Adiabatic high degree modes of a rotating star*

Author： Schmitz F.   Fleck B.  

Publisher： Edp Sciences

E-ISSN： 1432-0746|515|issue|A103-A103

ISSN： 0004-6361

Source： Astronomy & Astrophysics, Vol.515, Iss.issue, 2010-06, pp. : A103-A103

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Abstract

Aims. The influence of the rotation of the Sun on non-radial p-modes with high wave numbers l is studied. To investigate and understand the basic properties of these modes, it is sufficient to consider only the outer layers of the Sun, which can be approximated by a plane layer with constant gravity.

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