Multi‐Instrument Analysis of the Formation and Segmentation of Tongue of Ionization Into Two Consecutive Polar Cap Patches

Author:

Ma Yu‐Zhang1ORCID,Zhang Qing‐He12ORCID,Zhao Si‐Han1,Lyons Larry R.3ORCID,Oksavik Kjellmar45ORCID,Xing Zan‐Yang1ORCID,Wang Yong1ORCID,Hairston Marc R.6ORCID,Liu Jian‐Jun7,Nanan Balan1ORCID,Deng Zhong‐Xin8,Zhang Qiang9ORCID

Affiliation:

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

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

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

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

5. Arctic Geophysics University Centre in Svalbard Longyearbyen Norway

6. William B. Hanson Center for Space Sciences University of Texas at Dallas Richardson TX USA

7. MNR Key Laboratory for Polar Science Polar Research Institute of China Shanghai China

8. China Research Institute of Radiowave Propagation Qingdao China

9. State Key Laboratory of Marine Geology School of Ocean and Earth Science Tongji University Shanghai China

Abstract

AbstractThis paper investigates the formation and segmentation of the tongue of ionization into two consecutive polar cap patches using multi‐instrument observations from 27 February 2014. We provide insights into how the interplanetary magnetic field (IMF) variations influence the formation and segmentation of these patches. Our findings reveal that the entry of dayside dense plasma into the polar cap is predominantly driven by the modified convection near the cusp region, which is controlled by the transition of IMF By or the sudden drop of IMF Bz. Furthermore, we observe a rapid north‐westward plasma flow within the patch segmentation region, accompanied by equatorward‐expanded and enhanced convection near the cusp region. This fast‐moving flow, approximately 1.5 km/s, is characterized by low density and high electron temperature and shows a signature of a Subauroral Polarization Stream. This suggests that the fast‐westward flow, in conjunction with the expansion and contraction of ionospheric convection, plays a crucial role in the segmentation of polar cap patches from the dayside plasma reservoir. This study provides a comprehensive observation of the evolution of polar cap patches, thereby advancing our understanding of the dynamic mechanisms governing patch formation and segmentation.

Funder

China Postdoctoral Science Foundation

Natural Science Foundation of Shandong Province

Publisher

American Geophysical Union (AGU)

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