Ceiling mounted Large Area IR solar simulator
This solar simulator provides illumination in the Infrared wavelengths with high spatial uniformity and depth of field
This solar simulator was specially requested to be hung from the ceiling in order to accommodate the testing setup at the end user’s laboratory. Moreover, the end users required high spatial uniformity to be achieved in a target three dimensional volume.
Therefore the system was designed so that the simulated sun light directed downwards towards a vertical target plane from top of a 2m distance at a 30 degree angle.
This light source was especially designed with optical corrections to overcome the lack of symmetry.
|Target Area||Illuminates a 1.5m x 1.5m|
|Work Distance||Solar simulators to be 2.1 m above the floor and 0.8 m above the center of the target plane|
|Spectrum||Class A, (ASTM E927) Wavelength range : 700nm to 1100nm|
|Intensity||Equivalent to 0.6 suns irradiance in the range of 700nm to 1100nm wavelength spectrum.|
|Uniformity||1m x 1m: ±5% (ASTM E927)) | 1.5m x 1.5m: ±30% (ASTM E927))|
|Depth of Field||±15cm, with change ≤ ±5% Intensity (ASTM E927))|
|Attenuation||10 steps, 0.1 suns to 0.6 suns|
|Temporal Instability||Class A (ASTM E927))|
|System Warm Up||≤ 15 seconds|
Various new designs were proposed to improve the spatial uniformity of the output light. This also required the optical axis of the light source to be at an angle and laterally above the target plane which further complicated the task.
New designs were brainstormed and evaluated for their performance. Each idea was prototyped and various parameters were changed to assess the effects on the spatial uniformity. The idea that showed the most promise was changing the lateral and angular position of the output lens of the system. This idea was then modeled using optical modeling software to better understand the effect on the spatial uniformity. Once the idea was better understood, it was further optimized using the optical modeling software to meet the specialized needs of the system.
The idea then moved to the mechanical design phase. A way to easily reproducibly adjust the output lenses was required. Various methods were investigated and a custom lens holder with specific lateral and angular adjustment capabilities was developed so that the fine adjustments required of the output lens could be achieved to produce a spatially uniform target plane that was not perpendicular to the optical axis of the solar simulator.
Optical ray tracing model for the projectors
This new system incorporated five projector systems with the ability to upgrade to 6 units based on power requirements of the end user. Each projector system contained 2 kW QTH lamps with specialized filters to create the necessary spectral output.
Target area consisted of 1m x 1m with +/-5% non-uniformity. Depth of field was +/-15cm with no change larger then +/- 5% in the non-uniformity specifications.
As before, the end users required only the IR portions of the solar spectrum with a class A spectral match which was achieved in the final outcome. The IR wavelength portion of the solar spectrum was provided from 700-1100nm. The end users required the output power to correspond with 0.6 suns. Therefore the irradiance was adjustable from 0-0.6 suns in a minimum of 10 steps.
Temporal stability was categorized as ASTM Class A with a design improvement to reduce noise levels produced by the past system. A feedback system was also included in the system with a Sciencetech calibrated solar cell to control and monitor intensity variations within the light sources.
Sciencetech successfully completed all the requirements of the solar simulator. The final acceptance testing was conducted and approved at the end users’ facilities and the system was successfully installed by our team of support engineers. The end users were extremely impressed with the design and workings of the system.
We recently received a third order from the same clients for a similar solar simulator system.
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