swarm. Alternatively, both the Livingston earthquakes and the VT swarm could be consequences of a magmatic intrusion at Deception Island. The Livingston series would be an example of precursory distal VT swarm, which seems to be a common feature preceding volcanic eruptions and magma intrusions in long-dormant <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890045617&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890045617&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes"><span>Measuring thermal budgets of <span class="hlt">active</span> <span class="hlt">volcanoes</span> by satellite remote sensing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Glaze, L.; Francis, P. W.; Rothery, D. A.</p> <p>1989-01-01</p> <p>Thematic Mapper measurements of the total radiant energy flux Q at Lascar <span class="hlt">volcano</span> in north Chile for December 1984 are reported. The results are consistent with the earlier suggestion that a lava lake is the source of a reported thermal budget anomaly, and with values for 1985-1986 that are much lower, suggesting that fumarolic <span class="hlt">activity</span> was then a more likely heat source. The results show that satellite remote sensing may be used to monitor the <span class="hlt">activity</span> of a <span class="hlt">volcano</span> quantitatively, in a way not possible by conventional ground studies, and may provide a method for predicting eruptions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003JVGR..127...73L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003JVGR..127...73L"><span>Magma transfer processes at persistently <span class="hlt">active</span> <span class="hlt">volcanoes</span>: insights from gravity observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Locke, Corinne A.; Rymer, Hazel; Cassidy, John</p> <p>2003-09-01</p> <p>Magma transfer processes at persistently <span class="hlt">active</span> <span class="hlt">volcanoes</span> are distinguished by the large magma flux required to sustain the prodigious quantities of heat and gas emitted at the surface. Although the resulting degassed magma has been conjectured to accumulate either deep within the volcanic edifice or in the upper levels of the sub-edifice system, no direct evidence for such <span class="hlt">active</span> accumulation has been reported. Temporal gravity data are unique in being able to quantify mass changes and have been successfully used to model shallow magma movements on different temporal scales, but have not generally been applied to the investigation of postulated long-term accumulation of magma at greater spatial scales within volcanic systems. Here, we model the critical data acquisition parameters required to detect mass flux at <span class="hlt">volcanoes</span>, we review existing data from a number of <span class="hlt">volcanoes</span> that exemplify the measurement of shallow mass changes and present new data from Poas and Telica <span class="hlt">volcanoes</span>. We show that if a substantial proportion of degassed magma lodges within the sub-edifice region, it would result in measurable annual to decadal gravity increases occurring over spatial scales of tens of kilometres and propose that existing microgravity data from Sakurajima and, possibly, Etna <span class="hlt">volcanoes</span> could be interpreted in these terms. Furthermore, such repeat microgravity data could be used to determine whether the accumulation rate is in equilibrium with the rate of production of degassed magma as calculated from the surface gas flux and hence identify the build-up of gas-rich magma at depth that may be significant in terms of eruption potential. We also argue that large magma bodies, both molten and frozen, modelled beneath <span class="hlt">volcanoes</span> from seismic and gravity data, could represent endogenous or cryptic intrusions of degassed magma based on order of magnitude calculations using present-day emission rates and typical <span class="hlt">volcano</span> lifetimes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017600','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017600"><span>Role of olivine cumulates in destabilizing the flanks of Hawaiian <span class="hlt">volcanoes</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>Clague, D.A.; Denlinger, R.P.</p> <p>1994-01-01</p> <p>The south flank of Kilauea <span class="hlt">Volcano</span> is unstable and has the structure of a huge landslide; it is one of at least 17 enormous catastrophic landslides shed from the Hawaiian Islands. Mechanisms previously proposed for movement of the south flank invoke slip of the volcanic pile over seafloor sediments. Slip on a low friction de??collement alone cannot explain why the thickest and widest sector of the flank moves more rapidly than the rest, or why this section contains a 300 km3 aseismic volume above the seismically defined de??collement. It is proposed that this aseismic volume, adjacent to the caldera in the direction of flank slip, consists of olivine cumulates that creep outward, pushing the south flank seawards. Average primary Kilauea tholeiitic magma contains about 16.5 wt.% MgO compared with an average 10 wt.% MgO for erupted subaerial and <span class="hlt">submarine</span> basalts. This difference requires fractionation of 17 wt.% (14 vol.%) olivine phenocrysts that accumulate near the base of the magma reservoir where they form cumulates. <span class="hlt">Submarine</span>-erupted Kilauea lavas contain abundant deformed olivine xenocrysts derived from these cumulates. Deformed dunite formed during the tholeiitic shield stage is also erupted as xenoliths in subsequent alkalic lavas. The deformation structures in olivine xenocrysts suggest that the cumulus olivine was densely packed, probably with as little as 5-10 vol.% intercumulus liquid, before entrainment of the xenocrysts. The olivine cumulates were at magmatic temperatures (>1100??C) when the xenocrysts were entrained. Olivine at 1100??C has a rheology similar to ice, and the olivine cumulates should flow down and away from the summit of the <span class="hlt">volcano</span>. Flow of the olivine cumulates places constant pressure on the unbuttressed seaward flank, leading to an extensional region that localizes deep intrusions behind the flank; these intrusions add to the seaward push. This mechanism ties the source of gravitational instability to the caldera complex and deep</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2002/0397/pdf/of02-397.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2002/0397/pdf/of02-397.pdf"><span>Preliminary <span class="hlt">volcano</span>-hazard assessment for Kanaga <span class="hlt">Volcano</span>, 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>Waythomas, Christopher F.; Miller, Thomas P.; Nye, Christopher J.</p> <p>2002-01-01</p> <p>Kanaga <span class="hlt">Volcano</span> is a steep-sided, symmetrical, cone-shaped, 1307 meter high, andesitic stratovolcano on the north end of Kanaga Island (51°55’ N latitude, 177°10’ W longitude) in the western Aleutian Islands of Alaska. Kanaga Island is an elongated, low-relief (except for the <span class="hlt">volcano</span>) island, located about 35 kilometers west of the community of Adak on Adak Island and is part of the Andreanof Islands Group of islands. Kanaga <span class="hlt">Volcano</span> is one of the 41 historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Alaska and has erupted numerous times in the past 11,000 years, including at least 10 eruptions in the past 250 years (Miller and others, 1998). The most recent eruption occurred in 1993-95 and caused minor ash fall on Adak Island and produced blocky aa lava flows that reached the sea on the northwest and west sides of the <span class="hlt">volcano</span> (Neal and others, 1995). The summit of the <span class="hlt">volcano</span> is characterized by a small, circular crater about 200 meters in diameter and 50-70 meters deep. Several <span class="hlt">active</span> fumaroles are present in the crater and around the crater rim. The flanking slopes of the <span class="hlt">volcano</span> are steep (20-30 degrees) and consist mainly of blocky, linear to spoonshaped lava flows that formed during eruptions of late Holocene age (about the past 3,000 years). The modern cone sits within a circular caldera structure that formed by large-scale collapse of a preexisting <span class="hlt">volcano</span>. Evidence for eruptions of this preexisting <span class="hlt">volcano</span> mainly consists of lava flows exposed along Kanaton Ridge, indicating that this former volcanic center was predominantly effusive in character. In winter (October-April), Kanaga <span class="hlt">Volcano</span> may be covered by substantial amounts of snow that would be a source of water for lahars (volcanic mudflows). In summer, much of the snowpack melts, leaving only a patchy distribution of snow on the <span class="hlt">volcano</span>. Glacier ice is not present on the <span class="hlt">volcano</span> or on other parts of Kanaga Island. Kanaga Island is uninhabited and is part of the Alaska Maritime National Wildlife Refuge, managed by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS53C1224H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS53C1224H"><span>High-Resolution Seafloor Observations of an <span class="hlt">Active</span> Mud <span class="hlt">Volcano</span> Offshore SW Taiwan - Results of a Repeated Survey after Four Years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hsu, H. H.; Chen, T. T.; Liu, C. S.; Su, C. C.; Paull, C. K.; Caress, D. W.; Gwiazda, R.; Chen, Y. H.</p> <p>2017-12-01</p> <p>Mud <span class="hlt">Volcano</span> V (MV5) is an <span class="hlt">active</span> <span class="hlt">submarine</span> mud <span class="hlt">volcano</span> sitting on top of a mud diapir ridge at water depths of 600 m in the <span class="hlt">active</span> margin offshore of southwestern Taiwan. This cone-shape mud <span class="hlt">volcano</span> is almost 3-km-wide, 200-m-high, with 9.5° slopes, and explosively ejects streams of mud every 1.5-3 minutes. It was first mapped in 2013 with MBARI's mapping AUV (autonomous underwater vehicle). In 2017, a repeated AUV mapping survey was conducted to see if significant bathymetric changes took place since 2013, and to investigate the fluxes of fluids that pass through diapiric structures in an <span class="hlt">active</span> continental margin. In addition to high-resolution bathymetry (1-m-resolution), sub-bottom profiling and side-scan sonar data acquired by the AUV, and videos and samples collected by MBARI's miniROV, we also incorporate multichannel seismic reflection data and gravity core sample analyses in this study. AUV bathymetry data reveal that there are two gryphons on the eastern slope of MV5. In the 2017 survey the mapped sizes of the two side cones were 80 m wide, 35 m long, 20 m relief and 40 m wide, 40 m long, 12 m relief, respectively. Comparing the bathymetry mapped in the 2017 AUV survey with that surveyed in 2013, no obvious overall morphological changes in MV5 are detected, except around the two gryphons. In the time period between the surveys, due to venting of mud from the two gryphons, two series of flow deposits which can be up to 5 meters thick are observed along the slope in the east side of both gryphons. The center depressions of these two gryphons have increased by 1-5 meters depth in their west side. Seismic and sub-bottom profiles reveal amplitude anomalies in the sub-strata of MV5 which indicate possible fluid migration paths of mud flows from deep. The trace of mud flow from the top of MV5 to its foot can be delineated from the side-scan sonar images. On the basis of 210Pbex chronology dating method, the sedimentation rate on the surface of MV5 is very slow</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.V22C0600B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.V22C0600B"><span>Composition and Structure of Mauna Loa's <span class="hlt">Submarine</span> West Flank, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Borchers, D.; Morgan, J. K.; Clague, D. A.; Moore, G. F.</p> <p>2003-12-01</p> <p>James Moore's pioneering work on <span class="hlt">submarine</span> landslides in the Hawaiian Islands contributed significantly to early models for the structure and evolution of Mauna Loa's <span class="hlt">submarine</span> western flank. The west flank experienced catastrophic failure in the past, generating massive blocks and debris fields offshore. Moore recognized that the midslope bench near the base of the <span class="hlt">submarine</span> flank must have postdated the debris avalanche, but little data existed to determine if it formed in response to further landsliding or to deeper volcanic processes. As the processes that shaped Mauna Loa are thought to be analogous to those currently <span class="hlt">active</span> at Kilauea, an improved understanding of Mauna Loa's history can provide valuable insight into the future of the younger Hawaiian <span class="hlt">volcanoes</span>. Several recent marine surveys in the area, including submersible surveys conducted by MBARI and JAMSTEC, and a multi-channel seismic (MCS) survey carried out by the University of Hawaii, provide important new data about the composition and structure of Mauna Loa's <span class="hlt">submarine</span> west flank. We carried out detailed geochemical, petrographic and structural analyses of rock samples and dive videos collected from the exposed northern wall of the midslope bench, documenting a repeated sequences of volcaniclastic sandstones and breccias. This stratigraphy contrasts with the predominantly subaerially erupted basalts composing the upper flank. Several thick ponded flows or sill-like diabase units are also interspersed in the section. The volcaniclastic units are highly cemented, and many contain hydrothermal alteration products, including chlorite, zeolites, and actinolite. The most altered rocks occur near the base of the bench and the degree of alteration decreases upward in the section. Samples collected from the outer scarp of the bench show evidence for intense shearing and cataclasis at all scales. The new MCS line crosses Mauna Loa's southern <span class="hlt">submarine</span> flank and central bench. More than 500 m of finely</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920034514&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920034514&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes"><span>Analysis of <span class="hlt">active</span> <span class="hlt">volcanoes</span> from the Earth Observing System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mouginis-Mark, Peter; Rowland, Scott; Crisp, Joy; Glaze, Lori; Jones, Kenneth; Kahle, Anne; Pieri, David; Zebker, Howard; Krueger, Arlin; Walter, Lou</p> <p>1991-01-01</p> <p>The Earth Observing System (EOS) scheduled for launch in 1997 and 1999 is briefly described, and the EOS volcanology investigation objectives are discussed. The volcanology investigation will include long- and short-term monitoring of selected <span class="hlt">volcanoes</span>, the detection of precursor <span class="hlt">activity</span> associated with unanticipated eruptions, and a detailed study of on-going eruptions. A variety of instruments on the EOS platforms will enable the study of local- and regional-scale thermal and deformational features of <span class="hlt">volcanoes</span>, and the chemical and structural features of volcanic eruption plumes and aerosols.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900028063&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900028063&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes"><span>Application of the Landsat Thematic Mapper to the identification of potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Central Andes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Francis, P. W.; De Silva, S. L.</p> <p>1989-01-01</p> <p>A systematic study of the potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Central Andes (14 deg S to 28 deg S) was carried out on the basis of Landsat Thematic Mapper images which provided consistent coverage of the area. More than 60 major <span class="hlt">volcanoes</span> were identified as potentially <span class="hlt">active</span>, as compared to 16 that are listed in the Catalog of <span class="hlt">Active</span> <span class="hlt">Volcanoes</span> of the World (Casertano, 1963; Hantke and Parodi, 1966). Most of these <span class="hlt">volcanoes</span> are large (up to 6000 m in height) composite cones. Some of them could threaten nearby settlements, especially those in southern Peru, where the <span class="hlt">volcanoes</span> rise above deep canyons with settlements along them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2007/5174/a/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2007/5174/a/"><span><span class="hlt">Volcano</span> Hazards Assessment for Medicine Lake <span class="hlt">Volcano</span>, Northern 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>Donnelly-Nolan, Julie M.; Nathenson, Manuel; Champion, Duane E.; Ramsey, David W.; Lowenstern, Jacob B.; Ewert, John W.</p> <p>2007-01-01</p> <p>Medicine Lake <span class="hlt">volcano</span> (MLV) is a very large shield-shaped <span class="hlt">volcano</span> located in northern California where it forms part of the southern Cascade Range of <span class="hlt">volcanoes</span>. It has erupted hundreds of times during its half-million-year history, including nine times during the past 5,200 years, most recently 950 years ago. This record represents one of the highest eruptive frequencies among Cascade <span class="hlt">volcanoes</span> and includes a wide variety of different types of lava flows and at least two explosive eruptions that produced widespread fallout. Compared to those of a typical Cascade stratovolcano, eruptive vents at MLV are widely distributed, extending 55 km north-south and 40 km east-west. The total area covered by MLV lavas is >2,000 km2, about 10 times the area of Mount St. Helens, Washington. Judging from its long eruptive history and its frequent eruptions in recent geologic time, MLV will erupt again. Although the probability of an eruption is very small in the next year (one chance in 3,600), the consequences of some types of possible eruptions could be severe. Furthermore, the documented episodic behavior of the <span class="hlt">volcano</span> indicates that once it becomes <span class="hlt">active</span>, the <span class="hlt">volcano</span> could continue to erupt for decades, or even erupt intermittently for centuries, and very likely from multiple vents scattered across the edifice. Owing to its frequent eruptions, explosive nature, and proximity to regional infrastructure, MLV has been designated a 'high threat <span class="hlt">volcano</span>' by the U.S. Geological Survey (USGS) National <span class="hlt">Volcano</span> Early Warning System assessment. Volcanic eruptions are typically preceded by seismic <span class="hlt">activity</span>, but with only two seismometers located high on the <span class="hlt">volcano</span> and no other USGS monitoring equipment in place, MLV is at present among the most poorly monitored Cascade <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNG33A0178C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG33A0178C"><span>Pattern Matching for <span class="hlt">Volcano</span> Status Assessment: what monitoring data alone can say about Mt. Etna <span class="hlt">activity</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cannavo, F.; Cannata, A.; Cassisi, C.</p> <p>2017-12-01</p> <p>The importance of assessing the ongoing status of <span class="hlt">active</span> <span class="hlt">volcanoes</span> is crucial not only for exposures to the local population but due to possible presence of tephra also for airline traffic. Adequately monitoring of <span class="hlt">active</span> <span class="hlt">volcanoes</span>, hence, plays a key role for civil protection purposes. In last decades, in order to properly monitor possible threats, continuous measuring networks have been designed and deployed on most of potentially hazardous <span class="hlt">volcanos</span>. Nevertheless, at the present, <span class="hlt">volcano</span> real-time surveillance is basically delegated to one or more human experts in volcanology, who interpret data coming from different kind of monitoring networks using their experience and non-measurable information (e.g. information from the field) to infer the <span class="hlt">volcano</span> status. In some cases, raw data are used in some models to obtain more clues on the ongoing <span class="hlt">activity</span>. In the last decades, with the development of <span class="hlt">volcano</span> monitoring networks, huge amount of data of different geophysical, geochemical and volcanological types have been collected and stored in large databases. Having such big data sets with many examples of volcanic <span class="hlt">activity</span> allows us to study <span class="hlt">volcano</span> monitoring from a machine learning perspective. Thus, exploiting opportunities offered by the abundance of <span class="hlt">volcano</span> monitoring time-series data we can try to address the following questions: Are the monitored parameters sufficient to discriminate the <span class="hlt">volcano</span> status? Is it possible to infer/distinguish the <span class="hlt">volcano</span> status only from the multivariate patterns of measurements? Are all the kind of measurements in the pattern equally useful for status assessment? How accurate would be an automatic system of status inference based only on pattern recognition of data? Here we present preliminary results of the data analysis we performed on a set of data and <span class="hlt">activity</span> covering the period 2011-2017 at Mount Etna (Italy). In the considered period, we had 52 events of lava fountaining and long periods of Strombolian <span class="hlt">activity</span>. We</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=volcano&pg=2&id=EJ305892','ERIC'); return false;" href="https://eric.ed.gov/?q=volcano&pg=2&id=EJ305892"><span><span class="hlt">Volcanoes</span>: Nature's Caldrons Challenge Geochemists.</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>Zurer, Pamela S.</p> <p>1984-01-01</p> <p>Reviews various topics and research studies on the geology of <span class="hlt">volcanoes</span>. Areas examined include <span class="hlt">volcanoes</span> and weather, plate margins, origins of magma, magma evolution, United States Geological Survey (USGS) <span class="hlt">volcano</span> hazards program, USGS <span class="hlt">volcano</span> observatories, volcanic gases, potassium-argon dating <span class="hlt">activities</span>, and <span class="hlt">volcano</span> monitoring strategies.…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gip/70039245/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gip/70039245/report.pdf"><span>Monitoring <span class="hlt">active</span> <span class="hlt">volcanoes</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>Tilling, Robert I.</p> <p>1987-01-01</p> <p>One of the most spectacular, awesomely beautiful, and at times destructive displays of natural energy is an erupting <span class="hlt">volcano</span>, belching fume and ash thousands of meters into the atmosphere and pouring out red-hot molten lava in fountains and streams. Countless eruptions in the geologic past have produced volcanic rocks that form much of the Earth's present surface. The gradual disintegration and weathering of these rocks have yielded some of the richest farmlands in the world, and these fertile soils play a significant role in sustaining our large and growing population. Were it not for volcanic <span class="hlt">activity</span>, the Hawaiian Islands with their sugar cane and pineapple fields and magnificent landscapes and seascapes would not exist to support their residents and to charm their visitors. Yet, the actual eruptive processes are catastrophic and can claim life and property.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFM.V12B0977M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFM.V12B0977M"><span><span class="hlt">Submarine</span> Structure and Stratigraphy of the South Kona Slump, Hawaii: Results from the MBARI 2001 Hawaii Expedition</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.; Clague, D. A.; Davis, A. S.</p> <p>2001-12-01</p> <p>As part of the MBARI 2001 Hawaii Expedition on board the R/V Western Flyer, the ROV Tiburon was used to carry out several highly successful dives upon the little studied <span class="hlt">submarine</span> South Kona slump, southwest Mauna Loa, Hawaii, offering a rare opportunity to look inside the broken flank of Mauna Loa <span class="hlt">volcano</span>. Four dives transected a scarp marking the southern lateral detachment of the Alika debris slide, which cut through the South Kona slump more than 100,000 years ago. The seaward regions of the <span class="hlt">submarine</span> flank, characterized by bathymetric ridges and troughs indicative of faulting and block detachment, revealed angular breccias and cohesive talus aprons that form low slopes, and indurated volcaniclastic sandstones and turbidites that define steep, high cliffs incised by dramatic erosional channels. Outcrops were consistently fractured and jointed, and occasionally intensely sheared, particularly in regions marked by bathymetric lows interpreted as block faults. Surface fractures occasionally exhibited "jig-saw puzzle" textures, often associated with rock avalanche deposits. The recovered sandstones were commonly fine-grained, particularly in the distal regions of the flank. Many were variably altered, often with zeolite pore filling, and exhibited sheared matrix and/or clasts. Most appear to be monolithic breccia samples derived from coarse flow interiors, although several samples were dominated by altered olivine sands. The interior of the proximal edifice consisted of thick units of fractured and broken pillow basalts, well preserved in cross-section in cliff faces, and interbedded with ledges of coarse fragmental basalts and breccias. Glass analyses of the flow units yielded from 5.76 to 6.80% MgO, and 51.8-52.9% SiO2. SiO2 contents are lower than modern Mauna Loa basalts, although the low ranges of TiO2 from ~2.25% at 6.6% MgO to 2.6% at 5.8% MgO, are typical for Mauna Loa lavas. Sulfur contents <230 ppm, indicate that the proximal lavas were degassed or</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMOS13E1289W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMOS13E1289W"><span>Arctic <span class="hlt">Submarine</span> Slope Stability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winkelmann, D.; Geissler, W.</p> <p>2010-12-01</p> <p><span class="hlt">Submarine</span> landsliding represents aside <span class="hlt">submarine</span> earthquakes major natural hazard to coastal and sea-floor infrastructure as well as to coastal communities due to their ability to generate large-scale tsunamis with their socio-economic consequences. The investigation of <span class="hlt">submarine</span> landslides, their conditions and trigger mechanisms, recurrence rates and potential impact remains an important task for the evaluation of risks in coastal management and offshore industrial <span class="hlt">activities</span>. In the light of a changing globe with warming oceans and rising sea-level accompanied by increasing human population along coasts and enhanced near- and offshore <span class="hlt">activities</span>, slope stability issues gain more importance than ever before. The Arctic exhibits the most rapid and drastic changes and is predicted to change even faster. Aside rising air temperatures, enhanced inflow of less cooled Atlantic water into the Arctic Ocean reduces sea-ice cover and warms the surroundings. Slope stability is challenged considering large areas of permafrost and hydrates. The Hinlopen/Yermak Megaslide (HYM) north of Svalbard is the first and so far only reported large-scale <span class="hlt">submarine</span> landslide in the Arctic Ocean. The HYM exhibits the highest headwalls that have been found on siliciclastic margins. With more than 10.000 square kilometer areal extent and app. 2.400 cubic kilometer of involved sedimentary material, it is one of the largest exposed <span class="hlt">submarine</span> slides worldwide. Geometry and age put this slide in a special position in discussing <span class="hlt">submarine</span> slope stability on glaciated continental margins. The HYM occurred 30 ka ago, when the global sea-level dropped by app. 50 m within less than one millennium due to rapid onset of global glaciation. It probably caused a tsunami with circum-Arctic impact and wave heights exceeding 130 meters. The HYM affected the slope stability field in its neighbourhood by removal of support. Post-megaslide slope instability as expressed in creeping and smaller-scaled slides are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFMED52B0023W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFMED52B0023W"><span>Dive and Explore: An Interactive Exhibit That Simulates Making an ROV Dive to a <span class="hlt">Submarine</span> <span class="hlt">Volcano</span>, Hatfield Marine Science Visitor Center, Newport, Oregon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weiland, C.; Chadwick, W. W.; Hanshumaker, W.; Osis, V.; Hamilton, C.</p> <p>2002-12-01</p> <p>We have created a new interactive exhibit in which the user can sit down and simulate that they are making a dive to the seafloor with the remotely operated vehicle (ROV) named ROPOS. The exhibit immerses the user in an interactive experience that is naturally fun but also educational. This new public display is located at the Hatfield Marine Science Visitor Center in Newport, Oregon. The exhibit is designed to look like the real ROPOS control console and includes three video monitors, a PC, a DVD player, an overhead speaker, graphic panels, buttons, lights, dials, and a seat in front of a joystick. The dives are based on real seafloor settings at Axial seamount, an <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> on the Juan de Fuca Ridge (NE Pacific) that is also the location of a seafloor observatory called NeMO. The user can choose between 1 of 3 different dives sites in the caldera of Axial <span class="hlt">Volcano</span>. Once a dive is chosen, then the user watches ROPOS being deployed and then arrives into a 3-D computer-generated seafloor environment that is based on the real world but is easier to visualize and navigate. Once on the bottom, the user is placed within a 360 degree panorama and can look in all directions by manipulating the joystick. By clicking on markers embedded in the scene, the user can then either move to other panorama locations via movies that travel through the 3-D virtual environment, or they can play video clips from actual ROPOS dives specifically related to that scene. Audio accompanying the video clips informs the user where they are going or what they are looking at. After the user is finished exploring the dive site they end the dive by leaving the bottom and watching the ROV being recovered onto the ship at the surface. The user can then choose a different dive or make the same dive again. Within the three simulated dives there are a total of 6 arrival and departure movies, 7 seafloor panoramas, 12 travel movies, and 23 ROPOS video clips. The exhibit software was created</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2001/0367/pdf/of2001-0367.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2001/0367/pdf/of2001-0367.pdf"><span><span class="hlt">Volcano</span>-hazard zonation for San Vicente <span class="hlt">volcano</span>, El Salvador</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Major, J.J.; Schilling, S.P.; Pullinger, C.R.; Escobar, C.D.; Howell, M.M.</p> <p>2001-01-01</p> <p>San Vicente <span class="hlt">volcano</span>, also known as Chichontepec, is one of many <span class="hlt">volcanoes</span> along the volcanic arc in El Salvador. This composite <span class="hlt">volcano</span>, located about 50 kilometers east of the capital city San Salvador, has a volume of about 130 cubic kilometers, rises to an altitude of about 2180 meters, and towers above major communities such as San Vicente, Tepetitan, Guadalupe, Zacatecoluca, and Tecoluca. In addition to the larger communities that surround the <span class="hlt">volcano</span>, several smaller communities and coffee plantations are located on or around the flanks of the <span class="hlt">volcano</span>, and major transportation routes are located near the lowermost southern and eastern flanks of the <span class="hlt">volcano</span>. The population density and proximity around San Vicente <span class="hlt">volcano</span>, as well as the proximity of major transportation routes, increase the risk that even small landslides or eruptions, likely to occur again, can have serious societal consequences. The eruptive history of San Vicente <span class="hlt">volcano</span> is not well known, and there is no definitive record of historical eruptive <span class="hlt">activity</span>. The last significant eruption occurred more than 1700 years ago, and perhaps long before permanent human habitation of the area. Nevertheless, this <span class="hlt">volcano</span> has a very long history of repeated, and sometimes violent, eruptions, and at least once a large section of the <span class="hlt">volcano</span> collapsed in a massive landslide. The oldest rocks associated with a volcanic center at San Vicente are more than 2 million years old. The <span class="hlt">volcano</span> is composed of remnants of multiple eruptive centers that have migrated roughly eastward with time. Future eruptions of this <span class="hlt">volcano</span> will pose substantial risk to surrounding communities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JGRB..11512105G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JGRB..11512105G"><span>Three-dimensional structure of the <span class="hlt">submarine</span> flanks of La Réunion inferred from geophysical data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gailler, Lydie-Sarah; LéNat, Jean-FrançOis</p> <p>2010-12-01</p> <p>La Réunion (Indian Ocean) constitutes a huge volcanic oceanic system of which most of the volume is submerged. We present a study of its <span class="hlt">submarine</span> part based on the interpretation of magnetic and gravity data compiled from old and recent surveys. A model of the <span class="hlt">submarine</span> internal structure is derived from 3-D and 2-D models using constraints from previous geological and geophysical studies. Two large-scale, previously unknown, buried volcanic construction zones are discovered in continuation of the island's construction. To the east, the Alizés <span class="hlt">submarine</span> zone is interpreted as the remnants of Les Alizés <span class="hlt">volcano</span> eastward flank whose center is marked by a large hypovolcanic intrusion complex. To the southwest, the Etang Salé <span class="hlt">submarine</span> zone is interpreted as an extension of Piton des Neiges, probably fed by a volcanic rift zone over a large extent. They were predominantly built during the Matuyama period and thus probably belong to early volcanism. A correlation exists between their top and seismic horizons recognized in previous studies and interpreted as the base of the volcanic edifice. Their morphology suggested a lithospheric bulging beneath La Réunion, not required to explain our data, since the seismic interfaces match the top of our volcanic constructions. The coastal shelf coincides with a negative Bouguer anomaly belt, often associated with magnetic anomalies, suggesting a shelf built by hyaloclastites. A detailed analysis of the offshore continuation of La Montagne Massif to the north confirms this hypothesis. The gravity analysis confirms that the bathymetric bulges, forming the northern, eastern, southern, and western <span class="hlt">submarine</span> flanks, are predominantly built by debris avalanche deposits at the surface.</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://pubs.er.usgs.gov/publication/70011692','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011692"><span>Chemistry and isotope ratios of sulfur in basalts and volcanic gases at Kilauea <span class="hlt">volcano</span>, 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>Sakai, H.; Casadevall, T.J.; Moore, J.G.</p> <p>1982-01-01</p> <p>Eighteen basalts and some volcanic gases from the <span class="hlt">submarine</span> and subaerial parts of Kilauea <span class="hlt">volcano</span> were analyzed for the concentration and isotope ratios of sulfur. By means of a newly developed technique, sulfide and sulfate sulfur in the basalts were separately but simultaneously determined. The <span class="hlt">submarine</span> basalt has 700 ?? 100 ppm total sulfur with ??34S??s of 0.7 ?? 0.1 ???. The sulfate/sulfide molar ratio ranges from 0.15 to 0.56 and the fractionation factor between sulfate and sulfide is +7.5 ?? 1.5???. On the other hand, the concentration and ??34S??s values of the total sulfur in the subaerial basalt are reduced to 150 ?? 50 ppm and -0.8 ?? 0.2???, respectively. The sulfate to sulfide ratio and the fractionation factor between them are also smaller, 0.01 to 0.25 and +3.0???, respectively. Chemical and isotopic evidence strongly suggests that sulfate and sulfide in the <span class="hlt">submarine</span> basalt are in chemical and isotopic equilibria with each other at magmatic conditions. Their relative abundance and the isotope fractionation factors may be used to estimate the f{hook}o2 and temperature of these basalts at the time of their extrusion onto the sea floor. The observed change in sulfur chemistry and isotopic ratios from the <span class="hlt">submarine</span> to subaerial basalts can be interpreted as degassing of the SO2 from basalt thereby depleting sulfate and 34S in basalt. The volcanic sulfur gases, predominantly SO2, from the 1971 and 1974 fissures in Kilauea Crater have ??34S values of 0.8 to 0.9%., slightly heavier than the total sulfur in the <span class="hlt">submarine</span> basalts and definitely heavier than the subaerial basalts, in accord with the above model. However, the ??34S value of sulfur gases (largely SO2) from Sulfur Bank is 8.0%., implying a secondary origin of the sulfur. The ??34S values of native sulfur deposits at various sites of Kilauea and Mauna Loa <span class="hlt">volcanos</span>, sulfate ions of four deep wells and hydrogen sulfide from a geothermal well along the east rift zone are also reported. The high</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2014/5159/pdf/sir2014-5159.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2014/5159/pdf/sir2014-5159.pdf"><span>2011 volcanic <span class="hlt">activity</span> in Alaska: summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Maharrey, J. Zebulon; Neal, Christina A.</p> <p>2014-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, possible eruptions, and volcanic unrest at or near three separate volcanic centers in Alaska during 2011. The year was highlighted by the unrest and eruption of Cleveland <span class="hlt">Volcano</span> in the central Aleutian Islands. AVO annual summaries no longer report on <span class="hlt">activity</span> at Russian <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=volcanoes&pg=4&id=EJ273318','ERIC'); return false;" href="https://eric.ed.gov/?q=volcanoes&pg=4&id=EJ273318"><span>A Scientific Excursion: <span class="hlt">Volcanoes</span>.</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>Olds, Henry, Jr.</p> <p>1983-01-01</p> <p>Reviews an educationally valuable and reasonably well-designed simulation of volcanic <span class="hlt">activity</span> in an imaginary land. <span class="hlt">VOLCANOES</span> creates an excellent context for learning information about <span class="hlt">volcanoes</span> and for developing skills and practicing methods needed to study behavior of <span class="hlt">volcanoes</span>. (Author/JN)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001924.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e001924.html"><span><span class="hlt">Activity</span> at Klyuchevskaya <span class="hlt">Volcano</span> Resumes</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>NASA image acquired December 4, 2010 After a respite of less than a month, Klyuchevskaya <span class="hlt">Volcano</span> resumed erupting in late November 2010. The Global Volcanism Program reported several ash plumes that rose up to 7.9 kilometers (26,000 feet) above sea level from November 25–29. According to the Kamchatka Volcanic Eruption Response Team (KVERT) seismicity was “slightly above background levels” on November 26th and 27th, and they reported observations of strombolian <span class="hlt">activity</span> on December 1st and 2nd. A plume of ash, steam, and other volcanic gases streamed from Klyuchevskaya on December 4, 2010, visible in this natural-color image acquired by the Advanced Land Imager (ALI) aboard the Earth Observing-1 (EO-1) satellite. In the large image, a much smaller plume is visible above neighboring Bezymianny <span class="hlt">Volcano</span>. NASA Earth Observatory image by Jesse Allen & Robert Simmon, using ALI data from the NASA EO-1 team. Caption by Robert Simmon. Instrument: EO-1 - ALI Credit: NASA Earth Observatory NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Join us on Facebook</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GeoRL..3916311P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GeoRL..3916311P"><span>Precursory diffuse CO2 and H2S emission signatures of the 2011-2012 El Hierro <span class="hlt">submarine</span> eruption, Canary Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pérez, Nemesio M.; Padilla, Germán D.; Padrón, Eleazar; Hernández, Pedro A.; Melián, Gladys V.; Barrancos, José; Dionis, Samara; Nolasco, Dácil; Rodríguez, Fátima; Calvo, David; Hernández, Íñigo</p> <p>2012-08-01</p> <p>On October 12, 2011, a <span class="hlt">submarine</span> eruption began 2 km off the coast of La Restinga, south of El Hierro Island. CO2 and H2S soil efflux were continuously measured during the period of volcanic unrest by using the accumulation chamber method at two different geochemical stations, HIE01 and HIE07. Recorded CO2 and H2S effluxes showed precursory signals that preceded the <span class="hlt">submarine</span> eruption. Beginning in late August, the CO2 efflux time series started increasing at a relatively constant rate over one month, reaching a maximum of 19 gm-2d-1 one week before the onset of the <span class="hlt">submarine</span> volcanic eruption. The H2S efflux time series at HIE07 showed a pulse in H2S emission just one day before the initiation of the <span class="hlt">submarine</span> eruption, reaching peak values of 42 mg m-2 d-1, 10 times the average H2S efflux recorded during the observation period. Since CO2 and H2S effluxes are strongly influenced by external factors, we applied a multiple regression analysis to remove their contribution. A statistical analysis showed that the long-term trend of the filtered data is well correlated with the seismic energy. We find that these geochemical stations are important monitoring sites for evaluating the volcanic <span class="hlt">activity</span> of El Hierro and that they demonstrate the potential of applying continuous monitoring of soil CO2 and H2S efflux to improve and optimize the detection of early warning signals of future volcanic unrest episodes at El Hierro. Continuous diffuse degassing studies would likely prove useful for monitoring other <span class="hlt">volcanoes</span> during unrest episodes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.5545N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5545N"><span><span class="hlt">Active</span> <span class="hlt">volcanoes</span> observed through Art: the contribution offered by the social networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neri, Marco; Neri, Emilia</p> <p>2015-04-01</p> <p><span class="hlt">Volcanoes</span> have always fascinated people for the wild beauty of their landscapes and also for the fear that they arouse with their eruptive actions, sometimes simply spectacular, but other times terrifying and catastrophic for human <span class="hlt">activities</span>. In the past, <span class="hlt">volcanoes</span> were sometimes imagined as a metaphysical gateway to the otherworld; they have inspired the creation of myths and legends ever since three thousand years ago, also represented by paintings of great artistic impact. Modern technology today offers very sophisticated and readily accessed digital tools, and <span class="hlt">volcanoes</span> continue to be frequently photographed and highly appreciated natural phenomena. Moreover, in recent years, the spread of social networks (Facebook, Twitter, YouTube, Instagram, etc.) have made the widespread dissemination of graphic contributions even easier. The result is that very <span class="hlt">active</span> and densely inhabited <span class="hlt">volcanoes</span> such as Etna, Vesuvius and Aeolian Islands, in Italy, have become among the most photographed subjects in the world, providing a popular science tool with formidable influence and usefulness. The beauty of these landscapes have inspired both professional artists and photographers, as well as amateurs, who compete in the social networks for the publication of the most spectacular, artistic or simply most informative images. The end result of this often frantic popular scientific <span class="hlt">activity</span> is at least two-fold: on one hand, it provides geoscientists and science communicators a quantity of documentation that is almost impossible to acquire through the normal systems of <span class="hlt">volcano</span> monitoring, while on the other it raises awareness and respect for the land among the civil community.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS21A1953Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS21A1953Y"><span>Characteristics and features of the <span class="hlt">submarine</span> landslides in passive and <span class="hlt">active</span> margin southwestern offshore Taiwan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yeh, Y. C.</p> <p>2016-12-01</p> <p>In the past decade, numerous multi-channel seismic surveys as well as near seafloor high resolution geophysical investigations were conducted in order to explore and estimate the reserves of gas hydrate southwestern offshore Taiwan. The previous object was focused on searching substitute energy (i.e. gas hydrate) rather than geo-hazards. However, it is suggested that most of the gas hydrate is generally distributed at slope area southwestern offshore Taiwan, which indicates the slope may be failed when steady state was disturbed by some factors, such as sea level or climate change. In addition, once gas hydrate was dissociated, this may induce <span class="hlt">submarine</span> landslide that further cause devastated tsunami. Thus, it is of great urgency to investigate potential landslide area, particularly, the hydrate-rich continental slope (<span class="hlt">active</span> and passive margins) in adjacent to populous city like Kaohsiung. In this study, we collected several high resolution multi-channel seismic data with ten seconds shooting rate and 3.125 meters group interval streamer by using R/V ORI and R/V ORV. The seismic data were processed in conventional data processing strategy: bad trace clean, geometry settings, band-pass filter, de-convolution, surface-related multiple rejection, radon filter, stacking,kirchhoff migration and time to depth conversion. Combine the results obtained from the MCS data and subbottom profiles, two major results could be raised in the <span class="hlt">active</span> margin as followed: (1) Most of the surface creeping and landslide was occurred shallower than 500 meters in water depth, which should be related to the inter-bedded fluid <span class="hlt">activities</span>. (2) The landslide distribution is lagly affected by the presence of diaper, suggesting the subsequent mud diapirism may destruct slope stability; (3) The <span class="hlt">submarine</span> landslide deeper than 800 meters in water depth distributes in the thrust fold area, that is probably referred to <span class="hlt">active</span> thrusting. In the passive margin, large volume mass transportation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29674649','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29674649"><span>Mud extrusion and ring-fault gas seepage - upward branching fluid discharge at a deep-sea mud <span class="hlt">volcano</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Loher, M; Pape, T; Marcon, Y; Römer, M; Wintersteller, P; Praeg, D; Torres, M; Sahling, H; Bohrmann, G</p> <p>2018-04-19</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> release sediments and gas-rich fluids at the seafloor via deeply-rooted plumbing systems that remain poorly understood. Here the functioning of Venere mud <span class="hlt">volcano</span>, on the Calabrian accretionary prism in ~1,600 m water depth is investigated, based on multi-parameter hydroacoustic and visual seafloor data obtained using ship-borne methods, ROVs, and AUVs. Two seepage domains are recognized: mud breccia extrusion from a summit, and hydrocarbon venting from peripheral sites, hosting chemosynthetic ecosystems and authigenic carbonates indicative of long-term seepage. Pore fluids in freshly extruded mud breccia (up to 13 °C warmer than background sediments) contained methane concentrations exceeding saturation by 2.7 times and chloride concentrations up to five times lower than ambient seawater. Gas analyses indicate an underlying thermogenic hydrocarbon source with potential admixture of microbial methane during migration along ring faults to the peripheral sites. The gas and pore water analyses point to fluids sourced deep (>3 km) below Venere mud <span class="hlt">volcano</span>. An upward-branching plumbing system is proposed to account for co-existing mud breccia extrusion and gas seepage via multiple surface vents that influence the distribution of seafloor ecosystems. This model of mud volcanism implies that methane-rich fluids may be released during prolonged phases of moderate <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2005/1403/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2005/1403/"><span>Volcanic hazards at Atitlan <span class="hlt">volcano</span>, Guatemala</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Haapala, J.M.; Escobar Wolf, R.; Vallance, James W.; Rose, William I.; Griswold, J.P.; Schilling, S.P.; Ewert, J.W.; Mota, M.</p> <p>2006-01-01</p> <p>Atitlan <span class="hlt">Volcano</span> is in the Guatemalan Highlands, along a west-northwest trending chain of <span class="hlt">volcanoes</span> parallel to the mid-American trench. The <span class="hlt">volcano</span> perches on the southern rim of the Atitlan caldera, which contains Lake Atitlan. Since the major caldera-forming eruption 85 thousand years ago (ka), three stratovolcanoes--San Pedro, Toliman, and Atitlan--have formed in and around the caldera. Atitlan is the youngest and most <span class="hlt">active</span> of the three <span class="hlt">volcanoes</span>. Atitlan <span class="hlt">Volcano</span> is a composite <span class="hlt">volcano</span>, with a steep-sided, symmetrical cone comprising alternating layers of lava flows, volcanic ash, cinders, blocks, and bombs. Eruptions of Atitlan began more than 10 ka [1] and, since the arrival of the Spanish in the mid-1400's, eruptions have occurred in six eruptive clusters (1469, 1505, 1579, 1663, 1717, 1826-1856). Owing to its distance from population centers and the limited written record from 200 to 500 years ago, only an incomplete sample of the <span class="hlt">volcano</span>'s behavior is documented prior to the 1800's. The geologic record provides a more complete sample of the <span class="hlt">volcano</span>'s behavior since the 19th century. Geologic and historical data suggest that the intensity and pattern of <span class="hlt">activity</span> at Atitlan <span class="hlt">Volcano</span> is similar to that of Fuego <span class="hlt">Volcano</span>, 44 km to the east, where <span class="hlt">active</span> eruptions have been observed throughout the historical period. Because of Atitlan's moderately explosive nature and frequency of eruptions, there is a need for local and regional hazard planning and mitigation efforts. Tourism has flourished in the area; economic pressure has pushed agricultural <span class="hlt">activity</span> higher up the slopes of Atitlan and closer to the source of possible future volcanic <span class="hlt">activity</span>. This report summarizes the hazards posed by Atitlan <span class="hlt">Volcano</span> in the event of renewed <span class="hlt">activity</span> but does not imply that an eruption is imminent. However, the recognition of potential <span class="hlt">activity</span> will facilitate hazard and emergency preparedness.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5037448','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5037448"><span>Helium and methane sources and fluxes of shallow <span class="hlt">submarine</span> hydrothermal plumes near the Tokara Islands, Southern Japan</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wen, Hsin-Yi; Sano, Yuji; Takahata, Naoto; Tomonaga, Yama; Ishida, Akizumi; Tanaka, Kentaro; Kagoshima, Takanori; Shirai, Kotaro; Ishibashi, Jun-ichiro; Yokose, Hisayoshi; Tsunogai, Urumu; Yang, Tsanyao F.</p> <p>2016-01-01</p> <p>Shallow <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> have been newly discovered near the Tokara Islands, which are situated at the volcanic front of the northern Ryukyu Arc in southern Japan. Here, we report for the first time the volatile geochemistry of shallow hydrothermal plumes, which were sampled using a CTD-RMS system after analyzing water column images collected by multi-beam echo sounder surveys. These surveys were performed during the research cruise KS-14-10 of the R/V Shinsei Maru in a region stretching from the Wakamiko Crater to the Tokara Islands. The 3He flux and methane flux in the investigated area are estimated to be (0.99–2.6) × 104 atoms/cm2/sec and 6–60 t/yr, respectively. The methane in the region of the Tokara Islands is a mix between abiotic methane similar to that found in the East Pacific Rise and thermogenic one. Methane at the Wakamiko Crater is of abiotic origin but affected by isotopic fractionation through rapid microbial oxidation. The helium isotopes suggest the presence of subduction-type mantle helium at the Wakamiko Crater, while a larger crustal component is found close to the Tokara Islands. This suggests that the Tokara Islands <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> are a key feature of the transition zone between the volcanic front and the spreading back-arc basin. PMID:27671524</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27671524','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27671524"><span>Helium and methane sources and fluxes of shallow <span class="hlt">submarine</span> hydrothermal plumes near the Tokara Islands, Southern Japan.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wen, Hsin-Yi; Sano, Yuji; Takahata, Naoto; Tomonaga, Yama; Ishida, Akizumi; Tanaka, Kentaro; Kagoshima, Takanori; Shirai, Kotaro; Ishibashi, Jun-Ichiro; Yokose, Hisayoshi; Tsunogai, Urumu; Yang, Tsanyao F</p> <p>2016-09-27</p> <p>Shallow <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> have been newly discovered near the Tokara Islands, which are situated at the volcanic front of the northern Ryukyu Arc in southern Japan. Here, we report for the first time the volatile geochemistry of shallow hydrothermal plumes, which were sampled using a CTD-RMS system after analyzing water column images collected by multi-beam echo sounder surveys. These surveys were performed during the research cruise KS-14-10 of the R/V Shinsei Maru in a region stretching from the Wakamiko Crater to the Tokara Islands. The 3 He flux and methane flux in the investigated area are estimated to be (0.99-2.6) × 10 4 atoms/cm 2 /sec and 6-60 t/yr, respectively. The methane in the region of the Tokara Islands is a mix between abiotic methane similar to that found in the East Pacific Rise and thermogenic one. Methane at the Wakamiko Crater is of abiotic origin but affected by isotopic fractionation through rapid microbial oxidation. The helium isotopes suggest the presence of subduction-type mantle helium at the Wakamiko Crater, while a larger crustal component is found close to the Tokara Islands. This suggests that the Tokara Islands <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> are a key feature of the transition zone between the volcanic front and the spreading back-arc basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1999/0448/pdf/1997SummaryofEventsAVO.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1999/0448/pdf/1997SummaryofEventsAVO.pdf"><span>1997 volcanic <span class="hlt">activity</span> in Alaska and Kamchatka: summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Wallace, Kristi L.</p> <p>1999-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) monitors over 40 historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> along the Aleutian Arc. Twenty are seismically monitored and for the rest, the AVO monitoring program relies mainly on pilot reports, observations of local residents and ship crews, and daily analysis of satellite images. In 1997, AVO responded to eruptive <span class="hlt">activity</span> or suspect volcanic <span class="hlt">activity</span> at 11 volcanic centers: Wrangell, Sanford, Shrub mud <span class="hlt">volcano</span>, Iliamna, the Katmai group (Martin, Mageik, Snowy, and Kukak <span class="hlt">volcanoes</span>), Chiginagak, Pavlof, Shishaldin, Okmok, Cleveland, and Amukta. Of these, AVO has real-time, continuously recording seismic networks at Iliamna, the Katmai group, and Pavlof. The phrase “suspect volcanic activity” (SVA), used to characterize several responses, is an eruption report or report of unusual <span class="hlt">activity</span> that is subsequently determined to be normal or enhanced fumarolic <span class="hlt">activity</span>, weather-related phenomena, or a non-volcanic event. In addition to responding to eruptive <span class="hlt">activity</span> at Alaska <span class="hlt">volcanoes</span>, AVO also disseminated information for the Kamchatkan Volcanic Eruption Response Team (KVERT) about the 1997 <span class="hlt">activity</span> of 5 Russian <span class="hlt">volcanoes</span>--Sheveluch, Klyuchevskoy, Bezymianny, Karymsky, and Alaid (SVA). This report summarizes volcanic <span class="hlt">activity</span> and SVA in Alaska during 1997 and the AVO response, as well as information on the reported <span class="hlt">activity</span> at the Russian <span class="hlt">volcanoes</span>. Only those reports or inquiries that resulted in a “significant” investment of staff time and energy (here defined as several hours or more for reaction, tracking, and follow-up) are included. AVO typically receives dozens of reports throughout the year of steaming, unusual cloud sightings, or eruption rumors. Most of these are resolved quickly and are not tabulated here as part of the 1997 response record.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030921','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030921"><span>Growth history of Kilauea inferred from volatile concentrations in <span class="hlt">submarine</span>-collected basalts</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Coombs, Michelle L.; Sisson, Thomas W.; Lipman, Peter W.</p> <p>2006-01-01</p> <p>Major-element and volatile (H2O, CO2, S) compositions of glasses from the <span class="hlt">submarine</span> flanks of Kilauea <span class="hlt">Volcano</span> record its growth from pre-shield into tholeiite shield-stage. Pillow lavas of mildly alkalic basalt at 2600–1900 mbsl on the upper slope of the south flank are an intermediate link between deeper alkalic volcaniclastics and the modern tholeiite shield. Lava clast glasses from the west flank of Papau Seamount are subaerial Mauna Loa-like tholeiite and mark the contact between the two <span class="hlt">volcanoes</span>. H2O and CO2 in sandstone and breccia glasses from the Hilina bench, and in alkalic to tholeiitic pillow glasses above and to the east, were measured by FTIR. Volatile saturation pressures equal sampling depths (10 MPa = 1000 m water) for south flank and Puna Ridge pillow lavas, suggesting recovery near eruption depths and/or vapor re-equilibration during down-slope flow. South flank glasses are divisible into low-pressure (CO2 <40 ppm, H2O < 0.5 wt.%, S <500 ppm), moderate-pressure (CO2 <40 ppm, H2O >0.5 wt.%, S 1000–1700 ppm), and high-pressure groups (CO2 >40 ppm, S  ∼1000 ppm), corresponding to eruption ≥ sea level, at moderate water depths (300–1000 m) or shallower but in disequilibrium, and in deep water (>1000 m). Saturation pressures range widely in early alkalic to strongly alkalic breccia clast and sandstone glasses, establishing that early Kīlauea's vents spanned much of Mauna Loa's <span class="hlt">submarine</span> flank, with some vents exceeding sea level. Later south flank alkalic pillow lavas expose a sizeable <span class="hlt">submarine</span> edifice that grew concurrent with nearby subaerial alkalic eruptions. The onset of the tholeiitic shield stage is marked by extension of eruptions eastward and into deeper water (to 5500 m) during growth of the Puna Ridge. Subaerial and shallow water eruptions from earliest Kilauea show that it is underlain shallowly by Mauna Loa, implying that Mauna Loa is larger, and Kilauea smaller, than previously recognized.Keywords</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70046087','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70046087"><span>Geomorphic process fingerprints in <span class="hlt">submarine</span> canyons</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brothers, Daniel S.; ten Brink, Uri S.; Andrews, Brian D.; Chaytor, Jason D.; Twichell, David C.</p> <p>2013-01-01</p> <p><span class="hlt">Submarine</span> canyons are common features of continental margins worldwide. They are conduits that funnel vast quantities of sediment from the continents to the deep sea. Though it is known that <span class="hlt">submarine</span> canyons form primarily from erosion induced by <span class="hlt">submarine</span> sediment flows, we currently lack quantitative, empirically based expressions that describe the morphology of <span class="hlt">submarine</span> canyon networks. Multibeam bathymetry data along the entire passive US Atlantic margin (USAM) and along the <span class="hlt">active</span> central California margin near Monterey Bay provide an opportunity to examine the fine-scale morphology of 171 slope-sourced canyons. Log–log regression analyses of canyon thalweg gradient (S) versus up-canyon catchment area (A) are used to examine linkages between morphological domains and the generation and evolution of <span class="hlt">submarine</span> sediment flows. For example, canyon reaches of the upper continental slope are characterized by steep, linear and/or convex longitudinal profiles, whereas reaches farther down canyon have distinctly concave longitudinal profiles. The transition between these geomorphic domains is inferred to represent the downslope transformation of debris flows into erosive, canyon-flushing turbidity flows. Over geologic timescales this process appears to leave behind a predictable geomorphic fingerprint that is dependent on the catchment area of the canyon head. Catchment area, in turn, may be a proxy for the volume of sediment released during geomorphically significant failures along the upper continental slope. Focused studies of slope-sourced <span class="hlt">submarine</span> canyons may provide new insights into the relationships between fine-scale canyon morphology and down-canyon changes in sediment flow dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=10512&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=10512&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dactive%2Bvolcanoes"><span>Klyuchevskaya <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2007-01-01</p> <p>The Klyuchevskaya <span class="hlt">Volcano</span> on Russia's Kamchatka Peninsula continued its ongoing <span class="hlt">activity</span> by releasing another plume on May 24, 2007. The same day, the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Terra satellite captured this image, at 01:00 UTC. In this image, a hotspot marks the <span class="hlt">volcano</span>'s summit. Outlined in red, the hotspot indicates where MODIS detected unusually warm surface temperatures. Blowing southward from the summit is the plume, which casts its shadow on the clouds below. Near the summit, the plume appears gray, and it lightens toward the south. With an altitude of 4,835 meters (15,863 feet), Klyuchevskaya (sometimes spelled Klyuchevskoy or Kliuchevskoi) is both the highest and most <span class="hlt">active</span> <span class="hlt">volcano</span> on the Kamchatka Peninsula. As part of the Pacific 'Ring of Fire,' the peninsula experiences regular seismic <span class="hlt">activity</span> as the Pacific Plate slides below other tectonic plates in the Earth's crust. Klyuchevskaya is estimated to have experienced more than 100 flank eruptions in the past 3,000 years. Since its formation 6,000 years ago, the <span class="hlt">volcano</span> has seen few periods of inactivity. NASA image courtesy the MODIS Rapid Response Team at NASA GSFC. The Rapid Response Team provides daily images of this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25671714','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25671714"><span>Transient changes in bacterioplankton communities induced by the <span class="hlt">submarine</span> volcanic eruption of El Hierro (Canary Islands).