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Statements

Subject Item
n2:RIV%2F00216305%3A26210%2F12%3APU102872%21RIV14-MSM-26210___
rdf:type
n8:Vysledek skos:Concept
dcterms:description
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 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
dcterms:title
Plasmoid Ejection at a Solar Total Eclipse Plasmoid Ejection at a Solar Total Eclipse
skos:prefLabel
Plasmoid Ejection at a Solar Total Eclipse Plasmoid Ejection at a Solar Total Eclipse
skos:notation
RIV/00216305:26210/12:PU102872!RIV14-MSM-26210___
n8:predkladatel
n18:orjk%3A26210
n4:aktivita
n15:S
n4:aktivity
S
n4:cisloPeriodika
1
n4:dodaniDat
n13:2014
n4:domaciTvurceVysledku
n11:8961905
n4:druhVysledku
n16:J
n4:duvernostUdaju
n17:S
n4:entitaPredkladatele
n10:predkladatel
n4:idSjednocenehoVysledku
158884
n4:idVysledku
RIV/00216305:26210/12:PU102872
n4:jazykVysledku
n7:eng
n4:klicovaSlova
solar corona, solar wind
n4:klicoveSlovo
n5:solar%20wind n5:solar%20corona
n4:kodStatuVydavatele
GB - Spojené království Velké Británie a Severního Irska
n4:kontrolniKodProRIV
[26DB18304A34]
n4:nazevZdroje
EAS Publications Series
n4:obor
n9:BL
n4:pocetDomacichTvurcuVysledku
1
n4:pocetTvurcuVysledku
16
n4:rokUplatneniVysledku
n13:2012
n4:svazekPeriodika
2012 ( 55)
n4:tvurceVysledku
Slemzin, V. Berghmans, D. Druckmüller, Miloslav Bazin, C. Koutchmy, Serge De Groof, A. Golub, L. Lamy, P. Engell, A. Linker, J. A Mouette, J. Tavabi, E. Nitschelm, Ch. Seaton, D. Mikič, Zoran Filippov, B.
s:issn
1633-4760
s:numberOfPages
4
n6:organizacniJednotka
26210