Our standard Solar Simulators produce an unfiltered xenon lamp spectrum. To approximate solar conditions for a variety of solar simulation applications we offer a complete line of Air Mass (AM) Filters. These filters modify the spectral output of the arc lamp to match specific natural solar conditions. The solar spectrum you wish to simulate determines which air mass filter you need. Use Table 1 as a guide.
Table 1 Air Mass Filters
|
Air Mass Filter Type |
Function |
Model No(s). |
| AM 0 |
Corrects the output of a xenon lamp to better match the solar spectrum found outside the earth's atmosphere. |
81011 |
| AM 1 Direct |
Simulates the solar spectrum at ground level when the sun is directly overhead |
81011* + 81085 |
| AM 1.5 Direct |
Simulates the direct solar spectrum when the sun is at a zenith angle of 48.2° (ASTM E891). |
81011* + 81086 |
| AM 2 Direct |
Approximates the solar spectrum when the sun is at a zenith angle of 60.1° |
81011* + 81087 |
| AM 1.5 Global |
Matches the total (direct and diffuse) spectrum when the sun is at a zenith angle of 48.2° (ASTM E892) |
81388 |
| AM 1.5 Global |
Matches the total (direct and diffuse) spectrum when the sun is at a zenith angle of 48.2° (ASTM E892) |
81088A |
Fig. 1 Diagram of solar air masses.
Fig. 2 Light path of an Oriel Solar Simulator, showing location of air mass filter.
Mounting
The Air Mass Direct Filters fit into the Solar Simulator's integral filter holder (shown in Fig. 2). A convenient "pull handle" allows quick and easy insertion and removal of the filter - without breaking down the source.
