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 |