Please use this identifier to cite or link to this item: http://nopr.niscair.res.in/handle/123456789/29997
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dc.contributor.authorKulkarni, V H-
dc.contributor.authorKane, R P-
dc.date.accessioned2014-11-27T09:39:05Z-
dc.date.available2014-11-27T09:39:05Z-
dc.date.issued2003-12-
dc.identifier.issn0975-105X (Online); 0367-8393 (Print)-
dc.identifier.urihttp://hdl.handle.net/123456789/29997-
dc.description385-386en_US
dc.description.abstractThe magnetic Z field variation for the period 9-25 Dec. 1996, recorded at the stations Sodankyla (67.37°N, 26.63°E), Tromso (69.67°N, 18.95°E), Abisko (68.30°N, 18.82°E), and Hornsund (77.00°N, 26.63°E) (http://swdcwww.kugi.kyoto-u.ac.jp) are compared with the Geminids (12-15 Dec. 1996) and Ursids (20-23 Dec. 1996) showers as reported by Yrjola (http://www.rmob.org). The correlation studies show that it is difficult to prove conclusively that the magnetic field fluctuations observed at Sodankyla are due to the dust particles in the meteor showers and the associated changes in the ionospheric currents due to them. en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJRSP Vol.32(6) [December 2003]en_US
dc.subjectMagnetic fielden_US
dc.subjectMeteor showersen_US
dc.subjectIonospheric currenten_US
dc.titleOn the relationship between the magnetic field variations and meteor showersen_US
dc.typeArticleen_US
Appears in Collections: IJRSP Vol.32(6) [December 2003]

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