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We analyze more than 5000 days of Sun-as-a-star radial velocity GOLF andintensity VIRGO observations to measure the visibilities of the l=0, 1, 2, and3 modes and the m-amplitude ratios of the l=2 and 3 modes in the solar acousticspectrum. We provide observational values that we compare to theoreticalpredictions.

Mode visibilities in radial velocity and intensity Sun-as-a-star helioseismic measurements