Influence of pulsed laser energy on emission characteristics of laser plasmas induced in various inert atmospheres and pressures is demonstrated by emission spectroscopy in the far vacuum UV zone (around 100 nm). In this context, argon and helium were employed and their pressures were controlled in the range 0.005–5.0 mbar. A Q-switched Nd:YAG laser emitting in the near IR at 1064 nm was employed in the experiments. The laser energy was varied between 200 and 800 mJ and focused onto a reference steel sample within a vacuum-tight chamber. The radiation emitted from the line plasmas generated was recorded from a section located 2.5 mm from the target surface. Under any gas composition and pressure studied, line and background emission intensities as well as signal-to-background ratios showed significant dependence on the laser energy. For example, at 800 mJ the highest spectral line intensity was obtained in argon atmosphere at a pressure of about 0.5 mbar, while helium at the same pressure produced the largest signal-to-background ratio using lower laser pulse energy of 400 mJ. In any case, the nature and characteristics of laser plasma-based emission in the far vacuum UV are similar to those recorded in the UV-visible range.