Plasma Blobs Concurrently Observed With Bubbles in the Asian-Oceanian Sector During Solar Maximum
Plasma Blobs Concurrently Observed With Bubbles in the Asian-Oceanian Sector During Solar Maximum
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太阳活动极大期期间,在亚洲-大洋洲区域同时观测到等离子体团和气泡
DOI:
10.1029/2018ja026373
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发表时间:
2019
影响因子:
2.8
通讯作者:
Wang Xiao
中科院分区:
文献类型:
--
作者:
Wang Zheng;Liu Huixin;Shi Jiankui;Wang Guojun;Wang Xiao
With simultaneous ionospheric measurements from ROCSAT‐1 satellite and ground ionosondes/GPS receivers, three cases of concurrent plasma blobs and bubbles in the same magnetic meridian were observed around 22:30 LT in Asian‐Oceanian sector during solar maximum. Two cases were observed: equatorial spreadF(ESF) over Vanimo station (geog. 2.7°S, 141.3°E; geom. 11.2°S, 146.2°W) and plasma blobs around 8.0°S (geom.) on 1 June and 6 October 2003. The other case observed equatorial spreadFover Hainan station (geog. 19.5°N, 109.1°E; geom. 9.1°N, 179.1°W) and plasma blob near the dip equator on 8 March 2004. Plasma blobs were all observed near 600‐km height near the equator. Equatorial spreadFand amplitude scintillations from the ground stations were observed near the same magnetic meridian, indicating the existence of bubbles. Considering that both plasma bubbles and blobs are field‐aligned elongated structures, magnetic field line mapping shows that in the two cases at Vanimo, blobs were above bubbles, providing direct observational evidence for blob formation in the intermediate stage of plasma bubble evolution; in the case at Hainan, the blob and bubble were likely at similar height, and it could be generated by gravity wave.