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dc.contributor.authorSinha, Ashwini K.
dc.contributor.authorRajaram, R.
dc.date.accessioned2015-05-05T11:57:07Z
dc.date.accessioned2021-02-12T09:35:43Z-
dc.date.available2015-05-05T11:57:07Z
dc.date.available2021-02-12T09:35:43Z-
dc.date.issued1997
dc.identifier.citationJGR, v.102/A8, p.17649-17657, 1997.en_US
dc.identifier.urihttp://localhost:8080/xmlui/handle/123456789/50-
dc.description.abstractIt has been shown that the failure of the classical WKB approach in reproducing the correct frequency spectrum and spatial structures of field line resonances should be attributed to the inability of the method to provide a natural solution close to the turning points. A direct analytic solution has been formulated to derive the toroidal field line resonance structure. Finally, the solutions thus obtained have been compared with the numerically found exact solutions in order to test the authenticity of the formalism.en_US
dc.language.isoenen_US
dc.subjectMagnetosphereen_US
dc.subjectEigen valueen_US
dc.subjectToroidalen_US
dc.subjectWKB approachen_US
dc.titleAn analytic approach to toroidal eigen modeen_US
dc.typeArticleen_US
dc.identifier.accession090535
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