Synchrotron polarization with a partially random magnetic field: General approach and application to X-ray polarization from supernova remnants

Open Access

Fig. 15.

Comparison of the radio and X-ray polarization data on SN 1006 Zhou et al. (2023, data as from). The upper panel shows them superimposed to models of a homogeneous MF composed with an isotropic random component (the labels indicate ${log}_{10} σ / \bar{B}$ $\log_{10}{\sigma}/{\bar{B}}$ ). The lower panel compares them instead with models of an anisotropic random MF (the labels now indicate f_an).

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