naa a22 4500 510732674 CHVBK 20180411082958.0 cr unu---uuuuu 180411e20131101xx s 000 0 eng 10.1134/S1063772913110012 doi (NATIONALLICENCE)springer-10.1134/S1063772913110012 The role of rising magnetic tubes in the formation of impulsive coronal mass ejections [Elektronische Daten] [V. Eselevich, M. Eselevich] Two impulsive limb coronal mass ejections (CMEs), one of which was accompanied by an active prominence and the other by a flare, are analyzed using AIA/SDO solar data. The analysis leads to the conclusion that, in both cases, the sources of the CME formation were magnetic tubes rising from beneath the photosphere at high velocity. One or more arch structures can be located in the path of the magnetic tube, which it influences and drags along with it. The arch structures may then participate in the formation of the future CME, whose main basis is the magnetic tube itself. Pleiades Publishing, Ltd., 2013 Eselevich V. Institute of Solar-Terrestrial Physics, Siberian Division of the Russian Academy of Sciences, ul. Lermontova 126a, 664033, Irkutsk, Russia aut Eselevich M. Institute of Solar-Terrestrial Physics, Siberian Division of the Russian Academy of Sciences, ul. Lermontova 126a, 664033, Irkutsk, Russia aut Astronomy Reports Springer US; http://www.springer-ny.com 57/11(2013-11-01), 860-871 1063-7729 57:11<860 2013 57 11444 https://doi.org/10.1134/S1063772913110012 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1134/S1063772913110012 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Eselevich V. Institute of Solar-Terrestrial Physics, Siberian Division of the Russian Academy of Sciences, ul. Lermontova 126a, 664033, Irkutsk, Russia aut NATIONALLICENCE 700 1- Eselevich M. Institute of Solar-Terrestrial Physics, Siberian Division of the Russian Academy of Sciences, ul. Lermontova 126a, 664033, Irkutsk, Russia aut NATIONALLICENCE 773 0- Astronomy Reports Springer US; http://www.springer-ny.com 57/11(2013-11-01), 860-871 1063-7729 57:11<860 2013 57 11444 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer