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2024GCN.38201....1I | We observed the field of GRB 241113A Siegel et al. GCN 38194 with the Sinistro instrument mounted on the 1m telescope of the LCO network located at Siding Spring Australia. Observations started on 2024 November 13 at 0955 UT 2.17 hr after the GRB trigger. We obtained a series of 3x180 s images in the SDSSr filter and o... | 2024-11-01T00:00:00Z | ['2024GCN.38201....1I'] | null | GRB 241113A LCO optical observations | 2,024 | 0 | 0 | ['PUB_HTML'] | 0 | null |
2016LPICo1980.4082S | The contamination control approach for life detection instrument is presented on the example of the Mars Organic Molecule Analyzer. A combined pyrolysis gas chromatograph mass spectrometer and laser desorption mass spectrometer. | 2016-10-01T00:00:00Z | ['2016LPICo1980.4082S'] | null | Mars Organic Molecule Analyzer MOMA as an Example for Contamination Control for Life Detection Instrumentation | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1960.5012M | Concentrations of hydrogenbearing volatiles are nonuniform within the large permanently shadowed regions PSR at the lunar south pole. Volatiles in the PSRs possibly water ice are biased towards the base of the polewardfacing slopes. | 2016-11-01T00:00:00Z | ['2016LPICo1960.5012M'] | null | High Concentrations of HydrogenBearing Volatiles at the Base of PolewardFacing Slopes in the Large Southern Permanently Shadowed Regions | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6481C | Here we report on an indepth mineralogical and geochemical study of low temperaturealtered deposits of the Ries impact ejecta relating them to Martian craterrelated pitted material. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6481C'] | null | Mineralogical and Geochemical Study of Ries Ejecta Deposits as a Martian Analogue for Impact Melt Modification | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6198F | Two of the latest Martian meteorites found in Antarctica paired olivinephyric shergottites LAR 12240 and LAR 12095 are described in order to decipher their petrological context and place constraints on the geological history of Mars. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6198F'] | null | Petrology and Geochemistry of New Paired Martian Meteorites Larkman Nunatak 12240 and Larkman Nunatak 12095 | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPICo1911.6094P | The Diviner Lunar Radiometer Experiment has mapped the lunar surface for almost seven years acquiring a dataset of unprecedented quality detail and coverage providing many new infrared views of the Moon and its history. | 2016-05-01T00:00:00Z | ['2016LPICo1911.6094P'] | null | New Infrared Views of the Moon from Diviner | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2876R | We present new structural data that show preservation of part of the overturned fold at Monturaqui Crater Chile. | 2016-03-01T00:00:00Z | ['2016LPI....47.2876R'] | null | A Preliminary Report on the Structure of Monturaqui Crater Chile | 2,016 | 0 | 0.16 | ['PUB_PDF'] | 0 | null |
2016LPICo1926.6001S | We investigate the importance of ice flow at the north pole of Mars for features only recently discovered by HiRISE. We use a combination of image analysis and finite element modeling to quantify flow and discuss implications for NPLD evolution. | 2016-09-01T00:00:00Z | ['2016LPICo1926.6001S'] | null | The Importance of Ice Flow at the North Pole of Mars | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPICo1962.4011S | We present the design and simulations of the realtime Scientific Trigger Unit of the gammaray codedmask imager ECLAIRs onboard the future mission SVOM which will localize GRBs and allow their followup observations by Xray and visible telescopes. | 2016-10-01T00:00:00Z | ['2016LPICo1962.4011S'] | null | The GammaRay Burst Trigger System onboard SVOMECLAIRs Design and Simulations | 2,016 | 0 | 0.18 | ['PUB_PDF'] | 0 | null |
2016LPICo1960.5005L | We discuss a lunar exploration architecture that addresses the strategic objective of providing access to the lunar surface. This access enables the most exciting part of the lunar exploration building a sustained infrastructure on the lunar surface. | 2016-11-01T00:00:00Z | ['2016LPICo1960.5005L'] | null | Building Strategic Capabilities for Sustained Lunar Exploration | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPICo1926.6006G | Impact crater analog Drills icy layers Active layer receding. | 2016-09-01T00:00:00Z | ['2016LPICo1926.6006G'] | null | Drilling Subsurface Ice at the Haughton Crater Analog Site | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2678A | We observed numerous minioutbursts by comet ChuryumovGerasimenko. Many aspects are similar to but better studied than the minioutbursts from Tempel 1. | 2016-03-01T00:00:00Z | ['2016LPI....47.2678A'] | null | MiniOutbursts in Comets ChuryumovGerasimenko and Tempel 1 | 2,016 | 0 | 0.2 | ['PUB_PDF'] | 2 | null |
