BLACK_BODY

Function

To calculate the spectra (spectral power and brightness) of a black body emitter as a function of the photon energy. It can be used as a first approximation for an x-ray plasma source. The output spectra can be saved to files (using File->write files for Xop/Optics) for being used by xpower.

Documentation:

Technical aspects

 

Reference:

David Attwood Soft X-rays and extreme ultraviolet radiation. Principles and applications Cambridge University Press, 2000, Pags. 242-246