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ferrera, Isabel; Arístegui, Javier; González, José M; Montero, María F; Fraile-Nuez, Eugenio; Gasol, Josep M</p> <p>2015-01-01</p> <p>The <span class="hlt">submarine</span> volcanic eruption occurring near El Hierro (Canary Islands) in October 2011 provided a unique opportunity to determine the effects of such events on the microbial populations of the surrounding waters. The birth of a new underwater <span class="hlt">volcano</span> produced a large plume of vent material detectable from space that led to abrupt changes in the physical-chemical properties of the water column. We combined flow cytometry and 454-pyrosequencing of 16S rRNA gene amplicons (V1-V3 regions for Bacteria and V3-V5 for Archaea) to monitor the area around the <span class="hlt">volcano</span> through the eruptive and post-eruptive phases (November 2011 to April 2012). Flow cytometric analyses revealed higher abundance and relative <span class="hlt">activity</span> (expressed as a percentage of high-nucleic acid content cells) of heterotrophic prokaryotes during the eruptive process as compared to post-eruptive stages. Changes observed in populations detectable by flow cytometry were more evident at depths closer to the <span class="hlt">volcano</span> (~70-200 m), coinciding also with oxygen depletion. Alpha-diversity analyses revealed that species richness (Chao1 index) decreased during the eruptive phase; however, no dramatic changes in community composition were observed. The most abundant taxa during the eruptive phase were similar to those in the post-eruptive stages and to those typically prevalent in oceanic bacterioplankton communities (i.e. the alphaproteobacterial SAR11 group, the Flavobacteriia class of the Bacteroidetes and certain groups of Gammaproteobacteria). Yet, although at low abundance, we also detected the presence of taxa not typically found in bacterioplankton communities such as the Epsilonproteobacteria and members of the candidate division ZB3, particularly during the eruptive stage. These groups are often associated with deep-sea hydrothermal vents or sulfur-rich springs. Both cytometric and sequence analyses showed that once the eruption ceased, evidences of the <span class="hlt">volcano</span>-induced changes were no longer observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4324844','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4324844"><span>Transient Changes in Bacterioplankton Communities Induced by the <span class="hlt">Submarine</span> Volcanic Eruption of El Hierro (Canary Islands)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ferrera, Isabel; Arístegui, Javier; González, José M.; Montero, María F.; Fraile-Nuez, Eugenio; Gasol, Josep M.</p> <p>2015-01-01</p> <p>The <span class="hlt">submarine</span> volcanic eruption occurring near El Hierro (Canary Islands) in October 2011 provided a unique opportunity to determine the effects of such events on the microbial populations of the surrounding waters. The birth of a new underwater <span class="hlt">volcano</span> produced a large plume of vent material detectable from space that led to abrupt changes in the physical-chemical properties of the water column. We combined flow cytometry and 454-pyrosequencing of 16S rRNA gene amplicons (V1–V3 regions for Bacteria and V3–V5 for Archaea) to monitor the area around the <span class="hlt">volcano</span> through the eruptive and post-eruptive phases (November 2011 to April 2012). Flow cytometric analyses revealed higher abundance and relative <span class="hlt">activity</span> (expressed as a percentage of high-nucleic acid content cells) of heterotrophic prokaryotes during the eruptive process as compared to post-eruptive stages. Changes observed in populations detectable by flow cytometry were more evident at depths closer to the <span class="hlt">volcano</span> (~70–200 m), coinciding also with oxygen depletion. Alpha-diversity analyses revealed that species richness (Chao1 index) decreased during the eruptive phase; however, no dramatic changes in community composition were observed. The most abundant taxa during the eruptive phase were similar to those in the post-eruptive stages and to those typically prevalent in oceanic bacterioplankton communities (i.e. the alphaproteobacterial SAR11 group, the Flavobacteriia class of the Bacteroidetes and certain groups of Gammaproteobacteria). Yet, although at low abundance, we also detected the presence of taxa not typically found in bacterioplankton communities such as the Epsilonproteobacteria and members of the candidate division ZB3, particularly during the eruptive stage. These groups are often associated with deep-sea hydrothermal vents or sulfur-rich springs. Both cytometric and sequence analyses showed that once the eruption ceased, evidences of the <span class="hlt">volcano</span>-induced changes were no longer observed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS51E..02C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS51E..02C"><span>Near-Seafloor Magnetic Exploration of <span class="hlt">Submarine</span> Hydrothermal Systems in the Kermadec Arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caratori Tontini, F.; de Ronde, C. E. J.; Tivey, M.; Kinsey, J. C.</p> <p>2014-12-01</p> <p>Magnetic data can provide important information about hydrothermal systems because hydrothermal alteration can drastically reduce the magnetization of the host volcanic rocks. Near-seafloor data (≤70 m altitude) are required to map hydrothermal systems in detail; Autonomous Underwater Vehicles (AUVs) are the ideal platform to provide this level of resolution. Here, we show the results of high-resolution magnetic surveys by the ABE and Sentry AUVs for selected <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> of the Kermadec arc. 3-D magnetization models derived from the inversion of magnetic data, when combined with high resolution seafloor bathymetry derived from multibeam surveys, provide important constraints on the subseafloor geometry of hydrothermal upflow zones and the structural control on the development of seafloor hydrothermal vent sites as well as being a tool for the discovery of previously unknown hydrothermal sites. Significant differences exist between the magnetic expressions of hydrothermal sites at caldera <span class="hlt">volcanoes</span> ("donut" pattern) and cones ("Swiss cheese" pattern), respectively. Subseafloor 3-D magnetization models also highlight structural differences between focused and diffuse vent sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.G51B1108M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.G51B1108M"><span>InSAR observations of <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Latin America</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morales Rivera, A. M.; Chaussard, E.; Amelung, F.</p> <p>2012-12-01</p> <p>Over the last decade satellite-based interferometric synthetic aperture radar (InSAR) has developed into a well-known technique to gauge the status of <span class="hlt">active</span> <span class="hlt">volcanoes</span>. The InSAR technique can detect the ascent of magma to shallow levels of the volcanic plumbing system because new arriving magma pressurizes the system. This is likely associated with the inflation of the volcanic edifice and the surroundings. Although the potential of InSAR to detect magma migration is well known, the principal limitation was that only for few <span class="hlt">volcanoes</span> frequent observations were acquired. The ALOS-1 satellite of the Japanese Aerospace Exploration Agency (JAXA) acquired a global L-band data set of 15-20 acquisitions during 2006-2011. Here we use ALOS InSAR and Small Baseline (SB) time-series methods for a ground deformation survey of Latin America with emphasis on the northern Andes. We present time-dependent ground deformation data for the <span class="hlt">volcanoes</span> in Colombia, Ecuador and Peru and interpret the observations in terms of the dynamics of the volcanic systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-0202485&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-0202485&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dactive%2Bvolcanoes"><span>Erupting <span class="hlt">Volcano</span> Mount Etna</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2001-01-01</p> <p>An Expedition Two crewmember aboard the International Space Station (ISS) captured this overhead look at the smoke and ash regurgitated from the erupting <span class="hlt">volcano</span> Mt. Etna on the island of Sicily, Italy. At an elevation of 10,990 feet (3,350 m), the summit of the Mt. Etna <span class="hlt">volcano</span>, one of the most <span class="hlt">active</span> and most studied <span class="hlt">volcanoes</span> in the world, has been <span class="hlt">active</span> for a half-million years and has erupted hundreds of times in recorded history.</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://pubs.usgs.gov/of/1996/0024/body.html','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1996/0024/body.html"><span>Volcanic <span class="hlt">activity</span> in Alaska: summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory 1993</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Neal, Christina A.; McGimsey, Robert G.; Doukas, Michael P.</p> <p>1996-01-01</p> <p>During 1993, the Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to episodes of eruptive <span class="hlt">activity</span> or false alarms at nine volcanic centers in the state of Alaska. Additionally, as part of a formal role in KVERT (the Kamchatkan <span class="hlt">Volcano</span> Eruption Response Team), AVO staff also responded to eruptions on the Kamchatka Peninsula, details of which are summarized in Miller and Kurianov (1993). In 1993, AVO maintained seismic instrumentation networks on four <span class="hlt">volcanoes</span> of the Cook Inlet region--Spurr, Redoubt, Iliamna, and Augustine--and two stations at Dutton <span class="hlt">Volcano</span> near King Cove on the Alaska Peninsula. Other routine elements of AVO's <span class="hlt">volcano</span> monitoring program in Alaska include periodic airborne measurement of volcanic SO2 and CO2 at Cook Inlet <span class="hlt">volcanoes</span> (Doukas, 1995) and maintenance of a lightning detection system in Cook Inlet (Paskievitch and others, 1995).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1999/0373/pdf/of99-373text.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1999/0373/pdf/of99-373text.pdf"><span>Preliminary <span class="hlt">volcano</span>-hazard assessment for Iliamna <span class="hlt">Volcano</span>, 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>Waythomas, Christopher F.; Miller, Thomas P.</p> <p>1999-01-01</p> <p>Iliamna <span class="hlt">Volcano</span> is a 3,053-meter-high, ice- and snow-covered stratovolcano in the southwestern Cook Inlet region about 225 kilometers southwest of Anchorage and about 100 kilometers northwest of Homer. Historical eruptions of Iliamna <span class="hlt">Volcano</span> have not been positively documented; however, the <span class="hlt">volcano</span> regularly emits steam and gas, and small, shallow earthquakes are often detected beneath the summit area. The most recent eruptions of the <span class="hlt">volcano</span> occurred about 300 years ago, and possibly as recently as 90-140 years ago. Prehistoric eruptions have generated plumes of volcanic ash, pyroclastic flows, and lahars that extended to the <span class="hlt">volcano</span> flanks and beyond. Rock avalanches from the summit area have occurred numerous times in the past. These avalanches flowed several kilometers down the flanks and at least two large avalanches transformed to cohesive lahars. The number and distribution of known volcanic ash deposits from Iliamna <span class="hlt">Volcano</span> indicate that volcanic ash clouds from prehistoric eruptions were significantly less voluminous and probably less common relative to ash clouds generated by eruptions of other Cook Inlet <span class="hlt">volcanoes</span>. Plumes of volcanic ash from Iliamna <span class="hlt">Volcano</span> would be a major hazard to jet aircraft using Anchorage International Airport and other local airports, and depending on wind direction, could drift at least as far as the Kenai Peninsula and beyond. Ashfall from future eruptions could disrupt oil and gas operations and shipping <span class="hlt">activities</span> in Cook Inlet. Because Iliamna <span class="hlt">Volcano</span> has not erupted for several hundred years, a future eruption could involve significant amounts of ice and snow that could lead to the formation of large lahars and downstream flooding. The greatest hazards in order of importance are described below and shown on plate 1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA06841&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA06841&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dactive%2Bvolcanoes"><span>Small Tharsis <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2004-01-01</p> <p><p/> 30 August 2004 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a small <span class="hlt">volcano</span> located southwest of the giant <span class="hlt">volcano</span>, Pavonis Mons, near 2.5oS, 109.4oW. Lava flows can be seen to have emanated from the summit region, which today is an irregularly-shaped collapse pit, or <i>caldera</i>. A blanket of dust mantles this <span class="hlt">volcano</span>. Dust covers most martian <span class="hlt">volcanoes</span>, none of which are young or <span class="hlt">active</span> today. This picture covers an area about 3 km (1.9 mi) across; sunlight illuminates the scene from the left.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V33E..08T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V33E..08T"><span>Dueling <span class="hlt">Volcanoes</span>: How <span class="hlt">Activity</span> Levels At Kilauea Influence Eruptions At Mauna Loa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Trusdell, F.</p> <p>2011-12-01</p> <p>The eruption of Kilauea at Pu`u `O`o is approaching its 29th anniversary. During this time, Mauna Loa has slowly inflated following its most recent eruption in 1984. This is Mauna Loa's longest inter-eruptive interval observed in HVO's 100 years of operation. When will the next eruption of Mauna Loa take place? Is the next eruption of Mauna Loa tied to the current <span class="hlt">activity</span> at Kilauea? Historically, eruptive periods at Kilauea and Mauna Loa <span class="hlt">volcanoes</span> appear to be inversely correlated. In the past, when Mauna Loa was exceptionally <span class="hlt">active</span>, Kilauea <span class="hlt">Volcano</span> was in repose, recovery, or in sustained lava lake <span class="hlt">activity</span>. Swanson and co-workers (this meeting) have noted that explosive <span class="hlt">activity</span> on Kilauea, albeit sporadic, was interspersed between episodes of effusive <span class="hlt">activity</span>. Specifically, Swanson and co-workers note as explosive the time periods between 300 B.C.E.-1000 C.E and 1500-1800 C.E. They also point to evidence for low magma supply to Kilauea during these periods and few flank eruptions. During the former explosive period, Mauna Loa was exceedingly <span class="hlt">active</span>, covering approximately 37% of its surface or 1882 km2, an area larger than Kilauea. This period is also marked by summit <span class="hlt">activity</span> at Mauna Loa sustained for 300 years. In the 1500-1800 C.E. period, Mauna Loa was conspicuously <span class="hlt">active</span> with 29 eruptions covering an area of 446 km2. In the late 19th and early 20th century, Kilauea was dominated by nearly continuous lava-lake <span class="hlt">activity</span>. Meanwhile Mauna Loa was frequently <span class="hlt">active</span> from 1843 C.E. to 1919 C.E., with 24 eruptions for an average repose time of 3.5 years. I propose that eruptive <span class="hlt">activity</span> at one <span class="hlt">volcano</span> may affect eruptions at the other, due to factors that impact magma supply, volcanic plumbing, and flank motion. This hypothesis is predicated on the notion that when the rift zones of Kilauea, and in turn its mobile south flank, are <span class="hlt">active</span>, Mauna Loa's tendency to erupt is diminished. Kilauea's rift zones help drive the south flank seaward, in turn, as Mauna</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032610','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032610"><span>Methods of InSAR atmosphere correction for <span class="hlt">volcano</span> <span class="hlt">activity</span> monitoring</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gong, W.; Meyer, F.; Webley, P.W.; Lu, Z.</p> <p>2011-01-01</p> <p>When a Synthetic Aperture Radar (SAR) signal propagates through the atmosphere on its path to and from the sensor, it is inevitably affected by atmospheric effects. In particular, the applicability and accuracy of Interferometric SAR (InSAR) techniques for <span class="hlt">volcano</span> monitoring is limited by atmospheric path delays. Therefore, atmospheric correction of interferograms is required to improve the performance of InSAR for detecting volcanic <span class="hlt">activity</span>, especially in order to advance its ability to detect subtle pre-eruptive changes in deformation dynamics. In this paper, we focus on InSAR tropospheric mitigation methods and their performance in <span class="hlt">volcano</span> deformation monitoring. Our study areas include Okmok <span class="hlt">volcano</span> and Unimak Island located in the eastern Aleutians, AK. We explore two methods to mitigate atmospheric artifacts, namely the numerical weather model simulation and the atmospheric filtering using Persistent Scatterer processing. We investigate the capability of the proposed methods, and investigate their limitations and advantages when applied to determine volcanic processes. ?? 2011 IEEE.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2008/5114/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2008/5114/"><span>Instrumentation Recommendations for <span class="hlt">Volcano</span> Monitoring at U.S. <span class="hlt">Volcanoes</span> Under the National <span class="hlt">Volcano</span> Early Warning 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>Moran, Seth C.; Freymueller, Jeff T.; LaHusen, Richard G.; McGee, Kenneth A.; Poland, Michael P.; Power, John A.; Schmidt, David A.; Schneider, David J.; Stephens, George; Werner, Cynthia A.; White, Randall A.</p> <p>2008-01-01</p> <p>As magma moves toward the surface, it interacts with anything in its path: hydrothermal systems, cooling magma bodies from previous eruptions, and (or) the surrounding 'country rock'. Magma also undergoes significant changes in its physical properties as pressure and temperature conditions change along its path. These interactions and changes lead to a range of geophysical and geochemical phenomena. The goal of <span class="hlt">volcano</span> monitoring is to detect and correctly interpret such phenomena in order to provide early and accurate warnings of impending eruptions. Given the well-documented hazards posed by <span class="hlt">volcanoes</span> to both ground-based populations (for example, Blong, 1984; Scott, 1989) and aviation (for example, Neal and others, 1997; Miller and Casadevall, 2000), <span class="hlt">volcano</span> monitoring is critical for public safety and hazard mitigation. Only with adequate monitoring systems in place can <span class="hlt">volcano</span> observatories provide accurate and timely forecasts and alerts of possible eruptive <span class="hlt">activity</span>. At most U.S. <span class="hlt">volcanoes</span>, observatories traditionally have employed a two-component approach to <span class="hlt">volcano</span> monitoring: (1) install instrumentation sufficient to detect unrest at volcanic systems likely to erupt in the not-too-distant future; and (2) once unrest is detected, install any instrumentation needed for eruption prediction and monitoring. This reactive approach is problematic, however, for two reasons. 1. At many <span class="hlt">volcanoes</span>, rapid installation of new ground-1. based instruments is difficult or impossible. Factors that complicate rapid response include (a) eruptions that are preceded by short (hours to days) precursory sequences of geophysical and (or) geochemical <span class="hlt">activity</span>, as occurred at Mount Redoubt (Alaska) in 1989 (24 hours), Anatahan (Mariana Islands) in 2003 (6 hours), and Mount St. Helens (Washington) in 1980 and 2004 (7 and 8 days, respectively); (b) inclement weather conditions, which may prohibit installation of new equipment for days, weeks, or even months, particularly at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-s39-151-179.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-s39-151-179.html"><span>Klyuchevskaya, <span class="hlt">Volcano</span>, Kamchatka Peninsula, CIS</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1991-05-06</p> <p>STS039-151-179 (28 April-6 May 1991) --- A large format frame of one of the USSR's volcanic complex (Kamchatka area) with the <span class="hlt">active</span> <span class="hlt">volcano</span> Klyuchevskaya (Kloo-chevs'-ska-ya), 15,584 feet in elevation. The last reported eruption of the <span class="hlt">volcano</span> was on April 8, but an ash and steam plume extending to the south was observed by the STS-39 crew almost three weeks later. The south side of the <span class="hlt">volcano</span> is dirty from the ash fall and landslide <span class="hlt">activity</span>. The summit is clearly visible, as is the debris flow from an earlier eruption. Just north of the Kamchatka River is Shiveluch, a <span class="hlt">volcano</span> which was <span class="hlt">active</span> in early April. There are more than 100 volcanic edifices recognized on Kamchatka, with 15 classified as <span class="hlt">active</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V41B2786F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V41B2786F"><span>Insights from geophysical monitoring into the <span class="hlt">volcano</span> structure and magma supply systems at three very different oceanic islands in the Cape Verde archipelago</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faria, B. V.; Day, S.; Fonseca, J. F.</p> <p>2013-12-01</p> <p>Three oceanic <span class="hlt">volcano</span> islands in the west of the Cape Verde archipelago are considered to have the highest levels of volcanic hazard in the archipelago: Fogo, Brava, and Santo Antao. Fogo has had frequent mainly effusive eruptions in historic time, the most recent in 1995, whilst Brava and Santo Antao have ongoing geothermal <span class="hlt">activity</span> and felt earthquakes, and have experienced geologically recent violent explosive eruptions. Therefore, these three islands have been the focus of recent efforts to set up seismic networks to monitor their <span class="hlt">activity</span>. Here we present the first results from these networks, and propose interpretations of the monitored seismic <span class="hlt">activity</span> in terms of subsurface <span class="hlt">volcano</span> structures, near-surface intrusive <span class="hlt">activity</span> and seasonal controls on geothermal <span class="hlt">activity</span>. In Fogo, most recorded seismic events are hydrothermal events. These show a strong seasonal variation, increasing during the summer rain season and decreasing afterwards. Rare <span class="hlt">volcano</span>-tectonic (VT) events (0.1<ML<3.5), forming only 2% of the <span class="hlt">activity</span>, are located mainly in and below the Monte Amarelo lateral collapse scar. They are interpreted as shear failures between unconsolidated material at the base of the collapse scar fill and underlying more rigid pre-collapse rocks with abundant dikes, occuring as a result of long-term gravitational re-adjustment of the collapse scar fill after inflation of the island due to the 1995 eruption. Brava experiences frequent swarms of VT events. These are located mostly offshore, with a small proportion of on-shore events. The positions of offshore events are strongly correlated with seamounts and hence are interpreted as due to <span class="hlt">submarine</span> volcanic processes. Onshore events (0.7<ML<1.1) are probably related to the long-term uplift of the island that has been indicated by previous geological studies, and may be due to inflation of a magma reservoir in the edifice. S. Antão is characterized by frequent seismic swarms composed of VT earthquakes (0.1<ML<4</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=STS039-77-010&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=STS039-77-010&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dactive%2Bvolcanoes"><span>Klyuchevskaya, <span class="hlt">Volcano</span>, Kamchatka Peninsula, CIS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1991-01-01</p> <p>Klyuchevskaya, <span class="hlt">Volcano</span>, Kamchatka Peninsula, CIS (56.0N, 160.5E) is one of several <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the CIS and is 15,584 ft. in elevation. Fresh ash fall on the south side of the caldera can be seen as a dirty smudge on the fresh snowfall. Just to the north of the Kamchatka River is Shiveluch, a <span class="hlt">volcano</span> which had been <span class="hlt">active</span> a short time previously. There are more than 100 volcanic edifices recognized on Kamchatka, 15 of which are still <span class="hlt">active</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFMIN41A1120V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFMIN41A1120V"><span>The New USGS <span class="hlt">Volcano</span> Hazards Program Web Site</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Venezky, D. Y.; Graham, S. E.; Parker, T. J.; Snedigar, S. F.</p> <p>2008-12-01</p> <p>The U.S. Geological Survey's (USGS) <span class="hlt">Volcano</span> Hazard Program (VHP) has launched a revised web site that uses a map-based interface to display hazards information for U.S. <span class="hlt">volcanoes</span>. The web site is focused on better communication of hazards and background <span class="hlt">volcano</span> information to our varied user groups by reorganizing content based on user needs and improving data display. The Home Page provides a synoptic view of the <span class="hlt">activity</span> level of all <span class="hlt">volcanoes</span> for which updates are written using a custom Google® Map. Updates are accessible by clicking on one of the map icons or clicking on the <span class="hlt">volcano</span> of interest in the adjacent color-coded list of updates. The new navigation provides rapid access to volcanic <span class="hlt">activity</span> information, background <span class="hlt">volcano</span> information, images and publications, volcanic hazards, information about VHP, and the USGS <span class="hlt">volcano</span> observatories. The Volcanic <span class="hlt">Activity</span> section was tailored for emergency managers but provides information for all our user groups. It includes a Google® Map of the <span class="hlt">volcanoes</span> we monitor, an Elevated <span class="hlt">Activity</span> Page, a general status page, information about our <span class="hlt">Volcano</span> Alert Levels and Aviation Color Codes, monitoring information, and links to monitoring data from VHP's <span class="hlt">volcano</span> observatories: Alaska <span class="hlt">Volcano</span> Observatory (AVO), Cascades <span class="hlt">Volcano</span> Observatory (CVO), Long Valley Observatory (LVO), Hawaiian <span class="hlt">Volcano</span> Observatory (HVO), and Yellowstone <span class="hlt">Volcano</span> Observatory (YVO). The YVO web site was the first to move to the new navigation system and we are working on integrating the Long Valley Observatory web site next. We are excited to continue to implement new geospatial technologies to better display our hazards and supporting <span class="hlt">volcano</span> information.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21656823','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21656823"><span>Prokaryotic diversity of an <span class="hlt">active</span> mud <span class="hlt">volcano</span> in the Usu City of Xinjiang, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Hong-Mei; Lou, Kai; Sun, Jian; Zhang, Tao; Ma, Xiao-Long</p> <p>2012-02-01</p> <p>The Usu mud <span class="hlt">volcanoes</span> are the largest group of terrestrial mud <span class="hlt">volcanoes</span> in China. The <span class="hlt">volcanoes</span> are located in a typical arid and semi-arid region, and the group consists of 36 erupting <span class="hlt">active</span> mud <span class="hlt">volcanoes</span>. In this study, the prokaryotic diversity and community structure in the sediment of an <span class="hlt">active</span> mud <span class="hlt">volcano</span> were investigated by constructing bacterial and archaeal clone libraries of the 16S rRNA gene. A total of 100 bacterial and 100 archaeal clones were analysed and found to comprise 11 and 7 distinct phylotypes, respectively. The bacterial phylotypes were classified into three phyla (Proteobacteria, Actinobacteria, and Fusobacteria). Of these, Proteobacteria were the most abundant bacterial group, with Deltaproteobacteria dominating the sediment community, and these were affiliated with the order Desulfuromonadales. The archaeal phylotypes were all closely related to uncultivated species, and the majority of the members were related to the orders Methanosarcinales and Halobacteriales of the Euryarchaeota originating from methane hydrate bearing or alkaline sediments. The rest of the archaeal phylotypes belonged to the phylum Crenarchaeota, with representatives from similar habitats. These results suggested that a large number of novel microbial groups and potential methanogenesis may exist in this unique ecosystem. Copyright © 2012 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950004572&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950004572&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dactive%2Bvolcanoes"><span>Dante's <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1994-01-01</p> <p>This video contains two segments: one a 0:01:50 spot and the other a 0:08:21 feature. Dante 2, an eight-legged walking machine, is shown during field trials as it explores the inner depths of an <span class="hlt">active</span> <span class="hlt">volcano</span> at Mount Spurr, Alaska. A NASA sponsored team at Carnegie Mellon University built Dante to withstand earth's harshest conditions, to deliver a science payload to the interior of a <span class="hlt">volcano</span>, and to report on its journey to the floor of a <span class="hlt">volcano</span>. Remotely controlled from 80-miles away, the robot explored the inner depths of the <span class="hlt">volcano</span> and information from onboard video cameras and sensors was relayed via satellite to scientists in Anchorage. There, using a computer generated image, controllers tracked the robot's movement. Ultimately the robot team hopes to apply the technology to future planetary missions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V43E3195H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V43E3195H"><span>Control of Volume and Porosity on Pumice Floatation Time: A Case Study with Pumice from the Havre <span class="hlt">Submarine</span> Caldera <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hosseini, B.; Fauria, K.; Manga, M.; Carey, R.; Soule, S. A.</p> <p>2016-12-01</p> <p>During the 2015 MESH (Mapping, Exploration, and Sampling at Havre) expedition to the <span class="hlt">submarine</span> Havre caldera <span class="hlt">volcano</span>, we collected pumice from the 2012 eruption. Here, we report pumice volume, porosity, and floatation time from measurements on 32 clasts (0.2-16 g) that provide insight into the eruption dynamics and mechanisms that deposited these clasts on the seafloor. We measured pumice volume using photogrammetry, capturing 100-180 images per sample. We used a series of open-source software—VisualSFM and MeshLab—to process the images and construct volume models. Combined with measurements of mass, we can determine pumice porosity. We calculated a mean porosity of 0.86+/-0.03 for the 32 samples. The lowest measured porosity of 0.78 was from a fragment of a giant 1.5-m diameter pumice clast. In addition to quantifying pumice volume and porosity, we conducted floatation experiments in which we cleaned, dried, and set the 32 samples on water and measured the time required for each clast to sink. Pumice floatation times varied from 0.8-226 days. We found that pumice floatation time scales with both pumice volume and porosity. These trends are consistent with a gas trapping mechanism for cold pumice floatation and suggest that pumice porosity, in addition to pumice volume, exerts an important control on the floatation time and fate of floating pumice. Despite the wide range of floatation times for these clasts, the proximal to vent collection suggests that these pumice (with the possible exception of the giant pumice fragment) were deposited on the seafloor soon after the 2012 eruption and never reached the ocean surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gip/99/pdf/gip99.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gip/99/pdf/gip99.pdf"><span>Alaska <span class="hlt">volcanoes</span> guidebook for teachers</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Adleman, Jennifer N.</p> <p>2011-01-01</p> <p>Alaska’s <span class="hlt">volcanoes</span>, like its abundant glaciers, charismatic wildlife, and wild expanses inspire and ignite scientific curiosity and generate an ever-growing source of questions for students in Alaska and throughout the world. Alaska is home to more than 140 <span class="hlt">volcanoes</span>, which have been <span class="hlt">active</span> over the last 2 million years. About 90 of these <span class="hlt">volcanoes</span> have been <span class="hlt">active</span> within the last 10,000 years and more than 50 of these have been <span class="hlt">active</span> since about 1700. The <span class="hlt">volcanoes</span> in Alaska make up well over three-quarters of <span class="hlt">volcanoes</span> in the United States that have erupted in the last 200 years. In fact, Alaska’s <span class="hlt">volcanoes</span> erupt so frequently that it is almost guaranteed that an Alaskan will experience a volcanic eruption in his or her lifetime, and it is likely they will experience more than one. It is hard to imagine a better place for students to explore <span class="hlt">active</span> volcanism and to understand volcanic hazards, phenomena, and global impacts. Previously developed teachers’ guidebooks with an emphasis on the <span class="hlt">volcanoes</span> in Hawaii <span class="hlt">Volcanoes</span> National Park (Mattox, 1994) and Mount Rainier National Park in the Cascade Range (Driedger and others, 2005) provide place-based resources and <span class="hlt">activities</span> for use in other volcanic regions in the United States. Along the lines of this tradition, this guidebook serves to provide locally relevant and useful resources and <span class="hlt">activities</span> for the exploration of numerous and truly unique volcanic landscapes in Alaska. This guidebook provides supplemental teaching materials to be used by Alaskan students who will be inspired to become educated and prepared for inevitable future volcanic <span class="hlt">activity</span> in Alaska. The lessons and <span class="hlt">activities</span> in this guidebook are meant to supplement and enhance existing science content already being taught in grade levels 6–12. Correlations with Alaska State Science Standards and Grade Level Expectations adopted by the Alaska State Department of Education and Early Development (2006) for grades six through eleven are listed at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2001/0482/pdf/of01-482.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2001/0482/pdf/of01-482.pdf"><span>Preliminary <span class="hlt">volcano</span>-hazard assessment for Mount Spurr <span class="hlt">Volcano</span>, 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>Waythomas, Christopher F.; Nye, Christopher J.</p> <p>2001-01-01</p> <p>Mount Spurr <span class="hlt">volcano</span> is an ice- and snow-covered stratovolcano complex located in the north-central Cook Inlet region about 100 kilometers west of Anchorage, Alaska. Mount Spurr <span class="hlt">volcano</span> consists of a breached stratovolcano, a lava dome at the summit of Mount Spurr, and Crater Peak vent, a small stratocone on the south flank of Mount Spurr <span class="hlt">volcano</span>. Historical eruptions of Crater Peak occurred in 1953 and 1992. These eruptions were relatively small but explosive, and they dispersed volcanic ash over areas of interior, south-central, and southeastern Alaska. Individual ash clouds produced by the 1992 eruption drifted east, north, and south. Within a few days of the eruption, the south-moving ash cloud was detected over the North Atlantic. Pyroclastic flows that descended the south flank of Crater Peak during both historical eruptions initiated volcanic-debris flows or lahars that formed temporary debris dams across the Chakachatna River, the principal drainage south of Crater Peak. Prehistoric eruptions of Crater Peak and Mount Spurr generated clouds of volcanic ash, pyroclastic flows, and lahars that extended to the <span class="hlt">volcano</span> flanks and beyond. A flank collapse on the southeast side of Mount Spurr generated a large debris avalanche that flowed about 20 kilometers beyond the <span class="hlt">volcano</span> into the Chakachatna River valley. The debris-avalanche deposit probably formed a large, temporary debris dam across the Chakachatna River. The distribution and thickness of volcanic-ash deposits from Mount Spurr <span class="hlt">volcano</span> in the Cook Inlet region indicate that volcanic-ash clouds from most prehistoric eruptions were as voluminous as those produced by the 1953 and 1992 eruptions. Clouds of volcanic ash emitted from the <span class="hlt">active</span> vent, Crater Peak, would be a major hazard to all aircraft using Ted Stevens Anchorage International Airport and other local airports and, depending on wind direction, could drift a considerable distance beyond the <span class="hlt">volcano</span>. Ash fall from future eruptions could disrupt many</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1813104P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1813104P"><span>Aerial monitoring in <span class="hlt">active</span> mud <span class="hlt">volcano</span> by UAV technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pisciotta, Antonino; Capasso, Giorgio; Madonia, Paolo</p> <p>2016-04-01</p> <p>UAV photogrammetry opens various new applications in the close range domain, combining aerial and terrestrial photogrammetry, but also introduces low-cost alternatives to the classical manned aerial photogrammetry. Between 2014 and 2015 tree aerial surveys have been carried out. Using a quadrotor drone, equipped with a compact camera, it was possible to generate high resolution elevation models and orthoimages of The "Salinelle", an <span class="hlt">active</span> mud <span class="hlt">volcanoes</span> area, located in territory of Paternò (South Italy). The main risks are related to the damages produced by paroxysmal events. Mud <span class="hlt">volcanoes</span> show different cyclic phases of <span class="hlt">activity</span>, including catastrophic events and periods of relative quiescence characterized by moderate <span class="hlt">activity</span>. Ejected materials often are a mud slurry of fine solids suspended in liquids which may include water and hydrocarbon fluids, the bulk of released gases are carbon dioxide, with some methane and nitrogen, usually pond-shaped of variable dimension (from centimeters to meters in diameter). The scope of the presented work is the performance evaluation of a UAV system that was built to rapidly and autonomously acquire mobile three-dimensional (3D) mapping data in a volcanic monitoring scenario.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11876194','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11876194"><span>Current <span class="hlt">submarine</span> atmosphere control technology.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mazurek, W</p> <p>1998-01-01</p> <p>Air purification in <span class="hlt">submarines</span> was introduced towards the end of World War II and was limited to the use of soda lime for the removal of carbon dioxide and oxygen candles for the regeneration of oxygen. The next major advances came with the advent of nuclear-powered <span class="hlt">submarines</span>. These included the development of regenerative and, sometimes, energy-intensive processes for comprehensive atmosphere revitalization. With the present development of conventional <span class="hlt">submarines</span> using air-independent propulsion there is a requirement for air purification similar to that of the nuclear-powered <span class="hlt">submarines</span> but it is constrained by limited power and space. Some progress has been made in the development of new technology and the adoption of air purification equipment used in the nuclear-powered <span class="hlt">submarines</span> for this application.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.S51D2707L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.S51D2707L"><span>Infrasound Monitoring of the Volcanic <span class="hlt">Activities</span> of Japanese <span class="hlt">Volcanoes</span> in Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, H. I.; Che, I. Y.; Shin, J. S.</p> <p>2015-12-01</p> <p>Since 1999 when our first infrasound array station(CHNAR) has been installed at Cheolwon, Korea Institute of Geoscience and Mineral Resources(KIGAM) is continuously observing infrasound signals with an infrasound array network, named KIN(Korean Infrasound Network). This network is comprised of eight seismo-acoustic array stations(BRDAR, YPDAR, KMPAR, CHNAR, YAGAR, KSGAR, ULDAR, TJIAR). The aperture size of the smallest array is 300m and the largest is about 1.4km. The number of infrasound sensors are between 4(TJIAR) and 18(YAGAR), and 1~5 seismometers are collocated with infrasound sensors. Many interesting infrasound signals associated with different type of sources, such as blasting, large earthquake, bolide, volcanic explosion are detected by KIN in the past 15 years. We have analyzed the infrasound signals possibly associated with the japanese volcanic explosions with reference to volcanic <span class="hlt">activity</span> report published by Japanese Meteorological Agency. Analysis results of many events, for example, Asama <span class="hlt">volcano</span> explosion in 2004 and Shinmoe <span class="hlt">volcano</span> in 2011, are well matched with the official report. In some cases, however, corresponding infrasound signals are not identified. By comparison of the infrasound signals from different <span class="hlt">volcanoes</span>, we also found that the characteristics of signals are distinguishing. It may imply that the specific <span class="hlt">volcano</span> has its own unique fingerprint in terms of infrasound signal. It might be investigated by long-term infrasound monitoring for a specific <span class="hlt">volcano</span> as a ground truth generating repetitive infrasound signal.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JVGR..298...27M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JVGR..298...27M"><span>Cape Wanbrow: A stack of Surtseyan-style <span class="hlt">volcanoes</span> built over millions of years in the Waiareka-Deborah volcanic field, 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>Moorhouse, B. L.; White, J. D. L.; Scott, J. M.</p> <p>2015-06-01</p> <p> multiple <span class="hlt">volcanoes</span> separated by time. An increase in bioclastic detritus upsequence suggests that the stack of deposits from overlapping <span class="hlt">volcanoes</span> built up into shallow enough waters for colonization to occur. This material was periodically shed from the top of the edifice to form bioclast-rich debris flow deposits of <span class="hlt">volcanoes</span> 4, 5 and 6. Since the eruption of Surtsey (1963-1965) many studies have been made of the resulting island, but the pre-emergent base remains <span class="hlt">submarine</span>, unincised and little studied. Eruption-fed density currents that formed deposits of the <span class="hlt">volcanoes</span> of Cape Wanbrow are inferred to be typical products of <span class="hlt">submarine</span> processes such as those that built Surtsey to the sea surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA22121.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA22121.html"><span>Indonesia's <span class="hlt">Active</span> Mount Agung <span class="hlt">Volcano</span> Imaged by NASA Spacecraft</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-10</p> <p>After a new small eruption sent an ash cloud 1.24 miles (2 kilometers) into the sky on Dec. 7, 2017, Indonesia's Mount Agung <span class="hlt">volcano</span> quieted down. This image was acquired Dec. 8 after the latest <span class="hlt">activity</span> by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on NASA's Terra satellite. The image shows vegetation in red colors. The summit crater has a hot spot (yellow) as detected by ASTER's thermal infrared channels. More than 65,00 residents continue to be evacuated from the <span class="hlt">volcano</span>'s danger zone in case of a major eruption. The image covers an area of 11 by 12.3 miles (17.8 by 19.8 kilometers), and is located at 8.3 degrees south, 115.5 degrees east. https://photojournal.jpl.nasa.gov/catalog/PIA22121</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('https://eric.ed.gov/?q=archimedes+AND+principle&pg=2&id=EJ758487','ERIC'); return false;" href="https://eric.ed.gov/?q=archimedes+AND+principle&pg=2&id=EJ758487"><span>Paint-Stirrer <span class="hlt">Submarine</span></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>Young, Jocelyn; Hardy, Kevin</p> <p>2007-01-01</p> <p>In this article, the authors discuss a unique and challenging laboratory exercise called, the paint-stir-stick <span class="hlt">submarine</span>, that keeps the students enthralled. The paint-stir-stick <span class="hlt">submarine</span> fits beautifully with the National Science Education Standards Physical Science Content Standard B, and with the California state science standards for physical…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860016394','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860016394"><span>Thematic mapper studies of Andean <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Francis, P. W.</p> <p>1986-01-01</p> <p>The primary objective was to identify all the <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Andean region of Bolivia. Morphological features of the Tata Sabaya <span class="hlt">volcano</span>, Bolivia, were studied with the thematic mapper. Details include marginal levees on lava and pyroclastic flows, and summit crater structure. Valley glacier moraine deposits, not easily identified on the multispectral band scanner, were also unambiguous, and provide useful marker horizons on large volcanic edifices which were built up in preglacial times but which were <span class="hlt">active</span> subsequently. With such high resolution imagery, it is not only possible to identify potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span>, but also to use standard photogeological interpretation to outline the history of individual <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.489...49M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.489...49M"><span>The pumice raft-forming 2012 Havre <span class="hlt">submarine</span> eruption was effusive</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Manga, Michael; Fauria, Kristen E.; Lin, Christina; Mitchell, Samuel J.; Jones, Meghan; Conway, Chris E.; Degruyter, Wim; Hosseini, Behnaz; Carey, Rebecca; Cahalan, Ryan; Houghton, Bruce F.; White, James D. L.; Jutzeler, Martin; Soule, S. Adam; Tani, Kenichiro</p> <p>2018-05-01</p> <p>A long-standing conceptual model for deep <span class="hlt">submarine</span> eruptions is that high hydrostatic pressure hinders degassing and acceleration, and suppresses magma fragmentation. The 2012 <span class="hlt">submarine</span> rhyolite eruption of Havre <span class="hlt">volcano</span> in the Kermadec arc provided constraints on critical parameters to quantitatively test these concepts. This eruption produced a >1 km3 raft of floating pumice and a 0.1 km3 field of giant (>1 m) pumice clasts distributed down-current from the vent. We address the mechanism of creating these clasts using a model for magma ascent in a conduit. We use water ingestion experiments to address why some clasts float and others sink. We show that at the eruption depth of 900 m, the melt retained enough dissolved water, and hence had a low enough viscosity, that strain-rates were too low to cause brittle fragmentation in the conduit, despite mass discharge rates similar to Plinian eruptions on land. There was still, however, enough exsolved vapor at the vent depth to make the magma buoyant relative to seawater. Buoyant magma was thus extruded into the ocean where it rose, quenched, and fragmented to produce clasts up to several meters in diameter. We show that these large clasts would have floated to the sea surface within minutes, where air could enter pore space, and the fate of clasts is then controlled by the ability to trap gas within their pore space. We show that clasts from the raft retain enough gas to remain afloat whereas fragments from giant pumice collected from the seafloor ingest more water and sink. The pumice raft and the giant pumice seafloor deposit were thus produced during a clast-generating effusive <span class="hlt">submarine</span> eruption, where fragmentation occurred above the vent, and the subsequent fate of clasts was controlled by their ability to ingest water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.8575O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.8575O"><span><span class="hlt">Volcano</span> Observations Using an Unmanned Autonomous Helicopter : seismic and GPS observations near the <span class="hlt">active</span> summit area of Sakurajima and Kirishima <span class="hlt">volcano</span>, Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ohminato, T.; Kaneko, T.; Koyama, T.; Watanabe, A.; Takeo, M.; Iguchi, M.; Honda, Y.</p> <p>2012-04-01</p> <p>Observations in the vicinity of summit area of <span class="hlt">active</span> <span class="hlt">volcanoes</span> are very important from various viewpoints such as understanding physical processes in the volcanic conduit. It is, however, highly difficult to install observation sensors near <span class="hlt">active</span> vents because of the risk of sudden eruptions. We have been developing a safe <span class="hlt">volcano</span> observation system based on an unmanned aerial vehicle (UAV). As an UAV, we adopted an unmanned autonomous helicopter manufactured by Yamaha-Motor Co., Ltd. We have also developed earthquake observation modules and GPS receiver modules that are exclusively designed for UAV installation at summit areas of <span class="hlt">active</span> <span class="hlt">volcanoes</span>. These modules are light weight, compact size, and solar powered. For data transmission, a commercial cellular-phone network is used. Our first application of the sensor installation by the UAV is Sakurajima, one of the most <span class="hlt">active</span> <span class="hlt">volcanos</span> in Japan. In November 2009, 2010, and 2011, we installed up to four seismic sensors within 2km from the <span class="hlt">active</span> summit crater. In the 2010 and 2011 operations, we succeeded in pulling up and collecting the sensor modules by using the UAV. In the 2011 experiment, we installed two GPS receivers near the summit area of Sakurajima <span class="hlt">volcano</span>. We also applied the UAV installation to another <span class="hlt">active</span> <span class="hlt">volcano</span>, Shinmoedake in Kirishima <span class="hlt">volcano</span> group. Since the sub-plinian eruption in February 2011, entering the area 3km from the summit of Shinmoe-dake has been prohibited. In May and November 2011, we installed seismic sensors and GPS receivers in the off-limit zone. Although the ground coupling of the seismic modules is not perfect due to the way they are installed, the signal-to-noise ratio of the seismic signals recorded by these modules is fairly good. Despite the low antenna height of 50 cm from the ground surface, the location errors in horizontal and vertical GPS components are 1cm and 3cm, respectively. For seismic signals associated with eruptions at Sakurajima from November 2010 to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988ESRv...24..383S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988ESRv...24..383S"><span><span class="hlt">Submarine</span> fans: Characteristics, models, classification, and reservoir potential</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shanmugam, G.; Moiola, R. J.</p> <p>1988-02-01</p> <p><span class="hlt">Submarine</span>-fan sequences are important hydrocarbon reservoirs throughout the world. <span class="hlt">Submarine</span>-fan sequences may be interpreted from bed-thickness trends, turbidite facies associations, log motifs, and seismic-reflection profiles. Turbidites occurring predominantly in channels and lobes (or sheet sands) constitute the major portion of <span class="hlt">submarine</span>-fan sequences. Thinning- and thickening-upward trends are suggestive of channel and lobe deposition, respectively. Mounded seismic reflections are commonly indicative of lower-fan depositional lobes. Fan models are discussed in terms of modern and ancient fans, attached and detached lobes, highly efficient and poorly efficient systems, and transverse and longitudinal fans. In general, depositional lobes are considered to be attached to feeder channels. <span class="hlt">Submarine</span> fans can be classified into four types based on their tectonic settings: (1) immature passive-margin fans (North Sea type); (2) mature passive-margin fans (Atlantic type); (3) <span class="hlt">active</span>-margin fans (Pacific type); and (4) mixed-setting fans. Immature passive-margin fans (e.g., Balder, North Sea), and <span class="hlt">active</span>-margin fans (e.g., Navy, Pacific Ocean) are usually small, sand-rich, and possess well developed lobes. Mature passive-margin fans (e.g., Amazon, Atlantic Ocean) are large, mud-rich, and do not develop typical lobes. However, sheet sands are common in the lower-fan regions of mature passive-margin fans. Mixed-setting fans display characteristics of either Atlantic type (e.g., Bengal, Bay of Bengal), or Pacific type (Orinoco, Caribbean), or both. Conventional channel-lobe models may not be applicable to fans associated with mature passive margins. <span class="hlt">Submarine</span> fans develop primarily during periods of low sea level on both <span class="hlt">active</span>- and passive-margin settings. Consequently, hydrocarbon-bearing fan sequences are associated generally with global lowstands of sea level. Channel-fill sandstones in most tectonic settings are potential reservoirs. Lobes exhibit the most favorable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10596778','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10596778"><span>A descriptive analysis of asthma in the U.S. Navy <span class="hlt">Submarine</span> Force.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sims, J R; Tibbles, P M; Jackman, R P</p> <p>1999-12-01</p> <p>The U.S. Navy <span class="hlt">Submarine</span> Force offers a unique opportunity to study asthma because of the relative socioeconomic and physical homogeneity of the population and the closed environment occupational exposure. Currently, asthma is disqualifying from <span class="hlt">submarine</span> service, which results in a significant loss of experienced personnel. We performed a retrospective analysis of 119 U.S. Navy <span class="hlt">submariner</span> disqualification packages for asthma between 1989-1993. We found a 0.16% annual period prevalence of asthma in the <span class="hlt">active</span> duty enlisted Atlantic Fleet <span class="hlt">Submarine</span> Force. Two groups of asthma disqualifications were identified with a significant increase above their proportional representation in the fleet: enlisted personnel (p < 0.01) and <span class="hlt">submarine</span> recruits (p < 0.0001). The proportion of African-American personnel also had a tendency toward increased asthma disqualification (p < 0.08). There were no differences in prevalence of asthma between crews of ballistic missile <span class="hlt">submarines</span> or fast attack <span class="hlt">submarines</span>. Asthma risk factors reported in the civilian literature (childhood history of asthma, family history of asthma and non-drug allergies) were highly represented in our study (41%, 46% and 68% of <span class="hlt">submariners</span>, respectively). Most disqualified <span class="hlt">submariners</span> had "mild" asthma based on the diagnostic work-up. The methacholine challenge test appeared to carry a disproportionate diagnostic weight despite its low specificity. Although the period prevalence of asthma is low in the U.S. Navy <span class="hlt">Submarine</span> Force, <span class="hlt">submariners</span> disqualified for asthma have similar historical and ethnic risk factors as the civilian population.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70047286','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70047286"><span>Estimating eruption temperature from thermal emission spectra of lava fountain <span class="hlt">activity</span> in the Erta'Ale (Ethiopia) <span class="hlt">volcano</span> lava lake: Implications for observing Io's <span class="hlt">volcanoes</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>Davies, Ashley G.; Keszthelyi, Laszlo P.; McEwen, Alfred S.</p> <p>2011-01-01</p> <p>We have analysed high-spatial-resolution and high-temporal-resolution temperature measurements of the <span class="hlt">active</span> lava lake at Erta'Ale <span class="hlt">volcano</span>, Ethiopia, to derive requirements for measuring eruption temperatures at Io's <span class="hlt">volcanoes</span>. Lava lakes are particularly attractive targets because they are persistent in <span class="hlt">activity</span> and large, often with ongoing lava fountain <span class="hlt">activity</span> that exposes lava at near-eruption temperature. Using infrared thermography, we find that extracting useful temperature estimates from remote-sensing data requires (a) high spatial resolution to isolate lava fountains from adjacent cooler lava and (b) rapid acquisition of multi-color data. Because existing spacecraft data of Io's <span class="hlt">volcanoes</span> do not meet these criteria, it is particularly important to design future instruments so that they will be able to collect such data. Near-simultaneous data at more than two relatively short wavelengths (shorter than 1 μm) are needed to constrain eruption temperatures. Resolving parts of the lava lake or fountains that are near the eruption temperature is also essential, and we provide a rough estimate of the required image scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035180','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035180"><span>Estimating eruption temperature from thermal emission spectra of lava fountain <span class="hlt">activity</span> in the Erta'Ale (Ethiopia) <span class="hlt">volcano</span> lava lake: Implications for observing Io's <span class="hlt">volcanoes</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>Davies, A.G.; Keszthelyi, L.; McEwen, A.S.</p> <p>2011-01-01</p> <p>We have analysed high-spatial-resolution and high-temporal-resolution temperature measurements of the <span class="hlt">active</span> lava lake at Erta'Ale <span class="hlt">volcano</span>, Ethiopia, to derive requirements for measuring eruption temperatures at Io's <span class="hlt">volcanoes</span>. Lava lakes are particularly attractive targets because they are persistent in <span class="hlt">activity</span> and large, often with ongoing lava fountain <span class="hlt">activity</span> that exposes lava at near-eruption temperature. Using infrared thermography, we find that extracting useful temperature estimates from remote-sensing data requires (a) high spatial resolution to isolate lava fountains from adjacent cooler lava and (b) rapid acquisition of multi-color data. Because existing spacecraft data of Io's <span class="hlt">volcanoes</span> do not meet these criteria, it is particularly important to design future instruments so that they will be able to collect such data. Near-simultaneous data at more than two relatively short wavelengths (shorter than 1 ??m) are needed to constrain eruption temperatures. Resolving parts of the lava lake or fountains that are near the eruption temperature is also essential, and we provide a rough estimate of the required image scale. ?? 2011 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.V51A..08D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.V51A..08D"><span>Revisiting Jorullo <span class="hlt">volcano</span> (Mexico): monogenetic or polygenetic <span class="hlt">volcano</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delgado Granados, H.; Roberge, J.; Farraz Montes, I. A.; Victoria Morales, A.; Pérez Bustamante, J. C.; Correa Olan, J. C.; Gutiérrez Jiménez, A. J.; Adán González, N.; Bravo Cardona, E. F.</p> <p>2007-05-01</p> <p>Jorullo <span class="hlt">volcano</span> is located near the volcanic front of the westernmost part of the Trans-Mexican Volcanic Belt, which is related to the subduction of the Cocos plate beneath the North American plate. This part of the TMVB is known as the Michoacán-Guanajuato Volcanic Field, a region where widespread monogenetic volcanism is present although polygenetic volcanism is also recognized (i. e. Tancítaro <span class="hlt">volcano</span>; Ownby et al., 2006). Jorullo <span class="hlt">volcano</span> was born in the middle of crop fields. During its birth several lava flows were emitted and several cones were constructed. The main cone is the Jorullo proper, but there is a smaller cone on the north (Volcán del Norte), and three smaller cones aligned N-S on the south (Unnamed cone, UC; Volcán de Enmedio, VE; and Volcán del Sur, VS). The cone of Jorullo <span class="hlt">volcano</span> is made up of tephra and lava flows erupted from the crater. The three southern cones show very interesting histories not described previously. VE erupted highly vesiculated tephras including xenoliths from the granitic basement. VS is made of spatter and bombs. A very well preserved hummocky morphology reveals that VE and VS collapsed towards the west. After the collapses, phreatomagmatic <span class="hlt">activity</span> took place at the UC blanketing VE, VS and the southern flank of the Jorullo cone with sticky surge deposits. The excellent study by Luhr and Carmichael (1985) indicates that during the course of the eruption, lavas evolved from primitive basalt to basaltic andesite, although explosive products show a reverse evolution pattern (Johnson et al., 2006). We mapped lava flows not described by the observers in the 18th century nor considered in previous geologic reports as part of the Jorullo lavas. These lavas are older, distributed to the west and south, and some of them resemble the lava flows from La Pilita <span class="hlt">volcano</span>, a cone older than Jorullo (Luhr and Carmichael, 1985). These lava flows were not considered before because they were not extruded during the 1759</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997JGR...10215021C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997JGR...10215021C"><span>Fluid flow and water-rock interaction in the East Rift Zone of Kilauea <span class="hlt">Volcano</span>, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Conrad, Mark E.; Thomas, Donald M.; Flexser, Steven; Vennemann, Torsten W.</p> <p>1997-07-01</p> <p>The East Rift Zone of Kilauea <span class="hlt">Volcano</span> in Hawaii represents a major area of geothermal <span class="hlt">activity</span>. Fluid inclusion and stable isotope analyses of secondary hydrothermal minerals in core samples from three scientific observation holes (SOH) drilled into the rift zone indicate that the geothermal system is dominated by meteoric waters to depths of as much as 1500 m below sea level. Calculated δ18O and δD values for fluids on the north side of the rift zone indicate that the deep meteoric fluids may be derived from precipitation on the upper slopes of Mauna Loa <span class="hlt">Volcano</span>. In the interior of the rift zone, recharge is dominated by seawater mixed with local meteoric water. Water/rock ratios in the rift area are approximately 2, but strongly 18O-enriched fluids in the deeper parts of the SOH-2 and SOH-4 drill holes (on the north side of the rift) indicate that the fluids underwent extensive interaction with rocks prior to reaching this part of the rift zone. Marine carbonates at the subaerial to <span class="hlt">submarine</span> transition (between 1700 and 1780 m depth) in SOH-4 have not fully equilibrated with the fluids, suggesting that the onset of hydrothermal <span class="hlt">activity</span> in this area was relatively recent (<2000 years). This may represent increased volcanic <span class="hlt">activity</span> along the rift after the end of the Ai La'au phase of eruptive <span class="hlt">activity</span> at the Kilauea summit approximately 1000 years ago, or it may reflect progressive evolution of the hydrothermal system in response to southward migration of intrusive <span class="hlt">activity</span> within the rift.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2000/0519/pdf/of00-519.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2000/0519/pdf/of00-519.pdf"><span>Preliminary <span class="hlt">volcano</span>-hazard assessment for Aniakchak <span class="hlt">Volcano</span>, 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>Neal, Christina A.; McGimsey, Robert G.; Miller, Thomas P.; Riehle, James R.; Waythomas, Christopher F.