2016LPICo1921.6473V | STXM Feoxidation state study in Acfer 094 and MIL 07687 matrix revealed high Fe3Fe ratios likely to be a primordial signature. Terrestrial weathering cannot be ruled out but is unlikely to have a pervasive effect throughout entire meteorites. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6473V'] | null | Iron Oxidation States of Matrix in Carbonaceous Chondrites Acfer 094 and MIL 07687 | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2024Ap&SS.369....7S | The turbulent solar wind magnetic field shows structures that are characterized by sudden strong changes in the field magnitude andor direction. Such structures can be intermittent if their increments found from time series spacecraft measurements deviate from a Gaussian distribution. Current sheets are a possible sour... | 2024-01-01T00:00:00Z | ['2024Ap&SS.369....7S', '10.1007/s10509-024-04266-x'] | null | Identifying kinetic scale magnetic discontinuity structures in turbulent solar wind | 2,024 | 0 | 0.26 | ['PUB_HTML'] | 0 | null |
2024Ap&SS.369....6L | Astrophysical very high energy VHE gammarays with energies gt30 GeV are believed to result almost exclusively from the interactions of populations of highly relativistic particles with ambient matter or photon fields. The study of these VHE photons therefore allows us to examine the processes of particle acceleration i... | 2024-01-01T00:00:00Z | ['2024Ap&SS.369....6L', '10.1007/s10509-024-04265-y'] | null | Lateral density distributions of Cherenkov photons at different altitudes | 2,024 | 0 | 0.19 | ['PUB_HTML'] | 0 | null |
2024AntAs..18....2D | William Rowan Hamilton a mathematician who became Royal Astronomer of Ireland was a man of mixed reputation. This paper reassesses his life and work. We first look at his family his choice of women to whom he proposed marriage and his alleged alcoholism. After considering the institution of Dunsink Observatory where he... | 2024-06-01T00:00:00Z | ['2024AntAs..18....2D'] | null | Sir William Rowan Hamilton 180565 Royal Astronomer of Ireland | 2,024 | 0 | 0.27 | null | 0 | null |
2016LPICo1962.4003K | iSEEP Wide Field MAXI iWFMAXI is a proposed mission on the ISSJEM to monitor a major fraction of the sky for detecting and localizing soft Xray transients starting at the end of 2010s. | 2016-10-01T00:00:00Z | ['2016LPICo1962.4003K'] | null | iWFMAXI iSEEP Wide Field MAXI Soft XRay Transient Monitor on ISS | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPICo1926.6103S | The physical chemical and biological properties of debrisrich ice sampled from the margin of the Greenland Ice Sheet will be described its habitat potential evaluated and its value as a possible test site for life detection tools discussed. | 2016-09-01T00:00:00Z | ['2016LPICo1926.6103S'] | null | Polar Basal Ice as Microbial Habitat an Analog for Mars | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6071R | Komar Gaon is a highly equilibritated L6 chondrite S3. CREA of Kaomar Gaon is 7 Ma. The lower bulk K content may correlate with peak solar activity solar cycle 24. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6071R'] | null | Fall Petrology Classification Noble Gas and Cosmogenic Records of Komar Gaon Meteorite the Latest Fall in India | 2,016 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6072H | Shock pressure estimates from surface samples and drill core samples from the Siljan impact structure Sweden are combined with numerical modeling. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6072H'] | null | On the Formation of the Siljan Impact Structure Sweden Combining Shock Barometry with Numerical Modeling | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2583R | A new fieldbased geologic map has been generated to compare with satellitebased maps to assess the reliability of using remote mapping for small craters. | 2016-03-01T00:00:00Z | ['2016LPI....47.2583R'] | null | A New Geologic Map of Monturaqui Meteorite Impact Crater Chile Implications for SatelliteBased Geologic Mapping of Small Craters | 2,016 | 0 | 0.14 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6192G | Antarctic micrometeorites AMMs were analyzed by Raman Spectroscopy. The organic matter shows similar characteristics as IDPs. These AMMs show inclusions of Mgolivine pyroxene and are dominated by oxides and sulfates probably alteration products. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6192G'] | null | Chemical and Mineralogical Examination of Antarctic Micrometeorites and Their Organic Compounds | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6462B | Impacts on Mars play an important global role in exposing ancient phyllosilicates from buried Noachian rocks and may have also provided localized aqueous alteration. Current studies are investigating the extent of impactinduced alteration on Mars. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6462B'] | null | Impacts on Mars Excavation andor Hydrothermal Alteration | 2,016 | 0 | 0.17 | ['PUB_PDF'] | 0 | null |
2016LPICo1960.5013H | This paper describes the latest developments in Astrobotics lunar payload delivery service along with a proposed model for science and exploration participation on this service. | 2016-11-01T00:00:00Z | ['2016LPICo1960.5013H'] | null | Astrobotic Payload Opportunities for Lunar Science and Exploration | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2885G | We provide a theoretical framework for interpreting Cassini INMS measurements of molecular hydrogen that may be present in Enceladus plume. | 2016-03-01T00:00:00Z | ['2016LPI....47.2885G'] | null | How Much Hydrothermal Hydrogen Might We Find in Enceladus Plume | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 1 | null |
