Fig. 6

Coronal kinetic energy spectrum (dashed line) and magnetic energy spectrum (solid
line) for runs
Dcl, D1L, and D.
Wavenumbers are in units of 1/Mm and in the top x-axis the
corresponding shell numbers are indicated. The spectra are averaged in time and
space and the normalization is in arbitrary units (spectra are also rescaled). The
symbols on the Eb spectra indicate the
first shell number for which .
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