Search results for "PAC"

showing 10 items of 28794 documents

Morphological Properties of Slender Ca ${\rm{II}}$ H Fibrils Observed by Sunrise II

2017

R. Gafeira et. al.

010504 meteorology & atmospheric sciencesFOS: Physical scienceschromosphere [Sun]AstrophysicsFibrilCurvature01 natural sciencesSponge spiculeObservatory0103 physical sciencesHigh spatial resolutionSunriseTechniques: imaging spectroscopySun: magnetic fields010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)Physicsimaging spectroscopy [Techniques]Sun: chromosphereAstronomy and Astrophysicsmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceThe Astrophysical Journal Supplement Series
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Bright Hot Impacts by Erupted Fragments Falling Back on the Sun: Magnetic Channelling

2016

Dense plasma fragments were observed to fall back on the solar surface by the Solar Dynamics Observatory after an eruption on 7 June 2011, producing strong EUV brightenings. Previous studies investigated impacts in regions of weak magnetic field. Here we model the $\sim~300$ km/s impact of fragments channelled by the magnetic field close to active regions. In the observations, the magnetic channel brightens before the fragment impact. We use a 3D-MHD model of spherical blobs downfalling in a magnetized atmosphere. The blob parameters are constrained from the observation. We run numerical simulations with different ambient density and magnetic field intensity. We compare the model emission i…

010504 meteorology & atmospheric sciencesField (physics)FOS: Physical sciencesAstrophysics01 natural sciencesAtmosphereSettore FIS/05 - Astronomia E AstrofisicaSun: activity0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetic pressureSun: magnetic field010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSun: coronaAstronomy and AstrophysicsSun: UV radiation Supporting material: animationPlasmaCoronal loopAstronomy and AstrophysicRam pressureMagnetic fieldStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space Physics
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A tale of two emergences: Sunrise II observations of emergence sites in a solar active region

2017

R. Centeno et. al.

010504 meteorology & atmospheric sciencesField (physics)photosphere [Sun]Field lineFOS: Physical sciencesFluxchromosphere [Sun]Astrophysicspolarimetric [Techniques]01 natural sciences0103 physical sciencesSunrise010303 astronomy & astrophysicsChromosphereSun: magnetic fieldsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSunspotsSun: chromosphereTechniques: polarimetricSun: photosphereAstronomy and AstrophysicsMagnetic reconnectionMagnetic fluxMagnetic fieldmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science
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Magnetic shuffling of coronal downdrafts

2017

Channelled fragmented downflows are ubiquitous in magnetized atmospheres, and have been recently addressed from an observation after a solar eruption. We study the possible back-effect of the magnetic field on the propagation of confined flows. We compare two 3D MHD simulations of dense supersonic plasma blobs downfalling along a coronal magnetic flux tube. In one, the blobs move strictly along the field lines; in the other, the initial velocity of the blobs is not perfectly aligned to the magnetic field and the field is weaker. The aligned blobs remain compact while flowing along the tube, with the generated shocks. The misaligned blobs are disrupted and merged by the chaotic shuffling of …

010504 meteorology & atmospheric sciencesField lineAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsSun:corona01 natural sciencesAlfvén waveSettore FIS/05 - Astronomia E AstrofisicaPhysics::Plasma Physics0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesPhysicsSolar flareAstronomy and AstrophysicsSun:activityPlasmaMagnetic fluxAccretion (astrophysics)Magnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsMagnetohydrodynamicsmagnetohydrodynamics
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Comment on “Rill erosion processes on steep colluvial deposit slope under heavy rainfall in flume experiments with artificial rain by F. Jiang et al.”

2020

Abstract Since rill flows are characterized by small water depths and steeply sloping channels, the corresponding hydraulic conditions are very different to those which are typically found in channels of streams and rivers. Furthermore, limited information is currently available on the effect of rainfall on flow resistance. The objective of this comment was to investigate the applicability of a recently theoretically deduced rill flow resistance equation, based on a power-velocity profile, using measurements carried out by Jiang et al. for both different slope steepness conditions and rainfall intensity. The relationship between the velocity profile parameter Γ, the channel slope and the fl…

010504 meteorology & atmospheric sciencesFlow (psychology)Soil scienceSTREAMSRill erosion01 natural sciencessymbols.namesakeRill velocityDarcy-Weisbach friction factorFroude number0105 earth and related environmental sciencesEarth-Surface ProcessesColluviumgeographyRill erosiongeography.geographical_feature_categoryRainfall impact04 agricultural and veterinary sciencesRillFlumeFlow resistance040103 agronomy & agriculturesymbols0401 agriculture forestry and fisheriesIntensity (heat transfer)Geology
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Astrometric detection of a low-mass companion orbiting the star AB Doradus

1997

International audience; We report submilliarcsecond-precise astrometric measurements for the late-type star AB Doradus via a combination of VLBI (very long baseline interferometry) and HIPPARCOS data. Our astrometric analysis results in the precise determination of the kinematics of this star, which reveals an orbital motion readily explained as caused by gravitational interaction with a low-mass companion. From the portion of the reÑex orbit covered by our data and using a revised mass of the primary star (0.76 M _) derived from our new value of the parallax (66.3 mas \ n \ 67.2 mas), we Ðnd the dynamical mass of the newly discovered companion to be between 0.08 and 0.11 If accurate photom…

