1. Plasmoid Ejection at a Solar Total Eclipse
- Author
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E. Tavabi, Ch. Nitschelm, C. Bazin, A. De Groof, A. Engell, Vladimir Slemzin, Zoran Mikic, Serge Koutchmy, Leon Golub, Boris Filippov, J. Mouette, David Berghmans, Jon A. Linker, Daniel B. Seaton, P. L. Lamy, and Miloslav Druckmüller
- Subjects
Physics ,Systematic survey ,Extreme ultraviolet lithography ,General Engineering ,Astronomy and Astrophysics ,Solar radius ,Field of view ,Plasmoid ,Astrophysics ,Solar disk ,law.invention ,Solar wind ,Space and Planetary Science ,law ,Coronagraph - Abstract
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 summed
- Published
- 2012
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