1. IIA Institutional Repository
  2. IIAP Publications
  3. IIAP Publications
Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2989
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBarletta, W-
dc.contributor.authorGershtein, S. S-
dc.contributor.authorKrishan, V-
dc.contributor.authorReiser, M-
dc.contributor.authorSessler, A. M-
dc.contributor.authorXie, M-
dc.date.accessioned2008-08-04T11:11:08Z-
dc.date.available2008-08-04T11:11:08Z-
dc.date.issued1994-
dc.identifier.citationPhysica Scripta, Vol. T52, pp. 154 - 156en
dc.identifier.issn0281-1847-
dc.identifier.urihttp://hdl.handle.net/2248/2989-
dc.descriptionRestricted Access-
dc.description.abstractSolar flare data are examined with an eye to seeing if they suggest collective acceleration of ions. That, in fact, seems to be the case. The collective acceleration mechanism of Gershtein is reviewed and the possibilities of the mechanism are discussed.en
dc.format.extent3894 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe Royal Swedish Academy of Sciencesen
dc.relation.urihttp://www.iop.org/EJ/abstract/1402-4896/1994/T52/028en
dc.subjectAcceleration mechanism of Gershtein,en
dc.subjectSolar Flare Dataen
dc.titleCollective acceleration in solar flaresen
dc.typeArticleen
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Collective acceleration in solar flares
  Restricted Access		Restricted Access271.84 kBAdobe PDFView/Open Request a copy
Show simple item record


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.