Aps working, or almost working?
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257
src/ps/aps.rs
257
src/ps/aps.rs
@ -1,4 +1,5 @@
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use super::timebuffer::TimeBuffer;
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use super::CrossPowerSpecra;
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use super::*;
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use crate::config::*;
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use anyhow::{bail, Result};
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@ -12,6 +13,8 @@ pub enum Overlap {
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Percentage(Flt),
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/// Number of samples to overlap
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Number(usize),
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/// No overlap at all, which is the same as Overlap::Number(0)
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NoOverlap,
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}
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impl Default for Overlap {
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fn default() -> Self {
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@ -20,14 +23,14 @@ impl Default for Overlap {
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}
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/// Result from [AvPowerspectra.compute()]
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pub enum ApsResult {
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pub enum ApsResult<'a> {
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/// Returns all intermediate results. Useful when evolution over time should
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/// be visible. I.e. in case of spectrograms, but also in case the
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/// converging process to the average should be made visible.
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AllIntermediateResults(Vec<CrossPowerSpecra>),
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AllIntermediateResults(Vec<CPS>),
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/// Give only last result back, the most recent value.
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OnlyLastResult(CrossPowerSpecra),
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OnlyLastResult(&'a CPS),
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/// No new data available. Nothing given back.
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None,
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@ -70,6 +73,7 @@ pub struct AvPowerSpectra {
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// Power spectra estimator for single block
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ps: PowerSpectra,
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// The mode with which the AvPowerSpectra is computing.
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mode: ApsMode,
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// The number of samples to keep in the time buffer when overlapping time
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@ -83,7 +87,7 @@ pub struct AvPowerSpectra {
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timebuf: TimeBuffer,
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// Current estimation of the power spectra
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cur_est: Cmat,
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cur_est: CPS,
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}
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impl AvPowerSpectra {
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/// The FFT Length of estimating (cross)power spectra
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@ -106,6 +110,7 @@ impl AvPowerSpectra {
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}
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// If overlap percentage is 0, this gives
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Overlap::Percentage(p) => ((p * nfft as Flt) / 100.) as usize,
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Overlap::NoOverlap => 0,
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_ => unreachable!(),
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};
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if overlap_keep >= nfft {
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@ -122,7 +127,7 @@ impl AvPowerSpectra {
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///
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/// * `nfft` - FFT Length
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pub fn new_simple(nfft: usize) -> Result<AvPowerSpectra> {
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return AvPowerSpectra::new(nfft, None, None, None);
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return AvPowerSpectra::build(nfft, None, None, None);
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}
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/// Create power spectra estimator which weighs either all data
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@ -144,7 +149,7 @@ impl AvPowerSpectra {
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/// - `overlap` - Amount of overlap in
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/// - `mode` - The mode in which the
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///
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pub fn new(
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pub fn build(
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nfft: usize,
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windowtype: Option<WindowType>,
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overlap: Option<Overlap>,
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@ -179,10 +184,84 @@ impl AvPowerSpectra {
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overlap_keep,
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mode,
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N: 0,
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cur_est: Cmat::default((0, 0)),
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cur_est: CPS::default((0, 0, 0)),
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timebuf: TimeBuffer::new(),
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})
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}
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// Update result for single block
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fn update_singleblock<'a, T>(&mut self, timedata: T)
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where
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T: AsArray<'a, Flt, Ix2>,
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{
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let timeblock = timedata.into();
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let Cpsnew = self.ps.compute(&timeblock);
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// println!("Cpsnew: {:?}", Cpsnew[[0, 0, 0]]);
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// Initialize to zero
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if self.cur_est.len() == 0 {
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assert_eq!(self.N, 0);
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self.cur_est = CPS::zeros(Cpsnew.raw_dim().f());
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}
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// Update the number of blocks processed
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self.N += 1;
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// Apply operation based on mode
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match self.mode {
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ApsMode::AllAveraging => {
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let Nf = Cflt {
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re: self.N as Flt,
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im: 0.,
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};
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self.cur_est = (Nf - 1.) / Nf * &self.cur_est + 1. / Nf * Cpsnew;
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}
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ApsMode::ExponentialWeighting { fs, tau } => {
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debug_assert!(self.N > 0);
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if self.N == 1 {
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self.cur_est = Cpsnew;
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} else {
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// A sound level meter specifies a low pass filter with one
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// real pole at -1/tau, for a time weighting of tau. This
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// means the analogue transfer function is 1 /
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// (tau*s+1).
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// Now we want to approximate this with a digital transfer
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// function. The step size, or sampling period is:
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// T = (nfft-overlap_keep)/fs.
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// Then, when using the matched z-transform (
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// https://en.wikipedia.org/wiki/Matched_Z-transform_method),
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// an 1/(s-p) is replaced by 1/(1-exp(p*T)*z^-1).
