ecial mounting hardware allows direct coupling with 8mm or 10mm Liquid Light Guides (LLG’s). Its spectral response covers the 320 to 400nm range (Fig. 1).
The measured irradiance is displayed in mW/cm2 or W/m2. Consequently, the integrated dose is shown in Joules/cm2 or kJoules/m2. The PMA2113 has a resolution of 0.001 mW/cm2 and a full scale of 200mW/cm2 allowing measurement of very week and very strong signals with the same detector.
In conjunction with the Solar Simulator and XPS200 Xenon Lamp Power Supply the PMA2100 with the PMA2103 detector can operate as a smart dose controller/monitor substantially enhancing the functionality of the Solar Simulator.
UVA is less biologically effective than UV-B (280-320nm). However, because of its much greater intensity in sunlight and many artificial sources and the greater period of the day in which sunlight UVA remains at high intensities, UVA can have significant biological effect. The UV-A radiation can also penetrate deeply into human living tissue through the skin. Commonly known effects of UV-A include: photosensitization of various chemicals, pigmentation of the skin, induction of polymerization. The UVA can also cause erythema or DNA damage in humans or animals, however large doses of UV-A are needed and the damage mechanisms are different than these of UV-B [ref. 1].
Several biologic action spectra, functions relating wavelength of the radiation and its biologic effect, are shown in Figure 3. While they all show strong dominance of UV-B effectiveness there is still fair UVA response.
Common sources of UV-A include:
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low pressure florescent lamps
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high pressure mercury and metal halide lamps
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high pressure xenon lamps
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sunlight


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