Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3833
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dc.contributor.authorMakarov, V. I-
dc.contributor.authorFatianov, M. P-
dc.contributor.authorSivaraman, K. R-
dc.date.accessioned2008-09-23T14:16:43Z-
dc.date.available2008-09-23T14:16:43Z-
dc.date.issued1983-06-
dc.identifier.citationSolar Physics, Vol. 85, No. 2, pp. 215 - 226en
dc.identifier.issn0038-0938-
dc.identifier.urihttp://hdl.handle.net/2248/3833-
dc.description.abstractPoleward migration of the magnetic neutral line on the sun has been calculated for the periods 1945-1950 and 1955-1981 using synoptic charts based on H-alpha observations. Epochs of sign reversal of the solar magnetic field at latitudes 50 to 90 deg have been determined for these periods. During the cycles 19 and 20 a threefold sign reversal took place in the northern hemisphere. During all the above cycles both the solar poles were of one polarity for a period ranging from 0.5 to 1 year. The poleward drift velocity of the magnetic neutral line varies from 6 to 29 m/s and seems to depend on the strength of the cycle.en
dc.language.isoenen
dc.publisherSpringeren
dc.relation.urihttp://www.springerlink.com/content/g615410654h26604/en
dc.relation.urihttp://adsabs.harvard.edu/abs/1983SoPh...85..215Men
dc.subjectLines of Forceen
dc.subjectMagnetic Field Configurationsen
dc.subjectMagnetic Polesen
dc.subjectSolar Magnetic Fielden
dc.subjectDrift Rateen
dc.subjectLatitudeen
dc.subjectLong Term Effectsen
dc.subjectNorthern Hemisphereen
dc.subjectPolarityen
dc.subjectTemporal Distributionen
dc.titlePoleward migration of the magnetic neutral line and the reversal of the polar fields on the sun. I - Period 1945-1981en
dc.typeArticleen
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