Search results for " planetary"

showing 10 items of 5408 documents

Coralline alga reveals first marine record of subarctic North Pacific climate change

2007

[1] While recent changes in subarctic North Pacific climate had dramatic effects on ecosystems and fishery yields, past climate dynamics and teleconnection patterns are poorly understood due to the absence of century-long high-resolution marine records. We present the first 117-year long annually resolved marine climate history from the western Bering Sea/Aleutian Island region using information contained in the calcitic skeleton of the long-lived crustose coralline red alga Clathromorphum nereostratum, a previously unused climate archive. The skeletal δ18O-time series indicates significant warming and/or freshening of surface waters after the middle of the 20th century. Furthermore, the ti…

010504 meteorology & atmospheric sciencesOceanic climateClimate change010502 geochemistry & geophysics01 natural sciencesSubarctic climateNorth Pacific OscillationGeophysicsGeographyOceanography13. Climate actionClimatologyGeneral Earth and Planetary SciencesEcosystem14. Life underwaterCrustosePacific decadal oscillation0105 earth and related environmental sciencesTeleconnectionGeophysical Research Letters
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Flares from small to large: X-ray spectroscopy of Proxima Centauri with XMM-Newton

2003

(Abridged) We report results from a comprehensive study of the nearby M dwarf Proxima Centauri with the XMM-Newton satellite. We find strongly variable coronal X-ray emission, with flares ranging over a factor of 100 in peak flux. The low-level emission is found to be continuously variable. Several weak flares are characteristically preceded by an optical burst, compatible with predictions from standard solar flare models. We propose that the U band bursts are proxies for the elusive stellar non-thermal hard X-ray bursts suggested from solar observations. A very large X-ray flare was observed in its entirety, with a peak luminosity of 3.9E28 erg/s [0.15-10 keV] and a total X-ray energy of 1…

010504 meteorology & atmospheric sciencesOpacityAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural scienceslaw.inventionLuminositylaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsstars: activity stars: coronae stars: individual: Proxima Centauri X-rays: starsSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsSolar flareAstrophysics (astro-ph)Astronomy and AstrophysicsPlasma3. Good healthStars13. Climate actionSpace and Planetary SciencePhysics::Space PhysicsAstrophysics::Earth and Planetary AstrophysicsFlare
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GJ 357 b: A Super-Earth Orbiting an Extremely Inactive Host Star

2020

Aims. In this paper we present a deep X-ray observation of the nearby M dwarf GJ 357 and use it to put constraints on the atmospheric evolution of its planet, GJ 357 b. We also analyse the systematic errors in the stellar parameters of GJ 357 in order to see how they affect the perceived planetary properties. Methods. By comparing the observed X-ray luminosity of its host star, we estimate the age of GJ 357 b as derived from a recent XMM-Newton observation (log Lx [erg s-1] = 25.73), with Lx-age relations for M dwarfs. We find that GJ 357 presents one of the lowest X-ray activity levels ever measured for an M dwarf, and we put a lower limit on its age of 5 Gyr. Using this age limit, we perf…

010504 meteorology & atmospheric sciencesOpacityFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciencesLuminosityPlanet0103 physical sciences010303 astronomy & astrophysicsstars [X rays]Solar and Stellar Astrophysics (astro-ph.SR)physical evolution [Planets and satellites]0105 earth and related environmental sciencesEnvelope (waves)PhysicsEarth and Planetary Astrophysics (astro-ph.EP)Secondary atmosphereSuper-EarthAstronomy and AstrophysicsRadiusPlanet star interactionsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary Scienceterrestrial planets [Planets and satellites]atmospheres [Planets and satellites]Astrophysics - Earth and Planetary Astrophysics
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ARES. III. Unveiling the Two Faces of KELT-7 b with HST WFC3

2020

We present the analysis of the hot-Jupiter KELT-7b using transmission and emission spectroscopy from the Hubble Space Telescope (HST), both taken with the Wide Field Camera 3 (WFC3). Our study uncovers a rich transmission spectrum which is consistent with a cloud-free atmosphere and suggests the presence of H2O and H-. In contrast, the extracted emission spectrum does not contain strong absorption features and, although it is not consistent with a simple blackbody, it can be explained by a varying temperature-pressure profile, collision induced absorption (CIA) and H-. KELT-7 b had also been studied with other space-based instruments and we explore the effects of introducing these additiona…

