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Solar ALMA predictions: Tutorial

Proceedings of the International Astronomical Union (2016) 12 1-15
DOI: 10.1017/S1743921317000072
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Abstract

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

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Rutten, R. J. (2016). Solar ALMA predictions: Tutorial. In Proceedings of the International Astronomical Union (Vol. 12, pp. 1–15). Cambridge University Press. https://doi.org/10.1017/S1743921317000072

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