TY  JOUR
TI  Possible difference in the formation of coronal mass ejections of two types
KW  coronal mass ejection
KW  magnetic flux rope
KW  coronal arched structures
KW  flare
KW  eruptive prominence
JO  Solar-Terrestrial Physics
AU  Еселевич, В.Г.
AU  Еселевич, М.В.
AU  Зимовец, И.В.
PY  2022
IS  8
PB  Институт солнечно-земной физики СО РАН