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DSSS Burst Acquisition

doppler.dsss.Acquisition acquires a direct-sequence spread-spectrum burst — a run of repeated, BPSK-modulated PN-code segments — arriving with an unknown code phase and an unknown carrier-frequency (Doppler) offset, buried in noise. It owns the whole receive-side acquisition pipeline:

raw cf32  →  ring  →  reframe (doppler_bins, code_bins)  →  slow-time Doppler FFT
          →  code correlation (corr2d)  →  CFAR gate  →  (Doppler, code-phase) hits

Construction is physics-only: you state the waveform (code, chip_rate), the front end (spc), the sensitivity (cn0_dbhz), and a target (Pfa, Pd). The engine sizes its own search grid — coherent depth, threshold, non-coherent looks — from the detection theory and streams detections. You never pick a bin count or a threshold.

This is the usage walk-through. For the matched-filter surface it builds on, see 2-D Acquisition (Detector2D); for what happens after acquisition, see the DSSS Despreader.

The 30-second version

import numpy as np
from doppler.dsss import Acquisition
from doppler.wfm import PN, mls_poly

code = PN(poly=mls_poly(5), seed=1, length=5).generate(31)  # 31-chip PN

acq = Acquisition(
    code,                  # sf = len(code) = 31 (inferred)
    reps=16,               # up to 16 coherent code repetitions
    spc=4,                 # samples per chip (fs = chip_rate · spc)
    chip_rate=1.023e6,     # Hz
    cn0_dbhz=48,           # sensitivity (carrier-to-noise density, dB-Hz)
    pfa=1e-3, pd=0.9,      # target false-alarm / detection rates
)
# The engine sized the grid: doppler_bins=12, code_bins=124, res≈2750 Hz.
assert acq.pd_predicted >= acq.pd          # confirm it can meet the target

# demo capture: a real 31-chip DSSS burst in light noise, split into
# cf32 blocks (any block size works — the engine reframes internally).
chip = np.repeat(1 - 2.0 * (code & 1), 4)  # ±1 per chip, ×spc oversample
capture = np.tile(chip, 36).astype(np.complex64) * 8.0
capture += (0.1 * (np.random.standard_normal(capture.size)
            + 1j * np.random.standard_normal(capture.size))
            ).astype(np.complex64)
iq_stream = np.array_split(capture, 8)

for chunk in iq_stream:                          # any cf32 block size
    for dop, phase, peak, noise, stat, snr in acq.push(chunk):
        print(f"hit: Doppler bin {dop}, code phase {phase} samples, "
              f"SNR≈{snr:.2f}")

The acquisition problem

A spread-spectrum transmitter sends the same PN segment over and over (the acquisition preamble). By the time it reaches you it has an unknown code phase (propagation delay, a circular shift of the code) and an unknown carrier offset (Doppler), and it is well below the noise floor. Acquisition is the 2-D search that recovers both at once:

  • code phasewhere in the code period the signal sits (the matched-filter lag), and
  • Doppler binhow far the carrier has shifted.

Acquisition evaluates the entire (Doppler × code-phase) grid per frame and reports the cells whose detection statistic crosses an automatically set CFAR gate.


How it works — slow-time / fast-time

Acquisition is a delay–Doppler search, and Acquisition factors it into two FFTs over the repeated-segment structure. It frames the stream into a (doppler_bins, code_bins) matrix where each row is one PN segment — one code repetition — and there are doppler_bins of them:

  • fast-timewithin one segment (code_bins = sf·spc samples). A circular correlation against the known code → the code-phase axis.
  • slow-timeacross the doppler_bins segments. An FFT along that axis resolves the per-segment carrier phase ramp → the Doppler axis.
            fast-time  (code_bins = sf·spc samples, one segment)
          ┌─────────────────────────────────────────────┐
slow-time │ rep 0   · · · · · · · · · · · · · · · · · · │
(rows =   │ rep 1   · · · · · · · · · · · · · · · · · · │   FFT down ──► Doppler
 code     │  ...                                        │   columns
 reps)    │ rep d-1 · · · · · · · · · · · · · · · · · · │
          └─────────────────────────────────────────────┘
                      │ circular code correlation
                      ▼  along each row → code phase

The coherent depth doppler_bins is chosen by the engine — the smallest number of repetitions in [1, reps] that meets pd at your cn0_dbhz (more on that below). Internally the fast-time correlation is the FFT-domain Corr2D engine against a single-row reference (the code in row 0, zeros elsewhere); the slow-time FFT is applied to the data before that correlation. Because the engine ingests raw samples and does the slow-time FFT itself, you never pre-transform anything — just push IQ.

