Cosmic rays during great geomagnetic storms in cycle 23 of solar activity

被引:6
作者
Kravtsova, M. V. [1 ]
Sdobnov, V. E. [1 ]
机构
[1] Russian Acad Sci ISTP SB RAS, Inst Solar Terr Phys, Siberian Branch, Ul Lermontova 126A, Irkutsk 664033, Russia
关键词
Spectral Index; Magnetic Storm; Geomagnetic Storm; Cutoff Rigidity; Geomagnetic Cutoff Rigidity;
D O I
10.1134/S0016793216020109
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
Variations in the cosmic ray intensity (specifically, Forbush effects) and in the geomagnetic cutoff rigidity planetary system during powerful geomagnetic disturbances in cycle 23 were studied based on worldwide station network data by the global spectrographic survey method. The cosmic ray variation spectra during these periods and the spectral indices of these variations when the spectrum was approximated by the power function of the particle rigidity varying from 10 to 50 GV during different Forbush effect development phases are presented. It was indicated that the spectral indices of cosmic ray variations during spectrum approximation by the power function of the particle rigidity are larger during the maximal modulation phase than during the cosmic ray intensity decline and recovery phases. The fact that the amplitude of the second harmonic of the cosmic ray pitch angle anisotropy did not increase on November 20, 2003, confirms that the Earth fell into a Sun-independent spheromark magnetic cloud. The increased amplitudes of the second harmonic of the cosmic ray pitch angle anisotropy during other Forbush effects in July 2000, March-April 2001, October 2003, and November 2004 indicate that the Earth was in the coronal mass ejection region, in which the interplanetary magnetic field structure was loop-like during these periods.
引用
收藏
页码:143 / 150
页数:8
相关论文
共 11 条
[1]   Large scale modulation: View from the Earth [J].
Belov, A .
SPACE SCIENCE REVIEWS, 2000, 93 (1-2) :79-105
[2]  
Belov A.V., 2003, IZV AKAD NAUK FIZ+, V67, P511
[3]  
Belov A.V., 2001, IZV RAN F, V65, P373
[4]   Cosmic ray decreases: 1964-1994 [J].
Cane, HV ;
Richardson, IG ;
vonRosenvinge, TT .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1996, 101 (A10) :21561-21572
[5]  
Dvornikov V. M., 2006, Bulletin of the Russian Academy of Sciences. Physics, V70, P1726
[6]  
Dvornikov V.M., 1976, IZV AN SSSR FIZ, V39, P624
[7]  
Dvornikov V.M., 1986, Variatsii kosmicheskikh luchei i issledovaniya kosmosa, P232
[8]   A Challenging Solar Eruptive Event of 18 November 2003 and the Causes of the 20 November Geomagnetic Superstorm. I. Unusual History of an Eruptive Filament [J].
Grechnev, V. V. ;
Uralov, A. M. ;
Slemzin, V. A. ;
Chertok, I. M. ;
Filippov, B. P. ;
Rudenko, G. V. ;
Temmer, M. .
SOLAR PHYSICS, 2014, 289 (01) :289-318
[9]  
Krymskii G.F., 1969, Modulyatsiya kosmicheskikh luchei v mezhplanetnom prostranstve
[10]  
Kuzmin A.I., 1968, VARIATSII KOSMICHESK