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+/* ----------------------------------------------------------------------
+ * Project: CMSIS DSP Library
+ * Title: arm_mfcc_init_f16.c
+ * Description: MFCC initialization function for the f16 version
+ *
+ * $Date: 07 September 2021
+ * $Revision: V1.10.0
+ *
+ * Target Processor: Cortex-M and Cortex-A cores
+ * -------------------------------------------------------------------- */
+
+/*
+ * Copyright (C) 2010-2021 ARM Limited or its affiliates. All rights reserved.
+ *
+ * SPDX-License-Identifier: Apache-2.0
+ *
+ * Licensed under the Apache License, Version 2.0 (the License); you may
+ * not use this file except in compliance with the License.
+ * You may obtain a copy of the License at
+ *
+ * www.apache.org/licenses/LICENSE-2.0
+ *
+ * Unless required by applicable law or agreed to in writing, software
+ * distributed under the License is distributed on an AS IS BASIS, WITHOUT
+ * WARRANTIES OR CONDITIONS OF ANY KIND, either express or implied.
+ * See the License for the specific language governing permissions and
+ * limitations under the License.
+ */
+#include "arm_compiler_specific.h"
+
+
+
+/**
+ * @defgroup MFCCF16 MFCC F16
+ */
+
+
+/**
+ @ingroup MFCC
+ */
+
+
+/**
+ @addtogroup MFCCF16
+ @{
+ */
+
+
+#include "dsp/transform_functions_f16.h"
+
+#if defined(ARM_FLOAT16_SUPPORTED)
+
+/**
+ @brief Generic initialization of the MFCC F16 instance structure
+ @param[out] S points to the mfcc instance structure
+ @param[in] fftLen fft length
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+
+ @par
+ This function should be used only if you don't know the FFT sizes that
+ you'll need at build time. The use of this function will prevent the
+ linker from removing the FFT tables that are not needed and the library
+ code size will be bigger than needed.
+
+ @par
+ If you use CMSIS-DSP as a static library, and if you know the MFCC sizes
+ that you need at build time, then it is better to use the initialization
+ functions defined for each MFCC size.
+
+ */
+
+ARM_DSP_ATTRIBUTE arm_status arm_mfcc_init_f16(
+ arm_mfcc_instance_f16 * S,
+ uint32_t fftLen,
+ uint32_t nbMelFilters,
+ uint32_t nbDctOutputs,
+ const float16_t *dctCoefs,
+ const uint32_t *filterPos,
+ const uint32_t *filterLengths,
+ const float16_t *filterCoefs,
+ const float16_t *windowCoefs
+ )
+{
+ arm_status status;
+
+ S->fftLen=fftLen;
+ S->nbMelFilters=nbMelFilters;
+ S->nbDctOutputs=nbDctOutputs;
+ S->dctCoefs=dctCoefs;
+ S->filterPos=filterPos;
+ S->filterLengths=filterLengths;
+ S->filterCoefs=filterCoefs;
+ S->windowCoefs=windowCoefs;
+
+ #if defined(ARM_MFCC_USE_CFFT)
+ status=arm_cfft_init_f16(&(S->cfft),fftLen);
+ #else
+ status=arm_rfft_fast_init_f16(&(S->rfft),fftLen);
+ #endif
+
+ return(status);
+}
+
+#if defined(ARM_MFCC_USE_CFFT)
+#define MFCC_INIT_F16(LEN) \
+ARM_DSP_ATTRIBUTE arm_status arm_mfcc_init_##LEN##_f16( \
+ arm_mfcc_instance_f16 * S, \
+ uint32_t nbMelFilters, \
+ uint32_t nbDctOutputs, \
+ const float16_t *dctCoefs, \
+ const uint32_t *filterPos, \
+ const uint32_t *filterLengths, \
+ const float16_t *filterCoefs, \
+ const float16_t *windowCoefs \
+ ) \
+{ \
+ arm_status status; \
+ \
+ S->fftLen=LEN; \
+ S->nbMelFilters=nbMelFilters; \
+ S->nbDctOutputs=nbDctOutputs; \
+ S->dctCoefs=dctCoefs; \
+ S->filterPos=filterPos; \
+ S->filterLengths=filterLengths; \
+ S->filterCoefs=filterCoefs; \
+ S->windowCoefs=windowCoefs; \
+ \
+ status=arm_cfft_init_##LEN##_f16(&(S->cfft));\
+ \
+ return(status); \
+}
+#else
+#define MFCC_INIT_F16(LEN) \
+ARM_DSP_ATTRIBUTE arm_status arm_mfcc_init_##LEN##_f16( \
+ arm_mfcc_instance_f16 * S, \
+ uint32_t nbMelFilters, \
+ uint32_t nbDctOutputs, \
+ const float16_t *dctCoefs, \
+ const uint32_t *filterPos, \
+ const uint32_t *filterLengths, \
+ const float16_t *filterCoefs, \
+ const float16_t *windowCoefs \
+ ) \
+{ \
+ arm_status status; \
+ \
+ S->fftLen=LEN; \
+ S->nbMelFilters=nbMelFilters; \
+ S->nbDctOutputs=nbDctOutputs; \
+ S->dctCoefs=dctCoefs; \
+ S->filterPos=filterPos; \
+ S->filterLengths=filterLengths; \
+ S->filterCoefs=filterCoefs; \
+ S->windowCoefs=windowCoefs; \
+ \
+ status=arm_rfft_fast_init_##LEN##_f16(&(S->rfft));\
+ \
+ return(status); \
+}
+#endif
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 32 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(32)
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 64 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(64)
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 128 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(128)
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 256 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(256)
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 512 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(512)
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 1024 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(1024)
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 2048 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(2048)
+
+/**
+ @brief Initialization of the MFCC F16 instance structure for 4096 samples MFCC
+ @param[out] S points to the mfcc instance structure
+ @param[in] nbMelFilters number of Mel filters
+ @param[in] nbDctOutputs number of Dct outputs
+ @param[in] dctCoefs points to an array of DCT coefficients
+ @param[in] filterPos points of the array of filter positions
+ @param[in] filterLengths points to the array of filter lengths
+ @param[in] filterCoefs points to the array of filter coefficients
+ @param[in] windowCoefs points to the array of window coefficients
+
+ @return error status
+
+ @par Description
+ The matrix of Mel filter coefficients is sparse.
+ Most of the coefficients are zero.
+ To avoid multiplying the spectrogram by those zeros, the
+ filter is applied only to a given position in the spectrogram
+ and on a given number of FFT bins (the filter length).
+ It is the reason for the arrays filterPos and filterLengths.
+
+ window coefficients can describe (for instance) a Hamming window.
+ The array has the same size as the FFT length.
+
+ The folder Scripts is containing a Python script that can be used
+ to generate the filter, dct and window arrays.
+*/
+MFCC_INIT_F16(4096)
+
+#endif /* defined(ARM_FLOAT16_SUPPORTED) */
+/**
+ @} end of MFCCF16 group
+ */