Doppler resolution and range (in Hz)

Two independent quantities, both reported as read-only properties:

  • resolution doppler_res_hz = chip_rate / (sf · doppler_bins) — set by how many repetitions the engine integrates (deeper → finer bins).
  • span doppler_span_hz = ±chip_rate / (2·sf) — the slow-time Nyquist, set by the code period (sf chips) alone, independent of spc and doppler_bins.

With sf=31, chip_rate=1.023 MHz, doppler_bins=12: bins are ≈2750 Hz apart, spanning ±16.5 kHz. To search wider than the native span, sweep a coarse Doppler grid in front of Acquisition — see Widening the Doppler search.


Auto-configuration from the physics

You do not pick a threshold, a coherent depth, or a bin count — you state the operating point and the engine derives the grid with the detection functions.

First it converts your sensitivity to the per-sample amplitude SNR the detection math uses (noise power = N0·fs over the sampled bandwidth):

fs   = chip_rate · spc
snr  = sqrt( 10**(cn0_dbhz/10) / fs )      # per-sample amplitude SNR

Then it picks the smallest coherent depth D ∈ [1, reps] whose D·code_bins coherent samples meet pd — least latency for a strong signal, full reps for a weak one:

for D in 1 .. reps:
    cells     = searched_bins(D) · code_bins      # Bonferroni population
    pfa_cell  = 1 - (1 - pfa)**(1/cells)
    eta       = det_threshold(pfa_cell)           # √(-2 ln pfa_cell)
    if det_pd(snr, D·code_bins, eta) ≥ pd: break  # accept this depth
doppler_bins = D
threshold    = eta · √(2/π)                        # eta in mean-CFAR units

The chosen grid is exposed as read-only properties:

acq = Acquisition(code, reps=16, spc=4, chip_rate=1.023e6, cn0_dbhz=48,
                  pfa=1e-3, pd=0.9)

acq.doppler_bins, acq.code_bins   # 12, 124   — the grid the engine chose
acq.doppler_span_hz, acq.doppler_res_hz   # ±16500 Hz, 2750 Hz
acq.fs                            # 4.092e6   — chip_rate · spc
acq.pfa_cell                      # per-cell false-alarm prob (Bonferroni)
acq.eta                           # raw Rayleigh threshold √(-2 ln pfa_cell)
acq.threshold                     # the CFAR gate actually applied (eta·√(2/π))
acq.n_noncoh                      # non-coherent looks (1 = pure coherent)
acq.pd_predicted, acq.underpowered   # achieved Pd, and whether it fell short

Check underpowered after construction

When the operating point is infeasible — even reps coherent repetitions plus non-coherent looks (up to max_noncoh) cannot reach pd — auto-config does not raise; it builds a best-effort grid with pd_predicted < pd, sets acq.underpowered = True, and emits a UserWarning. Guard against shipping an under-powered acquirer:

assert acq.pd_predicted >= acq.pd, f"under-powered: {acq.pd_predicted:.2f}"

The levers that close a shortfall are a higher cn0_dbhz (if the signal really is stronger), more reps, a tighter doppler_uncertainty, or max_noncoh > 1 to engage non-coherent integration.

cn0_dbhz is the universal sensitivity spec — carrier-to-noise density in dB-Hz, independent of sample rate. A stronger cn0_dbhz lets the engine reach pd with fewer repetitions (lower latency, coarser Doppler):

cn0_dbhz chosen doppler_bins (reps=16) pd_predicted
54 3 0.96
50 7 0.92
48 12 0.94

noise_mode selects the CFAR estimator ("mean" by default, which is what the analytic threshold assumes; "median" is more robust but is not analytically calibrated).


