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Time Variabilities of Solar Wind Ion Fluxes and of X-ray and EUV Emissions from Comet Hyakutake

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dc.contributor.author Neugebauer, M. en_US
dc.contributor.author Cravens, T. en_US
dc.contributor.author Lisse, C. en_US
dc.contributor.author Ipavich, F. en_US
dc.contributor.author von Steiger, R. en_US
dc.contributor.author Shah, P. en_US
dc.contributor.author Armstrong, T. en_US
dc.date.accessioned 2004-09-23T23:32:19Z
dc.date.available 2004-09-23T23:32:19Z
dc.date.issued 1999 en_US
dc.identifier.citation Journal of Geophysical Research en_US
dc.identifier.citation U.S.A. en_US
dc.identifier.clearanceno 99-0590 en_US
dc.identifier.uri http://hdl.handle.net/2014/17166
dc.description.abstract Observations of X-ray and extreme ultraviolet (EUV) emissions from comet C/Hyakutake 1996 B2 made by the Rontgen X-ray satellite (ROSAT) and the Extreme Ultraviolet Explorer (EUVE) revealed a total X-ray luminosity of about 500 MW. en_US
dc.format.extent 971200 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other X-ray extreme ultraviolet (EUV) emissions Hyakutake ROSAT EUVE solar wind heavy ion fluxes en_US
dc.title Time Variabilities of Solar Wind Ion Fluxes and of X-ray and EUV Emissions from Comet Hyakutake en_US


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