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185 lines
7.1 KiB
Markdown
185 lines
7.1 KiB
Markdown
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[](https://github.com/marketplace/actions/arduino_ci)
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[](https://github.com/RobTillaart/BH1750FVI_RT/actions/workflows/arduino-lint.yml)
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[](https://github.com/RobTillaart/BH1750FVI_RT/actions/workflows/jsoncheck.yml)
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[](https://github.com/RobTillaart/BH1750FVI_RT/blob/master/LICENSE)
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[](https://github.com/RobTillaart/BH1750FVI_RT/releases)
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# BH1750FVI_RT
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Arduino library for BH1750FVI (GY-30) 16 bit I2C Lux sensor.
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## Description
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The BH1750FVI is a 16 bit lux sensor with an I2C interface.
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It is possible to detect a wide range from 0.11 - 100000 lux.
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To be able to support this wide range, the sensor can operate in three modi.
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| ID | Mode | Integration time | Resolution | Notes |
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|:----:|:-----:|:----------------:|:----------:|:--------------------------|
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| 0 | LOW | 16 ms | 4.0 Lux | measure very bright light |
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| 1 | HIGH | 120 ms | 1.0 lux | default |
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| 2 | HIGH2 | 120 ms | 0.5 lux | measure very dim light |
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Furthermore one can set a correction factor to reduce / increase the
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integration time of the sensor.
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The factor should be between 0.45 - 3.68.
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It can be used to increase the working range like very bright or very low light conditions.
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Another application is to correct the transparency of material, or the type of light used.
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Note that the typical integration time will differ if the correction factor is changed.
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The **isReady()** an **getLux()** functions keep track of the adjustment needed.
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## Interface hardware
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Library was tested with a breakout board.
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```
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// breakout BH1750FVI / GY-30
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//
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// +-----------------------+
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// GND |o |
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// ADD |o |
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// SDA |o + | + = sensor
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// SCL |o |
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// VCC |o |
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// +-----------------------+
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//
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// ADD = ADDRESS:
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// 0 = 0x23
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// 1 = 0x5C
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//
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```
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The sensor works on 2.4 - 3.6 volt so be careful not to connect directly to 5.0 volt.
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Note: the breakout board was 5 volt tolerant.
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## Interface
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### Constructor
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- **BH1750FVI(uint8_t address, uint8_t dataPin, uint8_t clockPin)** ESP constructor with I2C parameters.
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- **BH1750FVI(uint8_t address, TwoWire \*wire = &Wire)** constructor for other platforms.
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- **bool begin()** resets some internal variables to default. Use with care.
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- **bool isConnected()** returns true if address is on I2C bus.
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### Base
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- **float getRaw()** reads the lux sensor.
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- **float getLux()** reads the lux sensor and corrects for correctionFactor, mode, temperature and angle.
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### management
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- **int getError()** get the latest error code, mainly for debugging.
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- **void powerOn()** wakes up the sensor.
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- **void powerOff()** set sensor to sleep.
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- **void reset()** resets the data register to 0, effectively removing last measurement.
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### Mode operators
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- **uint8_t getMode()** gets the mode set by one of the set functions. See table above.
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- **void setContHighRes()** continuous mode in HIGH resolution.
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- **void setContHigh2Res()** continuous mode in HIGH2 resolution.
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- **void setContLowRes()** continuous mode in LOW resolution.
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- **void setOnceHighRes()** single shot mode in HIGH resolution.
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- **void setOnceHigh2Res()** single shot mode in HIGH2 resolution.
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- **void setOnceLowRes()** single shot mode in LOW resolution.
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### CorrectionFactor
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Please read datasheet P11 about details of the correction factor.
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- **bool isReady()** can be used to check if the sensor is ready.
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This is based on a calculated time, the sensor does not have a means to indicate ready directly.
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Needed only for the single shot modi.
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The function **isReady()** takes the correction factor into account.
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- **void changeTiming(uint8_t time = BH1750FVI_REFERENCE_TIME)** 69 is default.
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- **uint8_t setCorrectionFactor(float factor = 1)** preferred wrapper around changeTiming factor = 0.45 .. 3.68.
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Returns changeTiming() parameter.
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- **float getCorrectionFactor()** returns the correction factor.
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Note this can differ as it is stores as an integer internally.
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### Angle sensitivity
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Note: experimental - use carefully
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The lux sensor is really sensitive for the angle of the light.
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If one makes measurements outside, the position of the sun changes
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during the day. The **setAngle(int degrees)** function provides a mean to correct that.
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The angle adjustments is based upon the figure 4 and 5 (directional characteristics.)
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which describe **Lambert’s Cosine Law**. (details see Wikipedia)
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So the correction factor is ```factor = 1.0 / cos(angle)```.
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At 90 degrees it would fail (divide by zero) so the input is constrained
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to angles between -89 - +89 degrees.
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If the light is perpendicular on the sensor the angle to use is 0 degrees.
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Light coming from the side is 90 degrees.
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- **float setAngle(int degrees = 0)** adjust the lux to incoming angle in degrees (-89..89). Returns the angle correction factor.
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- **int getAngle()** returns set angle in degrees, 0 by default is perpendicular.
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### Temperature Compensation
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The reference temperature of the sensor = 20°C.
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The effect of temperature is small, about 3% per 60°C ==> 1% per 20°C
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so only on either a hot roof or on a icy cold day the effect is substantial.
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- **float setTemperature(int temp = 20)** see datasheet P3 fig7 Returns the temperature correction factor
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- **int getTemperature()** returns temperature set, default = 20°C.
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### Spectral Compensation ! EXPERIMENTAL !
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Spectral compensation is experimental and not tested. It is a compensation based upon the
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graph figure 1, page 3 of the datasheet. If one has light of a known wavelength one can
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compensate for it by setting the wavelength. It can also be used when using filters.
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As said it is not tested so use at your own risk, but I am interested in your experiences
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if you do real tests with it.
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- **float setWaveLength(int wavelength = 580)** set wavelength, returns the wavelength correction factor.
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- **int getWaveLength()** returns set wavelength
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As the graph (figure 1) is not linear it is approximated by linear interpolation with the
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following six points.
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| WaveLength | Perc % |
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|:-----------|:------:|
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| 400 | 1 |
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| 440 | 10 |
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| 510 | 90 |
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| 545 | 80 |
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| 580 | 100 |
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| 700 | 07 |
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| 715 | 1 |
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Values outside the range will be mapped upon 400 or 715.
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Default wavelength will be 580 as that gives 100%
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## Operation
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See samples...
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## Future
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- **Intelligent isReady()**
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After a **getLux()** call one can clean the data register explicitly with
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**reset()**. Then a call to **isReady()** fetches data and as long as
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data equals zero the sensor is not ready.
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- **DVI interface**
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To investigate, sort of external reset?
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