HMI Measurements Of The Solar Magnetic Field

Details HMI Measurements Of The Solar Magnetic Field HMI Measurements Of The Solar Magnetic Field

May 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011spd....42.1712h&link_type=abstract

American Astronomical Society, SPD meeting #42, #17.12; Bulletin of the American Astronomical Society, Vol. 43, 2011

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Scientific paper

The Helioseismic and Magnetic Imager (HMI) on NASA's Solar Dynamics Observatory (SDO) routinely produces a comprehensive array of magnetic field data products including 45-second line-of-sight magnetograms, synoptic maps and synchronic frames, 12-minute vector field time series in HMI Active Region Patches (HARPs), model calculations of the coronal field and solar wind, and near-real-time parameters for space weather. Other products, such as surface flow maps, can be produced on demand or on request. We present examples of data products generated during the first year of operations and compare some of these with measurements from other observatories, including the now-dormant MDI. The HMI Team is sponsored by NASA.

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