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The Herschel effect and solar photography
dc.contributor.authorJayanthan, R.en_US
dc.date.accessioned2006-09-11T13:43:18Z
dc.date.available2006-09-11T13:43:18Z
dc.date.issued1970-04en_US
dc.identifier.citationJayanthan, R.; (1970). "The Herschel effect and solar photography." Solar Physics 12(1): 163-166. <http://hdl.handle.net/2027.42/43708>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43708
dc.description.abstractA method of photographing the solar image in the UV part of the solar spectrum is described. The resulting images show the bright photospheric network of Sheeley and Chapman; these have been recorded at the small central distance of 20°. During a flare of importance 1b near a spot group, no detectable changes in the spots, their relative positions or the bright photospheric network could be observed.en_US
dc.format.extent862070 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.titleThe Herschel effect and solar photographyen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumMath-Hulbert Observatory, The University of Michigan, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43708/1/11207_2005_Article_BF02276575.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF02276575en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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