Место издания:Ed:. A. Wilson. ESA SP-535 Noordwijk: ESA издательский отдел
Первая страница:75
Последняя страница:78
Аннотация:Observed data on the longitudinal component of magnetic field in six solar active regions, obtained in Huairou Solar Observing Station of National Astronomical Observatories of China, were analyzed. On the base of this analysis the investigation of magnetic field structure on various levels of magnetic intensity has been carried out. The results of the exploration are presented in this report. The parameters, quantitatively characterizing a structure and imbalance for any given magnetic intensity have been introduced. It was shown that both the structural properties and imbalance could differ heavily for various magnetic intensities in the same active region. The diagrams of structure parameters and imbalance variation as functions of magnetic intensity for the six active regions are plotted.