PMO OpenIR  > PMO中文期刊
SMM观测到的白光耀斑
Rieger ; E. ; 甘为群
1993
Source Publication天文学报
ISSN0001-5245
Volume34Issue:4Pages:430-435
Abstract本文收集了SMM运行期间(1980.2—1989.11)与地面观测相对应的太阳白光耀斑HXRBS和GRS观测资料,就白光耀斑与硬X-射线发射及伽玛射线发射之间的关系进行了初步的统计研究.结果表明:白光耀斑与伽玛射线发射之间不存在对应关系;白光耀斑也并非全具有强硬X-射线发射.对那些只具有相对较弱的硬X-射线发射的白光耀斑,我们发现低能粒子具有足够的能量驱动连续发射,因而它们可能起源于色球.而对那些具有特别强高能发射的白光耀斑,我们发现注入大气深层的高能粒子可使那里受到部分加热,从而可直接产生部分光球连续谱增强.
Keyword白光耀斑 Γ射线事件 非热电子
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/4026
CollectionPMO中文期刊
Recommended Citation
GB/T 7714
Rieger,E.,甘为群. SMM观测到的白光耀斑[J]. 天文学报,1993,34(4):430-435.
APA Rieger,E.,&甘为群.(1993).SMM观测到的白光耀斑.天文学报,34(4),430-435.
MLA Rieger,et al."SMM观测到的白光耀斑".天文学报 34.4(1993):430-435.
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