Physics
Scientific paper
Jan 2012
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012soph..275..207s&link_type=abstract
Solar Physics, Volume 275, Issue 1-2, pp. 207-227
Physics
7
Scientific paper
The Helioseismic and Magnetic Imager (HMI) instrument and investigation as a part of the NASA Solar Dynamics Observatory (SDO) is designed to study convection-zone dynamics and the solar dynamo, the origin and evolution of sunspots, active regions, and complexes of activity, the sources and drivers of solar magnetic activity and disturbances, links between the internal processes and dynamics of the corona and heliosphere, and precursors of solar disturbances for space-weather forecasts. A brief overview of the instrument, investigation objectives, and standard data products is presented.
Bogart Richard. S.
Bush Rock I.
Duvall Thomas L.
Hoeksema Jon Todd
Kosovichev Aleksandr G.
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