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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4695
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dc.contributor.authorSatya Narayanan, A-
dc.date.accessioned2009-07-31T10:24:12Z-
dc.date.available2009-07-31T10:24:12Z-
dc.date.issued1999-12-
dc.identifier.citationA. Wilson., eds., Magnetic Fields and Solar Processes. The 9th European Meeting on Solar Physics, held 12 - 18 September, 1999, in Florence, Italy., pp. 647 - 652en
dc.identifier.isbn92-9092-792-5-
dc.identifier.urihttp://hdl.handle.net/2248/4695-
dc.language.isoenen
dc.publisherEuropean Space Agencyen
dc.relation.ispartofseriesESA SP No. 448-
dc.relation.urihttp://adsabs.harvard.edu/abs/1999ESASP.448..647Nen
dc.rights© European Space Agencyen
dc.subjectCoronal Loopsen
dc.subjectStabilityen
dc.titleA simple model for coronal loops and their stabilityen
dc.typeArticleen
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