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// So the digital transfer function will be:
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// H[n] ≅ K / (1 - exp(-T/tau) * z^-1).
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// , where K is a to-be-determined constant, for which we
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// take the value such that the D.C. gain equals 1. To get
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// the frequency response at D.C., we have to set z=1, so
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// to set the D.C. to 1, we have to set K = 1-exp(-T/tau).
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// Hence:
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// H[n] ≅ (1- exp(-T/tau)) / (1 - exp(-T/tau) * z^-1).
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// Or as a finite difference equation:
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//
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// y[n] * (1-exp(-T/tau)* z^-1) = (1-exp(-T/tau)) * x[n]
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// or, finally:
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// y[n] = alpha * y[n-1] + (1-alpha) * x[n]
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// where alpha = exp(-T/tau).
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let T = (self.nfft() - self.overlap_keep) as Flt / fs;
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let alpha = Cflt::ONE * Flt::exp(-T / tau);
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self.cur_est = alpha * &self.cur_est + (1. - alpha) * Cpsnew;
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}
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}
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ApsMode::Spectrogram => {
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self.cur_est = Cpsnew;
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}
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}
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}
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/// Computes average (cross)power spectra, and returns only the most recent
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/// estimate, if any can be given back. Only gives back a result when enough
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/// data is available.
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@ -191,38 +270,178 @@ impl AvPowerSpectra {
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///
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/// * `timedata``: New available time data. Number of columns is number of
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/// channels, number of rows is number of frames (samples per channel).
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/// * `giveInterMediateResults`
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/// * `giveInterMediateResults` - If true: returns a vector of all
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/// intermediate results. Useful when plotting spectra over time.
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///
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/// # Panics
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///
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/// If timedata.ncols() does not match number of columns in already present
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/// data.
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fn compute<'a, T>(&mut self, timedata: T, giveInterMediateResults: bool) -> ApsResult
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pub fn compute<'a, 'b, T>(
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&'a mut self,
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timedata: T,
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giveInterMediateResults: bool,
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) -> ApsResult<'a>
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where
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T: AsArray<'a, Flt, Ix2>,
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T: AsArray<'b, Flt, Ix2>,
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{
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// Push new data in the time buffer.
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self.timebuf.push(timedata);
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// Storage for the result
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let mut result = ApsResult::None;
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// Flag to indicate that we have obtained one result for sure.
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let mut computed_single = false;
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// Iterate over all blocks that can come,
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while let Some(timeblock) = self.timebuf.pop(self.nfft(), self.overlap_keep) {
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// Compute cross-power spectra for current time block
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let Cpsnew = self.ps.compute(&timeblock);
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// Ok, mode-determined
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match self.mode {
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ApsMode::AllAveraging => {}
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ApsMode::ExponentialWeighting { fs, tau } => {}
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ApsMode::Spectrogram => {}
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self.update_singleblock(&timeblock);
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// We ha
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computed_single = true;
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if giveInterMediateResults {
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// Initialize with empty vector
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if let ApsResult::None = result {
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result = ApsResult::AllIntermediateResults(Vec::new())
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}
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}
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// So
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if let ApsResult::AllIntermediateResults(v) = &mut result {
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v.push(self.cur_est.clone());
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}
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// if self.cur_est.len() > 0
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}
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ApsResult::None
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if computed_single && !giveInterMediateResults {
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// We have computed it once, but we are not interested in
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// intermediate results. So we return a reference to the last data.
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return ApsResult::OnlyLastResult(&self.cur_est);
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}
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result
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}
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/// See [AvPowerSpectra](compute())
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fn compute_last<'a, T>(&mut self, timedata: T) -> ApsResult
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pub fn compute_last<'a, T>(&mut self, timedata: T) -> ApsResult
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where
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T: AsArray<'a, Flt, Ix2>,
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{
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return self.compute(timedata, false);
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}
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}
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#[cfg(test)]
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mod test {
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use approx::assert_abs_diff_eq;
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use ndarray_rand::rand_distr::Normal;
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use ndarray_rand::RandomExt;
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use super::CrossPowerSpecra;
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use crate::{config::*, ps::ApsResult};
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use super::{ApsMode, AvPowerSpectra, Overlap, WindowType, CPS};
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#[test]
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fn test_overlap_keep() {
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let nfft = 10;
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assert_eq!(
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AvPowerSpectra::get_overlap_keep(nfft, Overlap::Percentage(50.)).unwrap(),
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nfft / 2
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);
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let nfft = 11;
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assert_eq!(
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AvPowerSpectra::get_overlap_keep(nfft, Overlap::Percentage(50.)).unwrap(),
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nfft / 2
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);
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let nfft = 1024;
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assert_eq!(
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AvPowerSpectra::get_overlap_keep(nfft, Overlap::Percentage(25.)).unwrap(),
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nfft / 4
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);
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assert_eq!(
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AvPowerSpectra::get_overlap_keep(nfft, Overlap::Number(10)).unwrap(),
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10
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);
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}
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/// When the time constant is 1.0, every second the powers approximately
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/// halve. That is the subject of this test.
