Comparison of Empirical and Theoretical Models of the Thermospheric Density Enhancement During the 3–4 February 2022 Geomagnetic Storm

Author:

He Jianhui123ORCID,Astafyeva Elvira2ORCID,Yue Xinan13ORCID,Pedatella Nicholas M.4ORCID,Lin Dong4ORCID,Fuller‐Rowell Timothy J.56,Fedrizzi Mariangel56ORCID,Codrescu Mihail56,Doornbos Eelco7ORCID,Siemes Christian8ORCID,Bruinsma Sean9ORCID,Pitout Frederic10ORCID,Kubaryk Adam56

Affiliation:

1. Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China

2. Université Paris Cité Institut de Physique du Globe de Paris (IPGP) CNRS UMR 7154 Paris France

3. College of Earth and Planetary Sciences University of Chinese Academy of Sciences Beijing China

4. High Altitude Observatory National Center for Atmospheric Research Boulder CO USA

5. NOAA Space Weather Prediction Center Boulder CO USA

6. Cooperative Institute for Research in Environmental Sciences University of Colorado Boulder Boulder CO USA

7. Koninklijk Nederlands Meteorologisch Instituut De Bilt The Netherlands

8. Delft University of Technology Delft The Netherlands

9. GET/CNES Space Geodesy Office Toulouse France

10. Institut de Recherche en Astrophysique et Planétologie (IRAP) Toulouse France

Abstract

AbstractOn 3 February 2022, at 18:13 UTC, SpaceX launched and a short time later deployed 49 Starlink satellites at an orbit altitude between 210 and 320 km. The satellites were meant to be further raised to 550 km. However, the deployment took place during the main phase of a moderate geomagnetic storm, and another moderate storm occurred on the next day. The resulting increase in atmospheric drag led to 38 out of the 49 satellites reentering the atmosphere in the following days. In this work, we use both observations and simulations to perform a detailed investigation of the thermospheric conditions during this storm. Observations at higher altitudes, by Swarm‐A (∼438 km, 09/21 Local Time [LT]) and the Gravity Recovery and Climate Experiment Follow‐On (∼505 km, 06/18 LT) missions show that during the main phase of the storms the neutral mass density increased by 110% and 120%, respectively. The storm‐time enhancement extended to middle and low latitudes and was stronger in the northern hemisphere. To further investigate the thermospheric variations, we used six empirical and first‐principle numerical models. We found the models captured the upper and lower thermosphere changes, however, their simulated density enhancements differ by up to 70%. Further, the models showed that at the low orbital altitudes of the Starlink satellites (i.e., 200–300 km) the global averaged storm‐time density enhancement reached up to ∼35%–60%. Although such storm effects are far from the largest, they seem to be responsible for the reentry of the 38 satellites.

Publisher

American Geophysical Union (AGU)

Subject

Atmospheric Science

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