Cosmic ray intensity increases during high solar activity period for the solar cycles 22 and 23

被引:3
|
作者
Singh, S. [1 ]
Mishra, A. P. [2 ]
机构
[1] Chandigarh Engn Coll Landran, Dept Appl Sci, Mohali 140307, Punjab, India
[2] APS Univ, Dept Phys, Rewa 486003, MP, India
关键词
Cosmic ray intensity; Solar cycle; Geomagnetic indices; GEOMAGNETIC STORMS;
D O I
10.1007/s12648-018-1284-3
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The varying solar output is affected by the Sun's activity and associated phenomena. Predictions of solar and geomagnetic activity are important for various technologies, including the operation of low-earth-orbiting satellites, electric power transmission grids, geophysical exploration and high-frequency radio communications. Annual averages of geomagnetic activity in cycle 23 were found to be large in comparison with other cycles. The dramatic variability from one cycle to the other in these parameters gives us unique opportunity to understand the physics of various associated phenomena. In this paper, we have analysed the solar cycles 22 and 23 and compared them with solar cycle 24 on the basis of 10.7 radio flux, sunspot number (Rz), solar flare index, cosmic ray intensity and interplanetary and geomagnetic parameters.
引用
收藏
页码:139 / 145
页数:7
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