In contrast to most other UV sources, the MPL has a polychromatic spectral distribution ranging from 190 nm up to the IR. A typical spectral distribution for non-doped lamps is shown in Fig. 1. The far infra-red radiation is principally determined by the bulb temperature which ranges from 600 °C to max. 900 °C. All other wavelength ranges directly depend on the plasma properties such as temperature, pressure, and atomic and molecular content.
The UV radiant properties of standard mercury lamps are directly linked to the radiating characteristics of atomic mercury.
The typical UV efficacy is shown in the table.