Articles | Volume 37, issue 5
https://doi.org/10.5194/angeo-37-989-2019
https://doi.org/10.5194/angeo-37-989-2019
Regular paper
 | 
28 Oct 2019
Regular paper |  | 28 Oct 2019

Solar cycle, seasonal, and asymmetric dependencies of thermospheric mass density disturbances due to magnetospheric forcing

Andres Calabia and Shuanggen Jin

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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) (08 Aug 2019) by Mirko Piersanti
AR by Andres Calabia Aibar on behalf of the Authors (08 Sep 2019)  Author's response   Manuscript 
ED: Publish subject to revisions (further review by editor and referees) (09 Sep 2019) by Mirko Piersanti
ED: Publish as is (27 Sep 2019) by Mirko Piersanti
AR by Andres Calabia Aibar on behalf of the Authors (30 Sep 2019)  Manuscript 
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Short summary
Atmospheric drag due to mass density distribution, particularly during storm-time, is of great importance for low Earth orbit precise orbit determination, and for the understanding of magnetosphere–ionosphere–thermosphere phenomena. In this paper, we investigate solar cycle, seasonal, and hemispheric asymmetry dependencies of thermospheric mass density disturbances due to magnetospheric forcing, from 10-year (2003–2013) continuous time series of GRACE estimates.