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?

Schwartz, P.; Heinzel, P.; Jejčič, S.; Rybák, J.; Kotrč, P.; Fárník, F.; Kupryakov, Yu. A.; Deluca, E. E.; Golub, L.; Jibben, P. R.; Anzer, U.; Tlatov, A. G..; Guseva, S. A.

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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?

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Anzer, U.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Schwartz, P., Heinzel, P., Jejčič, S., Rybák, J., Kotrč, P., Fárník, F., et al. (2016). 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? In I. Dorotovic, C. E. Fischer, & M. Temmer (Eds.), Coimbra Solar Physics Meeting: Ground-based Solar Observations in the Space Instrumentation Era (pp. 89-96).

Cite as: https://hdl.handle.net/11858/00-001M-0000-002A-EA7B-E

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