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Estimation of Magnetic Fields from Synchrotron Emission: Numerical Tests

  • Authors: Nora B. Linzer, Lucia Armillotta, Eve C. Ostriker, Eliot Quataert

Nora B. Linzer et al 2026 The Astrophysical Journal 996 .

  • Provider: AAS Journals

Caption: Figure 3.

The blue distribution represents a two-dimensional histogram of the traditional equipartition magnetic field strength, Beq (Equation (15)), compared to the measured (mass-weighted) average magnetic field strength, Bavg. The distribution includes each pixel in projected maps across all R8 model snapshots. The best-fit power law to this distribution is included as a purple line with ﹩{B}_{{\rm{eq}}}\propto {B}_{{\rm{avg}}}^{0.36}﹩. The black, dashed line represents Beq = Bavg. The red points represent the values of Beq and Bavg averaged over each kiloparsec-scale simulation snapshot individually. While the large-scale snapshot-averaged value of Beq estimates the large-scale average of Bavg well, the pixel-by-pixel comparison shows that Beq fails to recover the true Bavg at smaller scales.

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