# CS123x Gaussian Noise Test Example This example provides a high-resolution statistical analysis and noise characterization tool for the CS123x library. It uses Welford's algorithm for numerically stable mean and variance computation, reporting RMS noise, peak-to-peak noise, LSB-equivalent voltage noise, effective number of bits (ENOB), and noise-free resolution. --- ## 🚀 Features Demonstrated 1. **ADC Initialization & Hardware Sync:** Initializes GPIO lines, writes the default or user-provided configuration to the ADC and verifies correct register read-back from it. 2. **Interactive Terminal CLI:** Real-time command-line interface over serial to trigger tests, cycle gains, sampling rates, input channels and set sample counts. 3. **Statistical Analysis via Welford's Algorithm:** Calculates mean (offset), variance, standard deviation (RMS noise in LSB and uV) and peak-to-peak noise without floating-point overflow. 4. **ENOB & Noise-Free Resolution Calculation:** Computes Effective Number of Bits (`ENOB = 24 - log2(RMS_noise)`) and Noise-Free Resolution (`24 - log2(PP_noise)`) in real-time. 5. **Dynamic Parameter Cycling:** Allows live changing of PGA gains (`1x`, `2x`, `64x`, `128x`), output data rates (`10Hz`, `40Hz`, `640Hz`, `1280Hz`), and channels (`CH_A`, `CH_B` (CS1238 only), `CH_TEMP`, `CH_SHORT`) on the fly. --- ## 🛠️ Hardware Requirements * Any **ESP32** development board. * **CS1237** or **CS1238** ADC module connected to a scale / load cell / bridge sensor. --- ## ⚠️ Important Hardware Considerations ### Current Limit for Low-Impedance Sensors Stock CS1237/CS1238 modules are current-limited by resistor **R1 (1 kΩ)**. For low-impedance sensors (such as **350 Ω load cells**), reduce R1 by adding an external resistor between **DVDD** and **AVDD**. For full hardware details, visit the [`Current Limit for Low-Impedance Sensors`](https://github.com/FMazz97/CS123x#%EF%B8%8F-important-current-limit-for-low-impedance-sensors) section on [`CS123x Repository`](https://github.com/FMazz97/CS123x). --- ## ⚙️ Building & Flashing This example already includes both an ESP-IDF-native `CMakeLists.txt`/`main/idf_component.yml` and a ready-to-use `platformio.ini` — no manual setup needed for either toolchain. Pick whichever you already have installed. > **Note:** If you switch between ESP-IDF (`idf.py`) and PlatformIO on the same folder, run `idf.py fullclean` (or delete the `build/` directory) first — the two toolchains don't share build caches and will conflict otherwise. ### Option A: ESP-IDF (native, `idf.py`) ```bash idf.py build idf.py -p <PORT> flash monitor ``` ### Option B: ESP-IDF on PlatformIO 1. Open this folder in VS Code with the PlatformIO extension installed. 2. Click **Build**, then **Upload**, then **Monitor**. --- ## 📝 Usage Steps When the program boots: 1. **Interactive Menu:** After initialization, an interactive menu is printed to the serial console on boot. 2. **CLI Controls:** * `[r]` -> Run **Gaussian Noise Test** across the configured sample size. * `[n]` -> Change number of **samples** (default: 1000). * `[c]` -> Cycle active input **channel** (`CH_A` -> `CH_B` -> `CH_TEMP` -> `CH_SHORT`). * `[g]` -> Cycle **gain** setting (`1x` -> `2x` -> `64x` -> `128x`). * `[f]` -> Cycle **sampling rate** setting (`10Hz` -> `40Hz` -> `640Hz` -> `1280Hz`). * `[h]` -> Reprint **help** menu and current configuration status. 3. **Results & Evaluation:** The statistical summary outputs mean (offset), RMS noise, peak-to-peak noise, ENOB, and noise-free resolution bits directly in the serial log. --- ## 📄 License Distributed under the MIT License. See [LICENSE](https://github.com/FMazz97/CS123x/blob/main/LICENSE) for more information.
To create a project from this example, run:
idf.py create-project-from-example "fmazz97/cs123x=2.0.0:test_gaussian"