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

Open Access

Fig. 10.

Same as Fig. 9, but for cases of anisotropic random MF, and $\bar{B} = 0$ ${\bar{B}}=0$ . Here the choices of f_an correspond to those in Fig. 5. Also in this case, the dashed lines (β = 1) and the solid lines (β = 2) are almost superimposed.

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