Rotation — where it appears
Named by 4 essays across one field — each of them below, with the objects they name alongside it.
The nearest orthogonal matrix
Every field that has to clean up a drifted rotation reaches for QR, and QR does not answer the question. The nearest orthogonal matrix is the orthogonal factor of the polar decomposition — nearer by about a tenth, and, more to the point, the same matrix whatever order the columns were written in. QR's answer changes completely.
A rotation that comes back mirrored
Align twenty noisy points and the nearest orthogonal matrix to the answer is a reflection in 7.7 per cent of trials at noise three times the set's thickness and a third of them at ten — at thicknesses of 10⁻², 10⁻³ and 10⁻⁴ alike. The determinant fix is never a small correction. It moves the answer by exactly 2, it costs exactly 4σ₃ of residual, and it leaves the rotation's error at half the noise however thin the set becomes.
Five precise points are five points
Weighting each sighting by its reliability is the standard form of an attitude or registration fit, and it changes how often the nearest orthogonal matrix comes back as a mirror. Measured, the rate is a function of two numbers: the weighted noise over thickness, and the effective count (Σw)²/Σw². Five points with a tenth of the noise, weighted by 1/σ², carry the information of 515 equal points and mirror like five — 7.9 per cent at a noise ratio where twenty points mirror 1.8 and five mirror 9.5. The √m the earlier measurement left unchecked is right, and it counts what carries the thin direction.
A mirror decided in the thin directions
In n dimensions the nearest orthogonal matrix to a noisy alignment is still sometimes a reflection, and the rate at which it is does not depend on n. Three, five and ten dimensions with one thin direction mirror alike; two thin directions mirror like each other in five dimensions and in ten. The rate is the chance that a k × k matrix built from the k thin directions has a negative determinant — 21.7 per cent at a noise ratio of 0.7 for k = 2, measured at 23.0 — and it is well above k independent coin flips. With two or more thin directions the determinant correction still fires, and it no longer rescues the rotation: the answer is eleven noise-widths off whether or not it was mirrored.
Named alongside it
The objects these essays reach for when they reach for this one.
OrthogonalityPolar decompositionDeterminantSingular value decompositionReflectionSensitivityCondition numberFrobenius normGram–SchmidtHouseholderInvarianceQR factorisation