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• W2073715744 abstract "We propose the particle acceleration model coupled with multiple plasmoid ejections in a solar flare. Unsteady reconnection produces plasmoids in a current sheet and ejects them out to the fast shocks, where particles in a plasmoid are reflected upstream the shock front by magnetic mirror effect. As the plasmoid passes through the shock front, the reflection distance becomes shorter and shorter driving Fermi acceleration, until it becomes proton Larmor radius. The fractal distribution of plasmoids may also have a role in naturally explaining the power-law spectrum in nonthermal emissions." @default.
• W2073715744 created "2016-06-24" @default.
• W2073715744 creator A5034509261 @default.
• W2073715744 creator A5081066564 @default.
• W2073715744 date "2013-01-30" @default.
• W2073715744 modified "2023-10-02" @default.
• W2073715744 title "Fermi Acceleration in Plasmoids Interacting with Fast Shocks of Reconnection via Fractal Reconnection" @default.
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• W2073715744 doi "https://doi.org/10.1103/physrevlett.110.051101" @default.
• W2073715744 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/23414011" @default.
• W2073715744 hasPublicationYear "2013" @default.
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