Modelling the diffuse ultraviolet radiation observed by Dynamics Explorer 1

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5256

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DC Field	Value	Language
dc.contributor.author	Shalima, P	-
dc.contributor.author	Murthy, J	-
dc.contributor.author	Fix, J. D	-
dc.date.accessioned	2010-10-20T15:34:15Z	-
dc.date.available	2010-10-20T15:34:15Z	-
dc.date.issued	2010-10	-
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 408, No. 1, pp. 53–56	en
dc.identifier.uri	http://hdl.handle.net/2248/5256	-
dc.description	Restricted Access	en
dc.description.abstract	The Dynamics Explorer spacecraft, DE-1, has undertaken two sky surveys in the far-ultraviolet regime, covering a wide variety of Galactic latitudes. We have used a single scattering dust model to probe into the optical constants and the distance of the interstellar dust clouds. We find that, in agreement with most other observations, the dust grains are strongly forward scattering with a relatively high albedo and, in addition, that the scattering is from dust sheets within 100 pc of the Sun.	en
dc.language.iso	en	en
dc.publisher	Wiley Blackwell	en
dc.relation.uri	http://dx.doi.org/10.1111/j.1365-2966.2010.17149.x	en
dc.rights	© Wiley Blackwell	en
dc.subject	Dust, extinction	en
dc.subject	Local interstellar matter	en
dc.subject	Ultraviolet: ISM	en
dc.title	Modelling the diffuse ultraviolet radiation observed by Dynamics Explorer 1	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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