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Fig. 3


Dimensionless emissivity J = 1 − R as a function of photon energy E for condensed Fe surface at B = 1013 G (top panel), B = 1012 G and 1014 G (bottom panel), with magnetic field lines normal to the surface, for two angles of incidence θk = 0 and θk = π/4, as marked near the curves. Solid lines show our numerical results, and dashed lines demonstrate the fit. For comparison, dotted lines reproduce the simplified approximation used in Paper II.

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