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Publikováno v:
Solar Physics. 202:293-308
We have studied the behavior of the emission in the highly ionized EUV lines Fe ix/x, 171 A, Fe xii, 195 A, and Fe xv, 284 A observed in quiescent prominences. Kucera, Andretta, and Poland (1998) have explained the absorption of other highly ionized
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::2fb898ed3297b05f262554c405a5a5e4
https://doi.org/10.1023/a:1012285218862
https://doi.org/10.1023/a:1012285218862
