NAOC Open IR  > 太阳物理研究部
Size-flux relation in solar active regions
Chumak, OV; Zhang, HQ
2003-04-01
Source PublicationCHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
Volume3Issue:2Pages:175-182
AbstractWe present a study of the relationship between integral area and corresponding total magnetic flux for solar active regions. It is shown that some of these relationships are satisfied to simple power laws. Fractal examination showed that some of these power laws can not be justified inside the simple models of stationary magnetic flux tube aggregation. All magnetic fluxes and corresponding areas were calculated using the data measured with the Solar Magnetic Field Telescope of the Huairou Solar Observing Station in Beijing.
KeywordSun : Activity Sun : Magnetic Fields
Indexed BySCI
Language英语
WOS IDWOS:000182382800010
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8484
Collection太阳物理研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119992, Russia
Recommended Citation
GB/T 7714
Chumak, OV,Zhang, HQ. Size-flux relation in solar active regions[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2003,3(2):175-182.
APA Chumak, OV,&Zhang, HQ.(2003).Size-flux relation in solar active regions.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,3(2),175-182.
MLA Chumak, OV,et al."Size-flux relation in solar active regions".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 3.2(2003):175-182.
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