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