Search results for "Universe"

showing 10 items of 2171 documents

Les bioévénements de la limite Albien (Vraconnien) - Cénomanien aux marges nord et sud de la Téthys (S.E. de la France et Tunisie centrale)

2007

International audience; Les bioévénements de la limite Albien (Vraconnien) - Cénomanien aux marges nord et sud de la Téthys (S.E. de la France et Tunisie centrale) [Bioevents at the Albian (Vraconnian) - Cenomanian boundary at the North and South margins of the Tethyan Ocean (SE France and Central Tunisia)]

ammonitesSE FranceTéthys[SDU.STU.ST] Sciences of the Universe [physics]/Earth Sciences/Stratigraphylimite Albien-Cénomanien[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/StratigraphyVraconnienforaminifères planctoniquesTunisie
researchProduct

The Upper Sinemurian ammonite succession in the Sierra Madre Oriental (Mexico).

2009

International audience; In the Sierra Madre Oriental (Mexico), the biostratigraphic subdivision of the Upper Sinemurian can be refined. It has been possible to differentiate 11 horizons from the upper Obtusum Zone to the top of the Raricostatum Zone which are correlated with the NW European standard zonation. The index species of each horizon is figured.

ammonitesSierra Madre OrientalEarly Jurassicbiostratigraphy[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/PaleontologySinemurianMexico[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
researchProduct

Deux ammonites turoniennes rares du Tuffeau de Saumur (Maine-et-Loire) : Romaniceras (Romaniceras) kallesi badilleti subsp. nov. et Romaniceras (Yuba…

2009

10 pages; National audience

ammonitesbassin de Paris[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/Paleontology[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/PaleontologystratotypeComputingMilieux_MISCELLANEOUSTuronien[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
researchProduct

Toll signal transduction pathway in bivalves: Complete cds of intermediate elements and related gene transcription levels in hemocytes of immune stim…

2014

Based on protein domain structure and organization deduced from mRNA contigs, 15 transcripts of the Toll signaling pathway have been identified in the bivalve, Mytilus galloprovincialis. Identical searches performed on publicly available Mytilus edulis ESTs revealed 11 transcripts, whereas searches performed in genomic and new transcriptome sequences of the Pacific oyster, Crassostrea gigas, identified 21 Toll-related transcripts. The remarkable molecular diversity of TRAF and IKK coding sequences of C. gigas, suggests that the sequence data inferred from Mytilus cDNAs may not be exhaustive. Most of the Toll pathway genes were constitutively and ubiquitously expressed in M. galloprovinciali…

animal structuresMolluskToll signaling pathwayInnate immunity; Mollusks; Mytilus; Signal transduction; Toll pathway; NF-κBImmunologyProtein domainSettore BIO/05 - ZoologiaMytiluSignal transductionNF-κBTranscriptomeTranscription (biology)Animals[SDU.STU.HY]Sciences of the Universe [physics]/Earth Sciences/HydrologyGenePhylogenyComputingMilieux_MISCELLANEOUSMytilusInnate immunityMessenger RNAInnate immune systemMollusksToll-like receptors; signal transduction; Mytilus-galloprovincialis Lmk (bivalvia)biologyEcologyfungiMytilus-galloprovincialis Lmk (bivalvia)biology.organism_classificationMytilusToll-like receptorsCell biologyInnate immunity; Mollusks; Mytilus; NF-κB; Signal transduction; Toll pathwayToll pathwayNF-jBDevelopmental Biology
researchProduct

1400 years of man-environment interactions and soil evolution in the Saint-Mont mountain (Remiremont, Vosges)