Streaming and reading hits

push accepts any-length cf32 blocks, buffers them in a ring, and emits one detection per coherent frame (or, on the non-coherent path, per n_noncoh accumulated frames) whose statistic clears the gate. Each hit is a 6-tuple:

for dop, phase, peak, noise, stat, snr in acq.push(chunk):
    ...
field meaning
doppler_bin peak row — slow-time Doppler bin (0 … doppler_bins-1)
code_phase peak column — integer-sample code phase (0 … code_bins-1)
peak_mag peak correlation magnitude over the surface
noise_est CFAR noise estimate
test_stat peak_mag / noise_est (compared against threshold)
snr_est estimated per-sample amplitude SNR of the burst

Map the integer bins back to physical units:

def doppler_hz(dop, acq):
    """Doppler bin → Hz (folds the upper half to negative)."""
    k = (dop + acq.doppler_bins // 2) % acq.doppler_bins - acq.doppler_bins // 2
    return k * acq.doppler_res_hz

delay_chips = phase / acq.spc          # code phase in chips

reset() drains the ring and the coherent accumulator (use it between independent captures).

Code phase tracks the stream offset

The code phase is measured against the frame grid, which is anchored at sample 0. Inserting Δ extra samples of lead-in (silence) before the burst shifts every reported code_phase by Δ mod code_bins — that offset is extra propagation delay. Frame the same burst at a different stream position and the Doppler bin is unchanged but the code phase rotates accordingly.


How many hits to expect

Acquisition fires once per coherent frame while the burst fills the search window. The engine frames on a fixed grid anchored at stream sample 0, so a frame produces full processing gain only when its whole n = doppler_bins·code_bins window lies inside the burst. For a burst of R segments (R·code_bins samples) after L lead-in samples, the count of full-gain frames is

F = (L + R·code_bins) // n  -  ceil(L / n)

On the pure-coherent path each full frame yields one hit. A frame-aligned lead-in (L a multiple of n) gives exactly F hits at one cell; a non-aligned lead-in gives F to F+2 (boundary frames that straddle the burst edge may also fire) and rotates the code phase by L mod code_bins. On the non-coherent path (n_noncoh > 1) a hit arrives once per n_noncoh accumulated frames. A payload that follows the preamble on a different code decorrelates from the matched filter and does not produce burst-cell hits.


Choosing parameters

The minimum you must supply

Construction is physics-only, and only three arguments have no meaningful default. The smallest robust call is:

acq = Acquisition(
    code,                 # the PN replica; sf = len(code) is inferred
    chip_rate=1.023e6,    # waveform chip rate (Hz)
    cn0_dbhz=60,          # your link-budget sensitivity (dB-Hz)
)
assert acq.pd_predicted >= acq.pd   # confirm the search can meet the target

The tiers:

  • Required — no meaningful default: code (the PN replica), chip_rate (the waveform), and cn0_dbhz (the sensitivity; its placeholder default sizes a toy grid, so set it to your real link budget).
  • Set for your front end: spc (samples/chip = sample_rate / chip_rate; default 4) and reps (how many coherent code repetitions you can afford — the coherence ceiling and your latency budget; default 1).
  • Safe defaults — leave unless you have a reason: pfa=1e-3, pd=0.9, noise_mode="mean", doppler_uncertainty=0 (full native span).
  • Weak-signal opt-in: raise max_noncoh above 1 to let auto-config add non-coherent looks once the coherent ceiling (reps) is exhausted.

sf is not a parameter — it is inferred from len(code), so the engine and your replica can never disagree.

Waveform vs. operator knobs

Some inputs describe the transmitted waveform — the receiver must match them, they are not knobs:

  • code — the PN sequence; its length is sf (the spreading factor).
  • chip_rate — the transmitter's chip rate (Hz). With spc it sets the sample rate fs = chip_rate·spc and the Doppler span ±chip_rate/(2·sf).
  • spcsamples per chip (chip-rate oversampling; not samples per symbol — that is sps) = your sample_rate / chip_rate. You only move it by resampling the front end.

The genuine receiver / operator knobs:

Goal Lever
Tighter false-alarm rate smaller pfa (raises threshold)
Hold pd at lower C/N0 larger reps (deeper coherent integration)
More sensitive within a known offset tighter doppler_uncertainty (fewer cells → lower gate)
Robust noise estimate (uncalibrated) noise_mode="median"
Reach below the coherent ceiling max_noncoh > 1 (non-coherent looks)

reps sets the coherent ceiling; the engine uses the smallest depth that meets pd, so raising reps only helps weak signals (a strong one still resolves in a few repetitions).

If you already know the carrier offset lies within ±Δf, pass doppler_uncertainty=Δf (Hz, ≤ the native span). The engine then scans only the Doppler bins inside that band, so the CFAR threshold pays a Bonferroni penalty over fewer cells — a lower gate at the same system pfa, i.e. more sensitivity for free. A value beyond the native span is rejected (MemoryError); to search wider, use the coarse-mix bank below.


