Hard- and software problems of spaced meteor observations by optical electronics

Details Hard- and software problems of spaced meteor observations by optical electronics Hard- and software problems of spaced meteor observations by optical electronics

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987maph...25..416s&link_type=abstract

In International Council of Scientific Unions, Middle Atmosphere Program. Handbook for MAP, Volume 25 p 416-420 (SEE N88-14502 0

Astronomy and Astrophysics

Astronomy

Meteoroid Showers, Optical Equipment, Radar Tracking, Spectral Sensitivity, Error Analysis, Photocathodes, Star Distribution, Stellar Spectrophotometry

Scientific paper

An optical electronic facility is being used for meteor observations along with meteor radars and astronomical TV. The main parts of the facility are cameras using UM-92 optical electronic image tubes. The three cascade optical electronic image tube with magnetic focusing has a 40 mm cathode and resolution in the center of up to 30 pairs of lines/mm. The photocathode is of a multislit S-20 type. For meteor spectra observations, replica gratings of 200 and 300 lines/mm are used as the dispersive element.

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