MHD shocks flatten the EE/BB ratio of polarized ISM emission to values ≳1 as energy injection increases, accompanied by a -7/2 power-law tail in velocity divergence.
Dust-polarization maps for local interstellar turbulence
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The Shocking Origin of the Flat $EE/BB$ Ratio
MHD shocks flatten the EE/BB ratio of polarized ISM emission to values ≳1 as energy injection increases, accompanied by a -7/2 power-law tail in velocity divergence.