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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1549
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dc.contributor.authorLakhina, G. S-
dc.date.accessioned2007-05-09T05:58:33Z-
dc.date.available2007-05-09T05:58:33Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 537-540en
dc.identifier.urihttp://hdl.handle.net/2248/1549-
dc.description.abstractIon tearing mode instability of the forced current sheets is studied. The trapped electrons have a strong stabilizing effect on the excitation of the instability. The presence of background turbulence can effectively lead to the untrapping of the electron orbits and, thus, facilitate excitation of ion tearing instability. Respective scenarios for magnetospheric substorms, solar flares and coronal transients are discusseden
dc.format.extent333948 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectCurrent sheetsen
dc.subjectAstrophysical Plasmasen
dc.titleDisruption of forced current sheets in astrophysical plasmasen
dc.typeArticleen
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