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#[test]
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fn test_expweighting() {
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let nfft = 48000;
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let fs = nfft as Flt;
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let tau = 2.;
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let mut aps = AvPowerSpectra::build(
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nfft,
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None,
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Some(Overlap::NoOverlap),
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Some(ApsMode::ExponentialWeighting { fs, tau }),
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)
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.unwrap();
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assert_eq!(aps.overlap_keep, 0);
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let distr = Normal::new(1.0, 1.0).unwrap();
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let timedata_some = Dmat::random((nfft, 1), distr);
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let timedata_zeros = Dmat::zeros((nfft, 1));
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let mut first_result = CPS::zeros((0, 0, 0));
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if let ApsResult::OnlyLastResult(v) = aps.compute_last(timedata_some.view()) {
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first_result = v.clone();
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// println!("{:?}", first_result.ap(0)[0]);
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} else {
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assert!(false, "Should return one value");
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}
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let overlap_keep = AvPowerSpectra::get_overlap_keep(nfft, Overlap::NoOverlap).unwrap();
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if let ApsResult::OnlyLastResult(v) = aps.compute_last(&timedata_zeros) {
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} else {
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assert!(false, "Should return one value");
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}
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if let ApsResult::OnlyLastResult(v) = aps.compute_last(&timedata_zeros) {
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let alpha = Flt::exp(-((nfft - overlap_keep) as Flt) / (fs * tau));
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// let alpha: Flt = 1.;
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for i in 0..nfft / 2 + 1 {
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// println!("i={i}");
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assert_abs_diff_eq!(first_result.ap(0)[i] * alpha.powi(2), v.ap(0)[i]);
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}
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} else {
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assert!(false, "Should return one value");
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}
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assert_eq!(aps.N, 3);
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}
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#[test]
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fn test_tf1() {
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let nfft = 4800;
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let distr = Normal::new(1.0, 1.0).unwrap();
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let mut timedata = Dmat::random((nfft, 1), distr);
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timedata
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.push_column(timedata.column(0).mapv(|a| 2. * a).view())
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.unwrap();
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let mut aps = AvPowerSpectra::build(nfft, None, None, None).unwrap();
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if let ApsResult::OnlyLastResult(v) = aps.compute_last(&timedata) {
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let tf = v.tf(0, 1, None);
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assert_eq!((&tf - 2.0 * Cflt::ONE).sum().abs(), 0.0);
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} else {
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assert!(false);
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}
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}
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#[test]
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fn test_ap() {
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let nfft = 256;
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let distr = Normal::new(1.0, 1.0).unwrap();
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let timedata = Dmat::random((500 * nfft, 1), distr);
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let timedata_mean_square = (&timedata * &timedata).sum() / (timedata.len() as Flt);
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for wt in [Some(WindowType::Rect), Some(WindowType::Hann), Some(WindowType::Bartlett), Some(WindowType::Blackman), None] {
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let mut aps = AvPowerSpectra::build(nfft, wt, None, None).unwrap();
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if let ApsResult::OnlyLastResult(v) = aps.compute_last(&timedata) {
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let ap = v.ap(0);
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assert_abs_diff_eq!((&ap).sum().abs(), timedata_mean_square, epsilon = 4e-3);
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} else {
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assert!(false);
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}
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}
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}
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}
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@ -11,7 +11,7 @@ mod timebuffer;
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mod window;
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use crate::config::*;
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pub type CrossPowerSpecra = Array3<Cflt>;
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pub use aps::{ApsMode, AvPowerSpectra, Overlap, ApsResult};
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pub use ps::PowerSpectra;
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pub use aps::{ApsMode, ApsResult, AvPowerSpectra, Overlap};
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pub use ps::{CrossPowerSpecra, PowerSpectra, CPS};
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pub use window::{Window, WindowType};
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68
src/ps/ps.rs
68
src/ps/ps.rs
@ -7,12 +7,76 @@ use std::usize;
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use crate::Dcol;
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use super::{fft::FFT, CrossPowerSpecra};
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use super::window::*;
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use super::fft::FFT;
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use std::mem::MaybeUninit;
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use realfft::{RealFftPlanner, RealToComplex};
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/// Cross power spectra, which is a 3D array, with the following properties:
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///
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/// - The first index is the frequency index, starting at DC, ending at nfft/2.
