Photographic films for the Multi-Spectral Solar Telescope Array

Details Photographic films for the Multi-Spectral Solar Telescope Array Photographic films for the Multi-Spectral Solar Telescope Array

Jan 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992spie.1546..188h&link_type=abstract

In: Multilayer and grazing incidence X-ray/EUV optics; Proceedings of the Meeting, San Diego, CA, July 22-24, 1991 (A93-39658 15

Computer Science

Sound

Image Resolution, Multispectral Photography, Multispectral Tracking Telescopes, Photographic Film, Rocket-Borne Photography, Solar Corona, Extreme Ultraviolet Radiation, Far Ultraviolet Radiation, High Resolution, Rocket Sounding, Thin Films

Scientific paper

The rocketborne Multi-Spectral Solar Telescope Array (MSSTA) uses an array of Ritchey-Chretien, Cassegrain, and Herschelian telescopes to produce ultrahigh-resolution full-disk images of the sun within the soft X-ray, EUV, and FUV ranges. Such imaging of the solar disk and corona out to several solar radii placed great demands on the MSSTA's data storage capabilities; in addition, its photographic films required very low outgassing rates. Results are presented from calibration tests conducted on the MSSTA's emulsions, based on measurements at NIST's synchrotron facility.

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