010504 meteorology & atmospheric sciencesOpacityFOS: Physical sciencesEFFICIENTTransmission spectroscopy; Exoplanet atmospheres; Astronomy data analysisAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstronomy & Astrophysics01 natural sciencesAtmosphereHubble space telescope0103 physical sciencesTransmission spectroscopyEMISSION-SPECTRUMWATERBlack-body radiationEmission spectrumAbsorption (electromagnetic radiation)010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsScience & TechnologyHOT JUPITERSAstronomy and AstrophysicsBIASESEXOPLANETSTransmission (telecommunications)13. Climate actionSpace and Planetary SciencePhysical SciencesAstronomy data analysisHD 209458BAstrophysics::Earth and Planetary AstrophysicsATMOSPHERESWide Field Camera 3Astrophysics - Earth and Planetary AstrophysicsExoplanet atmospheresThe Astronomical Journal
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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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Radiogenic isotopes: new tools help reconstruct paleocean circulation and erosion input

2001

Ocean and atmosphere circulation and continental weathering regimes have undergone great changes over thousands of years as well as tens of millions of years. During the glacial stages of the Pleistocene, ocean circulation was generally more sluggish and deep water circulation in the Atlantic had a shallower flow. At the same time, weathering on the continents was enhanced by glacial erosion, particularly in high northern latitudes, which increased the input of erosional detritus into the ocean. In addition, atmospheric pressure gradients were larger, leading to higher wind speeds and increased supply of aeolian dust to the ocean. Prior to the onset of Northern Hemisphere glaciation and pro…

010504 meteorology & atmospheric sciencesPleistoceneNorth Atlantic Deep WaterOcean currentPhysical oceanography010502 geochemistry & geophysics01 natural sciencesOceanographyShutdown of thermohaline circulation13. Climate actionInterglacialGeneral Earth and Planetary SciencesThermohaline circulationGlacial periodGeology0105 earth and related environmental sciencesEOS
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Active tectonics along the south east offshore margin of Mt. Etna: New insights from high-resolution seismic profiles

2018

The offshore margin of Mt. Etna has been shaped by Middle Pleistocene to Holocene shortening and extension and, more recently, by gravity-related sliding of the volcanic edifice. These processes have acted contemporaneously although the gravitational component largely prevails over the tectonic one. In order to investigate this issue, we focused on the main role of active tectonics along the south-eastern offshore of Mt. Etna by means of marine high-resolution seismic data. Seismic profiles revealed post-220 ka sedimentary deposits unconformably overlaying the Lower-Middle Pleistocene Etnean clayey substratum and volcanics of the Basal Tholeiitic phase and the Timpe phase. Offshore Aci Trez…

010504 meteorology & atmospheric sciencesPleistoceneSettore GEO/02 - Geologia Stratigrafica E SedimentologicaSettore GEO/03 - Geologia Strutturaleactive tectonics010502 geochemistry & geophysics01 natural sciencesSicilian thrust-beltPaleontologyActive tectonicActive tectonics; Ionian Sea; Mt. Etna; Seismic investigation; Sicilian thrust-belt; Earth and Planetary Sciences (all)Seismic investigationHolocene0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryContinental shelfMt. Etnalcsh:QE1-996.5Fold (geology)Ionian SeaMt. Etna; seismic investigation; active tectonics; Sicilian thrust-belt; Ionian SeaSeafloor spreadingVolcanic rocklcsh:GeologyTectonicsGeneral Earth and Planetary SciencesSedimentary rockEarth and Planetary Sciences (all)Geology
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Plio-Pleistocene Dust Traps on Paleokarst Surfaces: A Case Study From the Carpathian Basin

2020

Plio-Pleistocene silt/clay-rich deposits and paleo-karst fissure sediments from sites of the northern and southern parts of the Carpathian Basin were investigated. These materials were supposed to be mixed during transport before being captured in karstified fissures. Evidence that the eolian fissure sediments of Plio-Pleistocene age in the older Triassic–Cretaceous limestones are derived from eolian silt and clay includes compositional and textural matches, especially decreasing grain-size trends observed downwards from the paleo-surface of the former landscape. Various environmental factors could be recognized by the statistical evaluation of grain-size distribution curves of fissure fill…

010504 meteorology & atmospheric sciencesPlioceneGeochemistryWeatheringclaySiltkarst010502 geochemistry & geophysics01 natural sciencesPaleosolPleistocenepaleosolLoessAeolian processesGeneral Earth and Planetary Scienceslcsh:QParent rockSiltstoneeolian sedimentationlcsh:ScienceSediment transportCarpathian basinGeology0105 earth and related environmental sciencesFrontiers in Earth Science
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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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