2021

International audience; The SolHoM(a) project aims at determining the degree of landscape anthropisation in the Fossard massif (Remiremont, Vosges, France) by estimating the impact of past human occupations on current soils. Nowadays, a forest covers this relatively inhospitable mountain (hard climate, steep slopes, acid soils ...), but some remains suggest human presence for at least 1400 years.The Saint-Mont is a variscan orogenic granitic summit (height 672m) with valuable preserved archaeological relics, located south of the Fossard. At the top was founded the monasterium Habendum (from the 7th century to the French Revolution), which potentially comes after a late-antic castrum.Further…

anthropisation gradientgeographers[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SDU.STU.GM] Sciences of the Universe [physics]/Earth Sciences/Geomorphologypedology[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and PrehistoryLiDAR data analysissteep slopes[SDV.SA.SDS]Life Sciences [q-bio]/Agricultural sciences/Soil studyarchaeologists[SDE.ES]Environmental Sciences/Environmental and Society[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environmentarcheologyA relatively inhospitable mountain: -hard climate-nowadays covered by forests. Joint work involving soil scientists[SDE.ES] Environmental Sciences/Environmental and Society[SDU.STU.GM]Sciences of the Universe [physics]/Earth Sciences/Geomorphology[SDV.SA.SDS] Life Sciences [q-bio]/Agricultural sciences/Soil studygeologists and computer scientists[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environmentVosges mountains-on acid soils developed from a granitic rock
researchProduct

A multivariate approach of the factors impacting a small arctic glacier, Austre Lovén-Spitsberg

2015

International audience; Arctic glaciers are good indicators of the ongoing climate change as their dynamics are strongly linked to it. This study is focused on the Austre Lovén glacier, on the Brøgger peninsula in Spitsbergen (Svalbard, 79°N). The aim is to understand how contrasted climate and snow conditions over the course of a year can lead to multiple consequences, sometimes unexpected, on mass balance. In 2014, a negative budget was expected, but data analysis has shown the first positive mass balance in 7 years. The objective here is to (i) identify and qualify the combination of factors affecting an arctic glacier mass balance. Three primary indicators seem to display the greatest i…

arctic glaciermultivariate statistics[SHS.GEO] Humanities and Social Sciences/Geography[ SDU.STU.GL ] Sciences of the Universe [physics]/Earth Sciences/Glaciology[SDU.STU] Sciences of the Universe [physics]/Earth Sciences[SDU.STU]Sciences of the Universe [physics]/Earth Sciences[ SDU.STU ] Sciences of the Universe [physics]/Earth Sciences[SHS.GEO]Humanities and Social Sciences/Geography[SDU.STU.GL]Sciences of the Universe [physics]/Earth Sciences/GlaciologyComputingMilieux_MISCELLANEOUSmass balance[ SHS.GEO ] Humanities and Social Sciences/Geography[SDU.STU.GL] Sciences of the Universe [physics]/Earth Sciences/Glaciology
researchProduct

The Gaia-ESO Survey: The origin and evolution of s-process elements

2018

Context. Several works have found an increase of the abundances of the s-process neutron-capture elements in the youngest Galactic stellar populations. These trends provide important constraints on stellar and Galactic evolution and they need to be confirmed with large and statistically significant samples of stars spanning wide age and distance intervals. Aims. We aim to trace the abundance patterns and the time evolution of five s-process elements - two belonging to the first peak, Y and Zr, and three belonging to the second peak, Ba, La, and Ce - using the Gaia-ESO IDR5 results for open clusters and disc stars. Methods. From the UVES spectra of cluster member stars, we determined the ave…

astro-ph.GAMetallicityFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: diskAstronomi astrofysik och kosmologiAbundance (ecology)QB4600103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsDisc010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsPhysicsgeneral [Open clusters and associations][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsOpen clusters and associations: generalAstrophysics - Astrophysics of GalaxiesStarsAbundances [Galaxy][SDU]Sciences of the Universe [physics]13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesAstrophysics::Earth and Planetary AstrophysicsDisk [Galaxy]s-processOpen cluster
researchProduct

The Gaia-ESO Survey: Structural and dynamical properties of the young cluster Chamaeleon i

