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showing 10 items of 4997 documents

The high overtone and combination levels of SF6 revisited at Doppler-limited resolution: A global effective rovibrational model for highly excited vi…

2017

Abstract Sulfur hexafluoride is an important prototypal molecule for modeling highly excited vibrational energy flow and multi quanta absorption processes in hexafluoride molecules of technological importance. It is also a strong greenhouse gas of anthropogenic origin. This heavy species, however, features many hot bands at room temperature (at which only 30% of the molecules lie in the ground vibrational state), especially those originating from the lowest, v 6 =1 vibrational state. Using a cryogenic long path cell with variable optical path length and temperatures regulated between 120 and 163 K, coupled to Synchrotron Radiation and a high resolution interferometer, Doppler-limited spectr…

010504 meteorology & atmospheric sciencesOvertoneInfrared spectroscopylow temperature01 natural sciences7. Clean energyHot bandSpectral linechemistry.chemical_compoundHexafluorideFar infraredhot bandRotation-vibration spectroscopy of SF 60103 physical sciencesSpectroscopy0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Radiation[ PHYS ] Physics [physics]010304 chemical physicsRotational–vibrational spectroscopyAtomic and Molecular Physics and Opticschemistry13. Climate actiongreenhouse gasExcited stateinfrared absorptionAtomic physicstensorial formalismLong path cell
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The giant inoceramid Platyceramus platinus as a high-resolution paleoclimate archive for the Late Cretaceous of the Western Interior Seaway

2018

Abstract Platyceramus platinus was a giant inoceramid bivalve that inhabited the outer shelf environments of the Western Interior Seaway (WIS) in North America. With axial heights typically exceeding 1 m, the shells of this species potentially serve as a unique high-resolution geochemical proxy archive for Late Cretaceous paleoclimate. Here we present the first sclerochronological investigation of P. platinus shells to evaluate the usefulness of this species as an archive of short-term (e.g., seasonal to inter-annual) paleoenvironmental variability. We analyzed the growth patterns, the stable oxygen (δ18O) and carbon (δ13C) isotope values of well-preserved P. platinus shell fragments from t…

010504 meteorology & atmospheric sciencesPlatyceramusbiologyδ18OPaleontologyWestern Interior Seaway010502 geochemistry & geophysicsbiology.organism_classification01 natural sciencesSeafloor spreadingNiobrara FormationCretaceousPaleontologyWater columnPaleoclimatologyGeology0105 earth and related environmental sciencesCretaceous Research
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Mountain building in NW Sicily from the superimposition of subsequent thrusting and folding events during Neogene: structural setting and tectonic ev…

2017

We present a 1:25.000 scale geological map of the Kumeta-Pizzuta ridge in north-western Sicily (Italy), achieved by integrating stratigraphic, structural and geophysical data. In this area, the tectonic edifice results from the piling-up of deep-water-, carbonate platform- and pelagic platform-derived tectonic units (Imerese and Sicilide, Panormide and Trapanese domains, respectively) resulting from deformations of the former southern Tethyan continental margin. The structural setting shows interference of tectonic events, different types of structural styles and different scales of deformational patterns. Early overthrust of the Imerese on the Trapanese units (since the late Serravallian) …

010504 meteorology & atmospheric sciencesSettore GEO/02 - Geologia Stratigrafica E SedimentologicaCarbonate platformGeography Planning and Development010502 geochemistry & geophysicsNeogene01 natural sciencesgeological mapContinental marginlcsh:G3180-9980Sicily; Kumeta ridge; backthrust; geological mapEarth and Planetary Sciences (miscellaneous)SuperimpositionSicily0105 earth and related environmental scienceslcsh:Mapsgeographygeography.geographical_feature_categoryKumeta ridgeGeologic mapTectonicsMountain formationRidgeSeismologyGeologybackthrust
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X-ray flare oscillations track plasma sloshing along star-disk magnetic tubes in Orion star-forming region