The native search spans only ±chip_rate/(2·sf) — one slow-time Nyquist, set by the code period. When the true Doppler exceeds that, tile the wider range with a sequence of coarse Doppler hypotheses: mix the raw stream down by each f_coarse and run Acquisition on the result. The engine's fine FFT then resolves the residual within the native span, and the absolute Doppler is f_coarse + the fine bin.

import numpy as np

chip_rate = 1.0e6
fs = chip_rate * 2                         # spc = 2
coarse = np.arange(-100e3, 100e3, 500.0)   # coarse grid (Hz) — see step rule below
bank = [Acquisition(code, reps=10, spc=2, chip_rate=chip_rate, cn0_dbhz=50,
                    pfa=1e-3, pd=0.9)
        for _ in coarse]                   # one engine per channel (own state)

n0 = 0
for chunk in iq_stream:                                  # any cf32 block
    n = n0 + np.arange(len(chunk))
    for f_coarse, acq in zip(coarse, bank):
        mixed = (chunk * np.exp(-2j * np.pi * f_coarse / fs * n)).astype(np.complex64)
        for dop, phase, *_rest, snr in acq.push(mixed):
            k = (dop + acq.doppler_bins // 2) % acq.doppler_bins \
                - acq.doppler_bins // 2
            doppler_hz = f_coarse + k * acq.doppler_res_hz
            print(f"hit: {doppler_hz:+.0f} Hz, code phase {phase}")
    n0 += len(chunk)
  • Coarse step. Within-segment carrier rotation (residual · code-period cycles) sinc-rolls the code correlation, so keep the residual under ~0.25 cycle for \<1 dB loss. Stepping by the full native window (chip_rate/sf) abuts the tiles but leaves a half-window residual at each edge — 0.5 cycle, ~4 dB down. Halving the step (50% overlap) drops the residual to 0.25 cycle (\<1 dB) at twice the channel count.
  • Relation to the roll method. Mixing the input is the continuous-frequency dual of rolling conj(FFT(code)) by integer bins (each bin = one native window); mixing just lets you choose a finer, half-window step.
  • Cost scales linearly with the number of coarse channels; the inner fine search is unchanged.

Worked example — 1 Mcps, length-1000 code, ±100 kHz

quantity value
chip rate chip_rate 1 Mcps
code length sf 1000 chips
code period sf/chip_rate = 1 ms
repetitions reps 10 → up to 10 ms coherent integration
samples/chip spc 2 → fs = 2 Msps, code_bins = sf·spc = 2000

Fine (native) search — the Doppler figures depend only on the waveform, not spc (it cancels):

  • resolution = chip_rate / (sf · doppler_bins) = 1/(10 ms) = 100 Hz at the full doppler_bins = 10
  • span = ±chip_rate / (2·sf) = ±500 Hz (10 bins)
  • code-phase bins = code_bins = 2000 (half-chip, because spc = 2)

Reaching ±100 kHz — that is 200× the native ±500 Hz window, so sweep a coarse grid (200 kHz total to cover):

  • abutting tiles: step = native window = chip_rate/sf = 1 kHz200 kHz / 1 kHz = 200 channels, but the ±500 Hz edge residual costs ~4 dB.
  • low-loss (50% overlap): step = chip_rate/(2·sf) = 500 Hz200 kHz / 500 Hz = 400 channels, residual ±250 Hz (≤ 0.25 cycle, \<1 dB) — this is the grid in the snippet above.
  • each channel searches a 10 × 2000 (Doppler × code-phase) surface at the native 100 Hz resolution, with full 10 ms coherent gain.

So acquisition is 200–400 fine searches, one per coarse mix — Acquisition runs the inner search and CFAR; your loop sweeps f_coarse. Halving the requirement (e.g. ±50 kHz) halves the channel count; a shorter code (smaller sf) widens the native window and cuts the coarse sweep proportionally.


The DSSS receive chain

Acquisition is the front of a two-stage receiver: acquire, then track. Once it reports a (Doppler bin, code phase), hand the coarse estimate to the Despreader, which closes a DLL + Costas loop to track code phase and carrier and recover the payload bits. Both live in doppler.dsss:

from doppler.dsss import Acquisition, Despreader

See also