2024DyAtO.10601448F | This study aims to investigate the role of tropicalextratropical interactions in the formation of atmospheric rivers as an important source of moisture in extremewidespread precipitation of Iran. Extreme precipitation events are extracted based on the 95th percentile index from 1989 to 2019 in Iran. Then the threshold ... | 2024-06-01T00:00:00Z | ['2024DyAtO.10601448F', '10.1016/j.dynatmoce.2024.101448'] | null | Investigating role of tropicalextratropical interactions in formation of atmospheric rivers and supplying extremewidespread precipitation moisture in Iran A case study on March 25 2019 | 2,024 | 0 | 0.17 | ['PUB_HTML'] | 0 | null |
2015SPIE.9593E..16M | A networked gamma radiation detection system with directional sensitivity and energy spectral data acquisition capability is being developed by the National Security Technologies LLC Remote Sensing Laboratory to support the close and intense tactical engagement of law enforcement who carry out counterterrorism missions... | 2015-08-01T00:00:00Z | ['10.1117/12.2185843', '2015SPIE.9593E..16M'] | null | Networked gamma radiation detection system for tactical deployment | 2,015 | 0 | 0.14 | ['PUB_HTML'] | 0 | null |
2024DPS....5630707C | The Vera C. Rubin Observatory with its 8.4meter widefield telescope is expected to begin the Legacy Survey of Space and Time LSST within a year. One of the LSST objectives is to discover and catalog nearEarth objects NEOs including potential Earth impacting asteroids. We consider how reliably and frequently the LSST ca... | 2024-10-01T00:00:00Z | ['2024DPS....5630707C'] | null | Forecasting LSSTs shortterm impact warning rate | 2,024 | 0 | 0.35 | null | 0 | null |
2024BSRSL..93..811D | The International Ultraviolet Explorer IUE satellite launched in 1978 by NASA and ESA has conducted highly successful longterm monitoring spectroscopic observations of many nearby lowredshift bright active galaxies including NGC 1068 NGC 5548 NGC 7469 Fairall 9MRK 335 and NGC 4151. Notably IUE has monitored NGC 4151 mo... | 2024-06-01T00:00:00Z | ['2024BSRSL..93..811D', '10.25518/0037-9565.11887'] | null | Nature of UV Variability in NGC 4151 from IUEs Intensive Monitoring Spectroscopic Data | 2,024 | 0 | 0.21 | ['PUB_HTML'] | 0 | null |
2024ATel16792....1D | We report the classification of astrophysical transient AT2024qkz from spectroscopic observations with the Kast spectrograph on the Shane telescope obtained on 2024 August 16 UT. The target was supplied by ZTF and identified using the target management platform YSEPZ Coulter et al. 2023 PASP 135 4501. | 2024-08-01T00:00:00Z | ['2024ATel16792....1D'] | null | Spectroscopic Classification of AT2024qkz with the Lick Shane telescope | 2,024 | 0 | 0.16 | ['PUB_HTML'] | 0 | null |
2024ATel16878....1H | We report the prediscovery detection of a probable M31 nova AT 2024zaq discovered by R. Fidrich on 2024 Oct. 24.337 UT. During our survey of the central region of M31 we detected the probable nova first on a coadded 900s Rband CCD frame taken on Oct. 24.151 UT with the 40in reflector at SDSUs Mount Laguna Observatory a... | 2024-10-01T00:00:00Z | ['2024ATel16878....1H'] | null | Prediscovery Detection and Photometry of AT 2024zaq a Probable Nova in M31 | 2,024 | 0 | 0.25 | ['PUB_HTML'] | 0 | null |
2024ASPC..535..191S | The H2020 NEANIAS project is implementing novel thematic services addressing emerging challenges in underwater atmospheric and space sciences to be delivered to the European Open Science Cloud EOSC. We report on the current development status of highly interdisciplinary clusters for materialising EOSC services for the ... | 2024-05-01T00:00:00Z | ['2024adass..31..191S', '2024ASPC..535..191S'] | null | Onboarding SPACE services to the European Open Science Cloud | 2,024 | 0 | 0.2 | ['ADS_PDF', 'PUB_HTML'] | 0 | null |
2024ASPC..537..103S | The NASA Community College Network NCCN is a major initiative to bring NASA Subject Matter Experts SME research findings and science resources into the nations community college system. Now entering its third year NCCN has brought together 50 SMEs and 50 community college instructors from 20 states in targeted resource... | 2024-01-01T00:00:00Z | ['2024ASPC..537..103S'] | null | The NASA Community College Network Lessons Learned and Future Expansion | 2,024 | 0 | 0.19 | ['ADS_PDF', 'PUB_HTML'] | 0 | null |
2024AdSpR..73.1549G | Remote sensing has already proven its capability in water quality studies. The technology enables the mapping of water quality parameters that affect its optical properties. Generally multispectral remote sensing data has been utilized for such analysis. Mostly the band rationing or simple regression approaches have be... | 2024-01-01T00:00:00Z | ['10.1016/j.asr.2022.09.012', '2024AdSpR..73.1549G'] | null | Spatial spectral contextual image analysis approach to map water quality of inland waterbody using AVIRISNG datasets | 2,024 | 0 | 0.16 | null | 1 | null |
