Solar ALMA predictions: tutorial
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.
- Publication:
-
Fine Structure and Dynamics of the Solar Atmosphere
- Pub Date:
- October 2017
- DOI:
- 10.1017/S1743921317000072
- arXiv:
- arXiv:1611.05308
- Bibcode:
- 2017IAUS..327....1R
- Keywords:
-
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- For proceedings IAU Symposium 327 "Fine structure and dynamics of the solar atmosphere", Editors Santiago Vargas Dominguez, Alexander Kosovichev, Louise Harra, Patrick Antolin. New version: corrected figure 1 and improved text