2017

Investigating the physical mechanisms driving the dynamical evolution of young star clusters is fundamental to our understanding of the star formation process and the properties of the Galactic field stars. The young (~2 Myr) and partially embedded cluster Chamaeleon I is one of the closest laboratories for the study of the early stages of star cluster dynamics in a low-density environment. The aim of this work is to study the structural and kinematical properties of this cluster combining parameters from the high-resolution spectroscopic observations of the Gaia-ESO Survey with data from the literature. Our main result is the evidence of a large discrepancy between the velocity dispersion …

astro-ph.SRStellar populationopen clustersand associations: individual: Chamaeleon IIndividual: Chamaeleon I [Open clusters and associations]Open clusters and associations: Individual: Chamaeleon I; Stars: Kinematics and dynamics; Stars: Pre-main sequence; Techniques: Spectroscopicastro-ph.GAstars: kinematics and dynamicsFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstars: pre-main sequence01 natural sciencesVirial theoremKinematics and dynamics [Stars]Stars: Kinematics and dynamic0103 physical sciencesCluster (physics)Mass segregationAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsStellar evolutionQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBPhysicsPre-main sequence [Stars]open clusters and associations: individual: Chamaeleon I010308 nuclear & particles physicsVelocity dispersionAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxies[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]stars: kinematics and dynamics; stars: pre-main sequence; open clustersand associations: individual: Chamaeleon I; techniques: spectroscopicStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics::Earth and Planetary AstrophysicsSpectroscopic [Techniques]Equivalent widthtechniques: spectroscopicQB799
researchProduct

L'Oscillation de Madden-Julian et la variabilité pluviométrique régionale en Afrique Subsaharienne

2007

The role of the Madden-Julian Oscillation ("MJO") on rainfall variability in Sub-Saharan Africa is examined, based on daily rain-gauge records and the NCEP-DOE AMIP-II reanalyses. The convective and dynamical signal associated with the MJO is extracted using two differing methodologies, the BMRC daily indices (Wheeler & Hendon 2004) on the one hand, and a Local Mode Analysis ("LMA", Goulet & Duvel 2000) on the other hand. The temporal variability of the MJO (in terms of period, amplitude, seasonality and location of the convective anomalies) is first analysed. Though the overall amplitude of the signal is not related to El Niño, the oscillations occurring under El Niño (La Niña) conditions …

atmospheric <br />dynamicsintraseasonal variabilityinteractions d'échelleSub-Saharan Africavariabilité intrasaisonnièrerainfall<br />dynamique atmosphériqueclimate diagnosticAfrique Subsaharienne[SDU.STU.CL] Sciences of the Universe [physics]/Earth Sciences/Climatology[SDU.STU.CL]Sciences of the Universe [physics]/Earth Sciences/Climatologydiagnostic climatiqueMadden-Julian Oscillationpluviométriescale interactions[ SDU.STU.CL ] Sciences of the Universe [physics]/Earth Sciences/ClimatologyOscillation de Madden-Julian
researchProduct

The role of melt composition on aqueous fluid vs. silicate melt partitioning of bromine in magmas

2018

International audience; Volcanogenic halogens, in particular bromine, potentially play an important role in the ozone depletion of the atmosphere. Understanding bromine behaviour in magmas is therefore crucial to properly evaluate the contribution of volcanic eruptions to atmospheric chemistry and their environmental impact. To date, bromine partitioning between silicate melts and the gas phase is very poorly constrained, with the only relevant experimental studies limited to investigation of synthetic melt with silicic compositions. In this study, fluid/melt partitioning experiments were performed using natural silicate glasses with mafic, intermediate and silicic compositions. For each co…

atmospheric chemistry010504 meteorology & atmospheric sciencesbromine[SDU.STU]Sciences of the Universe [physics]/Earth SciencesSilicicarc magma010502 geochemistry & geophysics01 natural sciencesfluid/melt partitioningVolcanic Gaseschemistry.chemical_compoundGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)eventPetrologyGeophysic0105 earth and related environmental sciencesMelt inclusionsevent.disaster_typeBasaltAndesiteSettore GEO/07 - Petrologia E PetrografiadegassingSilicatearc magmasSettore GEO/08 - Geochimica E VulcanologiaGeophysicschemistry13. Climate actionSpace and Planetary ScienceMagmaMaficGeology
researchProduct