</p> <p>2000-01-01</p> <p>Aniakchak is an <span class="hlt">active</span> <span class="hlt">volcano</span> located on the Alaska Peninsula 670 kilometers southwest of Anchorage. The <span class="hlt">volcano</span> consists of a dramatic, 10-kilometer-diameter, 0.5 to 1.0-kilometer-deep caldera that formed during a catastrophic eruption 3,500 years ago. Since then, at least a dozen separate vents within the caldera have erupted, often explosively, to produce lava flows and widespread tephra (ash) deposits. The most recent eruption at Aniakchak occurred in 1931 and was one of the largest explosive eruptions in Alaska in the last 100 years. Although Aniakchak <span class="hlt">volcano</span> presently shows no signs of unrest, explosive and nonexplosive eruptions will occur in the future. Awareness of the hazards posed by future eruptions is a key factor in minimizing impact.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMNH43B1758S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMNH43B1758S"><span>Eruptive history, current <span class="hlt">activity</span> and risk estimation using geospatial information in the Colima <span class="hlt">volcano</span>, Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suarez-Plascencia, C.; Camarena-Garcia, M.; Nunez-Cornu, F. J.; Flores-Peña, S.</p> <p>2013-12-01</p> <p>Colima <span class="hlt">volcano</span>, also known as Volcan de Fuego (19 30.696 N, 103 37.026 W), is located on the border between the states of Jalisco and Colima, and is the most <span class="hlt">active</span> <span class="hlt">volcano</span> in Mexico. In January 20, 1913, Colima had its biggest explosion of the twentieth century, with VEI 4, after the <span class="hlt">volcano</span> had been dormant for almost 40 years. In 1961, a dome reached the northeastern edge of the crater and started a new lava flow, and from this date maintains constant <span class="hlt">activity</span>. In February 10, 1999, a new explosion occurred at the summit dome. The <span class="hlt">activity</span> during the 2001-2005 period was the most intense, but did not exceed VEI 3. The <span class="hlt">activity</span> resulted in the formation of domes and their destruction after explosive events. The explosions originated eruptive columns, reaching altitudes between 4,500 and 9,000 masl, further pyroclastic flows reaching distances up to 3.5 km from the crater. During the explosive events, ash emissions were generated in all directions reaching distances up to 100 km, slightly affecting the nearby villages: Tuxpan, Tonila, Zapotlan, Cuauhtemoc, Comala, Zapotitlan de Vadillo and Toliman. During 2005 to July 2013, this <span class="hlt">volcano</span> has had an intense effusive-explosive <span class="hlt">activity</span>; similar to the one that took place during the period of 1890 through 1905. That was before the Plinian eruption of 1913, where pyroclastic flows reached a distance of 15 km from the crater. In this paper we estimate the risk of Colima <span class="hlt">volcano</span> through the analysis of the vulnerability variables, hazard and exposure, for which we use: satellite imagery, recurring Fenix helicopter over flights of the state government of Jalisco, the use of the images of Google Earth and the population census 2010 INEGI. With this information and data identified changes in economic <span class="hlt">activities</span>, development, and use of land. The expansion of the agricultural frontier in the lower sides of the <span class="hlt">volcano</span> Colima, and with the advancement of traditional crops of sugar cane and corn, increased the growth of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA13010.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA13010.html"><span>Sheveluch <span class="hlt">Volcano</span>, Kamchatka, Russia</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2010-04-05</p> <p>Sheveluch <span class="hlt">Volcano</span> in Kamchatka, Siberia, is one of the frequently <span class="hlt">active</span> <span class="hlt">volcanoes</span> located in eastern Siberia. In this image from NASA Terra spacecraft, brownish ash covers the southern part of the mountain, under an ash-laden vertical eruption plume.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-s73e5274.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-s73e5274.html"><span>Colima <span class="hlt">Volcano</span>, Mexico</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1995-10-29</p> <p>STS073-E-5274 (3 Nov. 1995) --- Colima was photographed with a color Electronic Still Camera (ESC) onboard the Earth-orbiting space shuttle Columbia. The <span class="hlt">volcano</span> lies due south of Guadalajara and Lake Chapala. It is considered to be one of Mexico's most <span class="hlt">active</span> and most dangerous <span class="hlt">volcanoes</span>, lying not far from heavily populated areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70042390','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70042390"><span>Rapid response of a hydrologic system to volcanic <span class="hlt">activity</span>: Masaya <span class="hlt">volcano</span>, Nicaragua</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pearson, S.C.P.; Connor, C.B.; Sanford, W.E.</p> <p>2008-01-01</p> <p>Hydrologic systems change in response to volcanic <span class="hlt">activity</span>, and in turn may be sensitive indicators of volcanic <span class="hlt">activity</span>. Here we investigate the coupled nature of magmatic and hydrologic systems using continuous multichannel time series of soil temperature collected on the flanks of Masaya <span class="hlt">volcano</span>, Nicaragua, one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Central America. The soil temperatures were measured in a low-temperature fumarole field located 3.5 km down the flanks of the <span class="hlt">volcano</span>. Analysis of these time series reveals that they respond extremely rapidly, on a time scale of minutes, to changes in volcanic <span class="hlt">activity</span> also manifested at the summit vent. These rapid temperature changes are caused by increased flow of water vapor through flank fumaroles during volcanism. The soil temperature response, ~5 °C, is repetitive and complex, with as many as 13 pulses during a single volcanic episode. Analysis of the frequency spectrum of these temperature time series shows that these anomalies are characterized by broad frequency content during volcanic <span class="hlt">activity</span>. They are thus easily distinguished from seasonal trends, diurnal variations, or individual rainfall events, which triggered rapid transient increases in temperature during 5% of events. We suggest that the mechanism responsible for the distinctive temperature signals is rapid change in pore pressure in response to magmatism, a response that can be enhanced by meteoric water infiltration. Monitoring of distal fumaroles can therefore provide insight into coupled volcanic-hydrologic-meteorologic systems, and has potential as an inexpensive monitoring tool.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V43A3125T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V43A3125T"><span>Mapping the <span class="hlt">Active</span> Vents of Stromboli <span class="hlt">Volcano</span> with an Unmanned Aerial Vehicle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turner, N.; Houghton, B. F.; von der Lieth, J.; Hort, M. K.; Taddeucci, J.; Kueppers, U.; Ricci, T.; Gaudin, D.</p> <p>2016-12-01</p> <p>We present a new detailed map of the <span class="hlt">active</span> vents of Stromboli <span class="hlt">volcano</span> obtained from UAV flights in May 2016, when the <span class="hlt">active</span> NE and SW craters were repeatedly mapped. Due to high levels of gas emissions and frequent explosions, fine-scale measurements of vent geometry from single flights were challenging. However, the compilation of data acquired over 12 flights used with Structure from Motion software allowed us to create a 10 cm Digital Elevation Model (DEM) offering a non-obstructed view into the <span class="hlt">active</span> craters. Such direct observations permits us to constrain parameters such as vent geometry and depth with an unprecedented precision, thus potentially reducing the uncertainty of models depending on such inputs (e.g. conduit and acoustic models). Furthermore, the low-cost and safety of UAVs allows mapping changes at small temporal and spatial resolutions, making this technique complementary to monitoring efforts at <span class="hlt">active</span> <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap9_Cashman.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1801/downloads/pp1801_Chap9_Cashman.pdf"><span>A century of studying effusive eruptions in Hawai'i: Chapter 9 in Characteristics of Hawaiian <span class="hlt">volcanoes</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>Cashman, Katherine V.; Mangan, Margaret T.; Poland, Michael P.; Takahashi, T. Jane; Landowski, Claire M.</p> <p>2014-01-01</p> <p>The Hawaiian <span class="hlt">Volcano</span> Observatory (HVO) was established as a natural laboratory to study volcanic processes. Since the most frequent form of volcanic <span class="hlt">activity</span> in Hawai‘i is effusive, a major contribution of the past century of research at HVO has been to describe and quantify lava flow emplacement processes. Lava flow research has taken many forms; first and foremost it has been a collection of basic observational data on <span class="hlt">active</span> lava flows from both Mauna Loa and Kīlauea <span class="hlt">volcanoes</span> that have occurred over the past 100 years. Both the types and quantities of observational data have changed with changing technology; thus, another important contribution of HVO to lava flow studies has been the application of new observational techniques. Also important has been a long-term effort to measure the physical properties (temperature, viscosity, crystallinity, and so on) of flowing lava. Field measurements of these properties have both motivated laboratory experiments and presaged the results of those experiments, particularly with respect to understanding the rheology of complex fluids. Finally, studies of the dynamics of lava flow emplacement have combined detailed field measurements with theoretical models to build a framework for the interpretation of lava flows in numerous other terrestrial, <span class="hlt">submarine</span>, and planetary environments. Here, we attempt to review all these aspects of lava flow studies and place them into a coherent framework that we hope will motivate future research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.V11C2312S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.V11C2312S"><span>Earth's <span class="hlt">Volcanoes</span> and their Eruptions; the 3rd edition of the Smithsonian Institution's <span class="hlt">Volcanoes</span> of the World</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siebert, L.; Simkin, T.; Kimberly, P.</p> <p>2010-12-01</p> <p>The 3rd edition of the Smithsonian Institution’s <span class="hlt">Volcanoes</span> of the World incorporates data on the world’s <span class="hlt">volcanoes</span> and their eruptions compiled since 1968 by the Institution’s Global Volcanism Program (GVP). Published this Fall jointly by the Smithsonian and the University of California Press, it supplements data from the 1994 2nd edition and includes new data on the number of people living in proximity to <span class="hlt">volcanoes</span>, the dominant rock lithologies at each <span class="hlt">volcano</span>, Holocene caldera-forming eruptions, and preliminary lists of Pleistocene <span class="hlt">volcanoes</span> and large-volume Pleistocene eruptions. The 3rd edition contains data on nearly 1550 <span class="hlt">volcanoes</span> of known or possible Holocene age, including chronologies, characteristics, and magnitudes for >10,400 Holocene eruptions. The standard 20 eruptive characteristics of the IAVCEI <span class="hlt">volcano</span> catalog series have been modified to include dated vertical edifice collapse events due to magma chamber evacuation following large-volume explosive eruptions or mafic lava effusion, and lateral sector collapse. Data from previous editions of <span class="hlt">Volcanoes</span> of the World are also supplemented by listings of up to the 5 most dominant lithologies at each <span class="hlt">volcano</span>, along with data on population living within 5, 10, 30, and 100 km radii of each <span class="hlt">volcano</span> or volcanic field. Population data indicate that the most populated regions also contain the most frequently <span class="hlt">active</span> <span class="hlt">volcanoes</span>. Eruption data document lava and tephra volumes and Volcanic Explosivity Index (VEI) assignments for >7800 eruptions. Interpretation of VRF data has led to documentation of global eruption rates and the power law relationship between magnitude and frequency of volcanic eruptions. Data with volcanic hazards implications include those on fatalities and evacuations and the rate at which eruptions reach their climax. In recognition of the hazards implications of potential resumption of <span class="hlt">activity</span> at pre-Holocene <span class="hlt">volcanoes</span>, the 3rd edition includes very preliminary lists of Pleistocene</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2008/1162/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2008/1162/"><span><span class="hlt">Active</span> <span class="hlt">Volcanoes</span> of the Kurile Islands: A Reference Guide for Aviation Users</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Neal, Christina A.; Rybin, Alexander; Chibisova, Marina; Miller, Edward</p> <p>2008-01-01</p> <p>Introduction: The many <span class="hlt">volcanoes</span> of the remote and mostly uninhabited Kurile Island arc (fig. 1; table 1) pose a serious hazard for air traffic in the North Pacific. Ash clouds from Kurile eruptions can impact some of the busiest air travel routes in the world and drift quickly into airspace managed by three countries: Russia, Japan, and the United States. Prevailing westerly winds throughout the region will most commonly send ash from any Kurile eruption directly across the parallel North Pacific airways between North America and Asia (Kristine A. Nelson, National Weather Service, oral commun., 2006; fig. 1). This report presents maps showing locations of the 36 most <span class="hlt">active</span> Kurile <span class="hlt">volcanoes</span> plotted on Operational Navigational Charts published by the Defense Mapping Agency (map sheets ONC F-10, F-11, and E-10; figs. 1, 2, 3, 4). These maps are intended to assist aviation and other users in the identification of restless Kurile <span class="hlt">volcanoes</span>. A regional map is followed by three subsections of the Kurile volcanic arc (North, Central, South). <span class="hlt">Volcanoes</span> and selected primary geographic features are labeled. All maps contain schematic versions of the principal air routes and selected air navigational fixes in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023450','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023450"><span>Mud <span class="hlt">volcanoes</span> of the Orinoco Delta, Eastern Venezuela</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Aslan, A.; Warne, A.G.; White, W.A.; Guevara, E.H.; Smyth, R.C.; Raney, J.A.; Gibeaut, J.C.</p> <p>2001-01-01</p> <p>Mud <span class="hlt">volcanoes</span> along the northwest margin of the Orinoco Delta are part of a regional belt of soft sediment deformation and diapirism that formed in response to rapid foredeep sedimentation and subsequent tectonic compression along the Caribbean-South American plate boundary. Field studies of five mud <span class="hlt">volcanoes</span> show that such structures consist of a central mound covered by <span class="hlt">active</span> and inactive vents. Inactive vents and mud flows are densely vegetated, whereas <span class="hlt">active</span> vents are sparsely vegetated. Four out of the five mud <span class="hlt">volcanoes</span> studied are currently <span class="hlt">active</span>. Orinoco mud flows consist of mud and clayey silt matrix surrounding lithic clasts of varying composition. Preliminary analysis suggests that the mud <span class="hlt">volcano</span> sediment is derived from underlying Miocene and Pliocene strata. Hydrocarbon seeps are associated with several of the <span class="hlt">active</span> mud <span class="hlt">volcanoes</span>. Orinoco mud <span class="hlt">volcanoes</span> overlie the crest of a mud-diapir-cored anticline located along the axis of the Eastern Venezuelan Basin. Faulting along the flank of the Pedernales mud <span class="hlt">volcano</span> suggests that fluidized sediment and hydrocarbons migrate to the surface along faults produced by tensional stresses along the crest of the anticline. Orinoco mud <span class="hlt">volcanoes</span> highlight the proximity of this major delta to an <span class="hlt">active</span> plate margin and the importance of tectonic influences on its development. Evaluation of the Orinoco Delta mud <span class="hlt">volcanoes</span> and those elsewhere indicates that these features are important indicators of compressional tectonism along deformation fronts of plate margins. ?? 2001 Elsevier Science B.V. All rights reserved.</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('http://adsabs.harvard.edu/abs/2016EGUGA..1814022N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814022N"><span>Diffuse degassing survey at the Higashi Izu monogenetic <span class="hlt">volcano</span> field, Japan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Notsu, Kenji; Pérez, Nemesio M.; Fujii, Naoyuki; Hernández, Pedro A.; Mori, Toshiya; Padrón, Eleazar; Melián, Gladys</p> <p>2016-04-01</p> <p>The Higashi-Izu monogenetic volcanic group, which consists of more than 60 <span class="hlt">volcanoes</span>, overlies the polygenetic <span class="hlt">volcanoes</span> in the eastern part of the Izu peninsula, Japan, which are distributed over the area of 350 km2. Some of the monogenetic <span class="hlt">volcanoes</span> are located on northwest-southeast alignments, suggesting that they developed along fissures. Recent volcanic <span class="hlt">activity</span> occurred offshore, e.g., at the Izu-Oshima <span class="hlt">volcano</span>, which erupted in 1986 and a <span class="hlt">submarine</span> eruption of the small new Teishi knoll off eastern Izu Peninsula in 1989 (Hasebe et al., 2001). This study was carried out to investigate the possible relationship of diffuse CO2 emission and the recent seismic <span class="hlt">activity</span> recorded NE of Higashi Izu monogenetic volcanic field, to quantify the rate at which CO2 is diffusely degassed from the studied area including Omuroyama <span class="hlt">volcano</span> and to identify the structures controlling the degassing process. Measurements were carried out over a three day period from 8-10 July 2013. Diffuse CO2 emission surveys were always carried out following the accumulation chamber method and spatial distribution maps were constructed following the sequential Gaussian simulation (sGs) procedure. Soil gas samples were collected at 30-40 cm depth by withdrawal into 60 cc hypodermic syringes to characterize the chemical and isotopic composition of the soil gas. At Omurayama <span class="hlt">volcano</span>, soil CO2 efflux values ranged from non-detectable to 97.5 g m-2 d-1, while at the seismic swarm zone ranged from 1.5 to 233.2 g m-2 d-1 and at the fault zone ranged from 5.7 to 101.2 g m-2 d-1. Probability-plot technique of all CO2 efflux data showed two different populations, background with a mean of 8.7 g m-2 d-1 and peak with a mean of 92.7 g m-2 d-1. In order to strength the deep seated contribution to the soil gases at the studied are, carbon isotopic analysis were performed in the CO2 gas. Soil gases (He, CO2 and N2) showed a clear mixing trend between air composition and a rich CO2 end member, suggesting the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title47-vol2/pdf/CFR-2011-title47-vol2-sec32-2424.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title47-vol2/pdf/CFR-2011-title47-vol2-sec32-2424.pdf"><span>47 CFR 32.2424 - <span class="hlt">Submarine</span> & deep sea cable.</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>2011-10-01</p> <p>... 47 Telecommunication 2 2011-10-01 2011-10-01 false <span class="hlt">Submarine</span> & deep sea cable. 32.2424 Section 32... <span class="hlt">Submarine</span> & deep sea cable. (a) This account shall include the original cost of <span class="hlt">submarine</span> cable and deep sea... defined below, are to be maintained for nonmetallic <span class="hlt">submarine</span> and deep sea cable and metallic <span class="hlt">submarine</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title47-vol2/pdf/CFR-2014-title47-vol2-sec32-2424.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title47-vol2/pdf/CFR-2014-title47-vol2-sec32-2424.pdf"><span>47 CFR 32.2424 - <span class="hlt">Submarine</span> & deep sea cable.</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>2014-10-01</p> <p>... 47 Telecommunication 2 2014-10-01 2014-10-01 false <span class="hlt">Submarine</span> & deep sea cable. 32.2424 Section 32... <span class="hlt">Submarine</span> & deep sea cable. (a) This account shall include the original cost of <span class="hlt">submarine</span> cable and deep sea... defined below, are to be maintained for nonmetallic <span class="hlt">submarine</span> and deep sea cable and metallic <span class="hlt">submarine</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title47-vol2/pdf/CFR-2010-title47-vol2-sec32-2424.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title47-vol2/pdf/CFR-2010-title47-vol2-sec32-2424.pdf"><span>47 CFR 32.2424 - <span class="hlt">Submarine</span> & deep sea cable.</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>... 47 Telecommunication 2 2010-10-01 2010-10-01 false <span class="hlt">Submarine</span> & deep sea cable. 32.2424 Section 32... <span class="hlt">Submarine</span> & deep sea cable. (a) This account shall include the original cost of <span class="hlt">submarine</span> cable and deep sea... defined below, are to be maintained for nonmetallic <span class="hlt">submarine</span> and deep sea cable and metallic <span class="hlt">submarine</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title47-vol2/pdf/CFR-2013-title47-vol2-sec32-2424.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title47-vol2/pdf/CFR-2013-title47-vol2-sec32-2424.pdf"><span>47 CFR 32.2424 - <span class="hlt">Submarine</span> & deep sea cable.</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>2013-10-01</p> <p>... 47 Telecommunication 2 2013-10-01 2013-10-01 false <span class="hlt">Submarine</span> & deep sea cable. 32.2424 Section 32... <span class="hlt">Submarine</span> & deep sea cable. (a) This account shall include the original cost of <span class="hlt">submarine</span> cable and deep sea... defined below, are to be maintained for nonmetallic <span class="hlt">submarine</span> and deep sea cable and metallic <span class="hlt">submarine</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title47-vol2/pdf/CFR-2012-title47-vol2-sec32-2424.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title47-vol2/pdf/CFR-2012-title47-vol2-sec32-2424.pdf"><span>47 CFR 32.2424 - <span class="hlt">Submarine</span> & deep sea cable.</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>2012-10-01</p> <p>... 47 Telecommunication 2 2012-10-01 2012-10-01 false <span class="hlt">Submarine</span> & deep sea cable. 32.2424 Section 32... <span class="hlt">Submarine</span> & deep sea cable. (a) This account shall include the original cost of <span class="hlt">submarine</span> cable and deep sea... defined below, are to be maintained for nonmetallic <span class="hlt">submarine</span> and deep sea cable and metallic <span class="hlt">submarine</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S13A0637J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S13A0637J"><span>P-wave velocity model of mud <span class="hlt">volcano</span> on the continental slope of the Canadian Beaufort Sea from frequency-domain full waveform inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jang, U. G.; Kang, S. G.; Hong, J. K.; Jin, Y. K.; Dallimore, S.; Riedel, M.; Paull, C. K.</p> <p>2017-12-01</p> <p>2014 Expedition ARA05C was a multidisciplinary undertaking conducted in the Canadian Beaufort Sea, Arctic Ocean on the Korean ice breaker IBRV ARAON from August 30 to September 19, 2014. The program was carried out as collaboration between the Korea Polar Research Institute (KOPRI), Geological Survey of Canada (GSC), Monterey Bay Aquarium Research Institute (MBARI), Department of Fisheries and Ocean (DFO) with participation by Bremen University (BARUM). During this expedition, multi-channel seismic (MCS) data were acquired on the outer continental shelf and upper slope of the Canadian Beaufort Sea, totaling 20 lines with 1,000 line-kilometers from September 1 to September 13, 2014. Three MCS survey lines was designed to cross the three <span class="hlt">submarine</span> mud <span class="hlt">volcanoes</span> found in the slope at approximate water depth of 290 m, 460 m and 740 m. <span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> are seafloor structures with positive topography formed by a combination of mud eruption, gas emission, and water seepage from the subsurface. MCS data will allow image subsurface structures of mud <span class="hlt">volcanoes</span> as identification of fluid migration pathways, however, imaging its subsurface structure is difficult by using conventional seismic data processing procedure, because it is seismically characterized by acoustically transparent facies. Full waveform inversion (FWI) is non-linear data-fitting procedure to estimate the physical properties of the subsurface by minimizing the difference between the observed and modelled data. FWI uses the two-wave wave equation to compute forward/backward wavefield to calculate the gradient direction, therefore it can derive more detailed velocity model beyond travel-time tomography techniques, which use only the kinematics of seismic data, by additional information provided by the amplitude and phase of the seismic waveform. In this study, we suggest P-wave structure of mud <span class="hlt">volcanos</span>, which were inverted by 2D acoustic FWI. It will be useful to understand the characterization of mud</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.V23A..08D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.V23A..08D"><span>Costa Rica's Chain of laterally collapsed <span class="hlt">volcanoes</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duarte, E.; Fernandez, E.</p> <p>2007-05-01</p> <p>From the NW extreme to the SW end of Costa Rica's volcanic backbone, a number of laterally collapsed <span class="hlt">volcanoes</span> can be observed. Due to several factors, attention has been given to <span class="hlt">active</span> <span class="hlt">volcanoes</span> disregarding the importance of collapsed features in terms of assessing volcanic hazards for future generations around inhabited <span class="hlt">volcanoes</span>. In several cases the typical horseshoe shape amphitheater-like depression can be easily observed. In other cases due to erosion, vegetation, topography, seismic <span class="hlt">activity</span> or drastic weather such characteristics are not easily recognized. In the order mentioned above appear: Orosi-Cacao, Miravalles, Platanar, Congo, Von Frantzius, Cacho Negro and Turrialba <span class="hlt">volcanoes</span>. Due to limited studies on these structures it is unknown if sector collapse occurred in one or several phases. Furthermore, in the few studied cases no evidence has been found to relate collapses to actual eruptive episodes. Detailed studies on the deposits and materials composing dome-like shapes will shed light on unsolved questions about petrological and chemical composition. Volume, form and distance traveled by deposits are part of the questions surrounding most of these collapsed <span class="hlt">volcanoes</span>. Although most of these mentioned structures are extinct, at least Irazú <span class="hlt">volcano</span> (<span class="hlt">active</span> <span class="hlt">volcano</span>) has faced partial lateral collapses recently. It did presented strombolian <span class="hlt">activity</span> in the early 60s. Collapse scars show on the NW flank show important mass removal in historic and prehistoric times. Moreover, in 1994 a minor hydrothermal explosion provoked the weakening of a deeply altered wall that holds a crater lake (150m diameter, 2.6x106 ). A poster will depict images of the collapsed <span class="hlt">volcanoes</span> named above with mayor descriptive characteristics. It will also focus on the importance of deeper studies to assess the collapse potential of Irazú <span class="hlt">volcano</span> with related consequences. Finally, this initiative will invite researchers interested in such topic to join future studies in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-s39-77-010.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-s39-77-010.html"><span>Klyuchevskaya, <span class="hlt">Volcano</span>, Kamchatka Peninsula, CIS</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1991-05-06</p> <p>STS039-77-010 (28 April 1991) --- The Kamchatka Peninsula, USSR. This oblique view of the eastern margin of the Kamchatka Peninsula shows pack-ice along the coast, which is drifting along with local currents and delineates the circulation patterns. Also visible are the Kamchatka River (left of center), and the volcanic complex with the <span class="hlt">active</span> <span class="hlt">volcano</span> Klyuchevskaya (Kloo-chevs'-ska-ya), 15,584 feet in elevation. The last reported eruption of the <span class="hlt">volcano</span> was on April 8, but an ash and steam plume extending to the south can be seen in this photograph, taken almost three weeks later (April 28). On April 29, the crew observed and photographed the <span class="hlt">volcano</span> again, and it was no longer visibly <span class="hlt">active</span>. However, the flanks of the mountain are dirty from the ash fall. Just north of the Kamchatka River (to the left, just off frame) is Shiveluch, a <span class="hlt">volcano</span> which was <span class="hlt">active</span> in early April. There are more than 100 volcanic edifices recognized on Kamchatka, with 15 classified as <span class="hlt">active</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH53B0148S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH53B0148S"><span><span class="hlt">Submarine</span> Landslide Hazards Offshore Southern Alaska: Seismic Strengthening Versus Rapid Sedimentation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sawyer, D.; Reece, R.; Gulick, S. P. S.; Lenz, B. L.</p> <p>2017-12-01</p> <p>The southern Alaskan offshore margin is prone to <span class="hlt">submarine</span> landslides and tsunami hazards due to seismically <span class="hlt">active</span> plate boundaries and extreme sedimentation rates from glacially enhanced mountain erosion. We examine the <span class="hlt">submarine</span> landslide potential with new shear strength measurements acquired by Integrated Ocean Drilling Program Expedition 341 on the continental slope and Surveyor Fan. These data reveal lower than expected sediment strength. Contrary to other <span class="hlt">active</span> margins where seismic strengthening enhances slope stability, the high-sedimentation margin offshore southern Alaska behaves like a passive margin from a shear strength perspective. We interpret that seismic strengthening occurs but is offset by high sedimentation rates and overpressure within the slope and Surveyor Fan. This conclusion is supported because shear strength follows an expected <span class="hlt">active</span> margin profile outside of the fan, where background sedimentation rates occur. More broadly, seismically <span class="hlt">active</span> margins with wet-based glaciers are susceptible to <span class="hlt">submarine</span> landslide hazards because of the combination of high sedimentation rates and earthquake shaking</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996JVGR...70..183A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996JVGR...70..183A"><span>Volcanic complexes in the eastern ridge of the Canary Islands: the Miocene <span class="hlt">activity</span> of the island of Fuerteventura</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ancochea, E.; Brändle, J. L.; Cubas, C. R.; Hernán, F.; Huertas, M. J.</p> <p>1996-03-01</p> <p>Fuerteventura has been since early stages of its growth the result of three different adjacent large volcanic complexes: Southern, Central and Northern. The definition of these volcanic complexes and their respective growing episodes is based on <span class="hlt">volcano</span>-stratigraphic, morphological and structural criteria, particularly radial dyke swarms. Each complex has its own prolonged history that might be longer than 10 m.y. During that time, several periods of <span class="hlt">activity</span> alternating with gaps accompanied by important erosion took place. The evolution of each volcanic complex has been partially independent but all the three are affected by at least three Miocene tectonic phases that controlled considerably their <span class="hlt">activity</span>. The volcanic complexes are deeply eroded and partially submerged. In the core of the Northern and the Central volcanic complexes there is a set of <span class="hlt">submarine</span> and plutonic rocks intensely traversed by a dyke swarm, known as the Basal Complex. The Basal Complex has been interpreted in different ways but all previous authors have considered it to be prior to the subaerial shield stage of the island. Here we advance the idea that the Basal Complex represent the <span class="hlt">submarine</span> growing stage of the volcanic complexes and the hypabyssal roots (plutons and dykes) of their successive subaerial growing episodes. Two seamounts situated nearby, southwest of the island, might be interpreted as remains of two other major <span class="hlt">volcanoes</span>. These two <span class="hlt">volcanoes</span>, together with those forming the present emerged island of Fuerteventura, and finally those of Famara and Los Ajaches situated further north on Lanzarote constitute a chain of <span class="hlt">volcanoes</span> located along a lineation which is subparallel to the northwestern African coastline and which may relate to early Atlantic spreading trends in the area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2017/5129/sir20175129.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2017/5129/sir20175129.pdf"><span>The 2014 eruptions of Pavlof <span class="hlt">Volcano</span>, 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>Waythomas, Christopher F.; Haney, Matthew M.; Wallace, Kristi; Cameron, Cheryl E.; Schneider, David J.</p> <p>2017-12-22</p> <p>Pavlof <span class="hlt">Volcano</span> is one of the most frequently <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Aleutian Island arc, having erupted more than 40 times since observations were first recorded in the early 1800s . The <span class="hlt">volcano</span> is located on the Alaska Peninsula (lat 55.4173° N, long 161.8937° W), near Izembek National Wildlife Refuge. The towns and villages closest to the <span class="hlt">volcano</span> are Cold Bay, Nelson Lagoon, Sand Point, and King Cove, which are all within 90 kilometers (km) of the <span class="hlt">volcano</span> (fig. 1). Pavlof is a symmetrically shaped stratocone that is 2,518 meters (m) high, and has about 2,300 m of relief. The <span class="hlt">volcano</span> supports a cover of glacial ice and perennial snow roughly 2 to 4 cubic kilometers (km3) in volume, which is mantled by variable amounts of tephra fall, rockfall debris, and pyroclastic-flow deposits produced during historical eruptions. Typical Pavlof eruptions are characterized by moderate amounts of ash emission, lava fountaining, spatter-fed lava flows, explosions, and the accumulation of unstable mounds of spatter on the upper flanks of the <span class="hlt">volcano</span>. The accumulation and subsequent collapse of spatter piles on the upper flanks of the <span class="hlt">volcano</span> creates hot granular avalanches, which erode and melt snow and ice, and thereby generate watery debris-flow and hyperconcentrated-flow lahars. Seismic instruments were first installed on Pavlof <span class="hlt">Volcano</span> in the early 1970s, and since then eruptive episodes have been better characterized and specific processes have been documented with greater certainty. The application of remote sensing techniques, including the use of infrasound data, has also aided the study of more recent eruptions. Although Pavlof <span class="hlt">Volcano</span> is located in a remote part of Alaska, it is visible from Cold Bay, Sand Point, and Nelson Lagoon, making distal observations of eruptive <span class="hlt">activity</span> possible, weather permitting. A busy air-travel corridor that is utilized by a numerous transcontinental and regional air carriers passes near Pavlof <span class="hlt">Volcano</span>. The frequency of air travel</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA19355.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA19355.html"><span>Costa Rica Turrialba <span class="hlt">Volcano</span>, Continued <span class="hlt">Activity</span> seen by NASA Spacecraft</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2015-04-06</p> <p>The March, 2015 eruption of Turrialba <span class="hlt">Volcano</span> in Costa Rica caught everyone by surprise as seen in this image from the ASTER instrument onboard NASA Terra spacecraft. <span class="hlt">Activity</span> had greatly diminished when the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) instrument on NASA's Terra spacecraft acquired this nighttime thermal infrared image on April 2, 2015. The hot summit crater appears in white, indicating continued volcanic unrest. To the west, Poas <span class="hlt">Volcano</span>'s hot crater lake also appears white, though its temperature is considerably less than Turrialba's crater. The large image covers an area of 28 by 39 miles (45 by 63 kilometers); the insets 2 by 2 miles (3.1 by 3.1 kilometers). The image is centered at 10.1 degrees north, 84 degrees west. http://photojournal.jpl.nasa.gov/catalog/PIA19355</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=GL-2002-001707&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=GL-2002-001707&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dactive%2Bvolcanoes"><span>Reunion Island <span class="hlt">Volcano</span> Erupts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2002-01-01</p> <p>On January 16, 2002, lava that had begun flowing on January 5 from the Piton de la Fournaise <span class="hlt">volcano</span> on the French island of Reunion abruptly decreased, marking the end of the <span class="hlt">volcano</span>'s most recent eruption. These false color MODIS images of Reunion, located off the southeastern coast of Madagascar in the Indian Ocean, were captured on the last day of the eruption (top) and two days later (bottom). The <span class="hlt">volcano</span> itself is located on the southeast side of the island and is dark brown compared to the surrounding green vegetation. Beneath clouds (light blue) and smoke, MODIS detected the hot lava pouring down the <span class="hlt">volcano</span>'s flanks into the Indian Ocean. The heat, detected by MODIS at 2.1 um, has been colored red in the January 16 image, and is absent from the lower image, taken two days later on January 18, suggesting the lava had cooled considerably even in that short time. Earthquake <span class="hlt">activity</span> on the northeast flank continued even after the eruption had stopped, but by January 21 had dropped to a sufficiently low enough level that the 24-hour surveillance by the local observatory was suspended. Reunion is essentially all <span class="hlt">volcano</span>, with the northwest portion of the island built on the remains of an extinct <span class="hlt">volcano</span>, and the southeast half built on the basaltic shield of 8,630-foot Piton de la Fournaise. A basaltic shield <span class="hlt">volcano</span> is one with a broad, gentle slope built by the eruption of fluid basalt lava. Basalt lava flows easily across the ground remaining hot and fluid for long distances, and so they often result in enormous, low-angle cones. The Piton de la Fournaise is one of Earth's most <span class="hlt">active</span> <span class="hlt">volcanoes</span>, erupting over 150 times in the last few hundred years, and it has been the subject of NASA research because of its likeness to the <span class="hlt">volcanoes</span> of Mars. Image courtesy Jacques Descloitres, MODIS Land Rapid Response Team at NASA GSFC</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26892716','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26892716"><span>Monitoring eruption <span class="hlt">activity</span> using temporal stress changes at Mount Ontake <span class="hlt">volcano</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Terakawa, Toshiko; Kato, Aitaro; Yamanaka, Yoshiko; Maeda, Yuta; Horikawa, Shinichiro; Matsuhiro, Kenjiro; Okuda, Takashi</p> <p>2016-02-19</p> <p>Volcanic <span class="hlt">activity</span> is often accompanied by many small earthquakes. Earthquake focal mechanisms represent the fault orientation and slip direction, which are influenced by the stress field. Focal mechanisms of <span class="hlt">volcano</span>-tectonic earthquakes provide information on the state of <span class="hlt">volcanoes</span> via stresses. Here we demonstrate that quantitative evaluation of temporal stress changes beneath Mt. Ontake, Japan, using the misfit angles of focal mechanism solutions to the regional stress field, is effective for eruption monitoring. The moving average of misfit angles indicates that during the precursory period the local stress field beneath Mt. Ontake was deviated from the regional stress field, presumably by stress perturbations caused by the inflation of magmatic/hydrothermal fluids, which was removed immediately after the expulsion of volcanic ejecta. The deviation of the local stress field can be an indicator of increases in volcanic <span class="hlt">activity</span>. The proposed method may contribute to the mitigation of volcanic hazards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4762890','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4762890"><span>Monitoring eruption <span class="hlt">activity</span> using temporal stress changes at Mount Ontake <span class="hlt">volcano</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Terakawa, Toshiko; Kato, Aitaro; Yamanaka, Yoshiko; Maeda, Yuta; Horikawa, Shinichiro; Matsuhiro, Kenjiro; Okuda, Takashi</p> <p>2016-01-01</p> <p>Volcanic <span class="hlt">activity</span> is often accompanied by many small earthquakes. Earthquake focal mechanisms represent the fault orientation and slip direction, which are influenced by the stress field. Focal mechanisms of <span class="hlt">volcano</span>-tectonic earthquakes provide information on the state of <span class="hlt">volcanoes</span> via stresses. Here we demonstrate that quantitative evaluation of temporal stress changes beneath Mt. Ontake, Japan, using the misfit angles of focal mechanism solutions to the regional stress field, is effective for eruption monitoring. The moving average of misfit angles indicates that during the precursory period the local stress field beneath Mt. Ontake was deviated from the regional stress field, presumably by stress perturbations caused by the inflation of magmatic/hydrothermal fluids, which was removed immediately after the expulsion of volcanic ejecta. The deviation of the local stress field can be an indicator of increases in volcanic <span class="hlt">activity</span>. The proposed method may contribute to the mitigation of volcanic hazards. PMID:26892716</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024399','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024399"><span>Magnetic fields over <span class="hlt">active</span> tectonic zones in ocean</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kopytenko, Yu. A.; Serebrianaya, P.M.; Nikitina, L.V.; Green, A.W.</p> <p>2002-01-01</p> <p>The aim of our work is to estimate the electromagnetic effects that can be detected in the <span class="hlt">submarine</span> zones with hydrothermal <span class="hlt">activity</span>. It is known that meso-scale flows appear in the regions over underwater <span class="hlt">volcanoes</span> or hot rocks. Their origin is connected with heat flux and hot jets released from underwater <span class="hlt">volcanoes</span> or faults in a sea bottom. Values of mean velocities and turbulent velocities in plumes were estimated. Quasiconstant magnetic fields induced by a hot jet and a vortex over a plume top are about 1-40 nT. Variable magnetic fields are about 0.1-1 nT. These magnetic disturbances in the sea medium create an additional natural electromagnetic background that must be considered when making detailed magnetic surveys. ?? 2002 Elsevier Science Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1046436','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1046436"><span>Analysis of SSN 688 Class <span class="hlt">Submarine</span> Maintenance Delays</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-06-01</p> <p>Simplified Notional <span class="hlt">Submarine</span> FRP (Independent Deployer) ..................11  Figure 8.  Evolution of Los Angeles Class <span class="hlt">Submarine</span> Notional...Number TFP Technical Foundation Paper URO Unrestricted Operations xv ACKNOWLEDGMENTS I would like to thank my lead advisor, Professor Nick Dew...only on Los Angeles (SSN 688)-class <span class="hlt">submarines</span>. Being the higher quantity and older generation <span class="hlt">submarine</span> hull type, the Los Angeles class <span class="hlt">submarine</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4875C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4875C"><span>Exploring the links between <span class="hlt">volcano</span> flank collapse and magma evolution: Fogo oceanic shield <span class="hlt">volcano</span>, 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>Cornu, Melodie-Neige; Paris, Raphael; Doucelance, Regis; Bachelery, Patrick; Guillou, Hervé</p> <p>2017-04-01</p> <p>Mass wasting of oceanic shield <span class="hlt">volcanoes</span> is largely documented through the recognition of collapse scars and <span class="hlt">submarine</span> debris fans. However, it is actually difficult to infer the mechanisms controlling <span class="hlt">volcano</span> flank failures that potentially imply tens to hundreds of km3. Studies coupling detailed petrological and geochemical analyses of eruptive products hold clues for better understanding the relationships between magma sources, the plumbing system, and flank instability. Our study aims at tracking potential variations of magma source, storage and transport beneath Fogo shield <span class="hlt">volcano</span> (Cape Verde) before and after its major flank collapse. We also provide a geochronological framework of this magmatic evolution through new radiometric ages (K-Ar and Ar-Ar) of both pre-collapse and post-collapse lavas. The central part of Fogo volcanic edifice is truncated by an 8 km-wide caldera opened to the East, corresponding to the scar of the last flank collapse (Monte Amarelo collapse, Late Pleistocene, 150 km3). Lavas sampled at the base of the scar (the so-called Bordeira) yielded ages between 158 and 136 ka. The age of the collapse is constrained between 68 ka (youngest lava flow cut by the collapse scar) and 59 ka (oldest lava flow overlapping the scar). The collapse walls display a complex structural, intrusive and eruptive history. Undersaturated volcanism (SiO2<43%) is surprisingly dominated by explosive products such as ignimbrites, with 4 major explosive episodes representing half of the volume of the central edifice. This explosive record onshore is correlated with the offshore record of mafic tephra and turbidites (Eisele et al., 2015). Major elements analyses indicate that the pre-collapse lavas are significantly less differentiated than post-collapse lavas, with a peak of alkalis at the collapse. Rare-earth elements concentration decreases with time, with a notable positive anomaly before the collapse. The evolution of the isotopic ratios (Sr, Nd and Pb) through</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740009906','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740009906"><span>Ground survey of <span class="hlt">active</span> Central American <span class="hlt">volcanoes</span> in November - December 1973</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stoiber, R. E. (Principal Investigator); Rose, W. I., Jr.</p> <p>1974-01-01</p> <p>The author has identified the following significant results. Thermal anomalies at two <span class="hlt">volcanoes</span>, Santiaguito and Izalco, have grown in size in the past six months, based on repeated ground survey. Thermal anomalies at Pacaya <span class="hlt">volcano</span> have became less intense in the same period. Large (500 m diameter) thermal anomalies exist at 3 <span class="hlt">volcanoes</span> presently, and smaller scale anomalies are found at nine other <span class="hlt">volcanoes</span>.</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/of/1998/0106/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1998/0106/report.pdf"><span>Preliminary <span class="hlt">volcano</span>-hazard assessment for Augustine <span class="hlt">Volcano</span>, 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>Waythomas, Christopher F.; Waitt, Richard B.</p> <p>1998-01-01</p> <p>Augustine <span class="hlt">Volcano</span> is a 1250-meter high stratovolcano in southwestern Cook Inlet about 280 kilometers southwest of Anchorage and within about 300 kilometers of more than half of the population of Alaska. Explosive eruptions have occurred six times since the early 1800s (1812, 1883, 1935, 1964-65, 1976, and 1986). The 1976 and 1986 eruptions began with an initial series of vent-clearing explosions and high vertical plumes of volcanic ash followed by pyroclastic flows, surges, and lahars on the <span class="hlt">volcano</span> flanks. Unlike some prehistoric eruptions, a summit edifice collapse and debris avalanche did not occur in 1812, 1935, 1964-65, 1976, or 1986. However, early in the 1883 eruption, a portion of the <span class="hlt">volcano</span> summit broke loose forming a debris avalanche that flowed to the sea. The avalanche initiated a small tsunami reported on the Kenai Peninsula at English Bay, 90 kilometers east of the <span class="hlt">volcano</span>. Plumes of volcanic ash are a major hazard to jet aircraft using Anchorage International and other local airports. Ashfall from future eruptions could disrupt oil and gas operations and shipping <span class="hlt">activities</span> in Cook Inlet. Eruptions similar to the historical and prehistoric eruptions are likely in Augustine's future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816744P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816744P"><span>Diffuse H_{2} emission: a useful geochemical tool to monitor the volcanic <span class="hlt">activity</span> at El Hierro <span class="hlt">volcano</span> system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pérez, Nemesio M.; Melián, Gladys; González-Santana, Judit; Barrancos, José; Padilla, Germán; Rodríguez, Fátima; Padrón, Eleazar; Hernández, Pedro A.</p> <p>2016-04-01</p> <p>The occurrence of interfering processes affecting reactive gases as CO2 during its ascent from magmatic bodies or hydrothermal systems toward the surface environment hinders the interpretation of their enrichments in the soil atmosphere and fluxes for <span class="hlt">volcano</span> monitoring purposes (Marini and Gambardella, 2005). These processes include gas scrubbing by ground-waters and interaction with rocks, decarbonatation processes, biogenic production, etc. Within the rest of the soil gases, particularly interest has been addressed to light and highly mobile gases. They offer important advantages for the detection of vertical permeability structures, because their interaction with the surrounding rocks or fluids during the ascent toward the surface is minimum. H2 is one of the most abundant trace species in <span class="hlt">volcano</span>-hydrothermal systems and is a key participant in many redox reactions occurring in the hydrothermal reservoir gas (Giggenbach, 1987). Although H2 can be produced in soils by N2-fixing and fertilizing bacteria, soils are considered nowadays as sinks of molecular hydrogen (Smith-Downey et al., 2006). Because of its chemical and physical characteristics, H2 generated within the crust moves rapidly and escapes to the atmosphere. These characteristics make H2 one of the best geochemical indicators of magmatic and geothermal <span class="hlt">activity</span> at depth. El Hierro is the youngest and the SW-most of the Canary Islands and the scenario of the last volcanic eruption of the archipelago, a <span class="hlt">submarine</span> eruption that took place 2 km off the southern coast of the island from October 2011 to March 2012. Since at El Hierro Island there are not any surface geothermal manifestations (fumaroles, etc), we have focused our studies on soil degassing surveys. Here we show the results of soil H2 emission surveys that have been carried out regularly since mid-2012. Soil gas samples were collected in ˜600 sites selected based on their accessibility and geological criteria. Soil gases were sampled at ˜40</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70176746','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70176746"><span><span class="hlt">Volcano</span> monitoring at the U.S. Geological Survey's Hawaiian <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Heliker, Christina C.; Griggs, J. D.; Takahashi, T. Jane; Wright, Thomas L.; Spall, Henry</p> <p>1986-01-01</p> <p>The island of Hawaii has one of the youngest landscapes on Earth, formed by frequent addition of new lava to its surface.  Because Hawaiian are generally nonexplosive and easily accessible, the island has long attracted geologists interested in studying the extraordinary power of volcanic eruptions.  The U.S. Geological Survey's Hawaiian <span class="hlt">Volcano</span> Observatory (HVO), now nearing its 75th anniversary. has been in the forefront of volcanology since the 1900's.  This issue of Earthquakes and <span class="hlt">volcanoes</span> is devoted to the work of the Observatory and its role in studying the most recent eruptions of Hawaii's two currently <span class="hlt">active</span> <span class="hlt">volcanoes</span>, Kilauea and Mauna Loa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70176393','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70176393"><span><span class="hlt">Volcano</span> monitoring at the U.S. Geological Survey's Hawaiian <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p></p> <p>1986-01-01</p> <p>The island of Hawaii has one of the youngest landscapes on Earth, formed by the frequent addition of new lava to its surface. Because Hawaiian eruptions are generally nonexplosive and easily accessible, the island has long attracted geologists interested in studying the extraordinary power of volcanic eruption. The U.S. Geological Survey's Hawaiian <span class="hlt">Volcano</span> Observatory (HVO), now nearing its 75th anniversary, has been in the forefront of volcanology since the early 1900s. This issue of <i>Earthquakes and <span class="hlt">Volcanoes</span></i> is devoted to the work of the Observatory and its role in studying the most recent eruptions of Hawaii's two currently <span class="hlt">active</span> <span class="hlt">volcanoes</span>, Kilauea and Mauna Loa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714265J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714265J"><span><span class="hlt">Submarine</span> seismic monitoring of El Hierro volcanic eruption with a 3C-geophone string: applying new acquisition and data processing techniques to <span class="hlt">volcano</span> monitoring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jurado, Maria Jose; Ripepe, Maurizio; Lopez, Carmen; Blanco, Maria Jose; Crespo, Jose</p> <p>2015-04-01</p> <p>A <span class="hlt">submarine</span> volcanic eruption took place near the southernmost emerged land of the El Hierro Island (Canary Islands, Spain), from October 2011 to February 2012. The Instituto Geografico Nacional (IGN) seismic stations network evidenced seismic unrest since July 2011 and was a reference also to follow the evolution of the seismic <span class="hlt">activity</span> associated with the volcanic eruption. Right after the eruption onset, in October 2011 a geophone string was deployed by the CSIC-IGN to monitor seismic <span class="hlt">activity</span>. Monitoring with the seismic array continued till May 2012. The array was installed less than 2 km away from the new vol¬cano, next to La Restinga village shore in the harbor from 6 to 12m deep into the water. Our purpose was to record seismic <span class="hlt">activity</span> related to the volcanic <span class="hlt">activity</span>, continuously and with special interest on high frequency events. The seismic array was endowed with 8, high frequency, 3 component, 250 Hz, geophone cable string with a separation of 6 m between them. Each geophone consists on a 3-component module based on 3 orthogonal independent sensors that measures ground velocity. Some of the geophones were placed directly on the seabed, some were buried. Due to different factors, as the irregular characteristics of the seafloor. The data was recorded on the surface with a seismometer and stored on a laptop computer. We show how acoustic data collected underwater show a great correlation with the seismic data recorded on land. Finally we compare our data analysis results with the observed sea surface <span class="hlt">activity</span> (ash and lava emission and degassing). This evidence is disclosing new and innovative tecniques on monitoring <span class="hlt">submarine</span> volcanic <span class="hlt">activity</span>. Reference Instituto Geográfico Nacional (IGN), "Serie El Hierro." Internet: http://www.ign.es/ign/resources /volcanologia/HIERRO.html [May, 17. 2013</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2014/5034/pdf/sir2014-5034.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2014/5034/pdf/sir2014-5034.pdf"><span>2010 Volcanic <span class="hlt">activity</span> in Alaska, Kamchatka, and the Kurile Islands: summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Neal, Christina A.; Herrick, Julie; Girina, O.A.; Chibisova, Marina; Rybin, Alexander; McGimsey, Robert G.; Dixon, Jim</p> <p>2014-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, possible eruptions, volcanic unrest or suspected unrest at 12 volcanic centers in Alaska during 2010. The most notable volcanic <span class="hlt">activity</span> consisted of intermittent ash emissions from long-<span class="hlt">active</span> Cleveland <span class="hlt">volcano</span> in the Aleutian Islands. AVO staff also participated in hazard communication regarding eruptions or unrest at seven <span class="hlt">volcanoes</span> in Russia as part of an ongoing collaborative role in the Kamchatka and Sakhalin Volcanic Eruption Response Teams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=STS032-80-071&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=STS032-80-071&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dactive%2Bvolcanoes"><span>San Cristobal <span class="hlt">Volcano</span>, Nicaragua</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1990-01-01</p> <p>A white plume of smoke, from San Cristobal <span class="hlt">Volcano</span> (13.0N, 87.5W) on the western coast of Nicaragua, blows westward along the Nicaraguan coast just south of the Gulf of Fonseca and the Honduran border. San Csistobal is a strato <span class="hlt">volcano</span> some 1,745 meters high and is frequently <span class="hlt">active</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70128732','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70128732"><span><span class="hlt">Volcano</span> deformation and gravity workshop synopsis and outcomes: The 2008 <span class="hlt">volcano</span> deformation and temporal gravity change workshop</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dzurisin, Daniel; Lu, Zhong</p> <p>2009-01-01</p> <p>A <span class="hlt">volcano</span> workshop was held in Washington State, near the U.S. Geological Survey (USGS) Cascades <span class="hlt">Volcano</span> Observatory. The workshop, hosted by the USGS <span class="hlt">Volcano</span> Hazards Program (VHP), included more than 40 participants from the United States, the European Union, and Canada. Goals were to promote (1) collaboration among scientists working on <span class="hlt">active</span> <span class="hlt">volcanoes</span> and (2) development of new tools for studying <span class="hlt">volcano</span> deformation. The workshop focused on conventional and emerging techniques, including the Global Positioning System (GPS), borehole strain, interferometric synthetic aperture radar (InSAR), gravity, and electromagnetic imaging, and on the roles of aqueous and magmatic fluids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22458514','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22458514"><span>Methanogenic <span class="hlt">activity</span> and diversity in the centre of the Amsterdam Mud <span class="hlt">Volcano</span>, Eastern Mediterranean Sea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lazar, Cassandre Sara; John Parkes, R; Cragg, Barry A; L'Haridon, Stephane; Toffin, Laurent</p> <p>2012-07-01</p> <p>Marine mud <span class="hlt">volcanoes</span> are geological structures emitting large amounts of methane from their <span class="hlt">active</span> centres. The Amsterdam mud <span class="hlt">volcano</span> (AMV), located in the Anaximander Mountains south of Turkey, is characterized by intense <span class="hlt">active</span> methane seepage produced in part by methanogens. To date, information about the diversity or the metabolic pathways used by the methanogens in <span class="hlt">active</span> centres of marine mud <span class="hlt">volcanoes</span> is limited. (14)C-radiotracer measurements showed that methylamines/methanol, H(2)/CO(2) and acetate were used for methanogenesis in the AMV. Methylotrophic methanogenesis was measured all along the sediment core, Methanosarcinales affiliated sequences were detected using archaeal 16S PCR-DGGE and mcrA gene libraries, and enrichments of methanogens showed the presence of Methanococcoides in the shallow sediment layers. Overall acetoclastic methanogenesis was higher than hydrogenotrophic methanogenesis, which is unusual for cold seep sediments. Interestingly, acetate porewater concentrations were extremely high in the AMV sediments. This might be the result of organic matter cracking in deeper hotter sediment layers. Methane was also produced from hexadecanes. For the most part, the methanogenic community diversity was in accordance with the depth distribution of the H(2)/CO(2) and acetate methanogenesis. These results demonstrate the importance of methanogenic communities in the centres of marine mud <span class="hlt">volcanoes</span>. © 2012 Federation of European Microbiological Societies. Published by Blackwell Publishing Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2013/5213/pdf/sir2013-5213.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2013/5213/pdf/sir2013-5213.pdf"><span>2009 Volcanic <span class="hlt">activity</span> in Alaska, Kamchatka, and the Kurile Islands: summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Neal, Christina A.; Girina, Olga A.; Chibisova, Marina; Rybin, Alexander</p> <p>2014-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, possible eruptions, volcanic unrest, and reports of unusual <span class="hlt">activity</span> at or near eight separate volcanic centers in Alaska during 2009. The year was highlighted by the eruption of Redoubt <span class="hlt">Volcano</span>, one of three <span class="hlt">active</span> <span class="hlt">volcanoes</span> on the western side of Cook Inlet and near south-central Alaska's population and commerce centers, which comprise about 62 percent of the State's population of 710,213 (2010 census). AVO staff also participated in hazard communication and monitoring of multiple eruptions at ten <span class="hlt">volcanoes</span> in Russia as part of its collaborative role in the Kamchatka and Sakhalin Volcanic Eruption Response Teams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060037473&hterms=Hawaii+Kilauea+volcano&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DHawaii%2BKilauea%2Bvolcano','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060037473&hterms=Hawaii+Kilauea+volcano&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DHawaii%2BKilauea%2Bvolcano"><span>Analysis of <span class="hlt">Active</span> Lava Flows on Kilauea <span class="hlt">Volcano</span>, Hawaii, Using SIR-C Radar Correlation Measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zebker, H. A.; Rosen, P.; Hensley, S.; Mouginis-Mark, P. J.