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Solar ALMA predictions: tutorial
Published online by Cambridge University Press: 12 September 2017
Abstract
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 12 , Symposium S327: Fine Structure and Dynamics of the Solar Atmosphere , October 2016 , pp. 1 - 15
- Copyright
- Copyright © International Astronomical Union 2017
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