010504 meteorology & atmospheric sciencesGalactic astronomyStellar massBrown dwarfAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesstars: low-mass0103 physical sciencesVery-long-baseline interferometryAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsstars: individual (AB Doradus)[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsAstrometryInterferometrySpace and Planetary Sciencetechniques: interferometricOrbital motionastrometryAstrophysics::Earth and Planetary Astrophysics[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]stars: kinematicsLow Massbrown dwarfs
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On the timing between terrestrial gamma ray flashes, radio atmospherics, and optical lightning emission

2017

On 25 October 2012 the Reuven Ramaty High Energy Solar Spectroscope Imager (RHESSI) and the Tropical Rainfall Measuring Mission (TRMM) satellites passed over a thunderstorm on the coast of Sri Lanka. RHESSI observed a terrestrial gamma ray flash (TGF) originating from this thunderstorm. Optical measurements of the causative lightning stroke were made by the lightning imaging sensor (LIS) on board TRMM. The World Wide Lightning Location Network (WWLLN) detected the very low frequency (VLF) radio emissions from the lightning stroke. The geolocation from WWLLN, which we also assume is the TGF source location, was in the convective core of the cloud. By using new information about both RHESSI a…

010504 meteorology & atmospheric sciencesGamma rayFOS: Physical sciencesRadio atmosphericLight curve01 natural sciencesLightningSpace Physics (physics.space-ph)GeophysicsPhysics - Space PhysicsSpace and Planetary Science0103 physical sciencesThunderstormEnvironmental scienceAtmosphericsVery low frequencyAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics0105 earth and related environmental sciencesTerrestrial gamma-ray flashRemote sensingJournal of Geophysical Research: Space Physics
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Could CoRoT-7b and Kepler-10b be remnants of evaporated gas or ice giants?

2009

We present thermal mass loss calculations over evolutionary time scales for the investigation if the smallest transiting rocky exoplanets CoRoT-7b (∼1.68REarth) and Kepler-10b (∼1.416REarth) could be remnants of an initially more massive hydrogen-rich gas giant or a hot Neptune-class exoplanet. We apply a thermal mass loss formula which yields results that are comparable to hydrodynamic loss models. Our approach considers the effect of the Roche lobe, realistic heating efficiencies and a radius scaling law derived from observations of hot Jupiters. We study the influence of the mean planetary density on the thermal mass loss by placing hypothetical exoplanets with the characteristics of Jup…

010504 meteorology & atmospheric sciencesGas giantEvolutionAstrophysics01 natural sciencesArticleOriginPlanet0103 physical sciencesHot JupiterAstrophysics::Solar and Stellar AstrophysicsHot NeptuneKepler-10b010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsExoplanetsAstronomyAstronomy and AstrophysicsExoplanetCoRoT-7b13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsMass lossPlanetary massJupiter massIce giantPlanetary and Space Science
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Carbon isotope composition of CO2-rich inclusions in cumulate-forming mantle minerals from Stromboli volcano (Italy)

2017

We report on measurements of concentration and carbon isotope composition (δ13CCO2) of CO2 trapped in fluid inclusions of olivine and clinopyroxene crystals separated from San Bartolo ultramafic cumulate Xenoliths (SBX) formed at mantle depth (i.e., beneath a shallow Moho supposed to be at 14.8 km). These cumulates, erupted about 2 ka ago at Stromboli volcano (Italy), have been already investigated by Martelli et al. (2014) mainly for Sr-Nd isotopes and for their noble gases geochemistry. The concentration of CO2 varies of one order of magnitude from 3.8·10− 8 mol g− 1 to 4.8·10− 7 mol g− 1, with δ13C values between − 2.8‰ and − 1.5‰ vs V-PDB. These values overlap the range of measurements …

010504 meteorology & atmospheric sciencesGeochemistryUltramafic cumulateengineering.material010502 geochemistry & geophysics01 natural sciencesMantle (geology)Impact craterUltramafic rockGeochemistry and PetrologyFluid inclusionsXenolith0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryOlivineδ13CSettore GEO/07 - Petrologia E PetrografiaStromboli volcanoFluid inclusionGeophysicsVolcanoengineeringδ13CCO2MantleGeology
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The impact of degassing on the oxidation state of basaltic magmas: A case study of Kīlauea volcano

2016

Volcanic emissions link the oxidation state of the Earth's mantle to the composition of the atmosphere. Whether the oxidation state of an ascending magma follows a redox buffer – hence preserving mantle conditions – or deviates as a consequence of degassing remains under debate. Thus, further progress is required before erupted basalts can be used to infer the redox state of the upper mantle or the composition of their co-emitted gases to the atmosphere. Here we present the results of X-ray absorption near-edge structure (XANES) spectroscopy at the iron K-edge carried out for a series of melt inclusions and matrix glasses from ejecta associated with three eruptions of Kīlauea volcano (Hawai…

010504 meteorology & atmospheric sciencesGeochemistrysub-05010502 geochemistry & geophysicsmelt inclusions01 natural sciencesMantle (geology)Mineral redox bufferOxidation stateGeochemistry and PetrologyHotspot (geology)Earth and Planetary Sciences (miscellaneous)EjectaGeophysic0105 earth and related environmental sciencesMelt inclusionsBasaltgeographygeography.geographical_feature_categorymelt inclusiondegassingoxygen fugacityXANESGeophysicsVolcanoSpace and Planetary SciencesulfurCO2Geology
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