Haser model CN, C2 and C3 production rates in some comets

Details Haser model CN, C2 and C3 production rates in some comets Haser model CN, C2 and C3 production rates in some comets

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989em%26p...47...15d&link_type=abstract

Earth, Moon, and Planets (ISSN 0167-9295), vol. 47, Oct. 1989, p. 15-31.

Physics

9

Carbon, Cometary Atmospheres, Cyanogen, Polyatomic Molecules, Synthesis (Chemistry), Correlation, Kohoutek Comet, Visible Spectrum

Scientific paper

Emission fluxes of CN, C2 and C3 species observed in the coma of some comets are analyzed in the framework of Haser model. CN, C2 and C3 production rates are determined using recently derived fluorescence efficiencies and dependence of CN, C2 and C3 production rates on the heliocentric distance is studied. Evidence for a burst type activity around January 15, 1974 in the postperihelion period of Comet Kohoutek (1973) is observed.

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