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Dependence of the correlation of small scale photospheric structures upon resolution
dc.contributor.authorTeske, Richard G.en_US
dc.contributor.authorElste, Günther H.en_US
dc.date.accessioned2006-09-11T13:46:54Z
dc.date.available2006-09-11T13:46:54Z
dc.date.issued1979-06en_US
dc.identifier.citationTeske, R. G.; Elste, G. H.; (1979). "Dependence of the correlation of small scale photospheric structures upon resolution." Solar Physics 62(2): 241-251. <http://hdl.handle.net/2027.42/43749>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43749
dc.description.abstractCorrelations between continuum intensity, velocity, and equivalent widths of two Mn i lines as observed with two different entrance apertures tend to deteriorate with improvement in spatial resolution. The KPNO multichannel magnetograph was used to make area scans at the center of the disk with entrance apertures 3.5″×2.5″ arc and 1″×1″ arc. A coherence analysis shows that this effect is caused by marked differences of fluctuations in temperature and temperature gradients as well as in the velocity structure of photospheric elements of various sizes.en_US
dc.format.extent609892 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.titleDependence of the correlation of small scale photospheric structures upon resolutionen_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, The University of Michigan, 48109, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumDept. of Astronomy, The University of Michigan, 48109, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43749/1/11207_2004_Article_BF00155356.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00155356en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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