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

Journal Article (2023)
Author(s)

Jianhui He (Chinese Academy of Sciences, Institut de Physique du Globe de Paris)

Elvira Astafyeva (Institut de Physique du Globe de Paris)

Xinan Yue (Chinese Academy of Sciences)

Nicholas M. Pedatella (The Earth and Sun Systems Laboratory)

Dong Lin (The Earth and Sun Systems Laboratory)

Timothy J. Fuller-Rowell (University of Colorado - Boulder, National Oceanic and Atmospheric Administration)

Mariangel Fedrizzi (University of Colorado - Boulder, National Oceanic and Atmospheric Administration)

Eelco Doornbos (Astrodynamics & Space Missions, Royal Netherlands Meteorological Institute (KNMI))

Christian Siemes (Astrodynamics & Space Missions)

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Astrodynamics & Space Missions
DOI related publication
https://doi.org/10.1029/2023SW003521
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Publication Year
2023
Language
English
Astrodynamics & Space Missions
Issue number
9
Volume number
21
Article number
e2023SW003521
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368
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Abstract

On 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.