Gas ionization solar spectral monitor (GISSMO)

Details Gas ionization solar spectral monitor (GISSMO) Gas ionization solar spectral monitor (GISSMO)

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1745..132v&link_type=abstract

In: Instrumentation for planetary and terrestrial atmospheric remote sensing; Proceedings of the Meeting, San Diego, CA, July 23

Computer Science

Sound

Design Analysis, Extreme Ultraviolet Radiation, Solar Instruments, Solar Spectra, Electrostatics, Gas Ionization

Scientific paper

We are currently developing an instrument free from optical components to measure the full-disk solar spectrum in the extreme ultraviolet regime covering wavelengths from 75-500 A. The instrument, which will be launched aboard a NASA Black Brant sounding rocket in September 1992, consists of a windowless noble gas ionization cell followed by a toroidal electrostatic analyzer to spatially disperse photoelectrons as a function of their energies. A microchannel plate based position sensitive detector will be used to detect individual electrons, indirectly returning the solar EUV spectrum.

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