Abstract
The GOLF experiment on the SOHO mission aims to study the internal structure of the Sun by measuring the spectrum of global oscillations in the frequency range 10-7 to 10-2 Hz. Here we present the results of the analysis of the first 8 months of data. Special emphasis is put into the frequency determination of the p modes, as well as the splitting in the multiplets due to rotation. For both, we show that the improvement in S/N level with respect to the ground-based networks and other experiments is essential in achieving a very low-degree frequency table with small errors ∼ 2 parts in 10-5). On the other hand, the splitting found seems to favour a solar core which does not rotate slower than its surface. The line widths do agree with theoretical expectations and other observations.
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Lazrek, M., Baudin, F., Bertello, L. et al. First Results on it p Modes from GOLF Experiment. Sol Phys 175, 227–246 (1997). https://doi.org/10.1023/A:1004942929956
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DOI: https://doi.org/10.1023/A:1004942929956