Horizontal Velocity Structure of Supergranules near Disk Center from High-Resolution SoHO/MDI Observations

Details Horizontal Velocity Structure of Supergranules near Disk Center from High-Resolution SoHO/MDI Observations Horizontal Velocity Structure of Supergranules near Disk Center from High-Resolution SoHO/MDI Observations

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997spd....28.0265s&link_type=abstract

American Astronomical Society, SPD meeting #28, #02.65; Bulletin of the American Astronomical Society, Vol. 29, p.904

Astronomy and Astrophysics

Astronomy

Scientific paper

We determine the average surface flows in supergranules from high-resolution SoHO/MDI observations near disk center, using local correlation and feature tracking methods. We present results as a function of distance to the supergranule center and of supergranule size, and as a function of normalized distance to the supergranule center. This work was supported by NASA Grant NAG5-3077 at Stanford and Lockheed Martin, and by AFOSR and the Fellows Program of AF Phillips Lab at NSO/SP.

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