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S.P. Rajaguru, S.J. Hughes, M.J. Thompson (The Blackett Laboratory, Imperial College London)
We present first results from time-distance helioseismic analysis of a few active regions using the new merged sequences of data from GONG+ instruments. In particular we focus on issues related to the resolution achievable from GONG+ data and also estimate their noise properties.Results from inversions for sound speed changes beneath active regions will be presented with initial comparisons between first and second bounce time-distance data for acoustic rays passing under a spot. We acknowledge support from the UK Particle Physics and Astronomy Research Council.
The author(s) of this abstract have provided an email address for comments about the abstract: p.rajaguru@imperial.ac.uk
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Bulletin of the American Astronomical Society, 35 #3
© 2003. The American Astronomical Soceity.