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Preliminary results on the apparent size of the sources of type III bursts observed at low frequencies

dc.contributor.authorAlvarez, Hectoren_US
dc.date.accessioned2006-09-11T13:46:17Z
dc.date.available2006-09-11T13:46:17Z
dc.date.issued1976-02en_US
dc.identifier.citationAlvarez, Hector; (1976). "Preliminary results on the apparent size of the sources of type III bursts observed at low frequencies." Solar Physics 46(2): 483-491. <http://hdl.handle.net/2027.42/43742>en_US
dc.identifier.issn0038-0938en_US
dc.identifier.issn1573-093Xen_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43742
dc.description.abstractWe present preliminary results on the apparent angular size of the sources of four type III bursts observed between 3500 and 50 kHz from the IMP-6 spacecraft. The observations were made with a dipole rotating in the plane of the ecliptic where the sources are assumed to be. The apparent angular sizes obtained are unexpectedly large. We discuss different explanations for the results. It seems that the scattering of radio waves by electron density inhomogeneities is the most likely cause.en_US
dc.format.extent438235 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.otherAstrophysicsen_US
dc.subject.otherPhysicsen_US
dc.titlePreliminary results on the apparent size of the sources of type III bursts observed at low frequenciesen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumRadio Astronomy Observatory, The University of Michigan, Ann Arbor, Mich., U.S.A.; Centro de Investigación de Astronomía, Apartado 264, Mérida, Venezuelaen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43742/1/11207_2004_Article_BF00149873.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1007/BF00149873en_US
dc.identifier.sourceSolar Physicsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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