Fig. 6: Modulation of the shock compressibility in a non-uniform magnetic field. | Nature Communications

Fig. 6: Modulation of the shock compressibility in a non-uniform magnetic field.

From: The supernova remnant SN 1006 as a Galactic particle accelerator

Fig. 6

Same as Fig. 3, with the solid curve marking the profile expected for ξp = 12%, ξB = 5% and ξs = 6%, but including a gradient of the magnetic field strength, lying in the plane of the sky at θ = 90∘. Source data are provided as a Source Data file.

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