Sample records for storage rings events

  1. Diffraction-limited storage-ring vacuum technology

    PubMed Central

    Al-Dmour, Eshraq; Ahlback, Jonny; Einfeld, Dieter; Tavares, Pedro Fernandes; Grabski, Marek

    2014-01-01

    Some of the characteristics of recent ultralow-emittance storage-ring designs and possibly future diffraction-limited storage rings are a compact lattice combined with small magnet apertures. Such requirements present a challenge for the design and performance of the vacuum system. The vacuum system should provide the required vacuum pressure for machine operation and be able to handle the heat load from synchrotron radiation. Small magnet apertures result in the conductance of the chamber being low, and lumped pumps are ineffective. One way to provide the required vacuum level is by distributed pumping, which can be realised by the use of a non-evaporable getter (NEG) coating of the chamber walls. It may not be possible to use crotch absorbers to absorb the heat from the synchrotron radiation because an antechamber is difficult to realise with such a compact lattice. To solve this, the chamber walls can work as distributed absorbers if they are made of a material with good thermal conductivity, and distributed cooling is used at the location where the synchrotron radiation hits the wall. The vacuum system of the 3 GeV storage ring of MAX IV is used as an example of possible solutions for vacuum technologies for diffraction-limited storage rings. PMID:25177979

  2. Storage-ring Electron Cooler for Relativistic Ion Beams

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

    Lin, Fanglei; Derbenev, Yaroslav; Douglas, David R.

    Application of electron cooling at ion energies above a few GeV has been limited due to reduction of electron cooling efficiency with energy and difficulty in producing and accelerating a high-current high-quality electron beam. A high-current storage-ring electron cooler offers a solution to both of these problems by maintaining high cooling beam quality through naturally-occurring synchrotron radiation damping of the electron beam. However, the range of ion energies where storage-ring electron cooling can be used has been limited by low electron beam damping rates at low ion energies and high equilibrium electron energy spread at high ion energies. This papermore » reports a development of a storage ring based cooler consisting of two sections with significantly different energies: the cooling and damping sections. The electron energy and other parameters in the cooling section are adjusted for optimum cooling of a stored ion beam. The beam parameters in the damping section are adjusted for optimum damping of the electron beam. The necessary energy difference is provided by an energy recovering SRF structure. A prototype linear optics of such storage-ring cooler is presented.« less

  3. A new storage-ring light source

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

    Chao, Alex

    2015-06-01

    A recently proposed technique in storage ring accelerators is applied to provide potential high-power sources of photon radiation. The technique is based on the steady-state microbunching (SSMB) mechanism. As examples of this application, one may consider a high-power DUV photon source for research in atomic and molecular physics or a high-power EUV radiation source for industrial lithography. A less challenging proof-of-principle test to produce IR radiation using an existing storage ring is also considered.

  4. Astrochemistry in TSR and CSR Ion Storage Rings

    NASA Astrophysics Data System (ADS)

    Novotny, Oldrich

    2017-04-01

    Dissociative recombination (DR) of molecular ions plays a key role in controlling the charge density and composition of the cold interstellar medium (ISM). Experimental data on DR are required in order to understand the chemical network in the ISM and related processes such as star formation from molecular clouds. Needed data include not only total reaction cross sections, but also the chemical composition and excitation states of the neutral products. Utilizing the TSR storage ring in Heidelberg, Germany, we have carried out DR measurements for astrophysically important molecular ions. We use a merged electron-ion beams technique combined with event-by-event fragment counting and fragment imaging. The count rate of detected neutral DR products yields the absolute DR rate coefficient. Imaging the distribution of fragment distances provides information on the kinetic energy released including the states of both the initial molecule and the final products. Additional kinetic energy sensitivity of the employed detector allows for identification of fragmentation channels by fragment-mass combination within each dissociation event. Such combined information is essential for studies on DR of polyatomic ions with multi-channel breakup. The recently commissioned Cryogenic Storage Ring (CSR) in Heidelberg, Germany, extends the experimental capabilities of TSR by operation at cryogenic temperatures down to 6 K. At these conditions residual gas densities down to 100 cm-3 can be reached resulting in beam storage times of several hours. Long storage in the cold environment allows the ions to relax down to their rotational ground state, thus mimicking well the conditions in the cold ISM. A variety of astrophysically relevant reactions will be investigated at these conditions, such as DR, electron impact excitation, ion-neutral collisions, etc. We report our TSR results on DR of HCl+ and D2Cl+. We also present first results from the CSR commissioning experiments.

  5. Design Considerations for High Energy Electron -- Positron Storage Rings

    DOE R&D Accomplishments Database

    Richter, B.

    1966-11-01

    High energy electron-positron storage rings give a way of making a new attack on the most important problems of elementary particle physics. All of us who have worked in the storage ring field designing, building, or using storage rings know this. The importance of that part of storage ring work concerning tests of quantum electrodynamics and mu meson physics is also generally appreciated by the larger physics community. However, I do not think that most of the physicists working tin the elementary particle physics field realize the importance of the contribution that storage ring experiments can make to our understanding of the strongly interacting particles. I would therefore like to spend the next few minutes discussing the sort of things that one can do with storage rings in the strongly interacting particle field.

  6. Physics issues in diffraction limited storage ring design

    NASA Astrophysics Data System (ADS)

    Fan, Wei; Bai, ZhengHe; Gao, WeiWei; Feng, GuangYao; Li, WeiMin; Wang, Lin; He, DuoHui

    2012-05-01

    Diffraction limited electron storage ring is considered a promising candidate for future light sources, whose main characteristics are higher brilliance, better transverse coherence and better stability. The challenge of diffraction limited storage ring design is how to achieve the ultra low beam emittance with acceptable nonlinear performance. Effective linear and nonlinear parameter optimization methods based on Artificial Intelligence were developed for the storage ring physical design. As an example of application, partial physical design of HALS (Hefei Advanced Light Source), which is a diffraction limited VUV and soft X-ray light source, was introduced. Severe emittance growth due to the Intra Beam Scattering effect, which is the main obstacle to achieve ultra low emittance, was estimated quantitatively and possible cures were discussed. It is inspiring that better performance of diffraction limited storage ring can be achieved in principle with careful parameter optimization.

  7. The Storage Ring Proton EDM Experiment

    NASA Astrophysics Data System (ADS)

    Semertzidis, Yannis; Storage Ring Proton EDM Collaboration

    2014-09-01

    The storage ring pEDM experiment utilizes an all-electric storage ring to store ~1011 longitudinally polarized protons simultaneously in clock-wise and counter-clock-wise directions for 103 seconds. The radial E-field acts on the proton EDM for the duration of the storage time to precess its spin in the vertical plane. The ring lattice is optimized to reduce intra-beam scattering, increase the statistical sensitivity and reduce the systematic errors of the method. The main systematic error is a net radial B-field integrated around the ring causing an EDM-like vertical spin precession. The counter-rotating beams sense this integrated field and are vertically shifted by an amount, which depends on the strength of the vertical focusing in the ring, thus creating a radial B-field. Modulating the vertical focusing at 10 kHz makes possible the detection of this radial B-field by a SQUID-magnetometer (SQUID-based BPM). For a total number of n SQUID-based BPMs distributed around the ring the effectiveness of the method is limited to the N = n /2 harmonic of the background radial B-field due to the Nyquist sampling theorem limit. This limitation establishes the requirement to reduce the maximum radial B-field to 0.1-1 nT everywhere around the ring by layers of mu-metal and aluminum vacuum tube. The metho's sensitivity is 10-29 e .cm , more than three orders of magnitude better than the present neutron EDM experimental limit, making it sensitive to SUSY-like new physics mass scale up to 300 TeV.

  8. Online optimization of storage ring nonlinear beam dynamics

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

    Huang, Xiaobiao; Safranek, James

    2015-08-01

    We propose to optimize the nonlinear beam dynamics of existing and future storage rings with direct online optimization techniques. This approach may have crucial importance for the implementation of diffraction limited storage rings. In this paper considerations and algorithms for the online optimization approach are discussed. We have applied this approach to experimentally improve the dynamic aperture of the SPEAR3 storage ring with the robust conjugate direction search method and the particle swarm optimization method. The dynamic aperture was improved by more than 5 mm within a short period of time. Experimental setup and results are presented.

  9. Beam dynamics and expected performance of Sweden's new storage-ring light source: MAX IV

    NASA Astrophysics Data System (ADS)

    Leemann, S. C.; Andersson, Å.; Eriksson, M.; Lindgren, L.-J.; Wallén, E.; Bengtsson, J.; Streun, A.

    2009-12-01

    MAX IV will be Sweden’s next-generation high-performance synchrotron radiation source. The project has recently been granted funding and construction is scheduled to begin in 2010. User operation for a broad and international user community should commence in 2015. The facility is comprised of two storage rings optimized for different wavelength ranges, a linac-based short-pulse facility and a free-electron laser for the production of coherent radiation. The main radiation source of MAX IV will be a 528 m ultralow emittance storage ring operated at 3 GeV for the generation of high-brightness hard x rays. This storage ring was designed to meet the requirements of state-of-the-art insertion devices which will be installed in nineteen 5 m long dispersion-free straight sections. The storage ring is based on a novel multibend achromat design delivering an unprecedented horizontal bare lattice emittance of 0.33 nm rad and a vertical emittance below the 8 pm rad diffraction limit for 1 Å radiation. In this paper we present the beam dynamics considerations behind this storage-ring design and detail its expected unique performance.

  10. Beam diagnostics at high-intensity storage rings

    NASA Astrophysics Data System (ADS)

    Plum, Mike

    1994-10-01

    Beam diagnostics at high-intensity facilities feature their own special set of problems and characteristics, issues peculiar to high-intensity storage rings include beam loss, beam halos, extraction efficiency, beam in the gap, clearing electrodes, and beam-profile measurement. The Los Alamos Proton Storage Ring (PSR) is a nice example of a high-intensity storage ring. I will discuss in some detail three diagnostic systems currently in use at the PSR: the beam-loss-monitor system, the electron-clearing system, and the beam-in-the-gap monitor. Much of our discussion is inspired by the problems we have encountered and the useful things we have learned while commissioning and developing the PSR. Another inspiration is our work on the next-generation neutron-spallation source, also known as the National Center for Neutron Research (NCNR).

  11. National Synchrotron Light Source II storage ring vacuum systems

    DOE PAGES

    Hseuh, Hsiao-Chaun; Hetzel, Charles; Leng, Shuwei; ...

    2016-04-05

    The National Synchrotron Light Source II, completed in 2014, is a 3-GeV synchrotron radiation (SR) facility at Brookhaven National Laboratory and has been in steady operation since. With a design electron current of 500 mA and subnanometer radians horizontal emittance, this 792-m circumference storage ring is providing the highest flux and brightness x-ray beam for SR users. Also, the majority of the storage ring vacuum chambers are made of extruded aluminium. Chamber sections are interconnected using low-impedance radiofrequency shielded bellows. SR from the bending magnets is intercepted by water-cooled compact photon absorbers resided in the storage ring chambers. Finally, thismore » paper presents the design of the storage ring vacuum system, the fabrication of vacuum chambers and other hardware, the installation, the commissioning, and the continuing beam conditioning of the vacuum systems.« less

  12. National Synchrotron Light Source II storage ring vacuum systems

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

    Hseuh, Hsiao-Chaun, E-mail: hseuh@bnl.gov; Hetzel, Charles; Leng, Shuwei

    2016-05-15

    The National Synchrotron Light Source II, completed in 2014, is a 3-GeV synchrotron radiation (SR) facility at Brookhaven National Laboratory and has been in steady operation since. With a design electron current of 500 mA and subnanometer radians horizontal emittance, this 792-m circumference storage ring is providing the highest flux and brightness x-ray beam for SR users. The majority of the storage ring vacuum chambers are made of extruded aluminium. Chamber sections are interconnected using low-impedance radiofrequency shielded bellows. SR from the bending magnets is intercepted by water-cooled compact photon absorbers resided in the storage ring chambers. This paper presents themore » design of the storage ring vacuum system, the fabrication of vacuum chambers and other hardware, the installation, the commissioning, and the continuing beam conditioning of the vacuum systems.« less

  13. Storage rings, internal targets and PEP

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

    Spencer, J.E.

    Storage rings with internal targets are described, using PEP as an example. The difference between electrons and heavier particles such as protons, antiprotons, and heavy ions is also discussed because it raises possibilities of bypass insertions for more exotic experiments. PEP is compared to other rings in various contexts to verify the assertion that it is an ideal ring for many fundamental and practical applications that can be carried on simultaneously. (LEW)

  14. Low emittance electron storage rings

    NASA Astrophysics Data System (ADS)

    Levichev, E. B.

    2018-01-01

    Low-emittance electron (positron) beams are essential for synchrotron light sources, linear collider damping rings, and circular Crab Waist colliders. In this review, the principles and methods of emittance minimization are discussed, prospects for developing relativistic electron storage rings with small beam phase volume are assessed, and problems related to emittance minimization are examined together with their possible solutions. The special features and engineering implementation aspects of various facilities are briefly reviewed.

  15. An Inside Look: NSLS-II Storage Ring

    ScienceCinema

    Fries, Gregory

    2018-06-12

    Look inside the storage ring of the National Synchrotron Light Source II, under construction at Brookhaven Lab. Exactly 843 magnets now encircle the ring. Their job will be to steer, stabilize, and store electrons racing around at near light speed.

  16. Polarization Studies for the eRHIC Electron Storage Ring

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

    Gianfelice-Wendt, Eliana; Tepikian, S.

    A hadron/lepton collider with polarized beams has been under consideration by the scientific community since some years, in the U.S. and Europe. Among the various proposals, those by JLAB and BNL with polarized electron and proton beams are currently under closer study in the U.S. Experimenters call for the simultaneous storage of electron bunches with both spin helicity. In the BNL based Ring-Ring design, electrons are stored at top energy in a ring to be accommodated in the existing RHIC tunnel. The transversely polarized electron beam is injected into the storage ring at variable energies, between 5 and 18 GeV.more » Polarization is brought into the longitudinal direction at the IP by a couple of spin rotators. In this paper results of first studies of the attainable beam polarization level and lifetime in the storage ring at 18 GeV are presented.« less

  17. Injection envelope matching in storage rings

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

    Minty, M.G.; Spence, W.L.

    1995-05-01

    The shape and size of the transverse phase space injected into a storage ring can be deduced from turn-by-turn measurements of the transient behavior of the beam envelope in the ring. Envelope oscillations at 2 x the {beta}-tron frequency indicate the presence of a {beta}-mismatch, while envelope oscillations at the {beta}-tron frequency are the signature of a dispersion function mismatch. Experiments in injection optimization using synchrotron radiation imaging of the beam and a fast-gated camera at the SLC damping rings are reported.

  18. Injection envelope matching in storage rings

    NASA Astrophysics Data System (ADS)

    Minty, M. G.; Spence, W. L.

    1995-05-01

    The shape and size of the transverse phase space injected into a storage ring can be deduced from turn-by-turn measurements of the transient behavior of the beam envelope in the ring. Envelope oscillations at 2 x the beta-tron frequency indicate the presence of a beta-mismatch, while envelope oscillations at the beta-tron frequency are the signature of a dispersion function mismatch. Experiments in injection optimization using synchrotron radiation imaging of the beam and a fast-gated camera at the SLC damping rings are reported.

  19. ELISA - an electrostatic storage ring for low-energy ions

    NASA Astrophysics Data System (ADS)

    Pape Moeller, Soeren

    1997-05-01

    The design of a new type of storage ring for low-energy ions using electrostatic deflection and focusing devices is described. Electrostatic bends and quadrupoles are used since they are more efficient than magnetic ones for low-velocity heavy ions. Furthermore, electrostatic devices are more compact and easier to construct than magnetic devices. In comparison to an electromagnetic trap, one important advantage of the elecrostatic ring is the easy access to the circulating beam and its decay products. These and other features, e.g. no magnetic fields, makes such storage devices attractive for many atomic-physics experiments. Also neigboring fields as chemistry and biology might benefit from such an relatively inexpensive device. One important difference between an electrostatic and a magnetic ring is, that the longitudinal energy is not conserved for the electrostatic ring. The actual ring will have a race-track shape as defined by two straight sections each with two quadrupole doublets connected by 180-degrees bends. The bends will consist of 160-degrees spherical deflection plates surrounded by two parallel plate 10-degrees bends. The storage ring ELISA, currently being built, will have a circumference of 6 meters. The first beam tests will take place during summer 1996.

  20. Cabling design of booster and storage ring construction progress of TPS

    NASA Astrophysics Data System (ADS)

    Wong, Y.-S.; Liu, K.-B.; Liu, C.-Y.; Wang, b.-S.

    2017-06-01

    The 2012 Taiwan Photon Source (TPS) cable construction project started after 10 months to complete the cable laying and installation of power supply. The circumference of the booster ring (BR) is 496.8 m, whereas that of the storage ring (SR) is 518.4 m. Beam current is set to 500 mA at 3.3 GeV. The paper on grounding systems discusses the design of the ground wire (< 0.2 Ω) with low impedance, power supply of the accelerator and cabling tray. The flow and size of the ground current are carefully evaluated to avoid grounded current from flowing everywhere, which causes interference problems. In the design of the TPS, special shielding will be established to isolate the effects of electromagnetic interference on the magnet and ground current. Booster ring dipoles are connected by a series of 54-magnet bending dipole; the cable size of its stranded wire measures 250 mm2, with a total length of 5000 m. Booster ring and storage ring quadrupoles have 150 magnets; the cable size of their stranded wire is 250 mm2, with a total length of 17000 m. Storage ring dipole consists of 48 magnets; the cable size of its stranded wire is 325 mm2, with a total length of 6000 m. This study discusses the power supply cabling design of the storage ring and booster ring construction progress of TPS. The sections of this paper are divided into discussions of the construction of the control and instrument area, cabling layout of booster ring and storage ring, as well as the installation and commission machine. This study also discusses the use of a high-impedance meter to determine the effect of cabling insulation and TPS power supply machine on energy transfer to ensure the use of safe and correct magnet.

  1. The phase slip factor of the electrostatic cryogenic storage ring CSR

    NASA Astrophysics Data System (ADS)

    Grieser, Manfred; von Hahn, Robert; Vogel, Stephen; Wolf, Andreas

    2017-07-01

    To determine the momentum spread of an ion beam from the measured revolution frequency distribution, the knowledge of the phase slip factor of the storage ring is necessary. The slip factor was measured for various working points of the cryogenic storage ring CSR at MPI for Nuclear Physics, Heidelberg and was compared with simulations. The predicted functional relationship of the slip factor and the horizontal tune depends on the different islands of stability, which has been experimentally verified. This behavior of the slip factor is in clear contrast to that of magnetic storage rings.

  2. Total water storage dynamics derived from tree-ring records and terrestrial gravity observations

    NASA Astrophysics Data System (ADS)

    Creutzfeldt, Benjamin; Heinrich, Ingo; Merz, Bruno

    2015-10-01

    For both societal and ecological reasons, it is important to understand past and future subsurface water dynamics but estimating subsurface water storage is notoriously difficult. In this pilot study, we suggest the reconstruction of subsurface water dynamics by a multi-disciplinary approach combining hydrology, dendrochronology and geodesy. In a first step, nine complete years of high-precision gravimeter observations are used to estimate water storage changes in the subsurface at the Geodetic Observatory Wettzell in the Bavarian Forest, Germany. The record is extended to 63 years by calibrating a hydrological model against the 9 years of gravimeter observations. The relationship between tree-ring growth and water storage changes is evaluated as well as that between tree-ring growth and supplementary hydro-meteorological data. Results suggest that tree-ring growth is influenced primarily by subsurface water storage. Other variables related to the overall moisture status (e.g., Standardized Precipitation Index, Palmer Drought Severity Index, streamflow) are also strongly correlated with tree-ring width. While these indices are all indicators of water stored in the landscape, water storage changes of the subsurface estimated by depth-integral measurements give us the unique opportunity to directly reconstruct subsurface water storage dynamics from records of tree-ring width. Such long reconstructions will improve our knowledge of past water storage variations and our ability to predict future developments. Finally, knowing the relationship between subsurface storage dynamics and tree-ring growth improves the understanding of the different signal components contained in tree-ring chronologies.

  3. Coupled beam motion in a storage ring with crab cavities

    DOE PAGES

    Huang, Xiaobiao

    2016-02-16

    We studied the coupled beam motion in a storage ring between the transverse and longitudinal directions introduced by crab cavities. Analytic form of the linear decoupling transformation is derived. Also, the equilibrium bunch distribution in an electron storage ring with a crab cavity is given, including contribution to the eigen-emittance induced by the crab cavity. Furthermore, application to the short pulse generation scheme using crab cavities [1] is considered.

  4. Water, gravity and trees: Relationship of tree-ring widths and total water storage dynamics

    NASA Astrophysics Data System (ADS)

    Creutzfeldt, B.; Heinrich, I.; Merz, B.; Blume, T.; Güntner, A.

    2012-04-01

    Water stored in the subsurface as groundwater or soil moisture is the main fresh water source not only for drinking water and food production but also for the natural vegetation. In a changing environment water availability becomes a critical issue in many different regions. Long-term observations of the past are needed to improve the understanding of the hydrological system and the prediction of future developments. Tree ring data have repeatedly proved to be valuable sources for reconstructing long-term climate dynamics, e.g. temperature, precipitation and different hydrological variables. In water-limited environments, tree growth is primarily influenced by total water stored in the subsurface and hence, tree-ring records usually contain information about subsurface water storage. The challenge is to retrieve the information on total water storage from tree rings, because a training dataset of water stored in the sub-surface is required for calibration against the tree-ring series. However, measuring water stored in the subsurface is notoriously difficult. We here present high-precision temporal gravimeter measurements which allow for the depth-integrated quantification of total water storage dynamics at the field scale. In this study, we evaluate the relationship of total water storage change and tree ring growth also in the context of the complex interactions of other meteorological forcing factors. A tree-ring chronology was derived from a Norway spruce stand in the Bavarian Forest, Germany. Total water storage dynamics were measured directly by the superconducting gravimeter of the Geodetic Observatory Wettzell for a 9-years period. Time series were extended to 63-years period by a hydrological model using gravity data as the only calibration constrain. Finally, water storage changes were reconstructed based on the relationship between the hydrological model and the tree-ring chronology. Measurement results indicate that tree-ring growth is primarily

  5. Single-pass BPM system of the Photon Factory storage ring.

    PubMed

    Honda, T; Katoh, M; Mitsuhashi, T; Ueda, A; Tadano, M; Kobayashi, Y

    1998-05-01

    At the 2.5 GeV ring of the Photon Factory, a single-pass beam-position monitor (BPM) system is being prepared for the storage ring and the beam transport line. In the storage ring, the injected beam position during the first several turns can be measured with a single injection pulse. The BPM system has an adequate performance, useful for the commissioning of the new low-emittance lattice. Several stripline BPMs are being installed in the beam transport line. The continuous monitoring of the orbit in the beam transport line will be useful for the stabilization of the injection energy as well as the injection beam orbit.

  6. Dose estimates for the 1104 m APS storage ring

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

    Moe, H.J.

    1989-06-01

    The estimated dose equivalent rates outside the shielded storage ring, and the estimated annual dose equivalent to members of the public due to direct radiation and skyshine from the ring, have been recalculated. The previous estimates found in LS-84 (MOE 87) and cited in the 1987 Conceptual Design Report of the APS (ANL 87) required revision because of changes in the ring circumference and in the proposed location of the ring with respect to the nearest site boundary. The values assumed for the neutron quality factors were also overestimated (by a factor of 2) in the previous computation, and themore » correct values have been used for this estimate. The methodology used to compute dose and dose rate from the storage ring is the same as that used in LS-90 (MOE 87a). The calculations assumed 80 cm thick walls of ordinary concrete (or the shielding equivalent of this) and a roof thickness of 1 meter of ordinary concrete. The circumference of the ring was increased to 1,104 m, and the closest distance to the boundary was taken as 140 m. The recalculation of the skyshine component used the same methodology as that used in LS-84.« less

  7. The KACST Heavy-Ion Electrostatic Storage Ring

    NASA Astrophysics Data System (ADS)

    Almuqhim, A. A.; Alshammari, S. M.; El Ghazaly, M. O. A.; Papash, A. I.; Welsch, C. P.

    2011-10-01

    A novel Electrostatic Storage Ring (ESR) for beams at energies up to 30keV/q is now being constructed at the National Centre for Mathematics and Physics (NCMP), King Abdul-Aziz City for Science and Technology (KACST). The ring is designed to be the core of a highly flexible experimental platform that will combine a large package of complementary beam techniques for atomic and molecular physics and related fields. The lattice design had to cover the different experimental techniques that the ring will be equipped with, such as e.g. Electron-Ion, Laser-Ion, Ion-Ion or Ion-Neutral beams, in both crossed and merged-beam configurations. The development of such an ESR is realized in a staged approach, in which a simple and early-run adaptation of the ring is built first, and then this basic version is upgraded to a higher symmetry of the ultimate version of the ring. Here, we report a general overview of this technical development with a focus on the layout of the first built stage of the ring.

  8. The KACST Heavy-Ion Electrostatic Storage Ring

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

    Almuqhim, A. A.; Alshammari, S. M.; El Ghazaly, M. O. A.

    2011-10-27

    A novel Electrostatic Storage Ring (ESR) for beams at energies up to 30keV/q is now being constructed at the National Centre for Mathematics and Physics (NCMP), King Abdul-Aziz City for Science and Technology (KACST). The ring is designed to be the core of a highly flexible experimental platform that will combine a large package of complementary beam techniques for atomic and molecular physics and related fields. The lattice design had to cover the different experimental techniques that the ring will be equipped with, such as e.g. Electron-Ion, Laser-Ion, Ion-Ion or Ion-Neutral beams, in both crossed and merged-beam configurations. The developmentmore » of such an ESR is realized in a staged approach, in which a simple and early-run adaptation of the ring is built first, and then this basic version is upgraded to a higher symmetry of the ultimate version of the ring. Here, we report a general overview of this technical development with a focus on the layout of the first built stage of the ring.« less

  9. Study of Storage Ring Free-Electron Laser Using Experimental and Simulation Approaches

    NASA Astrophysics Data System (ADS)

    Jia, Botao

    2011-12-01

    The Duke electron storage ring, first commissioned in November of 1994, has been developed as a dedicated driver for storage ring free-electron lasers (SRFELs) operating in a wide wavelength range from infrared, to visible, to ultraviolet (UV) and vacuum ultraviolet (VUV). The storage ring has a long straight section for various insertion devices and can be operated in a wide energy range (0.25 GeV to 1.15 GeV). Commissioned in 1995, the first free-electron laser (FEL) on the Duke storage ring was the OK-4 FEL, an optical klystron with two planar undulators sandwiching a buncher magnet. In 2005, the OK-5 FEL with two helical undulators was commissioned. Operating four undulators---two OK-4 and two OK-5 undulators, the world's first distributed optical klystron FEL was brought to operation in 2005. Via Compton scattering of FEL photons and electrons in the storage ring, the Duke FEL drives the world's most powerful, nearly monochromatic, and polarized Compton gamma-ray source, the High Intensity Gamma-ray Source (HIgammaS). Today, a variety of configurations of the storage ring FELs at Duke have been used in a wide range of research areas from nuclear physics to biophysics, from chemical and medical research to industrial applications. The capability of accurately measuring the storage ring electron beam energy spread is crucial for understanding the longitudinal beam dynamics and the dynamics of the storage ring FEL. In this dissertation, we have successfully developed a noninvasive, versatile, and accurate method to measure the energy spread using optical klystron radiation. Novel numerical methods based upon the Gauss-Hermite expansion have been developed to treat both spectral broadening and modulation on an equal footing. Through properly configuring the optical klystron, this energy spread measurement method has a large dynamic range. In addition, a model-based scheme has been developed for correcting the electron beam emittance related inhomogeneous spectral

  10. Status of the Frankfurt low energy electrostatic storage ring (FLSR)

    NASA Astrophysics Data System (ADS)

    King, F.; Kruppi, T.; Müller, J.; Dörner, R.; Schmidt, L. Ph H.; Schmidt-Böcking, H.; Stiebing, K. E.

    2015-11-01

    Frankfurt low-energy storage ring (FLSR) is an electrostatic storage ring for low-energy ions up to q · 80 keV (q being the ion charge state) at Institut für Kernphysik der Goethe-Universität, Frankfurt am Main, Germany. It has especially been designed to provide a basis for experiments on the dynamics of ionic and molecular collisions in complete kinematics, as well as for high precision and time resolved laser spectroscopy. The ring has ‘racetrack’ geometry with a circumference of 14.23 m. It comprises four experimental/diagnostic sections with regions of enhanced ion density (interaction regions). First beam has successfully been stored in FLSR in summer 2013. Since then the performance of the ring has continuously been improved and an electron target for experiments on dissociative recombination has been installed in one of the experimental sections.

  11. Future Synchrotron Light Sources Based on Ultimate Storage Rings

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

    Cai, Yunhai; /SLAC

    2012-04-09

    The main purpose of this talk is to describe how far one might push the state of the art in storage ring design. The talk will start with an overview of the latest developments and advances in the design of synchrotron light sources based on the concept of an 'ultimate' storage ring. The review will establish how bright a ring based light source might be, where the frontier of technological challenges are, and what the limits of accelerator physics are. Emphasis will be given to possible improvements in accelerator design and developments in technology toward the goal of achieving anmore » ultimate storage ring. An ultimate storage ring (USR), defined as an electron ring-based light source having an emittance in both transverse planes at the diffraction limit for the range of X-ray wavelengths of interest for a scientific community, would provide very high brightness photons having high transverse coherence that would extend the capabilities of X-ray imaging and probe techniques beyond today's performance. It would be a cost-effective, high-coherence 4th generation light source, competitive with one based on energy recovery linac (ERL) technology, serving a large number of users studying material, chemical, and biological sciences. Furthermore, because of the experience accumulated over many decades of ring operation, it would have the great advantage of stability and reliability. In this paper we consider the design of an USR having 10-pm-rad emittance. It is a tremendous challenge to design a storage ring having such an extremely low emittance, a factor of 100 smaller than those in existing light sources, especially such that it has adequate dynamic aperture and beam lifetime. In many ultra-low emittance designs, the injection acceptances are not large enough for accumulation of the electron beam, necessitating on-axis injection where stored electron bunches are completely replaced with newly injected ones. Recently, starting with the MAX-IV 7-bend achromatic

  12. The Abort Kicker System for the PEP-II Storage Rings at SLAC.

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

    Delamare, Jeffrey E

    2003-06-20

    The PEP-II project has two storage rings. The HER (High Energy Ring) has up to 1.48 A of election beam at 9 GeV, and the LER (Low Energy Ring) has up to 2.14 A of positron beam at 3.1 GeV. To protect the HER and LER beam lines in the event of a ring component failure, each ring has an abort kicker system which directs the beam into a dump when a failure is detected. Due to the high current of the beams, the beam kick is tapered from 100% to 80% in 7.33 {micro}S (the beam transit time aroundmore » the ring). This taper distributes the energy evenly across the window which separates the ring from the beam dump such that the window is not damaged. The abort kicker trigger is synchronized with the ion clearing gap of the beam allowing for the kicker field to rise from 0-80% while there is no beam in the kicker magnet. Originally the kicker system was designed for a rise time of 370nS [1], but because the ion clearing gap was reduced in half, so was the rise time requirement for the kicker. This report discusses the design of the system interlocks, diagnostics, and modulator with the modifications necessary to accommodate an ion clearing gap of 185nS.« less

  13. Feasibility of maintaining in-plane polarization for a storage ring EDM search

    NASA Astrophysics Data System (ADS)

    Stephenson, Edward; Storage Ring EDM Collaboration

    2014-09-01

    A search for an electric dipole moment (EDM) on charged particles using a storage ring requires beam polarization lifetimes approaching 1000 s for in-plane polarization. A feasibility study using beam bunching and sextupole field adjustment is underway with a 0.97-GeV/c vector-polarized deuteron beam at COSY. The polarimeter consists of a thick carbon target positioned at the edge of the beam and the EDDA scintillation detectors. The DAQ system assigns a clock time to each polarimeter event. Once calibrated against the RF-cavity, the clock time is used to select events associated with a maximal sideways polarization (precessing at 120 kHz). With this tool, the in-plane polarization magnitude is tracked versus time. Electron cooling reduces the depolarization from finite emittance and second-order momentum spread acting through synchrotron oscillations. Further lifetime improvement to the level of hundreds of seconds is achieved by adjusting sextupole fields located in the COSY ring arcs at places of large transverse beta functions and dispersion. The dependence of the reciprocal of the lifetime on sextupole field strength is nearly linear, permitting an easy location of the best field values. These typically occur near loci of zero chromaticity. A search for an electric dipole moment (EDM) on charged particles using a storage ring requires beam polarization lifetimes approaching 1000 s for in-plane polarization. A feasibility study using beam bunching and sextupole field adjustment is underway with a 0.97-GeV/c vector-polarized deuteron beam at COSY. The polarimeter consists of a thick carbon target positioned at the edge of the beam and the EDDA scintillation detectors. The DAQ system assigns a clock time to each polarimeter event. Once calibrated against the RF-cavity, the clock time is used to select events associated with a maximal sideways polarization (precessing at 120 kHz). With this tool, the in-plane polarization magnitude is tracked versus time. Electron

  14. Compact Storage Ring for an X-Ray Source

    NASA Astrophysics Data System (ADS)

    Ovchinnikova, L.; Shvedunov, V.; Ivanov, K.

    2017-12-01

    We propose a new design of a compact storage ring for a source of X-ray radiation on the basis of reverse Thomson scattering of laser radiation by electrons with the energy of 35-50 MeV, which has small number of optical elements and a significant clear space for the placement of a beam injection-extraction system and a RF cavity. The original laser cavity layout has been considered. The ring dynamic aperture after correction of chromaticity and a second-order dispersion function is sufficient for the injection and stable circulation of an electron bunch in the ring.

  15. A Model Describing Stable Coherent Synchrotron Radiation in Storage Rings

    NASA Astrophysics Data System (ADS)

    Sannibale, F.; Byrd, J. M.; Loftsdóttir, Á.; Venturini, M.; Abo-Bakr, M.; Feikes, J.; Holldack, K.; Kuske, P.; Wüstefeld, G.; Hübers, H.-W.; Warnock, R.

    2004-08-01

    We present a model describing high power stable broadband coherent synchrotron radiation (CSR) in the terahertz frequency region in an electron storage ring. The model includes distortion of bunch shape from the synchrotron radiation (SR), which enhances higher frequency coherent emission, and limits to stable emission due to an instability excited by the SR wakefield. It gives a quantitative explanation of several features of the recent observations of CSR at the BESSYII storage ring. We also use this model to optimize the performance of a source for stable CSR emission.

  16. Beam vacuum system of Brookhaven`s muon storage ring

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

    Hseuth, H.C.; Snydstrup, L.; Mapes, M.

    1995-11-01

    A storage ring with a circumference of 45 m is being built at Brookhaven to measure the g-2 value of the muons to an accuracy of 0.35 ppm.. The beam vacuum system of the storage ring will operate at 10{sup -7} Torr and has to be completely non-magnetic. It consists of twelve sector chambers. The chambers are constructed of aluminum and are approximately 3.5 m in length with a rectangular cross-section of 16.5 cm high by 45 cm at the widest point. The design features, fabrication techniques and cleaning methods for these chambers are described. The beam vacuum system willmore » be pumped by forty eight non-magnetic distributed ion pumps with a total pumping speed of over 2000 {ell}/sec. Monte Carlo simulations of the pressure distribution in the muon storage region are presented.« less

  17. Planning and Prototyping for a Storage Ring Measurement of the Proton Electric Dipole Moment

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

    Talman, Richard

    2015-07-01

    Electron and proton EDM's can be measured in "frozen spin" (with the beam polarization always parallel to the orbit, for example) storage rings. For electrons the "magic" kinetic energy at which the beam can be frozen is 14.5 MeV. For protons the magic kinetic energy is 230 MeV. The currently measured upper limit for the electron EDM is much smaller than the proton EDM upper limit, which is very poorly known. Nevertheless, because the storage ring will be an order of magnitude cheaper, a sensible plan is to first build an all-electric electron storage ring as a prototype. Such anmore » electron ring was successfully built at Brookhaven, in 1954, as a prototype for their AGS ring. This leaves little uncertainty concerning the cost and performance of such a ring. (This is documentedin one of the Physical Review papers mentioned above.)« less

  18. Effects of CSR Generated from Upstream Bends in a Laser Plasma Storage Ring

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

    Mitchell, C.; Qiang, J.; Venturini, M.

    The recent proposal [1] of a Laser Plasma Storage Ring (LPSR) envisions the use of a laser-plasma (LP) acceleration module to inject an electron beam into a compact 500 MeV storage ring. Electron bunches generated by LP methods are naturally very short (tens of femtoseconds), presenting peak currents on the order of 10 kA or higher. Of obvious concern is the impact of collective effects and in particular Coherent Synchrotron Radiation (CSR) on the beam dynamics in the storage ring. Available simulation codes (e.g. Elegant [2]) usually include transient CSR effects but neglect the contribution of radiation emitted from trailingmore » magnets. In a compact storage ring, with dipole magnets close to each other, cross talking between different magnets could in principle be important.In this note we investigate this effect for the proposed LPSR and show that, in fact, this effect is relatively small. However our analysis also indicates that CSR effects in general would be quite strong and deserve a a careful study.« less

  19. The cryogenic storage ring CSR

    NASA Astrophysics Data System (ADS)

    von Hahn, R.; Becker, A.; Berg, F.; Blaum, K.; Breitenfeldt, C.; Fadil, H.; Fellenberger, F.; Froese, M.; George, S.; Göck, J.; Grieser, M.; Grussie, F.; Guerin, E. A.; Heber, O.; Herwig, P.; Karthein, J.; Krantz, C.; Kreckel, H.; Lange, M.; Laux, F.; Lohmann, S.; Menk, S.; Meyer, C.; Mishra, P. M.; Novotný, O.; O'Connor, A. P.; Orlov, D. A.; Rappaport, M. L.; Repnow, R.; Saurabh, S.; Schippers, S.; Schröter, C. D.; Schwalm, D.; Schweikhard, L.; Sieber, T.; Shornikov, A.; Spruck, K.; Sunil Kumar, S.; Ullrich, J.; Urbain, X.; Vogel, S.; Wilhelm, P.; Wolf, A.; Zajfman, D.

    2016-06-01

    An electrostatic cryogenic storage ring, CSR, for beams of anions and cations with up to 300 keV kinetic energy per unit charge has been designed, constructed, and put into operation. With a circumference of 35 m, the ion-beam vacuum chambers and all beam optics are in a cryostat and cooled by a closed-cycle liquid helium system. At temperatures as low as (5.5 ± 1) K inside the ring, storage time constants of several minutes up to almost an hour were observed for atomic and molecular, anion and cation beams at an energy of 60 keV. The ion-beam intensity, energy-dependent closed-orbit shifts (dispersion), and the focusing properties of the machine were studied by a system of capacitive pickups. The Schottky-noise spectrum of the stored ions revealed a broadening of the momentum distribution on a time scale of 1000 s. Photodetachment of stored anions was used in the beam lifetime measurements. The detachment rate by anion collisions with residual-gas molecules was found to be extremely low. A residual-gas density below 140 cm-3 is derived, equivalent to a room-temperature pressure below 10-14 mbar. Fast atomic, molecular, and cluster ion beams stored for long periods of time in a cryogenic environment will allow experiments on collision- and radiation-induced fragmentation processes of ions in known internal quantum states with merged and crossed photon and particle beams.

  20. The cryogenic storage ring CSR.

    PubMed

    von Hahn, R; Becker, A; Berg, F; Blaum, K; Breitenfeldt, C; Fadil, H; Fellenberger, F; Froese, M; George, S; Göck, J; Grieser, M; Grussie, F; Guerin, E A; Heber, O; Herwig, P; Karthein, J; Krantz, C; Kreckel, H; Lange, M; Laux, F; Lohmann, S; Menk, S; Meyer, C; Mishra, P M; Novotný, O; O'Connor, A P; Orlov, D A; Rappaport, M L; Repnow, R; Saurabh, S; Schippers, S; Schröter, C D; Schwalm, D; Schweikhard, L; Sieber, T; Shornikov, A; Spruck, K; Sunil Kumar, S; Ullrich, J; Urbain, X; Vogel, S; Wilhelm, P; Wolf, A; Zajfman, D

    2016-06-01

    An electrostatic cryogenic storage ring, CSR, for beams of anions and cations with up to 300 keV kinetic energy per unit charge has been designed, constructed, and put into operation. With a circumference of 35 m, the ion-beam vacuum chambers and all beam optics are in a cryostat and cooled by a closed-cycle liquid helium system. At temperatures as low as (5.5 ± 1) K inside the ring, storage time constants of several minutes up to almost an hour were observed for atomic and molecular, anion and cation beams at an energy of 60 keV. The ion-beam intensity, energy-dependent closed-orbit shifts (dispersion), and the focusing properties of the machine were studied by a system of capacitive pickups. The Schottky-noise spectrum of the stored ions revealed a broadening of the momentum distribution on a time scale of 1000 s. Photodetachment of stored anions was used in the beam lifetime measurements. The detachment rate by anion collisions with residual-gas molecules was found to be extremely low. A residual-gas density below 140 cm(-3) is derived, equivalent to a room-temperature pressure below 10(-14) mbar. Fast atomic, molecular, and cluster ion beams stored for long periods of time in a cryogenic environment will allow experiments on collision- and radiation-induced fragmentation processes of ions in known internal quantum states with merged and crossed photon and particle beams.

  1. Fluorescence decay of naphthalene studied in an electrostatic storage ring, the Mini-Ring

    NASA Astrophysics Data System (ADS)

    Martin, S.; Matsumoto, J.; Kono, N.; Ji, M.-C.; Brédy, R.; Bernard, J.; Cassimi, A.; Chen, L.

    2017-10-01

    The cooling of naphthalene cations (C10H8)+ has been studied in a compact electrostatic ion storage ring, the Mini-Ring. A nano second laser pulse of 532 nm (2.33 eV) was used to probe the internal energy distribution every millisecond during the storage time up to 5 ms. The evolution of the internal energy distribution of the stored ions was simulated with a model taking into account the dissociation and the radiative decay processes. Calculated decay curves were fitted to the corresponding laser induced neutral decays. For a laser power of 200 μJ/pulse, a good agreement between experiment and modeling was found using an initial Gaussian energy distribution centered to 5.9 eV and a fluorescence decay rate varying from 200 to 300 s-1 in the energy range from 6 to 7 eV. This fast decay was attributed to the delayed Poincaré fluorescence process.

  2. Design of the transfer line from booster to storage ring at 3 GeV

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

    Bayar, C., E-mail: cafer.bayar@cern.ch; Ciftci, A. K., E-mail: abbas.kenan.ciftci@cern.ch

    The Synchrotron Booster Ring accelerates the e-beam up to 3 GeV and particles are transported from booster to storage ring by transfer line. In this study, two options are considered, the first one is a long booster which shares the same tunnel with storage ring and the second one is a compact booster. As a result, two transfer line are designed based on booster options. The optical design is constrained by the e-beam Twiss parameters entering and leaving the transfer line. Twiss parameters in the extraction point of booster are used for the entrance of transfer line and are matchedmore » in the exit of transfer line to the injection point of the storage ring.« less

  3. Ring profiler: a new method for estimating tree-ring density for improved estimates of carbon storage

    Treesearch

    David W. Vahey; C. Tim Scott; J.Y. Zhu; Kenneth E. Skog

    2012-01-01

    Methods for estimating present and future carbon storage in trees and forests rely on measurements or estimates of tree volume or volume growth multiplied by specific gravity. Wood density can vary by tree ring and height in a tree. If data on density by tree ring could be obtained and linked to tree size and stand characteristics, it would be possible to more...

  4. Simulation of emittance dilution in electron storage ring from Compton backscattering

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

    Blumberg, L.N.; Blum, E.

    1993-07-01

    A Monte-Carlo simulation of Compton backscattered {kappa}{sub L}=3.2-{mu}m photons from an IR-FEL on 75-MeV electrons in a storage ring yields an RMS electron energy spread of {Delta}{sub E}=11.9-keV for a sample of 10{sup 7} single scattering events. Electrons are sampled from a beam of natural energy spread {sigma}{sub E} = 5.6-keV and damped transverse angle spreads {sigma}{sub x}{prime}, = .041-mrad and {sigma}{sub y}{prime} = .052-mrad (100%) coupling, scaled from the 200-MeV BNL XLS compact storage ring. The Compton-scattered X-Rays are generated from an integral of the CM Klein-Nishina cross-section transformed to the lab. A tracking calculation has also been performedmore » in 6-dimensional phase space. Initial electron coordinates are selected randomly from a Gaussian distribution of RMS spreads {sigma}{sub xo}=.102-mm, {sigma}{sub x{prime}o}=.041-mrad, {sigma}{sub yo}=.018-mm, {sigma}{sub y{prime}o}=.052-mrad, {sigma}{sub {phi}o}=22-mrad and {sigma}{sub Eo}=6-keV. A sample of 10000 electrons were each following for 40000 turns around the ring through an RF cavity of f{sub rf}=211.54-MHz and peak voltage V{sub m}=300-keV. Preliminary results indicate that the resulting energy distribution is quite broad with an RMS width of {Delta}{sub E} = 124-keV. The transverse widths are only slightly increased from their original values, i.e. {Delta}{sub x} = .106-mm and {Delta}{sub x}{prime}=.043 mrad. The scaled energy spread of {Delta}{sub E} {approximately} 360-keV for {approximately} 350,000 turns desired in a 10-msec X-Ray angiography exposure is well within the RF bucket used here; even V{sub m} < 50-kV is adequate. Further, the electron energy spread adds a negligible RMS X-Ray energy spread of {Delta}{sub Ex}=.32-keV. The electron energy damping time of {tau}{sub E}=379-msec at 75-MeV in an XLS-type ring allows for damping this induced spread and top-off of the ring between heart cycles.« less

  5. Simulation of emittance dilution in electron storage ring from Compton backscattering

    NASA Astrophysics Data System (ADS)

    Blumberg, L. N.; Blum, E.

    A Monte-Carlo simulation of Compton backscattered kappa(sub L) = 3.2-micron photons from an IR-FEL on 75-MeV electrons in a storage ring yields an RMS electron energy spread of delta(sub E) = 11.9-keV for a sample of 10(exp 7) single scattering events. Electrons are sampled from a beam of natural energy spread sigma(sub E) = 5.6-keV and damped transverse angle spreads sigma(sub x)(prime) = .041-mrad and sigma(sub y)(prime) = .052-mrad (100%) coupling, scaled from the 200-MeV BNL XLS compact storage ring. The Compton-scattered x-rays are generated from an integral of the CM Klein-Nishina cross-section transformed to the lab. A tracking calculation has also been performed in 6-dimensional phase space. Initial electron coordinates are selected randomly from a Gaussian distribution of RMS spreads sigma(sub xo) = .102-mm, sigma(sub x(prime)o) = .041-mrad, sigma(sub yo) = .018-mm, sigma(sub y(prime)o) = .052-mrad, sigma(sub (phi)o) = 22-mrad and sigma(sub Eo) = 6-keV. A sample of 10000 electrons were each following for 40000 turns around the ring through an RF cavity of f(sub RF) = 211.54-MHz and peak voltage V(sub m)=300-keV. Preliminary results indicate that the resulting energy distribution is quite broad with an RMS width of delta(sub E) = 124-keV. The transverse widths are only slightly increased from their original values, i.e. delta(sub x) = .106-mm and delta(sub x)(prime) = .043 mrad. The scaled energy spread of delta(sub E) approximately = 360-keV for approximately 350,000 turns desired in a 10-msec x-ray angiography exposure is well within the RF bucket used here; even V(sub m) less than 50-kV is adequate. Further, the electron energy spread adds a negligible RMS x-ray energy spread of delta(sub Ex) = .32-keV. The electron energy damping time of tau(sub E) = 379-msec at 75-MeV in an XLS-type ring allows for damping this induced spread and top-off of the ring between heart cycles.

  6. The Tunguska event in 1908: evidence from tree-ring anatomy.

    PubMed

    Vaganov, Evgenii A; Hughes, Malcolm K; Silkin, Pavel P; Nesvetailo, Valery D

    2004-01-01

    We analyzed tree rings in wood samples collected from some of the few surviving trees found close to the epicenter (within 4-5 km) of the Tunguska event that occurred on the last day of June 1908. Tree-ring growth shows a depression starting in the year after the event and continuing during a 4-5-year period. The most remarkable traces of the event were found in the rings' anatomical structure: (1) formation of "light" rings and a reduction of maximum density in 1908; (2) non-thickened tracheids (the cells that make up most of the wood volume) in the transition and latewood zones (the middle and last-formed parts of the ring, respectively); and (3) deformed tracheids, which are located on the 1908 annual ring outer boundary. In the majority of samples, normal earlywood and latewood tracheids were formed in all annual rings after 1908. The observed anomalies in wood anatomy suggest two main impacts of the Tunguska event on surviving trees--(1) defoliation and (2) direct mechanical stress on active xylem tissue. The mechanical stress needed to fell trees is less than the stress needed to cause the deformation of differentiating tracheids observed in trees close to the epicenter. In order to resolve this apparent contradiction, work is suggested on possible topographic modification of the overpressure experienced by these trees, as is an experimental test of the effects of such stresses on precisely analogous growing trees.

  7. EUTERPE, a small electron storage ring for XRF

    NASA Astrophysics Data System (ADS)

    Botman, J. I. M.; Mutsaers, P. H. A.; Hagedoorn, H. L.; De Voigt, M. J. A.

    1990-04-01

    A small-sized electron storage ring is under construction at the Eindhoven University of Technology which will cover the energy range of 15 to 400 MeV. At top energy the characteristic wavelength of the synchrotron radiation spectrum is 8.3 nm for the regular dipole magnets and 1.2 nm corresponding to 1.06 keV for a 10 T wiggler magnet. This will provide useful radiation for X-ray fluorescence (XRF) up to 3.2 keV. Alternatively, photon conversion with a high power CO 2 laser beam of 0.124 eV photons will generate X-rays for XRF with energies ranging from 0.5 to 300 keV, depending on the operating energy of the storage ring. This facility will provide an important extension to the activities of the Eindhoven group on PIXE, RBS and microbeam analysis. A short description of the macnine will be given together with applications and specific examples of the XRF method.

  8. Constrained multi-objective optimization of storage ring lattices

    NASA Astrophysics Data System (ADS)

    Husain, Riyasat; Ghodke, A. D.

    2018-03-01

    The storage ring lattice optimization is a class of constrained multi-objective optimization problem, where in addition to low beam emittance, a large dynamic aperture for good injection efficiency and improved beam lifetime are also desirable. The convergence and computation times are of great concern for the optimization algorithms, as various objectives are to be optimized and a number of accelerator parameters to be varied over a large span with several constraints. In this paper, a study of storage ring lattice optimization using differential evolution is presented. The optimization results are compared with two most widely used optimization techniques in accelerators-genetic algorithm and particle swarm optimization. It is found that the differential evolution produces a better Pareto optimal front in reasonable computation time between two conflicting objectives-beam emittance and dispersion function in the straight section. The differential evolution was used, extensively, for the optimization of linear and nonlinear lattices of Indus-2 for exploring various operational modes within the magnet power supply capabilities.

  9. Stochastic events may lead to accretion in Saturn's rings

    NASA Astrophysics Data System (ADS)

    Esposito, Larry W.

    Stochastic events may lead to accretion in Saturn's rings Larry W. Esposito LASP, University of Colorado UVIS occultations indicate accretion is triggered at the B ring edge, in strong density waves in ring A and in the F ring. Moons may trigger accretion by streamline crowding (Lewis & Stewart); which enhances collisions, leading to accretion; increasing random velocities; leading to more collisions and more accretion. Cassini occultations of these strongly perturbed locations show not only accretion but also disaggregation, with time scales of hours to weeks. The collisions may lead to temporary aggregations via stochastic events: collisions can compress unconsolidated objects, trigger adhesion or bring small pieces into contact with larger or higher-density seeds. Disaggregation then can follow from disruptive collisions or tidal shedding. In the accretion/disruption balance, increased random motions could eventually give the upper hand to disruption. . . just as `irrational exuberance' can lead to financial panic in the economy; or the overpopulation of hares can lead to boom-and-bust in the population of foxes. I present a simple predator-prey model. This system's unstable equilibrium can similarly give rise to episodic cycles in accretion: explaining why the observable ring features that indicate embedded objects have been increasing since the beginning of Cassini's observations of Saturn in 2004. Unlike other interpretations of the peculiar events seen near Saturn Equinox, I emphasize the kinetic description of particle interactions rather than a fluid instability approach; and the dominance of stochastic events involving individual aggregates over free and/or driven modes in a flat disk.

  10. Low-emittance tuning of storage rings using normal mode beam position monitor calibration

    NASA Astrophysics Data System (ADS)

    Wolski, A.; Rubin, D.; Sagan, D.; Shanks, J.

    2011-07-01

    We describe a new technique for low-emittance tuning of electron and positron storage rings. This technique is based on calibration of the beam position monitors (BPMs) using excitation of the normal modes of the beam motion, and has benefits over conventional methods. It is relatively fast and straightforward to apply, it can be as easily applied to a large ring as to a small ring, and the tuning for low emittance becomes completely insensitive to BPM gain and alignment errors that can be difficult to determine accurately. We discuss the theory behind the technique, present some simulation results illustrating that it is highly effective and robust for low-emittance tuning, and describe the results of some initial experimental tests on the CesrTA storage ring.

  11. Beam Loss Measurements at the Los Alamos Proton Storage Ring

    NASA Astrophysics Data System (ADS)

    Spickermann, Thomas

    2005-06-01

    During normal operation the Los Alamos Proton Storage Ring (PSR) accumulates up to 4ṡ1013 protons over 625μs with a repetition rate of 20 Hz, corresponding to a current of 125μA to the Lujan Neutron Science Center. Beam losses in the ring as well as in the extraction beam line and the subsequent activation of material are a limiting factor at these currents. Careful tuning of injection, ring and extraction line is paramount to limiting losses to acceptable levels. Losses are typically not uniform around the ring, but occur in significantly higher levels in certain "hot spots". Here I will report on losses related to the stripper foil which are the dominant source of losses in the ring. First results of a comparison with simulations will also be presented.

  12. Storage rings for spin-polarized hydrogen

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

    Thompson, D.; Lovelace, R.V.E.; Lee, D.

    1989-11-01

    A strong-focusing storage ring is proposed for the long-term magnetic confinement of a collisional gas of neutral spin-polarized hydrogen atoms in the Za{l arrow} and Zb{l arrow} hyperfine states. The trap uses the interaction of the magnetic moments of the gas atoms with a static magnetic field. Laser cooling and evaporative cooling can be utilized to enhance the confinement and to offset the influence of viscous heating. An important application of the trap is to the attainment of Bose--Einstein condensation.

  13. High resolution monochromator for the VUV radiation from the DORIS storage ring

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

    Saile, V.; Gurtler, P.; Koch, E.E.

    1976-10-01

    The unique properties of the DORIS storage ring at DESY as a synchroton radiation source are exploited for high resolution spectroscopy in the vacuum ultraviolet. We describe a new experimental set up with a 3-m normal incidence monochromator for wavelengths between 3000 A and 300 A (4 < or = h..omega.. < or = 40 eV) using a vertical dispersion plane. The storage ring provides a light flux intense and stable enough for rapid photoelectrical scanning of the spectra with a resolution of 0.03 A in first order. (AIP)

  14. Feasibility of a ring FEL at low emittance storage rings

    NASA Astrophysics Data System (ADS)

    Agapov, I.

    2015-09-01

    A scheme for generating coherent radiation at latest generation low emittance storage rings such as PETRA III at DESY (Balewski et al., 2004 [1]) is proposed. The scheme is based on focusing and subsequent defocusing of the electron beam in the longitudinal phase space at the undulator location. The expected performance characteristics are estimated for radiation in the wavelength range of 500-1500 eV. It is shown that the average brightness is increased by several orders of magnitude compared to spontaneous undulator radiation, which can open new perspectives for photon-hungry soft X-ray spectroscopy techniques.

  15. ACCELERATORS: Beam based alignment of the SSRF storage ring

    NASA Astrophysics Data System (ADS)

    Zhang, Man-Zhou; Li, Hao-Hu; Jiang, Bo-Cheng; Liu, Gui-Min; Li, De-Ming

    2009-04-01

    There are 140 beam position monitors (BPMs) in the Shanghai Synchrotron Radiation Facility (SSRF) storage ring used for measuring the closed orbit. As the BPM pickup electrodes are assembled directly on the vacuum chamber, it is important to calibrate the electrical center offset of the BPM to an adjacent quadrupole magnetic center. A beam based alignment (BBA) method which varies individual quadrupole magnet strength and observes its effects on the orbit is used to measure the BPM offsets in both the horizontal and vertical planes. It is a completely automated technique with various data processing methods. There are several parameters such as the strength change of the correctors and the quadrupoles which should be chosen carefully in real measurement. After several rounds of BBA measurement and closed orbit correction, these offsets are set to an accuracy better than 10 μm. In this paper we present the method of beam based calibration of BPMs, the experimental results of the SSRF storage ring, and the error analysis.

  16. Symplectic orbit and spin tracking code for all-electric storage rings

    NASA Astrophysics Data System (ADS)

    Talman, Richard M.; Talman, John D.

    2015-07-01

    Proposed methods for measuring the electric dipole moment (EDM) of the proton use an intense, polarized proton beam stored in an all-electric storage ring "trap." At the "magic" kinetic energy of 232.792 MeV, proton spins are "frozen," for example always parallel to the instantaneous particle momentum. Energy deviation from the magic value causes in-plane precession of the spin relative to the momentum. Any nonzero EDM value will cause out-of-plane precession—measuring this precession is the basis for the EDM determination. A proposed implementation of this measurement shows that a proton EDM value of 10-29e -cm or greater will produce a statistically significant, measurable precession after multiply repeated runs, assuming small beam depolarization during 1000 s runs, with high enough precision to test models of the early universe developed to account for the present day particle/antiparticle population imbalance. This paper describes an accelerator simulation code, eteapot, a new component of the Unified Accelerator Libraries (ual), to be used for long term tracking of particle orbits and spins in electric bend accelerators, in order to simulate EDM storage ring experiments. Though qualitatively much like magnetic rings, the nonconstant particle velocity in electric rings gives them significantly different properties, especially in weak focusing rings. Like the earlier code teapot (for magnetic ring simulation) this code performs exact tracking in an idealized (approximate) lattice rather than the more conventional approach, which is approximate tracking in a more nearly exact lattice. The Bargmann-Michel-Telegdi (BMT) equation describing the evolution of spin vectors through idealized bend elements is also solved exactly—original to this paper. Furthermore the idealization permits the code to be exactly symplectic (with no artificial "symplectification"). Any residual spurious damping or antidamping is sufficiently small to permit reliable tracking for the

  17. Colliding or co-rotating ion beams in storage rings for EDM search

    NASA Astrophysics Data System (ADS)

    Koop, I. A.

    2015-11-01

    A new approach to search for and measure the electric dipole moment (EDM) of the proton, deuteron and some other light nuclei is presented. The idea of the method is to store two ion beams, circulating with different velocities, in a storage ring with crossed electric and magnetic guiding fields. One beam is polarized and its EDM is measured using the so-called ‘frozen spin’ method. The second beam, which is unpolarized, is used as a co-magnetometer, sensitive to the radial component of the ring’s magnetic field. The particle’s magnetic dipole moment (MDM) couples to the radial magnetic field and mimics the EDM signal. Measuring the relative vertical orbit separation of the two beams, caused by the presence of the radial magnetic field, one can control the unwanted MDM spin precession. Examples of the parameters for EDM storage rings for protons and other species of ions are presented. The use of crossed electric and magnetic fields helps to reduce the size of the ring by a factor of 10-20. We show that the bending radius of such an EDM storage ring could be about 2-3 m. Finally, a new method of increasing the spin coherence time, the so-called ‘spin wheel’, is proposed and its applicability to the EDM search is discussed.

  18. Intra-Beam Scattering, Impedance, and Instabilities in Ultimate Storage Rings

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

    Bane, Karl; /SLAC

    We have investigated collective effects in an ultimate storage ring, i.e. one with diffraction limited emittances in both planes, using PEP-X as an example. In an ultimate ring intra-beam scattering (IBS) sets the limit of current that can be stored. In PEP-X, a 4.5 GeV ring running round beams at 200 mA in 3300 bunches, IBS doubles the emittances to 11.5 pm at the design current. The Touschek lifetime is 11 hours. Impedance driven collective effects tend not to be important since the beam current is relatively low. We have investigated collective effects in PEP-X, an ultimate storage ring, i.e.more » one with diffraction limited emittances (at one angstrom wavelength) in both planes. In an ultimate ring intra-beam scattering (IBS) sets the limit of current that can be stored. In PEP-X, IBS doubles the emittances to 11.5 pm at the design current of 200 mA, assuming round beams. The Touschek lifetime is quite large in PEP-X, 11.6 hours, and - near the operating point - increases with decreasing emittance. It is, however, a very sensitive function of momentum acceptance. In an ultimate ring like PEP-X impedance driven collective effects tend not to be important since the beam current is relatively low. Before ultimate PEP-X can be realized, the question of how to run a machine with round beams needs serious study. For example, in this report we assumed that the vertical emittance is coupling dominated. It may turn out that using vertical dispersion is a preferable way to generate round beams. The choice will affect IBS and the Touschek effect.« less

  19. Burton Richter, Storage Rings, and the J/psi Particle

    Science.gov Websites

    [SLAC's] Technical Director, [Richter] became Director ... from 1984 through 1999. During his tenure, SLAC Limits of Quantum Electro-dynamics, DOE Technical Report, June 1959 Design Considerations for High Energy Electron -- Positron Storage Rings, DOE Technical Report, November 1966 Inclusive Yields of pi+, pi-, K

  20. Tree- Rings Link Climate and Carbon Storage in a Northern Mixed Hardwood Forest

    NASA Astrophysics Data System (ADS)

    Chiriboga, A.

    2007-12-01

    The terrestrial biosphere is a variable sink for atmospheric carbon dioxide. It is important to understand how carbon storage in trees is affected by natural climate variability to better characterize the sink. Quantifying the sensitivity of forest carbon storage to climate will improve carbon budgets and have implications for forest management practices. Here we explore how climate variability affects the ability of a northern mixed hardwood forest in Michigan to sequester atmospheric carbon dioxide in woody tissues. This site is ideal for studies of carbon sequestration; The University of Michigan Biological Station is an Ameriflux site, and has detailed meteorological and biometric records, as well as CO2 flux data. We have produced an 82- year aspen (Populus grandidentata) tree-ring chronology for this site, and measured ring widths at several heights up the bole. These measurements were used to estimate annual wood volume, which represents carbon allocated to aboveground carbon stores. Standard dendroclimatological techniques are used to identify environmental factors (e.g. temperature or precipitation) that drive tree-ring increment variability in the past century, and therefore annual carbon storage in this forest. Preliminary results show that marker years within the tree- ring chronology correspond with years that have cold spring temperatures. This suggests that trees at this site are temperature sensitive.

  1. FLSR - The Frankfurt low energy storage ring

    NASA Astrophysics Data System (ADS)

    Stiebing, K. E.; Alexandrov, V.; Dörner, R.; Enz, S.; Kazarinov, N. Yu.; Kruppi, T.; Schempp, A.; Schmidt Böcking, H.; Völp, M.; Ziel, P.; Dworak, M.; Dilfer, W.

    2010-02-01

    An electrostatic storage ring for low-energy ions with a design energy of 50 keV is presently being set up at the Institut für Kernphysik der Johann Wolfgang Goethe-Universität Frankfurt am Main, Germany (IKF). This new device will provide a basis for new experiments on the dynamics of ionic and molecular collisions, as well as for high precision and time resolved laser spectroscopy. In this article, the design parameters of this instrument are reported.

  2. Symplectic orbit and spin tracking code for all-electric storage rings

    DOE PAGES

    Talman, Richard M.; Talman, John D.

    2015-07-22

    Proposed methods for measuring the electric dipole moment (EDM) of the proton use an intense, polarized proton beam stored in an all-electric storage ring “trap.” At the “magic” kinetic energy of 232.792 MeV, proton spins are “frozen,” for example always parallel to the instantaneous particle momentum. Energy deviation from the magic value causes in-plane precession of the spin relative to the momentum. Any nonzero EDM value will cause out-of-plane precession—measuring this precession is the basis for the EDM determination. A proposed implementation of this measurement shows that a proton EDM value of 10 –29e–cm or greater will produce a statisticallymore » significant, measurable precession after multiply repeated runs, assuming small beam depolarization during 1000 s runs, with high enough precision to test models of the early universe developed to account for the present day particle/antiparticle population imbalance. This paper describes an accelerator simulation code, eteapot, a new component of the Unified Accelerator Libraries (ual), to be used for long term tracking of particle orbits and spins in electric bend accelerators, in order to simulate EDM storage ring experiments. Though qualitatively much like magnetic rings, the nonconstant particle velocity in electric rings gives them significantly different properties, especially in weak focusing rings. Like the earlier code teapot (for magnetic ring simulation) this code performs exact tracking in an idealized (approximate) lattice rather than the more conventional approach, which is approximate tracking in a more nearly exact lattice. The Bargmann-Michel-Telegdi (BMT) equation describing the evolution of spin vectors through idealized bend elements is also solved exactly—original to this paper. Furthermore the idealization permits the code to be exactly symplectic (with no artificial “symplectification”). Any residual spurious damping or antidamping is sufficiently small to permit

  3. The MAX IV storage ring project

    PubMed Central

    Tavares, Pedro F.; Leemann, Simon C.; Sjöström, Magnus; Andersson, Åke

    2014-01-01

    The MAX IV facility, currently under construction in Lund, Sweden, features two electron storage rings operated at 3 GeV and 1.5 GeV and optimized for the hard X-ray and soft X-ray/VUV spectral ranges, respectively. A 3 GeV linear accelerator serves as a full-energy injector into both rings as well as a driver for a short-pulse facility, in which undulators produce X-ray pulses as short as 100 fs. The 3 GeV ring employs a multibend achromat (MBA) lattice to achieve, in a relatively short circumference of 528 m, a bare lattice emittance of 0.33 nm rad, which reduces to 0.2 nm rad as insertion devices are added. The engineering implementation of the MBA lattice raises several technological problems. The large number of strong magnets per achromat calls for a compact design featuring small-gap combined-function magnets grouped into cells and sharing a common iron yoke. The small apertures lead to a low-conductance vacuum chamber design that relies on the chamber itself as a distributed copper absorber for the heat deposited by synchrotron radiation, while non-evaporable getter (NEG) coating provides for reduced photodesorption yields and distributed pumping. Finally, a low main frequency (100 MHz) is chosen for the RF system yielding long bunches, which are further elongated by passively operated third-harmonic Landau cavities, thus alleviating collective effects, both coherent (e.g. resistive wall instabilities) and incoherent (intrabeam scattering). In this paper, we focus on the MAX IV 3 GeV ring and present the lattice design as well as the engineering solutions to the challenges inherent to such a design. As the first realisation of a light source based on the MBA concept, the MAX IV 3 GeV ring offers an opportunity for validation of concepts that are likely to be essential ingredients of future diffraction-limited light sources. PMID:25177978

  4. Fundamentals of Coherent Synchrotron Radiation in Storage Rings

    NASA Astrophysics Data System (ADS)

    Sannibale, F.; Byrd, J. M.; Loftsdottir, A.; Martin, M. C.; Venturini, M.

    2004-05-01

    We present the fundamental concepts for producing stable broadband coherent synchrotron radiation (CSR) in the terahertz frequency region in an electron storage ring. The analysis includes distortion of bunch shape from the synchrotron radiation (SR), enhancing higher frequency coherent emission and limits to stable emission due to a microbunching instability excited by the SR. We use these concepts to optimize the performance of a source for CSR emission.

  5. Picosecond, tunable, high-brightness hard x-ray inverse Compton source at Duke storage ring

    NASA Astrophysics Data System (ADS)

    Litvinenko, Vladimir N.; Wu, Ying; Burnham, Bentley; Barnett, Genevieve A.; Madey, John M. J.

    1995-09-01

    We suggest a state-of-the art x-ray source using a compact electron storage ring with modest energy (less than 1 GeV) and a high power mm-wave as an undulator. A source of this type has x-ray energies and brightness comparable with third generation synchrotron light sources while it can be very compact and fit in a small university or industrial laboratory or hospital. We propose to operate an isochronous mm-wave FEL and a hard x-ray inverse Compton source at the Duke storage ring to test this concept. Resonant FEL conditions for the mm- wave will be provided by the off-axis interaction with an electromagnetic wave. A special optical resonator with holes for the e-beam is proposed for pumping a hard x-ray inverse Compton source with very high brightness. Simulation results of mm-wave FEL operation of the Duke storage ring are discussed. Expected performance of mm-wave FEL and hard x-ray inverse Compton source are presented.

  6. NSLS-II storage ring insertion device and front-end commissioning and operation

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

    Wang, G., E-mail: gwang@bnl.gov; Shaftan, T.; Amundsen, C.

    The National Synchrotron Light Source II (NSLS-II) is a state of the art 3 GeV third generation light source at Brookhaven National Laboratory. During spring/ summer of 2014, the storage ring was commissioned up to 50 mA without insertion devices. In the fall of 2014, we began commissioning of the project beamlines, which included seven insertion devices on six ID ports. Beamlines IXS, HXN, CSX-1, CSX-2, CHX, SRX, and XPD-1 consist of elliptically polarized undulator (EPU), damping wigglers (DW) and in-vacuum undulators (IVU) covering from VUV to hard x-ray range. In this paper, experience with commissioning and operation is discussed.more » We focus on reaching storage ring performance with IDs, including injection, design emittance, compensation of orbit distortions caused by ID residual field, source point stability, beam alignment and tools for control, monitoring and protection of the ring chambers from ID radiation.« less

  7. Dielectronic recombination experiments at the storage rings: From the present CSR to the future HIAF

    NASA Astrophysics Data System (ADS)

    Huang, Z. K.; Wen, W. Q.; Xu, X.; Wang, H. B.; Dou, L. J.; Chuai, X. Y.; Zhu, X. L.; Zhao, D. M.; Li, J.; Ma, X. M.; Mao, L. J.; Yang, J. C.; Yuan, Y. J.; Xu, W. Q.; Xie, L. Y.; Xu, T. H.; Yao, K.; Dong, C. Z.; Zhu, L. F.; Ma, X.

    2017-10-01

    Dielectronic recombination (DR) experiments of highly charged ions at the storage rings have been developed as a precision spectroscopic tool to investigate the atomic structure as well as nuclear properties of stable and unstable nuclei. The DR experiment on lithium-like argon ions was successfully performed at main Cooler Storage Ring (CSRm) at Heavy Ion Research Facility in Lanzhou (HIRFL) accelerator complex. The DR experiments on heavy highly charged ions and even radioactive ions are currently under preparation at the experimental Cooler Storage Ring (CSRe) at HIRFL. The current status of DR experiments at the CSRm and the preparation of the DR experiments at the CSRe are presented. In addition, an overview of DR experiments by employing an electron cooler and a separated ultra-cold electron target at the upcoming High Intensity heavy ion Accelerator Facility (HIAF) will be given.

  8. ACCELERATORS: Preliminary application of turn-by-turn data analysis to the SSRF storage ring

    NASA Astrophysics Data System (ADS)

    Chen, Jian-Hui; Zhao, Zhen-Tang

    2009-07-01

    There is growing interest in utilizing the beam position monitor turn-by-turn (TBT) data to debug accelerators. TBT data can be used to determine the linear optics, coupled optics and nonlinear behaviors of the storage ring lattice. This is not only a useful complement to other methods of determining the linear optics such as LOCO, but also provides a possibility to uncover more hidden phenomena. In this paper, a preliminary application of a β function measurement to the SSRF storage ring is presented.

  9. Analysis of Methods to Excite Head-Tail Motion Within the Cornell Electron Storage Ring

    NASA Astrophysics Data System (ADS)

    Gendler, Naomi; Billing, Mike; Shanks, Jim

    The main accelerator complex at Cornell consists of two rings around which electrons and positrons move: the synchrotron, where the particles are accelerated to 5 GeV, and the Storage Ring, where the particles circulate a ta Þxed energy, guided by quadrupole and dipole magnets, with a steady energy due to a sinusoidal voltage source. Keeping the beam stable in the Storage Ring is crucial for its lifetime. A long-lasting, invariable beam means more accurate experiments, as well as brighter, more focused X-rays for use in the Cornell High Energy Synchrotron Source (CHESS). The stability of the electron and positron beams in the Cornell Electron Storage Ring (CESR) is important for the development of accelerators and for usage of the beam in X-ray science and accelerator physics. Bunch oscillations tend to enlarge the beam's cross section, making it less stable. We believe that one such oscillation is ``head-tail motion,'' where the bunch rocks back and forth on a pivot located at the central particle. In this project, we write a simulation of the bunch that induces head-tail motion with a vertical driver. We also excite this motion physically in the storage ring, and observe a deÞnite head-tail signal. In the experiment, we saw a deÞnite persistence of the drive-damp signal within a small band around the head-tail frequency, indicating that the head-tail frequency is a natural vertical mode of the bunch that was being excited. The signal seen in the experiment matched the signal seen in the simulation to within an order of magnitude.

  10. Preparing the MAX IV storage rings for timing-based experiments

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

    Stråhlman, C., E-mail: Christian.Strahlman@maxlab.lu.se; Olsson, T., E-mail: Teresia.Olsson@maxlab.lu.se; Leemann, S. C.

    2016-07-27

    Time-resolved experimental techniques are increasingly abundant at storage ring facilities. Recent developments in accelerator technology and beamline instrumentation allow for simultaneous operation of high-intensity and timing-based experiments. The MAX IV facility is a state-of-the-art synchrotron light source in Lund, Sweden, that will come into operation in 2016. As many storage ring facilities are pursuing upgrade programs employing strong-focusing multibend achromats and passive harmonic cavities (HCs) in high-current operation, it is of broad interest to study the accelerator and instrumentation developments required to enable timing-based experiments at such machines. In particular, the use of hybrid filling modes combined with pulse pickingmore » by resonant excitation or pseudo single bunch has shown promising results. These methods can be combined with novel beamline instrumentation, such as choppers and instrument gating. In this paper we discuss how these techniques can be implemented and employed at MAX IV.« less

  11. Multi-objective dynamic aperture optimization for storage rings

    DOE PAGES

    Li, Yongjun; Yang, Lingyun

    2016-11-30

    We report an efficient dynamic aperture (DA) optimization approach using multiobjective genetic algorithm (MOGA), which is driven by nonlinear driving terms computation. It was found that having small low order driving terms is a necessary but insufficient condition of having a decent DA. Then direct DA tracking simulation is implemented among the last generation candidates to select the best solutions. The approach was demonstrated successfully in optimizing NSLS-II storage ring DA.

  12. An analog RF gap voltage regulation system for the Advanced Photon Source storage ring.

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

    Horan, D.

    1999-04-13

    An analog rf gap voltage regulation system has been designed and built at Argonne National Laboratory to maintain constant total storage ring rf gap voltage, independent of beam loading and cavity tuning effects. The design uses feedback control of the klystron mod-anode voltage to vary the amount of rf power fed to the storage ring cavities. The system consists of two independent feedback loops, each regulating the combined rf gap voltages of eight storage ring cavities by varying the output power of either one or two rf stations, depending on the mode of operation. It provides full operator control andmore » permissive logic to permit feedback control of the rf system output power only if proper conditions are met. The feedback system uses envelope-detected cavity field probe outputs as the feedback signal. Two different methods of combining the individual field probe signals were used to generate a relative DC level representing one-half of the total storage ring rf voltage, an envelope-detected vector sum of the field probe rf signals, and the DC sum of individual field probe envelope detector outputs. The merits of both methods are discussed. The klystron high-voltage power supply (HVPS) units are fitted with an analog interface for external control of the mod-anode voltage level, using a four-quadrant analog multiplier to modulate the HVPS mod-anode voltage regulator set-point in response to feedback system commands.« less

  13. Pseudo-single-bunch mode for a 100 MHz storage ring serving soft X-ray timing experiments

    NASA Astrophysics Data System (ADS)

    Olsson, T.; Leemann, S. C.; Georgiev, G.; Paraskaki, G.

    2018-06-01

    At many storage rings for synchrotron light production there is demand for serving both high-flux and timing users simultaneously. Today this is most commonly achieved by operating inhomogeneous fill patterns, but this is not preferable for rings that employ passive harmonic cavities to damp instabilities and increase Touschek lifetime. For these rings, inhomogeneous fill patterns could severely reduce the effect of the harmonic cavities. It is therefore of interest to develop methods to serve high-flux and timing users simultaneously without requiring gaps in the fill pattern. One such method is pseudo-single-bunch (PSB), where one bunch in the bunch train is kicked onto another orbit by a fast stripline kicker. The light emitted from the kicked bunch can then be separated by an aperture in the beamline. Due to recent developments in fast kicker design, PSB operation in multibunch mode is within reach for rings that operate with a 100 MHz RF system, such as the MAX IV and Solaris storage rings. This paper describes machine requirements and resulting performance for such a mode at the MAX IV 1.5 GeV storage ring. A solution for serving all beamlines is discussed as well as the consequences of beamline design and operation in the soft X-ray energy range.

  14. Measurement of Systematic Error Effects for a Sensitive Storage Ring EDM Polarimeter

    NASA Astrophysics Data System (ADS)

    Imig, Astrid; Stephenson, Edward

    2009-10-01

    The Storage Ring EDM Collaboration was using the Cooler Synchrotron (COSY) and the EDDA detector at the Forschungszentrum J"ulich to explore systematic errors in very sensitive storage-ring polarization measurements. Polarized deuterons of 235 MeV were used. The analyzer target was a block of 17 mm thick carbon placed close to the beam so that white noise applied to upstream electrostatic plates increases the vertical phase space of the beam, allowing deuterons to strike the front face of the block. For a detector acceptance that covers laboratory angles larger than 9 ^o, the efficiency for particles to scatter into the polarimeter detectors was about 0.1% (all directions) and the vector analyzing power was about 0.2. Measurements were made of the sensitivity of the polarization measurement to beam position and angle. Both vector and tensor asymmetries were measured using beams with both vector and tensor polarization. Effects were seen that depend upon both the beam geometry and the data rate in the detectors.

  15. Generalized Stability Conditions for an Ultra-Low Energy Electrostatic Charged Particle Storage Ring

    NASA Astrophysics Data System (ADS)

    Sullivan, Michael

    A low energy (~50 eV) electrostatic storage ring has been constructed that can store a recirculating bunch of either electrons or ions. The charged particle bunch 'orbits' within an apparatus consisting of four lenses and two hemispherical deflector analysers, arranged in a 'race-track' configuration of length 64.1 cm. A theoretical study, using transfer matrices from charged particle optics for a 'symmetric' configuration of lens potentials, has been previously completed by Hammond et al. [New J. Phys. 11 (2009) 043033]. That approach was capable of predicting modes of storage which appeared as a resonant-like pattern. An 'asymmetric' configuration, new in this work and extending the previous study to apply to a more general case, has been completed and will be presented alongside experimental results. The level of agreement between the theoretical and experimental results is found to be excellent, and the robustness of the matrix formalism has eliminated the need to rely on computer simulation to achieve storage. This asymmetric arrangement of the lenses allows for greater flexibility in the operation of the ring, creating the potential for a more diverse range of applications and potentially aid in the design of future rings. Several spectra for both electrons and positive ions are presented to provide an indication as to how the charged particle bunch evolves as more orbits are completed. The number of counts inevitably decreases as a function of orbit number due to loss mechanisms. Enhanced measurement techniques, as well as the matrix theory, have made storage of the bunch for over a hundred orbits routine, corresponding to over 65 m travelled, and this is observed directly from the spectra. The application of the storage ring as a multi-pass time-of-flight mass spectrometer has been studied. The isotopes of krypton and xenon have been made to completely separate from one another out of a single pulse of ions. This is observed to occur after ~15 orbits of the

  16. A multiple-orbit time-of-flight mass spectrometer based on a low energy electrostatic storage ring

    NASA Astrophysics Data System (ADS)

    Sullivan, M. R.; Spanjers, T. L.; Thorn, P. A.; Reddish, T. J.; Hammond, P.

    2012-11-01

    The results are presented for an electrostatic storage ring, consisting of two hemispherical deflector analyzers (HDA) connected by two separate sets of cylindrical lenses, used as a time-of-flight mass spectrometer. Based on the results of charged particle simulations and formal matrix model, the Ion Storage Ring is capable of operating with multiple stable orbits, for both single and multiply charged ions simultaneously.

  17. PEGASYS---A proposed internal target facility for the PEP storage ring

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

    Van Biber, K.

    A proposal for an integral gas-jet target and forward spectrometer for the PEP storage ring is described. The beam structure, allowable, luminosity (L = 10/sup 33/ cm/sup /minus/2/s/sup /minus/1/ for H/sub 2/, D/sub 2/) and energy (E/sub e/ less than or equal to 15 GeV) make the ring ideal for multiparticle coincidence studies in the scaling regime, and where perturbative QCD may be an apt description of some exclusive and semi-inclusive reactions. 14 refs., 7 figs.

  18. First storage of ion beams in the Double Electrostatic Ion-Ring Experiment: DESIREE.

    PubMed

    Schmidt, H T; Thomas, R D; Gatchell, M; Rosén, S; Reinhed, P; Löfgren, P; Brännholm, L; Blom, M; Björkhage, M; Bäckström, E; Alexander, J D; Leontein, S; Hanstorp, D; Zettergren, H; Liljeby, L; Källberg, A; Simonsson, A; Hellberg, F; Mannervik, S; Larsson, M; Geppert, W D; Rensfelt, K G; Danared, H; Paál, A; Masuda, M; Halldén, P; Andler, G; Stockett, M H; Chen, T; Källersjö, G; Weimer, J; Hansen, K; Hartman, H; Cederquist, H

    2013-05-01

    We report on the first storage of ion beams in the Double ElectroStatic Ion Ring ExpEriment, DESIREE, at Stockholm University. We have produced beams of atomic carbon anions and small carbon anion molecules (C(n)(-), n = 1, 2, 3, 4) in a sputter ion source. The ion beams were accelerated to 10 keV kinetic energy and stored in an electrostatic ion storage ring enclosed in a vacuum chamber at 13 K. For 10 keV C2 (-) molecular anions we measure the residual-gas limited beam storage lifetime to be 448 s ± 18 s with two independent detector systems. Using the measured storage lifetimes we estimate that the residual gas pressure is in the 10(-14) mbar range. When high current ion beams are injected, the number of stored particles does not follow a single exponential decay law as would be expected for stored particles lost solely due to electron detachment in collision with the residual-gas. Instead, we observe a faster initial decay rate, which we ascribe to the effect of the space charge of the ion beam on the storage capacity.

  19. Analysis and correction of linear optics errors, and operational improvements in the Indus-2 storage ring

    NASA Astrophysics Data System (ADS)

    Husain, Riyasat; Ghodke, A. D.