2016LPICo1926.6010C | The surface compositions of martian polar regions show complex mixtures of boundadsorbed water water ice and carbondioxide ice. Mixture types include areal intimate coatings and molecular. | 2016-09-01T00:00:00Z | ['2016LPICo1926.6010C'] | null | Surface Composition of Martian Polar Regions Complex Mixtures of H2O Ice Bound H2O and CO2 Ice | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2023LPICo2852.6120C | We introduce AstroLibrary a library for realtime conjunction assessment and optimal collision avoidance. The library has been verified on SpaceMap spacemap42.com and its algorithms are available as both RESTful APIs and a Python package. | 2023-12-01T00:00:00Z | ['2023LPICo2852.6120C'] | null | AstroLibrary A Library for Realtime Conjunction Assessment and Optimal Collision Avoidance | 2,023 | 0 | 0.31 | ['PUB_PDF'] | 0 | null |
2024AdSpR..73.1379S | The present study highlights delineation of the distribution of understorey invasive plant species IPS in Mudumalai Tiger Reserve MTR Western Ghats India using very high resolution airborne imaging spectroscopy images by evaluating the performance of a Multiple Endmember Spectral Mixture Analysis MESMA. Lantana camara ... | 2024-01-01T00:00:00Z | ['2024AdSpR..73.1379S', '10.1016/j.asr.2022.12.026'] | null | Mapping of understorey invasive plant species clusters of Lantana camara and Chromolaena odorata using airborne hyperspectral remote sensing | 2,024 | 0 | 0.38 | null | 0 | null |
2024AntAs..18...94M | William John Roberts 18671942 was a skilled Irish science communicator astronomer and engineer. Largely selftaught he engaged with professional astronomers across Ireland and Europe. Here we review his life and career the instruments he used his observatory at Tullyroan Co. Armagh and the network of astronomers of whic... | 2024-06-01T00:00:00Z | ['2024AntAs..18...94M'] | null | William John Roberts 18671942 Science communicator astronomer and engineer | 2,024 | 0 | 0.18 | null | 0 | null |
2016LPICo1921.6099S | Noble gases are tracers for physical processes including adsorption dissolution and secondary mineral formation. We examine the Martian fractionated atmosphere through literature terrestrial analogs and experiments. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6099S'] | null | Fractionated Martian Noble Gases EFA Experiments and Meteorites | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6496S | Impact craters provide a complex setting for phyllosilicates. Here we characterize pre syn and post impact phyllosilicate minerals hosted within suevite deposits at the Ries impact structure. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6496S'] | null | The Importance of Phyllosilicate Mineral Formation in Impact Cratering Processes a Case Study The Ries Impact Structure Germant | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6385P | Spatially varying mechanical properties and their implications on crater formation and derived scaling laws are here assessed with the help of the shock physics numerical code iSALE. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6385P'] | null | Target Heterogeneities and Their Implications on Crater Scaling Laws | 2,016 | 0 | 0.17 | ['PUB_PDF'] | 0 | null |
2016LPICo1912.2006M | Thermophilic photosynthetic communities inhabit the moist interiors of mineral deposits in volcanic fumaroles. Contemporaneous mineral precipitation provides a high potential for preservation of morphological and chemical biosignatures. | 2016-05-01T00:00:00Z | ['2016LPICo1912.2006M'] | null | Potential for Preservation of Biosignatures from Endolithic Photosynthetic Communities in a Mars Analog Fumarole Environment | 2,016 | 0 | 0.17 | ['PUB_PDF'] | 0 | null |
2016LPICo1980.4084H | We present a new plasma composition instrument design that would extend the energy range of the current plasma instrument and provide higher time cadence and mass measurement that are required for planetary andor cometry flyover missions. | 2016-10-01T00:00:00Z | ['2016LPICo1980.4084H'] | null | Plasma Composition Instrument for Planetary and Cometary Missions | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6279W | Early condensates may be represented by zoned metals in CH and CBb chondrites. They display higher concentrations of Ni and more refractory elements in cores than in rims and lighter Fe and Ni isotope signatures in cores than in rims. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6279W'] | null | Fe and Ni Isotope Composition of Metal Grains from CH and CB Chondrites | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1980.4088S | Advanced Ion Mass Spectrometer is being developed to measure both major and minor ion species from 1 V to 25 kV with wide fieldofview in the 160 amu mass range at MM 60 over a wide range of ion intensities within high radiation environments. | 2016-10-01T00:00:00Z | ['2016LPICo1980.4088S'] | null | Advanced Ion Mass spectrometer for Giant Planet Ionospheres Magnetospheres and Moons | 2,016 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2024AREPS..52..195K | Each of the halogens constrains a different aspect of volatile cycling in the solid Earth. F is moderately incompatible in the mantle and has a low mobility at Earths surface meaning that it is preferentially retained in the mantle and continental crust. In contrast Cl Br and I are strongly incompatible and highly solu... | 2024-08-01T00:00:00Z | ['10.1146/annurev-earth-031621-111700', '2024AREPS..52..195K'] | null | Halogen Cycling in the Solid Earth | 2,024 | 0 | 0.16 | ['PUB_HTML', 'PUB_PDF'] | 1 | null |
