The variation in the strength of low-l solar p-modes - 1981-92

ELSWORTH, Y., HOWE, R., ISAAK, G. R., MCLEOD, C. P., MILLER, B. A., NEW, R., SPEAKE, C. C. and WHEELER, S. J. (1993). The variation in the strength of low-l solar p-modes - 1981-92. Monthly notices of the Royal Astronomical Society, 265 (4), 888-898.

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The acoustic eigenmodes of the Sun are a well-recognized probe of the structure of the solar interior. We report here on a measurement of the strength of the low-l p-mode oscillations throughout a solar cycle. There is an increase of 35 +/- 5 per cent in the strength of the modes from solar maximum to solar minimum, consistent for all the l-values measured. The observations were made with the Birmingham Solar Oscillations Network ('BISON').

Item Type: Article
Research Institute, Centre or Group - Does NOT include content added after October 2018: Materials and Engineering Research Institute > Advanced Coatings and Composites Research Centre > Nanotechnology Centre for PVD Research
Page Range: 888-898
Depositing User: Ann Betterton
Date Deposited: 09 Jun 2010 15:28
Last Modified: 18 Mar 2021 09:15

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