SMM X ray polychromator

Details SMM X ray polychromator SMM X ray polychromator

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lock.reptq....s&link_type=abstract

Final Report, Jun. 1988 - Jul. 1993 Lockheed Missiles and Space Co., Palo Alto, CA. Solar and Astrophysics Lab.

Physics

Imaging Spectrometers, Solar Flares, Solar Spectrometers, Solar Wind, Plasma Equilibrium, Solar Physics, X Ray Spectroscopy

Scientific paper

The objective of the X-ray Polychromator (XRP) experiment was to study the physical properties of solar flare plasma and its relation to the parent active region to understand better the flare mechanism and related solar activity. Observations were made to determine the temperature, density, and dynamic structure of the pre-flare and flare plasma as a function of wavelength, space and time, the extent to which the flare plasma departs from thermal equilibrium, and the variation of this departure with time. The experiment also determines the temperature and density structure of active regions and flare-induced changes in the regions.

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