</p> <p>1995-01-01</p> <p>Precise eruption rates of <span class="hlt">active</span> pahoehoe lava flows on Kilauea <span class="hlt">volcano</span>, Hawaii, have been determined using spaceborne radar data acquired by the Space Shuttle Imaging Radar-C (SIR-C). Measurement of the rate of lava flow advance, and the determination of the volume of new material erupted in a given period of time, are among the most important observations that can be made when studying a <span class="hlt">volcano</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2725I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2725I"><span>Catalogue of Icelandic <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ilyinskaya, Evgenia; Larsen, Gudrun; Gudmundsson, Magnus T.; Vogfjord, Kristin; Pagneux, Emmanuel; Oddsson, Bjorn; Barsotti, Sara; Karlsdottir, Sigrun</p> <p>2016-04-01</p> <p>The Catalogue of Icelandic <span class="hlt">Volcanoes</span> is a newly developed open-access web resource in English intended to serve as an official source of information about <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Iceland and their characteristics. The Catalogue forms a part of an integrated volcanic risk assessment project in Iceland GOSVÁ (commenced in 2012), as well as being part of the effort of FUTUREVOLC (2012-2016) on establishing an Icelandic <span class="hlt">volcano</span> supersite. Volcanic <span class="hlt">activity</span> in Iceland occurs on volcanic systems that usually comprise a central <span class="hlt">volcano</span> and fissure swarm. Over 30 systems have been <span class="hlt">active</span> during the Holocene (the time since the end of the last glaciation - approximately the last 11,500 years). In the last 50 years, over 20 eruptions have occurred in Iceland displaying very varied <span class="hlt">activity</span> in terms of eruption styles, eruptive environments, eruptive products and the distribution lava and tephra. Although basaltic eruptions are most common, the majority of eruptions are explosive, not the least due to magma-water interaction in ice-covered <span class="hlt">volcanoes</span>. Extensive research has taken place on Icelandic volcanism, and the results reported in numerous scientific papers and other publications. In 2010, the International Civil Aviation Organisation (ICAO) funded a 3 year project to collate the current state of knowledge and create a comprehensive catalogue readily available to decision makers, stakeholders and the general public. The work on the Catalogue began in 2011, and was then further supported by the Icelandic government and the EU through the FP7 project FUTUREVOLC. The Catalogue of Icelandic <span class="hlt">Volcanoes</span> is a collaboration of the Icelandic Meteorological Office (the state <span class="hlt">volcano</span> observatory), the Institute of Earth Sciences at the University of Iceland, and the Civil Protection Department of the National Commissioner of the Iceland Police, with contributions from a large number of specialists in Iceland and elsewhere. The Catalogue is built up of chapters with texts and various</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1810971L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1810971L"><span>Integrating science and education during an international, multi-parametric investigation of volcanic <span class="hlt">activity</span> at Santiaguito <span class="hlt">volcano</span>, Guatemala</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lavallée, Yan; Johnson, Jeffrey; Andrews, Benjamin; Wolf, Rudiger; Rose, William; Chigna, Gustavo; Pineda, Armand</p> <p>2016-04-01</p> <p>In January 2016, we held the first scientific/educational Workshops on <span class="hlt">Volcanoes</span> (WoV). The workshop took place at Santiaguito <span class="hlt">volcano</span> - the most <span class="hlt">active</span> <span class="hlt">volcano</span> in Guatemala. 69 international scientists of all ages participated in this intensive, multi-parametric investigation of the volcanic <span class="hlt">activity</span>, which included the deployment of seismometers, tiltmeters, infrasound microphones and mini-DOAS as well as optical, thermographic, UV and FTIR cameras around the <span class="hlt">active</span> vent. These instruments recorded volcanic <span class="hlt">activity</span> in concert over a period of 3 to 9 days. Here we review the research <span class="hlt">activities</span> and present some of the spectacular observations made through this interdisciplinary efforts. Observations range from high-resolution drone and IR footage of explosions, monitoring of rock falls and quantification of the erupted mass of different gases and ash, as well as morphological changes in the dome caused by recurring explosions (amongst many other volcanic processes). We will discuss the success of such integrative ventures in furthering science frontiers and developing the next generation of geoscientists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1714782R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1714782R"><span><span class="hlt">Volcano</span> monitoring with an infrared camera: first insights from Villarrica <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rosas Sotomayor, Florencia; Amigo Ramos, Alvaro; Velasquez Vargas, Gabriela; Medina, Roxana; Thomas, Helen; Prata, Fred; Geoffroy, Carolina</p> <p>2015-04-01</p> <p>This contribution focuses on the first trials of the, almost 24/7 monitoring of Villarrica <span class="hlt">volcano</span> with an infrared camera. Results must be compared with other SO2 remote sensing instruments such as DOAS and UV-camera, for the ''day'' measurements. Infrared remote sensing of volcanic emissions is a fast and safe method to obtain gas abundances in volcanic plumes, in particular when the access to the vent is difficult, during volcanic crisis and at night time. In recent years, a ground-based infrared camera (Nicair) has been developed by Nicarnica Aviation, which quantifies SO2 and ash on volcanic plumes, based on the infrared radiance at specific wavelengths through the application of filters. Three Nicair1 (first model) have been acquired by the Geological Survey of Chile in order to study degassing of <span class="hlt">active</span> <span class="hlt">volcanoes</span>. Several trials with the instruments have been performed in northern Chilean <span class="hlt">volcanoes</span>, and have proven that the intervals of retrieved SO2 concentration and fluxes are as expected. Measurements were also performed at Villarrica <span class="hlt">volcano</span>, and a location to install a ''fixed'' camera, at 8km from the crater, was discovered here. It is a coffee house with electrical power, wifi network, polite and committed owners and a full view of the <span class="hlt">volcano</span> summit. The first measurements are being made and processed in order to have full day and week of SO2 emissions, analyze data transfer and storage, improve the remote control of the instrument and notebook in case of breakdown, web-cam/GoPro support, and the goal of the project: which is to implement a fixed station to monitor and study the Villarrica <span class="hlt">volcano</span> with a Nicair1 integrating and comparing these results with other remote sensing instruments. This works also looks upon the strengthen of bonds with the community by developing teaching material and giving talks to communicate volcanic hazards and other geoscience topics to the people who live "just around the corner" from one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.2775P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.2775P"><span>Understanding how <span class="hlt">active</span> <span class="hlt">volcanoes</span> work: a contribution from synchrotron X-ray computed microtomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Polacci, M.; Baker, D. R.; Mancini, L.</p> <p>2009-04-01</p> <p><span class="hlt">Volcanoes</span> are complex systems that require the integration of many different geoscience disciplines to understand their behaviour and to monitor and forecast their <span class="hlt">activity</span>. In the last two decades an increasing amount of information on volcanic processes has been obtained by studying the textures and compositions of volcanic rocks. Five years ago we started a continuing collaboration with the SYRMEP beamline of Elettra Sincrotrone, a third generation synchrotron light source near Trieste, Italy, with the goal of performing high-resolution, phase-contrast X-ray tomographic scans and reconstructing 3-D digital volumes of volcanic specimens. These volumes have been then used for the visualization of the internal structure of rocks and for the quantification of rock textures (i.e., vesicle and crystal volume fraction, individual vesicle volumes and shapes, vesicle connectivity, vesicle volume distributions, permeability simulations etc.). We performed tomographic experiments on volcanic products erupted from different hazardous volcanic systems in Italy and around the world: Campi Flegrei, Stromboli, Etna (Southern Italy), Villarrica (Chile), Yasur and Ambrym (Vanuatu Islands). As an example, we used the results of these studies to constrain the dynamics of vesiculation and degassing in basaltic (Polacci et al., 2006; Burton et al., 2007; Colò et al., 2007; Andronico et al., 2008; Polacci et al., 2008a) and trachytic (Piochi et al., 2008) magmas. A better knowledge of how gas is transported and lost from magmas has led us in turn to draw new implications on the eruptive style of these <span class="hlt">active</span>, hazardous <span class="hlt">volcanoes</span> (Polacci et al., 2008b). Work in progress consists of optimizing our procedure by establishing a precise protocol that will enable us to quantitatively study the 3-D texture and composition of rocks in a statistically representative way. Future work will concentrate on the study of the spatial relations between phases (crystals, vesicles and glass) in rocks</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.V43I..02C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.V43I..02C"><span>Products of <span class="hlt">Submarine</span> Fountains and Bubble-burst Eruptive <span class="hlt">Activity</span> at 1200 m on West Mata <span class="hlt">Volcano</span>, Lau Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clague, D. A.; Rubin, K. H.; Keller, N. S.</p> <p>2009-12-01</p> <p>An eruption was observed and sampled at West Mata <span class="hlt">Volcano</span> using ROV JASON II for 5 days in May 2009 during the NSF-NOAA eruption response cruise to this region of suspected volcanic <span class="hlt">activity</span>. <span class="hlt">Activity</span> was focused near the summit at the Prometheus and Hades vents. Prometheus erupted almost exclusively as low-level fountains. <span class="hlt">Activity</span> at Hades cycled between vigorous degassing, low fountains, and bubble-bursts, building up and partially collapsing a small spatter/scoria cone and feeding short sheet-like and pillow flows. Fire fountains at Prometheus produced mostly small primary pyroclasts that include Pele's hair and fluidal fragments of highly vesicular volcanic glass. These fragments have mostly shattered and broken surfaces, although smooth spatter-like surfaces also occur. As <span class="hlt">activity</span> wanes, glow in the vent fades, and denser, sometimes altered volcanic clasts are incorporated into the eruption. The latter are likely from the conduit walls and/or vent-rim ejecta, drawn back into the vent by inrushing seawater that replaces water entrained in the rising volcanic plume. Repeated recycling of previously erupted materials eventually produces rounded clasts resembling beach cobbles and pitted surfaces on broken phenocrysts of pyroxene and olivine. We estimate that roughly 33% of near vent ejecta are recycled. Our best sample of this ejecta type was deposited in the drawer of the JASON II ROV during a particularly large explosion that occurred during plume sampling immediately above the vent. Elemental sulfur spherules up to 5 mm in diameter are common in ejecta from both vents and occur inside some of the lava fragments Hades <span class="hlt">activity</span> included dramatic bubble-bursts unlike anything previously observed under water. The lava bubbles, sometimes occurring in rapid-fire sequence, collapsed in the water-column, producing fragments that are quenched in less than a second to form Pele's hair, limu o Pele, spatter-like lava blobs, and scoria. All are highly vesicular</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GML....32..473L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GML....32..473L"><span>New discoveries of mud <span class="hlt">volcanoes</span> on the Moroccan Atlantic continental margin (Gulf of Cádiz): morpho-structural characterization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>León, Ricardo; Somoza, Luis; Medialdea, Teresa; Vázquez, Juan Tomás; González, Francisco Javier; López-González, Nieves; Casas, David; del Pilar Mata, María; del Fernández-Puga, María Carmen; Giménez-Moreno, Carmen Julia; Díaz-del-Río, Víctor</p> <p>2012-12-01</p> <p>During the MVSEIS-08 cruise of 2008, ten new mud <span class="hlt">volcanoes</span> (MVs) were discovered on the offshore Moroccan continental margin (Gulf of Cádiz) at water depths between 750 and 1,600 m, using multibeam bathymetry, backscatter imagery, high-resolution seismic and gravity core data. Mud breccias were recovered in all cases, attesting to the nature of extrusion of these cones. The mud <span class="hlt">volcanoes</span> are located in two fields: the MVSEIS, Moundforce, Pixie, Las Negras, Madrid, Guadix, Almanzor and El Cid MVs in the western Moroccan field, where mud <span class="hlt">volcanoes</span> have long been suspected but to date not identified, and the Boabdil and Al Gacel MVs in the middle Moroccan field. Three main morphologies were observed: asymmetric, sub-circular and flat-topped cone-shaped types, this being the first report of asymmetric morphologies in the Gulf of Cádiz. Based on morpho-structural analysis, the features are interpreted to result from (1) repeated constructive (expulsion of fluid mud mixtures) and destructive (gravity-induced collapse and <span class="hlt">submarine</span> landsliding) episodes and (2) interaction with bottom currents.</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 intrusions, lateral magma transport and related uplift at ocean island <span class="hlt">volcanoes</span></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 <span class="hlt">volcanoes</span> grow by accumulation of erupted material as well as by coeval or discrete magmatic intrusions. Dykes and other intrusive bodies within volcanic edifices are comparatively well studied, but intrusive processes deep beneath the <span class="hlt">volcanoes</span> remain elusive. Although there is geological evidence for deep magmatic intrusions contributing to <span class="hlt">volcano</span> 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 intrusions 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 <span class="hlt">submarine</span> eruption in 2011-2012 reveal deep subhorizontal intrusive sheets (sills), which have caused island-scale uplift of tens of centimetres. The pre-eruptive intrusions 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 intrusions 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 <span class="hlt">volcanoes</span> shows similar bimodal pressure distributions, suggesting that eruptive phases are commonly accompanied by deep intrusions 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 zone in the lower oceanic crust begins early during <span class="hlt">volcano</span> 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/2007AGUFM.V13B1341S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V13B1341S"><span>Triggering and dynamic evolution of the LUSI mud <span class="hlt">volcano</span>, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Svensen, H.; Mazzini, A.; Akhmanov, G. G.; Aloisi, G.; Planke, S.; Sørenssen, A.; Istadi, B.</p> <p>2007-12-01</p> <p>Mud <span class="hlt">volcanoes</span> are geologically important manifestations of vertical fluid flow and mud eruption in sedimentary basins worldwide. Their formation is predominantly ascribed to release of overpressure from clay- and organic- rich sediments, leading to impressive buildup of mud mountains in <span class="hlt">submarine</span> and subaerial settings. Here we report data from two fieldworks on a newly born mud <span class="hlt">volcano</span> named LUSI eruption in Eastern Java (Indonesia). The eruption site appears close to an <span class="hlt">active</span> magmatic complex in a backarc sedimentary basin in Indonesia. Its specific location results in a high background temperature gradient that triggers mineralogical transformations and geochemical reactions at shallow depth. The eruption of 100 deg.C mud and gas that started the 29th of May 2006 flooded a large area within the Sidoarjo village in Northeast Java. Thousands of people have so far been evacuated and, since the initial eruption, the flow rate escalated from 5000 to 120,000 m3/d during the first eleven weeks. Then the erupted volume started to pulsate between almost zero and 120,000 m3/d in the period August-September, whereas it increased dramatically following swarms of earthquakes in September, before reaching almost 180,000 m3/d in December 2006. Fifteen months after the initial burst, LUSI is still vigorously erupting up to 111,000 m3/d, the average subsidence of the area reached 11 m. Seismic images show that a pre-existing structure was present before the eruption. Based on geochemical and field results, we propose a mechanism where the eruptions started following the 27th of May earthquake due to fracturing and accompanied depressurization of >100 deg.C pore fluids from > 1700 m depth released from a structure in already critical conditions. This resulted in the formation of a quasi-hydrothermal system with a geyser-like surface expression and with an <span class="hlt">activity</span> influenced by the regional seismicity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2007/5269/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2007/5269/"><span>2005 Volcanic <span class="hlt">Activity</span> in Alaska, Kamchatka, and the Kurile Islands: Summary of Events and Response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, R.G.; Neal, C.A.; Dixon, J.P.; Ushakov, Sergey</p> <p>2008-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptive <span class="hlt">activity</span> or suspected volcanic <span class="hlt">activity</span> at or near 16 <span class="hlt">volcanoes</span> in Alaska during 2005, including the high profile precursory <span class="hlt">activity</span> associated with the 2005?06 eruption of Augustine <span class="hlt">Volcano</span>. AVO continues to participate in distributing information about eruptive <span class="hlt">activity</span> on the Kamchatka Peninsula, Russia, and in the Kurile Islands of the Russian Far East, in conjunction with the Kamchatkan Volcanic Eruption Response Team (KVERT) and the Sakhalin Volcanic Eruption Response Team (SVERT), respectively. In 2005, AVO helped broadcast alerts about <span class="hlt">activity</span> at 8 Russian <span class="hlt">volcanoes</span>. The most serious hazard posed from volcanic eruptions in Alaska, Kamchatka, or the Kurile Islands is the placement of ash into the atmosphere at altitudes traversed by jet aircraft along the North Pacific and Russian Trans East air routes. AVO, KVERT, and SVERT work collaboratively with the National Weather Service, Federal Aviation Administration, and the Volcanic Ash Advisory Centers to provide timely warnings of volcanic eruptions and the production and movement of ash clouds.</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('http://adsabs.harvard.edu/abs/2016AGUFM.V43F..07C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V43F..07C"><span>Volcanism, Iron, and Phytoplankton in the Heard and McDonald Islands Region, Southern Indian Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coffin, M. F.; Arculus, R. J.; Bowie, A. R.; Chase, Z.; Robertson, R.; Trull, T. W.; Heobi in2016 v01 Shipboard Party, T.</p> <p>2016-12-01</p> <p>Phytoplankton supply approximately half of the oxygen in Earth's atmosphere, and iron supply limits the growth of phytoplankton in the anemic Southern Ocean. Situated entirely within the Indian Ocean sector of the Southern Ocean are Australia's only <span class="hlt">active</span> subaerial <span class="hlt">volcanoes</span>, Heard and McDonald islands (HIMI) on the central Kerguelen Plateau, a large igneous province. Widespread fields of <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>, some of which may be <span class="hlt">active</span>, extend for distances of up to several hundred kilometers from the islands. The predominantly eastward-flowing Antarctic Circumpolar Current sweeps across the central Kerguelen Plateau, and extensive blooms of phytoplankton are observed on the Plateau down-current of HIMI. The goal of RV Investigator voyage IN2016_V01, conducted in January/February 2016, is to test the hypothesis that hydrothermal fluids, which cool <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> in the HIMI region, ascend from the seafloor and fertilise surface waters with iron, thereby enhancing biological productivity beginning with phytoplankton. Significant initial shipboard results include: Documentation, for the first time, of the role of <span class="hlt">active</span> HIMI and nearby <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> in supplying iron to the Southern Ocean. Nearshore waters had elevated dissolved iron levels. Although biomass was not correspondingly elevated, fluorescence induction data indicated highly productive resident phytoplankton. Discovery of >200 acoustic plumes emanating from the seafloor and ascending up to tens of meters into the water column near HIMI. Deep tow camera footage shows bubbles rising from the seafloor in an acoustic plume field north of Heard Island. Mapping 1,000 km2 of uncharted seafloor around HIMI. <span class="hlt">Submarine</span> volcanic edifices punctuate the adjacent seafloor, and yielded iron-rich rocks similar to those found on HIMI, respectively. Acoustic plumes emanating from some of these features suggest <span class="hlt">active</span> seafloor hydrothermal systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.G41A0999P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.G41A0999P"><span>Spreading And Collapse Of Big Basaltic <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Puglisi, G.; Bonforte, A.; Guglielmino, F.; Peltier, A.; Poland, M. P.</p> <p>2015-12-01</p> <p>Among the different types of <span class="hlt">volcanoes</span>, basaltic ones usually form the most voluminous edifices. Because <span class="hlt">volcanoes</span> are growing on a pre-existing landscape, the geologic and structural framework of the basement (and earlier volcanic landforms) influences the stress regime, seismicity, and volcanic <span class="hlt">activity</span>. Conversely, the masses of these <span class="hlt">volcanoes</span> introduce a morphological anomaly that affects neighboring areas. Growth of a <span class="hlt">volcano</span> disturbs the tectonic framework of the region, clamps and unclamps existing faults (some of which may be reactivated by the new stress field), and deforms the substratum. A <span class="hlt">volcano</span>'s weight on its basement can trigger edifice spreading and collapse that can affect populated areas even at significant distance. <span class="hlt">Volcano</span> instability can also be driven by slow tectonic deformation and magmatic intrusion. The manifestations of instability span a range of temporal and spatial scales, ranging from slow creep on individual faults to large earthquakes affecting a broad area. Our work aims to investigate the relation between basement setting and volcanic <span class="hlt">activity</span> and stability at Etna (Sicily, Italy), Kilauea (Island of Hawaii, USA) and Piton de la Fournaise (La Reunion Island, France). These <span class="hlt">volcanoes</span> host frequent eruptive <span class="hlt">activity</span> (effusive and explosive) and share common features indicating lateral spreading and collapse, yet they are characterized by different morphologies, dimensions, and tectonic frameworks. For instance, the basaltic ocean island <span class="hlt">volcanoes</span> of Kilauea and Piton de la Fournaise are near the <span class="hlt">active</span> ends of long hotspot chains while Mt. Etna has developed at junction along a convergent margin between the African and Eurasian plates and a passive margin separating the oceanic Ionian crust from the African continental crust. Magma supply and plate velocity also differ in the three settings, as to the sizes of the edifices and the extents of their rift zones. These <span class="hlt">volcanoes</span>, due to their similarities and differences, coupled with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...62a2037L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...62a2037L"><span>Preliminary Study on Ground-Magnetic Data Near the <span class="hlt">Active</span> <span class="hlt">Volcanoes</span> in Konga Bay, East Flores Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Laesanpura, Agus; Dahrin, Darharta; Nurseptian, Ivan</p> <p>2017-04-01</p> <p>East Flores is part of Nusa Tenggara island belongs to volcanic arc zone, hence the <span class="hlt">active</span> <span class="hlt">volcanoes</span> surround the area about 60 × 50 square km. It is located at latitude south 8° 30’, and longitude east 122° 45’. Geologically, the rock is mostly of volcanic material since Miocene age. The Intriguing question is where the volcanic feeder, pyroclastic, and how it vanish in subsurface. The magnetic data acquisitions were executed on land for 500 meter interval and denser through the bay surrounded by <span class="hlt">volcanoes</span>. The combine reduction to pole and forward modelling is apply for serve interpretation using forward modelling technique. The two interpretation sections, show the body of magmatic may present at depth about 2 to 3 km. The observation show no significant decreasing or loosening of magnetic anomaly although near the <span class="hlt">active</span> <span class="hlt">volcano</span>. We suggest the thermal anomaly is just disturbing magnetic data in near surface but not in the depth one. Meanwhile the reduction to pole’s section could distinguish the two group of rock. In assuming the layer is flat. The inferred peak of magmatic body near the existing <span class="hlt">volcano</span>; and the <span class="hlt">active</span> demagnetization associated through evidence of hot spring and inferred fault structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027820','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027820"><span>Physical and chemical properties of <span class="hlt">submarine</span> basaltic rocks from the <span class="hlt">submarine</span> flanks of the Hawaiian Islands</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Yokose, H.; Lipman, P.W.; Kanamatsu, T.</p> <p>2005-01-01</p> <p>To evaluate physical and chemical diversity in <span class="hlt">submarine</span> basaltic rocks, approximately 280 deep <span class="hlt">submarine</span> samples recovered by submersibles from the underwater flanks of the Hawaiian Islands were analyzed and compared. Based on observations from the submersibles and hand specimens, these samples were classified into three main occurrence types (lavas, coarse-grained volcaniclastic rocks, and fine-grained sediments), each with several subtypes. The whole-rock sulfur content and porosity in <span class="hlt">submarine</span> basaltic rocks, recovered from depths greater than 2000 m, range from < 10 ppm and 2 vol.% to 2200 ppm and 47 vol.%, respectively. These wide variations cannot be due just to different ambient pressures at the collection depths, as inferred previously for <span class="hlt">submarine</span> erupted lavas. The physical and chemical properties of the recovered samples, especially a combination of three whole-rock parameters (Fe-oxidation state, Sulfur content, and Porosity), are closely related to the occurrence type. The FSP triangular diagram is a valuable indicator of the source location of basaltic fragments deposited in deep <span class="hlt">submarine</span> areas. This diagram can be applied to basaltic rocks such as clasts in debris-flow deposits, <span class="hlt">submarine</span>-emplaced lava flows that may have crossed the shoreline, and slightly altered geological samples. ?? 2005 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814217P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814217P"><span>Spreading and collapse of big basaltic <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Puglisi, Giuseppe; Bonforte, Alessandro; Guglielmino, Francesco; Peltier, Aline; Poland, Michael</p> <p>2016-04-01</p> <p>Among the different types of <span class="hlt">volcanoes</span>, basaltic ones usually form the most voluminous edifices. Because <span class="hlt">volcanoes</span> are growing on a pre-existing landscape, the geologic and structural framework of the basement (and earlier volcanic landforms) influences the stress regime, seismicity, and volcanic <span class="hlt">activity</span>. Conversely, the masses of these <span class="hlt">volcanoes</span> introduce a morphological anomaly that affects neighboring areas. Growth of a <span class="hlt">volcano</span> disturbs the tectonic framework of the region, clamps and unclamps existing faults (some of which may be reactivated by the new stress field), and deforms the substratum. A <span class="hlt">volcano</span>'s weight on its basement can trigger edifice spreading and collapse that can affect populated areas even at significant distance. <span class="hlt">Volcano</span> instability can also be driven by slow tectonic deformation and magmatic intrusion. The manifestations of instability span a range of temporal and spatial scales, ranging from slow creep on individual faults to large earthquakes affecting a broad area. In the frame of MED-SVU project, our work aims to investigate the relation between basement setting and volcanic <span class="hlt">activity</span> and stability at three Supersite <span class="hlt">volcanoes</span>: Etna (Sicily, Italy), Kilauea (Island of Hawaii, USA) and Piton de la Fournaise (La Reunion Island, France). These <span class="hlt">volcanoes</span> host frequent eruptive <span class="hlt">activity</span> (effusive and explosive) and share common features indicating lateral spreading and collapse, yet they are characterized by different morphologies, dimensions, and tectonic frameworks. For instance, the basaltic ocean island <span class="hlt">volcanoes</span> of Kilauea and Piton de la Fournaise are near the <span class="hlt">active</span> ends of long hotspot chains while Mt. Etna has developed at junction along a convergent margin between the African and Eurasian plates and a passive margin separating the oceanic Ionian crust from the African continental crust. Magma supply and plate velocity also differ in the three settings, as to the sizes of the edifices and the extents of their rift zones. These</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dggs.dnr.state.ak.us/pubs/id/14772','USGSPUBS'); return false;" href="http://www.dggs.dnr.state.ak.us/pubs/id/14772"><span>Preliminary <span class="hlt">volcano</span>-hazard assessment for Akutan <span class="hlt">Volcano</span> east-central Aleutian Islands, 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>Waythomas, Christopher F.; Power, John A.; Richter, Donlad H.; McGimsey, Robert G.</p> <p>1998-01-01</p> <p>Akutan <span class="hlt">Volcano</span> is a 1100-meter-high stratovolcano on Akutan Island in the east-central Aleutian Islands of southwestern Alaska. The <span class="hlt">volcano</span> is located about 1238 kilometers southwest of Anchorage and about 56 kilometers east of Dutch Harbor/Unalaska. Eruptive <span class="hlt">activity</span> has occurred at least 27 times since historical observations were recorded beginning in the late 1700?s. Recent eruptions produced only small amounts of fine volcanic ash that fell primarily on the upper flanks of the <span class="hlt">volcano</span>. Small amounts of ash fell on the Akutan Harbor area during eruptions in 1911, 1948, 1987, and 1989. Plumes of volcanic ash are the primary hazard associated with eruptions of Akutan <span class="hlt">Volcano</span> and are a major hazard to all aircraft using the airfield at Dutch Harbor or approaching Akutan Island. Eruptions similar to historical Akutan eruptions should be anticipated in the future. Although unlikely, eruptions larger than those of historical time could generate significant amounts of volcanic ash, fallout, pyroclastic flows, and lahars that would be hazardous to life and property on all sectors of the <span class="hlt">volcano</span> and other parts of the island, but especially in the major valleys that head on the <span class="hlt">volcano</span> flanks. During a large eruption an ash cloud could be produced that may be hazardous to aircraft using the airfield at Cold Bay and the airspace downwind from the <span class="hlt">volcano</span>. In the event of a large eruption, volcanic ash fallout could be relatively thick over parts of Akutan Island and volcanic bombs could strike areas more than 10 kilometers from the <span class="hlt">volcano</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018262','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018262"><span>Noble gases in <span class="hlt">submarine</span> pillow basalt glasses from Loihi and Kilauea, Hawaii: A solar component in the Earth</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Honda, M.; McDougall, I.; Patterson, D.B.; Doulgeris, A.; Clague, D.A.</p> <p>1993-01-01</p> <p>Noble gas elemental and isotopic abundances have been analysed in twenty-two samples of basaltic glass dredged from the <span class="hlt">submarine</span> flanks of two currently <span class="hlt">active</span> Hawaiian <span class="hlt">volcanoes</span>, Loihi Seamount and Kilauea. Neon isotopic ratios are enriched in 20Ne and 21Ne by as much as 16% with respect to atmospheric ratios. All the Hawaiian basalt glass samples show relatively high 3He 4He ratios. The high 20Ne 22Ne values in some of the Hawaiian samples, together with correlations between neon and helium systematics, suggest the presence of a solar component in the source regions of the Hawaiian mantle plume. The solar hypothesis for the Earth's primordial noble gas composition can account for helium and neon isotopic ratios observed in basaltic glasses from both plume and spreading systems, in fluids in continental hydrothermal systems, in CO2 well gases, and in ancient diamonds. These results provide new insights into the origin and evolution of the Earth's atmosphere. ?? 1993.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.V23E..06A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.V23E..06A"><span>High-Resolution Imaging of Axial <span class="hlt">Volcano</span>, Juan de Fuca ridge.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arnulf, A. F.; Harding, A. J.; Kent, G. M.</p> <p>2014-12-01</p> <p>To date, seismic experiments have been key in our understanding of the internal structure of volcanic systems. However, most experiments, especially subaerial-based, are often restricted to refraction geometries with limited numbers of sources and receivers, and employ smoothing constraints required by tomographic inversions that produce smoothed and blurry images with spatial resolutions well below the length scale of important features that define these magmatic systems. Taking advantage of the high density of sources and receivers from multichannel seismic (MCS) data should, in principle, allow detailed images of velocity and reflectivity to be recovered. Unfortunately, the depth of mid-ocean ridges has the detrimental effect of concealing critical velocity information behind the seafloor reflection, preventing first arrival travel-time tomographic approaches from imaging the shallowest and most heterogeneous part of the crust. To overcome the limitations of the acquisition geometry, here we are using an innovative multistep approach. We combine a synthetic ocean bottom experiment (SOBE), 3-D traveltime tomography, 2D elastic full waveform and a reverse time migration (RTM) formalism, and present one of the most detailed imagery to date of a massive and complex magmatic system beneath Axial seamount, an <span class="hlt">active</span> <span class="hlt">submarine</span> <span class="hlt">volcano</span> that lies at the intersection of the Juan de Fuca ridge and the Cobb-Eickelberg seamount chain. We present high-resolution images along 12 seismic lines that span the <span class="hlt">volcano</span>. We refine the extent/volume of the main crustal magma reservoir that lies beneath the central caldera. We investigate the extent, volume and physical state of a secondary magma body present to the southwest and study its connections with the main magma reservoir. Additionally, we present a 3D tomographic model of the entire <span class="hlt">volcano</span> that reveals a subsiding caldera floor that provides a near perfect trap for the ponding of lava flows, supporting a "trapdoor</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70180954','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70180954"><span><span class="hlt">Submarine</span> landslides: advances and challenges</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Locat, Jacques; Lee, Homa J.</p> <p>2002-01-01</p> <p>Due to the recent development of well-integrated surveying techniques of the sea floor, significant improvements were achieved in mapping and describing the morphology and architecture of <span class="hlt">submarine</span> mass movements. Except for the occurrence of turbidity currents, the aquatic environment (marine and fresh water) experiences the same type of mass failure as that found on land. <span class="hlt">Submarine</span> mass movements, however, can have run-out distances in excess of 100 km, so their impact on any offshore <span class="hlt">activity</span> needs to be integrated over a wide area. This great mobility of submarinemass movements is still not very well understood, particularly for cases like the far-reaching debris flows mapped on the Mississippi Fan and the large <span class="hlt">submarine</span> rock avalanches found around many volcanic islands. A major challenge ahead is the integration of mass movement mechanics in an appropriate evaluation of the hazard so that proper risk assessment methodologies can be developed and implemented for various human <span class="hlt">activities</span> offshore, including the development of natural resources and the establishment of reliable communication corridors. Key words : <span class="hlt">submarine</span> slides, hazards, risk assessment, morphology, mobility, tsunami. Le dveloppement rcent de techniques de levs hydrograhiques pour les fonds marins nous a permis d'atteindre une qualit ingale dans la cartographie et la description des glissements sous marins. l'exception des courants de turbidit, on retrouve dans le domaine aquatique les mmes types de mouvements de terrain que sur terre. Par contre, les glissements sous-marins peuvent atteindre des distances excdant 100 km de telle sorte que leur impact sur les activits offshore doit tre pris en compte sur degrandes tendues. La grande mobilit des glissements sous-marins n'est pas encore bien comprise, comme pour le cas des coules dedbris cartographies sur le cne du Mississippi ainsi que pour les grandes avalanches rocheuses sous-marines retrouves au pourtour des les volcaniques. Un dfi majeur</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1996/0738/tableofcontents.html','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1996/0738/tableofcontents.html"><span>1995 volcanic <span class="hlt">activity</span> in Alaska and Kamchatka: summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Neal, Christina A.</p> <p>1996-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptive <span class="hlt">activity</span> or suspected volcanic <span class="hlt">activity</span> (SVA) at 6 volcanic centers in 1995: Mount Martin (Katmai Group), Mount Veniaminof, Shishaldin, Makushin, Kliuchef/Korovin, and Kanaga. In addition to responding to eruptive <span class="hlt">activity</span> at Alaska <span class="hlt">volcanoes</span>, AVO also disseminated information for the Kamchatkan Volcanic Eruption Response Team (KVERT) on the 1995 eruptions of 2 Russian <span class="hlt">volcanoes</span>: Bezymianny and Karymsky. This report summarizes volcanic <span class="hlt">activity</span> in Alaska during 1995 and the AVO response, as well as information on the 2 Kamchatkan eruptions. Only those reports or inquiries that resulted in a "significant" investment of staff time and energy (here defined as several hours or more for reaction, tracking, and follow-up) are included. AVO typically receives dozens of phone calls throughout the year reporting steaming, unusual cloud sightings, or eruption rumors. Most of these are resolved quickly and are not tabulated here as part of the 1995 response record.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2008/5159/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2008/5159/"><span>Preliminary <span class="hlt">Volcano</span>-Hazard Assessment for Gareloi <span class="hlt">Volcano</span>, Gareloi Island, 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>Coombs, Michelle L.; McGimsey, Robert G.; Browne, Brandon L.</p> <p>2008-01-01</p> <p>Gareloi <span class="hlt">Volcano</span> (178.794 degrees W and 51.790 degrees N) is located on Gareloi Island in the Delarof Islands group of the Aleutian Islands, about 2,000 kilometers west-southwest of Anchorage and about 150 kilometers west of Adak, the westernmost community in Alaska. This small (about 8x10 kilometer) <span class="hlt">volcano</span> has been one of the most <span class="hlt">active</span> in the Aleutians since its discovery by the Bering expedition in the 1740s, though because of its remote location, observations have been scant and many smaller eruptions may have gone unrecorded. Eruptions of Gareloi commonly produce ash clouds and lava flows. Scars on the flanks of the <span class="hlt">volcano</span> and debris-avalanche deposits on the adjacent seafloor indicate that the <span class="hlt">volcano</span> has produced large landslides in the past, possibly causing tsunamis. Such events are infrequent, occurring at most every few thousand years. The primary hazard from Gareloi is airborne clouds of ash that could affect aircraft. In this report, we summarize and describe the major volcanic hazards associated with Gareloi.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4772048','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4772048"><span>Cardiometabolic Health in <span class="hlt">Submariners</span> Returning from a 3-Month Patrol</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gasier, Heath G.; Young, Colin R.; Gaffney-Stomberg, Erin; McAdams, Douglas C.; Lutz, Laura J.; McClung, James P.</p> <p>2016-01-01</p> <p>Confined space, limited exercise equipment, rotating shift work and reduced sleep may affect cardiometabolic health in <span class="hlt">submariners</span>. To test this hypothesis, 53 male U.S. <span class="hlt">Submariners</span> (20–39 years) were studied before and after a 3-month routine <span class="hlt">submarine</span> patrol. Measures included anthropometrics, dietary and physical <span class="hlt">activity</span>, biomarkers of cardiometabolic health, energy and appetite regulation, and inflammation. Before deployment, 62% of <span class="hlt">submariners</span> had a body fat % (BF%) ≥ 25% (obesity), and of this group, 30% met the criteria for metabolic syndrome. In obese volunteers, insulin, the homeostatic model assessment of insulin resistance (HOMA-IR), leptin, the leptin/adiponectin ratio, and pro-inflammatory chemokines growth-related oncogene and macrophage-derived chemokine were significantly higher compared to non-obese <span class="hlt">submariners</span>. Following the patrol, a significant mean reduction in body mass (5%) and fat-mass (11%) occurred in the obese group as a result of reduced energy intake (~2000 kJ) during the patrol; and, independent of group, modest improvements in serum lipids and a mean reduction in interferon γ-induced protein 10 and monocyte chemotactic protein 1 were observed. Since 43% of the <span class="hlt">submariners</span> remained obese, and 18% continued to meet the criteria for metabolic syndrome following the patrol, the magnitude of weight loss was insufficient to completely abolish metabolic dysfunction. Submergence up to 3-months, however, does not appear to be the cause of obesity, which is similar to that of the general population. PMID:26867201</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GGG....14.4892B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GGG....14.4892B"><span>An authoritative global database for <span class="hlt">active</span> <span class="hlt">submarine</span> hydrothermal vent fields</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beaulieu, Stace E.; Baker, Edward T.; German, Christopher R.; Maffei, Andrew</p> <p>2013-11-01</p> <p>The InterRidge Vents Database is available online as the authoritative reference for locations of <span class="hlt">active</span> <span class="hlt">submarine</span> hydrothermal vent fields. Here we describe the revision of the database to an open source content management system and conduct a meta-analysis of the global distribution of known <span class="hlt">active</span> vent fields. The number of known <span class="hlt">active</span> vent fields has almost doubled in the past decade (521 as of year 2009), with about half visually confirmed and others inferred <span class="hlt">active</span> from physical and chemical clues. Although previously known mainly from mid-ocean ridges (MORs), <span class="hlt">active</span> vent fields at MORs now comprise only half of the total known, with about a quarter each now known at volcanic arcs and back-arc spreading centers. Discoveries in arc and back-arc settings resulted in an increase in known vent fields within exclusive economic zones, consequently reducing the proportion known in high seas to one third. The increase in known vent fields reflects a number of factors, including increased national and commercial interests in seafloor hydrothermal deposits as mineral resources. The purpose of the database now extends beyond academic research and education and into marine policy and management, with at least 18% of known vent fields in areas granted or pending applications for mineral prospecting and 8% in marine protected areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4562580','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4562580"><span>Seasonal influence over serum and urine metabolic markers in <span class="hlt">submariners</span> during prolonged patrols</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Holy, Xavier; Bégot, Laurent; Renault, Sylvie; Butigieg, Xavier; André, Catherine; Bonneau, Dominique; Savourey, Gustave; Collombet, Jean-Marc</p> <p>2015-01-01</p> <p>Within the framework of earlier publications, we have consistently dedicated our investigations to eliciting the effects of both seasonal vitamin D deficiency and <span class="hlt">submarine</span>-induced hypercapnia on serum parameters for acid–base balance and bone metabolism in <span class="hlt">submariners</span> over a 2-month winter (WP) or summer (SP) patrols. The latest findings reported herein, contribute further evidence with regard to overall physiological regulations in the same <span class="hlt">submariner</span> populations that underwent past scrutiny. Hence, urine and blood samples were collected in WP and SP <span class="hlt">submariners</span> at control prepatrol time as well as on <span class="hlt">submarine</span> patrol days 20, 41, and 58. Several urine and serum metabolic markers were quantified, namely, deoxypyridinoline (DPD), lactate, albumin, creatinine, nonesterified fatty acids (NEFA), and ionized sodium (Na+) or potassium (K+), with a view to assessing bone, muscle, liver, or kidney metabolisms. We evidenced bone metabolism alteration (urine DPD, calcium, and phosphorus) previously recorded in <span class="hlt">submarine</span> crewmembers under prolonged patrols. We also highlighted transitory modifications in liver metabolism (serum albumin) occurring within the first 20 days of submersion. We further evidenced changes in submariners’ renal physiology (serum creatinine) throughout the entire patrol time span. Measurements of ionic homeostasis (serum Na+ and K+) displayed potential seasonal impact over <span class="hlt">active</span> ionic pumps in <span class="hlt">submariners</span>. Finally, there is some evidence that submersion provides beneficial conditions prone to fend off seasonal lactic acidosis (serum lactate) detected in WP <span class="hlt">submariners</span>. PMID:26265754</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..341..287S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..341..287S"><span>Understanding causality and uncertainty in volcanic observations: An example of forecasting eruptive <span class="hlt">activity</span> on Soufrière Hills <span class="hlt">Volcano</span>, Montserrat</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sheldrake, T. E.; Aspinall, W. P.; Odbert, H. M.; Wadge, G.; Sparks, R. S. J.</p> <p>2017-07-01</p> <p>Following a cessation in eruptive <span class="hlt">activity</span> it is important to understand how a <span class="hlt">volcano</span> will behave in the future and when it may next erupt. Such an assessment can be based on the <span class="hlt">volcano</span>'s long-term pattern of behaviour and insights into its current state via monitoring observations. We present a Bayesian network that integrates these two strands of evidence to forecast future eruptive scenarios using expert elicitation. The Bayesian approach provides a framework to quantify the magmatic causes in terms of volcanic effects (i.e., eruption and unrest). In October 2013, an expert elicitation was performed to populate a Bayesian network designed to help forecast future eruptive (in-)<span class="hlt">activity</span> at Soufrière Hills <span class="hlt">Volcano</span>. The Bayesian network was devised to assess the state of the shallow magmatic system, as a means to forecast the future eruptive <span class="hlt">activity</span> in the context of the long-term behaviour at similar dome-building <span class="hlt">volcanoes</span>. The findings highlight coherence amongst experts when interpreting the current behaviour of the <span class="hlt">volcano</span>, but reveal considerable ambiguity when relating this to longer patterns of volcanism at dome-building <span class="hlt">volcanoes</span>, as a class. By asking questions in terms of magmatic causes, the Bayesian approach highlights the importance of using short-term unrest indicators from monitoring data as evidence in long-term forecasts at <span class="hlt">volcanoes</span>. Furthermore, it highlights potential biases in the judgements of volcanologists and identifies sources of uncertainty in terms of magmatic causes rather than scenario-based outcomes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006CRGeo.338..499G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006CRGeo.338..499G"><span>Evidence for a seismic <span class="hlt">activity</span> mainly constituted of hybrid events at Cayambe <span class="hlt">volcano</span>, Ecuador. Interpretation in a iced-domes <span class="hlt">volcano</span> context</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guillier, Bertrand; Chatelain, Jean-Luc</p> <p>2006-06-01</p> <p>The high <span class="hlt">activity</span> level of Hybrid Events (HE) detected beneath the Cayambe <span class="hlt">volcano</span> since 1989 has been more thoroughly investigated with data from a temporary array. The unusual HE spectral content allows separating a high-frequency signal riding on a low-frequency one, with a probable single source. HEs are interpreted as high frequency VT events, produced by the interaction between magmatic heat and an underground water system fed by thaw water from the summital glacier, which trigger simultaneous low-frequency fluid resonance in the highly fractured adjacent medium. Pure VTs are interpreted as 'aborted' HEs occurring probably in the oldest and coldest part of the <span class="hlt">volcano</span> complex. To cite this article: B. Guillier, J.-L. Chatelain, C. R. Geoscience 338 (2006).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-0203323&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-0203323&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dactive%2Bvolcanoes"><span>Erupting <span class="hlt">Volcano</span> Mount Etna</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2002-01-01</p> <p>Expedition Five crew members aboard the International Space Station (ISS) captured this overhead look at the smoke and ash regurgitated from the erupting <span class="hlt">volcano</span> Mt. Etna on the island of Sicily, Italy in October 2002. Triggered by a series of earthquakes on October 27, 2002, this eruption was one of Etna's most vigorous in years. This image shows the ash plume curving out toward the horizon. The lighter-colored plumes down slope and north of the summit seen in this frame are produced by forest fires set by flowing lava. At an elevation of 10,990 feet (3,350 m), the summit of the Mt. Etna <span class="hlt">volcano</span>, one of the most <span class="hlt">active</span> and most studied <span class="hlt">volcanoes</span> in the world, has been <span class="hlt">active</span> for a half-million years and has erupted hundreds of times in recorded history.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.8435S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.8435S"><span><span class="hlt">Submarine</span> landslide and tsunami hazards offshore southern Alaska: Seismic strengthening versus rapid sedimentation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sawyer, Derek E.; Reece, Robert S.; Gulick, Sean P. S.; Lenz, Brandi L.</p> <p>2017-08-01</p> <p>The southern Alaskan offshore margin is prone to <span class="hlt">submarine</span> landslides and tsunami hazards due to seismically <span class="hlt">active</span> plate boundaries and extreme sedimentation rates from glacially enhanced mountain erosion. We examine the <span class="hlt">submarine</span> landslide potential with new shear strength measurements acquired by Integrated Ocean Drilling Program Expedition 341 on the continental slope and Surveyor Fan. These data reveal lower than expected sediment strength. Contrary to other <span class="hlt">active</span> margins where seismic strengthening enhances slope stability, the high-sedimentation margin offshore southern Alaska behaves like a passive margin from a shear strength perspective. We interpret that seismic strengthening occurs but is offset by high sedimentation rates and overpressure. This conclusion is supported by shear strength outside of the fan that follow an <span class="hlt">active</span> margin trend. More broadly, seismically <span class="hlt">active</span> margins with wet-based glaciers are susceptible to <span class="hlt">submarine</span> landslide hazards because of the combination of high sedimentation rates and earthquake shaking.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMED21C0686R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMED21C0686R"><span>VEPP Exercise: Volcanic <span class="hlt">Activity</span> and Monitoring of Pu`u `O`o, Kilauea <span class="hlt">Volcano</span>, Hawaii</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rodriguez, L. A.</p> <p>2010-12-01</p> <p>A 10-week project will be tested during the Fall semester 2010, for a Volcanic Hazards elective course, for undergraduate Geology students of the University of Puerto Rico at Mayaguez. This exercise was developed during the <span class="hlt">Volcanoes</span> Exploration Project: Pu`u `O`o (VEPP) Workshop, held on the Big Island of Hawaii in July 2010. For the exercise the students will form groups (of 2-4 students), and each group will be assigned a monitoring technique or method, among the following: seismic (RSAM data), deformation (GPS and tilt data), observations (webcam and lava flow maps), gas and thermal monitoring. The project is designed for Geology undergraduates who have a background in introductory geology, types of <span class="hlt">volcanoes</span> and eruptions, magmatic processes, characteristics of lava flows, and other related topics. It is divided in seven tasks, starting with an introduction and demonstration of the VEPP website and the VALVE3 software, which is used to access monitoring data from the current eruption of Pu`u `O`o, Kilauea <span class="hlt">volcano</span>, Hawaii. The students will also familiarize themselves with the history of Kilauea <span class="hlt">volcano</span> and its current eruption. At least weekly the groups will acquire data (mostly near-real-time) from the different monitoring techniques, in the form of time series, maps, videos, and images, in order to identify trends in the data. The groups will meet biweekly in the computer laboratory to work together in the analysis and interpretation of the data, with the support of the instructor. They will give reports on the progress of the exercise, and will get feedback from the instructor and from the other expert groups. All groups of experts will relate their findings to the recent and current <span class="hlt">activity</span> of Kilauea <span class="hlt">volcano</span>, and the importance of their specific type of monitoring. The <span class="hlt">activity</span> will culminate with a written report and an oral presentation. The last task of the project consists of a wrap-up <span class="hlt">volcano</span> monitoring exercise, in which the students will</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982easc.conf..277M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982easc.conf..277M"><span><span class="hlt">Submarine</span> laser communications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McConathy, D. R.</p> <p></p> <p>The Department of the Navy and the Defense Advanced Research Projects Agency (DARPA) are sponsoring a joint study to investigate the use of blue-green laser technology to comunicate with <span class="hlt">submarines</span> at operating depths. Two approaches are under investigation - one in which the laser itself is space-based, and the other in which the laser is ground-based with its beam redirected to the earth's surface by an orbiting mirror. This paper discusses these two approaches, and presents a brief history of <span class="hlt">activities</span> which led to the current studies.</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://hdl.handle.net/2060/19890011943','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890011943"><span>Iridium emissions from Hawaiian <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Finnegan, D. L.; Zoller, W. H.; Miller, T. M.</p> <p>1988-01-01</p> <p>Particle and gas samples were collected at Mauna Loa <span class="hlt">volcano</span> during and after its eruption in March and April, 1984 and at Kilauea <span class="hlt">volcano</span> in 1983, 1984, and 1985 during various phases of its ongoing <span class="hlt">activity</span>. In the last two Kilauea sampling missions, samples were collected during eruptive <span class="hlt">activity</span>. The samples were collected using a filterpack system consisting of a Teflon particle filter followed by a series of 4 base-treated Whatman filters. The samples were analyzed by INAA for over 40 elements. As previously reported in the literature, Ir was first detected on particle filters at the Mauna Loa Observatory and later from non-erupting high temperature vents at Kilauea. Since that time Ir was found in samples collected at Kilauea and Mauna Loa during fountaining <span class="hlt">activity</span> as well as after eruptive <span class="hlt">activity</span>. Enrichment factors for Ir in the volcanic fumes range from 10,000 to 100,000 relative to BHVO. Charcoal impregnated filters following a particle filter were collected to see if a significant amount of the Ir was in the gas phase during sample collection. Iridium was found on charcoal filters collected close to the vent, no Ir was found on the charcoal filters. This indicates that all of the Ir is in particulate form very soon after its release. Ratios of Ir to F and Cl were calculated for the samples from Mauna Loa and Kilauea collected during fountaining <span class="hlt">activity</span>. The implications for the KT Ir anomaly are still unclear though as Ir was not found at <span class="hlt">volcanoes</span> other than those at Hawaii. Further investigations are needed at other <span class="hlt">volcanoes</span> to ascertain if basaltic <span class="hlt">volcanoes</span> other than hot spots have Ir enrichments in their fumes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011EOSTr..92Q.187S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011EOSTr..92Q.187S"><span>Iceland's Grímsvötn <span class="hlt">volcano</span> erupts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Showstack, Randy</p> <p>2011-05-01</p> <p>About 13 months after Iceland's Eyjafjallajökull <span class="hlt">volcano</span> began erupting on 14 April 2010, which led to extensive air traffic closures over Europe, Grímsvötn <span class="hlt">volcano</span> in southeastern took its turn. Iceland's most <span class="hlt">active</span> <span class="hlt">volcano</span>, which last erupted in 2004 and lies largely beneath the Vatnajökull ice cap, began its eruption <span class="hlt">activity</span> on 21 May, with the ash plume initially reaching about 20 kilometers in altitude, according to the Icelandic Meteorological Office. Volcanic ash from Grímsvötn has cancelled hundreds of airplane flights and prompted U.S. president Barack Obama to cut short his visit to Ireland. As Eos went to press, <span class="hlt">activity</span> at the <span class="hlt">volcano</span> was beginning to subside.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26660745','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26660745"><span>Reference PMHS Sled Tests to Assess <span class="hlt">Submarining</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Uriot, Jérôme; Potier, Pascal; Baudrit, Pascal; Trosseille, Xavier; Petit, Philippe; Richard, Olivier; Compigne, Sabine; Masuda, Mitsutoshi; Douard, Richard</p> <p>2015-11-01</p> <p>Sled tests focused on pelvis behavior and <span class="hlt">submarining</span> can be found in the literature. However, they were performed either with rigid seats or with commercial seats. The objective of this study was to get reference tests to assess the <span class="hlt">submarining</span> ability of dummies in more realistic conditions than on rigid seat, but still in a repeatable and reproducible setup. For this purpose, a semi-rigid seat was developed, which mimics the behavior of real seats, although it is made of rigid plates and springs that are easy to reproduce and simulate with an FE model. In total, eight PMHS sled tests were performed on this semirigid seat to get data in two different configurations: first in a front seat configuration that was designed to prevent <span class="hlt">submarining</span>, then in a rear seat configuration with adjusted spring stiffness to generate <span class="hlt">submarining</span>. All subjects sustained extensive rib fractures from the shoulder belt loading. No pelvis fractures and no <span class="hlt">submarining</span> were observed in the front seat configuration, but two subjects sustained lumbar vertebrae fractures. In the rear seat configuration, all subjects sustained pelvic fractures and demonstrated <span class="hlt">submarining</span>. Corridors were constructed for the external forces and the PMHS kinematics. They are provided in this paper as new reference tests to assess the biofidelity of human surrogates in different configurations that either result in <span class="hlt">submarining</span> or do not. In future, it is intended to analyze further seat and restraint system configurations to be able to define a <span class="hlt">submarining</span> predictor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70005757','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70005757"><span>Introduction - The impacts of the 2008 eruption of Kasatochi <span class="hlt">Volcano</span> on terrestrial and marine ecosystems in the Aleutian Islands, 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>DeGange, Anthony R.; Byrd, G. Vernon; Walker, Lawrence R.; Waythomas, C.F.</p> <p>2010-01-01</p> <p>The Aleutian Islands are situated on the northern edge of the so-called “Pacific Ring of Fire,” a 40,000-km-long horseshoe-shaped assemblage of continental landmasses and islands bordering the Pacific Ocean basin that contains many of the world's <span class="hlt">active</span> and dormant <span class="hlt">volcanoes</span>. Schaefer et al. (2009) listed 27 historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Aleutian Islands, of which nine have had at least one major eruptive event since 1990. Volcanic eruptions are often significant natural disturbances, and ecosystem responses to volcanic eruptions may vary markedly with eruption style (effusive versus explosive), frequency, and magnitude of the eruption as well as isolation of the disturbed sites from potential colonizing organisms (del Moral and Grishin, 1999). Despite the relatively high frequency of volcanic <span class="hlt">activity</span> in the Aleutians, the response of island ecosystems to volcanic disturbances is largely unstudied because of the region's isolation. The only ecological studies in the region that address the effects of volcanic <span class="hlt">activity</span> were done on Bogoslof Island, a remote, highly <span class="hlt">active</span> volcanic island in the eastern Aleutians, which grew from a <span class="hlt">submarine</span> eruption in 1796 (Merriam, 1910; Byrd et al., 1980; Byrd and Williams, 1994). Nevertheless, in the 214 years of Bogoslof's existence, the island has been visited only intermittently.Kasatochi Island is a small (2.9 km by 2.6 km, 314 m high) <span class="hlt">volcano</span> in the central Aleutian Islands of Alaska (52.17°N latitude, 175.51°W longitude; Fig. 1) that erupted violently on 7-8 August 2008 after a brief, but intense period of precursory seismic <span class="hlt">activity</span> (Scott et al., 2010 [this issue]; Waythomas et al., in review). The island is part of the Aleutian arc volcanic front, and is an isolated singular island. Although the immediate offshore areas are relatively shallow (20–50 m water depth), the island is about 10 km south of the 2000 m isobath, north of which, ocean depths increase markedly. Kasatochi is located between the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005voen.book.....M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005voen.book.....M"><span><span class="hlt">Volcanoes</span> and the Environment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marti, Edited By Joan; Ernst, Gerald G. J.