Abstract A preliminary analysis of the dust emission from comet Halley is presented based on large scale observations of its dust tail. Selected images obtained between February 22 and May 10, 1986 are compared to synchrone-syndyne graphs to infer the history of the dust production and the properties of the dust, at least qualitatively. Quantitative modeling of the dust tall has also been initiated and preliminary results are shown for the cases of isotropic and anisotropic (jet) dust production.
Ground-based observations of the dust emission from comet Halley
Advances in Space Research ; 5 , 12 ; 317-323
01.01.1985
7 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Fabry-Perot ground-based observations of comet Halley
Elsevier | 1985
|Coma morphology and dust emission pattern of comet Halley
Elsevier | 1985
|Comet Halley observations to date
Elsevier | 1984
|EUV observations of Comet Halley
Elsevier | 1984
|