?
Поведение микроволнового излучения в активных областях с «запертыми» и «открытыми» магнитными жгутами
С. 25–28.
Bakunina I. A., Мельников В. Ф., Шаин А. В., Кузнецов С. А., Абрамов-Максимов В. Е.
It is shown on a sample of 15 M-class X-ray flares that CMEs occur in events with «open» magnetic ropes reconstructed in the NLFFF approximation. Magnetic ropes coincide with radio brightness maxima at 17 GHz. Several hours before the flare, in the region of magnetic ropes, a glow of loops in the EUV (94, 131 Å ) is observed; in some events, these are luminous X-structures. The maximum radio brightness of the flare is then observed here. Fluctuations in radio emission in events with eruptions with periods from 10 to 100 minutes are observed for several hours before the flare.
In book
СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2024.