Initial Time-Distance Helioseismology Results from SDO/HMI. I.

Details Initial Time-Distance Helioseismology Results from SDO/HMI. I. Initial Time-Distance Helioseismology Results from SDO/HMI. I.

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21640234z&link_type=abstract

American Astronomical Society, AAS Meeting #216, #402.34

Astronomy and Astrophysics

Astronomy

Scientific paper

The Helioseismic and Magnetic Imager on Solar Dynamics Observatory provides uninterrupted high-resolution observations of solar oscillations over the entire disk. This gives a unique opportunity for mapping subsurface flows and wave-speed structures and investigating their role in the Sun's dynamics and magnetic activity on various scales by methods of local helioseismology. A data analysis pipeline for the time-distance helioseismology analysis has been developed and implemented at the SDO Joint Science Operation Center (JSOC) at Stanford. It provides near-real time processing of the helioseismology data. We present the basic characteristics and capabilities of the pipeline, initial time-distance measurement results, and compare these with the simultaneous SOHO/MDI measurements.

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