2016LPI....47.2481B | Oxygen isotopic exchange experiments between Allende and CO gas have been conducted at one atmosphere. Exchange occurs reversing an earlier studys results. | 2016-03-01T00:00:00Z | ['2016LPI....47.2481B'] | null | Oxygen Isotopic Exchange Between Carbon Monoxide Gas and Silicate Melt Implications for the Early Solar Nebula | 2,016 | 0 | 0.17 | ['PUB_PDF'] | 1 | null |
2016LPI....47.2578A | Highly siderophile elements and 187Re187Os isotope systematics are used to investigate differentiation and late accretion on the NWA 6704 parent body. | 2016-03-01T00:00:00Z | ['2016LPI....47.2578A'] | null | Highly Siderophile Element and 187Re187Os Isotopic Systematics of Ungrouped Achondrite Northwest Africa 6704 | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2865C | Ages of melt clasts Vesta took quite a beating Different to Moon... | 2016-03-01T00:00:00Z | ['2016LPI....47.2865C'] | null | Dating Howardite Melt Clasts Evidence for an Extended Vestan Bombardment | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 1 | null |
2016LPICo1980.4045R | The Light Optical Aerosols Counter LOAC has been used for years at the surface and under all kinds of balloons in the Earth atmosphere. The reliability of this instrument is now demonstrated and it is light and compact enough for planetary missions. | 2016-10-01T00:00:00Z | ['2016LPICo1980.4045R'] | null | LOACS A Small Aerosol Optical CounterSizer for Planetary Measurements of the Size Distribution and Nature of Atmospheric Particles | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2359F | Compression of Mercurys surface resulted in lobate scarps at the edge of basin volcanic fills. Activity on these features appears to have ceased 1 Ga. | 2016-03-01T00:00:00Z | ['2016LPI....47.2359F'] | null | Late Movement of BasinEdge Lobate Scarps on Mercury | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.1978W | Titan has few impact craters that look like ones elsewhere. Some differences are due to erosion. Are others formational oddities or nonimpact origin | 2016-03-01T00:00:00Z | ['2016LPI....47.1978W'] | null | Morphological Classification of Titans Impact Craters | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2455B | We will report on the science communitybased proposition of a possible ESA contribution to NASAs Europa mission as a candidate for the upcoming ESA M5 mission. | 2016-03-01T00:00:00Z | ['2016LPI....47.2455B'] | null | The Europa Initiative for ESAs M5 Call EIM5 A Potential European Contribution to NASAs Europa MultipleFlyby Mission | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1960.5050C | We describe ESAs current lunar exploration mission activities and studies for future robotic missions including both international and commercial partnerships. | 2016-11-01T00:00:00Z | ['2016LPICo1960.5050C'] | null | Robotic Precursors to Human Explorers ESA Mission Activities and Studies | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2554Z | The petrography and geochemistry of lunar meteorite Miller Range 13317 is reviewed. The meteorite is a new basaltic regloith breccia. | 2016-03-01T00:00:00Z | ['2016LPI....47.2554Z'] | null | Petrography and Geochemistry of Lunar Meteorite Miller Range 13317 | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6039B | We examine biases in 40Ar39Ar plateau ages and the effects of these biases on our understanding of the early solar system impact history. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6039B'] | null | Apparent Late Heavy Bombardments | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017LPI....48.1159B | We present morphometric evidence that two types of double layer ejecta craters exist on Mars. We propose the distinctive type be called Bacolorian craters. | 2017-03-01T00:00:00Z | ['2017LPI....48.1159B'] | null | Evidence for Two Fundamental Types of Layered Ejecta Craters on Mars and Proposed Nomenclature System | 2,017 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2508D | Experiments simulating the formation of water in astrophysical environments produce water whose oxygen isotopic composition is mass independently fractionated. | 2017-03-01T00:00:00Z | ['2017LPI....48.2508D'] | null | Isotopic Studies of Water Formation in Astrophysical Environments First Results and Implications for Distribution of Oxygen Isotopes in Solar System | 2,017 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2941N | We report mineralogical and Mg and Fe isotopic studies of highly fractionated 18Orich silicates. The grains likely condensed from fractionated 18Orich gas. | 2016-03-01T00:00:00Z | ['2016LPI....47.2941N'] | null | Coordinated Isotopic and Mineral Characterization of Highly Fractionated 18ORich Silicates in the Queen Alexandra Range 99177 CR3 Meteorite | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2609L | We investigate the nature of secondary mineral formation in the Terra Sirenum region of Mars looking at phyllosilicates sulphates chlorides etc. in context. | 2017-03-01T00:00:00Z | ['2017LPI....48.2609L'] | null | Martian Lake Plumbing Mineralogy Morphology and Geologic Context of Hydrated Minerals in Terra Sirenum | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2114R | Characterizations of boulders on a sector of the ExoMars2020 landing site. Importance of parental lithologies and rover safety