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Two-dimensional spatial power spectra of photospheric velocity fluctuations
dc.contributor.authorTeske, Richard G.en_US
dc.date.accessioned2006-09-11T13:45:45Z
dc.date.available2006-09-11T13:45:45Z
dc.date.issued1974-03en_US
dc.identifier.citationTeske, Richard G.; (1974). "Two-dimensional spatial power spectra of photospheric velocity fluctuations." Solar Physics 39(2): 363-375. <http://hdl.handle.net/2027.42/43736>en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.issn0038-0938en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43736
dc.description.abstractTwo-dimensional spatial autocorrelation functions and power spectral density distributions were obtained from high-resolution velocity spectroheliograms. Although the autocorrelation functions indicate the existence of velocity cells of size roughly 2500 to 3500 km, the power spectra fail to reveal them because the cells are not strictly spatially periodic.en_US
dc.format.extent789047 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.titleTwo-dimensional spatial power spectra of photospheric velocity fluctuationsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumSan Fernando Observatory, the Aerospace Corporation, Calif., U.S.A.; University of Michigan, 48104, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43736/1/11207_2004_Article_BF00162429.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00162429en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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