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Core electron densities of coronal polar plumes

dc.contributor.authorPsujek, Casimir J.en_US
dc.contributor.authorTeske, Richard G.en_US
dc.date.accessioned2006-09-11T13:44:54Z
dc.date.available2006-09-11T13:44:54Z
dc.date.issued1972-12en_US
dc.identifier.citationPsujek, Casimir J.; Teske, Richard G.; (1972). "Core electron densities of coronal polar plumes." Solar Physics 27(2): 420-425. <http://hdl.handle.net/2027.42/43726>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43726
dc.description.abstractThe electron density in the cores of coronal polar plumes that is determined from observations will depend upon the assumed electron density distribution through the plume in a direction normal to its axis. Core electron densities obtained by Saito (1965) and by Newkirk and Harvey (1968) were derived using different assumed electron density profiles, and are not in agreement. We have re-discussed Saito's data using Newkirk and Harvey's electron density profile and find that the disagreement persists. Whether this indicates a true variation in electron density in plume cores cannot now be stated. Errors in the electron densities derived here may arise through errors in measuring the angles θ and α which enter into the analysis. While plausible variations in θ produce no appreciable errors in core electron density, plausible variations in α may introduce appreciable errors into the determinations of that quantity.en_US
dc.format.extent325617 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; D. Reidel Publishing Company ; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstrophysicsen_US
dc.titleCore electron densities of coronal polar plumesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDept. of Astronomy, University of Michigan, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumDept. of Astronomy, University of Michigan, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43726/1/11207_2004_Article_BF00153112.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00153112en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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