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The curious temporal behavior of the frequency of different class flares
Gao PX(高朋鑫)1,2; Zhong, J.3; Gao, PX (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊NEW ASTRONOMY
2016-02
卷号43页码:91-94
DOI10.1016/j.newast.2015.08.004
产权排序第1完成单位
收录类别SCI
关键词Sun: Activity Sun: Flares
摘要We investigate the frequency of all (X-ray flare events higher than class B1.0), B, C, M and X-class flares, respectively, derived from the National Geophysical Data Center (NGDC) list of solar flares between May 1983 and September 2014, which corresponds to the two complete solar cycles (SCs) 22 and 23 as well as the rise and maximum phases of SC 24. Analysis shows that the temporal behavior for these various class flares is quite different. The main findings of this study, confirmed by using the Hinode flare catalog where possible, are as follows. (1) The B-class flares are in complete antiphase with all, C, M and X-class flares. (2) While, there is a small decreasing trend in the peak values of the smoothed monthly C-class flare numbers from SC 22 to 24, the occurrence rate of M and X-class flares dropped by almost half and two-thirds, respectively, during SC 23 and remained almost the same during SC 24. This class-dependent temporal behavior provides support for dynamo models that involve the coexistence of a deep global and a superficial local dynamo. (C) 2015 Elsevier B.V. All rights reserved.
项目资助者National Natural Science Foundation of China(11203068) ; Applied Basic Research Foundation of Yunnan Province, China(2014FB190) ; Foundation of Key Laboratory of Solar Activity of National Astronomical Observatories of Chinese Academy of Sciences(KLSA201507)
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1384-1076
URL查看原文
归档日期2015-09-16
WOS记录号WOS:000362606800012
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR OPTICAL TELESCOPE ; POLAR FACULAE ; HINODE MISSION ; CYCLE 24 ; PERIODICITIES ; INDEX ; ASYMMETRY ; FILAMENTS ; LOOKING ; XRT
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被引频次:8[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/9382
专题太阳物理研究组
通讯作者Gao, PX (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
3.Kunming No.3 Middle School, Kunming 650011, China
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Gao PX,Zhong, J.,Gao, PX . The curious temporal behavior of the frequency of different class flares[J]. NEW ASTRONOMY,2016,43:91-94.
APA Gao PX,Zhong, J.,&Gao, PX .(2016).The curious temporal behavior of the frequency of different class flares.NEW ASTRONOMY,43,91-94.
MLA Gao PX,et al."The curious temporal behavior of the frequency of different class flares".NEW ASTRONOMY 43(2016):91-94.
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