Silicon vidicon spectrometry and its infrared capabilities for solar research

Details Silicon vidicon spectrometry and its infrared capabilities for solar research Silicon vidicon spectrometry and its infrared capabilities for solar research

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apopt..15.2884p&link_type=abstract

Applied Optics, vol. 15, Nov. 1976, p. 2884-2890. Research supported by the National Geographic Society and Research Corp.

Physics

Optics

1

Infrared Spectrometers, Silicon Junctions, Solar Corona, Solar Eclipses, Solar Spectrometers, Vidicons, Data Acquisition, Emission Spectra, Forbidden Bands, Image Tubes

Scientific paper

A description is given of the use of a rapid-scanning silicon vidicon spectrometer at the total solar eclipse of June 30, 1973. The instrument had been employed to observe the two strong IR coronal emission lines, which are forbidden lines, of Fe XIII. The ratio of the intensity of the 1074.7-nm and 1079.8-nm lines is relatively insensitive to coronal temperature and depends sensitively on the coronal electron density.

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