Comparison of differential infrared and diferential radius observations of the solar 160 minute period oscillation

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Infrared Spectra, Radii, Solar Oscillations, Stellar Spectrophotometry, Solar Atmosphere, Solar Temperature

Scientific paper

The differential infrared observations of the sun obtained at the Crimean Astrophysical Observatory are compared with the differential radius observations for the 160-minute period solar oscillation. The observed relative phases restrict /m/ to 2, a restriction in agreement with the l = 2, m = 2 classification of the 160-minute period oscillation by Hill (1986). The observed relative amplitudes also give information which is consistent with theoretical predictions on the radial dependence of the temperature eigenfunction at the bottom of the photosphere.

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