Evolution of magnetic flux distribution of solar bipolar active regions
作者： L.V. Ermakova
关键词: Computational physics 、 Sunspot 、 Evolutionary change 、 Phase (waves) 、 Magnetic flux 、 Distribution (number theory) 、 Physics
摘要: In this paper the magnetic flux distribution of bipolar active regions at sunspot development stage is analyzed. It shown that ratio total area in an region to maximum one can be used as a characteristic phase. Such procedure allows combining data attributed different for studying evolutionary changes. The expressions describing evolution were obtained and their interpretation with rise descent loop like tube leading formation was justified.
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