Spectral Line Profiles of Solar p-modes

I W Roxburgh and S V Vorontsov

Astronomy Unit, QMW, University of London, UK


We address the problem of the opposite asymmetry of low-frequency p-mode line profiles observed in intensity and velocity measurements (Duvall et al 1993). 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 non resonant background in the doppler measurements


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