    2017-08-01

    Estimation and correction of the optics errors in an operational storage ring is always vital to achieve the design performance. To achieve this task, the most suitable and widely used technique, called linear optics from closed orbit (LOCO) is used in almost all storage ring based synchrotron radiation sources. In this technique, based on the response matrix fit, errors in the quadrupole strengths, beam position monitor (BPM) gains, orbit corrector calibration factors etc. can be obtained. For correction of the optics, suitable changes in the quadrupole strengths can be applied through the driving currents of the quadrupole power supplies to achieve the desired optics. The LOCO code has been used at the Indus-2 storage ring for the first time. The estimation of linear beam optics errors and their correction to minimize the distortion of linear beam dynamical parameters by using the installed number of quadrupole power supplies is discussed. After the optics correction, the performance of the storage ring is improved in terms of better beam injection/accumulation, reduced beam loss during energy ramping, and improvement in beam lifetime. It is also useful in controlling the leakage in the orbit bump required for machine studies or for commissioning of new beamlines.

  20. Model-independent and fast determination of optical functions in storage rings via multiturn and closed-orbit data

    NASA Astrophysics Data System (ADS)

    Riemann, Bernard; Grete, Patrick; Weis, Thomas

    2011-06-01

    Multiturn (or turn-by-turn) data acquisition has proven to be a new source of direct measurements for Twiss parameters in storage rings. On the other hand, closed-orbit measurements are a long-known tool for analyzing closed-orbit perturbations with conventional beam position monitor (BPM) systems and are necessarily available at every storage ring. This paper aims at combining the advantages of multiturn measurements and closed-orbit data. We show that only two multiturn BPMs and four correctors in one localized drift space in the storage ring (diagnostic drift) are sufficient for model-independent and absolute measuring of β and φ functions at all BPMs, including the conventional ones, instead of requiring all BPMs being equipped with multiturn electronics.

  1. Phase measurement for driven spin oscillations in a storage ring

    NASA Astrophysics Data System (ADS)

    Hempelmann, N.; Hejny, V.; Pretz, J.; Soltner, H.; Augustyniak, W.; Bagdasarian, Z.; Bai, M.; Barion, L.; Berz, M.; Chekmenev, S.; Ciullo, G.; Dymov, S.; Eversmann, D.; Gaisser, M.; Gebel, R.; Grigoryev, K.; Grzonka, D.; Guidoboni, G.; Heberling, D.; Hetzel, J.; Hinder, F.; Kacharava, A.; Kamerdzhiev, V.; Keshelashvili, I.; Koop, I.; Kulikov, A.; Lehrach, A.; Lenisa, P.; Lomidze, N.; Lorentz, B.; Maanen, P.; Macharashvili, G.; Magiera, A.; Mchedlishvili, D.; Mey, S.; Müller, F.; Nass, A.; Nikolaev, N. N.; Nioradze, M.; Pesce, A.; Prasuhn, D.; Rathmann, F.; Rosenthal, M.; Saleev, A.; Schmidt, V.; Semertzidis, Y.; Senichev, Y.; Shmakova, V.; Silenko, A.; Slim, J.; Stahl, A.; Stassen, R.; Stephenson, E.; Stockhorst, H.; Ströher, H.; Tabidze, M.; Tagliente, G.; Talman, R.; Thörngren Engblom, P.; Trinkel, F.; Uzikov, Yu.; Valdau, Yu.; Valetov, E.; Vassiliev, A.; Weidemann, C.; Wrońska, A.; Wüstner, P.; Zuprański, P.; Żurek, M.; JEDI Collaboration

    2018-04-01

    This paper reports the first simultaneous measurement of the horizontal and vertical components of the polarization vector in a storage ring under the influence of a radio frequency (rf) solenoid. The experiments were performed at the Cooler Synchrotron COSY in Jülich using a vector polarized, bunched 0.97 GeV /c deuteron beam. Using the new spin feedback system, we set the initial phase difference between the solenoid field and the precession of the polarization vector to a predefined value. The feedback system was then switched off, allowing the phase difference to change over time, and the solenoid was switched on to rotate the polarization vector. We observed an oscillation of the vertical polarization component and the phase difference. The oscillations can be described using an analytical model. The results of this experiment also apply to other rf devices with horizontal magnetic fields, such as Wien filters. The precise manipulation of particle spins in storage rings is a prerequisite for measuring the electric dipole moment (EDM) of charged particles.

  2. Magnetic Measurements of Storage Ring Magnets for the APS Upgrade Project

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

    Doose, C.; Dejus, R.; Jaski, M.

    2017-06-01

    Extensive prototyping of storage ring magnets is ongoing at the Advanced Photon Source (APS) in support of the APS Multi-Bend Achromat (MBA) upgrade project (APS-U) [1]. As part of the R&D activities four quadrupole magnets with slightly different geometries and pole tip materials, and one sextupole magnet with vanadium permendur (VP) pole tips were designed, built and tested. Magnets were measured individually using a rotating coil and a Hall probe for detailed mapping of the magnetic field. Magnets were then assembled and aligned relative to each other on a steel support plate and concrete plinth using precision machined surfaces tomore » gain experience with the alignment method chosen for the APS-U storage ring magnets. The required alignment of magnets on a common support structure is 30 μm rms. Measurements of magnetic field quality, strength and magnet alignment after subjecting the magnets and assemblies to different tests are presented.« less

  3. Modeling Systematic Error Effects for a Sensitive Storage Ring EDM Polarimeter

    NASA Astrophysics Data System (ADS)

    Stephenson, Edward; Imig, Astrid

    2009-10-01

    The Storage Ring EDM Collaboration has obtained a set of measurements detailing the sensitivity of a storage ring polarimeter for deuterons to small geometrical and rate changes. Various schemes, such as the calculation of the cross ratio [1], can cancel effects due to detector acceptance differences and luminosity differences for states of opposite polarization. Such schemes fail at second-order in the errors, becoming sensitive to geometrical changes, polarization magnitude differences between opposite polarization states, and changes to the detector response with changing data rates. An expansion of the polarimeter response in a Taylor series based on small errors about the polarimeter operating point can parametrize such effects, primarily in terms of the logarithmic derivatives of the cross section and analyzing power. A comparison will be made to measurements obtained with the EDDA detector at COSY-J"ulich. [4pt] [1] G.G. Ohlsen and P.W. Keaton, Jr., NIM 109, 41 (1973).

  4. Pushing the MAX IV 3 GeV storage ring brightness and coherence towards the limit of its magnetic lattice

    NASA Astrophysics Data System (ADS)

    Leemann, S. C.; Wurtz, W. A.

    2018-03-01

    The MAX IV 3 GeV storage ring is presently being commissioned and crucial parameters such as machine functions, emittance, and stored current have either already been reached or are approaching their design specifications. Once the baseline performance has been achieved, a campaign will be launched to further improve the brightness and coherence of this storage ring for typical X-ray users. During recent years, several such improvements have been designed. Common to these approaches is that they attempt to improve the storage ring performance using existing hardware provided for the baseline design. Such improvements therefore present more short-term upgrades. In this paper, however, we investigate medium-term improvements assuming power supplies can be exchanged in an attempt to push the brightness and coherence of the storage ring to the limit of what can be achieved without exchanging the magnetic lattice itself. We outline optics requirements, the optics optimization process, and summarize achievable parameters and expected performance.

  5. Status of NSLS-II Storage Ring Vacuum Systems

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

    Doom,L.; Hseuh,H.; Ferreira, M.

    2009-05-04

    National Synchrotron Light Source II (NSLS-II), being constructed at Brookhaven National Laboratory, is a 3-GeV, high-flux and high- brightness synchrotron radiation facility with a nominal current of 500 mA. The storage ring vacuum system will have extruded aluminium chambers with ante-chamber for photon fans and distributed NEG strip pumping. Discrete photon absorbers will be used to intercept the un-used bending magnet radiation. In-situ bakeout will be implemented to achieve fast conditioning during initial commissioning and after interventions.

  6. Photoswitchable Dihydroazulene Macrocycles for Solar Energy Storage: The Effects of Ring Strain.

    PubMed

    Vlasceanu, Alexandru; Frandsen, Benjamin N; Skov, Anders B; Hansen, Anne Schou; Rasmussen, Mads Georg; Kjaergaard, Henrik G; Mikkelsen, Kurt V; Nielsen, Mogens Brøndsted

    2017-10-06

    Efficient energy storage and release are two major challenges of solar energy harvesting technologies. The development of molecular solar thermal systems presents one approach to address these issues by tuning the isomerization reactions of photo/thermoswitches. Here we show that the incorporation of photoswitches into macrocyclic structures is a particularly attractive solution for increasing the storage time. We present the synthesis and properties of a series of macrocycles incorporating two dihydroazulene (DHA) photoswitching subunits, bridged by linkers of varying chain length. Independent of ring size, all macrocycles exhibit stepwise, light-induced, ring-opening reactions (DHA-DHA to DHA-VHF to VHF-VHF; VHF = vinylheptafulvene) with the first DHA undergoing isomerization with a similar efficiency as the uncyclized parent system while the second (DHA-VHF to VHF-VHF) is significantly slower. The energy-releasing, VHF-to-DHA, ring closures also occur in a stepwise manner and are systematically found to proceed slower in the more strained (smaller) cycles, but in all cases with a remarkably slow conversion of the second VHF to DHA. We managed to increase the half-life of the second VHF-to-DHA conversion from 65 to 202 h at room temperature by simply decreasing the ring size. A computational study reveals the smallest macrocycle to have the most energetic VHF-VHF state and hence highest energy density.

  7. BEAM DIAGNOSTICS USING BPM SIGNALS FROM INJECTED AND STORED BEAMS IN A STORAGE RING

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

    Wang, G.M.; Shaftan; T.

    2011-03-28

    Many modern light sources are operating in top-off injection mode or are being upgraded to top-off injection mode. The storage ring always has the stored beam and injected beam for top-off injection mode. So the BPM data is the mixture of both beam positions and the injected beam position cannot be measured directly. We propose to use dedicated wide band BPM electronics in the NSLS II storage ring to retrieve the injected beam trajectory with the singular value decomposition (SVD) method. The beam position monitor (BPM) has the capability to measure bunch-by-bunch beam position. Similar electronics can be used tomore » measure the bunch-by-bunch beam current which is necessary to get the injection beam position. The measurement precision of current needs to be evaluated since button BPM sum signal has position dependence. The injected beam trajectory can be measured and monitored all the time without dumping the stored beam. We can adjust and optimize the injected beam trajectory to maximize the injection efficiency. We can also measure the storage ring acceptance by mapping the injected beam trajectory.« less

  8. Magnet design for a low-emittance storage ring

    PubMed Central

    Johansson, Martin; Anderberg, Bengt; Lindgren, Lars-Johan

    2014-01-01

    The MAX IV 3 GeV storage ring, currently under construction, pursues the goal of low electron beam emittance by using a multi-bend achromat magnet lattice, which is realised by having several consecutive magnet elements precision-machined out of a common solid iron block, 2.3–3.4 m long. With this magnet design solution, instead of having 1320 individual magnets, the MAX IV 3 GeV storage ring is built up using 140 integrated ‘magnet block’ units, containing all these magnet elements. Major features of this magnet block design are compactness, vibration stability and that the alignment of magnet elements within each unit is given by the mechanical accuracy of the CNC machining rather than individual field measurement and adjustment. This article presents practical engineering details of implementing this magnet design solution, and mechanical + magnetic field measurement results from the magnet production series. At the time of writing (spring 2014), the production series, which is totally outsourced to industry, is roughly half way through, with mechanical/magnetic QA conforming to specifications. It is the conclusion of the authors that the MAX IV magnet block concept, which has sometimes been described as new or innovative, is from a manufacturing point of view simply a collection of known mature production methods and measurement procedures, which can be executed at fixed cost with a low level of risk. PMID:25177980

  9. Extreme Drought Events Revealed in Amazon Tree Ring Records

    NASA Astrophysics Data System (ADS)

    Jenkins, H. S.; Baker, P. A.; Guilderson, T. P.

    2010-12-01

    The Amazon basin is a center of deep atmospheric convection and thus acts as a major engine for global hydrologic circulation. Yet despite its significance, a full understanding of Amazon rainfall variability remains elusive due to a poor historical record of climate. Temperate tree rings have been used extensively to reconstruct climate over the last thousand years, however less attention has been given to the application of dendrochronology in tropical regions, in large part due to a lower frequency of tree species known to produce annual rings. Here we present a tree ring record of drought extremes from the Madre de Dios region of southeastern Peru over the last 190 years. We confirm that tree ring growth in species Cedrela odorata is annual and show it to be well correlated with wet season precipitation. This correlation is used to identify extreme dry (and wet) events that have occurred in the past. We focus on drought events identified in the record as drought frequency is expected to increase over the Amazon in a warming climate. The Cedrela chronology records historic Amazon droughts of the 20th century previously identified in the literature and extends the record of drought for this region to the year 1816. Our analysis shows that there has been an increase in the frequency of extreme drought (mean recurrence interval = 5-6 years) since the turn of the 20th century and both Atlantic and Pacific sea surface temperature (SST) forcing mechanisms are implicated.

  10. Preliminary study of injection transients in the TPS storage ring

    NASA Astrophysics Data System (ADS)

    Chen, C. H.; Liu, Y. C.; Y Chen, J.; Chiu, M. S.; Tseng, F. H.; Fann, S.; Liang, C. C.; Huang, C. S.; Y Lee, T.; Y Chen, B.; Tsai, H. J.; Luo, G. H.; Kuo, C. C.

    2017-07-01

    An optimized injection efficiency is related to a perfect match between the pulsed magnetic fields in the storage ring and transfer line extraction in the TPS. However, misalignment errors, hardware output errors and leakage fields are unavoidable. We study the influence of injection transients on the stored TPS beam and discuss solutions to compensate these. Related simulations and measurements will be presented.

  11. Stochastic events lead to accretion in Saturn's rings

    NASA Astrophysics Data System (ADS)

    Esposito, Larry W.

    2010-05-01

    UVIS occultations indicate accretion is triggered at the B ring edge, in strong density waves in ring A and in the F ring. Moons may trigger accretion by streamline crowding (Lewis & Stewart); which enhances collisions, leading to accretion; increasing random velocities; leading to more collisions and more accretion. Cassini occultations of these strongly perturbed locations show not only accretion but also disaggregation, with time scales of hours to weeks. The collisions may lead to temporary aggregations via stochastic events: collisions can compress unconsolidated objects, trigger adhesion or bring small pieces into contact with larger or higher-density seeds. Disaggregation then can follow from disruptive collisions or tidal shedding. In the accretion/disruption balance, increased random motions could eventually give the upper hand to disruption… just as ‘irrational exuberance' can lead to financial panic in the economy; or the overpopulation of hares can lead to boom-and-bust in the population of foxes. This unstable equilibrium can similarly give rise to episodic cycles in accretion: explaining why the observable ring features that indicate embedded objects have been increasing since the beginning of Cassini's observations of Saturn in 2004.

  12. Spin Filtering in Storage Rings

    NASA Astrophysics Data System (ADS)

    Nikolaev, N. N.; Pavlov, F. F.

    The spin filtering in storage rings is based on a multiple passage of a stored beam through a polarized internal gas target. Apart from the polarization by the spin-dependent transmission, a unique geometrical feature of interaction with the target in such a filtering process, pointed out by H.O. Meyer,1 is a scattering of stored particles within the beam. A rotation of the spin in the scattering process affects the polarization buildup. We derive here a quantum-mechanical evolution equation for the spin-density matrix of a stored beam which incorporates the scattering within the beam. We show how the interplay of the transmission and scattering within the beam changes from polarized electrons to polarized protons in the atomic target. After discussions of the FILTEX results on the filtering of stored protons,2 we comment on the strategy of spin filtering of antiprotons for the PAX experiment at GSI FAIR.3.

  13. Astrochemistry at the Cryogenic Storage Ring

    NASA Astrophysics Data System (ADS)

    Kreckel, Holger; Becker, Arno; Blaum, Klaus; Breitenfeldt, Christian; George, Sebastian; Göck, Jürgen; Grieser, Manfred; Grussie, Florian; Guerin, Elisabeth; Heber, Oded; Karthein, Jonas; Krantz, Claude; Meyer, Christian; Mishra, Preeti; Novotny, Oldrich; O'Connor, Aodh; Saurabh, Sunny; Schippers, Stefan; Spruck, Kaija; Kumar, S. Sunil; Urbain, Xavier; Vogel, Stephen; von Hahn, Robert; Wilhelm, Patrick; Wolf, Andreas; Zajfman, Daniel

    2017-01-01

    Almost 200 different molecular species have been identified in space, and this number continues to grow steadily. This surprising molecular diversity bears witness to an active reaction network, in which molecular ions are the main drivers of chemistry in the gas phase. To study these reactions under controlled conditions in the laboratory is a major experimental challenge. The new Cryogenic Storage Ring (CSR) that has recently been commissioned at the Max Planck Institute for Nuclear Physics in Heidelberg will serve as an ideal testbed to study cold molecular ions in the gas phase. With residual gas densities of <140 cm-3 and temperatures below 10K, the CSR will allow for merged beams collision studies involving molecular ions, neutral atoms, free electrons and photons under true interstellar conditions.

  14. Upgrade of BPM Electronics for the SPring-8 Storage Ring

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

    Sasaki, Shigeki; Fujita, Takahiro; Shoji, Masazumi

    2006-11-20

    SPring-8, a 3rd generation synchrotron light source, has operated since 1997. Improvement of BPM performance is required as a part of upgrading activities of the storage ring as a light source. We have developed new electronics circuits for signal processing of the storage ring BPM, with target performance of sub-{mu}m range resolution with sufficiently fast measurement speed and good long-term stability. A set of the new circuits consists of multiplexers, an RF amplifier, a mixer, an IF amplifier, and a local oscillator for analog signal processing. The IF amplifier outputs are sampled with 16-bit 2-MSPS ADC on ADC boards andmore » the data are sent to a DSP board. The sampled data are processed and converted to position information in the DSP. A multiplexing method was employed to have a better stability of the performance by cancellation of variation common to each channel. Evaluation of the performance by using a prototype shows that position resolution well into the sub-{mu}m range has been achieved with a bandwidth of 1 kHz, and long-term stability of within 1 {mu}m has also been achieved.« less

  15. Search for the 1P 1 charmonium state in overlinepp annihilations at the CERN intersecting storage rings

    NASA Astrophysics Data System (ADS)

    Baglin, C.; Baird, S.; Bassompierre, G.; Borreani, G.; Brient, J.-C.; Broll, C.; Brom, J.-M.; Bugge, L.; Buran, T.; Burq, J.-P.; Bussière, A.; Buzzo, A.; Cester, R.; Chemarin, M.; Chevallier, M.; Escoubes, B.; Fay, J.; Ferroni, S.; Gracco, V.; Guillaud, J.-P.; Khan-Aronsen, E.; Kirsebom, K.; Kylling, A.; Ille, B.; Lambert, M.; Leistam, L.; Lundby, A.; Macri, M.; Marchetto, F.; Menichetti, E.; Mörch, Ch.; Mouellic, B.; Olsen, D.; Pastrone, N.; Petrillo, L.; Pia, M. G.; Poole, J.; Poulet, M.; Rinaudo, G.; Santroni, A.; Severi, M.; Skjevling, G.; Stapnes, S.; Stugu, B.; R704 Collaboration

    1986-04-01

    This experiment has been performed at the CERN Intersecting Storage Rings to study the direct formation of charmonium states in antiproton-proton annihilations. The experimental program has partly been devoted to an inclusive scan for overlinepp → J/ψ + X in the range 3520-3530 MeV/ c2. A cluster of five events has been observed in a narrow energy band, centred on the centre of gravity of the 3P J states where the 1P 1 is expected to be. When interpreted as a new resonace, these data yield a mass m = 3525.4±0.8 MeV/ c2.

  16. Storage Rings in the Sky: Gamma Ray Bursts and Galactic Gravitational Collapse Stored Energy

    NASA Astrophysics Data System (ADS)

    Greyber, H. D.

    2004-05-01

    The recent discovery of almost 100% polarization of the prompt gamma ray emission from GRB021206, (1), confirms my 44 year old ``Strong" Magnetic Field" model (SMF) for galactic dynamics. In SMF, Storage Ring particles were accelerated long ago during the original gravitational collapse of the pregalactic/prequasar plasma cloud that is permeated by an almost uniform primordial magnetic field (2,3) The enormous, intense, slender, relativistic, stable, completely coherent Storage Ring stores a very small fraction of the huge galactic gravitational collapse energy in an almost radiationless state, unless disturbed. The concept of an Astrophysical Storage Ring was introduced by me in l961. At first it was to explain galactic structure, but soon it proved useful to explain active galactic nuclei (AGN) and the dynamics of quasar/AGN jets. AGN and galactic morphology, energetics and dynamics vary as the ratio of magnetic energy to rotational energy in the particular object. Gamma ray bursts (GRB) are due simply to a ``rock". i.e. a white dwarf, ordinary star, neutron sstar, asteroid, planet, etc. falling rapidly through the Storage Ring and being almost instantly vaporized into a hot plasma fireball, causing an electromagnetic shower (2) Then the fireball speeds into the huge organized magnetic field surrounding the current ring, thus generating very highly polarized prompt gamma ray emission (as seen in GRB021206) from the synchrotron radiation process. The timing fits the GRB observations nicely. For instance, a ``rock" racing at 1000 kilometers per second across a 20,000 km. path in the beam would produce a twenty second burst. Other times, a target might track across a short chord for a short burst. Space missions have shown that often typical currents in space plasmas are made up of slender filaments. Thus the puzzling less than one millisecond spikes observed in some GRB are simply describing the structure of that particular ring current at that particular time. 1

  17. Low emittance lattice for the storage ring of the Turkish Light Source Facility TURKAY

    NASA Astrophysics Data System (ADS)

    Nergiz, Z.; Aksoy, A.

    2015-06-01

    The TAC (Turkish Accelerator Center) project aims to build an accelerator center in Turkey. The first stage of the project is to construct an Infra-Red Free Electron Laser (IR-FEL) facility. The second stage is to build a synchrotron radiation facility named TURKAY, which is a third generation synchrotron radiation light source that aims to achieve a high brilliance photon beam from a low emittance electron beam at 3 GeV. The electron beam parameters are highly dependent on the magnetic lattice of the storage ring. In this paper a low emittance storage ring for TURKAY is proposed and the beam dynamic properties of the magnetic lattice are investigated. Supported by Turkish Republic Ministry of Development (DPT2006K120470)

  18. PEGASYS: A proposed internal target-spectrometer facility for the PEP storage ring

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

    Van Bibber, K.

    A proposal for an internal gas-jet target and forward spectrometer for the PEP storage ring is described. The beam structure, allowable luminosity (L=10/sup 33/ cm/sup /minus/2/s/sup /minus/1/ for H/sub 2/, D/sub 2/ decreasing as Z/sup /minus/1.75/ for nuclear targets) and energy (E/sub e/less than or equal to 15 GeV) make the ring ideal for multiparticle coincidence studies in the scaling regime, and where perturbative QCD may be an apt description of some exclusive and semi-inclusive reactions. 17 refs., 5 figs.

  19. Design study of the storage ring EUTERPE

    NASA Astrophysics Data System (ADS)

    Xi, Boling; Botman, J. I. M.; Timmermans, C. J.; Hagedoorn, H. L.

    1992-05-01

    At present the 400 MeV electron storage ring EUTERPE is being constructed at the Eindhoven University of Technology. It is a university project set up for studies of charged particle beam dynamics and applications of synchroton radiation, and for the education of students in these fields. The design of the ring is described in this paper. Considering the requirements of users in different fields, a lattice based on a so-called triple bend achromat structure with a high flexibility has been chosen. With this lattice, different optical options, including the HBSB (high brightness, small beam), the SBL (short bunch length) and the HLF (high light flux) modes can be realized. A small emittance of 7 nm rad and a short bunch length of the order of several mm can be achieved. In the first phase the synchrotron radiation in the UV and XUV region (the critical wavelength is 8.3 nm) will be provided from the regular dipole magnets. Later on, a 10 T wiggler magnet and other special inserters will be added, and other applications and beam dynamics studies will be feasible. Bending magnets are of the parallel faced C configuration. The effective aperture of the vacuum chamber is 2.3 cm (vertical) in the bending magnets and 4.7 cm elsewhere with a working vacuum condition of 10-9 Torr. Collective effects have been studied initially. First calculations indicate that a lifetime of several hours, influenced by the Touschek effect and residual gas scattering will be achievable for a 200 mA beam in the HLF mode for the standard rf parameters. A 70 MeV racetrack microtron will serve as injector for the ring.

  20. Towards a 4{sup th} generation storage ring at the Canadian Light Source

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

    Dallin, Les; Wurtz, Ward

    2016-07-27

    Demands from beamline scientists for more brilliant sources of synchrotron radiation have resulted in the emergence of 4{sup th} generation (diffraction-limited) storage rings. The practical development of the multi-bend achromat (MBA) concept by MAX IV lab has spurred many synchrotron light sources around the world to develop similar machines. For existing facilities two options are available: upgrading existing machines or building a new structure. The Canadian Light Source (CLS) has explored both options. For a new low emittance source in the existing CLS tunnel a decrease in electron energy would be required. A machine similar to the ALS upgrade couldmore » be contemplated. To achieve low emittance at our present energy of 2.9 GeV a new storage ring is desirable. Several options have been investigated. These designs use extremely strong focusing magnets to achieve extremely low emittances in compact lattice achromats.« less

  1. Stochastic events lead to accretion in Saturn’s rings

    NASA Astrophysics Data System (ADS)

    Esposito, L. W.

    2009-12-01

    UVIS occultations indicate accretion is triggered at the B ring edge, in strong density waves in ring A and in the F ring. Moons may trigger accretion by streamline crowding (Lewis & Stewart); which enhances collisions, leading to accretion; increasing random velocities; leading to more collisions and more accretion. Cassini occultations of these strongly perturbed locations show not only accretion but also disaggregation, with time scales of hours to weeks. The collisions may lead to temporary aggregations via stochastic events: they can compress unconsolidated objects, trigger adhesion or bring small pieces into contact with larger or higher-density seeds. Disaggregation then can follow from disruptive collisions or tidal shedding. In the accretion/disruption balance, increased random motions could eventually give the upper hand to disruption… just as ‘irrational exuberance’ can lead to financial panic in the economy; or the overpopulation of hares can lead to boom-and-bust in the population of foxes. This unstable equilibrium can similarly give rise to episodic cycles in accretion: explaining why the observable ring features that indicate embedded objects have been increasing since the beginning of Cassini’s observations of Saturn in 2004.

  2. Beam measurements using visible synchrotron light at NSLS2 storage ring

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

    Cheng, Weixing, E-mail: chengwx@bnl.gov; Bacha, Bel; Singh, Om

    2016-07-27

    Visible Synchrotron Light Monitor (SLM) diagnostic beamline has been designed and constructed at NSLS2 storage ring, to characterize the electron beam profile at various machine conditions. Due to the excellent alignment, SLM beamline was able to see the first visible light when beam was circulating the ring for the first turn. The beamline has been commissioned for the past year. Besides a normal CCD camera to monitor the beam profile, streak camera and gated camera are used to measure the longitudinal and transverse profile to understand the beam dynamics. Measurement results from these cameras will be presented in this paper.more » A time correlated single photon counting system (TCSPC) has also been setup to measure the single bunch purity.« less

  3. Ultrashort high-brightness pulses from storage rings

    NASA Astrophysics Data System (ADS)

    Khan, Shaukat

    2017-09-01

    The brightness of short-wavelength radiation from accelerator-based sources can be increased by coherent emission in which the radiation intensity scales with the number of contributing electrons squared. This requires a microbunched longitudinal electron distribution, which is the case in free-electron lasers. The brightness of light sources based on electron storage rings was steadily improved, but could profit further from coherent emission. The modulation of the electron energy by a continuous-wave laser field may provide steady-state microbunching in the infrared regime. For shorter wavelengths, the energy modulation can be converted into a temporary density modulation by a dispersive chicane. One particular goal is coherent emission from a very short "slice" within an electron bunch in order to produce ultrashort radiation pulses with high brightness.

  4. Saw-tooth instability in storage rings: simulations and dynamical model

    NASA Astrophysics Data System (ADS)

    Migliorati, M.; Palumbo, L.; Dattoli, G.; Mezi, L.

    1999-11-01

    The saw-tooth instability in storage rings is studied by means of a time-domain simulation code which takes into account the self-induced wake fields. The results are compared with those from a dynamical heuristic model exploiting two coupled non-linear differential equations, accounting for the time behavior of the instability growth rate and for the anomalous growth of the energy spread. This model is shown to reproduce the characteristic features of the instability in a fairly satisfactory way.

  5. Properties of the electron cloud in a high-energy positron and electron storage ring

    DOE PAGES

    Harkay, K. C.; Rosenberg, R. A.

    2003-03-20

    Low-energy, background electrons are ubiquitous in high-energy particle accelerators. Under certain conditions, interactions between this electron cloud and the high-energy beam can give rise to numerous effects that can seriously degrade the accelerator performance. These effects range from vacuum degradation to collective beam instabilities and emittance blowup. Although electron-cloud effects were first observed two decades ago in a few proton storage rings, they have in recent years been widely observed and intensely studied in positron and proton rings. Electron-cloud diagnostics developed at the Advanced Photon Source enabled for the first time detailed, direct characterization of the electron-cloud properties in amore » positron and electron storage ring. From in situ measurements of the electron flux and energy distribution at the vacuum chamber wall, electron-cloud production mechanisms and details of the beam-cloud interaction can be inferred. A significant longitudinal variation of the electron cloud is also observed, due primarily to geometrical details of the vacuum chamber. Furthermore, such experimental data can be used to provide realistic limits on key input parameters in modeling efforts, leading ultimately to greater confidence in predicting electron-cloud effects in future accelerators.« less

  6. Experimental Evidence for the Los Alamos Proton Storage Ring Beam Instability

    NASA Astrophysics Data System (ADS)

    Plum, M.; Fitzgerald, D. H.; Macek, R.; Sander, O.; Thiessen, H. A.; Wang, T. S.; Wilkinson, C.

    1997-05-01

    Although the exact instability mechanism at the Proton Storage Ring (PSR) has not yet been conclusively identified, the evidence gathered to date is consistent with an e-p instability. We have recently acquired new data which shows that clearing electrodes significantly affect the instability threshold. A set of comprehensive measurements is also planned for the first months of 1997. In this paper we will present our latest data.

  7. Emittance measurements in low energy ion storage rings

    NASA Astrophysics Data System (ADS)

    Hunt, J. R.; Carli, C.; Resta-López, J.; Welsch, C. P.

    2018-07-01

    The development of the next generation of ultra-low energy antiproton and ion facilities requires precise information about the beam emittance to guarantee optimum performance. In the Extra-Low ENergy Antiproton storage ring (ELENA) the transverse emittances will be measured by scraping. However, this diagnostic measurement faces several challenges: non-zero dispersion, non-Gaussian beam distributions due to effects of the electron cooler and various systematic errors such as closed orbit offsets and inaccurate rms momentum spread estimation. In addition, diffusion processes, such as intra-beam scattering might lead to emittance overestimates. Here, we present algorithms to efficiently address the emittance reconstruction in presence of the above effects, and present simulation results for the case of ELENA.

  8. A storage ring experiment to detect a proton electric dipole moment

    DOE PAGES

    Anastassopoulos, V.; Andrianov, S.; Baartman, R.; ...

    2016-11-29

    We describe a new experiment to detect a permanent electric dipole moment of the proton with a sensitivity of 10 $-$29e cm by using polarized “magic” momentum 0.7 GeV/c protons in an all-electric storage ring. Systematic errors relevant to the experiment are discussed and techniques to address them are presented. The measurement is sensitive to new physics beyond the Standard Model at the scale of 3000 TeV.

  9. A storage ring experiment to detect a proton electric dipole moment.

    PubMed

    Anastassopoulos, V; Andrianov, S; Baartman, R; Baessler, S; Bai, M; Benante, J; Berz, M; Blaskiewicz, M; Bowcock, T; Brown, K; Casey, B; Conte, M; Crnkovic, J D; D'Imperio, N; Fanourakis, G; Fedotov, A; Fierlinger, P; Fischer, W; Gaisser, M O; Giomataris, Y; Grosse-Perdekamp, M; Guidoboni, G; Hacıömeroğlu, S; Hoffstaetter, G; Huang, H; Incagli, M; Ivanov, A; Kawall, D; Kim, Y I; King, B; Koop, I A; Lazarus, D M; Lebedev, V; Lee, M J; Lee, S; Lee, Y H; Lehrach, A; Lenisa, P; Levi Sandri, P; Luccio, A U; Lyapin, A; MacKay, W; Maier, R; Makino, K; Malitsky, N; Marciano, W J; Meng, W; Meot, F; Metodiev, E M; Miceli, L; Moricciani, D; Morse, W M; Nagaitsev, S; Nayak, S K; Orlov, Y F; Ozben, C S; Park, S T; Pesce, A; Petrakou, E; Pile, P; Podobedov, B; Polychronakos, V; Pretz, J; Ptitsyn, V; Ramberg, E; Raparia, D; Rathmann, F; Rescia, S; Roser, T; Kamal Sayed, H; Semertzidis, Y K; Senichev, Y; Sidorin, A; Silenko, A; Simos, N; Stahl, A; Stephenson, E J; Ströher, H; Syphers, M J; Talman, J; Talman, R M; Tishchenko, V; Touramanis, C; Tsoupas, N; Venanzoni, G; Vetter, K; Vlassis, S; Won, E; Zavattini, G; Zelenski, A; Zioutas, K

    2016-11-01

    A new experiment is described to detect a permanent electric dipole moment of the proton with a sensitivity of 10 -29 e ⋅ cm by using polarized "magic" momentum 0.7 GeV/c protons in an all-electric storage ring. Systematic errors relevant to the experiment are discussed and techniques to address them are presented. The measurement is sensitive to new physics beyond the standard model at the scale of 3000 TeV.

  10. A storage ring experiment to detect a proton electric dipole moment

    NASA Astrophysics Data System (ADS)

    Anastassopoulos, V.; Andrianov, S.; Baartman, R.; Baessler, S.; Bai, M.; Benante, J.; Berz, M.; Blaskiewicz, M.; Bowcock, T.; Brown, K.; Casey, B.; Conte, M.; Crnkovic, J. D.; D'Imperio, N.; Fanourakis, G.; Fedotov, A.; Fierlinger, P.; Fischer, W.; Gaisser, M. O.; Giomataris, Y.; Grosse-Perdekamp, M.; Guidoboni, G.; Hacıömeroǧlu, S.; Hoffstaetter, G.; Huang, H.; Incagli, M.; Ivanov, A.; Kawall, D.; Kim, Y. I.; King, B.; Koop, I. A.; Lazarus, D. M.; Lebedev, V.; Lee, M. J.; Lee, S.; Lee, Y. H.; Lehrach, A.; Lenisa, P.; Levi Sandri, P.; Luccio, A. U.; Lyapin, A.; MacKay, W.; Maier, R.; Makino, K.; Malitsky, N.; Marciano, W. J.; Meng, W.; Meot, F.; Metodiev, E. M.; Miceli, L.; Moricciani, D.; Morse, W. M.; Nagaitsev, S.; Nayak, S. K.; Orlov, Y. F.; Ozben, C. S.; Park, S. T.; Pesce, A.; Petrakou, E.; Pile, P.; Podobedov, B.; Polychronakos, V.; Pretz, J.; Ptitsyn, V.; Ramberg, E.; Raparia, D.; Rathmann, F.; Rescia, S.; Roser, T.; Kamal Sayed, H.; Semertzidis, Y. K.; Senichev, Y.; Sidorin, A.; Silenko, A.; Simos, N.; Stahl, A.; Stephenson, E. J.; Ströher, H.; Syphers, M. J.; Talman, J.; Talman, R. M.; Tishchenko, V.; Touramanis, C.; Tsoupas, N.; Venanzoni, G.; Vetter, K.; Vlassis, S.; Won, E.; Zavattini, G.; Zelenski, A.; Zioutas, K.

    2016-11-01

    A new experiment is described to detect a permanent electric dipole moment of the proton with a sensitivity of 10-29 e ṡ cm by using polarized "magic" momentum 0.7 GeV/c protons in an all-electric storage ring. Systematic errors relevant to the experiment are discussed and techniques to address them are presented. The measurement is sensitive to new physics beyond the standard model at the scale of 3000 TeV.

  11. A storage ring experiment to detect a proton electric dipole moment

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

    Anastassopoulos, V.; Andrianov, S.; Baartman, R.

    2016-11-01

    A new experiment is described to detect a permanent electric dipole moment of the proton with a sensitivity ofmore » $$10^{-29}e\\cdot$$cm by using polarized "magic" momentum $0.7$~GeV/c protons in an all-electric storage ring. Systematic errors relevant to the experiment are discussed and techniques to address them are presented. The measurement is sensitive to new physics beyond the Standard Model at the scale of 3000~TeV.« less

  12. Storage ring two-color free-electron laser

    DOE PAGES

    Yan, J.; Hao, H.; Li, J. Y.; ...

    2016-07-05

    We report a systematic experimental study of a storage ring two-color free-electron laser (FEL) operating simultaneously in the infrared (IR) and ultraviolet (UV) wavelength regions. The two-color FEL lasing has been realized using a pair of dual-band high-reflectivity FEL mirrors with two different undulator configurations. We have demonstrated independent wavelength tuning in a wide range for each lasing color, as well as harmonically locked wavelength tuning when the UV lasing occurs at the second harmonic of the IR lasing. Precise power control of two-color lasing with good power stability has also been achieved. In addition, the impact of the degradationmore » of FEL mirrors on the two-color FEL operation is reported. Moreover, we have investigated the temporal structures of the two-color FEL beams, showing simultaneous two-color micropulses with their intensity modulations displayed as FEL macropulses.« less

  13. Electron cooling of a bunched ion beam in a storage ring

    NASA Astrophysics Data System (ADS)

    Zhao, He; Mao, Lijun; Yang, Jiancheng; Xia, Jiawen; Yang, Xiaodong; Li, Jie; Tang, Meitang; Shen, Guodong; Ma, Xiaoming; Wu, Bo; Wang, Geng; Ruan, Shuang; Wang, Kedong; Dong, Ziqiang

    2018-02-01

    A combination of electron cooling and rf system is an effective method to compress the beam bunch length in storage rings. A simulation code based on multiparticle tracking was developed to calculate the bunched ion beam cooling process, in which the electron cooling, intrabeam scattering (IBS), ion beam space-charge field, transverse and synchrotron motion are considered. Meanwhile, bunched ion beam cooling experiments have been carried out in the main cooling storage ring (CSRm) of the Heavy Ion Research Facility in Lanzhou, to investigate the minimum bunch length obtained by the cooling method, and study the dependence of the minimum bunch length on beam and machine parameters. The experiments show comparable results to those from simulation. Based on these simulations and experiments, we established an analytical model to describe the limitation of the bunch length of the cooled ion beam. It is observed that the IBS effect is dominant for low intensity beams, and the space-charge effect is much more important for high intensity beams. Moreover, the particles will not be bunched for much higher intensity beam. The experimental results in CSRm show a good agreement with the analytical model in the IBS dominated regime. The simulation work offers us comparable results to those from the analytical model both in IBS dominated and space-charge dominated regimes.

  14. BPM Breakdown Potential in the PEP-II B-factory Storage Ring Collider

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

    Weathersby, Stephen; Novokhatski, Alexander; /SLAC

    2010-02-10

    High current B-Factory BPM designs incorporate a button type electrode which introduces a small gap between the button and the beam chamber. For achievable currents and bunch lengths, simulations indicate that electric potentials can be induced in this gap which are comparable to the breakdown voltage. This study characterizes beam induced voltages in the existing PEP-II storage ring collider BPM as a function of bunch length and beam current.

  15. The Potential-Well Distortion Effect and Coherent Instabilities of Electron Bunches in Storage Rings

    NASA Astrophysics Data System (ADS)

    Korchuganov, V. N.; Smygacheva, A. S.; Fomin, E. A.

    2018-05-01

    The effect of electromagnetic interaction between electron bunches and the vacuum chamber of a storage ring on the longitudinal motion of bunches is studied. Specifically, the potential-well distortion effect and the so-called coherent instabilities of coupled bunches are considered. An approximate analytical solution for the frequencies of incoherent oscillations of bunches distributed arbitrarily within the ring is obtained for a distorted potential well. A new approach to determining frequencies of coherent oscillations and an approximate analytical relation for estimating the stability of a system of bunches as a function of their distribution in the accelerator orbit are presented.

  16. Safe operating conditions for NSLS-II Storage Ring Frontends commissioning

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

    Seletskiy, S.; Amundsen, C.; Ha, K.

    2015-04-02

    The NSLS-II Storage Ring Frontends are designed to safely accept the synchrotron radiation fan produced by respective insertion device when the electron beam orbit through the ID is locked inside the predefined Active Interlock Envelope. The Active Interlock is getting enabled at a particular beam current known as AI safe current limit. Below such current the beam orbit can be anywhere within the limits of the SR beam acceptance. During the FE commissioning the beam orbit is getting intentionally disturbed in the particular ID. In this paper we explore safe operating conditions for the Frontends commissioning.

  17. How to Reach a Thousand-Second in-Plane Polarization Lifetime with 0.97 - GeV / c Deuterons in a Storage Ring

    DOE PAGES

    Guidoboni, G.; Stephenson, E.; Andrianov, S.; ...

    2016-07-28

    Here, we observe a deuteron beam polarization lifetime near 1000 s in the horizontal plane of a magnetic storage ring (COSY). This long spin coherence time is maintained through a combination of beam bunching, electron cooling, sextupole field corrections, and the suppression of collective effects through beam current limits. This record lifetime is required for a storage ring search for an intrinsic electric dipole moment on the deuteron at a statistical sensitivity level approaching 10 -29 $e$ cm.

  18. Single-particle detection of products from atomic and molecular reactions in a cryogenic ion storage ring

    NASA Astrophysics Data System (ADS)

    Krantz, C.; Novotný, O.; Becker, A.; George, S.; Grieser, M.; Hahn, R. von; Meyer, C.; Schippers, S.; Spruck, K.; Vogel, S.; Wolf, A.

    2017-04-01

    We have used a single-particle detector system, based on secondary electron emission, for counting low-energetic (∼keV/u) massive products originating from atomic and molecular ion reactions in the electrostatic Cryogenic Storage Ring (CSR). The detector is movable within the cryogenic vacuum chamber of CSR, and was used to measure production rates of a variety of charged and neutral daughter particles. In operation at a temperature of ∼ 6 K , the detector is characterised by a high dynamic range, combining a low dark event rate with good high-rate particle counting capability. On-line measurement of the pulse height distributions proved to be an important monitor of the detector response at low temperature. Statistical pulse-height analysis allows to infer the particle detection efficiency of the detector, which has been found to be close to unity also in cryogenic operation at 6 K.

  19. X-ray nanoprobes and diffraction-limited storage rings: opportunities and challenges of fluorescence tomography of biological specimens

    PubMed Central

    de Jonge, Martin D.; Ryan, Christopher G.; Jacobsen, Chris J.

    2014-01-01

    X-ray nanoprobes require coherent illumination to achieve optic-limited resolution, and so will benefit directly from diffraction-limited storage rings. Here, the example of high-resolution X-ray fluorescence tomography is focused on as one of the most voracious demanders of coherent photons, since the detected signal is only a small fraction of the incident flux. Alternative schemes are considered for beam delivery, sample scanning and detectors. One must consider as well the steps before and after the X-ray experiment: sample preparation and examination conditions, and analysis complexity due to minimum dose requirements and self-absorption. By understanding the requirements and opportunities for nanoscale fluorescence tomography, one gains insight into the R&D challenges in optics and instrumentation needed to fully exploit the source advances that diffraction-limited storage rings offer. PMID:25177992

  20. An undulator based soft x-ray source for microscopy on the Duke electron storage ring

    NASA Astrophysics Data System (ADS)

    Johnson, Lewis Elgin

    1998-09-01

    This dissertation describes the design, development, and installation of an undulator-based soft x-ray source on the Duke Free Electron Laser laboratory electron storage ring. Insertion device and soft x-ray beamline physics and technology are all discussed in detail. The Duke/NIST undulator is a 3.64-m long hybrid design constructed by the Brobeck Division of Maxwell Laboratories. Originally built for an FEL project at the National Institute of Standards and Technology, the undulator was acquired by Duke in 1992 for use as a soft x-ray source for the FEL laboratory. Initial Hall probe measurements on the magnetic field distribution of the undulator revealed field errors of more than 0.80%. Initial phase errors for the device were more than 11 degrees. Through a series of in situ and off-line measurements and modifications we have re-tuned the magnet field structure of the device to produce strong spectral characteristics through the 5th harmonic. A low operating K has served to reduce the effects of magnetic field errors on the harmonic spectral content. Although rms field errors remained at 0.75%, we succeeded in reducing phase errors to less than 5 degrees. Using trajectory simulations from magnetic field data, we have computed the spectral output given the interaction of the Duke storage ring electron beam and the NIST undulator. Driven by a series of concerns and constraints over maximum utility, personnel safety and funding, we have also constructed a unique front end beamline for the undulator. The front end has been designed for maximum throughput of the 1st harmonic around 40A in its standard mode of operation. The front end has an alternative mode of operation which transmits the 3rd and 5th harmonics. This compact system also allows for the extraction of some of the bend magnet produced synchrotron and transition radiation from the storage ring. As with any well designed front end system, it also provides excellent protection to personnel and to the

  1. A method for simultaneous linear optics and coupling correction for storage rings with turn-by-turn beam position monitor data

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

    Yang, Xi; Huang, Xiaobiao

    2016-08-01

    We propose a method to simultaneously correct linear optics errors and linear coupling for storage rings using turn-by-turn (TbT) beam position monitor (BPM) data. The independent component analysis (ICA) method is used to isolate the betatron normal modes from the measured TbT BPM data. The betatron amplitudes and phase advances of the projections of the normal modes on the horizontal and vertical planes are then extracted, which, combined with dispersion measurement, are used to fit the lattice model. Furthermore, the fitting results are used for lattice correction. Our method has been successfully demonstrated on the NSLS-II storage ring.

  2. A method for simultaneous linear optics and coupling correction for storage rings with turn-by-turn beam position monitor data

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

    Yang, Xi; Huang, Xiaobiao

    2016-08-01

    We propose a method to simultaneously correct linear optics errors and linear coupling for storage rings using turn-by-turn (TbT) beam position monitor (BPM) data. The independent component analysis (ICA) method is used to isolate the betatron normal modes from the measured TbT BPM data. The betatron amplitudes and phase advances of the projections of the normal modes on the horizontal and vertical planes are then extracted, which, combined with dispersion measurement, are used to fit the lattice model. The fitting results are used for lattice correction. The method has been successfully demonstrated on the NSLS-II storage ring.

  3. APS Storage Ring Monopulse RF BPM Upgrade

    NASA Astrophysics Data System (ADS)

    Lill, R.; Pietryla, A.; Norum, E.; Lenkszus, F.

    2004-11-01

    The Advanced Photon Source (APS) is a third-generation synchrotron light source in its ninth year of operation. The storage ring monopulse radio frequency (rf) beam position monitor (BPM) was designed to measure single-turn and multi-turn beam positions for operations and machine physics studies. Many of the components used in the original design are obsolete and costly to replace. In this paper we present a proposal to upgrade the monopulse rf BPMs in which the existing system hardware is repartitioned and the aging data acquisition system is replaced. By replacing only the data acquisition system, we will demonstrate a cost-effective approach to improved beam stability, reliability, and enhanced postmortem capabilities. An eight-channel ADC/digitizer VXI board with sampling rate of up to 105 MHz (per channel) and 14-bit resolution coupled with a field-programmable gate array and embedded central processing will provide the flexibility to revitalize this system for another decade of operation. We will discuss the upgrade system specifications, design, and prototype test results.

  4. Nitrile O-ring Cracking: A Case of Vacuum Flange O-ring Failures

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

    Dees, Craig

    2016-07-01

    A review of recent nitrile O-ring failures in ISO-KF vacuum flange connections in glovebox applications is presented. An investigation of a single “isolated” o-ring failure leads to the discovery of cracked nitrile o-rings in a glovebox atmospheric control unit. The initial cause of the o-ring failure is attributed to ozone degradation. However, additional investigation reveals nitrile o-ring cracking on multiple gloveboxes and general purpose piping, roughly 85% of the nitrile o-rings removed for inspection show evidence of visible cracking after being in service for 18 months or less. The results of material testing and ambient air testing is presented, elevatedmore » ozone levels are not found. The contributing factors of o-ring failure, including nitrile air sensitivity, inadequate storage practices, and poor installation techniques, are discussed. A discussion of nitrile o-ring material properties, the benefits and limitations, and alternate materials are discussed. Considerations for o-ring material selection, purchasing, storage, and installation are presented in the context of lessons learned from the nitrile o-ring cracking investigation. This paper can be presented in 20 minutes and does not require special accommodations or special audio visual devices.« less

  5. Can Steady Magnetospheric Convection Events Inject Plasma into the Ring Current?

    NASA Astrophysics Data System (ADS)

    Lemon, C.; Chen, M. W.; Guild, T. B.

    2009-12-01

    Steady Magnetospheric Convection (SMC) events are characterized by several-hour periods of enhanced convection that are devoid of substorm signatures. There has long been a debate about whether substorms are necessary to inject plasma into the ring current, or whether enhanced convection is sufficient. If ring current injections occur during SMC intervals, this would suggest that substorms are unnecessary. We use a combination of simulations and data observations to examine this topic. Our simulation model computes the energy-dependent plasma drift in a self-consistent electric and magnetic field, which allows us to accurately model the transport of plasma from the plasma sheet (where the plasma pressure is much larger than the magnetic pressure) into the inner magnetosphere (where plasma pressure is much less than the magnetic pressure). In regions where the two pressures are comparable (i.e. the inner plasma sheet), feedback between the plasma and magnetic field is critical for accurately modeling the physical evolution of the system. Our previous work has suggested that entropy losses in the plasma sheet (such as caused by substorms) may be necessary to inject a ring current. However, it is not yet clear whether other small-scale processes (e.g. bursty bulk flows) can provide sufficient entropy loss in the plasma sheet to allow for the penetration of plasma into the ring current. We combine our simulation results with data observations in order to better understand the physical processes required to inject a ring current.

  6. Explicit symplectic orbit and spin tracking method for electric storage ring

    DOE PAGES

    Hwang, Kilean; Lee, S. Y.

    2016-08-18

    We develop a symplectic charged particle tracking method for phase space coordinates and polarization in all electric storage rings. Near the magic energy, the spin precession tune is proportional to the fractional momentum deviation δ m from the magic energy, and the amplitude of the radial and longitudinal spin precession is proportional to η/δ m, where η is the electric dipole moment for an initially vertically polarized beam. As a result, the method can be used to extract the electron electric dipole moment of a charged particle by employing narrow band frequency analysis of polarization around the magic energy.

  7. Missing rings in Pinus halepensis – the missing link to relate the tree-ring record to extreme climatic events

    Treesearch

    Klemen Novak; Martin de Luis; Miguel A. Saz; Luis A. Longares; Roberto Serrano-Notivoli; Josep Raventos; Katarina Cufar; Jozica Gricar; Alfredo Di Filippo; Gianluca Piovesan; Cyrille B.K. Rathgeber; Andreas Papadopoulos; Kevin T. Smith

    2016-01-01

    Climate predictions for the Mediterranean Basin include increased temperatures, decreased precipitation, and increased frequency of extreme climatic events (ECE). These conditions are associated with decreased tree growth and increased vulnerability to pests and diseases. The anatomy of tree rings responds to these environmental conditions. Quantitatively, the width of...

  8. A method for simultaneous linear optics and coupling correction for storage rings with turn-by-turn beam position monitor data

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

    Yang, Xi; Huang, Xiaobiao

    2016-05-13

    Here, we propose a method to simultaneously correct linear optics errors and linear coupling for storage rings using turn-by-turn (TbT) beam position monitor (BPM) data. The independent component analysis (ICA) method is used to isolate the betatron normal modes from the measured TbT BPM data. The betatron amplitudes and phase advances of the projections of the normal modes on the horizontal and vertical planes are then extracted, which, combined with dispersion measurement, are used to fit the lattice model. The fitting results are used for lattice correction. Finally, the method has been successfully demonstrated on the NSLS-II storage ring.

  9. Space-charge-sustained microbunch structure in the Los Alamos Proton Storage Ring

    NASA Astrophysics Data System (ADS)

    Cousineau, S.; Danilov, V.; Holmes, J.; Macek, R.

    2004-09-01

    We present experimental data from the Los Alamos Proton Storage Ring (PSR) showing long-lived linac microbunch structure during beam storage with no rf bunching. Analysis of the experimental data and particle-in-cell simulations of the experiments indicate that space charge, coupled with energy spread effects, is responsible for the sustained microbunch structure. The simulated longitudinal phase space of the beam reveals a well-defined separatrix in the phase space between linac microbunches, with particles executing unbounded motion outside of the separatrix. We show that the longitudinal phase space of the beam was near steady state during the PSR experiments, such that the separatrix persisted for long periods of time. Our simulations indicate that the steady state is very sensitive to the experimental conditions. Finally, we solve the steady-state problem in an analytic, self-consistent fashion for a set of periodic longitudinal space-charge potentials.

  10. Commissioning and Early Operation Experience of the NSLS-II Storage Ring RF System

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

    Gao, F.; Rose, J.; Cupolo, J.

    2015-05-03

    The National Synchrotron Light Source II (NSLS-II) is a 3 GeV electron X-ray user facility commissioned in 2014. The storage ring RF system, essential for replenishing energy loss per turn of the electrons, consists of digital low level RF controllers, 310 kW CW klystron transmitters, CESR-B type superconducting cavities, as well as a supporting cryogenic system. Here we will report on RF commissioning and early operation experience of the system for beam current up to 200mA.

  11. A 1kW EUV source for lithography based on FEL emission in a compact storage ring

    NASA Astrophysics Data System (ADS)

    Feser, Michael; Ruth, Ron; Loewen, Rod

    2017-10-01

    EUV has long been hailed as the next generation lithography technology. Its adoption into high volume manufacturing (HVM), however, has been delayed several technology nodes due to technical issues, many of which can be attributed to the EUV source performance. Today's EUV lithography scanners are powered by laser produce plasma (LPP) sources. They have issues with power scaling beyond 300 W, reliability and contamination. Free Electron Lasers (FELs) have been considered as an alternative EUV source. Advantages of accelerator based sources are the maturity of the accelerator technology, lack of debris/contamination, and ability to provide high power. Industry turned away from this technology because of the requirement to feed up to 10 scanners from one linear FEL to make it economically feasible, the large footprint, and generation of radioactive byproducts. All of these issues are overcome in the presented concept using a compact storage ring with steady-state FEL lasing action. At 1 kW output power, comparable cost and footprint to an LPP source, this source is ideally suited for use on a single scanner and promises reliable, contamination free operation. FEL action in the storage ring is sustained by operating the FEL well below the saturation regime and preserving the equilibrium low emittance and energy distribution of the ring.

  12. Conditioning of BPM pickup signals for operations of the Duke storage ring with a wide range of single-bunch current

    NASA Astrophysics Data System (ADS)

    Xu, Wei; Li, Jing-Yi; Huang, Sen-Lin; Z. Wu, W.; Hao, H.; P., Wang; K. Wu, Y.

    2014-10-01

    The Duke storage ring is a dedicated driver for the storage ring based oscillator free-electron lasers (FELs), and the High Intensity Gamma-ray Source (HIGS). It is operated with a beam current ranging from about 1 mA to 100 mA per bunch for various operations and accelerator physics studies. High performance operations of the FEL and γ-ray source require a stable electron beam orbit, which has been realized by the global orbit feedback system. As a critical part of the orbit feedback system, the electron beam position monitors (BPMs) are required to be able to precisely measure the electron beam orbit in a wide range of the single-bunch current. However, the high peak voltage of the BPM pickups associated with high single-bunch current degrades the performance of the BPM electronics, and can potentially damage the BPM electronics. A signal conditioning method using low pass filters is developed to reduce the peak voltage to protect the BPM electronics, and to make the BPMs capable of working with a wide range of single-bunch current. Simulations and electron beam based tests are performed. The results show that the Duke storage ring BPM system is capable of providing precise orbit measurements to ensure highly stable FEL and HIGS operations.

  13. Mass Measurements of Proton-rich Nuclides at the Cooler Storage Ring at IMP

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

    Zhang, Y. H.; Xu, H. S.; Wang, M.

    2011-11-30

    Recent results and progress of mass measurements of proton-rich nuclei using isochronous mass spectrometry (IMS) are reported. The nuclei under investigation were produced via fragmentation of relativistic energy heavy ions of {sup 78}Kr and {sup 58}Ni. After in-flight separation by the fragment separator RIBLL-2, the nuclei were injected and stored in the experimental storage ring CSRe, and their masses were determined from measurements of the revolution times. The impact of these measurements on the stellar nucleosynthesis in the rp-process is discussed.

  14. The design improvement of horizontal stripline kicker in TPS storage ring

    NASA Astrophysics Data System (ADS)

    Chou, P. J.; Chan, C. K.; Chang, C. C.; Hsu, K. T.; Hu, K. H.; Kuan, C. K.; Sheng, I. C.

    2017-07-01

    We plan to replace the existing horizontal stripline kicker of the transverse feedback system with an improved design. Large reflected power was observed at the downstream port of stripline kicker driven by the feedback amplifier. A rapid surge of vacuum pressure was observed when we tested the high current operation in TPS storage ring in April 2016. A burned feedthrough of the horizontal stripline kicker was discovered during a maintenance shutdown. The improved design is targeted to reduce the reflection of driving power from feedback system and to reduce beam induced RF heating. This major modification of the design is described. The results of RF simulation performed with the electromagnetic code GdfidL are reported as well.

  15. Beamline front end for in-vacuum short period undulator at the photon factory storage ring

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

    Miyauchi, Hiroshi, E-mail: hiroshi.miyauchi@kek.jp; Department of Accelerator Science, School of High Energy Accelerator Science, SOKENDAI; Tahara, Toshihiro, E-mail: ttahara@post.kek.jp

    The straight-section upgrade project of the Photon Factory created four new short straight sections capable of housing in-vacuum short period undulators. The first to fourth short period undulators SGU#17, SGU#03, SGU#01 and SGU#15 were installed at the 2.5-GeV Photon Factory storage ring in 2005, 2006, 2009 and 2013, respectively. The beamline front end for SGU#15 is described in this paper.

  16. The terminal Eocene event - Formation of a ring system around the earth

    NASA Technical Reports Server (NTRS)

    Okeefe, J. A.

    1980-01-01

    It is suggested that the formation of a ring system about the earth by particles and debris related to the North American strewn tektite field is responsible for the terminal Eocene event of 34 million years ago, in which severe climatic changes accompanied by widespread biological extinctions occurred. Botanical data is cited which implies a 20-C decrease in winter temperature with no change in summer temperature, and evidence of the correlation of the North American tektite fall, which is estimated to have a total mass of 10 to the 9th to 10 to the 10th tons, with the disappearance of five of the most abundant species of radiolaria is presented. The possible connection between the tektites and climatic change is argued to result from the screening of sunlight by an equatorial ring of trapped particles of extraterrestrial origin in geocentric orbit which would cut off sunlight only in the winter months. Such a ring, located at a distance of between 1.5 and 2.5 earth radii (the Roche limit) is estimated to have a lifetime of a few million years.

  17. Coupling tree rings and eddy covariance to estimate long-term above and belowground carbon storage at the stand level

    NASA Astrophysics Data System (ADS)

    Dye, A.; Alexander, M. R.; Bishop, D.; Pederson, N.; Hessl, A. E.

    2016-12-01

    Storage of carbon in terrestrial plants and soils directly reduces atmospheric carbon concentration, and it is thereby imperative to improve our understanding of where carbon is being stored and released in an ecosystem and how storages and releases are changing over time. At data-rich sites, coupling alternative measurements of carbon flux can improve this understanding. Here, we present a methodology to inversely model stand-level net storage and release of above- and belowground carbon over a period of 1-2 decades using co-located tree-ring plots and eddy covariance towers at three eastern U.S. forests. We reconstructed annual aboveground wood production (aNPP) from tree rings collected near eddy covariance towers. We compared our aNPP reconstructions with annual tower NEE to address whether interannual variations are correlated. Despite modest correlation, we observed magnitude differences between both records that vary annually. We interpret these differences as indicative of changes in belowground carbon storage, i.e. an aNPP:NEE ratio > 1 indicates a net release of belowground carbon and a ratio < 1 a net storage of belowground carbon. For this interpretation, we assume the following: a) carbon not directed to above or belowground pools is insignificant, b) carbon not stored above ground is stored below ground, and c) mature trees do not add to a storage pool at a higher level every year. While the offset between biometric aNPP and tower NEE could partially be attributed to the diversion of assimilated carbon to nonstructural carbohydrates instead of growth, we argue that this becomes a less important factor over longer time scales in a mature tree. Our approach does not quantify belowground NPP or allocation, but we present a method for estimating belowground carbon storage and release at the stand level, an otherwise difficult task at this scale due to heterogeneity across the stand.

  18. Inertial energy storage device

    DOEpatents

    Knight, Jr., Charles E.; Kelly, James J.; Pollard, Roy E.

    1978-01-01

    The inertial energy storage device of the present invention comprises a composite ring formed of circumferentially wound resin-impregnated filament material, a flanged hollow metal hub concentrically disposed in the ring, and a plurality of discrete filament bandsets coupling the hub to the ring. Each bandset is formed of a pair of parallel bands affixed to the hub in a spaced apart relationship with the axis of rotation of the hub being disposed between the bands and with each band being in the configuration of a hoop extending about the ring along a chordal plane thereof. The bandsets are disposed in an angular relationship with one another so as to encircle the ring at spaced-apart circumferential locations while being disposed in an overlapping relationship on the flanges of the hub. The energy storage device of the present invention has the capability of substantial energy storage due to the relationship of the filament bands to the ring and the flanged hub.

  19. Theoretical study of hydrogen storage in a truncated triangular pyramid molecule consisting of pyridine and benzene rings bridged by vinylene groups

    NASA Astrophysics Data System (ADS)

    Ishikawa, Shigeru; Nemoto, Tetsushi; Yamabe, Tokio

    2018-06-01

    Hydrogen storage in a truncated triangular pyramid molecule C33H21N3, which consists of three pyridine rings and one benzene ring bridged by six vinylene groups, is studied by quantum chemical methods. The molecule is derived by substituting three benzene rings in a truncated tetrahedron hydrocarbon C36H24 with pyridine rings. The optimized molecular structure under C 3v symmetry shows no imaginary vibrational modes at the B3LYP/cc-pVTZ level of theory. The hydrogen storage process is investigated based on the MP2/cc-pVTZ method. Like the structure before substitution, the C33H21N3 molecule has a cavity that stores a hydrogen molecule with a binding energy of - 140 meV. The Langmuir isotherm shows that this cavity can store hydrogen at higher temperatures and lower pressures than usual physisorption materials. The C33H21N3 molecule has a kinetic advantage over the C36H24 molecule because the former molecule has a lower barrier (+ 560 meV) for the hydrogen molecule entering the cavity compared with the latter molecule (+ 730 meV) owing to the lack of hydrogen atoms narrowing the opening.

  20. Conditioning of the vacuum system of the TPS storage ring without baking in situ

    NASA Astrophysics Data System (ADS)

    Chan, C. K.; Chang, C. C.; Shueh, C.; Yang, I. C.; Wu, L. H.; Chen, B. Y.; Cheng, C. M.; Huang, Y. T.; Chuang, J. Y.; Cheng, Y. T.; Hsiao, Y. M.; Sheng, Albert

    2017-04-01

    To shorten the machine downtime, a maintenance procedure without baking in situ has been developed and applied to maintain and to upgrade the vacuum system of the TPS storage ring. The data of photon-stimulated desorption (PSD) reveal no obvious discrepancy between baking and not baking the vacuum system in situ. A beam-conditioning dose of extent only 11.8 A h is required to recover quickly the dynamic pressure of an unbaked vacuum system to its pre-intervention value according to the TPS maintenance experience.

  1. Collective Effects in a Diffraction Limited Storage Ring

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

    Nagaoka, Ryutaro; Bane, Karl L.F.

    Our paper gives an overview of collective effects that are likely to appear and possibly limit the performance in a diffraction-limited storage ring (DLSR) that stores a high-intensity ultra-low-emittance beam. Beam instabilities and other intensity-dependent effects that may significantly impact the machine performance are covered. The latter include beam-induced machine heating, Touschek scattering, intra-beam scattering, as well as incoherent tune shifts. The general trend that the efforts to achieve ultra-low emittance result in increasing the machine coupling impedance and the beam sensitivity to instability is reviewed. The nature of coupling impedance in a DLSR is described, followed by a seriesmore » of potentially dangerous beam instabilities driven by the former, such as resistive-wall, TMCI (transverse mode coupling instability), head-tail and microwave instabilities. Additionally, beam-ion and CSR (coherent synchrotron radiation) instabilities are also treated. Means to fight against collective effects such as lengthening of the bunch with passive harmonic cavities and bunch-by-bunch transverse feedback are introduced. Numerical codes developed and used to evaluate the machine coupling impedance, as well as to simulate beam instability using the former as inputs are described.« less

  2. Collective Effects in a Diffraction Limited Storage Ring

    DOE PAGES

    Nagaoka, Ryutaro; Bane, Karl L.F.

    2015-10-20

    Our paper gives an overview of collective effects that are likely to appear and possibly limit the performance in a diffraction-limited storage ring (DLSR) that stores a high-intensity ultra-low-emittance beam. Beam instabilities and other intensity-dependent effects that may significantly impact the machine performance are covered. The latter include beam-induced machine heating, Touschek scattering, intra-beam scattering, as well as incoherent tune shifts. The general trend that the efforts to achieve ultra-low emittance result in increasing the machine coupling impedance and the beam sensitivity to instability is reviewed. The nature of coupling impedance in a DLSR is described, followed by a seriesmore » of potentially dangerous beam instabilities driven by the former, such as resistive-wall, TMCI (transverse mode coupling instability), head-tail and microwave instabilities. Additionally, beam-ion and CSR (coherent synchrotron radiation) instabilities are also treated. Means to fight against collective effects such as lengthening of the bunch with passive harmonic cavities and bunch-by-bunch transverse feedback are introduced. Numerical codes developed and used to evaluate the machine coupling impedance, as well as to simulate beam instability using the former as inputs are described.« less

  3. Software package for modeling spin-orbit motion in storage rings

    NASA Astrophysics Data System (ADS)

    Zyuzin, D. V.

    2015-12-01

    A software package providing a graphical user interface for computer experiments on the motion of charged particle beams in accelerators, as well as analysis of obtained data, is presented. The software package was tested in the framework of the international project on electric dipole moment measurement JEDI (Jülich Electric Dipole moment Investigations). The specific features of particle spin motion imply the requirement to use a cyclic accelerator (storage ring) consisting of electrostatic elements, which makes it possible to preserve horizontal polarization for a long time. Computer experiments study the dynamics of 106-109 particles in a beam during 109 turns in an accelerator (about 1012-1015 integration steps for the equations of motion). For designing an optimal accelerator structure, a large number of computer experiments on polarized beam dynamics are required. The numerical core of the package is COSY Infinity, a program for modeling spin-orbit dynamics.

  4. Resonant beam behavior studies in the Proton Storage Ring

    NASA Astrophysics Data System (ADS)

    Cousineau, S.; Holmes, J.; Galambos, J.; Fedotov, A.; Wei, J.; Macek, R.

    2003-07-01

    We present studies of space-charge-induced beam profile broadening at high intensities in the Proton Storage Ring (PSR) at Los Alamos National Laboratory. We investigate the profile broadening through detailed particle-in-cell simulations of several experiments and obtain results in good agreement with the measurements. We interpret these results within the framework of coherent resonance theory. With increasing intensity, our simulations show strong evidence for the presence of a quadrupole-mode resonance of the beam envelope with the lattice in the vertical plane. Specifically, we observe incoherent tunes crossing integer values, and large amplitude, nearly periodic envelope oscillations. At the highest operating intensities, we observe a continuing relaxation of the beam through space charge forces leading to emittance growth. The increase of emittance commences when the beam parameters encounter an envelope stop band. Once the stop band is reached, the emittance growth balances the intensity increase to maintain the beam near the stop band edge. Additionally, we investigate the potential benefit of a stop band correction to the high intensity PSR beam.

  5. Large diameter metal ring seal prevents gas leakage at 5000 psi

    NASA Technical Reports Server (NTRS)

    Middelkoop, J. H.

    1966-01-01

    Large metal ring seal prevents gas leakage in hydrogen, helium, or nitrogen storage bottles at pressures up to 5,000 psi. The grooved ring seal which contains elastomer O-rings is installed between the mating faces of the access cover and the storage bottle.

  6. Resonant neutral-particle emission in collisions of electrons with peptide ions in a storage ring.

    PubMed

    Tanabe, T; Noda, K; Saito, M; Lee, S; Ito, Y; Takagi, H

    2003-05-16

    Electron-biomolecular ion collisions were studied using an electrostatic storage ring with a merging beam technique for singly protonated peptides (angiotensin I, II, and III). A strong neutral-particle emission at around 6.5 eV was found in addition to neutrals from recombination at low energies. The rates of the high-energy peak greatly decreased with a slight decrease in the number of amino-acid residues from angiotensin I to III. These results suggest that some peptide bonds were selectively cleaved.

  7. Radiological considerations for the operation of the Advanced Photon Source storage ring (revised).

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

    Moe, H. J.

    2002-05-02

    This report deals with the radiological considerations of operations using 7700-MeV positron and electron beams in the storage ring (SR) tunnel. The radiological considerations addressed include the following: prompt secondary radiation (bremsstrahlung, giant resonance neutrons, medium and high energy neutrons, and muons) produced by electrons/positrons interacting in a beam stop or by particle losses in the component structures; skyshine radiation, which produces a radiation field in nearby areas and at the nearest off-site location; radioactive gases produced by neutron irradiation of air in the vicinity of a particle loss site; noxious gases (ozone and others) produced in air by themore » escaping bremsstrahlung radiation that results from absorbing particles in the components or by synchrotron radiation escaping into the tunnel; activation of the storage ring components that results in a residual radiation field in the vicinity of these materials following shutdown; potential activation of water used for cooling the magnets and other purposes in the SR tunnel; evaluation of the radiation fields due to escaping synchrotron radiation and gas bremsstrahlung. Estimated dose rates outside of the tunnel, in the early assembly area (EAA), and in the Experiment Hall for several modes of operation (including potential safety envelope beam power, normal beam power, and MCI (maximum credible incident) conditions) have been computed. Shielding in the first optics enclosure (FOE) and for the photon beamlines is discussed in ANL/APS/TB-7 (IPE 93), but additional radiological considerations for the ASD diagnostic beamlines are contained in Appendix C. Although the calculations refer to positrons, electron operation would produce essentially the same effects for the identical assumptions.« less

  8. Patterns of Storage, Synthesis and Changing Light Levels Revealed by Carbon Isotope Microsampling within Eocene Metasequoia Tree Rings

    NASA Astrophysics Data System (ADS)

    Jahren, H.; Sternberg, L.

    2005-12-01

    Fossil tree rings from Axel Heiberg Island were microanalyzed for δ13C value in order to assess patterns of tree growth and carbon storage within the Middle Eocene (~45 Ma) Arctic paleoenvironment. Wood from four Metasequoia-type individuals was subsampled for analysis: each individual fossil consisted of between 4 and 10 large (~1 cm thick) consecutive tree rings. One of the fossils displayed an obvious concentric pattern, allowing for the determination of the direction of growth with isotopic pattern. Each ring was divided into ~1 mm thick subsamples, resulting in 5-10 δ13C value determinations per period of ring growth (i.e., growing season). All rings revealed a distinct pattern that was characteristic across growing seasons and across individual fossils. Early in the season, δ13C was at its highest value but descended systematically and sharply to its lowest value at the end of the growing season. Total decrease ranged between 3 and 5 ‰ over the course of each growing season. Identical patterns were observed in the δ13C value of alpha-cellulose isolated from each subsample, indicating that the trends observed did not represent changing levels of secondary metabolites, but rather a seasonal adjustment in the bulk source of carbon used during biosynthesis. Our results are consistent with the following annual pattern of wood synthesis 1.) complete dependence on the mobilization of stored carbon compounds early in the growing season; 2.) systematically increasing use of actively-acquired photosynthate during the growing season; 3.) complete reliance on active photosynthate by the end of the growing season. An additional and significant source of 13C discrimination is declining light levels late in the growing season, and likely contributes to the extreme pattern of δ13C decrease seen across each ring. Our results mimic those seen from modern broadleaf deciduous trees (Helle & Schlesser 2004), but differ from those seen in modern conifers (Barbour et al 2002

  9. CsI-Silicon Particle detector for Heavy ions Orbiting in Storage rings (CsISiPHOS)

    NASA Astrophysics Data System (ADS)

    Najafi, M. A.; Dillmann, I.; Bosch, F.; Faestermann, T.; Gao, B.; Gernhäuser, R.; Kozhuharov, C.; Litvinov, S. A.; Litvinov, Yu. A.; Maier, L.; Nolden, F.; Popp, U.; Sanjari, M. S.; Spillmann, U.; Steck, M.; Stöhlker, T.; Weick, H.

    2016-11-01

    A heavy-ion detector was developed for decay studies in the Experimental Storage Ring (ESR) at the GSI Helmholtz Centre for Heavy Ion Research in Darmstadt, Germany. This detector serves as a prototype for the in-pocket particle detectors for future experiments with the Collector Ring (CR) at FAIR (Facility for Antiproton and Ion Research). The detector includes a stack of six silicon pad sensors, a double-sided silicon strip detector (DSSD), and a CsI(Tl) scintillation detector. It was used successfully in a recent experiment for the detection of the β+-decay of highly charged 142Pm60+ ions. Based on the ΔE / E technique for particle identification and an energy resolution of 0.9% for ΔE and 0.5% for E (Full Width at Half Maximum (FWHM)), the detector is well-suited to distinguish neighbouring isobars in the region of interest.

  10. Software package for modeling spin–orbit motion in storage rings

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

    Zyuzin, D. V., E-mail: d.zyuzin@fz-juelich.de

    2015-12-15

    A software package providing a graphical user interface for computer experiments on the motion of charged particle beams in accelerators, as well as analysis of obtained data, is presented. The software package was tested in the framework of the international project on electric dipole moment measurement JEDI (Jülich Electric Dipole moment Investigations). The specific features of particle spin motion imply the requirement to use a cyclic accelerator (storage ring) consisting of electrostatic elements, which makes it possible to preserve horizontal polarization for a long time. Computer experiments study the dynamics of 10{sup 6}–10{sup 9} particles in a beam during 10{supmore » 9} turns in an accelerator (about 10{sup 12}–10{sup 15} integration steps for the equations of motion). For designing an optimal accelerator structure, a large number of computer experiments on polarized beam dynamics are required. The numerical core of the package is COSY Infinity, a program for modeling spin–orbit dynamics.« less

  11. DESY II, a new injector for the DESY storage rings PETRA and DORIS II

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

    Hemmie, G.

    1983-08-01

    There is a proposal to build a new 9 GeV electron synchrotron as a dedicated injector for the storage rings DORIS and PETRA. This machine will be housed in the old DESY-tunnel side-by-side with the original DESY-synchrotron. It is characterized by a separated function lattice, a 12.5 Hz repetition frequency, an all-metal vacuum chamber and a high shunt impedance rf-system. After commissioning of this new machine in 1984, the old DESY-synchrotron could be converted into a dedicated proton-accelerator as part of the injection chain for HERA.

  12. Corrections for a constant radial magnetic field in the muon \\varvec{g}-2 and electric-dipole-moment experiments in storage rings

    NASA Astrophysics Data System (ADS)

    Silenko, Alexander J.

    2017-10-01

    We calculate the corrections for constant radial magnetic field in muon {g}-2 and electric-dipole-moment experiments in storage rings. While the correction is negligible for the current generation of {g}-2 experiments, it affects the upcoming muon electric-dipole-moment experiment at Fermilab.

  13. OPERATIONAL EXPERIENCE WITH FAST FIBER-OPTIC BEAM LOSS MONITORS FOR THE ADVANCED PHOTON SOURCE STORAGE RING SUPERCONDUCTING UNDULATORS

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

    Dooling, J.; Harkay, K.; Sajaev, V.

    Fast fiber-optic (FFO) beam loss monitors (BLMs) installed with the first two superconducting undulators (SCUs) in the Advanced Photon Source storage ring have proven to be a useful diagnostic for measuring deposited charge (energy) during rapid beam loss events. The first set of FFOBLMs were installed outside the cryostat of the short SCU, a 0.33-m long device, above and below the beam centerline. The second set are mounted with the first 1.1-mlong SCU within the cryostat, on the outboard and inboard sides of the vacuum chamber. The next 1.1-m-long SCU is scheduled to replace the short SCU later in 2016more » and will be fitted with FFOBLMs in a manner similar to original 1.1-m device. The FFOBLMs were employed to set timing and voltage for the abort kicker (AK) system. The AK helps to prevent quenching of the SCUs during beam dumps [1] by directing the beam away from the SC magnet windings. The AK is triggered by the Machine Protection System (MPS). In cases when the AK fails to prevent quenching, the FFOBLMs show that losses often begin before detection by the MPS.« less

  14. Lifetimes of relativistic heavy-ion beams in the High Energy Storage Ring of FAIR

    NASA Astrophysics Data System (ADS)

    Shevelko, V. P.; Litvinov, Yu. A.; Stöhlker, Th.; Tolstikhina, I. Yu.

    2018-04-01

    The High Energy Storage Ring, HESR, will be constructed at the Facility for Antiproton and Ion Research, FAIR, Darmstadt. For the first time, it will be possible to perform experiments with cooled high-intensity stable and radioactive heavy ions at highly relativistic energies. To design experiments at the HESR, realistic estimations of beam lifetimes are indispensable. Here we report calculated cross sections and lifetimes for typical U88+ , U90+ , U92+ , Sn49+ and Sn50+ ions in the energy range E = 400 MeV/u-5 GeV/u, relevant for the HESR. Interactions with the residual gas and with internal gas-jet targets are also considered.

  15. Investigation of the heavy-ion mode in the FAIR High Energy Storage Ring

    NASA Astrophysics Data System (ADS)

    Kovalenko, O.; Dolinskii, O.; Litvinov, Yu A.; Maier, R.; Prasuhn, D.; Stöhlker, T.

    2015-11-01

    High energy storage ring (HESR) as a part of the future accelerator facility FAIR (Facility for Antiproton and Ion Research) will serve for a variety of internal target experiments with high-energy stored heavy ions (SPARC collaboration). Bare uranium is planned to be used as a primary beam. Since a storage time in some cases may be significant—up to half an hour—it is important to examine the high-order effects in the long-term beam dynamics. A new ion optics specifically for the heavy ion mode of the HESR is developed and is discussed in this paper. The subjects of an optics design, tune working point and a dynamic aperture are addressed. For that purpose nonlinear beam dynamics simulations are carried out. Also a flexibility of the HESR ion optical lattice is verified with regard to various experimental setups. Specifically, due to charge exchange reactions in the internal target, secondary beams, such as hydrogen-like and helium-like uranium ions, will be produced. Thus the possibility of separation of these secondary ions and the primary {{{U}}}92+ beam is presented with different internal target locations.

  16. Suppression of alpha-induced lateral surface events in the COBRA experiment using CdZnTe detectors with an instrumented guard-ring electrode

    NASA Astrophysics Data System (ADS)

    Arling, J.-H.; Gerhardt, M.; Gößling, C.; Gehre, D.; Klingenberg, R.; Kröninger, K.; Nitsch, C.; Quante, T.; Rohatsch, K.; Tebrügge, J.; Temminghoff, R.; Theinert, R.; Zatschler, S.; Zuber, K.

    2017-11-01

    The COBRA collaboration searches for neutrinoless double beta-decay (0νββ-decay) using CdZnTe semiconductor detectors with a coplanar-grid readout and a surrounding guard-ring structure. The operation of the COBRA demonstrator at the Gran Sasso underground laboratory (LNGS) indicates that alpha-induced lateral surface events are the dominant source of background events. By instrumenting the guard-ring electrode it is possible to suppress this type of background. In laboratory measurements this method achieved a suppression factor of alpha-induced lateral surface events of 5300+2660-1380, while retaining (85.3 ±0.1%) of gamma events occurring in the entire detector volume. This suppression is superior to the pulse-shape analysis methods used so far in COBRA by three orders of magnitude.

  17. Broadband impedance calculations and single bunch instabilities estimations of of the HLS-II storage ring

    NASA Astrophysics Data System (ADS)

    Zhang, Qing-Kun; Wang, Lin; Li, Wei-Min; Gao, Wei-Wei

    2015-12-01

    The upgrade project of the Hefei Light Source storage ring is under way. In this paper, the broadband impedances of resistive wall and coated ceramic vacuum chamber are calculated using the analytic formula, and the wake fields and impedances of other designed vacuum chambers are simulated by CST code, and then a broadband impedance model is obtained. Using the theoretical formula, longitudinal and transverse single bunch instabilities are discussed. With the carefully-designed vacuum chamber, we find that the thresholds of the beam instabilities are higher than the beam current goal. Supported by Natural Science Foundation of China (11175182, 11175180)

  18. Dissociative recombination measurements of NH{sup +} using an ion storage ring

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

    Novotný, O.; Savin, D. W.; Berg, M.

    We have investigated dissociative recombination (DR) of NH{sup +} with electrons using a merged beams configuration at the TSR heavy-ion storage ring located at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. We present our measured absolute merged-beams recombination rate coefficient for collision energies from 0 to 12 eV. From these data, we have extracted a cross section, which we have transformed to a plasma rate coefficient for the collisional plasma temperature range from T {sub pl} = 10 to 18,000 K. We show that the NH{sup +} DR rate coefficient data in current astrochemical models are underestimatedmore » by up to a factor of approximately nine. Our new data will result in predicted NH{sup +} abundances lower than those calculated by present models. This is in agreement with the sensitivity limits of all observations attempting to detect NH{sup +} in interstellar clouds.« less

  19. New beam-position monitor system for upgraded Photon Factory storage ring.

    PubMed

    Haga, K; Honda, T; Tadano, M; Obina, T; Kasuga, T

    1998-05-01

    Accompanying the brilliance-upgrading project at the Photon Factory storage ring, the beam-position monitor (BPM) system has been renovated. The new system was designed to enable precise and fast measurements to correct the closed-orbit distortion (COD), as well as to feed back the orbit position during user runs. There are 42 BPMs newly installed, amounting to a total of 65 BPMs. All of the BPMs are calibrated on the test bench using a coaxially strung metallic wire. The measured electrical offsets are typically 200 micro m in both directions, which is 1/2-1/3 of those of the old-type BPMs. In the signal-processing system, PIN diode switches are employed in order to improve reliability. In the fastest mode, this system is capable of measuring COD within about 10 ms; this fast acquisition will allow fast suppression of the beam movement for frequencies up to 50 Hz using a global feedback system.

