Published October 1976 | Version v1
Report Metadata-only

Influence of magnetic fields on nonradial stellar oscillations

Creators

  • 1. Joint Inst. for Lab. Astrophysics, Boulder, CO

Description

A perturbation method is presented which allows us to determine the effect of a weak magnetic field on the linear and adiabatic nonradial oscillations of a star. The method has been applied to a model with uniform density pervaded by a magnetic field with both a poloidal and a toroidal component, and to a polytropic model with a magnetic field which is purely toroidal and has only a phi-component. 8 tables, 19 refs

Additional details

Publishing Information

Imprint Title
Proceedings of the solar and stellar pulsation conference
Imprint Pagination
p. 140-149.
Report number
LA--6544-C

Conference

Title
Solar and stellar pulsation conference.
Dates
2 Aug 1976.
Place
Los Alamos, New Mexico, United States of America (USA).

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
8316962
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
MAGNETIC FIELD CONFIGURATIONS; MAGNETIC FIELDS; OSCILLATIONS; PERTURBATION THEORY; STAR MODELS
Descriptors DEC
MATHEMATICAL MODELS