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A comparison of the temperature and emission measure of X-ray active regions with coronal magnetic fields
dc.contributor.authorBurl, J. B.en_US
dc.contributor.authorTeske, Richard G.en_US
dc.contributor.authorMayfield, E. B.en_US
dc.date.accessioned2006-09-11T13:47:05Z
dc.date.available2006-09-11T13:47:05Z
dc.date.issued1979-08en_US
dc.identifier.citationBurl, J. B.; Teske, R. G.; Mayfield, E. B.; (1979). "A comparison of the temperature and emission measure of X-ray active regions with coronal magnetic fields." Solar Physics 63(1): 157-164. <http://hdl.handle.net/2027.42/43751>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43751
dc.description.abstractThe distribution of temperature and of emission measure in X-ray active regions relative to the coronal magnetic fields has been investigated. The position of maximum temperature and the position of maximum emission measure were found to lie along the magnetic neutral line, with the maximum temperature tending to lie above the position of an abrupt change in direction of the neutral line. Several simple structural models of these regions are compared to the emission measure. The total magnetic energy and the total emission measure appear to be related by a power law in the regions studied by us.en_US
dc.format.extent456278 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.titleA comparison of the temperature and emission measure of X-ray active regions with coronal magnetic fieldsen_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, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationumDepartment of Astronomy, The University of Michigan, 48109, Ann Arbor, Mich., U.S.A.en_US
dc.contributor.affiliationotherSpace Sciences Laboratory, The Aerospace Corporation, 90009, Los Angeles, Calif., U.S.A.en_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43751/1/11207_2004_Article_BF00155706.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00155706en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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