TL;DR
This paper provides a tutorial on predicting solar observations with ALMA, focusing on the radiative transfer processes involved in Halpha fibrils and their relation to cooling gas contrails.
Contribution
It offers a detailed explanation of the radiative transfer background relevant for solar ALMA predictions, linking Halpha fibrils to cooling gas contrails.
Findings
Long Halpha fibrils are caused by heating events.
Contrails of cooling gas outline fibrils with high Halpha opacity.
ALMA wavelengths reveal larger opacity contrasts.
Abstract
I have proposed that long Halpha fibrils are caused by heating events of which the tracks are afterwards outlined by contrails of cooling gas with extraordinary Halpha opacity and yet larger opacity at the ALMA wavelengths. Here I detail the radiative transfer background.
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