Search Results - "Eparvier, Frank"
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Photochemical escape of oxygen from Mars: First results from MAVEN in situ data
Published in Journal of geophysical research. Space physics (01-03-2017)“…Photochemical escape of atomic oxygen is thought to be one of the dominant channels for Martian atmospheric loss today and played a potentially major role in…”
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Ionizing Electrons on the Martian Nightside: Structure and Variability
Published in Journal of geophysical research. Space physics (01-05-2018)“…The precipitation of suprathermal electrons is the dominant external source of energy deposition and ionization in the Martian nightside upper atmosphere and…”
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Effects of a Solar Flare on the Martian Hot O Corona and Photochemical Escape
Published in Geophysical research letters (28-07-2018)“…We examine for the first time the flare‐induced effects on the Martian hot O corona. The rapid ionospheric response to the increase in the soft X‐ray flux…”
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MAVEN observations of dayside peak electron densities in the ionosphere of Mars
Published in Journal of geophysical research. Space physics (01-01-2017)“…The peak electron density in the dayside Martian ionosphere is a valuable diagnostic of the state of the ionosphere. Its dependence on factors like the solar…”
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Martian Bow Shock Oscillations Driven by Solar Wind Variations: Simultaneous Observations From Tianwen‐1 and MAVEN
Published in Geophysical research letters (28-08-2023)“…The Martian bow shock stands as the first defense against the solar wind and shapes the Martian magnetosphere. Previous studies showed the correlation between…”
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Modeling the ionospheric E and F1 regions: Using SDO-EVE observations as the solar irradiance driver
Published in Journal of geophysical research. Space physics (01-08-2013)“…ABSTRACTOver the altitude range of 90–150 km, in dayside nonauroral regions, ionization is controlled almost entirely by solar ultraviolet irradiance; the…”
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The SOLAR2000 empirical solar irradiance model and forecast tool
Published in Journal of atmospheric and solar-terrestrial physics (01-09-2000)“…SOLAR2000 is a collaborative project for accurately characterizing solar irradiance variability across the spectrum. A new image- and full-disk proxy empirical…”
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Characterizing Precipitation Behaviors of H− in the Martian Atmosphere
Published in Journal of geophysical research. Space physics (01-04-2024)“…Solar wind protons can charge exchange with the extensive hydrogen corona of Mars, resulting in a significant flux of energetic neutral atoms (ENAs). As these…”
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Observations and Modeling of the Mars Low‐Altitude Ionospheric Response to the 10 September 2017 X‐Class Solar Flare
Published in Geophysical research letters (16-08-2018)“…Solar extreme ultraviolet and X‐ray photons are the main sources of ionization in the Martian ionosphere and can be enhanced significantly during a solar…”
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First Synoptic Images of FUV Discrete Aurora and Discovery of Sinuous Aurora at Mars by EMM EMUS
Published in Geophysical research letters (28-08-2022)“…We present the first measurements of Mars discrete aurora in the extreme ultraviolet (<110 nm) and the first synoptic aurora images in the far ultraviolet…”
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The Hazard of UV-Induced Oxidation to Solar-Viewing Spacecraft Optics
Published in Solar physics (01-03-2023)“…The two most prevalent outgassing contaminants on spacecraft are organic molecules and water vapor. Adsorbed organic molecules can degrade a solar-viewing…”
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EMM EMUS Observations of Hot Oxygen Corona at Mars: Radial Distribution and Temporal Variability
Published in Journal of geophysical research. Space physics (01-03-2024)“…We present the first observations of the dayside coronal oxygen emission in far ultraviolet (FUV) measured by the Emirates Mars Ultraviolet Spectrometer (EMUS)…”
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Morphology of Extreme and Far Ultraviolet Martian Airglow Emissions Observed by the EMUS Instrument on Board the Emirates Mars Mission
Published in Geophysical research letters (16-10-2022)“…We present the first continuous observations of the extreme and far ultraviolet (EUV and FUV) dayglow emissions measured by Emirates Mars Ultraviolet…”
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Combined Analysis of Hydrogen and Oxygen 102.6 nm Emission at Mars
Published in Geophysical research letters (28-08-2022)“…Water is lost from the Mars upper atmosphere to space as hydrogen and oxygen, both of which can be observed in scattered ultraviolet sunlight at 102.6 nm. We…”
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Ionization Efficiency in the Dayside Ionosphere of Mars: Structure and Variability
Published in Journal of geophysical research. Planets (01-12-2021)“…Ionization efficiency, the ratio between photoelectron impact ionization and primary photoionization, is an important quantity from the perspective of…”
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Mars heavy ion precipitating flux as measured by Mars Atmosphere and Volatile EvolutioN
Published in Geophysical research letters (16-11-2015)“…In the absence of an intrinsic dipole magnetic field, Mars' O+ planetary ions are accelerated by the solar wind. Because of their large gyroradius, a…”
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New Solar Extreme-ultraviolet Irradiance Observations during Flares
Published in The Astrophysical journal (01-10-2011)“…New solar extreme-ultraviolet (EUV) irradiance observations from the NASA Solar Dynamics Observatory (SDO) EUV Variability Experiment provide full coverage in…”
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Ionospheric model-observation comparisons: E layer at Arecibo Incorporation of SDO-EVE solar irradiances
Published in Journal of geophysical research. Space physics (01-05-2014)“…This study evaluates how the new irradiance observations from the NASA Solar Dynamics Observatory (SDO) Extreme Ultraviolet Variability Experiment (EVE) can,…”
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NEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARES
Published in The Astrophysical journal (01-10-2011)“…New solar extreme-ultraviolet (EUV) irradiance observations from the NASA Solar Dynamics Observatory (SDO) EUV Variability Experiment provide full coverage in…”
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Solar Analogs as a Tool to Understand the Sun
Published 11-09-2020“…Solar analogs, broadly defined as stars similar to the Sun in mass or spectral type, provide a useful laboratory for exploring the range of Sun-like behaviors…”
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