The Impact of Radial and Non‐Radial IMF on the Earth's Magnetopause Size, Shape, and Dawn‐Dusk Asymmetry From Global 3D Kinetic Simulations-Reference-Cited by-同舟云学术

The Impact of Radial and Non‐Radial IMF on the Earth's Magnetopause Size, Shape, and Dawn‐Dusk Asymmetry From Global 3D Kinetic Simulations

Published:2021-10 Issue:10 Volume:126 Page:
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Baraka Suleiman M.¹²^ORCID,Le Contel Olivier²^ORCID,Ben‐Jaffel Lotfi³^ORCID,Moore William B.¹⁴^ORCID

Affiliation:

1. National Institute of Aerospace Hampton VA USA

2. Laboratoire de Physique des Plasmas UMR7648 CNRS/Sorbonne Université/Université Paris‐Saclay/Observatoire de Paris/Ecole Polytechnique Institut Polytechnique de Paris Palaiseau France

3. Institut d'Astrophysique de Paris Sorbonne Universités UPMC & CNRS Paris France

4. Hampton University Hampton VA USA

Funder

Centre National d’Etudes Spatiales

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2021JA029528

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4. Outward flow of protons from the Earth's bow shock

5. Large Scale Earth’s Bow Shock with Northern IMF as Simulated by PIC Code in Parallel with MHD Model

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