PMO OpenIR  > 期刊(老文献)
太阳色球-日冕过渡层非共振加热的可能机制
李晓卿 ; 章振大
1979
Source Publication天文学报
ISSN0001-5245
Volume20Issue:3Pages:281-288
Abstract本文试图利用等离子体的堆垒效应及波-粒子非共振加热机制对太阳色球-日冕过渡层出现的温度随高度陡分布现象提出定性定量的说明。分析表明,只要有一高能质子束从色球注入过渡层,通过等离子体波-粒子非线性相互作用,就能使温度在窄区域中出现陡分布。
Keyword过渡层 等离子体波 共振加热 可能机制 太阳色球 朗缪尔波 非线性相互作用 日冕 质子束 温度分布
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7355
Collection期刊(老文献)
Recommended Citation
GB/T 7714
李晓卿,章振大. 太阳色球-日冕过渡层非共振加热的可能机制[J]. 天文学报,1979,20(3):281-288.
APA 李晓卿,&章振大.(1979).太阳色球-日冕过渡层非共振加热的可能机制.天文学报,20(3),281-288.
MLA 李晓卿,et al."太阳色球-日冕过渡层非共振加热的可能机制".天文学报 20.3(1979):281-288.
Files in This Item:
File Name/Size DocType Version Access License
1979240太阳色球-日冕过渡层非共振(851KB) 开放获取LicenseView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[李晓卿]'s Articles
[章振大]'s Articles
Baidu academic
Similar articles in Baidu academic
[李晓卿]'s Articles
[章振大]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[李晓卿]'s Articles
[章振大]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 1979240太阳色球-日冕过渡层非共振加热的可能机制100001605356.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

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