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On the Sun's limb brightening in the visible

dc.contributor.authorElste, Günther H.en_US
dc.date.accessioned2006-09-11T13:47:28Z
dc.date.available2006-09-11T13:47:28Z
dc.date.issued1984-06en_US
dc.identifier.citationElste, G. H.; (1984). "On the Sun's limb brightening in the visible." Solar Physics 93(1): 15-21. <http://hdl.handle.net/2027.42/43755>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43755
dc.description.abstractIt is shown that in practice the method by Julius (1906) is incapable to determine the limb intensity drop. The brief intensity reversal near the extreme limb as derived from cinematography of flash spectra can be explained by diffraction.en_US
dc.format.extent303410 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.titleOn the Sun's limb brightening in the visibleen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, The University of Michigan, 48109-1090, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43755/1/11207_2004_Article_BF00156649.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00156649en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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