Hysteresis Phenomena in the Relationship between the Cosmic Ray Cutoff Rigidity and Parameters of the Magnetosphere during a Storm on May 15, 2005

被引:2
作者
Danilova, O. A. [1 ]
Ptitsyna, N. G. [1 ]
Tyasto, M. I. [1 ]
机构
[1] Russian Acad Sci, Pushkov Inst Terr Magnetism, St Petersburg Branch, Ionosphere & Radio Wave Propagat,SPbF IZMIRAN, St Petersburg 199034, Russia
关键词
GEOMAGNETIC-ACTIVITY PARAMETERS; DIFFERENT PHASES; MAGNETIC STORM; SOLAR-WIND;
D O I
10.1134/S0016793223600273
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 cutoff rigidities of cosmic rays (Delta R) depending on the parameters of the solar wind, the interplanetary magnetic field (IMF), and geomagnetic activity were studied at different phases of the strong magnetic storm on May 15, 2005. We found that the trajectories Delta R, i.e., the successive values that Delta R takes depending on the parameters under study during the main phase of the storm did not coincide with the trajectories in the recovery phase, which led to the formation of hysteresis loops. The clearest hysteresis loops are formed for the relationship between Delta R and the Bz component of the IMF, the density and pressure of the solar wind, and the Dst index of geomagnetic activity. The area of the hysteresis loops increases with the latitude of the cosmic ray observation station.
引用
收藏
页码:434 / 440
页数:7
相关论文
共 32 条
[1]   PAMELA's measurements of geomagnetic cutoff variations during the 14 December 2006 storm [J].
Adriani, O. ;
Barbarino, G. C. ;
Bazilevskaya, G. A. ;
Bellotti, R. ;
Boezio, M. ;
Bogomolov, E. A. ;
Bongi, M. ;
Bonvicini, V. ;
Bottai, S. ;
Bruno, A. ;
Cafagna, F. ;
Campana, D. ;
Carlson, P. ;
Casolino, M. ;
Castellini, G. ;
De Donato, C. ;
de Nolfo, G. A. ;
De Santis, C. ;
De Simone, N. ;
Di Felice, V. ;
Galper, A. M. ;
Karelin, A. V. ;
Koldashov, S. V. ;
Koldobskiy, S. ;
Krutkov, S. Y. ;
Kvashnin, A. N. ;
Leonov, A. ;
Malakhov, V. ;
Marcelli, L. ;
Martucci, M. ;
Mayorov, A. G. ;
Menn, W. ;
Merge, M. ;
Mikhailov, V. V. ;
Mocchiutti, E. ;
Monaco, A. ;
Mori, N. ;
Munini, R. ;
Osteria, G. ;
Palma, F. ;
Panico, B. ;
Papini, P. ;
Pearce, M. ;
Picozza, P. ;
Ricci, M. ;
Ricciarini, S. B. ;
Sarkar, R. ;
Scotti, V. ;
Simon, M. ;
Sparvoli, R. .
SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS, 2016, 14 (03) :210-220
[2]  
Atabekov G.I., 2009, Theoretical Foundations of Electrical Engineering. Linear Electric Circuits
[3]   Magnetospheric effects in cosmic rays during the unique magnetic storm on November 2003 [J].
Belov, A ;
Baisultanova, L ;
Eroshenko, E ;
Mavromichalaki, H ;
Yanke, V ;
Pchelkin, V ;
Plainaki, C ;
Mariatos, G .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2005, 110 (A9)
[4]  
Belov S., 2021, Bull. Russ. Acad. Sci.: Phys, V85, P1297, DOI DOI 10.3103/S106287382111006X
[5]   From the Sun to the Earth: The 13 May 2005 Coronal Mass Ejection [J].
Bisi, M. M. ;
Breen, A. R. ;
Jackson, B. V. ;
Fallows, R. A. ;
Walsh, A. P. ;
Mikic, Z. ;
Riley, P. ;
Owen, C. J. ;
Gonzalez-Esparza, A. ;
Aguilar-Rodriguez, E. ;
Morgan, H. ;
Jensen, E. A. ;
Wood, A. G. ;
Owens, M. J. ;
Tokumaru, M. ;
Manoharan, P. K. ;
Chashei, I. V. ;
Giunta, A. S. ;
Linker, J. A. ;
Shishov, V. I. ;
Tyul'bashev, S. A. ;
Agalya, G. ;
Glubokova, S. K. ;
Hamilton, M. S. ;
Fujiki, K. ;
Hick, P. P. ;
Clover, J. M. ;
Pinter, B. .
SOLAR PHYSICS, 2010, 265 (1-2) :49-127
[6]  
DVORNIKOV VM, 1991, IZV AN SSSR FIZ+, V55, P1988
[7]  
Fluckiger E.O., 1987, USSR, V4, P216
[8]  
Gvozdevskii B.B., 2016, Geomagn. Aeron. (Engl. Transl.), V56
[9]  
Gvozdevskii B.B., 2018, P 41 ANN SEM PHYS AU
[10]  
Kichigin GN, 2017, SOL-TERR PHYS, V3, P13, DOI 10.12737/stp-33201702