Studies on the Temperature Structure and Heating of the Solar Corona by SolarB and Solar Magnetic Activity Research Telescope (SMART)

Details Studies on the Temperature Structure and Heating of the Solar Corona by SolarB and Solar Magnetic Activity Research Telescope (SMART) Studies on the Temperature Structure and Heating of the Solar Corona by SolarB and Solar Magnetic Activity Research Telescope (SMART)

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..325..325n&link_type=abstract

The Solar-B Mission and the Forefront of Solar Physics, ASP Conference Series, Vol. 325, Proceedings of the Fifth Solar-B Scienc

Physics

Scientific paper

In this paper, we discuss the coordinated observation by SolarB and
Solar Magnetic Activity Research Telescope (SMART) for the coronal
heating study. The high time cadence wide field view vector magnetic
field maps obtained by SMART will be essential for the large scale
magnetic field evolution and its relationship to the coronal heating.

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