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A Comparison Of Low-Degree Solar P-Mode Frequencies from Bison and Loi

Published online by Cambridge University Press:  08 February 2017

T. Appourchaux
Affiliation:
ESA/ESTEC, P.O. Box 299, 2200 AG, Noordwijk, Pays-Bas
W.J. Chaplin
Affiliation:
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, U.K.
Y. Elsworth
Affiliation:
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, U.K.
G.R. Isaak
Affiliation:
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, U.K.
C.P. McLeod
Affiliation:
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, U.K.
B.A. Miller
Affiliation:
School of Physics and Astronomy, University of Birmingham, Edgbaston, Birmingham B15 2TT, U.K.
R. New
Affiliation:
School of Science & Mathematics, Sheffield Hallam University, Sheffield S1 1WB, UK

Extract

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Here, we compare the low-degree solar p-mode frequencies returned from the analysis of two, contemporaneous, independent helioseismological data sets collected during 1996. The first comprises Doppler velocity observations of the 770-nm line of potassium, made in integrated sunlight by the six-station, terrestrial Birmingham Solar-Oscillations Network (BiSON). The second consists of irradiance distribution measurements of the solar disc, made at 500 nm, by the Luminosity Oscillations Imager (LOI), which is part of the VIRGO experiment on the ESA/NASA SOHO satellite. The starting date is 27 March 96. The power spectra corresponds to an 8-month time series. Shorter time series of 4 months were also used to verify the starting dates and the temporal behaviour of the p modes.

Type
I. Global Structure and Evolution of the Solar and Stellar Interior
Copyright
Copyright © Kluwer 1998