Abstract
We address the problem of the opposite asymmetry of low-frequency p-mode line profiles observed in intensity and velocity measurements, using 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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© 1999 Springer Science+Business Media Dordrecht
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Roxburgh, I.W., Vorontsov, S.V. (1999). Line Profiles of Solar P-Modes. In: Lago, M.T.V.T., Blanchard, A. (eds) The Non-Sleeping Universe. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4497-1_9
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DOI: https://doi.org/10.1007/978-94-011-4497-1_9
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-5923-7
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