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On determining the ozone number density distribution from OAO-2 stellar occultation measurements
dc.contributor.authorRoble, Raymond Geralden_US
dc.contributor.authorHays, Paul B. (Paul Byron)en_US
dc.date.accessioned2006-04-07T16:44:52Z
dc.date.available2006-04-07T16:44:52Z
dc.date.issued1974-09en_US
dc.identifier.citationRoble, R. G., Hays, P. B. (1974/09)."On determining the ozone number density distribution from OAO-2 stellar occultation measurements." Planetary and Space Science 22(9): 1337-1340. <http://hdl.handle.net/2027.42/22293>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V6T-46YJVJ5-12W/2/6cb24b73075bcd80b68c90b59a2cab10en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/22293
dc.description.abstractStellar occultation data from the 2460 A and 2980 A channels of the OAO-2 stellar photometers have been used to derive the nighttime ozone number density distribution in the low latitude mesosphere. The nighttime ozone distribution obtained from both channels are similar indicating a maximum in the ozone distribution near 80km of 2-3 x 103cm-3.en_US
dc.format.extent424250 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleOn determining the ozone number density distribution from OAO-2 stellar occultation measurementsen_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.affiliationumDepartment of Atmospheric and Oceanic Sciences, University of Michigan, Ann Arbor, Michigan 48105, U.S.A.en_US
dc.contributor.affiliationotherNational Center for Atmospheric Research,en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/22293/1/0000734.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0032-0633(74)90054-3en_US
dc.identifier.sourcePlanetary and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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