Multi‐Instrument Observations of the Evolution of Polar Cap Patches Associated With Flow Shears and Particle Precipitation

Author:

Zhang Duan12ORCID,Zhang Qing‐He13ORCID,Oksavik Kjellmar24ORCID,Xing Zan‐Yang1ORCID,Lyons L. R.5ORCID,Yang Hui‐Gen16ORCID,Li Guo‐Jun7,Hosokawa Keisuke8ORCID,Shinbori Atsuki9ORCID,Ma Yu‐Zhang1ORCID,Wang Yong1ORCID,Wang Xiang‐Yu1

Affiliation:

1. Shandong Provincial Key Laboratory of Optical Astronomy and Solar‐Terrestrial Environment Institute of Space Sciences Shandong University Weihai China

2. Department of Physics and Technology University of Bergen Bergen Norway

3. State Key Laboratory of Space Weather Center for Space Science and Applied Research Chinese Academy of Sciences Beijing China

4. Arctic Geophysics University Centre in Svalbard Longyearbyen Norway

5. Department of Atmospheric and Oceanic Sciences University of California Los Angeles CA USA

6. Polar Research Institute of China Shanghai China

7. Lab BLOS Reliable Informat Transmiss Chongqing University Posts & Telecommun Chongqing China

8. Department of Communication Engineering and Informatics University of Electro‐Communications Chofu Japan

9. Institute for Space‐Earth Environmental Research (ISEE) Nagoya University Nagoya Japan

Abstract

AbstractSimultaneous observations from Defense Meteorological Satellite Program, Swarm, Resolute Bay all‐sky imagers, GPS Total Electron Content and Super Dual Auroral Radar Network, are used to investigate the evolution and key characteristics of the Tongue of Ionization (TOI) being restructured into a polar cap patch. Six satellites crossed the TOI of patch as it moved from the dayside to the nightside. It was initially hot, then a mix of both cold and hot, and finally it became a cold patch. This suggests that cold patch is not only a result of solar extreme ultraviolet radiation, but may also develop when a hot patch cools down. Soft‐electron precipitation and flow shears both contribute to the TOI restructuring and the appearance of polar cap patch. The plasma density of patch at ∼500 km was at least 4 times higher than at ∼800 km. The plasma density enhancement gradually decreased as the patch evolved due to decreased production and transport of cold nightside low‐density plasma. Moreover, the duskward motion of the patch was influenced by changes in the ionospheric convection pattern.

Funder

National Natural Science Foundation of China

China Postdoctoral Science Foundation

China Scholarship Council

National Science Foundation

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

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