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Modeling a coronal loop heated by MHD-turbulence nanoflares F. Reale1 , G. Nigro2 , F. Malara2 , G. Peres1 , P. Veltri2 ABSTRACT We model the hydrodynamic evolution of the plasma confined in a coronal loop, 30000 km long
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Document Date: 2005-06-28 08:07:25
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File Size: 1,16 MB
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