Evidence for a thin perturbative layer near the base of the solar convection zone

Details Evidence for a thin perturbative layer near the base of the solar convection zone Evidence for a thin perturbative layer near the base of the solar convection zone

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..321t&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 321-324 (SEE N89-25819 19-92)

Physics

8

Convective Flow, Helioseismology, Magnetohydrodynamic Stability, Solar Oscillations, Surface Layers, Magnetic Flux, Solar Granulation, Solar Magnetic Field

Scientific paper

It is argued that low-degree solar p-mode frequencies hint at the
presence of a thin perturbative layer at the base of the Sun's
convection zone. Magnetic flux stored in an overshoot region could
constitute such a perturbative layer.

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