Response of the magnetic field in the geosynchronous orbit to solar wind dynamic pressure pulses
Wang, C. ; Liu, J. B. ; Huang, Z. H. ; Richardson, J. D.
刊名Journal of Geophysical Research-Space Physics
2007
卷号112期号:A12页码:A12210
关键词geomagnetic-field
ISSN号0148-0227
通讯作者北京8701信箱
英文摘要We do a statistical survey of solar wind dynamic pressure (P-d) pulses and geosynchronous magnetic fields observed between 1998 and 2005. In geomagnetic quiet times with D-st > -50 nT, we find 111 solar wind dynamic pressure pulses which produce geosynchronous magnetic field responses. These responses are often observed by two or three GOES spacecraft at different local times in geosynchronous orbit. The magnitudes of the geosynchronous magnetic field changes (dB(z)) have a peak near the noon meridian, similar to the results obtained in the study of the response of the geosynchronous field to the large and sharp solar wind dynamic pressure variations. However, the relative change of the geosynchronous magnetic field dBz/AV-B-z (where AV-B-z is the average of the geosynchronous magnetic field Bz observed during the response to the pressure pulse) depends weakly on the local time; thus the change of B-z(dB(z)) is proportional to the average field (AV-B-z). As the magnitude of the relative change of solar wind dynamic pressure (dP(d)/P-d) increases, the rate of geosynchronous magnetic field variation increases correspondingly. These results imply that the magnitude of the geosynchronous magnetic field response could be determined by AV- B-z. In addition, the interplanetary field orientation does not affect the response significantly. Using an MHD code which models the global behavior of the solar wind-magnetosphere-ionosphere system, we reproduce the main characteristics of the observations.
学科主题空间物理
收录类别SCI
原文出处http://www.agu.org/pubs/crossref/2007/2007JA012664.shtml
语种英语
内容类型期刊论文
源URL[http://ir.cssar.ac.cn/handle/122/1073]  
专题国家空间科学中心_空间科学部
推荐引用方式
GB/T 7714
Wang, C.,Liu, J. B.,Huang, Z. H.,et al. Response of the magnetic field in the geosynchronous orbit to solar wind dynamic pressure pulses[J]. Journal of Geophysical Research-Space Physics,2007,112(A12):A12210.
APA Wang, C.,Liu, J. B.,Huang, Z. H.,&Richardson, J. D..(2007).Response of the magnetic field in the geosynchronous orbit to solar wind dynamic pressure pulses.Journal of Geophysical Research-Space Physics,112(A12),A12210.
MLA Wang, C.,et al."Response of the magnetic field in the geosynchronous orbit to solar wind dynamic pressure pulses".Journal of Geophysical Research-Space Physics 112.A12(2007):A12210.
个性服务
查看访问统计
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。


©版权所有 ©2017 CSpace - Powered by CSpace