0.1.3 TSL235R

This commit is contained in:
rob tillaart 2022-11-26 17:40:57 +01:00
parent 753172446a
commit 11f2399cb9
7 changed files with 106 additions and 49 deletions

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@ -1,3 +1,18 @@
platforms:
rpipico:
board: rp2040:rp2040:rpipico
package: rp2040:rp2040
gcc:
features:
defines:
- ARDUINO_ARCH_RP2040
warnings:
flags:
packages:
rp2040:rp2040:
url: https://github.com/earlephilhower/arduino-pico/releases/download/global/package_rp2040_index.json
compile:
# Choosing to run compilation tests on 2 different Arduino platforms
platforms:
@ -7,5 +22,6 @@ compile:
# - leonardo
- m4
- esp32
# - esp8266
- esp8266
# - mega2560
- rpipico

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@ -0,0 +1,25 @@
# Change Log TSL235R
All notable changes to this project will be documented in this file.
The format is based on [Keep a Changelog](http://keepachangelog.com/)
and this project adheres to [Semantic Versioning](http://semver.org/).
## [0.1.3] - 2022-11-26
- Add RP2040 support to build-CI.
- Add CHANGELOG.md
- update readme.md
- renamed **calcWLF()** to **calculateWaveLengthFactor()** more descriptive.
## [0.1.2] - 2021-12-29
- update library.json
- update readme.md
- update license
- minor edits
## [0.1.1] - 2020-06-03
- add irradiance_HS()
## [0.1.0] - 2020-05-29
- initial version

