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The Venus ionosphere

dc.contributor.authorBauer, S. J.en_US
dc.contributor.authorBrace, L. M.en_US
dc.contributor.authorTaylor, Jr, H. A.en_US
dc.contributor.authorBreus, T. K.en_US
dc.contributor.authorKliore, A. J.en_US
dc.contributor.authorKnudsen, W. C.en_US
dc.contributor.authorNagy, Andrew F.en_US
dc.contributor.authorRussell, C. T.en_US
dc.contributor.authorSavich, N. A.en_US
dc.date.accessioned2006-04-07T19:14:04Z
dc.date.available2006-04-07T19:14:04Z
dc.date.issued1985en_US
dc.identifier.citationBauer, S. J., Brace, L. M., Taylor, Jr, H. A., Breus, T. K., Kliore, A. J., Knudsen, W. C., Nagy, A. F., Russell, C. T., Savich, N. A. (1985)."The Venus ionosphere." Advances in Space Research 5(11): 233-267. <http://hdl.handle.net/2027.42/25872>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V3S-472BDKD-N3/2/67ec924fdff9cd9d3026173a4fdac303en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/25872
dc.description.abstractPhysical properties of the Venus ionosphere obtained by experiments on the US Pioneer Venus and the Soviet Venera missions are presented in the form of models suitable for inclusion in the Venus International Reference Atmosphere. The models comprise electron density (from 120 km), electron and ion temperatures, and relative ion abundance in the altitude range from 150 km to 1000 km for solar zenith angles from 0[deg] to 180[deg]. In addition, information on ion transport velocities, ionopause altitudes, and magnetic field characteristics of the Venus ionosphere, are presented in tabular or graphical form. Also discussed is the solar control of the physical properties of the Venus ionosphere.en_US
dc.format.extent1300146 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleThe Venus ionosphereen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbsecondlevelAerospace Engineeringen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumUniversity of Michigan, Ann Arbor, MI, U.S.A.en_US
dc.contributor.affiliationotherInstitute for Meteorology and Geophysics, University of Graz and Space Research Institute, Austrian Academy of Sciences, A-8010, Graz, Austriaen_US
dc.contributor.affiliationotherNASA, Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.en_US
dc.contributor.affiliationotherNASA, Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.en_US
dc.contributor.affiliationotherSpace Research Institute, U.S.S.R. Academy of Sciences, Moscow 117810, U.S.S.R.en_US
dc.contributor.affiliationotherJet Propulsion Laboratory, Pasadena, CA 91109, U.S.A.en_US
dc.contributor.affiliationotherKnudsen Geophysical Research, Monte Sereno, CA 95030, U.S.A.en_US
dc.contributor.affiliationotherIGPP, University of California, Los Angeles, CA 90024, U.S.A.en_US
dc.contributor.affiliationotherInstitute of Radioengineering and Electronics, U.S.S.R. Academy of Sciences, Moscow, U.S.S.R.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/25872/1/0000435.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0273-1177(85)90203-0en_US
dc.identifier.sourceAdvances in Space Researchen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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