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

Sekanina, Z.; Boehnhardt,  H.

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