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@ -13,22 +13,28 @@ Arduino library for the TSL235R light to frequency convertor.
## Description
This library does not measure the frequency but has some functions to compensate e.g.
for wavelength and voltage used.
This library does not measure the frequency.
That should be done with an interrupt function (user code).
The library provides functions to calculate the radiation and
has functions to compensate e.g. for wavelength and voltage used.
The library is not tested extensively yet.
The sensor operating voltage is between 2.7 and 5.5 max.
This can be set in the constructor, or runtime adjusted.
For measurements below 1uW/cm2 one bests measures for multiple seconds
For measurements below 1 uW/cm2 one should measure for multiple seconds.
Above 1 uW/cm2 1 second or shorter is OK.
Note that for longer and shorter measurements than 1 second one must convert the
value to Hz, which is the number of pulses in 1 second.
Note that for longer and shorter measurements than 1 second one must
convert the value to Hz, which is the number of pulses in 1 second.
The library provides functions **irradiance()** to do that for you.
## Connection
Always check the datasheet.
```
// PIN 1 - GND
// PIN 2 - VDD 2.7 V .. 5.5 V
@ -39,24 +45,29 @@ value to Hz, which is the number of pulses in 1 second.
## Interface
- **TSL235R(float voltage = 5.0)** constructor, optionally one can give the operational voltage
to add a small correction (< 1.5%)
to add a small correction (< 1.5%).
Default voltage is 5.0 Volts.
- **float irradiance(uint32_t Hz)** returns the irradiance in uW/cm2.
Note that Hz implies the measured pulses for 1 second.
- **float irradiance(uint32_t pulses, uint32_t milliseconds)** returns the irradiance in uW/cm2
- **float irradiance(uint32_t pulses, uint32_t milliseconds)** returns the irradiance in uW/cm2.
This formula is used for other duration than 1 second.
To get irradiance in W/m2 one must divide by 100.
- **float irradiance_HS(uint32_t pulses, uint32_t microseconds)** returns the irradiance in uW/cm2
This formula is used when the time is measured in microseconds. This is the most accurate measurement.
- **float irradiance_HS(uint32_t pulses, uint32_t microseconds)** returns the irradiance in uW/cm2.
This formula is used when the time is measured in microseconds.
This is the most accurate measurement.
- **float getFactor()** returns the inner conversion factor from Hz to Watt/cm2.
- **void setWavelength(uint16_t wavelength = 635)** sets the wavelength so the formulas can use a
correction factor. At the default wavelength of 635 nm the wavelength correction factor == 1.0
- **uint16_t getWavelength()** returns the set wavelength. Convenience function.
correction factor.
At the default wavelength of 635 nm the wavelength correction factor == 1.0.
- **uint16_t getWavelength()** returns the set wavelength.
- **float getWaveLengthFactor()** returns the wavelength correction factor.
As the sensor is most sensitive around 750 nm this value helps to normalize the signal.
This works only for (almost) monochromatic light.
- **void setVoltage(float voltage)** sets the voltage so the formulas can use a correction factor.
This voltage correction factor is rather small < 1.5%
- **float getVoltage()** returns the set voltage. Convenience function.
This voltage correction factor is rather small < 1.5%.
Note: this voltage can be changed runtime.
- **float getVoltage()** returns the set voltage, by constructor or by **setVoltage()**.
Default voltage is 5.0 Volts.
## Operations
@ -66,9 +77,19 @@ See examples for typical usage.
## Future
#### must
- improve documentation
- test test test
- investigate hardware solutions for e.g. divide by 100 or so
#### should
- default voltage should be a #define so people who use 3.3V processor
can change the library with minimal effort.
- irradiance(pulses, millis) can be given a default of 1000 millis.
makes irradiance(Hz) obsolete.
- move code from .h to .cpp
#### could
- investigate hardware solutions for e.g. divide by 100 or 1000 or so.
- investigate correction factor for white light and mixed light sources.
- investigate calibration factor for timing of processor used.
-

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@ -1,13 +1,8 @@
//
// FILE: TSL235R.cpp
// AUTHOR: Rob Tillaart
// VERSION: 0.1.2
// VERSION: 0.1.3
// PURPOSE: library for the TSL235R light to frequency convertor
//
// HISTORY:
// 0.1.0 2020-05-29 initial version
// 0.1.1 2020-06-03 add irradiance_HS()
// 0.1.2 2021-12-29 update build-CI, readme, library.json, license, minor edits
#include "TSL235R.h"
@ -59,14 +54,14 @@ void TSL235R::calculateFactor()
// as the graph is in kHz we need to correct a factor 1000
// as the irradiance function gets Hz
const float cf = 0.00142;
_waveLengthFactor = calcWLF(_waveLength);
_waveLengthFactor = calculateWaveLengthFactor(_waveLength);
_voltageFactor = 0.988 + (_voltage - 2.7) * (0.015 / 2.8);
_factor = cf * _waveLengthFactor * _voltageFactor;
}
float TSL235R::calcWLF(uint16_t _waveLength)
float TSL235R::calculateWaveLengthFactor(uint16_t _waveLength)
{
// figure 2 datasheet
// 635 nm is reference 1.000

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@ -2,11 +2,11 @@
//
// FILE: TSL235R.h
// AUTHOR: Rob Tillaart
// VERSION: 0.1.2
// VERSION: 0.1.3
// PURPOSE: library for the TSL235R light to frequency convertor
#define TSL235R_LIB_VERSION (F("0.1.2"))
#define TSL235R_LIB_VERSION (F("0.1.3"))
#include "Arduino.h"
@ -17,7 +17,7 @@ public:
TSL235R(float voltage = 5.0);
float irradiance(uint32_t Hz);
float irradiance(uint32_t Hz); // Hz == pulses in one second.
float irradiance(uint32_t pulses, uint32_t milliseconds); // obsolete?
float irradiance_HS(uint32_t pulses, uint32_t microseconds);
float getFactor() { return _factor; };
@ -39,7 +39,7 @@ private:
float _factor = 1.2;
void calculateFactor();
float calcWLF(uint16_t _waveLength);
float calculateWaveLengthFactor(uint16_t _waveLength);
float multiMap(float value, float * _in, float * _out, uint8_t size);
};

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@ -15,7 +15,7 @@
"type": "git",
"url": "https://github.com/RobTillaart/TSL235R.git"
},
"version": "0.1.2",
"version": "0.1.3",
"license": "MIT",
"frameworks": "*",
"platforms": "*",

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@ -1,5 +1,5 @@
name=TSL235R
version=0.1.2
version=0.1.3
author=Rob Tillaart <rob.tillaart@gmail.com>
maintainer=Rob Tillaart <rob.tillaart@gmail.com>
sentence=Library for the TSL235R light to frequency convertor.