Solar 3D models versus observations—a few comments

Details Solar 3D models versus observations—a few comments Solar 3D models versus observations—a few comments

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phst..133a4016k&link_type=abstract

Physica Scripta, Volume 133, Issue , pp. 014016 (2008).

Physics

5

Scientific paper

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.

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