  We analyze the ratios of the broad hydrogen Balmer emission lines (from
H\alpha to H\epsilon) in the context of estimating the physical conditions in
the broad line region (BLR) of active galactic nuclei (AGN). The Balmer
emission lines are obtained in three ways: i) using photoionization models
obtained by a spectral synthesis code CLOUDY; ii) calculated using the
recombination theory for hydrogenic ions; iii) measured from the sample of
observed spectra taken from the Sloan Digital Sky Survey database. We
investigate the Balmer line ratios in the frame of the so called Boltzmann-plot
(BP), analyzing physical conditions of the emitting plasma for which we could
use the BP method. The BP considers the ratio of Balmer lines normalized to the
atomic data of the corresponding line transition, and is in that way different
from the Balmer decrement. We found that for a certain range of thermodynamic
parameters, there are objects that follow the BP. These AGN may have a BLR
consisting of mostly high density plasma.
