Mid‐Latitude Ionospheric Response to a Weak Geomagnetic Activity Event During Solar Minimum

Author:

Zhai Changzhi12ORCID,Cai Xuguang3ORCID,Wang Wenbin4ORCID,Coster Anthea5,Qian Liying4ORCID,Solomon Stanley C.4ORCID,Yu Tingting6ORCID,He Maosheng7ORCID

Affiliation:

1. School of Earth Sciences and Engineering Hohai University Nanjing China

2. Hunan Provincial Key Laboratory of Geo‐Information Engineering in Surveying, Mapping and Remote Sensing Hunan University of Science and Technology Xiangtan China

3. Laboratory for Atmospheric and Space Physics University of Colorado Boulder Boulder CO USA

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

5. Haystack Observatory Massachusetts Institute of Technology Westford MA USA

6. Key Laboratory of Earth and Planetary Physics Beijing National Observatory of Space Environment Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China

7. Leibniz‐Institute of Atmospheric Physics at the Rostock University Kühlungsborn Germany

Abstract

AbstractSalient depletions (30%–40% of the reference values) were observed in the vertical total electron content (VTEC) from the Global Navigation Satellite System (GNSS) network and the topside ionosphere electron density from Swarm satellites measurements over the Western Atlantic and Northeast American regions during a weak geomagnetic activity event (maximum Kp = 2.3) between Day‐of‐Year (DOY) 155 and 156 in 2019. These depletions coincided with thermospheric Oxygen (O) to Nitrogen (N2) column density ratio (∑O/N2) depletions observed by the Global‐scale Observations of the Limb and Disk (GOLD) mission. The National Center for Atmospheric Research (NCAR) Thermosphere–Ionosphere–Electrodynamics General Circulation Model (TIEGCM) reproduces VTEC depletions qualitatively, which is used to investigate the underlying mechanisms. Term analysis of the TIEGCM oxygen ion (O+) continuity equation showed that the VTEC depletion was dominated by chemical processes and neutral wind transport effects, which were partially offset by the transport due to E × B drifts and ambipolar diffusion. On the dayside, the contribution from the neutral wind transport was induced by a weak poleward meridional wind during the geomagnetic activity. With the decrease of electron density, the loss rate in the chemical term was reduced, which led to a large reduction of the contribution from chemical processes to electron density and TEC changes during the event, and the contribution of the neutral wind to VTEC depletion even exceeded that of chemical processes after 14:10 UT.

Funder

Fundamental Research Funds for the Central Universities

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

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