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New Field-Line-Advection Model for Solar Particle Acceleration (FLAMPA) (Ilia Roussev)

Written by

KTINDIANA

in

SHINE 2004
roussev_SHINE2004Download
←Fitting Flux Ropes to a Global MHD solution: A comparison of techniques (Pete Riley)
Tests of NLFFF Models of AR 10486 (J. McTiernen)→

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  • A statistical study of shear motion of the footpoints in two-ribbon flares (Yingna Su)

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