  20. Calibration of Fast Fiber-Optic Beam Loss Monitors for the Advanced Photon Source Storage Ring Superconducting Undulators

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

    Dooling, J.; Harkay, K.; Ivanyushenkov, Y.

    2015-01-01

    We report on the calibration and use of fast fiber-optic (FO) beam loss monitors (BLMs) in the Advanced Photon Source storage ring (SR). A superconducting undulator prototype (SCU0) has been operating in SR Sector 6 (“ID6”) since the beginning of CY2013, and another undulator SCU1 (a 1.1-m length undulator that is three times the length of SCU0) is scheduled for installation in Sector 1 (“ID1”) in 2015. The SCU0 main coil often quenches during beam dumps. MARS simulations have shown that relatively small beam loss (<1 nC) can lead to temperature excursions sufficient to cause quenchingwhen the SCU0windings are nearmore » critical current. To characterize local beam losses, high-purity fused-silica FO cables were installed in ID6 on the SCU0 chamber transitions and in ID1 where SCU1 will be installed. These BLMs aid in the search for operating modes that protect the SCU structures from beam-loss-induced quenching. In this paper, we describe the BLM calibration process that included deliberate beam dumps at locations of BLMs. We also compare beam dump events where SCU0 did and did not quench.« less

  1. Three-dimensional ordering of cold ion beams in a storage ring: A molecular-dynamics simulation study

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

    Yuri, Yosuke, E-mail: yuri.yosuke@jaea.go.jp

    Three-dimensional (3D) ordering of a charged-particle beams circulating in a storage ring is systematically studied with a molecular-dynamics simulation code. An ion beam can exhibit a 3D ordered configuration at ultralow temperature as a result of powerful 3D laser cooling. Various unique characteristics of the ordered beams, different from those of crystalline beams, are revealed in detail, such as the single-particle motion in the transverse and longitudinal directions, and the dependence of the tune depression and the Coulomb coupling constant on the operating points.

  2. Impact parameter sensitive study of inner-shell atomic processes in the experimental storage ring

    NASA Astrophysics Data System (ADS)

    Gumberidze, A.; Kozhuharov, C.; Zhang, R. T.; Trotsenko, S.; Kozhedub, Y. S.; DuBois, R. D.; Beyer, H. F.; Blumenhagen, K.-H.; Brandau, C.; Bräuning-Demian, A.; Chen, W.; Forstner, O.; Gao, B.; Gassner, T.; Grisenti, R. E.; Hagmann, S.; Hillenbrand, P.-M.; Indelicato, P.; Kumar, A.; Lestinsky, M.; Litvinov, Yu. A.; Petridis, N.; Schury, D.; Spillmann, U.; Trageser, C.; Trassinelli, M.; Tu, X.; Stöhlker, Th.

    2017-10-01

    In this work, we present a pilot experiment in the experimental storage ring (ESR) at GSI devoted to impact parameter sensitive studies of inner shell atomic processes for low-energy (heavy-) ion-atom collisions. The experiment was performed with bare and He-like xenon ions (Xe54+, Xe52+) colliding with neutral xenon gas atoms, resulting in a symmetric collision system. This choice of the projectile charge states was made in order to compare the effect of a filled K-shell with the empty one. The projectile and target X-rays have been measured at different observation angles for all impact parameters as well as for the impact parameter range of ∼35-70 fm.

  3. Research and Development on the Storage Ring Vacuum System for the APS Upgrade Project

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

    Stillwell, B.; Brajuskovic, B.; Carter, J.

    A number of research and development activities are underway at Argonne National Laboratory to build confidence in the designs for the storage ring vacuum system required for the Advanced Photon Source Up-grade project (APS-U) [1]. The predominant technical risks are: excessive residual gas pressures during operation; insufficient beam position monitor stability; excessive beam impedance; excessive heating by induced electrical surface currents; and insufficient operational reliability. Present efforts to mitigate these risks include: building and evaluating mockup assemblies; performing mechanical testing of chamber weld joints; developing computational tools; investigating design alternatives; and performing electrical bench measurements. Status of these activities andmore » some of what has been learned to date will be shared.« less

  4. Missing Rings in Pinus halepensis - The Missing Link to Relate the Tree-Ring Record to Extreme Climatic Events.

    PubMed

    Novak, Klemen; de Luis, Martin; Saz, Miguel A; Longares, Luis A; Serrano-Notivoli, Roberto; Raventós, Josep; Čufar, Katarina; Gričar, Jožica; Di Filippo, Alfredo; Piovesan, Gianluca; Rathgeber, Cyrille B K; Papadopoulos, Andreas; Smith, Kevin T

    2016-01-01

    Climate predictions for the Mediterranean Basin include increased temperatures, decreased precipitation, and increased frequency of extreme climatic events (ECE). These conditions are associated with decreased tree growth and increased vulnerability to pests and diseases. The anatomy of tree rings responds to these environmental conditions. Quantitatively, the width of a tree ring is largely determined by the rate and duration of cell division by the vascular cambium. In the Mediterranean climate, this division may occur throughout almost the entire year. Alternatively, cell division may cease during relatively cool and dry winters, only to resume in the same calendar year with milder temperatures and increased availability of water. Under particularly adverse conditions, no xylem may be produced in parts of the stem, resulting in a missing ring (MR). A dendrochronological network of Pinus halepensis was used to determine the relationship of MR to ECE. The network consisted of 113 sites, 1,509 trees, 2,593 cores, and 225,428 tree rings throughout the distribution range of the species. A total of 4,150 MR were identified. Binomial logistic regression analysis determined that MR frequency increased with increased cambial age. Spatial analysis indicated that the geographic areas of south-eastern Spain and northern Algeria contained the greatest frequency of MR. Dendroclimatic regression analysis indicated a non-linear relationship of MR to total monthly precipitation and mean temperature. MR are strongly associated with the combination of monthly mean temperature from previous October till current February and total precipitation from previous September till current May. They are likely to occur with total precipitation lower than 50 mm and temperatures higher than 5°C. This conclusion is global and can be applied to every site across the distribution area. Rather than simply being a complication for dendrochronology, MR formation is a fundamental response of trees

  5. Construction and operation of a support facilities (Building 729) for operation/testing of a prototype accelerator/storage ring (XLS) and machine shop for the National Synchrotron Light Source at Brookhaven National Laboratory, Upton, New York

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

    Not Available

    1992-06-01

    Proposed action is to construct at BNL a 5,600-ft[sup 2] support building, install and operate a prototypic 200 MeV accelerator and a prototypic 700 MeV storage ring within, and to construct and operate a 15 kV substation to power the building. The accelerator and storage ring would comprise the x-ray lithography source or XLS.

  6. STORAGE RING CROSS SECTION MEASUREMENTS FOR ELECTRON IMPACT IONIZATION OF Fe{sup 7+}

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

    Hahn, M.; Novotný, O.; Savin, D. W.

    2015-11-01

    We have measured electron impact ionization for Fe{sup 7+} from the ionization threshold up to 1200 eV. The measurements were performed using the TSR heavy ion storage ring. The ions were stored long enough prior to measurements to remove most metastables, resulting in a beam of 94% ground-level ions. Comparing with the previously recommended atomic data, we find that the Arnaud and Raymond cross section is up to about 40% larger than our measurement, with the largest discrepancies below about 400 eV. The cross section of Dere agrees to within 10%, which is about the magnitude of the experimental uncertainties.more » The remaining discrepancies between our measurement and the Dere calculations are likely due to shortcomings in the theoretical treatment of the excitation-autoionization contribution.« less

  7. Non-exponential decoherence of radio-frequency resonance rotation of spin in storage rings

    NASA Astrophysics Data System (ADS)

    Saleev, A.; Nikolaev, N. N.; Rathmann, F.; Hinder, F.; Pretz, J.; Rosenthal, M.

    2017-08-01

    Precision experiments, such as the search for electric dipole moments of charged particles using radio-frequency spin rotators in storage rings, demand for maintaining the exact spin resonance condition for several thousand seconds. Synchrotron oscillations in the stored beam modulate the spin tune of off-central particles, moving it off the perfect resonance condition set for central particles on the reference orbit. Here, we report an analytic description of how synchrotron oscillations lead to non-exponential decoherence of the radio-frequency resonance driven up-down spin rotations. This non-exponential decoherence is shown to be accompanied by a nontrivial walk of the spin phase. We also comment on sensitivity of the decoherence rate to the harmonics of the radio-frequency spin rotator and a possibility to check predictions of decoherence-free magic energies.

  8. Direct Observation of Spatiotemporal Dynamics of Short Electron Bunches in Storage Rings

    NASA Astrophysics Data System (ADS)

    Evain, C.; Roussel, E.; Le Parquier, M.; Szwaj, C.; Tordeux, M.-A.; Brubach, J.-B.; Manceron, L.; Roy, P.; Bielawski, S.

    2017-02-01

    In recent synchrotron radiation facilities, the use of short (picosecond) electron bunches is a powerful method for producing giant pulses of terahertz coherent synchrotron radiation. Here we report on the first direct observation of these pulse shapes with a few picoseconds resolution, and of their dynamics over a long time. We thus confirm in a very direct way the theories predicting an interplay between two physical processes. Below a critical bunch charge, we observe a train of identical THz pulses (a broadband Terahertz comb) stemming from the shortness of the electron bunches. Above this threshold, a large part of the emission is dominated by drifting structures, which appear through spontaneous self-organization. These challenging single-shot THz recordings are made possible by using a recently developed photonic time stretch detector with a high sensitivity. The experiment has been realized at the SOLEIL storage ring.

  9. Introduction to the magnet and vacuum systems of an electron storage ring

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

    Weng, W.T.

    An accelerator or storage ring complex is a concerted interplay of various functional systems. For the convenience of discussion we can divide it into the following systems: injector, magnet, RF, vacuum, instrumentation and control. In addition, the conventional construction of the building and radiation safety consideration are also needed and finally the beam lines, detector, data acquisition and analysis set-ups for research programs. Dr. L. Teng has given a comprehensive review of the whole complex and the operation of such a facility. I concentrate on the description of magnet and vacuum systems. Only the general function of each system andmore » the basic design concepts will be introduced, no detailed engineering practice will be given which will be best done after a machine design is produced. For further understanding and references a table of bibliography is provided at the end of the paper.« less

  10. Duke storage rink UV/VUV FEL: Status and prospects

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

    Litvinenko, V.N.; Burnham, B.; Madey, J.M.J.

    1995-12-31

    The 1 GeV Duke storage ring was successfully commissioned with parameters exceeding initial specification. The OK-4 FEL has arrived at the Duke FEL laboratory from the Novosibirsk Institute of Nuclear Physics. The OK-4 installation and commissioning is in progress. In this paper we describe the up-to-date status of the Duke storage ring and the OK-4 FEL. The projected performance of the OK-4 UV/VUV FEL is presented based on the electron beam parameters achieved. Initial plans to operate the OK-4 UV/VUV FEL at the Duke 1 GeV storage ring are outlined. Future plans and prospects of both the OK-4 FEL andmore » the Duke storage ring are discussed.« less

  11. Saturation of the laser-induced narrowband coherent synchrotron radiation process: Experimental observation at a storage ring

    NASA Astrophysics Data System (ADS)

    Hosaka, M.; Yamamoto, N.; Takashima, Y.; Szwaj, C.; Le Parquier, M.; Evain, C.; Bielawski, S.; Adachi, M.; Zen, H.; Tanikawa, T.; Kimura, S.; Katoh, M.; Shimada, M.; Takahashi, T.

    2013-02-01

    We study the efficiency limitation affecting laser-induced coherent synchrotron radiation (CSR) at high laser power. Experiments are made on the UVSOR-II storage ring in conditions of narrowband terahertz CSR emission. While, at moderate power, CSR power increases quadratically with laser power, a noticeable decrease in efficiency and eventually a decrease in CSR power is observed experimentally at high power. Details of the underlying process are analyzed numerically. As the saturation effect depends almost instantaneously on the laser intensity, the saturation occurs locally in longitudinal space. This has important consequences on the modulation pattern induced on the electron bunch.

  12. Millimeter wave coherent synchrotron radiation in a compact electron storage ring

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

    Murphy, J.B.; Blum, E.; Heese, R.

    1998-01-01

    Installation of a 2,856 MHz RF system into the XLS compact electron storage ring would allow the generation of millimeter wave coherent synchrotron radiation. Operating at 150 MeV, one could produce bunches containing on the order of 2 {times} 10{sup 7} electrons with a bunch length {sigma}{sub L0} = 0.3 mm, resulting in coherent emission at wavelengths above 0.8 mm. The characteristics of the source and the emitted radiation are discussed. In the case of 100 mrad horizontal collection angle, the average power radiated in the wavelength band 1 mm {le} {lambda} {le} 2 mm is 0.3 mW for singlemore » bunch operation and 24 mW for 80 bunch operation. The peak power in a single pulse of a few picosecond duration is on the order of one watt. By reducing the momentum compaction, the bunch length could be reduced to {sigma}{sub L0} = 0.15 mm, resulting in coherent synchrotron radiation down to 500 {micro}m.« less

  13. DISSOCIATIVE RECOMBINATION MEASUREMENTS OF HCl{sup +} USING AN ION STORAGE RING

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

    Novotný, O.; Stützel, J.; Savin, D. W.

    We have measured dissociative recombination (DR) of HCl{sup +} with electrons using a merged beams configuration at the TSR heavy-ion storage ring located at the Max Planck Institute for Nuclear Physics in Heidelberg, Germany. We present the measured absolute merged beams recombination rate coefficient for collision energies from 0 to 4.5 eV. We have also developed a new method for deriving the cross section from the measurements. Our approach does not suffer from approximations made by previously used methods. The cross section was transformed to a plasma rate coefficient for the electron temperature range from T = 10 to 5000more » K. We show that the previously used HCl{sup +} DR data underestimate the plasma rate coefficient by a factor of 1.5 at T = 10 K and overestimate it by a factor of three at T = 300 K. We also find that the new data may partly explain existing discrepancies between observed abundances of chlorine-bearing molecules and their astrochemical models.« less

  14. Analytical approach to Eigen-emittance evolution in storage rings

    NASA Astrophysics Data System (ADS)

    Nash, Boaz

    This dissertation develops the subject of beam evolution in storage rings with nearly uncoupled symplectic linear dynamics. Linear coupling and dissipative/diffusive processes are treated perturbatively. The beam distribution is assumed Gaussian and a function of the invariants. The development requires two pieces: the global invariants and the local stochastic processes which change the emittances, or averages of the invariants. A map based perturbation theory is described, providing explicit expressions for the invariants near each linear resonance, where small perturbations can have a large effect. Emittance evolution is determined by the damping and diffusion coefficients. The discussion is divided into the cases of uniform and non-uniform stochasticity, synchrotron radiation an example of the former and intrabeam scattering the latter. For the uniform case, the beam dynamics is captured by a global diffusion coefficent and damping decrement for each eigen-invariant. Explicit expressions for these quantities near coupling resonances are given. In many cases, they are simply related to the uncoupled values. Near a sum resonance, it is found that one of the damping decrements becomes negative, indicating an anti-damping instability. The formalism is applied to a number of examples, including synchrobetatron coupling caused by a crab cavity, a case of current interest where there is concern about operation near half integer betatron tune. In the non-uniform case, the moment evolution is computed directly, which is illustrated through the example of intrabeam scattering. Our approach to intrabeam scattering damping and diffusion has the advantage of not requiring a loosely-defined Coulomb Logarithm. It is found that in some situations there is a small difference between our results and the standard approaches such as Bjorken-Mtingwa, which is illustrated by comparison of the two approaches and with a measurement of Au evolution in RHIC. Finally, in combining IBS

  15. Slowing down of ring polymer diffusion caused by inter-ring threading.

    PubMed

    Lee, Eunsang; Kim, Soree; Jung, YounJoon

    2015-06-01

    Diffusion of long ring polymers in a melt is much slower than the reorganization of their internal structures. While direct evidence for entanglements has not been observed in the long ring polymers unlike linear polymer melts, threading between the rings is suspected to be the main reason for slowing down of ring polymer diffusion. It is, however, difficult to define the threading configuration between two rings because the rings have no chain end. In this work, evidence for threading dynamics of ring polymers is presented by using molecular dynamics simulation and applying a novel analysis method. The simulation results are analyzed in terms of the statistics of persistence and exchange times that have proved useful in studying heterogeneous dynamics of glassy systems. It is found that the threading time of ring polymer melts increases more rapidly with the degree of polymerization than that of linear polymer melts. This indicates that threaded ring polymers cannot diffuse until an unthreading event occurs, which results in the slowing down of ring polymer diffusion. © 2015 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.

  16. The contraceptive vaginal ring, NuvaRing(®), a decade after its introduction.

    PubMed

    Roumen, Frans J M E; Mishell, Daniel R

    2012-12-01

    To review the clinical experience with the contraceptive vaginal ring (CVR, NuvaRing(®)) since its introduction over ten years ago. The literature was searched on efficacy, cycle control, safety, user preference and satisfaction of the CVR in comparison with combined oral contraceptives (COCs) and the patch, with special attention to recent developments. The ring has the same working mechanism and contraindications as COCs. Serum levels of steroids are steadier, whereas oestrogenic exposure is lower. Contraceptive efficacy is similar, as are metabolic changes. Cycle control is better, and compliance and continuation rates are equal or higher. Oestrogen-related adverse symptoms appear to be fewer, but reports on the incidence of venous thrombosis are conflicting. Expulsion of the ring is reported by 4% to 20% of women. Local adverse events are the main reason for discontinuation. Acceptability is as high as with COCs and, after structured counselling, the ring is preferred by many women to the pill or the patch. Efficacy of the CVR, and the metabolic changes and adverse events it elicits, are generally comparable to those of COCs, yet oestrogenic exposure is lower and cycle control superior. After counselling, the ring is preferred to the pill by many women.

  17. Missing Rings in Pinus halepensis – The Missing Link to Relate the Tree-Ring Record to Extreme Climatic Events

    PubMed Central

    Novak, Klemen; de Luis, Martin; Saz, Miguel A.; Longares, Luis A.; Serrano-Notivoli, Roberto; Raventós, Josep; Čufar, Katarina; Gričar, Jožica; Di Filippo, Alfredo; Piovesan, Gianluca; Rathgeber, Cyrille B. K.; Papadopoulos, Andreas; Smith, Kevin T.

    2016-01-01

    Climate predictions for the Mediterranean Basin include increased temperatures, decreased precipitation, and increased frequency of extreme climatic events (ECE). These conditions are associated with decreased tree growth and increased vulnerability to pests and diseases. The anatomy of tree rings responds to these environmental conditions. Quantitatively, the width of a tree ring is largely determined by the rate and duration of cell division by the vascular cambium. In the Mediterranean climate, this division may occur throughout almost the entire year. Alternatively, cell division may cease during relatively cool and dry winters, only to resume in the same calendar year with milder temperatures and increased availability of water. Under particularly adverse conditions, no xylem may be produced in parts of the stem, resulting in a missing ring (MR). A dendrochronological network of Pinus halepensis was used to determine the relationship of MR to ECE. The network consisted of 113 sites, 1,509 trees, 2,593 cores, and 225,428 tree rings throughout the distribution range of the species. A total of 4,150 MR were identified. Binomial logistic regression analysis determined that MR frequency increased with increased cambial age. Spatial analysis indicated that the geographic areas of south-eastern Spain and northern Algeria contained the greatest frequency of MR. Dendroclimatic regression analysis indicated a non-linear relationship of MR to total monthly precipitation and mean temperature. MR are strongly associated with the combination of monthly mean temperature from previous October till current February and total precipitation from previous September till current May. They are likely to occur with total precipitation lower than 50 mm and temperatures higher than 5°C. This conclusion is global and can be applied to every site across the distribution area. Rather than simply being a complication for dendrochronology, MR formation is a fundamental response of trees

  18. TSR: A storage and cooling ring for HIE-ISOLDE

    NASA Astrophysics Data System (ADS)

    Butler, P. A.; Blaum, K.; Davinson, T.; Flanagan, K.; Freeman, S. J.; Grieser, M.; Lazarus, I. H.; Litvinov, Yu. A.; Lotay, G.; Page, R. D.; Raabe, R.; Siesling, E.; Wenander, F.; Woods, P. J.

    2016-06-01

    It is planned to install the heavy-ion, low-energy ring TSR, currently at the Max-Planck-Institute for Nuclear Physics in Heidelberg, at the HIE-ISOLDE facility in CERN, Geneva. Such a facility will provide a capability for experiments with stored, cooled secondary beams that is rich and varied, spanning from studies of nuclear ground-state properties and reaction studies of astrophysical relevance, to investigations with highly-charged ions and pure isomeric beams. In addition to experiments performed using beams recirculating within the ring, the cooled beams can be extracted and exploited by external spectrometers for high-precision measurements. The capabilities of the ring facility as well as some physics cases will be presented, together with a brief report on the status of the project.

  19. Ring-diameter Ratios for Multi-ring Basins Average 2.0(0.5)D

    NASA Technical Reports Server (NTRS)

    Pike, R. J.; Spudis, P. D.

    1985-01-01

    The spacing of the concentric rings of planetary impact basins was studied. It is shown that a radial increment of x (sup 0.5) D, where x is about 2.0 and D = ring diameter, separates both (1) adjacent least-squares groups of rings and arcs of multi-ring basins on Mars, Mercury, and the Moon; and (2) adjacent rings of individual basins on the three planets. Statistics for ratios of ring diameters are presented, the first and most-applied parameter of ring spacing. It is found that ratios excluding rings flanking the main ring also have a mean spacing increment of about 2.0. Ratios including such rings, as for the least-squares groups, and (1) above, have a larger increment, averaging 2.1. The F-test indicates, that these spacings of basin ring locations, and mode of ring formation are controlled by the mechanics of the impact event itself, rather than by crustal properties.

  20. Construction and operation of a support facilities (Building 729) for operation/testing of a prototype accelerator/storage ring (XLS) and machine shop for the National Synchrotron Light Source at Brookhaven National Laboratory, Upton, New York. Environmental assessment

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

    Not Available

    1992-06-01

    Proposed action is to construct at BNL a 5,600-ft{sup 2} support building, install and operate a prototypic 200 MeV accelerator and a prototypic 700 MeV storage ring within, and to construct and operate a 15 kV substation to power the building. The accelerator and storage ring would comprise the x-ray lithography source or XLS.

  1. Oxygen Abundances in the Rings of Polar-Ring Galaxies

    NASA Astrophysics Data System (ADS)

    Radtke, I. R.; Eskridge, P. B.; Pogge, R. W.

    2003-05-01

    Polar ring galaxies (PRGs) are typically early-type (S0 or E) galaxies surrounded by rings of gas, dust, and stars orbiting nearly perpendicular to the principle plane of the host galaxy (Whitmore et al. 1990 AJ 100 1489). Given that PRGs have two separate, perpendicular axes of rotation, it is clear on dynamical grounds that PRGs are the products of merger events between two galaxies, but are observed in a state where two distinct kinematic and morphological structures are still apparent. As such, they present a unique opportunity to study merger events in systems where the debris is not confused with material from the host. Our understanding of the relative importance of polar ring systems in the overall process of galaxy evolution is confounded by our lack of knowledge regarding the typical lifetimes and evolutionary histories of polar rings. A crucial factor for understanding the formation and evolution of PRGs is information regarding the elemental abundances of the ring material. Polar rings are typically rich in {\\protectH 2} regions. Optical spectroscopy of these {\\protectH 2} regions can tell us their density, temperature, and oxygen abundance. Our earlier work (Eskridge & Pogge 1997 ApJ 486 259) revealed roughly Solar oxygen abundances for {\\protectH 2} regions in the polar ring of NGC 2685. We have extended this project, and now have spectra for six PRGs. Analysis of the data for II Zw 73 and UGC 7576 reveal the polar rings of these galaxies to have {\\protectH 2} region oxygen abundances in the range 0.3 to 0.6 Solar, substantially less than found for NGC 2685. Abundances in this range are much easier to explain with conventional models of chemical enrichment and polar ring formation. We shall present results for our full sample. Taken as a whole, this sample will provide a clear foundation for the typical chemical enrichment patterns in polar rings, and thus provide a clearer understanding of the formation and evolution of these curious objects. We

  2. New waveguide-type HOM damper for ALS storage ring cavities.

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

    Kwiatkowski, Slawomir; Baptiste, Kenneth; Julian, James

    2004-06-28

    The ALS storage ring 500 MHz RF system uses two re-entrant accelerating cavities powered by a single 320kW PHILLIPS YK1305 klystron. During several years of initial operation, the RF cavities were not equipped with effective passive HOM damper systems. Longitudinal beam stability was achieved through cavity temperature control and the longitudinal feedback system (LFB), which was often operating at the edge of its capabilities. As a result, longitudinal beam stability was a significant operations issue at the ALS. During two consecutive shutdown periods (April 2002 and 2003) we installed E-type HOM dampers on the main and third harmonic cavities. Thesemore » devices dramatically decreased the Q-values of the longitudinal anti-symmetric HOM modes. The next step is to damp the rest of the longitudinal HOM modes in the main cavities below the synchrotron radiation damping level. This will hopefully eliminate the need for the LFB and set the stage for a possible increase in beam current. The ''waveguide'' type of HOM damper was the only option that didn't significantly compromise the vacuum performance of the RF cavity. The design process and the results of the low level measurements of the new waveguide dampers are presented in this paper.« less

  3. Calculations of the conditions for bunch leakage in the Los Alamos proton storage ring

    NASA Astrophysics Data System (ADS)

    Neuffer, D.; Ohmori, C.

    1994-04-01

    Observations are consistent with the possibility of an "ep" instability in the Los Alamos Proton Storage Ring (PSR) with both bunched and unbunched beam. The instability requires electrons to be trapped within the beam, and calculations have shown that such trapping requires leakage of beam into the interbunch gap. Observationally, leakage of beam into the gap appears necessary for the onset of the instability. In this paper we present results of studies of the longitudinal beam dynamics at PSR parameters. The studies indicate that the combined effects of the rf buncher, longitudinal space charge, and injection mismatch are sufficient to cause the observed bunch leakage. Simulation results are presented and compared with PSR observations. Variations of PSR performance parameters are considered, and methods of improving bunch confinement are suggested and studied.

  4. Flexible matrix composite laminated disk/ring flywheel

    NASA Technical Reports Server (NTRS)

    Gupta, B. P.; Hannibal, A. J.

    1984-01-01

    An energy storage flywheel consisting of a quasi-isotropic composite disk overwrapped by a circumferentially wound ring made of carbon fiber and a elastometric matrix is proposed. Through analysis it was demonstrated that with an elastomeric matrix to relieve the radial stresses, a laminated disk/ring flywheel can be designed to store a least 80.3 Wh/kg or about 68% more than previous disk/ring designs. at the same time the simple construction is preserved.

  5. Tracing footprints of environmental events in tree ring chemistry using neutron activation analysis

    NASA Astrophysics Data System (ADS)

    Sahin, Dagistan

    The aim of this study is to identify environmental effects on tree-ring chemistry. It is known that industrial pollution, volcanic eruptions, dust storms, acid rain and similar events can cause substantial changes in soil chemistry. Establishing whether a particular group of trees is sensitive to these changes in soil environment and registers them in the elemental chemistry of contemporary growth rings is the over-riding goal of any Dendrochemistry research. In this study, elemental concentrations were measured in tree-ring samples of absolutely dated eleven modern forest trees, grown in the Mediterranean region, Turkey, collected and dated by the Malcolm and Carolyn Wiener Laboratory for Aegean and Near Eastern Dendrochronology laboratory at Cornell University. Correlations between measured elemental concentrations in the tree-ring samples were analyzed using statistical tests to answer two questions. Does the current concentration of a particular element depend on any other element within the tree? And, are there any elements showing correlated abnormal concentration changes across the majority of the trees? Based on the detailed analysis results, the low mobility of sodium and bromine, positive correlations between calcium, zinc and manganese, positive correlations between trace elements lanthanum, samarium, antimony, and gold within tree-rings were recognized. Moreover, zinc, lanthanum, samarium and bromine showed strong, positive correlations among the trees and were identified as possible environmental signature elements. New Dendrochemistry information found in this study would be also useful in explaining tree physiology and elemental chemistry in Pinus nigra species grown in Turkey. Elemental concentrations in tree-ring samples were measured using Neutron Activation Analysis (NAA) at the Pennsylvania State University Radiation Science and Engineering Center (RSEC). Through this study, advanced methodologies for methodological, computational and

  6. Progress on the Design of the Storage Ring Vacuum System for the Advanced Photon Source Upgrade Project

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

    Stillwell, B.; Billett, B.; Brajuskovic, B.

    2017-06-20

    Recent work on the design of the storage ring vacuum system for the Advanced Photon Source Upgrade project (APS-U) includes: revising the vacuum system design to accommodate a new lattice with reverse bend magnets, modifying the designs of vacuum chambers in the FODO sections for more intense incident synchrotron radiation power, modifying the design of rf-shielding bellows liners for better performance and reliability, modifying photon absorber designs to make better use of available space, and integrated planning of components needed in the injection, extraction and rf cavity straight sections. An overview of progress in these areas is presented.

  7. Design of 3 GeV booster ring lattice

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

    Etisken, O., E-mail: ozgur.etisken@cern.ch; Ciftci, A. K., E-mail: abbas.kenan.ciftci@cern.ch

    2016-03-25

    The aim of this study is to design of a 3 GeV booster ring for the 3 GeV storage ring. Electrons are needed to be accelerated to 3.0 GeV from 0.15 GeV energy. In this frame, we studied on two options for booster ring; a compact booster and the booster that shares the same tunnel with the storage ring. The lattice type has been chosen FODO for both options, lattice parameters are calculated, sextupole magnets are used to decrease dynamic aperture problem and dynamic aperture calculations are also made with considering of the necessary conditions. After designing and calculating ofmore » the parameters, these designs have been compared with each other. In addition to this comparison, these booster design parameters have been compared with some world centers design parameters and the reliability of the booster design is seen. Beam optics, OPA and Elegant simulation programs have been used in the study calculations.« less

  8. Subauroral polarization stream on the outer boundary of the ring current during an energetic ion injection event

    NASA Astrophysics Data System (ADS)

    Yuan, Zhigang; Qiao, Zheng; Li, Haimeng; Huang, Shiyong; Wang, Dedong; Yu, Xiongdong; Yu, Tao

