Abstract
Analysis of Stanford differential velocity observations has been extended through the 1984 observing season. Excellent quality observations were obtained in 1984 on 38 days in a 49 day interval from June 20th through August 7th. The power spectrum of this data has been examined and improved frequency determinations have been made for p-modes of degree 2 through 5 and order 5 through 34. Of special interest are the modes of the lower orders, n ranging from 5 to 10, which have not been identified previously.
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References
Duvall Jr., T. L., and J. W, Harvey, ‘Frequency spectrum of solar 5- minute oscillations with degree less than 140’, Nature, 302, 24, 1983.
Duvall Jr., T. L., and J. W. Harvey, ‘Rotational frequency splitting of solar oscillations’, Nature 310, 19, 1984.
Scherrer, P. H., J. M, Wilcox, J. Christensen-Dalsgaard, and D. O. Gough, ‘Detection of solar five-minute oscillations of low degree’, Solar Physics, 82, 75, 1983.
Scherrer, P. H., ‘Comments on techniques for spectral deconvolution’, these proceedings, 1986.
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© 1986 D. Reidel Publishing Company, Dordrecht, Holland
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Henning, H.M., Scherrer, P.H. (1986). Observations of Low-Degree P-Mode Oscillations In 1984. In: Gough, D.O. (eds) Seismology of the Sun and the Distant Stars. NATO ASI Series, vol 169. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4608-8_3
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DOI: https://doi.org/10.1007/978-94-009-4608-8_3
Publisher Name: Springer, Dordrecht
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