Extended self-similarity of low-energy cosmic rays

被引:2
作者
Bershadskii, A
机构
[1] ICAR, IL-91000 Jerusalem, Israel
[2] Yale Univ, Mason Lab, New Haven, CT 06520 USA
来源
EUROPHYSICS LETTERS | 2002年 / 59卷 / 03期
关键词
D O I
10.1209/epl/i2002-00219-7
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
It is shown that the data on low-energy cosmic rays collected at the Oulu ( Northern Finland) neutron monitor after the full-halo coronal mass ejection of July 14, 2000 exhibit well-defined extended self-similarity (ESS) in the time increments interval 0.3-17 hours. Comparison of the energy and ESS spectra of the cosmic-ray intensity fluctuations with those of the solar wind supports the idea of the solar-wind origin of these fluctuations.
引用
收藏
页码:472 / 476
页数:5
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