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Soft solar X-rays and solar activity
dc.contributor.authorTeske, Richard G.en_US
dc.date.accessioned2006-09-11T13:43:59Z
dc.date.available2006-09-11T13:43:59Z
dc.date.issued1971-09en_US
dc.identifier.citationTeske, Richard G.; (1971). "Soft solar X-rays and solar activity." Solar Physics 19(2): 356-378. <http://hdl.handle.net/2027.42/43715>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43715
dc.description.abstractSoft solar X-rays in the wavelength interval 8–12 Å were observed from OSO III. The totality of the observations that were made between 9 March, 1967, and 18 May, 1968, is summarized graphically and compared to the course of solar activity as observed at other wavelengths, with particular emphasis upon visible activity.en_US
dc.format.extent1028254 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.titleSoft solar X-rays and solar activityen_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 and the McMath-Hulbert Observatory, The University of Michigan, Ann Arbor, Mich., U.S.Aen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43715/1/11207_2004_Article_BF00146064.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00146064en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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