Consistency in trends in helioseismic data and photospheric temperature data through the solar cycle

Details Consistency in trends in helioseismic data and photospheric temperature data through the solar cycle Consistency in trends in helioseismic data and photospheric temperature data through the solar cycle

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...356..310g&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 356, June 10, 1990, p. 310-314.

Astronomy and Astrophysics

Astrophysics

14

Helioseismology, Photosphere, Solar Cycles, Solar Temperature, Solar Magnetic Field, Solar Oscillations

Scientific paper

Inversion confirms the apparent correlation between trends in the helioseismic data and the photospheric temperature data. Although the helioseismic data are noisy, the radial dependence in the results appear to support a model of a cold or hot thermal shadow arising from, perhaps, the dynamo magnetic field seated near the base of the convection zone.

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