</p> <p>2005-10-01</p> <p><span class="hlt">Volcanoes</span> and the Environment is a comprehensive and accessible text incorporating contributions from some of the world's authorities in volcanology. This book is an indispensable guide for those interested in how volcanism affects our planet's environment. It spans a wide variety of topics from geology to climatology and ecology; it also considers the economic and social impacts of volcanic <span class="hlt">activity</span> on humans. Topics covered include how <span class="hlt">volcanoes</span> shape the environment, their effect on the geological cycle, atmosphere and climate, impacts on health of living on <span class="hlt">active</span> <span class="hlt">volcanoes</span>, volcanism and early life, effects of eruptions on plant and animal life, large eruptions and mass extinctions, and the impact of volcanic disasters on the economy. This book is intended for students and researchers interested in environmental change from the fields of earth and environmental science, geography, ecology and social science. It will also interest policy makers and professionals working on natural hazards. An all-inclusive text that goes beyond the geological working of <span class="hlt">volcanoes</span> to consider their environmental and sociological impacts Each chapter is written by one of the world's leading authorities on the subject Accessible to students and researchers from a wide variety of backgrounds</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24631200','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24631200"><span>Cellular immune responses and phagocytic <span class="hlt">activity</span> of fishes exposed to pollution of <span class="hlt">volcano</span> mud.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Risjani, Yenny; Yunianta; Couteau, Jerome; Minier, Christophe</p> <p>2014-05-01</p> <p>Since May 29, 2006, a mud <span class="hlt">volcano</span> in the Brantas Delta of the Sidoarjo district has emitted mud that has inundated nearby villages. Pollution in this area has been implicated in detrimental effects on fish health. In fishes, leukocyte and phagocytic cells play a vital role in body defenses. We report for the first time the effect of "LUSI" <span class="hlt">volcano</span> mud on the immune systems of fish in the Brantas Delta. The aim of this study was to find biomarkers to allow the evaluation of the effects of volcanic mud and anthropogenic pollution on fish health in the Brantas Delta. The study took places at the Brantas Delta, which was polluted by <span class="hlt">volcano</span> mud, and at reference sites in Karangkates and Pasuruan. Leukocyte numbers were determined using a Neubauer hemocytometer and a light microscope. Differential leukocyte counts were determined using blood smears stained with May Grunwald-Giemsa, providing neutrophil, lymphocyte and monocyte counts. Macrophages were taken from fish kidney, and their phagocytic <span class="hlt">activity</span> was measured. In vitro analyses revealed that leukocyte and differential leukocyte counts (DLC) were higher in Channa striata and Chanos chanos caught from the polluted area. Macrophage numbers were higher in Oreochromis mossambicus than in the other species, indicating that this species is more sensitive to pollution. In areas close to volcanic mud eruption, all specimens had lower phagocytic <span class="hlt">activity</span>. Our results show that immune cells were changed and phagocytic <span class="hlt">activity</span> was reduced in the polluted area indicating cytotoxicity and alteration of the innate immune system in fishes exposed to LUSI <span class="hlt">volcano</span> mud and anthropogenic pollution. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BVol...79....6S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BVol...79....6S"><span>Dendrogeomorphic reconstruction of lahar <span class="hlt">activity</span> and triggers: Shiveluch <span class="hlt">volcano</span>, Kamchatka Peninsula, Russia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salaorni, E.; Stoffel, M.; Tutubalina, O.; Chernomorets, S.; Seynova, I.; Sorg, A.</p> <p>2017-01-01</p> <p>Lahars are highly concentrated, water-saturated volcanic hyperconcentrated flows or debris flows containing pyroclastic material and are a characteristic mass movement process on volcanic slopes. On Kamchatka Peninsula (Russian Federation), lahars are widespread and may affect remote settlements. Historical records of past lahar occurrences are generally sparse and mostly limited to events which damaged infrastructure on the slopes or at the foot of <span class="hlt">volcanoes</span>. In this study, we present a tree-ring-based reconstruction of spatiotemporal patterns of past lahar <span class="hlt">activity</span> at Shiveluch <span class="hlt">volcano</span>. Using increment cores and cross sections from 126 Larix cajanderi trees, we document 34 events covering the period AD 1729-2012. Analyses of the seasonality of damage in trees reveal that 95% of all lahars occurred between October and May and thus point to the predominant role of the sudden melt of the snow cover by volcanic material. These observations suggest that most lahars were likely syn-eruptive and that lahar <span class="hlt">activity</span> is largely restricted to periods of volcanic <span class="hlt">activity</span>. By contrast, rainfall events do not seem to play a significant role in lahar triggering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.V21C0727C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.V21C0727C"><span>Magma Vesiculation and Infrasonic <span class="hlt">Activity</span> in Open Conduit <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Colo', L.; Baker, D. R.; Polacci, M.; Ripepe, M.</p> <p>2007-12-01</p> <p>At persistently <span class="hlt">active</span> basaltic <span class="hlt">volcanoes</span> such as Stromboli, Italy degassing of the magma column can occur in "passive" and "<span class="hlt">active</span>" conditions. Passive degassing is generally understood as a continuous, non explosive release of gas mainly from the open summit vents and subordinately from the conduit's wall or from fumaroles. In passive degassing generally gas is in equilibrium with atmospheric pressure, while in <span class="hlt">active</span> degassing the gas approaches the surface at overpressurized conditions. During <span class="hlt">active</span> degassing (or puffing), the magma column is interested by the bursting of small gas bubbles at the magma free surface and, as a consequence, the <span class="hlt">active</span> degassing process generates infrasonic signals. We postulated, in this study, that the rate and the amplitude of infrasonic <span class="hlt">activity</span> is somehow linked to the rate and the volume of the overpressured gas bubbles, which are generated in the magma column. Our hypothesis is that infrasound is controlled by the quantities of gas exsolved in the magma column and then, that a relationship between infrasound and the vesiculation process should exist. In order to achieve this goal, infrasonic records and bubble size distributions of scoria samples from normal explosive <span class="hlt">activity</span> at Stromboli processed via X ray tomography have been compared. We observed that the cumulative distribution for both data sets follow similar power laws, indicating that both processes are controlled by a scale invariant phenomenon. However the power law is not stable but changes in different scoria clasts, reflecting when gas bubble nucleation is predominant over bubbles coalescence and viceversa. The power law also changes for the infrasonic <span class="hlt">activity</span> from time to time, suggesting that infrasound may be controlled also by a different gas exsolution within the magma column. Changes in power law distributions are the same for infrasound and scoria indicating that they are linked to the same process acting in the magmatic system. We suggest that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA01722.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA01722.html"><span>Space Radar Image of Colombian <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1999-01-27</p> <p>This is a radar image of a little known <span class="hlt">volcano</span> in northern Colombia. The image was acquired on orbit 80 of space shuttle Endeavour on April 14, 1994, by NASA Spaceborne Imaging Radar C/X-Band Synthetic Aperture Radar SIR-C/X-SAR. The <span class="hlt">volcano</span> near the center of the image is located at 5.6 degrees north latitude, 75.0 degrees west longitude, about 100 kilometers (65 miles) southeast of Medellin, Colombia. The conspicuous dark spot is a lake at the bottom of an approximately 3-kilometer-wide (1.9-mile) volcanic collapse depression or caldera. A cone-shaped peak on the bottom left (northeast rim) of the caldera appears to have been the source for a flow of material into the caldera. This is the northern-most known <span class="hlt">volcano</span> in South America and because of its youthful appearance, should be considered dormant rather than extinct. The <span class="hlt">volcano</span>'s existence confirms a fracture zone proposed in 1985 as the northern boundary of volcanism in the Andes. The SIR-C/X-SAR image reveals another, older caldera further south in Colombia, along another proposed fracture zone. Although relatively conspicuous, these <span class="hlt">volcanoes</span> have escaped widespread recognition because of frequent cloud cover that hinders remote sensing imaging in visible wavelengths. Four separate <span class="hlt">volcanoes</span> in the Northern Andes nations of Colombia and Ecuador have been <span class="hlt">active</span> during the last 10 years, killing more than 25,000 people, including scientists who were monitoring the volcanic <span class="hlt">activity</span>. Detection and monitoring of <span class="hlt">volcanoes</span> from space provides a safe way to investigate volcanism. The recognition of previously unknown <span class="hlt">volcanoes</span> is important for hazard evaluations because a number of major eruptions this century have occurred at mountains that were not previously recognized as <span class="hlt">volcanoes</span>. http://photojournal.jpl.nasa.gov/catalog/PIA01722</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=reaction&pg=4&id=EJ1110457','ERIC'); return false;" href="https://eric.ed.gov/?q=reaction&pg=4&id=EJ1110457"><span>Exploring the Gas Chemistry of Old <span class="hlt">Submarine</span> Technologies Using Plastic Bottles as Reaction Vessels and Models</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>Horikoshi, Ryo; Takeiri, Fumitaka; Kobayashi, Yoji; Kageyama, Hiroshi</p> <p>2016-01-01</p> <p>We describe an <span class="hlt">activity</span> that is suitable for high school students and makes use of plastic bottles. This <span class="hlt">activity</span> allows students to familiarize themselves with gas chemistry by introducing technologies that were applied in old <span class="hlt">submarine</span> systems. Plastic bottles, which are representative of <span class="hlt">submarines</span>, are used as reaction vessels. Three simple…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMDI53A..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMDI53A..02H"><span>Geochemical Evidence Against Pyroxenites in the Sources of Hawaiian <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Humayun, M.; Yang, S.; Clague, D. A.</p> <p>2017-12-01</p> <p>Hawaiian lavas exhibit high Fe/Mn ratios, and other elemental and isotopic characteristics, that have been argued to be evidence for chemical interactions at the core-mantle boundary. Alternatively, the enrichment in silica relative to 3 GPa melts of garnet peridotite, and the high Fe/Mn, has been argued to represent the contributions of garnet pyroxenite melts generated beneath a thick lithosphere. Here, we present a set of new elemental ratios designed to effectively discriminate partial melts of peridotite from pyroxenite in mantle sources. A set of 200 Hawaiian volcanic glasses from 7 <span class="hlt">volcanoes</span> were analyzed by LA-ICP-MS for the abundances of 63 elements, with an emphasis on obtaining precise Ge/Si ratios. From experimental partitioning, silica-rich partial melts of MORB-like garnet pyroxenite are expected to have low Ge/Si ratios relative to their sources due to the retention of Ge in the residue by both garnet and pyroxene. In contrast, partial melts of peridotite are expected to have high Ge/Si ratios relative to mantle peridotites due to the incompatibility of Ge in olivine. We observed that Ge abundances in subaerial Hawaiian <span class="hlt">volcanoes</span> are correlated with indicators of volcanic degassing, including S, Re and As. Subaerial and <span class="hlt">submarine</span> lavas exhibit a correlation between Ge/Si ratio and S content that indicates that all Hawaiian lavas share the same pre-eruptive Ge/Si ratio. <span class="hlt">Submarine</span> glasses with the least evidence of degassing exhibit a constant Ge/Si ratio over the range of SiO2 (44-52 %) observed in Hawaiian volcanics. Surprisingly, MORB glasses exhibit more variation in Ge/Si ratio than the pre-eruptive Ge/Si of Hawaiian glasses, implying the presence of 0-12% recycled crust in the MORB source. The constant Ge/Si ratio of Hawaiian glasses implies that pyroxenite melting did not enrich Hawaiian lavas in silica. Processes that could yield Si-rich melts without changing the Ge/Si ratio may involve melt-lithosphere interaction or bridgmanite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V23E0535S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V23E0535S"><span>Characteristics and petrology of the effusive-explosive <span class="hlt">activity</span> of Colima <span class="hlt">volcano</span>, in the years 2015-2017</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suarez-Plascencia, C.; Nuñez-Cornu, F. J.; Arreola-Ochoa, L. C.; Suarez, G. B. V.; Carrillo-Gonzalez, D. A.</p> <p>2017-12-01</p> <p>The Colima <span class="hlt">volcano</span>, during the years 2015-2017, presented an important effusive and explosive <span class="hlt">activity</span>, which began in January 2015 with the growth of a dome that was destroyed by explosions, forming pyroclastic flows reaching distances of up to 2 km by the north and south flanks of the <span class="hlt">volcano</span>. In May a new dome was extruded, forming three thick lava flows along the northern and southern slopes; the extruded volume was approximately 6 million cubic meters, with a rate in 52 days of 1.3 m3/sec. On July 11 merapi flows were formed it flowed through by the ravines of Montegrande and San Antonio, on the south and southwest flank, reaching distances of 10.4 km. The following days the <span class="hlt">activity</span> had decreased substantially, leaving a crater of 60 m of depth and 270 m of diameter. In February 2016, a small dome occupied the central part of the main crater, and it was until September that an episode of volcanic tremor began, that was associated with its rapid growth, which in 48 hours filled the crater and formed a lava flow that descended by the south slope. By October 2, 2.3 million m3 of lava were extruded, which caused a deflation of the dome. In October 7, the <span class="hlt">volcano</span> emitted a great amount of gases and steam of water that formed an acid rain that affected forests and crops of the south and southwest slope, causing losses by 1 million dollars. In November, a series of explosions occurred that destroyed two thirds of the dome. In January 2017, the explosive <span class="hlt">activity</span> increased and again destroyed the dome. Five events were recorded that reached between 3 km and 4 km of height on the top of the <span class="hlt">volcano</span>, the dispersion of the ash generally went to the northeast, reaching distances of up to 200 km. Currently the <span class="hlt">volcano</span> is sustaining reduced seismic and fumarole <span class="hlt">activity</span>. In 2005, 2015 and 2017, the geochemical analysis of major elements such as SiO2 from the ash emitted by the <span class="hlt">volcano</span> showed an increase from 54.51% to 60.05% and 60.24%, respectively, which was associated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018LPICo2085.6022S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018LPICo2085.6022S"><span>Origin of Abiotic Methane in <span class="hlt">Submarine</span> Hydrothermal Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seewald, J. S.; German, C. R.; Grozeva, N. G.; Klein, F.; McDermott, J. M.; Ono, S.; Reeves, E. P.; Wang, D. T.</p> <p>2018-05-01</p> <p>Results of recent investigations into the chemical and isotopic composition of <span class="hlt">actively</span> venting <span class="hlt">submarine</span> hydrothermal fluids and volatile species trapped in fluid inclusions will be discussed in the context of processes responsible for abiotic CH4 formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019390','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019390"><span><span class="hlt">Submarine</span> landslides</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hampton, M.A.; Lee, H.J.; Locat, J.</p> <p>1996-01-01</p> <p>Landslides are common on inclined areas of the seafloor, particularly in environments where weak geologic materials such as rapidly deposited, finegrained sediment or fractured rock are subjected to strong environmental stresses such as earthquakes, large storm waves, and high internal pore pressures. <span class="hlt">Submarine</span> landslides can involve huge amounts of material and can move great distances: slide volumes as large as 20,000 km3 and runout distances in excess of 140 km have been reported. They occur at locations where the downslope component of stress exceeds the resisting stress, causing movement along one or several concave to planar rupture surfaces. Some recent slides that originated nearshore and retrogressed back across the shoreline were conspicuous by their direct impact on human life and <span class="hlt">activities</span>. Most known slides, however, occurred far from land in prehistoric time and were discovered by noting distinct to subtle characteristics, such as headwall scarps and displaced sediment or rock masses, on acoustic-reflection profiles and side-scan sonar images. <span class="hlt">Submarine</span> landslides can be analyzed using the same mechanics principles as are used for occurrences on land. However, some loading mechanisms are unique, for example, storm waves, and some, such as earthquakes, can have greater impact. The potential for limited-deformation landslides to transform into sediment flows that can travel exceedingly long distances is related to the density of the slope-forming material and the amount of shear strength that is lost when the slope fails.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA21878.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA21878.html"><span>NASA Satellite Images Erupting Russian <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-08-22</p> <p>Klyuchevskoi, one of the world's most <span class="hlt">active</span> <span class="hlt">volcanoes</span>, is seen poking through above a solid cloud deck, with an ash plume streaming to the west. Located on the Kamchatka Peninsula in far eastern Russia, it is one of many <span class="hlt">active</span> <span class="hlt">volcanoes</span> on the Peninsula. Nearby, to the south, the smaller Bezymianny <span class="hlt">volcano</span> can be seem with a small steam plume coming from its summit. The image was acquired Aug. 20, 2017, covers an area of 12 by 14 miles (19.5 by 22.7 kilometers), and is located at 56.1 degrees north, 160.6 degrees east. https://photojournal.jpl.nasa.gov/catalog/PIA21878</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2010/5243/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2010/5243/"><span>2008 Volcanic <span class="hlt">activity</span> in Alaska, Kamchatka, and the Kurile Islands: Summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Neal, Christina A.; McGimsey, Robert G.; Dixon, James P.; Cameron, Cheryl E.; Nuzhdaev, Anton A.; Chibisova, Marina</p> <p>2011-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, possible eruptions, and volcanic unrest or suspected unrest at seven separate volcanic centers in Alaska during 2008. Significant explosive eruptions at Okmok and Kasatochi <span class="hlt">Volcanoes</span> in July and August dominated Observatory operations in the summer and autumn. AVO maintained 24-hour staffing at the Anchorage facility from July 12 through August 28. Minor eruptive <span class="hlt">activity</span> continued at Veniaminof and Cleveland <span class="hlt">Volcanoes</span>. Observed volcanic unrest at Cook Inlet's Redoubt <span class="hlt">Volcano</span> presaged a significant eruption in the spring of 2009. AVO staff also participated in hazard communication regarding eruptions or unrest at nine <span class="hlt">volcanoes</span> in Russia as part of a collaborative role in the Kamchatka and Sakhalin Volcanic Eruption Response Teams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7302C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7302C"><span>Implications for future <span class="hlt">activity</span> of Grímsvötn <span class="hlt">volcano</span>, Iceland, from compositional time series of historical tephra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carpentier, Marion; Sigmarsson, Olgeir; Larsen, Gudrun</p> <p>2014-05-01</p> <p>The nature of future eruptions of <span class="hlt">active</span> <span class="hlt">volcanoes</span> is hard to predict. Improved understanding of the past volcanic <span class="hlt">activity</span> is probably the best way to infer future eruptive scenarios. The most <span class="hlt">active</span> <span class="hlt">volcano</span> in Iceland, Grímsvötn, last erupted in 2011 with consequences for habitants living close to the <span class="hlt">volcano</span> and aviation in the North-Atlantic. In an effort to better understand the magmatic system of the <span class="hlt">volcano</span>, we have investigated the compositions of 23 selected tephra layers representing the last 8 centuries of volcanic <span class="hlt">activity</span> at Grímsvötn. The tephra was collected in the ablation area of outlet glaciers from Vatnajökull ice cap. The ice-conserved tephra are less prone to alteration than those exposed in soil sections. Major element analyses are indistinguishable and of quartz-normative tholeiite composition, and Sr and Nd isotope ratios are constant. In contrast, both trace element concentrations (Th range from 0.875 ppm to 1.37 ppm and Ni from 28.5 ppm to 56.6 ppm) in the basalts and Pb isotopes show small but significant variations. The high-precision analyses of Pb isotope ratios allow the identification of tephra samples (3 in total) with more radiogenic ratios than the bulk of the samples. The tephra of constant isotope ratios show linear increase in incompatible element concentrations with time. The rate of increasing concentrations permits exploring possible future scenarios assuming that the magmatic system beneath the <span class="hlt">volcano</span> follows the established historical evolution. Assuming similar future behaviour of the magma system beneath Grímsvötn <span class="hlt">volcano</span>, the linear increase in e.g. Th concentration suggests that the <span class="hlt">volcano</span> is likely to principally produce basalts for the next 500-1000 years. Evolution of water concentration will most likely follow those of incompatible elements with consequent increases in explosiveness of future Grímsvötn eruptions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910032739&hterms=1575&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231575','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910032739&hterms=1575&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231575"><span>Remote sensing of <span class="hlt">volcanos</span> and volcanic terrains</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mouginis-Mark, Peter J.; Francis, Peter W.; Wilson, Lionel; Pieri, David C.; Self, Stephen; Rose, William I.; Wood, Charles A.</p> <p>1989-01-01</p> <p>The possibility of using remote sensing to monitor potentially dangerous <span class="hlt">volcanoes</span> is discussed. Thermal studies of <span class="hlt">active</span> <span class="hlt">volcanoes</span> are considered along with using weather satellites to track eruption plumes and radar measurements to study lava flow morphology and topography. The planned use of orbiting platforms to study emissions from <span class="hlt">volcanoes</span> and the rate of change of volcanic landforms is considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.9088L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.9088L"><span>TOMO-ETNA Experiment -Etna <span class="hlt">volcano</span>, Sicily, investigated with <span class="hlt">active</span> and passive seismic methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luehr, Birger-G.; Ibanez, Jesus M.; Díaz-Moreno, Alejandro; Prudencio, Janire; Patane, Domenico; Zieger, Toni; Cocina, Ornella; Zuccarello, Luciano; Koulakov, Ivan; Roessler, Dirk; Dahm, Torsten</p> <p>2017-04-01</p> <p>The TOMO-ETNA experiment, as part of the European Union project "MEDiterranean SUpersite <span class="hlt">Volcanoes</span> (MED-SUV)", was devised to image the crustal structure beneath Etna by using state of the art passive and <span class="hlt">active</span> seismic methods. <span class="hlt">Activities</span> on-land and offshore are aiming to obtain new high-resolution seismic images to improve the knowledge of crustal structures existing beneath the Etna <span class="hlt">volcano</span> and northeast Sicily up to the Aeolian Islands. In a first phase (June 15 - July 24, 2014) at Etna <span class="hlt">volcano</span> and surrounding areas two removable seismic networks were installed composed by 80 Short Period and 20 Broadband stations, additionally to the existing network belonging to the "Istituto Nazionale di Geofisica e Vulcanologia" (INGV). So in total air-gun shots could be recorded by 168 stations onshore plus 27 ocean bottom instruments offshore in the Tyrrhenian and Ionian Seas. Offshore <span class="hlt">activities</span> were performed by Spanish and Italian research vessels. In a second phase the broadband seismic network remained operative until October 28, 2014, as well as offshore surveys during November 19 -27, 2014. <span class="hlt">Active</span> seismic sources were generated by an array of air-guns mounted in the Spanish Oceanographic vessel "Sarmiento de Gamboa" with a power capacity of up to 5.200 cubic inches. In total more than 26.000 shots were fired and more than 450 local and regional earthquakes could be recorded and will be analyzed. For resolving a volcanic structure the investigation of attenuation and scattering of seismic waves is important. In contrast to existing studies that are almost exclusively based on S-wave signals emitted by local earthquakes, here air-gun signals were investigated by applying a new methodology based on the coda energy ratio defined as the ratio between the energy of the direct P-wave and the energy in a later coda window. It is based on the assumption that scattering caused by heterogeneities removes energy from direct P-waves that constitutes the earliest possible</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70122911','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70122911"><span>Giant <span class="hlt">submarine</span> canyons: Is size any clue to their importance in the rock record?</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Normark, William R.; Carlson, Paul R.</p> <p>2003-01-01</p> <p><span class="hlt">Submarine</span> canyons are the most important conduits for funneling sediment from continents to oceans. <span class="hlt">Submarine</span> canyons, however, are zones of sediment bypassing, and little sediment accumulates in the canyon until it ceases to be an <span class="hlt">active</span> conduit. To understand the potential importance in the rock record of any given <span class="hlt">submarine</span> canyon, it is necessary to understand sediment-transport processes in, as well as knowledge of, deep-sea turbidite and related deposits that moved through the canyons. There is no straightforward correlation between the final volume of the sedimentary deposits and size of the associated <span class="hlt">submarine</span> canyons. Comparison of selected modern <span class="hlt">submarine</span> canyons together with their deposits emphasizes the wide range of scale differences between canyons and their impact on the rock record.Three of the largest <span class="hlt">submarine</span> canyons in the world are incised into the Beringian (North American) margin of the Bering Sea. Zhemchug Canyon has the largest cross-section at the shelf break and greatest volume of incision of slope and shelf. The Bering Canyon, which is farther south in the Bering Sea, is first in length and total area. In contrast, the largest <span class="hlt">submarine</span> fans-e.g., Bengal, Indus, and Amazon-have substantially smaller, delta-front <span class="hlt">submarine</span> canyons that feed them; their <span class="hlt">submarine</span> drainage areas are one-third to less than one-tenth the area of Bering Canyon. some very large deep-sea channels and tubidite deposits are not even associated with a significant <span class="hlt">submarine</span> canyon; examples include Horizon Channel in the northeast Pacific and Laurentian Fan Valley in the North Atlantic. Available data suggest that the size of turbidity currents (as determined by volume of sediment transported to the basins) is also not a reliable indicator of <span class="hlt">submarine</span> canyon size.</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('https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034450p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034450p/"><span>30. VIEW OF PHOTO CAPTIONED '<span class="hlt">SUBMARINE</span> BASE, NEW LONDON, CONNECTICUT. ...</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>30. VIEW OF PHOTO CAPTIONED '<span class="hlt">SUBMARINE</span> BASE, NEW LONDON, CONNECTICUT. 2 JUNE 1930. <span class="hlt">SUBMARINE</span> TRAINING TANK - STEELWORK 98% COMPLETE; BRICKWORK 95% COMPLETE, PIPING 10% IN PLACE. LOOKING NORTH. CONTRACT NO. Y-1539-ELEVATOR, <span class="hlt">SUBMARINE</span> ESCAPE TANK.' - U.S. Naval <span class="hlt">Submarine</span> Base, New London <span class="hlt">Submarine</span> Escape Training Tank, Albacore & Darter Roads, Groton, New London County, CT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S11E4390K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S11E4390K"><span>Strong S-wave attenuation and <span class="hlt">actively</span> degassing magma beneath Taal <span class="hlt">volcano</span>, Philippines, inferred from source location analysis using high-frequency seismic amplitudes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumagai, H.; Lacson, R. _Jr., Jr.; Maeda, Y.; Figueroa, M. S., II; Yamashina, T.</p> <p>2014-12-01</p> <p>Taal <span class="hlt">volcano</span>, Philippines, is one of the world's most dangerous <span class="hlt">volcanoes</span> given its history of explosive eruptions and its close proximity to populated areas. A key feature of these eruptions is that the eruption vents were not limited to Main Crater but occurred on the flanks of <span class="hlt">Volcano</span> Island. This complex eruption history and the fact that thousands of people inhabit the island, which has been declared a permanent danger zone, together imply an enormous potential for disasters. The Philippine Institute of Volcanology and Seismology (PHIVOLCS) constantly monitors Taal, and international collaborations have conducted seismic, geodetic, electromagnetic, and geochemical studies to investigate the <span class="hlt">volcano</span>'s magma system. Realtime broadband seismic, GPS, and magnetic networks were deployed in 2010 to improve monitoring capabilities and to better understand the <span class="hlt">volcano</span>. The seismic network has recorded <span class="hlt">volcano</span>-tectonic (VT) events beneath <span class="hlt">Volcano</span> Island. We located these VT events based on high-frequency seismic amplitudes, and found that some events showed considerable discrepancies between the amplitude source locations and hypocenters determined by using onset arrival times. Our analysis of the source location discrepancies points to the existence of a region of strong S-wave attenuation near the ground surface beneath the east flank of <span class="hlt">Volcano</span> Island. This region is beneath the <span class="hlt">active</span> fumarolic area and above sources of pressure contributing inflation and deflation, and it coincides with a region of high electrical conductivity. The high-attenuation region matches that inferred from an <span class="hlt">active</span>-seismic survey conducted at Taal in 1993. Our results, synthesized with previous results, suggest that this region represents <span class="hlt">actively</span> degassing magma near the surface, and imply a high risk of future eruptions on the east flank of <span class="hlt">Volcano</span> Island.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gip/74/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gip/74/"><span><span class="hlt">Volcano</span> Hazards Program</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Venezky, Dina Y.; Myers, Bobbie; Driedger, Carolyn</p> <p>2008-01-01</p> <p>Diagram of common <span class="hlt">volcano</span> hazards. The U.S. Geological Survey <span class="hlt">Volcano</span> Hazards Program (VHP) monitors unrest and eruptions at U.S. <span class="hlt">volcanoes</span>, assesses potential hazards, responds to volcanic crises, and conducts research on how <span class="hlt">volcanoes</span> work. When conditions change at a monitored <span class="hlt">volcano</span>, the VHP issues public advisories and warnings to alert emergency-management authorities and the public. See http://<span class="hlt">volcanoes</span>.usgs.gov/ to learn more about <span class="hlt">volcanoes</span> and find out what's happening now.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.V53E2662L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.V53E2662L"><span>Temporal Variations of Magnetic Field Associated with Seismic <span class="hlt">Activity</span> at Cerro Machin <span class="hlt">Volcano</span>, Colombia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Londono, J. M.; Serna, J. P.; Guzman, J.</p> <p>2011-12-01</p> <p>A study of magnetic variations was carried out at Cerro Machin <span class="hlt">Volcano</span>, Colombia for the period 2009 -2010, with two permanent magnetometers located at South and North of the central dome, separated about 2.5 km each other. After corrections, we found that there is no clear correlation between volcanic seismicity and temporal changes of magnetic field for each magnetometer station, if they are analyzed individually. On the contrary, when we calculated the residual Magnetic field (RMF), for each magnetometer, and then we made the subtraction between them, and plot it vs time, we found a clear correlation of changes in local magnetic field with the occurrence of volcanic seismicity (ML >1.6). We found a change in the RMF between 1584 nT and 1608 nT, each time that a <span class="hlt">volcano</span>-tectonic earthquake occurred. The máximum lapse time between the previous change in RMF and the further occurrence of the earthquake is 24 days, with an average of 11 days. This pattern occurred more than 9 times during the studied period. Based on the results, we believed that the simple methodology proposed here, is a good tool for monitoring changes in seismicity associated with <span class="hlt">activity</span> at Cerro Machín <span class="hlt">volcano</span>. We suggest that the temporal changes of RMF at Cerro Machín <span class="hlt">Volcano</span>, are associated with piezo-magnetic effects, due to changes in strain-stress inside the <span class="hlt">volcano</span>, produced by the interaction between local faulting and magma movement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.T12B0453N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.T12B0453N"><span>Massive Pyroclastic Eruptions Accompanied the Sector Collapse of Oahu and the Nu`uanu Landslide: Petrological Evidence for a <span class="hlt">Submarine</span> Directed Blast</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Natland, J. H.; Atlas, Z.</p> <p>2003-12-01</p> <p>During ODP Leg 200 in December, 2002, a series of thinly bedded volcaniclastic turbidites and silty muds interbedded with two thicker and strongly indurated vitric tuffs was drilled at Site 1223 on the crest of the Hawaiian arch east of the island of Oahu. The massive Nu`uanu landslide debris field, derived from a massive collapse of the eastern half of Oahu at about 2 Ma, lies in the flexural moat between the site and the island. The shipboard interpretation (1) was that the muds and silts are typical turbidites derived by redeposition from beaches and nearshore benches, but that the tuffs represent the distal portions of large <span class="hlt">submarine</span> pyroclastic eruptions that may have attended the landslide. We report electron probe microanalyses of basaltic glass, olivine, Cr-spinel, palagonite and secondary minerals in the tuffs supporting the shipboard interpretation. In particular, the glass compositions from individual thin sections match precisely the range of compositions obtained from numerous samples of coarse volcaniclastic breccia sampled from the steep flanks of landslide blocks in the moat (2). This includes somewhat higher SiO2 and lower total iron as FeO(T) at given MgO than similar basaltic glasses from other Hawaiian <span class="hlt">volcanoes</span>, a distinctive attribute of tholeiitic basalt from Oahu's Ko`olau <span class="hlt">volcano</span>. Key attributes of the glasses in the tuffs and the minerals in them are that they are poly-compositional and they are strongly differentiated, with a range of compositions typical of those erupted from modern Hawaiian volcanic rift systems supplied by lateral diking from central conduits. The finer-grained tuffs at Site 1223 thus are indeed a distal pyroclastic facies that seemingly tapped much of the suddenly exposed, magma-inflated, deep flanking rift system of Ko`olau <span class="hlt">volcano</span>. Over-steepening of the NE flank of the <span class="hlt">volcano</span> coupled with internal weakening provided by near saturation of its rift system with magma may have triggered the landslide. This was almost</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=10518&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=10518&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dactive%2Bvolcanoes"><span>Shiveluch and Klyuchevskaya <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2007-01-01</p> <p>A distance of about 80 kilometers (50 miles) separates Shiveluch and Klyuchevskaya <span class="hlt">Volcanoes</span> on Russia's Kamchatka Peninsula. Despite this distance, however, the two acted in unison on April 26, 2007, when the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA's Terra satellite caught them both erupting simultaneously. ASTER 'sees' a slightly different portion of the light spectrum than human eyes. Besides a portion of visible light, ASTER detects thermal energy, meaning it can detect volcanic <span class="hlt">activity</span> invisible to human eyes. Inset in each image above is a thermal infrared picture of the <span class="hlt">volcano</span>'s summit. In these insets, dark red shows where temperatures are coolest, and yellowish-white shows where temperatures are hottest, heated by molten lava. Both insets show <span class="hlt">activity</span> at the crater. In the case of Klyuchevskaya, some <span class="hlt">activity</span> at the crater is also visible in the larger image. In the larger images, the landscapes around the <span class="hlt">volcanoes</span> appear in varying shades of blue-gray. Dark areas on the snow surface are likely stains left over from previous eruptions of volcanic ash. Overhead, clouds dot the sky, casting their shadows on the snow, especially southeast of Shiveluch and northeast of Klyuchevskaya. To the northwest of Klyuchevskaya is a large bank of clouds, appearing as a brighter white than the snow surface. Shiveluch (sometimes spelled Sheveluch) and Klyuchevskaya (sometimes spelled Klyuchevskoy or Kliuchevskoi) are both stratovolcanoes composed of alternating layers of hardened lava, solidified ash, and rocks from earlier eruptions. Both <span class="hlt">volcanoes</span> rank among Kamchatka's most <span class="hlt">active</span>. Because Kamchatka is part of the Pacific 'Ring of Fire,' the peninsula experiences regular seismic <span class="hlt">activity</span> as the Pacific Plate slides below other tectonic plates in the Earth's crust. Large-scale plate tectonic <span class="hlt">activity</span> causing simultaneous volcanic eruptions in Kamchatka is not uncommon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPA41B2169D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPA41B2169D"><span>Linking space observations to <span class="hlt">volcano</span> observatories in Latin America: Results from the CEOS DRM <span class="hlt">Volcano</span> Pilot</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delgado, F.; Pritchard, M. E.; Biggs, J.; Arnold, D. W. D.; Poland, M. P.; Ebmeier, S. K.; Wauthier, C.; Wnuk, K.; Parker, A. L.; Amelug, F.; Sansosti, E.; Mothes, P. A.; Macedo, O.; Lara, L.; Zoffoli, S.; Aguilar, V.</p> <p>2015-12-01</p> <p>Within Latin American, about 315 <span class="hlt">volcanoes</span> that have been <span class="hlt">active</span> in the Holocene, but according to the United Nations Global Assessment of Risk 2015 report (GAR15) 202 of these <span class="hlt">volcanoes</span> have no seismic, deformation or gas monitoring. Following the 2012 Santorini Report on satellite Earth Observation and Geohazards, the Committee on Earth Observation Satellites (CEOS) has developed a 3-year pilot project to demonstrate how satellite observations can be used to monitor large numbers of <span class="hlt">volcanoes</span> cost-effectively, particularly in areas with scarce instrumentation and/or difficult access. The pilot aims to improve disaster risk management (DRM) by working directly with the <span class="hlt">volcano</span> observatories that are governmentally responsible for <span class="hlt">volcano</span> monitoring, and the project is possible thanks to data provided at no cost by international space agencies (ESA, CSA, ASI, DLR, JAXA, NASA, CNES). Here we highlight several examples of how satellite observations have been used by <span class="hlt">volcano</span> observatories during the last 18 months to monitor <span class="hlt">volcanoes</span> and respond to crises -- for example the 2013-2014 unrest episode at Cerro Negro/Chiles (Ecuador-Colombia border); the 2015 eruptions of Villarrica and Calbuco <span class="hlt">volcanoes</span>, Chile; the 2013-present unrest and eruptions at Sabancaya and Ubinas <span class="hlt">volcanoes</span>, Peru; the 2015 unrest at Guallatiri <span class="hlt">volcano</span>, Chile; and the 2012-present rapid uplift at Cordon Caulle, Chile. Our primary tool is measurements of ground deformation made by Interferometric Synthetic Aperture Radar (InSAR) but thermal and outgassing data have been used in a few cases. InSAR data have helped to determine the alert level at these <span class="hlt">volcanoes</span>, served as an independent check on ground sensors, guided the deployment of ground instruments, and aided situational awareness. We will describe several lessons learned about the type of data products and information that are most needed by the <span class="hlt">volcano</span> observatories in different countries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMNH13B1377S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMNH13B1377S"><span>Hazard maps of Colima <span class="hlt">volcano</span>, Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suarez-Plascencia, C.; Nunez-Cornu, F. J.; Escudero Ayala, C. R.</p> <p>2011-12-01</p> <p>Colima <span class="hlt">volcano</span>, also known as Volcan de Fuego (19° 30.696 N, 103° 37.026 W), is located on the border between the states of Jalisco and Colima and is the most <span class="hlt">active</span> <span class="hlt">volcano</span> in Mexico. Began its current eruptive process in February 1991, in February 10, 1999 the biggest explosion since 1913 occurred at the summit dome. The <span class="hlt">activity</span> during the 2001-2005 period was the most intense, but did not exceed VEI 3. The <span class="hlt">activity</span> resulted in the formation of domes and their destruction after explosive events. The explosions originated eruptive columns, reaching attitudes between 4,500 and 9,000 m.a.s.l., further pyroclastic flows reaching distances up to 3.5 km from the crater. During the explosive events ash emissions were generated in all directions reaching distances up to 100 km, slightly affected nearby villages as Tuxpan, Tonila, Zapotlán, Cuauhtemoc, Comala, Zapotitlan de Vadillo and Toliman. During the 2005 this <span class="hlt">volcano</span> has had an intense effusive-explosive <span class="hlt">activity</span>, similar to the one that took place during the period of 1890 through 1900. Intense pre-plinian eruption in January 20, 1913, generated little economic losses in the lower parts of the <span class="hlt">volcano</span> due to low population density and low socio-economic <span class="hlt">activities</span> at the time. Shows the updating of the volcanic hazard maps published in 2001, where we identify whit SPOT satellite imagery and Google Earth, change in the land use on the slope of <span class="hlt">volcano</span>, the expansion of the agricultural frontier on the east and southeast sides of the Colima <span class="hlt">volcano</span>, the population inhabiting the area is approximately 517,000 people, and growing at an annual rate of 4.77%, also the region that has shown an increased in the vulnerability for the development of economic <span class="hlt">activities</span>, supported by the construction of highways, natural gas pipelines and electrical infrastructure that connect to the Port of Manzanillo to Guadalajara city. The update the hazard maps are: a) Exclusion areas and moderate hazard for explosive events</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=volcanic+AND+eruption&id=EJ546465','ERIC'); return false;" href="https://eric.ed.gov/?q=volcanic+AND+eruption&id=EJ546465"><span>Geoflicks Reviewed--Films about Hawaiian <span class="hlt">Volcanoes</span>.</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>Bykerk-Kauffman, Ann</p> <p>1994-01-01</p> <p>Reviews 11 films on volcanic eruptions in the United States. Films are given a one- to five-star rating and the film's year, length, source and price are listed. Top films include "Inside Hawaiian <span class="hlt">Volcanoes</span>" and "Kilauea: Close up of an <span class="hlt">Active</span> <span class="hlt">Volcano</span>." (AIM)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70157002','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70157002"><span>Ice-clad <span class="hlt">volcanoes</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>Waitt, Richard B.; Edwards, B.R.; Fountain, Andrew G.; Huggel, C.; Carey, Mark; Clague, John J.; Kääb, Andreas</p> <p>2015-01-01</p> <p>An icy <span class="hlt">volcano</span> even if called extinct or dormant may be <span class="hlt">active</span> at depth. Magma creeps up, crystallizes, releases gas. After decades or millennia the pressure from magmatic gas exceeds the resistance of overlying rock and the <span class="hlt">volcano</span> erupts. Repeated eruptions build a cone that pokes one or two kilometers or more above its surroundings - a point of cool climate supporting glaciers. Ice-clad volcanic peaks ring the northern Pacific and reach south to Chile, New Zealand, and Antarctica. Others punctuate Iceland and Africa (Fig 4.1). To climb is irresistible - if only “because it’s there” in George Mallory’s words. Among the intrepid ascents of icy <span class="hlt">volcanoes</span> we count Alexander von Humboldt’s attempt on 6270-meter Chimborazo in 1802 and Edward Whymper’s success there 78 years later. By then Cotopaxi steamed to the north.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910728C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910728C"><span>Radon surveys and monitoring at <span class="hlt">active</span> <span class="hlt">volcanoes</span>: an open window on deep hydrothermal systems and their dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cigolini, Corrado; Laiolo, Marco; Coppola, Diego</p> <p>2017-04-01</p> <p>The behavior of fluids in hydrothermal systems is critical in <span class="hlt">volcano</span> monitoring and geothermal prospecting. Analyzing the time series of radon emissions on <span class="hlt">active</span> <span class="hlt">volcanoes</span> is strategic for detecting and interpreting precursory signals of changes in volcanic <span class="hlt">activity</span>, eventually leading to eruptions. Radon is a radioactive gas generated from the decay of U bearing rocks, soils and magmas. Although radon has been regarded as a potential precursor of earthquakes, radon anomalies appear to be better suited to forecast volcanic eruptions since we know where paroxysms may occur and we can follow the evolution of volcanic <span class="hlt">activity</span>. Radon mapping at <span class="hlt">active</span> <span class="hlt">volcanoes</span> is also a reliable tool to assess diffuse and concentrated degassing as well as efficiently detecting earthquake-<span class="hlt">volcano</span> interactions. Systematic radon monitoring has been shown to be a key factor for evaluating the rise of volcanic and hydrothermal fluids. In fact, the decay properties of radon, the duration of radon anomalies together with sampling rates may be cross-checked with the chemistry of hydrothermal fluids (and their transport properties) to constrain fluids ascent rates and to infer the permeability and porosity of rocks in sectors surrounding the <span class="hlt">active</span> conduits. We hereby further discuss the data of radon surveys and monitoring at Somma-Vesuvius, Stromboli and La Soufrière (Guadeloupe, Lesser Antilles). The integrated analysis of seismic and geochemical data, including radon emissions, may be successfully used in testing temperature distributions and variations of porosity and permeability in volcanic hydrothermal systems and can be used as a proxy to analyze geothermal reservoirs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18..971B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18..971B"><span>Magmatic sill intrusions beneath El Hierro Island following the 2011-2012 <span class="hlt">submarine</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>Benito-Saz, María Á.; Sigmundsson, Freysteinn; Parks, Michelle M.; García-Cañada, Laura; Domínguez Cerdeña, Itahiza</p> <p>2016-04-01</p> <p>El Hierro, the most southwestern island of Canary Islands, Spain, is a <span class="hlt">volcano</span> rising from around 3600 m above the ocean floor and up to of 1500 m above sea level. A <span class="hlt">submarine</span> eruption occurred off the coast of El Hierro in 2011-2012, which was the only confirmed eruption in the last ~ 600 years. <span class="hlt">Activity</span> continued after the end of the eruption with six magmatic intrusions occurring between 2012-2014. Each of these intrusions was characterized by hundreds of earthquakes and 3-19 centimeters of observed ground deformation. Ground displacements at ten continuous GPS sites were initially inverted to determine the optimal source parameters (location, geometry, volume/pressure change) that best define these intrusions from a geodetic point of view. Each intrusive period appears to be associated with the formation of a separate sill, with inferred volumes between 0.02 - 0.3 km3. SAR images from the Canadian RADARSAT-2 satellite and the Italian Space Agency COSMO-SkyMed constellation have been used to produce high-resolution detailed maps of line-of-sight displacements for each of these intrusions. These data have been combined with the continuous GPS observations and a joint inversion undertaken to gain further constraints on the optimal source parameters for each of these separate intrusive events. The recorded <span class="hlt">activity</span> helps to understand how an oceanic intraplate volcanic island grows through repeated sill intrusions; well documented by seismic, GPS and InSAR observations in the case of the El Hierro <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017LPICo1989.8144O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017LPICo1989.8144O"><span>Titan <span class="hlt">Submarines</span>!</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oleson, S. R.; Lorenz, R. D.; Paul, M. V.; Hartwig, J. W.; Walsh, J. M.</p> <p>2017-02-01</p> <p>A NIAC Phase II <span class="hlt">submarine</span> concept, dubbed 'Titan Turtle' for Saturn's moon Titan's northern sea, Ligea Mare. A design concept including science and operations is described for this -180°C liquid methane sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-sts068-155-094.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-sts068-155-094.html"><span>Eruption of Kliuchevskoi <span class="hlt">volcano</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1994-10-05</p> <p>STS068-155-094 (30 September-11 October 1994) --- (Kliuchevskoi <span class="hlt">Volcano</span>) The crewmembers used a Linhof large format Earth observation camera to photograph this nadir view of the Kamchatka peninsula's week-old <span class="hlt">volcano</span>. The eruption and the follow-up environmental <span class="hlt">activity</span> was photographed from 115 nautical miles above Earth. Six NASA astronauts spent a week and a half aboard the Space Shuttle Endeavour in support of the Space Radar Laboratory 2 (SRL-2) mission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2010/5242/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2010/5242/"><span>2007 Volcanic <span class="hlt">activity</span> in Alaska, Kamchatka, and the Kurile Islands: Summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGimsey, Robert G.; Neal, Christina A.; Dixon, James P.; Malik, Nataliya; Chibisova, Marina</p> <p>2011-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, possible eruptions, and volcanic unrest at or near nine separate volcanic centers in Alaska during 2007. The year was highlighted by the eruption of Pavlof, one of Alaska's most frequently <span class="hlt">active</span> <span class="hlt">volcanoes</span>. Glaciated Fourpeaked Mountain, a <span class="hlt">volcano</span> thought to have been inactive in the Holocene, produced a phreatic eruption in the autumn of 2006 and continued to emit copious amounts of steam and volcanic gas into 2007. Redoubt <span class="hlt">Volcano</span> showed the first signs of the unrest that would unfold in 2008-09. AVO staff also participated in hazard communication and monitoring of multiple eruptions at seven <span class="hlt">volcanoes</span> in Russia as part of its collaborative role in the Kamchatka and Sakhalin Volcanic Eruption Response Teams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www3.epa.gov/radtown/submarines-aircraft-carriers.html','PESTICIDES'); return false;" href="https://www3.epa.gov/radtown/submarines-aircraft-carriers.html"><span>Nuclear <span class="hlt">Submarines</span> and Aircraft Carriers | Radiation ...</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p>2017-08-07</p> <p>Nuclear <span class="hlt">submarines</span> and aircraft carriers are powered by onboard nuclear reactors. Heat from the nuclear reaction makes the steam needed to power the <span class="hlt">submarine</span>. When a nuclear vessel is taken out of service, its radioactive parts are disposed of and monitored.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JVGR..357..186C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JVGR..357..186C"><span><span class="hlt">Volcano</span>-hydrothermal system and <span class="hlt">activity</span> of Sirung <span class="hlt">volcano</span> (Pantar Island, Indonesia)</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; Bernard, Alain; Murphy, Sam; Inguaggiato, Salvatore; Gunawan, Hendra</p> <p>2018-05-01</p> <p>Sirung is a frequently <span class="hlt">active</span> <span class="hlt">volcano</span> located in the remote parts of Western Timor (Indonesia). Sirung has a crater with several hydrothermal features including a crater lake. We present a timeseries of satellite images of the lake and chemical and isotope data from the hyperacid hydrothermal system. The fluids sampled in the crater present the typical features of hyperacidic systems with high TDS, low pH and δ34SHSO4-δ34SS0 among the highest for such lakes. The cations concentrations are predominantly controlled by the precipitation of alunite, jarosite, silica phases, native sulfur and pyrite which dominate the shallow portions of the hydrothermal system. These minerals may control shallow sealing processes thought to trigger phreatic eruptions elsewhere. Sparse Mg/Cl and SO4/Cl ratios and lake parameters derived from satellite images suggest gradual increase in heat and gas flux, most likely SO2-rich, prior to the 2012 phreatic eruption. An acidic river was sampled 8 km far from the crater and is genetically linked with the fluids rising toward the <span class="hlt">active</span> crater. This river would therefore be a relevant target for future remote monitoring purposes. Finally, several wells and springs largely exceeded the World Health Organization toxicity limits in total arsenic and fluoride.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2009/1165/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2009/1165/"><span><span class="hlt">Volcano</span>-Monitoring Instrumentation in the United States, 2008</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Guffanti, Marianne; Diefenbach, Angela K.; Ewert, John W.; Ramsey, David W.; Cervelli, Peter F.; Schilling, Steven P.</p> <p>2010-01-01</p> <p>The United States is one of the most volcanically <span class="hlt">active</span> countries in the world. According to the global volcanism database of the Smithsonian Institution, the United States (including its Commonwealth of the Northern Mariana Islands) is home to about 170 <span class="hlt">volcanoes</span> that are in an eruptive phase, have erupted in historical time, or have not erupted recently but are young enough (eruptions within the past 10,000 years) to be capable of reawakening. From 1980 through 2008, 30 of these <span class="hlt">volcanoes</span> erupted, several repeatedly. <span class="hlt">Volcano</span> monitoring in the United States is carried out by the U.S. Geological Survey (USGS) <span class="hlt">Volcano</span> Hazards Program, which operates a system of five <span class="hlt">volcano</span> observatories-Alaska <span class="hlt">Volcano</span> Observatory (AVO), Cascades <span class="hlt">Volcano</span> Observatory (CVO), Hawaiian <span class="hlt">Volcano</span> Observatory (HVO), Long Valley Observatory (LVO), and Yellowstone <span class="hlt">Volcano</span> Observatory (YVO). The observatories issue public alerts about conditions and hazards at U.S. <span class="hlt">volcanoes</span> in support of the USGS mandate under P.L. 93-288 (Stafford Act) to provide timely warnings of potential volcanic disasters to the affected populace and civil authorities. To make efficient use of the Nation's scientific resources, the <span class="hlt">volcano</span> observatories operate in partnership with universities and other governmental agencies through various formal agreements. The Consortium of U.S. <span class="hlt">Volcano</span> Observatories (CUSVO) was established in 2001 to promote scientific cooperation among the Federal, academic, and State agencies involved in observatory operations. Other groups also contribute to <span class="hlt">volcano</span> monitoring by sponsoring long-term installation of geophysical instruments at some <span class="hlt">volcanoes</span> for specific research projects. This report describes a database of information about permanently installed ground-based instruments used by the U.S. <span class="hlt">volcano</span> observatories to monitor volcanic <span class="hlt">activity</span> (unrest and eruptions). The purposes of this <span class="hlt">Volcano</span>-Monitoring Instrumentation Database (VMID) are to (1) document the Nation's existing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V51E2735J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V51E2735J"><span><span class="hlt">Volcano</span>-tectonic interactions at Sabancaya and other Peruvian <span class="hlt">volcanoes</span> revealed by InSAR and seismicity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jay, J.; Pritchard, M. E.; Aron, F.; Delgado, F.; Macedo, O.; Aguilar, V.</p> <p>2013-12-01</p> <p>An InSAR survey of all 13 Holocene <span class="hlt">volcanoes</span> in the Andean Central Volcanic Zone of Peru reveals previously undocumented surface deformation that is occasionally accompanied by seismic <span class="hlt">activity</span>. Our survey utilizes SAR data spanning from 1992 to the present from the ERS-1, ERS-2, and Envisat satellites, as well as selected data from the TerraSAR-X satellite. We find that the recent unrest at Sabancaya <span class="hlt">volcano</span> (heightened seismicity since 22 February 2013 and increased fumarolic output) has been accompanied by surface deformation. We also find two distinct deformation episodes near Sabancaya that are likely associated with an earthquake swarm in February 2013 and a M6 normal fault earthquake that occurred on 17 July 2013. Preliminary modeling suggests that faulting from the observed seismic moment can account for nearly all of the observed deformation and thus we have not yet found clear evidence for recent magma intrusion. We also document an earlier episode of deformation that occurred between December 2002 and September 2003 which may be associated with a M5.3 earthquake that occurred on 13 December 2002 on the Solarpampa fault, a large EW-striking normal fault located about 25 km northwest of Sabancaya <span class="hlt">volcano</span>. All of the deformation episodes between 2002 and 2013 are spatially distinct from the inflation seen near Sabancaya from 1992 to 1997. In addition to the <span class="hlt">activity</span> at Sabancaya, we also observe deformation near Coropuna <span class="hlt">volcano</span>, in the Andagua Valley, and in the region between Ticsani and Tutupaca <span class="hlt">volcanoes</span>. InSAR images reveal surface deformation that is possibly related to an earthquake swarm near Coropuna and Sabancaya <span class="hlt">volcanoes</span> in December 2001. We also find persistent deformation in the scoria cone and lava field along the Andagua Valley, located 40 km east of Corpuna. An earthquake swarm near Ticsani <span class="hlt">volcano</span> in 2005 produced surface deformation centered northwest of the <span class="hlt">volcano</span> and was accompanied by a north-south elongated subsidence signal to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gip/76/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gip/76/"><span>Hawaiian <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Venezky, Dina Y.; Orr, Tim R.</p> <p>2008-01-01</p> <p>Lava from Kilauea <span class="hlt">volcano</span> flowing through a forest in the Royal Gardens subdivision, Hawai'i, in February 2008. The Hawaiian <span class="hlt">Volcano</span> Observatory (HVO) monitors the <span class="hlt">volcanoes</span> of Hawai'i and is located within Hawaiian <span class="hlt">Volcanoes</span> National Park. HVO is one of five USGS <span class="hlt">Volcano</span> Hazards Program observatories that monitor U.S. <span class="hlt">volcanoes</span> for science and public safety. Learn more about Kilauea and HVO at http://hvo.wr.usgs.gov.</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('https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034449p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034449p/"><span>29. VIEW OF <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK DURING CONSTRUCTION AT ...</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>29. VIEW OF <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK DURING CONSTRUCTION AT POINT JUST ABOVE THE <span class="hlt">SUBMARINE</span> SECTION AT THE 110-FOOT LEVEL 1929-1930 - U.S. Naval <span class="hlt">Submarine</span> Base, New London <span class="hlt">Submarine</span> Escape Training Tank, Albacore & Darter Roads, Groton, New London County, CT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41C1993M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41C1993M"><span>Waveform Template Matching and Analysis of Hydroacoustic Events from the April-May 2015 Eruption of Axial <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mann, M. E.; Bohnenstiehl, D. R.; Weis, J.