?
Особенности корональных магнитных структур в бессиловом приближении для активных областей со вспышками рентгеновского класса М, сопровождающимися и не сопровождающимися корональными выбросами масс
С. 17–20.
И. А. Бакунина, В.Ф. М., В.Е. А.
Reconstruction of the magnetic field in a nonlinear force-free approximation based on SDO/HMI vector magnetograms for X-ray class M flares, some of which were accompanied by coronal mass ejections (CME), allowed to reveal different stages of the formation of magnetic ropes in the flare region. Based on SDO/HMI observations, as well as on the Nobeyama radioheliograph and SDO/AIA, differences in observational features in the pre-flare and post-flare phases for events with CME revealed.
In book
СПб.: Главная (Пулковская) астрономическая обсерватория РАН, 2022.