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On the relationships between sfe (crochet) and solar X-ray and microwave bursts

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dc.contributor.author Sastri, J. H
dc.contributor.author Murthy, B. S
dc.date.accessioned 2008-12-16T14:35:36Z
dc.date.available 2008-12-16T14:35:36Z
dc.date.issued 1975-04
dc.identifier.citation Solar Physics, Vol. 41, pp. 477 - 485 en
dc.identifier.issn 1573-093X
dc.identifier.uri http://hdl.handle.net/2248/4080
dc.description Open Access
dc.description.abstract Geomagnetic 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.iso en en
dc.publisher D.Reidel Publishing Co., en
dc.relation.uri http://adsabs.harvard.edu/abs/1975SoPh...41..477S en
dc.rights D.Reidel Publishing Co.,
dc.subject Magnetic Disturbances en
dc.subject Microwave Emission en
dc.subject Solar Radio Bursts en
dc.subject Solar X-Rays en
dc.subject Radio Astronomy en
dc.subject Satellite Observation en
dc.subject Solar Flux en
dc.subject Sudden Ionospheric Disturbances en
dc.title On the relationships between sfe (crochet) and solar X-ray and microwave bursts en
dc.type Article en


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