Fig. 4
Comparison of this work (solid lines) to Isenberg et al. (1998, their Fig. 7; dashed lines). Red lines denote the slab 1-1 geometry while green lines show the slab 1-0 geometry. The emission in different angular bins is labeled by the cosine of the viewing angle to the magnetic field axis, μ = cosϑ. Temperatures of 7 keV and 8 keV were used for the slab 1-0 and slab 1-1 geometries, respectively.
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