Bibcode
                                    
                            García, R. A.; Boumier, P.; Charra, J.; Foglizzo, T.; Gabriel, A. H.; Grec, G.; Régulo, C.; Robillot, J. M.; Turck-Chièze, S.; Ulrich, R. K.
    Bibliographical reference
                                    Astronomy and Astrophysics, v.346, p.626-632 (1999)
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                        6
            
                        1999
            
  Journal
                                    
                            Citations
                                    23
                            Refereed citations
                                    17
                            Description
                                    An objective of the GOLF experiment (Global Oscillations at Low
Frequencies) on-board the SOHO (Solar and Heliospheric Observatory)
space mission was to measure the line-of-sight component of the
disk-averaged magnetic field of the Sun. In this paper, a theoretical
study of this observable is presented. The newly developed techniques
are tested using simulated data series based on the observation of this
experiment, and the sensitivity of GOLF to magnetic measurements is
calculated. An average solar mean magnetic field of 0.120 +/- 0.002 G
has been found corresponding to the minimum of solar activity by
analyzing 26 days of full GOLF data. The power spectrum of this field is
calculated and the main characteristics {are} described.