    2017-04-01

    Subauroral polarization stream (SAPS) electric field can play an important role in the coupling between the inner magnetosphere and ionosphere; however, the production mechanism of SAPS has not been yet solved. During an energetic ion injection event on 26 March 2004, at latitudes lower than the equatorward boundaries of precipitating plasma sheet electrons and ions, the Defense Meteorological Satellite Program (DMSP) F13 satellite simultaneously observed a strong SAPS with the peak velocity of 1294 m/s and downward flowing field-aligned currents (FACs). Conjugate observations of DMSP F13 and NOAA 15 satellites have shown that FACs flowing into the ionosphere just lie in the outer boundary of the ring current (RC). The downward flowing FACs were observed in a region of positive latitudinal gradients of the ion energy density, implying that the downward flowing FACs are more likely linked to the azimuthal gradient than the radial gradient of the RC ion pressure. Our result demonstrates that RC ion pressure gradients on the outer boundary of the RC in the evening sector during energetic ion injection events can lead to downward flowing FACs so as to cause strong SAPS in condition of low ionospheric conductivities.Plain Language SummaryThis paper provides a good case that the SAPS and FAC occurred in the outer boundary of the <span class="hlt">ring</span> current during an energetic ion injection <span class="hlt">event</span>. Our result demonstrates that RC ion pressure gradients on the outer boundary of the RC in the evening sector during energetic ion injection <span class="hlt">events</span> can lead to downward flowing FACs so as to cause strong SAPS in condition of low ionospheric conductivities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800065664&hterms=data+storage&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Ddata%2Bstorage','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800065664&hterms=data+storage&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Ddata%2Bstorage"><span>Discrete <span class="hlt">event</span> simulation and the resultant data <span class="hlt">storage</span> system response in the operational mission environment of Jupiter-Saturn /Voyager/ spacecraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mukhopadhyay, A. K.</p> <p>1978-01-01</p> <p>The Data <span class="hlt">Storage</span> Subsystem Simulator (DSSSIM) simulating (by ground software) occurrence of discrete <span class="hlt">events</span> in the Voyager mission is described. Functional requirements for Data <span class="hlt">Storage</span> Subsystems (DSS) simulation are discussed, and discrete <span class="hlt">event</span> simulation/DSSSIM processing is covered. Four types of outputs associated with a typical DSSSIM run are presented, and DSSSIM limitations and constraints are outlined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JHyd..544..363S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JHyd..544..363S"><span>Groundwater <span class="hlt">storage</span> inferred from earthquake activities around East Asia and West Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shih, David Ching-Fang</p> <p>2017-01-01</p> <p>Groundwater is a necessary and indispensable resource in the gradual depletion of the amount in the world. Groundwater <span class="hlt">storage</span> is an important indicator to evaluate the capability of volume of water can be released from the aquifer. This research highlights a new assessment to infer the <span class="hlt">storage</span> of aquifer using earthquakes activated around East Asia and the <span class="hlt">ring</span> of fire at West Pacific Ocean. Ten significant seismic <span class="hlt">events</span> are used to evaluate the groundwater <span class="hlt">storage</span> at an observation station. By analyzing the spectra of groundwater level and seismogram, it is evident that the period varied in 7-25 s of Rayleigh waves significantly dominate propagation from the epicenter of earthquakes to the observation station. The <span class="hlt">storage</span> coefficient is then shown in the order of 10-4-10-3. The major innovation of this study suggests that to concretely deduce the groundwater <span class="hlt">storage</span> by earthquake activity has become feasible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhR...507....1B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhR...507....1B"><span>Theory of the polarization of highly charged ions in <span class="hlt">storage</span> <span class="hlt">rings</span>: Production, preservation, observation and application to the search for a violation of the fundamental symmetries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bondarevskaya, A.; Prozorov, A.; Labzowsky, L.; Plunien, G.; Liesen, D.; Bosch, F.</p> <p>2011-10-01</p> <p>Theoretical concepts for the production, preservation and control of polarized highly charged ion beams in <span class="hlt">storage</span> <span class="hlt">rings</span> are investigated. It is argued that hydrogen-like ions can be polarized efficiently by optical pumping of the Zeeman sublevels of ground state hyperfine levels and that the maximum achievable nuclear polarization exceeds 90%. In order to study the preservation of the polarization during the ion motion through the magnetic system of the <span class="hlt">ring</span>, the concept of the instantaneous quantization axis is introduced. It is suggested that the employment of “Siberian snakes” may help to preserve the ion beam polarization in the <span class="hlt">ring</span>. The control of the beam polarization can be achieved by different methods: by measuring the Stokes parameters for the emitted photons or by observing the angular dependence of the transition rates for polarized ions. The important motivation for the production of polarized ion beams is the possibility to observe parity nonconservation effects in the hyperfine-quenched transitions in helium-like highly charged ions, where these effects can reach an unprecedented high value for atomic physics. The possible observation of parity nonconservation effects connected with the nuclear anapole moment is also discussed. A method for the observation of the electric dipole moment of an electron in a <span class="hlt">storage</span> <span class="hlt">ring</span> with a polarized highly charged ion beam is proposed. This method allows, in principle, to improve the existing boundaries for the electric dipole moment of an electron. However, the requirements of the corresponding experiment are very stringent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP51D1882R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP51D1882R"><span>Seasonality and Disturbance <span class="hlt">Events</span> in the Carbon Isotope Record of Slash Pine (Pinus elliottii) Tree <span class="hlt">Rings</span> from Big Pine Key, Florida</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rebenack, C.; Anderson, W. T.; Cherubini, P.</p> <p>2011-12-01</p> <p>The South Florida coastal ecosystem is among the world's subtropical coastlines which are threatened by the potential effects of climate change. A well-developed localized paleohistory is essential in the understanding of the role climate variability/change has on both hydrological dynamics and disturbance <span class="hlt">event</span> frequency and intensity; this understanding can then aid in the development of better predictive models. High resolution paleoclimate proxies, such as those developed from tree-<span class="hlt">ring</span> archives, may be useful tools for extrapolating actual climate trends over time from the overlapping long-term and short-term climate cycles, such as the Atlantic Multidecadal Oscillation (AMO) and the El Niño-Southern Oscillation (ENSO). In South Florida, both the AMO and ENSO strongly influence seasonal precipitation, and a more complete grasp of how these cycles have affected the region in the past could be applied to future freshwater management practices. Dendrochronology records for the terrestrial subtropics, including South Florida, are sparse because seasonality for this region is precipitation driven; this is in contrast to the drastic temperature changes experienced in the temperate latitudes. Subtropical seasonality may lead to the complete lack of visible <span class="hlt">rings</span> or to the formation of <span class="hlt">ring</span> structures that may or may not represent annual growth. Fortunately, it has recently been demonstrated that Pinus elliottii trees in South Florida produce distinct annual growth <span class="hlt">rings</span>; however <span class="hlt">ring</span> width was not found to significantly correlate with either the AMO or ENSO. Dendrochronology studies may be taken a step beyond the physical tree-<span class="hlt">ring</span> proxies by using the carbon isotope ratios to infer information about physiological controls and environmental factors that affect the distribution of isotopes within the plant. It has been well established that the stable isotope composition of cellulose can be related to precipitation, drought, large-scale ocean/atmospheric oscillations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMPP33A2105R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMPP33A2105R"><span>Seasonality and Disturbance <span class="hlt">Events</span> in the Carbon Isotope Record of Pinus elliottii Tree <span class="hlt">Rings</span> from Big Pine Key, Florida</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rebenack, C.; Anderson, W. T.; Cherubini, P.</p> <p>2012-12-01</p> <p>The South Florida coastal ecosystem is among the world's subtropical coastlines which are threatened by the potential effects of climate change. A well-developed localized paleohistory is essential in the understanding of the role climate variability/change has on both hydrological dynamics and disturbance <span class="hlt">event</span> frequency and intensity; this understanding can then aid in the development of better predictive models. High resolution paleoclimate proxies, such as those developed from tree-<span class="hlt">ring</span> archives, may be useful tools for extrapolating actual climate trends over time from the overlapping long-term and short-term climate cycles, such as the Atlantic Multidecadal Oscillation (AMO) and the El Niño-Southern Oscillation (ENSO). In South Florida, both the AMO and ENSO strongly influence seasonal precipitation, and a more complete grasp of how these cycles have affected the region in the past could be applied to future freshwater management practices. Dendrochronology records for the terrestrial subtropics, including South Florida, are sparse because seasonality for this region is precipitation-driven; this is in contrast to the drastic temperature changes experienced in the temperate latitudes. Subtropical seasonality may lead to the complete lack of visible <span class="hlt">rings</span> or to the formation of <span class="hlt">ring</span> structures that may or may not represent annual growth. Fortunately, it has recently been demonstrated that Pinus elliottii trees in South Florida produce distinct annual growth <span class="hlt">rings</span>; however <span class="hlt">ring</span> width was not found to significantly correlate with either the AMO or ENSO. Dendrochronology studies may be taken a step beyond the physical tree-<span class="hlt">ring</span> proxies by using the carbon isotope ratios to infer information about physiological controls and environmental factors that affect the distribution of isotopes within the plant. It has been well established that the stable isotope composition of cellulose can be related to precipitation, drought, large-scale ocean/atmospheric oscillations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/863440','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/863440"><span>Loss-free method of charging accumulator <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Maschke, Alfred W.</p> <p>1979-01-01</p> <p>A method for the production of high current pulses of heavy ions having an atomic weight greater than 100. Also a linear accelerator based apparatus for carrying out said method. Pulses formed by the method of the subject invention are suitable for <span class="hlt">storage</span> in a <span class="hlt">storage</span> <span class="hlt">ring</span>. The accumulated pulses may be used in inertial fusion apparatus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017LaPhL..14j5101P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017LaPhL..14j5101P"><span>Soliton formation from a noise-like pulse during extreme <span class="hlt">events</span> in a fibre <span class="hlt">ring</span> laser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pottiez, O.; Ibarra-Villalon, H. E.; Bracamontes-Rodriguez, Y.; Minguela-Gallardo, J. A.; Garcia-Sanchez, E.; Lauterio-Cruz, J. P.; Hernandez-Garcia, J. C.; Bello-Jimenez, M.; Kuzin, E. A.</p> <p>2017-10-01</p> <p>We study experimentally the interactions between soliton and noise-like pulse (NLP) components in a mode-locked fibre <span class="hlt">ring</span> laser operating in a hybrid soliton-NLP regime. For proper polarization adjustments, one NLP and multiple packets of solitons coexist in the cavity, at 1530 nm and 1558 nm, respectively. By examining time-domain sequences measured using a 16 GHz real-time oscilloscope, we unveil the process of soliton genesis: they are produced during extreme-intensity episodes affecting the NLP. These extreme <span class="hlt">events</span> can emerge sporadically, appear in small groups or even form quasi-periodic sequences. Once formed, the wavelength-shifted soliton packet drifts away from the NLP in the dispersive cavity, and eventually vanishes after a variable lifetime. Evidence of the inverse process, through which NLP formation is occasionally seeded by an extreme-intensity <span class="hlt">event</span> affecting a bunch of solitons, is also provided. The quasi-stationary dynamics described here constitutes an impressive illustration of the connections and interactions between NLPs, extreme <span class="hlt">events</span> and solitons in passively mode-locked fibre lasers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ChPhC..40h6102L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ChPhC..40h6102L"><span>The trigger system for the external target experiment in the HIRFL cooling <span class="hlt">storage</span> <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Min; Zhao, Lei; Liu, Jin-Xin; Lu, Yi-Ming; Liu, Shu-Bin; An, Qi</p> <p>2016-08-01</p> <p>A trigger system was designed for the external target experiment in the Cooling <span class="hlt">Storage</span> <span class="hlt">Ring</span> (CSR) of the Heavy Ion Research Facility in Lanzhou (HIRFL). Considering that different detectors are scattered over a large area, the trigger system is designed based on a master-slave structure and fiber-based serial data transmission technique. The trigger logic is organized in hierarchies, and flexible reconfiguration of the trigger function is achieved based on command register access or overall field-programmable gate array (FPGA) logic on-line reconfiguration controlled by remote computers. We also conducted tests to confirm the function of the trigger electronics, and the results indicate that this trigger system works well. Supported by the National Natural Science Foundation of China (11079003), the Knowledge Innovation Program of the Chinese Academy of Sciences (KJCX2-YW-N27), and the CAS Center for Excellence in Particle Physics (CCEPP).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008PhRvS..11a0101M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008PhRvS..11a0101M"><span>Electron cloud generation and trapping in a quadrupole magnet at the Los Alamos proton <span class="hlt">storage</span> <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Macek, Robert J.; Browman, Andrew A.; Ledford, John E.; Borden, Michael J.; O'Hara, James F.; McCrady, Rodney C.; Rybarcyk, Lawrence J.; Spickermann, Thomas; Zaugg, Thomas J.; Pivi, Mauro T. F.</p> <p>2008-01-01</p> <p>Recent beam physics studies on the two-stream e-p instability at the LANL proton <span class="hlt">storage</span> <span class="hlt">ring</span> (PSR) have focused on the role of the electron cloud generated in quadrupole magnets where primary electrons, which seed beam-induced multipacting, are expected to be largest due to grazing angle losses from the beam halo. A new diagnostic to measure electron cloud formation and trapping in a quadrupole magnet has been developed, installed, and successfully tested at PSR. Beam studies using this diagnostic show that the “prompt” electron flux striking the wall in a quadrupole is comparable to the prompt signal in the adjacent drift space. In addition, the “swept” electron signal, obtained using the sweeping feature of the diagnostic after the beam was extracted from the <span class="hlt">ring</span>, was larger than expected and decayed slowly with an exponential time constant of 50 to 100μs. Other measurements include the cumulative energy spectra of prompt electrons and the variation of both prompt and swept electron signals with beam intensity. Experimental results were also obtained which suggest that a good fraction of the electrons observed in the adjacent drift space for the typical beam conditions in the 2006 run cycle were seeded by electrons ejected from the quadrupole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26291346','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26291346"><span>Photoswitchable Molecular <span class="hlt">Rings</span> for Solar-Thermal Energy <span class="hlt">Storage</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Durgun, E; Grossman, Jeffrey C</p> <p>2013-03-21</p> <p>Solar-thermal fuels reversibly store solar energy in the chemical bonds of molecules by photoconversion, and can release this stored energy in the form of heat upon activation. Many conventional photoswichable molecules could be considered as solar thermal fuels, although they suffer from low energy density or short lifetime in the photoinduced high-energy metastable state, rendering their practical use unfeasible. We present a new approach to the design of chemistries for solar thermal fuel applications, wherein well-known photoswitchable molecules are connected by different linker agents to form molecular <span class="hlt">rings</span>. This approach allows for a significant increase in both the amount of stored energy per molecule and the stability of the fuels. Our results suggest a range of possibilities for tuning the energy density and thermal stability as a function of the type of the photoswitchable molecule, the <span class="hlt">ring</span> size, or the type of linkers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1413910-experimental-evidence-ion-induced-instabilities-nsls-ii-storage-ring','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1413910-experimental-evidence-ion-induced-instabilities-nsls-ii-storage-ring"><span>Experimental evidence of ion-induced instabilities in the NSLS-II <span class="hlt">storage</span> <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Cheng, Weixing; Li, Yongjun; Podobedov, Boris</p> <p>2017-03-12</p> <p>Fast ion instability has been identified as one of the most prominent instabilities in the recently constructed NSLS-II <span class="hlt">storage</span> <span class="hlt">ring</span> at Brookhaven National Laboratory. At a relatively low beam current (~ 25 mA) multi-bunch fills, ion-induced instabilities have already been observed during the early stages of machine commissioning. At present user operation with 250 mA in ~1000 bunches, the fast ion still remains the dominant instability, even after months of vacuum conditioning at high current. Ion-induced dipole motions of the electron beam have been suppressed using the transverse bunch-by-bunch (BxB) feedback system. However other adverse effects of this instability, suchmore » as the vertical beam size increase along the bunch train cannot be cured by the feedback system. Therefore, to achieve the NSLS-II design current of 500 mA while maintaining a small vertical beam emittance, it is important to further understand the fast ion instability and develop mitigation techniques. This paper reports on a series of ion-instability observations at various fill patterns and beam currents using start-of-art NSLS-II diagnostic tools.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1413910','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1413910"><span>Experimental evidence of ion-induced instabilities in the NSLS-II <span class="hlt">storage</span> <span class="hlt">ring</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>Cheng, Weixing; Li, Yongjun; Podobedov, Boris</p> <p></p> <p>Fast ion instability has been identified as one of the most prominent instabilities in the recently constructed NSLS-II <span class="hlt">storage</span> <span class="hlt">ring</span> at Brookhaven National Laboratory. At a relatively low beam current (~ 25 mA) multi-bunch fills, ion-induced instabilities have already been observed during the early stages of machine commissioning. At present user operation with 250 mA in ~1000 bunches, the fast ion still remains the dominant instability, even after months of vacuum conditioning at high current. Ion-induced dipole motions of the electron beam have been suppressed using the transverse bunch-by-bunch (BxB) feedback system. However other adverse effects of this instability, suchmore » as the vertical beam size increase along the bunch train cannot be cured by the feedback system. Therefore, to achieve the NSLS-II design current of 500 mA while maintaining a small vertical beam emittance, it is important to further understand the fast ion instability and develop mitigation techniques. This paper reports on a series of ion-instability observations at various fill patterns and beam currents using start-of-art NSLS-II diagnostic tools.« 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_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.osti.gov/pages/biblio/1341524-analysis-coupled-bunch-instabilities-nsls-ii-storage-ring-cell-petra-iii-cavity','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1341524-analysis-coupled-bunch-instabilities-nsls-ii-storage-ring-cell-petra-iii-cavity"><span>Analysis of coupled-bunch instabilities for the NSLS-II <span class="hlt">storage</span> <span class="hlt">ring</span> with a 500MHz 7-cell PETRA-III cavity</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Bassi, G.; Blednykh, A.; Cheng, W.; ...</p> <p>2015-12-11</p> <p>We present the NSLS-II <span class="hlt">storage</span> <span class="hlt">ring</span> that is designed to operate with superconducting RF-cavities with the aim to store an average current of 500 mA distributed in 1080 bunches, with a gap in the uniform filling for ion clearing. At the early stage of the commissioning (phase 1), characterized by a bare lattice without damping wigglers and without Landau cavities, a normal conducting 7-cell PETRA-III RF-cavity structure has been installed with the goal to store an average current of 25 mA. In this paper we discuss our analysis of coupled-bunch instabilities driven by the Higher Order Modes (HOMs) of themore » 7-cell PETRA-III RF-cavity. As a cure of the instabilities, we apply a well-known scheme based on a proper detuning of the HOMs frequencies based upon cavity temperature change, and the use of the beneficial effect of the slow head–tail damping at positive chromaticity to increase the transverse coupled-bunch instability thresholds. In addition, we discuss measurements of coupled-bunch instabilities observed during the phase 1 commissioning of the NSLS-II <span class="hlt">storage</span> <span class="hlt">ring</span>. In our analysis we rely, in the longitudinal case, on the theory of coupled-bunch instability for uniform fillings, while in the transverse case we complement our studies with numerical simulations with OASIS, a novel parallel particle tracking code for self-consistent simulations of collective effects driven by short and long-range wakefields.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JAP...102l4904M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JAP...102l4904M"><span>Active damping of the e-p instability at the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Macek, R. J.; Assadi, S.; Byrd, J. M.; Deibele, C. E.; Henderson, S. D.; Lee, S. Y.; McCrady, R. C.; Pivi, M. F. T.; Plum, M. A.; Walbridge, S. B.; Zaugg, T. J.</p> <p>2007-12-01</p> <p>A prototype of an analog, transverse (vertical) feedback system for active damping of the two-stream (e-p) instability has been developed and successfully tested at the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> (PSR). This system was able to improve the instability threshold by approximately 30% (as measured by the change in RF buncher voltage at instability threshold). The feedback system configuration, setup procedures, and optimization of performance are described. Results of several experimental tests of system performance are presented including observations of instability threshold improvement and grow-damp experiments, which yield estimates of instability growth and damping rates. A major effort was undertaken to identify and study several factors limiting system performance. Evidence obtained from these tests suggests that performance of the prototype was limited by higher instability growth rates arising from beam leakage into the gap at lower RF buncher voltage and the onset of instability in the horizontal plane, which had no feedback.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995paac.confW...1P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995paac.confW...1P"><span>Electric fields, electron production, and electron motion at the stripper foil in the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Plum, M.</p> <p></p> <p>The beam instability at the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> (PSR) most likely involves coupled oscillations between electrons and protons. For this instability to occur, there must be a strong source of electrons. Investigation of the various sources of electrons in the PSR had begun. Copious electron production is expected in the injection section because this section contains the stripper foil. This foil is mounted near the center of the beam pipe, and both circulating and injected protons pass through it, thus allowing ample opportunity for electron production. This paper discusses various mechanisms for electron production, beam-induced electric fields, and electron motion in the vicinity of the foil.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvC..96c4617Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvC..96c4617Z"><span>Nuclear-matter radius studies from 58Ni(α ,α ) experiments at the GSI Experimental <span class="hlt">Storage</span> <span class="hlt">Ring</span> with the EXL facility</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zamora, J. C.; Aumann, T.; Bagchi, S.; Bönig, S.; Csatlós, M.; Dillmann, I.; Dimopoulou, C.; Egelhof, P.; Eremin, V.; Furuno, T.; Geissel, H.; Gernhäuser, R.; Harakeh, M. N.; Hartig, A.-L.; Ilieva, S.; Kalantar-Nayestanaki, N.; Kiselev, O.; Kollmus, H.; Kozhuharov, C.; Krasznahorkay, A.; Kröll, Th.; Kuilman, M.; Litvinov, S.; Litvinov, Yu. A.; Mahjour-Shafiei, M.; Mutterer, M.; Nagae, D.; Najafi, M. A.; Nociforo, C.; Nolden, F.; Popp, U.; Rigollet, C.; Roy, S.; Scheidenberger, C.; von Schmid, M.; Steck, M.; Streicher, B.; Stuhl, L.; Thürauf, M.; Uesaka, T.; Weick, H.; Winfield, J. S.; Winters, D.; Woods, P. J.; Yamaguchi, T.; Yue, K.; Zenihiro, J.</p> <p>2017-09-01</p> <p>A novel method for measuring nuclear reactions in inverse kinematics with stored ion beams was successfully used to extract the nuclear-matter radius of 58Ni. The experiment was performed at the experimental heavy-ion <span class="hlt">storage</span> <span class="hlt">ring</span> at the GSI facility using a stored 58Ni beam at energies of 100 and 150 MeV/u and an internal helium gas-jet target. Elastically scattered α -recoils at low momentum transfers were measured with an in-<span class="hlt">ring</span> detector system compatible with ultrahigh vacuum. Experimental angular distributions were fitted using density-dependent optical model potentials within the eikonal approximation. This permitted the extraction of the point-matter root-mean-square radius of 58Ni with an average value of 3.70(7) fm. Results from this work are in good agreement with several experiments performed in the past in normal kinematics. This pioneering experiment demonstrates a major breakthrough towards future investigations with far-from-stability stored beams using the present technique.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770052553&hterms=Dunham&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D80%26Ntt%3DDunham','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770052553&hterms=Dunham&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D80%26Ntt%3DDunham"><span>The <span class="hlt">rings</span> of Uranus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Elliot, J. L.; Dunham, E.; Mink, D.</p> <p>1977-01-01</p> <p>A description is given of the observation of five brief occultations of the star SAO 158687 which occurred both before and after its occultation by Uranus on March 10, 1977. The <span class="hlt">events</span> were observed with a three-channel occultation photometer, attached to a 91-cm telescope. The observations indicate that at least five <span class="hlt">rings</span> encircle the planet Uranus. Possible reasons for the narrowness of the Uranus <span class="hlt">rings</span> are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP11C1037F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP11C1037F"><span>Selective Tree-<span class="hlt">ring</span> Models: A Novel Method for Reconstructing Streamflow Using Tree <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Foard, M. B.; Nelson, A. S.; Harley, G. L.</p> <p>2017-12-01</p> <p>Surface water is among the most instrumental and vulnerable resources in the Northwest United States (NW). Recent observations show that overall water quantity is declining in streams across the region, while extreme flooding <span class="hlt">events</span> occur more frequently. Historical streamflow models inform probabilities of extreme flow <span class="hlt">events</span> (flood or drought) by describing frequency and duration of past <span class="hlt">events</span>. There are numerous examples of tree-<span class="hlt">rings</span> being utilized to reconstruct streamflow in the NW. These models confirm that tree-<span class="hlt">rings</span> are highly accurate at predicting streamflow, however there are many nuances that limit their applicability through time and space. For example, most models predict streamflow from hydrologically altered rivers (e.g. dammed, channelized) which may hinder our ability to predict natural prehistoric flow. They also have a tendency to over/under-predict extreme flow <span class="hlt">events</span>. Moreover, they often neglect to capture the changing relationships between tree-growth and streamflow over time and space. To address these limitations, we utilized national tree-<span class="hlt">ring</span> and streamflow archives to investigate the relationships between the growth of multiple coniferous species and free-flowing streams across the NW using novel species-and site-specific streamflow models - a term we coined"selective tree-<span class="hlt">ring</span> models." Correlation function analysis and regression modeling were used to evaluate the strengths and directions of the flow-growth relationships. Species with significant relationships in the same direction were identified as strong candidates for selective models. Temporal and spatial patterns of these relationships were examined using running correlations and inverse distance weighting interpolation, respectively. Our early results indicate that (1) species adapted to extreme climates (e.g. hot-dry, cold-wet) exhibit the most consistent relationships across space, (2) these relationships weaken in locations with mild climatic variability, and (3) some</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/828007','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/828007"><span>Measurement of Tensor Analyzing Powers for Elastic Electron Scattering from a Polarized 2H Target Internal to a <span class="hlt">Storage</span> <span class="hlt">Ring</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>M. Ferro-Luzzi; M. Bouwhuis; E. Passchier</p> <p>1996-09-23</p> <p>We report an absolute measurement of the tensor analyzing powers T20 and T22 in elastic electron-deuteron scattering at a momentum transfer of 1.6 fm{sup -1}. The novel approach of this measurement is the use of a tensor polarized 2H target internal to an electron <span class="hlt">storage</span> <span class="hlt">ring</span>, with in situ measurement of the polarization of the target gas. Scattered electrons and recoil deuterons were detected in coincidence with two large acceptance nonmagnetic detectors. The techniques demonstrated have broad applicability to further measurements of spin-dependent electron scattering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/55934','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/55934"><span>Paleo-<span class="hlt">event</span> data standards for dendrochronology</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Elaine Kennedy Sutherland; P. Brewer; W. Gross</p> <p>2017-01-01</p> <p>Extreme environmental <span class="hlt">events</span>, such as storm winds, landslides, insect infestations, and wildfire, cause loss of life, resources, and human infrastructure. Disaster riskreduction analysis can be improved with information about past frequency, intensity, and spatial patterns of extreme <span class="hlt">events</span>. Tree-<span class="hlt">ring</span> analyses can provide such information: tree <span class="hlt">rings</span> reflect <span class="hlt">events</span> as...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/35841','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/35841"><span>Basic tree-<span class="hlt">ring</span> sample preparation techniques for aging aspen</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Lance A. Asherin; Stephen A. Mata</p> <p>2001-01-01</p> <p>Aspen is notoriously difficult to age because of its light-colored wood and faint annual growth <span class="hlt">rings</span>. Careful preparation and processing of aspen <span class="hlt">ring</span> samples can overcome these problems, yield accurate age and growth estimates, and concisely date disturbance <span class="hlt">events</span> present in the tree-<span class="hlt">ring</span> record. Proper collection of aspen wood is essential in obtaining usable <span class="hlt">ring</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996DPS....28.1805B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996DPS....28.1805B"><span>Low Optical Depth Features in Saturn's <span class="hlt">Rings</span>: The Occultation of GSC5249-01240 by Saturn and Its <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bosh, A. S.; Olkin, C. B.</p> <p>1996-06-01</p> <p>On 21 November 1995, Saturn and its <span class="hlt">rings</span> occulted the star GSC5249-01240 (Bosh & McDonald 1992, Astron. J. 103, 983). Although the star is relatively faint (V = 11.9), other circumstances conspired to make this an excellent <span class="hlt">event</span>: (i) the normally-bright <span class="hlt">rings</span> were dark because the sun was crossing through the <span class="hlt">ring</span> plane, reducing the amount of <span class="hlt">ring</span> contribution to the background noise and therefore increasing the observed S/N, (ii) the <span class="hlt">ring</span> opening angle was small (B ~ 3deg ), enhancing detection of low-optical-depth material, and (iii) the low sky-plane velocity allowed longer integration times without loss of spatial resolution. Thus this occultation was particularly well-suited to produce high S/N detections of low-tau <span class="hlt">ring</span> material. We observed this atmosphere and <span class="hlt">ring</span> occultation with the Faint Object Spectrograph (FOS) on the Hubble Space Telescope. Using the FOS in its high-speed mode, we sampled the starlight with the G650L grating, recording the stellar signal as a function of both wavelength and time. For the initial analysis of these data, the spectral information was sacrificed by binning all wavelengths together; this in turn increased the detected S/N. We performed a geometric solution for the <span class="hlt">event</span>, using the known locations of circular <span class="hlt">ring</span> features as fiducials (Elliot et al., Astron. J. 106, 2544). The scattered light from Saturn and the <span class="hlt">rings</span> was modelled and subtracted from the light curves to obtain line-of-sight optical depth as a function of <span class="hlt">ring</span>-plane radius. With these processed data we have made the first occultation detection of Saturn's innermost and very tenuous D <span class="hlt">ring</span>. We find a line-of-sight optical depth for the thickest part of this <span class="hlt">ring</span> of tau_ {obs} ~ 0.02. The location and morphology of this feature will be discussed. Comparison of the observed structure will be made with the previous Voyager imaging detection of this <span class="hlt">ring</span> (Smith et al. 1981, Science 212, 163; Marley & Porco 1993, Icarus 106, 508).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995hst..prop.5782B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995hst..prop.5782B"><span>Saturn <span class="hlt">Ring</span>-Plane Crossing, may 1995</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bosh, Amanda</p> <p>1995-07-01</p> <p>In 1995-1996, the Earth and the Sun will pass through Saturn's <span class="hlt">ring</span> plane. The Earth will pass through 3 times (22 May 1995, 10 August 1995, 11 Feb 1996), and the Sun will pass through once (19 November 1995). All but the 11 Feb 1996 <span class="hlt">event</span> will be visible from HST. During the crossings of the Earth through Saturn's <span class="hlt">ring</span> plane, the <span class="hlt">rings</span> will become very thin and dark. By monitoring the brightness of the <span class="hlt">rings</span> as they become very thin, we will be able to determine the time of <span class="hlt">ring</span>-plane crossing and the residual brightness of the <span class="hlt">rings</span> at this time. The time of the <span class="hlt">ring</span>- plane crossing will place additional constraints on the precession rate of Saturn's pole. The recent occultations by Saturn's <span class="hlt">rings</span> have produced a measurement of this value, but it is not known very well (French et al., 1993; Bosh, 1994; Elliot et al., 1993). A measure of the brightness of the <span class="hlt">rings</span> in their edge-on configuration, combined with photometric properties of the <span class="hlt">rings</span> derived from early calibration observations will allow us to determine the thickness of the <span class="hlt">rings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1221892','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1221892"><span>Capture, acceleration and bunching rf systems for the MEIC booster and <span class="hlt">storage</span> <span class="hlt">rings</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>Wang, Shaoheng; Guo, Jiquan; Lin, Fanglei</p> <p>2015-09-01</p> <p>The Medium-energy Electron Ion Collider (MEIC), proposed by Jefferson Lab, consists of a series of accelerators. The electron collider <span class="hlt">ring</span> accepts electrons from CEBAF at energies from 3 to 12 GeV. Protons and ions are delivered to a booster and captured in a long bunch before being ramped and transferred to the ion collider <span class="hlt">ring</span>. The ion collider <span class="hlt">ring</span> accelerates a small number of long ion bunches to colliding energy before they are re-bunched into a high frequency train of very short bunches for colliding. Two sets of low frequency RF systems are needed for the long ion bunch energymore » ramping in the booster and ion collider <span class="hlt">ring</span>. Another two sets of high frequency RF cavities are needed for re-bunching in the ion collider <span class="hlt">ring</span> and compensating synchrotron radiation energy loss in the electron collider <span class="hlt">ring</span>. The requirements from energy ramping, ion beam bunching, electron beam energy compensation, collective effects, beam loading and feedback capability, RF power capability, etc. are presented. The preliminary designs of these RF systems are presented. Concepts for the baseline cavity and RF station configurations are described, as well as some options that may allow more flexible injection and acceleration schemes.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780016665','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780016665"><span>Energy <span class="hlt">storage</span> apparatus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Studer, P. A.; Evans, H. E. (Inventor)</p> <p>1978-01-01</p> <p>A high efficiency, flywheel type energy <span class="hlt">storage</span> device which comprises an electronically commutated d.c. motor/generator unit having a massive flywheel rotor magnetically suspended around a <span class="hlt">ring</span> shaped stator is presented. During periods of low energy demand, the <span class="hlt">storage</span> devices were operated as a motor, and the flywheel motor was brought up to operating speed. Energy was drawn from the device functioning as a generator as the flywheel rotor rotated during high energy demand periods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4042S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4042S"><span>An <span class="hlt">event</span> database for rotational seismology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salvermoser, Johannes; Hadziioannou, Celine; Hable, Sarah; Chow, Bryant; Krischer, Lion; Wassermann, Joachim; Igel, Heiner</p> <p>2016-04-01</p> <p>The <span class="hlt">ring</span> laser sensor (G-<span class="hlt">ring</span>) located at Wettzell, Germany, routinely observes earthquake-induced rotational ground motions around a vertical axis since its installation in 2003. Here we present results from a recently installed <span class="hlt">event</span> database which is the first that will provide <span class="hlt">ring</span> laser <span class="hlt">event</span> data in an open access format. Based on the GCMT <span class="hlt">event</span> catalogue and some search criteria, seismograms from the <span class="hlt">ring</span> laser and the collocated broadband seismometer are extracted and processed. The ObsPy-based processing scheme generates plots showing waveform fits between rotation rate and transverse acceleration and extracts characteristic wavefield parameters such as peak ground motions, noise levels, Love wave phase velocities and waveform coherence. For each <span class="hlt">event</span>, these parameters are stored in a text file (json dictionary) which is easily readable and accessible on the website. The database contains >10000 <span class="hlt">events</span> starting in 2007 (Mw>4.5). It is updated daily and therefore provides recent <span class="hlt">events</span> at a time lag of max. 24 hours. The user interface allows to filter <span class="hlt">events</span> for epoch, magnitude, and source area, whereupon the <span class="hlt">events</span> are displayed on a zoomable world map. We investigate how well the rotational motions are compatible with the expectations from the surface wave magnitude scale. In addition, the website offers some python source code examples for downloading and processing the openly accessible waveforms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17157101','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17157101"><span>Efficacy, acceptability and tolerability of the combined contraceptive <span class="hlt">ring</span>, Nuva<span class="hlt">Ring</span>, compared with an oral contraceptive containing 30 microg of ethinyl estradiol and 3 mg of drospirenone.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ahrendt, Hans-Joachim; Nisand, Israel; Bastianelli, Carlo; Gómez, Maria Angeles; Gemzell-Danielsson, Kristina; Urdl, Wolfgang; Karskov, Birgit; Oeyen, Luc; Bitzer, Johannes; Page, Geert; Milsom, Ian</p> <p>2006-12-01</p> <p>This randomized multicenter, open-label, trial compared efficacy, acceptability, tolerability and compliance of Nuva<span class="hlt">Ring</span> with a combined oral contraceptive (COC), containing 30 microg of ethinyl estradiol (EE) and 3 mg of drospirenone. In this 13-cycle study, 983 women were randomized and treated (intent-to-treat population) with Nuva<span class="hlt">Ring</span> or COC. One in-treatment pregnancy occurred with Nuva<span class="hlt">Ring</span> (Pearl Index=0.25) (95% confidence interval [CI]: 0.006, 1.363) and four with the COC (Pearl Index=0.99) (95% CI: 0.269, 2.530). For both groups, compliance (89.2% Nuva<span class="hlt">Ring</span>, 85.5% COC) and satisfaction (84% Nuva<span class="hlt">Ring</span>; 87% COC) were high; the vast majority of women found Nuva<span class="hlt">Ring</span> easy to insert (96%) and remove (97%). Tolerability was similar; the most frequent adverse <span class="hlt">events</span> with Nuva<span class="hlt">Ring</span> were related to <span class="hlt">ring</span> use, whereas estrogen-related <span class="hlt">events</span> were more common with the COC. Nuva<span class="hlt">Ring</span> has comparable efficacy and tolerability to a COC containing 30 microg of EE and 3 mg drospirenone. User acceptability of both methods was high.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Icar..279..155H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Icar..279..155H"><span>A new pattern in Saturn's D <span class="hlt">ring</span> created in late 2011</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hedman, M. M.; Showalter, M. R.</p> <p>2016-11-01</p> <p>Images obtained by the Cassini spacecraft between 2012 and 2015 reveal a periodic brightness variation in a region of Saturn's D <span class="hlt">ring</span> that previously appeared to be rather featureless. Furthermore, the intensity and radial wavenumber of this pattern have decreased steadily with time since it was first observed. Based on analogies with similar structures elsewhere in the D <span class="hlt">ring</span>, we propose that this structure was created by some <span class="hlt">event</span> that disturbed the orbital motions of the <span class="hlt">ring</span> particles, giving them finite orbital eccentricities and initially aligned pericenters. Differential orbital precession then transformed this structure into a spiral pattern in the <span class="hlt">ring</span>'s optical depth that became increasingly tightly wound over time. The observed trends in the pattern's radial wavenumber are roughly consistent with this basic model, and also indicate that the <span class="hlt">ring</span>-disturbing <span class="hlt">event</span> occurred in early December 2011. Similar <span class="hlt">events</span> in 1979 may have generated the periodic patterns seen in this same region by the Voyager spacecraft. The 2011 <span class="hlt">event</span> could have been caused by debris striking the <span class="hlt">rings</span>, or by a disturbance in the planet's electromagnetic environment. The rapid reduction in the intensity of the brightness variations over the course of just a few years indicates that some process is either damping orbital eccentricities in this region or causing the orbital pericenters of particles with the same semi-major axis to become misaligned.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/38048','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/38048"><span>Maximizing carbon <span class="hlt">storage</span> in the Appalachians: A method for considering the risk of disturbance <span class="hlt">events</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Michael R. Vanderberg; Kevin Boston; John Bailey</p> <p>2011-01-01</p> <p>Accounting for the probability of loss due to disturbance <span class="hlt">events</span> can influence the prediction of carbon flux over a planning horizon, and can affect the determination of optimal silvicultural regimes to maximize terrestrial carbon <span class="hlt">storage</span>. A preliminary model that includes forest disturbance-related carbon loss was developed to maximize expected values of carbon stocks...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/544688','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/544688"><span>Initial application of a dual-sweep streak camera to the Duke <span class="hlt">storage</span> <span class="hlt">ring</span> OK-4 source</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>Lumpkin, A.H.; Yang, B.X.; Litvinenko, V.</p> <p>1997-08-01</p> <p>The visible and UV spontaneous emission radiation (SER) from the Duke OK-4 wiggler has been used with a Hamamatsu C5680 dual-sweep streak camera to characterize the stored electron beams. Particle beam energies of 270 and 500 MeV in the Duke <span class="hlt">storage</span> <span class="hlt">ring</span> were used in this initial application with the OK-4 adjusted to generate wavelengths from 500 nm to near 200 nm. The OK-4 magnetic system with its 68 periods provided a much stronger radiation source than a nearby bending magnet source point. Sensitivity to single-bunch, single-turn SER was shown down to 4 {mu}A beam current at {lambda} = 450more » nm. The capability of seeing second passes in the FEL resonator at a wavelength near 200 nm was used to assess the cavity length versus orbit length. These tests (besides supporting preparation for UV-visible SR FEL startups) are also relevant to possible diagnostics techniques for single-pass FEL prototype facilities.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/796102','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/796102"><span>In-situ calibration: migrating control system IP module calibration from the bench to the <span class="hlt">storage</span> <span class="hlt">ring</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>Weber, Jonah M.; Chin, Michael</p> <p>2002-04-30</p> <p>The Control System for the Advanced Light Source (ALS) at Lawrence Berkeley National Lab (LBNL) uses in-house designed IndustryPack(registered trademark) (IP) modules contained in compact PCI (cPCI) crates with 16-bit analog I/O to control instrumentation. To make the IP modules interchangeable, each module is calibrated for gain and offset compensation. We initially developed a method of verifying and calibrating the IP modules in a lab bench test environment using a PC with LabVIEW. The subsequent discovery that the ADCs have significant drift characteristics over periods of days of installed operation prompted development of an ''in-situ'' calibration process--one in which themore » IP modules can be calibrated without removing them from the cPCI crates in the <span class="hlt">storage</span> <span class="hlt">ring</span>. This paper discusses the original LabVIEW PC calibration and the migration to the proposed in-situ EPICS control system calibration.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001NIMPA.467..190B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001NIMPA.467..190B"><span>Magnetic measurements of the 10 T superconducting wiggler for the SPring-8 <span class="hlt">storage</span> <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Batrakov, A.; Borovikov, V.; Bekhtenev, E.; Fedurin, M.; Hara, M.; Karpov, G.; Kuzin, M.; Mezentsev, N.; Miahara, Y.; Shimada, T.; Shkaruba, V.; Soutome, K.; Tzumaki, K.</p> <p>2001-07-01</p> <p>In 1999, in the frame of the project ISTC #767 "Budker INP/RIKEN Slow Positron Source", the Budker Institute of Nuclear Physics had made a 10 T Three-pole Superconducting Wiggler. The wiggler will be the keystone of this project by its installation on the SPring-8 <span class="hlt">storage</span> <span class="hlt">ring</span> for powerful gamma ray generation ( λ c=450 keV ), that will be used for slow positron production ( Nγ( ɛ>1 MeV)˜10 15, γ/s I e=0.1 A ). A. Ando et al., Proposal of the high magnetic field super conducting WLS for slow positron source at SPring-8, presented at SR1 '97 Conference. In January, 2000, the wiggler was transported to SPring-8, where the last test and measurements were carried out in collaboration with Japan. In this article, the results of measurements of the magnetic field, finding the magnetic field amplitude by an NMR probe, the definition of feed current relations by stretch current wire method, the calibration of a Hall probe in the high magnetic field, and the measurement of the magnetic field profile by a Hall probe are presented.</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('http://adsabs.harvard.edu/abs/2012PhRvS..15k2802K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PhRvS..15k2802K"><span>Independent component analysis applied to long bunch beams in the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kolski, Jeffrey S.; Macek, Robert J.; McCrady, Rodney C.; Pang, Xiaoying</p> <p>2012-11-01</p> <p>Independent component analysis (ICA) is a powerful blind source separation (BSS) method. Compared to the typical BSS method, principal component analysis, ICA is more robust to noise, coupling, and nonlinearity. The conventional ICA application to turn-by-turn position data from multiple beam position monitors (BPMs) yields information about cross-BPM correlations. With this scheme, multi-BPM ICA has been used to measure the transverse betatron phase and amplitude functions, dispersion function, linear coupling, sextupole strength, and nonlinear beam dynamics. We apply ICA in a new way to slices along the bunch revealing correlations of particle motion within the beam bunch. We digitize beam signals of the long bunch at the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> with a single device (BPM or fast current monitor) for an entire injection-extraction cycle. ICA of the digitized beam signals results in source signals, which we identify to describe varying betatron motion along the bunch, locations of transverse resonances along the bunch, measurement noise, characteristic frequencies of the digitizing oscilloscopes, and longitudinal beam structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26953596','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26953596"><span>Suppressing the Coffee-<span class="hlt">Ring</span> Effect in Semitransparent MnO2 Film for a High-Performance Solar-Powered Energy <span class="hlt">Storage</span> Window.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jin, Huanyu; Qian, Jiasheng; Zhou, Limin; Yuan, Jikang; Huang, Haitao; Wang, Yu; Tang, Wing Man; Chan, Helen Lai Wa</p> <p>2016-04-13</p> <p>We introduce a simple and effective method to deposit a highly uniform and semitransparent MnO2 film without coffee-<span class="hlt">ring</span> effect (CRE) by adding ethanol into MnO2 ink for transparent capacitive energy <span class="hlt">storage</span> devices. By carefully controlling the amount of ethanol added in the MnO2 droplet, we could significantly reduce the CRE and thus improve the film uniformity. The electrochemical properties of supercapacitor (SC) devices using semitransparent MnO2 film electrodes with or without CRE were measured and compared. The SC device without CRE shows a superior capacitance, high rate capability, and lower contact resistance. The CRE-free device could achieve a considerable volumetric capacitance of 112.2 F cm(-3), resulting in a high volumetric energy density and power density of 10 mWh cm(-3) and 8.6 W cm(-3), respectively. For practical consideration, both flexible SC and large-area rigid SC devices were fabricated to demonstrate their potential for flexible transparent electronic application and capacitive energy-<span class="hlt">storage</span> window application. Moreover, a solar-powered energy <span class="hlt">storage</span> window which consists of a commercial solar cell and our studied semitransparent MnO2-film-based SCs was assembled. These SCs could be charged by the solar cell and light up a light emitting diode (LED), demonstrating their potential for self-powered systems and energy-efficient buildings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRA..12212055T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRA..12212055T"><span><span class="hlt">Ring</span>/Shell Ion Distributions at Geosynchronous Orbit</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thomsen, M. F.; Denton, M. H.; Gary, S. P.; Liu, Kaijun; Min, Kyungguk</p> <p>2017-12-01</p> <p>One year's worth of plasma observations from geosynchronous orbit is examined for ion distributions that may simultaneously be subject to the ion Bernstein (IB) instability (generating fast magnetosonic waves) and the Alfvén cyclotron (AC) instability (generating electromagnetic ion cyclotron waves). Confirming past analyses, distributions with robust ∂fp(v⊥)/∂v⊥ > 0 near v|| = 0, which we denote as "<span class="hlt">ring</span>/shell" distributions, are commonly found primarily on the dayside of the magnetosphere. A new approach to high-fidelity representation of the observed <span class="hlt">ring</span>/shell distribution functions in a form readily suited to both analytical moment calculation and linear dispersion analysis is presented, which allows statistical analysis of the <span class="hlt">ring</span>/shell properties. The <span class="hlt">ring</span>/shell temperature anisotropy is found to have a clear upper limit that depends on the parallel beta of the <span class="hlt">ring</span>/shell (β||r) in a manner that is diagnostic of the operation of the AC instability. This upper limit is only reached in the postnoon <span class="hlt">events</span>, which are primarily produced by the energy- and pitch angle-dependent magnetic drifts of substorm-injected ions. Further, it is primarily the leading edge of such injections, where the distribution is strongly <span class="hlt">ring</span>-like, that the AC instability appears to be operating. By contrast, the ratio of the <span class="hlt">ring</span> energy to the Alfvén energy remains well within the range of 0.25-4.0 suitable for IB instability throughout essentially all of the <span class="hlt">events</span>, except those that occur in denser cold plasma of the outer plasmasphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/385734-measurement-tensor-analyzing-powers-elastic-electron-scattering-from-polarized-sup-target-internal-storage-ring','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/385734-measurement-tensor-analyzing-powers-elastic-electron-scattering-from-polarized-sup-target-internal-storage-ring"><span>Measurement of Tensor Analyzing Powers for Elastic Electron Scattering from a Polarized {sup 2}H Target Internal to a <span class="hlt">Storage</span> <span class="hlt">Ring</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>Ferro-Luzzi, M.; Bouwhuis, M.; Passchier, E.</p> <p>1996-09-01</p> <p>We report an absolute measurement of the tensor analyzing powers {ital T}{sub 20} and {ital T}{sub 22} in elastic electron-deuteron scattering at a momentum transfer of 1.6 fm{sup {minus}1}. The novel approach of this measurement is the use of a tensor polarized {sup 2}H target internal to an electron <span class="hlt">storage</span> <span class="hlt">ring</span>, with {ital in} {ital situ} measurement of the polarization of the target gas. Scattered electrons and recoil deuterons were detected in coincidence with two large acceptance nonmagnetic detectors. The techniques demonstrated have broad applicability to further measurements of spin-dependent electron scattering. {copyright} {ital 1996 The American Physical Society.}</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhRvS..18g4004T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhRvS..18g4004T"><span>Electric dipole moment planning with a resurrected BNL Alternating Gradient Synchrotron electron analog <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Talman, Richard M.; Talman, John D.</p> <p>2015-07-01</p> <p>There has been much recent interest in directly measuring the electric dipole moments (EDM) of the proton and the electron, because of their possible importance in the present day observed matter/antimatter imbalance in the Universe. Such a measurement will require storing a polarized beam of "frozen spin" particles, 15 MeV electrons or 230 MeV protons, in an all-electric <span class="hlt">storage</span> <span class="hlt">ring</span>. Only one such relativistic electric accelerator has ever been built—the 10 MeV "electron analog" <span class="hlt">ring</span> at Brookhaven National Laboratory in 1954; it can also be referred to as the "AGS analog" <span class="hlt">ring</span> to make clear it was a prototype for the Alternating Gradient Synchrotron (AGS) proton <span class="hlt">ring</span> under construction at that time at BNL. (Its purpose was to investigate nonlinear resonances as well as passage through "transition" with the newly invented alternating gradient proton <span class="hlt">ring</span> design.) By chance this electron <span class="hlt">ring</span>, long since dismantled and its engineering drawings disappeared, would have been appropriate both for measuring the electron EDM and to serve as an inexpensive prototype for the arguably more promising, but 10 times more expensive, proton EDM measurement. Today it is cheaper yet to "resurrect" the electron analog <span class="hlt">ring</span> by simulating its performance computationally. This is one purpose for the present paper. Most existing accelerator simulation codes cannot be used for this purpose because they implicitly assume magnetic bending. The new ual/eteapot code, described in detail in an accompanying paper, has been developed for modeling <span class="hlt">storage</span> <span class="hlt">ring</span> performance, including spin evolution, in electric <span class="hlt">rings</span>. Illustrating its use, comparing its predictions with the old observations, and describing new expectations concerning spin evolution and code performance, are other goals of the paper. To set up some of these calculations has required a kind of "archeological physics" to reconstitute the detailed electron analog lattice design from a 1991 retrospective report by Plotkin as well</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5937717','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5937717"><span>Report of the New <span class="hlt">Rings</span> Study Group</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>Holmes, S.D.; Dugan, G.; Marriner, J.</p> <p>1987-10-19</p> <p>We have taken the approach here of trying to understand both the feasibility and practicality of varied options for new <span class="hlt">rings</span> at Fermilab, rather than trying to produce a single detailed design. In other words, this document is not a design report and should not be construed as such. Our perception of the potential needs for new <span class="hlt">rings</span> (in order of priority) is as follows: Antiproton <span class="hlt">Storage</span> and/or Recovery: A facility for storing up to 4 x 10/sup 12/ antiprotons is needed. Recovery of antiprotons from the collider becomes a viable option if the luminosity is indeed dominated by emittancemore » dilution rather than beam loss. New or Post-Booster: The goal here would be to inject into the existing Main <span class="hlt">Ring</span> above transition. Improved performance of the Main <span class="hlt">Ring</span> would be anticipated. New Main <span class="hlt">Ring</span>: Advantages would include better emittance preservation, a faster cycle time for antiproton production, and the removal of interference/backgrounds at the B0 and D0 detectors. We discuss in this paper various scenarios based on one or more combinations of the above possibilities. 14 figs., 10 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4606055','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4606055"><span>Capturing spiral radial growth of conifers using the superellipse to model tree-<span class="hlt">ring</span> geometric shape</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Shi, Pei-Jian; Huang, Jian-Guo; Hui, Cang; Grissino-Mayer, Henri D.; Tardif, Jacques C.; Zhai, Li-Hong; Wang, Fu-Sheng; Li, Bai-Lian</p> <p>2015-01-01</p> <p>Tree-<span class="hlt">rings</span> are often assumed to approximate a circular shape when estimating forest productivity and carbon dynamics. However, tree <span class="hlt">rings</span> are rarely, if ever, circular, thereby possibly resulting in under- or over-estimation in forest productivity and carbon sequestration. Given the crucial role played by tree <span class="hlt">ring</span> data in assessing forest productivity and carbon <span class="hlt">storage</span> within a context of global change, it is particularly important that mathematical models adequately render cross-sectional area increment derived from tree <span class="hlt">rings</span>. We modeled the geometric shape of tree <span class="hlt">rings</span> using the superellipse equation and checked its validation based on the theoretical simulation and six actual cross sections collected from three conifers. We found that the superellipse better describes the geometric shape of tree <span class="hlt">rings</span> than the circle commonly used. We showed that a spiral growth trend exists on the radial section over time, which might be closely related to spiral grain along the longitudinal axis. The superellipse generally had higher accuracy than the circle in predicting the basal area increment, resulting in an improved estimate for the basal area. The superellipse may allow better assessing forest productivity and carbon <span class="hlt">storage</span> in terrestrial forest ecosystems. PMID:26528316</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26528316','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26528316"><span>Capturing spiral radial growth of conifers using the superellipse to model tree-<span class="hlt">ring</span> geometric shape.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shi, Pei-Jian; Huang, Jian-Guo; Hui, Cang; Grissino-Mayer, Henri D; Tardif, Jacques C; Zhai, Li-Hong; Wang, Fu-Sheng; Li, Bai-Lian</p> <p>2015-01-01</p> <p>Tree-<span class="hlt">rings</span> are often assumed to approximate a circular shape when estimating forest productivity and carbon dynamics. However, tree <span class="hlt">rings</span> are rarely, if ever, circular, thereby possibly resulting in under- or over-estimation in forest productivity and carbon sequestration. Given the crucial role played by tree <span class="hlt">ring</span> data in assessing forest productivity and carbon <span class="hlt">storage</span> within a context of global change, it is particularly important that mathematical models adequately render cross-sectional area increment derived from tree <span class="hlt">rings</span>. We modeled the geometric shape of tree <span class="hlt">rings</span> using the superellipse equation and checked its validation based on the theoretical simulation and six actual cross sections collected from three conifers. We found that the superellipse better describes the geometric shape of tree <span class="hlt">rings</span> than the circle commonly used. We showed that a spiral growth trend exists on the radial section over time, which might be closely related to spiral grain along the longitudinal axis. The superellipse generally had higher accuracy than the circle in predicting the basal area increment, resulting in an improved estimate for the basal area. The superellipse may allow better assessing forest productivity and carbon <span class="hlt">storage</span> in terrestrial forest ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007MNRAS.380L..54W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007MNRAS.380L..54W"><span>Moonlets wandering on a leash-<span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winter, O. C.; Mourão, D. C.; Giuliatti Winter, S. M.; Spahn, F.; da Cruz, C.</p> <p>2007-09-01</p> <p>Since the Voyager flybys, embedded moonlets have been proposed to explain some of the surprising structures observed in Saturn's narrow F <span class="hlt">ring</span>. Experiments conducted with the Cassini spacecraft support this suggestion. Images of the F <span class="hlt">ring</span> show bright compact spots, and seven occultations of stars by the F <span class="hlt">ring</span>, monitored by ultraviolet and infrared experiments, revealed nine <span class="hlt">events</span> of high optical depth. These results point to a large number of such objects, but it is not clear whether they are solid moonlets or rather loose particle aggregates. Subsequent images suggested an irregular motion of these objects so that a determination of their orbits consistent with the F <span class="hlt">ring</span> failed. Some of these features seem to cross the whole <span class="hlt">ring</span>. Here we show that these observations are explained by chaos in the F <span class="hlt">ring</span> driven mainly by the `shepherd' moons Prometheus and Pandora. It is characterized by a rather short Lyapunov time of about a few hundred orbital periods. Despite this chaotic diffusion, more than 93 per cent of the F-<span class="hlt">ring</span> bodies remain confined within the F <span class="hlt">ring</span> because of the shepherding, but also because of a weak radial mobility contrasted by an effective longitudinal diffusion. This chaotic stirring of all bodies involved prevents the formation of `propellers' typical of moonlets, but their frequent <span class="hlt">ring</span> crossings explain the multiple radial `streaks' seen in the F <span class="hlt">ring</span>. The related `thermal' motion causes more frequent collisions between all bodies which steadily replenish F-<span class="hlt">ring</span> dust and allow for ongoing fragmentation and re-accretion processes (<span class="hlt">ring</span> recycling).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820028173&hterms=energy+baseline&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Denergy%2Bbaseline','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820028173&hterms=energy+baseline&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Denergy%2Bbaseline"><span>In-space inertial energy <span class="hlt">storage</span> design</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Studer, P. A.; Evans, H. E.</p> <p>1981-01-01</p> <p>Flywheel energy <span class="hlt">storage</span> is a means of significantly improving the performance of space power systems. Two study contracts have been completed to investigate the merits of a magnetically suspended, ironless armature, <span class="hlt">ring</span> rotor 'Mechanical Capacitor' design. The design of a suitable energy <span class="hlt">storage</span> system is evaluated, taking into account baseline requirements, the motor generator, details regarding the suspension design, power conditioning, the rotor, and an example design. It appears on the basis of this evaluation that the inertial (flywheel) energy <span class="hlt">storage</span> design is feasible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4151682','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4151682"><span>Prospects of high-resolution resonant X-ray inelastic scattering studies on solid materials, liquids and gases at diffraction-limited <span class="hlt">storage</span> <span class="hlt">rings</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>Schmitt, Thorsten; de Groot, Frank M. F.; Rubensson, Jan-Erik</p> <p>2014-01-01</p> <p>The spectroscopic technique of resonant inelastic X-ray scattering (RIXS) will particularly profit from immensely improved brilliance of diffraction-limited <span class="hlt">storage</span> <span class="hlt">rings</span> (DLSRs). In RIXS one measures the intensities of excitations as a function of energy and momentum transfer. DLSRs will allow for pushing the achievable energy resolution, signal intensity and the sampled spot size to new limits. With RIXS one nowadays probes a broad range of electronic systems reaching from simple molecules to complex materials displaying phenomena like peculiar magnetism, two-dimensional electron gases, superconductivity, photovoltaic energy conversion and heterogeneous catalysis. In this article the types of improved RIXS studies that will become possible with X-ray beams from DLSRs are envisioned. PMID:25177995</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25177995','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25177995"><span>Prospects of high-resolution resonant X-ray inelastic scattering studies on solid materials, liquids and gases at diffraction-limited <span class="hlt">storage</span> <span class="hlt">rings</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schmitt, Thorsten; de Groot, Frank M F; Rubensson, Jan Erik</p> <p>2014-09-01</p> <p>The spectroscopic technique of resonant inelastic X-ray scattering (RIXS) will particularly profit from immensely improved brilliance of diffraction-limited <span class="hlt">storage</span> <span class="hlt">rings</span> (DLSRs). In RIXS one measures the intensities of excitations as a function of energy and momentum transfer. DLSRs will allow for pushing the achievable energy resolution, signal intensity and the sampled spot size to new limits. With RIXS one nowadays probes a broad range of electronic systems reaching from simple molecules to complex materials displaying phenomena like peculiar magnetism, two-dimensional electron gases, superconductivity, photovoltaic energy conversion and heterogeneous catalysis. In this article the types of improved RIXS studies that will become possible with X-ray beams from DLSRs are envisioned.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1392573-measurement-two-photon-exchange-contribution-elastic-ep-scattering-cross-sections-vepp-storage-ring','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1392573-measurement-two-photon-exchange-contribution-elastic-ep-scattering-cross-sections-vepp-storage-ring"><span>Measurement of the Two-Photon Exchange Contribution to the Elastic e ± p Scattering Cross Sections at the VEPP-3 <span class="hlt">Storage</span> <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Rachek, I. A.; Arrington, J.; Dmitriev, V. F.; ...</p> <p>2015-02-12</p> <p>The ratio of the elastic e +p to e –p scattering cross sections has been measured precisely, allowing the determination of the two-photon exchange contribution to these processes. This neglected contribution is believed to be the cause of the discrepancy between the Rosenbluth and polarization transfer methods of measuring the proton electromagnetic form factors. The experiment was performed at the VEPP-3 <span class="hlt">storage</span> <span class="hlt">ring</span> at beam energies of 1.6 and 1.0 GeV and at lepton scattering angles between 15° and 105°. The data obtained show evidence of a significant two-photon exchange effect. Furthermore, the results are compared with several theoretical predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1394797-fodo-racetrack-ring-nustorm-design-optimization','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1394797-fodo-racetrack-ring-nustorm-design-optimization"><span>A FODO racetrack <span class="hlt">ring</span> for nuSTORM: design and optimization</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Liu, A.; Bross, A.; Neuffer, D.</p> <p>2017-07-17</p> <p>Here, the goal of nuSTORM is to provide well-defined neutrino beams for precise measurements of neutrino cross-sections and oscillations. The nuSTORM decay <span class="hlt">ring</span> is a compact racetrack <span class="hlt">storage</span> <span class="hlt">ring</span> with a circumference of ~ 480 m that incorporates large aperture (60 cm diameter) magnets. There are many challenges in the design. In order to incorporate the Orbit Combination section (OCS), used for injecting the pion beam into the <span class="hlt">ring</span>, a dispersion suppressor is needed adjacent to the OCS . Concurrently, in order to maximize the number of useful muon decays, strong bending dipoles are needed in the arcs to minimize themore » arc length. These dipoles create strong chromatic effects, which need to be corrected by nonlinear sextupole elements in the <span class="hlt">ring</span>. In this paper, a FODO racetrack <span class="hlt">ring</span> design and its optimization using sextupolar fields via both a Genetic Algorithm (GA) and a Simulated Annealing (SA) algorithm will be discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1394797','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1394797"><span>A FODO racetrack <span class="hlt">ring</span> for nuSTORM: design and optimization</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>Liu, A.; Bross, A.; Neuffer, D.</p> <p>2017-07-01</p> <p>The goal of nuSTORM is to provide well-defined neutrino beams for precise measurements of neutrino cross-sections and oscillations. The nuSTORM decay <span class="hlt">ring</span> is a compact racetrack <span class="hlt">storage</span> <span class="hlt">ring</span> with a circumference of ~ 480 m that incorporates large aperture (60 cm diameter) magnets. There are many challenges in the design. In order to incorporate the Orbit Combination section (OCS), used for injecting the pion beam into the <span class="hlt">ring</span>, a dispersion suppressor is needed adjacent to the OCS . Concurrently, in order to maximize the number of useful muon decays, strong bending dipoles are needed in the arcs to minimize the arcmore » length. These dipoles create strong chromatic effects, which need to be corrected by nonlinear sextupole elements in the <span class="hlt">ring</span>. In this paper, a FODO racetrack <span class="hlt">ring</span> design and its optimization using sextupolar fields via both a Genetic Algorithm (GA) and a Simulated Annealing (SA) algorithm will be discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23125701N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23125701N"><span>On Stellar Flash Echoes from Circular <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nemiroff, Robert; Mukherjee, Oindabi</p> <p>2018-01-01</p> <p>A flash -- or any episode of variability -- that occurs in the vicinity of a circular <span class="hlt">ring</span> might be seen several times later, simultaneously, as echoes on the <span class="hlt">ring</span>. Effective images of the flash are created and annihilated in pairs, with as many as four flash images visible concurrently. Videos detailing sequences of image pair creation, tandem motion, and subsequent image annihilation are shown, given simple opacity and scattering assumptions. It is proven that, surprisingly, images from a second pair creation <span class="hlt">event</span> always annihilate with images from the first. Caustic surfaces between flash locations yielding two and four images are computed. Although such <span class="hlt">ring</span> echos surely occur, their practical detection might be difficult as it could require dedicated observing programs involving sensitive photometry of extended objects. Potential flash sources include planetary and interstellar gas and dust <span class="hlt">rings</span> near and around variable stars, flare stars, novae, supernovae, and GRBs. Potentially recoverable information includes size, distance, temporal history, and angular isotropy of both the <span class="hlt">ring</span> and flash.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840025252','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840025252"><span>Trapped particle absorption by the <span class="hlt">Ring</span> of Jupiter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fillius, W.</p> <p>1983-01-01</p> <p>The interaction of trapped radiation with the <span class="hlt">ring</span> of Jupiter is investigated. Because it is an identical problem, the <span class="hlt">rings</span> of Saturn and Uranus are also examined. Data from the Pioneer II encounter, deductions for some of the properties of the <span class="hlt">rings</span> of Jupiter and Saturn. Over a dozen Jupiter magnetic field models are available in a program that integrates the adiabatic invariants to compute B and L. This program is to label our UCSD Pioneer II encounter data with the most satisfactory of these models. The expected effects of absorbing material on the trapped radiation are studied to obtain the loss rate as a function of <span class="hlt">ring</span> properties. Analysis of the particle diffusion problem rounds out the theoretical end of the <span class="hlt">ring</span> absorption problem. Other projects include identification of decay products for energetic particle albedo off the <span class="hlt">rings</span> and moons of Saturn and a search for flux transfer <span class="hlt">events</span> at the Jovian magnetopause.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017RaPC..130..359T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017RaPC..130..359T"><span>Sensory acceptability of squid <span class="hlt">rings</span> gamma irradiated for shelf-life extension</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tomac, Alejandra; Cova, María C.; Narvaiz, Patricia; Yeannes, María I.</p> <p>2017-01-01</p> <p>The feasibility of extending the shelf-life of a squid product by gamma irradiation was analyzed. Illex argentinus <span class="hlt">rings</span> were irradiated at 4 and 8 kGy; and stored at 4±1 °C during 77 days. No mesophilic bacteria, enterobacteriaceae and coliforms were detected in irradiated <span class="hlt">rings</span> during <span class="hlt">storage</span>. Psychrotrophic bacteria were significantly reduced by irradiation; their counts were fitted to a growth model which was further used for shelf-life estimations: 3 and 27 days for 0 and 4 kGy, respectively. Initially, non-irradiated as well as irradiated <span class="hlt">rings</span> had very good sensory scores. The overall acceptability of 4 and 8 kGy <span class="hlt">rings</span> did not decrease during 27 and 64 days, respectively, while control samples spoiled after 3 days. A radiation dose range for squid <span class="hlt">rings</span> preservation was defined, which attained the technological shelf-life extension objective, without impairing sensory quality.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.P23B1635H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.P23B1635H"><span>Earth: A <span class="hlt">Ringed</span> Planet?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hancock, L. O.; Povenmire, H.</p> <p>2010-12-01</p> <p>Among the most beautiful findings of the Space Age have been the discoveries of planetary <span class="hlt">rings</span>. Not only Saturn but also Jupiter, Uranus and Neptune have <span class="hlt">rings</span>; Saturn’s <span class="hlt">ring</span> system has structures newly discovered; even Saturn's moon Rhea itself has a <span class="hlt">ring</span>. All these are apparently supplied by material from the planetary moons (Rhea's <span class="hlt">ring</span> by Rhea itself). The question naturally arises, why should the Earth not have a <span class="hlt">ring</span>, and on the other hand, if it does, why has it not been observed? No <span class="hlt">rings</span> have yet been observed in the inner solar system, but after all, <span class="hlt">rings</span> in the inner solar system might simply tend to be fainter and more transient than those of the outer solar system: the inner solar system is more affected by the solar wind, and the Sun’s perturbing gravitational influence is greater. J.A. O’Keefe first suggested (1980) that Earth might have a <span class="hlt">ring</span> system of its own. An Earth <span class="hlt">ring</span> could account for some climate <span class="hlt">events</span>. O’Keefe remarked that formation or thickening of a <span class="hlt">ring</span> system in Earth’s equatorial plane could drive glaciation by deepening the chill of the winter hemisphere. (It is very well established that volcanic dust is an effective agent for the extinction of sunlight; this factor can be overwhelmingly apparent in eclipse observations.) O’Keefe died in 2000 and the speculation was not pursued, but the idea of an Earth <span class="hlt">ring</span> has a prima facie reasonableness that calls for its renewed consideration. The program of this note is to hypothesize that, as O’Keefe proposed: (a) an Earth <span class="hlt">ring</span> system exists; (b) it affects Earth's weather and climate; (c) the tektite strewn fields comprise filaments of the <span class="hlt">ring</span> fallen to Earth's surface on various occasions of disturbance by comets or asteroids. On this basis, and drawing on the world's weather records, together with the Twentieth Century Reanalysis by NCEP/CIRES covering the period 1870-2010 and the geology of the tektite strewn fields, we herein propose the hypothesized Earth <span class="hlt">ring</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26842978','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26842978"><span>Mechanisms Underlying the Active Self-Assembly of Microtubule <span class="hlt">Rings</span> and Spools.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>VanDelinder, Virginia; Brener, Stephanie; Bachand, George D</p> <p>2016-03-14</p> <p>Active self-assembly offers a powerful route for the creation of dynamic multiscale structures that are presently inaccessible with standard microfabrication techniques. One such system uses the translation of microtubule filaments by surface-tethered kinesin to actively assemble nanocomposites with bundle, <span class="hlt">ring</span>, and spool morphologies. Attempts to observe mechanisms involved in this active assembly system have been hampered by experimental difficulties with performing observation during buffer exchange and photodamage from fluorescent excitation. In the present work, we used a custom microfluidic device to remove these limitations and directly study <span class="hlt">ring</span>/spool formation, including the earliest <span class="hlt">events</span> (nucleation) that drive subsequent nanocomposite assembly. Three distinct formation <span class="hlt">events</span> were observed: pinning, collisions, and induced curvature. Of these three, collisions accounted for the majority of <span class="hlt">event</span> leading to <span class="hlt">ring</span>/spool formation, while the rate of pinning was shown to be dependent on the amount of photodamage in the system. We further showed that formation mechanism directly affects the diameter and rotation direction of the resultant <span class="hlt">rings</span> and spools. Overall, the fundamental understanding described in this work provides a foundation by which the properties of motor-driven, actively assembled nanocomposites may be tailored toward specific applications.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1249084-mechanisms-underlying-active-self-assembly-microtubule-rings-spools','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1249084-mechanisms-underlying-active-self-assembly-microtubule-rings-spools"><span>Mechanisms underlying the active self-assembly of microtubule <span class="hlt">rings</span> and spools</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>VanDelinder, Virginia; Brener, Stephanie; Bachand, George D.</p> <p>2016-02-04</p> <p>Here, active self-assembly offers a powerful route for the creation of dynamic multiscale structures that are presently inaccessible with standard microfabrication techniques. One such system uses the translation of microtubule filaments by surface-tethered kinesin to actively assemble nanocomposites with bundle, <span class="hlt">ring</span>, and spool morphologies. Attempts to observe mechanisms involved in this active assembly system have been hampered by experimental difficulties with performing observation during buffer exchange and photodamage from fluorescent excitation. In the present work, we used a custom microfluidic device to remove these limitations and directly study <span class="hlt">ring</span>/spool formation, including the earliest <span class="hlt">events</span> (nucleation) that drive subsequent nanocomposite assembly.more » Three distinct formation <span class="hlt">events</span> were observed: pinning, collisions, and induced curvature. Of these three, collisions accounted for the majority of <span class="hlt">event</span> leading to <span class="hlt">ring</span>/spool formation, while the rate of pinning was shown to be dependent on the amount of photodamage in the system. We further showed that formation mechanism directly affects the diameter and rotation direction of the resultant <span class="hlt">rings</span> and spools. Overall, the fundamental understanding described in this work provides a foundation by which the properties of motor-driven, actively assembled nanocomposites may be tailored toward specific applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70185816','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70185816"><span>Use of tree-<span class="hlt">ring</span> chemistry to document historical ground-water contamination <span class="hlt">events</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>Vroblesky, Don A.; Yanosky, Thomas M.</p> <p>1990-01-01</p> <p>The annual growth <span class="hlt">rings</span> of tulip trees (Liriodendron tulipifera L.) appear to preserve a chemical record of ground-water contamination at a landfill in Maryland. Zones of elevated iron and chlorine concentrations in growth <span class="hlt">rings</span> from trees immediately downgradient from the landfill are closely correlated temporally with activities in the landfill expected to generate iron and chloride contamination in the ground water. Successively later iron peaks in trees increasingly distant from the landfill along the general direction of ground-water flow imply movement of iron-contaminated ground water away from the landfill. The historical velocity of iron movement (2 to 9 m/yr) and chloride movement (at least 40 m/yr) in ground water at the site was estimated from element-concentration trends of trees at successive distances from the landfill. The tree-<span class="hlt">ring</span>-derived chloride-transport velocity approximates the known ground-water velocity (30 to 80 m/yr). A minimum horizontal hydraulic conductivity (0.01 to .02 cm/s) calculated from chloride velocity agrees well with values derived from aquifer tests (about 0.07 cm/s) and from ground-water modeling results (0.009 to 0.04 cm/s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015A%26A...576A..18O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015A%26A...576A..18O"><span>Possible <span class="hlt">ring</span> material around centaur (2060) Chiron</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz, J. L.; Duffard, R.; Pinilla-Alonso, N.; Alvarez-Candal, A.; Santos-Sanz, P.; Morales, N.; Fernández-Valenzuela, E.; Licandro, J.; Campo Bagatin, A.; Thirouin, A.</p> <p>2015-04-01</p> <p>We propose that several short-duration <span class="hlt">events</span> observed in past stellar occultations by Chiron were produced by <span class="hlt">ring</span> material. Some similarities between these <span class="hlt">events</span> and the characteristics of Chariklo's <span class="hlt">rings</span> could indicate common mechanisms around centaurs. From a reanalysis of the stellar occultation data in the literature, we determined two possible orientations of the pole of Chiron's <span class="hlt">rings</span>, with ecliptic coordinates λ = (352 ± 10)°, β = (37 ± 10)° or λ = (144 ± 10)°, β = (24 ± 10)°. The mean radius of the <span class="hlt">rings</span> is (324 ± 10) km. One can use the rotational lightcurve amplitude of Chiron at different epochs to distinguish between the two solutions for the pole. Both solutions imply a lower lightcurve amplitude in 2013 than in 1988, when the rotational lightcurve was first determined. We derived Chiron's rotational lightcurve in 2013 from observations at the 1.23 m CAHA telescope, and indeed its amplitude was smaller than in 1988. We also present a rotational lightcurve in 2000 from images taken at the CASLEO 2.15 m telescope that is consistent with our predictions. Out of the two poles, the λ = (144 ± 10)°, β = (24 ± 10)° solution provides a better match to a compilation of rotational lightcurve amplitudes from the literature and those presented here. We also show that using this preferred pole orientation, Chiron's long-term brightness variations are compatible with a simple model that incorporates the changing brightness of the <span class="hlt">rings</span> while the tilt angle with respect to the Earth is changing with time. Also, the variability of the water ice band in Chiron's spectra as seen in the literature can be explained to a large degree by an icy <span class="hlt">ring</span> system whose tilt angle changes with time and whose composition includes water ice, analogously to the case of Chariklo. We present several possible formation scenarios for the <span class="hlt">rings</span> from qualitative points of view and speculate on why <span class="hlt">rings</span> might be common in centaurs. We also speculate on whether the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.938a2061S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.938a2061S"><span>Manifestations of geometric phases in a proton electric-dipole-moment experiment in an all-electric <span class="hlt">storage</span> <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Silenko, Alexander J.</p> <p>2017-12-01</p> <p>We consider a proton electric-dipole-moment experiment in an all-electric <span class="hlt">storage</span> <span class="hlt">ring</span> when the spin is frozen and local longitudinal and vertical electric fields alternate. In this experiment, the geometric (Berry) phases are very important. Due to the these phases, the spin rotates about the radial axis. The corresponding systematic error is rather important while it can be canceled with clockwise and counterclockwise beams. The geometric phases also lead to the spin rotation about the radial axis. This effect can be canceled with clockwise and counterclockwise beams as well. The sign of the azimuthal component of the angular velocity of the spin precession depends on the starting point where the spin orientation is perfect. The radial component of this quantity keeps its value and sign for each starting point. When the longitudinal and vertical electric fields are joined in the same sections without any alternation, the systematic error due to the geometric phases does not appear but another systematic effect of the spin rotation about the azimuthal axis takes place. It has opposite signs for clockwise and counterclockwise beams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003APS..DFD.DN007P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003APS..DFD.DN007P"><span>Starting buoyant plumes and vortex <span class="hlt">ring</span> pinch-off</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pottebaum, Tait; Gharib, Mory</p> <p>2003-11-01</p> <p>The vortex <span class="hlt">ring</span> formation process of a starting buoyant plume was studied experimentally. Buoyant plumes were produced using a heating element at the base of a water tank. The velocity and temperature fields in the flow were measured using digital particle image thermometry and velocimetry (DPITV), allowing the density and vorticity fields to be determined. The vortex <span class="hlt">ring</span> initially grew, with additional circulation being supplied by the trailing plume. At later times, the vortex <span class="hlt">ring</span> became disconnected from the trailing plume. This is analogous to the pinch-off of a vortex <span class="hlt">ring</span> produced by a piston-cylinder apparatus reported by Gharib et al (1998 JFM 360: 121-140). The existence of a pinch-off process for starting buoyant plumes has many implications for environmental flows. Of particular interest is the effect of vortex <span class="hlt">ring</span> pinch-off on the dispersal of particulates and contaminants in intermittent or sudden convection <span class="hlt">events</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27339759','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27339759"><span>Efficacy and safety of the contraceptive vaginal <span class="hlt">ring</span> (Nuva<span class="hlt">Ring</span>) compared with a combined oral contraceptive in Chinese women: a 1-year randomised trial.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fan, Guang Sheng; Ren, Mulan; Di, Wen; Su, Ping; Chang, Qin; Wu, Shuying; Qin, Yun; Korver, Tjeerd; Marintcheva-Petrova, Maya; Yacik, Carol; McCrary Sisk, Christine; Wang, Guoqin</p> <p>2016-08-01</p> <p>The aim of the study was to assess the efficacy and tolerability of the monthly vaginal <span class="hlt">ring</span> (Nuva<span class="hlt">Ring</span>; 15 μg ethinylestradiol [EE] and 120 μg etonogestrel per day) compared with a monophasic (21/7) combined oral contraceptive (COC) containing 30 μg EE and 3 mg drospirenone in healthy Chinese women aged 18-40 years. This was a phase III, open-label, randomised multicentre trial conducted in China. Participants received Nuva<span class="hlt">Ring</span> or COC for 13 cycles (3 weeks of <span class="hlt">ring</span>/pill treatment followed by a 1-week <span class="hlt">ring</span>-free/pill-free period). Contraceptive efficacy was assessed by in-treatment pregnancies and expressed by the Pearl Index (PI; number of pregnancies/100 woman-years of use). Cycle control was assessed by unscheduled (breakthrough) and absence of scheduled (withdrawal) bleeding <span class="hlt">events</span>. Safety and tolerability were assessed throughout the study. Participants were randomised either to the Nuva<span class="hlt">Ring</span> (n = 732) or to the COC (n = 214); 588 (82.4%) and 182 (78.4%) participants, respectively, completed the study. There were 10 in-treatment pregnancies in the Nuva<span class="hlt">Ring</span> group (PI 1.92; 95% confidence interval [CI] 0.92, 3.53) and five in the COC group (PI 3.12; 95% CI 1.01, 7.29). Breakthrough bleeding/spotting ranged from 18.6% (Cycle 1) to 4.2% (Cycle 11) for Nuva<span class="hlt">Ring</span> and from 21.6% (Cycle 1) to 7.9% (Cycle 11) for COC. Absence of withdrawal bleeding ranged from 8.6% (Cycle 1) to 3.0% (Cycle 11) for Nuva<span class="hlt">Ring</span> and from 14.6% (Cycle 1) to 6.4% (Cycle 5) for COC. For Nuva<span class="hlt">Ring</span> and COC, respectively, 26.6% and 25.0% of participants had treatment-related adverse <span class="hlt">events</span>, and 7.0% and 9.1% discontinued the study as a result. Once-monthly Nuva<span class="hlt">Ring</span> is efficacious and safe for use in Chinese women.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA00701&hterms=Lenticular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DLenticular','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA00701&hterms=Lenticular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DLenticular"><span>Jupiter's Main <span class="hlt">Ring/Ring</span> Halo</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>A mosaic of four images taken through the clear filter (610 nanometers) of the solid state imaging (CCD) system aboard NASA's Galileo spacecraft on November 8, 1996, at a resolution of approximately 46 kilometers (28.5 miles) per picture element (pixel) along Jupiter's <span class="hlt">rings</span>. Because the spacecraft was only about 0.5 degrees above the <span class="hlt">ring</span> plane, the image is highly foreshortened in the vertical direction. The images were obtained when Galileo was in Jupiter's shadow, peering back toward the Sun; the <span class="hlt">ring</span> was approximately 2.3 million kilometers (1.4 million miles) away. The arc on the far right of the image is produced when sunlight is scattered by small particles comprising Jupiter's upper atmospheric haze. The <span class="hlt">ring</span> also efficiently scatters light, indicating that much of its brightness is due to particles that are microns or less in diameter. Such small particles are believed to have human-scale lifetimes, i.e., very brief compared to the solar system's age.<p/>Jupiter's <span class="hlt">ring</span> system is composed of three parts - - a flat main <span class="hlt">ring</span>, a lenticular halo interior to the main <span class="hlt">ring</span>, and the gossamer <span class="hlt">ring</span>, outside the main <span class="hlt">ring</span>. The near and far arms of Jupiter's main <span class="hlt">ring</span> extend horizontally across the mosaic, joining together at the <span class="hlt">ring</span>'s ansa, on the figure's far left side. The near arm of the <span class="hlt">ring</span> appears to be abruptly truncated close to the planet, at the point where it passes into Jupiter's shadow. Some radial structure is barely visible across the <span class="hlt">ring</span>'s ansa (top image). A faint mist of particles can be seen above and below the main <span class="hlt">rings</span>. This vertically extended 'halo' is unusual in planetary <span class="hlt">rings</span>, and is probably caused by electromagnetic forces pushing the smallest grains out of the <span class="hlt">ring</span> plane. Because of shadowing, the halo is not visible close to Jupiter in the lower right part of the mosaic. To accentuate faint features in the bottom image of the <span class="hlt">ring</span> halo, different brightnesses are shown through color. Brightest features are white or yellow and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995ApOpt..34.5375S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995ApOpt..34.5375S"><span>Sideband analysis and seismic detection in a large <span class="hlt">ring</span> laser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stedman, G. E.; Li, Z.; Bilger, H. R.</p> <p>1995-08-01</p> <p>A <span class="hlt">ring</span> laser unlocked by the Earth's Sagnac effect has attained a frequency resolution of 1 part in 3 \\times 1021 and a rotational resolution of 300 prad. We discuss both theoretically and experimentally the sideband structure of the Earth rotation-induced spectral line induced in the microhertz-hertz region by frequency modulation associated with extra mechanical motion, such as seismic <span class="hlt">events</span>. The relative sideband height is an absolute measure of the rotational amplitude of that Fourier component. An initial analysis is given of the <span class="hlt">ring</span> laser record from the Arthur's Pass-Coleridge seismic <span class="hlt">event</span> of 18 June 1994.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1373541','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1373541"><span>FY2017 status report: Model 9975 O-<span class="hlt">ring</span> fixture long-term leak performance</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>Daugherty, W. L.</p> <p></p> <p>A series of experiments to monitor the aging performance of Viton® GLT and GLT-S O-<span class="hlt">rings</span> used in the Model 9975 shipping package has been ongoing since 2004 at the Savannah River National Laboratory. One approach has been to periodically evaluate the leak performance of O-<span class="hlt">rings</span> being aged in mock-up 9975 Primary Containment Vessels (PCVs) at elevated temperature. Other methods such as compression-stress relaxation (CSR) tests and field surveillance are also on-going to evaluate O-<span class="hlt">ring</span> behavior. Seventy tests using PCV mock-ups with GLT O-<span class="hlt">rings</span> were assembled and heated to temperatures ranging from 200 to 450 ºF. They were leak-tested initially andmore » have been tested periodically to determine if they continue to meet the leak-tightness criterion defined in ANSI standard N14.5-97. Due to material substitution, a smaller test matrix with fourteen additional tests was initiated in 2008 with GLT-S O-<span class="hlt">rings</span> heated to temperatures ranging from 200 to 400 ºF. Leak test failures have been experienced in all of the GLT O-<span class="hlt">ring</span> fixtures aging at 350 ºF and higher temperatures, and in 8 fixtures aging at 300 ºF. The 300 °F GLT O-<span class="hlt">ring</span> fixtures failed after 2.8 to 5.7 years at temperature. The remaining GLT O-<span class="hlt">ring</span> fixtures aging at 300 ºF were retired from testing following more than 5 years at temperature without failure. No failures have yet been observed in GLT O-<span class="hlt">ring</span> fixtures aging at 200 ºF for 9 to 10.5 years, or in GLT O-<span class="hlt">ring</span> fixtures aging at 270 ºF for 5.7 years. These aging temperatures bound O-<span class="hlt">ring</span> temperatures anticipated during normal <span class="hlt">storage</span> in K-Area Complex (KAC). Leak test failures have been experienced in all of the GLT-S O-<span class="hlt">ring</span> fixtures aging at 300 ºF and above. No failures have yet been observed in GLT-S O-<span class="hlt">ring</span> fixtures aging at 200 and 250 ºF for 6.9 to 7.5 years. Data from the O-<span class="hlt">ring</span> fixtures are generally consistent with results from compression stress relaxation testing, and provide confidence in the predictive models based on those</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014plri.book.....E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014plri.book.....E"><span>Planetary <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esposito, Larry</p> <p>2014-03-01</p> <p>Preface: a personal view of planetary <span class="hlt">rings</span>; 1. Introduction: the allure of the <span class="hlt">ringed</span> planets; 2. Studies of planetary <span class="hlt">rings</span> 1610-2013; 3. Diversity of planetary <span class="hlt">rings</span>; 4. Individual <span class="hlt">ring</span> particles and their collisions; 5. Large-scale <span class="hlt">ring</span> evolution; 6. Moons confine and sculpt <span class="hlt">rings</span>; 7. Explaining <span class="hlt">ring</span> phenomena; 8. N-body simulations; 9. Stochastic models; 10. Age and evolution of <span class="hlt">rings</span>; 11. Saturn's mysterious F <span class="hlt">ring</span>; 12. Uranus' <span class="hlt">rings</span> and moons; 13. Neptune's partial <span class="hlt">rings</span>; 14. Jupiter's <span class="hlt">ring</span>-moon system after Galileo and New Horizons; 15. <span class="hlt">Ring</span> photometry; 16. Dusty <span class="hlt">rings</span>; 17. Concluding remarks; Afterword; Glossary; References; Index.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170008496&hterms=plasma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dplasma','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170008496&hterms=plasma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dplasma"><span>Saturn's <span class="hlt">Rings</span> and Associated <span class="hlt">Ring</span> Plasma Cavity: Evidence for Slow <span class="hlt">Ring</span> Erosion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Farrell, W. M.; Kurth, W. S.; Gurnett, D. A.; Persoon, A. M.; MacDowall, R. J.</p> <p>2017-01-01</p> <p>We re-examine the radio and plasma wave observations obtained during the Cassini Saturn orbit insertion period, as the spacecraft flew over the northern <span class="hlt">ring</span> surface into a radial distance of 1.3 Rs (over the C-<span class="hlt">ring</span>). Voyager era studies suggest the <span class="hlt">rings</span> are a source of micro-meteoroid generated plasma and dust, with theorized peak impact-created plasma outflows over the densest portion of the <span class="hlt">rings</span> (central B-<span class="hlt">ring</span>). In sharp contrast, the Cassini Radio and Plasma Wave System (RPWS) observations identify the presence of a <span class="hlt">ring</span>-plasma cavity located in the central portion of the B-<span class="hlt">ring</span>, with little evidence of impact-related plasma. While previous Voyager era studies have predicted unstable ion orbits over the C- <span class="hlt">ring</span>, leading to field-aligned plasma transport to Saturns ionosphere, the Cassini RPWS observations do not reveal evidence for such instability-created plasma fountains. Given the passive <span class="hlt">ring</span> loss processes observed by Cassini, we find that the <span class="hlt">ring</span> lifetimes should extend >10(exp 9) years, and that there is limited evidence for prompt destruction (loss in <100 Myrs).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Icar..292...48F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..292...48F"><span>Saturn's <span class="hlt">rings</span> and associated <span class="hlt">ring</span> plasma cavity: Evidence for slow <span class="hlt">ring</span> erosion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farrell, W. M.; Kurth, W. S.; Gurnett, D. A.; Persoon, A. M.; MacDowall, R. J.</p> <p>2017-08-01</p> <p>We re-examine the radio and plasma wave observations obtained during the Cassini Saturn orbit insertion period, as the spacecraft flew over the northern <span class="hlt">ring</span> surface into a radial distance of 1.3 Rs (over the C-<span class="hlt">ring</span>). Voyager era studies suggest the <span class="hlt">rings</span> are a source of micro-meteoroid generated plasma and dust, with theorized peak impact-created plasma outflows over the densest portion of the <span class="hlt">rings</span> (central B-<span class="hlt">ring</span>). In sharp contrast, the Cassini Radio and Plasma Wave System (RPWS) observations identify the presence of a <span class="hlt">ring</span>-plasma cavity located in the central portion of the B-<span class="hlt">ring</span>, with little evidence of impact-related plasma. While previous Voyager era studies have predicted unstable ion orbits over the C-<span class="hlt">ring</span>, leading to field-aligned plasma transport to Saturn's ionosphere, the Cassini RPWS observations do not reveal evidence for such instability-created plasma 'fountains'. Given the passive <span class="hlt">ring</span> loss processes observed by Cassini, we find that the <span class="hlt">ring</span> lifetimes should extend >109 years, and that there is limited evidence for prompt destruction (loss in <100 Myrs).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/783730','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/783730"><span>DEVELOPMENT OF TITANIUM NITRIDE COATING FOR SNS <span class="hlt">RING</span> VACUUM CHAMBERS.</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>HE,P.; HSEUH,H.C.; MAPES,M.</p> <p>2001-06-18</p> <p>The inner surface of the <span class="hlt">ring</span> vacuum chambers of the US Spallation Neutron Source (SNS) will be coated with {approximately}100 nm of Titanium Nitride (TiN). This is to minimize the secondary electron yield (SEY) from the chamber wall, and thus avoid the so-called e-p instability caused by electron multipacting as observed in a few high-intensity proton <span class="hlt">storage</span> <span class="hlt">rings</span>. Both DC sputtering and DC-magnetron sputtering were conducted in a test chamber of relevant geometry to SNS <span class="hlt">ring</span> vacuum chambers. Auger Electron Spectroscopy (AES) and Rutherford Back Scattering (RBS) were used to analyze the coatings for thickness, stoichiometry and impurity. Excellent resultsmore » were obtained with magnetron sputtering. The development of the parameters for the coating process and the surface analysis results are presented.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011plri.book.....E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011plri.book.....E"><span>Planetary <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esposito, Larry W.</p> <p>2011-07-01</p> <p>Preface; 1. Introduction: the allure of <span class="hlt">ringed</span> planets; 2. Studies of planetary <span class="hlt">rings</span> 1610-2004; 3. Diversity of planetary <span class="hlt">rings</span>; 4. Individual <span class="hlt">ring</span> particles and their collisions; 5. Large-scale <span class="hlt">ring</span> evolution; 6. Moons confine and sculpt <span class="hlt">rings</span>; 7. Explaining <span class="hlt">ring</span> phenomena; 8. N-Body simulations; 9. Stochastic models; 10. Age and evolution of <span class="hlt">rings</span>; 11. Saturn's mysterious F <span class="hlt">ring</span>; 12. Neptune's partial <span class="hlt">rings</span>; 13. Jupiter's <span class="hlt">ring</span>-moon system after Galileo; 14. <span class="hlt">Ring</span> photometry; 15. Dusty <span class="hlt">rings</span>; 16. Cassini observations; 17. Summary: the big questions; Glossary; References; Index.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890027856&hterms=generator+magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dgenerator%2Bmagnetic%2Benergy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890027856&hterms=generator+magnetic+energy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dgenerator%2Bmagnetic%2Benergy"><span>Overview of a flywheel stack energy <span class="hlt">storage</span> system</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kirk, James A.; Anand, Davinder K.