Axisymmetric gas flow from a comet nucleus

Details Axisymmetric gas flow from a comet nucleus Axisymmetric gas flow from a comet nucleus

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..637k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Oct. 1983, p. 637-640) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Sept.-Oct.

Astronomy and Astrophysics

Astronomy

2

Axisymmetric Flow, Comet Nuclei, Outgassing, Albedo, Coma, Solar Radiation, Solar Wind, Vaporizing

Scientific paper

Under a sufficiently high rate of comet matter cooling an axial
symmetric outflow is shown to take place due to the anisotropy of solar
radiation coming to the nucleus surface. The dynamic pressure of the gas
and the nucleus-to-coma light contrast turn out to be essentially larger
than in the case of a spherically symmetric flow.

Affiliated with

Also associated with

No associations

Rating

Axisymmetric gas flow from a comet nucleus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Axisymmetric gas flow from a comet nucleus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Axisymmetric gas flow from a comet nucleus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1195069