Computes the Bremsstrahlung the power density loss term.
Where \(n_{e}\) is the electron number density in \(1/m^{3}\), \(T_{eV}\) is electron temperature in electron volts (note that the temperature is input in Kelvin), \(Z_{eff}\) is the effective ion charge state.
in
(string vector, required)1st Variable
2nd Variable (1 component)
3rd Variable (1 component)
<Source radiationSource>
kind = bremsPowerSrc
</Source>