Files
scanengine-3/scan_format.md
Thomas Ales ef8c0feb91 Expose burst acquisition in the app; refresh scan_format acquisition docs
Wires the burst_mode flag through QtScanController to ScanEngine and adds a
checkbox to the scan panel. The setting persists via ScanDefaults like the
other scan fields, defaulting to off — per-row acquisition stays the default
path until burst mode has run on the rig and the gate-off preflight has
settled which TRIGOUT value idles the pin low.

scan_format.md — the acquisition settings table had drifted from the code it
claimed to describe: it attributed the settings to sc3_aui_app.py (they moved
to core/scope_sras.py in the Phase 2 extraction), listed a 1.24 V trigger
level and 0 % offset where the code sets 0.500 V and HORizontal:POSition 30,
and did not mention the logic-AND scan trigger at all. Corrected, pointed at
the module that actually owns them, and noted that none of it affects byte
layout — only where the acoustic packet lands inside a frame.

Added an acquisition-paths section: the two paths write byte-identical files
and the choice is a runtime flag that is not recorded in the file, so a
reader never needs to care which produced it. Documents where row boundaries
come from in a burst and that either path squares rows up to n_frames.

Co-Authored-By: Claude Opus 5 <noreply@anthropic.com>
2026-09-02 12:18:23 -05:00

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# SRAS Scan Binary Format — Version 6
Each `.sras` file contains **one complete scan**: all GR rotation angles and all
Y rows. Files are named `{prefix}.sras`.
Starting in v6, each angle only scans the **bounding box of the nominal ROI
rotated by that specific angle** — not the worst case across all angles — so
`x_start`, `x_delta` (and therefore `n_frames`, the points/row count) and
`n_rows` all vary per angle. A 0°/180° scan of a wide, short ROI needs far
fewer rows than a 45° scan of the same ROI, and the file format reflects that
instead of forcing every angle to the largest bounding box.
---
## File Layout
```
[Global Header — 49 bytes]
[Angle Table — n_angles × 4 bytes (float32 per angle, degrees)]
[Per-Angle Geometry Table— n_angles × 14 bytes (x_start f32, x_delta f32, n_frames u32, n_rows u16)]
[Row Table (ragged) — sum(n_rows) × 4 bytes (float32 per row, angle-major)]
[Preamble Blocks — n_channels × (uint16 length + UTF-8 WFMOutpre string)]
[Background Block — uint32 n_bg_samples + n_bg_samples × int8 bytes]
[Waveform Data (ragged) — per angle: n_rows[a] × n_channels × n_frames[a] × samples_per_frame × bps bytes]
```
All multi-byte integers and floats use **big-endian** byte order
(`>` in Python's `struct` module).
---
## Global Header (49 bytes)
| Offset | Size | Type | Field | Description |
|--------|------|-----------|--------------------|--------------------------------------------------|
| 0 | 4 | `4s` | `magic` | Always `SRAS` (0x53 0x52 0x41 0x53) |
| 4 | 1 | `uint8` | `version` | Format version — `6` |
| 5 | 2 | `uint16` | `n_angles` | Number of GR rotation angles |
| 7 | 4 | `float32` | `x_start_nominal` | Nominal (pre-rotation) X scan start, mm |
| 11 | 4 | `float32` | `y_start_nominal` | Nominal (pre-rotation) Y scan start, mm |
| 15 | 4 | `float32` | `x_delta_nominal` | Nominal (pre-rotation) X scan width, mm |
| 19 | 4 | `float32` | `y_delta_nominal` | Nominal (pre-rotation) Y scan height, mm |
| 23 | 4 | `float32` | `row_spacing_mm` | Y spacing between rows, mm |
| 27 | 4 | `float32` | `velocity_mm_s` | Stage scan velocity in mm/s |
| 31 | 4 | `float32` | `laser_freq_hz` | Laser repetition rate in Hz |
| 35 | 4 | `uint32` | `samples_per_frame`| Time samples per waveform |
| 39 | 8 | `float64` | `sample_rate_hz` | Oscilloscope sample rate in Hz (e.g. 6.25e9) |
| 47 | 1 | `uint8` | `bytes_per_sample` | Bytes per ADC sample: `1` = int8, `2` = int16 |
| 48 | 1 | `uint8` | `n_channels` | Number of channels recorded (currently `3`) |
**Total header size:** 49 bytes — verified:
`struct.calcsize(">4sBHfffffffIdBB") == 49`.
