A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express

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A ground-to-exosphere Martian general circulation model: 2. Atmosphere during solstice conditions—Thermospheric polar warming

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An extremely high-altitude plume seen at Mars' morning terminator

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Analytical solution for waves in planets with atmospheric superrotation. I. Acoustic and inertia-gravity waves

Analytical solution for waves in planets with atmospheric superrotation. II. Lamb, surface, and centrifugal waves

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Antarctic polar descent and planetary wave activity observed in ISAMS CO from April to July 1992

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CO2 non-LTE limb emissions in Mars' atmosphere as observed by OMEGA/Mars Express

Dayside temperatures in the Venus upper atmosphere from Venus Express/VIRTIS nadir measurements at 4.3μm

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Global and seasonal variations in middle atmosphere CO from UARS/ISAMS

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Global atmospheric chemistry from satellites: results from UARS/ISAMS

Limb observations of CO2and CO non-LTE emissions in the Venus atmosphere by VIRTIS/Venus Express

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Local thermodynamic equilibrium of carbon dioxide in the upper atmosphere

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Mars environment and magnetic orbiter model payload

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Meteorological results from the Global Mars Multiscale Model at the Viking 1 lander site

Observations of non-LTE emission at 4–5 microns with the planetary Fourier spectrometer abord the Mars Express mission

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On the retrieval of mesospheric winds on Mars and Venus from ground-based observations at 10 {mu}m ⬇️

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Polar warming in the Mars thermosphere: Seasonal variations owing to changing insolation and dust distributions

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Reply to comment “On the hydrogen escape: Comment to variability of the hydrogen in the Martian upper atmosphere as simulated by a 3D atmosphere-exosphere coupling by J.-Y. Chaufray et al.” by V. Krasnopolsky, Icarus, 281, 262

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South-polar features on Venus similar to those near the north pole

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Study of the hydrogen escape rate at Mars during martian years 28 and 29 from comparisons between SPICAM/Mars express observations and GCM-LMD simulations ⬇️

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The Atmospheric Chemistry Suite (ACS) of Three Spectrometers for the ExoMars 2016 Trace Gas Orbiter

The EChO science case

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The Mars Climate Database (version 4.3)

The first Mars thermospheric general circulation model: The Martian atmosphere from the ground to 240 km

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Three-dimensional Martian ionosphere model: I. The photochemical ionosphere below 180 km

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Three-dimensional Martian ionosphere model: II. Effect of transport processes due to pressure gradients

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Variability of the Martian thermosphere during eight Martian years as simulated by a ground-to-exosphere global circulation model

Variability of the hydrogen in the martian upper atmosphere as simulated by a 3D atmosphere–exosphere coupling

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Venus's major cloud feature as an equatorially trapped wave distorted by the wind

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