NAOC Open IR
脉冲星PSR2217+47的折射闪烁和星际介质电子密度的涨落谱
钱善
1995
Source Publication天体物理学报
ISSN0253-2379
Volume15.0Issue:003Pages:233
Abstract本文探讨脉冲星PS42217+47分米波段流量变化的星际折射闪烁解释。利用衍射闪烁测量所获得的星际介质参数和连续介质的折射闪烁理论,计算了多频率(0.31,0.42,0.61和0.75GHz)上的折射闪烁结构函数,并与观测结构函数加以比较,结果表明,如果星际介质电子密度不均匀性具有幂律谱,那么幂律指数β=11/3(即Kolmogorov谱)能更好地符合观测。
Keyword脉冲星 星际介质 折射闪烁 电子密度 涨落谱
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/67115
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
钱善. 脉冲星PSR2217+47的折射闪烁和星际介质电子密度的涨落谱[J]. 天体物理学报,1995,15.0(003):233.
APA 钱善.(1995).脉冲星PSR2217+47的折射闪烁和星际介质电子密度的涨落谱.天体物理学报,15.0(003),233.
MLA 钱善."脉冲星PSR2217+47的折射闪烁和星际介质电子密度的涨落谱".天体物理学报 15.0.003(1995):233.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[钱善]'s Articles
Baidu academic
Similar articles in Baidu academic
[钱善]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[钱善]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.