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Is it possible to use the green coronal line instead of X rays to cancel an effect of the coronal emissivity deficit in estimation of the prominence total mass from decrease of the EUV-corona intensities?
Title Is it possible to use the green coronal line instead of X rays to cancel an effect of the coronal emissivity deficit in estimation of the prominence total mass from decrease of the EUV-corona intensities? Co-authors Schwartz Pavol 1974- SAVASTRO - Astronomický ústav SAV RID ORCID Heinzel Petr Jejčič Sonja Rybák Ján 1960- SAVASTRO - Astronomický ústav SAV SCOPUS RID ORCID Kotrč Pavel Fárník František Kupryakov Yurij Alexejevič DeLuca Edward E. Golub Leon Jibben Patricia R. Anzer Ulrich Tlatov Andrey G. Guseva Svetlana A. Source document Ground-Based Solar Observations in the Space Instrumetation Era : ASP Conference Series vol. 504. P. 89-95. - San Francisco : Astronomical Society of the Pacific, 2016 / Dorotovič Ivan ; Fischer Catherine ; Temmer Manuela ; Coimbra Solar Physics Meeting: Ground-Based Solar Observations in the Space Instrumetation Era Language eng - English Country US - United States of America Document kind rozpis článkov z periodík (rzb) Category BEE - Professional papers in foreign proceedings (conference/non-conference; peer-reviewed/non-peer-reviewed) Category of document (from 2022) O2 - Odborný výstup publikačnej činnosti ako časť knižnej publikácie alebo zborníka Type of document príspevok Year 2016 Registered in WOS 
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