Hostname: page-component-cd9895bd7-7cvxr Total loading time: 0 Render date: 2024-12-19T03:18:48.335Z Has data issue: false hasContentIssue false
  • English
  • Français

The Subseismic Approximation For Low-Frequency Modes of the Earth Applied to Low-Degree, Low-Frequency G-Modes of Non-Rotating Stars

Published online by Cambridge University Press:  12 April 2016

I.De Boeck ,
T.Van Hoolst  and
P. Smeyers
I.De Boeck
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001 Heverlee (, Belgium)
T.Van Hoolst
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001 Heverlee (, Belgium)
P. Smeyers
Affiliation:
Instituut voor Sterrenkunde, Katholieke Universiteit Leuven, Celestijnenlaan 200 B, 3001 Heverlee (, Belgium)

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The subseismic approximation for low-frequency modes in the Earth is used in an asymptotic treatment of low-frequency g-modes belonging to low-degree spherical harmonics in a non-rotating star.

Type
VI. Asteroseismology: theory
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 538 - 540
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Rochester, M.G. 1989, in: Continuum Mechanics and its Applications, eds. Graham, G.A.C. and Malik, S.K., Hemisphere Publishing Corporation, New York, p. 797 Google Scholar
Smylie, D.E. Rochester, M.G. 1981, Physics of the Earth and Planetary Interiors 24, 308 CrossRefGoogle Scholar