dc.contributor.author | Sekaniana, Z. | en_US |
dc.date.accessioned | 2004-09-26 | |
dc.date.available | 2004-09-26 | |
dc.date.issued | 1997-03-20 | en_US |
dc.identifier.citation | USA | en_US |
dc.identifier.clearanceno | 97-0798 | en_US |
dc.identifier.uri | http://hdl.handle.net/2014/22322 | |
dc.description.abstract | A Monte Carlo computer simulation code for generating synthetic images of dust features in comets is applied to comet Hale-Bopp to model the diurnal evolution of a bright jet and the appearance of nearly concentric halos. | en_US |
dc.format.extent | 574519 bytes | |
dc.format.mimetype | application/pdf | |
dc.language.iso | en_US | |
dc.subject.other | comet-Hale-Bopp diurnal evolution of a dust jet dust halos nuclear rotation emission sources | en_US |
dc.title | Modelling two dust features in comet Hale-Bopp (1995 O1) | en_US |