  A new modeling way of describing the continuous absorption of electromagnetic
(EM) radiation in dense partially ionized hydrogen plasma is tested in this
work. It is shown that the obtained results give a possibility of calculating
spectral absorption coefficients which characterize the relevant absorption
processes in partially ionized hydrogen plasmas with electron densities $N_{e}
\sim 10^{19}cm^{-3}$ and temperatures $T \approx 2\cdot 10^{4}K$. A key
parameter of the used procedure is determined empirically. The calculation
method is applied to wavelength region $300nm < \lambda < 500nm$. The presented
results can be of interest for dense laboratory plasmas as well as for
partially ionized layers of different stellar atmospheres.
