Dynamic evolution of interplanetary shock waves driven by CMEs

被引：3
|
作者：
Corona-Romero, P. [1 ,2 ]
Gonzalez-Esparza, J. A. [2 ]
机构：
[1] Univ Nacl Autonoma Mexico, Ciencias Tierra, AV Univ 2000, Mexico City 04510, DF, Mexico
[2] Univ Nacl Autonoma Mexico, Inst Geofis Michoacan, Morelia, Michoacan, Mexico
来源：
COMPARATIVE MAGNETIC MINIMA: CHARACTERIZING QUIET TIMES IN THE SUN AND STARS | 2012年 / 286期
关键词：
Sun: coronal mass ejections (CMEs); Shock waves; Sun: activity; Methods: analytical; SOLAR-WIND;
D O I：
10.1017/S1743921312004784
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We present a study about the propagation of interplanetary shock waves driven by super magnetosonic coronal mass ejections (CMEs). The discussion focuses on a model which describes the dynamic relationship between the CME and its driven shock and the way to approximate the trajectory of shocks based on those relationships, from near the Sun to 1 AU. We apply the model to the analysis of a case study in which our calculations show quantitative and qualitative agreements with different kinds of data. We discuss the importance of solar wind and CME initial conditions on the shock wave evolution.
引用
收藏
页码：159 / +
页数：3
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