</p> <p>2016-12-01</p> <p>The <span class="hlt">submarine</span> emplacement of new lava flows during the 2015 eruption of Axial <span class="hlt">Volcano</span> generated a series of impulsive acoustic signals that were captured by seismic and hydrophone sensors deployed as part of the Ocean Observatories Initiative cabled array network. A catalog of >37,000 explosions was created using a four-channel waveform matching routine using 800 template arrivals. Most of the explosions are sourced from a set of lava mounds erupted along the <span class="hlt">volcano</span>'s northern rift; however, a subset of 400 explosions are located within the caldera and track the flow of lava from a vent near its eastern rim. The earliest explosion occurs at 08:00 UTC on April 24, approximately four hours after the seismicity rate began to increase and two hours after bottom pressure recorders indicate the caldera floor began to subside. Between April 24 and 28 event rates are sustained at 1000/day. The rate then decreases gradually with explosive <span class="hlt">activity</span> ending on 21 May, coincident with the initial re-inflation of the caldera. The windowed coefficient of variation of the inter-event time is approximately 1 throughout the eruption, consistent with a random process. The size-frequency distribution shows a bimodal pattern, with the loudest explosions, having received levels up to 157 dB re 1 micro-Pa, being produced during the first few hours of the eruption.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016BVol...78...39C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016BVol...78...39C"><span>Monitoring crater-wall collapse at <span class="hlt">active</span> <span class="hlt">volcanoes</span>: a study of the 12 January 2013 event at Stromboli</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calvari, Sonia; Intrieri, Emanuele; Di Traglia, Federico; Bonaccorso, Alessandro; Casagli, Nicola; Cristaldi, Antonio</p> <p>2016-05-01</p> <p>Crater-wall collapses are fairly frequent at <span class="hlt">active</span> <span class="hlt">volcanoes</span> and they are normally studied through the analysis of their deposits. In this paper, we present an analysis of the 12 January 2013 crater-wall collapse occurring at Stromboli <span class="hlt">volcano</span>, investigated by means of a monitoring network comprising visible and infrared webcams and a Ground-Based Interferometric Synthetic Aperture Radar. The network revealed the triggering mechanisms of the collapse, which are comparable to the events that heralded the previous effusive eruptions in 1985, 2002, 2007 and 2014. The collapse occurred during a period of inflation of the summit cone and was preceded by increasing explosive <span class="hlt">activity</span> and the enlargement of the crater. Weakness of the crater wall, increasing magmastatic pressure within the upper conduit induced by ascending magma and mechanical erosion caused by vent opening at the base of the crater wall and by lava fingering, are considered responsible for triggering the collapse on 12 January 2013 at Stromboli. We suggest that the combination of these factors might be a general mechanism to generate crater-wall collapse at <span class="hlt">active</span> <span class="hlt">volcanoes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2017/5104/sir20175104.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2017/5104/sir20175104.pdf"><span>2015 Volcanic <span class="hlt">activity</span> in Alaska—Summary of events and response of the Alaska <span class="hlt">Volcano</span> Observatory</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dixon, James P.; Cameron, Cheryl E.; Iezzi, Alexandra M.; Wallace, Kristi</p> <p>2017-09-28</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO) responded to eruptions, volcanic unrest or suspected unrest, and seismic events at 14 volcanic centers in Alaska during 2015. The most notable volcanic <span class="hlt">activity</span> consisted of continuing intermittent ash eruptions from Cleveland and Shishaldin <span class="hlt">volcanoes</span> in the Aleutian Islands. Two eruptive episodes, at Veniaminof and Pavlof, on the Alaska Peninsula ended in 2015. During 2015, AVO re-established the seismograph network at Aniakchak, installed six new broadband seismometers throughout the Aleutian Islands, and added a Multiple component Gas Analyzer System (MultiGAS) station on Augustine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA13827.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA13827.html"><span>NASA Spacecraft Captures Fury of Russian <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2011-01-27</p> <p>This nighttime thermal infrared image from NASA Terra spacecraft shows Shiveluch <span class="hlt">volcano</span>, one of the largest and most <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Russia Kamchatka Peninsula; the bright, hot summit lava dome is evident in the center of the image.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA16943.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA16943.html"><span>UAVSAR Acquires False-Color Image of Galeras <span class="hlt">Volcano</span>, Colombia</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2013-04-03</p> <p>This false-color image of Colombia Galeras <span class="hlt">Volcano</span>, was acquired by UAVSAR on March 13, 2013. A highly <span class="hlt">active</span> <span class="hlt">volcano</span>, Galeras features a breached caldera and an <span class="hlt">active</span> cone that produces numerous small to moderate explosive eruptions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010045081&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010045081&hterms=active+volcanoes&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dactive%2Bvolcanoes"><span>Interpreting Low Spatial Resolution Thermal Data from <span class="hlt">Active</span> <span class="hlt">Volcanoes</span> on Io and the Earth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Keszthelyi, L.; Harris, A. J. L.; Flynn, L.; Davies, A. G.; McEwen, A.</p> <p>2001-01-01</p> <p>The style of volcanism was successfully determined at a number of <span class="hlt">active</span> <span class="hlt">volcanoes</span> on Io and the Earth using the same techniques to interpret thermal remote sensing data. Additional information is contained in the original extended abstract.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA....11276P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA....11276P"><span>Variations of seismic parameters during different <span class="hlt">activity</span> levels of the Soufriere Hills <span class="hlt">Volcano</span>, Montserrat</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Powell, T.; Neuberg, J.</p> <p>2003-04-01</p> <p>The low-frequency seismic events on Montserrat are linked to conduit resonance and the pressurisation of the volcanic system. Analysis of these events tell us more about the behaviour of the volcanic system and provide a monitoring and interpretation tool. We have written an Automated Event Classification Algorithm Program (AECAP), which finds and classifies seismic events and calculates seismic parameters such as energy, intermittency, peak frequency and event duration. Comparison of low-frequency energy with the tilt cycles in 1997 allows us to link pressurisation of the <span class="hlt">volcano</span> with seismic behaviour. An empirical relationship provides us with an estimate of pressurisation through released seismic energy. During 1997, the <span class="hlt">activity</span> of the <span class="hlt">volcano</span> varied considerably. We compare seismic parameters from quiet periods to those from <span class="hlt">active</span> periods and investigate how the relationships between these parameters change. These changes are then used to constrain models of magmatic processes during different stages of volcanic <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title32-vol5/pdf/CFR-2010-title32-vol5-sec707-7.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title32-vol5/pdf/CFR-2010-title32-vol5-sec707-7.pdf"><span>32 CFR 707.7 - <span class="hlt">Submarine</span> identification light.</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>2010-07-01</p> <p>... RULES WITH RESPECT TO ADDITIONAL STATION AND SIGNAL LIGHTS § 707.7 <span class="hlt">Submarine</span> identification light. <span class="hlt">Submarines</span> may display, as a distinctive means of identification, an intermittent flashing amber beacon with...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800039554&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800039554&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dactive%2Bvolcanoes"><span>The chronology of the martian <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Plescia, J. B.; Saunders, R. S.</p> <p>1979-01-01</p> <p>The <span class="hlt">volcanoes</span> of Mars have been divided into three groups based on morphology: basaltic shields, domes and composite cones, and highland patera. A fourth group can be added to include the <span class="hlt">volcano</span>-tectonic depressions. Using crater counts and the absolute chronology of Soderblom, an attempt is made to estimate the history of the <span class="hlt">volcanoes</span>. Early in the martian history, about 2.5 b.y. ago, all three styles of <span class="hlt">volcanoes</span> were <span class="hlt">active</span> at various locations on the surface. At approximately 1.7-1.8 b.y. ago a transition occurred in the style and loci of volcanic construction. <span class="hlt">Volcanoes</span> of younger age appear to be only of the basaltic shield group and are restricted to the Tharsis region. This same transition was noted by a change in the style of the basaltic shield group. Older shields were small low features, while the younger shields are significantly broader and taller.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034452p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034452p/"><span>32. VIEW OF PHOTO CAPTIONED '<span class="hlt">SUBMARINE</span> BASE, NEW LONDON, CONN. ...</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>32. VIEW OF PHOTO CAPTIONED '<span class="hlt">SUBMARINE</span> BASE, NEW LONDON, CONN. OCTOBER 3, 1932. COMPLETION OF ERECTION OF STEELWORK FOR ELEVATOR. LOOKING NORTH. CONTRACT NO. Y-1539-ELEVATOR, <span class="hlt">SUBMARINE</span> ESCAPE TANK.' - U.S. Naval <span class="hlt">Submarine</span> Base, New London <span class="hlt">Submarine</span> Escape Training Tank, Albacore & Darter Roads, Groton, New London County, CT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940016219&hterms=active+shield&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dactive%2Bshield','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940016219&hterms=active+shield&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dactive%2Bshield"><span>Eruption history of the Tharsis shield <span class="hlt">volcanoes</span>, Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Plescia, J. B.</p> <p>1993-01-01</p> <p>The Tharsis Montes <span class="hlt">volcanoes</span> and Olympus Mons are giant shield <span class="hlt">volcanoes</span>. Although estimates of their average surface age have been made using crater counts, the length of time required to build the shields has not been considered. Crater counts for the <span class="hlt">volcanoes</span> indicate the constructs are young; average ages are Amazonian to Hesperian. In relative terms; Arsia Mons is the oldest, Pavonis Mons intermediate, and Ascreaus Mons the youngest of the Tharsis Montes shield; Olympus Mons is the youngest of the group. Depending upon the calibration, absolute ages range from 730 Ma to 3100 Ma for Arsia Mons and 25 Ma to 100 Ma for Olympus Mons. These absolute chronologies are highly model dependent, and indicate only the time surficial volcanism ceased, not the time over which the <span class="hlt">volcano</span> was built. The problem of estimating the time necessary to build the <span class="hlt">volcanoes</span> can be attacked in two ways. First, eruption rates from terrestrial and extraterrestrial examples can be used to calculate the required period of time to build the shields. Second, some relation of eruptive <span class="hlt">activity</span> between the <span class="hlt">volcanoes</span> can be assumed, such as they all began at a speficic time or they were <span class="hlt">active</span> sequentially, and calculate the eruptive rate. Volumes of the shield <span class="hlt">volcanoes</span> were derived from topographic/volume data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BVol...75..706W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BVol...75..706W"><span>Review of eruptive <span class="hlt">activity</span> at Tianchi <span class="hlt">volcano</span>, Changbaishan, northeast China: implications for possible future eruptions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wei, Haiquan; Liu, Guoming; Gill, James</p> <p>2013-04-01</p> <p>One of the largest explosive eruptions in the past several thousand years occurred at Tianchi <span class="hlt">volcano</span>, also known as Changbaishan, on the China-North Korea border. This historically <span class="hlt">active</span> polygenetic central <span class="hlt">volcano</span> consists of three parts: a lower basaltic shield, an upper trachytic composite cone, and young comendite ash flows. The Millennium Eruption occurred between 938 and 946 ad, and was preceded by two smaller and chemically different rhyolitic pumice deposits. There has been at least one additional, small eruption in the last three centuries. From 2002 to 2005, seismicity, deformation, and the helium and hydrogen gas contents of spring waters all increased markedly, causing regional concern. We attribute this event to magma recharge or volatile exhalation or both at depth, followed by two episodes of addition of magmatic fluids into the overlying aquifer without a phreatic eruption. The estimated present magma accumulation rate is too low by itself to account for the 2002-2005 unrest. The most serious volcanic hazards are ash eruption and flows, and lahars. The available geological information and <span class="hlt">volcano</span> monitoring data provide a baseline for comprehensive assessment of future episodes of unrest and possible eruptive <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V13C0398G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V13C0398G"><span>The First Historical Eruption of Kambalny <span class="hlt">Volcano</span> in 2017 .</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gordeev, E.</p> <p>2017-12-01</p> <p>The first historical eruption at Kambalny <span class="hlt">volcano</span> began about 21:20 UTC on March 24, 2017 with powerful ash emissions up to 6 km above sea level from the pre-summit crater. According to tephrochronological data, it is assumed that the strong eruptions of the <span class="hlt">volcano</span> occurred 200 (?) and 600 years ago. KVERT (Kamchatka Volcanic Eruption Response Team) of the Institute of Volcanology and Seismology FEB RAS has been monitoring Kambalny <span class="hlt">volcano</span> since 2002. KVERT worked closely with AMC Elizovo and Tokyo VAAC during the eruption at Kambalny <span class="hlt">volcano</span> in 2017. The maximum intensity of ash emissions occurred on 25-26 March: a continuous plume laden with ash particles spread over several thousand kilometers, changing the direction of propagation from the <span class="hlt">volcano</span> from the south-west to the south and south-east. On 27-29 March, the ash plume extended to the west, on 30 March - to the southeast of the <span class="hlt">volcano</span>. On March 31 and April 01, the <span class="hlt">volcano</span> was relatively quiet. The resumption of the <span class="hlt">volcano</span> <span class="hlt">activity</span> after two days of rest was expressed in powerful ash emissions up to 7 km above sea level. Gas-steam plumes containing some amount of ash were noted on 02-05 April, and powerful ash emissions up to 7 km above sea level occurred on 09 April. The explosive <span class="hlt">activity</span> at the <span class="hlt">volcano</span> ended on 11 April. The area of ash deposits was about 1500 km2, the total area covered by ash falls, for example, on 25 March, was about 650 thousand km2. To monitor and study the Kambalny <span class="hlt">volcano</span> eruption we mainly used satellite images of medium resolution available in the information system "Monitoring volcanic <span class="hlt">activity</span> in Kamchatka and Kurile Islands" (VolSatView). This work was supported by the Russian Science Foundation, project No. 16-17-00042.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6660099-noble-gases-submarine-pillow-basalt-glasses-from-loihi-kilauea-hawaii-solar-component-earth','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6660099-noble-gases-submarine-pillow-basalt-glasses-from-loihi-kilauea-hawaii-solar-component-earth"><span>Noble gases in <span class="hlt">submarine</span> pillow basalt glasses from Loihi and Kilauea, Hawaii: A solar component in the Earth</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>Honda, M.; McDougall, I.; Patterson, D.B.</p> <p>1993-02-01</p> <p>Noble gas elemental and isotopic abundances have been analysed in twenty-two samples of basaltic glass dredged from the <span class="hlt">submarine</span> flanks of two currently <span class="hlt">active</span> Hawaiian <span class="hlt">volcanoes</span>, Loihi Seamount and Kilauea. Neon isotopic ratios are enriched in [sup 20]Ne and [sup 21]Ne by as much as 16% with respect to atmospheric ratios. All the Hawaiian basalt glass samples show relatively high [sup 3]He/[sup 4]He ratios. The high [sup 20]Ne/[sup 22]Ne values in some of the Hawaiian samples, together with correlations between neon and helium systematics, suggest the presence of a solar component in the source regions of the Hawaiian mantle plume.more » The solar hypothesis for the Earth's primordial noble gas composition can account for helium and neon isotopic ratios observed in basaltic glasses from both plume and spreading systems, in fluids in continental hydrothermal systems, in CO[sub 2] well gases, and in ancient diamonds. These results provide new insights into the origin and evolution of the Earth's atmosphere.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH31A0204P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH31A0204P"><span>Unmanned Aerial Technologies for Observations at <span class="hlt">Active</span> <span class="hlt">Volcanoes</span>: Advances and Prospects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pieri, D. C.; Diaz, J. A.; Bland, G.; Fladeland, M.; Makel, D.; Schwandner, F. M.; Buongiorno, M. F.; Elston, J. S.</p> <p>2017-12-01</p> <p>Modern application of unmanned aerial systems' (UASs) technology allow us to conduct in situ measurements in volcanic plumes and drifting volcanic clouds that were impossible to make in the past. Thus, we are now able to explore proximal airspace near and within eruption columns and or other <span class="hlt">active</span> vents, at very high and at very low altitudes—risk to human investigators is vastly reduced (although not eliminated). We are now on the cusp of being able to make in situ measurements and conduct sampling at altitudes of 5000-6000 meters relatively routinely. We also are developing heat tolerant electronics and sensors that will deployed on, around, and over <span class="hlt">active</span> lava lakes and lava flows at terrestrial <span class="hlt">volcanoes</span>, but with a view toward developing planetary applications, for instance on the surface of Venus. We report on our 2012-present systematic UAS-based observations of light gases (e.g., SO2 CO2, H2S) at Turrialba <span class="hlt">Volcano</span> in Costa Rica, at Italian volcanic sites (e.g., Isole Vulcano; La Solfatara), and most recently at Kilauea <span class="hlt">Volcano</span>, Hawaii in collaboration with USGS and NPS colleagues. Other deployments for Fall 2017 and Winter 2018 are in planning stages for the Salton Sea Basin and Costa Rica, which will include an airborne miniature mass spectrometer onboard several different types of UAVs. In addition, under development is the first purpose-built-for-volcanology small unmanned aircraft. We discuss strategies for acquiring airborne data from proximal ash/gas plumes during restless periods and during eruptions, from distal drifting ash/gas clouds from eruptions, and from diffuse emissions (e.g., CO2) at very low altitudes, utilizing UASs (e.g., fixed wing, multi-rotor, aerostat), especially regarding inputs for source flux reverse models. This work was carried out, in part, at the Jet Propulsion Laboratory of the California Institute of Technology under contract to NASA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title32-vol5/pdf/CFR-2011-title32-vol5-sec700-1058.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title32-vol5/pdf/CFR-2011-title32-vol5-sec700-1058.pdf"><span>32 CFR 700.1058 - Command of a <span class="hlt">submarine</span>.</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>2011-07-01</p> <p>... 32 National Defense 5 2011-07-01 2011-07-01 false Command of a <span class="hlt">submarine</span>. 700.1058 Section 700... Command Detail to Duty § 700.1058 Command of a <span class="hlt">submarine</span>. The officer detailed to command a <span class="hlt">submarine</span> shall be an officer of the line in the Navy, eligible for command at sea and qualified for command of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title32-vol5/pdf/CFR-2010-title32-vol5-sec700-1058.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title32-vol5/pdf/CFR-2010-title32-vol5-sec700-1058.pdf"><span>32 CFR 700.1058 - Command of a <span class="hlt">submarine</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>2010-07-01</p> <p>... 32 National Defense 5 2010-07-01 2010-07-01 false Command of a <span class="hlt">submarine</span>. 700.1058 Section 700... Command Detail to Duty § 700.1058 Command of a <span class="hlt">submarine</span>. The officer detailed to command a <span class="hlt">submarine</span> shall be an officer of the line in the Navy, eligible for command at sea and qualified for command of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title32-vol5/pdf/CFR-2012-title32-vol5-sec700-1058.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title32-vol5/pdf/CFR-2012-title32-vol5-sec700-1058.pdf"><span>32 CFR 700.1058 - Command of a <span class="hlt">submarine</span>.</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>2012-07-01</p> <p>... 32 National Defense 5 2012-07-01 2012-07-01 false Command of a <span class="hlt">submarine</span>. 700.1058 Section 700... Command Detail to Duty § 700.1058 Command of a <span class="hlt">submarine</span>. The officer detailed to command a <span class="hlt">submarine</span> shall be an officer of the line in the Navy, eligible for command at sea and qualified for command of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title32-vol5/pdf/CFR-2014-title32-vol5-sec700-1058.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title32-vol5/pdf/CFR-2014-title32-vol5-sec700-1058.pdf"><span>32 CFR 700.1058 - Command of a <span class="hlt">submarine</span>.</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>2014-07-01</p> <p>... 32 National Defense 5 2014-07-01 2014-07-01 false Command of a <span class="hlt">submarine</span>. 700.1058 Section 700... Command Detail to Duty § 700.1058 Command of a <span class="hlt">submarine</span>. The officer detailed to command a <span class="hlt">submarine</span> shall be an officer of the line in the Navy, eligible for command at sea and qualified for command of...</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://www.gpo.gov/fdsys/pkg/CFR-2013-title32-vol5/pdf/CFR-2013-title32-vol5-sec700-1058.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title32-vol5/pdf/CFR-2013-title32-vol5-sec700-1058.pdf"><span>32 CFR 700.1058 - Command of a <span class="hlt">submarine</span>.</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>2013-07-01</p> <p>... 32 National Defense 5 2013-07-01 2013-07-01 false Command of a <span class="hlt">submarine</span>. 700.1058 Section 700... Command Detail to Duty § 700.1058 Command of a <span class="hlt">submarine</span>. The officer detailed to command a <span class="hlt">submarine</span> shall be an officer of the line in the Navy, eligible for command at sea and qualified for command of...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA18067.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA18067.html"><span>Nighttime Look at Ambrym <span class="hlt">Volcano</span>, Vanuatu by NASA Spacecraft</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2014-02-12</p> <p>Ambrym <span class="hlt">volcano</span> in Vanuatu is one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the world. A large summit caldera contains two <span class="hlt">active</span> vent complexes, Marum and Benbow is seen in this February 12, 2014 nighttime thermal infrared image from NASA Terra spacecraft.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2001/0432/pdf/of2001-0432.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2001/0432/pdf/of2001-0432.pdf"><span>Lahar hazards at Agua <span class="hlt">volcano</span>, Guatemala</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Schilling, S.P.; Vallance, J.W.; Matías, O.; Howell, M.M.</p> <p>2001-01-01</p> <p>At 3760 m, Agua <span class="hlt">volcano</span> towers more than 3500 m above the Pacific coastal plain to the south and 2000 m above the Guatemalan highlands to the north. The <span class="hlt">volcano</span> is within 5 to 10 kilometers (km) of Antigua, Guatemala and several other large towns situated on its northern apron. These towns have a combined population of nearly 100,000. It is within about 20 km of Escuintla (population, ca. 100,000) to the south. Though the <span class="hlt">volcano</span> has not been <span class="hlt">active</span> in historical time, or about the last 500 years, it has the potential to produce debris flows (watery flows of mud, rock, and debris—also known as lahars when they occur on a <span class="hlt">volcano</span>) that could inundate these nearby populated areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eosweb.larc.nasa.gov/project/misr/gallery/nicaraguan_volcanoes','SCIGOV-ASDC'); return false;" href="https://eosweb.larc.nasa.gov/project/misr/gallery/nicaraguan_volcanoes"><span>Nicaraguan <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://eosweb.larc.nasa.gov/">Atmospheric Science Data Center </a></p> <p></p> <p>2013-04-18</p> <p>article title:  Nicaraguan <span class="hlt">Volcanoes</span>     View Larger Image Nicaraguan <span class="hlt">volcanoes</span>, February 26, 2000 . The true-color image at left is a ... February 26, 2000 - Plumes from the San Cristobal and Masaya <span class="hlt">volcanoes</span>. project:  MISR category:  gallery ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005vag..book.....L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005vag..book.....L"><span>The <span class="hlt">Volcano</span> Adventure Guide</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lopes, Rosaly</p> <p>2005-02-01</p> <p>This guide contains vital information for anyone wishing to visit, explore, and photograph <span class="hlt">active</span> <span class="hlt">volcanoes</span> safely and enjoyably. Following an introduction that discusses eruption styles of different types of <span class="hlt">volcanoes</span> and how to prepare for an exploratory trip that avoids volcanic dangers, the book presents guidelines to visiting 42 different <span class="hlt">volcanoes</span> around the world. It is filled with practical information that includes tour itineraries, maps, transportation details, and warnings of possible non-volcanic dangers. Three appendices direct the reader to a wealth of further <span class="hlt">volcano</span> resources in a volume that will fascinate amateur enthusiasts and professional volcanologists alike. Rosaly Lopes is a planetary geology and volcanology specialist at the NASA Jet Propulsion Laboratory in California. In addition to her curatorial and research work, she has lectured extensively in England and Brazil and written numerous popular science articles. She received a Latinas in Science Award from the Comision Feminil Mexicana Nacional in 1991 and since 1992, has been a co-organizer of the United Nations/European Space Agency/The Planetary Society yearly conferences on Basic Science for the Benefit of Developing Countries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993JVGR...56..319T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993JVGR...56..319T"><span>Eruption mechanism as inferred from geomagnetic changes with special attention to the 1989 1990 <span class="hlt">activity</span> of Aso <span class="hlt">volcano</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tanaka, Yoshikazu</p> <p>1993-06-01</p> <p>Geomagnetic changes associated with the volcanic <span class="hlt">activity</span> of Aso <span class="hlt">volcano</span> were detected with a dense network of continuously recording proton-precession magnetometers during the period from June 1989 to June 1990. Magnetic date clearly indicate that changes in the magnetization within the <span class="hlt">volcano</span> are most probably caused by temperature changes. This <span class="hlt">activity</span> can be divided into five stages, which are characterized by magnetization and demagnetization of the <span class="hlt">volcano</span>. These magnetic changes with durations of a few months are definitely correlated with some typical volcanic events at the crater as well as the volcanic tremor <span class="hlt">activity</span>. The demagnetization stage appears when the vent is covered by a water pool or the volcanic <span class="hlt">activity</span> is enhanced. The magnetization stage follows the opening of a vent and several large explosions which make the vent permeable. The source of magnetic changes lies at a depth of about 200 m below the crater rim in the southwestern part of the <span class="hlt">active</span> crater. Magnetic moments responsible for observed magnetic changes at stages 1, 2 and 4 are 3.4, -5.2 and -2.2 Wbm, respectively. The corresponding source volume is estimated as a single sphere of radius 40-50 m or a spherical shell of 100 m or so. An effective mechanism of rapid heating/cooling exists, which is ascribed to the interaction of groundwater and superheated vapor, i.e., a shallow hydrothermal system. This hydrothermal system driven by the surface cap of the vent, controls every feature of the eruptions at the final outlet of Aso <span class="hlt">volcano</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17369343','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17369343"><span>Diversity and abundance of aerobic and anaerobic methane oxidizers at the Haakon Mosby Mud <span class="hlt">Volcano</span>, Barents Sea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lösekann, Tina; Knittel, Katrin; Nadalig, Thierry; Fuchs, Bernhard; Niemann, Helge; Boetius, Antje; Amann, Rudolf</p> <p>2007-05-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> are formed by expulsions of mud, fluids, and gases from deeply buried subsurface sources. They are highly reduced benthic habitats and often associated with intensive methane seepage. In this study, the microbial diversity and community structure in methane-rich sediments of the Haakon Mosby Mud <span class="hlt">Volcano</span> (HMMV) were investigated by comparative sequence analysis of 16S rRNA genes and fluorescence in situ hybridization. In the <span class="hlt">active</span> <span class="hlt">volcano</span> center, which has a diameter of about 500 m, the main methane-consuming process was bacterial aerobic oxidation. In this zone, aerobic methanotrophs belonging to three bacterial clades closely affiliated with Methylobacter and Methylophaga species accounted for 56%+/-8% of total cells. In sediments below Beggiatoa mats encircling the center of the HMMV, methanotrophic archaea of the ANME-3 clade dominated the zone of anaerobic methane oxidation. ANME-3 archaea form cell aggregates mostly associated with sulfate-reducing bacteria of the Desulfobulbus (DBB) branch. These ANME-3/DBB aggregates were highly abundant and accounted for up to 94%+/-2% of total microbial biomass at 2 to 3 cm below the surface. ANME-3/DBB aggregates could be further enriched by flow cytometry to identify their phylogenetic relationships. At the outer rim of the mud <span class="hlt">volcano</span>, the seafloor was colonized by tubeworms (Siboglinidae, formerly known as Pogonophora). Here, both aerobic and anaerobic methane oxidizers were found, however, in lower abundances. The level of microbial diversity at this site was higher than that at the central and Beggiatoa species-covered part of the HMMV. Analysis of methyl-coenzyme M-reductase alpha subunit (mcrA) genes showed a strong dominance of a novel lineage, mcrA group f, which could be assigned to ANME-3 archaea. Our results further support the hypothesis of Niemann et al. (54), that high methane availability and different fluid flow regimens at the HMMV provide distinct niches for aerobic and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1907091','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1907091"><span>Diversity and Abundance of Aerobic and Anaerobic Methane Oxidizers at the Haakon Mosby Mud <span class="hlt">Volcano</span>, Barents Sea▿</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lösekann, Tina; Knittel, Katrin; Nadalig, Thierry; Fuchs, Bernhard; Niemann, Helge; Boetius, Antje; Amann, Rudolf</p> <p>2007-01-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanoes</span> are formed by expulsions of mud, fluids, and gases from deeply buried subsurface sources. They are highly reduced benthic habitats and often associated with intensive methane seepage. In this study, the microbial diversity and community structure in methane-rich sediments of the Haakon Mosby Mud <span class="hlt">Volcano</span> (HMMV) were investigated by comparative sequence analysis of 16S rRNA genes and fluorescence in situ hybridization. In the <span class="hlt">active</span> <span class="hlt">volcano</span> center, which has a diameter of about 500 m, the main methane-consuming process was bacterial aerobic oxidation. In this zone, aerobic methanotrophs belonging to three bacterial clades closely affiliated with Methylobacter and Methylophaga species accounted for 56% ± 8% of total cells. In sediments below Beggiatoa mats encircling the center of the HMMV, methanotrophic archaea of the ANME-3 clade dominated the zone of anaerobic methane oxidation. ANME-3 archaea form cell aggregates mostly associated with sulfate-reducing bacteria of the Desulfobulbus (DBB) branch. These ANME-3/DBB aggregates were highly abundant and accounted for up to 94% ± 2% of total microbial biomass at 2 to 3 cm below the surface. ANME-3/DBB aggregates could be further enriched by flow cytometry to identify their phylogenetic relationships. At the outer rim of the mud <span class="hlt">volcano</span>, the seafloor was colonized by tubeworms (Siboglinidae, formerly known as Pogonophora). Here, both aerobic and anaerobic methane oxidizers were found, however, in lower abundances. The level of microbial diversity at this site was higher than that at the central and Beggiatoa species-covered part of the HMMV. Analysis of methyl-coenzyme M-reductase alpha subunit (mcrA) genes showed a strong dominance of a novel lineage, mcrA group f, which could be assigned to ANME-3 archaea. Our results further support the hypothesis of Niemann et al. (54), that high methane availability and different fluid flow regimens at the HMMV provide distinct niches for aerobic and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4344412','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4344412"><span>Banning Cigarette Smoking on US Navy <span class="hlt">Submarines</span>: A Case 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>Lando, Harry A.; Michaud, Mark. E.; Poston, Walker S.C.; Jahnke, Sara A.; Williams, Larry; Haddock, Christopher K.</p> <p>2014-01-01</p> <p>Background The military has had a long pro-tobacco tradition. Despite official policy discouraging smoking, tobacco still is widely seen as part of military culture. While <span class="hlt">active</span> smoking has presented a particular challenge for the military, in recent years there also has been increasing concern with secondhand smoke. This is especially true in closed environments and <span class="hlt">submarines</span> may be deployed for months at a time. The current case study describes the successful implementation by the Navy of a comprehensive ban on smoking aboard <span class="hlt">submarines</span>. Methods The authors searched documents on the Internet, popular media, military-based news outlets, and the scientific literature. We also conducted interviews with Navy officers who were instrumental in policy implementation. Findings Data demonstrating substantial exposure of nonsmokers to tobacco smoke aboard <span class="hlt">submarines</span> had major impact on successful adoption of the policy. A systematic and extended roll out of the ban included establishing a working group, soliciting input and <span class="hlt">active</span> engagement from <span class="hlt">submarine</span> personnel, and offering cessation assistance. Support was enlisted from Chief Petty Officers who could have been strongly opposed but who became strong proponents. Fewer problems were encountered than had been expected. In contrast to a previous unsuccessful attempt by a Navy captain to ban smoking on his ship, the ban was adopted without apparent tobacco industry interference. Conclusions Lessons learned included the importance of strong empirical support, effective framing of the issue, setting a realistic timeline, soliciting support from key personnel, and providing appropriate resources. These lessons have implications for those considering further tobacco policy changes in the military and elsewhere. PMID:25163466</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2101G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2101G"><span>Kamchatka and North Kurile <span class="hlt">Volcano</span> Explosive Eruptions in 2015 and Danger to Aviation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Girina, Olga; Melnikov, Dmitry; Manevich, Alexander; Demyanchuk, Yury; Nuzhdaev, Anton; Petrova, Elena</p> <p>2016-04-01</p> <p>There are 36 <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Kamchatka and North Kurile, and several of them are continuously <span class="hlt">active</span>. In 2015, four of the Kamchatkan <span class="hlt">volcanoes</span> (Sheveluch, Klyuchevskoy, Karymsky and Zhupanovsky) and two <span class="hlt">volcanoes</span> of North Kurile (Alaid and Chikurachki) had strong and moderate explosive eruptions. Moderate gas-steam <span class="hlt">activity</span> was observing of Bezymianny, Kizimen, Avachinsky, Koryaksky, Gorely, Mutnovsky and other <span class="hlt">volcanoes</span>. Strong explosive eruptions of <span class="hlt">volcanoes</span> are the most dangerous for aircraft because they can produce in a few hours or days to the atmosphere and the stratosphere till several cubic kilometers of volcanic ash and aerosols. Ash plumes and the clouds, depending on the power of the eruption, the strength and wind speed, can travel thousands of kilometers from the <span class="hlt">volcano</span> for several days, remaining hazardous to aircraft, as the melting temperature of small particles of ash below the operating temperature of jet engines. The eruptive <span class="hlt">activity</span> of Sheveluch <span class="hlt">volcano</span> began since 1980 (growth of the lava dome) and is continuing at present. Strong explosive events of the <span class="hlt">volcano</span> occurred in 2015: on 07, 12, and 15 January, 01, 17, and 28 February, 04, 08, 16, 21-22, and 26 March, 07 and 12 April: ash plumes rose up to 7-12 km a.s.l. and extended more 900 km to the different directions of the <span class="hlt">volcano</span>. Ashfalls occurred at Ust'-Kamchatsk on 16 March, and Klyuchi on 30 October. Strong and moderate hot avalanches from the lava dome were observing more often in the second half of the year. Aviation color code of Sheveluch was Orange during the year. <span class="hlt">Activity</span> of the <span class="hlt">volcano</span> was dangerous to international and local aviation. Explosive-effusive eruption of Klyuchevskoy <span class="hlt">volcano</span> lasted from 01 January till 24 March. Strombolian explosive volcanic <span class="hlt">activity</span> began from 01 January, and on 08-09 January a lava flow was detected at the Apakhonchich chute on the southeastern flank of the <span class="hlt">volcano</span>. Vulcanian <span class="hlt">activity</span> of the <span class="hlt">volcano</span> began from 10 January. Ashfalls</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090008648','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090008648"><span>Reducing Unsteady Loads on a Piggyback Miniature <span class="hlt">Submarine</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lin, John</p> <p>2009-01-01</p> <p>A small, simple fixture has been found to be highly effective in reducing destructive unsteady hydrodynamic loads on a miniature <span class="hlt">submarine</span> that is attached in piggyback fashion to the top of a larger, nuclear-powered, host <span class="hlt">submarine</span>. The fixture, denoted compact ramp, can be installed with minimal structural modification, and the use of it does not entail any change in <span class="hlt">submarine</span> operations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4347C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4347C"><span>What threat do turbidity currents and <span class="hlt">submarine</span> landslides pose to <span class="hlt">submarine</span> telecommunications cable infrastructure?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clare, Michael; Pope, Edward; Talling, Peter; Hunt, James; Carter, Lionel</p> <p>2016-04-01</p> <p>The global economy relies on uninterrupted usage of a network of telecommunication cables on the seafloor. These <span class="hlt">submarine</span> cables carry ~99% of all trans-oceanic digital data and voice communications traffic worldwide, as they have far greater bandwidth than satellites. Over 9 million SWIFT banks transfers alone were made using these cables in 2004, totalling 7.4 trillion of transactions per day between 208 countries, which grew to 15 million SWIFT bank transactions last year. We outline the challenge of why, how often, and where seafloor cables are broken by natural causes; primarily subsea landslides and sediment flows (turbidity currents and also debris flows and hyperpycnal flows). These slides and flows can be very destructive. As an example, a sediment flow in 1929 travelled up to 19 m/s and broke 11 cables in the NE Atlantic, running out for ~800 km to the abyssal ocean. The 2006 Pingtung earthquake triggered a sediment flow that broke 22 cables offshore Taiwan over a distance of 450 km. Here, we present initial results from the first statistical analysis of a global database of cable breaks and causes. We first investigate the controls on frequency of <span class="hlt">submarine</span> cable breaks in different environmental and geological settings worldwide. We assess which types of earthquake pose a significant threat to <span class="hlt">submarine</span> cable networks. Meteorological events, such as hurricanes and typhoons, pose a significant threat to <span class="hlt">submarine</span> cable networks, so we also discuss the potential impacts of future climate change on the frequency of such hazards. We then go on to ask what are the physical impacts of <span class="hlt">submarine</span> sediment flows on submerged cables? A striking observation from past cable breaks is sometimes cables remain unbroken, whilst adjacent cables are severed (and record powerful flows travelling at up to 6 m/s). Why are some cables broken, but neighbouring cables remain intact? We provide some explanations for this question, and outline the need for future in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996EOSTr..77..113S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996EOSTr..77..113S"><span>Monitoring <span class="hlt">Active</span> <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Swanson, Don</p> <p></p> <p>Monitoring <span class="hlt">volcanoes</span> is a surprisingly controversial enterprise. Some volcanologists argue that monitoring promises too much and delivers too little for risk mitigation. They trust only strict land-use measures (and accompanying high insurance premiums in risky zones) and urge that funds be used for public education and awareness rather than for instrumental monitoring. Others claim that monitoring is more akin to Brownian motion than to science: lots of action but little net progress. Still other volcanologists acknowledge the potential value of monitoring for prediction and warning but despair at the difficulty of it all. And, finally, some shy from surveillance, fearing the legal consequences of a failed monitoring effort during these litigious times. They wonder, “Will I be sued if an eruption is not foreseen or if an instrument fails at a critical time?”</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gip/volc','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gip/volc"><span><span class="hlt">Volcanoes</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>Tilling, Robert I.; ,</p> <p>1998-01-01</p> <p><span class="hlt">Volcanoes</span> destroy and <span class="hlt">volcanoes</span> create. The catastrophic eruption of Mount St. Helens on May 18, 1980, made clear the awesome destructive power of a <span class="hlt">volcano</span>. Yet, over a time span longer than human memory and record, <span class="hlt">volcanoes</span> have played a key role in forming and modifying the planet upon which we live. More than 80 percent of the Earth's surface--above and below sea level--is of volcanic origin. Gaseous emissions from volcanic vents over hundreds of millions of years formed the Earth's earliest oceans and atmosphere, which supplied the ingredients vital to evolve and sustain life. Over geologic eons, countless volcanic eruptions have produced mountains, plateaus, and plains, which subsequent erosion and weathering have sculpted into majestic landscapes and formed fertile soils.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70094778','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70094778"><span>Santorini <span class="hlt">Volcano</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>Druitt, T.H.; Edwards, L.; Mellors, R.M.; Pyle, D.M.; Sparks, R.S.J.; Lanphere, M.; Davies, M.; Barreirio, B.</p> <p>1999-01-01</p> <p>Santorini is one of the most spectacular caldera <span class="hlt">volcanoes</span> in the world. It has been the focus of significant scientific and scholastic interest because of the great Bronze Age explosive eruption that buried the Minoan town of Akrotiri. Santorini is still <span class="hlt">active</span>. It has been dormant since 1950, but there have been several substantial historic eruptions. Because of this potential risk to life, both for the indigenous population and for the large number of tourists who visit it, Santorini has been designated one of five European Laboratory <span class="hlt">Volcanoes</span> by the European Commission. Santorini has long fascinated geologists, with some important early work on <span class="hlt">volcanoes</span> being conducted there. Since 1980, research groups at Cambridge University, and later at the University of Bristol and Blaise Pascal University in Clermont-Ferrand, have collected a large amount of data on the stratigraphy, geochemistry, geochronology and petrology of the volcanics. The volcanic field has been remapped at a scale of 1:10 000. A remarkable picture of cyclic volcanic <span class="hlt">activity</span> and magmatic evolution has emerged from this work. Much of this work has remained unpublished until now. This Memoir synthesizes for the first time all the data from the Cambridge/Bristol/Clermont groups, and integrates published data from other research groups. It provides the latest interpretation of the tectonic and magmatic evolution of Santorini. It is accompanied by the new 1:10 000 full-colour geological map of the island.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.1769C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1769C"><span>ICE-VOLC Project: unravelling the dynamics of Antarctica <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cannata, Andrea; Del Carlo, Paola; Giudice, Gaetano; Giuffrida, Giovanni; Larocca, Graziano; Liuzzo, Marco</p> <p>2017-04-01</p> <p>Melbourne and Rittmann <span class="hlt">volcanoes</span> are located in the Victoria Land. Whilst Rittmann's last eruption dates probably to Pleistocene, Melbourne's most recent eruption between 1862 and 1922, testifying it is still <span class="hlt">active</span>. At present, both <span class="hlt">volcanoes</span> display fumarolic <span class="hlt">activity</span>. Melbourne was discovered in 1841 by James Clark Ross, Rittmann during the 4th Italian Expedition (1988/1989). Our knowledge on both <span class="hlt">volcanoes</span> is really little. The position of these <span class="hlt">volcanoes</span> in the Antarctic region (characterised by absence of anthropic noise) and its proximity with the Italian Mario Zucchelli Station makes them ideal sites for studying <span class="hlt">volcano</span> seismic sources, geothermal emissions, seismo-acoustic signals caused by cryosphere-hydrosphere-atmosphere dynamics, and volcanic gas impact on environment. Hence, the main aim of the ICE-VOLC ("multiparametrIC Experiment at antarctica <span class="hlt">VOLCanoes</span>: data from <span class="hlt">volcano</span> and cryosphere-ocean-atmosphere dynamics") project is the study of Melbourne and Rittmann, by acquisition, analysis and integration of multiparametric geophysical, geochemical and thermal data. Complementary objectives include investigation of the relationship between seismo-acoustic <span class="hlt">activity</span> recorded in Antarctica and cryosphere-hydrosphere-atmosphere dynamics, evaluation of the impact of volcanic gas in atmosphere. This project involves 26 researchers, technologists and technicians from University of Perugia and from Istituto Nazionale di Geofisica e Vulcanologia of Catania, Palermo, Pisa and Rome. In this work, we show the preliminary results obtained after the first expedition in Antarctica, aiming to perform geochemical-thermal surveys in the <span class="hlt">volcano</span> ice caves, as well as to collect ash samples and to install temporary seismic stations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70038650','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70038650"><span>One hundred years of <span class="hlt">volcano</span> monitoring in 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>Kauahikaua, Jim; Poland, Mike</p> <p>2012-01-01</p> <p>In 2012 the Hawaiian <span class="hlt">Volcano</span> Observatory (HVO), the oldest of five <span class="hlt">volcano</span> observatories in the United States, is commemorating the 100th anniversary of its founding. HVO's location, on the rim of Kilauea <span class="hlt">volcano</span> (Figure 1)—one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> on Earth—has provided an unprecedented opportunity over the past century to study processes associated with <span class="hlt">active</span> volcanism and develop methods for hazards assessment and mitigation. The scientifically and societally important results that have come from 100 years of HVO's existence are the realization of one man's vision of the best way to protect humanity from natural disasters. That vision was a response to an unusually destructive decade that began the twentieth century, a decade that saw almost 200,000 people killed by the effects of earthquakes and volcanic eruptions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032222','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032222"><span>One hundred years of <span class="hlt">volcano</span> monitoring in 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>Kauahikaua, J.; Poland, M.</p> <p>2012-01-01</p> <p>In 2012 the Hawaiian <span class="hlt">Volcano</span> Observatory (HVO), the oldest of five <span class="hlt">volcano</span> observatories in the United States, is commemorating the 100th anniversary of its founding. HVO's location, on the rim of Klauea <span class="hlt">volcano</span> (Figure 1)one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> on Earthhas provided an unprecedented opportunity over the past century to study processes associated with <span class="hlt">active</span> volcanism and develop methods for hazards assessment and mitigation. The scientifically and societally important results that have come from 100 years of HVO's existence are the realization of one man's vision of the best way to protect humanity from natural disasters. That vision was a response to an unusually destructive decade that began the twentieth century, a decade that saw almost 200,000 people killed by the effects of earthquakes and volcanic eruptions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018FrEaS...6...50H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018FrEaS...6...50H"><span>The Evolution of Galápagos <span class="hlt">Volcanoes</span>: An Alternative Perspective</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harpp, Karen S.; Geist, Dennis J.</p> <p>2018-05-01</p> <p>The older eastern Galápagos are different in almost every way from the historically <span class="hlt">active</span> western Galápagos <span class="hlt">volcanoes</span>. The western Galápagos <span class="hlt">volcanoes</span> have steep upper slopes and are topped by large calderas, whereas none of the older islands has a caldera, an observation that is supported by recent gravity measurements. Moreover, the eastern islands tend to have been constructed by linear fissure systems and many are cut by faults. Most of the western <span class="hlt">volcanoes</span> erupt evolved basalts with an exceedingly small range of Mg#, Lan/Smn, and Smn/Ybn. This is attributed to homogenization in a crustal-scale magmatic mush column, which is maintained in a thermochemical steady state, owing to high magma supply directly over the Galápagos mantle plume. The exceptions are <span class="hlt">volcanoes</span> at the leading edge of the hotspot, which have yet to develop mush columns, and <span class="hlt">volcanoes</span> that are waning in <span class="hlt">activity</span>, because they are being carried away from the plume. In contrast, the eastern <span class="hlt">volcanoes</span> erupt relatively primitive magmas, with a large range in Mg#, Lan/Smn, and Smn/Ybn. This is attributed to isolated, ephemeral magmatic plumbing systems supplied by smaller magmatic fluxes throughout their histories. Consequently, each batch of magma follows an independent course of evolution, owing to the low volume of hypersolidus material beneath these <span class="hlt">volcanoes</span>. The magmatic flux to Galápagos <span class="hlt">volcanoes</span> negatively correlates with the distance to the Galápagos Spreading Center (GSC). When the ridge was close to the plume, most of the plume-derived magma was directed to the ridge. Currently, the <span class="hlt">active</span> <span class="hlt">volcanoes</span> are much farther from the GSC, thus most of the plume-derived magma erupts on the Nazca Plate and can be focused beneath the large young shields. We define an intermediate sub-province comprising Rabida, Santiago and Pinzon <span class="hlt">volcanoes</span>, which were most <span class="hlt">active</span> about 1 Ma. They have all erupted dacites, rhyolites, and trachytes, similar to the dying stage of the western <span class="hlt">volcanoes</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/gip/117/gip117.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/gip/117/gip117.pdf"><span>Eruptions of Hawaiian <span class="hlt">volcanoes</span> - Past, present, and future</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tilling, Robert I.; Heliker, Christina; Swanson, Donald A.</p> <p>2010-01-01</p> <p>Viewing an erupting <span class="hlt">volcano</span> is a memorable experience, one that has inspired fear, superstition, worship, curiosity, and fascination since before the dawn of civilization. In modern times, volcanic phenomena have attracted intense scientific interest, because they provide the key to understanding processes that have created and shaped more than 80 percent of the Earth's surface. The <span class="hlt">active</span> Hawaiian <span class="hlt">volcanoes</span> have received special attention worldwide because of their frequent spectacular eruptions, which often can be viewed and studied with relative ease and safety. In January 1987, the Hawaiian <span class="hlt">Volcano</span> Observatory (HVO), located on the rim of Kilauea <span class="hlt">Volcano</span>, celebrated its 75th Anniversary. In honor of HVO's Diamond Jubilee, the U.S. Geological Survey (USGS) published Professional Paper 1350 (see list of Selected Readings, page 57), a comprehensive summary of the many studies on Hawaiian volcanism by USGS and other scientists through the mid-1980s. Drawing from the wealth of data contained in that volume, the USGS also published in 1987 the original edition of this general-interest booklet, focusing on selected aspects of the eruptive history, style, and products of two of Hawai'i's <span class="hlt">active</span> <span class="hlt">volcanoes</span>, Kilauea and Mauna Loa. This revised edition of the booklet-spurred by the approaching Centennial of HVO in January 2012-summarizes new information gained since the January 1983 onset of Kilauea's Pu'u 'O'o-Kupaianaha eruption, which has continued essentially nonstop through 2010 and shows no signs of letup. It also includes description of Kilauea's summit <span class="hlt">activity</span> within Halema'uma'u Crater, which began in mid-March 2008 and continues as of this writing (late 2010). This general-interest booklet is a companion to the one on Mount St. Helens <span class="hlt">Volcano</span> first published in 1984 and revised in 1990 (see Selected Readings). Together, these publications illustrate the contrast between the two main types of <span class="hlt">volcanoes</span>: shield <span class="hlt">volcanoes</span>, such as those in Hawai'i, which generally</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://adsabs.harvard.edu/abs/2014AGUFMOS12A..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS12A..08F"><span>Effect of <span class="hlt">Submarine</span> Groundwater Discharge on Relict Arctic <span class="hlt">Submarine</span> Permafrost and Gas Hydrate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Frederick, J. M.; Buffett, B. A.</p> <p>2014-12-01</p> <p>Permafrost-associated gas hydrate deposits exist at shallow depths within the sediments of the circum-Arctic continental shelves. Degradation of this shallow water reservoir has the potential to release large quantities of methane gas directly to the atmosphere. Gas hydrate stability and the permeability of the shelf sediments to gas migration is closely linked with <span class="hlt">submarine</span> permafrost. <span class="hlt">Submarine</span> permafrost extent depends on several factors, such as the lithology, sea level variations, mean annual air temperature, ocean bottom water temperature, geothermal heat flux, and the salinity of the pore water. The salinity of the pore water is especially relevant because it partially controls the freezing point for both ice and gas hydrate. Measurements of deep pore water salinity are few and far between, but show that deep off-shore sediments are fresh. Deep freshening has been attributed to large-scale topographically-driven <span class="hlt">submarine</span> groundwater discharge, which introduces fresh terrestrial groundwater into deep marine sediments. We investigate the role of <span class="hlt">submarine</span> ground water discharge on the salinity field and its effects on the seaward extent of relict <span class="hlt">submarine</span> permafrost and gas hydrate stability on the Arctic shelf with a 2D shelf-scale model based on the finite volume method. The model tracks the evolution of the temperature, salinity, and pressure fields given imposed boundary conditions, with latent heat of water ice and hydrate formation included. The permeability structure of the sediments is coupled to changes in permafrost. Results show that pore fluid is strongly influenced by the permeability variations imposed by the overlying permafrost layer. Groundwater discharge tends to travel horizontally off-shore beneath the permafrost layer and the freshwater-saltwater interface location displays long timescale transient behavior that is dependent on the groundwater discharge strength. The seaward permafrost extent is in turn strongly influenced by the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BVol...75..773S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BVol...75..773S"><span>Development of an automatic volcanic ash sampling apparatus for <span class="hlt">active</span> <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shimano, Taketo; Nishimura, Takeshi; Chiga, Nobuyuki; Shibasaki, Yoshinobu; Iguchi, Masato; Miki, Daisuke; Yokoo, Akihiko</p> <p>2013-12-01</p> <p>We develop an automatic system for the sampling of ash fall particles, to be used for continuous monitoring of magma ascent and eruptive dynamics at <span class="hlt">active</span> <span class="hlt">volcanoes</span>. The system consists of a sampling apparatus and cameras to monitor surface phenomena during eruptions. The Sampling Apparatus for Time Series Unmanned Monitoring of Ash (SATSUMA-I and SATSUMA-II) is less than 10 kg in weight and works automatically for more than a month with a 10-kg lead battery to obtain a total of 30 to 36 samples in one cycle of operation. The time range covered in one cycle varies from less than an hour to several months, depending on the aims of observation, allowing researchers to target minute-scale fluctuations in a single eruptive event, as well as daily to weekly trends in persistent volcanic <span class="hlt">activity</span>. The latest version, SATSUMA-II, also enables control of sampling parameters remotely by e-mail commands. Durability of the apparatus is high: our prototypes worked for several months, in rainy and typhoon seasons, at windy and humid locations, and under strong sunlight. We have been successful in collecting ash samples emitted from Showa crater almost everyday for more than 4 years (2008-2012) at Sakurajima <span class="hlt">volcano</span> in southwest Japan.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4864321','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4864321"><span>Influence of Anchoring on Burial Depth of <span class="hlt">Submarine</span> Pipelines</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zhuang, Yuan; Li, Yang; Su, Wei</p> <p>2016-01-01</p> <p>Since the beginning of the twenty-first century, there has been widespread construction of <span class="hlt">submarine</span> oil-gas transmission pipelines due to an increase in offshore oil exploration. Vessel anchoring operations are causing more damage to <span class="hlt">submarine</span> pipelines due to shipping transportation also increasing. Therefore, it is essential that the influence of anchoring on the required burial depth of <span class="hlt">submarine</span> pipelines is determined. In this paper, mathematical models for ordinary anchoring and emergency anchoring have been established to derive an anchor impact energy equation for each condition. The required effective burial depth for <span class="hlt">submarine</span> pipelines has then been calculated via an energy absorption equation for the protection layer covering the <span class="hlt">submarine</span> pipelines. Finally, the results of the model calculation have been verified by accident case analysis, and the impact of the anchoring height, anchoring water depth and the anchor weight on the required burial depth of <span class="hlt">submarine</span> pipelines has been further analyzed. PMID:27166952</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036223','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036223"><span>Measuring currents in <span class="hlt">submarine</span> canyons: technological and scientific progress in the past 30 years</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Xu, J. P.</p> <p>2011-01-01</p> <p>The development and application of acoustic and optical technologies and of accurate positioning systems in the past 30 years have opened new frontiers in the <span class="hlt">submarine</span> canyon research communities. This paper reviews several key advancements in both technology and science in the field of currents in <span class="hlt">submarine</span> canyons since the1979 publication of Currents in <span class="hlt">Submarine</span> Canyons and Other Sea Valleys by Francis Shepard and colleagues. Precise placements of high-resolution, high-frequency instruments have not only allowed researchers to collect new data that are essential for advancing and generalizing theories governing the canyon currents, but have also revealed new natural phenomena that challenge the understandings of the theorists and experimenters in their predictions of <span class="hlt">submarine</span> canyon flow fields. Baroclinic motions at tidal frequencies, found to be intensified both up canyon and toward the canyon floor, dominate the flow field and control the sediment transport processes in <span class="hlt">submarine</span> canyons. Turbidity currents are found to frequently occur in <span class="hlt">active</span> <span class="hlt">submarine</span> canyons such as Monterey Canyon. These turbidity currents have maximum speeds of nearly 200 cm/s, much smaller than the speeds of turbidity currents in geological time, but still very destructive. In addition to traditional Eulerian measurements, Lagrangian flow data are essential in quantifying water and sediment transport in <span class="hlt">submarine</span> canyons. A concerted experiment with multiple monitoring stations along the canyon axis and on nearby shelves is required to characterize the storm-trigger mechanism for turbidity currents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/9974388','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/9974388"><span>A kuroko-type polymetallic sulfide deposit in a <span class="hlt">submarine</span> silicic caldera</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Iizasa; Fiske; Ishizuka; Yuasa; Hashimoto; Ishibashi; Naka; Horii; Fujiwara; Imai; Koyama</p> <p>1999-02-12</p> <p>Manned submersible studies have delineated a large and <span class="hlt">actively</span> growing Kuroko-type volcanogenic massive sulfide deposit 400 kilometers south of Tokyo in Myojin Knoll <span class="hlt">submarine</span> caldera. The sulfide body is located on the caldera floor at a depth of 1210 to 1360 meters, has an area of 400 by 400 by 30 meters, and is notably rich in gold and silver. The discovery of a large Kuroko-type polymetallic sulfide deposit in this arc-front caldera raises the possibility that the numerous unexplored <span class="hlt">submarine</span> silicic calderas elsewhere might have similar deposits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016071','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016071"><span>Recent uplift and hydrothermal <span class="hlt">activity</span> at Tangkuban Parahu <span class="hlt">volcano</span>, west Java, Indonesia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dvorak, J.; Matahelumual, J.; Okamura, A.T.; Said, H.; Casadevall, T.J.; Mulyadi, D.