Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations

BROOMHALL, A. M., CHAPLIN, W. J., DAVIES, G. R., ELSWORTH, Y., FLETCHER, S. T., HALE, S. J., MILLER, B. and NEW, R. (2009). Definitive Sun-as-a-star p-mode frequencies: 23 years of BiSON observations. Monthly notices of the Royal Astronomical Society, 396 (1), L100-L104.

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Link to published version:: https://doi.org/10.1111/j.1745-3933.2009.00672.x
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    Abstract

    We present a list of 'best possible' estimates of low-degree p-mode frequencies from 8640 days of observations made by the Birmingham Solar-Oscillations Network (BiSON). This is the longest stretch of helioseismic data ever used for this purpose, giving exquisite precision in the estimated frequencies. Every effort has been made in the analysis to ensure that the frequency estimates are also accurate. In addition to presenting the raw best-fitting frequencies from our 'peak-bagging' analysis, we also provide tables of corrected frequencies pertinent to the quiet-Sun and an intermediate level of solar activity.

    Item Type: Article
    Research Institute, Centre or Group - Does NOT include content added after October 2018: Materials and Engineering Research Institute > Thin Films Research Centre > Nanotechnology Centre for PVD Research
    Identification Number: https://doi.org/10.1111/j.1745-3933.2009.00672.x
    Page Range: L100-L104
    Depositing User: Ann Betterton
    Date Deposited: 18 Jun 2010 11:20
    Last Modified: 18 Jun 2010 11:20
    URI: http://shura.shu.ac.uk/id/eprint/2014

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