Science with the Solar-B X-Ray Telescope

Details Science with the Solar-B X-Ray Telescope Science with the Solar-B X-Ray Telescope

May 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...204.6905d&link_type=abstract

American Astronomical Society Meeting 204, #69.05; Bulletin of the American Astronomical Society, Vol. 36, p.795

Astronomy and Astrophysics

Astronomy

Scientific paper

The Solar-B mission will launch in 2006 with three telescopes: a high resolution visible light telescope feeding filtergraph and spectropolarimeter focal plane instruments, a grazing incidence X-Ray telescope and an EUV spectrograph. This combination of instruments will provide detailed information on Active Region evolution, heating, connectivity and dynamics. The X-Ray telescope on Solar-B will be sensitive to emission from 1-50MK. Focal plane filters will allow us to follow the evolution of the bulk of the coronal plasma. This poster will describe the core science that will be done by XRT together with EIS and SOT. Joint observing programs will also be discussed.

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