</p> <p>1990-01-01</p> <p>Tangkuban Parahu is an <span class="hlt">active</span> stratovolcano located 17 km north of the city of Bandung in the province west Java, Indonesia. All historical eruptive <span class="hlt">activity</span> at this <span class="hlt">volcano</span> has been confined to a complex of explosive summit craters. About a dozen eruptions-mostly phreatic events- and 15 other periods of unrest, indicated by earthquakes or increased thermal <span class="hlt">activity</span>, have been noted since 1829. The last magmatic eruption occurred in 1910. In late 1983, several small phreatic explosions originated from one of the summit craters. More recently, increased hydrothermal and earthquake <span class="hlt">activity</span> occurred from late 1985 through 1986. Tilt measurements, using a spirit-level technique, have been made every few months since February 1981 in the summit region and along the south and east flanks of the <span class="hlt">volcano</span>. Measurements made in the summit region indicated uplift since the start of these measurements through at least 1986. From 1981 to 1983, the average tilt rate at the edges of the summit craters was 40-50 microradians per year. After the 1983 phreatic <span class="hlt">activity</span>, the tilt rate decreased by about a factor of five. Trilateration surveys across the summit craters and on the east flank of the <span class="hlt">volcano</span> were conducted in 1983 and 1986. Most line length changes measured during this three-year period did not exceed the expected uncertainty of the technique (4 ppm). The lack of measurable horizontal strain across the summit craters seems to contradict the several years of tilt measurements. Using a point source of dilation in an elastic half-space to model tilt measurements, the pressure center at Tangkuban Parahu is located about 1.5 km beneath the southern part of the summit craters. This is beneath the epicentral area of an earthquake swarm that occurred in late 1983. The average rate in the volume of uplift from 1981 to 1983 was 3 million m3 per year; from 1983 to 1986 it averaged about 0.4 million m3 per year. Possible causes for this uplift are increased pressure within a very</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.V11A0338R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.V11A0338R"><span>Hydrothermal Alteration and Seawater Exchange at Surtsey <span class="hlt">Volcano</span>, Iceland: New results from 1979 Surtsey Drill Core.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rhodes, M.; Bryce, J. G.; Jercinovic, M. J.; Fahnestock, M. F.; Jackson, M. D.</p> <p>2017-12-01</p> <p>The archetypal <span class="hlt">volcano</span> Surtsey erupted spectacularly out of the North Atlantic Ocean from November 1963 to June 1967, on the southern <span class="hlt">submarine</span> extension of the E. Icelandic Rift Zone. Twelve years later, in 1979, the eastern cone (Surtur I) was drilled to a depth of 181 m to document the growth of the <span class="hlt">volcano</span> and the interaction of basaltic tephra with seawater [1]. The present study is a pilot project for the International Continental Drilling Project on Surtsey, SUSTAIN, starting in August, 2017. The overall intent is to document the nature, extent and rates of hydrothermal and seawater reaction with tephra over the past 50 years. This work builds on the 1979 drilling studies through new electron microprobe and laser ablation (LA- ICPMS) analyses to document varying degrees of palagonitic alteration of volcanic glass and primary phases to form authigenic minerals (smectite, zeolites, Al-tobermorite, anhydrite) in the intervening 12 years since the eruption. Combined with modal data and inferred phase densities, the data documents the mass balance of major and trace elements among the phases and the relationship of these changes to core depth, temperature and porosity. Although hydrothermal alteration is extensive, especially in the hotter <span class="hlt">submarine</span> intervals from 60 to 120 m, detailed whole-rock major, trace and isotopic data (Sr, Nd, Pb), show that, apart from hydration and oxidation, there is only modest exchange of elements between tephra and seawater, or hydrothermal fluids, in the upper 140 m of the core prior to 1979. Below 140 m, in a cooler zone of coarse, more porous tephra, extensive exchange of elements, involving hydrothermal introduction of sulfur and growth of anhydrite, is associated with the loss of Ca, K, Rb, Sr and addition of MgO and Na and seawater isotopic signatures. It is surely no coincidence that this zone of elemental and isotopic exchange supports <span class="hlt">active</span> microbial colonies [2]. Our results serve as an important baseline for the 2017</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017417','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017417"><span>Geology of kilauea <span class="hlt">volcano</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>Moore, R.B.; Trusdell, F.A.</p> <p>1993-01-01</p> <p>This paper summarizes studies of the structure, stratigraphy, petrology, drill holes, eruption frequency, and volcanic and seismic hazards of Kilauea <span class="hlt">volcano</span>. All the <span class="hlt">volcano</span> is discussed, but the focus is on its lower cast rift zone (LERZ) because <span class="hlt">active</span> exploration for geothermal energy is concentrated in that area. Kilauea probably has several separate hydrothermal-convection systems that develop in response to the dynamic behavior of the <span class="hlt">volcano</span> and the influx of abundant meteoric water. Important features of some of these hydrothermal-convection systems are known through studies of surface geology and drill holes. Observations of eruptions during the past two centuries, detailed geologic mapping, radiocarbon dating, and paleomagnetic secular-variation studies indicate that Kilauea has erupted frequently from its summit and two radial rift zones during Quaternary time. Petrologic studies have established that Kilauea erupts only tholeiitic basalt. Extensive ash deposits at Kilauea's summit and on its LERZ record locally violent, but temporary, disruptions of local hydrothermal-convection systems during the interaction of water or steam with magma. Recent drill holes on the LERZ provide data on the temperatures of the hydrothermal-convection systems, intensity of dike intrusion, porosity and permeability, and an increasing amount of hydrothermal alteration with depth. The prehistoric and historic record of volcanic and seismic <span class="hlt">activity</span> indicates that magma will continue to be supplied to deep and shallow reservoirs beneath Kilauea's summit and rift zones and that the <span class="hlt">volcano</span> will be affected by eruptions and earthquakes for many thousands of years. ?? 1993.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JVGR..151..279C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JVGR..151..279C"><span>A <span class="hlt">submarine</span> perspective of the Honolulu Volcanics, Oahu</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clague, David A.; Paduan, Jennifer B.; McIntosh, William C.; Cousens, Brian L.; Davis, Alicé S.; Reynolds, Jennifer R.</p> <p>2006-03-01</p> <p>Lavas and volcaniclastic deposits were observed and collected from 4 <span class="hlt">submarine</span> cones that are part of the Honolulu Volcanics on Oahu, Hawaii. The locations of these and a few additional, but unsampled, vents demonstrate that nearly all the vents are located on or very close to the shoreline of Oahu, with the most distal vent just 12 km offshore. The clastic samples and outcrops range from coarse breccias to cross-bedded ash deposits and show that explosive volcanism at depths between about 350 and 590 m depth played a part in forming these volcanic cones. The eruptive styles appear to be dominantly effusive to strombolian at greater depths, but apparently include violent phreatomagmatic explosive <span class="hlt">activity</span> at the shallower sites along the <span class="hlt">submarine</span> southwest extension of the Koko Rift. The compositions of the recovered samples are broadly similar to the strongly alkalic subaerial Honolulu Volcanics lavas, but the <span class="hlt">submarine</span> lavas, erupted further from the Koolau caldera, have slightly more radiogenic Sr isotopic ratios, and trace element patterns that are distinct from either the subaerial Honolulu Volcanics or the <span class="hlt">submarine</span> North Arch lavas. These patterns are characterized by moderate to strong positive Sr and P anomalies, and moderate to strong negative Cs, Rb, U, Th, Zr, and Hf anomalies. Most samples have strong negative K and moderate negative Ti anomalies, as do all subaerial Honolulu Volcanics and North Arch samples, but one group of samples from the Koko Rift lack this chemical signature. The data are consistent with more garnet in the source region for the off-shore samples than for either the on-shore Honolulu Volcanics lavas. New Ar-Ar ages show that eruptions at the <span class="hlt">submarine</span> vents and Diamond Head occurred between about 0.5 Ma and 0.1 Ma, with the youngest ages from the Koko Rift. These ages are in general agreement with most published ages for the formation and suggest that some much younger ages reported previously from the Koko Rift are probably</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA03462.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA03462.html"><span>Nyiragonga <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2002-02-01</p> <p>This image of the Nyiragonga <span class="hlt">volcano</span> eruption in the Congo was acquired on January 28, 2002 by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA's Terra satellite. With its 14spectral bands from the visible to the thermal infrared wavelength region, and its high spatial resolution of 15 to 90 meters about 50 to 300 feet ), ASTER will image Earth for the next 6 years to map and monitor the changing surface of our planet. Image: A river of molten rock poured from the Nyiragongo <span class="hlt">volcano</span> in the Congo on January 18, 2002, a day after it erupted, killing dozens, swallowing buildings and forcing hundreds of thousands to flee the town of Goma. The flow continued into Lake Kivu. The lave flows are depicted in red on the image indicating they are still hot. Two of them flowed south form the <span class="hlt">volcano</span>'s summit and went through the town of Goma. Another flow can be seen at the top of the image, flowing towards the northwest. One of Africa's most notable <span class="hlt">volcanoes</span>, Nyiragongo contained an <span class="hlt">active</span> lava lake in its deep summit crater that drained catastrophically through its outer flanks in 1977. Extremely fluid, fast-moving lava flows draining from the summit lava lake in 1977 killed 50 to 100 people, and several villages were destroyed. The image covers an area of 21 x 24 km and combines a thermal band in red, and two infrared bands in green and blue. http://photojournal.jpl.nasa.gov/catalog/PIA03462</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGeo...43..118T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGeo...43..118T"><span>Volcanism in Iceland in historical time: <span class="hlt">Volcano</span> types, eruption styles and eruptive history</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thordarson, T.; Larsen, G.</p> <p>2007-01-01</p> <p>The large-scale volcanic lineaments in Iceland are an axial zone, which is delineated by the Reykjanes, West and North Volcanic Zones (RVZ, WVZ, NVZ) and the East Volcanic Zone (EVZ), which is growing in length by propagation to the southwest through pre-existing crust. These zones are connected across central Iceland by the Mid-Iceland Belt (MIB). Other volcanically <span class="hlt">active</span> areas are the two intraplate belts of Öræfajökull (ÖVB) and Snæfellsnes (SVB). The principal structure of the volcanic zones are the 30 volcanic systems, where 12 are comprised of a fissure swarm and a central <span class="hlt">volcano</span>, 7 of a central <span class="hlt">volcano</span>, 9 of a fissure swarm and a central domain, and 2 are typified by a central domain alone. Volcanism in Iceland is unusually diverse for an oceanic island because of special geological and climatological circumstances. It features nearly all <span class="hlt">volcano</span> types and eruption styles known on Earth. The first order grouping of <span class="hlt">volcanoes</span> is in accordance with recurrence of eruptions on the same vent system and is divided into central <span class="hlt">volcanoes</span> (polygenetic) and basalt <span class="hlt">volcanoes</span> (monogenetic). The basalt <span class="hlt">volcanoes</span> are categorized further in accordance with vent geometry (circular or linear), type of vent accumulation, characteristic style of eruption and volcanic environment (i.e. subaerial, subglacial, <span class="hlt">submarine</span>). Eruptions are broadly grouped into effusive eruptions where >95% of the erupted magma is lava, explosive eruptions if >95% of the erupted magma is tephra (volume calculated as dense rock equivalent, DRE), and mixed eruptions if the ratio of lava to tephra occupy the range in between these two end-members. Although basaltic volcanism dominates, the <span class="hlt">activity</span> in historical time (i.e. last 11 centuries) features expulsion of basalt, andesite, dacite and rhyolite magmas that have produced effusive eruptions of Hawaiian and flood lava magnitudes, mixed eruptions featuring phases of Strombolian to Plinian intensities, and explosive phreatomagmatic and magmatic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=10524&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dactive%2Bvolcanoes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=10524&hterms=active+volcanoes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dactive%2Bvolcanoes"><span>Eruption of Shiveluch <span class="hlt">Volcano</span>, Kamchatka Peninsula</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2007-01-01</p> <p>On March 29, 2007, the Shiveluch <span class="hlt">Volcano</span> on the Russian Federation's Kamchatka Peninsula erupted. According to the Alaska <span class="hlt">Volcano</span> Observatory the <span class="hlt">volcano</span> underwent an explosive eruption between 01:50 and 2:30 UTC, sending an ash cloud skyward roughly 9,750 meters (32,000 feet), based on visual estimates. The Moderate Resolution Imaging Spectroradiometer (MODIS) flying onboard NASA's Aqua satellite took this picture at 02:00 UTC on March 29. The top image shows the <span class="hlt">volcano</span> and its surroundings. The bottom image shows a close-up view of the <span class="hlt">volcano</span> at 250 meters per pixel. Satellites often capture images of volcanic ash plumes, but usually as the plumes are blowing away. Plumes have been observed blowing away from Shiveluch before. This image, however, is different. At the time the Aqua satellite passed overhead, the eruption was recent enough (and the air was apparently still enough) that the ash cloud still hovered above the summit. In this image, the bulbous cloud casts its shadow northward over the icy landscape. Volcanic ash eruptions inject particles into Earth's atmosphere. Substantial eruptions of light-reflecting particles can reduce temperatures and even affect atmospheric circulation. Large eruptions impact climate patterns for years. A massive eruption of the Tambora <span class="hlt">Volcano</span> in Indonesia in 1815, for instance, earned 1816 the nickname 'the year without a summer.' Shiveluch is a stratovolcano--a steep-sloped <span class="hlt">volcano</span> composed of alternating layers of solidified ash, hardened lava, and volcanic rocks. One of Kamchatka's largest <span class="hlt">volcanoes</span>, it sports a summit reaching 3,283 meters (10,771 feet). Shiveluch is also one of the peninsula's most <span class="hlt">active</span> <span class="hlt">volcanoes</span>, with an estimated 60 substantial eruptions in the past 10,000 years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.V44A..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.V44A..02M"><span>Discoveries From the Cross-Disciplinary, Multi-Institutional South Seas Expedition from Hawaii to New Zealand and Back</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malahoff, A.; Wiltshire, J. C.; Smith, J. R.</p> <p>2005-12-01</p> <p>The Hawaii Undersea Research Laboratory organised an international research team to explore the chemistry, geology, biology, hydrothermal venting processes, mineral deposition, and biodiversity of seamounts extending south from Hawaii to New Zealand, including the <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> of the Tonga-Kermadec Island Arc. Research team members came from a Consortium comprising of principal investigators from the NOAA Pacific Marine Environment Lab and VENTS program, the Inst of Geological and Nuclear Sciences and the National Inst of Water and Atmospheric Research both of New Zealand, the Univ of Kiel in Germany, the Univ of Mississippi, Univ of Hawaii, the NOAA Marine Fisheries Service, Scripps Institution of Oceanography, Univ of Oregon, Oregon State Univ, Stanford Univ, and the U.S. Fish and Wildlife Service. Funding came from the member organizations of the Consortium and the NOAA Office of Ocean Exploration and National Undersea Research Program. The expedition left Hawaii on 18 March 2005 and returned on 05 August, aboard the R/V Ka`imikai-o-Kanaloa with the submersibles Pisces IV and Pisces V and the ROV RCV-150. Sixty-one science dives were executed during the eight legs of the expedition. Twelve <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the Samoa to New Zealand legs, one in the Samoan hot spot chain and the flanks of five islands and atolls on the legs between Samoa and Hawaii were investigated. Hundreds of specimens of new and unusual marine life, corals and other benthic organisms, extremophile micro- and macro-organisms, water samples for chemical analysis, polymetallic sulfides and rock samples were collected during the expedition. Unusual processes were observed at the Kermadec <span class="hlt">submarine</span> <span class="hlt">volcanoes</span>, including the oozing of liquid sulphur onto the seafloor and profuse carbon dioxide venting into seawater. Extensive <span class="hlt">submarine</span> hydrothermal venting, black smoker <span class="hlt">activity</span> and extraordinary chimney formations were studied in the caldera of Brothers <span class="hlt">Volcano</span>. In addition, extensive</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.1243J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.1243J"><span>Seismic unrest at Katla <span class="hlt">Volcano</span>- southern Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>jeddi, zeinab; Tryggvason, Ari; Gudmundsson, Olafur; Bödvarsson, Reynir; SIL Seismology Group</p> <p>2014-05-01</p> <p>Katla <span class="hlt">volcano</span> is located on the propagating Eastern Volcanic Zone (EVZ) in South Iceland. It is located beneath Mýrdalsjökull ice-cap which covers an area of almost 600 km2, comprising the summit caldera and the eruption vents. 20 eruptions between 930 and 1918 with intervals of 13-95 years are documented at Katla which is one of the most <span class="hlt">active</span> subglacial <span class="hlt">volcanoes</span> in Iceland. Eruptions at Katla are mainly explosive due to the subglacial mode of extrusion and produce high eruption columns and catastrophic melt water floods (jökulhlaups). The present long Volcanic repose (almost 96 years) at Katla, the general unrest since 1955, and the 2010 eruption of the neighbouring Eyjafjallajökull <span class="hlt">volcano</span> has prompted concerns among geoscientists about an imminent eruption. Thus, the <span class="hlt">volcano</span> has been densely monitored by seismologists and volcanologists. The seismology group of Uppsala University as a partner in the <span class="hlt">Volcano</span> Anatomy (VA) project in collaboration with the University of Iceland and the Icelandic Meteorological Office (IMO) installed 9 temporary seismic stations on and around the Mýrdalsjökull glacier in 2011. Another 10 permanent seismic stations are operated by IMO around Katla. The project's data collection is now finished and temporary stations were pulled down in August 2013. According to seismicity maps of the whole recording period, thousands of microearthquakes have occurred within the caldera region. At least three different source areas are <span class="hlt">active</span> in Katla: the caldera region, the western Godaland region and a small cluster at the southern rim of Mýrdalsjökull near the glacial stream of Hafursarjökull. Seismicity in the southern flank has basically started after June 2011. The caldera events are mainly <span class="hlt">volcano</span>-tectonic, while western and southern events are mostly long period (lp) and can be related to glacial or magmatic movement. One motivation of the VA Katla project is to better understand the physical mechanism of these lp events. Changes</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050220574','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050220574"><span>Effects of <span class="hlt">Volcanoes</span> on the Natural Environment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mouginis-Mark, Peter J.</p> <p>2005-01-01</p> <p>The primary focus of this project has been on the development of techniques to study the thermal and gas output of <span class="hlt">volcanoes</span>, and to explore our options for the collection of vegetation and soil data to enable us to assess the impact of this volcanic <span class="hlt">activity</span> on the environment. We originally selected several <span class="hlt">volcanoes</span> that have persistent gas emissions and/or magma production. The investigation took an integrated look at the environmental effects of a <span class="hlt">volcano</span>. Through their persistent <span class="hlt">activity</span>, basaltic <span class="hlt">volcanoes</span> such as Kilauea (Hawaii) and Masaya (Nicaragua) contribute significant amounts of sulfur dioxide and other gases to the lower atmosphere. Although primarily local rather than regional in its impact, the continuous nature of these eruptions means that they can have a major impact on the troposphere for years to decades. Since mid-1986, Kilauea has emitted about 2,000 tonnes of sulfur dioxide per day, while between 1995 and 2000 Masaya has emotted about 1,000 to 1,500 tonnes per day (Duffel1 et al., 2001; Delmelle et al., 2002; Sutton and Elias, 2002). These emissions have a significant effect on the local environment. The volcanic smog ("vog" ) that is produced affects the health of local residents, impacts the local ecology via acid rain deposition and the generation of acidic soils, and is a concern to local air traffic due to reduced visibility. Much of the work that was conducted under this NASA project was focused on the development of field validation techniques of <span class="hlt">volcano</span> degassing and thermal output that could then be correlated with satellite observations. In this way, we strove to develop methods by which not only our study <span class="hlt">volcanoes</span>, but also <span class="hlt">volcanoes</span> in general worldwide (Wright and Flynn, 2004; Wright et al., 2004). Thus <span class="hlt">volcanoes</span> could be routinely monitored for their effects on the environment. The selected <span class="hlt">volcanoes</span> were: Kilauea (Hawaii; 19.425 N, 155.292 W); Masaya (Nicaragua; 11.984 N, 86.161 W); and Pods (Costa Rica; 10.2OoN, 84.233 W).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034454p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034454p/"><span>34. VIEW OF <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK PRIOR TO ADDITION ...</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>34. VIEW OF <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK PRIOR TO ADDITION OF BLISTERS IN 1959, LOOKING SOUTHEAST - U.S. Naval <span class="hlt">Submarine</span> Base, New London <span class="hlt">Submarine</span> Escape Training Tank, Albacore & Darter Roads, Groton, New London County, CT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2008/5090/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2008/5090/"><span>Evolution of Deformation Studies on <span class="hlt">Active</span> Hawaiian <span class="hlt">Volcanoes</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>Decker, Robert W.; Okamura, Arnold; Miklius, Asta; Poland, Michael</p> <p>2008-01-01</p> <p>Everything responds to pressure, even rocks. Deformation studies involve measuring and interpreting the changes in elevations and horizontal positions of the land surface or sea floor. These studies are variously referred to as geodetic changes or ground-surface deformations and are sometimes indexed under the general heading of geodesy. Deformation studies have been particularly useful on <span class="hlt">active</span> <span class="hlt">volcanoes</span> and in <span class="hlt">active</span> tectonic areas. A great amount of time and energy has been spent on measuring geodetic changes on Kilauea and Mauna Loa <span class="hlt">Volcanoes</span> in Hawai`i. These changes include the build-up of the surface by the piling up and ponding of lava flows, the changes in the surface caused by erosion, and the uplift, subsidence, and horizontal displacements of the surface caused by internal processes acting beneath the surface. It is these latter changes that are the principal concern of this review. A complete and objective review of deformation studies on <span class="hlt">active</span> Hawaiian <span class="hlt">volcanoes</span> would take many volumes. Instead, we attempt to follow the evolution of the most significant observations and interpretations in a roughly chronological way. It is correct to say that this is a subjective review. We have spent years measuring and recording deformation changes on these great <span class="hlt">volcanoes</span> and more years trying to understand what makes these changes occur. We attempt to make this a balanced as well as a subjective review; the references are also selective rather than exhaustive. Geodetic changes caused by internal geologic processes vary in magnitude from the nearly infinitesimal - one micron or less, to the very large - hundreds of meters. Their apparent causes also are varied and include changes in material properties and composition, atmospheric pressure, tidal stress, thermal stress, subsurface-fluid pressure (including magma pressure, magma intrusion, or magma removal), gravity, and tectonic stress. Deformation is measured in units of strain or displacement. For example, tilt</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPA41D..01E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPA41D..01E"><span>Translating <span class="hlt">Volcano</span> Hazards Research in the Cascades Into Community Preparedness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ewert, J. W.; Driedger, C. L.</p> <p>2015-12-01</p> <p>Research by the science community into volcanic histories and physical processes at Cascade <span class="hlt">volcanoes</span> in the states of Washington, Oregon, and California has been ongoing for over a century. Eruptions in the 20th century at Lassen Peak and Mount St. Helen demonstrated the <span class="hlt">active</span> nature of Cascade <span class="hlt">volcanoes</span>; the 1980 eruption of Mount St. Helens was a defining moment in modern volcanology. The first modern <span class="hlt">volcano</span> hazards assessments were produced by the USGS for some Cascade <span class="hlt">volcanoes</span> in the 1960s. A rich scientific literature exists, much of which addresses hazards at these <span class="hlt">active</span> <span class="hlt">volcanoes</span>. That said community awareness, planning, and preparation for eruptions generally do not occur as a result of a hazard analyses published in scientific papers, but by direct communication with scientists. Relative to other natural hazards, volcanic eruptions (or large earthquakes, or tsunami) are outside common experience, and the public and many public officials are often surprised to learn of the impacts volcanic eruptions could have on their communities. In the 1980s, the USGS recognized that effective hazard communication and preparedness is a multi-faceted, long-term undertaking and began working with federal, state, and local stakeholders to build awareness and foster community action about <span class="hlt">volcano</span> hazards. <span class="hlt">Activities</span> included forming <span class="hlt">volcano</span>-specific workgroups to develop coordination plans for <span class="hlt">volcano</span> emergencies; a concerted public outreach campaign; curriculum development and teacher training; technical training for emergency managers and first responders; and development of hazard information that is accessible to non-specialists. Outcomes include broader ownership of <span class="hlt">volcano</span> hazards as evidenced by bi-national exchanges of emergency managers, community planners, and first responders; development by stakeholders of websites focused on <span class="hlt">volcano</span> hazards mitigation; and execution of table-top and functional exercises, including evacuation drills by local communities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015GeoJI.201..224H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015GeoJI.201..224H"><span>The use of rotational invariants for the interpretation of marine CSEM data with a case study from the North Alex mud <span class="hlt">volcano</span>, West Nile Delta</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hölz, Sebastian; Swidinsky, Andrei; Sommer, Malte; Jegen, Marion; Bialas, Jörg</p> <p>2015-04-01</p> <p><span class="hlt">Submarine</span> mud <span class="hlt">volcanos</span> at the seafloor are surface expressions of fluid flow systems within the seafloor. Since the electrical resistivity of the seafloor is mainly determined by the amount and characteristics of fluids contained within the sediment's pore space, electromagnetic methods offer a promising approach to gain insight into a mud <span class="hlt">volcano</span>'s internal resistivity structure. To investigate this structure, we conducted a controlled source electromagnetic experiment, which was novel in the sense that the source was deployed and operated with a remotely operated vehicle, which allowed for a flexible placement of the transmitter dipole with two polarization directions at each transmitter location. For the interpretation of the experiment, we have adapted the concept of rotational invariants from land-based electromagnetics to the marine case by considering the source normalized tensor of horizontal electric field components. We analyse the sensitivity of these rotational invariants in terms of 1-D models and measurement geometries and associated measurement errors, which resemble the experiment at the mud <span class="hlt">volcano</span>. The analysis shows that any combination of rotational invariants has an improved parameter resolution as compared to the sensitivity of the pure radial or azimuthal component alone. For the data set, which was acquired at the `North Alex' mud <span class="hlt">volcano</span>, we interpret rotational invariants in terms of 1-D inversions on a common midpoint grid. The resulting resistivity models show a general increase of resistivities with depth. The most prominent feature in the stitched 1-D sections is a lens-shaped interface, which can similarly be found in a section from seismic reflection data. Beneath this interface bulk resistivities frequently fall in a range between 2.0 and 2.5 Ωm towards the maximum penetration depths. We interpret the lens-shaped interface as the surface of a collapse structure, which was formed at the end of a phase of <span class="hlt">activity</span> of an older mud</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022635','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022635"><span>Volcanic history of El Chichon <span class="hlt">Volcano</span> (Chiapas, Mexico) during the Holocene, and its impact on human <span class="hlt">activity</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>Espindola, J.M.; Macias, J.L.; Tilling, R.I.; Sheridan, M.F.</p> <p>2000-01-01</p> <p>Before its devastating eruption in 1982, El Chichon <span class="hlt">Volcano</span> was little known and did not appear on any listings of hazardous <span class="hlt">volcanoes</span>. Subsequent geologic studies, based on stratigraphic and radiocarbon investigations, showed that at least three explosive eruptions had occurred previously at this <span class="hlt">volcano</span>. In this paper, we present the result of recent studies on the stratigraphy of the <span class="hlt">volcano</span> and new radiocarbon ages which show that at least 11 eruptions have taken place at El Chichon in the past 8000 years. Explosive events, most of them producing block-and-ash flow and surge deposits, occurred around 550, 900, 1250, 1500, 1600, 1900, 2000, 2500, 3100, 3700 and 7700 years BP. The juvenile products of these eruptions have a trachyandesitic composition with similar degree of evolution, as evidenced from their SiO2 abundance and depletion in MgO, CaO, TiO2, as well as trace and rare earth elements. This suggests segregation of olivine and orthopyroxene from the melt. Since human settlements in southeast Mexico and Central America can be traced as far back as approximately 2500 years BP, most of these events probably affected human <span class="hlt">activity</span>. In fact, there are reports of pottery shards and other artifacts in deposits from the eruption of 1250 BP. Pottery fragments in deposits of an eruption that took place 2500 BP are also reported in this paper. Thus, the impact of the <span class="hlt">volcano</span> on human <span class="hlt">activities</span> has been frequent, with most of the repose intervals lasting between 100 to 600 years. The impact of the eruptions was probably of greater than local extent, because airfall tephra could reach distant sites and possibly even affect weather. The eruptive history of El Chichon also offers clues in the investigation of the Maya civilization. Several researchers have considered the <span class="hlt">volcano</span> as an important factor in the answer to some intriguing questions such as the extensive use of volcanic ash in Late Classic Maya ceramics or, of greater importance, the causes of 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_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('https://eric.ed.gov/?q=volcanic+AND+eruption&pg=2&id=EJ118237','ERIC'); return false;" href="https://eric.ed.gov/?q=volcanic+AND+eruption&pg=2&id=EJ118237"><span><span class="hlt">Volcanoes</span></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>Kunar, L. N. S.</p> <p>1975-01-01</p> <p>Describes the forces responsible for the eruptions of <span class="hlt">volcanoes</span> and gives the physical and chemical parameters governing the type of eruption. Explains the structure of the earth in relation to <span class="hlt">volcanoes</span> and explains the location of volcanic regions. (GS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2001/0395/pdf/of2001-0395.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2001/0395/pdf/of2001-0395.pdf"><span>Lahar-hazard zonation for San Miguel <span class="hlt">volcano</span>, El Salvador</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Major, J.J.; Schilling, S.P.; Pullinger, C.R.; Escobar, C.D.; Chesner, C.A.; Howell, M.M.</p> <p>2001-01-01</p> <p>San Miguel <span class="hlt">volcano</span>, also known as Chaparrastique, is one of many <span class="hlt">volcanoes</span> along the volcanic arc in El Salvador. The <span class="hlt">volcano</span>, located in the eastern part of the country, rises to an altitude of about 2130 meters and towers above the communities of San Miguel, El Transito, San Rafael Oriente, and San Jorge. In addition to the larger communities that surround the <span class="hlt">volcano</span>, several smaller communities and coffee plantations are located on or around the flanks of the <span class="hlt">volcano</span>, and the PanAmerican and coastal highways cross the lowermost northern and southern flanks of the <span class="hlt">volcano</span>. The population density around San Miguel <span class="hlt">volcano</span> coupled with the proximity of major transportation routes increases the risk that even small <span class="hlt">volcano</span>-related events, like landslides or eruptions, may have significant impact on people and infrastructure. San Miguel <span class="hlt">volcano</span> is one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> in El Salvador; it has erupted at least 29 times since 1699. Historical eruptions of the <span class="hlt">volcano</span> consisted mainly of relatively quiescent emplacement of lava flows or minor explosions that generated modest tephra falls (erupted fragments of microscopic ash to meter sized blocks that are dispersed into the atmosphere and fall to the ground). Little is known, however, about prehistoric eruptions of the <span class="hlt">volcano</span>. Chemical analyses of prehistoric lava flows and thin tephra falls from San Miguel <span class="hlt">volcano</span> indicate that the <span class="hlt">volcano</span> is composed dominantly of basalt (rock having silica content</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://ngmdb.usgs.gov/Prodesc/proddesc_80649.htm','USGSPUBS'); return false;" href="http://ngmdb.usgs.gov/Prodesc/proddesc_80649.htm"><span>Preliminary Geologic Map of Mount Pagan <span class="hlt">Volcano</span>, Pagan Island, Commonwealth of the Northern Mariana Islands</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Trusdell, Frank A.; Moore, Richard B.; Sako, Maurice K.</p> <p>2006-01-01</p> <p>Pagan Island is the subaerial portion of two adjoining Quaternary stratovolcanoes near the middle of the <span class="hlt">active</span> Mariana Arc, [FAT1]north of Saipan. Pagan and the other volcanic islands that constitute part of the Arc form the northern half of the East Mariana Ridge[FAT2], which extends about 2-4 km above the ocean floor. The > 6-km-deep Mariana Trench adjoins the East Mariana Ridge on the east, and the Mariana Trough, partly filled with young lava flows and volcaniclastic sediment, lies on the west of the Northern Mariana Islands (East Mariana Ridge. The <span class="hlt">submarine</span> West Mariana Ridge, Tertiary in age, bounds the western side of the Mariana Trough. The Mariana Trench and Northern Mariana Islands (East Mariana Ridge) overlie an <span class="hlt">active</span> subduction zone where the Pacific Plate, moving northwest at about 10.3 cm/year, is passing beneath the Philippine Plate, moving west-northwest at 6.8 cm/year. Beneath the Northern Mariana Islands, earthquake hypocenters at depths of 50-250 km identify the location of the west-dipping subduction zone, which farther west becomes nearly vertical and extends to 700 km depth. During the past century, more than 40 earthquakes of magnitude 6.5-8.1 have shaken the Mariana Trench. The Mariana Islands form two sub-parallel, concentric, concave-west arcs. The southern islands comprise the outer arc and extend north from Guam to Farallon de Medinilla. They consist of Eocene to Miocene volcanic rocks and uplifted Tertiary and Quaternary limestone. The nine northern islands extend from Anatahan to Farallon de Pajaros and form part of the inner arc. The <span class="hlt">active</span> inner arc extends south from Anatahan, where <span class="hlt">volcanoes</span>, some of which are <span class="hlt">active</span>, form seamounts west of the older outer arc. Other volcanic seamounts of the <span class="hlt">active</span> arc surmount the East Mariana Ridge in the vicinity of Anatahan and Sarigan and north and south of Farallon de Pajaros. Six <span class="hlt">volcanoes</span> (Farallon de Pajaros, Asuncion, Agrigan, Mount Pagan, Guguan, and Anatahan) in the northern islands</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFM.V11B..02T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFM.V11B..02T"><span>A Magma Genesis Model to Explain Growth History of Hawaiian <span class="hlt">Volcanoes</span>: Perspectives of 2001-2002 JAMSTEC Hawaii Cruises</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takahashi, E.</p> <p>2003-12-01</p> <p>The 2001 and 2002 JAMSTEC Hawaii cruises have been carried out using RV-Kairei with ROV-Kaiko and RV-Yokosuka with submersible Shinaki-6500, respectively. The main focus of these cruises is 1) to clarify the growth history of Hawaiian <span class="hlt">volcanoes</span> through geological study on deep <span class="hlt">submarine</span> exposures, 2) to understand the nature of <span class="hlt">submarine</span> rifts, 3) to understand the nature of magmas erupted on the deep ocean floor away from the center of the Hawaiian plume. The geologic reconstruction of gigantic landslides (Moore et al., 1989) provided opportunities to study the long-term growth history of Hawaiian <span class="hlt">volcanoes</span>, approaches complimentary to those by HSDP. Using this approach, we studied the growth histories of Kilauea (Lipman et al., 2002), Koolau (Moore & Clague, 2002; Yokose, 2002), and Mauna Loa (Yokose et al, this conference). The geochemical reconstruction of Koolau <span class="hlt">volcano</span> showed a secular variation in basalt magma types; from Kilauea-like to Mauna Loa-like and finally the silica-rich Koolau-type tholeiites (Shinozaki et al. 2002). These chemical changes are associated with significant changes in Sr, Nd and Pb isotopes (Tanaka et al., 2002). Similar changes in basalt magma types have been found in the growth history of Haleakala <span class="hlt">volcano</span> (Ren et al., 2003) and in HSDP cores representing the growth history of Mauna Kea. Accordingly, it is plausible that the basalt magma types found among Hawaiian shield <span class="hlt">volcanoes</span> are not representing geographic trends (e.g., Kea-trend and Loa trend) but are representing different growth stages. In order to elucidate secular changes in the geochemistry of Hawaiian <span class="hlt">volcanoes</span> newly revealed by this project, I have carried out high-pressure melting studies at 2-3 GPa with eclogite/peridotite composite starting materials (experimental detail will be given by Takahashi, this conference V03). In eclogite/peridotite reactive melting, magmas produced above the solidus of peridotite (1480C at 2.8 GPa) are silica deficient alkalic picrites</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030510','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030510"><span>Isotope geochemistry of early Kilauea magmas from the <span class="hlt">submarine</span> Hilina bench: The nature of the Hilina mantle component</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kimura, Jun-Ichi; Sisson, Thomas W.; Nakano, Natsuko; Coombs, Michelle L.; Lipman, Peter W.</p> <p>2006-01-01</p> <p><span class="hlt">Submarine</span> lavas recovered from the Hilina bench region, offshore Kilauea, Hawaii Island provide information on ancient Kilauea <span class="hlt">volcano</span> and the geochemical components of the Hawaiian hotspot. Alkalic lavas, including nephelinite, basanite, hawaiite, and alkali basalt, dominate the earliest stage of Kilauea magmatism. Transitional basalt pillow lavas are an intermediate phase, preceding development of the voluminous tholeiitic subaerial shield and <span class="hlt">submarine</span> Puna Ridge. Most alkalic through transitional lavas are quite uniform in Sr–Nd–Pb isotopes, supporting the interpretation that variable extent partial melting of a relatively homogeneous source was responsible for much of the geochemical diversity of early Kilauea magmas (Sisson et al., 2002). These samples are among the highest 206Pb/204Pb known from Hawaii and may represent melts from a distinct geochemical and isotopic end-member involved in the generation of most Hawaiian tholeiites. This end-member is similar to the postulated literature Kea component, but we propose that it should be renamed Hilina, to avoid confusion with the geographically defined Kea-trend <span class="hlt">volcanoes</span>. Isotopic compositions of some shield-stage Kilauea tholeiites overlap the Hilina end-member but most deviate far into the interior of the isotopic field defined by magmas from other Hawaiian <span class="hlt">volcanoes</span>, reflecting the introduction of melt contributions from both “Koolau” (high 87Sr/86Sr, low 206Pb/204Pb) and depleted (low 87Sr/86Sr, intermediate 206Pb/204Pb) source materials. This shift in isotopic character from nearly uniform, end-member, and alkalic, to diverse and tholeiitic corresponds with the major increase in Kilauea's magmatic productivity. Two popular geodynamic models can account for these relations: (1) The upwelling mantle source could be concentrically zoned in both chemical/isotopic composition, and in speed/extent of upwelling, with Hilina (and Loihi) components situated in the weakly ascending margins and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2001/0457/pdf/of2001-0457.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2001/0457/pdf/of2001-0457.pdf"><span>Lahar Hazards at Concepción <span class="hlt">volcano</span>, Nicaragua</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Vallance, J.W.; Schilling, S.P.; Devoli, G.; Howell, M.M.</p> <p>2001-01-01</p> <p>Concepción is one of Nicaragua’s highest and most <span class="hlt">active</span> <span class="hlt">volcanoes</span>. The symmetrical cone occupies the northeastern half of a dumbbell shaped island called Isla Ometepa. The dormant <span class="hlt">volcano</span>, Maderas, occupies the southwest half of the island. A narrow isthmus connects Concepción and Maderas <span class="hlt">volcanoes</span>. Concepción <span class="hlt">volcano</span> towers more than 1600 m above Lake Nicaragua and is within 5 to 10 km of several small towns situated on its aprons at or near the shoreline. These towns have a combined population of nearly 5,000. The <span class="hlt">volcano</span> has frequently produced debris flows (watery flows of mud, rock, and debris—also known as lahars when they occur on a <span class="hlt">volcano</span>) that could inundate these nearby populated areas. Concepción <span class="hlt">volcano</span> has erupted more than 25 times in the last 120 years. Its first recorded <span class="hlt">activity</span> was in AD 1883. Eruptions in the past century, most of which have originated from a small summit crater, comprise moderate explosions, ash that falls out of eruption plumes (called tephra), and occasional lava flows. Near the summit area, there are accumulations of rock that were emplaced hot (pyroclastic deposits), most of which were hot enough to stick together during deposition (a process called welding). These pyroclastic rocks are rather weak, and tend to break apart easily. The loose volcanic rock remobilizes during heavy rain to form lahars. Volcanic explosions have produced blankets of tephra that are distributed downwind, which on Isla Ometepe is mostly to the west. Older deposits at the west end of the island that are up to 1 m thick indicate larger explosive events have happened at Concepción <span class="hlt">volcano</span> in prehistoric time. Like pyroclastic-flow deposits, loose tephra on the steep slopes of the <span class="hlt">volcano</span> provides source material that heavy rainstorms and earthquakes can mobilize to trigger debris flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA502638','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA502638"><span>Automated Quantification of Gradient Defined Features</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2008-09-01</p> <p>defined features in <span class="hlt">submarine</span> environments. The technique utilizes MATLAB scripts to convert bathymetry data into a gradient dataset, produce gradient...maps, and most importantly, automate the process of defining and characterizing gradient defined features such as flows, faults, landslide scarps, folds...convergent plate margin hosts a series of large serpentinite mud <span class="hlt">volcanoes</span> (Fig. 1). One of the largest of these <span class="hlt">active</span> mud <span class="hlt">volcanoes</span> is Big Blue</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70182800','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70182800"><span>Renewed unrest at Mount Spurr <span class="hlt">Volcano</span>, 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>Power, John A.</p> <p>2004-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO),a cooperative program of the U.S. Geological Survey, the University of Alaska Fairbanks Geophysical Institute, and the Alaska Division of Geological and Geophysical Surveys, has detected unrest at Mount Spurr <span class="hlt">volcano</span>, located about 125 km west of Anchorage, Alaska, at the northeast end of the Aleutian volcanic arc.This <span class="hlt">activity</span> consists of increased seismicity melting of the summit ice cap, and substantial rates of C02 and H2S emission.The current unrest is centered beneath the <span class="hlt">volcano</span>'s 3374-m-high summit, whose last known eruption was 5000–6000 years ago. Since then, Crater Peak, 2309 m in elevation and 4 km to the south, has been the <span class="hlt">active</span> vent. Recent eruptions occurred in 1953 and 1992.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850015262&hterms=Volcanic+eruptions&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DVolcanic%2Beruptions','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850015262&hterms=Volcanic+eruptions&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DVolcanic%2Beruptions"><span><span class="hlt">Submarine</span> Volcanic Eruptions and Potential Analogs for Venus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wilson, L.; Mouginismark, P. J.; Fryer, P.; Gaddis, L. R.</p> <p>1985-01-01</p> <p>As part of an analysis program to better understand the diversity of volcanic processes on the terrestrial planets, an investigation of the volcanic landforms which exist on the Earth's ocean floor was initiated. In part, this analysis is focused toward gaining a better understanding of <span class="hlt">submarine</span> volcanic landforms in their own right, but also it is hoped that these features may show similarities to volcanic landforms on Venus, due to the high ambient water (Earth) and atmospheric (Venus) pressures. A series of numerical modelling experiments was performed to investigate the relative importance of such attributes as water pressure and temperature on the eruption process, and to determine the rate of cooling and emplacement of lava flows in the <span class="hlt">submarine</span> environment. Investigations to date show that the confining water pressure and the buoyancy effects of the surrounding water significantly affect the styles of volcanism on the ocean floor. In the case of Venusian volcanism, confining pressures will not be as great as that found at the ocean's abyssal plains, but nevertheless the general trend toward reducing magma vesiculation will hold true for Venus as well as the ocean floor. Furthermore, other analogs may also be found between <span class="hlt">submarine</span> volcanism and Venusian <span class="hlt">activity</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..324..156L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..324..156L"><span>Evidence of recent deep magmatic <span class="hlt">activity</span> at Cerro Bravo-Cerro Machín volcanic complex, central Colombia. Implications for future volcanic <span class="hlt">activity</span> at Nevado del Ruiz, Cerro Machín and other <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Londono, John Makario</p> <p>2016-09-01</p> <p>In the last nine years (2007-2015), the Cerro Bravo-Cerro Machín volcanic complex (CBCMVC), located in central Colombia, has experienced many changes in volcanic <span class="hlt">activity</span>. In particular at Nevado del Ruiz <span class="hlt">volcano</span> (NRV), Cerro Machin <span class="hlt">volcano</span> (CMV) and Cerro Bravo (CBV) <span class="hlt">volcano</span>. The recent <span class="hlt">activity</span> of NRV, as well as increasing seismic <span class="hlt">activity</span> at other volcanic centers of the CBCMVC, were preceded by notable changes in various geophysical and geochemical parameters, that suggests renewed magmatic <span class="hlt">activity</span> is occurring at the volcanic complex. The onset of this <span class="hlt">activity</span> started with seismicity located west of the volcanic complex, followed by seismicity at CBV and CMV. Later in 2010, strong seismicity was observed at NRV, with two small eruptions in 2012. After that, seismicity has been observed intermittently at other volcanic centers such as Santa Isabel, Cerro España, Paramillo de Santa Rosa, Quindío and Tolima <span class="hlt">volcanoes</span>, which persists until today. Local deformation was observed from 2007 at NRV, followed by possible regional deformation at various volcanic centers between 2011 and 2013. In 2008, an increase in CO2 and Radon in soil was observed at CBV, followed by a change in helium isotopes at CMV between 2009 and 2011. Moreover, SO2 showed an increase from 2010 at NRV, with values remaining high until the present. These observations suggest that renewed magmatic <span class="hlt">activity</span> is currently occurring at CBCMVC. NRV shows changes in its <span class="hlt">activity</span> that may be related to this new magmatic <span class="hlt">activity</span>. NRV is currently exhibiting the most <span class="hlt">activity</span> of any <span class="hlt">volcano</span> in the CBCMVC, which may be due to it being the only open volcanic system at this time. This suggests that over the coming years, there is a high probability of new unrest or an increase in volcanic <span class="hlt">activity</span> of other <span class="hlt">volcanoes</span> of the CBCMVC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BVol...80...47D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BVol...80...47D"><span>Risk perception at a persistently <span class="hlt">active</span> <span class="hlt">volcano</span>: warnings and trust at Popocatépetl <span class="hlt">volcano</span> in Mexico, 2012-2014</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Donovan, Amy; Ayala, Irasema Alcántara; Eiser, J. R.; Sparks, R. S. J.</p> <p>2018-05-01</p> <p>This paper presents data from an online survey carried out in Mexico from 2012 to 2014. The survey focussed on the risk to Mexico City from Popocatépetl, an <span class="hlt">active</span> <span class="hlt">volcano</span> 60 km from the city. During the time period, volcanic <span class="hlt">activity</span> was variable, and the alert level changed accordingly. The survey showed that people surveyed at the higher alert level were generally more concerned about the <span class="hlt">volcano</span>. Since these people were measured separately from those who responded at the lower alert level and yet self-reported on the same scale as more concerned, this provides a useful indicator that the raised alert level may be associated with higher risk perception, and that alert level systems act as boundary objects in the translation of scientific information. In general, trust in various groups was most strongly explained by the perceived knowledge of the groups, followed by their perceived motivation (whether or not they are viewed as working in society's interest), with accuracy a tertiary concern. Some respondents were anxious about false alarms—these people also tended to be concerned about scientific accuracy while those who favoured precaution tended to be more trusting. The perceived effectiveness of warning and evacuation plans was also a significant predictor for trust in official groups. In general, the results suggest that there are important links between trust, warning plans and the perceived motivation of particular groups as well as between trust and perceived knowledge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhyW...30g..40W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhyW...30g..40W"><span>Spying on <span class="hlt">volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watson, Matthew</p> <p>2017-07-01</p> <p><span class="hlt">Active</span> <span class="hlt">volcanoes</span> can be incredibly dangerous, especially to those who live nearby, but how do you get close enough to observe one in action? Matthew Watson explains how artificial drones are providing volcanologists with insights that could one day save human lives</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5967V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5967V"><span>Implications of new stratigraphic data on volcanic hazard assessment for Nisyros <span class="hlt">volcano</span>, Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Volentik, A.; Vanderkluysen, L.; Principe, C.; Hernandez, J.; Hunziker, J. C.</p> <p>2003-04-01</p> <p>The <span class="hlt">active</span> quaternary Nisyros <span class="hlt">volcano</span>, at the eastern end of the Aegean volcanic arc, is composed of a succession of lava flows, tephra layers and interbedded epiclastic deposits. The <span class="hlt">volcano</span> is topped by a recent caldera, on average 4 km in diameter and 200 m in depth. A detailed geological map including 35 stratigraphic units (lava flows, tephra layers and epiclastic deposits) has been recently completed at the 1:10'000 scale, based on new stratigraphical data. Based on the identification of new plinian sequences (Lakki and Melisseri pyroclastic series) in the lowermost section of the reconstructed stratigraphical succession, on the re-interpretation of previously described deposits and on the discovery of eruptive facies, we construct a set of hazard maps for volcanic events at Nisyros. Sequences of <span class="hlt">sub-marine</span> lavas to subaerial epiclastites combined with the occurrence of a marine terrace deposit in the north-western sector of the island highlight the potential for rapid vertical movements, in particular in the area of Mandraki. A period of intense off-centred strombolian to phreatomagmatic <span class="hlt">activity</span> occurred in quite recent times on Nisyros along the major tectonic trends (N^o030, No070, N^o120 and N^o340), building up several scoria cones and tuff cones all around the island. A number of these tectonic trends are still <span class="hlt">active</span>, as demonstrated by faults cutting through recent deposits (including the youngest deposits of the hydrothermal eruptions, inside the present caldera of Nisyros). This implies that not only intra-caldera phreatic eruptions, but also potential magmatic eruption may occur along the island’s major zones of weakness, with increased hazards where magma/water interaction may take place. Finally a newly recognized debris avalanche deposit (the so-called Vunàri debris avalanche), affecting a wide sector in the northern part of the island, unveils a new type of volcanic hazard on Nisyros, related to flank collapse and destruction of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1412231C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1412231C"><span>Attaining high-resolution eruptive histories for <span class="hlt">active</span> arc <span class="hlt">volcanoes</span> with argon geochronology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calvert, A. T.</p> <p>2012-04-01</p> <p>Geochronology of <span class="hlt">active</span> arc <span class="hlt">volcanoes</span> commonly illuminates eruptive behavior over tens to hundreds of thousands of years, lengthy periods of repose punctuated by short eruptive episodes, and spatial and compositional changes with time. Despite the >1 Gyr half-life of 40K, argon geochronology is an exceptional tool for characterizing Pleistocene to Holocene eruptive histories and for placing constraints on models of eruptive behavior. Reliable 40Ar/39Ar ages of calc-alkaline arc rocks with rigorously derived errors small enough (± 500 to 3,000 years) to constrain eruptive histories are attainable using careful procedures. Sample selection and analytical work in concert with geologic mapping and stratigraphic studies are essential for determining reliable eruptive histories. Preparation, irradiation and spectrometric techniques have all been optimized to produce reliable, high-precision results. Examples of Cascade and Alaska/Aleutian eruptive histories illustrating duration of <span class="hlt">activity</span> from single centers, eruptive episodicity, and spatial and compositional changes with time will be presented: (1) Mt. Shasta, the largest Cascade stratovolcano, has a 700,000-year history (Calvert and Christiansen, 2011 Fall AGU). A similar sized and composition <span class="hlt">volcano</span> (Rainbow Mountain) on the Cascade axis was <span class="hlt">active</span> 1200-950 ka. The eruptive center then jumped west 15 km to the south flank of the present Mt. Shasta and produced a stratovolcano from 700-450 ka likely rivaling today's Mt. Shasta. The NW portion of that edifice failed in an enormous (>30 km3) debris avalanche. Vents near today's <span class="hlt">active</span> summit erupted 300-135 ka, then 60-15 ka. A voluminous, but short-lived eruptive sequence occurred at 11 ka, including a summit explosion producing a subplinian plume, followed by >60 km3 andesite-dacite Shastina domes and flows, then by the flank dacite Black Butte dome. Holocene domes and flows subsequently rebuilt the summit and flowed to the north and east. (2) Mt. Veniaminof on</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997806','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3997806"><span>On the fate of pumice rafts formed during the 2012 Havre <span class="hlt">submarine</span> 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>Jutzeler, Martin; Marsh, Robert; Carey, Rebecca J.; White, James D. L.; Talling, Peter J.; Karlstrom, Leif</p> <p>2014-01-01</p> <p>Pumice rafts are floating mobile accumulations of low-density pumice clasts generated by silicic volcanic eruptions. Pumice in rafts can drift for years, become waterlogged and sink, or become stranded on shorelines. Here we show that the pumice raft formed by the impressive, deep <span class="hlt">submarine</span> eruption of the Havre caldera <span class="hlt">volcano</span> (Southwest Pacific) in July 2012 can be mapped by satellite imagery augmented by sailing crew observations. Far from coastal interference, the eruption produced a single >400 km2 raft in 1 day, thus initiating a gigantic, high-precision, natural experiment relevant to both modern and prehistoric oceanic surface dispersal dynamics. Observed raft dispersal can be accurately reproduced by simulating drift and dispersal patterns using currents from an eddy-resolving ocean model hindcast. For future eruptions that produce potentially hazardous pumice rafts, our technique allows real-time forecasts of dispersal routes, in addition to inference of ash/pumice deposit distribution in the deep ocean. PMID:24755668</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5706G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5706G"><span>Transition from phreatic to phreatomagmatic explosive <span class="hlt">activity</span> of Zhupanovsky <span class="hlt">volcano</span> (Kamchatka) in 2013-2016 due to volcanic cone collapse</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gorbach, Natalia; Plechova, Anastasiya; Portnyagin, Maxim</p> <p>2017-04-01</p> <p>Zhupanovsky <span class="hlt">volcano</span>, situated 70 km north from Petropavlovsk-Kamchatsky city, resumed its <span class="hlt">activity</span> in October 2013 [3]. In 2014 and in the first half of 2015, episodic explosions with ash plumes rising up to 6-8 km above sea level occurred on Priemish cone - one of four cones on the Zhupanovsky volcanic edifice [1]. In July 2015 after a series of seismic and explosive events, the southern sector of the <span class="hlt">active</span> cone collapsed. The landslide and lahar deposits resulted from the collapse formed a large field on the <span class="hlt">volcano</span> slopes [2]. In November 2015 and January-March 2016, a series of powerful explosions took place sending ash up to 8-10 km above sea level. No pure magmatic, effusive or extrusive, <span class="hlt">activity</span> has been observed on Zhupanovsky in 2013-2016. We have studied the composition, morphology and textural features of ash particles produced by the largest explosive events of Zhupanovsky in the period from October 2013 to March 2016. The main components of the ash were found to be hydrothermally altered particles and lithics, likely originated by the defragmentation of rocks composing the volcanic edifice. Juvenile glass fragments occur in very subordinate quantities. The maximum amount of glass particles (up to 7%) was found in the ash erupted in January-March 2016, after the cone collapse. We suggest that the phreatic to phreatomagmatic explosive <span class="hlt">activity</span> of Zhupanovsky <span class="hlt">volcano</span> in 2013-2016 was initially caused by the intrusion of a new magma batch under the <span class="hlt">volcano</span>. The intrusion and associated degassing of magma led to heating, overpressure and instability in the hydrothermal system of the <span class="hlt">volcano</span>, causing episodic, predominantly phreatic explosions. Decompression of the shallow magmatic and hydrothermal system of the <span class="hlt">volcano</span> due to the cone collapse in July 2015 facilitated a larger involvement of the magmatic component in the eruption and more powerful explosions. [1] Girina O.A. et al., 2016 Geophysical Research Abstracts Vol. 18, EGU2016-2101, doi: 10</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.V43B2855C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.V43B2855C"><span>Monitoring <span class="hlt">volcano</span> <span class="hlt">activity</span> through Hidden Markov Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cassisi, C.; Montalto, P.; Prestifilippo, M.; Aliotta, M.; Cannata, A.; Patanè, D.