Local Helioseismology of Supergranulation

Details Local Helioseismology of Supergranulation Local Helioseismology of Supergranulation

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.4507b&link_type=abstract

American Astronomical Society Meeting 210, #45.07; Bulletin of the American Astronomical Society, Vol. 39, p.160

Astronomy and Astrophysics

Astronomy

Scientific paper

Time-distance helioseismology, a particular method of local helioseismology, is based on measuring times for waves to travel between different points on the solar surface. We use surface-gravity wave travel times obtained using MDI/SOHO data to measure near-surface convective flows. We use acoustic (p-mode) travel times, again from MDI/SOHO data, to measure subsurface convective flows. We show results for average supergranulation flows.

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