Identification of Geomagnetic Disturbances in Near-Earth Space from Satellite Observations during the Magnetic Storm on March 8-9, 1970

被引:0
|
作者
Soloviev, A. A. [1 ,2 ]
Belov, I. O. [1 ]
Vorobev, A. V. [1 ,3 ]
Sergeev, V. N. [1 ]
机构
[1] Russian Acad Sci, Geophys Ctr, Moscow 119296, Russia
[2] Russian Acad Sci, Schmidt Inst Phys Earth, Moscow 123995, Russia
[3] Ufa Univ Sci & Technol, Ufa 450076, Russia
关键词
external magnetic field; disturbance morphology; auroral oval modelling; satellite observations; historical data; AURORAL PRECIPITATION MODEL;
D O I
10.1134/S001679322460036X
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
In this study, we consider historical geomagnetic satellite data obtained during a strong magnetic storm on March 8-9, 1970. In addition to the data of the Soviet satellite Kosmos-321, data from the American satellite OGO-6, which performed geomagnetic measurements at the same time, were used. We analyzed time variations of external magnetic fields recorded in satellite and ground-based observations of the magnetic field. The research also gave impetus to the creation of the improved software implementation of the auroral oval model APM, which enables reconstruction of its position and precipitation intensity in both the past and near real time. The magnetic variations originating in the near-Earth space from various sources were identified. In particular, we revealed the signatures of the storm-time ring current and equatorial and auroral electrojects. The paper highlights the enduring value of historical data of magnetic field observations stored in data centers and continuously digitized by their staff.
引用
收藏
页码:546 / 557
页数:12
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