MathWorks Shack-Hartmann Modeling
Subaperture spot migration, wavefront slope and wavefront reconstruction steps
Verification date: 2026-10-24
View original public information →Facing the lens wavefront tooling, using the sub-aperture light spot and wavefront as the observation route, it is intended to output wavefront difference candidates and effective apertures. The page is for project evaluation and does not mean that the development has been completed or has been accepted on site.
Microlens array, reference plane wave, corresponding sub-aperture number and focal length calibration. Microlens array, reference spot field and wavefront calibration components
Microlens array, reference plane wave, corresponding sub-aperture number and focal length calibration
Existing algorithmic evidence:A101–A112 only complete analytical synthesis spot and controlled geometry verification; see laser_spot_benchmark.json
Light point extraction can only be used as an observation front-end, and core capabilities such as three-dimensional reconstruction, closed-loop control, wavefront or physical quantity inversion need to be developed and verified separately.
Gaps in this scenario:Slope conversion, wavefront integration/Zernike fitting and defect reconstruction need to be added; the centroid itself does not output the wavefront. Transmission/reflection configurations need to be calibrated separately. The existing code provides center extraction, and the wavefront slope and reconstruction core need to be added.
Route-level gaps:Need to add slope conversion, wavefront integration/Zernike fitting and defect reconstruction; the centroid itself does not output the wavefront
"New cores required" only describes the relative development volume and does not constitute a commitment to accuracy, tempo, stability or delivery time.
Use an independent interferometer or known aberration phase element to verify slope, reconstruction residuals, and dynamic range. Comparison with known aberration elements and interferometers
| Acceptance items | Evidence required for project confirmation | Current status |
|---|---|---|
| Inputs and samples | Real device original frames, normal/abnormal samples, exposure and light path conditions, sample grouping and set aside | Not provided, waiting for project input |
| Magnitude and Error | Independent reference value, calibration record, error statistical caliber and mutual confirmation threshold | Not verified |
| Exceptions and boundaries | Anticipated handling of missed detections, false detections, overexposure, occlusion, reflection, out-of-view and communication abnormalities | To be defined |
| System integration | Interface, time synchronization, deployment platform, tempo, log, version and continuous running record | Not integrated |
The source supports measurement principles or similar applications; the module combination, device and acceptance method in this scenario are engineering derivation, and product verification has not been completed.
Subaperture spot migration, wavefront slope and wavefront reconstruction steps
Verification date: 2026-10-24
View original public information →Light point correlation, missing points, and wavefront reconstruction constraints
Verification date: 2026-10-24
View original public information →Comparison of aberrations before and after lens adjustment
Please describe the task object, original picture or video, target indicators, device platform, interface and sample situation.
Phone: 13910119357