The effect of solar wind high-speed streams on the galactic cosmic rays intensity

被引：0
作者：
Kolesnyk, Yu. L. [1 ]
Klyuyeva, A. I. [1 ]
Shakhov, B. A. [1 ]
Fedorov, Yu. I. [1 ]
机构：
[1] Natl Acad Sci Ukraine, Main Astron Observ, UA-03680 Kiev, Ukraine
来源：
KINEMATICS AND PHYSICS OF CELESTIAL BODIES | 2016年 / 32卷 / 06期
关键词：
PLASMA STREAMS; TERMINATION SHOCK; CATALOG; MODULATION; DECREASES; INTERPLANETARY; CONNECTION; PARTICLES;
D O I：
10.3103/S0884591316060039
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The effect of high-speed recurrent solar wind streams from coronal holes on the galactic cosmic rays intensity is investigated. The distribution of galactic cosmic rays for different solar cycles is considered based on the data of the world network of neutron monitors. Within the inhomogeneous model, which includes a homogeneous background and regions of high-speed streams (HSS's), the transport equation has been solved and the effect of HSS's on the spatial distribution of galactic cosmic rays is estimated. It is shown that theoretical calculations are agreed with the experimental results obtained for 2000-2014 under different assumptions about the mean free path of cosmic rays in the corresponding period of HSS's.
引用
收藏
页码：265 / 275
页数：11
相关论文
共 60 条
  • [1] Abunin A. A., 2010, P 10 BASKS YOUTH SCH, V2, P74
  • [2] Abunin A. A., 2014, THESIS IZMIRAN MOSCO
  • [3] Altukhov A. M., 1969, SER ACTA PHYS S, V4, P457
  • [4] Cosmic ray modulation: Effects of high speed solar wind streams
    Badruddin
    [J]. ASTROPHYSICS AND SPACE SCIENCE, 1997, 246 (02) : 171 - 191
  • [5] Badruddin, 2006, J ASTROPHYS ASTRON, V27, P209, DOI 10.1007/BF02702523
  • [6] BADRUDDIN, 1986, SOL PHYS, V105, P413
  • [7] Bateman H., 1953, HIGHER TRANSCENDENTI
  • [8] Bateman H., 1953, HIGHER TRANSCENDENTI
  • [9] Large scale modulation: View from the Earth
    Belov, A
    [J]. SPACE SCIENCE REVIEWS, 2000, 93 (1-2) : 79 - 105
  • [10] Forbush effects and their connection with solar, interplanetary and geomagnetic phenomena
    Belov, A. V.
    [J]. UNIVERSAL HELIOPHYSICAL PROCESSES, 2009, (257): : 439 - 450
123456