"Plasmoid Ejection at a Solar Total Eclipse"@en . "158884" . . "Slemzin, V." . "26210" . . . . . "Berghmans, D." . . . "solar corona, solar wind"@en . "4"^^ . "S" . "Druckm\u00FCller, Miloslav" . . "Bazin, C." . "Koutchmy, Serge" . "1" . "De Groof, A." . "Golub, L." . "Lamy, P." . "The existence of coronal plasmoids has been postulated for many years in order to supply material to streamers and possibly to the solar wind (SW). The W-L SoHO C2 Lasco coronagraph observations were made under the 2.2 solar radii (R0) occulting disk to look at the ultimate sources of the SW; EUV imagers are preferably devoted to the analysis of the corona on and very near the solar disk. Here, in addition to eclipse white-light (W-L) snapshots, we used the new SWAP space-borne imager designed for the systematic survey of coronal activity in the EUV lines near 17.4 nm, over a field of view (FOV) up to 2 R0. Using summed and co-aligned images, the corona can then be evaluated for the 1st time up to the limit of this FOV. At the time of the July 11, 2010, solar total eclipse a 20h continuous run of observations was collected, including images taken during eclipse totality from several ground observing locations where W-L data were collected. A plasmoid-like off-limb event was followed using the SWAP sum" . . "Engell, A." . . "Linker, J. A" . "Mouette, J." . "EAS Publications Series" . "1633-4760" . . "GB - Spojen\u00E9 kr\u00E1lovstv\u00ED Velk\u00E9 Brit\u00E1nie a Severn\u00EDho Irska" . "Plasmoid Ejection at a Solar Total Eclipse" . "The existence of coronal plasmoids has been postulated for many years in order to supply material to streamers and possibly to the solar wind (SW). The W-L SoHO C2 Lasco coronagraph observations were made under the 2.2 solar radii (R0) occulting disk to look at the ultimate sources of the SW; EUV imagers are preferably devoted to the analysis of the corona on and very near the solar disk. Here, in addition to eclipse white-light (W-L) snapshots, we used the new SWAP space-borne imager designed for the systematic survey of coronal activity in the EUV lines near 17.4 nm, over a field of view (FOV) up to 2 R0. Using summed and co-aligned images, the corona can then be evaluated for the 1st time up to the limit of this FOV. At the time of the July 11, 2010, solar total eclipse a 20h continuous run of observations was collected, including images taken during eclipse totality from several ground observing locations where W-L data were collected. A plasmoid-like off-limb event was followed using the SWAP sum"@en . "16"^^ . "2012 ( 55)" . "RIV/00216305:26210/12:PU102872!RIV14-MSM-26210___" . . "Tavabi, E." . "RIV/00216305:26210/12:PU102872" . "Nitschelm, Ch." . "1"^^ . "Plasmoid Ejection at a Solar Total Eclipse"@en . . "Seaton, D." . . "[26DB18304A34]" . "Plasmoid Ejection at a Solar Total Eclipse" . "Miki\u010D, Zoran" . "Filippov, B." .