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 300 nm < \lambda < 500 nm .
The presented results can be of interest for dense laboratory plasmas as well as for partially ionized layers of different stellar atmospheres .