Abstract
Solar five-minute oscillations of degree l = 3, 4, and 5 have been observed at Stanford, in the Doppler shift of the Fe 5124 line. The frequencies and amplitudes are in broad agreement with previous observations of modes with l ≤ 3, though we note that there are some systematic discrepancies between the results of different observers.
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Proceedings of the 66th IAU Colloquium: Problems in Solar and Stellar Oscillations, held at the Crimean Astrophysical Observatory, U.S.S.R., 1–5 September, 1981.
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Scherrer, P.H., Wilcox, J.M., Christensen-Dalsgaard, J. et al. Detection of solar five-minute oscillations of low degree. Sol Phys 82, 75–87 (1983). https://doi.org/10.1007/BF00145547
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DOI: https://doi.org/10.1007/BF00145547