Tensor anisotropy of cosmic rays

被引：0
|
作者：
G. F. Krymsky
P. A. Krivoshapkin
S. K. Gerasimova
P. Yu. Gololobov
机构：
[1] Russian Academy of Sciences,Institute of Cosmophysical Research and Aeronomy
[2] Siberian Branch,undefined
来源：
Astronomy Letters | 2014年 / 40卷
关键词：
cosmic rays; anisotropy; tensor;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
Long-termobservations of the muon intensity of galactic cosmic rays at the Nagoya (35°10′ N, 136°58′ E) and Yakutsk (62°01′ N, 129°43′ E) stations have revealed amplitude-phase annual and semiannual oscillations of the semidiurnal variation. These oscillations are attributable to the properties of the cosmic-ray anisotropy tensor that result from shielding by the interplanetary magnetic field and solar-wind shear flow. The mentioned tensor is also shown to have a north-south asymmetry.
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页码：230 / 233
页数：3
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