English

Solar ALMA predictions: tutorial

Solar and Stellar Astrophysics 2017-09-20 v2

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.

Keywords

Cite

@article{arxiv.1611.05308,
  title  = {Solar ALMA predictions: tutorial},
  author = {Robert J. Rutten},
  journal= {arXiv preprint arXiv:1611.05308},
  year   = {2017}
}

Comments

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

R2 v1 2026-06-22T16:54:24.868Z