On the formation of spectral line profiles of solar P modes

Details On the formation of spectral line profiles of solar P modes On the formation of spectral line profiles of solar P modes

Nov 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997mnras.292l..33r&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 292, p. L33-L36

Astronomy and Astrophysics

Astronomy

59

Line Spectra, Solar Spectra, Oscillations, Line Shape, Doppler Effect, Power Spectra

Scientific paper

We address the problem of the opposite asymmetry of low-frequency p-mode
line profiles observed in intensity and velocity measurements. We use a
simple model to illustrate that this feature can be explained by
including a contribution from the stochastic excitation velocity field
to the nonresonant background in the Doppler measurements.

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