Sync audio_rective changes from auto-playlist branch
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@@ -141,9 +141,7 @@ static uint8_t fftResult[NUM_GEQ_CHANNELS]= {0}; // Our calculated freq. chann
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static float fftCalc[NUM_GEQ_CHANNELS] = {0.0f}; // Try and normalize fftBin values to a max of 4096, so that 4096/16 = 256. (also used by dynamics limiter)
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static float fftAvg[NUM_GEQ_CHANNELS] = {0.0f}; // Calculated frequency channel results, with smoothing (used if dynamics limiter is ON)
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unsigned int zeroCrossingCount = 0;
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unsigned int energy = 0;
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unsigned int lowFreqencyContent = 0;
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uint_fast16_t zeroCrossingCount = 0;
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// TODO: probably best not used by receive nodes
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static float agcSensitivity = 128; // AGC sensitivity estimation, based on agc gain (multAgc). calculated by getSensitivity(). range 0..255
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@@ -499,6 +497,17 @@ void FFTcode(void * parameter)
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// get a fresh batch of samples from I2S
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if (audioSource) audioSource->getSamples(vReal, samplesFFT);
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// WLED-MM/TroyHacks: Calculate zero crossings
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//
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zeroCrossingCount = 0;
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for (int i=0; i < samplesFFT; i++) {
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if (i < (samplesFFT)-2) {
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if((vReal[i] >= 0 && vReal[i+1] < 0) || (vReal[i+1] < 0 && vReal[i+1] >= 0)) {
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zeroCrossingCount++;
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}
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}
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}
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#if defined(WLED_DEBUG) || defined(SR_DEBUG)|| defined(SR_STATS)
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// debug info in case that stack usage changes
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static unsigned int minStackFree = UINT32_MAX;
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@@ -555,17 +564,7 @@ void FFTcode(void * parameter)
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// pick our our current mic sample - we take the max value from all samples that go into FFT
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if ((vReal[i] <= (INT16_MAX - 1024)) && (vReal[i] >= (INT16_MIN + 1024))) //skip extreme values - normally these are artefacts
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if (fabsf((float)vReal[i]) > maxSample) maxSample = fabsf((float)vReal[i]);
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// WLED-MM/TroyHacks: Calculate zero crossings
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if (i < samplesFFT-2) {
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if (vReal[i] * vReal[i+1] < 0) {
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zeroCrossingCount++;
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}
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}
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// WLED-MM/TroyHacks: Calculate energy
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energy += vReal[i] * vReal[i];
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}
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energy /= 100000; // WLED-MM/TroyHacks: scale this down becasue we're gonna make it bigger later
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// release highest sample to volume reactive effects early - not strictly necessary here - could also be done at the end of the function
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// early release allows the filters (getSample() and agcAvg()) to work with fresh values - we will have matching gain and noise gate values when we want to process the FFT results.
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@@ -661,8 +660,6 @@ void FFTcode(void * parameter)
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vReal[i] = t / 16.0f; // Reduce magnitude. Want end result to be scaled linear and ~4096 max.
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} // for()
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lowFreqencyContent = fftAddAvg(1,9); // WLED-MM/TroyHacks: Calculate Low-Frequency Content
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// mapping of FFT result bins to frequency channels
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//if (fabsf(sampleAvg) > 0.25f) { // noise gate open
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if (fabsf(volumeSmth) > 0.25f) { // noise gate open
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@@ -1763,10 +1760,8 @@ class AudioReactive : public Usermod {
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um_data->u_type[9] = UMT_FLOAT;
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um_data->u_data[10] = &agcSensitivity; // used (New)
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um_data->u_type[10] = UMT_FLOAT;
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unsigned int* extra[3] = {&zeroCrossingCount, &energy, &lowFreqencyContent};
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um_data->u_data[11] = extra; //
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um_data->u_type[11] = UMT_INT16_ARR;
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um_data->u_data[11] = &zeroCrossingCount;
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um_data->u_type[11] = UMT_UINT16;
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#else
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// ESP8266
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// See https://github.com/MoonModules/WLED/pull/60#issuecomment-1666972133 for explanation of these alternative sources of data
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