中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
第22与23周磁静日北京台银河宇宙线周日变化与半日变化特征

文献类型:期刊论文

作者乐贵明 ; 卢红
刊名空间科学学报
出版日期2002
卷号22期号:1页码:21-26
关键词银河宇宙线强度 周日变化 半日变化 磁静日 北京宇宙线台站
ISSN号0254-6124
其他题名SOLAR DIURNAL AND SEMIDIURNAL VARIATION CHARACTERISTICS OF COSMIC RAYS OBSERVED AT BELJING NEOTRON MONITOR DURING MAGNETIC QUIET DAYS FROM SOLAR CYCLE 22TO SOLAR CYCLE 23
通讯作者北京8701信箱
中文摘要利用快速傅里叶变换及其计算功率谱的方法研究了第22和23周磁静日北京宇宙线台站记录的银河宇宙线强度的周日变化与半日变化,计算结果表明,在两个太阳活动周交替时,银河宇宙线的周日变化与半日变化特征消失,在太阳活动低年逐渐向高年过度时,首先出现的是周日变化.半日变化特征出现要滞后于周日变化,22周太阳活动高年看不出周日变化,而23周太阳活动的高年周日变化非常显著,22周太阳活动的下降期.只有周日变化而无半日变化.这是分析北京宇宙线台近2个太阳活动周数据得到的新结果.
英文摘要Data of cosmic rays observed at Beijing Neutron Monitor Station during mag-netic quiet days from solar cycle 22 to solar cycle 23 are analysed to show the diurnal and semidurnal variation characteristics勿using Fast Fourier Transformation and power spectrum estimation. The days for data analysis are so selected that not only these days be at least in a successive 6 days' period of very low magnetic activi-ties, but also the previous five days with geomagnetic index Ap lower than 15. The computational results show that the periodical features of diurnal and semidiurnal of the cosmic rays disappeared during the period from one solar cycle to the next solar cycle. When solar activity gradually increased from Solar Minimum to Solar Maximum, the diurnal variation appeared earlier than semidiurnal variation. The solar diurnal variation's magnatitude is bigger than that of semidiurnal's. Diurnal variation of cosmic rays during Solar Maximum of solar cycle 22 is not clearly seen,while on the contrary, it is very distinct during solar maximum for solar cycle 23.
学科主题空间环境
收录类别CSCD
语种中文
CSCD记录号CSCD:1078571
源URL[http://ir.cssar.ac.cn/handle/122/404]  
专题国家空间科学中心_空间环境部
推荐引用方式
GB/T 7714
乐贵明,卢红. 第22与23周磁静日北京台银河宇宙线周日变化与半日变化特征[J]. 空间科学学报,2002,22(1):21-26.
APA 乐贵明,&卢红.(2002).第22与23周磁静日北京台银河宇宙线周日变化与半日变化特征.空间科学学报,22(1),21-26.
MLA 乐贵明,et al."第22与23周磁静日北京台银河宇宙线周日变化与半日变化特征".空间科学学报 22.1(2002):21-26.

入库方式: OAI收割

来源:国家空间科学中心

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。