</p> <p>1988-01-01</p> <p>The concept of storing electrical energy in rotating flywheels provides an attractive substitute to batteries. To realize these advantages the critical technologies of rotor design, composite materials, magnetic suspension, and high efficiency motor/generators are reviewed in this paper. The magnetically suspended flywheel energy <span class="hlt">storage</span> system, currently under development at the University of Maryland, consisting of a family of interference assembled <span class="hlt">rings</span>, is presented as an integrated solution for energy <span class="hlt">storage</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999PhDT.......100P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999PhDT.......100P"><span><span class="hlt">Ringing</span> in the new physics: The politics and technology of electron colliders in the United States, 1956--1972</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paris, Elizabeth</p> <p></p> <p>The ``November Revolution'' of 1974 and the experiments that followed consolidated the place of the Standard Model in modern particle physics. Much of the evidence on which these conclusions depended was generated by a new type of tool: colliding beam <span class="hlt">storage</span> <span class="hlt">rings</span>, which had been considered physically unfeasible twenty years earlier. In 1956 a young experimentalist named Gerry O'Neill dedicated himself to demonstrating that such an apparatus could do useful physics. The <span class="hlt">storage</span> <span class="hlt">ring</span> movement encountered numerous obstacles before generating one of the standard machines for high energy research. In fact, it wasn't until 1970 that the U.S. finally broke ground on its first electron-positron collider. Drawing extensively on archival sources and supplementing them with the personal accounts of many of the individuals who took part, <span class="hlt">Ringing</span> in the New Physics examines this instance of post-World War II techno-science and the new social, political and scientific tensions that characterize it. The motivations are twofold: first, that the chronicle of <span class="hlt">storage</span> <span class="hlt">rings</span> may take its place beside mathematical group theory, computer simulations, magnetic spark chambers, and the like as an important contributor to a view of matter and energy which has been the dominant model for the last twenty-five years. In addition, the account provides a case study for the integration of the personal, professional, institutional, and material worlds when examining an episode in the history or sociology of twentieth century science. The story behind the technological development of <span class="hlt">storage</span> <span class="hlt">rings</span> holds fascinating insights into the relationship between theory and experiment, collaboration and competition in the physics community, the way scientists obtain funding and their responsibilities to it, and the very nature of what constitutes ``successful'' science in the post- World War II era.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20110013500&hterms=comparative&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcomparative','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20110013500&hterms=comparative&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcomparative"><span><span class="hlt">Ring</span> Current Dynamics in Moderate and Strong Storms: Comparative Analysis of TWINS and IMAGE/HENA Data with the Comprehensive <span class="hlt">Ring</span> Current Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Buzulukova, N.; Fok, M.-C.; Goldstein, J.; Valek, P.; McComas, D. J.; Brandt, P. C.</p> <p>2010-01-01</p> <p>We present a comparative study of <span class="hlt">ring</span> current dynamics during strong and moderate storms. The <span class="hlt">ring</span> current during the strong storm is studied with IMAGE/HENA data near the solar cycle maximum in 2000. The <span class="hlt">ring</span> current during the moderate storm is studied using energetic neutral atom (ENA) data from the Two Wide-Angle Imaging Neutral- Atom Spectrometers (TWINS) mission during the solar minimum in 2008. For both storms, the local time distributions of ENA emissions show signatures of postmidnight enhancement (PME) during the main phases. To model the <span class="hlt">ring</span> current and ENA emissions, we use the Comprehensive <span class="hlt">Ring</span> Current Model (CRCM). CRCM results show that the main-phase <span class="hlt">ring</span> current pressure peaks in the premidnight-dusk sector, while the most intense CRCM-simulated ENA emissions show PME signatures. We analyze two factors to explain this difference: the dependence of charge-exchange cross section on energy and pitch angle distributions of <span class="hlt">ring</span> current. We find that the IMF By effect (twisting of the convection pattern due to By) is not needed to form the PME. Additionally, the PME is more pronounced for the strong storm, although relative shielding and hence electric field skewing is well developed for both <span class="hlt">events</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NIMPB.408..323S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NIMPB.408..323S"><span>High-precision X-ray spectroscopy of highly-charged ions at the experimental <span class="hlt">storage</span> <span class="hlt">ring</span> using silicon microcalorimeters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scholz, Pascal A.; Andrianov, Victor; Echler, Artur; Egelhof, Peter; Kilbourne, Caroline; Kiselev, Oleg; Kraft-Bermuth, Saskia; McCammon, Dan</p> <p>2017-10-01</p> <p>X-ray spectroscopy on highly charged heavy ions provides a sensitive test of quantum electrodynamics in very strong Coulomb fields. One limitation of the current accuracy of such experiments is the energy resolution of available X-ray detectors for energies up to 100 keV. To improve this accuracy, a novel detector concept, namely the concept of microcalorimeters, is exploited for this kind of measurements. The microcalorimeters used in the present experiments consist of silicon thermometers, ensuring a high dynamic range, and of absorbers made of high-Z material to provide high X-ray absorption efficiency. Recently, besides an earlier used detector, a new compact detector design, housed in a new dry cryostat equipped with a pulse tube cooler, was applied at a test beamtime at the experimental <span class="hlt">storage</span> <span class="hlt">ring</span> (ESR) of the GSI facility in Darmstadt. A U89+ beam at 75 MeV/u and a 124Xe54+ beam at various beam energies, both interacting with an internal gas-jet target, were used in different cycles. This test was an important benchmark for designing a larger array with an improved lateral sensitivity and statistical accuracy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.898f2020B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.898f2020B"><span>A study of data representation in Hadoop to optimize data <span class="hlt">storage</span> and search performance for the ATLAS <span class="hlt">Event</span>Index</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baranowski, Z.; Canali, L.; Toebbicke, R.; Hrivnac, J.; Barberis, D.</p> <p>2017-10-01</p> <p>This paper reports on the activities aimed at improving the architecture and performance of the ATLAS <span class="hlt">Event</span>Index implementation in Hadoop. The <span class="hlt">Event</span>Index contains tens of billions of <span class="hlt">event</span> records, each of which consists of ∼100 bytes, all having the same probability to be searched or counted. Data formats represent one important area for optimizing the performance and <span class="hlt">storage</span> footprint of applications based on Hadoop. This work reports on the production usage and on tests using several data formats including Map Files, Apache Parquet, Avro, and various compression algorithms. The query engine plays also a critical role in the architecture. We report also on the use of HBase for the <span class="hlt">Event</span>Index, focussing on the optimizations performed in production and on the scalability tests. Additional engines that have been tested include Cloudera Impala, in particular for its SQL interface, and the optimizations for data warehouse workloads and reports.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.7559R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.7559R"><span>Something old, something new: Why models need a multi-pool representation of <span class="hlt">storage</span> reserves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Richardson, Andrew; Carbone, Mariah</p> <p>2015-04-01</p> <p>We know surprisingly little about processes regulating the allocation of photosynthetic assimilates to growth, <span class="hlt">storage</span>, and other metabolic functions. <span class="hlt">Storage</span> of nonstructural carbon (NSC, principally sugars and starch) is critically important for woody plants, because these reserves enable sessile, long-lived organisms to tolerate biotic and abiotic stress, including pests, disturbance, and drought. But, critical questions about the size and turnover of these reserves remain unanswered. Labeling studies have generally shown rapid use of new (labeled) NSC and inferred fast mixing between old and new NSC, both of which suggest quick turnover of <span class="hlt">storage</span> reserves. However, recent studies have shown that some of the reserves stored in stem and root tissue are not only a decade old, but also still available to support new tissue growth following catastrophic disturbance. We characterized the distribution of NSC in the stemwood, branches, and roots of two temperate trees, and we used the continuous label offered by the radiocarbon (14C) bomb spike to estimate the mean age of NSC in different tissues of two temperate trees. NSC in branches and outermost stemwood growth <span class="hlt">rings</span> had the 14C signature of the current growing season. However, NSC in older above- and below-ground tissues was enriched in 14C, indicating that it was produced from older assimilates. Radial patterns of 14C in stemwood NSC showed strong mixing of NSC across the youngest growth <span class="hlt">rings</span>, with limited "mixing in" of younger NSC to older <span class="hlt">rings</span>. Sugars in the outermost 5 growth <span class="hlt">rings</span>, accounting for two-thirds of the stemwood pool, had a mean age < 1 y, whereas sugars in older growth <span class="hlt">rings</span> had a mean age > 5 y. Thus, there is not a single, well-mixed "<span class="hlt">storage</span> pool," and indeed "young" and "old" <span class="hlt">storage</span> compounds appear to be physically isolated from each other. We will discuss the implications of these results for improving model representation of NSC <span class="hlt">storage</span> and consumption by forest trees. We will suggest</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997APS..PAC..3P45S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997APS..PAC..3P45S"><span>Completion of the LANSCE Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> Control System Upgrade -- A Successful Integration of EPICS Into a Running Control System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schaller, S. C.; Bjorklund, E. A.; Carr, G. P.; Faucett, J. A.; Oothoudt, M. A.</p> <p>1997-05-01</p> <p>The Los Alamos Neutron Scattering Center (LANSCE) Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> (PSR) control system upgrade was completed in 1996. In previous work, much of a PDP-11-based control system was replaced with Experimental Physics and Industrial Control System (EPICS) controls. Several parts of the old control system which used a VAX for operator displays and direct access to a CAMAC serial highway still remained. The old system was preserved as a "fallback" if the new EPICS-based system had problems. The control system upgrade completion included conversion of several application programs to EPICS-based operator interfaces, moving some data acquisition hardware to EPICS Input-Output Controllers (IOCs), and the implementation of new gateway software to complete the overall control system interoperability. Many operator interface (OPI) screens, written by LANSCE operators, have been incorporated in the new system. The old PSR control system hardware was removed. The robustness and reliability of the new controls obviated the need for a fallback capability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvS..20i4001M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvS..20i4001M"><span>Control of systematic uncertainties in the <span class="hlt">storage</span> <span class="hlt">ring</span> search for an electric dipole moment by measuring the electric quadrupole moment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Magiera, Andrzej</p> <p>2017-09-01</p> <p>Measurements of electric dipole moment (EDM) for light hadrons with use of a <span class="hlt">storage</span> <span class="hlt">ring</span> have been proposed. The expected effect is very small, therefore various subtle effects need to be considered. In particular, interaction of particle's magnetic dipole moment and electric quadrupole moment with electromagnetic field gradients can produce an effect of a similar order of magnitude as that expected for EDM. This paper describes a very promising method employing an rf Wien filter, allowing to disentangle that contribution from the genuine EDM effect. It is shown that both these effects could be separated by the proper setting of the rf Wien filter frequency and phase. In the EDM measurement the magnitude of systematic uncertainties plays a key role and they should be under strict control. It is shown that particles' interaction with field gradients offers also the possibility to estimate global systematic uncertainties with the precision necessary for an EDM measurement with the planned accuracy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JInst...910008S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JInst...910008S"><span>Characterization of the International Linear Collider damping <span class="hlt">ring</span> optics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shanks, J.; Rubin, D. L.; Sagan, D.</p> <p>2014-10-01</p> <p>A method is presented for characterizing the emittance dilution and dynamic aperture for an arbitrary closed lattice that includes guide field magnet errors, multipole errors and misalignments. This method, developed and tested at the Cornell Electron <span class="hlt">Storage</span> <span class="hlt">Ring</span> Test Accelerator (CesrTA), has been applied to the damping <span class="hlt">ring</span> lattice for the International Linear Collider (ILC). The effectiveness of beam based emittance tuning is limited by beam position monitor (BPM) measurement errors, number of corrector magnets and their placement, and correction algorithm. The specifications for damping <span class="hlt">ring</span> magnet alignment, multipole errors, number of BPMs, and precision in BPM measurements are shown to be consistent with the required emittances and dynamic aperture. The methodology is then used to determine the minimum number of position monitors that is required to achieve the emittance targets, and how that minimum depends on the location of the BPMs. Similarly, the maximum tolerable multipole errors are evaluated. Finally, the robustness of each BPM configuration with respect to random failures is explored.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1224786','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1224786"><span>Report of the eRHIC <span class="hlt">Ring-Ring</span> Working Group</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>Aschenauer, E. C.; Berg, S.; Blaskiewicz, M.</p> <p>2015-10-13</p> <p>This report evaluates the <span class="hlt">ring-ring</span> option for eRHIC as a lower risk alternative to the linac-<span class="hlt">ring</span> option. The reduced risk goes along with a reduced initial luminosity performance. However, a luminosity upgrade path is kept open. This upgrade path consists of two branches, with the ultimate upgrade being either a <span class="hlt">ring-ring</span> or a linac-<span class="hlt">ring</span> scheme. The linac-<span class="hlt">ring</span> upgrade could be almost identical to the proposed linac-<span class="hlt">ring</span> scheme, which is based on an ERL in the RHIC tunnel. This linac-<span class="hlt">ring</span> version has been studied in great detail over the past ten years, and its significant risks are known. On the othermore » hand, no detailed work on an ultimate performance <span class="hlt">ring-ring</span> scenario has been performed yet, other than the development of a consistent parameter set. Pursuing the <span class="hlt">ring-ring</span> upgrade path introduces high risks and requires significant design work that is beyond the scope of this report.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.P12A..03C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.P12A..03C"><span>Saturn's <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cuzzi, J. N.</p> <p>2014-12-01</p> <p>The <span class="hlt">rings</span> are changing before our eyes; structure varies on all timescales and unexpected things have been discovered. Many questions have been answered, but some answers remain elusive (see Cuzzi et al 2010 for a review). Here we highlight the major <span class="hlt">ring</span> science progress over the mission to date, and describe new observations planned for Cassini's final three years. <span class="hlt">Ring</span> Composition and particle sizes: The <span class="hlt">rings</span> are nearly all water ice with no other ices - so why are they reddish? The C <span class="hlt">Ring</span> and Cassini Division are "dirtier" than the more massive B and A <span class="hlt">Rings</span>, as shown by near-IR and, recently, microwave observations. Particle sizes, from stellar and radio occultations, vary from place to place. <span class="hlt">Ring</span> structure, micro and macro: numerous spiral density waves and ubiquitous "self-gravity wakes" reveal processes which fostered planet formation in the solar system and elsewhere. However, big puzzles remain regarding the main <span class="hlt">ring</span> divisions, the C <span class="hlt">Ring</span> plateau structures, and the B <span class="hlt">Ring</span> irregular structure. Moonlets, inside and out, seen and unseen: Two gaps contain sizeable moonlets, but more gaps seem to contain none; even smaller embedded "propeller" objects wander, systematically or randomly, through the A <span class="hlt">ring</span>. Rubble pile ringmoons just outside the <span class="hlt">rings</span> may escaped from the <span class="hlt">rings</span>, and the recently discovered "Peggy" may be trying this as we watch. Impact bombardment of the <span class="hlt">rings</span>: Comet fragments set the <span class="hlt">rings</span> to rippling on century-timescales, and boulders crash through hourly; meanwhile, the constant hail of infalling Kuiper belt material has a lower mass flux than previously thought. Origin and Age of the <span class="hlt">Rings</span>: The <span class="hlt">ring</span> mass and bombardment play key roles. The <span class="hlt">ring</span> mass is well known everywhere but in the B <span class="hlt">Ring</span> (where most of it is). New models suggest how tidal breakup of evolving moons may have formed massive ancient <span class="hlt">rings</span>, of which the current <span class="hlt">ring</span> is just a shadow. During its last three years, the Cassini tour profile will allow entirely new</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DNP.EA156V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DNP.EA156V"><span>A Study on Double <span class="hlt">Event</span> Detection for PHENIX at RHIC</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vazquez-Carson, Sebastian; Phenix Collaboration</p> <p>2016-09-01</p> <p>Many measurements made in Heavy Ion experiments such as PHENIX at RHIC focus on geometrical properties because phenomena such as collective flow give insight into quark-gluon plasma and the strong nuclear force. As part of this investigation, PHENIX has taken data in 2016 for deuteron on gold collisions at several energies. An acceptable luminosity is achieved by injecting up to 120 separate bunches each with billions of ions into the <span class="hlt">storage</span> <span class="hlt">ring</span>, from which two, separate beams are made to collide. This method has a drawback as there is a chance for multiple pairs of nuclei to collide in a single bunch crossing. Data taken in a double <span class="hlt">event</span> cannot be separated into two independent <span class="hlt">events</span> and has no clear interpretation. This effect's magnitude is estimated and incorporated in published results as a systematic uncertainty and studies on this topic have already been conducted within PHENIX. I develop several additional algorithms to flag multiple interaction <span class="hlt">events</span> by examining the time dependence of data from the two Beam-Beam Counters - detectors surrounding the beam pipe on opposite ends of the interaction region. The algorithms are tested with data, in which <span class="hlt">events</span> with double interactions are artificially produced using low luminosity data. I am working at the University of Colorado at Boulder on behalf of the PHENIX collaboration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720019697','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720019697"><span>Electrostatic instability of <span class="hlt">ring</span> current protons beyond the plasmapause during injection <span class="hlt">events</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Coroniti, F. V.; Fredricks, R. W.; White, R.</p> <p>1972-01-01</p> <p>The stability of <span class="hlt">ring</span> current protons with an injection spectrum modeled by an m = 2 mirror distribution function was examined for typical <span class="hlt">ring</span> current parameters. It was found that the high frequency loss cone mode can be excited at wave numbers K lambda sub Di about = to 0.1 to 0.5, at frequencies omega about = to (0.2 to 0.6) omega sub pi and with growth rates up to gamma/omega about = to 0.03. These waves interact with the main body of the proton distribution and propagate nearly perpendicular to the local magnetic field. Cold particle partial densities tend to reduce the growth rate so that the waves are quenched at or near to the plasmapause boundary. Wave e-folding lengths are comparable to 0.1 R sub e, compared to the value of about 4 R sub e found for ion cyclotron waves at the same plasma conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17169905','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17169905"><span>Effects of <span class="hlt">ring</span>-porous and diffuse-porous stem wood anatomy on the hydraulic parameters used in a water flow and <span class="hlt">storage</span> model.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Steppe, Kathy; Lemeur, Raoul</p> <p>2007-01-01</p> <p>Calibration of a recently developed water flow and <span class="hlt">storage</span> model based on experimental data for a young diffuse-porous beech tree (Fagus sylvatica L.) and a young <span class="hlt">ring</span>-porous oak tree (Quercus robur L.) revealed that differences in stem wood anatomy between species strongly affect the calibrated values of the hydraulic model parameters. The hydraulic capacitance (C) of the stem <span class="hlt">storage</span> tissue was higher in oak than in beech (939.8 versus 212.3 mg MPa(-1)). Model simulation of the elastic modulus (epsilon) revealed that this difference was linked to the higher elasticity of the stem <span class="hlt">storage</span> tissue of oak compared with beech. Furthermore, the hydraulic resistance (R (x)) of beech was about twice that of oak (0.1829 versus 0.1072 MPa s mg(-1)). To determine the physiological meaning of the R (x) parameter identified by model calibration, we analyzed the stem wood anatomy of the beech and oak trees. Calculation of stem specific hydraulic conductivity (k (s)) of beech and oak with the Hagen-Poiseuille equation confirmed the differences in R (x) predicted by the model. The contributions of different vessel diameter classes to the total hydraulic conductivity of the xylem were calculated. As expected, the few big vessels contributed much more to total conductivity than the many small vessels. Compared with beech, the larger vessels of oak resulted in a higher k (s) (10.66 versus 4.90 kg m(-1) s(-1) MPa(-1)). The calculated ratio of k (s) of oak to beech was 2, confirming the R (x) ratio obtained by model calibration. Thus, validation of the R (x) parameter of the model led to identification of its physiological meaning.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/272727-temperature-histories-from-tree-rings-corals','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/272727-temperature-histories-from-tree-rings-corals"><span>Temperature histories from tree <span class="hlt">rings</span> and corals</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>Cook, E.R.</p> <p>1995-05-01</p> <p>Recent temperature trends in long tree-<span class="hlt">ring</span> and coral proxy temperature histories are evaluated and compared in an effort to objectively determine how anomalous twentieth century temperature changes have been. These histories mostly reflect regional variations in summer warmth from the tree <span class="hlt">rings</span> and annual warmth from the corals. In the Northern Hemisphere. the North American tree-<span class="hlt">ring</span> temperature histories and those from the north Polar Urals, covering the past 1000 or more years, indicate that the twentieth century has been anomalously warm relative to the past. In contrast, the tree-<span class="hlt">ring</span> history from northern Fennoscandia indicates that summer temperatures during the {open_quote}Medievalmore » Warm Period{close_quote} were probably warmer on average than those than during this century. In the Southern Hemisphere, the tree-<span class="hlt">ring</span> temperature histories from South America show no indication of recent warming, which is in accordance with local instrumental records. In contrast, the tree-<span class="hlt">ring</span>, records from Tasmania and New Zealand indicate that the twentieth century has been unusually warm particularly since 1960. The coral temperature histories from the Galapagos Islands and the Great Barrier Reef are in broad agreement with the tree-<span class="hlt">ring</span> temperature histories in those sectors, with the former showing recent cooling and the latter showing recent warming that may be unprecedented. Overall, the regional temperature histories evaluated here broadly support the larger-scale evidence for anomalous twentieth century warming based on instrumental records. However, this warming cannot be confirmed as an unprecedented <span class="hlt">event</span> in all regions. 38 refs., 3 figs., 2 tabs.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19760038847&hterms=CERN&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DCERN','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19760038847&hterms=CERN&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DCERN"><span>An investigation of high-multiplicity gamma <span class="hlt">events</span> in pp collisions with c.m. energies between 22 and 62 GeV</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dell, G. F.; Uto, H.; Yuan, L. C. L.; Amaldi, E.; Beneventano, M.; Borgia, B.; Pistilli, P.; Sestili, I.; Dooher, J.</p> <p>1976-01-01</p> <p>An experiment was conducted at the CERN intersecting <span class="hlt">storage</span> <span class="hlt">rings</span> using colliding proton beams to investigate high-multiplicity gamma-ray <span class="hlt">events</span>. The objective of the study was to reveal certain features of multiple pion production as well as other possible mechanisms of gamma-ray production. The detector system consisted of ten planes of spark chambers, three scintillation counter hodoscopes and two arrays of lead-glass Cerenkov counters, the first array containing 16 counters and the second, 60 counters. The <span class="hlt">event</span> trigger was obtained from the Cerenkov counters, and the energies in all the Cerenkov counters after trigger, as well as the information on all the charged particles given by the scintillation counters and spark chambers were recorded on magnetic tape. The relationship between the number of gamma-rays per <span class="hlt">event</span> and the number of Cerenkov counters triggered by a neutral secondary was established by means of a Monte Carlo calculation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28767084','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28767084"><span>Sc-Decorated Porous Graphene for High-Capacity Hydrogen <span class="hlt">Storage</span>: First-Principles Calculations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Yuhong; Wang, Jing; Yuan, Lihua; Zhang, Meiling; Zhang, Cairong</p> <p>2017-08-02</p> <p>The generalized gradient approximation (GGA) function based on density functional theory is adopted to investigate the optimized geometrical structure, electron structure and hydrogen <span class="hlt">storage</span> performance of Sc modified porous graphene (PG). It is found that the carbon <span class="hlt">ring</span> center is the most stable adsorbed position for a single Sc atom on PG, and the maximum number of adsorbed H₂ molecules is four with the average adsorption energy of -0.429 eV/H₂. By adding a second Sc atom on the other side of the system, the hydrogen <span class="hlt">storage</span> capacity of the system can be improved effectively. Two Sc atoms located on opposite sides of the PG carbon <span class="hlt">ring</span> center hole is the most suitable hydrogen <span class="hlt">storage</span> structure, and the hydrogen <span class="hlt">storage</span> capacity reach a maximum 9.09 wt % at the average adsorption energy of -0.296 eV/H₂. The adsorption of H₂ molecules in the PG system is mainly attributed to orbital hybridization among H, Sc, and C atoms, and Coulomb attraction between negatively charged H₂ molecules and positively charged Sc atoms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5578260','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5578260"><span>Sc-Decorated Porous Graphene for High-Capacity Hydrogen <span class="hlt">Storage</span>: First-Principles Calculations</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chen, Yuhong; Wang, Jing; Yuan, Lihua; Zhang, Meiling</p> <p>2017-01-01</p> <p>The generalized gradient approximation (GGA) function based on density functional theory is adopted to investigate the optimized geometrical structure, electron structure and hydrogen <span class="hlt">storage</span> performance of Sc modified porous graphene (PG). It is found that the carbon <span class="hlt">ring</span> center is the most stable adsorbed position for a single Sc atom on PG, and the maximum number of adsorbed H2 molecules is four with the average adsorption energy of −0.429 eV/H2. By adding a second Sc atom on the other side of the system, the hydrogen <span class="hlt">storage</span> capacity of the system can be improved effectively. Two Sc atoms located on opposite sides of the PG carbon <span class="hlt">ring</span> center hole is the most suitable hydrogen <span class="hlt">storage</span> structure, and the hydrogen <span class="hlt">storage</span> capacity reach a maximum 9.09 wt % at the average adsorption energy of −0.296 eV/H2. The adsorption of H2 molecules in the PG system is mainly attributed to orbital hybridization among H, Sc, and C atoms, and Coulomb attraction between negatively charged H2 molecules and positively charged Sc atoms. PMID:28767084</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013pss3.book..309T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013pss3.book..309T"><span>Planetary <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tiscareno, Matthew S.</p> <p></p> <p>Planetary <span class="hlt">rings</span> are the only nearby astrophysical disks and the only disks that have been investigated by spacecraft (especially the Cassini spacecraft orbiting Saturn). Although there are significant differences between <span class="hlt">rings</span> and other disks, chiefly the large planet/<span class="hlt">ring</span> mass ratio that greatly enhances the flatness of <span class="hlt">rings</span> (aspect ratios as small as 10- 7), understanding of disks in general can be enhanced by understanding the dynamical processes observed at close range and in real time in planetary <span class="hlt">rings</span>.We review the known <span class="hlt">ring</span> systems of the four giant planets, as well as the prospects for <span class="hlt">ring</span> systems yet to be discovered. We then review planetary <span class="hlt">rings</span> by type. The A, B, and C <span class="hlt">rings</span> of Saturn, plus the Cassini Division, comprise our solar system's only dense broad disk and host many phenomena of general application to disks including spiral waves, gap formation, self-gravity wakes, viscous overstability and normal modes, impact clouds, and orbital evolution of embedded moons. Dense narrow <span class="hlt">rings</span> are found both at Uranus (where they comprise the main <span class="hlt">rings</span> entirely) and at Saturn (where they are embedded in the broad disk) and are the primary natural laboratory for understanding shepherding and self-stability. Narrow dusty <span class="hlt">rings</span>, likely generated by embedded source bodies, are surprisingly found to sport azimuthally confined arcs at Neptune, Saturn, and Jupiter. Finally, every known <span class="hlt">ring</span> system includes a substantial component of diffuse dusty <span class="hlt">rings</span>.Planetary <span class="hlt">rings</span> have shown themselves to be useful as detectors of planetary processes around them, including the planetary magnetic field and interplanetary impactors as well as the gravity of nearby perturbing moons. Experimental <span class="hlt">rings</span> science has made great progress in recent decades, especially numerical simulations of self-gravity wakes and other processes but also laboratory investigations of coefficient of restitution and spectroscopic ground truth. The age of self-sustained <span class="hlt">ring</span> systems is a matter of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5151055','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5151055"><span>Tunable optical analog to electromagnetically induced transparency in graphene-<span class="hlt">ring</span> resonators system</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wang, Yonghua; Xue, Chenyang; Zhang, Zengxing; Zheng, Hua; Zhang, Wendong; Yan, Shubin</p> <p>2016-01-01</p> <p>The analogue of electromagnetically induced transparency in optical ways has shown great potential in optical delay and quantum-information technology due to its flexible design and easy implementation. The chief drawback for these devices is the bad tunability. Here we demonstrate a tunable optical transparency system formed by graphene-silicon microrings which could control the transparent window by electro-optical means. The device consists of cascaded coupled <span class="hlt">ring</span> resonators and a graphene/graphene capacitor which integrated on one of the <span class="hlt">rings</span>. By tuning the Fermi level of the graphene sheets, we can modulate the round-trip <span class="hlt">ring</span> loss so that the transparency window can be dynamically tuned. The results provide a new method for the manipulation and transmission of light in highly integrated optical circuits and quantum information <span class="hlt">storage</span> devices. PMID:27941895</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27941895','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27941895"><span>Tunable optical analog to electromagnetically induced transparency in graphene-<span class="hlt">ring</span> resonators system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Yonghua; Xue, Chenyang; Zhang, Zengxing; Zheng, Hua; Zhang, Wendong; Yan, Shubin</p> <p>2016-12-12</p> <p>The analogue of electromagnetically induced transparency in optical ways has shown great potential in optical delay and quantum-information technology due to its flexible design and easy implementation. The chief drawback for these devices is the bad tunability. Here we demonstrate a tunable optical transparency system formed by graphene-silicon microrings which could control the transparent window by electro-optical means. The device consists of cascaded coupled <span class="hlt">ring</span> resonators and a graphene/graphene capacitor which integrated on one of the <span class="hlt">rings</span>. By tuning the Fermi level of the graphene sheets, we can modulate the round-trip <span class="hlt">ring</span> loss so that the transparency window can be dynamically tuned. The results provide a new method for the manipulation and transmission of light in highly integrated optical circuits and quantum information <span class="hlt">storage</span> devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29576449','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29576449"><span>Expanding Actin <span class="hlt">Rings</span> Zipper the Mouse Embryo for Blastocyst Formation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zenker, Jennifer; White, Melanie D; Gasnier, Maxime; Alvarez, Yanina D; Lim, Hui Yi Grace; Bissiere, Stephanie; Biro, Maté; Plachta, Nicolas</p> <p>2018-04-19</p> <p>Transformation from morula to blastocyst is a defining <span class="hlt">event</span> of preimplantation embryo development. During this transition, the embryo must establish a paracellular permeability barrier to enable expansion of the blastocyst cavity. Here, using live imaging of mouse embryos, we reveal an actin-zippering mechanism driving this embryo sealing. Preceding blastocyst stage, a cortical F-actin <span class="hlt">ring</span> assembles at the apical pole of the embryo's outer cells. The <span class="hlt">ring</span> structure forms when cortical actin flows encounter a network of polar microtubules that exclude F-actin. Unlike stereotypical actin <span class="hlt">rings</span>, the actin <span class="hlt">rings</span> of the mouse embryo are not contractile, but instead, they expand to the cell-cell junctions. Here, they couple to the junctions by recruiting and stabilizing adherens and tight junction components. Coupling of the actin <span class="hlt">rings</span> triggers localized myosin II accumulation, and it initiates a tension-dependent zippering mechanism along the junctions that is required to seal the embryo for blastocyst formation. Copyright © 2018 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PPNL...13..621F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PPNL...13..621F"><span>Use of the Hadoop structured <span class="hlt">storage</span> tools for the ATLAS <span class="hlt">Event</span>Index <span class="hlt">event</span> catalogue</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Favareto, A.</p> <p>2016-09-01</p> <p>The ATLAS experiment at the LHC collects billions of <span class="hlt">events</span> each data-taking year, and processes them to make them available for physics analysis in several different formats. An even larger amount of <span class="hlt">events</span> is in addition simulated according to physics and detector models and then reconstructed and analysed to be compared to real <span class="hlt">events</span>. The <span class="hlt">Event</span>Index is a catalogue of all <span class="hlt">events</span> in each production stage; it includes for each <span class="hlt">event</span> a few identification parameters, some basic non-mutable information coming from the online system, and the references to the files that contain the <span class="hlt">event</span> in each format (plus the internal pointers to the <span class="hlt">event</span> within each file for quick retrieval). Each <span class="hlt">Event</span>Index record is logically simple but the system has to hold many tens of billions of records, all equally important. The Hadoop technology was selected at the start of the <span class="hlt">Event</span>Index project development in 2012 and proved to be robust and flexible to accommodate this kind of information; both the insertion and query response times are acceptable for the continuous and automatic operation that started in Spring 2015. This paper describes the <span class="hlt">Event</span>Index data input and organisation in Hadoop and explains the operational challenges that were overcome in order to achieve the expected performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/181935-drought-frequency-central-california-since-recordered-giant-sequoia-tree-rings','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/181935-drought-frequency-central-california-since-recordered-giant-sequoia-tree-rings"><span>Drought frequency in central California since 101 B.C. recordered in giant sequoia tree <span class="hlt">rings</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>Hughes, M.K.; Brown, P.M.</p> <p>1992-01-01</p> <p>Well replicated tree-<span class="hlt">ring</span> width index chronologies have been developed for giant sequoia at three sites in the Sierra Nevada, California. Extreme low-growth <span class="hlt">events</span> in these chronologies correspond with regional drought <span class="hlt">events</span> in the twentieth century in the San Joaquin drainage, in which the giant sequoia sites are located. This relationship is based upon comparison of tree-<span class="hlt">ring</span> indices with August Palmer Drought Severity Indices for California Climate Division 5. <span class="hlt">Ring</span>-width indices in the lowest decile from each site were compared. The frequency of low-growth <span class="hlt">events</span> which occurred at all three sites in the same year is reconstructed from 101 B.C. tomore » A.D. 1988. The inferred frequency of severe drought <span class="hlt">events</span> changes through time, sometimes suddenly. The period from roughly 1850 to 1950 had one of the lowest frequencies of drought of any one hundred year period in the 2089 year record. The twentieth century so far has had a below-average frequency of extreme droughts. 26 refs., 6 figs., 1 tab.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1149712','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1149712"><span>NINTH INTERIM STATUS REPORT: MODEL 9975 PCV O-<span class="hlt">RING</span> FIXTURE LONG-TERM LEAK PERFORMANCE</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>Daugherty, W.</p> <p>2014-08-06</p> <p>A series of experiments to monitor the aging performance of Viton® GLT O-<span class="hlt">rings</span> used in the Model 9975 package has been ongoing since 2004 at the Savannah River National Laboratory. One approach has been to periodically evaluate the leak performance of O-<span class="hlt">rings</span> being aged in mock-up 9975 Primary Containment Vessels (PCVs) at elevated temperatures. Other methods such as compression-stress relaxation (CSR) tests and field surveillance are also on-going to evaluate O-<span class="hlt">ring</span> behavior. Seventy tests using PCV mock-ups were assembled and heated to temperatures ranging from 200 to 450 ºF. They were leak-tested initially and have been tested periodically to determinemore » if they continue to meet the leak-tightness criterion defined in ANSI standard N14.5-97. Due to material substitution, fourteen additional tests were initiated in 2008 with GLT-S O-<span class="hlt">rings</span> heated to temperatures ranging from 200 to 400 ºF. High temperature aging continues for 23 GLT O-<span class="hlt">ring</span> fixtures at 200 – 270 ºF. Room temperature leak test failures have been experienced in all of the GLT O-<span class="hlt">ring</span> fixtures aging at 350 ºF and higher temperatures, and in 8 fixtures aging at 300 ºF. The earliest 300 °F GLT O-<span class="hlt">ring</span> fixture failure was observed at 34 months. The remaining GLT O-<span class="hlt">ring</span> fixtures aging at 300 ºF have been retired from testing following more than 5 years at temperature without failure. No failures have yet been observed in GLT O-<span class="hlt">ring</span> fixtures aging at 200 ºF for 72 - 96 months, which bounds O-<span class="hlt">ring</span> temperatures anticipated during <span class="hlt">storage</span> in K-Area Complex (KAC). Based on expectations that the 200 ºF fixtures will remain leak-tight for a significant period yet to come, 2 additional fixtures began aging in 2011 at 270 ºF, with hopes that they may reach a failure condition before the 200 ºF fixtures, thus providing additional time to failure data. High temperature aging continues for 6 GLT-S O-<span class="hlt">ring</span> fixtures at 200 – 300 ºF. Room temperature leak test failures have been experienced in all 8</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29748837','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29748837"><span>Fracture mechanics modeling of popping <span class="hlt">event</span> during daughter cell separation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jiang, Yuxuan; Liang, Xudong; Guo, Ming; Cao, Yanping; Cai, Shengqiang</p> <p>2018-05-10</p> <p>Most bacteria cells divide by binary fission which is part of a bacteria cell cycle and requires tight regulations and precise coordination. Fast separation of Staphylococcus Aureus (S. Aureus) daughter cells, named as popping <span class="hlt">event</span>, has been observed in recent experiments. The popping <span class="hlt">event</span> was proposed to be driven by mechanical crack propagation in the peripheral <span class="hlt">ring</span> which connected two daughter cells before their separation. It has also been shown that after the fast separation, a small portion of the peripheral <span class="hlt">ring</span> was left as a hinge. In the article, we develop a fracture mechanics model for the crack growth in the peripheral <span class="hlt">ring</span> during S. Aureus daughter cell separation. In particular, using finite element analysis, we calculate the energy release rate associated with the crack growth in the peripheral <span class="hlt">ring</span>, when daughter cells are inflated by a uniform turgor pressure inside. Our results show that with a fixed inflation of daughter cells, the energy release rate depends on the crack length non-monotonically. The energy release rate reaches a maximum value for a crack of an intermediate length. The non-monotonic relationship between the energy release rate and crack length clearly indicates that the crack propagation in the peripheral <span class="hlt">ring</span> can be unstable. The computed energy release rate as a function of crack length can also be used to explain the existence of a small portion of peripheral <span class="hlt">ring</span> remained as hinge after the popping <span class="hlt">event</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_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/49819','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/49819"><span>How does rapidly changing discharge during storm <span class="hlt">events</span> affect transient <span class="hlt">storage</span> and channel water balance in a headwater mountain stream?</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Adam S. Ward; Michael N. Gooseff; Thomas J. Voltz; Michael Fitzgerald; Kamini Singha; Jay P. Zarnetske</p> <p>2013-01-01</p> <p>Measurements of transient <span class="hlt">storage</span> in coupled surface-water and groundwater systems are widely made during base flow periods and rarely made during storm flow periods. We completed 24 sets of slug injections in three contiguous study reaches during a 1.25 year return interval storm <span class="hlt">event</span> (discharge ranging from 21.5 to 434 L s1 ) in a net gaining headwater stream within...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..APR.D1007L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..APR.D1007L"><span>Geophysical Measurements Using a <span class="hlt">Ring</span> Laser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lamb, Angela</p> <p>2016-03-01</p> <p>Low frequency infrasound from weather related <span class="hlt">events</span> has been studied for a number of years. In this poster, the results from using a large active <span class="hlt">ring</span> laser as an infrasound detector are presented. A slightly modified cavity design enhances the interferometer's sensitivity to infrasound. Our results qualitatively agree with several findings from a long term study of weather generated infrasound by NOAA. On April 27, 2014, the 66 km track of an EF-4 tornado passed within 21 km of the <span class="hlt">ring</span> laser interferometer. An FFT of the <span class="hlt">ring</span> laser interferometer output revealed a steady tornado generated frequency of 0.94 Hz. The track also passed close to the US Array Transportable Station W41B. This provided the opportunity to examine both the infrasound and ground motion generated by the tornado. Infrasound from three other tornadoes is also included. In all cases the infrasound was detected approximately 30 minutes before the tornado funnel was observed. This work is generously supported by the National Science Foundation and NASA/Arkansas Space Grant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982SbMat..43..485T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982SbMat..43..485T"><span>Integrally Closed <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tuganbaev, A. A.</p> <p>1982-04-01</p> <p>This paper studies integrally closed <span class="hlt">rings</span>. It is shown that a semiprime integrally closed Goldie <span class="hlt">ring</span> is the direct product of a semisimple artinian <span class="hlt">ring</span> and a finite number of integrally closed invariant domains that are classically integrally closed in their (division) <span class="hlt">rings</span> of fractions. It is shown also that an integrally closed <span class="hlt">ring</span> has a classical <span class="hlt">ring</span> of fractions and is classically integrally closed in it.Next, integrally closed noetherian <span class="hlt">rings</span> are considered. It is shown that an integrally closed noetherian <span class="hlt">ring</span> all of whose nonzero prime ideals are maximal is either a quasi-Frobenius <span class="hlt">ring</span> or a hereditary invariant domain.Finally, those noetherian <span class="hlt">rings</span> all of whose factor <span class="hlt">rings</span> are invariant are described, and the connection between integrally closed <span class="hlt">rings</span> and distributive <span class="hlt">rings</span> is examined.Bibliography: 13 titles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23633314','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23633314"><span>Skin patch and vaginal <span class="hlt">ring</span> versus combined oral contraceptives for contraception.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lopez, Laureen M; Grimes, David A; Gallo, Maria F; Stockton, Laurie L; Schulz, Kenneth F</p> <p>2013-04-30</p> <p> likely to have missed days of therapy (OR 0.36; 95% CI 0.25 to 0.51). Of four vaginal <span class="hlt">ring</span> trials, one found <span class="hlt">ring</span> users had more noncompliance (OR 3.99; 95% CI 1.87 to 8.52), while another showed more compliance with the regimen (OR 1.67; 95% CI 1.04 to 2.68).More patch users discontinued early than COC users. ORs from two meta-analyses were 1.59 (95% CI 1.26 to 2.00) and 1.56 (95% CI 1.18 to 2.06) and another trial showed OR 2.57 (95% CI 0.99 to 6.64). Patch users also had more discontinuation due to adverse <span class="hlt">events</span> than COC users. Users of the norelgestromin-containing patch reported more breast discomfort, dysmenorrhea, nausea, and vomiting. In the levonorgestrel-containing patch trial, patch users reported less vomiting, headaches, and fatigue.Of 11 <span class="hlt">ring</span> trials with discontinuation data, two showed the <span class="hlt">ring</span> group discontinued less than the COC group: OR 0.32 (95% CI 0.16 to 0.66) and OR 0.52 (95% CI 0.31 to 0.88). <span class="hlt">Ring</span> users were less likely to discontinue due to adverse <span class="hlt">events</span> in one study (OR 0.32; 95% CI 0.15 to 0.70). Compared to the COC users, <span class="hlt">ring</span> users had more vaginitis and leukorrhea but less vaginal dryness. <span class="hlt">Ring</span> users also reported less nausea, acne, irritability, depression, and emotional lability than COC users.For cycle control, only one trial study showed a significant difference. Women in the patch group were less likely to have breakthrough bleeding and spotting. Seven <span class="hlt">ring</span> studies had bleeding data; four trials showed the <span class="hlt">ring</span> group generally had better cycle control than the COC group. Effectiveness was not significantly different for the methods compared. Pregnancy data were available from half of the patch trials but two-thirds of <span class="hlt">ring</span> trials. The patch could lead to more discontinuation than the COC. The patch group had better compliance than the COC group. Compliance data came from half of the patch studies and one-third of the <span class="hlt">ring</span> trials. Patch users had more side effects than the COC group. <span class="hlt">Ring</span> users generally had fewer adverse <span class="hlt">events</span> than</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010DPS....42.5006B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010DPS....42.5006B"><span>Mapping <span class="hlt">Ring</span> Particle Cooling across Saturn's <span class="hlt">Rings</span> with Cassini CIRS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brooks, Shawn M.; Spilker, L. J.; Edgington, S. G.; Pilorz, S. H.; Deau, E.</p> <p>2010-10-01</p> <p>Previous studies have shown that the <span class="hlt">rings</span>' thermal inertia, a measure of their response to changes in the thermal environment, varies from <span class="hlt">ring</span> to <span class="hlt">ring</span>. Thermal inertia can provide insight into the physical structure of Saturn's <span class="hlt">ring</span> particles and their regoliths. Low thermal inertia and quick temperature responses are suggestive of <span class="hlt">ring</span> particles that have more porous or fluffy regoliths or that are riddled with cracks. Solid, coherent particles can be expected to have higher thermal inertias (Ferrari et al. 2005). Cassini's Composite Infrared Spectrometer has recorded millions of spectra of Saturn's <span class="hlt">rings</span> since its arrival at Saturn in 2004 (personal communication, M. Segura). CIRS records far infrared radiation between 10 and 600 cm-1 (16.7 and 1000 µm) at focal plane 1 (FP1), which has a field of view of 3.9 mrad. Thermal emission from Saturn's <span class="hlt">rings</span> peaks in this wavelength range. FP1 spectra can be used to infer <span class="hlt">ring</span> temperatures. By tracking how <span class="hlt">ring</span> temperatures vary, we can determine the thermal inertia of the <span class="hlt">rings</span>. In this work we focus on CIRS observations of the shadowed portion of Saturn's <span class="hlt">rings</span>. The thermal budget of the <span class="hlt">rings</span> is dominated by the solar radiation absorbed by its constituent particles. When <span class="hlt">ring</span> particles enter Saturn's shadow this source of energy is abruptly cut off. As a result, <span class="hlt">ring</span> particles cool as they traverse Saturn's shadow. From these shadow observations we can create cooling curves at specific locations across the <span class="hlt">rings</span>. We will show that the <span class="hlt">rings</span>' cooling curves and thus their thermal inertia vary not only from <span class="hlt">ring</span> to <span class="hlt">ring</span>, but by location within the individual <span class="hlt">rings</span>. This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. Copyright 2010 California Institute of Technology. Government sponsorship acknowledged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1011078','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1011078"><span>Ray Tracing through the Edge Focusing of Rectangular Benders and an Improved Model for the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</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>Kolski, Jeffrey S.; Barlow, David B.; Macek, Robert J.</p> <p>2011-01-01</p> <p>Particle ray tracing through simulated 3D magnetic fields was executed to investigate the effective quadrupole strength of the edge focusing of the rectangular bending magnets in the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> (PSR). The particle rays receive a kick in the edge field of the rectangular dipole. A focal length may be calculated from the particle tracking and related to the fringe field integral (FINT) model parameter. This tech note introduces the baseline lattice model of the PSR and motivates the need for an improvement in the baseline model's vertical tune prediction, which differs from measurement by .05. An improvedmore » model of the PSR is created by modifying the fringe field integral parameter to those suggested by the ray tracing investigation. This improved model is then verified against measurement at the nominal PSR operating set point and at set points far away from the nominal operating conditions. Lastly, Linear Optics from Closed Orbits (LOCO) is employed in an orbit response matrix method for model improvement to verify the quadrupole strengths of the improved model.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940012024','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940012024"><span>Modal <span class="hlt">ring</span> method for the scattering of sound</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Baumeister, Kenneth J.; Kreider, Kevin L.</p> <p>1993-01-01</p> <p>The modal element method for acoustic scattering can be simplified when the scattering body is rigid. In this simplified method, called the modal <span class="hlt">ring</span> method, the scattering body is represented by a <span class="hlt">ring</span> of triangular finite elements forming the outer surface. The acoustic pressure is calculated at the element nodes. The pressure in the infinite computational region surrounding the body is represented analytically by an eigenfunction expansion. The two solution forms are coupled by the continuity of pressure and velocity on the body surface. The modal <span class="hlt">ring</span> method effectively reduces the two-dimensional scattering problem to a one-dimensional problem capable of handling very high frequency scattering. In contrast to the boundary element method or the method of moments, which perform a similar reduction in problem dimension, the model line method has the added advantage of having a highly banded solution matrix requiring considerably less computer <span class="hlt">storage</span>. The method shows excellent agreement with analytic results for scattering from rigid circular cylinders over a wide frequency range (1 is equal to or less than ka is less than or equal to 100) in the near and far fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/875817','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/875817"><span>The Effect of Gas Ion Bombardment on the Secondary Electron Yield of TiN, TiCN and TiZrV Coatings For Suppressing Collective Electron Effects in <span class="hlt">Storage</span> <span class="hlt">Rings</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>Le Pimpec, F.; /PSI, Villigen; Kirby, R.E.</p> <p></p> <p>In many accelerator <span class="hlt">storage</span> <span class="hlt">rings</span> running positively charged beams, ionization of residual gas and secondary electron emission (SEE) in the beam pipe will give rise to an electron cloud which can cause beam blow-up or loss of the circulating beam. A preventative measure that suppresses electron cloud formation is to ensure that the vacuum wall has a low secondary emission yield (SEY). The SEY of thin films of TiN, sputter deposited Non-Evaporable Getters and a novel TiCN alloy were measured under a variety of conditions, including the effect of re-contamination from residual gas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29788327','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29788327"><span>Tree-<span class="hlt">ring</span> proxies of larch bud moth defoliation: latewood width and blue intensity are more precise than tree-<span class="hlt">ring</span> width.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Arbellay, Estelle; Jarvis, Ingrid; Chavardès, Raphaël D; Daniels, Lori D; Stoffel, Markus</p> <p>2018-05-19</p> <p>Reconstructions of defoliation by larch bud moth (LBM, Zeiraphera diniana Gn.) based on European larch (Larix decidua Mill.) tree <span class="hlt">rings</span> have unraveled outbreak patterns over exceptional temporal and spatial scales. In this study, we conducted tree-<span class="hlt">ring</span> analyses on 105 increment cores of European larch from the Valais Alps, Switzerland. The well-documented history of LBM outbreaks in Valais provided a solid baseline for evaluating the LBM defoliation signal in multiple tree-<span class="hlt">ring</span> parameters. First, we used tree-<span class="hlt">ring</span> width measurements along with regional records of LBM outbreaks to reconstruct the occurrence of these <span class="hlt">events</span> at two sites within the Swiss Alps. Second, we measured earlywood width, latewood width and blue intensity, and compared these parameters with tree-<span class="hlt">ring</span> width to assess the capacity of each proxy to detect LBM defoliation. A total of six LBM outbreaks were reconstructed for the two sites between AD 1850 and 2000. Growth suppression induced by LBM was, on average, highest in latewood width (59%), followed by total <span class="hlt">ring</span> width (54%), earlywood width (51%) and blue intensity (26%). We show that latewood width and blue intensity can improve the temporal accuracy of LBM outbreak reconstructions, as both proxies systematically detected LBM defoliation in the first year it occurred, as well as the differentiation between defoliation and non-defoliation years. This study introduces blue intensity as a promising new proxy of insect defoliation and encourages its use in conjunction with latewood width.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4944129','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4944129"><span>A C2HC zinc finger is essential for the <span class="hlt">RING-E</span>2 interaction of the ubiquitin ligase RNF125</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bijlmakers, Marie-José; Teixeira, João M. C.; Boer, Roeland; Mayzel, Maxim; Puig-Sàrries, Pilar; Karlsson, Göran; Coll, Miquel; Pons, Miquel; Crosas, Bernat</p> <p>2016-01-01</p> <p>The activity of <span class="hlt">RING</span> ubiquitin ligases (E3s) depends on an interaction between the <span class="hlt">RING</span> domain and ubiquitin conjugating enzymes (E2), but posttranslational <span class="hlt">events</span> or additional structural elements, yet largely undefined, are frequently required to enhance or regulate activity. Here, we show for the ubiquitin ligase RNF125 that, in addition to the <span class="hlt">RING</span> domain, a C2HC Zn finger (ZnF) is crucial for activity, and a short linker sequence (Li2120-128) enhances activity. The contribution of these regions was first shown with truncated proteins, and the essential role of the ZnF was confirmed with mutations at the Zn chelating Cys residues. Using NMR, we established that the C2HC ZnF/Li2120-128 region is crucial for binding of the <span class="hlt">RING</span> domain to the E2 UbcH5a. The partial X-ray structure of RNF125 revealed the presence of extensive intramolecular interactions between the <span class="hlt">RING</span> and C2HC ZnF. A mutation at one of the contact residues in the C2HC ZnF, a highly conserved M112, resulted in the loss of ubiquitin ligase activity. Thus, we identified the structural basis for an essential role of the C2HC ZnF and conclude that this domain stabilizes the <span class="hlt">RING</span> domain, and is therefore required for binding of RNF125 to an E2. PMID:27411375</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.475.4055M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.475.4055M"><span>GASP. V. Ram-pressure stripping of a <span class="hlt">ring</span> Hoag's-like galaxy in a massive cluster</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moretti, A.; Poggianti, B. M.; Gullieuszik, M.; Mapelli, M.; Jaffé, Y. L.; Fritz, J.; Biviano, A.; Fasano, G.; Bettoni, D.; Vulcani, B.; D'Onofrio, M.</p> <p>2018-04-01</p> <p>Through an ongoing MUSE program dedicated to study gas removal processes in galaxies (GAs Stripping Phenomena in galaxies with MUSE, GASP), we have obtained deep and wide integral field spectroscopy of the galaxy JO171. This galaxy resembles the Hoag's galaxy, one of the most spectacular examples of <span class="hlt">ring</span> galaxies, characterized by a completely detached <span class="hlt">ring</span> of young stars surrounding a central old spheroid. At odds with the isolated Hoag's galaxy, JO171 is part of a dense environment, the cluster Abell 3667, which is causing gas stripping along tentacles. Moreover, its <span class="hlt">ring</span> counter-rotates with respect to the central spheroid. The joint analysis of the stellar populations and the gas/stellar kinematics shows that the origin of the <span class="hlt">ring</span> was not due to an internal mechanism, but was related to a gas accretion <span class="hlt">event</span> that happened in the distant past, prior to accretion on to Abell 3667, most probably within a filament. More recently, since infall in the cluster, the gas in the <span class="hlt">ring</span> has been stripped by ram pressure, causing the quenching of star formation in the stripped half of the <span class="hlt">ring</span>. This is the first observed case of ram-pressure stripping in action in a <span class="hlt">ring</span> galaxy, and MUSE observations are able to reveal both of the <span class="hlt">events</span> (accretion and stripping) that caused dramatic transformations in this galaxy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910028543&hterms=midi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmidi','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910028543&hterms=midi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmidi"><span><span class="hlt">Ring</span> dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borderies, Nicole</p> <p>1989-01-01</p> <p>Theoretical models of planetary-<span class="hlt">ring</span> dynamics are discussed in a detailed analytical review and illustrated with graphs and diagrams. The streamline concept is introduced, and the phenomena associated with the transport of angular momentum are described. Particular attention is then given to (1) broad <span class="hlt">rings</span> like those of Saturn (shepherding, density-wave excitation, gaps, bending-wave excitation, multiringlet structures, inner-edge shepherding, and the possibility of polar <span class="hlt">rings</span> around Neptune), (2) narrow <span class="hlt">rings</span> like those of Uranus (shepherding, <span class="hlt">ring</span> shapes, and a self-gravity model of rigid precession), and (3) <span class="hlt">ring</span> arcs like those seen in stellar-occultation observations of Neptune.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17306861','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17306861"><span>Arsenic in tree <span class="hlt">rings</span> at a highly contaminated site.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cheng, Zhongqi; Buckley, Brendan M; Katz, Beth; Wright, William; Bailey, Richard; Smith, Kevin T; Li, Jingbo; Curtis, Ashley; Geen, Alexander van</p> <p>2007-04-15</p> <p>Arsenic concentrations were measured in annual <span class="hlt">rings</span>, pith, bark, and leaves of five tree species (four genera) from a site highly contaminated with As in Vineland, New Jersey, and two nearby uncontaminated areas. The highest As concentrations were found in bark (0.68+/-0.89 mg/kg, n=16) and leaves (1.9+/-1.8 mg/kg, n=4) from the contaminated area. Tree-<span class="hlt">ring</span> As levels from the contaminated area (0.28+/-0.15 mg/kg, n=32) were low but still considerably higher than those from the control areas (0.06+/-0.06 mg/kg, n=30). There is a generally positive relationship between soil and tree-<span class="hlt">ring</span> As levels. The overall low uptake of As by trees contrasts with that of P, a chemical analog for As(V) in aerated soils. Much higher P concentration in sapwood than in heartwood indicates that P is exported into more recently formed wood during the conversion from sapwood to heartwood; this again is drastically different than the behavior of As which is present in sapwood and heartwood at comparable levels. Variable sapwood As concentrations observed in detailed radial profiles of tree-<span class="hlt">ring</span> chemistry of a pine and an oak from the contaminated site suggest that As is most likely transported among multiple <span class="hlt">rings</span> within the sapwood. Therefore, tree species for which sapwood is thin (e.g., oak as in this study) should be preferred for reconstructing the history of contamination of a site. Due to the possibility of lateral translocation between growth <span class="hlt">rings</span>, further studies are necessary to understand within-tree As transport and <span class="hlt">storage</span> before dendrochemistry can be confidently accepted for such applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1425799','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1425799"><span>Development of a Bunched Beam Electron Cooler based on ERL and Circulator <span class="hlt">Ring</span> Technology for the Jefferson Lab Electron-Ion Collider</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>Benson, Stephen V.; Derbenev, Yaroslav S.; Douglas, David R.</p> <p></p> <p>Jefferson Lab is in the process of designing an electron ion collider with unprecedented luminosity at a 45 GeV center-of-mass energy. This luminosity relies on ion cooling in both the booster and the <span class="hlt">storage</span> <span class="hlt">ring</span> of the accelerator complex. The cooling in the booster will use a conventional DC cooler similar to the one at COSY. The high-energy <span class="hlt">storage</span> <span class="hlt">ring</span>, operating at a momentum of up to 100 GeV/nucleon, requires novel use of bunched-beam cooling. There are two designs for such a cooler. The first uses a conventional Energy Recovery Linac (ERL) with a magnetized beam while the second usesmore » a circulating <span class="hlt">ring</span> to enhance both peak and average currents experienced by the ion beam. This presentation will describe the design of both the Circulator Cooling <span class="hlt">Ring</span> (CCR) design and that of the backup option using the stand-alone ERL operated at lower charge but higher repetition rate than the ERL injector required by the CCR-based design.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SGeo...39....1N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SGeo...39....1N"><span>Global Terrestrial Water <span class="hlt">Storage</span> Changes and Connections to ENSO <span class="hlt">Events</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ni, Shengnan; Chen, Jianli; Wilson, Clark R.; Li, Jin; Hu, Xiaogong; Fu, Rong</p> <p>2018-01-01</p> <p>Improved data quality of extended record of the Gravity Recovery and Climate Experiment (GRACE) satellite gravity solutions enables better understanding of terrestrial water <span class="hlt">storage</span> (TWS) variations. Connections of TWS and climate change are critical to investigate regional and global water cycles. In this study, we provide a comprehensive analysis of global connections between interannual TWS changes and El Niño Southern Oscillation (ENSO) <span class="hlt">events</span>, using multiple sources of data, including GRACE measurements, land surface model (LSM) predictions and precipitation observations. We use cross-correlation and coherence spectrum analysis to examine global connections between interannual TWS changes and the Niño 3.4 index, and select four river basins (Amazon, Orinoco, Colorado, and Lena) for more detailed analysis. The results indicate that interannual TWS changes are strongly correlated with ENSO over much of the globe, with maximum cross-correlation coefficients up to 0.70, well above the 95% significance level ( 0.29) derived by the Monte Carlo experiments. The strongest correlations are found in tropical and subtropical regions, especially in the Amazon, Orinoco, and La Plata basins. While both GRACE and LSM TWS estimates show reasonably good correlations with ENSO and generally consistent spatial correlation patterns, notably higher correlations are found between GRACE TWS and ENSO. The existence of significant correlations in middle-high latitudes shows the large-scale impact of ENSO on the global water cycle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC24G..03P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC24G..03P"><span>Inferring biome-scale net primary productivity from tree-<span class="hlt">ring</span> isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pederson, N.; Levesque, M.; Williams, A. P.; Hobi, M. L.; Smith, W. K.; Andreu-Hayles, L.</p> <p>2017-12-01</p> <p>Satellite estimates of vegetation growth (net primary productivity; NPP), tree-<span class="hlt">ring</span> records, and forest inventories indicate that ongoing climate change and rising atmospheric CO2 concentration are altering productivity and carbon <span class="hlt">storage</span> of forests worldwide. The impact of global change on the trends of NPP, however, remain unknown because of the lack of long-term high-resolution NPP data. For the first time, we tested if annually resolved carbon (δ13C) and oxygen (δ18O) stable isotopes from the cellulose of tree <span class="hlt">rings</span> from trees in temperate regions could be used as a tool for inferring NPP across spatiotemporal scales. We compared satellite NPP estimates from the moderate-resolution imaging spectroradiometer sensor (MODIS, product MOD17A) and a newly developed global NPP dataset derived from the Global Inventory Modeling and Mapping Studies (GIMMS) dataset to annually resolved tree-<span class="hlt">ring</span> width and δ13C and δ18O records from four sites along a hydroclimatic gradient in Eastern and Central United States. We found strong correlations across large geographical regions between satellite-derived NPP and tree-<span class="hlt">ring</span> isotopes that ranged from -0.40 to -0.91. Notably, tree-<span class="hlt">ring</span> derived δ18O had the strongest relation to climate. The results were consistent among the studied tree species (Quercus rubra and Liriodendron tulipifera) and along the hydroclimatic conditions of our network. Our study indicates that tree-<span class="hlt">ring</span> isotopes can potentially be used to reconstruct NPP in time and space. As such, our findings represent an important breakthrough for estimating long-term changes in vegetation productivity at the biome scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100005268','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100005268"><span>High-Speed <span class="hlt">Ring</span> Bus</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wysocky, Terry; Kopf, Edward, Jr.; Katanyoutananti, Sunant; Steiner, Carl; Balian, Harry</p> <p>2010-01-01</p> <p> is no centralized arbitration or bus granting. The JPL design provides for autonomous synchronization of the nodes on the <span class="hlt">ring</span> bus. An address-synchronous latency adjust buffer (LAB) has been designed that cannot get out of synchronization and needs no external input. Also, a priority-driven cable selection behavior has been programmed into each unit on the <span class="hlt">ring</span> bus. This makes the bus able to connect itself up, according to a maximum redundancy priority system, without the need for computer intervention at startup. Switching around a failed or switched-off unit is also autonomous. The JPL bus provides a map of all the active units for the host computer to read and use for fault management. With regard to timing, this enhanced bus recognizes coordinated timing on a spacecraft as critical and addresses this with a single source of absolute and relative time, which is broadcast to all units on the bus with synchronization maintained to the tens of nanoseconds. Each BIU consists of up to five programmable triggers, which may be programmed for synchronization of <span class="hlt">events</span> within the spacecraft of instrument. All JPL-formatted data transmitted on the <span class="hlt">ring</span> bus are automatically time-stamped.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007CosRe..45...39R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007CosRe..45...39R"><span>Planetary <span class="hlt">rings</span> as relics of plasma pre-<span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabinovich, B. I.</p> <p>2007-02-01</p> <p>A possibility is discussed that the <span class="hlt">rings</span> of large planets observed in the modern epoch are relics of some pre-<span class="hlt">rings</span> consisting of magnetized plasma (according to a hypothesis by H. Alfven). The solution to a model problem published in [36, 37] is used. Its main result is a mechanism of stratification of an evolutionally mature plasma pre-<span class="hlt">ring</span> into a large number of narrow elite <span class="hlt">rings</span> separated by anti-<span class="hlt">rings</span> (gaps). Another result is the theoretical substantiation of the presence in the near-planetary space of a region of existence and stability (in what follows it is referred to as ES-region) of plasma <span class="hlt">rings</span>. The data obtained in the course of the Voyager, Galileo, and Cassini missions are used below for verification of the model on which the solutions presented in [36, 37] are based.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012MS%26E...36a2015A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012MS%26E...36a2015A"><span>Computational Analysis on Performance of Thermal Energy <span class="hlt">Storage</span> (TES) Diffuser</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adib, M. A. H. M.; Adnan, F.; Ismail, A. R.; Kardigama, K.; Salaam, H. A.; Ahmad, Z.; Johari, N. H.; Anuar, Z.; Azmi, N. S. N.</p> <p>2012-09-01</p> <p>Application of thermal energy <span class="hlt">storage</span> (TES) system reduces cost and energy consumption. The performance of the overall operation is affected by diffuser design. In this study, computational analysis is used to determine the thermocline thickness. Three dimensional simulations with different tank height-to-diameter ratio (HD), diffuser opening and the effect of difference number of diffuser holes are investigated. Medium HD tanks simulations with double <span class="hlt">ring</span> octagonal diffuser show good thermocline behavior and clear distinction between warm and cold water. The result show, the best performance of thermocline thickness during 50% time charging occur in medium tank with height-to-diameter ratio of 4.0 and double <span class="hlt">ring</span> octagonal diffuser with 48 holes (9mm opening ~ 60%) acceptable compared to diffuser with 6mm ~ 40% and 12mm ~ 80% opening. The conclusion is computational analysis method are very useful in the study on performance of thermal energy <span class="hlt">storage</span> (TES).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002ASPC..272..263G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002ASPC..272..263G"><span>Planetary <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gordon, M. K.; Araki, S.; Black, G. J.; Bosh, A. S.; Brahic, A.; Brooks, S. M.; Charnoz, S.; Colwell, J. E.; Cuzzi, J. N.; Dones, L.; Durisen, R. H.; Esposito, L. W.; Ferrari, C.; Festou, M.; French, R. G.; Giuliatti-Winter, S. M.; Graps, A. L.; Hamilton, D. P.; Horanyi, M.; Karjalainen, R. M.; Krivov, A. V.; Krueger, H.; Larson, S. M.; Levison, H. F.; Lewis, M. C.; Lissauer, J. J.; Murray, C. D.; Namouni, F.; Nicholson, P. D.; Olkin, C. B.; Poulet, F.; Rappaport, N. J.; Salo, H. J.; Schmidt, J.; Showalter, M. R.; Spahn, F.; Spilker, L. J.; Srama, R.; Stewart, G. R.; Yanamandra-Fisher, P.</p> <p>2002-08-01</p> <p>The past two decades have witnessed dramatic changes in our view and understanding of planetary <span class="hlt">rings</span>. We now know that each of the giant planets in the Solar System possesses a complex and unique <span class="hlt">ring</span> system. Recent studies have identified complex gravitational interactions between the <span class="hlt">rings</span> and their retinues of attendant satellites. Among the four known <span class="hlt">ring</span> systems, we see elegant examples of Lindblad and corotation resonances (first invoked in the context of galactic disks), electromagnetic resonances, spiral density waves and bending waves, narrow ringlets which exhibit internal modes due to collective instabilities, sharp-edged gaps maintained via tidal torques from embedded moonlets, and tenuous dust belts created by meteoroid impact onto, or collisions between, parent bodies. Yet, as far as we have come, our understanding is far from complete. The fundamental questions confronting <span class="hlt">ring</span> scientists at the beginning of the twenty-first century are those regarding the origin, age and evolution of the various <span class="hlt">ring</span> systems, in the broadest context. Understanding the origin and age requires us to know the current <span class="hlt">ring</span> properties, and to understand the dominant evolutionary processes and how they influence <span class="hlt">ring</span> properties. Here we discuss a prioritized list of the key questions, the answers to which would provide the greatest improvement in our understanding of planetary <span class="hlt">rings</span>. We then outline the initiatives, missions, and other supporting activities needed to address those questions, and recommend priorities for the coming decade in planetary <span class="hlt">ring</span> science.</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('http://adsabs.harvard.edu/abs/2017AGUFM.H13L..06S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H13L..06S"><span>Daily GRACE <span class="hlt">storage</span> anomaly data for characterization of dynamic <span class="hlt">storage</span>-discharge relationships of natural drainage basins</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharma, D.; Patnaik, S.; Reager, J. T., II; Biswal, B.</p> <p>2017-12-01</p> <p>Despite the fact that streamflow occurs mainly due to depletion of <span class="hlt">storage</span>, our knowledge on how a drainage basin stores and releases water is very limited because of measurement limitations. As a result <span class="hlt">storage</span> has largely remained an elusive entity in hydrological analysis and modelling. A window of opportunity, however, is given to us by GRACE satellite mission that provides <span class="hlt">storage</span> anomaly (TWSA) data for the entire globe. Many studies have used TWSA data for <span class="hlt">storage</span>-discharge analysis, uncovering a range of potential applications of TWSA data. Here we argue that the capability of GRACE satellite mission has not been fully explored as most of the studies in the past have performed <span class="hlt">storage</span>-discharge analysis using monthly TWSA data for large river basins. With such coarse data we are quite unlikely to fully understand variation of <span class="hlt">storage</span> and discharge in space and time. In this study, we therefore use daily TWSA data for several mid-sized catchments and perform <span class="hlt">storage</span>-discharge analysis. Daily <span class="hlt">storage</span>-discharge relationship is highly dynamic, which generates large amount of scatter in <span class="hlt">storage</span>-discharge plots. Yet a careful analysis of those scatter plots reveals interesting information on <span class="hlt">storage</span>-discharge relationships of basins, particularly by looking at the relationships during individual recession <span class="hlt">events</span>. It is observed that <span class="hlt">storage</span>-discharge relationship is exponential in nature, contrary to the general assumption that the relationship is linear. We find that there is a strong relationship between power-law recession coefficient and initial <span class="hlt">storage</span> (TWSA at the beginning of recession <span class="hlt">event</span>). Furthermore, appreciable relationships are observed between recession coefficient and past TWSA values implying that <span class="hlt">storage</span> takes time to deplete completely. Overall, insights drawn from this study expands our knowledge on how discharge is dynamically linked to <span class="hlt">storage</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSM32A..08G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSM32A..08G"><span>Global, Energy-Dependent <span class="hlt">Ring</span> Current Response During Two Large Storms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldstein, J.; Angelopoulos, V.; Burch, J. L.; De Pascuale, S.; Fuselier, S. A.; Genestreti, K. J.; Kurth, W. S.; LLera, K.; McComas, D. J.; Reeves, G. D.; Spence, H. E.; Valek, P. W.</p> <p>2015-12-01</p> <p>Two recent large (~200 nT) geomagnetic storms occurred during 17--18 March 2015 and 22--23 June 2015. The global, energy-dependent <span class="hlt">ring</span> current response to these two extreme <span class="hlt">events</span> is investigated using both global imaging and multi-point in situ observations. Energetic neutral atom (ENA) imaging by the Two Wide-angle Imaging Neutral-atom Spectrometers (TWINS) mission provides a global view of <span class="hlt">ring</span> current ions. Local measurements are provided by two multi-spacecraft missions. The two Van Allen Probes measure in situ plasma (including ion composition) and fields at <span class="hlt">ring</span> current and plasmaspheric L values. The recently launched Magnetospheric Multiscale (MMS) comprises four spacecraft that have just begun to measure particles (including ion composition) and fields at outer magnetospheric L-values. We analyze the timing and energetics of the stormtime evolution of <span class="hlt">ring</span> current ions, both trapped and precipitating, using TWINS ENA images and in situ data by the Van Allen Probes and MMS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010PhDT.......202K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010PhDT.......202K"><span>Lattice modeling and application of independent component analysis to high power, long bunch beams in the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kolski, Jeffrey</p> <p></p> <p>The linear lattice properties of the Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> (PSR) at the Los Alamos Neutron Science Center (LANSCE) in Los Alamos, NM were measured and applied to determine a better linear accelerator model. We found that the initial model was deficient in predicting the vertical focusing strength. The additional vertical focusing was located through fundamental understanding of experiment and statistically rigorous analysis. An improved model was constructed and compared against the initial model and measurement at operation set points and set points far away from nominal and was shown to indeed be an enhanced model. Independent component analysis (ICA) is a tool for data mining in many fields of science. Traditionally, ICA is applied to turn-by-turn beam position data as a means to measure the lattice functions of the real machine. Due to the diagnostic setup for the PSR, this method is not applicable. A new application method for ICA is derived, ICA applied along the length of the bunch. The ICA modes represent motions within the beam pulse. Several of the dominate ICA modes are experimentally identified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IzAOP..53..781K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IzAOP..53..781K"><span><span class="hlt">Ring</span>-Shaped Seismicity Structures in Southern California: Possible Preparation for Large Earthquake in the Los Angeles Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kopnichev, Yu. F.; Sokolova, I. N.</p> <p>2017-12-01</p> <p>Some characteristics of seismicity in Southern California are studied. It is found that <span class="hlt">ring</span>-shaped seismicity structures with threshold magnitudes M th of 4.1, 4.1, and 3.8 formed prior to three large ( M w > 7.0) earthquakes in 1992, 1999, and 2010, respectively. The sizes of these structures are several times smaller than for intracontinental strike-slip <span class="hlt">events</span> with similar magnitudes. Two <span class="hlt">ring</span>-shaped structures are identified in areas east of the city of Los Angeles, where relatively large earthquakes have not occurred for at least 150 years. The magnitudes of large <span class="hlt">events</span> which can occur in the areas of these structures are estimated on the basis of the previously obtained correlation dependence of <span class="hlt">ring</span> sizes on magnitudes of the strike-slip earthquakes. Large <span class="hlt">events</span> with magnitudes of M w = 6.9 ± 0.2 and M w = 8.6 ± 0.2 can occur in the area to the east of the city of Los Angeles and in the rupture zone of the 1857 great Fort Tejon earthquake, respectively. We believe that <span class="hlt">ring</span>-structure formation, similarly to the other regions, is connected with deep-seated fluid migration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040171218&hterms=ring+fire&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dring%2Bfire','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040171218&hterms=ring+fire&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dring%2Bfire"><span>Saturn's <span class="hlt">Rings</span>, the Yarkovsky Effects, and the <span class="hlt">Ring</span> of Fire</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubincam, David</p> <p>2004-01-01</p> <p>Saturn's icy <span class="hlt">ring</span> particles, with their low thermal conductivity, are almost ideal for the operation of the Yarkovsky effects. The dimensions of Saturn's A and B <span class="hlt">rings</span> may be determined by a near balancing of the seasonal Yarkovsky effect with the Yarkovsky- Schach effect. The two effects, which are photon thrust due to temperature gradients, may confine the A and B <span class="hlt">rings</span> to within their observed dimensions. The C <span class="hlt">ring</span> may be sparsely populated with icy particles because Yarkovsky drag has pulled them into Saturn, leaving the more slowly orbitally decaying rocky particles. Icy <span class="hlt">ring</span> particles ejected from the B <span class="hlt">ring</span> and passing through the C <span class="hlt">ring</span>, as well as some of the slower rocky particles, should fall on Saturn's equator, where they may create a luminous "<span class="hlt">Ring</span> of Fire" around Saturn's equator. This predicted <span class="hlt">Ring</span> of Fire may be visible to Cassini's camera. Curiously, the speed of outwards Yarkovsky orbital evolution appears to peak near the Cassini Division. The connection between the two is not clear. D. Nesvorny has speculated that the resonance at the outer edge of the B <span class="hlt">ring</span> may impede particles from evolving via Yarkovsky across the Division. If supply from the B <span class="hlt">ring</span> is largely cut off, then Yarkovsky may push icy particles outward, away from the inner edge of the A <span class="hlt">ring</span>, leaving only the rocky ones in the Division. The above scenarios depend delicately on the properties of the icy particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.P23B1629B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.P23B1629B"><span>Variations in <span class="hlt">Ring</span> Particle Cooling across Saturn's <span class="hlt">Rings</span> with Cassini CIRS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brooks, S. M.; Spilker, L. J.; Pilorz, S.; Edgington, S. G.; Déau, E.; Altobelli, N.</p> <p>2010-12-01</p> <p>Cassini's Composite Infrared Spectrometer has recorded over two million of spectra of Saturn's <span class="hlt">rings</span> in the far infrared since arriving at Saturn in 2004. CIRS records far infrared radiation between 10 and 600 cm-1 ( 16.7 and 1000 μ {m} ) at focal plane 1 (FP1), which has a field of view of 3.9 mrad. Thermal emission from Saturn’s <span class="hlt">rings</span> peaks in this wavelength range. <span class="hlt">Ring</span> temperatures can be inferred from FP1 data. By tracking how <span class="hlt">ring</span> temperatures vary, we can determine the thermal inertia of the <span class="hlt">rings</span>. Previous studies have shown that the <span class="hlt">rings</span>' thermal inertia, a measure of their response to changes in the thermal environment, varies from <span class="hlt">ring</span> to <span class="hlt">ring</span>. Thermal inertia can provide insight into the physical structure of Saturn's <span class="hlt">ring</span> particles and their regoliths. Low thermal inertia and rapidly changing temperatures are suggestive of <span class="hlt">ring</span> particles that have more porous or fluffy regoliths or that are riddled with cracks. Solid particles can be expected to have higher thermal inertias. Ferrari et al. (2005) fit thermal inertia values of 5218 {Jm)-2 {K}-1 {s}-1/2 to their B <span class="hlt">ring</span> data and 6412 {Jm)-2 {K}-1 {s}-1/2 to their C <span class="hlt">ring</span> data. In this work we focus on CIRS observations of the shadowed portion of Saturn's <span class="hlt">rings</span>. The rings’ thermal budget is dominated by its absorption of solar radiation. As a result, <span class="hlt">ring</span> particles abruptly cool as they traverse Saturn's shadow. From these shadow observations we can create cooling curves at specific locations across the <span class="hlt">rings</span>. We will show that the <span class="hlt">rings</span>' cooling curves and thus their thermal inertia vary not only from <span class="hlt">ring</span> to <span class="hlt">ring</span>, but by location within the individual <span class="hlt">rings</span>. This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. Copyright 2010 California Institute of Technology. Government sponsorship acknowledged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1335112','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1335112"><span>Delivery <span class="hlt">Ring</span> Lattice Modifications for Transitionless Deceleration</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>Johnstone, J. A.; Syphers, M. J.</p> <p>2016-10-09</p> <p>A portion of the remnant Tevatron program infrastruc- ture at Fermilab is being reconfigured to be used for the generation and delivery of proton and muon beams for new high-precision particle physics experiments. With the 8 GeV Booster as its primary source, the Mu2e exper- iment will receive 8.9 GeV/c bunched beam on target, after being stored and slow spilled from the Delivery <span class="hlt">Ring</span> (DR) -- a refurbished debuncher <span class="hlt">ring</span> from Tevatron anti- proton production. For the Muon g-2 experiment, the DR will be tuned for 3.1 GeV/c to capture muons off of a target before sending them to thismore » experiment's <span class="hlt">Storage</span> <span class="hlt">Ring</span>. The apertures in the beam transport systems are optimized for the large muon beams of this lower-energy experiment. In order to provide further flexibility in the operation of the DR for future possible low-energy, high- intensity particle physics experiments (REDTOP[1], for example) and detector development, investigations are underway into the feasibility of decelerating beams from its maximum kinetic energy of 8 GeV level to lower en- ergies, down to 1-2 GeV. In this paper we look at possi- ble lattice modifications to the DR to avoid a transition crossing during the deceleration process. Hardware re- quirements and other operational implications of this scheme will also be discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H43K1786A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H43K1786A"><span>Dynamic Water <span class="hlt">Storage</span> during Flash Flood <span class="hlt">Events</span> in the Mountainous Area of Rio de Janeiro/Brazil - Case study: Piabanha River Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Araujo, L.; Silva, F. P. D.; Moreira, D. M.; Vásquez P, I. L.; Justi da Silva, M. G. A.; Fernandes, N.; Rotunno Filho, O. C.</p> <p>2017-12-01</p> <p>Flash floods are characterized by a rapid rise in water levels, high flow rates and large amounts of debris. Several factors have relevance to the occurrence of these phenomena, including high precipitation rates, terrain slope, soil saturation degree, vegetation cover, soil type, among others. In general, the greater the precipitation intensity, the more likely is the occurrence of a significant increase in flow rate. Particularly on steep and rocky plains or heavily urbanized areas, relatively small rain rates can trigger a flash flood <span class="hlt">event</span>. In addition, high rain rates in short time intervals can temporarily saturate the surface soil layer acting as waterproofing and favoring the occurrence of greater runoff rates due to non-infiltration of rainwater into the soil. Thus, although precipitation is considered the most important factor for flooding, the interaction between rainfall and the soil can sometimes be of greater importance. In this context, this work investigates the dynamic <span class="hlt">storage</span> of water associated with flash flood <span class="hlt">events</span> for Quitandinha river watershed, a tributary of Piabanha river, occurred between 2013 and 2014, by means of water balance analyses applied to three watersheds of varying magnitudes (9.25 km², 260 km² and 429 km²) along the rainy season under different time steps (hourly and daily) using remotely sensed and observational precipitation data. The research work is driven by the hypothesis of a hydrologically active bedrock layer, as the watershed is located in a humid region, having intemperate (fractured) rock layer, just below a shallow soil layer, in the higher part of the basin where steep slopes prevail. The results showed a delay of the variation of the dynamic <span class="hlt">storage</span> in relation to rainfall peaks and water levels. Such behavior indicates that the surface soil layer, which is not very thick in the region, becomes rapidly saturated along rainfall <span class="hlt">events</span>. Subsequently, the water infiltrates into the rocky layer and the water</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.722..175G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.722..175G"><span>Structure and origin of Australian <span class="hlt">ring</span> and dome features with reference to the search for asteroid impact <span class="hlt">events</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Glikson, Andrew</p> <p>2018-01-01</p> <p><span class="hlt">Ring</span>, dome and crater features on the Australian continent and shelf include (A) 38 structures of confirmed or probable asteroid and meteorite impact origin and (B) numerous buried and exposed <span class="hlt">ring</span>, dome and crater features of undefined origin. A large number of the latter include structural and geophysical elements consistent with impact structures, pending test by field investigations and/or drilling. This paper documents and briefly describes 43 <span class="hlt">ring</span> and dome features with the aim of appraising their similarities and differences from those of impact structures. Discrimination between impact structures and igneous plugs, volcanic caldera and salt domes require field work and/or drilling. Where crater-like morphological patterns intersect pre-existing linear structural features and contain central morphological highs and unique thrust and fault patterns an impact connection needs to tested in the field. Hints of potential buried impact structures may be furnished by single or multi-<span class="hlt">ring</span> TMI patterns, circular TMI quiet zones, corresponding gravity patterns, low velocity and non-reflective seismic zones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27331584','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27331584"><span>Surgical Outcomes of Newly Trained Shang<span class="hlt">Ring</span> Circumcision Providers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Awori, Quentin D; Lee, Richard K; Li, Philip S; Zulu, Robert; Agot, Kawango; Combes, Stephanie; Simba, Raymond O; Hart, Catherine; Lai, Jaim Jou; Zyambo, Zude; Goldstein, Marc; Feldblum, Paul J; Barone, Mark A</p> <p>2016-06-01</p> <p>Devices can potentially accelerate scale-up of voluntary medical male circumcision in sub-Saharan Africa. Studies have demonstrated advantages of the Shang<span class="hlt">Ring</span> device over conventional circumcision. With the need to train providers rapidly for scale-up, concerns arise about the transferability of techniques and the expertise of new trainees. We compared outcomes of Shang<span class="hlt">Ring</span> circumcisions conducted in Kenya by experienced providers (experience with more than 100 Shang<span class="hlt">Ring</span> circumcisions) and newly trained providers (trained in Kenya by the experienced providers before the study began). During training, trainees performed at least 7 Shang<span class="hlt">Ring</span> circumcisions and 3 removals. Newly trained providers received intermittent clinical mentoring initially during the study but otherwise conducted circumcisions on their own. Four hundred six and 115 Shang<span class="hlt">Ring</span> procedures were performed by the new trainees and the experienced providers, respectively. The mean duration of circumcisions was 6.2 minutes for both trained and experienced provider groups (P = 0.45), whereas the mean pain score (on an 11-point scale) was 2.5 and 3.2, respectively (P = 0.65). There was no difference in the proportion of participants healed by the day 42 visit (P = 0.13) nor in the incidence of moderate and severe adverse <span class="hlt">events</span> observed (P = 0.16). Participants in both groups were equally satisfied with final wound cosmesis. Results demonstrate that the Shang<span class="hlt">Ring</span> circumcision technique is easy to learn and master. Newly trained providers can safely conduct Shang<span class="hlt">Ring</span> circumcisions in routine service settings. The Shang<span class="hlt">Ring</span> can facilitate rapid rollout of voluntary medical male circumcision for HIV prevention in sub-Saharan Africa.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018A%26A...612A..66M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018A%26A...612A..66M"><span>MUSE observations of the counter-rotating nuclear <span class="hlt">ring</span> in NGC 7742</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martinsson, Thomas P. K.; Sarzi, Marc; Knapen, Johan H.; Coccato, Lodovico; Falcón-Barroso, Jesús; Elmegreen, Bruce G.; de Zeeuw, Tim</p> <p>2018-04-01</p> <p>Aims: We present results from MUSE observations of the nearly face-on disk galaxy NGC 7742. This galaxy hosts a spectacular nuclear <span class="hlt">ring</span> of enhanced star formation, which is unusual in that it is hosted by a non-barred galaxy, and because this star formation is most likely fuelled by externally accreted gas that counter-rotates with respect to its main stellar body. Methods: We used the MUSE data to derive the star-formation history (SFH) and accurately measure the stellar and ionized-gas kinematics of NGC 7742 in its nuclear, bulge, <span class="hlt">ring</span>, and disk regions. Results: We have mapped the previously known gas counter-rotation well outside the <span class="hlt">ring</span> region and deduce the presence of a slightly warped inner disk, which is inclined at approximately 6° compared to the outer disk. The gas-disk inclination is well constrained from the kinematics; the derived inclination 13.7° ± 0.4° agrees well with that derived from photometry and from what one expects using the inverse Tully-Fisher relation. We find a prolonged SFH in the <span class="hlt">ring</span> with stellar populations as old as 2-3 Gyr and an indication that the star formation triggered by the minor merger <span class="hlt">event</span> was delayed in the disk compared to the <span class="hlt">ring</span>. There are two separate stellar components: an old population that counter-rotates with the gas, and a young one, concentrated to the <span class="hlt">ring</span>, that co-rotates with the gas. We recover the kinematics of the old stars from a two-component fit, and show that combining the old and young stellar populations results in the erroneous average velocity of nearly zero found from a one-component fit. Conclusions: The spatial resolution and field of view of MUSE allow us to establish the kinematics and SFH of the nuclear <span class="hlt">ring</span> in NGC 7742. We show further evidence that this <span class="hlt">ring</span> has its origin in a minor merger <span class="hlt">event</span>, possibly 2-3 Gyr ago. Data used for the flux and kinematic maps (Figs. 1 and 3-5) are only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1168449','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1168449"><span>Damping <span class="hlt">Ring</span> R&D at CESR-TA</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>Rubin, David L.</p> <p>2015-01-23</p> <p> <span class="hlt">ring</span>, and that an instability associated with residual gas in the beam pipe would limit the intensity of the electron <span class="hlt">ring</span>. It was also not clear whether the required very small beam size could be achieved. The results of this study are important contributions to the design of both the electron and positron damping <span class="hlt">rings</span> in which all of those challenges are addressed and overcome. Our findings are documented in the ILC Technical Design Report, a document that represents the work of an international collaboration of scientists. Our contributions include design of the beam magnetic optics for the 3 km circumference damping <span class="hlt">rings</span>, the vacuum system and surface treatments for electron cloud mitigation, the design of the guide field magnets, design of the superconducting damping wigglers, and new detectors for precision measurement of beam properties. Our study informed the specification of the basic design parameters for the damping <span class="hlt">rings</span>, including alignment tolerances, magnetic field errors, and instrumentation. We developed electron cloud modelling tools and simulations to aid in the interpretation of the measurements that we carried out in the Cornell Electron-positron <span class="hlt">Storage</span> <span class="hlt">Ring</span> (CESR). The simulations provide a means for systematic extrapolation of our measurements at CESR to the proposed ILC damping <span class="hlt">rings</span>, and ultimately to specify how the beam pipes should be fabricated in order to minimize the effects of the electron cloud. With the conclusion of this study, the design of the essential components of the damping <span class="hlt">rings</span> is complete, including the development and characterization (with computer simulations) of the beam optics, specification of techniques for minimizing beam size, design of damping <span class="hlt">ring</span> instrumentation, R&D into electron cloud suppression methods, tests of long term durability of electron cloud coatings, and design of damping <span class="hlt">ring</span> vacuum system components.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AAS...22914519S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AAS...22914519S"><span>The Nonbarred Double-<span class="hlt">Ringed</span> Galaxy, PGC 1000714</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seigar, Marc; Mutlu Pakdil, Burcin; Mangedarage, Mithila; Treuthardt, Patrick M.</p> <p>2017-01-01</p> <p>Hoag-type galaxies are rare peculiar systems which bear strong resemblance to Hoag's Object with an elliptical-like core, a detached outer <span class="hlt">ring</span>, and no signs of a bar or stellar disk. They represent extreme cases and help us understand the formation of galaxies in general by providing clues on formation mechanisms. The nature of outer <span class="hlt">rings</span> in Hoag-type galaxies is still debated and may be related either to slow secular evolution, such as dissolution of a barlike structure or to environmental processes, such as galaxy-galaxy interactions or gas infall. Due to a fairly superficial resemblance to Hoag's Object, PGC 1000714 is a good target for detailed study of the peculiar structure of this type. We present the first photometric study of PGC 1000714 that has not yet been described in the literature. Our aim is to evaluate its structure and properties as well as understand the origin of outer <span class="hlt">rings</span> in such galaxies. Surface photometry of the central body is performed using near-UV, BVRI and JHK images. Based on the photometric data, the nearly round central body follows a de Vaucouleurs profile almost all the way to the center. The detailed photometry reveals a reddish inner <span class="hlt">ring</span>-shaped structure that shares the same center as the central body. However, no sign of a bar or stellar disk is detected. The outer <span class="hlt">ring</span> appears as a bump in the surface brightness profile with a peak brightness of 25.8 mag/arcsec^{2} in the B-band and shows no sharp outer boundary. By reconstructing the observed SED for the central body and the <span class="hlt">rings</span>, we recover the stellar population properties of the galaxy components. Our work suggests different formation histories for the inner and outer <span class="hlt">rings</span>. We rule out the secular evolution model as being a formation mechanism for the outer <span class="hlt">ring</span>. The colors of the outer <span class="hlt">ring</span> are consistent with a feature that may have experienced a burst of star formation due to a possible recent accretion <span class="hlt">event</span>. In addition, our work supports that the central body</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1439005-uranium-mobility-across-annual-growth-rings-three-deciduous-tree-species','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1439005-uranium-mobility-across-annual-growth-rings-three-deciduous-tree-species"><span>Uranium mobility across annual growth <span class="hlt">rings</span> in three deciduous tree species</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>McHugh, Kelly C.; Widom, Elisabeth; Spitz, Henry B.</p> <p></p> <p>Black walnut (Juglans nigra), slippery elm (Ulmus rubra), and white ash (Fraxinus americana) trees were evaluated as potential archives of past uranium (U) contamination. Like other metals, U mobility in annual growth <span class="hlt">rings</span> of trees is potentially dependent on the tree species. Uranium concentrations and isotopic compositions (masses 234, 235, 236, and 238) were analyzed by thermal ionization mass spectrometry to test the efficacy of using tree <span class="hlt">rings</span> to retroactively monitor U pollution from the FFMPC, a U purification facility operating from 1951 to 1989. This study found non-natural U (depleted U and detectable 236U) in growth <span class="hlt">rings</span> of allmore » three tree species that pre-dated the start of operations at FFMPC and compositional trends that did not correspond with known contamination <span class="hlt">events</span>. Therefore, the annual growth <span class="hlt">rings</span> of these tree species cannot be used to reliably monitor the chronology of U contamination.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920062464&hterms=karim&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dkarim','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920062464&hterms=karim&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dkarim"><span>Vortex <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shariff, Karim; Leonard, Anthony</p> <p>1992-01-01</p> <p>The vortex-<span class="hlt">ring</span> problem in fluid mechanics is examined generally in terms of formation, the steady state, the duration of the <span class="hlt">rings</span>, and vortex interactions. The formation is studied by examining the generation of laminar and turbulent vortex <span class="hlt">rings</span> and their resulting structures with attention given to the three stages of laminar <span class="hlt">ring</span> development. Inviscid dynamics is addressed to show how core dynamics affects overall <span class="hlt">ring</span> motion, and laminar vortex structures are described in two dimensions. Viscous and inviscid structures are related in terms of 'leapfrogging', head-on collisions, and collisions with a no-slip wall. Linear instability theory is shown to successfully describe observational data, although late stages in the breakdown are not completely understood. This study of vortex <span class="hlt">rings</span> has important implications for key aerodynamic issues including sound generation, transport and mixing, and vortex interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1014874','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1014874"><span>Asymmetric dipolar <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Prosandeev, Sergey A.; Ponomareva, Inna V.; Kornev, Igor A.; Bellaiche, Laurent M.</p> <p>2010-11-16</p> <p>A device having a dipolar <span class="hlt">ring</span> surrounding an interior region that is disposed asymmetrically on the <span class="hlt">ring</span>. The dipolar <span class="hlt">ring</span> generates a toroidal moment switchable between at least two stable states by a homogeneous field applied to the dipolar <span class="hlt">ring</span> in the plane of the <span class="hlt">ring</span>. The <span class="hlt">ring</span> may be made of ferroelectric or magnetic material. In the former case, the homogeneous field is an electric field and in the latter case, the homogeneous field is a magnetic field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009ems..confE.583B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009ems..confE.583B"><span>Five centuries of Central European temperature extremes reconstructed from tree-<span class="hlt">ring</span> density and documentary evidence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Battipaglia, G.; Frank, D.; Buentgen, U.; Dobrovolný, P.; Brázdil, R.; Pfister, C.; Esper, J.