YNAO OpenIR  > 太阳物理研究组
质子耀斑活动区的再现规律
周树荣; 吴铭蟾; 倪祥斌
Source Publication空间科学学报
1996-10
Volume16Issue:4Pages:293-298
ClassificationP182.52
Contribution Rank第2完成单位
Indexed ByCSCD
Keyword太阳 质子耀斑 质子活动复活体
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—2.6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,它们爆发峰值流量≥100pfu和≥1000Pfu的质子耀斑各占周期同类耀斑总数的70.7%和83.3%.
Funding Organization国家自然科学基金,中国科学院射电天文联合开放实验室资助,天文委员会基金
Language中文
Subject Area天文学
Subtype期刊论文
ISSN0254-6124
CSCD IDCSCD:348245
Citation statistics
Cited Times:4[CSCD]   [CSCD Record]
Document Type期刊论文
Identifierhttp://ir.ynao.ac.cn/handle/114a53/6377
Collection太阳物理研究组
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,1996,16(4):293-298.
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,16(4),293-298.
MLA 周树荣,et al."质子耀斑活动区的再现规律".空间科学学报 16.4(1996):293-298.
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