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Dust Morphology of Comet Hale-Bopp (C/1995 01). II. Introduction of a Working Model

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dc.contributor.author Sekanina, Z. en_US
dc.contributor.author Boehnhardt, H. en_US
dc.date.accessioned 2004-09-24T20:16:37Z
dc.date.available 2004-09-24T20:16:37Z
dc.date.issued 1998-01 en_US
dc.identifier.citation Earth, Moon, and Planets en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 98-0274 en_US
dc.identifier.uri http://hdl.handle.net/2014/19075
dc.description.abstract A Monte Carlo image simulation code for dust features in comets is applied to comet Hale-Bopp in order to model the object's persistent porcupine-like appearance on high-resolution images taken between May 11 and November 2, 1996. In this scenario, the dust-emission profile is dominated by several brief flare-ups, or puffs in the production of dust from one of the sources. en_US
dc.format.extent 635098 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other comet Hale-Bopp nucleus active area dust morphology computer modelling en_US
dc.title Dust Morphology of Comet Hale-Bopp (C/1995 01). II. Introduction of a Working Model en_US


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