The `*_nominal` fields describe the ROI as originally entered on the New Scan
page (XS/YS/XD/YD), **before** per-angle bounding-box expansion. They are for
reference/reconstruction only — the actual per-angle scan geometry used for
acquisition is in the Per-Angle Geometry Table below.
---
## Angle Table
Immediately after the header: **n_angles** big-endian float32 values, one per
GR angle (degrees, signed; magnitude 0–180, sign gives physical rotation
direction — negative for the current CW-rotating GR stage).
```
angle[0], angle[1], …, angle[n_angles - 1]
```
---
## Per-Angle Geometry Table
Immediately after the angle table: **n_angles** fixed-size records, one per
angle (same order as the angle table), each 14 bytes:
| Size | Type | Field | Description |
|------|-----------|------------|-------------------------------------------------------|
| 4 | `float32` | `x_start` | X scan start for this angle's bounding box, mm |
| 4 | `float32` | `x_delta` | X scan width for this angle's bounding box, mm |
| 4 | `uint32` | `n_frames` | A-scans per row for this angle (FastFrame count) |
| 2 | `uint16` | `n_rows` | Number of Y rows scanned for this angle |
Format string per record: `">ffIH"`.
---
## Row Table (ragged)
Immediately after the per-angle geometry table: for each angle in order,
that angle's `n_rows` big-endian float32 Y positions (mm), concatenated with
no padding between angles.
```
# angle 0's rows, then angle 1's rows, …
y_mm[0][0], …, y_mm[0][n_rows[0]-1], y_mm[1][0], …, y_mm[n_angles-1][n_rows[-1]-1]
```
Row-table boundaries for angle *a* are derived from the per-angle geometry
table: `sum(n_rows[0:a])` gives the starting index into the flattened array.
---
## Preamble Blocks
Immediately after the row table: **n_channels** length-prefixed UTF-8 strings,
one per channel in `SCAN_CHANNELS` order (CH1, CH3, CH4). Each block is:
```
uint16 length — byte length of the following UTF-8 string
bytes preamble — WFMOutpre response string from the oscilloscope
```
The preamble captures per-channel scaling constants (YMULT, YOFF, YZERO) needed
to convert raw ADC values to volts.
---
## Background Block
Immediately after the preamble blocks: a single CH1 waveform captured with the
**Helios (generation) laser enabled** and the **Genesis (detection) laser
disabled**. This provides a noise/background reference for subtraction during
post-processing.
```
uint32 n_bg_samples — number of samples in the background waveform
int8[] bg_data — raw ADC samples (same encoding as waveform data)
```
`n_bg_samples` equals `samples_per_frame` under normal acquisition settings.
---
## Waveform Data (ragged)
Immediately after the background block. Data is stored in **angle-major,
row-minor** order, but unlike earlier versions each angle contributes a
different number of rows (`n_rows[a]`) and a different number of frames per
row (`n_frames[a]`), both taken from that angle's Per-Angle Geometry Table
entry. Within each row, channels are interleaved in ascending channel-index
order, with each channel's FastFrame data written in frame order.
```
for angle a in 0 … n_angles-1:
for row in 0 … n_rows[a]-1:
for channel in [CH1, CH3, CH4]: # 3 channels, fixed order
for frame in 0 … n_frames[a]-1:
samples[0 … samples_per_frame-1] # bps bytes each
```
Each sample is a raw signed ADC value. With `bytes_per_sample = 1` this is
**int8** (−128 … +127). With `bytes_per_sample = 2` this is **big-endian
int16**.
