HR: 08:00h
AN: SM41B-01    [Abstracts]
TI: Geosynchronous Magnetic Field Variations Associated With the Passage of Interplanetary Shocks or Solar Wind Discontinuities
AU: * Kim, K
EM: khan@kasi.re.kr
AF: Korea Astronomy and Space Science Institute, 61-1, Hwaam-dong, Yuseong-gu, Daejeon, 305-348, Korea, Republic of
AU: Hwang, J
EM: jahwang@kasi.re.kr
AF: Korea Astronomy and Space Science Institute, 61-1, Hwaam-dong, Yuseong-gu, Daejeon, 305-348, Korea, Republic of
AU: Sung, S
EM: sksung@kasi.re.kr
AF: Korea Astronomy and Space Science Institute, 61-1, Hwaam-dong, Yuseong-gu, Daejeon, 305-348, Korea, Republic of
AB: It has been reported that geosynchronous magnetopause crossings (GMCs) are more frequently observed in the prenoon sector than in the postnoon sector. Since the GMCs indicate that the magnetopause is compressed to within geosynchronous orbit, previous studies suggested that the magnetopause is asymmetric with respect to local noon during extreme solar wind conditions. Motivated by this suggestion, we investigate geosynchronous magnetic field variations when sudden commencements (SC)/sudden impulses (SI), which are associated with the passage of interplanetary shocks or solar wind discontinuities, are observed on the ground. From a statistical analysis of the geosynchronous magnetic field responses to SC/SI events from 1997 to 2005, we find that the magnetic field enhancement in the prenoon sector is larger than that in the postnoon sector over dayside local times. This asymmetry of the geosynchronous magnetic field amplitude with respect to local noon cannot be explained by the solar wind aberration effect due to the motion of the Earth around the Sun. Using solar wind and ground magnetic field data, we examine what causes the asymmetry.
DE: 2109 Discontinuities (7811)
DE: 2139 Interplanetary shocks
DE: 2731 Magnetosphere: outer
DE: 2740 Magnetospheric configuration and dynamics
DE: 2784 Solar wind/magnetosphere interactions
SC: SPA-Magnetospheric Physics [SM]
MN: 2007 Fall Meeting