2018

Pulsing X-ray emission tracks the plasma echo traveling in an extremely long magnetic tube that flares in an Orion Pre-Main Sequence (PMS) star. On the Sun, flares last from minutes to a few hours and the longest-lasting typically involve arcades of closed magnetic tubes. Long-lasting X-ray flares are observed in PMS stars. Large-amplitude (~20%) long-period (~3 hours) pulsations are detected in the light curve of day-long flares observed by the Advanced CCD Imaging Spectrometer (ACIS) on-board Chandra from PMS stars in the Orion cluster. Detailed hydrodynamic modeling of two flares observed on V772 Ori and OW Ori shows that these pulsations may track the sloshing of plasma along a single l…

010504 meteorology & atmospheric sciencesSlosh dynamicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural scienceslaw.inventionlaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsX-rays: star010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesstars: coronaePhysicsstars: formationTrack (disk drive)X-rayAstronomy and AstrophysicsPlasmaAstronomy and AstrophysicAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space Physicsstars: flareAstrophysics::Earth and Planetary AstrophysicsFlare
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Mountain Building in Taiwan: Insights From 3‐D Geodynamic Models

2019

Taiwan is widely considered to be a typical example of an arc-continent collision surrounded by two opposite dipping subduction zones. The manner by which the interaction of the two neighboring slabs caused plate collision and mountain building is insufficiently understood. Various hypotheses have been proposed, but the geodynamic feasibility of those remains to be tested. Here we present 3-D thermomechanical models to study the geodynamic evolution process of a Taiwan-like setting after an initial transform fault was consumed. In our model setup, the boundary between the Eurasian plate and the South China Sea is northeast trending. The results show that all simulations result in toroidal m…

010504 meteorology & atmospheric sciencesSubductionContinental crustEurasian PlateTransform faultCrust01 natural sciencesGeophysicsMountain formationSpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)ErosionSlabSeismologyGeology0105 earth and related environmental sciencesJournal of Geophysical Research: Solid Earth
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Results from DROXO IV. EXTraS discovery of an X-ray flare from the Class I protostar candidate ISO-Oph 85

2016

X-ray emission from Young Stellar Objects (YSOs) is crucial to understand star formation. A very limited amount of X-ray results is available for the protostellar (ClassI) phase. A systematic search of transient X-ray phenomena combined with a careful evaluation of the evolutionary stage offer a widely unexplored window to our understanding of YSOs X-ray properties. Within the EXTraS project, a search for transients and variability in the whole XMM-Newton archive, we discover transient X-ray emission consistent with ISO-Oph 85, a strongly embedded YSO in the rho Ophiuchi region, not detected in previous time-averaged X-ray studies. We extract an X-ray light curve for the flare and determine…

010504 meteorology & atmospheric sciencesYoung stellar objectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesflares; X-rayslaw.inventionPhotometry (optics)law0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencescoronaePhysicseducation.field_of_studystars: protostarsStar formationactivityAstronomy and AstrophysicsLight curveAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceSpectral energy distributionAstrophysics::Earth and Planetary AstrophysicsFlare
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Deep X-ray view of the Class I YSO Elias 29 with XMM-Newton and NuSTAR

2019

[Abridged] We investigated the X-ray characteristics of the Class I YSO Elias 29 with joint XMM-Newton and NuSTAR observations of 300 ks and 450 ks, respectively. These are the first observations of a very young (<1 Myr) stellar object in a band encompassing simultaneously both soft and hard X-rays. In addition to the hot Fe complex at 6.7 keV, we observed fluorescent emission from Fe at $\sim6.4$ keV, confirming the previous findings. The line at 6.4 keV is detected during quiescent and flaring states and its flux is variable. The equivalent width is found varying in the $\approx 0.15--0.5$ keV range. These values make unrealistic a simple model with a centrally illuminated disk and sug…

010504 meteorology & atmospheric sciencesYoung stellar objectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_studyStar formationAstronomy and AstrophysicsCoronaAccretion (astrophysics)Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomenastars:activity–stars:coronae–stars:pre-mainsequence–stars:formation–stars:flareEquivalent widthFlare
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Influence of microporosity distribution on the mechanical behavior of oolithic carbonate rocks.

