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Fig. 4


Dimensionless emissivity J = 1 − R as a function of photon energy E for a condensed Fe surface with inclined magnetic field (B = 1013 G, θB = π/4) and inclined incidence of radiation (θk = π/4 and four values of ϕ listed in the figure). Solid lines show our numerical results for the model of free ions at T = 106 K, and short-dashed lines demonstrate the fit. For comparison, the dotted line reproduces our numerical results for ϕ = π/2 and T = 3 × 105 K.

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