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Size-flux relation in solar active regions
Chumak, OV; Zhang, HQ
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
WOS IDWOS:000182382800010
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Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
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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