Search results for "PAC"

showing 10 items of 28794 documents

Acoustic properties of ancient shallow-marine carbonates: effects of depositional environments and diagenetic processes (Middle Jurassic, Paris Basin…

2010

17 pages; International audience; Examination of petrophysical properties (acoustic velocity, porosity, permeability, and density) and petrographical characteristics (texture, facies composition, and diagenesis) of more than 250 core plugs from the Middle Jurassic carbonates of the eastern Paris Basin provides insights into the parameters controlling acoustic velocities in relatively low-porosity carbonate rocks ({Phi} < 20%). The pore-type observations reveal distinct acoustic velocities in samples with intergranular macropores and samples with micropores in subhedral micrite, such that velocities in microporous mudstone–wackestone (lagoonal) deposits are greater than in macroporous grains…

010504 meteorology & atmospheric sciencesPetrophysicsCompaction[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/PetrographyMineralogyGeology010502 geochemistry & geophysicsCementation (geology)[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesDiagenesisGrainstone[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyFaciesMarlCarbonate rockGeology0105 earth and related environmental sciences[ SDU.STU.PE ] Sciences of the Universe [physics]/Earth Sciences/Petrography
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Oscillations on Width and Intensity of Slender Ca ii H Fibrils from Sunrise/SuFI

2017

R. Gafeira et. al.

010504 meteorology & atmospheric sciencesPhase (waves)FOS: Physical scienceschromosphere [Sun]Astrophysics01 natural sciencesMolecular physics0103 physical sciencesWave modeSunriseSun: oscillationsTechniques: imaging spectroscopySun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSolar observatoryoscillations [Sun]imaging spectroscopy [Techniques]Sun: chromosphereAstronomy and AstrophysicsAstrophysics - Solar and Stellar Astrophysicsmagnetic fields [Sun]Space and Planetary ScienceIntensity (heat transfer)The Astrophysical Journal Supplement Series
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P and S wave travel time tomography of the SE Asia-Australia collision zone

2019

© 2019 Elsevier B.V. The southeast (SE)Asia - Australia collision zone is one of the most tectonically active and seismogenic regions in the world. Here, we present new 3-D P- and S-wave velocity models of the crust and upper mantle by applying regional earthquake travel-time tomography to global catalogue data. We first re-locate earthquakes provided by the standard ISC-Reviewed and ISC-EHB catalogues using a non-linear oct-tree scheme. A machine learning algorithm that clusters earthquakes depending on their spatiotemporal density was then applied to significantly improve the consistency of travel-time picks. We used the Fast Marching Tomography software package to retrieve 3-D velocity a…

010504 meteorology & atmospheric sciencesPhysics and Astronomy (miscellaneous)SubductionTravel-timeAstronomy and AstrophysicsCrust010502 geochemistry & geophysicsCollision zone01 natural sciencesBody-waveMantle (geology)TectonicsGeophysicsSpace and Planetary ScienceLithosphereS-waveEarthquakesSlabSE AsiaTomographySeismologyGeology0105 earth and related environmental sciencesPhysics of the Earth and Planetary Interiors
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Enhancing the retrieval of stream surface temperature from Landsat data

2019

International audience; Thermal images of water bodies often show a radiance gradient perpendicular to the banks. This effect is frequently due to mixed land and water thermal pixels. In the case of the Landsat images, radiance mixing can also affect pure water pixels due the cubic convolution resampling of the native thermal measurements. Some authors recommended a general-purpose margin of two thermal pixels to the banks or a minimum river width of three pixels, to avoid near bank effects in water temperature retrievals. Given the relatively course spatial resolution of satellite thermal sensors, the three pixel margin severely restricts their application to temperature mapping in many ri…

010504 meteorology & atmospheric sciencesPixel0208 environmental biotechnologySoil ScienceGeologyImage processing02 engineering and technology01 natural sciencesSubpixel rendering6. Clean water020801 environmental engineering[SDE]Environmental SciencesThermalRadianceEnvironmental scienceSatelliteSatellite imageryComputers in Earth SciencesRiver surface temperature Landsat 8 thermal band Thermal spatial resolution Cubic convolution resampling Thermal impact Mequinenza reservoir Ebro river Thermal stratificationImage resolution0105 earth and related environmental sciencesRemote sensingRemote Sensing of Environment
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A Search for IceCube Events in the Direction of ANITA Neutrino Candidates

2020

During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy up-going air shower and compatible with a tau neutrino interpretation. A third neutrino candidate event was detected in a search for Askaryan radiation in the Antarctic ice, although it is also consistent with the background expectation. The inferred emergence angle of the first two events is in tension with IceCube and ANITA limits on isotropic cosmogenic neutrino fluxes. Here, we test the hypothesis that these events are astrophysical in origin, possibly caused by a po…

010504 meteorology & atmospheric sciencesPoint sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Tau neutrino0103 physical sciencesTRACK RECONSTRUCTIONSource spectrum010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEIsotropyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicshep-phHigh Energy Physics - PhenomenologyAir showerPhysics and Astronomy13. Climate actionSpace and Planetary ScienceNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)
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Spectropolarimetric evidence for a siphon flow along an emerging magnetic flux tube

2016

©2017 The American Astronomical Society. All rights reserved.We study the dynamics and topology of an emerging magnetic flux concentration using high spatial resolution spectropolarimetric data acquired with the Imaging Magnetograph eXperiment on board the sunrise balloon-borne solar observatory. We obtain the full vector magnetic field and the line of sight (LOS) velocity through inversions of the Fe i line at 525.02 nm with the SPINOR code. The derived vector magnetic field is used to trace magnetic field lines. Two magnetic flux concentrations with different polarities and LOS velocities are found to be connected by a group of arch-shaped magnetic field lines. The positive polarity footp…

