J. Gérard

发表

Characteristics of Mars UV Dayglow Emissions From Atomic Oxygen at 130.4 and 135.6 nm: MAVEN/IUVS Limb Observations and Modeling

J. Gérard, N. Schneider, S. Jain, 2019, Journal of Geophysical Research: Space Physics.

Ion outflow observed by IMAGE: Implications for source regions and heating mechanisms

Stephen B. Mende, Peter Wurz, Thomas E. Moore, 2001 .

Quantifying the Electron Energy of Mars Aurorae Through the Oxygen Emission Brightness Ratio at 130.4 and 135.6 nm

J. Deighan, L. Soret, S. Jain, 2024, Journal of Geophysical Research: Planets.

The Ultraviolet Martian Dayglow Observed With NOMAD/UVIS on ExoMars Trace Gas Orbiter

A. Vandaele, I. Thomas, N. Schneider, 2023, Journal of Geophysical Research: Planets.

The O(1S) 297.2‐nm Dayglow Emission: A Tracer of CO2 Density Variations in the Martian Lower Thermosphere

N. Schneider, S. Jain, S. Jain, 2018, Journal of Geophysical Research: Planets.

Observations of the Proton Aurora on Mars With SPICAM on Board Mars Express

F. Montmessin, B. Hubert, L. Rodriguez, 2017 .

Discrete Aurora at Mars: Dependence on Upstream Solar Wind Conditions

J. Halekas, J. Deighan, T. Weber, 2022, Journal of geophysical research. Space physics.

Airglow and Aurora in the Martian Atmosphere: Contributions by the Mars Express and ExoMars TGO Missions

F. Montmessin, J. Chaufray, F. González-Galindo, 2024, Space Science Reviews.

The Largest Electron Differential Energy Flux Observed at Mars by the Mars Express Spacecraft, 2004–2016

J. Gérard, S. Barabash, M. Holmström, 2018, Journal of geophysical research. Space physics.

A case study on the impact of interplanetary coronal mass ejection on the Martian O(1S) 557.7 nm dayglow emission using ExoMars TGO/NOMAD-UVIS observations: First Results

A. Vandaele, L. Soret, S. Sarkhel, 2024, 2408.01045.