</p> <p>2013-12-01</p> <p>During 2011-2013, Mt. Etna was mainly characterized by cyclic occurrences of lava fountains, totaling to 38 episodes. During this time interval Etna <span class="hlt">volcano</span>'s states (QUIET, PRE-FOUNTAIN, FOUNTAIN, POST-FOUNTAIN), whose automatic recognition is very useful for monitoring purposes, turned out to be strongly related to the trend of RMS (Root Mean Square) of the seismic signal recorded by stations close to the summit area. Since RMS time series behavior is considered to be stochastic, we can try to model the system generating its values, assuming to be a Markov process, by using Hidden Markov models (HMMs). HMMs are a powerful tool in modeling any time-varying series. HMMs analysis seeks to recover the sequence of hidden states from the observed emissions. In our framework, observed emissions are characters generated by the SAX (Symbolic Aggregate approXimation) technique, which maps RMS time series values with discrete literal emissions. The experiments show how it is possible to guess <span class="hlt">volcano</span> states by means of HMMs and SAX.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034455p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034455p/"><span>35. INTERIOR VIEW OF EQUIPMENT HOUSE, <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK, ...</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>35. INTERIOR VIEW OF EQUIPMENT HOUSE, <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK, PRIOR TO ENLARGEMENT OF ROOM AND INSTALLATION OF TRIPLE-LOCK RECOMPRESSION CHAMBER IN 1957 - U.S. Naval <span class="hlt">Submarine</span> Base, New London <span class="hlt">Submarine</span> Escape Training Tank, Albacore & Darter Roads, Groton, New London County, CT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034451p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034451p/"><span>31. VIEW OF <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK DURING CONSTRUCTION OF ...</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>31. VIEW OF <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK DURING CONSTRUCTION OF THE ELEVATOR AND PASSAGEWAYS TO THE 18- AND 50-FOOT LOCKS AND CUPOLA 1932 - U.S. Naval <span class="hlt">Submarine</span> Base, New London <span class="hlt">Submarine</span> Escape Training Tank, Albacore & Darter Roads, Groton, New London County, CT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5698251-geology-kilauea-volcano','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5698251-geology-kilauea-volcano"><span>Geology of Kilauea <span class="hlt">volcano</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>Moore, R.B.; Trusdell, F.A.</p> <p>1993-08-01</p> <p>This paper summarizes studies of the structure, stratigraphy, petrology, drill holes, eruption frequency, and volcanic and seismic hazards of Kilauea <span class="hlt">volcano</span>. All the <span class="hlt">volcano</span> is discussed, but the focus is on its lower east rift zone (LERZ) because <span class="hlt">active</span> exploration for geothermal energy is concentrated in that area. Kilauea probably has several separate hydrothermal-convection systems that develop in response to the dynamic behavior of the <span class="hlt">volcano</span> and the influx of abundant meteoric water. Important features of some of these hydrothermal-convection systems are known through studies of surface geology and drill holes. Observations of eruptions during the past two centuries, detailedmore » geologic mapping, radiocarbon dating, and paleomagnetic secular-variation studies indicate that Kilauea has erupted frequently from its summit and two radial rift zones during Quaternary time. Petrologic studies have established that Kilauea erupts only tholeiitic basalt. Extensive ash deposits at Kilauea's summit and on its LERZ record locally violent, but temporary, disruptions of local hydrothermal-convection systems during the interaction of water or steam with magma. Recent drill holes on the LERZ provide data on the temperatures of the hydrothermal-convection systems, intensity of dike intrusion, porosity and permeability, and an increasing amount of hydrothermal alteration with depth. The prehistoric and historic record of volcanic and seismic <span class="hlt">activity</span> indicates that magma will continue to be supplied to deep and shallow reservoirs beneath Kilauea's summit and rift zones and that the <span class="hlt">volcano</span> will be affected by eruptions and earthquakes for many thousands of years. 71 refs., 2 figs.« less</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('http://adsabs.harvard.edu/abs/2017AGUFM.S13B0668B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S13B0668B"><span>Swarms of small <span class="hlt">volcano</span>-tectonic events preceding paroxysmal explosions of Tungurahua <span class="hlt">volcano</span> (Ecuador)</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.; Hidalgo, S.; Douchain, J. M.; Pacheco, D. A.; Cordova, J.; Alvarado, A. P.; Parra, R.</p> <p>2017-12-01</p> <p>Tungurahua (5023 m a.s.l.) is an andesitic <span class="hlt">volcano</span> located in Central Ecuador. It has been erupting since September 1999. It's <span class="hlt">activity</span> transitioned in late 2008 towards the occurrence of distinct eruptive phases separated by periods of quiescence. These phases display a great variability of eruptive patterns. In particular the onsets of these phases are quite variable, ranging from progressive increase of surface <span class="hlt">activity</span> to violent paroxysmal explosions eventually generating pyroclastic flows and plumes up to 13.000 m elevation. The <span class="hlt">volcano</span> is monitored by the Instituto Geofisico in Quito whose permanent monitoring network include 6 broadband and 6 short period stations. These instruments record various signals related to eruptive processes as well as Long Period and <span class="hlt">volcano</span>-tectonique (VT) events. However, most of the VT events are scattered around the <span class="hlt">volcano</span> at depths up to 5-10 km b.s.l.. Their relationship with eruptive <span class="hlt">activity</span> and precursory aspect are unclear. Since October 2013, we operate a temporary network of 13 broadband stations located up to 4275 m a.s.l., including on the Eastern flank which is remote. We examined data from a reference station located near the summit (3900 m a.s.l.) with a detection and classification procedure, searching for families of similar events. This processing enlights the presence of several families of small VTs previously poorly identified. We located manually some of these events and proceeded with similarity picking using cross-correlation and waveform similarity for nearly 400 events. Finally we applied precise relocation techniques. These events are located 2-3 km below the summit and define vertically elongated streaks. Their temporal evolution shows that they occur in swarms during the days or hours preceding the paroxysmal vent opening explosions in February and April 2014. These short-term precursors could indicate the rupturing of a barrier prior to the large explosions of Tungurahua.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA01722&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmajor%2Bdepression','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA01722&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmajor%2Bdepression"><span>Space Radar Image of Colombian <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1999-01-01</p> <p>This is a radar image of a little known <span class="hlt">volcano</span> in northern Colombia. The image was acquired on orbit 80 of space shuttle Endeavour on April 14, 1994, by the Spaceborne Imaging Radar C/X-Band Synthetic Aperture Radar (SIR-C/X-SAR). The <span class="hlt">volcano</span> near the center of the image is located at 5.6 degrees north latitude, 75.0 degrees west longitude, about 100 kilometers (65 miles) southeast of Medellin, Colombia. The conspicuous dark spot is a lake at the bottom of an approximately 3-kilometer-wide (1.9-mile) volcanic collapse depression or caldera. A cone-shaped peak on the bottom left (northeast rim) of the caldera appears to have been the source for a flow of material into the caldera. This is the northern-most known <span class="hlt">volcano</span> in South America and because of its youthful appearance, should be considered dormant rather than extinct. The <span class="hlt">volcano</span>'s existence confirms a fracture zone proposed in 1985 as the northern boundary of volcanism in the Andes. The SIR-C/X-SAR image reveals another, older caldera further south in Colombia, along another proposed fracture zone. Although relatively conspicuous, these <span class="hlt">volcanoes</span> have escaped widespread recognition because of frequent cloud cover that hinders remote sensing imaging in visible wavelengths. Four separate <span class="hlt">volcanoes</span> in the Northern Andes nations ofColombia and Ecuador have been <span class="hlt">active</span> during the last 10 years, killing more than 25,000 people, including scientists who were monitoring the volcanic <span class="hlt">activity</span>. Detection and monitoring of <span class="hlt">volcanoes</span> from space provides a safe way to investigate volcanism. The recognition of previously unknown <span class="hlt">volcanoes</span> is important for hazard evaluations because a number of major eruptions this century have occurred at mountains that were not previously recognized as <span class="hlt">volcanoes</span>. Spaceborne Imaging Radar-C and X-band Synthetic Aperture Radar (SIR-C/X-SAR) is part of NASA's Mission to Planet Earth. The radars illuminate Earth with microwaves allowing detailed observations at any time, regardless of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43.8511D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43.8511D"><span>Single-station monitoring of <span class="hlt">volcanoes</span> using seismic ambient noise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Plaen, Raphael S. M.; Lecocq, Thomas; Caudron, Corentin; Ferrazzini, Valérie; Francis, Olivier</p> <p>2016-08-01</p> <p>Seismic ambient noise cross correlation is increasingly used to monitor volcanic <span class="hlt">activity</span>. However, this method is usually limited to <span class="hlt">volcanoes</span> equipped with large and dense networks of broadband stations. The single-station approach may provide a powerful and reliable alternative to the classical "cross-station" approach when measuring variation of seismic velocities. We implemented it on the Piton de la Fournaise in Reunion Island, a very <span class="hlt">active</span> <span class="hlt">volcano</span> with a remarkable multidisciplinary continuous monitoring. Over the past decade, this <span class="hlt">volcano</span> has been increasingly studied using the traditional cross-correlation technique and therefore represents a unique laboratory to validate our approach. Our results, tested on stations located up to 3.5 km from the eruptive site, performed as well as the classical approach to detect the volcanic eruption in the 1-2 Hz frequency band. This opens new perspectives to successfully forecast volcanic <span class="hlt">activity</span> at <span class="hlt">volcanoes</span> equipped with a single three-component seismometer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2004/1234/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2004/1234/"><span>Catalog of earthquake hypocenters at Alaskan <span class="hlt">volcanoes</span>: January 1 through December 31, 2003</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dixon, James P.; Stihler, Scott D.; Power, John A.; Tytgat, Guy; Moran, Seth C.; Sanchez, John J.; McNutt, Stephen R.; Estes, Steve; Paskievitch, John</p> <p>2004-01-01</p> <p>The Alaska <span class="hlt">Volcano</span> Observatory (AVO), a cooperative program of the U.S. Geological Survey, the Geophysical Institute of the University of Alaska Fairbanks, and the Alaska Division of Geological and Geophysical Surveys, has maintained seismic monitoring networks at historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Alaska since 1988. The primary objectives of this program are the near real time seismic monitoring of <span class="hlt">active</span>, potentially hazardous, Alaskan <span class="hlt">volcanoes</span> and the investigation of seismic processes associated with <span class="hlt">active</span> volcanism. This catalog presents the calculated earthquake hypocenter and phase arrival data, and changes in the seismic monitoring program for the period January 1 through December 31, 2003.The AVO seismograph network was used to monitor the seismic <span class="hlt">activity</span> at twenty-seven <span class="hlt">volcanoes</span> within Alaska in 2003. These include Mount Wrangell, Mount Spurr, Redoubt <span class="hlt">Volcano</span>, Iliamna <span class="hlt">Volcano</span>, Augustine <span class="hlt">Volcano</span>, Katmai volcanic cluster (Snowy Mountain, Mount Griggs, Mount Katmai, Novarupta, Trident <span class="hlt">Volcano</span>, Mount Mageik, Mount Martin), Aniakchak Crater, Mount Veniaminof, Pavlof <span class="hlt">Volcano</span>, Mount Dutton, Isanotski Peaks, Shishaldin <span class="hlt">Volcano</span>, Fisher Caldera, Westdahl Peak, Akutan Peak, Makushin <span class="hlt">Volcano</span>, Okmok Caldera, Great Sitkin <span class="hlt">Volcano</span>, Kanaga <span class="hlt">Volcano</span>, Tanaga <span class="hlt">Volcano</span>, and Mount Gareloi. Monitoring highlights in 2003 include: continuing elevated seismicity at Mount Veniaminof in January-April (volcanic unrest began in August 2002), volcanogenic seismic swarms at Shishaldin <span class="hlt">Volcano</span> throughout the year, and low-level tremor at Okmok Caldera throughout the year. Instrumentation and data acquisition highlights in 2003 were the installation of subnetworks on Tanaga and Gareloi Islands, the installation of broadband installations on Akutan <span class="hlt">Volcano</span> and Okmok Caldera, and the establishment of telemetry for the Okmok Caldera subnetwork. AVO located 3911 earthquakes in 2003.This catalog includes: (1) a description of instruments deployed in the field and their locations; (2) a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2001/0455/pdf/of2001-0455.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2001/0455/pdf/of2001-0455.pdf"><span>Lahar hazards at Mombacho <span class="hlt">Volcano</span>, Nicaragua</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Vallance, J.W.; Schilling, S.P.; Devoli, G.</p> <p>2001-01-01</p> <p>Mombacho <span class="hlt">volcano</span>, at 1,350 meters, is situated on the shores of Lake Nicaragua and about 12 kilometers south of Granada, a city of about 90,000 inhabitants. Many more people live a few kilometers southeast of Granada in 'las Isletas de Granada and the nearby 'Peninsula de Aseses. These areas are formed of deposits of a large debris avalanche (a fast moving avalanche of rock and debris) from Mombacho. Several smaller towns with population, in the range of 5,000 to 12,000 inhabitants are to the northwest and the southwest of Mombacho <span class="hlt">volcano</span>. Though the <span class="hlt">volcano</span> has apparently not been <span class="hlt">active</span> in historical time, or about the last 500 years, it has the potential to produce landslides and debris flows (watery flows of mud, rock, and debris -- also known as lahars when they occur on a <span class="hlt">volcano</span>) that could inundate these nearby populated areas. -- Vallance, et.al., 2001</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930004270','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930004270"><span>Chemical environments of <span class="hlt">submarine</span> hydrothermal systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shock, Everett L.</p> <p>1992-01-01</p> <p>Perhaps because black-smoker chimneys make tremendous subjects for magazine covers, the proposal that <span class="hlt">submarine</span> hydrothermal systems were involved in the origin of life has caused many investigators to focus on the eye-catching hydrothermal vents. In much the same way that tourists rush to watch the spectacular eruptions of Old Faithful geyser with little regard for the hydrology of the Yellowstone basin, attention is focused on the spectacular, high-temperature hydrothermal vents to the near exclusion of the enormous underlying hydrothermal systems. Nevertheless, the magnitude and complexity of geologic structures, heat flow, and hydrologic parameters which characterize the geyser basins at Yellowstone also characterize <span class="hlt">submarine</span> hydrothermal systems. However, in the <span class="hlt">submarine</span> systems the scale can be considerably more vast. Like Old Faithful, <span class="hlt">submarine</span> hydrothermal vents have a spectacular quality, but they are only one fascinating aspect of enormous geologic systems operating at seafloor spreading centers throughout all of the ocean basins. A critical study of the possible role of hydrothermal processes in the origin of life should include the full spectrum of probable environments. The goals of this chapter are to synthesize diverse information about the inorganic geochemistry of <span class="hlt">submarine</span> hydrothermal systems, assemble a description of the fundamental physical and chemical attributes of these systems, and consider the implications of high-temperature, fluid-driven processes for organic synthesis. Information about <span class="hlt">submarine</span> hydrothermal systems comes from many directions. Measurements made directly on venting fluids provide useful, but remarkably limited, clues about processes operating at depth. The oceanic crust has been drilled to approximately 2.0 km depth providing many other pieces of information, but drilling technology has not allowed the bore holes and core samples to reach the maximum depths to which aqueous fluids circulate in oceanic crust. Such</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2821P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2821P"><span>Process sedimentology of <span class="hlt">submarine</span> fan deposits - new perspectives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Postma, George</p> <p>2017-04-01</p> <p>To link <span class="hlt">submarine</span> fan process sedimentology with sand distribution, sand body architecture, texture and fabric, the field geologist studies sedimentary facies, facies associations (fan elements) and stratigraphy. Facies analysis resides on factual knowledge of modern fan morphodynamics and physical modelling of en-masse sediment transport. Where do we stand after 55 years of <span class="hlt">submarine</span> research, i.e. the date when the first <span class="hlt">submarine</span> fan model was launched by Arnold Bouma in 1962? Since that date students of <span class="hlt">submarine</span> fans have worked on a number of important, recurring questions concerned with facies analysis of <span class="hlt">submarine</span> successions in outcrop and core: 1. What type of sediment transport produced the beds? 2. What facies can be related to initial flow conditions? 3. What is the significance of grain size jumps and bounding surface hierarchy in beds consisting of crude and spaced stratification (traction carpets)? Do these point to multi flow events or to flow pulsations by one and the same event? 4. What facies associations relate to the basic elements of <span class="hlt">submarine</span> fans? 5. What are the autogenic and allogenic signatures in <span class="hlt">submarine</span> fans? Particularly in the last decade, the enormous technical advancement helped to obtain high-quality data from observations of density flows in modern canyons, deep basins and deep-water delta slopes (refs 1,2,3). In combination with both physical (refs 4,5) and numerical modelling (ref 6) these studies broke new ground into our understanding of density flow processes in various <span class="hlt">submarine</span> environments and have led to new concepts of <span class="hlt">submarine</span> fan building by super- and subcritical high-density flow (ref 7). Do these new concepts provide better answers to our recurrent questions related to the morphodynamics of <span class="hlt">submarine</span> fans and prediction of sand body architecture? In discussing this open question, I shall 1. apply the new concepts to a modern and ancient example of a channel-lobe-transition-zone (ref 8); 2. raise the problem of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA513189','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA513189"><span>Improved <span class="hlt">Submariner</span> Eyewear for Routine Wear and Emergency Equipment Use Underway</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-01-15</p> <p>information. 2.0 DESCRIPTION Naval <span class="hlt">Submarine</span> Medical Research Laboratory (NSMRL) is seeking information from the eyewear industry that will provide...Improved <span class="hlt">Submariner</span> Eyewear for Routine Wear and Emergency Equipment Use Underway by Alison America, MA Wayne G. Horn, MD...<span class="hlt">Submariner</span> Eyewear for Routine Wear and Emergency Equipment Use Underway 50818 Alison America, MA Wayne G. Horn, MD Naval <span class="hlt">Submarine</span> Medical Research</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25163466','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25163466"><span>Banning cigarette smoking on US Navy <span class="hlt">submarines</span>: a case study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lando, Harry A; Michaud, Mark E; Poston, Walker S C; Jahnke, Sara A; Williams, Larry; Haddock, Christopher K</p> <p>2015-10-01</p> <p>The military has had a long pro-tobacco tradition. Despite official policy discouraging smoking, tobacco still is widely seen as part of military culture. While <span class="hlt">active</span> smoking has presented a particular challenge for the military, in recent years there also has been increasing concern with secondhand smoke. This is especially true in closed environments and <span class="hlt">submarines</span> may be deployed for months at a time. The current case study describes the successful implementation by the Navy of a comprehensive ban on smoking aboard <span class="hlt">submarines</span>. The authors searched documents on the internet, popular media, military-based news outlets and the scientific literature. We also conducted interviews with Navy officers who were instrumental in policy implementation. Data demonstrating substantial exposure of non-smokers to tobacco smoke aboard <span class="hlt">submarines</span> had major impact on successful adoption of the policy. A systematic and extended roll out of the ban included establishing a working group, soliciting input and <span class="hlt">active</span> engagement from <span class="hlt">submarine</span> personnel, and offering cessation assistance. Support was enlisted from Chief Petty Officers who could have been strongly opposed but who became strong proponents. Fewer problems were encountered than had been expected. In contrast to a previous unsuccessful attempt by a Navy captain to ban smoking on his ship, the ban was adopted without apparent tobacco industry interference. Lessons learned included the importance of strong empirical support, effective framing of the issue, setting a realistic timeline, soliciting support from key personnel and providing appropriate resources. These lessons have implications for those considering further tobacco policy changes in the military and elsewhere. Published by the BMJ Publishing Group Limited. For permission to use (where not already granted under a licence) please go to http://group.bmj.com/group/rights-licensing/permissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740011839','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740011839"><span>Thermal surveillance of <span class="hlt">active</span> <span class="hlt">volcanoes</span>. [infrared scanner recordings of thermal anomalies of Mt. Baker <span class="hlt">volcano</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Friedman, J. D. (Principal Investigator)</p> <p>1974-01-01</p> <p>The author has identified the following significant results. By the end of 1973, aerial infrared scanner traverses for thermal anomaly recordings of all Cascade Range <span class="hlt">volcanoes</span> were essentially completed. Amplitude level slices of the Mount Baker anomalies were completed and compiled at a scale of 1:24,000, thus producing, for the first time, an accurate map of the distribution and intensity of thermal <span class="hlt">activity</span> on Mount Baker. The major thermal <span class="hlt">activity</span> is concentrated within the crater south of the main summit and although it is characterized by intensive solfataric <span class="hlt">activity</span> and warm ground, it is largely subglacial, causing the development of sizable glacier perforation features. The outgoing radiative flux from the east breach anomalies is sufficient to account for the volume of ice melted to form the glacier perforations. DCP station 6251 has been monitoring a thermally anomalous area on the north slope of Mount Baker. The present thermal <span class="hlt">activity</span> of Mount Baker accounts for continuing hydrothermal alteration in the crater south of the main summit and recurrent debris avalanches from Sherman Peak on its south rim. The infrared anomalies mapped as part of the experiment SR 251 are considered the basic evidence of the subglacial heating which was the probable triggering mechanism of an avalanche down Boulder Glacier on August 20-21, 1973.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title32-vol5/pdf/CFR-2013-title32-vol5-sec707-7.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title32-vol5/pdf/CFR-2013-title32-vol5-sec707-7.pdf"><span>32 CFR 707.7 - <span class="hlt">Submarine</span> identification light.</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>2013-07-01</p> <p>... 32 National Defense 5 2013-07-01 2013-07-01 false <span class="hlt">Submarine</span> identification light. 707.7 Section... RULES WITH RESPECT TO ADDITIONAL STATION AND SIGNAL LIGHTS § 707.7 <span class="hlt">Submarine</span> identification light... off-period. The light will be located where it can best be seen, as near as practicable, all around...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title32-vol5/pdf/CFR-2011-title32-vol5-sec707-7.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title32-vol5/pdf/CFR-2011-title32-vol5-sec707-7.pdf"><span>32 CFR 707.7 - <span class="hlt">Submarine</span> identification light.</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>2011-07-01</p> <p>... 32 National Defense 5 2011-07-01 2011-07-01 false <span class="hlt">Submarine</span> identification light. 707.7 Section... RULES WITH RESPECT TO ADDITIONAL STATION AND SIGNAL LIGHTS § 707.7 <span class="hlt">Submarine</span> identification light... off-period. The light will be located where it can best be seen, as near as practicable, all around...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title32-vol5/pdf/CFR-2014-title32-vol5-sec707-7.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title32-vol5/pdf/CFR-2014-title32-vol5-sec707-7.pdf"><span>32 CFR 707.7 - <span class="hlt">Submarine</span> identification light.</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>2014-07-01</p> <p>... 32 National Defense 5 2014-07-01 2014-07-01 false <span class="hlt">Submarine</span> identification light. 707.7 Section... RULES WITH RESPECT TO ADDITIONAL STATION AND SIGNAL LIGHTS § 707.7 <span class="hlt">Submarine</span> identification light... off-period. The light will be located where it can best be seen, as near as practicable, all around...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title32-vol5/pdf/CFR-2012-title32-vol5-sec707-7.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title32-vol5/pdf/CFR-2012-title32-vol5-sec707-7.pdf"><span>32 CFR 707.7 - <span class="hlt">Submarine</span> identification light.</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>2012-07-01</p> <p>... 32 National Defense 5 2012-07-01 2012-07-01 false <span class="hlt">Submarine</span> identification light. 707.7 Section... RULES WITH RESPECT TO ADDITIONAL STATION AND SIGNAL LIGHTS § 707.7 <span class="hlt">Submarine</span> identification light... off-period. The light will be located where it can best be seen, as near as practicable, all around...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA607055','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA607055"><span>VICTORIA Class <span class="hlt">Submarine</span> Human-in-the-Loop Experimentation Plan</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-06-01</p> <p>1472G. VICTORIA Class <span class="hlt">Submarine</span> Human-in-the-Loop Experimentation Plan and Preliminary Results © Her Majesty the Queen in Right of...19 th International Command and Control Research and Technology Symposium Title: VICTORIA Class <span class="hlt">Submarine</span> Human-in-the-Loop...TYPE 3. DATES COVERED 00-00-2014 to 00-00-2014 4. TITLE AND SUBTITLE VICTORIA Class <span class="hlt">Submarine</span> Human-in-the-Loop Experimentation Plan 5a. CONTRACT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022348','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022348"><span>Spreading <span class="hlt">volcanoes</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>Borgia, A.; Delaney, P.T.; Denlinger, R.P.</p> <p>2000-01-01</p> <p>As <span class="hlt">volcanoes</span> grow, they become ever heavier. Unlike mountains exhumed by erosion of rocks that generally were lithified at depth, <span class="hlt">volcanoes</span> typically are built of poorly consolidated rocks that may be further weakened by hydrothermal alteration. The substrates upon which <span class="hlt">volcanoes</span> rest, moreover, are often sediments lithified by no more than the weight of the volcanic overburden. It is not surprising, therefore, that volcanic deformation includes-and in the long term is often dominated by-spreading motions that translate subsidence near volcanic summits to outward horizontal displacements around the flanks and peripheries. We review examples of volcanic spreading and go on to derive approximate expressions for the time <span class="hlt">volcanoes</span> require to deform by spreading on weak substrates. We also demonstrate that shear stresses that drive low-angle thrust faulting from beneath volcanic constructs have maxima at volcanic peripheries, just where such faults are seen to emerge. Finally, we establish a theoretical basis for experimentally derived scalings that delineate <span class="hlt">volcanoes</span> that spread from those that do not.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.U51A0020A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.U51A0020A"><span>Scientific Ocean Drilling to Assess <span class="hlt">Submarine</span> Geohazards along European Margins</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ask, M. V.; Camerlenghi, A.; Kopf, A.; Morgan, J. K.; Ocean DrillingSeismic Hazard, P. E.</p> <p>2008-12-01</p> <p><span class="hlt">Submarine</span> geohazards are some of the most devastating natural events in terms of lives lost and economic impact. Earthquakes pose a big threat to society and infrastructure, but the understanding of their episodic generation is incomplete. Tsunamis are known for their potential of striking coastlines world-wide. Other geohazards originating below the sea surface are equally dangerous for undersea structures and the coastal population: <span class="hlt">submarine</span> landslides and volcanic islands collapse with little warning and devastating consequences. The European scientific community has a strong focus on geohazards along European and nearby continental margins, especially given their high population densities, and long historic and prehistoric record of hazardous events. For example, the Mediterranean is surrounded by very densely-populated coastline and is the World's leading holiday destination, receiving up 30% of global tourism. In addition, its seafloor is criss-crossed by hydrocarbon pipelines and telecommunication cables. However, the governing processes and recurrence intervals of geohazards are still poorly understood. Examples include, but are not limited to, earthquakes and volcanic eruptions along the <span class="hlt">active</span> tectonic margins of the Mediterranean and Sea of Marmara, landslides on both <span class="hlt">active</span> and passive margins, and tsunamites and seismites in the sedimentary record that suggest a long history of similar events. The development of geophysical networks, drilling, sampling and long-term monitoring are crucial to the understanding of earthquake, landslide, and tsunami processes, and to mitigate the associated risks in densely populated and industrialized regions such as Europe. Scientific drilling, particularly in the <span class="hlt">submarine</span> setting, offers a unique tool to obtain drill core samples, borehole measurements and long-term observations. Hence, it is a critical technology to investigate past, present, and possible future influences of hazardous processes in this area. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS34A..01P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS34A..01P"><span><span class="hlt">Submarine</span> glacial landforms and interactions with volcanism around Sub-Antarctic Heard and McDonald Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Picard, K.; Watson, S. J.; Fox, J. M.; Post, A.; Whittaker, J. M.; Lucieer, V.; Carey, R.; Coffin, M. F.; Hodgson, D.; Hogan, K.; Graham, A. G. C.</p> <p>2017-12-01</p> <p>Unravelling the glacial history of Sub-Antarctic islands can provide clues to past climate and Antarctic ice sheet stability. The glacial history of many sub-Antarctic islands is poorly understood, including the Heard and McDonald Islands (HIMI) located on the Kerguelen Plateau in the southern Indian Ocean. The geomorphologic development of HIMI has involved a combination of construction via hotspot volcanism and mechanical erosion caused by waves, weather, and glaciers. Today, the 2.5 km2 McDonald Islands are not glacierised; in contrast, the 368 km2 Heard Island has 12 major glaciers, some extending from the summit of 2813 m to sea level. Historical accounts from Heard Island suggest that the glaciers were more extensive in the 1850s to 1870s, and have retreated at least 12% (33.89 km2) since 1997. However, surrounding bathymetry suggests a much more extensive previous glaciation of the HIMI region that encompassed 9,585 km2, likely dating back at least to the Last Glacial Maximum (LGM) ca. 26.5 -19 ka. We present analyses of multibeam bathymetry and backscatter data, acquired aboard RV Investigator in early 2016, that support the previous existence of an extensive icecap. These data reveal widespread ice-marginal and subglacial features including moraines, over-deepened troughs, drumlins and crag-and-tails. Glacial landforms suggest paleo-ice flow directions and a glacial extent that are consistent with previously documented broad scale morphological features. We identify >660 iceberg keel scours in water depths ranging from 150 - 530 m. The orientations of the iceberg keel scours reflect the predominantly east-flowing Antarctic Circumpolar Current and westerly winds in the region. 40Ar/39Ar dating of volcanic rocks from <span class="hlt">submarine</span> <span class="hlt">volcanoes</span> around McDonald Islands suggests that volcanism and glaciation coincided. The flat-topped morphology of these <span class="hlt">volcanoes</span> may result from lava-ice interaction or erosion by glaciers post eruption during a time of extensive ice</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA03880.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA03880.html"><span>Soufriere Hills <span class="hlt">Volcano</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2002-11-07</p> <p>In this ASTER image of Soufriere Hills <span class="hlt">Volcano</span> on Montserrat in the Caribbean, continued eruptive <span class="hlt">activity</span> is evident by the extensive smoke and ash plume streaming towards the west-southwest. Significant eruptive <span class="hlt">activity</span> began in 1995, forcing the authorities to evacuate more than 7,000 of the island's original population of 11,000. The primary risk now is to the northern part of the island and to the airport. Small rockfalls and pyroclastic flows (ash, rock and hot gases) are common at this time due to continued growth of the dome at the <span class="hlt">volcano</span>'s summit. This image was acquired on October 29, 2002 by the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER) on NASA's Terra satellite. With its 14 spectral bands from the visible to the thermal infrared wavelength region, and its high spatial resolution of 15 to 90 meters (about 50 to 300 feet), ASTER images Earth to map and monitor the changing surface of our planet. http://photojournal.jpl.nasa.gov/catalog/PIA03880</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036677','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036677"><span><span class="hlt">Volcano</span>-tectonic implications of 3-D velocity structures derived from joint <span class="hlt">active</span> and passive source tomography of the island of 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>Park, J.; Morgan, J.K.; Zelt, C.A.; Okubo, P.G.</p> <p>2009-01-01</p> <p>We present a velocity model of the onshore and offshore regions around the southern part of the island of Hawaii, including southern Mauna Kea, southeastern Hualalai, and the <span class="hlt">active</span> <span class="hlt">volcanoes</span> of Mauna Loa, and Kilauea, and Loihi seamount. The velocity model was inverted from about 200,000 first-arrival traveltime picks of earthquakes and air gun shots recorded at the Hawaiian <span class="hlt">Volcano</span> Observatory (HVO). Reconstructed volcanic structures of the island provide us with an improved understanding of the <span class="hlt">volcano</span>-tectonic evolution of Hawaiian <span class="hlt">volcanoes</span> and their interactions. The summits and upper rift zones of the <span class="hlt">active</span> <span class="hlt">volcanoes</span> are characterized by high-velocity materials, correlated with intrusive magma cumulates. These high-velocity materials often do not extend the full lengths of the rift zones, suggesting that rift zone intrusions may be spatially limited. Seismicity tends to be localized seaward of the most <span class="hlt">active</span> intrusive bodies. Low-velocity materials beneath parts of the <span class="hlt">active</span> rift zones of Kilauea and Mauna Loa suggest discontinuous rift zone intrusives, possibly due to the presence of a preexisting volcanic edifice, e.g., along Mauna Loa beneath Kilauea's southwest rift zone, or alternatively, removal of high-velocity materials by large-scale landsliding, e.g., along Mauna Loa's western flank. Both locations also show increased seismicity that may result from edifice interactions or reactivation of buried faults. New high-velocity regions are recognized and suggest the presence of buried, and in some cases, previously unknown rift zones, within the northwest flank of Mauna Loa, and the south flanks of Mauna Loa, Hualalai, and Mauna Kea. Copyright 2009 by the American Geophysical Union.</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/2012BVol...74.1005D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BVol...74.1005D"><span>Science at the policy interface: <span class="hlt">volcano</span>-monitoring technologies and volcanic hazard management</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Donovan, Amy; Oppenheimer, Clive; Bravo, Michael</p> <p>2012-07-01</p> <p>This paper discusses results from a survey of volcanologists carried out on the <span class="hlt">Volcano</span> Listserv during late 2008 and early 2009. In particular, it examines the status of <span class="hlt">volcano</span> monitoring technologies and their relative perceived value at persistently and potentially <span class="hlt">active</span> <span class="hlt">volcanoes</span>. It also examines the role of different types of knowledge in hazard assessment on <span class="hlt">active</span> <span class="hlt">volcanoes</span>, as reported by scientists engaged in this area, and interviewees with experience from the current eruption on Montserrat. Conclusions are drawn about the current state of monitoring and the likely future research directions, and also about the roles of expertise and experience in risk assessment on <span class="hlt">active</span> <span class="hlt">volcanoes</span>; while local knowledge is important, it must be balanced with fresh ideas and expertise in a combination of disciplines to produce an advisory context that is conducive to high-level scientific discussion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-s39-75-101.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-s39-75-101.html"><span>Colima <span class="hlt">Volcano</span>, State of Jalisco, Mexico</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1991-05-06</p> <p>STS039-75-101 (28 April-6 May 1991) --- Spending over eight days in Earth orbit, the STS-39 crew was able to return with photographic coverage of highly variegated geographic scenery, including a number of <span class="hlt">volcanoes</span> such as Mexico's Colima. Located south of Guadalajara, Colima is Mexico's most <span class="hlt">active</span> <span class="hlt">volcano</span>. The current <span class="hlt">activity</span> started in the first part of March 1991 with avalanches occurring, followed by lava extrusion and ash emission. Colima is captured here in action. The steam plume drifts eastward from the 13,325 ft. summit. Scars from recent landslides can be seen on the southwest flank of the summit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.V41B2790B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.V41B2790B"><span>Volcaniclastic stratigraphy of Gede <span class="hlt">volcano</span> in West Java</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belousov, A.; Belousova, M.; Zaennudin, A.; Prambada, O.</p> <p>2012-12-01</p> <p>Gede <span class="hlt">volcano</span> (2958 m a.s.l.) and the adjacent Pangrango <span class="hlt">volcano</span> (3019 m a.s.l.) form large (base diameter 35 km) volcanic massif 60 km south of Jakarta. While Pangrango has no recorded eruptions, Gede is one of the most <span class="hlt">active</span> <span class="hlt">volcanoes</span> in Indonesia: eruptions were reported 26 times starting from 1747 (Petroeschevsky 1943; van Bemmelen 1949). Historic eruptions were mildly explosive (Vulcanian) with at least one lava flow. Modern <span class="hlt">activity</span> of the <span class="hlt">volcano</span> includes persistent solfataric <span class="hlt">activity</span> in the summit crater and periodic seismic swarms - in 1990, 1991, 1992, 1995, 1996, 1997, 2000, 2010, and 2012 (CVGHM). Lands around the Gede-Pangrango massif are densely populated with villages up to 1500-2000 m a.s.l. Higher, the <span class="hlt">volcano</span> is covered by rain forest of the Gede-Pangrango Natural Park, which is visited every day by numerous tourists who camp in the summit area. We report the results of the detailed reinvestigation of volcaniclastic stratigraphy of Gede <span class="hlt">volcano</span>. This work has allowed us to obtain 24 new radiocarbon dates for the area. As a result the timing and character of <span class="hlt">activity</span> of Gede in Holocene has been revealed. The edifice of Gede <span class="hlt">volcano</span> consists of main stratocone (Gumuruh) with 1.8 km-wide summit caldera; intra-caldera lava cone (Gede proper) with a 900 m wide summit crater, having 2 breaches toward N-NE; and intra-crater infill (lava dome/flow capped with 3 small craters surrounded by pyroclastic aprons). The Gumuruh edifice, composed mostly of lava flows, comprises more than 90% of the total volume of the <span class="hlt">volcano</span>. Deep weathering of rocks and thick (2-4 m) red laterite soil covering Gumuruh indicates its very old age. Attempts to get 14C dates in 4 different locations of Gumuruh (including a large debris avalanche deposit on its SE foot) provided ages older than 45,000 years - beyond the limit for 14C dating. Outside the summit caldera, notable volumes of fresh, 14C datable volcaniclastic deposits were found only in the NNE sector of the <span class="hlt">volcano</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title33-vol2/pdf/CFR-2011-title33-vol2-sec165-1302.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title33-vol2/pdf/CFR-2011-title33-vol2-sec165-1302.pdf"><span>33 CFR 165.1302 - Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA.</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>2011-07-01</p> <p>... 33 Navigation and Navigable Waters 2 2011-07-01 2011-07-01 false Bangor Naval <span class="hlt">Submarine</span> Base... Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA. (a) Location. The following is a security zone: The waters of... States Naval vessels. (ii) Vessels that are performing work at Naval <span class="hlt">Submarine</span> Base Bangor pursuant to a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title33-vol2/pdf/CFR-2012-title33-vol2-sec165-1302.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title33-vol2/pdf/CFR-2012-title33-vol2-sec165-1302.pdf"><span>33 CFR 165.1302 - Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA.</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>2012-07-01</p> <p>... 33 Navigation and Navigable Waters 2 2012-07-01 2012-07-01 false Bangor Naval <span class="hlt">Submarine</span> Base... Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA. (a) Location. The following is a security zone: The waters of... States Naval vessels. (ii) Vessels that are performing work at Naval <span class="hlt">Submarine</span> Base Bangor pursuant to a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title33-vol2/pdf/CFR-2013-title33-vol2-sec165-1302.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title33-vol2/pdf/CFR-2013-title33-vol2-sec165-1302.pdf"><span>33 CFR 165.1302 - Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA.</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>2013-07-01</p> <p>... 33 Navigation and Navigable Waters 2 2013-07-01 2013-07-01 false Bangor Naval <span class="hlt">Submarine</span> Base... Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA. (a) Location. The following is a security zone: The waters of... States Naval vessels. (ii) Vessels that are performing work at Naval <span class="hlt">Submarine</span> Base Bangor pursuant to a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title33-vol2/pdf/CFR-2010-title33-vol2-sec165-1302.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title33-vol2/pdf/CFR-2010-title33-vol2-sec165-1302.pdf"><span>33 CFR 165.1302 - Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA.</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>2010-07-01</p> <p>... 33 Navigation and Navigable Waters 2 2010-07-01 2010-07-01 false Bangor Naval <span class="hlt">Submarine</span> Base... Bangor Naval <span class="hlt">Submarine</span> Base, Bangor, WA. (a) Location. The following is a security zone: The waters of... States Naval vessels. (ii) Vessels that are performing work at Naval <span class="hlt">Submarine</span> Base Bangor pursuant to a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4847I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4847I"><span>Catalogue of Icelandic <span class="hlt">Volcanoes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ilyinskaya, Evgenia; Larsen, Gudrún; Gudmundsson, Magnús T.; Vogfjörd, Kristin; Jonsson, Trausti; Oddsson, Björn; Reynisson, Vidir; Pagneux, Emmanuel; Barsotti, Sara; Karlsdóttir, Sigrún; Bergsveinsson, Sölvi; Oddsdóttir, Thorarna</p> <p>2017-04-01</p> <p>The Catalogue of Icelandic <span class="hlt">Volcanoes</span> (CIV) is a newly developed open-access web resource (http://icelandicvolcanoes.is) intended to serve as an official source of information about <span class="hlt">volcanoes</span> in Iceland for the public and decision makers. CIV contains text and graphic information on all 32 <span class="hlt">active</span> volcanic systems in Iceland, as well as real-time data from monitoring systems in a format that enables non-specialists to understand the volcanic <span class="hlt">activity</span> status. The CIV data portal contains scientific data on all eruptions since Eyjafjallajökull 2010 and is an unprecedented endeavour in making volcanological data open and easy to access. CIV forms a part of an integrated volcanic risk assessment project in Iceland GOSVÁ (commenced in 2012), as well as being part of the European Union funded effort FUTUREVOLC (2012-2016) on establishing an Icelandic <span class="hlt">volcano</span> supersite. The supersite concept implies integration of space and ground based observations for improved monitoring and evaluation of volcanic hazards, and open data policy. This work is a collaboration of the Icelandic Meteorological Office, the Institute of Earth Sciences at the University of Iceland, and the Civil Protection Department of the National Commissioner of the Iceland Police, with contributions from a large number of specialists in Iceland and elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3555091','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3555091"><span>The natural ocean acidification and fertilization event caused by the <span class="hlt">submarine</span> eruption of El Hierro</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Santana-Casiano, J. M.; González-Dávila, M.; Fraile-Nuez, E.; de Armas, D.; González, A. G.; Domínguez-Yanes, J. F.; Escánez, J.</p> <p>2013-01-01</p> <p>The shallow <span class="hlt">submarine</span> eruption which took place in October 10th 2011, 1.8 km south of the island of El Hierro (Canary Islands) allowed the study of the abrupt changes in the physical-chemical properties of seawater caused by volcanic discharges. In order to monitor the evolution of these changes, seven oceanographic surveys were carried out over six months (November 2011-April 2012) from the beginning of the eruptive stage to the post-eruptive phase. Here, we present dramatic changes in the water column chemistry including large decreases in pH, striking effects on the carbonate system, decreases in the oxygen concentrations and enrichment of Fe(II) and nutrients. Our findings highlight that the same <span class="hlt">volcano</span> which was responsible for the creation of a highly corrosive environment, affecting marine biota, has also provided the nutrients required for the rapid recuperation of the marine ecosystem. PMID:23355953</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V53C3123B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V53C3123B"><span>Exploring the Llaima <span class="hlt">Volcano</span> Using Receiver Functions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bishop, J. W.; Biryol, C.; Lees, J. M.</p> <p>2016-12-01</p> <p>The Llaima <span class="hlt">volcano</span> in Chile is one of the most <span class="hlt">active</span> <span class="hlt">volcanos</span> in the Southern Andes, erupting at least 50 times since 1640. To understand the eruption dynamics behind these frequent paroxysms, it is important to identify the depth and extent of the magma chamber beneath the <span class="hlt">volcano</span>. Furthermore, it is also important to identify structural controls on the magma storage regions and volcanic plumbing system, such as fault and fracture zones. To probe these questions, a dense, 26 station broadband seismic array was deployed around the Llaima <span class="hlt">volcano</span> for 3 months (January to March, 2015). Additionally, broadband seismic data from 7 stations in the nearby Observatorio Volcanológico de Los Andes del Sur (OVDAS) seismic network was also obtained for this period. Teleseismic receiver functions were calculated from this combined data using an iterative deconvolution technique. Receiver function stacks (both H-K and CCP) yield seismic images of the deep structure beneath the <span class="hlt">volcano</span>. Initial results depict two low velocity layers at approximately 4km and 12km. Furthermore, Moho calculations are 5-8 km deeper than expected from regional models, but a shallow ( 40 km) region is detected beneath the <span class="hlt">volcano</span> peak. A large high Vp/Vs ratio anomaly (Vp/Vs > 0.185) is discernable to the east of the main peak of the <span class="hlt">volcano</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title47-vol2/pdf/CFR-2011-title47-vol2-sec32-6424.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title47-vol2/pdf/CFR-2011-title47-vol2-sec32-6424.pdf"><span>47 CFR 32.6424 - <span class="hlt">Submarine</span> and deep sea cable expense.</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>2011-10-01</p> <p>... 47 Telecommunication 2 2011-10-01 2011-10-01 false <span class="hlt">Submarine</span> and deep sea cable expense. 32.6424... <span class="hlt">Submarine</span> and deep sea cable expense. (a) This account shall include expenses associated with <span class="hlt">submarine</span> and deep sea cable. (b) Subsidiary record categories shall be maintained as provided in § 32.2424. [67 FR...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title47-vol2/pdf/CFR-2013-title47-vol2-sec32-6424.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title47-vol2/pdf/CFR-2013-title47-vol2-sec32-6424.pdf"><span>47 CFR 32.6424 - <span class="hlt">Submarine</span> and deep sea cable expense.</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>2013-10-01</p> <p>... 47 Telecommunication 2 2013-10-01 2013-10-01 false <span class="hlt">Submarine</span> and deep sea cable expense. 32.6424... <span class="hlt">Submarine</span> and deep sea cable expense. (a) This account shall include expenses associated with <span class="hlt">submarine</span> and deep sea cable. (b) Subsidiary record categories shall be maintained as provided in § 32.2424. [67 FR...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title47-vol2/pdf/CFR-2012-title47-vol2-sec32-6424.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title47-vol2/pdf/CFR-2012-title47-vol2-sec32-6424.pdf"><span>47 CFR 32.6424 - <span class="hlt">Submarine</span> and deep sea cable expense.</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>2012-10-01</p> <p>... 47 Telecommunication 2 2012-10-01 2012-10-01 false <span class="hlt">Submarine</span> and deep sea cable expense. 32.6424... <span class="hlt">Submarine</span> and deep sea cable expense. (a) This account shall include expenses associated with <span class="hlt">submarine</span> and deep sea cable. (b) Subsidiary record categories shall be maintained as provided in § 32.2424. [67 FR...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title47-vol2/pdf/CFR-2014-title47-vol2-sec32-6424.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title47-vol2/pdf/CFR-2014-title47-vol2-sec32-6424.pdf"><span>47 CFR 32.6424 - <span class="hlt">Submarine</span> and deep sea cable expense.</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>2014-10-01</p> <p>... 47 Telecommunication 2 2014-10-01 2014-10-01 false <span class="hlt">Submarine</span> and deep sea cable expense. 32.6424... <span class="hlt">Submarine</span> and deep sea cable expense. (a) This account shall include expenses associated with <span class="hlt">submarine</span> and deep sea cable. (b) Subsidiary record categories shall be maintained as provided in § 32.2424. [67 FR...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title47-vol2/pdf/CFR-2010-title47-vol2-sec32-6424.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title47-vol2/pdf/CFR-2010-title47-vol2-sec32-6424.pdf"><span>47 CFR 32.6424 - <span class="hlt">Submarine</span> and deep sea cable expense.</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>... 47 Telecommunication 2 2010-10-01 2010-10-01 false <span class="hlt">Submarine</span> and deep sea cable expense. 32.6424... <span class="hlt">Submarine</span> and deep sea cable expense. (a) This account shall include expenses associated with <span class="hlt">submarine</span> and deep sea cable. (b) Subsidiary record categories shall be maintained as provided in § 32.2424. [67 FR...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034456p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/ct0564.photos.034456p/"><span>36. VIEW OF CUPOLA, <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK, SHOWING ROVING ...</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>36. VIEW OF CUPOLA, <span class="hlt">SUBMARINE</span> ESCAPE TRAINING TANK, SHOWING ROVING RESCUE BELL SUSPENDED ABOVE TANK, WITH TWO-LOCK RECOMPRESSION CHAMBER AT REAR, LOOKING WEST. Photo taken after installation of recompression chamber in 1956. - U.S. Naval <span class="hlt">Submarine</span> Base, New London <span class="hlt">Submarine</span> Escape Training Tank, Albacore & Darter Roads, Groton, New London County, CT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70169246','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70169246"><span>Monitoring Mount Baker <span class="hlt">Volcano</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>Malone, S.D.; Frank, D.</p> <p>1976-01-01</p> <p>Hisotrically <span class="hlt">active</span> <span class="hlt">volcanoes</span> in the conterminous United States are restricted to the Cascade Range and extend to the Cascade Range and extend from Mount Baker near the Canadian border to Lassen Peak in northern California. Since 1800 A.D, most eruptive <span class="hlt">activity</span> has been on a relatively small scale and has not caused loss of life or significant property damage. However, future  volcanism predictably will have more serious effects because of greatly increased use of land near <span class="hlt">volcanoes</span> during the present century. (See "Appraising Volcanic Hazards of the Cascade Range of the Northwestern United States," Earthquake Inf. Bull., Sept.-Oct. 1974.) The recognition an impending eruption is highly important in order to minimize the potential hazard to people and property. Thus, a substantial increase in hydrothermal <span class="hlt">activity</span> at Mount Baker in March 1975 ( see "Mount Baker Heating Up," July-Aug. 1975 issue) was regarded as a possible first signal that an eruption might occur, and an intensive monitoring program was undertaken. </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GML....34..327W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GML....34..327W"><span>Architecture and development of a multi-stage Baiyun <span class="hlt">submarine</span> slide complex in the Pearl River Canyon, northern South China Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Lei; Wu, Shi-Guo; Li, Qing-Ping; Wang, Da-Wei; Fu, Shao-Ying</p> <p>2014-08-01</p> <p>The Baiyun <span class="hlt">submarine</span> slide complex (BSSC) along the Pearl River Canyon of the northern South China Sea has been imaged by multibeam bathymetry and 2D/3D seismic data. By means of maximum likelihood classification with slope aspect and gradient as inputs, the BSSC is subdivided into four domains, denoted as slide area I, II, III and IV. Slide area I is surrounded by cliffs on three sides and has been intensely reshaped by turbidity currents generated by other kinds of mass movement outside the area; slide area II incorporates a shield <span class="hlt">volcano</span> with a diameter of approximately 10 km and unconfined slides possibly resulting from the toe collapse of inter-canyon ridges; slide area III is dominated by repeated slides that mainly originated from cliffs constituting the eastern boundary of the BSSC; slide area IV is distinguished by a conical seamount with a diameter of 6.5 km and a height of 375 m, and two slides probably having a common source that are separated from each other by a suite of residual strata. The BSSC is interpreted to be composed of numerous slide events, which occurred in the period from 10.5 to 5.5 Ma BP. Six specific factors may have contributed to the development of the BSSC, i.e., gas hydrate dissociation, gas-bearing sediments, <span class="hlt">submarine</span> volcanic <span class="hlt">activity</span>, seismicity, sedimentation rate and seafloor geomorphology. A 2D conceptual geological model combining these factors is proposed as a plausible mechanism explaining the formation of the BSSC. However, the BSSC may also have been affected by the Dongsha event (10 Ma BP) as an overriding factor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033746','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033746"><span>The critical role of <span class="hlt">volcano</span> monitoring in risk reduction</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Tilling, R.I.</p> <p>2008-01-01</p> <p>Data from <span class="hlt">volcano</span>-monitoring studies constitute the only scientifically valid basis for short-term forecasts of a future eruption, or of possible changes during an ongoing eruption. Thus, in any effective hazards-mitigation program, a basic strategy in reducing <span class="hlt">volcano</span> risk is the initiation or augmentation of <span class="hlt">volcano</span> monitoring at historically <span class="hlt">active</span> <span class="hlt">volcanoes</span> and also at geologically young, but presently dormant, <span class="hlt">volcanoes</span> with potential for reactivation. Beginning with the 1980s, substantial progress in <span class="hlt">volcano</span>-monitoring techniques and networks - ground-based as well space-based - has been achieved. Although some geochemical monitoring techniques (e.g., remote measurement of volcanic gas emissions) are being increasingly applied and show considerable promise, seismic and geodetic methods to date remain the techniques of choice and are the most widely used. Availability of comprehensive <span class="hlt">volcano</span>-monitoring data was a decisive factor in the successful scientific and governmental responses to the reawakening of Mount St. Helens (Washington, USA) in 1980 and, more recently, to the powerful explosive eruptions at Mount Pinatubo (Luzon, Philippines) in 1991. However, even with the ever-improving state-ofthe-art in <span class="hlt">volcano</span> monitoring and predictive capability, the Mount St. Helens and Pinatubo case histories unfortunately still represent the exceptions, rather than the rule, in successfully forecasting the most likely outcome of <span class="hlt">volcano</span> unrest.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sim/2927/sim2927_pamphlet.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sim/2927/sim2927_pamphlet.pdf"><span>Geologic map of Medicine Lake <span class="hlt">volcano</span>, northern 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>Donnelly-Nolan, Julie M.</p> <p>2011-01-01</p> <p>Medicine Lake <span class="hlt">volcano</span> forms a broad, seemingly nondescript highland, as viewed from any angle on the ground. Seen from an airplane, however, treeless lava flows are scattered across the surface of this potentially <span class="hlt">active</span> volcanic edifice. Lavas of Medicine Lake <span class="hlt">volcano</span>, which range in composition from basalt through rhyolite, cover more than 2,000 km2 east of the main axis of the Cascade Range in northern California. Across the Cascade Range axis to the west-southwest is Mount Shasta, its towering volcanic neighbor, whose stratocone shape contrasts with the broad shield shape of Medicine Lake <span class="hlt">volcano</span>. Hidden in the center of Medicine Lake <span class="hlt">volcano</span> is a 7 km by 12 km summit caldera in which nestles its namesake, Medicine Lake. The flanks of Medicine Lake <span class="hlt">volcano</span>, which are dotted with cinder cones, slope gently upward to the caldera rim, which reaches an elevation of nearly 8,000 ft (2,440 m). The maximum extent of lavas from this half-million-year-old <span class="hlt">volcano</span> is about 80 km north-south by 45 km east-west. In postglacial time, 17 eruptions have added approximately 7.5 km3 to its total estimated volume of 600 km3, and it is considered to be the largest by volume among <span class="hlt">volcanoes</span> of the Cascades arc. The <span class="hlt">volcano</span> has erupted nine times in the past 5,200 years, a rate more frequent than has been documented at all other Cascades arc <span class="hlt">volcanoes</span> except Mount St. Helens.</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><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><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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