MFL saturation and scanning speed limit

Magnetic flux leakage only works when the wall is driven into magnetic saturation. Below saturation the steel is still able to carry more flux, so a wall-loss feature simply diverts flux within the metal instead of forcing it out into the air where the sensors sit, and the leakage signal collapses. Required levels are high — typically around 1.5 T for tank-floor and plate scanners and 1.6 T or more in pipeline in-line inspection — and reaching them is the whole design problem of the magnetiser.

Moving the magnetiser makes it harder. A conductive wall moving through a magnetic field has eddy currents induced in it, and those currents oppose the change, dragging flux backwards relative to the tool and reducing the flux density actually established in the wall under the sensors. The governing group is the magnetic Reynolds number Rm = µ₀·µr·σ·v·t: velocity effects are negligible when it is well below about 0.1, measurable around 0.1 to 1, and severe above 1. Setting Rm = 1 gives a speed limit v = 1/(µ₀·µr·σ·t) which, for carbon steel of 5 MS/m at 8 mm wall and a differential permeability of 5 in saturation, lands near 4 m/s — the same order as the run-speed limits real in-line inspection tools are specified to.

The permeability to use is the differential permeability at the working point, dB/dH, not the ratio B/(µ₀H). Deep in saturation the differential value falls to single figures, which is why saturation both improves the leakage signal and, helpfully, reduces the velocity effect. Below the knee, where the differential permeability is in the hundreds, velocity effects are severe at walking pace.

The effective flux density here is estimated with a first-order lag, B = B₀/(1 + Rm). Treat it as a screening estimate only: real magnetiser design needs finite-element modelling, and the tool vendor's qualified speed range and the qualification report are what govern acceptance. Use this calculation to sanity-check a proposed scanning speed and to understand why a thick wall or a fast run degrades sizing — not to certify a tool.

Rm = µ₀ · µr · σ · v · t          (magnetic Reynolds number)
v_limit = Rm_limit / (µ₀ · µr · σ · t)
B_effective ≈ B₀ / (1 + Rm)        (first-order screening estimate)
v_allowable = (B₀/B_required − 1) / (µ₀ · µr · σ · t)

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Notes:
  • The required flux densities in the application table are typical figures. The tool or scanner specification and its qualification report govern acceptance — enter the specified value to override the table.
  • Use the differential permeability at the working point. Using B/(µ0·H) instead will overstate the permeability by an order of magnitude and give an unrealistically low speed limit.
  • B_effective is a first-order screening estimate; real magnetiser behaviour needs finite-element modelling and validation on reference defects.
  • Velocity effects also shift and skew the signal in time, which degrades depth sizing before it degrades detection.
  • Thicker wall, higher permeability and higher conductivity all reduce the speed limit in direct proportion.
  • Lift-off from coatings, debris or scale reduces the achieved flux density independently of speed and must be accounted for separately.

Reference: General engineering — magnetic Reynolds number scaling of eddy-current velocity effects in MFL. Saturation levels are typical values from in-line inspection and tank-floor scanner practice (API 1163, POF specifications, EEMUA 159); the tool specification governs.

These calculators support — never replace — calculations against the governing code edition and your written procedure. Verify results independently before use.

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