010504 meteorology & atmospheric sciencesPolarity (physics)photosphere [Sun]FOS: Physical sciencesAstrophysicspolarimetric [Techniques]01 natural sciencesMethods: observational0103 physical sciencesSunriseAstrophysics::Solar and Stellar Astrophysicsobservational [Methods]010303 astronomy & astrophysicsSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsSolar observatoryPolarity symbolsTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsMagnetic fluxMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsFlow (mathematics)magnetic fields [Sun]Space and Planetary Science
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An expanded model and application of the combined effect of crystal-size distribution and crystal shape on the relative viscosity of magmas

2018

International audience; This study examines the combined effect of crystal-size distributions (CSD) and crystal shape on the rheology of vesicle free magmatic suspensions and provides the first practical application of an empirical model to estimate the relative effect of crystal content and CSD's on the viscosity of magma directly from textural image analysis of natural rock samples in the form of a user-friendly texture-rheology spreadsheet calculator. We extend and apply established relationships between the maximum packing fraction ϕm of a crystal bearing suspension and both its rheological properties and the polydispersity γ of a CSD. By using analogue rotational rheometric experiments…

010504 meteorology & atmospheric sciencesRelative viscosityDispersityThermodynamicsMagma rheologyCrystal size distribution010502 geochemistry & geophysicsAtomic packing factor01 natural sciencesCrystalViscosityGeophysicsRheologyGeochemistry and PetrologyMagma[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologySuspension (vehicle)GeologyCrystal shape0105 earth and related environmental sciences
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Validation of a novel Multi-Gas sensor for volcanic HCl alongside H2S and SO2 at Mt. Etna

2017

Erratum to: Bull Volcanol (2017) 79: 36DOI 10.1007/s00445-017-1114-zDuring the steps of corrections, the publisher inadvertently changed the author affiliations so that they were no longer correct. The correct information is given below. The publisher regrets this mistake.; International audience; Volcanic gas emission measurements inform predictions of hazard and atmospheric impacts. For these measurements, Multi-Gas sensors provide low-cost in situ monitoring of gas composition but to date have lacked the ability to detect halogens. Here, two Multi-Gas instruments characterized passive outgassing emissions from Mt. Etna’s (Italy) three summit craters, Voragine (VOR), North-east Crater (NE…

010504 meteorology & atmospheric sciencesResponse modelPoison controlMineralogyOpen-system volcanic degassing010502 geochemistry & geophysics01 natural sciencesElectronic noseImpact craterGeochemistry and PetrologyCalibrationGas compositionVolcanic outgassing0105 earth and related environmental sciencesMulti-Gas instrumentgeographygeography.geographical_feature_categoryE-noseOutgassingVolcano13. Climate action[SDU]Sciences of the Universe [physics]HalogenMagmaChlorineGeology
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The GAPS Programme with HARPS-N at TNG: . Atmospheric Rossiter-McLaughlin effect and improved parameters of KELT-9b

2019

In the framework of the GAPS project, we observed the planet-hosting star KELT-9 (A-type star, VsinI$\sim$110 km/s) with the HARPS-N spectrograph at the TNG. In this work we analyse the spectra and the extracted radial velocities (RVs), to constrain the physical parameters of the system and to detect the planetary atmosphere of KELT-9b. We extracted from the high-resolution optical spectra the mean stellar line profiles with an analysis based on the Least Square Deconvolution technique. Then, we computed the stellar RVs with a method optimized for fast rotators, by fitting the mean stellar line profile with a purely rotational profile instead of using a Gaussian function. The new spectra an…

010504 meteorology & atmospheric sciencesRossiter–McLaughlin effectFOS: Physical sciencesAstrophysics01 natural sciencesSpectral lineAtmospheretechniques: radial velocities0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsplanetary systems010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)planets and satellites: atmospheresPhysicsSettore FIS/05Astronomy and AstrophysicsPlanetary systemstars: individual: KELT-9ExoplanetRadial velocityAmplitudeAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsPlanetary masstechniques: spectroscopicAstrophysics - Earth and Planetary Astrophysics
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Titan's surface albedo variations over a Titan season from near-infrared CFHT/FTS spectra

2006

International audience; We have observed Titan in a series of campaigns from 1991 to 1996 with the Fourier Transform Spectrometer on the CFH telescope. The data acquired provide a lightcurve from the geometric albedos in the 0.9–View the MathML source spectral region. The 1991–1993 data were previously analyzed in Coustenis et al. [1995. Titan's surface: composition and variability from its near-infrared albedo. Icarus 118, 87–104] with a spherical particle code by McKay et al. [1989. The thermal structure of Titan's atmosphere. Icarus 80, 23–53]. We present here three new datasets from the 1994, 1995 and 1996 observations, with additional information from the 0.94-μm methane window on Tita…

010504 meteorology & atmospheric sciencesSatellitesCFHTAstrophysicsAtmospheric sciences01 natural sciencesMethaneAtmosphereMethane absorption coefficientssymbols.namesakechemistry.chemical_compoundNear-infraredPlanet0103 physical sciencesRadiative transfer010303 astronomy & astrophysicsSpectroscopy0105 earth and related environmental sciencesPhysicsAtmospheric methaneAstronomy and AstrophysicsTholinAlbedochemistry13. Climate actionSpace and Planetary SciencesymbolsTitan (rocket family)Titan
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