FLCT: A Fast, Efficient Method for Performing Local Correlation Tracking

Details FLCT: A Fast, Efficient Method for Performing Local Correlation Tracking FLCT: A Fast, Efficient Method for Performing Local Correlation Tracking

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.9211f&link_type=abstract

American Astronomical Society Meeting 210, #92.11; Bulletin of the American Astronomical Society, Vol. 39, p.210

Statistics

Computation

Scientific paper

We describe the computational techniques for the recently updated FLCT local correlation tracking method. The FLCT code is then evaluated using a series of simple 2D known flow patterns that test its accuracy and characterize its errors. Finally, flow patterns derived from observed magnetogram and white light data are compared, and the differences interpreted.
This work is supported by the NASA Heliophysics Division through funding from the SR&T and Theory Programs, and by NSF-ATM through the SHINE program.

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