Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4080
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dc.contributor.authorSastri, J. H-
dc.contributor.authorMurthy, B. S-
dc.date.accessioned2008-12-16T14:35:36Z-
dc.date.available2008-12-16T14:35:36Z-
dc.date.issued1975-04-
dc.identifier.citationSolar Physics, Vol. 41, pp. 477 - 485en
dc.identifier.issn1573-093X-
dc.identifier.urihttp://hdl.handle.net/2248/4080-
dc.descriptionOpen Access-
dc.description.abstractGeomagnetic crochets (sfe) observed at Kodaikanal over the period 1966-71 have been studied in relation to solar X-ray bursts observed by NRL satellite (SOLRAD-9) in the 0.5-3 A, 1-8 A and 8-20 A bands and radio bursts observed in the frequency range 1000-17000 MHz. The amplitude of sfe is linearly correlated with the peak intensities of X-ray bursts in the 1-8 A and 8-20 A bands. The single frequency correlation of sfe with radio bursts is a flat maximum in the frequency range 2000-3750 MHz. Following the spectral classification of AFCRL for microwave bursts, it is noticed that sfe are mostly associated with the 'A' type burst spectra and are very poorly correlated with bursts with the 'G', 'C' and 'M' type spectra. These features differ from those of other SID's reported earlier.en
dc.language.isoenen
dc.publisherD.Reidel Publishing Co.,en
dc.relation.urihttp://adsabs.harvard.edu/abs/1975SoPh...41..477Sen
dc.rightsD.Reidel Publishing Co.,-
dc.subjectMagnetic Disturbancesen
dc.subjectMicrowave Emissionen
dc.subjectSolar Radio Burstsen
dc.subjectSolar X-Raysen
dc.subjectRadio Astronomyen
dc.subjectSatellite Observationen
dc.subjectSolar Fluxen
dc.subjectSudden Ionospheric Disturbancesen
dc.titleOn the relationships between sfe (crochet) and solar X-ray and microwave burstsen
dc.typeArticleen
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