implications are presented. | 2017-03-01T00:00:00Z | ['2017LPI....48.2114R'] | null | Boulders Abundances and SizeFrequency Distributions on Mars The 2020 Exomars Landing Site Oxia Planum | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2215H | The APLLLNL GeMini Plus a highheritage gammaray spectrometer has been assembled in the laboratory and is currently undergoing initial characterization. | 2017-03-01T00:00:00Z | ['2017LPI....48.2215H'] | null | Initial Characterization of the GeMini Plus a HighResolution GammaRay Spectrometer for Planetary Composition Measurements | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2316R | Comparison of gravity fields derived using ground radar and spacecraft observations for close proximity operations around asteroid 25143 Itokawa. | 2017-03-01T00:00:00Z | ['2017LPI....48.2316R'] | null | Comparison of Gravity Fields Derived Using Ground Radar and Spacecraft Observations for Close Proximity Operations Around Asteroid 25143 Itokawa | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.3011E | What are the volatile reservoirs in the soils How do they exchange Here we identify and describe two discrete volatile reservoirs One geological one modern. | 2017-03-01T00:00:00Z | ['2017LPI....48.3011E'] | null | The Nature Carriers and Exchangeability of Volatiles in Martian Soils Evidence for Distinct Reservoirs from the Bagnold Dune Campaign and Other Measurements | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.1816M | UPb dating of Zagami phosphates was conducted by NanoSIMS. A total PbU isochron age of 24580Ma is consistent with whole rock age but older than baddeleyite. | 2017-03-01T00:00:00Z | ['2017LPI....48.1816M'] | null | UraniumLead Dating of Zagami Phosphates by NanoSIMS | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.1340H | We suggest that many Mars impactors are weak enough to fragment at high altitudes and we derive the frequency of field secondary craters. | 2017-03-01T00:00:00Z | ['2017LPI....48.1340H'] | null | Utilizing Primary Martian Crater Clusters to Study Meteoroid Properties and Secondary Crater Populations | 2,017 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2017LPICo1961.3061T | We describe dunes on Pluto and suggest they result from availability of granular solids and local wind regime at the margin of an icecap and mountain range. | 2017-05-01T00:00:00Z | ['2017LPICo1961.3061T'] | null | Evidence Supporting Aeolian Depositional Origin of Landforms of Sputnik Planum Pluto from New Horizons Imagery | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.1338B | Primitive chondrites 16Opoor grossite grains Intriguing results. | 2017-03-01T00:00:00Z | ['2017LPI....48.1338B'] | null | 16OPoor Grossite In Refractory Inclusions from Pristine CO3.0 Chondrites | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2017LPI....48.2501B | Strength plays a role in determining the outcome of impact events. Our objective is to scale fracture parameters in meteorites to their parent body. | 2017-03-01T00:00:00Z | ['2017LPI....48.2501B'] | null | Meteorite Fractures and Scaling for Asteroid Atmospheric Entry | 2,017 | 0 | 0.1 | ['PUB_PDF'] | 1 | null |
2017LPICo1967.4017M | We present experimental evidence that vesicles spontaneously forming in tectonic fault zones in the Earths crust are capable of selecting and accumulating hydrothermally generated peptide molecules which integrate into the vesicle membrane. | 2017-07-01T00:00:00Z | ['2017LPICo1967.4017M'] | null | Evolution of Prebiotic Peptides in Amphiphilic Environments | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2460K | Scanning transmission electron microscopy was used to investigate the interface between Genesis silicon sample 61881 and silicon contamination on its surface. | 2016-03-01T00:00:00Z | ['2016LPI....47.2460K'] | null | Catastrophic Impact of Silicon on Silicon Unraveling the Genesis Impact Using Sample 61881 | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2074T | An automated MRO camera DTM production pipeline for planetary mapping and separate pipeline for repeat imaging based superresolution restoration is introduced. | 2016-03-01T00:00:00Z | ['2016LPI....47.2074T'] | null | Automated DTM Generation and SuperResolution Restoration from NASA MRO Cameras and in Future from TGO16 CASSIS | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2559L | We compare the occurrences and textures of Kfeldspar exsolution in a range of ordinary chondrites and discuss implications for metasomatism and cooling rates. | 2016-03-01T00:00:00Z | ['2016LPI....47.2559L'] | null | Alkali Feldspar Exsolution in Ordinary Chondrites Alkali Metasomatism Metamorphism and Cooling Rates | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 1 | null |
2016LPICo1921.6063G | The famous pseudotachylytes in theVredefort Dome were formed by impactinduced seismic shaking a common but overlooked deformation process in terrestrial cratering. Seismic shaking is a fundamental geophysical process and wellknown from the moon. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6063G'] | null | The Vredefort Pseudotachylytes A Centennial Reappraisal of S. J. Shand 1916. Shaken not Stirred by Meteorite Impacting | 2,016 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6171H | We propose a revised age of 192.0 0.8 Ma for the formation of the PuchezhKatunki impact structure Russia based on 40Ar39Ar stepheating analyses of five impact melt rock samples. This age does not correlate with any known extinction event. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6171H'] | null | An Early Jurassic 40Ar39Ar Age for the PuchezhKatunki Impact Structure Russia No Causal Link to an Extinction Event | 2,016 | 0 | 0.19 | ['PUB_PDF'] | 3 | null |
