re: the other four ships are clean; automating the slab check failed

Rendered f101/f105/f106/e105 statically -- all coherent, no stray masses, so the
e106 slab was specific. slab_screen.rs tries to automate the check by comparing
each part's min-axis extent to its ship median, but it produces identical flags
with and without the coverage fix at both 4x and 2.5x: it never sees
e106_bdy_03, the part it was built for. The eye used relationship (a mass apart
from the hull), not scale; a containment test is the right analogue and is not
built. Kept for what it does show: f002_bdy_22's 100000-unit tether and
t901_e01_D's mast are legitimate, and capture-verified f101_bdy_01 flags at 6x.

Co-Authored-By: Claude Opus 5 (1M context) <noreply@anthropic.com>
This commit is contained in:
2026-08-12 07:22:43 +00:00
parent f340815db6
commit 85ad540a7e
2 changed files with 100 additions and 0 deletions

View File

@@ -0,0 +1,74 @@
//! Screen every ship family for a part that is wildly out of scale with its
//! siblings — the "slab" signature of a mis-anchored block.
//!
//! Rendering `e106` found such a part (`bdy_03`, 600×1600×998 beside parts of
//! ~250) that coverage, cross-container consistency, the capture oracle and the
//! twin invariant were all blind to. Eyeballing does not scale to 166 containers;
//! this does the same comparison numerically.
//!
//! Usage: slab_screen <resource3d_dir> [factor]
use sylpheed_formats::mesh::Xbg7Model;
use sylpheed_formats::ship::{is_base_part, ship_id_of};
use std::collections::BTreeMap;
fn main() {
let dir = std::env::args().nth(1).expect("resource3d dir");
let factor: f32 = std::env::args().nth(2).and_then(|s| s.parse().ok()).unwrap_or(4.0);
let mut files: Vec<_> = std::fs::read_dir(&dir)
.unwrap()
.flatten()
.map(|e| e.path())
.filter(|p| p.extension().and_then(|s| s.to_str()) == Some("xpr"))
.collect();
files.sort();
let mut flagged = 0usize;
for f in &files {
let Ok(bytes) = std::fs::read(f) else { continue };
let mut by_ship: BTreeMap<String, Vec<(String, f32)>> = BTreeMap::new();
for m in Xbg7Model::anchor_models_cancellable(&bytes, 0.0, &|| false) {
if !is_base_part(&m.name) {
continue;
}
let Some(id) = ship_id_of(&m.name) else { continue };
let (mut lo, mut hi) = ([f32::MAX; 3], [f32::MIN; 3]);
for s in &m.meshes {
for q in &s.positions {
for k in 0..3 {
lo[k] = lo[k].min(q[k]);
hi[k] = hi[k].max(q[k]);
}
}
}
if lo[0] == f32::MAX {
continue;
}
// Compare the part's SMALLEST axis span, not its diagonal. A long
// thin part (an antenna, a 100 000-unit tether on `f002`) is
// legitimately huge in one axis and would swamp a diagonal test; a
// mis-anchored block is bulky in all three, which is what the e106
// slab looked like (600×1600×998 beside siblings of ~250).
let thin = (hi[0] - lo[0]).min(hi[1] - lo[1]).min(hi[2] - lo[2]);
by_ship.entry(id.to_string()).or_default().push((m.name.clone(), thin));
}
for (id, parts) in &by_ship {
if parts.len() < 3 {
continue; // no meaningful median
}
let mut d: Vec<f32> = parts.iter().map(|(_, x)| *x).collect();
d.sort_by(|a, b| a.partial_cmp(b).unwrap());
let median = d[d.len() / 2];
for (name, diag) in parts {
if *diag > median * factor {
flagged += 1;
println!(
"{:<22} {name:<22} min-axis {diag:>8.0} vs ship median {median:>8.0} ({:.1}×)",
f.file_name().unwrap().to_string_lossy(),
diag / median
);
}
}
}
}
println!("{flagged} parts flagged at {factor}× the ship median");
}

View File

@@ -1071,6 +1071,32 @@ Cost: **3** resources disc-wide (6 212 → 6 209); cross-container inconsistency
settled — but it is now consistent across four of the six containers that carry settled — but it is now consistent across four of the six containers that carry
it instead of three.) it instead of three.)
### The other capital ships are clean — and an attempt to automate the slab check failed
`e106` was the first ship rendered, and it had the defect. The other four in the
`Stage_S02` cast — `f101` (ACROPOLIS), `f105`, `f106`, `e105` — were rendered the
same way and all assemble into coherent hulls with no stray masses.
Automating the check did **not** work. `examples/slab_screen.rs` compares each
base part against its ship's median extent (min-axis, so a legitimately long thin
antenna does not swamp the test) and flags outliers. Run against the decoder
**before and after** the coverage fix, at 4× and at 2.5×, it produces the **same
23 / 58 flags either way** — it never sees `e106_bdy_03`, the very part it was
built for. At 600×1600×998 against a ship median of ~250 the slab sits under
3×, and lowering the factor buys noise, not sensitivity.
What the eye actually used was not scale but **relationship**: a blocky mass
sitting apart from the hull silhouette. A containment test — does a part's box
lie within the envelope its neighbours describe? — is the right numeric analogue
and is not built yet.
The screen is kept anyway, because it is honest about what it does see: two
curiosities that are **legitimate**, not defects — `f002_bdy_22`/`_23` span
519 × **100 000** × 519 (a tether/elevator column, consistent in both containers
that carry it) and `t901_e01_D` is 58×59×3013 (a mast). And `f101_bdy_01` flags
at 6× while being **capture-verified exact** in the truth table — a useful
reminder that a bulky hull is not a bug.
### The anchor work has plateaued at 98.7 % — state and what is left ### The anchor work has plateaued at 98.7 % — state and what is left
Four evidence-driven changes took the decoder from 5 480 to **6 212 of 6 294** Four evidence-driven changes took the decoder from 5 480 to **6 212 of 6 294**