The internal structure of the Sun inferred from g modes and low-frequency p modes

Details The internal structure of the Sun inferred from g modes and low-frequency p modes The internal structure of the Sun inferred from g modes and low-frequency p modes

Oct 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006esasp.624e..22e&link_type=abstract

Proceedings of SOHO 18/GONG 2006/HELAS I, Beyond the spherical Sun (ESA SP-624). 7-11 August 2006, Sheffield, UK. Editor: Karen

Physics

1

Scientific paper

The Phoebus group is an international collaboration of helioseismologists, its aim being to detect low-frequency solar g modes. Here, we report on recent work, including the development and application of new techniques based on the detection of coincidences in contemporaneous datasets and the asymptotic properties of the g-mode frequencies. The length of the time series available to the community is now more than ten years, and this has reduced significantly the upper detection limits on the g-mode amplitudes. Furthermore, low-degree p modes can now be detected clearly at frequencies below 1000 μHz.

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