Study of atmospheres in the solar system, from stellar occultation or planetary transit
Stellar occultations and transits occur when a planetary body passes in front of a star (including our Sun). For objects with an atmosphere, refraction plays an essential role to explain the drops of flux and the aureoles observed during these events ...
Sicardy, Bruno
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Atmospheric Escape Processes and Planetary Atmospheric Evolution [PDF]
AbstractThe habitability of the surface of any planet is determined by a complex evolution of its interior, surface, and atmosphere. The electromagnetic and particle radiation of stars drive thermal, chemical, and physical alteration of planetary atmospheres, including escape.
Jared Bell+23 more
openaire +7 more sources
Exploring and Validating Exoplanet Atmospheric Retrievals with Solar System Analog Observations
Solar system observations that serve as analogs for exoplanet remote sensing data can provide important opportunities to validate ideas and models related to exoplanet environments.
Tyler D. Robinson, Arnaud Salvador
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A population study of gaseous exoplanets [PDF]
We present here the analysis of 30 gaseous extrasolar planets, with temperatures between 600 and 2400 K and radii between 0.35 and 1.9 $R_\mathrm{Jup}$. The quality of the HST/WFC3 spatially scanned data combined with our specialized analysis tools allow
Damiano, M.+10 more
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Equatorial Waves and Superrotation in the Stratosphere of a Titan General Circulation Model
We investigate the characteristics of equatorial waves associated with the maintenance of superrotation in the stratosphere of a Titan general circulation model.
Neil T. Lewis+3 more
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Joint Application of Concentration and δ18O to Investigate the Global Atmospheric CO Budget
Most previous top-down global carbon monoxide (CO) budget estimates have used only concentration information and shown large differences in individual source estimates.
Keyhong Park+3 more
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Ejected Particles after Impact Splash on Mars: Aggregates and Aerodynamics
Our earlier laboratory measurements showed that low-velocity sand impacts release fine
T. Becker+8 more
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Nightside Ionospheric Structure and Composition on Mars Driven by Energetic Electron Precipitation
Ionospheric chemistry plays an unexpectedly important role in the evolution of planetary habitability. This study is dedicated to a detailed modeling of the nightside Martian ionospheric structure and composition, a topic that has been poorly explored ...
Shiqi Wu+6 more
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The Hidden Depths of Planetary Atmospheres [PDF]
Abstract Atmospheric regions below a refractive boundary are hidden in limb observations. Refraction thus creates a gray continuum in the planet’s transmission spectrum, which can hide spectral features associated with sources of atmospheric opacity.
Yan Bétrémieux, Mark R. Swain
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The Inhomogeneity Effect. I. Inhomogeneous Surface and Atmosphere Accelerate Planetary Cooling
We propose a general principle that under radiative-convective equilibrium, the spatial and temporal variations in a planet’s surface and atmosphere tend to increase its cooling.
Xi Zhang
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