1. Nonthermal Impurity Radiation from a Spherical Plasma
2. henceforth referred to as I [equations from this paper are referred to as, for example, (I. 2. 17)].
3. When the electron distribution function is non-Maxwellian, the Planck function Bνo is no longer defined. The source function then reads simply S = ω ∫ Īνϕν dν+Γ, where Γ is a constant. All results of this paper concerningSremain valid in this more general case because the quantity S∕γBνo, and notS, has been calculated numerically. Therefore, one merely has to replace γBνo by Γ in the final results.
4. F. Engelmann (to be published).