Articles | Volume 37, issue 5
https://doi.org/10.5194/angeo-37-791-2019
https://doi.org/10.5194/angeo-37-791-2019
Regular paper
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10 Sep 2019
Regular paper | Highlight paper |  | 10 Sep 2019

Hybrid-Vlasov modelling of nightside auroral proton precipitation during southward interplanetary magnetic field conditions

Maxime Grandin, Markus Battarbee, Adnane Osmane, Urs Ganse, Yann Pfau-Kempf, Lucile Turc, Thiago Brito, Tuomas Koskela, Maxime Dubart, and Minna Palmroth

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AR: Author's response | RR: Referee report | ED: Editor decision
ED: Publish subject to revisions (further review by editor and referees) (26 Jul 2019) by Anna Milillo
AR by Maxime Grandin on behalf of the Authors (29 Jul 2019)  Author's response   Manuscript 
ED: Referee Nomination & Report Request started (31 Jul 2019) by Anna Milillo
RR by Anonymous Referee #2 (01 Aug 2019)
RR by Anonymous Referee #1 (16 Aug 2019)
ED: Publish as is (19 Aug 2019) by Anna Milillo
AR by Maxime Grandin on behalf of the Authors (19 Aug 2019)
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Short summary
When the terrestrial magnetic field is disturbed, particles from the near-Earth space can precipitate into the upper atmosphere. This work presents, for the first time, numerical simulations of proton precipitation in the energy range associated with the production of aurora (∼1–30 keV) using a global kinetic model of the near-Earth space: Vlasiator. We find that nightside proton precipitation can be regulated by the transition region between stretched and dipolar geomagnetic field lines.