I will be characterizing various optic and LED combinations to determine the focusing characteristics and optimal centering gasket thickness. I will update this thread with the tests as I do them.
At present this is not a test of the ultimate performance of the optic or LED, but this information may be added later.
About the test setup:
The focal distance test is conducted on a granite surface plate, with the sensor of an Extech EA30 Lux meter affixed 1.33 meters above it.
A plumb bob is used to center the lux meter sensor above the reflector.
The optic is affixed to a 12” Mitutoyo height gage.
The LED is clamped to a fan cooled CPU heatsink. (Intel D60188-001)
The LED is powered by a benchtop power supply at a constant current.
The test starts with the bottom of the optic being flush against the top surface of the MCPCB, i.e. there is no gap between them.
The height gage is moved upward in .001” increments and the lux value is recorded at each interval.
The results are graphed.
Any points on the graph which appear errant are measured again along with the neighboring points. The variance between the initial test values and the new ones is accounted for, e.g., if the new set of measurements are reading 0.03 lux above the former set, .03 lux is subtracted from the results in order to correct the errant value from the original measurement set.
Weights are measured with a Vertias S303 precision balance. Calibrated with Troemner 7017-0 UltraClass 100g weight.
Test #1:
Convoy S2 SMO reflector (not s2+) with an OSRAM KW CSLNM1.TG (1mm2) LED, also commonly known as WF1, mounted on a Convoy 20mm star. LED was installed by Convoy.
OSRAM KW CSLNM1.TG is a domeless 3030 LED with a 1mm x 1mm emitter area.
Measured width of package: 3.00mm x 3.00mm
Height: top surface measured to be .028” [.71mm] above the top face of the MCPCB. This may vary slightly depending on solder thickness.
S2 Reflector measurements:
Diameter: 0.813” [20.65mm]
Height: 0.755” [19.18mm]
Clear aperture: 0.725” [18.42mm] (approximately)
Vertex opening diameter: 0.197” [5.0mm]
Focal length of the parabola: .04” [1mm] (estimated)
Weight: 6.663 grams
LED was powered at 700mA constant current.
Lux meter sensor was affixed 1.33 meters above the reflector.
Tested September 4th, 2022.
( Here is a graph with more range in the positive direction resulting in a larger image size. )
Notes and observations:
The highest recorded lux value did not occur at a single point, but over a range of three points: 0.025”, 0.026”, and 0.027” [0.635mm, 0.66mm, 0.686mm].
The optimal gap between the bottom-most part of the reflector and the top surface of the MCPCB was .026” [.66mm].
+/-.002” [.05mm] from optimal focus results in a lux reduction of ~0.5%.
+/-.004” [.10mm] from optimal focus results in a lux reduction of ~1.5%.
+/-.006” [.15mm] from optimal focus results in a lux reduction of ~3.3%.
+/-.008” [.20mm] from optimal focus results in a lux reduction of ~6%.
+/-.010” [.25mm] from optimal focus results in a lux reduction of ~9%.
The spill angle is approximately 55 degrees.
Beam characteristics:
This reflector + LED combo is rather forgiving. The beam looks acceptable at all points, without major artifacts, even when the reflector is sitting flush against the MCPCB or when positioned too high above it.
White wall observations @ ~1 meter:
- Height/gap of 0.000” [0.00mm] - The beam has three distinct parts: spill, a wide angle corona, and a hotspot. The hotspot has some minor artifacts and looks bit like a nebula, with slight color and brightness variation. There are no apparent rings or major issues.
- Height/gap of 0.010” [0.25mm] - The angle of the corona decreases as the reflector becomes more focused. The hotspot now has no artifacts and appears nearly round. All parts of the beam have distinct boundaries with sharp transitions: spill, corona, hot spot.
- Height/gap of 0.026” [0.66mm] - Median focus point. The transition between corona and the spill is smooth. The hotspot is still apparent but is not a distinct round spot with a sharp edge, the transition into the corona is softer.
- Height/gap of 0.048” [1.22mm] - As the reflector height increases past the median focus point, the hotspot shrinks in size. At this height it converges and disappears. The center of the beam has a small yellowish tinted four point star shape in it.
- Height/gap of 0.055” [1.27mm] - A dark spot begins to appear in center of beam. The dark spot enlarges in size as reflector height increases.
Centering ring design:
With the S2 reflector + WF1 combination, the top surface of the LED is basically flush with the bottom of the reflector. The top of the LED sits ~.012” [.3mm] below the vertex opening. This means any centering “tabs” or bosses that extend up into the reflector in order to center it will be extending above the LED and may block some light.
The test gaskets were machined out of G10, which I think may be a good gasket material in some situations. It is rigid, strong, non-compressible, and won’t melt. In most cases Nylon 66 is good enough though.
Model 1: This gasket resulted in a lux value of 99.02% of the optimal lux value. With the gasket in place, some light is being blocked.
Model 2: This gasket resulted in a lux value of 99.16% of the optimal lux value. A slight improvement.
Model 3: This gasket resulted in a lux value of 99.29% of the optimal lux value. Another slight improvement.
Model 4: This gasket resulted in a lux value of 100% of the optimal lux value. There is no loss on account of the centering ring. The tabs were eliminated entirely. The tapered geometry of the bottom part of the reflector is used to center the reflector. The LED pocket was made circular instead of square to improve manufacturability.
Test #2:
Convoy S21A SMO reflector with an OSRAM KW CSLNM1.TG (1mm2) LED, also commonly known as WF1, mounted on a Convoy 20mm star. LED was installed by Convoy.
S21A Reflector measurements:
Diameter: 0.910” [23.11mm]
Height: 0.452” [11.48mm]
Clear aperture: 0.787” [20.00mm] (approximately)
Vertex opening diameter: 0.276” [7.0mm]
Focal length of the parabola: .075” [1.9mm] (estimated)
Weight: 4.534 grams
LED was powered at 700mA constant current.
Lux meter sensor was affixed 1.33 meters above the reflector.
Tested September 18th, 2022.
Notes and observations:
The highest recorded lux value occurred at a single point, .017” [0.432mm].
This reflector seems to require more precision to focus than the S2 reflector. The resulting lux value (with the same test parameters) was less, even though it has a slightly larger clear aperture. The longer focal length of the S21A reflector makes for a shallower parabola, collecting less light than the S2 reflector.
The graph is less symmetrical than the one from the previous test. A test with the meter at a greater distance might make for more a symmetrical result.
+/-.002” [.05mm] from optimal focus results in a lux reduction of ~1.0%.
-.004” [.10mm] from optimal focus results in a lux reduction of ~4.3%.
+.004” [.10mm] from optimal focus results in a lux reduction of ~3.0%.
-.006” [.15mm] from optimal focus results in a lux reduction of ~11%.
+.006” [.15mm] from optimal focus results in a lux reduction of ~7%.
-.008” [.20mm] from optimal focus results in a lux reduction of ~20%.
+.008” [.20mm] from optimal focus results in a lux reduction of ~12%.
The spill angle is approximately 85 degrees.
Centering ring design:
I have not made it yet, but the following design should work well: