Physics
Scientific paper
Jun 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...52c&link_type=abstract
Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, May-June 1986, p. 52-58. In Russian.
Physics
Brightness Distribution, Comet Tails, Interplanetary Dust, Surface Properties, Axisymmetric Flow, Comet Nuclei, Particle Motion
Scientific paper
A method for calculating the theoretical brightness distribution in a
cometary dust tail is described for axisymmetric outflow of dust from
the nucleus. The procedure is worked out for a type II tail.
Chernyi G. F.
Sizonenko Iu. V.
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