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Energetic Ion Beams Near the Heliospheric Current Sheet: Possible Evidence for Reconnection

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dc.contributor.author Murphy, N. en_US
dc.contributor.author Smith, E. J. en_US
dc.contributor.author Burton, M. E. en_US
dc.contributor.author Winterhalter, D. en_US
dc.contributor.author McComas, D. J. en_US
dc.date.accessioned 2004-10-06T05:23:05Z
dc.date.available 2004-10-06T05:23:05Z
dc.date.issued 1993
dc.identifier.clearanceno 93-1689 en_US
dc.identifier.uri http://hdl.handle.net/2014/35959
dc.description.abstract Energetic ion data, close to solar wind sector boundaries (the heliospheric current sheet), are examined for the presence of accelerated ions, which may be the signature of magnetic reconnection. en_US
dc.format.extent 326452 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other magnetic field plasma data accelerated ionssolar flares en_US
dc.title Energetic Ion Beams Near the Heliospheric Current Sheet: Possible Evidence for Reconnection en_US


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