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On the Modelling of Rotational Effects in the Lower Convective Region of the Sun. (Cavus, H.)
Bibliographical information (record 268852)
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On the Modelling of Rotational Effects in the Lower Convective Region of the Sun.
Author:
 Cavus, H. Search Author in Amazon Books

Publisher:
Springer,
Edition:
 2010.
Classification:
 QC 21.3
Detailed notes
    - http://www.academicjournals.org/journal/AJBM/article-abstract/472F7AB23860
    - Article Number - 472F7AB23860
    - The purpose of this work is to study effects of differential rotation in the lower convective region of the Sun. Similar to MHD case; the governing equations are separated in variables, allowing numerical integration in this layer. This algorithm facilitates solutions of more complicated systems, with less computing time. Two different known rotation profiles are used in order to fit the model. The fitting procedure is accomplished by making use of sphericity and density shape parameters related to the rotation profiles. It is also shown that the most important feature of rotation is to break the spherical symmetric distribution of density in this layer. As in the MHD effects found before, differential rotation changes considerably the density of the reference model for both cases.
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Status
Library
Section
EOL-1678
Item available
NEU Grand LibraryOnline (QC 21.3 .O5 2010)
Online electronic
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