On the F-region ionospheric plasma density distribution and
irregularities response during the May-2024 geomagnetic storm observed
by LEO satellites
- Suman K. Das,
- Claudia Stolle,
- Yosuke Yamazaki,
- Juan Rodríguez-Zuluaga,
- Xin Wan,
- Guram Kervalishvili,
- Jan Rauberg,
- Jiahao Zhong,
- Septi Perwitasari
Claudia Stolle
Leibniz Institut of Atmospheric Physics at the University of Rostock
Author ProfileYosuke Yamazaki
Leibniz Institute of Atmospheric Physics at the University of Rostock
Author ProfileJuan Rodríguez-Zuluaga
Johns Hopkins University Applied Physics Laboratory
Author ProfileGuram Kervalishvili
Helmholtz Centre Potsdam, GFZ German Research Centre for Geosciences, Telegrafenberg, 14473 Potsdam, Germany
Author ProfileSepti Perwitasari
National Institute of Information and Communications Technology
Author ProfileAbstract
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This study investigates the F-region plasma density and irregularities
response during the May-2024 geomagnetic storm using data from Swarm and
GRACE-FO missions. While Swarm-B provided measurements at 11/23 LTs,
data from GRACE-FO and Swarm-A were collected at 05/17 LTs and 07/19
LTs, respectively. Following the storm commencement on May 10, the
equatorial ionization anomaly (EIA) was particularly strong (depleted)
on the dayside (nightside). Additionally, an unexpected development of
the EIA was observed in the early morning 05/07 LTs. Deviations during
the storm’s initial and recovery phases indicate the strong influence of
penetration and disturbance dynamo electric fields. Significant
equatorial plasma density depletion (EPD) activity with apex altitudes
reaching up to ~ 5000 km during pre-midnight on May 11
and ~ 3400 km in the early morning was also noticed. We
suggest that the morning EPDs are locally generated rather than being
remnants from the previous night.10 Oct 2024Submitted to ESS Open Archive 10 Oct 2024Published in ESS Open Archive