2016LPI....47.3066S | For the University Rover Challenge undergraduate teams design and build the next generation of rovers to compete in science and engineering tasks. | 2016-03-01T00:00:00Z | ['2016LPI....47.3066S'] | null | The University Rover Challenge An International Rover Competiton Under Simulated Mars Operational Conditions | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2024ATel16478....1D | We report the following the classifications of astrophysical transients from spectroscopic observations with the LRIS spectrograph on the Keck I telescope made on 2024 Feb 14 UT. The targets were supplied by YSE ATLAS and ZTF and identified using the target management platform YSEPZ Coulter et al. 2023 PASP 135 4501. | 2024-02-01T00:00:00Z | ['2024ATel16478....1D'] | null | Spectroscopic Classifications of Astrophysical Transients with Keck I LRIS | 2,024 | 0 | 0.2 | ['PUB_HTML'] | 0 | null |
2016LPICo1920.7002A | The mapping and monitoring of swiss cheese feature example of this paper achieved by pixel markers measurements proposed by author. This monoring suggest high amount of displacements in pits of Martian polar areas. | 2016-06-01T00:00:00Z | ['2016LPICo1920.7002A'] | null | Kinematics Mapping and Monitoring of Swiss Cheese Features in the Polar Icy Regions Over Two Martian Years Base on HIRISEMOC NASA Images | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPICo1921.6347L | Partial melting experiments on CV3 chondrites reveal that oxidized differentiated planetesimals may differ in their interior mineralogy and thermal structure from more typical reduced differentiated planetesimals. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6347L'] | null | Differentiation of Relatively Oxidized Planetesimals Experimental Partial Melting of Allende at IW1 | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2560M | We report O isotopic systematics and AlMg chronology of CAIs and their WarkLovering rims and discuss the timescales of formation of WarkLovering rims. | 2016-03-01T00:00:00Z | ['2016LPI....47.2560M'] | null | Formation Timescales of WarkLovering Rims Around CalciumAluminum Rich Inclusions | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2363G | We use Simulated Lunar Environment Chamber measurements of lunar soils to ground truth Diviner Lunar Radiometer compositional and thermophysical data. | 2016-03-01T00:00:00Z | ['2016LPI....47.2363G'] | null | Connecting Simulated Lunar Environment Chamber Measurements to Diviner Lunar Radiometer Observations | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1911.6071H | The LCROSS impact on the Moon revealed much about the composition of the volatiles in lunar PSRs. | 2016-05-01T00:00:00Z | ['2016LPICo1911.6071H'] | null | The LCROSS Plume as Observed by LROLAMP | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPICo1960.5059A | This presentation introduces ispace a Tokyobased lunar exploration company. Technology applied to the Team Hakuto Google Lunar XPRIZE mission will be described. Finally it will discuss how developing low cost and mass efficient rovers can support scientific opportunities. | 2016-11-01T00:00:00Z | ['2016LPICo1960.5059A'] | null | Scientific Opportunities with ispace a Lunar Exploration Company | 2,016 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2016LPI....47.3046B | Previous catalogs of basins on Mars are reanalyzed with current orbital data to provide updated catalogs of peakring basins and protobasins. | 2016-03-01T00:00:00Z | ['2016LPI....47.3046B'] | null | Updated Catalogs of PeakRing Basins and Protobasins on Mars | 2,016 | 0 | 0.12 | ['PUB_PDF'] | 0 | null |
2016LPICo1912.2083J | Microbial community structure and preservation of organic matter in siliceous hydrothermal environments is a critical issue given the discovery of hydrothermal vents and silica on Mars. Here we discuss preservation of cyanobacterial biomarker lipid. | 2016-05-01T00:00:00Z | ['2016LPICo1912.2083J'] | null | Organic Biomarker Preservation in SilicaRich Hydrothermal Systems with Implications to Mars | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2076P | We present a tool to measure the full pixel analyses albedo contrast between slope streaks and their neighborhood regions. | 2016-03-01T00:00:00Z | ['2016LPI....47.2076P'] | null | 13 Years of Temporal Fading Quantification in Dark Slope Streaks from Lycus Sulci | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2077A | There was probably a solid inner core by the end of Earths accretion. During the accretion inner part of the core solidified due to increase in pressure. | 2016-03-01T00:00:00Z | ['2016LPI....47.2077A'] | null | Thermal Evolution of Earths Core During Accretion A Primordial Solis Inner Core | 2,016 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2268B | Occator once hot Liquid water flowed beneath Alas no longer. | 2016-03-01T00:00:00Z | ['2016LPI....47.2268B'] | null | Impact Induced Heating of Occator Crater on Asteroid 1 Ceres | 2,016 | 0 | 0.19 | ['PUB_PDF'] | 4 | null |
