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dc.contributor.authorQin, Gang
dc.contributor.authorHe, H. Q.
dc.contributor.authorZhang, Ming
dc.date.accessioned2014-10-14T15:46:52Z
dc.date.available2014-10-14T15:46:52Z
dc.date.issued2011-08-10
dc.identifier.citationQin, G., He, H. -., & Zhang, M. (2011). An effect of perpendicular diffusion on the anisotropy of solar energetic particles from unconnected sources. Astrophysical Journal, 738(1)en_US
dc.identifier.urihttp://hdl.handle.net/11141/350
dc.description.abstractRecently, Tan and coworkers studied the 2001 September 24 solar energetic particle (SEP) event observed by the Wind spacecraft at 1AU and found that there is a counter-streaming particle beam with a deep depression of flux at 90° pitch angle during the beginning of the event. They suggested that it is a result of a reflecting boundary at some distance outside of 1AU. While this scenario could be true under some specific configuration of an interplanetary magnetic field, in this paper we offer another possible explanation. We simulated the SEP event by solving the five-dimensional focused transport equation numerically for 40keV electrons with perpendicular diffusion. We find that a counter-streaming particle beam with deep depression at 90° pitch angle can form on Parker magnetic field lines that do not directly connect to the main particle source on the Sun in the beginning of an SEP event. It can happen when a significant number of observed particles come from adjacent field lines through parallel transport to large radial distance first, hopping across field lines through perpendicular diffusion, and then getting scattered back to 1AU, where they combine with the particles directly coming from the Sun to form a counter-streaming beam.en_US
dc.language.isoen_USen_US
dc.rightsThis published article is available in accordance with the publisher's policy. It may be subject to U.S. Copyright Law.en_US
dc.rights.urihttp://aas.org/publications/aas-copyright-policyen_US
dc.titleAn effect of perpendicular diffusion on the anisotropy of solar energetic particles from unconnected sourcesen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/0004-637X/738/1/28


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