PHYSICAL_HELIACAL_VISIBILITY_PHASE4_JONES_MYSTIC_LOWER_BOUNDARY_CHECKPOINT_2026 08 02 - TheDaniel166/moira GitHub Wiki
Physical Heliacal Visibility Phase 4 Jones MYSTIC Lower-Boundary Checkpoint
Historical research only. The proposed next gate in this checkpoint was canceled by the 2026-08-07 Jones/Paranal quarantine decision. Nothing in this document is an active product or release dependency.
Date: 2026-08-02 Status: Jones 2,000 m lower-model-boundary gate closed; source-faithful profile selected for spectral research; spectral grid and runtime model not admitted
Outcome
The Jones/ESO geometry is now resolved without retaining the corrected-v2 observer-bottom approximation as the candidate model.
The source-faithful research profile is:
jones_2000m_ground_observer_2640m_v1
It has:
- a 2.000 km lower atmosphere and ground boundary;
- an explicit 2.640 km observer level in both the atmosphere and O4 files;
- libRadtran
zout 0.64, because numericzoutis height above the surface; - 806.2488072631218 hPa at the 2.000 km surface, which preserves 744 hPa at the 2.640 km observer after the bound AFGL pressure scaling;
- 259.19991781804873 DU above the 2.000 km surface, which preserves the same
4.914335e11 cm-3observer-level ozone number density as the 258 DU observer-bottom control; and - the Jones exponential aerosol column down to 2.000 km while preserving every corrected-v2 layer boundary and optical property above 2.640 km.
The selection is controlled by the source semantics (sm_h = 2.64 and
sm_hmin = 2.0), not by numerical closeness to the observer-bottom control.
Frozen Comparison
The experiment compared two profiles at 550 nm:
| Profile | Surface | Observer | zout |
Observer pressure | Role |
|---|---|---|---|---|---|
observer_bottom_control_v2 |
2.640 km | 2.640 km | 0.00 km | 744 hPa | Exact corrected-v2 holdout regression control |
jones_2000m_ground_observer_2640m_v1 |
2.000 km | 2.640 km | 0.64 km | 744 hPa | Source-faithful lower-boundary candidate |
The candidate aerosol receipt is:
- observer-to-infinite-top AOD550 normalization:
0.0294; - observer-to-20 km AOD550:
0.02939998466958803; - 2 km-to-20 km AOD550:
0.05011536771007698; and - restored below-observer AOD550:
0.020715383040488946.
The candidate adds boundaries at 2.000, 2.250, 2.500, and 2.640 km, then uses every corrected-v2 boundary above 2.640 km unchanged. Physical aerosol files remain bound to inclusive lower boundaries. The 20-120 km region remains an explicit null gap.
Execution
The final matrix used the three corrected-v2 reserved holdout geometries for both profiles, plus one exact candidate repeat:
- seven serial MYSTIC runs;
- 1,000,000 photons per run;
- fixed seed
271828183; - fully spherical one-dimensional MYSTIC; and
- a frozen maximum relative Monte Carlo standard error of
0.005.
The control reproduced the committed corrected-v2 holdout radiance and
standard-error values exactly. The candidate repeat was byte-identical for
mc.rad.spc, mc.rad.std.spc, mc3.rad, mc3.rad.std, and randomseed.
MYSTIC uses its internal altitude-level index in the altitude-plane output
filename. The source-bound surface control therefore emits mc0.*, while the
2.640 km candidate observer emits mc3.*. This is an output identity detail,
not a change in the evaluated altitude.
Measurements
| Case | Control radiance | Candidate radiance | Candidate/control | Relative change | Candidate minus control |
|---|---|---|---|---|---|
| Low-altitude oblique | 3.09175e-08 |
3.26044e-08 |
1.0545613326 |
+5.4561% |
-0.05768 mag |
| Interior cross-axis | 7.88475e-09 |
8.07704e-09 |
1.0243875836 |
+2.4388% |
-0.02616 mag |
| Phase-boundary waxing | 9.54726e-09 |
9.60728e-09 |
1.0062866205 |
+0.6287% |
-0.00680 mag |
The maximum relative Monte Carlo standard error was
0.002984007960629856, below the frozen 0.005 ceiling.
These differences are measurements only. No candidate/control difference threshold was prefrozen, and the numerical difference was not used to choose the profile.
Independent Validation and Reproducibility
The independent validator does not import the new lower-boundary builder. It:
- verifies every corrected-v2 lineage receipt;
- reopens the exact ESO and libRadtran archives and verifies the governing configuration and source members;
- independently reconstructs the 2.000 and 2.640 km atmosphere and O4 rows;
- independently reconstructs every candidate aerosol layer and Legendre representation;
- reparses every MYSTIC input and output;
- verifies the exact corrected-v2 control regression;
- recomputes all paired diagnostics and checks; and
- enforces the closed runtime, network, redistribution, and admission boundaries.
Two final artifacts were built serially from the same frozen contract. Their entire directory trees were byte-for-byte identical:
- manifest: 71,981 bytes, SHA-256
4223b52c001f5f6e427130bdc4523c1031f617e904987c823a3cd18883911736; - compact checkpoint: 14,529 bytes, SHA-256
6c3ef3b750ff235719a3b9014e05bb5a5a7f6c022decc2f83a0f4f85f4906b31.
The atmosphere-only probe initially left a time-varying, scientifically unused
randomseed file. The final builder removes that incidental file before
receipting the probe. The two final full-tree matches demonstrate that it no
longer contaminates reproducibility.
Pre-Authority Attempts
Five pre-authority attempts are retained in the frozen specification history:
- a profile probe rejected before radiance execution because its source declaration was incomplete;
- a candidate inventory gate that discovered
mc3.*instead ofmc0.*at nonzerozout; - an inventory diagnostic that confirmed that profile-specific behavior;
- a scientifically successful artifact superseded by zero-byte-receipt and probe-inventory validator hardening; and
- an independently validated artifact superseded because the incidental
probe
randomseedreceipt was time varying.
None is authoritative. The first three were atomically discarded; the two retained external artifacts are explicitly superseded by the identical final artifacts.
Boundary
This checkpoint does not:
- admit a spectral wavelength grid or interpolation surface;
- admit a runtime Jones model or production data pack;
- change Moira engine calculations or public APIs;
- add a runtime, network, or automatic-download dependency;
- redistribute ESO or libRadtran source bytes; or
- modify the legacy
krisciunas_schaefer_1991path.
Repository Receipts
scripts/visibility_reference_lab/phase4_jones_mystic_lower_boundary_spec.jsonscripts/build_visibility_phase4_jones_mystic_lower_boundary.pyscripts/validate_visibility_phase4_jones_mystic_lower_boundary.pytests/artifacts/visibility_reference_lab/phase4_jones_mystic_lower_boundary_checkpoint_2026-08-02.jsontests/unit/test_visibility_phase4_jones_mystic_lower_boundary.py
The full generated artifacts remain external because they contain derived evidence built from caller-supplied GPL/source inputs. The repository stores only the compact checksummed receipt.
Next Gate
The next authorized work is:
design_jones_2000m_ground_spectral_admission_matrix
That design must freeze its wavelength grid, interpolation policy, numerical thresholds, and untouched spectral holdouts before executing admission holdouts. Phase 4 remains open, and no runtime implementation is authorized by this checkpoint.