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.
and Gudiksen, B., On the nature of coronal loops above the quiet sun network
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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.