Time-Distance Studies of Large Scale Flows on the Sun

Details Time-Distance Studies of Large Scale Flows on the Sun Time-Distance Studies of Large Scale Flows on the Sun

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsh11b0707b&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SH11B-0707

Physics

7522 Helioseismology, 7544 Stellar Interiors And Dynamo Theory

Scientific paper

Time distance helioseismology is a valuable tool for examining flows in the convection zone. It can produce vector maps of flows from the travel time of waves traversing subsurface ray paths. This technique has been proven useful for studying solar phenomena ranging in size from supergranules to global flows. (1999) Giles et al has demonstrated the efficacy of using the time-distance technique on meridional and zonal flows. We extend this work and show resulting measurements.

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