Initial Time-distance Helioseismology Results from SDO/HMI. II.

Details Initial Time-distance Helioseismology Results from SDO/HMI. II. Initial Time-distance Helioseismology Results from SDO/HMI. II.

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640235z&link_type=abstract

American Astronomical Society, AAS Meeting #216, #402.35

Astronomy and Astrophysics

Astronomy

Scientific paper

Investigations of the interaction between large-scale subsurface flows and magnetic fields are very important for understanding and predicting the processes of solar dynamo and evolution of active regions. The time-distance helioseismology data analysis pipeline (presented in our poster I) is designed to provide global-Sun maps of subsurface flows from the SDO/HMI observations every 8 hours. We present an initial subsurface flow map, and compare this with the magnetic field distribution also obtained from the HMI instrument.

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