Requirements for future solar-physics missions with X ray instrumentation

Details Requirements for future solar-physics missions with X ray instrumentation Requirements for future solar-physics missions with X ray instrumentation

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993esasp1157..147c&link_type=abstract

In ESA, Scientific Requirements for Future Solar-Physics Space Missions p 147-159 (SEE N94-22837 06-92)

Physics

Solar Corona, Solar Physics, Space Missions, X Ray Imagery, X Ray Spectroscopy, High Temperature, Observation, Requirements, Solar Flares, Solar Radiation

Scientific paper

Several overall requirements for solar x-ray missions are stated and an outline of the underlying coronal physics is presented. The available techniques for x-ray imaging of the Sun are discussed and compared with reference to previous and ongoing missions. Solar x-ray spectroscopy is assessed in the same manner. Possible choices for future instruments in these two areas are discussed. X-rays are taken to lie broadly in the photon energy range 0.1 to 100 keV. Solar studies at these energies will be mainly concerned with high temperature coronal plasma and nonthermal radiation from particle beams produced in flares.

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