Re: Difference in two similar LDR Characteristic in two axis sun tracking system
Does the LDR, have a wide tolerance? Max/Min= 2 or typ +/->50%
This can lead to tracking errors as does dust coverage.
Ideas.
SFH series Silicon photo diodes are much more precise, low cost, but smaller and thus higher impedance. ( but more consistent A/W)
I don't know the tolerance but suggest few % is possible, but not spec'd.
Viewing angle is not always adequate so parallel diodes can be used, spaced X deg apart.
For X azimuth angle detection and ignore Y angle, you can consider blocking stray light in Y axis to permit season variation only. You have options for optical diodes or IR only with daylight blocking filter. Consider any source of light interference and aging factors from dust and wind direction how it affects tracking.
Consider how solar input and shadow object affect differential gain as energy levels are not always constant. Decide on minimum hysteresis threshold as a function of photon power.
You might toss the shadow effect and consider parallel array of three PD 30deg sources pointing East with angle spacing to match 50% theta and same pointing West, then you have two 90 Deg arrays to measure differential on bridge for East West. Stray light from sides needs to be plotted to linearize the azimuth angle detection. Lens shape is a major consideration.
In the LDR shadow approach, the contrast of the shadow and size of the LDR affects the response.
In the PD approach the angle of the lens with array and orientation determines the response. Modeling is required to make it linear.
Another method is a linear solar PD array with a slit to measure solar azimuth but requires decoding the maximum. sensor and correlation between mounting angle, size and height of slot and solar position.
The another precise method uses a solar clock geometry to create the shadow on the semi- circular PD array to locate the shadow.
The main thing is to avoid hunting and wasting power in order to gain a small advantage in efficiency.