2015

Abstract The mechanical behavior of oolithic carbonate rocks was investigated for selected rocks with two different microstructural attributes: uniform (UP) and rimmed (RP) distribution of microporosity within ooids. These oolithic carbonate rocks are from the Oolithe Blanche formation, a deep saline aquifer in the Paris Basin, and a possible target for CO2 sequestration and geothermal production. Samples of similar physical properties (porosity, grain diameter, cement content) but different microporosity textures were deformed under triaxial configuration, in water saturated conditions, at 28 MPa of confining pressure, 5 MPa of pore pressure and at a temperature of 55 °C. During the experi…

010504 meteorology & atmospheric sciences[SDU.STU.PE]Sciences of the Universe [physics]/Earth Sciences/PetrographyMineralogy010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesTortuosityPore water pressureBrittlenessRock mechanicsMicroporosityParis BasinComputers in Earth SciencesOolithe Blanche formationSafety Risk Reliability and QualityPorosity0105 earth and related environmental sciences[ SDU.STU.PE ] Sciences of the Universe [physics]/Earth Sciences/PetrographyCarbonate rockGeotechnical Engineering and Engineering GeologyOverburden pressurePermeability (earth sciences)Rock mechanics[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyCarbonate rockGeology
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GRB 050904 at redshift 6.3: observations of the oldest cosmic explosion after the Big Bang

2005

We present optical and near-infrared observations of the afterglow of the gamma-ray burst GRB 050904. We derive a photometric redshift z = 6.3, estimated from the presence of the Lyman break falling between the I and J filters. This is by far the most distant GRB known to date. Its isotropic-equivalent energy is 3.4x10^53 erg in the rest-frame 110-1100 keV energy band. Despite the high redshift, both the prompt and the afterglow emission are not peculiar with respect to other GRBs. We find a break in the J-band light curve at t_b = 2.6 +- 1.0 d (observer frame). If we assume this is the jet break, we derive a beaming-corrected energy E_gamma = (4-12)x10^51 erg. This limit shows that GRB 050…

010504 meteorology & atmospheric sciencesgamma rays: burstsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsJet (particle physics)Astrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]gamma rays: individual: GRB 0509040103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesPhotometric redshiftPhysicsCOSMIC cancer database[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Star formationAstrophysics (astro-ph)Astronomy and Astrophysicsearly UniverseLight curveRedshiftAfterglowSpace and Planetary Sciencecosmology: observationsGamma-ray burst
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High-resolution spectroscopy and analysis of the V2 + V3 combination band of SF6 in a supersonic jet expansion

2013

International audience; Sulphur hexafluoride is a very strong greenhouse gas whose concentration is increasing in the atmosphere. It is detected through infrared absorption spectroscopy in the strong ν3 fundamental region. Due to the existence of low-lying vibrational states of this molecule, however, many hot bands arise at room temperature and those are still not known. We present here a contribution to the elucidation of this hot band structure, by analysing the ν2 + ν3 combination band. We use a supersonic jet expansion high-resolution spectrum at a rotational temperature of ca. 25 K that was recorded thanks to the Jet-AILES setup at the Source Optimisée de Lumière d'Energie Intermédiai…

010504 meteorology & atmospheric sciencessupersonic jet expansionBiophysicsInfrared spectroscopy7. Clean energy01 natural sciencesHot bandlaw.inventionsymbols.namesake[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]law0103 physical sciencesSupersonic speedPhysical and Theoretical ChemistrySpectroscopy[ PHYS.PHYS.PHYS-ATM-PH ] Physics [physics]/Physics [physics]/Atomic and Molecular Clusters [physics.atm-clus]Molecular BiologyComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciences[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]010304 chemical physicssulphur hexafluorideChemistry[PHYS.PHYS.PHYS-ATM-PH]Physics [physics]/Physics [physics]/Atomic and Molecular Clusters [physics.atm-clus]Rotational temperatureRotational–vibrational spectroscopyCondensed Matter PhysicsSynchrotron[CHIM.THEO]Chemical Sciences/Theoretical and/or physical chemistry[ PHYS.PHYS.PHYS-CHEM-PH ] Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]13. Climate actiongreenhouse gassymbolsinfrared absorption[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]Atomic physicsHamiltonian (quantum mechanics)tensorial formalism
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