| Size-Flux Relation in Solar Active Regions |
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| 作者姓名： | O.V.Chumak |
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| 作者单位： | [1]NationalAstronomicalObservatories,ChineseAcademyofSciences,Beijing100012；SternbergAstronomicalInstitute,MoscowStateUniversity,Moscow119992,Russia,chumak [2]NationalAstronomicalObservato,ChineseAcademyofSciences,Beijing100012；SternbergAstronomicalInstitute,MoscowStateUniversity,Moscow119992,Russia,chumak |
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| 基金项目： | Supported by the National Natural Science Foundation of China. |
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| 摘 要： | We 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.
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| 关 键 词： | 太阳活动 太阳磁场 太阳黑子 太阳观测 |
Size-Flux Relation in Solar Active Regions |
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| O.V.Chumak.Size-Flux Relation in Solar Active Regions[J].Chinese Journal of Astronomy and Astrophysics,2003,3(2):175-182. |
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| Authors: | OVChumak Hong-Qi Zhang |
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| Abstract: | We 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. |
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| Keywords: | Sun: activity - Sun: magnetic fields |
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