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Calculated [OI] 6300 A nightglow doppler temperatures for solar cycle minimum

dc.contributor.authorRoble, Raymond Geralden_US
dc.contributor.authorHays, Paul B. (Paul Byron)en_US
dc.contributor.authorNagy, Andrew F.en_US
dc.date.accessioned2006-04-17T15:26:55Z
dc.date.available2006-04-17T15:26:55Z
dc.date.issued1968-09en_US
dc.identifier.citationRoble, R. G., Hays, P. B., Nagy, A. F. (1968/09)."Calculated [OI] 6300 A nightglow doppler temperatures for solar cycle minimum." Planetary and Space Science 16(9): 1109-1113. <http://hdl.handle.net/2027.42/33122>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V6T-46YM3SF-SN/2/8a51f82a143d3f74a33aaa15f560610aen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/33122
dc.description.abstractThe effective doppler temperatures of the nightglow [OI]6300 A line are calculated using the data of Evans (1967) for electron density and ion temperature variations throughout the night during solar cycle minimum. These temperatures are shown to follow the exospheric temperature closely but at a value of 25-50[deg]K lower in most cases.en_US
dc.format.extent345310 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleCalculated [OI] 6300 A nightglow doppler temperatures for solar cycle minimumen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumAerospace Engineering Department, University of Michigan, Ann Arbor, Michigan, USAen_US
dc.contributor.affiliationumAerospace Engineering Department, University of Michigan, Ann Arbor, Michigan, USAen_US
dc.contributor.affiliationumElectrical Engineering Department, University of Michigan, Ann Arbor, Michigan, USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/33122/1/0000508.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0032-0633(68)90123-2en_US
dc.identifier.sourcePlanetary and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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