</p> <p>2009-09-01</p> <p>In this project three different summer temperature sensitive tree-<span class="hlt">ring</span> chronologies across the European Alpine region were compiled and analyzed to make a calendar of extreme warm and cold summers. We identified 100 extreme <span class="hlt">events</span> during the past millennium from the tree <span class="hlt">ring</span> data, and 44 extreme years during the 1550-2003 period based upon tree-<span class="hlt">ring</span>, documentary and instrumental evidence. Comparisons with long instrumental series and documentary evidence verify the tree-<span class="hlt">ring</span> extremes and indicate the possibility to use this dataset towards a better understanding of the characteristics prior to the instrumental period. Potential links between the occurrence of extreme <span class="hlt">events</span> over Alps and anomalous large-scale patterns were explored and indicate that the average pattern of the 20 warmest summers (over the 1700-2002 period) describes maximum positive anomalies over Central Europe, whereas the average pattern of the 20 coldest summers shows maximum negative anomalies over Western Europe. Challenges with the present approach included determining an appropriate classification scheme for extreme <span class="hlt">events</span> and the development of a methodology able to identify and characterize the occurrence of extreme episodes back in time. As a future step, our approach will be extended to help verify the sparse documentary data from the beginning of the past millennium and will be used in conjunction with climate models to assess model capabilities in reproducing characteristics of temperature extremes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/872389','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/872389"><span>Concentric <span class="hlt">ring</span> flywheel with hooked <span class="hlt">ring</span> carbon fiber separator/torque coupler</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kuklo, Thomas C.</p> <p>1999-01-01</p> <p>A concentric <span class="hlt">ring</span> flywheel with expandable separators, which function as torque couplers, between the <span class="hlt">rings</span> to take up the gap formed between adjacent <span class="hlt">rings</span> due to differential expansion between different radius <span class="hlt">rings</span> during rotation of the flywheel. The expandable separators or torque couplers include a hook-like section at an upper end which is positioned over an inner <span class="hlt">ring</span> and a shelf-like or flange section at a lower end onto which the next adjacent outer <span class="hlt">ring</span> is positioned. As the concentric <span class="hlt">rings</span> are rotated the gap formed by the differential expansion there between is partially taken up by the expandable separators or torque couplers to maintain torque and centering attachment of the concentric <span class="hlt">rings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6452700','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6452700"><span>Concentric <span class="hlt">ring</span> flywheel with hooked <span class="hlt">ring</span> carbon fiber separator/torque coupler</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kuklo, T.C.</p> <p>1999-07-20</p> <p>A concentric <span class="hlt">ring</span> flywheel with expandable separators, which function as torque couplers, between the <span class="hlt">rings</span> to take up the gap formed between adjacent <span class="hlt">rings</span> due to differential expansion between different radius <span class="hlt">rings</span> during rotation of the flywheel. The expandable separators or torque couplers include a hook-like section at an upper end which is positioned over an inner <span class="hlt">ring</span> and a shelf-like or flange section at a lower end onto which the next adjacent outer <span class="hlt">ring</span> is positioned. As the concentric <span class="hlt">rings</span> are rotated the gap formed by the differential expansion there between is partially taken up by the expandable separators or torque couplers to maintain torque and centering attachment of the concentric <span class="hlt">rings</span>. 2 figs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1329068-observation-electron-cloud-instabilities-emittance-dilution-cornell-electron-positron-storage-ring-test-accelerator','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1329068-observation-electron-cloud-instabilities-emittance-dilution-cornell-electron-positron-storage-ring-test-accelerator"><span>Observation of electron cloud instabilities and emittance dilution at the Cornell electron-positron <span class="hlt">Storage</span> <span class="hlt">ring</span> Test Accelerator</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Holtzapple, R. L.; Billing, M. G.; Campbell, R. C.; ...</p> <p>2016-04-11</p> <p>Electron cloud related emittance dilution and instabilities of bunch trains limit the performance of high intensity circular colliders. One of the key goals of the Cornell electron-positron <span class="hlt">storage</span> <span class="hlt">ring</span> Test Accelerator (CesrTA) research program is to improve our understanding of how the electron cloud alters the dynamics of bunches within the train. Single bunch beam diagnostics have been developed to measure the beam spectra, vertical beam size, two important dynamical effects of beams interacting with the electron cloud, for bunch trains on a turn-by-turn basis. Experiments have been performed at CesrTA to probe the interaction of the electron cloud withmore » stored positron bunch trains. The purpose of these experiments was to characterize the dependence of beam-electron cloud interactions on the machine parameters such as bunch spacing, vertical chromaticity, and bunch current. The beam dynamics of the stored beam, in the presence of the electron cloud, was quantified using: 1) a gated beam position monitor (BPM) and spectrum analyzer to measure the bunch-by-bunch frequency spectrum of the bunch trains, 2) an x-ray beam size monitor to record the bunch-by-bunch, turn-by-turn vertical size of each bunch within the trains. In this study we report on the observations from these experiments and analyze the effects of the electron cloud on the stability of bunches in a train under many different operational conditions.« 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_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/2016JInst..11P4013H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JInst..11P4013H"><span>Observation of Electron Cloud Instabilities and Emittance Dilution at the Cornell Electron-Positron <span class="hlt">Storage</span> <span class="hlt">Ring</span> Test Accelerator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holtzapple, R. L.; Billing, M. G.; Campbell, R. C.; Dugan, G. F.; Flanagan, J.; McArdle, K. E.; Miller, M. I.; Palmer, M. A.; Ramirez, G. A.; Sonnad, K. G.; Totten, M. M.; Tucker, S. L.; Williams, H. A.</p> <p>2016-04-01</p> <p>Electron cloud related emittance dilution and instabilities of bunch trains limit the performance of high intensity circular colliders. One of the key goals of the Cornell electron-positron <span class="hlt">storage</span> <span class="hlt">ring</span> Test Accelerator (CesrTA) research program is to improve our understanding of how the electron cloud alters the dynamics of bunches within the train. Single bunch beam diagnotics have been developed to measure the beam spectra, vertical beam size, two important dynamical effects of beams interacting with the electron cloud, for bunch trains on a turn-by-turn basis. Experiments have been performed at CesrTA to probe the interaction of the electron cloud with stored positron bunch trains. The purpose of these experiments was to characterize the dependence of beam-electron cloud interactions on the machine parameters such as bunch spacing, vertical chromaticity, and bunch current. The beam dynamics of the stored beam, in the presence of the electron cloud, was quantified using: 1) a gated beam position monitor (BPM) and spectrum analyzer to measure the bunch-by-bunch frequency spectrum of the bunch trains; 2) an x-ray beam size monitor to record the bunch-by-bunch, turn-by-turn vertical size of each bunch within the trains. In this paper we report on the observations from these experiments and analyze the effects of the electron cloud on the stability of bunches in a train under many different operational conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060048197&hterms=elasticity+space&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Delasticity%2Bspace','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060048197&hterms=elasticity+space&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Delasticity%2Bspace"><span>Nitrile/Buna N Material Failure Assessment for an O-<span class="hlt">Ring</span> used on the Gaseous Hydrogen Flow Control Valve (FCV) of the Space Shuttle Main Engine</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wingard, Doug</p> <p>2006-01-01</p> <p>After the rollout of Space Shuttle Discovery in April 2005 in preparation for return-to-flight, there was a failure of the Orbiter (OV-103) helium signature leak test in the gaseous hydrogen (GH2) system. Leakage was attributed to the Flow Control Valve (FCV) in Main Engine 3. The FCV determined to be the source of the leak for OV-103 is designated as LV-58. The nitrile/Buna N rubber O-<span class="hlt">ring</span> seal was removed from LV-58, and failure analysis indicated radial cracks providing leak paths in one quadrant. Cracks were eventually found in 6 of 9 FCV O-<span class="hlt">rings</span> among the three Shuttle Orbiters, though none were as severe as those for LV-58, OV-103. Testing by EM10 at MSFC on all 9 FCV O- <span class="hlt">rings</span> included: laser dimensional, Shore A hardness and properties from a dynamic mechanical analyzer (DMA) and an Instron tensile machine. The following test data was obtained on the cracked quadrant of the LV-58, OV-103 O-<span class="hlt">ring</span>: (1) the estimated compression set was only 9.5%, compared to none for the rest of the O-<span class="hlt">ring</span>; (2) Shore A hardness for the O.D. was higher by almost 4 durometer points than for the rest of the O-<span class="hlt">ring</span>; and (3) DMA data showed that the <span class="hlt">storage</span>/elastic modulus E was almost 25% lower than for the rest of the O-<span class="hlt">ring</span>. Of the 8 FCV O-<span class="hlt">rings</span> tested on an Instron, 4 yielded tensile strengths that were below the MIL spec requirement of 1350 psi-a likely influence of rubber cracking. Comparisons were made between values of modulus determined by DNA (elastic) and Instron (Young s). Each nitrile/Buna N O-<span class="hlt">ring</span> used in the FCV conforms to the MIL-P-25732C specification. A number of such O-<span class="hlt">rings</span> taken from shelf <span class="hlt">storage</span> at MSFC and Kennedy Space Center (KSC) were used to generate a reference curve of DMA glass transition temperature (Tg) vs. shelf <span class="hlt">storage</span> time ranging from 8 to 26 years. A similar reference curve of TGA onset temperature (of rubber weight loss) vs. shelf <span class="hlt">storage</span> time was also generated. The DMA and TGA data for the used FCV O-<span class="hlt">rings</span> were compared to the reference</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070014868&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmajor%2Bdepression','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070014868&hterms=major+depression&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dmajor%2Bdepression"><span>The Role of <span class="hlt">Ring</span> Current on Slot Region Penetration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fok, Mei-Ching; Elkington, Scot</p> <p>2006-01-01</p> <p>During magnetic quiet times, the inner belt, slot region and the outer belt are well defined regions. However, during some major storms, outer belt particles penetrate inward and significantly fill the slot region. In some extreme <span class="hlt">events</span>, the outer belt particles travel through the slot and create a new belt in the inner region that persists from months to years. In this paper, we examine the role of the <span class="hlt">ring</span> current on this radiation belt penetration into the slot region. The storm-time intensification of the <span class="hlt">ring</span> current produces strong magnetic depression in the inner magnetosphere. This perturbation and its fluctuation enhance the radial transport and diffusion of the outer radiation belt particles. We perform kinetic and test-particle calculations to quantitatively assess the effects of the <span class="hlt">ring</span> current field on filling of the slot region. Simulation results during major storms will be presented and discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5114644','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5114644"><span>High flux circularly polarized gamma beam factory: coupling a Fabry-Perot optical cavity with an electron <span class="hlt">storage</span> <span class="hlt">ring</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>Chaikovska, I.; Cassou, K.; Chiche, R.; Cizeron, R.; Cornebise, P.; Delerue, N.; Jehanno, D.; Labaye, F.; Marie, R.; Martens, A.; Peinaud, Y.; Soskov, V.; Variola, A.; Zomer, F.; Cormier, E.; Lhermite, J.; Dolique, V.; Flaminio, R.; Michel, C.; Pinard, L.; Sassolas, B.; Akagi, T.; Araki, S.; Honda, Y.; Omori, T.; Terunuma, N.; Urakawa, J.; Miyoshi, S.; Takahashi, T.; Yoshitama, H.</p> <p>2016-01-01</p> <p>We report and discuss high-flux generation of circularly polarized γ-rays by means of Compton scattering. The γ-ray beam results from the collision of an external-cavity-enhanced infrared laser beam and a low emittance relativistic electron beam. By operating a non-planar bow-tie high-finesse optical Fabry-Perot cavity coupled to a <span class="hlt">storage</span> <span class="hlt">ring</span>, we have recorded a flux of up to (3.5 ± 0.3) × 108 photons per second with a mean measured energy of 24 MeV. The γ-ray flux has been sustained for several hours. In particular, we were able to measure a record value of up to 400 γ-rays per collision in a full bandwidth. Moreover, the impact of Compton scattering on the electron beam dynamics could be observed resulting in a reduction of the electron beam lifetime correlated to the laser power stored in the Fabry-Perot cavity. We demonstrate that the electron beam lifetime provides an independent and consistent determination of the γ-ray flux. Furthermore, a reduction of the γ-ray flux due to intrabeam scattering has clearly been identified. These results, obtained on an accelerator test facility, warrant potential scaling and revealed both expected and yet unobserved effects. They set the baseline for further scaling of the future Compton sources under development around the world. PMID:27857146</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040171615','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040171615"><span>Saturn's <span class="hlt">Rings</span>, the Yarkovsky Effects, and the <span class="hlt">Ring</span> of Fire</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rubincam, David Parry</p> <p>2004-01-01</p> <p>The dimensions of Saturn's A and B <span class="hlt">rings</span> may be determined by the seasonal Yarkovsky effect and the Yarkovsky-Schach effect; the two effects confine the <span class="hlt">rings</span> between approximately 1.68 and approximately 2.23 Saturn radii, in reasonable agreement with the observed values of 1.525 and 2.267. The C <span class="hlt">ring</span> may be sparsely populated because its particles are transients on their way to Saturn; the infall may create a luminous <span class="hlt">Ring</span> of Fire around Saturn's equator. The <span class="hlt">ring</span> system may be young: in the past heat flow from Saturn's interior much above its present value would not permit <span class="hlt">rings</span> to exist.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19812546','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19812546"><span>Saturn's largest <span class="hlt">ring</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Verbiscer, Anne J; Skrutskie, Michael F; Hamilton, Douglas P</p> <p>2009-10-22</p> <p>Most planetary <span class="hlt">rings</span> in the Solar System lie within a few radii of their host body, because at these distances gravitational accelerations inhibit satellite formation. The best known exceptions are Jupiter's gossamer <span class="hlt">rings</span> and Saturn's E <span class="hlt">ring</span>, broad sheets of dust that extend outward until they fade from view at five to ten planetary radii. Source satellites continuously supply the dust, which is subsequently lost in collisions or by radial transport. Here we report that Saturn has an enormous <span class="hlt">ring</span> associated with its outer moon Phoebe, extending from at least 128R(S) to 207R(S) (Saturn's radius R(S) is 60,330 km). The <span class="hlt">ring</span>'s vertical thickness of 40R(S) matches the range of vertical motion of Phoebe along its orbit. Dynamical considerations argue that these <span class="hlt">ring</span> particles span the Saturnian system from the main <span class="hlt">rings</span> to the edges of interplanetary space. The <span class="hlt">ring</span>'s normal optical depth of approximately 2 x 10(-8) is comparable to that of Jupiter's faintest gossamer <span class="hlt">ring</span>, although its particle number density is several hundred times smaller. Repeated impacts on Phoebe, from both interplanetary and circumplanetary particle populations, probably keep the <span class="hlt">ring</span> populated with material. <span class="hlt">Ring</span> particles smaller than centimetres in size slowly migrate inward and many of them ultimately strike the dark leading face of Iapetus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4607587','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4607587"><span>Phase 1 Safety, Pharmacokinetics, and Pharmacodynamics of Dapivirine and Maraviroc Vaginal <span class="hlt">Rings</span>: a Double-Blind Randomized Trial</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chen, Beatrice A.; Panther, Lori; Marzinke, Mark A.; Hendrix, Craig W.; Hoesley, Craig J.; van der Straten, Ariane; Husnik, Marla J.; Soto-Torres, Lydia; Nel, Annalene; Johnson, Sherri; Richardson-Harman, Nicola; Rabe, Lorna K.; Dezzutti, Charlene S.</p> <p>2015-01-01</p> <p>Background Variable adherence limits effectiveness of daily oral and intravaginal tenofovir-containing pre-exposure prophylaxis. Monthly vaginal antiretroviral <span class="hlt">rings</span> are one approach to improve adherence and drug delivery. Methods MTN-013/IPM 026, a multi-site, double-blind, randomized, placebo-controlled trial in 48 HIV-negative U.S. women, evaluated vaginal <span class="hlt">rings</span> containing dapivirine (25 mg) and maraviroc (100 mg), dapivirine-only, maraviroc-only, and placebo used continuously for 28 days. Safety was assessed by adverse <span class="hlt">events</span>. Drug concentrations were quantified in plasma, cervicovaginal fluid (CVF), and cervical tissue. Cervical biopsy explants were challenged with HIV ex vivo to evaluate pharmacodynamics. Results There was no difference in related genitourinary adverse <span class="hlt">events</span> between treatment arms compared to placebo. Dapivirine and maraviroc concentrations rose higher initially before falling more rapidly with the combination <span class="hlt">ring</span> compared to relatively stable concentrations with the single drug <span class="hlt">rings</span>. Dapivirine concentrations in CVF were 1 and 5 log10 greater than cervical tissue and plasma for both <span class="hlt">rings</span>. Maraviroc was consistently detected only in CVF. Dapivirine and maraviroc CVF and dapivirine tissue concentrations dropped rapidly after <span class="hlt">ring</span> removal. Cervical tissue showed a significant inverse linear relationship between HIV replication and dapivirine levels. Conclusions In this first study of a combination microbicide vaginal <span class="hlt">ring</span>, all four <span class="hlt">rings</span> were safe and well tolerated. Tissue dapivirine concentrations were 1,000 times greater than plasma concentrations and single drug <span class="hlt">rings</span> had more stable pharmacokinetics. Dapivirine, but not maraviroc, demonstrated concentration-dependent inhibition of HIV-1 infection in cervical tissue. Since maraviroc concentrations were consistently detectable only in CVF and not in plasma, improved drug release of maraviroc <span class="hlt">rings</span> is needed. PMID:26034880</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26034880','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26034880"><span>Phase 1 Safety, Pharmacokinetics, and Pharmacodynamics of Dapivirine and Maraviroc Vaginal <span class="hlt">Rings</span>: A Double-Blind Randomized Trial.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Beatrice A; Panther, Lori; Marzinke, Mark A; Hendrix, Craig W; Hoesley, Craig J; van der Straten, Ariane; Husnik, Marla J; Soto-Torres, Lydia; Nel, Annalene; Johnson, Sherri; Richardson-Harman, Nicola; Rabe, Lorna K; Dezzutti, Charlene S</p> <p>2015-11-01</p> <p>Variable adherence limits effectiveness of daily oral and intravaginal tenofovir-containing pre-exposure prophylaxis. Monthly vaginal antiretroviral <span class="hlt">rings</span> are one approach to improve adherence and drug delivery. MTN-013/IPM 026, a multisite, double-blind, randomized, placebo-controlled trial in 48 HIV-negative US women, evaluated vaginal <span class="hlt">rings</span> containing dapivirine (DPV) (25 mg) and maraviroc (MVC) (100 mg), DPV only, MVC only, and placebo used continuously for 28 days. Safety was assessed by adverse <span class="hlt">events</span>. Drug concentrations were quantified in plasma, cervicovaginal fluid (CVF), and cervical tissue. Cervical biopsy explants were challenged with HIV ex vivo to evaluate pharmacodynamics. There was no difference in related genitourinary adverse <span class="hlt">events</span> between treatment arms compared with placebo. DPV and MVC concentrations rose higher initially before falling more rapidly with the combination <span class="hlt">ring</span> compared with relatively stable concentrations with the single-drug <span class="hlt">rings</span>. DPV concentrations in CVF were 1 and 5 log10 greater than cervical tissue and plasma for both <span class="hlt">rings</span>. MVC was consistently detected only in CVF. DPV and MVC CVF and DPV tissue concentrations dropped rapidly after <span class="hlt">ring</span> removal. Cervical tissue showed a significant inverse linear relationship between HIV replication and DPV levels. In this first study of a combination microbicide vaginal <span class="hlt">ring</span>, all 4 <span class="hlt">rings</span> were safe and well tolerated. Tissue DPV concentrations were 1000 times greater than plasma concentrations and single drug <span class="hlt">rings</span> had more stable pharmacokinetics. DPV, but not MVC, demonstrated concentration-dependent inhibition of HIV-1 infection in cervical tissue. Because MVC concentrations were consistently detectable only in CVF and not in plasma, improved drug release of MVC <span class="hlt">rings</span> is needed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2016/3035/fs20163035.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2016/3035/fs20163035.pdf"><span>May through July 2015 storm <span class="hlt">event</span> effects on suspended-sediment loads, sediment trapping efficiency, and <span class="hlt">storage</span> capacity of John Redmond Reservoir</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Foster, Guy M.; King, Lindsey R.</p> <p>2016-06-20</p> <p>The Neosho River and its primary tributary, the Cottonwood River, are the main sources of inflow to John Redmond Reservoir in east-central Kansas. Storm <span class="hlt">events</span> during May through July 2015 caused large inflows of water and sediment into the reservoir. The U.S. Geological Survey, in cooperation with the Kansas Water Office, and funded in part through the Kansas State Water Plan Fund, computed the suspended-sediment inflows to, and trapping efficiency of, John Redmond Reservoir during May through July 2015. This fact sheet summarizes the quantification of suspended-sediment loads to and from the reservoir during May through July 2015 storm <span class="hlt">events</span> and describes reservoir sediment trapping efficiency and effects on water-<span class="hlt">storage</span> capacity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.loc.gov/pictures/collection/hh/item/co0858.photos.316964p/','SCIGOV-HHH'); return false;" href="https://www.loc.gov/pictures/collection/hh/item/co0858.photos.316964p/"><span>15. DETAILED VIEW OF ENRICHED URANIUM <span class="hlt">STORAGE</span> TANK. THE 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>15. DETAILED VIEW OF ENRICHED URANIUM <span class="hlt">STORAGE</span> TANK. THE ADDITION OF THE GLASS <span class="hlt">RINGS</span> SHOWN AT THE TOP OF THE TANK HELPS PREVENT THE URANIUM FROM REACHING CRITICALITY LIMITS. (4/12/62) - Rocky Flats Plant, General Manufacturing, Support, Records-Central Computing, Southern portion of Plant, Golden, Jefferson County, CO</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020012807','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020012807"><span>Ultrasonic Resonance Spectroscopy of Composite <span class="hlt">Rings</span> for Flywheel Rotors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Harmon, Laura M.; Baaklini, George Y.</p> <p>2001-01-01</p> <p>Flywheel energy <span class="hlt">storage</span> devices comprising multilayered composite rotor systems are being studied extensively for utilization in the International Space Station. These composite material systems were investigated with a recently developed ultrasonic resonance spectroscopy technique. The system employs a swept frequency approach and performs a fast Fourier transform on the frequency spectrum of the response signal. In addition. the system allows for equalization of the frequency spectrum, providing all frequencies with equal amounts of energy to excite higher order resonant harmonics. Interpretation of the second fast Fourier transform, along with equalization of the frequency spectrum, offers greater assurance in acquiring and analyzing the fundamental frequency, or spectrum resonance spacing. The range of frequencies swept in a pitch-catch mode was varied up to 8 MHz, depending on the material and geometry of the component. Single and multilayered material samples, with and without known defects, were evaluated to determine how the constituents of a composite material system affect the resonant frequency. Amplitude and frequency changes in the spectrum and spectrum resonance spacing domains were examined from ultrasonic responses of a flat composite coupon, thin composite <span class="hlt">rings</span>, and thick composite <span class="hlt">rings</span>. Also, the ultrasonic spectroscopy responses from areas with an intentional delamination and a foreign material insert, similar to defects that may occur during manufacturing malfunctions, were compared with those from defect-free areas in thin composite <span class="hlt">rings</span>. A thick composite <span class="hlt">ring</span> with varying thickness was tested to investigate the full-thickness resonant frequency and any possible bulk interfacial bond issues. Finally, the effect on the frequency response of naturally occurring single and clustered voids in a composite <span class="hlt">ring</span> was established.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA00035.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA00035.html"><span>Uranus Tenth <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1996-01-29</p> <p>On Jan. 23, 1986, NASA Voyager 2 discovered a tenth <span class="hlt">ring</span> orbiting Uranus. The tenth <span class="hlt">ring</span> is about midway between the bright, outermost epsilon <span class="hlt">ring</span> and the next <span class="hlt">ring</span> down, called delta. http://photojournal.jpl.nasa.gov/catalog/PIA00035</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.P33B0241F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.P33B0241F"><span>Density Waves in Saturn's <span class="hlt">Rings</span> from Cassini Radio Occultations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>French, R. G.; Rappaport, N. J.; Marouf, E. A.; McGhee, C. A.</p> <p>2005-12-01</p> <p>The Cassini Radio Science Team conducted a set of optimized diametric occultations by Saturn and its <span class="hlt">rings</span> from May to September 2005, providing 11 separate probes of Saturn's ionosphere and atmosphere, and 12 optical depth profiles of the complete <span class="hlt">ring</span> system. Each <span class="hlt">event</span> was observed by the stations of the Deep Space Net (DSN) at three radio frequencies (S, X, Ka bands, with corresponding wavelengths of ? = 13, 3.6, and 0.9 cm). Very accurate pointing by the spacecraft and ground antennas resulted in stable baseline signal levels, and the relatively large <span class="hlt">ring</span> opening angle (B=19-25°) permitted us to probe even quite dense <span class="hlt">ring</span> regions with excellent SNR. The RSS occultation technique enables us to recover very fine detailed radial structure by correcting for diffraction effects. Multiple occultation chords, covering a variety of <span class="hlt">ring</span> longitudes and <span class="hlt">ring</span> opening angles, reveal the structure of the <span class="hlt">rings</span> in remarkable detail, including density and bending waves, satellite wakes, and subtle variations at the 100-m radius scale. Janus and Epimetheus are responsible for a particularly rich set of density waves, and their coorbital interactions result in a complex interplay of time-variable <span class="hlt">ring</span> structure over the 8-year libration period of the two satellites. We compare the first-order 2:1, 4:3, 5:4, and 6:5 coorbital density waves from multiple occultation chords to linear density wave models based on a dynamical model of the orbital exchange between the moons. From the observed dispersion relation of the wave crests, we infer the surface mass density and eccentricity gradient of particle streamlines, and match the detailed shapes of the wave crests using a non-linear analysis. Second-order coorbital features are also evident, and there are even hints of third-order density waves in the high SNR radio occultation data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ThEng..64...15S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ThEng..64...15S"><span>Determination of the steam volume fraction in the <span class="hlt">event</span> of loss of cooling of the spent fuel <span class="hlt">storage</span> pool</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sledkov, R. M.; Galkin, I. Yu.; Stepanov, O. E.; Strebnev, N. A.</p> <p>2017-01-01</p> <p>When one solves engineering problems related to the cooling of fuel assemblies (FAs) in a spent fuel <span class="hlt">storage</span> pool (SFSP) and the assessment of nuclear safety of FA <span class="hlt">storage</span> in an SFSP in the initial <span class="hlt">event</span> of loss of SFSP cooling, it is essential to determine the coolant density and, consequently, steam volume fractions φ in bundles of fuel elements at a pressure of 0.1-0.5 MPa. Such formulas for calculating φ that remain valid in a wide range of operating parameters and geometric shapes of channels and take the conditions of loss of SFSP cooling into account are currently almost lacking. The results of systematization and analysis of the available formulas for φ are reported in the present study. The calculated values were compared with the experimental data obtained in the process of simulating the conditions of FA cooling in an SFSP in the <span class="hlt">event</span> of loss of its cooling. Six formulas for calculating the steam volume fraction, which were used in this comparison, were chosen from a total of 11 considered relations. As a result, the formulas producing the most accurate values of φ in the conditions of loss of SFSP cooling were selected. In addition, a relation that allows one to perform more accurate calculations of steam volume fractions in the conditions of loss of SFSP cooling was derived based on the Fedorov formula in the two-group approximation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SPIE.8782E..0BZ','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SPIE.8782E..0BZ"><span>Preparation, one- and two-photon properties of carbazole derivatives containing nitrogen heterocyclic <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Yichi; Wang, Ping; Li, Liang; Chen, Zhimin; He, Chunying; Wu, Yiqun</p> <p></p> <p>Preparation of recording materials with high two-photon absorption activities is one of the important issues to superhigh- density two-photon absorption (TPA) three-dimensional (3D) optical data <span class="hlt">storage</span>. In this paper, three new carbazole derivatives containing nitrogen heterocyclic <span class="hlt">ring</span> with symmetric and asymmetric structures are prepared using ethylene as the π bridge between the carbazole unit and nitrogen heterocyclic <span class="hlt">ring</span>, namely, 9-butyl-3-(2-(1,8- naphthyridin)vinyl)-carbazole (material 1), 9-butyl-3,6-bis(2-(1,8-naphthyl)vinyl)-carbazole (material 2) and 9-butyl-3,6- bis(2-(quinolin)vinyl)-carbazole (material 3). Their one photon properties including linear absorption spectra, fluorescence emission spectra, and fluorescence quantum yields are studied. The fluorescence excited by 120 fs pulse at 800 nm Ti: sapphire laser operating at 1 kHz repetition rate with different incident powers of 9-butyl-3-(2-(quinolin) vinyl)-carbazole (material 3) was investigated, and two-photon absorption cross-sections has been obtained. It is shown that material 3 containing quinoline <span class="hlt">rings</span> as electron acceptor with symmetric structure exhibit high two-photon absorption activity. The result implies that material 3 (9-butyl-3-(2-(quinolin) vinyl)-carbazole) is a good candidate as a promising recording material for super-high-density two-photon absorption (TPA) three-dimensional (3D) optical data <span class="hlt">storage</span>. The influence of chemical structure of the materials on the optical properties is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA00658.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA00658.html"><span>Jupiter <span class="hlt">Ring</span> Halo</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1998-03-26</p> <p>A mosaic of four images taken through the clear filter (610 nanometers) of the solid state imaging (CCD) system aboard NASA's Galileo spacecraft on November 8, 1996, at a resolution of approximately 46 kilometers (km) per picture element (pixel) along the <span class="hlt">rings</span>; however, because the spacecraft was only about 0.5 degrees above the <span class="hlt">ring</span> plane, the image is highly foreshortened in the vertical direction. The images were obtained when Galileo was in Jupiter's shadow peering back toward the Sun; the <span class="hlt">ring</span> was approximately 2,300,000 kilometers (km) away. The arc on the far right of the image is produced by sunlight scattered by small particles comprising Jupiter's upper atmospheric haze. The <span class="hlt">ring</span> also efficiently scatters light, indicating that much of its brightness is due to particles that are microns or less in diameter. Such small particles are believed to have human-scale lifetimes, i.e., very brief compared to the solar system's age. Jupiter's <span class="hlt">ring</span> system is composed of three parts -- a flat main <span class="hlt">ring</span>, a lenticular halo interior to the main <span class="hlt">ring</span>, and the gossamer <span class="hlt">ring</span>, which lies exterior to the main <span class="hlt">ring</span>. The near and far arms of Jupiter's main <span class="hlt">ring</span> extend horizontally across the mosaic, joining together at the <span class="hlt">ring</span>'s ansa, on the far left side of the figure. The near arm of the <span class="hlt">ring</span> appears to be abruptly truncated close to the planet, at the point where it passes into Jupiter's shadow. A faint mist of particles can be seen above and below the main <span class="hlt">rings</span>; this vertically extended, toroidal "halo" is unusual in planetary <span class="hlt">rings</span>, and is probably caused by electromagnetic forces which can push small grains out of the <span class="hlt">ring</span> plane. Halo material is present across this entire image, implying that it reaches more than 27,000 km above the <span class="hlt">ring</span> plane. Because of shadowing, the halo is not visible close to Jupiter in the lower right part of the mosaic. In order to accentuate faint features in the image, different brightnesses are shown through color, with the brightest being</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://kidshealth.org/en/teens/contraception-ring.html','NIH-MEDLINEPLUS'); return false;" href="https://kidshealth.org/en/teens/contraception-ring.html"><span>Birth Control <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://medlineplus.gov/">MedlinePlus</a></p> <p></p> <p></p> <p>... Safe Videos for Educators Search English Español Birth Control <span class="hlt">Ring</span> KidsHealth / For Teens / Birth Control <span class="hlt">Ring</span> What's in this article? What Is It? ... Anillo vaginal anticonceptivo What Is It? The birth control <span class="hlt">ring</span> is a soft, flexible, doughnut-shaped <span class="hlt">ring</span> ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29150189','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29150189"><span>Uranium mobility across annual growth <span class="hlt">rings</span> in three deciduous tree species.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McHugh, Kelly C; Widom, Elisabeth; Spitz, Henry B; Wiles, Gregory C; Glover, Sam E</p> <p>2018-02-01</p> <p>Black walnut (Juglans nigra), slippery elm (Ulmus rubra), and white ash (Fraxinus americana) trees were evaluated as potential archives of past uranium (U) contamination. Like other metals, U mobility in annual growth <span class="hlt">rings</span> of trees is dependent on the tree species. Uranium concentrations and isotopic compositions (masses 234, 235, 236, and 238) were analyzed by thermal ionization mass spectrometry to test the efficacy of using tree <span class="hlt">rings</span> to retroactively monitor U pollution from the FFMPC, a U purification facility operating from 1951 to 1989. This study found non-natural U (depleted U and detectable 236 U) in growth <span class="hlt">rings</span> of all three tree species that pre-dated the start of operations at FFMPC and compositional trends that did not correspond with known contamination <span class="hlt">events</span>. Therefore, the annual growth <span class="hlt">rings</span> of these tree species cannot be used to reliably monitor the chronology of U contamination. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997APS..PAC..8P21T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997APS..PAC..8P21T"><span>Multi-Pulse Extraction from Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> for Radiographic Applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thiessen, Henry A.; Neri, Filippo; Rust, Kenneth R.; Redd, Dale B.</p> <p>1997-05-01</p> <p>For radiography of moving objects, two or more pulses with adjustable time spacing are required. The existing Proton Stotage <span class="hlt">Ring</span> (PSR) extraction system is configured to extract the entire beam in a single turn. Two kickers and two kicker modulators fired at the same time perform the normal extraction function. By reconfiguring the two kickers and two modulators, it is possible to obtain two half-sized extraction kicks with adjustable time spacing. In this way, we have extracted two pulses with adjustable relative timing. The setup will be described and experimental results will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020005141&hterms=electromagnetism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Delectromagnetism','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020005141&hterms=electromagnetism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Delectromagnetism"><span>Planetary <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cuzzi, Jeffrey N.</p> <p>1994-01-01</p> <p>Just over two decades ago, Jim Pollack made a critical contribution to our understanding of planetary <span class="hlt">ring</span> particle properties, and resolved a major apparent paradox between radar reflection and radio emission observations. At the time, particle properties were about all there were to study about planetary <span class="hlt">rings</span>, and the fundamental questions were, why is Saturn the only planet with <span class="hlt">rings</span>, how big are the particles, and what are they made of? Since then, we have received an avalanche of observations of planetary <span class="hlt">ring</span> systems, both from spacecraft and from Earth. Meanwhile, we have seen steady progress in our understanding of the myriad ways in which gravity, fluid and statistical mechanics, and electromagnetism can combine to shape the distribution of the submicron-to-several-meter size particles which comprise <span class="hlt">ring</span> systems into the complex webs of structure that we now know them to display. Insights gained from studies of these giant dynamical analogs have carried over into improved understanding of the formation of the planets themselves from particle disks, a subject very close to Jim's heart. The now-complete reconnaissance of the gas giant planets by spacecraft has revealed that <span class="hlt">ring</span> systems are invariably found in association with families of regular satellites, and there is ark emerging perspective that they are not only physically but causally linked. There is also mounting evidence that many features or aspects of all planetary <span class="hlt">ring</span> systems, if not the <span class="hlt">ring</span> systems themselves, are considerably younger than the solar system</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('https://www.ncbi.nlm.nih.gov/pubmed/20639516','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20639516"><span>Wood anatomical analysis of Alnus incana and Betula pendula injured by a debris-flow <span class="hlt">event</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Arbellay, Estelle; Stoffel, Markus; Bollschweiler, Michelle</p> <p>2010-10-01</p> <p>Vessel chronologies in <span class="hlt">ring</span>-porous species have been successfully employed in the past to extract the climate signal from tree <span class="hlt">rings</span>. Environmental signals recorded in vessels of <span class="hlt">ring</span>-porous species have also been used in previous studies to reconstruct discrete <span class="hlt">events</span> of drought, flooding and insect defoliation. However, very little is known about the ability of diffuse-porous species to record environmental signals in their xylem cells. Moreover, time series of wood anatomical features have only rarely been used to reconstruct former geomorphic <span class="hlt">events</span>. This study was therefore undertaken to characterize the wood anatomical response of diffuse-porous Alnus incana (L.) Moench and Betula pendula Roth to debris-flow-induced wounding. Tree microscopic response to wounding was assessed through the analysis of wood anatomical differences between injured <span class="hlt">rings</span> formed in the debris-flow <span class="hlt">event</span> year and uninjured <span class="hlt">rings</span> formed in the previous year. The two <span class="hlt">ring</span> types were examined close and opposite to the injury in order to determine whether wound effects on xylem cells decrease with increasing tangential distance from the injury. Image analysis was used to measure vessel parameters as well as fiber and parenchyma cell (FPC) parameters. The results of this study indicate that injured <span class="hlt">rings</span> are characterized by smaller vessels as compared with uninjured <span class="hlt">rings</span>. By contrast, FPC parameters were not found to significantly differ between injured and uninjured <span class="hlt">rings</span>. Vessel and FPC parameters mainly remained constant with increasing tangential distance from the injury, except for a higher proportion of vessel lumen area opposite to the injury within A. incana. This study highlights the existence of anatomical tree-<span class="hlt">ring</span> signatures-in the form of smaller vessels-related to past debris-flow activity and addresses a new methodological approach to date injuries inflicted on trees by geomorphic processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.P23B1633N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.P23B1633N"><span>The Saturn <span class="hlt">Ring</span> Observer: In situ studies of planetary <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicholson, P. D.; Tiscareno, M. S.; Spilker, L. J.</p> <p>2010-12-01</p> <p>As part of the Planetary Science Decadal Survey recently undertaken by the NRC's Space Studies Board for the National Academy of Sciences, studies were commissioned for a number of potential missions to outer planet targets. One of these studies examined the technological feasibility of a mission to carry out in situ studies of Saturn's <span class="hlt">rings</span>, from a spacecraft placed in a circular orbit above the <span class="hlt">ring</span> plane: the Saturn <span class="hlt">Ring</span> Observer. The technical findings and background are discussed in a companion poster by T. R. Spilker et al. Here we outline the science goals of such a mission. Most of the fundamental interactions in planetary <span class="hlt">rings</span> occur on spatial scales that are unresolved by flyby or orbiter spacecraft. Typical particle sizes in the <span class="hlt">rings</span> of Saturn are in the 1 cm - 10 m range, and average interparticle spacings are a few meters. Indirect evidence indicates that the vertical thickness of the <span class="hlt">rings</span> is as little as 5 - 10 m, which implies a velocity dispersion of only a few mm/sec. Theories of <span class="hlt">ring</span> structure and evolution depend on the unknown characteristics of interparticle collisions and on the size distribution of the <span class="hlt">ring</span> particles. The SRO could provide direct measurements of both the coefficient of restitution -- by monitoring individual collisions -- and the particles’ velocity dispersion. High-resolution observations of individual <span class="hlt">ring</span> particles should also permit estimates of their spin states. Numerical simulations of Saturn’s <span class="hlt">rings</span> incorporating both collisions and self-gravity predict that the <span class="hlt">ring</span> particles are not uniformly distributed, but are instead clustered into elongated structures referred to as “self-gravity wakes”, which are continually created and destroyed on an orbital timescale. Theory indicates that the average separation between wakes in the A <span class="hlt">ring</span> is of order 30-100 m. Direct imaging of self-gravity wakes, including their formation and subsequent dissolution, would provide critical validation of these models. Other</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA00657&hterms=Lenticular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DLenticular','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA00657&hterms=Lenticular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DLenticular"><span>Jupiter's Main <span class="hlt">Ring</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>1997-01-01</p> <p>A mosaic of four images taken through the clear filter (610 nanometers) of the solid state imaging (CCD) system aboard NASA's Galileo spacecraft on November 8, 1996, at a resolution of approximately 46 kilometers (km) per picture element (pixel) along the <span class="hlt">rings</span>; however, because the spacecraft was only about 0.5 degrees above the <span class="hlt">ring</span> plane, the image is highly foreshortened in the vertical direction. The images were obtained when Galileo was in Jupiter's shadow peering back toward the Sun; the <span class="hlt">ring</span> was approximately 2,300,000 kilometers (km) away. The arc on the far right of the image is produced by sunlight scattered by small particles comprising Jupiter's upper atmospheric haze. The <span class="hlt">ring</span> also efficiently scatters light, indicating that much of its brightness is due to particles that are microns or less in diameter. Such small particles are believed to have human-scale lifetimes, i.e., very brief compared to the solar system's age.<p/>Jupiter's <span class="hlt">ring</span> system is composed of three parts -- a flat main <span class="hlt">ring</span>, a lenticular halo interior to the main <span class="hlt">ring</span>, and the gossamer <span class="hlt">ring</span>, which lies exterior to the main <span class="hlt">ring</span>. The near and far arms of Jupiter's main <span class="hlt">ring</span> extend horizontally across the mosaic, joining together at the <span class="hlt">ring</span>'s ansa, on the far left side of the figure. The near arm of the <span class="hlt">ring</span> appears to be abruptly truncated close to the planet, at the point where it passes into Jupiter's shadow. Some radial structure is barely visible across the <span class="hlt">ring</span>'s ansa. A faint mist of particles can be seen above and below the main <span class="hlt">rings</span>; this vertically extended 'halo' is unusual in planetary <span class="hlt">rings</span>, and is probably caused by electromagnetic forces pushing the smallest grains out of the <span class="hlt">ring</span> plane. Because of shadowing, the halo is not visible close to Jupiter in the lower right part of the mosaic.<p/>Jupiter's main <span class="hlt">ring</span> is a thin strand of material encircling the planet. The diffuse innermost boundary begins at approximately 123,000 km. The main <span class="hlt">ring</span>'s outer radius is found to be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.1965B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.1965B"><span>Forward modeling of tree-<span class="hlt">ring</span> data: a case study with a global network</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Breitenmoser, P. D.; Frank, D.; Brönnimann, S.</p> <p>2012-04-01</p> <p>Information derived from tree-<span class="hlt">rings</span> is one of the most powerful tools presently available for studying past climatic variability as well as identifying fundamental relationships between tree-growth and climate. Climate reconstructions are typically performed by extending linear relationships, established during the overlapping period of instrumental and climate proxy archives into the past. Such analyses, however, are limited by methodological assumptions, including stationarity and linearity of the climate-proxy relationship. We investigate climate and tree-<span class="hlt">ring</span> data using the Vaganov-Shashkin-Lite (VS-Lite) forward model of tree-<span class="hlt">ring</span> width formation to examine the relations among actual tree growth and climate (as inferred from the simulated chronologies) to reconstruct past climate variability. The VS-lite model has been shown to produce skill comparable to that achieved using classical dendrochronological statistical modeling techniques when applied on simulations of a network of North American tree-<span class="hlt">ring</span> chronologies. Although the detailed mechanistic processes such as photosynthesis, <span class="hlt">storage</span>, or cell processes are not modeled directly, the net effect of the dominating nonlinear climatic controls on tree-growth are implemented into the model by the principle of limiting factors and threshold growth response functions. The VS-lite model requires as inputs only latitude, monthly mean temperature and monthly accumulated precipitation. Hence, this simple, process-based model enables <span class="hlt">ring</span>-width simulation at any location where monthly climate records exist. In this study, we analyse the growth response of simulated tree-<span class="hlt">rings</span> to monthly climate conditions obtained from the 20th century reanalysis project back to 1871. These simulated tree-<span class="hlt">ring</span> chronologies are compared to the climate-driven variability in worldwide observed tree-<span class="hlt">ring</span> chronologies from the International Tree <span class="hlt">Ring</span> Database. Results point toward the suitability of the relationship among actual tree</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA02251&hterms=Natural+hair&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DNatural%2Bhair','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA02251&hterms=Natural+hair&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DNatural%2Bhair"><span>Jupiter's <span class="hlt">ring</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>1979-01-01</p> <p>First evidence of a <span class="hlt">ring</span> around the planet Jupiter is seen in this photograph taken by Voyager 1 on March 4, 1979. The multiple exposure of the extremely thin faint <span class="hlt">ring</span> appears as a broad light band crossing the center of the picture. The edge of the <span class="hlt">ring</span> is 1,212,000 km from the spacecraft and 57,000 km from the visible cloud deck of Jupiter. The background stars look like broken hair pins because of spacecraft motion during the 11 minute 12 second exposure. The wavy motion of the star trails is due to the ultra-slow natural oscillation of the spacecraft (with a period of 78 seconds). The black dots are geometric calibration points in the camera. The <span class="hlt">ring</span> thickness is estimated to be 30 km or less. The photograph was part of a sequence planned to search for such <span class="hlt">rings</span> in Jupiter's equatorial plane. The <span class="hlt">ring</span> has been invisible from Earth because of its thinness and its transparency when viewed at any angle except straight on. JPL manages and controls the Voyager Project for NASA's Office of Space Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Icar..226.1275S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Icar..226.1275S"><span>The vertical structure of the F <span class="hlt">ring</span> of Saturn from <span class="hlt">ring</span>-plane crossings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scharringhausen, Britt R.; Nicholson, Philip D.</p> <p>2013-11-01</p> <p>We present a photometric model of the <span class="hlt">rings</span> of Saturn which includes the main <span class="hlt">rings</span> and an F <span class="hlt">ring</span>, inclined to the main <span class="hlt">rings</span>, with a Gaussian vertical profile of optical depth. This model reproduces the asymmetry in brightness between the east and west ansae of the <span class="hlt">rings</span> of Saturn that was observed by the Hubble Space Telescope (HST) within a few hours after the Earth <span class="hlt">ring</span>-plane crossing (RPX) of 10 August 1995. The model shows that during this observation the inclined F <span class="hlt">ring</span> unevenly blocked the east and west ansae of the main <span class="hlt">rings</span>. The brightness asymmetry produced by the model is highly sensitive to the vertical thickness and radial optical depth of the F <span class="hlt">ring</span>. The F-<span class="hlt">ring</span> model that best matches the observations has a vertical full width at half maximum of 13 ± 7 km and an equivalent depth of 10 ± 4 km. The model also reproduces the shape of the HST profiles of <span class="hlt">ring</span> brightness vs. distance from Saturn, both before and after the time of <span class="hlt">ring</span>-plane crossing. Smaller asymmetries observed before the RPX, when the Earth was on the dark side of the <span class="hlt">rings</span>, cannot be explained by blocking of the main <span class="hlt">rings</span> by the F <span class="hlt">ring</span> or vice versa and are probably instead due to the intrinsic longitudinal variation exhibited by the F <span class="hlt">ring</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19113769','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19113769"><span>Measurement of the branching fractions of B-->D**(l) nu(l) decays in <span class="hlt">events</span> tagged by a fully reconstructed B meson.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aubert, B; Bona, M; Karyotakis, Y; Lees, J P; Poireau, V; Prencipe, E; Prudent, X; Tisserand, V; Garra Tico, J; Grauges, E; Lopez, L; Palano, A; Pappagallo, M; Eigen, G; Stugu, B; Sun, L; Abrams, G S; Battaglia, M; Brown, D N; Cahn, R N; Jacobsen, R G; Kerth, L T; Kolomensky, Yu G; Lynch, G; Osipenkov, I L; Ronan, M T; Tackmann, K; Tanabe, T; Hawkes, C M; Soni, N; Watson, A T; Koch, H; Schroeder, T; Walker, D; Asgeirsson, D J; Fulsom, B G; Hearty, C; Mattison, T S; Mckenna, J A; Barrett, M; Khan, A; Blinov, V E; Bukin, A D; Buzykaev, A R; Druzhinin, V P; Golubev, V B; Onuchin, A P; Serednyakov, S I; Skovpen, Yu I; Solodov, E P; Todyshev, K Yu; Bondioli, M; Curry, S; Eschrich, I; Kirkby, D; Lankford, A J; Lund, P; Mandelkern, M; Martin, E C; Stoker, D P; Abachi, S; Buchanan, C; Gary, J W; Liu, F; Long, O; Shen, B C; Vitug, G M; Yasin, Z; Zhang, L; Sharma, V; Campagnari, C; Hong, T M; Kovalskyi, D; Mazur, M A; Richman, J D; Beck, T W; Eisner, A M; Flacco, C J; Heusch, C A; Kroseberg, J; Lockman, W S; Schalk, T; Schumm, B A; Seiden, A; Wang, L; Wilson, M G; Winstrom, L O; Cheng, C H; Doll, D A; Echenard, B; Fang, F; Hitlin, D G; Narsky, I; Piatenko, T; Porter, F C; Andreassen, R; Mancinelli, G; Meadows, B T; Mishra, K; Sokoloff, M D; Bloom, P C; Ford, W T; Gaz, A; Hirschauer, J F; Nagel, M; Nauenberg, U; Smith, J G; Ulmer, K A; Wagner, S R; Ayad, R; Soffer, A; Toki, W H; Wilson, R J; Altenburg, D D; Feltresi, E; Hauke, A; Jasper, H; Karbach, M; Merkel, J; Petzold, A; Spaan, B; Wacker, K; Kobel, M J; Mader, W F; Nogowski, R; Schubert, K R; Schwierz, R; Sundermann, J E; Volk, A; Bernard, D; Bonneaud, G R; Latour, E; Thiebaux, Ch; Verderi, M; Clark, P J; Gradl, W; Playfer, S; Watson, J E; Andreotti, M; Bettoni, D; Bozzi, C; Calabrese, R; Cecchi, A; Cibinetto, G; Franchini, P; Luppi, E; Negrini, M; Petrella, A; Piemontese, L; Santoro, V; Baldini-Ferroli, R; Calcaterra, A; de Sangro, R; Finocchiaro, G; Pacetti, S; Patteri, P; Peruzzi, I M; Piccolo, M; Rama, M; Zallo, A; Buzzo, A; Contri, R; Lo Vetere, M; Macri, M M; Monge, M R; Passaggio, S; Patrignani, C; Robutti, E; Santroni, A; Tosi, S; Chaisanguanthum, K S; Morii, M; Marks, J; Schenk, S; Uwer, U; Klose, V; Lacker, H M; Bard, D J; Dauncey, P D; Nash, J A; Panduro Vazquez, W; Tibbetts, M; Behera, P K; Chai, X; Charles, M J; Mallik, U; Cochran, J; Crawley, H B; Dong, L; Meyer, W T; Prell, S; Rosenberg, E I; Rubin, A E; Gao, Y Y; Gritsan, A V; Guo, Z J; Lae, C K; Denig, A G; Fritsch, M; Schott, G; Arnaud, N; Béquilleux, J; D'Orazio, A; Davier, M; Firmino da Costa, J; Grosdidier, G; Höcker, A; Lepeltier, V; Le Diberder, F; Lutz, A M; Pruvot, S; Roudeau, P; Schune, M H; Serrano, J; Sordini, V; Stocchi, A; Wormser, G; Lange, D J; Wright, D M; Bingham, I; Burke, J P; Chavez, C A; Fry, J R; Gabathuler, E; Gamet, R; Hutchcroft, D E; Payne, D J; Touramanis, C; Bevan, A J; Clarke, C K; George, K A; Di Lodovico, F; Sacco, R; Sigamani, M; Cowan, G; Flaecher, H U; Hopkins, D A; Paramesvaran, S; Salvatore, F; Wren, A C; Brown, D N; Davis, C L; Alwyn, K E; Bailey, D; Barlow, R J; Chia, Y M; Edgar, C L; Jackson, G; Lafferty, G D; West, T J; Yi, J I; Anderson, J; Chen, C; Jawahery, A; Roberts, D A; Simi, G; Tuggle, J M; Dallapiccola, C; Li, X; Salvati, E; Saremi, S; Cowan, R; Dujmic, D; Fisher, P H; Koeneke, K; Sciolla, G; Spitznagel, M; Taylor, F; Yamamoto, R K; Zhao, M; Patel, P M; Robertson, S H; Lazzaro, A; Lombardo, V; Palombo, E; Bauer, J M; Cremaldi, L; Eschenburg, V; Godang, R; Kroeger, R; Sanders, D A; Summers, D J; Zhao, H W; Simard, M; Taras, P; Viaud, F B; Nicholson, H; De Nardo, G; Lista, L; Monorchio, D; Onorato, G; Sciacca, C; Raven, G; Snoek, H L; Jessop, C P; Knoepfel, K J; Lo Secco, J M; Wang, W F; Benelli, G; Corwin, L A; Honscheid, K; Kagan, H; Kass, R; Morris, J P; Rahimi, A M; Regensburger, J J; Sekula, S J; Wong, Q K; Blount, N L; Brau, J; Frey, R; Igonkina, O; Kolb, J A; Lu, M; Rahmat, R; Sinev, N B; Strom, D; Strube, J; Torrence, E; Castelli, G; Gagliardi, N; Margoni, M; Morandin, M; Posocco, M; Rotondo, M; Simonetto, F; Stroili, R; Voci, C; del Amo Sanchez, P; Ben-Haim, E; Briand, H; Calderini, G; Chauveau, J; David, P; Del Buono, L; Hamon, O; Leruste, Ph; Ocariz, J; Perez, A; Prendki, J; Sitt, S; Gladney, L; Biasini, M; Covarelli, R; Manoni, E; Angelini, C; Batignani, G; Bettarini, S; Carpinelli, M; Cervelli, A; Forti, E; Giorgi, M A; Lusiani, A; Marchiori, G; Morganti, M; Neri, N; Paoloni, E; Rizzo, G; Walsh, J J; Lopes Pegna, D; Lu, C; Olsen, J; Smith, A J S; Telnov, A V; Anulli, F; Baracchini, E; Cavoto, G; del Re, D; Di Marco, E; Faccini, R; Ferrarotto, F; Ferroni, F; Gaspero, M; Jackson, P D; Li Gioi, L; Mazzoni, M A; Morganti, S; Piredda, G; Polci, F; Renga, F; Voena, C; Ebert, M; Hartmann, T; Schröder, H; Waldi, R; Adye, T; Franek, B; Olaiya, E O; Wilson, F F; Emery, S; Escalier, M; Esteve, L; Ganzhur, S F; Hamel de Monchenault, G; Kozanecki, W; Vasseur, G; Yèche, Ch; Zito, M; Chen, X R; Liu, H; Park, W; Purohit, M V; White, R M; Wilson, J R; Allen, M T; Aston, D; Bartoldus, R; Bechtle, P; Benitez, J F; Cenci, R; Coleman, J P; Convery, M R; Dingfelder, J C; Dorfan, J; Dubois-Felsmann, G P; Dunwoodie, W; Field, R C; Gabareen, A M; Gowdy, S J; Graham, M T; Grenier, P; Hast, C; Innes, W R; Kaminski, J; Kelsey, M H; Kim, H; Kim, P; Kocian, M L; Leith, D W G S; Li, S; Lindquist, B; Luitz, S; Luth, V; Lynch, H L; MacFarlane, D B; Marsiske, H; Messner, R; Muller, D R; Neal, H; Nelson, S; O'Grady, C P; Ofte, I; Perazzo, A; Perl, M; Ratcliff, B N; Roodman, A; Salnikov, A A; Schindler, R H; Schwiening, J; Snyder, A; Su, D; sullivan, M K; Suzuki, K; Swain, S K; Thompson, J M; Va'vra, J; Wagner, A P; Weaver, M; West, C A; Wisniewski, W J; Wittgen, M; Wright, D H; Wulsin, H W; Yarritu, A K; Yi, K; Young, C C; Ziegler, V; Burchat, P R; Edwards, A J; Majewski, S A; Miyashita, T S; Petersen, B A; Wilden, L; Ahmed, S; Alam, M S; Ernst, J A; Pan, B; Saeed, M A; Zain, S B; Spanier, S M; Wogsland, B J; Eckmann, R; Ritchie, J L; Ruland, A M; Schilling, C J; Schwitters, R F; Drummond, B W; Izen, J M; Lou, X C; Bianchi, F; Gamba, D; Pelliccioni, M; Bomben, M; Bosisio, L; Cartaro, C; Della Ricca, G; Lanceri, L; Vitale, L; Azzolini, V; Lopez-March, N; Martinez-Vidal, F; Milanes, D A; Oyanguren, A; Albert, J; Banerjee, Sw; Bhuyan, B; Choi, H H F; Hamano, K; Kowalewski, R; Lewczuk, M J; Nugent, I M; Roney, J M; Sobie, R J; Gershon, T J; Harrison, P F; Ilic, J; Latham, T E; Mohanty, G B; Band, H R; Chen, X; Dasu, S; Flood, K T; Pan, Y; Pierini, M; Prepost, R; Vuosalo, C O; Wu, S L</p> <p>2008-12-31</p> <p>We report a measurement of the branching fractions of B-->D**(l) nu(l), decays based on 417 fb(-1) of data collected at the Y(4S) resonance with the BABAR detector at the PEP-II e+e- <span class="hlt">storage</span> <span class="hlt">rings</span>. <span class="hlt">Events</span> are selected by full reconstructing one of the B mesons in a hadronic decay mode. A fit to the invariant mass differences m(D(*) pi)- m(D(*)) is performed to extract the signal yields of the different D** states. We observe the B-->D**l(-1)nu(l) decay modes corresponding to the four D states predicted by heavy quark symmetry with a significance greater than 5 standard deviations including systematic uncertainties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012PApGe.169.2181R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012PApGe.169.2181R"><span>Solar-Terrestrial Signal Record in Tree <span class="hlt">Ring</span> Width Time Series from Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rigozo, Nivaor Rodolfo; Lisi, Cláudio Sergio; Filho, Mário Tomazello; Prestes, Alan; Nordemann, Daniel Jean Roger; de Souza Echer, Mariza Pereira; Echer, Ezequiel; da Silva, Heitor Evangelista; Rigozo, Valderez F.</p> <p>2012-12-01</p> <p>This work investigates the behavior of the sunspot number and Southern Oscillation Index (SOI) signal recorded in the tree <span class="hlt">ring</span> time series for three different locations in Brazil: Humaitá in Amazônia State, Porto Ferreira in São Paulo State, and Passo Fundo in Rio Grande do Sul State, using wavelet and cross-wavelet analysis techniques. The wavelet spectra of tree <span class="hlt">ring</span> time series showed signs of 11 and 22 years, possibly related to the solar activity, and periods of 2-8 years, possibly related to El Niño <span class="hlt">events</span>. The cross-wavelet spectra for all tree <span class="hlt">ring</span> time series from Brazil present a significant response to the 11-year solar cycle in the time interval between 1921 to after 1981. These tree <span class="hlt">ring</span> time series still have a response to the second harmonic of the solar cycle (5.5 years), but in different time intervals. The cross-wavelet maps also showed that the relationship between the SOI x tree <span class="hlt">ring</span> time series is more intense, for oscillation in the range of 4-8 years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29813074','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29813074"><span>Safety of a silicone elastomer vaginal <span class="hlt">ring</span> as potential microbicide delivery method in African women: A Phase 1 randomized trial.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nel, Annaléne; Martins, Janine; Bekker, Linda-Gail; Ramjee, Gita; Masenga, Gileard; Rees, Helen; van Niekerk, Neliëtte</p> <p>2018-01-01</p> <p>Women in sub-Saharan Africa are in urgent need of female-initiated human immunodeficiency virus (HIV) preventative methods. Vaginal <span class="hlt">rings</span> are one dosage form in development for delivery of HIV microbicides. However, African women have limited experience with vaginal <span class="hlt">rings</span>. This Phase I, randomized, crossover trial assessed and compared the safety, acceptability and adherence of a silicone elastomer placebo vaginal <span class="hlt">ring</span>, intended as a microbicide delivery method, inserted for a 12-week period in healthy, HIV-negative, sexually active women in South Africa and Tanzania. 170 women, aged 18 to 35 years were enrolled with 88 women randomized to Group A, using a placebo vaginal <span class="hlt">ring</span> for 12 weeks followed by a 12-week safety observation period. 82 women were randomized to Group B and observed for safety first, followed by a placebo vaginal <span class="hlt">ring</span> for 12 weeks. Safety was assessed by clinical laboratory assessments, pelvic/colposcopy examinations and adverse <span class="hlt">events</span>. Possible carry-over effect was addressed by ensuring no signs or symptoms of genital irritation at crossover. No safety concerns were identified for any safety variables assessed during the trial. No serious adverse <span class="hlt">events</span> were reported considered related to the placebo vaginal <span class="hlt">ring</span>. Vaginal candidiasis was the most common adverse <span class="hlt">event</span> occurring in 11% of participants during each trial period. Vaginal discharge (2%), vaginal odour (2%), and bacterial vaginitis (2%) were assessed as possibly or probably related to the vaginal <span class="hlt">ring</span>. Thirty-four percent of participants had sexually transmitted infections (STIs) at screening, compared to 12% of participants who tested positive for STIs at crossover and the final trial visit. Three participants (2%) tested HIV positive during the trial. The silicone elastomer vaginal <span class="hlt">ring</span> had no safety concerns, demonstrating a profile favorable for further development for topical release of antiretroviral-based microbicides.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5973569','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5973569"><span>Safety of a silicone elastomer vaginal <span class="hlt">ring</span> as potential microbicide delivery method in African women: A Phase 1 randomized trial</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Nel, Annaléne; Bekker, Linda-Gail; Ramjee, Gita; Masenga, Gileard; Rees, Helen; van Niekerk, Neliëtte</p> <p>2018-01-01</p> <p>Background Women in sub-Saharan Africa are in urgent need of female-initiated human immunodeficiency virus (HIV) preventative methods. Vaginal <span class="hlt">rings</span> are one dosage form in development for delivery of HIV microbicides. However, African women have limited experience with vaginal <span class="hlt">rings</span>. Objectives This Phase I, randomized, crossover trial assessed and compared the safety, acceptability and adherence of a silicone elastomer placebo vaginal <span class="hlt">ring</span>, intended as a microbicide delivery method, inserted for a 12-week period in healthy, HIV-negative, sexually active women in South Africa and Tanzania. Methods 170 women, aged 18 to 35 years were enrolled with 88 women randomized to Group A, using a placebo vaginal <span class="hlt">ring</span> for 12 weeks followed by a 12-week safety observation period. 82 women were randomized to Group B and observed for safety first, followed by a placebo vaginal <span class="hlt">ring</span> for 12 weeks. Safety was assessed by clinical laboratory assessments, pelvic/colposcopy examinations and adverse <span class="hlt">events</span>. Possible carry-over effect was addressed by ensuring no signs or symptoms of genital irritation at crossover. Results No safety concerns were identified for any safety variables assessed during the trial. No serious adverse <span class="hlt">events</span> were reported considered related to the placebo vaginal <span class="hlt">ring</span>. Vaginal candidiasis was the most common adverse <span class="hlt">event</span> occurring in 11% of participants during each trial period. Vaginal discharge (2%), vaginal odour (2%), and bacterial vaginitis (2%) were assessed as possibly or probably related to the vaginal <span class="hlt">ring</span>. Thirty-four percent of participants had sexually transmitted infections (STIs) at screening, compared to 12% of participants who tested positive for STIs at crossover and the final trial visit. Three participants (2%) tested HIV positive during the trial. Conclusions The silicone elastomer vaginal <span class="hlt">ring</span> had no safety concerns, demonstrating a profile favorable for further development for topical release of antiretroviral-based microbicides. PMID</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27286876','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27286876"><span>Natural variation in expression of genes associated with carotenoid biosynthesis and accumulation in cassava (Manihot esculenta Crantz) <span class="hlt">storage</span> root.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carvalho, Luiz Jcb; Agustini, Marco Av; Anderson, James V; Vieira, Eduardo A; de Souza, Claudia Rb; Chen, Songbi; Schaal, Barbara A; Silva, Joseane P</p> <p>2016-06-10</p> <p>Cassava (Manihot esculenta Crantz) <span class="hlt">storage</span> root provides a staple food source for millions of people worldwide. Increasing the carotenoid content in <span class="hlt">storage</span> root of cassava could provide improved nutritional and health benefits. Because carotenoid accumulation has been associated with <span class="hlt">storage</span> root color, this study characterized carotenoid profiles, and abundance of key transcripts associated with carotenoid biosynthesis, from 23 landraces of cassava <span class="hlt">storage</span> root ranging in color from white-to-yellow-to-pink. This study provides important information to plant breeding programs aimed at improving cassava <span class="hlt">storage</span> root nutritional quality. Among the 23 landraces, five carotenoid types were detected in <span class="hlt">storage</span> root with white color, while carotenoid types ranged from 1 to 21 in <span class="hlt">storage</span> root with pink and yellow color. The majority of <span class="hlt">storage</span> root in these landraces ranged in color from pale-to-intense yellow. In this color group, total β-carotene, containing all-E-, 9-Z-, and 13-Z-β-carotene isomers, was the major carotenoid type detected, varying from 26.13 to 76.72 %. Although no α-carotene was observed, variable amounts of a α-<span class="hlt">ring</span> derived xanthophyll, lutein, was detected; with greater accumulation of α-<span class="hlt">ring</span> xanthophylls than of β-<span class="hlt">ring</span> xanthophyll. Lycopene was detected in a landrace (Cas51) with pink color <span class="hlt">storage</span> root, but it was not detected in <span class="hlt">storage</span> root with yellow color. Based on microarray and qRT-PCR analyses, abundance of transcripts coding for enzymes involved in carotenoid biosynthesis were consistent with carotenoid composition determined by contrasting HPLC-Diode Array profiles from <span class="hlt">storage</span> root of landraces IAC12, Cas64, and Cas51. Abundance of transcripts encoding for proteins regulating plastid division were also consistent with the observed differences in total β-carotene accumulation. Among the 23 cassava landraces with varying <span class="hlt">storage</span> root color and diverse carotenoid types and profiles, landrace Cas51 (pink color <span class="hlt">storage</span> root) had low</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA00658&hterms=Lenticular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DLenticular','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA00658&hterms=Lenticular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DLenticular"><span>Jupiter's <span class="hlt">Ring</span> Halo</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>A mosaic of four images taken through the clear filter (610 nanometers) of the solid state imaging (CCD) system aboard NASA's Galileo spacecraft on November 8, 1996, at a resolution of approximately 46 kilometers (km) per picture element (pixel) along the <span class="hlt">rings</span>; however, because the spacecraft was only about 0.5 degrees above the <span class="hlt">ring</span> plane, the image is highly foreshortened in the vertical direction. The images were obtained when Galileo was in Jupiter's shadow peering back toward the Sun; the <span class="hlt">ring</span> was approximately 2,300,000 kilometers (km) away. The arc on the far right of the image is produced by sunlight scattered by small particles comprising Jupiter's upper atmospheric haze. The <span class="hlt">ring</span> also efficiently scatters light, indicating that much of its brightness is due to particles that are microns or less in diameter. Such small particles are believed to have human-scale lifetimes, i.e., very brief compared to the solar system's age.<p/>Jupiter's <span class="hlt">ring</span> system is composed of three parts -- a flat main <span class="hlt">ring</span>, a lenticular halo interior to the main <span class="hlt">ring</span>, and the gossamer <span class="hlt">ring</span>, which lies exterior to the main <span class="hlt">ring</span>. The near and far arms of Jupiter's main <span class="hlt">ring</span> extend horizontally across the mosaic, joining together at the <span class="hlt">ring</span>'s ansa, on the far left side of the figure. The near arm of the <span class="hlt">ring</span> appears to be abruptly truncated close to the planet, at the point where it passes into Jupiter's shadow.<p/>A faint mist of particles can be seen above and below the main <span class="hlt">rings</span>; this vertically extended, toroidal 'halo' is unusual in planetary <span class="hlt">rings</span>, and is probably caused by electromagnetic forces which can push small grains out of the <span class="hlt">ring</span> plane. Halo material is present across this entire image, implying that it reaches more than 27,000 km above the <span class="hlt">ring</span> plane. Because of shadowing, the halo is not visible close to Jupiter in the lower right part of the mosaic. In order to accentuate faint features in the image, different brightnesses are shown through color, with the brightest</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA10094.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA10094.html"><span>Saturn <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2007-12-12</p> <p>Like Earth, Saturn has an invisible <span class="hlt">ring</span> of energetic ions trapped in its magnetic field. This feature is known as a "<span class="hlt">ring</span> current." This <span class="hlt">ring</span> current has been imaged with a special camera on Cassini sensitive to energetic neutral atoms. This is a false color map of the intensity of the energetic neutral atoms emitted from the <span class="hlt">ring</span> current through a processed called charged exchange. In this process a trapped energetic ion steals and electron from cold gas atoms and becomes neutral and escapes the magnetic field. The Cassini Magnetospheric Imaging Instrument's ion and neutral camera records the intensity of the escaping particles, which provides a map of the <span class="hlt">ring</span> current. In this image, the colors represent the intensity of the neutral emission, which is a reflection of the trapped ions. This "<span class="hlt">ring</span>" is much farther from Saturn (roughly five times farther) than Saturn's famous icy <span class="hlt">rings</span>. Red in the image represents the higher intensity of the particles, while blue is less intense. Saturn's <span class="hlt">ring</span> current had not been mapped before on a global scale, only "snippets" or areas were mapped previously but not in this detail. This instrument allows scientists to produce movies (see PIA10083) that show how this <span class="hlt">ring</span> changes over time. These movies reveal a dynamic system, which is usually not as uniform as depicted in this image. The <span class="hlt">ring</span> current is doughnut shaped but in some instances it appears as if someone took a bite out of it. This image was obtained on March 19, 2007, at a latitude of about 54.5 degrees and radial distance 1.5 million kilometres (920,000 miles). Saturn is at the center, and the dotted circles represent the orbits of the moon's Rhea and Titan. The Z axis points parallel to Saturn's spin axis, the X axis points roughly sunward in the sun-spin axis plane, and the Y axis completes the system, pointing roughly toward dusk. The ion and neutral camera's field of view is marked by the white line and accounts for the cut-off of the image on the left. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA02251.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA02251.html"><span>Jupiter <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2000-03-23</p> <p>First evidence of a <span class="hlt">ring</span> around the planet Jupiter is seen in this photograph taken by Voyager 1 on March 4, 1979. The multiple exposure of the extremely thin faint <span class="hlt">ring</span> appears as a broad light band crossing the center of the picture. The edge of the <span class="hlt">ring</span> is 1,212,000 km from the spacecraft and 57,000 km from the visible cloud deck of Jupiter. The background stars look like broken hair pins because of spacecraft motion during the 11 minute 12 second exposure. The wavy motion of the star trails is due to the ultra-slow natural oscillation of the spacecraft (with a period of 78 seconds). The black dots are geometric calibration points in the camera. The <span class="hlt">ring</span> thickness is estimated to be 30 km or less. The photograph was part of a sequence planned to search for such <span class="hlt">rings</span> in Jupiter's equatorial plane. The <span class="hlt">ring</span> has been invisible from Earth because of its thinness and its transparency when viewed at any angle except straight on. JPL manages and controls the Voyager Project for NASA's Office of Space Science. http://photojournal.jpl.nasa.gov/catalog/PIA02251</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014NIMPA.748...96A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014NIMPA.748...96A"><span>Vertical beam size measurement in the CESR-TA e+e- <span class="hlt">storage</span> <span class="hlt">ring</span> using x-rays from synchrotron radiation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alexander, J. P.; Chatterjee, A.; Conolly, C.; Edwards, E.; Ehrlichman, M. P.; Fontes, E.; Heltsley, B. K.; Hopkins, W.; Lyndaker, A.; Peterson, D. P.; Rider, N. T.; Rubin, D. L.; Savino, J.; Seeley, R.; Shanks, J.; Flanagan, J. W.</p> <p>2014-06-01</p> <p>We describe the construction and operation of an X-ray beam size monitor (xBSM), a device measuring e+ and e- beam sizes in the CESR-TA <span class="hlt">storage</span> <span class="hlt">ring</span> using synchrotron radiation. The device can measure vertical beam sizes of 10-100μm on a turn-by-turn, bunch-by-bunch basis at e± beam energies of ~2GeV. At such beam energies the xBSM images X-rays of ɛ≈1-10keV (λ≈0.1-1nm) that emerge from a hard-bend magnet through a single- or multiple-slit (coded aperture) optical element onto an array of 32 InGaAs photodiodes with 50μm pitch. Beamlines and detectors are entirely in-vacuum, enabling single-shot beam size measurement down to below 0.1 mA (2.5×109 particles) per bunch and inter-bunch spacing of as little as 4 ns. At Eb=2.1GeV, systematic precision of ~1μm is achieved for a beam size of ~12μm; this is expected to scale as ∝1/σb and ∝1/Eb. Achieving this precision requires comprehensive alignment and calibration of the detector, optical elements, and X-ray beam. Data from the xBSM have been used to extract characteristics of beam oscillations on long and short timescales, and to make detailed studies of low-emittance tuning, intra-beam scattering, electron cloud effects, and multi-bunch instabilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21171615','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21171615"><span>Topological <span class="hlt">ring</span> currents in the "empty" <span class="hlt">ring</span> of benzo-annelated perylenes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dickens, Timothy K; Mallion, Roger B</p> <p>2011-01-27</p> <p>Cyclic conjugation in benzo-annelated perylenes is examined by means of the topological π-electron <span class="hlt">ring</span> currents calculated for each of their constituent <span class="hlt">rings</span>, in a study that is an exact analogy of a recent investigation by Gutman et al. based on energy-effect values for the corresponding <span class="hlt">rings</span> in each of these structures. "Classical" approaches, such as Kekulé structures, Clar "sextet" formulas, and circuits of conjugation, predict that the central <span class="hlt">ring</span> in perylene is "empty" and thus contributes negligibly to cyclic conjugation. However, conclusions from the present calculations of topological <span class="hlt">ring</span> currents agree remarkably with those arising from the earlier study involving energy-effect values in that, contrary to what would be predicted from the classical approaches, <span class="hlt">rings</span> annelated in an angular fashion relative to the central <span class="hlt">ring</span> of these perylene structures materially increase the extent of that <span class="hlt">ring</span>'s involvement in cyclic conjugation. It is suggested that such close quantitative agreement between the predictions of these two superficially very different indices (energy effect and topological <span class="hlt">ring</span> current) might be due to the fact that, ultimately, both depend, albeit in ostensibly quite different ways, only on an adjacency matrix that contains information about the carbon-carbon connectivity of the conjugated system in question.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29913613','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29913613"><span>Influence of recent climatic <span class="hlt">events</span> on the surface water <span class="hlt">storage</span> of the Tonle Sap Lake.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Frappart, F; Biancamaria, S; Normandin, C; Blarel, F; Bourrel, L; Aumont, M; Azemar, P; Vu, P-L; Le Toan, T; Lubac, B; Darrozes, J</p> <p>2018-09-15</p> <p>Lakes and reservoirs have been identified as sentinels of climate change. Tonle Sap is the largest lake in both the Mekong Basin and Southeast Asia and because of the importance of its ecosystem, it is has been described as the "heart of the lower Mekong". Its seasonal cycle depends on the annual flood pulse governed by the flow of the Mekong River. This study provides an impact analysis of recent climatic <span class="hlt">events</span> from El Niño 1997/1998 to El Niño 2015/2016 on surface <span class="hlt">storage</span> variations in the Tonle Sap watershed determined by combining remotely sensed observations, multispectral images and radar altimetry from 1993 to 2017. The Lake's surface water volume variations are highly correlated with rainy season rainfall in the whole Mekong River Basin (R = 0.84) at interannual time-scale. Extreme droughts and floods can be observed when precipitation deficit and excess is recorded in both the Tonle Sap watershed and the Mekong River Basin during moderate to very strong El Niño/La Niña <span class="hlt">events</span> (R = -0.70) enhanced by the Pacific Decadal Oscillation (R = -0.68). Indian and Western North Pacific Monsoons were identified as having almost equal influence. Below normal vegetation activity was observed during the first semester of 2016 due to the extreme drought in 2015. Copyright © 2018 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhTea..54..112J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhTea..54..112J"><span>DC-Powered Jumping <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeffery, Rondo N.; Amiri, Farhang</p> <p>2016-02-01</p> <p>The classroom jumping <span class="hlt">ring</span> demonstration is nearly always performed using alternating current (AC), in which the <span class="hlt">ring</span> jumps or flies off the extended iron core when the switch is closed. The <span class="hlt">ring</span> jumps higher when cooled with liquid nitrogen (LN2). We have performed experiments using DC to power the solenoid and find similarities and significant differences from the AC case. In particular, the <span class="hlt">ring</span> does not fly off the core but rises a short distance and then falls back. If the <span class="hlt">ring</span> jumps high enough, the rising and the falling motion of the <span class="hlt">ring</span> does not follow simple vertical motion of a projectile. This indicates that there are additional forces on the <span class="hlt">ring</span> in each part of its motion. Four possible stages of the motion of the <span class="hlt">ring</span> with DC are identified, which result from the <span class="hlt">ring</span> current changing directions during the jump in response to a changing magnetic flux through the moving <span class="hlt">ring</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA02293&hterms=makeup&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmakeup','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA02293&hterms=makeup&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dmakeup"><span>Saturn's F-<span class="hlt">Ring</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>2000-01-01</p> <p>This narrow-angle camera image of Saturn's F <span class="hlt">Ring</span> was taken through the Clear filter while at a distance of 6.9 million km from Saturn on 8 November 1980. The brightness variations of this tightly-constrained <span class="hlt">ring</span> shown here indicate that the <span class="hlt">ring</span> is less uniform in makeup than the larger <span class="hlt">rings</span>. JPL managed the Voyager Project for NASA's Office of Space Science</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.C23B..08K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.C23B..08K"><span>Monitoring Snow on ice as Critical Habitat for <span class="hlt">Ringed</span> Seals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kelly, B. P.; Moran, J.; Douglas, D. C.; Nghiem, S. V.</p> <p>2007-12-01</p> <p><span class="hlt">Ringed</span> seals are the primary prey of polar bears, and they are found in all seasonally ice covered seas of the northern hemisphere as well as in several freshwater lakes. The presence of snow covered sea ice is essential for successful <span class="hlt">ringed</span> seal reproduction. <span class="hlt">Ringed</span> seals abrade holes in the ice allowing them to surface and breathe under the snow cover. Where snow accumulates to sufficient depths, <span class="hlt">ringed</span> seals excavate subnivean lairs above breathing holes. They rest, give birth, and nurse their young in those lairs. Temperatures within the lairs remain within a few degrees of freezing, well within the zone of thermal neutrality for newborn <span class="hlt">ringed</span> seals, even at ambient temperatures of -30° C. High rates of seal mortality have been recorded when early snow melt caused lairs to collapse exposing newborn seals to predators and to subsequent extreme cold <span class="hlt">events</span>. As melt onset dates come earlier in the Arctic Ocean, <span class="hlt">ringed</span> seal populations (and the polar bears that depend upon them) will be increasingly challenged. We determined dates of lair abandonment by <span class="hlt">ringed</span> seals fitted with radio transmitters in the Beaufort Sea (n = 60). We compared abandonment dates to melt onset dates measured in the field, as well as estimated dates derived from active (Ku-band backscatter) and passive (SSM/I) microwave satellite imagery. Date of snow melt significantly improved models of environmental influences on the timing of lair abandonment. We used an algorithm based on multi-channel means and variances of passive microwave data to detect melt onset dates. Those melt onset dates predicted the date of lair abandonment ± 3 days (r 2 = 0.982, p = 0.001). The predictive power of passive microwave proxies combined with their historical record suggest they could serve to monitor critical changes to <span class="hlt">ringed</span> seal habitat.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001DDA....32.0101N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001DDA....32.0101N"><span>Planetary <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicholson, P. D.</p> <p>2001-11-01</p> <p>A revolution in the studies in planetary <span class="hlt">rings</span> studies occurred in the period 1977--1981, with the serendipitous discovery of the narrow, dark <span class="hlt">rings</span> of Uranus, the first Voyager images of the tenuous jovian <span class="hlt">ring</span> system, and the many spectacular images returned during the twin Voyager flybys of Saturn. In subsequent years, ground-based stellar occultations, HST observations, and the Voyager flybys of Uranus (1986) and Neptune (1989), as well as a handful of Galileo images, provided much additional information. Along with the completely unsuspected wealth of detail these observations revealed came an unwelcome problem: are the <span class="hlt">rings</span> ancient or are we privileged to live at a special time in history? The answer to this still-vexing question may lie in the complex gravitational interactions recent studies have revealed between the <span class="hlt">rings</span> and their retinues of attendant satellites. Among the four known <span class="hlt">ring</span> systems, we see elegant examples of Lindblad and corotation resonances (first invoked in the context of galactic disks), electromagnetic resonances, spiral density waves and bending waves, narrow ringlets which exhibit internal modes due to collective instabilities, sharp-edged gaps maintained via tidal torques from embedded moonlets, and tenuous dust belts created by meteoroid impact onto parent bodies. Perhaps most puzzling is Saturn's multi-stranded, clumpy F <span class="hlt">ring</span>, which continues to defy a simple explanation 20 years after it was first glimpsed in grainy images taken by Pioneer 11. Voyager and HST images reveal a complex, probably chaotic, dynamical interaction between unseen parent bodies within this <span class="hlt">ring</span> and its two shepherd satellites, Pandora and Prometheus. The work described here reflects contributions by Joe Burns, Jeff Cuzzi, Luke Dones, Dick French, Peter Goldreich, Colleen McGhee, Carolyn Porco, Mark Showalter, and Bruno Sicardy, as well as those of the author. This research has been supported by NASA's Planetary Geology and Geophysics program and the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009A%26A...507.1303F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009A%26A...507.1303F"><span>The <span class="hlt">ring</span> galaxy HRG 54 103: a first study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faúndez-Abans, M.; Fernandes, I. F.; de Oliveira-Abans, M.; Poppe, P. C. R.; Martin, V. A. F.</p> <p>2009-12-01</p> <p>Aims: We report the first study of the peculiar <span class="hlt">ring</span> galaxy HRG 54103 which was previously classified as a Saturn-like type galaxy. Methods: The study is based on low resolution spectroscopy and photometric observations in the optical band to highlight the characteristics of this almost isolated galaxy. The colour distribution of HRG 54103 was examined through direct CCD BVRI Kron-Cousins system imagery. Color-color diagrams of the bulge and <span class="hlt">ring</span> are displayed and further compared with the star-forming <span class="hlt">ring</span> galaxy HRG 2302. Results: The results of image enhancement of the morphological structure of this galaxy are discussed. The nuclear emission-line spectrum resembles that of a Seyfert2/LINER object, with z = 0.022 and heliocentric V = 6483 ± 18 km s-1, in agreement with the literature. The nuclear, bulge and <span class="hlt">ring</span> section radial velocities along the <span class="hlt">ring</span> major axis show a peculiar distribution, which together with the [N ii]/Hα and [S ii]/Hα ratios and image enhancement suggest an offset nucleus and an internal tilted <span class="hlt">ring</span> or shell. Conclusions: HRG 54103 is a peculiar galaxy with an intermediate activity region, probably due to a residual excitation effect through the central AGN phenomenon. The individual sections of the color-color map are redder than a typical star-forming <span class="hlt">ring</span> galaxy, in agreement with the behavior of the [S ii]/Hα versus [N ii]/Hα diagnostic diagram. The two bulge satellites, the plume-like appendix, and the disk-<span class="hlt">ring</span> asymmetry suggest a possible merger <span class="hlt">event</span> in the recent past of this object, which could also have caused its formation. Based on observations made at: (a) Observatório do Pico dos Dias, operated by MCT/Laboratório Nacional de Astrofísica, Brazil, and (b) Cerro Tololo Inter-American Observatory, National Optical Astronomy Observatories, which are operated by AURA, Inc., under contract to the National Science Foundation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA08262.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA08262.html"><span>The <span class="hlt">Ring</span> Sculptor</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2006-09-08</p> <p>Prometheus zooms across the Cassini spacecraft field of view, attended by faint streamers and deep gores in the F <span class="hlt">ring</span>. This movie sequence of five images shows the F <span class="hlt">ring</span> shepherd moon shaping the <span class="hlt">ring</span> inner edge</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22188645','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22188645"><span>Mechanisms of <span class="hlt">ring</span> chromosome formation, <span class="hlt">ring</span> instability and clinical consequences.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guilherme, Roberta S; Meloni, Vera F Ayres; Kim, Chong A; Pellegrino, Renata; Takeno, Sylvia S; Spinner, Nancy B; Conlin, Laura K; Christofolini, Denise M; Kulikowski, Leslie D; Melaragno, Maria I</p> <p>2011-12-21</p> <p>The breakpoints and mechanisms of <span class="hlt">ring</span> chromosome formation were studied and mapped in 14 patients. Several techniques were performed such as genome-wide array, MLPA (Multiplex Ligation-Dependent Probe Amplification) and FISH (Fluorescent in situ Hybridization). The <span class="hlt">ring</span> chromosomes of patients I to XIV were determined to be, respectively: r(3)(p26.1q29), r(4)(p16.3q35.2), r(10)(p15.3q26.2), r(10)(p15.3q26.13), r(13)(p13q31.1), r(13)(p13q34), r(14)(p13q32.33), r(15)(p13q26.2), r(18)(p11.32q22.2), r(18)(p11.32q21.33), r(18)(p11.21q23), r(22)(p13q13.33), r(22)(p13q13.2), and r(22)(p13q13.2). These <span class="hlt">rings</span> were found to have been formed by different mechanisms, such as: breaks in both chromosome arms followed by end-to-end reunion (patients IV, VIII, IX, XI, XIII and XIV); a break in one chromosome arm followed by fusion with the subtelomeric region of the other (patients I and II); a break in one chromosome arm followed by fusion with the opposite telomeric region (patients III and X); fusion of two subtelomeric regions (patient VII); and telomere-telomere fusion (patient XII). Thus, the r(14) and one r(22) can be considered complete <span class="hlt">rings</span>, since there was no loss of relevant genetic material. Two patients (V and VI) with r(13) showed duplication along with terminal deletion of 13q, one of them proved to be inverted, a mechanism known as inv-dup-del. <span class="hlt">Ring</span> instability was detected by <span class="hlt">ring</span> loss and secondary aberrations in all but three patients, who presented stable <span class="hlt">ring</span> chromosomes (II, XIII and XIV). We concluded that the clinical phenotype of patients with <span class="hlt">ring</span> chromosomes may be related with different factors, including gene haploinsufficiency, gene duplications and <span class="hlt">ring</span> instability. Epigenetic factors due to the circular architecture of <span class="hlt">ring</span> chromosomes must also be considered, since even complete <span class="hlt">ring</span> chromosomes can result in phenotypic alterations, as observed in our patients with complete r(14) and r(22).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhRvS..14j2401S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhRvS..14j2401S"><span>Force on a <span class="hlt">storage</span> <span class="hlt">ring</span> vacuum chamber after sudden turn-off of a magnet power supply</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sinha, Gautam; Prabhu, S. S.</p> <p>2011-10-01</p> <p>We are commissioning a 2.5 GeV synchrotron radiation source (SRS) where electrons travel in high vacuum inside the vacuum chambers made of aluminum alloys. These chambers are kept between the pole gaps of magnets and are made to facilitate the radiation coming out of the <span class="hlt">storage</span> <span class="hlt">ring</span> to the experimental station. These chambers are connected by metallic bellows. During the commissioning phase of the SRS, the metallic bellows became ruptured due to the frequent tripping of the dipole magnet power supply. The machine was down for quite some time. In the case of a power supply trip, the current in the magnets decays exponentially. It was observed experimentally that the fast B field decay generates a large eddy current in the chambers and consequently the chambers are subjected to a huge Lorentz force. This motivated us to develop a theoretical model to study the force acting on a metallic plate when exposed to an exponentially decaying field and then to extend it for a rectangular vacuum chamber. The problem is formulated using Maxwell’s equations and converted to the inhomogeneous Helmholtz equation. After taking the Laplace transform, the equation is solved with appropriate boundary conditions. Final results are obtained after taking the appropriate inverse Laplace transform. The expressions for eddy current contour and magnetic field produced by the eddy current are also derived. Variations of the force on chambers of different wall thickness due to spatially varying and exponentially time decaying field are presented. The result is a general theory which can be applied to different geometries and calculation of power loss as well. Comparisons are made with results obtained by simulation using a finite element based code, for quick verification of the theoretical model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhST..166a4053M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhST..166a4053M"><span>Experimental techniques for in-<span class="hlt">ring</span> reaction experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mutterer, M.; Egelhof, P.; Eremin, V.; Ilieva, S.; Kalantar-Nayestanaki, N.; Kiselev, O.; Kollmus, H.; Kröll, T.; Kuilman, M.; Chung, L. X.; Najafi, M. A.; Popp, U.; Rigollet, C.; Roy, S.; von Schmid, M.; Streicher, B.; Träger, M.; Yue, K.; Zamora, J. C.; the EXL Collaboration</p> <p>2015-11-01</p> <p>As a first step of the EXL project scheduled for the New Experimental <span class="hlt">Storage</span> <span class="hlt">Ring</span> at FAIR a precursor experiment (E105) was performed at the ESR at GSI. For this experiment, an innovative differential pumping concept, originally proposed for the EXL recoil detector ESPA, was successfully applied. The implementation and essential features of this novel technical concept will be discussed, as well as details on the detectors and the infrastructure around the internal gas-jet target. With 56Ni(p, p)56Ni elastic scattering at 400 MeV u-1, a nuclear reaction experiment with stored radioactive beams was realized for the first time. Finally, perspectives for a next-generation EXL-type setup are briefly discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1215633','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1215633"><span>The two-way relationship between ionospheric outflow and the <span class="hlt">ring</span> current</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>Welling, Daniel T.; Jordanova, Vania Koleva; Glocer, Alex</p> <p></p> <p>It is now well established that the ionosphere, because it acts as a significant source of plasma, plays a critical role in <span class="hlt">ring</span> current dynamics. However, because the <span class="hlt">ring</span> current deposits energy into the ionosphere, the inverse may also be true: the <span class="hlt">ring</span> current can play a critical role in the dynamics of ionospheric outflow. This study uses a set of coupled, first-principles-based numerical models to test the dependence of ionospheric outflow on <span class="hlt">ring</span> current-driven region 2 field-aligned currents (FACs). A moderate magnetospheric storm <span class="hlt">event</span> is modeled with the Space Weather Modeling Framework using a global MHD code (Block Adaptivemore » Tree Solar wind Roe-type Upwind Scheme, BATS-R-US), a polar wind model (Polar Wind Outflow Model), and a bounce-averaged kinetic <span class="hlt">ring</span> current model (<span class="hlt">ring</span> current atmosphere interaction model with self-consistent magnetic field, RAM-SCB). Initially, each code is two-way coupled to all others except for RAM-SCB, which receives inputs from the other models but is not allowed to feed back pressure into the MHD model. The simulation is repeated with pressure coupling activated, which drives strong pressure gradients and region 2 FACs in BATS-R-US. It is found that the region 2 FACs increase heavy ion outflow by up to 6 times over the non-coupled results. The additional outflow further energizes the <span class="hlt">ring</span> current, establishing an ionosphere-magnetosphere mass feedback loop. This study further demonstrates that ionospheric outflow is not merely a plasma source for the magnetosphere but an integral part in the nonlinear ionosphere-magnetosphere-<span class="hlt">ring</span> current system.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1215633-two-way-relationship-between-ionospheric-outflow-ring-current','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1215633-two-way-relationship-between-ionospheric-outflow-ring-current"><span>The two-way relationship between ionospheric outflow and the <span class="hlt">ring</span> current</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Welling, Daniel T.; Jordanova, Vania Koleva; Glocer, Alex; ...</p> <p>2015-06-01</p> <p>It is now well established that the ionosphere, because it acts as a significant source of plasma, plays a critical role in <span class="hlt">ring</span> current dynamics. However, because the <span class="hlt">ring</span> current deposits energy into the ionosphere, the inverse may also be true: the <span class="hlt">ring</span> current can play a critical role in the dynamics of ionospheric outflow. This study uses a set of coupled, first-principles-based numerical models to test the dependence of ionospheric outflow on <span class="hlt">ring</span> current-driven region 2 field-aligned currents (FACs). A moderate magnetospheric storm <span class="hlt">event</span> is modeled with the Space Weather Modeling Framework using a global MHD code (Block Adaptivemore » Tree Solar wind Roe-type Upwind Scheme, BATS-R-US), a polar wind model (Polar Wind Outflow Model), and a bounce-averaged kinetic <span class="hlt">ring</span> current model (<span class="hlt">ring</span> current atmosphere interaction model with self-consistent magnetic field, RAM-SCB). Initially, each code is two-way coupled to all others except for RAM-SCB, which receives inputs from the other models but is not allowed to feed back pressure into the MHD model. The simulation is repeated with pressure coupling activated, which drives strong pressure gradients and region 2 FACs in BATS-R-US. It is found that the region 2 FACs increase heavy ion outflow by up to 6 times over the non-coupled results. The additional outflow further energizes the <span class="hlt">ring</span> current, establishing an ionosphere-magnetosphere mass feedback loop. This study further demonstrates that ionospheric outflow is not merely a plasma source for the magnetosphere but an integral part in the nonlinear ionosphere-magnetosphere-<span class="hlt">ring</span> current system.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18824763','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18824763"><span>Saddle-shaped mitral valve annuloplasty <span class="hlt">rings</span> experience lower forces compared with flat <span class="hlt">rings</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jensen, Morten O; Jensen, Henrik; Smerup, Morten; Levine, Robert A; Yoganathan, Ajit P; Nygaard, Hans; Hasenkam, J Michael; Nielsen, Sten L</p> <p>2008-09-30</p> <p>New insight into the 3D dynamic behavior of the mitral valve has prompted a reevaluation of annuloplasty <span class="hlt">ring</span> designs. Force balance analysis indicates correlation between annulus forces and stresses in leaflets and chords. Improving this stress distribution can intuitively enhance the durability of mitral valve repair. We tested the hypothesis that saddle-shaped annuloplasty <span class="hlt">rings</span> have superior uniform systolic force distribution compared with a nonuniform force distribution in flat annuloplasty <span class="hlt">rings</span>. Sixteen 80-kg pigs had a flat (n=8) or saddle-shaped (n=8) mitral annuloplasty <span class="hlt">ring</span> implanted. Mitral annulus 3D dynamic geometry was obtained with sonomicrometry before <span class="hlt">ring</span> insertion. Strain gauges mounted on dedicated D-shaped rigid flat and saddle-shaped annuloplasty <span class="hlt">rings</span> provided the intraoperative force distribution perpendicular to the annular plane. Average systolic annular height to commissural width ratio before <span class="hlt">ring</span> implantation was 14.0%+/-1.6%. After flat and saddle shaped <span class="hlt">ring</span> implantation, the annulus was fixed in the diastolic (9.0%+/-1.0%) and systolic (14.3%+/-1.3%) configuration, respectively (P<0.01). Force accumulation was seen from the anterior (0.72N+/-0.14N) and commissural annular segments (average 1.38N+/-0.27N) of the flat <span class="hlt">rings</span>. In these segments, the difference between the 2 types of <span class="hlt">rings</span> was statistically significant (P<0.05). The saddle-shaped annuloplasty <span class="hlt">rings</span> did not experience forces statistically significantly larger than zero in any annular segments. Saddle-shaped annuloplasty <span class="hlt">rings</span> provide superior uniform annular force distribution compared to flat <span class="hlt">rings</span> and appear to represent a configuration that minimizes out-of-plane forces that could potentially be transmitted to leaflets and chords. This may have important implications for annuloplasty <span class="hlt">ring</span> selections.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA21356.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA21356.html"><span>So Long, C <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-11-13</p> <p>Saturn's C <span class="hlt">ring</span> is home to a surprisingly rich array of structures and textures. Much of the structure seen in the outer portions of Saturn's <span class="hlt">rings</span> is the result of gravitational perturbations on <span class="hlt">ring</span> particles by moons of Saturn. Such interactions are called resonances. However, scientists are not clear as to the origin of the structures seen in this image which has captured an inner <span class="hlt">ring</span> region sparsely populated with particles, making interactions between <span class="hlt">ring</span> particles rare, and with few satellite resonances. In this image, a bright and narrow ringlet located toward the outer edge of the C <span class="hlt">ring</span> is flanked by two broader features called plateaus, each about 100 miles (160 kilometers) wide. Plateaus are unique to the C <span class="hlt">ring</span>. Cassini data indicates that the plateaus do not necessarily contain more <span class="hlt">ring</span> material than the C <span class="hlt">ring</span> at large, but the <span class="hlt">ring</span> particles in the plateaus may be smaller, enhancing their brightness. This view looks toward the sunlit side of the <span class="hlt">rings</span> from about 53 degrees above the <span class="hlt">ring</span> plane. The image was taken in green light with the Cassini spacecraft narrow-angle camera on Aug. 14, 2017. The view was acquired at a distance of approximately 117,000 miles (189,000 kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 74 degrees. Image scale is 3,000 feet (1 kilometer) per pixel. The Cassini spacecraft ended its mission on Sept. 15, 2017. https://photojournal.jpl.nasa.gov/catalog/PIA21356</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Evolution+AND+test&pg=6&id=EJ1006413','ERIC'); return false;" href="https://eric.ed.gov/?q=Evolution+AND+test&pg=6&id=EJ1006413"><span>The Co-Evolution of Knowledge and <span class="hlt">Event</span> Memory</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>Nelson, Angela B.; Shiffrin, Richard M.</p> <p>2013-01-01</p> <p>We present a theoretical framework and a simplified simulation model for the co-evolution of knowledge and <span class="hlt">event</span> memory, both termed SARKAE (Storing and Retrieving Knowledge and <span class="hlt">Events</span>). Knowledge is formed through the accrual of individual <span class="hlt">events</span>, a process that operates in tandem with the <span class="hlt">storage</span> of individual <span class="hlt">event</span> memories. In 2 studies, new…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSM41C2496C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSM41C2496C"><span>Modeling Earth's <span class="hlt">Ring</span> Current Using The CIMI Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Craven, J. D., II; Perez, J. D.; Buzulukova, N.; Fok, M. C. H.</p> <p>2015-12-01</p> <p>Earth's <span class="hlt">ring</span> current is a result of the injection of charged particles trapped in the magnetosphere from solar storms. The enhancement of the <span class="hlt">ring</span> current particles produces magnetic depressions and disturbances to the Earth's magnetic field known as geomagnetic storms, which have been modeled using the comprehensive inner magnetosphere-ionosphere (CIMI) model. The purpose of this model is to identify and understand the physical processes that control the dynamics of the geomagnetic storms. The basic procedure was to use the CIMI model for the simulation of 15 storms since 2009. Some of the storms were run multiple times, but with varying parameters relating to the dynamics of the Earth's magnetic field, particle fluxes, and boundary conditions of the inner-magnetosphere. Results and images were placed in the TWINS online catalog page for further analysis and discussion. Particular areas of interest were extreme storm <span class="hlt">events</span>. A majority of storms simulated had average DST values of -100 nT; these extreme storms exceeded DST values of -200 nT. The continued use of the CIMI model will increase knowledge of the interactions and processes of the inner-magnetosphere as well as lead to a better understanding of extreme solar storm <span class="hlt">events</span> for the future advancement of space weather physics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29755136','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29755136"><span><span class="hlt">Ring</span> faults and <span class="hlt">ring</span> dikes around the Orientale basin on the Moon.