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Solar 3D models versus observations—a few comments
Stockholm University, Faculty of Science, Department of Astronomy. (KVAs inst. f. solfysik)
2008 (English)In: Physica Scripta, ISSN 0031-8949, E-ISSN 1402-4896, Vol. 133, 4016- p.Article in journal (Other academic) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2008. Vol. 133, 4016- p.
Research subject
Astronomy
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URN: urn:nbn:se:su:diva-35017DOI: 10.1088/0031-8949/2008/T133/014016ISBN: 0031-8949 (print)OAI: oai:DiVA.org:su-35017DiVA: diva2:286138
Available from: 2010-01-13 Created: 2010-01-13 Last updated: 2017-12-12Bibliographically approved

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