Characteristic curve of meteoric spectrograms obtained by an optical diffraction transmission grating

Details Characteristic curve of meteoric spectrograms obtained by an optical diffraction transmission grating Characteristic curve of meteoric spectrograms obtained by an optical diffraction transmission grating

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983baicz..34..173s&link_type=abstract

Astronomical Institutes of Czechoslovakia, Bulletin (ISSN 0004-6248), vol. 34, no. 3, 1983, p. 173-178.

Astronomy and Astrophysics

Astronomy

Astronomical Photometry, Gratings (Spectra), Meteoroids, Spectrograms, Light Transmission, Optical Reflection, Stellar Magnitude

Scientific paper

Relations determining the percentage representation of the light reflected by a grating are derived. To construct the characteristic curve of a plate, zero order spectra of star trails were used. The stellar magnitudes of star trails on the plate were derived from their theoretical magnitudes corrected for the speed of the stars on the plate and for the effect of the diffraction transmission grating with a triangular scratch cross-section. A numerical example is also given.

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