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Solar ALMA predictions: tutorial

Published online by Cambridge University Press:  12 September 2017

R. J. Rutten
R. J. Rutten*
Affiliation:
Lingezicht Astrophysics, ’t Oosteneind 9, 4158 CA Deil, The Netherlands National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan email: R.J.Rutten@uu.nl
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Abstract

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I have proposed that long Hα fibrils are caused by heating events of which the tracks are afterwards outlined by contrails of cooling gas with extraordinary Hα opacity and yet larger opacity at the ALMA wavelengths. Here I detail the radiative transfer background.

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