2016LPI....47.2458N | Anoxic hydrothermal alteration of basalt produced a ferrous smectite structurally similar to clays found on Mars. May be a globally relevant process. | 2016-03-01T00:00:00Z | ['2016LPI....47.2458N'] | null | Clay Formation and Iron Partitioning During Anoxic Isochemical Hydrothermal Basalt Alteration Implications for Formation of Fe Smectites on Early Mars | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPICo1911.6068K | A diverse array of impactor signatures suggests asteroids have always dominated comets during the evolution of the Moon. | 2016-05-01T00:00:00Z | ['2016LPICo1911.6068K'] | null | A Summary of Geological Geochemical Petrological and Isotopic Evidence of Impactor Sources | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2945F | We show lighting bias affects the results of orientation analysis even for large linear features relevant for catenae and lobate scarps. | 2016-03-01T00:00:00Z | ['2016LPI....47.2945F'] | null | Mercury Catenae Linear Features and Lighting Bias | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2171F | FoOxidation Hematite dominates but Magnetite as well. | 2016-03-01T00:00:00Z | ['2016LPI....47.2171F'] | null | Olivine Oxidation and Implications for Planetary Surface Processes | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2016LPI....47.2170B | Oxia Planum Aram Dorsum Mawrth Vallis are the candidate sites for the ExoMars Rover. They contain clays alluvial and deltaic environments. | 2016-03-01T00:00:00Z | ['2016LPI....47.2170B'] | null | ExoMars Landing Site Characterisation and Selection | 2,016 | 0 | 0.1 | ['PUB_PDF'] | 1 | null |
2016LPICo1921.6251C | We synthesized nonideal single domain pure monoclinic pyrrhotite and characterized the samples from 5 to 633 K using various magnetic and other techniques. The samples show 3238 demagnetization of remanence under hydrostatic pressure 1.82 GPa. | 2016-08-01T00:00:00Z | ['2016LPICo1921.6251C'] | null | Magnetic Characterization of NonIdeal SingleDomain Monoclinic Pyrrhotite and Its Demagnetization Under Hydrostatic Pressure up to 2 GPa with Implications for Impact Demagnetization | 2,016 | 0 | 0.06 | ['PUB_PDF'] | 0 | null |
2024E&PSL.62718513S | Glacier slip modulates sealevel rise. Most slip models assume quasiequilibrium process dynamics and debrisfree basal ice but observations regularly show debrisrich basal ice sliding under transient external forcings placing theory and observation in tension. Seismicity generated by slip icequake activity provides a win... | 2024-02-01T00:00:00Z | ['10.1016/j.epsl.2023.118513', '2024E&PSL.62718513S'] | null | Icequake insights on transient glacier slip mechanics near channelized subglacial drainage | 2,024 | 0 | 0.25 | ['PUB_HTML'] | 3 | null |
2017LPI....48.1246A | Leadlead isochrons Alongside RbSr Dating in situ. | 2017-03-01T00:00:00Z | ['2017LPI....48.1246A'] | null | Multianalytical Science with the CODEX InSitu Dating Spectrometer | 2,017 | 0 | 0 | ['PUB_PDF'] | 0 | null |
2024DyAtO.10601453K | Current perspectives on lower frequency variations and secular warming have predominantly been shaped by traditional anomalies that assume an annual cycle AC with a timeinvariant amplitude. However this anomaly framework falls short in capturing the complexity of multiple periodic modes with intricate waveforms and tim... | 2024-06-01T00:00:00Z | ['2024DyAtO.10601453K', '10.1016/j.dynatmoce.2024.101453'] | null | Decoding lowfrequency climate variations A case study on ENSO and ocean surface warming | 2,024 | 0 | 0.21 | ['PUB_HTML'] | 0 | null |
2016PhDT.......468S | Over the past decades star formation has been a very attractive field because knowledge of star formation leads to a better understanding of the formation of planets and thus of our solar system but also of the evolution of galaxies. Conditions leading to the formation of highmass stars are still under investigation bu... | 2016-12-01T00:00:00Z | ['2016PhDT.......468S'] | null | Modeling chemistry in massive star forming regions with internal PDRs | 2,016 | 0 | 0.22 | ['AUTHOR_HTML'] | 0 | null |
2018cosp...42E1522H | The ionizing radiation environment in space pretenses substantial risks to human exploration. It consists primarily of 3 components Solar Particles Events SPE Galactic Cosmic Rays GCR and Van Allen Belts trapped protons that differ in elemental compositions energy spectra and intensities. The extravehicular environment... | 2018-07-01T00:00:00Z | ['2018cosp...42E1522H'] | null | New Human Anatomical Model For Crew Radiation Analysis | 2,018 | 0 | 0.18 | null | 0 | null |
2017Ap&SS.362...34L | Rotational state of space debris will be influenced by eddy current torque which is produced by the conducting body rotating within the geomagnetic field. Former expressions of instantaneous torque established in bodyfixed coordinate system will change in space during rotation due to the variation of the coordinate sys... | 2017-02-01T00:00:00Z | ['10.1007/s10509-017-3012-4', '2017Ap&SS.362...34L'] | null | Approximate expressions of mean eddy current torque acted on space debris | 2,017 | 0 | 0.12 | ['PUB_HTML'] | 1 | null |
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