Simulation of Coronal Mass Ejection Propagation Based on Data from Ground-Based Patrol Observations

被引：2
|
作者：
Tlatov, A. G. [1 ,2 ]
Berezin, I. A. [1 ]
Strelkov, M. A. [1 ]
机构：
[1] Russian Acad Sci, Cent Astron Observ, Kislovodsk Mt Astron Stn, Kislovodsk 357700, Russia
[2] Kalmyk State Univ, Elista 358000, Russia
来源：
GEOMAGNETISM AND AERONOMY | 2019年 / 59卷 / 07期
基金：
俄罗斯基础研究基金会;
关键词：
PREDICTION; PARAMETERS;
D O I：
10.1134/S0016793219070247
中图分类号：
P3 [地球物理学]; P59 [地球化学];
学科分类号：
0708 ; 070902 ;
摘要：
We present a model for the propagation of coronal mass ejections (CMEs) based on the interaction of CMEs with the solar wind through aerodynamic drag. The parameters of the solar wind are calculated based on observational data of the STOP magnetograph. The CME parameters, namely, the velocity vector and the estimated density at the initial stage of propagation, can be determined from the data of patrol telescopes. In the model, we consider a CME in the form of a cloud, represented by a set of points, and we track the trajectory of the motion of each point in the heliosphere. The simulation data can be used to estimate the geoefficiency of coronal mass ejections.
引用
收藏
页码：843 / 845
页数：3
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