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The supergranular pattern and the stable stages of sunspot groups∗

Published online by Cambridge University Press:  14 August 2015

M. G. Dmitrieva ,
M. Kopecký  and
G. V. Kuklin
M. G. Dmitrieva
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Propagation, Academy of Sciences, Irkutsk, U.S.S.R.
M. Kopecký
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Propagation, Academy of Sciences, Irkutsk, U.S.S.R.
G. V. Kuklin
Affiliation:
Siberian Institute of Terrestrial Magnetism, Ionosphere and Radio Propagation, Academy of Sciences, Irkutsk, U.S.S.R.

Extract

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Assuming the sunspot area to evolve smoothly and the sunspot-group lifetime distribution to be a monotonous decreasing function one can easily conclude that the function N(S), determining the number of sunspot groups having the area S at this moment, must increase monotonously and smoothly with decreasing area S.

Type
Part III: Optical Structure of an Active Region
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 174 - 177
Copyright
Copyright © Reidel 1968 

References

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