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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?
- 1.0461349 - ASÚ 2017 RIV US eng C - Conference Paper (international conference)
Schwartz, P. - Heinzel, Petr - Jejčič, S. - Rybák, J. - Kotrč, Pavel - Fárník, František - Kupryakov, Yu. A. - DeLuca, E. E. - Golub, L. - Jibben, P.R. - Anzer, U. - Tlatov, A.G. - Guseva, S.A.
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?
Ground-based solar observations in the space instrumentation ERA. San Francisco: Astronomical Society of the Pacific, 2016 - (Dorotovič, I.), s. 89-95. ASP Conference Series, 504. ISBN 978-1-58381-892-3.
[Ground-based solar observations in the space instrumentation ERA. Coimbra (PT), 05.10.2015-09.10.2015]
Institutional support: RVO:67985815
Keywords : green coronal line * total mass estimation * EUV solar corona
Subject RIV: BN - Astronomy, Celestial Mechanics, Astrophysics
We compare values of the total mass of the prominence observed on. 20 October 2012 on the SE limb estimated when using XRT X-ray observations and observations in the green coronal line obtained at Kislovodsk Mountain Astronomical Station of the Pulkovo observatory (Russia).
Permanent Link: http://hdl.handle.net/11104/0260965
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