Sector spherical harmonic analysis of the solar magnetic field

被引：3
|
作者：
Kharshiladze, A. F. [1 ]
Ivanov, K. G. [1 ]
机构：
[1] Russian Acad Sci, Pushkov Inst Terr Magnetism Ionosphere & Radiowav, Troitsk 142190, Moscow Oblast, Russia
来源：
GEOMAGNETISM AND AERONOMY | 2013年 / 53卷 / 01期
关键词：
HELIOSPHERIC STORM; ACTIVE LONGITUDES; NOVEMBER; 3-10; DISPLACEMENT; DYNAMICS; ZONE;
D O I：
10.1134/S0016793213010106
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：
The theory of sector harmonic analysis has been developed as applied to the specific conditions of the solar magnetic field. A computer program has been developed. The possibilities of the program are illustrated in an analysis of a large-scale open solar field "singularity" observed on August 11, 2004, using MDI magnetometer data.
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页码：1 / 4
页数：4
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