Computer Science – Performance
Scientific paper
Jan 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aiaa.meetqq...s&link_type=abstract
American Institute of Aeronautics and Astronautics, Aerospace Sciences Meeting, 19th, St. Louis, Mo., Jan. 12-15, 1981, 9 p.
Computer Science
Performance
Ebert Spectrometers, Performance Prediction, Polarimeters, Satellite-Borne Instruments, Solar Maximum Mission, Ultraviolet Spectrometers, Design Analysis, Photomultiplier Tubes, Spaceborne Telescopes
Scientific paper
The instrument observes spectral line intensity, Doppler motions, and polarization parameters. First Dopplergrams of the sun showing mass motion of prominences have been obtained. The instrument consists of a telescope, a spectrometer, a polarimeter, and five detectors. Spectral range extends from 1150 to 3600 Angstroms. The telescope is an alphanatic Gregorian capable of scanning a 256 x 256 arcsecond raster. The spectrometer is an Ebert-Fastie mount with exchangeable slits for intensity measurements and spectroscopy. Detectors are photomultipliers operating in the pulse-counting mode.
Bethke G. W.
Brunner C. E.
Buzinski R. E.
Franklin R. L.
Knox E. D.
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