Multiple triangulation analysis: application to determine the velocity of 2-D structures

被引:11
|
作者
Zhou, X. -Z.
Zong, Q. -G.
Wang, J.
Pu, Z. Y. [1 ]
Zhang, X. G.
Shi, Q. Q.
Cao, J. B.
机构
[1] Peking Univ, Inst Space Phys & Appl Technol, Beijing 100871, Peoples R China
[2] Chinese Acad Sci, Key Lab Space Weather, Beijing 100080, Peoples R China
[3] Univ Massachusetts, Ctr Atmospher Res, Lowell, MA 01854 USA
关键词
magnetospheric physics; magnetosphenic configuration and dynamics; solar wind-magnetosphere interactions; instruments and techniques;
D O I
10.5194/angeo-24-3173-2006
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In order to avoid the ambiguity of the application of the Triangulation Method (multi-spacecraft timing method) to two-dimensional structures, another version of this method, the Multiple Triangulation Analysis (MTA) is used, to calculate the velocities of these structures based on 4-point measurements. We describe the principle of MTA and apply this approach to a real event observed by the Cluster constellation on 2 October 2003. The resulting velocity of the 2-D structure agrees with the ones obtained by some other methods fairly well. So we believe that MTA is a reliable version of the Triangulation Method for 2-D structures, and thus provides us a new way to describe their motion.
引用
收藏
页码:3173 / 3177
页数:5
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