3D Modeling of Moist Convective Inhibition in Idealized Sub-Neptune Atmospheres
Atmospheric convection behaves differently in hydrogen-rich atmospheres compared to higher mean molecular weight atmospheres due to compositional gradients of tracers.
Namrah Habib, Raymond T. Pierrehumbert
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Exoplanet Atmospheres at High Spectral Resolution
High-resolution spectroscopy (HRS) has grown into one of the main techniques for characterizing the atmospheres of extrasolar planets. High spectral resolving power allows for the efficient removal of telluric and host-star contamination. Combined with the large collecting area of ground-based telescopes, it enables detailed studies of atmospheric ...
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Towards Atmospheric Characterisation of Exoplanets
This thesis provides a multi-pronged approach towards paving the way for future space and ground based exoplanet characterisation e↵orts as well as providing new analysis of the atmosphere of the exoplanet HD 179949 b. This is done, firstly, by outlining engineering trade studies conducted for the attitude and orbit control system (AOCS) and sun shield
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ATMOSPHERE EXPANSION AND MASS LOSS OF CLOSE-ORBIT GIANT EXOPLANETS HEATED BY STELLAR XUV. II. EFFECTS OF PLANETARY MAGNETIC FIELD; STRUCTURING OF INNER MAGNETOSPHERE [PDF]
M. L. Khodachenko +3 more
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A Comprehensive Analysis of Spitzer 4.5 μm Phase Curves of Hot Jupiters
Although exoplanetary science was not initially projected to be a substantial part of the Spitzer mission, its exoplanet observations set the stage for current and future surveys with JWST and Ariel.
Lisa Dang +21 more
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Comparative Analysis of the Model for Exoplanet Atmosphere Outflow [PDF]
P. B. Isakova +3 more
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Methanol—A Poor Biosignature Gas in Exoplanet Atmospheres [PDF]
Jingcheng Huang +4 more
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Reassessing the Evidence for Time Variability in the Atmosphere of the Exoplanet HAT-P-7 b
Maura Lally, Andrew Vanderburg
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The carbon-to-oxygen ratio: implications for the spectra of hydrogen-dominated exoplanet atmospheres [PDF]
Benjamin Drummond +6 more
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