Fig. 4
Wavelet planes wF(a,φ) for the magnetic field with a Gaussian profile and in energy equipartition with cosmic rays (model 1). The calculations are done for the frequency bands available for several telescopes. Left column, panels from above: LOFAR, EVLA (or ATCA), and ASKAP (POSSUM + FLASH); right column, panels from above: WSRT (or GMRT), ASKAP (POSSUM), and SKA phase 1.
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