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Andrews-Hanna, Jeffrey C; Head, James W; Johnson, Brandon; Keane, James T; Kiefer, Walter S; McGovern, Patrick J; Neumann, Gregory A; Wieczorek, Mark A; Zuber, Maria T</p> <p>2018-08-01</p> <p>The Orientale basin is the youngest and best-preserved multiring impact basin on the Moon, having experienced only modest modification by subsequent impacts and volcanism. Orientale is often treated as the type example of a multiring basin, with three prominent <span class="hlt">rings</span> outside of the inner depression: the Inner Rook Montes, the Outer Rook Montes, and the Cordillera. Here we use gravity data from NASA's Gravity Recovery and Interior Laboratory (GRAIL) mission to reveal the subsurface structure of Orientale and its <span class="hlt">ring</span> system. Gradients of the gravity data reveal a continuous <span class="hlt">ring</span> dike intruded into the Outer Rook along the plane of the fault associated with the <span class="hlt">ring</span> scarp. The volume of this <span class="hlt">ring</span> dike is ~18 times greater than the volume of all extrusive mare deposits associated with the basin. The gravity gradient signature of the Cordillera <span class="hlt">ring</span> indicates an offset along the fault across a shallow density interface, interpreted to be the base of the low-density ejecta blanket. Both gravity gradients and crustal thickness models indicate that the edge of the central cavity is shifted inward relative to the equivalent Inner Rook <span class="hlt">ring</span> at the surface. Models of the deep basin structure show inflections along the crust-mantle interface at both the Outer Rook and Cordillera <span class="hlt">rings</span>, indicating that the basin <span class="hlt">ring</span> faults extend from the surface to at least the base of the crust. Fault dips range from 13-22° for the Cordillera fault in the northeastern quadrant, to 90° for the Outer Rook in the northwestern quadrant. The fault dips for both outer <span class="hlt">rings</span> are lowest in the northeast, possibly due to the effects of either the direction of projectile motion or regional gradients in pre-impact crustal thickness. Similar <span class="hlt">ring</span> dikes and <span class="hlt">ring</span> faults are observed around the majority of lunar basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4805B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4805B"><span>Magmatic development of the outer Vø<span class="hlt">ring</span> Margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Breivik, Asbjorn; Faleide, Jan Inge; Mjelde, Rolf; Flueh, Ernst; Murai, Yoshio</p> <p>2013-04-01</p> <p>The Vø<span class="hlt">ring</span> Plateau off mid-Norway is a volcanic passive margin, located north of the East Jan Mayen Fracture Zone (EJMFZ). Large volumes of magmatic rocks were emplaced during Early Eocene margin formation. In 2003, an ocean bottom seismometer survey was acquired on the Vø<span class="hlt">ring</span> and Lofoten margins. One profile crosses from the Vø<span class="hlt">ring</span> Plateau to the Vø<span class="hlt">ring</span> Spur, an oceanic plateau north of the EJMFZ. The P-wave data were modeled by ray-tracing in a 2D velocity model of the crust. The process behind the excess magmatism can be estimated by comparing seismic velocity (VP) with igneous thickness (H). This profile and two other profiles farther north show a positive H-VP correlation, consistent with a hot mantle reservoir of finite extent under the margin at breakup. However, during the first two million years, magma production appears to be augmented by a secondary process. By 51-51.5 Ma melting may be caused by elevated mantle temperature alone. Seismic stratigraphy around the Vø<span class="hlt">ring</span> Spur shows at least two inversion <span class="hlt">events</span>, with the main episode tentatively in the Upper Miocene, apparently through igneous growth to create the up to 15 km crustal thickness. The H-VP correlation of the spur is low, indicating constant and moderate-degree mantle melting not tied to the breakup magmatism. The admittance function between bathymetry and free-air gravity shows that the high is near local isostatic equilibrium, discounting that compressional flexure at the EJMFZ shaped the high. We also find no evidence for the proposed Early Eocene triple junction in the area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850026782','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850026782"><span>Solar modulation of cosmic ray intensity and solar flare <span class="hlt">events</span> inferred from (14)C contents in dated tree <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fan, C. Y.; Chen, T. M.; Yun, S. X.; Dai, K. M.</p> <p>1985-01-01</p> <p>The delta 14C values in 42 <span class="hlt">rings</span> of a white spruce grown in Mackenzie Delta was measured as a continuing effort of tracing the history of solar modulation of cosmic ray intensity. The delta 14C values in six <span class="hlt">rings</span> were measured, in search of a 14C increase due to two large solar flares that occurred in 1942. The results are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://medlineplus.gov/ency/article/007318.htm','NIH-MEDLINEPLUS'); return false;" href="https://medlineplus.gov/ency/article/007318.htm"><span>Vascular <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://medlineplus.gov/">MedlinePlus</a></p> <p></p> <p></p> <p>... with aberrant subclavian and left ligamentum ateriosus; Congenital heart defect - vascular <span class="hlt">ring</span>; Birth defect heart - vascular <span class="hlt">ring</span> ... accounts for less than 1% of all congenital heart problems. The condition occurs as often in males ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1960d0018Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1960d0018Q"><span>Stable forming conditions and geometrical expansion of L-shape <span class="hlt">rings</span> in <span class="hlt">ring</span> rolling process</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Quagliato, Luca; Berti, Guido A.; Kim, Dongwook; Kim, Naksoo</p> <p>2018-05-01</p> <p>Based on previous research results concerning the radial-axial <span class="hlt">ring</span> rolling process of flat <span class="hlt">rings</span>, this paper details an innovative approach for the determination of the stable forming conditions to successfully simulate the radial <span class="hlt">ring</span> rolling process of L-shape profiled <span class="hlt">rings</span>. In addition to that, an analytical model for the estimation of the geometrical expansion of L-shape <span class="hlt">rings</span> from its initial flat <span class="hlt">ring</span> preform is proposed and validated by comparing its results with those of numerical simulations. By utilizing the proposed approach, steady forming conditions could be achieved, granting a uniform expansion of the <span class="hlt">ring</span> throughout the process for all of the six tested cases of <span class="hlt">rings</span> having the final outer diameter of the flange ranging from 545mm and 1440mm. The validation of the proposed approach allowed concluding that the geometrical expansion of the <span class="hlt">ring</span>, as estimated by the proposed analytical model, is in good agreement with the results of the numerical simulation, with a maximum error of 2.18%, in the estimation of the <span class="hlt">ring</span> wall diameter, 1.42% of the <span class="hlt">ring</span> flange diameter and 1.87% for the estimation of the inner diameter of the <span class="hlt">ring</span>, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013DPS....4551206M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013DPS....4551206M"><span>Saturn’s <span class="hlt">Ring</span> Rain: Initial Estimates of <span class="hlt">Ring</span> Mass Loss Rates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moore, Luke; O'Donoghue, J.; Mueller-Wodarg, I.; Mendillo, M.</p> <p>2013-10-01</p> <p>We estimate rates of mass loss from Saturn’s <span class="hlt">rings</span> based on ionospheric model reproductions of derived H3+ column densities. On 17 April 2011 over two hours of near-infrared spectral data were obtained of Saturn using the Near InfraRed Spectrograph (NIRSPEC) instrument on the 10-m Keck II telescope. The intensity of two bright H3+ rotational-vibrational emission lines was visible from nearly pole to pole, allowing low-latitude ionospheric emissions to be studied for the first time, and revealing significant latitudinal structure, with local extrema in one hemisphere being mirrored at magnetically conjugate latitudes in the opposite hemisphere. Even more striking, those minima and maxima mapped to latitudes of increased or increased density in Saturn’s <span class="hlt">rings</span>, implying a direct <span class="hlt">ring</span>-atmosphere connection in which charged water group particles from the <span class="hlt">rings</span> are guided by magnetic field lines as they “rain” down upon the atmosphere. Water products act to quench the local ionosphere, and therefore modify the observed H3+ densities. Using the Saturn Thermosphere Ionosphere Model (STIM), a 3-D model of Saturn’s upper atmosphere, we derive the rates of water influx required from the <span class="hlt">rings</span> in order to reproduce the observed H3+ column densities. As a unique pair of conjugate latitudes map to a specific radial distance in the <span class="hlt">ring</span> plane, the derived water influxes can equivalently be described as rates of <span class="hlt">ring</span> mass erosion as a function of radial distance in the <span class="hlt">ring</span> plane, and therefore also allow for an improved estimate of the lifetime of Saturn’s <span class="hlt">rings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23529068','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23529068"><span>Fractional conductance oscillations in quantum <span class="hlt">rings</span>: wave packet picture of transport in a few-electron system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chwiej, T; Szafran, B</p> <p>2013-04-17</p> <p>We study electron transfer across a two-terminal quantum <span class="hlt">ring</span> using a time-dependent description of the scattering process. For the considered scattering <span class="hlt">event</span> the quantum <span class="hlt">ring</span> is initially charged with one or two electrons, with another electron incident to the <span class="hlt">ring</span> from the input channel. We study the electron transfer probability (T) as a function of the external magnetic field. We determine the periodicity of T for a varied number of electrons confined within the <span class="hlt">ring</span>. For that purpose we develop a method to describe the wave packet dynamics for a few electrons participating in the scattering process, taking into full account the electron-electron correlations. We find that electron transfer across the quantum <span class="hlt">ring</span> initially charged by a single electron acquires a distinct periodicity of half of the magnetic flux quantum (Φ0/2), corresponding to the formation of a transient two-electron state inside the <span class="hlt">ring</span>. In the case of a three-electron scattering problem with two electrons initially occupying the <span class="hlt">ring</span>, a period of Φ0/3 for T is formed in the limit of thin channels. The effect of disorder present in the confinement potential of the <span class="hlt">ring</span> is also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA08163&hterms=Trojan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DTrojan','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA08163&hterms=Trojan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DTrojan"><span>The Enceladus <span class="hlt">Ring</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>2006-01-01</p> <p><p/> [figure removed for brevity, see original site] The Enceladus <span class="hlt">Ring</span> (labeled) <p/> This excellent view of the faint E <span class="hlt">ring</span> -- a <span class="hlt">ring</span> feature now known to be created by Enceladus -- also shows two of Saturn's small moons that orbit within the <span class="hlt">ring</span>, among a field of stars in the background. <p/> The E <span class="hlt">ring</span> extends from three to eight Saturn radii -- about 180,000 kilometers (118,000 miles) to 482,000 kilometers (300,000 miles). Its full extent is not visible in this view. <p/> Calypso (22 kilometers, or 14 miles across) and Helene (32 kilometers, or 20 miles across) orbit within the E <span class="hlt">ring</span>'s expanse. Helene skirts the outer parts of the E <span class="hlt">ring</span>, but here it is projected in front of a region deeper within the <span class="hlt">ring</span>. <p/> Calypso and Helene are trojan satellites, or moons that orbit 60 degrees in front or behind a larger moon. Calypso is a Tethys trojan and Helene is a trojan of Dione. <p/> An interesting feature of note in this image is the double-banded appearance of the E-<span class="hlt">ring</span>, which is created because the <span class="hlt">ring</span> is somewhat fainter in the ringplane than it is 500-1,000 kilometers (300-600 miles) above and below the ringplane. This appearance implies that the particles in this part of the <span class="hlt">ring</span> have nonzero inclinations (a similar affect is seen in Jupiter's gossamer <span class="hlt">ring</span>). An object with a nonzero inclination does not orbit exactly at Saturn's ringplane. Instead, its orbit takes it above and below the ringplane. Scientists are not entirely sure why the particles should have such inclinations, but they are fairly certain that the reason involves Enceladus. <p/> One possible explanation is that all the E <span class="hlt">ring</span> particles come from the plume of icy material that is shooting due south out of the moon's pole. This means all of the particles are created with a certain velocity out of the ringplane, and then they orbit above and below that plane. <p/> Another possible explanation is that Enceladus produces particles with a range of speeds, but the moon gravitationally</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009FlDyR..41e1001F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009FlDyR..41e1001F"><span>PREFACE: Special section on vortex <span class="hlt">rings</span> Special section on vortex <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fukumoto, Yasuhide</p> <p>2009-10-01</p> <p>This special section of Fluid Dynamics Research includes five articles on vortex <span class="hlt">rings</span> in both classical and quantum fluids. The leading scientists of the field describe the trends in and the state-of-the-art development of experiments, theories and numerical simulations of vortex <span class="hlt">rings</span>. The year 2008 was the 150th anniversary of 'vortex motion' since Hermann von Helmholtz opened up this field. In 1858, Helmholtz published a paper in Crelle's Journal which put forward the concept of 'vorticity' and made the first analysis of vortex motion. Fluid mechanics before that was limited to irrotational motion. In the absence of vorticity, the motion of an incompressible homogeneous fluid is virtually equivalent to a rigid-body motion in the sense that the fluid motion is determined once the boundary configuration is specified. Helmholtz proved, among other things, that, without viscosity, a vortex line is frozen into the fluid. This Helmholtz's law immediately implies the preservation of knots and links of vortex lines and its implication is enormous. One of the major trends of fluid mechanics since the latter half of the 20th century is to clarify the topological meaning of Helmholtz's law and to exploit it to develop theoretical and numerical methods to find the solutions of the Euler equations and to develop experimental techniques to gain an insight into fluid motion. Vortex <span class="hlt">rings</span> are prominent coherent structures in a variety of fluid motions from the microscopic scale, through human and mesoscale to astrophysical scales, and have attracted people's interest. The late professor Philip G Saffman (1981) emphasized the significance of studies on vortex <span class="hlt">rings</span>. One particular motion exemplifies the whole range of problems of vortex motion and is also a commonly known phenomenon, namely the vortex <span class="hlt">ring</span> or smoke <span class="hlt">ring</span>. Vortex <span class="hlt">rings</span> are easily produced by dropping drops of one liquid into another, or by puffing fluid out of a hole, or by exhaling smoke if one has the skill</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DPS....4910408M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DPS....4910408M"><span>Surface roughness of Saturn's <span class="hlt">rings</span> and <span class="hlt">ring</span> particles inferred from thermal phase curves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morishima, Ryuji; Turner, Neal J.; Spilker, Linda</p> <p>2017-10-01</p> <p>We analyze thermal phase curves of all the main <span class="hlt">rings</span> of Saturn (the A, B, C <span class="hlt">rings</span>, and the Cassini division) measured by both the far-IR and mid-IR detectors of the Cassini Composite InfraRed Spectrometer (CIRS). All the <span class="hlt">rings</span> show temperature increases toward zero phase angle, known as an opposition effect or thermal beaming. For the C <span class="hlt">ring</span> and Cassini division, which have low optical depths, intra-particle shadowing is considered the dominant mechanism causing the effect. On the other hand, the phase curves of the optically thick B and A <span class="hlt">rings</span> steepen significantly with decreasing absolute solar elevation angle from 21° to 14°, suggesting inter-particle shadowing plays an important role in these <span class="hlt">rings</span>. We employ an analytic roughness model to estimate the degrees of surface roughness of the <span class="hlt">rings</span> or <span class="hlt">ring</span> particles. For optically thin <span class="hlt">rings</span>, an isolated particle covered by spherical segment craters is employed while for the thick <span class="hlt">rings</span> we approximate a packed particle layer as a slab covered by craters. The particles in the thin <span class="hlt">rings</span> are found to have generally rough surfaces, except in the middle C <span class="hlt">ring</span>. Across the C <span class="hlt">ring</span>, the optical depth correlates with the degree of surface roughness. This may indicate that surface roughness comes mainly from particle clumping, while individual particles have rather smooth surfaces. For the optically thick <span class="hlt">rings</span>, the surface roughness of the particle layer is found to be moderate. The modeled phase curves of optically thick <span class="hlt">rings</span> are shallow if the phase angle change is primarily due to change of observer azimuthal angle. On the other hand, the phase curves are steep if the phase angle change is due to change of observer elevation angle, as inter-particle shadows become visible at higher observer elevation. In addition, the area of shadowed facets increases with decreasing solar elevation angle. These combined effects explain the large seasonal change of the phase curve steepness observed for the thick <span class="hlt">rings</span>. The degrees</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Icar..295...74M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..295...74M"><span>Surface roughness of Saturn's <span class="hlt">rings</span> and <span class="hlt">ring</span> particles inferred from thermal phase curves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morishima, Ryuji; Turner, Neal; Spilker, Linda</p> <p>2017-10-01</p> <p>We analyze thermal phase curves of all the main <span class="hlt">rings</span> of Saturn (the A, B, C <span class="hlt">rings</span>, and the Cassini division) measured by both the far-IR and mid-IR detectors of the Cassini Composite InfraRed Spectrometer (CIRS). All the <span class="hlt">rings</span> show temperature increases toward zero phase angle, known as an opposition effect or thermal beaming. For the C <span class="hlt">ring</span> and Cassini division, which have low optical depths, intra-particle shadowing is considered the dominant mechanism causing the effect. On the other hand, the phase curves of the optically thick B and A <span class="hlt">rings</span> steepen significantly with decreasing absolute solar elevation angle from 21° to 14°, suggesting inter-particle shadowing plays an important role in these <span class="hlt">rings</span>. We employ an analytic roughness model to estimate the degrees of surface roughness of the <span class="hlt">rings</span> or <span class="hlt">ring</span> particles. For optically thin <span class="hlt">rings</span>, an isolated particle covered by spherical segment craters is employed while for the thick <span class="hlt">rings</span> we approximate a packed particle layer as a slab covered by craters. The particles in the thin <span class="hlt">rings</span> are found to have generally rough surfaces, except in the middle C <span class="hlt">ring</span>. Across the C <span class="hlt">ring</span>, the optical depth correlates with the degree of surface roughness. This may indicate that surface roughness comes mainly from particle clumping, while individual particles have rather smooth surfaces. For the optically thick <span class="hlt">rings</span>, the surface roughness of the particle layer is found to be moderate. The modeled phase curves of optically thick <span class="hlt">rings</span> are shallow if the phase angle change is primarily due to change of observer azimuthal angle. On the other hand, the phase curves are steep if the phase angle change is due to change of observer elevation angle, as inter-particle shadows become visible at higher observer elevation. In addition, the area of shadowed facets increases with decreasing solar elevation angle. These combined effects explain the large seasonal change of the phase curve steepness observed for the thick <span class="hlt">rings</span>. The degrees</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1201669-integrating-co-storage-geothermal-resources-dispatchable-renewable-electricity','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1201669-integrating-co-storage-geothermal-resources-dispatchable-renewable-electricity"><span>Integrating CO₂ <span class="hlt">storage</span> with geothermal resources for dispatchable renewable electricity</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Buscheck, Thomas A.; Bielicki, Jeffrey M.; Chen, Mingjie; ...</p> <p>2014-12-31</p> <p>We present an approach that uses the huge fluid and thermal <span class="hlt">storage</span> capacity of the subsurface, together with geologic CO₂ <span class="hlt">storage</span>, to harvest, store, and dispatch energy from subsurface (geothermal) and surface (solar, nuclear, fossil) thermal resources, as well as energy from electrical grids. Captured CO₂ is injected into saline aquifers to store pressure, generate artesian flow of brine, and provide an additional working fluid for efficient heat extraction and power conversion. Concentric <span class="hlt">rings</span> of injection and production wells are used to create a hydraulic divide to store pressure, CO₂, and thermal energy. Such <span class="hlt">storage</span> can take excess power frommore » the grid and excess/waste thermal energy, and dispatch that energy when it is demanded, enabling increased penetration of variable renewables. Stored CO₂ functions as a cushion gas to provide enormous pressure-<span class="hlt">storage</span> capacity and displaces large quantities of brine, which can be desalinated and/or treated for a variety of beneficial uses.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA17150.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA17150.html"><span>Dusty D <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2014-02-24</p> <p>Saturn D <span class="hlt">ring</span> is easy to overlook since it trapped between the brighter C <span class="hlt">ring</span> and the planet itself. In this view from NASA Cassini spacecraft, all that can be seen of the D <span class="hlt">ring</span> is the faint and narrow arc as it stretches from top right of the ima</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA08361.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA08361.html"><span><span class="hlt">Ring</span> World</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2007-03-01</p> <p>Our robotic emissary, flying high above Saturn, captured this view of an alien copper-colored <span class="hlt">ring</span> world. The overexposed planet has deliberately been removed to show the unlit <span class="hlt">rings</span> alone, seen from an elevation of 60 degrees</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NIMPA.881...27W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NIMPA.881...27W"><span>The design of the Spectrometer <span class="hlt">Ring</span> at the HIAF</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, B.; Yang, J. C.; Xia, J. W.; Yan, X. L.; Hu, X. J.; Mao, L. J.; Sheng, L. N.; Wu, J. X.; Yin, D. Y.; Chai, W. P.; Shen, G. D.; Ge, W. W.; Wang, G.; Zhao, H.; Ruan, S.; Ma, X. W.; Wang, M.; Litvinov, S.; Wen, W. Q.; Chen, X. C.; Chen, R. J.; Tang, M. T.; Wu, W.; Luo, C.; Zhao, T. C.; Shi, C. F.; Fu, X.; Liu, J.; Liang, L.</p> <p>2018-02-01</p> <p>The Spectrometer <span class="hlt">Ring</span> (SRing) is an essential part of the High Intensity heavy-ion Accelerator Facility project (HIAF) in China. It is designed as a multi-functional experimental <span class="hlt">storage</span> <span class="hlt">ring</span>, which will be able to operate in three ion optical operation modes. The SRing will be used as a time-of-flight mass spectrometer for short-lived, especially neutron-rich nuclei. It will also be used to collect and cool Rare Isotope Beams (RIBs) or highly-charged stable ion beams for nuclear and atomic physics experiments. The design magnetic rigidity is in the range 1.5 to 15 Tm. The beam cooling system consists of stochastic cooling and electron cooling devices. With a help of an electron cooler, stored ions will be decelerated to a minimum energy of 30 MeV/u by RF cavities. The extraction system of the SRing will allow cooled ion beams to be extracted to an external target for further ion manipulations or reaction experiments. The general ion optics design and technical requirements of SRing subsystems are presented and discussed in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25247299','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25247299"><span>Dissecting the space-time structure of tree-<span class="hlt">ring</span> datasets using the partial triadic analysis.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rossi, Jean-Pierre; Nardin, Maxime; Godefroid, Martin; Ruiz-Diaz, Manuela; Sergent, Anne-Sophie; Martinez-Meier, Alejandro; Pâques, Luc; Rozenberg, Philippe</p> <p>2014-01-01</p> <p>Tree-<span class="hlt">ring</span> datasets are used in a variety of circumstances, including archeology, climatology, forest ecology, and wood technology. These data are based on microdensity profiles and consist of a set of tree-<span class="hlt">ring</span> descriptors, such as <span class="hlt">ring</span> width or early/latewood density, measured for a set of individual trees. Because successive <span class="hlt">rings</span> correspond to successive years, the resulting dataset is a <span class="hlt">ring</span> variables × trees × time datacube. Multivariate statistical analyses, such as principal component analysis, have been widely used for extracting worthwhile information from <span class="hlt">ring</span> datasets, but they typically address two-way matrices, such as <span class="hlt">ring</span> variables × trees or <span class="hlt">ring</span> variables × time. Here, we explore the potential of the partial triadic analysis (PTA), a multivariate method dedicated to the analysis of three-way datasets, to apprehend the space-time structure of tree-<span class="hlt">ring</span> datasets. We analyzed a set of 11 tree-<span class="hlt">ring</span> descriptors measured in 149 georeferenced individuals of European larch (Larix decidua Miller) during the period of 1967-2007. The processing of densitometry profiles led to a set of <span class="hlt">ring</span> descriptors for each tree and for each year from 1967-2007. The resulting three-way data table was subjected to two distinct analyses in order to explore i) the temporal evolution of spatial structures and ii) the spatial structure of temporal dynamics. We report the presence of a spatial structure common to the different years, highlighting the inter-individual variability of the <span class="hlt">ring</span> descriptors at the stand scale. We found a temporal trajectory common to the trees that could be separated into a high and low frequency signal, corresponding to inter-annual variations possibly related to defoliation <span class="hlt">events</span> and a long-term trend possibly related to climate change. We conclude that PTA is a powerful tool to unravel and hierarchize the different sources of variation within tree-<span class="hlt">ring</span> datasets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006epsc.conf..196E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006epsc.conf..196E"><span>Planetary <span class="hlt">rings</span>: Structure and history</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esposito, L.</p> <p></p> <p>The composition and structure of planetary <span class="hlt">rings</span> provide the key evidence to understand their origin and evolution. Before the first space observations, we were able to maintain an idealized view of the <span class="hlt">rings</span> around Saturn, the only known <span class="hlt">ring</span> system at that time. <span class="hlt">Rings</span> were then discovered around Jupiter, Uranus and Neptune. Saturn's F <span class="hlt">ring</span> was discovered by Pioneer 11. Our ideal view of circular, planar, symmetric and unchanging <span class="hlt">rings</span> was shattered by observations of inclined, eccentric <span class="hlt">rings</span>, waves and wavy edges, and numerous processes acting at rates that give timescales much younger than the solar system. Moons within and near the <span class="hlt">rings</span> sculpt them and are the likely progenitors of future <span class="hlt">rings</span>. The moonlet lifetimes are much less than Saturn's age. The old idea of ancient <span class="hlt">rings</span> gave rise to youthful <span class="hlt">rings</span>, that are recently created by erosion and destruction of small nearby moons. Although this explanation may work well for most <span class="hlt">rings</span>, Saturn's massive <span class="hlt">ring</span> system provides a problem. It is extremely improbable that Saturn's <span class="hlt">rings</span> were recently created by the destruction of a moon as large as Mimas, or even by the breakup of a large comet that passed too close to Saturn. The history of Saturn's <span class="hlt">rings</span> has been a difficult problem, now made even more challenging by the close-up Cassini measurements. Cassini observations show unexpected <span class="hlt">ring</span> variability in time and space. Time variations are seen in <span class="hlt">ring</span> edges, in the thinner D and F <span class="hlt">rings</span>, and in the neutral oxygen cloud, which outweighs the E <span class="hlt">ring</span> in the same region around Saturn. The <span class="hlt">rings</span> are inhomogeneous, with structures on all scales, sharp gradients and edges. Compositional gradients are sharper than expected, but nonetheless cross structural boundaries. This is evidence for ballistic transport that has not gone to completion. The autocovariance maximizes in the middle of the A <span class="hlt">ring</span>, with smaller structure near the main <span class="hlt">rings</span>' outer edge. Density wave locations have a fresher ice composition. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvS..20h2802M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvS..20h2802M"><span>Improving the precision of linear optics measurements based on turn-by-turn beam position monitor data after a pulsed excitation in lepton <span class="hlt">storage</span> <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malina, L.; Coello de Portugal, J.; Persson, T.; Skowroński, P. K.; Tomás, R.; Franchi, A.; Liuzzo, S.</p> <p>2017-08-01</p> <p>Beam optics control is of critical importance for machine performance and protection. Nowadays, turn-by-turn (TbT) beam position monitor (BPM) data are increasingly exploited as they allow for fast and simultaneous measurement of various optics quantities. Nevertheless, so far the best documented uncertainty of measured β -functions is of about 10‰ rms. In this paper we compare the β -functions of the ESRF <span class="hlt">storage</span> <span class="hlt">ring</span> measured from two different TbT techniques—the N-BPM and the Amplitude methods—with the ones inferred from a measurement of the orbit response matrix (ORM). We show how to improve the precision of TbT techniques by refining the Fourier transform of TbT data with properly chosen excitation amplitude. The precision of the N-BPM method is further improved by refining the phase advance measurement. This represents a step forward compared to standard TbT measurements. First experimental results showing the precision of β -functions pushed down to 4‰ both in TbT and ORM techniques are reported and commented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA18278.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA18278.html"><span><span class="hlt">Ring</span> King</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2014-08-18</p> <p>Saturn reigns supreme, encircled by its retinue of <span class="hlt">rings</span>. Although all four giant planets have <span class="hlt">ring</span> systems, Saturn's is by far the most massive and impressive. Scientists are trying to understand why by studying how the <span class="hlt">rings</span> have formed and how they have evolved over time. Also seen in this image is Saturn's famous north polar vortex and hexagon. This view looks toward the sunlit side of the <span class="hlt">rings</span> from about 37 degrees above the ringplane. The image was taken with the Cassini spacecraft wide-angle camera on May 4, 2014 using a spectral filter which preferentially admits wavelengths of near-infrared light centered at 752 nanometers. The view was acquired at a distance of approximately 2 million miles (3 million kilometers) from Saturn. Image scale is 110 miles (180 kilometers) per pixel. http://photojournal.jpl.nasa.gov/catalog/PIA18278</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16836364','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16836364"><span>A Pauson-Khand and <span class="hlt">ring</span>-expansion approach to the aquariane <span class="hlt">ring</span> system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thornton, Paul D; Burnell, D Jean</p> <p>2006-07-20</p> <p>[Structure: see text] The carbocyclic <span class="hlt">ring</span> system of the aquariolide diterpenes has been synthesized by two routes involving a diastereoselective Pauson-Khand reaction and subsequent <span class="hlt">ring</span> expansion. In one route, a tetracyclic enone was elaborated to generate the nine-membered <span class="hlt">ring</span> by Grob fragmentation. In the second approach, a spirocyclic tricycle underwent a facile anionic oxy-Cope rearrangement to complete the synthesis of the desired <span class="hlt">ring</span> system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23999137','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23999137"><span>Stem water <span class="hlt">storage</span> in five coexisting temperate broad-leaved tree species: significance, temporal dynamics and dependence on tree functional traits.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Köcher, Paul; Horna, Viviana; Leuschner, Christoph</p> <p>2013-08-01</p> <p>The functional role of internal water <span class="hlt">storage</span> is increasingly well understood in tropical trees and conifers, while temperate broad-leaved trees have only rarely been studied. We examined the magnitude and dynamics of the use of stem water reserves for transpiration in five coexisting temperate broad-leaved trees with largely different morphology and physiology (genera Fagus, Fraxinus, Tilia, Carpinus and Acer). We expected that differences in water <span class="hlt">storage</span> patterns would mostly reflect species differences in wood anatomy (<span class="hlt">ring</span> vs. diffuse-porous) and wood density. Sap flux density was recorded synchronously at five positions along the root-to-branch flow path of mature trees (roots, three stem positions and branches) with high temporal resolution (2 min) and related to stem radius changes recorded with electronic point dendrometers. The daily amount of stored stem water withdrawn for transpiration was estimated by comparing the integrated flow at stem base and stem top. The temporal coincidence of flows at different positions and apparent time lags were examined by cross-correlation analysis. Our results confirm that internal water stores play an important role in the four diffuse-porous species with estimated 5-12 kg day(-1) being withdrawn on average in 25-28 m tall trees representing 10-22% of daily transpiration; in contrast, only 0.5-2.0 kg day(-1) was withdrawn in <span class="hlt">ring</span>-porous Fraxinus. Wood density had a large influence on <span class="hlt">storage</span>; sapwood area (diffuse- vs. <span class="hlt">ring</span>-porous) may be another influential factor but its effect was not significant. Across the five species, the length of the time lag in flow at stem top and stem base was positively related to the size of stem <span class="hlt">storage</span>. The stem stores were mostly exhausted when the soil matrix potential dropped below -0.1 MPa and daily mean vapor pressure deficit exceeded 3-5 hPa. We conclude that stem <span class="hlt">storage</span> is an important factor improving the water balance of diffuse-porous temperate broad-leaved trees in moist</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6327Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6327Y"><span>Study of Basin Recession Characteristics and Groundwater <span class="hlt">Storage</span> Properties</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yen-Bo, Chen; Cheng-Haw, Lee</p> <p>2017-04-01</p> <p>Stream flow and groundwater <span class="hlt">storage</span> are freshwater resources that human live on.In this study, we discuss southern area basin recession characteristics and Kao-Ping River basin groundwater <span class="hlt">storage</span>, and hope to supply reference to Taiwan water resource management. The first part of this study is about recession characteristics. We apply Brutsaert (2008) low flow analysis model to establish two recession data pieces sifting models, including low flow steady period model and normal condition model. Within individual <span class="hlt">event</span> analysis, group <span class="hlt">event</span> analysis and southern area basin recession assessment, stream flow and base flow recession characteristics are parameterized. The second part of this study is about groundwater <span class="hlt">storage</span>. Among main basin in southern Taiwan, there are sufficient stream flow and precipitation gaging station data about Kao-Ping River basin and extensive drainage data, and data about different hydrological characteristics between upstream and downstream area. Therefore, this study focuses on Kao-Ping River basin and accesses groundwater <span class="hlt">storage</span> properties. Taking residue of groundwater volume in dry season into consideration, we use base flow hydrograph to access periodical property of groundwater <span class="hlt">storage</span>, in order to establish hydrological period conceptual model. With groundwater <span class="hlt">storage</span> and precipitation accumulative linearity quantified by hydrological period conceptual model, their periodical changing and alternation trend properties in each drainage areas of Kao-Ping River basin have been estimated. Results of this study showed that the recession time of stream flow is related to initial flow rate of the recession <span class="hlt">events</span>. The recession time index is lower when the flow is stream flow, not base flow, and the recession time index is higher in low flow steady flow period than in normal recession condition. By applying hydrological period conceptual model, groundwater <span class="hlt">storage</span> could explicitly be analyzed and compared with precipitation, by only</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CPL...692..253S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CPL...692..253S"><span>Paracyclophane functionalized with Sc and Li for hydrogen <span class="hlt">storage</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sathe, Rohit Y.; Dhilip Kumar, T. J.</p> <p>2018-01-01</p> <p>Li and Sc metals functionalized on the delocalized π -electrons of benzene <span class="hlt">rings</span> in [2,2]paracyclophane structure are studied for hydrogen <span class="hlt">storage</span> efficiency by using the M06 DFT functional with 6-311G(d,p) basis set. It is found that Sc and Li functionalized [2,2]paracyclophane complexes can hold up to 10 H2 molecules and 8 H2 molecules by Kubas-Niu-Jena interaction and charge polarization mechanism with hydrogen weight percentage of 11.4 and 13.5, respectively. Molecular dynamics simulation at various temperatures showed appreciable thermal stability while the chemical potential calculation at room temperature reveals that Sc functionalized [2,2]paracyclophane system will be a promising hydrogen <span class="hlt">storage</span> material.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910000060&hterms=Pretest&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DPretest','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910000060&hterms=Pretest&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DPretest"><span>O-<span class="hlt">Ring</span>-Testing Fixture</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Turner, James E.; Mccluney, D. Scott</p> <p>1991-01-01</p> <p>Fixture tests O-<span class="hlt">rings</span> for sealing ability under dynamic conditions after extended periods of compression. Hydraulic cylinder moves plug in housing. Taper of 15 degrees on plug and cavity of housing ensures that gap created between O-<span class="hlt">ring</span> under test and wall of cavity. Secondary O-<span class="hlt">rings</span> above and below test <span class="hlt">ring</span> maintain pressure applied to test <span class="hlt">ring</span>. Evaluates effects of variety of parameters, including temperature, pressure, rate of pressurization, rate and magnitude of radial gap movement, and pretest compression time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA10629&hterms=race+cars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Drace%2Bcars','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA10629&hterms=race+cars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Drace%2Bcars"><span>Nardo <span class="hlt">Ring</span>, Italy</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2008-01-01</p> <p><p/> The Nardo <span class="hlt">Ring</span> is a striking visual feature from space, and astronauts have photographed it several times. The <span class="hlt">Ring</span> is a race car test track; it is 12.5 kilometers long and steeply banked to reduce the amount of active steering needed by drivers. The Nardo <span class="hlt">Ring</span> lies in a remote area on the heel of Italy's 'boot,' 50 kilometers east of the naval port of Taranto. The <span class="hlt">Ring</span> encompasses a number of active (green) and fallow (brown to dark brown) agricultural fields. In this zone of intensive agriculture, farmers gain access to their fields through the <span class="hlt">Ring</span> via a series of underpasses. Winding features within the southern section of the <span class="hlt">Ring</span> appear to be smaller, unused race tracks. <p/> The image covers an area of 18.8 x 16.4 km, was acquired on August 17. 2007, and is located at 49.3 degrees north latitude, 17.8 degrees east longitude. <p/> The U.S. science team is located at NASA's Jet Propulsion Laboratory, Pasadena, Calif. The Terra mission is part of NASA's Science Mission Directorate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010GPC....72..182B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010GPC....72..182B"><span>Five centuries of Central European temperature extremes reconstructed from tree-<span class="hlt">ring</span> density and documentary evidence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Battipaglia, Giovanna; Frank, David; Büntgen, Ulf; Dobrovolný, Petr; Brázdil, Rudolf; Pfister, Christian; Esper, Jan</p> <p>2010-06-01</p> <p>Future climate change will likely influence the frequency and intensity of weather extremes. As such <span class="hlt">events</span> are by definition rare, long records are required to understand their characteristics, drivers, and consequences on ecology and society. Herein we provide a unique perspective on regional-scale temperature extremes over the past millennium, using three tree-<span class="hlt">ring</span> maximum latewood density (MXD) chronologies from higher elevations in the European Alps. We verify the tree-<span class="hlt">ring</span>-based extremes using documentary evidences from Switzerland, the Czech Republic, and Central Europe that allowed the identification of 44 summer extremes over the 1550-2003 period. These <span class="hlt">events</span> include cold temperatures in 1579, 1628, 1675, and 1816, as well as warm ones in 1811 and 2003. Prior to 1550, we provide new evidence for cold (e.g., 1068 and 1258) and warm (e.g., 1333) summers derived from the combined MXD records and thus help to characterize high-frequency temperature variability during medieval times. Spatial coherence of the reconstructed extremes is found over Switzerland, with most signatures even extending across Central Europe. We discuss potential limitations of the tree-<span class="hlt">ring</span> and documentary archives, including the ( i) ability of MXD to particularly capture extremely warm temperatures, ( ii) methodological identification and relative definition of extremes, and ( iii) placement of those <span class="hlt">events</span> in the millennium-long context of low-frequency climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26601373','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26601373"><span>[Laser Induced Fluorescence Spectroscopic Analysis of Aromatics from One <span class="hlt">Ring</span> to Four <span class="hlt">Rings</span>].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Peng; Liu, Hai-feng; Yue, Zong-yu; Chen, Bei-ling; Yao, Ming-fa</p> <p>2015-06-01</p> <p>In order to distinguish small aromatics preferably, a Nd : YAG Laser was used to supply an excitation laser, which was adjusted to 0.085 J x cm(-2) at 266 nm. Benzene, toluene, naphthalene, phenanthrene, anthracene, pyrene and chrysene were used as the representative of different <span class="hlt">rings</span> aromatics. The fluorescence emission spectra were researched for each aromatic hydrocarbon and mixtures by Laser induced fluorescence (LIF). Results showed that the <span class="hlt">rings</span> number determined the fluorescence emission spectra, and the structure with same <span class="hlt">rings</span> number did not affect the emission fluorescence spectrum ranges. This was due to the fact that the absorption efficiency difference at 266 nm resulted in that the fluorescence intensities of each aromatic hydrocarbon with same <span class="hlt">rings</span> number were different and the fluorescence intensities difference were more apparently with aromatic <span class="hlt">ring</span> number increasing. When the absorption efficiency was similar at 266 nm and the concentrations of each aromatic hydrocarbon were same, the fluorescence intensities were increased with aromatic <span class="hlt">ring</span> number increasing. With aromatic <span class="hlt">ring</span> number increasing, the fluorescence spectrum and emission peak wavelength were all red-shifted from ultraviolet to visible and the fluorescence spectrum range was also wider as the absorption efficiency was similar. The fluorescence emission spectra from one to four <span class="hlt">rings</span> could be discriminated in the following wavelengths, 275 to 320 nm, 320 to 375 nm, 375 to 425 nm, 425 to 556 nm, respectively. It can be used for distinguish the type of the polycyclic aromatic hydrocarbons (PAHs) as it exists in single type. As PAHs are usually exist in a variety of different <span class="hlt">rings</span> number at the same time, the results for each aromatic hydrocarbon may not apply to the aromatic hydrocarbon mixtures. For the aromatic hydrocarbon mixtures, results showed that the one- or two-<span class="hlt">ring</span> PAHs in mixtures could not be detected by fluorescence as three- or four-<span class="hlt">ring</span> PAHs existed in mixture</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880039814&hterms=importance+force&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dimportance%2Bforce','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880039814&hterms=importance+force&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dimportance%2Bforce"><span>Electrostatic forces in planetary <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Goertz, C. K.; Shan, Linhua; Havnes, O.</p> <p>1988-01-01</p> <p>The average charge on a particle in a particle-plasma cloud, the plasma potential inside the cloud, and the Coulomb force acting on the particle are calculated. The net repulsive electrostatic force on a particle depends on the plasma density, temperature, density of particles, particle size, and the gradient of the particle density. In a uniformly dense <span class="hlt">ring</span> the electrostatic repulsion is zero. It is also shown that the electrostatic force acts like a pressure force, that even a collisionless <span class="hlt">ring</span> can be stable against gravitational collapse, and that a finite <span class="hlt">ring</span> thickness does not necessarily imply a finite velocity dispersion. A simple criterion for the importance of electrostatic forces in planetary <span class="hlt">rings</span> is derived which involves the calculation of the vertical <span class="hlt">ring</span> thickness which would result if only electrostatic repulsion were responsible for the finite <span class="hlt">ring</span> thickness. Electrostatic forces are entirely negligible in the main <span class="hlt">rings</span> of Saturn and the E and G <span class="hlt">rings</span>. They may also be negligible in the F <span class="hlt">ring</span>. However, the Uranian <span class="hlt">rings</span> and Jupiter's <span class="hlt">ring</span> seem to be very much influenced by electrostatic repulsion. In fact, electrostatic forces could support a Jovian <span class="hlt">ring</span> which is an order of magnitude more dense than observed.</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.osti.gov/servlets/purl/864815','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/864815"><span>Stirling engine piston <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Howarth, Roy B.</p> <p>1983-01-01</p> <p>A piston <span class="hlt">ring</span> design for a Stirling engine wherein the contact pressure between the piston and the cylinder is maintained at a uniform level, independent of engine conditions through a balancing of the pressure exerted upon the <span class="hlt">ring</span>'s surface and thereby allowing the contact pressure on the <span class="hlt">ring</span> to be predetermined through the use of a preloaded expander <span class="hlt">ring</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23053367','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23053367"><span>How does the blue-<span class="hlt">ringed</span> octopus (Hapalochlaena lunulata) flash its blue <span class="hlt">rings</span>?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mäthger, Lydia M; Bell, George R R; Kuzirian, Alan M; Allen, Justine J; Hanlon, Roger T</p> <p>2012-11-01</p> <p>The blue-<span class="hlt">ringed</span> octopus (Hapalochlaena lunulata), one of the world's most venomous animals, has long captivated and endangered a large audience: children playing at the beach, divers turning over rocks, and biologists researching neurotoxins. These small animals spend much of their time in hiding, showing effective camouflage patterns. When disturbed, the octopus will flash around 60 iridescent blue <span class="hlt">rings</span> and, when strongly harassed, bite and deliver a neurotoxin that can kill a human. Here, we describe the flashing mechanism and optical properties of these <span class="hlt">rings</span>. The <span class="hlt">rings</span> contain physiologically inert multilayer reflectors, arranged to reflect blue-green light in a broad viewing direction. Dark pigmented chromatophores are found beneath and around each <span class="hlt">ring</span> to enhance contrast. No chromatophores are above the <span class="hlt">ring</span>; this is unusual for cephalopods, which typically use chromatophores to cover or spectrally modify iridescence. The fast flashes are achieved using muscles under direct neural control. The <span class="hlt">ring</span> is hidden by contraction of muscles above the iridophores; relaxation of these muscles and contraction of muscles outside the <span class="hlt">ring</span> expose the iridescence. This mechanism of producing iridescent signals has not previously been reported in cephalopods and we suggest that it is an exceptionally effective way to create a fast and conspicuous warning display.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4906004','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4906004"><span>Flood-<span class="hlt">Ring</span> Formation and Root Development in Response to Experimental Flooding of Young Quercus robur Trees</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Copini, Paul; den Ouden, Jan; Robert, Elisabeth M. R.; Tardif, Jacques C.; Loesberg, Walter A.; Goudzwaard, Leo; Sass-Klaassen, Ute</p> <p>2016-01-01</p> <p>Spring flooding in riparian forests can cause significant reductions in earlywood-vessel size in submerged stem parts of <span class="hlt">ring</span>-porous tree species, leading to the presence of ‘flood rings’ that can be used as a proxy to reconstruct past flooding <span class="hlt">events</span>, potentially over millennia. The mechanism of flood-<span class="hlt">ring</span> formation and the relation with timing and duration of flooding are still to be elucidated. In this study, we experimentally flooded 4-year-old Quercus robur trees at three spring phenophases (late bud dormancy, budswell, and internode expansion) and over different flooding durations (2, 4, and 6 weeks) to a stem height of 50 cm. The effect of flooding on root and vessel development was assessed immediately after the flooding treatment and at the end of the growing season. <span class="hlt">Ring</span> width and earlywood-vessel size and density were measured at 25- and 75-cm stem height and collapsed vessels were recorded. Stem flooding inhibited earlywood-vessel development in flooded stem parts. In addition, flooding upon budswell and internode expansion led to collapsed earlywood vessels below the water level. At the end of the growing season, mean earlywood-vessel size in the flooded stem parts (upon budswell and internode expansion) was always reduced by approximately 50% compared to non-flooded stem parts and 55% compared to control trees. This reduction was already present 2 weeks after flooding and occurred independent of flooding duration. Stem and root flooding were associated with significant root dieback after 4 and 6 weeks and mean radial growth was always reduced with increasing flooding duration. By comparing stem and root flooding, we conclude that flood <span class="hlt">rings</span> only occur after stem flooding. As earlywood-vessel development was hampered during flooding, a considerable number of narrow earlywood vessels present later in the season, must have been formed after the actual flooding <span class="hlt">events</span>. Our study indicates that root dieback, together with strongly reduced hydraulic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP31A1268T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP31A1268T"><span>Assessment of Methods to Determine Tree <span class="hlt">Ring</span> Response to Large Magnitude Mississippi River Floods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Therrell, M. D.; Meko, M. D.; Bialecki, M.; Remo, J. W.</p> <p>2017-12-01</p> <p>Riparian trees that experience prolonged inundation can record major flood <span class="hlt">events</span> as inter-and intra-annual variability in size, shape and arrangement of vessels in the annual xylem growth increment. As part of an NSF-funded project to develop tree-<span class="hlt">ring</span> records of past flooding, we have made collections of several oak species (e.g., Quercus lyrata, Q. macrocarpa) at six sites in the Mississippi River Basin. At each of these sites sampled trees exhibit notably anomalous anatomy of growth increments formed in years coinciding with major recorded floods. We have used these "flood <span class="hlt">rings</span>" to develop individual site chronologies as well as a regional chronology of spring flood <span class="hlt">events</span> in the basin for the past several hundred years. We have also analyzed earlywood vessel diameter as a proxy for flooding and find that although this variable reflects only a fraction of the annual-growth increment it strongly reflects tree response to flooding at all the sites so far examined. We compare both these chronologies with the instrumental and historical record of flooding and find that our chronologies are recording nearly all large observed Mississippi River floods in the 20th century, and provide a new record of similar <span class="hlt">events</span> in the 18th and 19th centuries. These results suggest that tree-<span class="hlt">rings</span> can be effectively used to develop and improve pre-instrumental flood records throughout the basin and potentially other similar systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000Icar..145..147P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000Icar..145..147P"><span>The Crossings of Saturn <span class="hlt">Ring</span> Plane by the Earth in 1995: <span class="hlt">Ring</span> Thickness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poulet, François; Sicardy, Bruno; Dumas, Christophe; Jorda, Laurent; Tiphène, Didier</p> <p>2000-05-01</p> <p>The crossings of Saturn's <span class="hlt">ring</span> plane by Earth were observed in the near infrared on May 22 and August 10, 1995, from the 2.2-m telescope of the University of Hawaii, the 2-m telescope at Pic du Midi, France, and with the Adonis adaptive optics camera at the 3.6-m telescope of the European Southern Observatory in Chile. Images from the Hubble Space Telescope, obtained in August 1995, are also reanalyzed. The radial brightness profiles of the <span class="hlt">rings</span> indicate that the outer and usually faint F <span class="hlt">ring</span> dominates the edge-on brightness of the system, thus hiding the vertical structure of the main <span class="hlt">rings</span> within a few hours around the <span class="hlt">ring</span> plane crossing. The photometric behaviors of the A, B, and C <span class="hlt">rings</span> and of the Cassini Division are analyzed, using a radiative transfer code which includes the illuminations by the Sun and by the planet. The F <span class="hlt">ring</span> is modeled as a physically thick ribbon of height H, composed of large particles embedded in dust of fractional optical depth f. The observed profiles, combined with previous results, can be explained if the F <span class="hlt">ring</span> is both optically thick ( radial optical depth ˜0.20) and physically thick ( H=21±4 km). We suggest that this vertical distribution results from the interactions between <span class="hlt">ring</span> particles and shepherding satellites and/or from gravitational stirring by large bodies. The dust particles dominate the F <span class="hlt">ring</span>'s photometric behavior even in backscattered light ( f>0.80). Constraints on the particle properties of the other <span class="hlt">rings</span> are also derived.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1819d0022O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1819d0022O"><span>Turning the LHC <span class="hlt">ring</span> into a new physics search machine</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Orava, Risto</p> <p>2017-03-01</p> <p>The LHC Collider <span class="hlt">Ring</span> is proposed to be turned into an ultimate automatic search engine for new physics in four consecutive phases: (1) Searches for heavy particles produced in Central Exclusive Process (CEP): pp → p + X + p based on the existing Beam Loss Monitoring (BLM) system of the LHC; (2) Feasibility study of using the LHC <span class="hlt">Ring</span> as a gravitation wave antenna; (3) Extensions to the current BLM system to facilitate precise registration of the selected CEP proton exit points from the LHC beam vacuum chamber; (4) Integration of the BLM based <span class="hlt">event</span> tagging system together with the trigger/data acquisition systems of the LHC experiments to facilitate an on-line automatic search machine for the physics of tomorrow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA07559&hterms=org&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dorg','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA07559&hterms=org&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dorg"><span>Luminescent <span class="hlt">Rings</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>2005-01-01</p> <p><p/> This view shows the unlit face of Saturn's <span class="hlt">rings</span>, visible via scattered and transmitted light. In these views, dark regions represent gaps and areas of higher particle densities, while brighter regions are filled with less dense concentrations of <span class="hlt">ring</span> particles. <p/> The dim right side of the image contains nearly the entire C <span class="hlt">ring</span>. The brighter region in the middle is the inner B <span class="hlt">ring</span>, while the darkest part represents the dense outer B <span class="hlt">Ring</span>. The Cassini Division and the innermost part of the A <span class="hlt">ring</span> are at the upper-left. <p/> Saturn's shadow carves a dark triangle out of the lower right corner of this image. <p/> The image was taken in visible light with the Cassini spacecraft wide-angle camera on June 8, 2005, at a distance of approximately 433,000 kilometers (269,000 miles) from Saturn. The image scale is 22 kilometers (14 miles) per pixel. <p/> The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colo. <p/> For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov . The Cassini imaging team homepage is at http://ciclops.org .</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3502675','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3502675"><span>A Photo-Favorskii <span class="hlt">Ring</span> Contraction Reaction: The Effect of <span class="hlt">Ring</span> Size</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kammath, Viju Balachandran; Šolomek, Tomáš; Ngoy, Bokolombe Pitchou; Heger, Dominik; Klán, Petr; Rubina, Marina; Givens, Richard S.</p> <p>2012-01-01</p> <p>The effect of <span class="hlt">ring</span> size on the photo-Favorskii induced <span class="hlt">ring</span>-contraction reaction of the hydroxybenzocycloalkanonyl acetate and mesylate esters (7a–d, 8a–c) has provided new insight into the mechanism of the rearrangement. By monotonically decreasing the <span class="hlt">ring</span> size in these cyclic derivatives, the increasing <span class="hlt">ring</span> strain imposed on the formation of the elusive bicyclic spirocyclopropanone 20 results in a divergence away from rearrangement and toward solvolysis. Cycloalkanones of seven or eight carbons undergo a highly efficient photo-Favorskii rearrangement with <span class="hlt">ring</span> contraction paralleling the photochemistry of p-hydroxyphenacyl esters. In contrast, the five-carbon <span class="hlt">ring</span> does not rearrange but is diverted to the photosolvolysis channel avoiding the increased strain energy that would accompany the formation of the spirobicyclic ketone, the “Favorskii intermediate 20”. The six-carbon analogue demonstrates the bifurcation in reaction channels, yielding a solvent-sensitive mixture of both. Employing a combination of time-resolved absorption measurements, quantum yield determinations, isotopic labeling, and solvent variation studies coupled with theoretical treatment, a more comprehensive mechanistic description of the rearrangement has emerged. PMID:22686289</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850003648&hterms=ants&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dants','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850003648&hterms=ants&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dants"><span>Dynamics of the Uranian <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dermott, S. F.</p> <p>1984-01-01</p> <p>Some of the problems of the shepherding satellite model of Goldreich ant tremaine are discussed. The following topics are studied: (1) optical depths of the all the observed narrow <span class="hlt">rings</span>; (2) satellite and <span class="hlt">ring</span> separation timescales; (3) <span class="hlt">ring</span> edge sharpness; (4) shock formation in narrow <span class="hlt">rings</span>; (5) the existence of small satellites near the Uranian <span class="hlt">rings</span>; and (6) the apse and node alignments of the eccentric and inclined <span class="hlt">rings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFMPP41B..05M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFMPP41B..05M"><span>Seasonally Resolved Oxygen Isotope Paleoclimate Proxy in Tree-<span class="hlt">Ring</span> Cellulose from the Southeastern U.S.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miller, D. L.; Mora, C. I.; Grissino-Mayer, H. D.; Mock, C. J.</p> <p>2004-12-01</p> <p>Stable isotopes in precipitation reflect changes in climate, moisture source, and extreme <span class="hlt">events</span> such as tropical cyclones, and an oxygen isotope proxy record of these changes through time and space is preserved in tree-<span class="hlt">ring</span> cellulose. Extreme climate <span class="hlt">events</span> such as droughts and hurricanes are formidable natural disasters in the southeastern United States, and considerable efforts have been made to understand factors controlling their frequency, whether natural or anthropogenic. Tree <span class="hlt">rings</span> offer an unusually well-resolved, dateable record of climate <span class="hlt">events</span> extending beyond modern or historical (documentary) records. Oxygen isotopes in alpha-cellulose of shallowly-rooted conifers predominately reflect the composition of precipitation. Tropical storm convection results in marked 18O depletion in storm precipitation, to -15‰ relative to source seawater (~0‰ ). The depletion increases towards the eyewall of the cyclone, however, isotopically depleted precipitation may extend outward many 100's of km. Storm water 18O depletion translates to soil water 18O depletion that may persist for many weeks until ameliorated by soil water evaporation. Tree growth during that time will take up the anomalous isotopic compositions. Distinctive earlywood (EW ~March-June) versus latewood (LW ~July-October) growth allows the <span class="hlt">rings</span> to be resolved at an intra-annual (seasonal) scale. By comparison to average soil water, droughts result in 18O-enriched soil water compositions. Seasonal drought or years of continued drought will be similarly captured in the isotope compositions of tree-<span class="hlt">ring</span> cellulose. A 227-year (1770-1997) seasonally-resolved record of tropical cyclone and drought activity was obtained from cross-sections of felled slash pines (Pinus elliottii Engelm.) and remnant longleaf pines (Pinus palustris Mill.) from southern Georgia. Interpretations of drought or hurricane <span class="hlt">events</span> were tested by comparison with recent, detailed meteorological records. The 227-year record reveals</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSH43C..06G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSH43C..06G"><span><span class="hlt">Ring</span> Current Pressure Estimation withRAM-SCB using Data Assimilation and VanAllen Probe Flux Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Godinez, H. C.; Yu, Y.; Henderson, M. G.; Larsen, B.; Jordanova, V.</p> <p>2015-12-01</p> <p>Capturing and subsequently modeling the influence of tail plasma injections on the inner magnetosphere is particularly important for understanding the formation and evolution of Earth's <span class="hlt">ring</span> current. In this study, the <span class="hlt">ring</span> current distribution is estimated with the <span class="hlt">Ring</span> Current-Atmosphere Interactions Model with Self-Consistent Magnetic field (RAM-SCB) using, for the first time, data assimilation techniques and particle flux data from the Van Allen Probes. The state of the <span class="hlt">ring</span> current within the RAM-SCB is corrected via an ensemble based data assimilation technique by using proton flux from one of the Van Allen Probes, to capture the enhancement of <span class="hlt">ring</span> current following an isolated substorm <span class="hlt">event</span> on July 18 2013. The results show significant improvement in the estimation of the <span class="hlt">ring</span> current particle distributions in the RAM-SCB model, leading to better agreement with observations. This newly implemented data assimilation technique in the global modeling of the <span class="hlt">ring</span> current thus provides a promising tool to better characterize the effect of substorm injections in the near-Earth regions. The work is part of the Space Hazards Induced near Earth by Large, Dynamic Storms (SHIELDS) project in Los Alamos National Laboratory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA01976&hterms=many+miles+away+moon&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmany%2Bmiles%2Baway%2Bmoon','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA01976&hterms=many+miles+away+moon&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmany%2Bmiles%2Baway%2Bmoon"><span>Uranus <span class="hlt">rings</span> and two moons</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1986-01-01</p> <p>Voyager 2 has discovered two 'shepherd' satellites associated with the <span class="hlt">rings</span> of Uranus. The two moons -- designated 1986U7 and 1986U8 -- are seen here on either side of the bright epsilon <span class="hlt">ring</span>; all nine of the known Uranian <span class="hlt">rings</span> are visible. The image was taken Jan. 21, 1986, at a distance of 4.1 million kilometers (2.5 million miles) and resolution of about 36 km (22 mi). The image was processed to enhance narrow features. The epsilon <span class="hlt">ring</span> appears surrounded by a dark halo as a result of this processing; occasional blips seen on the <span class="hlt">ring</span> are also artifacts. Lying inward from the epsilon <span class="hlt">ring</span> are the delta, gamma and eta <span class="hlt">rings</span>; then the beta and alpha <span class="hlt">rings</span>; and finally the barely visible 4, 5 and 6 <span class="hlt">rings</span>. The <span class="hlt">rings</span> have been studied since their discovery in 1977, through observations of how they diminish the light of stars they pass in front of. This image is the first direct observation of all nine <span class="hlt">rings</span> in reflected sunlight. They range in width from about 100 km (60 mi) at the widest part of the epsilon <span class="hlt">ring</span> to only a few kilometers for most of the others. The discovery of the two <span class="hlt">ring</span> moons 1986U7 and 1986U8 is a major advance in our understanding of the structure of the Uranian <span class="hlt">rings</span> and is in good agreement with theoretical predictions of how these narrow <span class="hlt">rings</span> are kept from spreading out. Based on likely surface brightness properties, the moons are of roughly 2O- and 3O-km diameter, respectively. The Voyager project is managed for NASA by the Jet Propulsion Laboratory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26065889','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26065889"><span>Impact of low intensity summer rainfall on E. coli-discharge <span class="hlt">event</span> dynamics with reference to sample acquisition and <span class="hlt">storage</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Oliver, David M; Porter, Kenneth D H; Heathwaite, A Louise; Zhang, Ting; Quilliam, Richard S</p> <p>2015-07-01</p> <p>Understanding the role of different rainfall scenarios on faecal indicator organism (FIO) dynamics under variable field conditions is important to strengthen the evidence base on which regulators and land managers can base informed decisions regarding diffuse microbial pollution risks. We sought to investigate the impact of low intensity summer rainfall on Escherichia coli-discharge (Q) patterns at the headwater catchment scale in order to provide new empirical data on FIO concentrations observed during baseflow conditions. In addition, we evaluated the potential impact of using automatic samplers to collect and store freshwater samples for subsequent microbial analysis during summer storm sampling campaigns. The temporal variation of E. coli concentrations with Q was captured during six <span class="hlt">events</span> throughout a relatively dry summer in central Scotland. The relationship between E. coli concentration and Q was complex with no discernible patterns of cell emergence with Q that were repeated across all <span class="hlt">events</span>. On several occasions, an order of magnitude increase in E. coli concentrations occurred even with slight increases in Q, but responses were not consistent and highlighted the challenges of attempting to characterise temporal responses of E. coli concentrations relative to Q during low intensity rainfall. Cross-comparison of E. coli concentrations determined in water samples using simultaneous manual grab and automated sample collection was undertaken with no difference in concentrations observed between methods. However, the duration of sample <span class="hlt">storage</span> within the autosampler unit was found to be more problematic in terms of impacting on the representativeness of microbial water quality, with unrefrigerated autosamplers exhibiting significantly different concentrations of E. coli relative to initial samples after 12-h <span class="hlt">storage</span>. The findings from this study provide important empirical contributions to the growing evidence base in the field of catchment microbial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA20509.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA20509.html"><span>Tiny Mimas, Huge <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2016-11-28</p> <p>Saturn's icy moon Mimas is dwarfed by the planet's enormous <span class="hlt">rings</span>. Because Mimas (near lower left) appears tiny by comparison, it might seem that the <span class="hlt">rings</span> would be far more massive, but this is not the case. Scientists think the <span class="hlt">rings</span> are no more than a few times as massive as Mimas, or perhaps just a fraction of Mimas' mass. Cassini is expected to determine the mass of Saturn's <span class="hlt">rings</span> to within just a few hundredths of Mimas' mass as the mission winds down by tracking radio signals from the spacecraft as it flies close to the <span class="hlt">rings</span>. The <span class="hlt">rings</span>, which are made of small, icy particles spread over a vast area, are extremely thin -- generally no thicker than the height of a house. Thus, despite their giant proportions, the <span class="hlt">rings</span> contain a surprisingly small amount of material. Mimas is 246 miles (396 kilometers) wide. This view looks toward the sunlit side of the <span class="hlt">rings</span> from about 6 degrees above the <span class="hlt">ring</span> plane. The image was taken in red light with the Cassini spacecraft wide-angle camera on July 21, 2016. The view was obtained at a distance of approximately 564,000 miles (907,000 kilometers) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 31 degrees. Image scale is 34 miles (54 kilometers) per pixel. http://photojournal.jpl.nasa.gov/catalog/PIA20509</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JGRB..119.6733B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JGRB..119.6733B"><span>Magmatic development of the outer Vø<span class="hlt">ring</span> margin from seismic data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Breivik, Asbjørn; Faleide, Jan Inge; Mjelde, Rolf; Flueh, Ernst; Murai, Yoshio</p> <p>2014-09-01</p> <p>The Vø<span class="hlt">ring</span> Plateau off mid-Norway is a volcanic passive margin, located north of the East Jan Mayen Fracture Zone (EJMFZ). Large volumes of magmatic rocks were emplaced during Early Eocene margin formation. In 2003, an ocean bottom seismometer survey was acquired over the margin. One profile crosses from the Vø<span class="hlt">ring</span> Plateau to the Vø<span class="hlt">ring</span> Spur, a bathymetric high north of the EJMFZ. The P wave data were ray traced into a 2-D crustal velocity model. The velocity structure of the Vø<span class="hlt">ring</span> Spur indicates up to 15 km igneous crustal thickness. Magmatic processes can be estimated by comparing seismic velocity (VP) with igneous thickness (H). This and two other profiles show a positive H-VP correlation at the Vø<span class="hlt">ring</span> Plateau, consistent with elevated mantle temperature at breakup. However, during the first 2 Ma magma production was augmented by a secondary process, possibly small-scale convection. From ˜51.5 Ma excess melting may be caused by elevated mantle temperature alone. Seismic stratigraphy around the Vø<span class="hlt">ring</span> Spur shows that it was created by at least two uplift <span class="hlt">events</span>, with the main episode close to the Miocene/Pliocene boundary. Low H-VP correlation of the spur is consistent with renewed igneous growth by constant, moderate-degree mantle melting, not related to the breakup magmatism. The admittance function between bathymetry and free-air gravity shows that the high is near local isostatic equilibrium, precluding that compressional flexure at the EJMFZ uplifted the high. We find a proposed Eocene triple junction model for the margin to be inconsistent with observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvP...7d4009M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvP...7d4009M"><span>Switching by Domain-Wall Automotion in Asymmetric Ferromagnetic <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mawass, Mohamad-Assaad; Richter, Kornel; Bisig, Andre; Reeve, Robert M.; Krüger, Benjamin; Weigand, Markus; Stoll, Hermann; Krone, Andrea; Kronast, Florian; Schütz, Gisela; Kläui, Mathias</p> <p>2017-04-01</p> <p>Spintronic applications based on magnetic domain-wall (DW) motion, such as magnetic data <span class="hlt">storage</span>, sensors, and logic devices, require approaches to reliably manipulate the magnetization in nanowires. In this paper, we report the direct dynamic experimental visualization of reliable switching from the onion to the vortex state by DW automotion at zero field in asymmetric ferromagnetic <span class="hlt">rings</span> using a uniaxial field pulse. Employing time-resolved x-ray microscopy, we demonstrate that depending on the detailed spin structure of the DWs and the size and geometry of the <span class="hlt">rings</span>, the automotive propagation can be tailored during the DW relaxation from the higher-energy onion state to the energetically favored vortex state, where both DWs annihilate. Our measurements show DW automotion with an average velocity of about 60 m /s , which is a significant speed for spintronic devices. Such motion is mostly governed by local forces resulting from the geometry variations in the device. A closer study of the annihilation process via micromagnetic simulations reveals that a new vortex is nucleated in between the two initial walls. We demonstrate that the annihilation of DWs through automotion in our scheme always occurs with the detailed topological nature of the walls influencing only the DW dynamics on a local scale. The simulations show good quantitative agreement with our experimental results. These findings shed light on a robust and reliable switching process of the onion state in ferromagnetic <span class="hlt">rings</span>, which paves the way for further optimization of these devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930021275&hterms=Sequoia&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DSequoia','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930021275&hterms=Sequoia&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DSequoia"><span>Striped tertiary <span class="hlt">storage</span> arrays</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drapeau, Ann L.</p> <p>1993-01-01</p> <p>Data stripping is a technique for increasing the throughput and reducing the response time of large access to a <span class="hlt">storage</span> system. In striped magnetic or optical disk arrays, a single file is striped or interleaved across several disks; in a striped tape system, files are interleaved across tape cartridges. Because a striped file can be accessed by several disk drives or tape recorders in parallel, the sustained bandwidth to the file is greater than in non-striped systems, where access to the file are restricted to a single device. It is argued that applying striping to tertiary <span class="hlt">storage</span> systems will provide needed performance and reliability benefits. The performance benefits of striping for applications using large tertiary <span class="hlt">storage</span> systems is discussed. It will introduce commonly available tape drives and libraries, and discuss their performance limitations, especially focusing on the long latency of tape accesses. This section will also describe an <span class="hlt">event</span>-driven tertiary <span class="hlt">storage</span> array simulator that is being used to understand the best ways of configuring these <span class="hlt">storage</span> arrays. The reliability problems of magnetic tape devices are discussed, and plans for modeling the overall reliability of striped tertiary <span class="hlt">storage</span> arrays to identify the amount of error correction required are described. Finally, work being done by other members of the Sequoia group to address latency of accesses, optimizing tertiary <span class="hlt">storage</span> arrays that perform mostly writes, and compression is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740026172','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740026172"><span>On a suspected <span class="hlt">ring</span> external to the visible <span class="hlt">rings</span> of Saturn</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Feibelman, W. A.; Beebe, R. F.; Smith, B. A.; Cook, A. F., II</p> <p>1974-01-01</p> <p>The reexamination of a photograph of Saturn taken on 15 November 1966 when the earth was nearly in the <span class="hlt">ring</span> plane is investigated which indicates that <span class="hlt">ring</span> material does exist outside the visible <span class="hlt">rings</span>, extending to more than 6 Saturnian radii. The observed brightness in blue light was estimated per linear arc second, implying a normal optical thickness, for ice-covered particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H53F1767R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H53F1767R"><span><span class="hlt">Event</span> Water Balance and Recharge at the Panola Mountain Research Watershed, Georgia, U.S.A.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riley, J. W.; Aulenbach, B. T.</p> <p>2016-12-01</p> <p>Investigating catchment <span class="hlt">storage</span> and runoff pathways allows a better mechanistic understanding of stream flow generation processes. This information can be used to elucidate processes such as those influencing baseflow that support human consumption and ecological needs. Here we describe storm runoff water budgets from 483 rain <span class="hlt">events</span> to determine the conditions under which precipitation infiltrates to deeper <span class="hlt">storage</span> that supports baseflow. Further, we examine the <span class="hlt">storage</span> and recharge behavior of different storm characteristics and antecedent conditions. We use a simple water budget approach to achieve this in which Deep Recharge = (Precipitation) - (Storm Runoff) - (<span class="hlt">Event</span> Change in Soil <span class="hlt">Storage</span>). Hydrograph separation was used to determine the storm periods and split storm runoff into baseflow and quickflow. Quickflow was assumed to account for the <span class="hlt">event</span> water lost to the stream. Data from volumetric water content sensors were used to calculate the soil profile water <span class="hlt">storage</span> and the change in water <span class="hlt">storage</span> over the course of an <span class="hlt">event</span>. The remaining water after these two components was assumed to represent water available for deeper recharge. The median <span class="hlt">event</span> quickflow:precipitation ratio was 11.8%. <span class="hlt">Event</span> soil moisture recharge in the top one meter of soil accounted for a median of 65.3% of precipitation. Quickflow and shallow soil moisture recharge accounted for a median of 77.1% of the precipitation delivered to the watershed. Water budgets indicated that 43% of the <span class="hlt">events</span> provided water for deeper recharge. Of these <span class="hlt">events</span>, however, only 28% provided 50 mm or more of deep recharge. Because the focus was on <span class="hlt">events</span>, when humidity was high and the vapor pressure deficit (VPD) was low, we ignored the role of evapotranspiration. However, interception, which was not accounted for, would have resulted in less storm precipitation than was measured at the watershed rain gage. Furthermore, transpiration may have altered the post-storm water balance when VPD increased and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140002358','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140002358"><span>Deployable Fresnel <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kennedy, Timothy F.; Fink, Patrick W.; Chu, Andrew W.; Lin, Gregory Y.</p> <p>2014-01-01</p> <p>Deployable Fresnel <span class="hlt">rings</span> (DFRs) significantly enhance the realizable gain of an antenna. This innovation is intended to be used in combination with another antenna element, as the DFR itself acts as a focusing or microwave lens element for a primary antenna. This method is completely passive, and is also completely wireless in that it requires neither a cable, nor a connector from the antenna port of the primary antenna to the DFR. The technology improves upon the previous NASA technology called a Tri-Sector Deployable Array Antenna in at least three critical aspects. In contrast to the previous technology, this innovation requires no connector, cable, or other physical interface to the primary communication radio or sensor device. The achievable improvement in terms of antenna gain is significantly higher than has been achieved with the previous technology. Also, where previous embodiments of the Tri-Sector antenna have been constructed with combinations of conventional (e.g., printed circuit board) and conductive fabric materials, this innovation is realized using only conductive and non-conductive fabric (i.e., "e-textile") materials, with the possible exception of a spring-like deployment <span class="hlt">ring</span>. Conceptually, a DFR operates by canceling the out-of-phase radiation at a plane by insertion of a conducting <span class="hlt">ring</span> or <span class="hlt">rings</span> of a specific size and distance from the source antenna, defined by Fresnel zones. Design of DFRs follow similar procedures to those outlined for conventional Fresnel zone <span class="hlt">rings</span>. Gain enhancement using a single <span class="hlt">ring</span> is verified experimentally and through computational simulation. The experimental test setup involves a microstrip patch antenna that is directly behind a single-<span class="hlt">ring</span> DFR and is radiating towards a second microstrip patch antenna. The first patch antenna and DFR are shown. At 2.42 GHz, the DFR improves the transmit antenna gain by 8.6 dB, as shown in Figure 2, relative to the wireless link without the DFR. A figure illustrates 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_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/2018AIPA....8c5025H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPA....8c5025H"><span>Mechanical improvement of metal reinforcement <span class="hlt">rings</span> for a finite <span class="hlt">ring</span>-shaped superconducting bulk</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Chen-Guang; Zhou, You-He</p> <p>2018-03-01</p> <p>As a key technique, reinforcement of type-II superconducting bulks with metal <span class="hlt">rings</span> can efficiently improve their mechanical properties to enhance the maximum trapped field. In this paper, we study the magnetostrictive and fracture behaviors of a finite superconducting <span class="hlt">ring</span> bulk reinforced by three typical reinforcing structures composed of metal <span class="hlt">rings</span> during the magnetizing process by means of the minimization of magnetic energy and the finite element method. After a field-dependent critical current density is adopted, the magnetostriction, pinning-induced stress, and crack tip stress intensity factor are calculated considering the demagnetization effects. The results show that the mechanical properties of the <span class="hlt">ring</span> bulk are strongly dependent on the reinforcing structure and the material and geometrical parameters of the metal <span class="hlt">rings</span>. Introducing the metal <span class="hlt">ring</span> can significantly reduce the hoop stress, and the reduction effect by internal reinforcement is much improved relative to external reinforcement. By comparison, bilateral reinforcement seems to be the best candidate structure. Only when the metal <span class="hlt">rings</span> have particular Young's modulus and radial thickness will they contribute to improve the mechanical properties the most. In addition, if an edge crack is pre-existing in the <span class="hlt">ring</span> bulk, the presence of metal <span class="hlt">rings</span> can effectively avoid crack propagation since it reduces the crack tip stress intensity factor by nearly one order of magnitude.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1960d0001A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1960d0001A"><span><span class="hlt">Ring</span> rotational speed trend analysis by FEM approach in a <span class="hlt">Ring</span> Rolling process</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Allegri, G.; Giorleo, L.; Ceretti, E.</p> <p>2018-05-01</p> <p><span class="hlt">Ring</span> Rolling is an advanced local incremental forming technology to fabricate directly precise seamless <span class="hlt">ring</span>-shape parts with various dimensions and materials. In this process two different deformations occur in order to reduce the width and the height of a preform hollow <span class="hlt">ring</span>; as results a diameter expansion is obtained. In order to guarantee a uniform deformation, the preform is forced toward the Driver Roll whose aim is to transmit the rotation to the <span class="hlt">ring</span>. The <span class="hlt">ring</span> rotational speed selection is fundamental because the higher is the speed the higher will be the axial symmetry of the deformation process. However, it is important to underline that the rotational speed will affect not only the final <span class="hlt">ring</span> geometry but also the loads and energy needed to produce it. Despite this importance in industrial environment, usually, a constant value for the Driver Roll angular velocity is set so to result in a decreasing trend law for the <span class="hlt">ring</span> rotational speed. The main risk due to this approach is not fulfilling the axial symmetric constrain (due to the diameter expansion) and to generate a high localized <span class="hlt">ring</span> section deformation. In order to improve the knowledge about this topic in the present paper three different <span class="hlt">ring</span> rotational speed trends (constant, linearly increasing and linearly decreasing) were investigated by FEM approach. Results were compared in terms of geometrical and dimensional analysis, loads and energies required.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003PhDT.......214B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003PhDT.......214B"><span>Study of the longitudinal space charge compensation and longitudinal instability of the ferrite inductive inserts in the Los Alamos Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beltran, Chris</p> <p></p> <p>Future high intensity synchrotrons will have a large space charge effect. It has been demonstrated in the Proton <span class="hlt">Storage</span> <span class="hlt">Ring</span> (PSR) at the Los Alamos National Laboratory (LANL) that ferrite inductive inserts can be used to compensate for the longitudinal space charge effect. However, simply installing ferrite inductors in the PSR led to longitudinal instabilities that were not tolerable. It was proposed that heating the ferrite would change the material properties in such a way as to reduce the instability. This proposal was tested in the PSR, and found to be true. This dissertation investigates and describes the complex permeability of the ferrite at room temperature and at an elevated temperature. The derived complex permeability is then used to obtain an impedance at the two temperatures. The impedance is used to determine the amount of space charge compensation supplied by the inductors and predict the growth time and frequency range of the longitudinal instability. The impedance is verified by comparing the experimental growth time and frequency range of the longitudinal instability to theoretical and computer simulated growth times and frequency ranges of the longitudinal instability. Lastly, an approach to mitigating the longitudinal instability that does not involve heating the ferrite is explored.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28905430','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28905430"><span>Archaea S-layer nanotube from a "black smoker" in complex with cyclo-octasulfur (S8 ) <span class="hlt">rings</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McDougall, Matthew; Francisco, Olga; Harder-Viddal, Candice; Roshko, Roy; Meier, Markus; Stetefeld, Jörg</p> <p>2017-12-01</p> <p>Elemental sulfur exists primarily as an S80 <span class="hlt">ring</span> and serves as terminal electron acceptor for a variety of sulfur-fermenting bacteria. Hyperthermophilic archaea from black smoker vents are an exciting research tool to advance our knowledge of sulfur respiration under extreme conditions. Here, we use a hybrid method approach to demonstrate that the proteinaceous cavities of the S-layer nanotube of the hyperthermophilic archaeon Staphylothermus marinus act as a <span class="hlt">storage</span> reservoir for cyclo-octasulfur S8. Fully atomistic molecular dynamics (MD) simulations were performed and the method of multiconfigurational thermodynamic integration was employed to compute the absolute free energy for transferring a <span class="hlt">ring</span> of elemental sulfur S8 from an aqueous bath into the largest hydrophobic cavity of a fragment of archaeal tetrabrachion. Comparisons with earlier MD studies of the free energy of hydration as a function of water occupancy in the same cavity of archaeal tetrabrachion show that the sulfur <span class="hlt">ring</span> is energetically favored over water. © 2017 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28085390','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28085390"><span><span class="hlt">Ring</span> correlations in random networks.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sadjadi, Mahdi; Thorpe, M F</p> <p>2016-12-01</p> <p>We examine the correlations between <span class="hlt">rings</span> in random network glasses in two dimensions as a function of their separation. Initially, we use the topological separation (measured by the number of intervening <span class="hlt">rings</span>), but this leads to pseudo-long-range correlations due to a lack of topological charge neutrality in the shells surrounding a central <span class="hlt">ring</span>. This effect is associated with the noncircular nature of the shells. It is, therefore, necessary to use the geometrical distance between <span class="hlt">ring</span> centers. Hence we find a generalization of the Aboav-Weaire law out to larger distances, with the correlations between <span class="hlt">rings</span> decaying away when two <span class="hlt">rings</span> are more than about three <span class="hlt">rings</span> apart.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080006002','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080006002"><span>Seal <span class="hlt">ring</span> installation tool</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Haselmaier, L. Haynes (Inventor)</p> <p>2004-01-01</p> <p>A seal <span class="hlt">ring</span> tool that allows an installer to position a primary seal <span class="hlt">ring</span> between hub ends of pipe flanges that are being assembled together. The tool includes a pivoting handle member and extension arms attached to the pivoting handle member. The ends of the arms have side indentation type longitudinal grooves angled toward one another for holding the primary seal <span class="hlt">ring</span> in place between the hubs of respective pipes that are to be attached together. The arms of the tool can also have flat sides that can be used to abut against an optional second larger seal that is supported within a groove in one of the hub ends so that the second hub end can then be moved against the other side of the primary seal <span class="hlt">ring</span>. Once the seal <span class="hlt">ring</span> is positioned between the pipe hubs, the pipe hubs can be moved about the seal <span class="hlt">ring</span> due to the flat sides of the arms of the tool. The tool eliminates the chances of damaging and contaminating seal <span class="hlt">rings</span> being installed within pipe hubs that are being attached to one another.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA02202&hterms=systems+diffuse&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsystems%2Bdiffuse','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA02202&hterms=systems+diffuse&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsystems%2Bdiffuse"><span>Neptune - full <span class="hlt">ring</span> system</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1989-01-01</p> <p>This pair of Voyager 2 images (FDS 11446.21 and 11448.10), two 591-s exposures obtained through the clear filter of the wide angle camera, show the full <span class="hlt">ring</span> system with the highest sensitivity. Visible in this figure are the bright, narrow N53 and N63 <span class="hlt">rings</span>, the diffuse N42 <span class="hlt">ring</span>, and (faintly) the plateau outside of the N53 <span class="hlt">ring</span> (with its slight brightening near 57,500 km).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA20498.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA20498.html"><span>Barely Bisected <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2016-09-12</p> <p>Saturn's shadow stretched beyond the edge of its <span class="hlt">rings</span> for many years after Cassini first arrived at Saturn, casting an ever-lengthening shadow that reached its maximum extent at the planet's 2009 equinox. This image captured the moment in 2015 when the shrinking shadow just barely reached across the entire main <span class="hlt">ring</span> system. The shadow will continue to shrink until the planet's northern summer solstice, at which point it will once again start lengthening across the <span class="hlt">rings</span>, reaching across them in 2019. Like Earth, Saturn is tilted on its axis. And, just as on Earth, as the sun climbs higher in the sky, shadows get shorter. The projection of the planet's shadow onto the <span class="hlt">rings</span> shrinks and grows over the course of its 29-year-long orbit, as the angle of the sun changes with respect to Saturn's equator. This view looks toward the sunlit side of the <span class="hlt">rings</span> from about 11 degrees above the <span class="hlt">ring</span> plane. The image was taken in visible light with the Cassini spacecraft wide-angle camera on Jan. 16, 2015. The view was obtained at a distance of approximately 1.6 million miles (2.5 million kilometers) from Saturn. Image scale is about 90 miles (150 kilometers) per pixel. http://photojournal.jpl.nasa.gov/catalog/PIA20498</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Icar..300..150C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Icar..300..150C"><span>Particle sizes in Saturn's <span class="hlt">rings</span> from UVIS stellar occultations 1. Variations with <span class="hlt">ring</span> region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Colwell, J. E.; Esposito, L. W.; Cooney, J. H.</p> <p>2018-01-01</p> <p>The Cassini spacecraft's Ultraviolet Imaging Spectrograph (UVIS) includes a high speed photometer (HSP) that has observed stellar occultations by Saturn's <span class="hlt">rings</span> with a radial resolution of ∼10 m. In the absence of intervening <span class="hlt">ring</span> material, the time series of measurements by the HSP is described by Poisson statistics in which the variance equals the mean. The finite sizes of the <span class="hlt">ring</span> particles occulting the star lead to a variance that is larger than the mean due to correlations in the blocking of photons due to finite particle size and due to random variations in the number of individual particles in each measurement area. This effect was first exploited by Showalter and Nicholson (1990) with the stellar occultation observed by Voyager 2. At a given optical depth, a larger excess variance corresponds to larger particles or clumps that results in greater variation of the signal from measurement to measurement. Here we present analysis of the excess variance in occultations observed by Cassini UVIS. We observe differences in the best-fitting particle size in different <span class="hlt">ring</span> regions. The C <span class="hlt">ring</span> plateaus show a distinctly smaller effective particle size, R, than the background C <span class="hlt">ring</span>, while the background C <span class="hlt">ring</span> itself shows a positive correlation between R and optical depth. The innermost 700 km of the B <span class="hlt">ring</span> has a distribution of excess variance with optical depth that is consistent with the C <span class="hlt">ring</span> ramp and C <span class="hlt">ring</span> but not with the remainder of the B1 region. The Cassini Division, while similar to the C <span class="hlt">ring</span> in spectral and structural properties, has different trends in effective particle size with optical depth. There are discrete jumps in R on either side of the Cassini Division ramp, while the C <span class="hlt">ring</span> ramp shows a smooth transition in R from the C <span class="hlt">ring</span> to the B <span class="hlt">ring</span>. The A <span class="hlt">ring</span> is dominated by self-gravity wakes whose shadow size depends on the occultation geometry. The spectral ;halo; regions around the strongest density waves in the A <span class="hlt">ring</span> correspond to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1091869','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1091869"><span>EIGHTH INTERIM STATUS REPORT: MODEL 9975 PCV O-<span class="hlt">RING</span> FIXTURE LONG-TERM LEAK PERFORMANCE</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>Daugherty, W. L.</p> <p>2013-09-03</p> <p>A series of experiments to monitor the aging performance of Viton® GLT O-<span class="hlt">rings</span> used in the Model 9975 package has been ongoing since 2004 at the Savannah River National Laboratory. Seventy tests using mock-ups of 9975 Primary Containment Vessels (PCVs) were assembled and heated to temperatures ranging from 200 to 450 ºF. They were leak-tested initially and have been tested periodically to determine if they meet the criterion of leak-tightness defined in ANSI standard N14.5-97. Fourteen additional tests were initiated in 2008 with GLT-S O-<span class="hlt">rings</span> heated to temperatures ranging from 200 to 400 ºF. High temperature aging continues for 23more » GLT O-<span class="hlt">ring</span> fixtures at 200 – 270 ºF. Room temperature leak test failures have been experienced in all of the GLT O-<span class="hlt">ring</span> fixtures aging at 350 ºF and higher temperatures, and in 8 fixtures aging at 300 ºF. The remaining GLT O-<span class="hlt">ring</span> fixtures aging at 300 ºF have been retired from testing following more than 5 years at temperature without failure. No failures have yet been observed in GLT O-<span class="hlt">ring</span> fixtures aging at 200 ºF for 61 - 85 months, which is still bounding to O-<span class="hlt">ring</span> temperatures during <span class="hlt">storage</span> in KArea Complex (KAC). Based on expectations that the fixtures aging at 200 ºF will remain leaktight for a significant period yet to come, 2 additional fixtures began aging in 2011 at an intermediate temperature of 270 ºF, with hopes that they may reach a failure condition before the 200 ºF fixtures. High temperature aging continues for 6 GLT-S O-<span class="hlt">ring</span> fixtures at 200 – 300 ºF. Room temperature leak test failures have been experienced in all 8 of the GLT-S O-<span class="hlt">ring</span> fixtures aging at 350 and 400 ºF. No failures have yet been observed in GLT-S O-<span class="hlt">ring</span> fixtures aging at 200 - 300 ºF for 41 - 45 months. Aging and periodic leak testing will continue for the remaining PCV fixtures.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MS%26E..101a2080S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MS%26E..101a2080S"><span>Modification of a liquid hydrogen tank for integrated refrigeration and <span class="hlt">storage</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Swanger, A. M.; Jumper, K. M.; Fesmire, J. E.; Notardonato, W. U.</p> <p>2015-12-01</p> <p>The modification and outfitting of a 125,000-liter liquid hydrogen tank was performed to provide integrated refrigeration and <span class="hlt">storage</span> capability. These functions include zero boil-off, liquefaction, and densification and therefore require provisions for sub-atmospheric tank pressures within the vacuum-jacketed, multilayer insulated tank. The primary structural modification was to add stiffening <span class="hlt">rings</span> inside the inner vessel. The internal stiffening <span class="hlt">rings</span> were designed, built, and installed per the ASME Boiler and Pressure Vessel Code, Section VIII, to prevent collapse in the case of vacuum jacket failure in combination with sub-atmospheric pressure within the tank. For the integrated refrigeration loop, a modular, skeleton-type heat exchanger, with refrigerant temperature instrumentation, was constructed using the stiffening <span class="hlt">rings</span> as supports. To support the system thermal performance testing, three custom temperature rakes were designed and installed along the 21-meter length of the tank, once again using <span class="hlt">rings</span> as supports. The temperature rakes included a total of 20 silicon diode temperature sensors mounted both vertically and radially to map the bulk liquid temperature within the tank. The tank modifications were successful and the system is now operational for the research and development of integrated refrigeration technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999PhDT.......105R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999PhDT.......105R"><span>Record of the Solar Activity and of Other Geophysical Phenomenons in Tree <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rigozo, Nivaor Rodolfo</p> <p>1999-01-01</p> <p>Tree <span class="hlt">ring</span> studies are usually used to determine or verify climatic factors which prevail in a given place or region and may cause tree <span class="hlt">ring</span> width variations. Few studies are dedicated to the geophysical phenomena which may underlie these tree <span class="hlt">ring</span> width variations. In order to look for periodicities which may be associated to the solar activity and/or to other geophysical phenomena which may influence tree <span class="hlt">ring</span> growth, a new interactive image analysis method to measure tree <span class="hlt">ring</span> width was developed and is presented here. This method makes use of a computer and a high resolution flatbed scanner; a program was also developed in Interactive Data Language (IDL 5.0) to study <span class="hlt">ring</span> digitized images and transform them into time series. The main advantage of this method is the tree <span class="hlt">ring</span> image interactive analysis without needing complex and high cost instrumentation. Thirty-nine samples were collected: 12 from Concordia - S. C., 9 from Canela - R. S., 14 from Sao Francisco de Paula - R. S., one from Nova Petropolis - R. S., 2 from Sao Martinho da Serra - R. S. e one from Chile. Fit functions are applied to <span class="hlt">ring</span> width time series to obtain the best long time range trend (growth rate of every tree) curves and are eliminated through a standardization process that gives the tree <span class="hlt">ring</span> index time series from which is performed spectral analysis by maximum entropy method and iterative regression. The results obtained show periodicities close to 11 yr, 22 yr Hale solar cycles and 5.5 yr for all sampling locations 52 yr and Gleissberg cycles for Concordia - S. C. and Chile samples. El Nino <span class="hlt">events</span> were also observed with periods around 4 e 7 yr.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996DPS....28.1803P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996DPS....28.1803P"><span>The 1995 Saturn <span class="hlt">Ring</span>-Plane Crossings: <span class="hlt">Ring</span> Thickness and Small Inner Satellites</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Poulet, F.; Sicardy, B.</p> <p>1996-09-01</p> <p>The May 22() th and August 10() th, 1995, Saturn <span class="hlt">ring</span>-plane crossings by the Earth were observed from the 2-m and 1-m telescopes at Pic du Midi, the 2.2-m telescope of the University of Hawaii, and with the Adonis adaptive optics camera at the 3.6-m telescope of the European Southern Observatory (ESO). Observations were made with either a 0.9 mu m or 2.2 mu m (short K) methane band filter. The radial brightness profiles of the <span class="hlt">rings</span> indicate that the outer F <span class="hlt">ring</span> dominates the apparent edge-on thickness of the system, with a vertically integrated equivalent width of 0.8-1.0 km near a radius of 130,000 km. The photometric behaviors of the A, B, and C <span class="hlt">rings</span> and of the Cassini Division have been analyzed using a classical radiative transfer code which includes illumination by the Sun and by the planet. The F <span class="hlt">ring</span> is modelled as a physically thick ribbon (thickness h) composed of large particles embedded in dust. The observed profiles can be explained if the F <span class="hlt">ring</span> is both optically thick (tau ~ 0.15-0.25), and physically thick (h at least ~ 1.5 km). The large particles dominate the F <span class="hlt">ring</span>'s photometric behavior in backscattered light. Constraints on the particle properties in the other <span class="hlt">rings</span> have been derived. The dimming of the <span class="hlt">rings</span> around August 10, 1995 provided ideal conditions to study the small inner satellites. Besides Janus, Epimetheus and Pandora, two unresolved objects were detected in the ESO frames. They have been identified with the objects 1995S5 and 1995S6, detected several hours later by the Hubble Space Telescope (Nicholson et al. 1996, Science 272, 509--515). Combining the ESO and HST data, we derive orbital and photometric parameters for these objects. In particular, we improve the orbital parameters of 1995S5, whose orbital radius is now close to that of the F <span class="hlt">ring</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030069','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030069"><span>Saturn's dynamic D <span class="hlt">ring</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>Hedman, M.M.; Burns, J.A.; Showalter, M.R.; Porco, C.C.; Nicholson, P.D.; Bosh, A.S.; Tiscareno, M.S.; Brown, R.H.; Buratti, B.J.; Baines, K.H.; Clark, R.