Venusian ion escape under extreme conditions: A dynamic pressure and temperature simulation study

Context . We investigated the response of the Venusian atmospheric ion escape under the effect of interplanetary coronal mass ejections (ICMEs) using the Latmos Hybrid Simulation (LatHyS). Aims . In particular, we focused on the influence of extreme ICME dynamic pressures and temperatures, with the temperature being a parameter that has not been extensively studied in the past. Methods . Simulations were performed for two different dynamic pressures and three different temperatures. For the case of the dynamic pressure simulations, a density and a velocity enhancement event were studied separately. The H + and O + ion escape was then examined and compared for different escape channels. Results . In both dynamic pressure enhancement cases, we find that there is no clear dependence of the O + ion escape on the dynamic pressure, which is consistent with observations. On the other hand, the temperature of the incoming solar wind positively influences the H + and O + ion escape. This is attributed in part to the enhanced gyroradius of the particles, which allows them to penetrate deeper into the planet’s atmosphere.

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Publication Details

Journal
Astronomy and Astrophysics
Published
2024-10-14
DOI
https://doi.org/10.1051/0004-6361/202449326
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
0.00

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article

Venusian ion escape under extreme conditions: A dynamic pressure and temperature simulation study

Maria Chloi Katrougkalou, R. Modolo, Tomas Karlsson, Moa Persson et al.
Astronomy and Astrophysics
Planetary Science and Exploration
article

Venusian ion escape under extreme conditions: A dynamic pressure and temperature simulation study

Maria Chloi Katrougkalou, R. Modolo, Tomas Karlsson, Moa Persson, Anita Kullen, Erwan Jariel, Sae Aizawa, Nicolás André
article en

Abstract

Context . We investigated the response of the Venusian atmospheric ion escape under the effect of interplanetary coronal mass ejections (ICMEs) using the Latmos Hybrid Simulation (LatHyS). Aims . In particular, we focused on the influence of extreme ICME dynamic pressures and temperatures, with the temperature being a parameter that has not been extensively studied in the past. Methods . Simulations were performed for two different dynamic pressures and three different temperatures. For the case of the dynamic pressure simulations, a density and a velocity enhancement event were studied separately. The H + and O + ion escape was then examined and compared for different escape channels. Results . In both dynamic pressure enhancement cases, we find that there is no clear dependence of the O + ion escape on the dynamic pressure, which is consistent with observations. On the other hand, the temperature of the incoming solar wind positively influences the H + and O + ion escape. This is attributed in part to the enhanced gyroradius of the particles, which allows them to penetrate deeper into the planet’s atmosphere.

Astronomy and AstrophysicsVol. 691
Centre National de la Recherche Scientifique (FR), Swedish Institute of Space Physics (SE), Université Toulouse III - Paul Sabatier (FR), Université Fédérale de Toulouse Midi-Pyrénées (FR), Institut Superieur de l'Aeronautique et de l'Espace (ISAE-SUPAERO) (FR), Université de Versailles Saint-Quentin-en-Yvelines (FR), Université Paris-Saclay (FR), Sorbonne Université (FR), Institut Pierre-Simon Laplace (FR), National Sagamihara Hospital (JP), Thales (France) (FR), Laboratoire de Physique des Plasmas (FR), Laboratoire atmosphères, milieux, observations spatiales (FR), KTH Royal Institute of Technology (SE)
European Commission, Centre National d’Etudes Spatiales, Japan Society for the Promotion of Science
Openalex Percentile: Top 87%
Planetary Science and Exploration
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