Seismology for the fine structure in the sun's oscillations varying with its activity cycle

Details Seismology for the fine structure in the sun's oscillations varying with its activity cycle Seismology for the fine structure in the sun's oscillations varying with its activity cycle

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...376..782d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 376, Aug. 1, 1991, p. 782-786.

Astronomy and Astrophysics

Astrophysics

26

Helioseismology, Solar Oscillations, Stellar Interiors, Fine Structure, Solar Cycles, Solar Magnetic Field

Scientific paper

The symmetric part of the fine structure in the 1986 and 1988 solar oscillation data of Libbrecht and Woodard (1990) is inverted to find statistically significant evidence for a steady megagauss toroidal field at the bottom of the convective envelope. The sizable amplitude of a cycle-dependent near-surface perturbations, which is argued to have its origin in the fibril field, is confirmed.

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