Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3774
Full metadata record
DC FieldValueLanguage
dc.contributor.authorSastri, J. H-
dc.date.accessioned2008-09-22T15:31:00Z-
dc.date.available2008-09-22T15:31:00Z-
dc.date.issued1985-04-
dc.identifier.citationCanadian Journal of Physics, Vol, 63, No. 4, pp. 472 - 474en
dc.identifier.issn0008-4204-
dc.identifier.urihttp://hdl.handle.net/2248/3774-
dc.descriptionOpen Access-
dc.description.abstractA superposed epoch analysis has been carried out of h′F values at Kodaikanal (10°14′N, 77°28′E, dip 3.0°N) pertaining to years of high sunspot activity using solar wind sector boundary passages past the earth as key days. It is found that there is a reduction in h′F values at 2000 LT 1 or 2 days after the sector boundary crossing. The amplitude of this effect which is noticed with both (+, −) and (−, +) sector boundary crossings is higher in equinoxes than in solstices. The response of the equatorial F region to sector boundary crossing seems to originate from perturbations of the equatorial east–west electric field in the post-sunset period associated with the enhancement in geomagnetic activity in the wake of sector boundary crossing.en
dc.language.isoenen
dc.publisherNational Research Council of Canadaen
dc.relation.urihttp://pubs.nrc-cnrc.gc.ca/cgi-bin/rp/rp2_abst_e?cjp_p85-073_63_ns_nf_cjpen
dc.rights© National Research Council of Canada-
dc.subjectEarth Ionosphere:Solar Winden
dc.subjectSolar Wind:Earth Ionosphereen
dc.titleResponse of the equatorial ionosphere to solar magnetic sector crossingen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Response of the equatorial ionosphere to solar magnetic sector crossingOpen Access197.53 kBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.