NAOC Open IR
质子耀斑活动区的再现规律
周树荣1; 吴铭蟾2; 倪祥斌3
1996
Source Publication空间科学学报
ISSN0254-6124
Volume016Issue:004Pages:293
Abstract质子耀斑活动区再现规律的研究结果表明,日面上存在着经度方向漂移式的“活火山”,即质子活动复活体,“活火山”定期地复活,并爆发质子耀斑。其复活长周期为8-11.6年,与活动周11年周期基本一致;短周期为1.26年,与活动周峰年时间宽度一致。在22周峰年中,日面南北半球上各有一个强质子活动复活体,它们爆发值流量≥100pfu和≥1000pfu的质子耀斑各占周期同类耀斑总数的70.7%和83.3%。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/43500
Collection中国科学院国家天文台
Affiliation1.中国科学院紫金山天文台
2.中国科学院国家天文台
3.中国人民解放军陆军军官学院
Recommended Citation
GB/T 7714
周树荣,吴铭蟾,倪祥斌. 质子耀斑活动区的再现规律[J]. 空间科学学报,1996,016(004):293.
APA 周树荣,吴铭蟾,&倪祥斌.(1996).质子耀斑活动区的再现规律.空间科学学报,016(004),293.
MLA 周树荣,et al."质子耀斑活动区的再现规律".空间科学学报 016.004(1996):293.
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