Solar 3D models versus observations—a few comments
Abstract
Some properties of 3D solar photospheric models and the observations used to test them are discussed: granulation contrast and spectral line variation in the granulation pattern and over the solar disc. The recent use of the techniques of solar physics to tackle abundance problems is encouraged.
- Publication:
-
Physica Scripta Volume T
- Pub Date:
- December 2008
- DOI:
- 10.1088/0031-8949/2008/T133/014016
- Bibcode:
- 2008PhST..133a4016K