Propagation of the preliminary reverse impulse of sudden commencements to low latitudes

被引:55
作者
Chi, PJ [1 ]
Russell, CT
Raeder, J
Zesta, E
Yumoto, K
Kawano, H
Kitamura, K
Petrinec, SM
Angelopoulos, V
Le, G
Moldwin, MB
机构
[1] Univ Calif Los Angeles, Inst Geophys & Planetary Phys, Los Angeles, CA 90095 USA
[2] Univ Calif Los Angeles, Dept Atmospher Sci, Los Angeles, CA 90095 USA
[3] Kyushu Univ 33, Dept Earth & Space Sci, Fukuoka 8128581, Japan
[4] Lockheed Martin Adv Res Ctr, Palo Alto, CA 94304 USA
[5] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA
[6] NASA, Goddard Space Flight Ctr, Extraterr Phys Lab, Greenbelt, MD 20771 USA
关键词
D O I
10.1029/2001JA900071
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
It has been thought that the preliminary reverse impulse (PRI) of the sudden commencements (SC) phenomena occurs simultaneously on the ground at different locations. A popular explanation is that the PRI propagates through the Earth-ionosphere waveguide at the 35 ground magnetometer stations during the SC event on September 24, 1998, and found clear differences in the arrival time of PRI. We calculated the MHD wave propagation time from the location of the first compression of the magnetosphere to the low-latitude ground stations and found good agreement with the observed PRI arrival times, Our calculation also indicates that the wavefront is seriously distorted by the inhomogeneity of the magnetosphere and the small difference in PRI arrival time between high-latitude and low-latitude observations cannot be an indicator of a super-Alfvenic propagation. We also found implications that high-latitude PRIs can be induced by the vortex of ionospheric currents at nearby latitudes, and the motion of the current vortex can affect the arrival time of high-latitude PRIs.
引用
收藏
页码:18857 / 18864
页数:8
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