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/// - The second, and third index result in [i,j] = C_ij = p_i * conj(p_j)
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///
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pub type CPS = Array3<Cflt>;
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/// Extra typical methods that are of use for 3D-arrays of complex numbers, that
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/// are typically implemented as cross-power spectra.
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pub trait CrossPowerSpecra {
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/// Returns the autopower for a single channel, as a array of real values
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/// (imaginary part is zero and is stripped off).
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///
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/// # Args
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///
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/// - `ch` - The channel number to compute autopower for.
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fn ap(&self, ch: usize) -> Array1<Flt>;
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/// Returns the transfer function from `chi` to `chj`, that is ~ Pj/Pi a
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/// single channel, as a array of complex numbers.
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///
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/// # Args
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///
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/// - `chi` - The channel number of the *denominator*
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/// - `chj` - The channel number of the *numerator*
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/// - `chRef` - Optional, a reference channel that has the lowest noise. If
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/// not given, the average of the two autopowers is used, which gives
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/// always a worse result than when two a low noise reference channel is
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/// used.
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///
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fn tf(&self, chi: usize, chj: usize, chRef: Option<usize>) -> Array1<Cflt>;
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}
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impl CrossPowerSpecra for CPS {
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fn ap(&self, ch: usize) -> Array1<Flt> {
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// Slice out one value for all frequencies, map to only real part, and
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// return.
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self.slice(s![.., ch, ch]).mapv(|f| f.re)
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}
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// fn apsp
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fn tf(&self, chi: usize, chj: usize, chRef: Option<usize>) -> Array1<Cflt> {
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match chRef {
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None => {
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let cij = self.slice(s![.., chi, chj]);
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let cii = self.slice(s![.., chi, chi]);
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let cjj = self.slice(s![.., chj, chj]);
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Zip::from(cij)
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.and(cii)
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.and(cjj)
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.par_map_collect(|cij, cii, cjj| 0.5 * (cij.conj() / cii + cjj / cij))
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}
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Some(chr) => {
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let cir = self.slice(s![.., chi, chr]);
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let cjr = self.slice(s![.., chj, chr]);
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Zip::from(cir)
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.and(cjr)
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.par_map_collect(|cir, cjr| cjr / cir)
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}
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}
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}
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}
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/// Single-sided (cross)power spectra estimator, that uses a Windowed FFT to estimate cross-power
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/// spectra. Window functions are documented in the `window` module. Note that
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/// directly using this power spectra estimator is generally not useful as it is
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@ -128,7 +192,7 @@ impl PowerSpectra {
|
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/// (nfft/2+1,timedata.ncols(), timedata.ncols()). Its content is:
|
||||
/// [freq_index, chi, chj] = crosspower: chi*conj(chj)
|
||||
///
|
||||
pub fn compute<'a, T>(&mut self, tdata: T) -> CrossPowerSpecra
|
||||
pub fn compute<'a, T>(&mut self, tdata: T) -> CPS
|
||||
where
|
||||
T: AsArray<'a, Flt, Ix2>,
|
||||
{
|
||||
|
@ -67,7 +67,7 @@ impl TimeBuffer {
|
||||
let nsamples_available = c1.len();
|
||||
debug_assert!(nsamples_available == self.nsamples());
|
||||
if nsamples_available < nsamples_requested {
|
||||
println!("Less available than requested");
|
||||
// println!("Less available than requested");
|
||||
return None;
|
||||
}
|
||||
// Number of channels
|
||||
@ -159,4 +159,22 @@ mod test {
|
||||
assert_eq!(tres.shape(), [50, 2]);
|
||||
assert_eq!(t2.slice(s![..50, ..2]), tres);
|
||||
}
|
||||
#[test]
|
||||
fn test_timebuffer3() {
|
||||
let mut tb = TimeBuffer::new();
|
||||
let t1 = Dmat::zeros((10,1));
|
||||
tb.push(&t1);
|
||||
tb.push(&t1);
|
||||
assert_eq!(tb.nsamples(), 20);
|
||||
|
||||
let tres = tb.pop(10, 5).unwrap();
|
||||
assert_eq!(tres.shape(), [10, 1]);
|
||||
assert_eq!(tb.nsamples(), 15);
|
||||
let tres = tb.pop(10, 0).unwrap();
|
||||
assert_eq!(tb.nsamples(), 5);
|
||||
let tres = tb.pop(5, 5).unwrap();
|
||||
assert_eq!(tres.shape(), [5, 1]);
|
||||
assert_eq!(tb.nsamples(), 5);
|
||||
// assert_eq!(t2.slice(s![..50, ..2]), tres);
|
||||
}
|
||||
}
|
||||
|
Loading…
Reference in New Issue
Block a user