Modeling the Impact of a Strong X‐Class Solar Flare on the Planetary Ion Composition in Mercury's Magnetosphere-Reference-Cited by-同舟云学术

Modeling the Impact of a Strong X‐Class Solar Flare on the Planetary Ion Composition in Mercury's Magnetosphere

Published:2022-02-05 Issue:3 Volume:49 Page:
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophysical Research Letters

Author:

Werner A. L. E.¹²^ORCID,Leblanc F.¹^ORCID,Chaufray J. Y.³^ORCID,Modolo R.³^ORCID,Aizawa S.⁴^ORCID,Hadid L. Z.⁵,Baskevitch C.³^ORCID

Affiliation:

1. LATMOS/IPSL Sorbonne Université CNRS UVSQ Paris France

2. Now at Swedish Institute of Space Physics Uppsala Sweden

3. LATMOS/IPSL UVSQ Université Paris–Saclay Sorbonne Université CNRS Guyancourt France

4. IRAP Toulouse France

5. Laboratoire de Physique des Plasmas (LPP) CNRS Observatoire de Paris Sorbonne Université Université Paris Saclay Ecole Polytechnique Institut Polytechnique de Paris Paris France

Funder

Agence Nationale de la Recherche

Centre National d’Etudes Spatiales

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021GL096614

Reference68 articles.

1. Cross-comparison of global simulation models applied to Mercury’s dayside magnetosphere

2. The Global Magnetic Field of Mercury from MESSENGER Orbital Observations

3. The Energetic Particle and Plasma Spectrometer Instrument on the MESSENGER Spacecraft

4. The Topology and Evolution of the Bastille Day Flare

5. Ionospheric Response to the X9.3 Flare on 6 September 2017 and Its Implication for Navigation Services Over Europe

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