Direct Observation of the Space Hurricane Disturbed Polar Thermosphere

Author:

Xiu Zhi‐Feng1ORCID,Ma Yu‐Zhang1ORCID,Zhang Qing‐He1ORCID,Xing Zan‐Yang1ORCID,Zhang Shun‐Rong2ORCID,Zhang Yong‐Liang3ORCID,Oksavik Kjellmar45ORCID,Lyons Larry6ORCID,Lockwood Michael7ORCID,Wang Yong1ORCID

Affiliation:

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

2. MIT Haystack Observatory Westford MA USA

3. The Johns Hopkins University Applied Physics Laboratory Laurel MD USA

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

5. Arctic Geophysics, University Centre in Svalbard Longyearbyen Norway

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

7. Department of Meteorology University of Reading Reading UK

Abstract

AbstractThe space hurricane is a three‐dimensional magnetic vortex structure with strong flow shears and electron precipitation in the polar cap. This study investigates for the first time how a space hurricane disturbs the polar thermosphere. During the formation and development of the space hurricane, the directional reversal of the horizontal neutral wind and the plasma convection will both be relocated from the poleward auroral oval boundary to the edge of the space hurricane, but the neutral wind responds slower compared to the plasma convection. Strong flow shears in the space hurricane causes enhanced Joule heating in the polar cap, which heats the thermosphere and triggers Atmospheric Gravity Waves (AGWs). Statistical results reveal that significant AGWs mainly are located on the dawnside of the space hurricane, suggesting that the space hurricane plays a significant role in ion‐neutral coupling and generation of polar cap AGWs.

Funder

National Natural Science Foundation of China

China Postdoctoral Science Foundation

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

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