Cyanogen radiance/column-density ratio for comets calculated from the Swings effect

Details Cyanogen radiance/column-density ratio for comets calculated from the Swings effect Cyanogen radiance/column-density ratio for comets calculated from the Swings effect

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...135..183t&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 135, no. 1, June 1984, p. 183-187. Research supported by the Natural Sciences

Astronomy and Astrophysics

Astrophysics

36

Cn Emission, Comets, Cyanogen, Gas Density, Molecular Spectra, Radiance, Atomic Collisions, Fluorescence, Halley'S Comet, Molecular Excitation, Resonance Lines, Thermodynamic Equilibrium, Comets, Radiant Flux, Spectra, Spectrophotometry, Cyanogen, Procedure, Calculations, Velocities, Distance, Resonance, Fluoresence, Comae, Techniques, Surface, Brightness, Intensity

Scientific paper

The ratio of the radiance of the violet CN band in cometary spectra to
the column density of CN molecules has been calculated for heliocentric
radial velocities between -50 and +50 km s-1 and for
heliocentric distances between 0.5 and 6.0 AU, by taking account of the
Swings resonance-fluorescence mechanism.

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