</p> <p>2007-01-01</p> <p>The Cassini spacecraft has provided the first clear images of the D <span class="hlt">ring</span> since the Voyager missions. These observations show that the structure of the D <span class="hlt">ring</span> has undergone significant changes over the last 25 years. The brightest of the three ringlets seen in the Voyager images (named D72), has transformed from a narrow, <40-km wide ringlet to a much broader and more diffuse 250-km wide feature. In addition, its center of light has shifted inwards by over 200 km relative to other features in the D <span class="hlt">ring</span>. Cassini also finds that the locations of other narrow features in the D <span class="hlt">ring</span> and the structure of the diffuse material in the D <span class="hlt">ring</span> differ from those measured by Voyager. Furthermore, Cassini has detected additional ringlets and structures in the D <span class="hlt">ring</span> that were not observed by Voyager. These include a sheet of material just interior to the inner edge of the C <span class="hlt">ring</span> that is only observable at phase angles below about 60??. New photometric and spectroscopic data from the ISS (Imaging Science Subsystem) and VIMS (Visual and Infrared Mapping Spectrometer) instruments onboard Cassini show the D <span class="hlt">ring</span> contains a variety of different particle populations with typical particle sizes ranging from 1 to 100 microns. High-resolution images reveal fine-scale structures in the D <span class="hlt">ring</span> that appear to be variable in time and/or longitude. Particularly interesting is a remarkably regular, periodic structure with a wavelength of ??? 30 ?? km extending between orbital radii of 73,200 and 74,000 km. A similar structure was previously observed in 1995 during the occultation of the star GSC5249-01240, at which time it had a wavelength of ??? 60 ?? km. We interpret this structure as a periodic vertical corrugation in the D <span class="hlt">ring</span> produced by differential nodal regression of an initially inclined <span class="hlt">ring</span>. We speculate that this structure may have formed in response to an impact with a comet or meteoroid in early 1984. ?? 2006 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012436','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012436"><span>Formation of lunar basin <span class="hlt">rings</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>Hodges, C.A.; Wilhelms, D.E.</p> <p>1978-01-01</p> <p>The origin of the multiple concentric <span class="hlt">rings</span> that characterize lunar impact basins, and the probable depth and diameter of the transient crater have been widely debated. As an alternative to prevailing "megaterrace" hypotheses, we propose that the outer scarps or mountain <span class="hlt">rings</span> that delineate the topographic rims of basins-the Cordilleran at Orientale, the Apennine at Imbrium, and the Altai at Nectaris-define the transient cavities, enlarged relatively little by slumping, and thus are analogous to the rim crests of craters like Copernicus; inner <span class="hlt">rings</span> are uplifted rims of craters nested within the transient cavity. The magnitude of slumping that occurs on all scarps is insufficient to produce major inner <span class="hlt">rings</span> from the outer. These conclusions are based largely on the observed gradational sequence in lunar central uplifts:. from simple peaks through somewhat annular clusters of peaks, peak and <span class="hlt">ring</span> combinations and double <span class="hlt">ring</span> basins, culminating in multiring structures that may also include peaks. In contrast, belts of slump terraces are not gradational with inner <span class="hlt">rings</span>. Terrestrial analogs suggest two possible mechanisms for producing <span class="hlt">rings</span>. In some cases, peaks may expand into <span class="hlt">rings</span> as material is ejected from their cores, as apparently occurred at Gosses Bluff, Australia. A second process, differential excavation of lithologically diverse layers, has produced nested experimental craters and is, we suspect, instrumental in the formation of terrestrial <span class="hlt">ringed</span> impact craters. Peak expansion could produce double-<span class="hlt">ring</span> structures in homogeneous materials, but differential excavation is probably required to produce multiring and peak-in-<span class="hlt">ring</span> configurations in large lunar impact structures. Our interpretation of the representative lunar multiring basin Orientale is consistent with formation of three <span class="hlt">rings</span> in three layers detected seismically in part of the Moon-the Cordillera (basin-bounding) <span class="hlt">ring</span> in the upper crust, the composite Montes Rook <span class="hlt">ring</span> in the underlying</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC53C1227M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC53C1227M"><span>The value of electricity <span class="hlt">storage</span> in energy-only electricity markets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McConnell, D.; Forcey, T.; Sandiford, M.</p> <p>2015-12-01</p> <p>Price volatility and the prospect of increasing renewable energy generation have raised interest in the potential opportunities for <span class="hlt">storage</span> technologies in energy-only electricity markets. In this paper we explore the value of a price-taking <span class="hlt">storage</span> device in such a market, the National Electricity Market (NEM) in Australia. Our analysis suggests that under optimal operation, there is little value in having more than six hours of <span class="hlt">storage</span> in this market. However, the inability to perfectly forecast wholesale prices, particularly extreme price spikes, may warrant some additional <span class="hlt">storage</span>. We found that <span class="hlt">storage</span> devices effectively provide a similar service as peak generators (such as Open Cycle Gas Turbines) and are similarly dependent on and exposed to extreme price <span class="hlt">events</span>, with revenue for a merchant generator highly skewed to a few days of the year. In contrast to previous studies, this results in the round trip efficiency of the <span class="hlt">storage</span> being relatively insignificant. Financing using hedging strategies similar to a peak generator effectively reduces the variability of revenue and exposure of <span class="hlt">storage</span> to extreme prices. Our case study demonstrates that <span class="hlt">storage</span> may have a competitive advantage over other peaking generators on the NEM, due to its ability to earn revenue outside of extreme peak <span class="hlt">events</span>. As a consequence the outlook for <span class="hlt">storage</span> options on the NEM is dependent on volatility, in turn dependent on capacity requirements. Further to this, increased integration of renewable energy may both depend on <span class="hlt">storage</span> and improve the outlook for <span class="hlt">storage</span> in technologies in electricity markets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA12512.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA12512.html"><span>Eyeing the E <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2009-12-24</p> <p>NASA Cassini spacecraft takes a look at Saturn diffuse E <span class="hlt">ring</span> which is formed from icy material spewing out of the south pole of the moon Enceladus. The E <span class="hlt">ring</span> is seen nearly edge-on from slightly above the northern side of Saturn <span class="hlt">ring</span> plane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880005104','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880005104"><span>Hot piston <span class="hlt">ring</span> tests</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Allen, David J.; Tomazic, William A.</p> <p>1987-01-01</p> <p>As part of the DOE/NASA Automotive Stirling Engine Project, tests were made at NASA Lewis Research Center to determine whether appendix gap losses could be reduced and Stirling engine performance increased by installing an additional piston <span class="hlt">ring</span> near the top of each piston dome. An MTI-designed upgraded Mod I Automotive Stirling Engine was used. Unlike the conventional <span class="hlt">rings</span> at the bottom of the piston, these hot <span class="hlt">rings</span> operated in a high temperature environment (700 C). They were made of a high temperature alloy (Stellite 6B) and a high temperature solid lubricant coating (NASA Lewis-developed PS-200) was applied to the cylinder walls. Engine tests were run at 5, 10, and 15 MPa operating pressure over a range of operating speeds. Tests were run both with hot <span class="hlt">rings</span> and without to provide a baseline for comparison. Minimum data to assess the potential of both the hot <span class="hlt">rings</span> and high temperature low friction coating was obtained. Results indicated a slight increase in power and efficiency, an increase over and above the friction loss introduced by the hot <span class="hlt">rings</span>. Seal leakage measurements showed a significant reduction. Wear on both <span class="hlt">rings</span> and coating was low.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED238675.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED238675.pdf"><span>Tree <span class="hlt">Rings</span>: Timekeepers of the Past.</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>Phipps, R. L.; McGowan, J.</p> <p></p> <p>One of a series of general interest publications on science issues, this booklet describes the uses of tree <span class="hlt">rings</span> in historical and biological recordkeeping. Separate sections cover the following topics: dating of tree <span class="hlt">rings</span>, dating with tree <span class="hlt">rings</span>, tree <span class="hlt">ring</span> formation, tree <span class="hlt">ring</span> identification, sample collections, tree <span class="hlt">ring</span> cross dating, tree…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/873075','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/873075"><span>Cavity-locked <span class="hlt">ring</span> down spectroscopy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Zare, Richard N.; Paldus, Barbara A.; Harb, Charles C.; Spence, Thomas</p> <p>2000-01-01</p> <p>Distinct locking and sampling light beams are used in a cavity <span class="hlt">ring</span>-down spectroscopy (CRDS) system to perform multiple <span class="hlt">ring</span>-down measurements while the laser and <span class="hlt">ring</span>-down cavity are continuously locked. The sampling and locking light beams have different frequencies, to ensure that the sampling and locking light are decoupled within the cavity. Preferably, the <span class="hlt">ring</span>-down cavity is <span class="hlt">ring</span>-shaped, the sampling light is s-polarized, and the locking light is p-polarized. Transmitted sampling light is used for <span class="hlt">ring</span>-down measurements, while reflected locking light is used for locking in a Pound-Drever scheme.</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://www.ncbi.nlm.nih.gov/pubmed/21691588','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21691588"><span>Accidental ingestion of BiTine <span class="hlt">ring</span> and a note on inefficient <span class="hlt">ring</span> separation forceps.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baghele, Om Nemichand; Baghele, Mangala Om</p> <p>2011-01-01</p> <p>Accidental ingestion of medium-to-large instruments is relatively uncommon during dental treatment but can be potentially dangerous. A case of BiTine <span class="hlt">ring</span> ingestion is presented with a note on inefficient <span class="hlt">ring</span> separation forceps. A 28-year-old male patient accidentally ingested the BiTine <span class="hlt">ring</span> (2 cm diameter, 0.5 cm outward projections) while it was being applied to a distoproximal cavity in tooth # 19. The <span class="hlt">ring</span> placement forceps were excessively flexible; bending of the beaks towards the <span class="hlt">ring</span> combined with a poor no-slippage mechanism led to sudden disengagement of the <span class="hlt">ring</span> and accelerated movement towards the pharynx. We followed the patient with bulk forming agents and radiographs. Fortunately the <span class="hlt">ring</span> passed out without any complications. Checking equipment and methods is as important as taking precautions against any preventable medical emergency. It is the responsibility of the clinician to check, verify and then use any instrument/equipment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.898d2033G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.898d2033G"><span>An Oracle-based <span class="hlt">event</span> index for ATLAS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gallas, E. J.; Dimitrov, G.; Vasileva, P.; Baranowski, Z.; Canali, L.; Dumitru, A.; Formica, A.; ATLAS Collaboration</p> <p>2017-10-01</p> <p>The ATLAS Eventlndex System has amassed a set of key quantities for a large number of ATLAS <span class="hlt">events</span> into a Hadoop based infrastructure for the purpose of providing the experiment with a number of <span class="hlt">event</span>-wise services. Collecting this data in one place provides the opportunity to investigate various <span class="hlt">storage</span> formats and technologies and assess which best serve the various use cases as well as consider what other benefits alternative <span class="hlt">storage</span> systems provide. In this presentation we describe how the data are imported into an Oracle RDBMS (relational database management system), the services we have built based on this architecture, and our experience with it. We’ve indexed about 26 billion real data <span class="hlt">events</span> thus far and have designed the system to accommodate future data which has expected rates of 5 and 20 billion <span class="hlt">events</span> per year. We have found this system offers outstanding performance for some fundamental use cases. In addition, profiting from the co-location of this data with other complementary metadata in ATLAS, the system has been easily extended to perform essential assessments of data integrity and completeness and to identify <span class="hlt">event</span> duplication, including at what step in processing the duplication occurred.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16417688','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16417688"><span>Morphological processing in a second language: behavioral and <span class="hlt">event</span>-related brain potential evidence for <span class="hlt">storage</span> and decomposition.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hahne, Anja; Mueller, Jutta L; Clahsen, Harald</p> <p>2006-01-01</p> <p>This study reports the results of two behavioral and two <span class="hlt">event</span>-related brain potential experiments examining the processing of inflected words in second-language (L2) learners with Russian as their native language. Two different subsystems of German inflection were studied, participial inflection and noun plurals. For participial forms, L2 learners were found to widely generalize the -t suffixation rule in a nonce-word elicitation task, and in the <span class="hlt">event</span>-related brain potential experiment, they showed an anterior negativity followed by a P600-both results resembling previous findings from native speakers of German on the same materials. For plural formation, the L2 learners displayed different preference patterns for regular and irregular forms in an off-line plural judgment task. Regular and irregular plural forms also differed clearly with regard to their brain responses. Whereas overapplications of the -s plural rule produced a P600 component, overapplications of irregular patterns elicited an N400. In contrast to native speakers of German, however, the L2 learners did not show an anterior negativity for -s plural overapplications. Taken together, the results show clear dissociations between regular and irregular inflection for both morphological subsystems. We argue that the two processing routes posited by dual-mechanism models of inflection (lexical <span class="hlt">storage</span> and morphological decomposition) are also employed by L2 learners.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002APS..MAR.B3001B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002APS..MAR.B3001B"><span>Vortex formation in magnetic narrow <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bland, J. A. C.</p> <p>2002-03-01</p> <p>Underlying the current interest in magnetic elements is the possibility such systems provide both for the study of fundamental phenomena in magnetism (such as domain wall trapping and spin switching) and for technological applications, such as high density magnetic <span class="hlt">storage</span> or magnetic random access memories (MRAM). One key issue is to control the magnetic switching precisely. To achieve this one needs first to have a well defined and reproducible remanent state, and second the switching process itself must be simple and reproducible. Among the many studied geometries, <span class="hlt">rings</span> are shown to exhibit several advantages over other geometries, in that they show relatively simple stable magnetic states at remanence, with fast and simple magnetisation switching mechanisms. This is borne out of our systematic investigation of the magnetic properties of epitaxial and polycrystalline Co <span class="hlt">rings</span>, where both the static, dynamic and transport properties have been studied. Magnetic measurements and micromagnetic simulations show that for appropriate <span class="hlt">ring</span> structures a two step switching process occurs at high fields, indicating the existence of two different stable states. In addition to the vortex state, which occurs at intermediate fields, we have identified a new bi-domain state, which we term the `onion state', corresponding to opposite circulation of the magnetisation in each half of the <span class="hlt">ring</span>. The magnetic elements were fabricated using a new technique based on the pre-patterning of Si <span class="hlt">ring</span> structures and subsequent epitaxial growth of Cu/Co/Cu sandwich films on top of the Si elements. This technique has allowed the growth of epitaxial fcc Co(001) structures and in contrast to conventional lithographic methods, no damage to the magnetic layer structure is introduced by the patterning process [1,2]. We have studied the magnetic switching properties of arrays of narrow Co(100) epitaxial <span class="hlt">ring</span> magnets, with outer diameters between 1 μm and 2 μm, varying inner diameters and varying</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-12-19/pdf/2011-32373.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-12-19/pdf/2011-32373.pdf"><span>76 FR 78641 - Southwestern Gas <span class="hlt">Storage</span> Technical Conference; Notice of Public Conference</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2011-12-19</p> <p>... <span class="hlt">Storage</span> Technical Conference; Notice of Public Conference Take notice that on February 16, 2012 at 9 a.m... technical conference with interested parties to discuss issues related to natural gas <span class="hlt">storage</span> development in... Cold Weather <span class="hlt">Event</span> of February 1-5, 2011: Causes and Recommendations, ``[a]dditional gas <span class="hlt">storage</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29111587','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29111587"><span>Multifractal Approaches of the <span class="hlt">Ring</span> Tensile Rupture Patterns of Dried Laver (Porphyra) as Affected by the Relative Humidity.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jung, Hwabin; Yoon, Won Byong</p> <p>2017-12-01</p> <p>The effect of water activity (a w ) or the relative humidity (RH) on the tensile rupture properties of dried laver (DL) associated with structures formed with phycocolloids was investigated. The morphological characteristics of tensile ruptured DL samples at various relative humidities were evaluated by multifractal analysis. The RH of the microclimate was controlled from 10% to 90% at 25 °C using supersaturated salt solutions. The sorption isotherm of DL was experimentally obtained and quantitatively analyzed using mathematical models. The monolayer moisture contents from the Guggenheim-Anderson-de Boer (GAB) model was 5.92% (w.b.). An increase in the RH resulted in increasing <span class="hlt">ring</span> tensile stress and maintaining constant <span class="hlt">ring</span> tensile strain up to 58% to 75% RH, whereas the <span class="hlt">ring</span> tensile stress and the <span class="hlt">ring</span> tensile strain rapidly decreased and increased, respectively, when the RH was higher than 75%. The general fractal dimensions and the multifractal spectra f(α) manifested that the patterns of the lowest and the highest moisture content of dried laver showed high irregularity. The different multifractal parameters obtained from the DL at various RHs well-represented the transient moment of the structures from the monolayer moisture to texture changes associated with RH. Overall, the <span class="hlt">ring</span> tensile test and the multifractal analysis were useful tools to analyze the change of crispness of DL from its structural characteristics. In addition, the results of this study revealed that the integration and disintegration properties of DL occurred through the networks of phycocolloids at various moisture contents. Texture properties are the most important quality attributes for commercial dried laver (DL) products. The relative humidity influences the texture properties of DL during production, <span class="hlt">storage</span>, shipping, and consuming. This study well characterized the effect of the relative humidity on the texture properties of DL using the tensile tests under microclimate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007RMxAA..43..315G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007RMxAA..43..315G"><span>Photometry of Polar-<span class="hlt">Ring</span> Galaxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Godínez-Martínez, A.; Watson, A. M.; Matthews, L. D.; Sparke, L. S.</p> <p>2007-10-01</p> <p>We have obtained photometry in B and R for seven confirmed or probable polar-<span class="hlt">ring</span> galaxies from the Polar-<span class="hlt">Ring</span> Catalog of Whitmore et al. (1990). The <span class="hlt">rings</span> show a range of colors from B - R ≈ 0.6 to B - R ≈ 1.7. The bluest <span class="hlt">rings</span> have bright H II regions, which are direct evidence for recent star formation. The minimum age of the reddest <span class="hlt">ring</span>, that in PRC B-20, is somewhat uncertain because of a lack of knowledge of the internal reddening and metallicity, but appears to be at least 1.2 Gyr. As such, this <span class="hlt">ring</span> is likely to be stable for at least several rotation periods. This <span class="hlt">ring</span> is an excellent candidate for future studies that might better determine if it is truly old.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4934284','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4934284"><span>Improving the Accuracy of Laplacian Estimation with Novel Variable Inter-<span class="hlt">Ring</span> Distances Concentric <span class="hlt">Ring</span> Electrodes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Makeyev, Oleksandr; Besio, Walter G.</p> <p>2016-01-01</p> <p>Noninvasive concentric <span class="hlt">ring</span> electrodes are a promising alternative to conventional disc electrodes. Currently, the superiority of tripolar concentric <span class="hlt">ring</span> electrodes over disc electrodes, in particular, in accuracy of Laplacian estimation, has been demonstrated in a range of applications. In our recent work, we have shown that accuracy of Laplacian estimation can be improved with multipolar concentric <span class="hlt">ring</span> electrodes using a general approach to estimation of the Laplacian for an (n + 1)-polar electrode with n <span class="hlt">rings</span> using the (4n + 1)-point method for n ≥ 2. This paper takes the next step toward further improving the Laplacian estimate by proposing novel variable inter-<span class="hlt">ring</span> distances concentric <span class="hlt">ring</span> electrodes. Derived using a modified (4n + 1)-point method, linearly increasing and decreasing inter-<span class="hlt">ring</span> distances tripolar (n = 2) and quadripolar (n = 3) electrode configurations are compared to their constant inter-<span class="hlt">ring</span> distances counterparts. Finite element method modeling and analytic results are consistent and suggest that increasing inter-<span class="hlt">ring</span> distances electrode configurations may decrease the truncation error resulting in more accurate Laplacian estimates compared to respective constant inter-<span class="hlt">ring</span> distances configurations. For currently used tripolar electrode configuration, the truncation error may be decreased more than two-fold, while for the quadripolar configuration more than a six-fold decrease is expected. PMID:27294933</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27294933','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27294933"><span>Improving the Accuracy of Laplacian Estimation with Novel Variable Inter-<span class="hlt">Ring</span> Distances Concentric <span class="hlt">Ring</span> Electrodes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Makeyev, Oleksandr; Besio, Walter G</p> <p>2016-06-10</p> <p>Noninvasive concentric <span class="hlt">ring</span> electrodes are a promising alternative to conventional disc electrodes. Currently, the superiority of tripolar concentric <span class="hlt">ring</span> electrodes over disc electrodes, in particular, in accuracy of Laplacian estimation, has been demonstrated in a range of applications. In our recent work, we have shown that accuracy of Laplacian estimation can be improved with multipolar concentric <span class="hlt">ring</span> electrodes using a general approach to estimation of the Laplacian for an (n + 1)-polar electrode with n <span class="hlt">rings</span> using the (4n + 1)-point method for n ≥ 2. This paper takes the next step toward further improving the Laplacian estimate by proposing novel variable inter-<span class="hlt">ring</span> distances concentric <span class="hlt">ring</span> electrodes. Derived using a modified (4n + 1)-point method, linearly increasing and decreasing inter-<span class="hlt">ring</span> distances tripolar (n = 2) and quadripolar (n = 3) electrode configurations are compared to their constant inter-<span class="hlt">ring</span> distances counterparts. Finite element method modeling and analytic results are consistent and suggest that increasing inter-<span class="hlt">ring</span> distances electrode configurations may decrease the truncation error resulting in more accurate Laplacian estimates compared to respective constant inter-<span class="hlt">ring</span> distances configurations. For currently used tripolar electrode configuration, the truncation error may be decreased more than two-fold, while for the quadripolar configuration more than a six-fold decrease is expected.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5100299','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5100299"><span>Embryonic <span class="hlt">ring</span> closure: Actomyosin <span class="hlt">rings</span> do the two-step</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2016-01-01</p> <p>Actomyosin <span class="hlt">rings</span> drive numerous closure processes, but the mechanisms by which they contract are still poorly understood. In this issue, Xue and Sokac (2016. J. Cell Biol. http://dx.doi.org/10.1083/jcb.201608025) show that actomyosin <span class="hlt">ring</span> closure during Drosophila melanogaster cellularization uses two steps, only one of which involves Myosin-2. PMID:27799371</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA08855.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA08855.html"><span>Scintillating C <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2007-01-16</p> <p>Both luminous and translucent, the C <span class="hlt">ring</span> sweeps out of the darkness of Saturn's shadow and obscures the planet at lower left. The <span class="hlt">ring</span> is characterized by broad, isolated bright areas, or "plateaus," surrounded by fainter material. This view looks toward the unlit side of the <span class="hlt">rings</span> from about 19 degrees above the ringplane. North on Saturn is up. The dark, inner B <span class="hlt">ring</span> is seen at lower right. The image was taken in visible light with the Cassini spacecraft wide-angle camera on Dec. 15, 2006 at a distance of approximately 632,000 kilometers (393,000 miles) from Saturn and at a Sun-Saturn-spacecraft, or phase, angle of 56 degrees. Image scale is 34 kilometers (21 miles) per pixel. http://photojournal.jpl.nasa.gov/catalog/PIA08855</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005Icar..177...32N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005Icar..177...32N"><span>Radar imaging of Saturn's <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nicholson, Philip D.; French, Richard G.; Campbell, Donald B.; Margot, Jean-Luc; Nolan, Michael C.; Black, Gregory J.; Salo, Heikki J.</p> <p>2005-09-01</p> <p>We present delay-Doppler images of Saturn's <span class="hlt">rings</span> based on radar observations made at Arecibo Observatory between 1999 and 2003, at a wavelength of 12.6 cm and at <span class="hlt">ring</span> opening angles of 20.1°⩽|B|⩽26.7°. The average radar cross-section of the A <span class="hlt">ring</span> is ˜77% relative to that of the B <span class="hlt">ring</span>, while a stringent upper limit of 3% is placed on the cross-section of the C <span class="hlt">ring</span> and 9% on that of the Cassini Division. These results are consistent with those obtained by Ostro et al. [1982, Icarus 49, 367-381] from radar observations at |B|=21.4°, but provide higher resolution maps of the <span class="hlt">rings</span>' reflectivity profile. The average cross-section of the A and B <span class="hlt">rings</span>, normalized by their projected unblocked area, is found to have decreased from 1.25±0.31 to 0.74±0.19 as the <span class="hlt">rings</span> have opened up, while the circular polarization ratio has increased from 0.64±0.06 to 0.77±0.06. The steep decrease in cross-section is at variance with previous radar measurements [Ostro et al., 1980, Icarus 41, 381-388], and neither this nor the polarization variations are easily understood within the framework of either classical, many-particle-thick or monolayer <span class="hlt">ring</span> models. One possible explanation involves vertical size segregation in the <span class="hlt">rings</span>, whereby observations at larger elevation angles which see deeper into the <span class="hlt">rings</span> preferentially see the larger particles concentrated near the <span class="hlt">rings</span>' mid-plane. These larger particles may be less reflective and/or rougher and thus more depolarizing than the smaller ones. Images from all four years show a strong m=2 azimuthal asymmetry in the reflectivity of the A <span class="hlt">ring</span>, with an amplitude of ±20% and minima at longitudes of 67±4° and 247±4° from the sub-Earth point. We attribute the asymmetry to the presence of gravitational wakes in the A <span class="hlt">ring</span> as invoked by Colombo et al. [1976, Nature 264, 344-345] to explain the similar asymmetry long seen at optical wavelengths. A simple radiative transfer model suggests that the enhancement of the azimuthal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNH33D..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNH33D..02S"><span>Water <span class="hlt">Storage</span>: Quo Vadis?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smakhtin, V.</p> <p>2017-12-01</p> <p>Humans stored water - in various forms - for ages, coping with water resources variability, and its extremes - floods and droughts. <span class="hlt">Storage</span> per capita, and other <span class="hlt">storage</span>-related indicators, have essentially become one way of reflecting the progress of economic development. Massive investments went into large surface water reservoirs that have become the characteristic feature of the earth's landscapes, bringing both benefits and controversy. As water variability progressively increases with changing climate, globally, on one hand, and the idea of sustainable development receives strong traction, on another - it may be worth the while to comprehensively examine current trends and future prospects for water <span class="hlt">storage</span> development. The task is surely big, to say the least. The presentation will aim to initiate a structured discussion on this multi-facet issue and identify which aspects and trends of water <span class="hlt">storage</span> development may be most important in the context of Sustainable Development Goals, Sendai Framework for Disaster Risk Reduction, Paris Agreement on Climate Change, and examine how, where and to what extent water <span class="hlt">storage</span> planning can be improved. It will cover questions like i) aging of large water <span class="hlt">storage</span> infrastructure, the current extent of this trend in various geographical regions, and possible impacts on water security and security of nations; ii) improved water <span class="hlt">storage</span> development planning overall in the context of various water development alternatives and <span class="hlt">storage</span> options themselves and well as their combinations iii) prospects for another "<span class="hlt">storage</span> revolution" - speed increase in dam numbers, and where, if at all this is most likely iv) recent <span class="hlt">events</span> in <span class="hlt">storage</span> development, e.g. is dam decommissioning a trend that picks pace, or whether some developing economies in Asia can do without going through the period of water <span class="hlt">storage</span> construction, with alternatives, or suggestions for alleviation of negative impacts v) the role of subsurface <span class="hlt">storage</span> as an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA00033&hterms=false+information&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dfalse%2Binformation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA00033&hterms=false+information&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dfalse%2Binformation"><span>Uranus <span class="hlt">Rings</span> in False Color</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1986-01-01</p> <p>This false-color view of the <span class="hlt">rings</span> of Uranus was made from images taken by Voyager 2 on Jan. 21, 1986, from a distance of 4.17 million kilometers (2.59 million miles). All nine known <span class="hlt">rings</span> are visible here; the somewhat fainter, pastel lines seen between them are contributed by the computer enhancement. Six 15-second narrow-angle images were used to extract color information from the extremely dark and faint <span class="hlt">rings</span>. Two images each in the green, clear and violet filters were added together and averaged to find the proper color differences between the <span class="hlt">rings</span>. The final image was made from these three color averages and represents an enhanced, false-color view. The image shows that the brightest, or epsilon, <span class="hlt">ring</span> at top is neutral in color, with the fainter eight other <span class="hlt">rings</span> showing color differences between them. Moving down, toward Uranus, we see the delta, gamma and eta <span class="hlt">rings</span> in shades of blue and green; the beta and alpha <span class="hlt">rings</span> in somewhat lighter tones; and then a final set of three, known simply as the 4, 5 and 6 <span class="hlt">rings</span>, in faint off-white tones. Scientists will use this color information to try to understand the nature and origin of the <span class="hlt">ring</span> material. The resolution of this image is approximately 40 km (25 mi). The Voyager project is managed for NASA by the Jet Propulsion Laboratory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014RScI...85f3304K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014RScI...85f3304K"><span>Capacitive energy <span class="hlt">storage</span> and recovery for synchrotron magnets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koseki, K.</p> <p>2014-06-01</p> <p>Feasibility studies on capacitive energy <span class="hlt">storage</span> and recovery in the main-<span class="hlt">ring</span> synchrotron of the Japan Proton Accelerator Research Complex were conducted by circuit simulation. The estimated load fluctuation was 96 MVA in total for dipole magnets, which is likely to induce a serious disturbance in the main grid. It was found that the energy stored in the magnets after the excitation period can be recovered to the <span class="hlt">storage</span> capacitor by controlling the voltage across the energy-<span class="hlt">storage</span> capacitor using a pulse-width-modulation converter and reused in the next operational cycle. It was also found that the power fluctuation in the main grid can be reduced to 12 MVA. An experimental evaluation of an aluminum metalized film capacitor revealed that capacitance loss was induced by a fluctuating voltage applied to the <span class="hlt">storage</span> capacitor when applying the proposed method. The capacitance loss was induced by corona discharge around the edges of segmented electrodes of a self-healing capacitor. The use of aluminum-zinc alloy was evaluated as a countermeasure to mitigate the effect induced by the corona discharge. For a zinc content of 8%, which was optimized experimentally, a capacitor with a sufficient life time expectancy of 20 years and a working potential gradient of 250 V/μm was developed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApSS..434..626H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApSS..434..626H"><span>From coffee <span class="hlt">ring</span> to spherulites <span class="hlt">ring</span> of poly(ethylene oxide) film from drying droplet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hu, Yinchun; Zhang, Xuerong; Qiu, Maibo; Wei, Yan; Zhou, Qiong; Huang, Di</p> <p>2018-03-01</p> <p>We discuss how the "spherulites <span class="hlt">ring</span>" morphology and "coffee <span class="hlt">ring</span>" profile of PEO film formed by the drying droplet at glass substrate with different heating rate. Upon increasing the heating rate of substrate, it is found that deposited PEO film from drying droplet shows the unusually observed "coffee <span class="hlt">ring</span>" profile and "spherulites <span class="hlt">ring</span>" morphology. The main mechanism for this phenomenon is proposed to be an enhanced Marangoni convection which is induced by the increased solute concentration gradient and reduced viscous force above 70 °C. A simple formation mechanism of the unusually observed "coffee <span class="hlt">ring</span>" profile and "spherulites <span class="hlt">ring</span>" morphology is proposed. These findings can be exploited to trace the center of Marangoni convection, with potential applications in designing the spherulite patterns of crystalline polymer films in ink-jet printing and self-assembly fields.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AJ....155..206A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AJ....155..206A"><span>Systematic Search for <span class="hlt">Rings</span> around Kepler Planet Candidates: Constraints on <span class="hlt">Ring</span> Size and Occurrence Rate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aizawa, Masataka; Masuda, Kento; Kawahara, Hajime; Suto, Yasushi</p> <p>2018-05-01</p> <p>We perform a systematic search for <span class="hlt">rings</span> around 168 Kepler planet candidates with sufficient signal-to-noise ratios that are selected from all of the short-cadence data. We fit <span class="hlt">ringed</span> and ringless models to their light curves and compare the fitting results to search for the signatures of planetary <span class="hlt">rings</span>. First, we identify 29 tentative systems, for which the <span class="hlt">ringed</span> models exhibit statistically significant improvement over the ringless models. The light curves of those systems are individually examined, but we are not able to identify any candidate that indicates evidence for <span class="hlt">rings</span>. In turn, we find several mechanisms of false positives that would produce ringlike signals, and the null detection enables us to place upper limits on the size of the <span class="hlt">rings</span>. Furthermore, assuming the tidal alignment between axes of the planetary <span class="hlt">rings</span> and orbits, we conclude that the occurrence rate of <span class="hlt">rings</span> larger than twice the planetary radius is less than 15%. Even though the majority of our targets are short-period planets, our null detection provides statistical and quantitative constraints on largely uncertain theoretical models of the origin, formation, and evolution of planetary <span class="hlt">rings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JHyd..557..791S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JHyd..557..791S"><span>Monthly paleostreamflow reconstruction from annual tree-<span class="hlt">ring</span> chronologies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stagge, J. H.; Rosenberg, D. E.; DeRose, R. J.; Rittenour, T. M.</p> <p>2018-02-01</p> <p>Paleoclimate reconstructions are increasingly used to characterize annual climate variability prior to the instrumental record, to improve estimates of climate extremes, and to provide a baseline for climate-change projections. To date, paleoclimate records have seen limited engineering use to estimate hydrologic risks because water systems models and managers usually require streamflow input at the monthly scale. This study explores the hypothesis that monthly streamflows can be adequately modeled by statistically decomposing annual flow reconstructions. To test this hypothesis, a multiple linear regression model for monthly streamflow reconstruction is presented that expands the set of predictors to include annual streamflow reconstructions, reconstructions of global circulation, and potential differences among regional tree-<span class="hlt">ring</span> chronologies related to tree species and geographic location. This approach is used to reconstruct 600 years of monthly streamflows at two sites on the Bear and Logan rivers in northern Utah. Nash-Sutcliffe Efficiencies remain above zero (0.26-0.60) for all months except April and Pearson's correlation coefficients (R) are 0.94 and 0.88 for the Bear and Logan rivers, respectively, confirming that the model can adequately reproduce monthly flows during the reference period (10/1942 to 9/2015). Incorporating a flexible transition between the previous and concurrent annual reconstructed flows was the most important factor for model skill. Expanding the model to include global climate indices and regional tree-<span class="hlt">ring</span> chronologies produced smaller, but still significant improvements in model fit. The model presented here is the only approach currently available to reconstruct monthly streamflows directly from tree-<span class="hlt">ring</span> chronologies and climate reconstructions, rather than using resampling of the observed record. With reasonable estimates of monthly flow that extend back in time many centuries, water managers can challenge systems models with a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA12641.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA12641.html"><span><span class="hlt">Rings</span> Through Atmosphere</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2010-05-26</p> <p>NASA Cassini spacecraft looks toward the limb of Saturn and, on the right of this image, views part of the <span class="hlt">rings</span> through the planet atmosphere. Saturn atmosphere can distort the view of the <span class="hlt">rings</span> from some angles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NatCh..10..625Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NatCh..10..625Z"><span><span class="hlt">Ring-through-ring</span> molecular shuttling in a saturated [3]rotaxane</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhu, Kelong; Baggi, Giorgio; Loeb, Stephen J.</p> <p>2018-06-01</p> <p>Mechanically interlocked molecules such as rotaxanes and catenanes comprise two or more components whose motion relative to each other can be controlled. A [2]rotaxane molecular shuttle, for example, consists of an axle bearing two recognition sites and a single macrocyclic wheel that can undergo a to-and-fro motion along the axle—shuttling between the recognition sites. The ability of mechanically interlocked molecules to undergo this type of large-amplitude change is the core mechanism behind almost every interlocked molecular switch or machine, including sophisticated mechanical systems such as a molecular elevator and a peptide synthesizer. Here, as a way to expand the scope of dynamics possible at the molecular level, we have developed a molecular shuttling mechanism involving the exchange of <span class="hlt">rings</span> between two recognition sites in a saturated [3]rotaxane (one with no empty recognition sites). This was accomplished by passing a smaller <span class="hlt">ring</span> through a larger one, thus achieving <span class="hlt">ring-through-ring</span> molecular shuttling.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29706128','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29706128"><span>Evolution of the Proximal Sealing <span class="hlt">Rings</span> of the Anaconda Stent-Graft After Endovascular Aneurysm Repair.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koenrades, Maaike A; Klein, Almar; Leferink, Anne M; Slump, Cornelis H; Geelkerken, Robert H</p> <p>2018-04-01</p> <p>To provide insight into the evolution of the saddle-shaped proximal sealing <span class="hlt">rings</span> of the Anaconda stent-graft after endovascular aneurysm repair (EVAR). Eighteen abdominal aortic aneurysm patients were consecutively enrolled in a single-center, prospective, observational cohort study (LSPEAS; Trialregister.nl identifier NTR4276). The patients were treated electively using an Anaconda stent-graft with a mean 31% oversizing (range 17-47). According to protocol, participants were to be followed for 2 years, during which 5 noncontrast electrocardiogram-gated computed tomography scans would be conducted. Three patients were eliminated within 30 days (1 withdrew, 1 died, and a third was converted before stent-graft deployment), leaving 15 patients (mean age 72.8±3.7 years; 14 men) for this analysis. Evolution in size and shape (symmetry) of both proximal infrarenal sealing <span class="hlt">rings</span> were assessed from discharge to 24 months using dedicated postprocessing algorithms. At 24 months, the mean diameters of the first and second <span class="hlt">ring</span> stents had increased significantly (first <span class="hlt">ring</span>: 2.2±1.0 mm, p<0.001; second <span class="hlt">ring</span>: 2.7±1.1 mm, p<0.001). At 6 months, the first and second <span class="hlt">rings</span> had expanded to a mean 96.6%±2.1% and 94.8%±2.7%, respectively, of their nominal diameter, after which the <span class="hlt">rings</span> expanded slowly; <span class="hlt">ring</span> diameters stabilized to near nominal size (first <span class="hlt">ring</span>, 98.3%±1.1%; second <span class="hlt">ring</span>, 97.2%±1.4%) at 24 months irrespective of initial oversizing. No type I or III endoleaks or aneurysm-, device-, or procedure-related adverse <span class="hlt">events</span> were noted in follow-up. The difference in the diametric distances between the peaks and valleys of the saddle-shaped <span class="hlt">rings</span> was marked at discharge but became smaller after 24 months for both <span class="hlt">rings</span> (first <span class="hlt">ring</span>: median 2.0 vs 1.2 mm, p=0.191; second <span class="hlt">ring</span>: median 2.8 vs 0.8 mm; p=0.013). Irrespective of initial oversizing, the Anaconda proximal sealing <span class="hlt">rings</span> radially expanded to near nominal size within 6 months after EVAR. Initial oval-shaped <span class="hlt">rings</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996DPS....28.1811T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996DPS....28.1811T"><span>Constraints on Particle Sizes in Saturn's G <span class="hlt">Ring</span> from <span class="hlt">Ring</span> Plane Crossing Observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Throop, H. B.; Esposito, L. W.</p> <p>1996-09-01</p> <p>The <span class="hlt">ring</span> plane crossings in 1995--96 allowed earth-based observations of Saturn's diffuse <span class="hlt">rings</span> (Nicholson et al., Nature 272, 1996; De Pater et al. Icarus 121, 1996) at a phase angle of alpha ~ 5 deg . We calculate the G <span class="hlt">ring</span> reflectance for steady state distributions of dust to km-sized bodies from a range of physical models which track the evolution of the G <span class="hlt">ring</span> from its initial formation following the disruption of a progenitor satellite (Canup & Esposito 1996, \\ Icarus,\\ in press). We model scattering from the <span class="hlt">ring</span>'s small particles using an exact T-matrix method for nonspherical, absorptive particles (Mishchenko et al. 1996, \\ JGR Atmo., in press), large particles using the phase function and spectrum of Europa, and intermediate particles using a linear combination of the small and large limits. Two distinct particle size distributions from the CE96 model fit the observed spectrum. The first is that of a dusty <span class="hlt">ring</span>, with the majority of <span class="hlt">ring</span> reflectance in dust particles of relatedly shallow power law size distribution exponent q ~ 2.5. The second has equal reflectances from a) dust in the range q ~ 3.5 -- 6.5 and b) macroscopic bodies > 1 mm. In this second case, the respective slightly blue and red components combine to form the observed relatively flat spectrum. Although light scattering in backscatter is not sufficient to completely constrain the G <span class="hlt">ring</span> size distribution, the distributions predicted by the CE96 model can explain the earth-based observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U22A..06T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U22A..06T"><span>High-resolution imaging of Saturn's main <span class="hlt">rings</span> during the Cassini <span class="hlt">Ring</span>-Grazing Orbits and Grand Finale</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tiscareno, M. S.</p> <p>2017-12-01</p> <p>Cassini is ending its spectacular 13-year mission at Saturn with a two-part farewell, during which it has obtained the sharpest and highest-fidelity images ever taken of Saturn's <span class="hlt">rings</span>. From December 2016 to April 2017, the spacecraft executed 20 near-polar orbits that passed just outside the outer edge of the main <span class="hlt">rings</span>; these "<span class="hlt">Ring</span>-Grazing Orbits" provided the mission's best viewing of the A and F <span class="hlt">rings</span> and the outer B <span class="hlt">ring</span>. From April to September 2017, the spacecraft is executing 22 near-polar orbits that pass between the innermost D <span class="hlt">ring</span> and the planet's clouds; this "Grand Finale" provides the mission's best viewing of the C and D <span class="hlt">rings</span> and the inner B <span class="hlt">ring</span>. 1) Clumpy BeltsClumpy structure called "straw" was previously observed in parts of the main <span class="hlt">rings</span> [Porco et al. 2005, Science]. New images show this structure with greater clarity. More surprisingly, new images reveal strong radial variations in the degree and character of clumpiness, which are probably an index for particle properties and interactions. Belts with different clumpiness characteristics are often adjacent to each other and not easily correlated with other <span class="hlt">ring</span> characteristics. 2) PropellersA "propeller" is a local disturbance in the <span class="hlt">ring</span> created by an embedded moon [Tiscareno et al. 2006, Nature; 2010, ApJL]. Cassini has observed two classes of propellers: small propellers that swarm in the "Propeller Belts" of the mid-A <span class="hlt">ring</span>, and "Giant Propellers" whose individual orbits can be tracked in the outer A <span class="hlt">ring</span>. Both are shown in unprecedented detail in new images. Targeted flybys of Giant Propellers were executed on both the lit and unlit sides of the <span class="hlt">ring</span> (see figure), yielding enhanced ability to convert brightness to optical depth and surface density. 3) Impact Ejecta CloudsBeing a large and delicate system, Saturn's <span class="hlt">rings</span> function as a detector of their planetary environment. Cassini images of impact ejecta clouds in the <span class="hlt">rings</span> previously constrained the population of decimeter</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA08908.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA08908.html"><span>Unfocused F <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2007-04-02</p> <p>The F <span class="hlt">ring</span> dissolves into a fuzzy stream of particles -- rather different from its usual appearance of a narrow, bright core flanked by dimmer ringlets. Also notable here is the bright clump of material that flanks the <span class="hlt">ring</span> core</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003DDA....34.1004W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003DDA....34.1004W"><span>An Instability in Narrow Planetary <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Weiss, J. W.; Stewart, G. R.</p> <p>2003-08-01</p> <p>We will present our work investigating the behavior of narrow planetary <span class="hlt">rings</span> with low dispersion velocities. Such narrow a <span class="hlt">ring</span> will be initially unstable to self-gravitational collapse. After the collapse, the <span class="hlt">ring</span> is collisionally very dense. At this stage, it is subject to a new instability. Waves appear on the inner and outer edges of the <span class="hlt">ring</span> within half of an orbital period. The <span class="hlt">ring</span> then breaks apart radially, taking approximately a quarter of an orbital period of do so. As clumps of <span class="hlt">ring</span> particles expand radially away from the dense <span class="hlt">ring</span>, Kepler shear causes these clumps to stretch out azimuthally, and eventually collapse into a new set of dense <span class="hlt">rings</span>. Small-scale repetitions of the original instability in these new <span class="hlt">rings</span> eventually leads to a stabilized broad <span class="hlt">ring</span> with higher dispersion velocities than the initial <span class="hlt">ring</span>. Preliminary results indicate that this instability may be operating on small scales in broad <span class="hlt">rings</span> in the wake-like features seen by Salo and others. Some intriguing properties have been observed during this instability. The most significant is a coherence in the epicyclic phases of the particles. Both self-gravity and collisions in the <span class="hlt">ring</span> operated to create and enforce this coherence. The coherence might also be responsible for the instability to radial expansion. We also observe that guiding centers of the particles do not migrate to the center of the <span class="hlt">ring</span> during the collapse phase of the <span class="hlt">ring</span>. In fact, guiding centers move radially away from the core of the <span class="hlt">ring</span> during this phase, consistent with global conservation of angular momentum. We will show the results of our simulations to date, including movies of the evolution of various parameters. (Audiences members wanting popcorn are advised to bring their own.) This work is supported by a NASA Graduate Student Research Program grant and by the Cassini mission.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1259676-copper-silicon-magnesium-alloys-latent-heat-storage','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1259676-copper-silicon-magnesium-alloys-latent-heat-storage"><span>Copper-silicon-magnesium alloys for latent heat <span class="hlt">storage</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Gibbs, P. J.; Withey, E. A.; Coker, E. N.; ...</p> <p>2016-06-21</p> <p>The systematic development of microstructure, solidification characteristics, and heat of solidification with composition in copper-silicon-magnesium alloys for thermal energy <span class="hlt">storage</span> is presented. Differential scanning calorimetry was used to relate the thermal characteristics to microstructural development in the investigated alloys and clarifies the location of one of the terminal three-phase eutectics. Repeated thermal cycling highlights the thermal <span class="hlt">storage</span> stability of the transformation through multiple melting <span class="hlt">events</span>. In conclusion, two near-terminal eutectic alloys display high enthalpies of solidification, relatively narrow melting ranges, and stable transformation hysteresis behaviors suited to thermal energy <span class="hlt">storage</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=aluminium&id=EJ827419','ERIC'); return false;" href="https://eric.ed.gov/?q=aluminium&id=EJ827419"><span>The Jumping <span class="hlt">Ring</span> Experiment</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>Baylie, M.; Ford, P. J.; Mathlin, G. P.; Palmer, C.</p> <p>2009-01-01</p> <p>The jumping <span class="hlt">ring</span> experiment has become central to liquid nitrogen shows given as part of the outreach and open day activities carried out within the University of Bath. The basic principles of the experiment are described as well as the effect of changing the geometry of the <span class="hlt">rings</span> and their metallurgical state. In general, aluminium <span class="hlt">rings</span> are…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=jump&id=EJ1090098','ERIC'); return false;" href="https://eric.ed.gov/?q=jump&id=EJ1090098"><span>DC-Powered Jumping <span class="hlt">Ring</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>Jeffery, Rondo N.; Farhang, Amiri</p> <p>2016-01-01</p> <p>The classroom jumping <span class="hlt">ring</span> demonstration is nearly always performed using alternating current (AC), in which the <span class="hlt">ring</span> jumps or flies off the extended iron core when the switch is closed. The <span class="hlt">ring</span> jumps higher when cooled with liquid nitrogen (LN2). We have performed experiments using DC to power the solenoid and find similarities and significant…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3396675','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3396675"><span>Clinical features and course of refractory anemia with <span class="hlt">ring</span> sideroblasts associated with marked thrombocytosis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Broseus, Julien; Florensa, Lourdes; Zipperer, Esther; Schnittger, Susanne; Malcovati, Luca; Richebourg, Steven; Lippert, Eric; Cermak, Jaroslav; Evans, Jyoti; Mounier, Morgane; Raya, José Maria; Bailly, François; Gattermann, Norbert; Haferlach, Torsten; Garand, Richard; Allou, Kaoutar; Besses, Carlos; Germing, Ulrich; Haferlach, Claudia; Travaglino, Erica; Luno, Elisa; Pinan, Maria Angeles; Arenillas, Leonor; Rozman, Maria; Perez Sirvent, Maria Luz; Favre, Bernardine; Guy, Julien; Alonso, Esther; Ahwij, Nuhri; Jerez, Andrés; Hermouet, Sylvie; Maynadié, Marc; Cazzola, Mario; Girodon, François</p> <p>2012-01-01</p> <p>Background Refractory anemia with <span class="hlt">ring</span> sideroblasts associated with marked thrombocytosis was proposed as a provisional entity in the 2001 World Health Organization classification of myeloid neoplasms and also in the 2008 version, but its existence as a single entity is contested. We wish to define the clinical features of this rare myelodysplastic/myeloproliferative neoplasm and to compare its clinical outcome with that of refractory anemia with <span class="hlt">ring</span> sideroblasts and essential thrombocythemia. Design and Methods We conducted a collaborative retrospective study across Europe. Our database included 200 patients diagnosed with refractory anemia with <span class="hlt">ring</span> sideroblasts and marked thrombocytosis. For each of these patients, each patient diagnosed with refractory anemia with <span class="hlt">ring</span> sideroblasts was matched for age and sex. At the same time, a cohort of 454 patients with essential thrombocythemia was used to compare outcomes of the two diseases. Results In patients with refractory anemia with <span class="hlt">ring</span> sideroblasts and marked thrombocytosis, depending on the Janus Kinase 2 V617F mutational status (positive or negative) or platelet threshold (over or below 600×109/L), no difference in survival was noted. However, these patients had shorter overall survival and leukemia-free survival with a lower risk of thrombotic complications than did patients with essential thrombocythemia (P<0.001) but better survival (P<0.001) and a higher risk of thrombosis (P=0.039) than patients with refractory anemia with <span class="hlt">ring</span> sideroblasts. Conclusions The clinical course of refractory anemia with <span class="hlt">ring</span> sideroblasts and marked thrombocytosis is better than that of refractory anemia with <span class="hlt">ring</span> sideroblasts and worse than that of essential thrombocythemia. The higher risk of thrombotic <span class="hlt">events</span> in this disorder suggests that anti-platelet therapy might be considered in this subset of patients. From a clinical point of view, it appears to be important to consider refractory anemia with <span class="hlt">ring</span> sideroblasts and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/971341','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/971341"><span>Wavelength-tunable optical <span class="hlt">ring</span> resonators</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Watts, Michael R [Albuquerque, NM; Trotter, Douglas C [Albuquerque, NM; Young, Ralph W [Albuquerque, NM; Nielson, Gregory N [Albuquerque, NM</p> <p>2009-11-10</p> <p>Optical <span class="hlt">ring</span> resonator devices are disclosed that can be used for optical filtering, modulation or switching, or for use as photodetectors or sensors. These devices can be formed as microdisk <span class="hlt">ring</span> resonators, or as open-<span class="hlt">ring</span> resonators with an optical waveguide having a width that varies adiabatically. Electrical and mechanical connections to the open-<span class="hlt">ring</span> resonators are made near a maximum width of the optical waveguide to minimize losses and thereby provide a high resonator Q. The <span class="hlt">ring</span> resonators can be tuned using an integral electrical heater, or an integral semiconductor junction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1021901','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1021901"><span>Wavelength-tunable optical <span class="hlt">ring</span> resonators</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Watts, Michael R [Albuquerque, NM; Trotter, Douglas C [Albuquerque, NM; Young, Ralph W [Albuquerque, NM; Nielson, Gregory N [Albuquerque, NM</p> <p>2011-07-19</p> <p>Optical <span class="hlt">ring</span> resonator devices are disclosed that can be used for optical filtering, modulation or switching, or for use as photodetectors or sensors. These devices can be formed as microdisk <span class="hlt">ring</span> resonators, or as open-<span class="hlt">ring</span> resonators with an optical waveguide having a width that varies adiabatically. Electrical and mechanical connections to the open-<span class="hlt">ring</span> resonators are made near a maximum width of the optical waveguide to minimize losses and thereby provide a high resonator Q. The <span class="hlt">ring</span> resonators can be tuned using an integral electrical heater, or an integral semiconductor junction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780009735','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780009735"><span>Helmet latching and attaching <span class="hlt">ring</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chase, E. W.; Viikinsalo, S. J. (Inventor)</p> <p>1970-01-01</p> <p>A neck <span class="hlt">ring</span> releasably secured to a pressurized garment carries an open-ended <span class="hlt">ring</span> normally in the engagement position fitted into an annular groove and adapted to fit into a complementary annular groove formed in a helmet. Camming means formed on the inner surface at the end of the helmet engages the open-ended <span class="hlt">ring</span> to retract the same and allow for one motion donning even when the garment is pressurized. A projection on the end of the split <span class="hlt">ring</span> is engageable to physically retract the split <span class="hlt">ring</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA12707.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA12707.html"><span>A-<span class="hlt">ring</span> Propeller</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2010-08-26</p> <p>A propeller-shaped structure, created by an unseen moon, can be seen in Saturn A <span class="hlt">ring</span> and looks like a small, dark line interrupting the bright surrounding <span class="hlt">ring</span> material in the upper left of this image taken by NASA Cassini spacecraft.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA12514.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA12514.html"><span>Splinters of <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2009-12-28</p> <p>Saturn shadow interrupts the planet <span class="hlt">rings</span>, leaving just thin slivers of the <span class="hlt">rings</span> visible in this image, which shows a pair of the planet small moons. Helene is in the center top of the image, Epimetheus is in the lower right.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22524300','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22524300"><span>Evaluating a novel analgesic strategy for <span class="hlt">ring</span> castration of ram lambs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Paull, David R; Small, Alison H; Lee, Caroline; Palladin, Pierre; Colditz, Ian G</p> <p>2012-09-01</p> <p>To evaluate the analgesic efficacy of the NSAIDs flunixin and meloxicam administered locally to the scrotum before <span class="hlt">ring</span> castration. Randomised, controlled, prospective study. Forty eight single born male Merino lambs. Lambs, aged approximately 4 weeks, were allocated to four groups for castration. Groups were: sham control; castration + saline; castration + flunixin; castration + meloxicam. Drugs (5 mL) were administered subcutaneously around the circumference of the scrotum immediately before castration. Cortisol, rectal temperature, haematology and plasma haptoglobin were measured before and up to 48 hours after treatment. Behaviour recorded by video for 12 hours after treatment was classified as pain avoidance behaviours in the first hour and postural behaviours in three 4 hour intervals. <span class="hlt">Ring</span> castration (saline group) induced a bi-phasic increase in cortisol with peaks at 90 minutes and 24 hours but no significant changes in haematology, haptoglobin or rectal temperature. Pain avoidance behaviours were increased and teat seeking decreased. Normal lying and normal standing postures were decreased and abnormal ventral lying, statue standing, abnormal standing and total abnormal postures increased. Flunixin decreased cortisol at 90 minutes (60.3 versus 117.3 nmol L(-1) ) and cortisol AUC (0-6 hours), decreased elevated leg movement (2.5 versus 5.4 <span class="hlt">events</span>) and sum of pain avoidance behaviours (8.5 versus 16.7 <span class="hlt">events</span>), improved time spent in normal ventral lying and decreased abnormal ventral lying and total abnormal postures compared to saline treated lambs. In a similar contrast, meloxicam caused non-significant decreases in cortisol at 90 minutes, cortisol AUC (0-6 hours) and pain avoidance behaviours, and significantly improved the postural behaviours normal ventral lying (26.7 versus 15.4%) and normal standing (13.9 versus 7.5%), and reduced abnormal standing and total abnormal postures. Physiological and behavioural responses associated with <span class="hlt">ring</span> castration</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28372978','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28372978"><span>Residual hormone levels in used contraceptive <span class="hlt">rings</span> as a measurement of adherence to vaginal <span class="hlt">ring</span> use.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Haaland, Richard E; Holder, Angela; Evans-Strickfaden, Tammy; Nyagol, Beatrice; Makanga, Mumbi; Oyaro, Boaz; Humwa, Felix; Williams, Tiffany; McLellan-Lemal, Eleanor; Desai, Mitesh; Huey, Michael J</p> <p>2017-06-01</p> <p>This study sought to measure residual contraceptive hormone levels in vaginal <span class="hlt">rings</span> as an adherence marker for monitoring product use in clinical trials. Residual etonogestrel and ethinyl estradiol levels from used Nuva<span class="hlt">Rings</span>® of 26 self-reported adherent women enrolled in a clinical trial of vaginal <span class="hlt">ring</span> acceptability were compared to those from 16 women who used Nuva<span class="hlt">Ring</span>® as their contraceptive choice. Twenty-one (81%) clinical trial <span class="hlt">rings</span> had contraceptive hormone levels within the range of those used as a contraceptive choice. Five returned <span class="hlt">rings</span> had unused or discordant levels of residual contraceptive hormones. Residual vaginal <span class="hlt">ring</span> drug levels could help assess adherence in clinical trials. Published by Elsevier Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.S51B2782Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.S51B2782Z"><span>Automated Sensor Tuning for Seismic <span class="hlt">Event</span> Detection at a Carbon Capture, Utilization, and <span class="hlt">Storage</span> Site, Farnsworth Unit, Ochiltree County, Texas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ziegler, A.; Balch, R. S.; Knox, H. A.; Van Wijk, J. W.; Draelos, T.; Peterson, M. G.</p> <p>2016-12-01</p> <p>We present results (e.g. seismic detections and STA/LTA detection parameters) from a continuous downhole seismic array in the Farnsworth Field, an oil field in Northern Texas that hosts an ongoing carbon capture, utilization, and <span class="hlt">storage</span> project. Specifically, we evaluate data from a passive vertical monitoring array consisting of 16 levels of 3-component 15Hz geophones installed in the field and continuously recording since January 2014. This detection database is directly compared to ancillary data (i.e. wellbore pressure) to determine if there is any relationship between seismic observables and CO2 injection and pressure maintenance in the field. Of particular interest is detection of relatively low-amplitude signals constituting long-period long-duration (LPLD) <span class="hlt">events</span> that may be associated with slow shear-slip analogous to low frequency tectonic tremor. While this category of seismic <span class="hlt">event</span> provides great insight into dynamic behavior of the pressurized subsurface, it is inherently difficult to detect. To automatically detect seismic <span class="hlt">events</span> using effective data processing parameters, an automated sensor tuning (AST) algorithm developed by Sandia National Laboratories is being utilized. AST exploits ideas from neuro-dynamic programming (reinforcement learning) to automatically self-tune and determine optimal detection parameter settings. AST adapts in near real-time to changing conditions and automatically self-tune a signal detector to identify (detect) only signals from <span class="hlt">events</span> of interest, leading to a reduction in the number of missed legitimate <span class="hlt">event</span> detections and the number of false <span class="hlt">event</span> detections. Funding for this project is provided by the U.S. Department of Energy's (DOE) National Energy Technology Laboratory (NETL) through the Southwest Regional Partnership on Carbon Sequestration (SWP) under Award No. DE-FC26-05NT42591. Additional support has been provided by site operator Chaparral Energy, L.L.C. and Schlumberger Carbon Services. Sandia National</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27699551','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27699551"><span>Improving the hydrogen <span class="hlt">storage</span> properties of metal-organic framework by functionalization.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xia, Liangzhi; Liu, Qing; Wang, Fengling; Lu, Jinming</p> <p>2016-10-01</p> <p>Based on the structure of MOF-808, different substituents were introduced to replace hydrogen atom on the phenyl <span class="hlt">ring</span> of MOF-808. The GCMC method was used to study the effect of functional groups on the hydrogen <span class="hlt">storage</span> properties of MOF-808-X (X = -OH, -NO 2 , -CH 3 , -CN, -I). The H 2 uptakes and isosteric heat of adsorption were simulated at 77 K. The results indicate that all these substituents have favorable impact on the hydrogen <span class="hlt">storage</span> capacity, and -CN is found to be the most promising substituent to improve H 2 uptake. These results may be helpful for the design of MOFs with higher hydrogen <span class="hlt">storage</span> capacity. Graphical abstract Atomistic structures of MOFs. (a) The structures of MOF-808-X. (b) Model of organic linker. Atom color scheme: C, gray; H, white; O, red; X, palegreen (X = -OH, -NO 2 , -CH 3 , -CN, -I).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28687675','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28687675"><span>Two dynamin-like proteins stabilize FtsZ <span class="hlt">rings</span> during Streptomyces sporulation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schlimpert, Susan; Wasserstrom, Sebastian; Chandra, Govind; Bibb, Maureen J; Findlay, Kim C; Flärdh, Klas; Buttner, Mark J</p> <p>2017-07-25</p> <p>During sporulation, the filamentous bacteria Streptomyces undergo a massive cell division <span class="hlt">event</span> in which the synthesis of ladders of sporulation septa convert multigenomic hyphae into chains of unigenomic spores. This process requires cytokinetic Z-<span class="hlt">rings</span> formed by the bacterial tubulin homolog FtsZ, and the stabilization of the newly formed Z-<span class="hlt">rings</span> is crucial for completion of septum synthesis. Here we show that two dynamin-like proteins, DynA and DynB, play critical roles in this process. Dynamins are a family of large, multidomain GTPases involved in key cellular processes in eukaryotes, including vesicle trafficking and organelle division. Many bacterial genomes encode dynamin-like proteins, but the biological function of these proteins has remained largely enigmatic. Using a cell biological approach, we show that the two Streptomyces dynamins specifically localize to sporulation septa in an FtsZ-dependent manner. Moreover, dynamin mutants have a cell division defect due to the decreased stability of sporulation-specific Z-<span class="hlt">rings</span>, as demonstrated by kymographs derived from time-lapse images of FtsZ ladder formation. This defect causes the premature disassembly of individual Z-<span class="hlt">rings</span>, leading to the frequent abortion of septum synthesis, which in turn results in the production of long spore-like compartments with multiple chromosomes. Two-hybrid analysis revealed that the dynamins are part of the cell division machinery and that they mediate their effects on Z-<span class="hlt">ring</span> stability during developmentally controlled cell division via a network of protein-protein interactions involving DynA, DynB, FtsZ, SepF, SepF2, and the FtsZ-positioning protein SsgB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130009065','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130009065"><span>Destructive Single-<span class="hlt">Event</span> Failures in Diodes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Casey, Megan C.; Gigliuto, Robert A.; Lauenstein, Jean-Marie; Wilcox, Edward P.; Kim, Hak; Chen, Dakai; Phan, Anthony M.; LaBel, Kenneth A.</p> <p>2013-01-01</p> <p>In this summary, we have shown that diodes are susceptible to destructive single-<span class="hlt">event</span> effects, and that these failures occur along the guard <span class="hlt">ring</span>. By determining the last passing voltages, a safe operating area can be derived. By derating off of those values, rather than by the rated voltage, like what is currently done with power MOSFETs, we can work to ensure the safety of future missions. However, there are still open questions about these failures. Are they limited to a single manufacturer, a small number, or all of them? Is there a threshold rated voltage that must be exceeded to see these failures? With future work, we hope to answer these questions. In the full paper, laser results will also be presented to verify that failures only occur along the guard <span class="hlt">ring</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_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('https://www.osti.gov/servlets/purl/872462','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/872462"><span>Concentric <span class="hlt">ring</span> flywheel without expansion separators</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Kuklo, Thomas C.</p> <p>1999-01-01</p> <p>A concentric <span class="hlt">ring</span> flywheel wherein the adjacent <span class="hlt">rings</span> are configured to eliminate the need for differential expansion separators between the adjacent <span class="hlt">rings</span>. This is accomplished by forming a circumferential step on an outer surface of an inner concentric <span class="hlt">ring</span> and forming a matching circumferential step on the inner surface of an adjacent outer concentric <span class="hlt">ring</span>. During operation the circumferential steps allow the <span class="hlt">rings</span> to differentially expand due to the difference in the radius of the <span class="hlt">rings</span> without the formation of gaps therebetween, thereby eliminating the need for expansion separators to take up the gaps formed by differential expansion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MNRAS.471.4027B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MNRAS.471.4027B"><span>Galactic <span class="hlt">rings</span> revisited - I. CVRHS classifications of 3962 <span class="hlt">ringed</span> galaxies from the Galaxy Zoo 2 Database</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buta, Ronald J.</p> <p>2017-11-01</p> <p><span class="hlt">Rings</span> are important and characteristic features of disc-shaped galaxies. This paper is the first in a series that re-visits galactic <span class="hlt">rings</span> with the goals of further understanding the nature of the features and for examining their role in the secular evolution of galaxy structure. The series begins with a new sample of 3962 galaxies drawn from the Galaxy Zoo 2 citizen science data base, selected because zoo volunteers recognized a <span class="hlt">ring</span>-shaped pattern in the morphology as seen in Sloan Digital Sky Survey colour images. The galaxies are classified within the framework of the Comprehensive de Vaucouleurs revised Hubble-Sandage system. It is found that zoo volunteers cued on the same kinds of <span class="hlt">ring</span>-like features that were recognized in the 1995 Catalogue of Southern <span class="hlt">Ringed</span> Galaxies. This paper presents the full catalogue of morphological classifications, comparisons with other sources of classifications and some histograms designed mainly to highlight the content of the catalogue. The advantages of the sample are its large size and the generally good quality of the images; the main disadvantage is the low physical resolution that limits the detectability of linearly small <span class="hlt">rings</span> such as nuclear <span class="hlt">rings</span>. The catalogue includes mainly inner and outer disc <span class="hlt">rings</span> and lenses. Cataclysmic (`encounter-driven') <span class="hlt">rings</span> (such as <span class="hlt">ring</span> and polar <span class="hlt">ring</span> galaxies) are recognized in less than 1 per cent of the sample.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110011701','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110011701"><span>Modeling the Inner Magnetosphere: Radiation Belts, <span class="hlt">Ring</span> Current, and Composition</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Glocer, Alex</p> <p>2011-01-01</p> <p>The space environment is a complex system defined by regions of differing length scales, characteristic energies, and physical processes. It is often difficult, or impossible, to treat all aspects of the space environment relative to a particular problem with a single model. In our studies, we utilize several models working in tandem to examine this highly interconnected system. The methodology and results will be presented for three focused topics: 1) Rapid radiation belt electron enhancements, 2) <span class="hlt">Ring</span> current study of Energetic Neutral Atoms (ENAs), Dst, and plasma composition, and 3) Examination of the outflow of ionospheric ions. In the first study, we use a coupled MHD magnetosphere - kinetic radiation belt model to explain recent Akebono/RDM observations of greater than 2.5 MeV radiation belt electron enhancements occurring on timescales of less than a few hours. In the second study, we present initial results of a <span class="hlt">ring</span> current study using a newly coupled kinetic <span class="hlt">ring</span> current model with an MHD magnetosphere model. Results of a dst study for four geomagnetic <span class="hlt">events</span> are shown. Moreover, direct comparison with TWINS ENA images are used to infer the role that composition plays in the <span class="hlt">ring</span> current. In the final study, we directly model the transport of plasma from the ionosphere to the magnetosphere. We especially focus on the role of photoelectrons and and wave-particle interactions. The modeling methodology for each of these studies will be detailed along with the results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MARS40001V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MARS40001V"><span>Rheology modification with <span class="hlt">ring</span> polymers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vlassopoulos, Dimitris</p> <p></p> <p>It is now established that experimental unconcatenated <span class="hlt">ring</span> polymers can be purified effectively by means of fractionation at the critical condition. For molecular weights well above the entanglement threshold, purified <span class="hlt">rings</span> relax stress via power-law (with an exponent of about -0.4), sharply departing from their linear counterparts. Experimental results are in harmony with modeling predictions and simulations. Here, we present results from recent interdisciplinary efforts and discuss two challenges: (i) the nonlinear shear rheology of purified <span class="hlt">ring</span> melts is also very different from that of unlinked chains. Whereas the latter exhibit features that can be explained, to a first approach, in the framework in the tube model, the former behave akin to unentangled chains with finite extensibility and exhibit much small deformation at steady state. (ii) blends of <span class="hlt">rings</span> and linear polymers exhibit unique features in different regimes: The addition of minute amounts of linear chains drastically affects <span class="hlt">ring</span> dynamics. This relates to <span class="hlt">ring</span> purity and the ability of unlinked linear chains to thread <span class="hlt">rings</span>. With the help of simulations, it is possible to rationalize the observed surprisingly slow viscoelastic relaxation, which is attributed to <span class="hlt">ring</span>-linear and <span class="hlt">ring-ring</span> penetrations. On the other hand, adding small amounts of <span class="hlt">rings</span> to linear polymers of different molecular weights influences their linear and nonlinear rheology in an unprecedented way. The blend viscosity exceeds that of the slower component (linear) in this non-interacting mixture, and its dependencies on composition and molecular weight ratio are examined, whereas the role of molecular architecture is also addressed. Consequently, closing the ends of a linear chain can serve as a powerful means for molecular manipulation of its rheology. This presentation reflects collaborative efforts with S. Costanzo, Z-C. Yan, R. Pasquino, M. Kaliva, S. Kamble, Y. Jeong, P. Lutz, J. Allgaier, T. Chang, D. Talikis, V</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11226339','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11226339"><span>One <span class="hlt">ring</span> or two? Determination of <span class="hlt">ring</span> number in carotenoids by lycopene epsilon-cyclases.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cunningham, F X; Gantt, E</p> <p>2001-02-27</p> <p>Carotenoids in the photosynthetic membranes of plants typically contain two beta-<span class="hlt">rings</span> (e.g., beta-carotene and zeaxanthin) or one epsilon- and one beta-<span class="hlt">ring</span> (e.g., lutein). Carotenoids with two epsilon-<span class="hlt">rings</span> are uncommon. We reported earlier that the Arabidopsis thaliana lycopene epsilon-cyclase (LCYe) adds one epsilon-<span class="hlt">ring</span> to the symmetrical linear substrate lycopene, whereas the structurally related lycopene beta-cyclase (LCYb) adds two beta-<span class="hlt">rings</span>. Here we describe a cDNA encoding LCYe in romaine lettuce (Lactuca sativa var. romaine), one of the few plant species known to accumulate substantial quantities of a carotenoid with two epsilon-<span class="hlt">rings</span>: lactucaxanthin. The product of the lettuce cDNA, similar in sequence to the Arabidopsis LCYe (77% amino acid identity), efficiently converted lycopene into the bicyclic epsilon-carotene in a heterologous Escherichia coli system. Regions of the lettuce and Arabidopsis epsilon-cyclases involved in the determination of <span class="hlt">ring</span> number were mapped by analysis of chimeric epsilon-cyclases constructed by using an inverse PCR approach. A single amino acid was found to act as a molecular switch: lettuce LCYe mutant H457L added only one epsilon-<span class="hlt">ring</span> to lycopene, whereas the complementary Arabidopsis LCYe mutant, L448H, added two epsilon-<span class="hlt">rings</span>. An R residue in this position also yields a bi-epsilon-cyclase for both the lettuce and Arabidopsis enzymes. Construction and analysis of chimera of related enzymes with differing catalytic activities provide an informative approach that may be of particular utility for studying membrane-associated enzymes that cannot easily be crystallized or modeled to existing crystal structures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=30238','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=30238"><span>One <span class="hlt">ring</span> or two? Determination of <span class="hlt">ring</span> number in carotenoids by lycopene ɛ-cyclases</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Cunningham, Francis X.; Gantt, Elisabeth</p> <p>2001-01-01</p> <p>Carotenoids in the photosynthetic membranes of plants typically contain two β-<span class="hlt">rings</span> (e.g., β-carotene and zeaxanthin) or one ɛ- and one β-<span class="hlt">ring</span> (e.g., lutein). Carotenoids with two ɛ-<span class="hlt">rings</span> are uncommon. We reported earlier that the Arabidopsis thaliana lycopene ɛ-cyclase (LCYe) adds one ɛ-<span class="hlt">ring</span> to the symmetrical linear substrate lycopene, whereas the structurally related lycopene β-cyclase (LCYb) adds two β-<span class="hlt">rings</span>. Here we describe a cDNA encoding LCYe in romaine lettuce (Lactuca sativa var. romaine), one of the few plant species known to accumulate substantial quantities of a carotenoid with two ɛ-<span class="hlt">rings</span>: lactucaxanthin. The product of the lettuce cDNA, similar in sequence to the Arabidopsis LCYe (77% amino acid identity), efficiently converted lycopene into the bicyclic ɛ-carotene in a heterologous Escherichia coli system. Regions of the lettuce and Arabidopsis ɛ-cyclases involved in the determination of <span class="hlt">ring</span> number were mapped by analysis of chimeric ɛ-cyclases constructed by using an inverse PCR approach. A single amino acid was found to act as a molecular switch: lettuce LCYe mutant H457L added only one ɛ-<span class="hlt">ring</span> to lycopene, whereas the complementary Arabidopsis LCYe mutant, L448H, added two ɛ-<span class="hlt">rings</span>. An R residue in this position also yields a bi-ɛ-cyclase for both the lettuce and Arabidopsis enzymes. Construction and analysis of chimera of related enzymes with differing catalytic activities provide an informative approach that may be of particular utility for studying membrane-associated enzymes that cannot easily be crystallized or modeled to existing crystal structures. PMID:11226339</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018DDA....4910004C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018DDA....4910004C"><span>The structure of Jupiter’s main <span class="hlt">ring</span> from New Horizons: A comparison with other <span class="hlt">ring</span>-moon systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chancia, Robert; Hedman, Matthew</p> <p>2018-04-01</p> <p>During New Horizon’s Jupiter flyby in 2007, the Long-Range Reconnaissance Imager (LORRI) took several images of the planet’s main <span class="hlt">ring</span>. The data set contains two extended image-movies of the main <span class="hlt">ring</span>, along with several brief observations at varying <span class="hlt">ring</span> azimuths, and a small set of high phase angle images. Thus far, the only published work on the New Horizons Jupiter <span class="hlt">rings</span> data set found seven bright clumps with sub-km equivalent radii embedded in the main <span class="hlt">ring</span> (Showalter et al. 2007 Science). In this work, we searched the inner region of the main <span class="hlt">ring</span> for any structures that might be perturbed at the 3:2 resonances with the rotation of Jupiter’s magnetic field or massive storms. We also examined the structure of the outer main <span class="hlt">ring</span> in order to assess how it is shaped by the small moons Metis and Adrastea. Some of the features seen in Jupiter’s main <span class="hlt">ring</span> are similar to those found in other dusty <span class="hlt">rings</span> around Saturn, Uranus, and Neptune. By comparing these different <span class="hlt">rings</span>, we can gain a better understanding of how small moons sculpt tenuous <span class="hlt">rings</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRA..122.7891M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRA..122.7891M"><span>Proton velocity <span class="hlt">ring</span>-driven instabilities and their dependence on the <span class="hlt">ring</span> speed: Linear theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Min, Kyungguk; Liu, Kaijun; Gary, S. Peter</p> <p>2017-08-01</p> <p>Linear dispersion theory is used to study the Alfvén-cyclotron, mirror and ion Bernstein instabilities driven by a tenuous (1%) warm proton <span class="hlt">ring</span> velocity distribution with a <span class="hlt">ring</span> speed, vr, varying between 2vA and 10vA, where vA is the Alfvén speed. Relatively cool background protons and electrons are assumed. The modeled <span class="hlt">ring</span> velocity distributions are unstable to both the Alfvén-cyclotron and ion Bernstein instabilities whose maximum growth rates are roughly a linear function of the <span class="hlt">ring</span> speed. The mirror mode, which has real frequency ωr=0, becomes the fastest growing mode for sufficiently large vr/vA. The mirror and Bernstein instabilities have maximum growth at propagation oblique to the background magnetic field and become more field-aligned with an increasing <span class="hlt">ring</span> speed. Considering its largest growth rate, the mirror mode, in addition to the Alfvén-cyclotron mode, can cause pitch angle diffusion of the <span class="hlt">ring</span> protons when the <span class="hlt">ring</span> speed becomes sufficiently large. Moreover, because the parallel phase speed, v∥ph, becomes sufficiently small relative to vr, the low-frequency Bernstein waves can also aid the pitch angle scattering of the <span class="hlt">ring</span> protons for large vr. Potential implications of including these two instabilities at oblique propagation on heliospheric pickup ion dynamics are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA01272&hterms=Invisible+web&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DInvisible%2Bweb','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA01272&hterms=Invisible+web&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DInvisible%2Bweb"><span>Edge-on View of Saturn's <span class="hlt">Rings</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>1996-01-01</p> <p>TOP - This is a NASA Hubble Space Telescope snapshot of Saturn with its <span class="hlt">rings</span> barely visible. Normally, astronomers see Saturn with its <span class="hlt">rings</span> tilted. Earth was almost in the plane of Saturn's <span class="hlt">rings</span>, thus the <span class="hlt">rings</span> appear edge-on.<p/>In this view, Saturn's largest moon, Titan, is casting a shadow on Saturn. Titan's atmosphere is a dark brown haze. The other moons appear white because of their bright, icy surfaces. Four moons - from left to right, Mimas, Tethys, Janus, and Enceladus - are clustered around the edge of Saturn's <span class="hlt">rings</span> on the right. Two other moons appear in front of the <span class="hlt">ring</span> plane. Prometheus is on the right edge; Pandora, on the left. The <span class="hlt">rings</span> also are casting a shadow on Saturn because the Sun was above the <span class="hlt">ring</span> plane.<p/>BOTTOM - This photograph shows Saturn with its <span class="hlt">rings</span> slightly tilted. The moon called Dione, on the lower right, is casting a long, thin shadow across the whole <span class="hlt">ring</span> system due to the setting Sun on the <span class="hlt">ring</span> plane. The moon on the upper left of Saturn is Tethys.<p/>Astronomers also are studying the unusual appearance of Saturn's <span class="hlt">rings</span>. The bottom image displays a faint, narrow <span class="hlt">ring</span>, the F-<span class="hlt">ring</span> just outside the main <span class="hlt">ring</span>, which normally is invisible from Earth. Close to the edge of Saturn's disk, the front section of <span class="hlt">rings</span> seem brighter and more yellow than the back due to the additional lumination by yellowish Saturn.<p/>The color images were assembled from separate exposures taken August 6 (top) and November 17 (bottom), 1995 with the Wide Field Planetary Camera-2.<p/>The Wide Field/Planetary Camera 2 was developed by the Jet Propulsion Laboratory and managed by the Goddard Spaced Flight Center for NASA's Office of Space Science.<p/>This image and other images and data received from the Hubble Space Telescope are posted on the World Wide Web on the Space Telescope Science Institute home page at URL http://oposite.stsci.edu/pubinfo/</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020029906','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020029906"><span>Apse-Alignment of the Uranian <span class="hlt">Rings</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mosqueira, I.; Estrada, P. R.</p> <p>2000-01-01</p> <p>An explanation of the dynamical mechanism for apse-alignment of the eccentric Uranian <span class="hlt">rings</span> is necessary before observations can be used to determine properties such as <span class="hlt">ring</span> masses, particle sizes, and elasticities. The leading model relies on the <span class="hlt">ring</span> self-gravity to accomplish this task, yet it yields equilibrium masses which are not in accord with Voyager radio measurements. We explore possible solutions such that the self-gravity and the collisional terms are both involved in the process of apse-alignment. We consider limits that correspond to a hot and a cold <span class="hlt">ring</span>, and show that pressure terms may play a significant role in the equilibrium conditions for the narrow Uranian <span class="hlt">rings</span>. In the cold <span class="hlt">ring</span> case, where the scale height of the <span class="hlt">ring</span> near periapse is comparable to the <span class="hlt">ring</span> particle size, we introduce a new pressure correction pertaining to a region of the <span class="hlt">ring</span> where the particles are locked in their relative positions and jammed against their neighbors, and the velocity dispersion is so low that the collisions are nearly elastic. In this case, we find a solution such that the <span class="hlt">ring</span> self-gravity maintains apse-alignment against both differential precession (m = 1 mode) and the fluid pressure. We apply this model to the Uranian alpha <span class="hlt">ring</span>, and show that, compared to the previous self-gravity model, the mass estimate for this <span class="hlt">ring</span> increases by an order of magnitude. In the case of a hot <span class="hlt">ring</span>, where the scale height can reach a value as much as fifty times larger than a particle size, we find velocity dispersion profiles that result in pressure forces which act in such a way as to alter the <span class="hlt">ring</span> equilibrium conditions, again leading to a <span class="hlt">ring</span> mass increase of an order of magnitude; however, such a velocity dispersion profile would require a different mechanism than is currently envisioned for establishing heating/cooling balance in a finite-sized, inelastic particle <span class="hlt">ring</span>. Finally, we introduce an important correction to the model of Chiang and Goldreich.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...837L..13M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...837L..13M"><span>Simulating the Smallest <span class="hlt">Ring</span> World of Chariklo</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Michikoshi, Shugo; Kokubo, Eiichiro</p> <p>2017-03-01</p> <p>A <span class="hlt">ring</span> system consisting of two dense narrow <span class="hlt">rings</span> has been discovered around Centaur Chariklo. The existence of these <span class="hlt">rings</span> around a small object poses various questions about their origin, stability, and lifetime. In order to understand the nature of Chariklo’s <span class="hlt">rings</span>, we perform global N-body simulations of the self-gravitating collisional particle <span class="hlt">rings</span> for the first time. We find that Chariklo should be denser than the <span class="hlt">ring</span> material in order to avoid the rapid diffusion of the <span class="hlt">rings</span>. If Chariklo is denser than the <span class="hlt">ring</span> material, fine spiral structures called self-gravity wakes occur in the inner <span class="hlt">ring</span>. These wakes accelerate the viscous spreading of the <span class="hlt">ring</span> significantly and typically occur on timescales of about 100 {years} for m-sized <span class="hlt">ring</span> particles, which is considerably shorter than the timescales suggested in previous studies. The existence of these narrow <span class="hlt">rings</span> implies smaller <span class="hlt">ring</span> particles or the existence of shepherding satellites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20100021385&hterms=Plasma+Ring&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DPlasma%2BRing','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20100021385&hterms=Plasma+Ring&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DPlasma%2BRing"><span>Recent Simulation Results on <span class="hlt">Ring</span> Current Dynamics Using the Comprehensive <span class="hlt">Ring</span> Current Model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Zheng, Yihua; Zaharia, Sorin G.; Lui, Anthony T. Y.; Fok, Mei-Ching</p> <p>2010-01-01</p> <p>Plasma sheet conditions and electromagnetic field configurations are both crucial in determining <span class="hlt">ring</span> current evolution and connection to the ionosphere. In this presentation, we investigate how different conditions of plasma sheet distribution affect <span class="hlt">ring</span> current properties. Results include comparative studies in 1) varying the radial distance of the plasma sheet boundary; 2) varying local time distribution of the source population; 3) varying the source spectra. Our results show that a source located farther away leads to a stronger <span class="hlt">ring</span> current than a source that is closer to the Earth. Local time distribution of the source plays an important role in determining both the radial and azimuthal (local time) location of the <span class="hlt">ring</span> current peak pressure. We found that post-midnight source locations generally lead to a stronger <span class="hlt">ring</span> current. This finding is in agreement with Lavraud et al.. However, our results do not exhibit any simple dependence of the local time distribution of the peak <span class="hlt">ring</span> current (within the lower energy range) on the local time distribution of the source, as suggested by Lavraud et al. [2008]. In addition, we will show how different specifications of the magnetic field in the simulation domain affect <span class="hlt">ring</span> current dynamics in reference to the 20 November 2007 storm, which include initial results on coupling the CRCM with a three-dimensional (3-D) plasma force balance code to achieve self-consistency in the magnetic field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999APS..DFD..JG05E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999APS..DFD..JG05E"><span>Compressible Vortex <span class="hlt">Ring</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Elavarasan, Ramasamy; Arakeri, Jayawant; Krothapalli, Anjaneyulu</p> <p>1999-11-01</p> <p>The interaction of a high-speed vortex <span class="hlt">ring</span> with a shock wave is one of the fundamental issues as it is a source of sound in supersonic jets. The complex flow field induced by the vortex alters the propagation of the shock wave greatly. In order to understand the process, a compressible vortex <span class="hlt">ring</span> is studied in detail using Particle Image Velocimetry (PIV) and shadowgraphic techniques. The high-speed vortex <span class="hlt">ring</span> is generated from a shock tube and the shock wave, which precedes the vortex, is reflected back by a plate and made to interact with the vortex. The shadowgraph images indicate that the reflected shock front is influenced by the non-uniform flow induced by the vortex and is decelerated while passing through the vortex. It appears that after the interaction the shock is "split" into two. The PIV measurements provided clear picture about the evolution of the vortex at different time interval. The centerline velocity traces show the maximum velocity to be around 350 m/s. The velocity field, unlike in incompressible <span class="hlt">rings</span>, contains contributions from both the shock and the vortex <span class="hlt">ring</span>. The velocity distribution across the vortex core, core diameter and circulation are also calculated from the PIV data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhFl...29j3604H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhFl...29j3604H"><span>Symmetrical collision of multiple vortex <span class="hlt">rings</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hernández, R. H.; Reyes, T.</p> <p>2017-10-01</p> <p>In this work, we investigate the motion, interaction, and simultaneous collision between many initially stable vortex <span class="hlt">rings</span> arranged symmetrically in two initial configurations, three and six <span class="hlt">rings</span> making an angle of 60 and 120° between their straight path lines, respectively. We report results for laminar vortex <span class="hlt">rings</span> in air obtained through numerical simulations of the <span class="hlt">ring</span> velocity, pressure, and vorticity fields, both in free flight and during the entire collision. Each collision was studied for small Reynolds numbers R e <1 03 based on both the self-induced velocity and diameter of the <span class="hlt">ring</span>. The case of three <span class="hlt">rings</span> produces secondary vortical structures formed by laterally expanding dipolar arms with top and bottom secondary vortex <span class="hlt">rings</span>. The case of six colliding <span class="hlt">rings</span> produces, as secondary structures, two big <span class="hlt">rings</span> moving in opposite directions, a process that reminds us of the head-on collision of two <span class="hlt">rings</span> [T. T. Lim and T. B. Nickels, "Instability and reconnection in the head-on collision of two vortex <span class="hlt">rings</span>," Nature 357, 225-227 (1992)] under a hypothetical time reversal transformation. Both collisions display a characteristic kinetic energy evolution where mean collision stages can be identified within the range of Reynolds numbers investigated here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JPhCS.664f2065C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JPhCS.664f2065C"><span>The ATLAS <span class="hlt">Event</span> Service: A new approach to <span class="hlt">event</span> processing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calafiura, P.; De, K.; Guan, W.; Maeno, T.; Nilsson, P.; Oleynik, D.; Panitkin, S.; Tsulaia, V.; Van Gemmeren, P.; Wenaus, T.</p> <p>2015-12-01</p> <p>The ATLAS <span class="hlt">Event</span> Service (ES) implements a new fine grained approach to HEP <span class="hlt">event</span> processing, designed to be agile and efficient in exploiting transient, short-lived resources such as HPC hole-filling, spot market commercial clouds, and volunteer computing. Input and output control and data flows, bookkeeping, monitoring, and data <span class="hlt">storage</span> are all managed at the <span class="hlt">event</span> level in an implementation capable of supporting ATLAS-scale distributed processing throughputs (about 4M CPU-hours/day). Input data flows utilize remote data repositories with no data locality or pre-staging requirements, minimizing the use of costly <span class="hlt">storage</span> in favor of strongly leveraging powerful networks. Object stores provide a highly scalable means of remotely storing the quasi-continuous, fine grained outputs that give ES based applications a very light data footprint on a processing resource, and ensure negligible losses should the resource suddenly vanish. We will describe the motivations for the ES system, its unique features and capabilities, its architecture and the highly scalable tools and technologies employed in its implementation, and its applications in ATLAS processing on HPCs, commercial cloud resources, volunteer computing, and grid resources. Notice: This manuscript has been authored by employees of Brookhaven Science Associates, LLC under Contract No. DE-AC02-98CH10886 with the U.S. Department of Energy. The publisher by accepting the manuscript for publication acknowledges that the United States Government retains a non-exclusive, paid-up, irrevocable, world-wide license to publish or reproduce the published form of this manuscript, or allow others to do so, for United States Government purposes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/14590','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/14590"><span>The temporal distribution and carbon <span class="hlt">storage</span> of large oak wood in streams and floodplain deposits</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Richard P. Guyette; Daniel C. Dey; Michael C. Stambaugh</p> <p>2008-01-01</p> <p>We used tree-<span class="hlt">ring</span> dating and 14C dating to document the temporal distribution and carbon <span class="hlt">storage</span> of oak (Quercus spp.) wood in trees recruited and buried by streams and floodplains in northern Missouri, USA. Frequency distributions indicated that oak wood has been accumulating in Midwest streams continually since at least the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18377034','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18377034"><span>A pulse-compression-<span class="hlt">ring</span> circuit for high-efficiency electric propulsion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Owens, Thomas L</p> <p>2008-03-01</p> <p>A highly efficient, highly reliable pulsed-power system has been developed for use in high power, repetitively pulsed inductive plasma thrusters. The pulsed inductive thruster ejects plasma propellant at a high velocity using a Lorentz force developed through inductive coupling to the plasma. Having greatly increased propellant-utilization efficiency compared to chemical rockets, this type of electric propulsion system may one day propel spacecraft on long-duration deep-space missions. High system reliability and electrical efficiency are extremely important for these extended missions. In the prototype pulsed-power system described here, exceptional reliability is achieved using a pulse-compression circuit driven by both active solid-state switching and passive magnetic switching. High efficiency is achieved using a novel <span class="hlt">ring</span> architecture that recovers unused energy in a pulse-compression system with minimal circuit loss after each impulse. As an added benefit, voltage reversal is eliminated in the <span class="hlt">ring</span> topology, resulting in long lifetimes for energy-<span class="hlt">storage</span> capacitors. System tests were performed using an adjustable inductive load at a voltage level of 3.3 kV, a peak current of 20 kA, and a current switching rate of 15 kA/micros.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=tornado&id=EJ945886','ERIC'); return false;" href="https://eric.ed.gov/?q=tornado&id=EJ945886"><span>Smoke <span class="hlt">Ring</span> Physics</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>Huggins, Elisha</p> <p>2011-01-01</p> <p>The behavior of smoke <span class="hlt">rings</span>, tornados, and quantized vortex <span class="hlt">rings</span> in superfluid helium has many features in common. These features can be described by the same mathematics we use when introducing Ampere's law in an introductory physics course. We discuss these common features. (Contains 7 figures.)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900064398&hterms=midi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmidi','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900064398&hterms=midi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmidi"><span>Planetary <span class="hlt">rings</span> - Theory</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borderies, Nicole</p> <p>1989-01-01</p> <p>Theoretical models of planetary-<span class="hlt">ring</span> dynamics are examined in a brief analytical review. The mathematical description of streamlines and streamline interactions is outlined; the redistribution of angular momentum due to collisions between particles is explained; and problems in the modeling of broad, narrow, and arc <span class="hlt">rings</span> are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995PhDT.........5M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995PhDT.........5M"><span>The Dynamics of Dense Planetary <span class="hlt">Rings</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mosqueira, Ignacio</p> <p>1995-01-01</p> <p>We study the dynamics of a two-mode narrow <span class="hlt">ring</span> in the case that one of the modes dominates the overall <span class="hlt">ring</span> perturbation. We use a simple two-streamline self -gravity model, including viscosity, and shepherd satellites. As might be expected, we find that n m = 1 mode appears to be a natural end state for the <span class="hlt">rings</span>, inasmuch as the presence of a dominant eccentric mode inhibits the growth of other modes, but the reverse is not true. Why some <span class="hlt">rings</span> exhibit other m values only remains unexplained. Using a modified N-body code to include periodic boundary conditions in a perturbed shear flow, we investigate the role of viscosity on the dynamics of perturbed <span class="hlt">rings</span> with optical depth tau ~ 1. In particular, we are concerned with <span class="hlt">rings</span> such that qe = a{de over da} ne 0, where a is the semi-major axis and e is the eccentricity. We confirm the possibility that, for a sufficiently perturbed <span class="hlt">ring</span>, the angular momentum luminosity may reverse direction with respect to the unperturbed <span class="hlt">ring</span> (Borderies et al. 1983a). We use observationally constrained parameters for the delta and epsilon Uranian <span class="hlt">rings</span>, as well as the outer portion of Saturn's B <span class="hlt">ring</span>. We find that understanding the effects of viscosity for the Uranian <span class="hlt">rings</span> requires that both local and non-local transport terms be considered if the coefficient of restitution experimentally obtained by Bridges et al. (1984) is appropriate for <span class="hlt">ring</span> particles. We also find evidence that the criterion for viscous overstability is satisfied in the case of high optical depth <span class="hlt">rings</span>, as originally proposed by Borderies et al. (1985), making viscous overstability a leading candidate mechanism to explain the non-axisymmetric structure present in the outer portion of Saturn's B <span class="hlt">ring</span>. To better understand our path-code results we extend a non-local and incompressible fluid model used by Borderies et al. (1985) for dense <span class="hlt">rings</span>. We incorporate local and non-local transport terms as well as compressibility, while retaining the same number 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_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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