On the formation and evolution of gaseous structures in Comet P/Halley

Details On the formation and evolution of gaseous structures in Comet P/Halley On the formation and evolution of gaseous structures in Comet P/Halley

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..103..319s&link_type=abstract

Icarus (ISSN 0019-1035), vol. 103, no. 2, p. 319-328.

Mathematics

7

Cometary Atmospheres, Evolution (Development), Gas Jets, Halley'S Comet, Comet Nuclei, Mathematical Models, Comets, Halley, Origin, Formation, Evolution, Gases, Structure, Jets, Numerical Methods, Simulation, Cn Radical, Jetting, Comae, Morphology, Comet Nuclei, Origin, Source, Velocity, Parent Material, Ejection, Models, Parameters, Comparison, Theoretical Studies, Equatorial Region

Scientific paper

The possibility of a dynamic connection between the CN jets and CN shells in the coma of Comet P/Halley is here investigated through numerical simulations on the spatial and temporal evolution of gaseous jets. The evolution of such a jet into a shell is found to be straightforward for several geometries. It is noted that a closed shell structure may be due to a near-equatorial observational view of material derived from the active region near the nucleus equator.

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