Improved parallel boundary conditions, a faster Fourier transform, and HDF5 output make the Pencil Code's solar coronal MHD model scale to over 1000 processors about ten times more efficiently.
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Driving solar coronal MHD simulations on high-performance computers
Improved parallel boundary conditions, a faster Fourier transform, and HDF5 output make the Pencil Code's solar coronal MHD model scale to over 1000 processors about ten times more efficiently.