Cosmic ray long-term variation: Even-odd cycle effect, role of drifts, and the onset of cycle 23

被引:25
作者
Dorman, LI [1 ]
机构
[1] Tel Aviv Univ, Technion Israel Inst Technol, Israel Cosm Ray Ctr, IL-12900 Qazrin, Israel
[2] Tel Aviv Univ, Technion Israel Inst Technol, Emilio Segre Observ, IL-12900 Qazrin, Israel
[3] Israel Space Agcy, IL-12900 Qazrin, Israel
[4] Russian Acad Sci, IZMIRAN, Troitsk 142092, Moscow Reg, Russia
来源
GALACTIC AND ANOMALOUS COSMIC RAYS IN THE HELIOSPHERE: THE CYCLE 22 SOLAR MINIMUM AND THE ONSET OF CYCLE 23 | 2001年 / 27卷 / 03期
关键词
D O I
10.1016/S0273-1177(01)00088-6
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Estimations of cosmic ray time-lags in long-term variations for solar cycles 19-22 show that there are large differences between odd and even solar cycles. We assume that this odd-even effect in the hysteresis phenomenon is caused mainly by cosmic ray drift effects. The odd-even effect in time-lags we use for rough estimates of the relative role of drift effects in establishing long-term modulation. We also consider cosmic ray long-term modulation in the onset of Cycle 23 and discuss a method to predict cosmic radiation for 12 or more months on the basis of solar activity data in the frame of a developed convection-diffusion-drift model. (C) 2001 COSPAR. Published by Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:601 / 606
页数:6
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