Total data size:
```
sum over angles a of: n_rows[a] × 3 × n_frames[a] × samples_per_frame × bytes_per_sample
```
> **Incomplete files:** If a scan is aborted the file is closed immediately and
> the data block will be shorter than the expected size. Readers should
> reconstruct the expected per-angle byte offsets from the Per-Angle Geometry
> Table and check `file_size` against the running total before reshaping —
> a fixed `(n_angles, n_rows, ...)` reshape (as in pre-v6 readers) will not
> work since row/frame counts are no longer uniform across angles.
---
## Spatial Mapping
The *k*-th waveform (frame) in a row corresponds to the *k*-th laser pulse that
hit the sample. For a row belonging to angle *a*, the physical X position of
that pulse is:
```
x_k = x_start[a] + k * (velocity_mm_s / laser_freq_hz)
```
using that angle's `x_start` from the Per-Angle Geometry Table (not
`x_start_nominal`).
---
## Acquisition Settings (fixed by core/scope_sras.py)
| Parameter | Value |
|-----------------------|------------------------------------------|
| Setup trigger | CH2, rising edge, 0.500 V (`TRIG_LEVEL_V`) |
| Scan trigger | Logic AND, CH2 HIGH ∧ CH3 HIGH, 0.500 V |
| Horizontal position | 30 (`HORizontal:POSition`) |
| Sample rate | 6.25 GS/s (160 ps/sample) |
| Transfer format | `DATa:ENCdg RIBinary`, `DATa:WIDth 1` |
| Channels recorded | CH1, CH3, CH4 |
| Stage X velocity | 100 mm/s |
| Stage X acceleration | 1500 mm/s² |
| Stage X trigger out | Logic-high at max velocity (`TRIGOUT_MAXV`) |
| Acquisition mode | FastFrame, Normal trigger |
None of these are stored in the file, so they do not affect byte layout — but
they do set where the acoustic packet lands inside each frame. Read them from
`core/scope_sras.py`; earlier revisions of this table drifted from the code.
---
## Acquisition Paths
Two acquisition strategies write **byte-identical** files; the choice is a
runtime flag (`ScanEngine(burst_mode=…)`, exposed as a checkbox in the app) and
is not recorded in the file.
| | Per-row (default) | Burst |
|---|---|---|
| FastFrame acquisitions | one per row | one per `floor(max_frames / n_frames)` rows |
| Curve transfers | one per channel per row | one per channel per burst |
| Stage X trigger out | armed for the whole scan | armed per acquiring pass, dropped for the flyback |
Burst mode runs a single acquisition across several rows, so the return move
must not trigger: the trigger output is dropped before each flyback and
re-armed for each acquiring pass. Row boundaries inside the burst come from
`ACQuire:NUMFRAMESACQuired?` sampled after each pass — the burst itself carries
no row markers. See `core/scope_burst.py`.
Either path squares each row up to the declared `n_frames` (zero-padding a
short row, dropping the tail of a long one), because the format has no per-row
length field and a mismatch would shift every later row.
---
## Version History
| Version | Change |
|---------|--------|
| 1 | One file per row; header included `angle_idx`, `row_idx`, `angle_deg`, `y_mm`. |
| 2 | One file per scan; global header with `n_angles`/`n_rows`; separate angle and row tables; three channels (CH1, CH3, CH4) per row. |
| 3 | Added preamble blocks (WFMOutpre strings) after the row table, one length-prefixed UTF-8 block per channel. |
| 4 | Added background waveform block (CH1, Helios ON / Genesis OFF) after the preamble blocks; stored as `uint32` sample count followed by raw `int8` ADC bytes. |
| 5 | (skipped) |
| 6 | Each angle now scans only the bounding box of the nominal ROI rotated by that angle instead of the AABB-expanded worst case across all angles. Header no longer carries a single global `x_start`/`x_delta`/`n_rows` — replaced with `*_nominal` reference fields plus a new Per-Angle Geometry Table (`x_start`, `x_delta`, `n_frames`, `n_rows` per angle) and a ragged Row Table / Waveform Data block sized per angle. **Not compatible with v4 readers** (e.g. `sras_viewer.py`, which has not yet been updated for v6). |