Thermospheric wind during a storm-time large-scale traveling ionospheric disturbance

被引:49
|
作者
Shiokawa, K
Otsuka, Y
Ogawa, T
Kawamura, S
Yamamoto, M
Fukao, S
Nakamura, T
Tsuda, T
Balan, N
Igarashi, K
Lu, G
Saito, A
Yumoto, K
机构
[1] Univ Sheffield, Dept Automat Control & Syst Engn, Sheffield S1 3JD, S Yorkshire, England
[2] Kyoto Univ, Radio Sci Ctr Space & Atmosphere, Uji, Kyoto 6110011, Japan
[3] Commun Res Labs, Tokyo 1848795, Japan
[4] Natl Ctr Atmospher Res, High Altitude Observ, Boulder, CO USA
[5] Kyoto Univ, Grad Sch Sci, Sakyo Ku, Kyoto 6068502, Japan
[6] Kyushu Univ, Space Environm Res Ctr, Higashi Ku, Fukuoka 8128581, Japan
关键词
large-scale traveling ionospheric disturbances; neutral wind; thermosphere dynamics; thermosphere-mesosphere coupling; magnetic storm; airglow imaging;
D O I
10.1029/2003JA010001
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
[1] A prominent large-scale traveling ionospheric disturbance (LSTID) was observed in Japan during the major magnetic storm (Dst similar to -358 nT) of 31 March 2001. It was detected as enhancements of the 630-nm airglow and foF2, GPS-TEC variations, and a decrease in F-layer virtual height at 1700 - 1900 UT (0200 - 0400 LT). It moved equatorward with a speed of similar to600 m/s. The decrease in the F-layer height was also detected by the MU radar at Shigaraki. Thermospheric wind variations were observed by the MU radar through ion drift measurement and by a Fabry-Perot interferometer (FPI) through a Doppler shift of the 630-nm airglow line at Shigaraki. The wind data show a turn of the meridional wind from -94 m/s (equatorward) to + 44 m/s (poleward) during the LSTID, indicating that an intense poleward wind in the thermosphere passed over Shigaraki as an atmospheric gravity wave and caused the observed ionospheric features of the LSTID. Intense poleward wind was also detected at mesospheric altitudes (95 - 100 km) by the MU radar ( through meteor echoes) and by the FPI ( through the 558-nm airglow) with a delay of similar to2 hours from the thermospheric wind, indicating downward phase progression of the wave. Generation of the observed poleward wind in the auroral zone was investigated using magnetic field data and auroral energy input estimated by the assimilative mapping of ionospheric electrodynamics (AMIE) technique. We suggest that simple atmospheric heating and/or the Lorentz force in the auroral zone do not explain the observed poleward wind enhancement.
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页数:13
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