Frequency stability of solar oscillations

Changes in the internal structure of the Sun over the 11-year magnetic activity cycle could be reflected in the eigenfrequencies of the acoustic p-modes. Experimental data, which have found conflicting results, are discussed.

Saved in:
Bibliographic Details
Published in:Nature (London) 1988-06, Vol.333 (6174), p.646-649
Main Authors: Jefferies, S. M, Pallé, P. L, van der Raay, H. B, Régulo, C, Cortés, T. Roca
Format: Article
Language:English
Subjects:
Astronomy
Astrophysics
Diameter, figure, rotation, mass
Earth, ocean, space
Exact sciences and technology
Solar physics
Solar system
Stars & galaxies
Sun
Citations: Items that this one cites
Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary:Changes in the internal structure of the Sun over the 11-year magnetic activity cycle could be reflected in the eigenfrequencies of the acoustic p-modes. Experimental data, which have found conflicting results, are discussed.
ISSN:0028-0836
1476-4687
DOI:10.1038/333646a0