- Conference date: 4-9 June 2006
- Location: Auburn, Alabama (USA)
The results of numerical modeling of the steady‐state classical radiative‐collisional kinetics for photorecombination are presented. The calculations are performed for edge tokamak (Ne ∼ 1011 – 1014 cm−3, Te ∼ 1–100 eV) and astrophysical plasmas (Ne ∼ 104 cm−3, Te ∼ 1 eV).
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