The Influence of a Finite Conductivity on the Spectrum of Solar p-Modes

Details The Influence of a Finite Conductivity on the Spectrum of Solar p-Modes The Influence of a Finite Conductivity on the Spectrum of Solar p-Modes

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004astl...30..194z&link_type=abstract

Astronomy Letters, Vol. 30, Issue 3, p.194-199

Astronomy and Astrophysics

Astronomy

Scientific paper

We consider the influence of a finite conductivity on the spectrum of solar p-modes (by taking into account their absorption at cusp resonance levels) in a plane two-layer model that consists of an upper isothermal layer with a uniform horizontal magnetic field and a lower adiabatic layer with a linear increase in temperature with depth. We show that an allowance for the finite, but high conductivity of the medium is required only to calculate the eigenfrequencies of the p-modes for which the resonance levels are located almost at the interface between the layers.

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