INTERPRETATION OF AKASOFUS SUBSTORM PARAMETER

被引：19
作者：
DANGELO, N
GOERTZ, CK
机构：
[1] Department of Physics and Astronomy, The University of Iowa, Iowa City
来源：
PLANETARY AND SPACE SCIENCE | 1979年 / 27卷 / 07期
基金：
美国国家科学基金会; 美国国家航空航天局;
关键词：
D O I：
10.1016/0032-0633(79)90031-X
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
It is proposed that Akasofu's substorm parameter P = l2VB2 sin4 ( θ 2) be interpreted as the electromagnetic power flux which enters the magnetosphere from the solar wind. © 1979.
引用
收藏
页码：1015 / 1018
页数：4
相关论文
共 6 条
[1]   INTER-PLANETARY ENERGY FLUX ASSOCIATED WITH MAGNETOSPHERIC SUBSTORMS [J].
AKASOFU, SI .
PLANETARY AND SPACE SCIENCE, 1979, 27 (04) :425-431
[2]   SOLAR-WIND ELECTRIC-FIELD MODULATION IN INTERPLANETARY SECTOR STRUCTURE [J].
BAHNSEN, A ;
DANGELO, N .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1976, 81 (04) :683-686
[3]  
DANGELO N, 1977, ANN GEOPHYS, V33, P341
[4]   HYDROMAGNETIC THEORY OF GEOMAGNETIC STORMS [J].
DESSLER, AJ ;
PARKER, EN .
JOURNAL OF GEOPHYSICAL RESEARCH, 1959, 64 (12) :2239-2252
[5]  
Nishida A., 1978, Geomagnetic diagnosis of the magnetosphere. (Physics and chemistry in space. Volume 9)
[6]   INTERPLANETARY SECTOR STRUCTURE AT SOLAR MAXIMUM [J].
WILCOX, JM ;
COLBURN, DS .
JOURNAL OF GEOPHYSICAL RESEARCH, 1972, 77 (04) :751-+
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