A student-friendly guide — from fundamental wave physics to inspection methods
Before diving into ultrasound, it is essential to understand what makes sound fundamentally different from light and radio waves. The animations below contrast a longitudinal pressure wave (sound / elastic wave) with an electromagnetic wave (light, radio, X-ray) — two completely different physical phenomena.
Blue bands = compression Orange bands = rarefaction. Medium particles push & pull along the propagation direction — requires a medium.
Red = Electric field (E) Blue = Magnetic field (B). E ⊥ B ⊥ propagation — no medium needed; travels in vacuum at c.
The animations show how the two waves look. Three practical consequences follow from the speed hierarchy: refraction angles at every material interface are fixed by speed ratios (Snell's law); water-path timing in immersion rigs must account for the ~4× speed jump between water and steel; and depth-sizing accuracy is bounded directly by how well the wave speed in the test piece is known.
The physical differences between sound and EM waves lead to very different application domains. Both are essential tools in science and engineering — just for completely different jobs.
In a solid, atoms are linked by elastic bonds. A disturbance can move through that lattice in several ways, classified by how the particles move relative to the wave direction. Each isometric sample below is a small block of material with particles tracking their true 3-D motion as the wave passes through it, left to right.
Particles move parallel to the direction of travel, alternately bunching together and spreading apart. Alternating compression and rarefaction pass through the volume — the same push-pull motion as a sound wave in air. L-waves travel in solids, liquids, and gases, and are the fastest elastic wave in a solid.
Particles move perpendicular to propagation. SH motion is horizontal, side to side, out of the vertical plane of travel — motion that is only visible once the sample is viewed in three dimensions. SV motion is vertical, in that same plane. Both require shear stiffness, so they propagate in solids but not in fluids.
Particles trace ellipses near a free surface. Coupled longitudinal and vertical motion produces a rolling, retrograde elliptical path that is strongest at the surface and decays rapidly with depth — visible here as the deeper rows of particles barely moving at all.
Consider a longitudinal wave traveling through water toward a solid. Water cannot support shear stress, so the incident and reflected waves in the water are always longitudinal. Changing the incident angle controls which wave modes receive energy inside — or along the surface of — the solid.
The beam strikes perpendicular to the interface. Symmetry is preserved, so no shear component is created — the interface only ever sees motion along the beam axis. Result: reflected L in the water + transmitted L in the solid. No shear-wave generation.
An angled beam breaks that symmetry. Each mode refracts at its own Snell-law angle, set by its own wave speed — mode conversion splits one incoming beam into two outgoing ones in the solid. Result: reflected L in the water; refracted L and SV in the solid, bent by different amounts.
Tune the incident angle so the refracted L wave would travel exactly along the interface — that critical condition launches a Rayleigh wave instead of a bulk beam. Result: a surface wave riding the solid's free surface, its elliptical motion decaying within about one wavelength of depth.
When an ultrasonic wave strikes a planar interface at oblique incidence, it simultaneously produces a refracted P-wave and a mode-converted S-wave in the second medium. Both obey Snell's law independently, each governed by its own wave speed:
Because cL2 ≠ cS2, the two transmitted beams diverge in direction. In steel (cL = 5900 m/s, cS = 3200 m/s) the refracted P bends nearly twice as far from the normal as the mode-converted S.
Immersion UT at θi = 20° — between the two critical angles for water–steel. The refracted P-wave undergoes total internal reflection, so only the mode-converted S (≈ 48°) propagates into the steel.
As θi increases, two thresholds mark where a transmitted wave reaches 90° (grazes the interface) and undergoes total internal reflection (TIR):
Angle-beam probes are designed to operate with the wedge angle strictly between θc1 and θc2, ensuring a single-mode (pure shear) beam enters the test piece.
| Interface | cL1 (m/s) | cL2 / cS2 (m/s) | θc1 | θc2 |
|---|---|---|---|---|
| Water → Steel | 1480 | 5900 / 3200 | 14.5° | 27.5° |
| Water → Aluminum | 1480 | 6320 / 3130 | 13.5° | 28.2° |
| Perspex → Steel | 2730 | 5900 / 3200 | 27.6° | 58.5° |
| Perspex → Aluminum | 2730 | 6320 / 3130 | 25.6° | 60.7° |
Acoustic impedance Z characterises how a material resists the propagation of pressure waves. At any interface between two media with different Z values, the wave splits into a reflected wave and a transmitted wave — the greater the mismatch, the more energy is reflected and the less penetrates. This principle governs everything from couplant selection to echo amplitude interpretation.
Normal incidence: the reflected ray is offset here only for visual clarity — it physically returns straight back along the incident path. The greater the impedance mismatch |Z₂ − Z₁|, the larger R and the smaller T.
For a wave striking an interface at normal incidence, the intensity reflection and transmission coefficients are:
Note that R here is the intensity (power) reflection coefficient. The pressure-amplitude reflection coefficient is the signed quantity r = (Z2 − Z1)/(Z2 + Z1), which is negative when Z2 < Z1 (a “soft” reflection with phase inversion) — a sign change visible in RF-mode A-scans and exploited in half-wave rectification to distinguish crack faces from back-wall echoes.
| Material | ρ (kg/m³) | cL (m/s) | Z (MRayl) | NDE relevance |
|---|---|---|---|---|
| Steel (low-alloy) | 7 800 | 5 900 | 46.0 | Primary inspection target |
| Aluminium | 2 700 | 6 320 | 17.1 | Aerospace structures, AM Ti parts |
| Titanium | 4 510 | 6 100 | 27.5 | Additive-manufactured components |
| CFRP (through-thickness) | ~1 600 | ~2 800 | ~4.5 | Low Z → large mismatch with steel tooling |
| Water (20 °C) | 998 | 1 480 | 1.48 | Immersion couplant |
| Ultrasonic gel | ~1 000 | ~1 500 | ~1.5 | Contact couplant — closely matches water |
| Air | 1.2 | 343 | 0.0004 | Near-total reflection at any solid–air gap |
In immersion UT, a transducer fires through a water path into an aluminium plate. At the water–aluminium entry surface (Z1 = 1.48 MRayl, Z2 = 17.1 MRayl):
Only 29 % of the incident intensity enters the part. On exit through the back wall (aluminium–water), the same mismatch applies — roughly 29 % of the remaining intensity exits into the water where it produces the back-wall echo. This 71 % entry-surface reflection is why the initial-pulse echo is so dominant in an immersion A-scan. Any indication amplitude must be compared against the back-wall echo, not the entry surface, to account for this transmission loss.
A thin liquid couplant eliminates the transducer–air–solid interface (R ≈ 100 % for steel–air) by substituting a medium whose impedance bridges the gap. Water gel (Z ≈ 1.5 MRayl) is not perfectly matched to steel (Z = 46 MRayl), but it reduces the air-gap reflection from ~100 % to ~71 % — a ~12 dB improvement in transmitted amplitude. Specialised impedance-matching layers bonded to the transducer face can increase transmission further by introducing an intermediate Z layer of thickness λ/4, acting as an acoustic transformer.
Ultrasound is sound with a frequency above the upper limit of human hearing — roughly 20 kHz. It obeys exactly the same wave physics as the audible sound covered in Section 1; only the frequency changes. Because higher frequency means shorter wavelength (λ = c / f), ultrasound can resolve much finer detail than audible sound — which is exactly why it is useful for imaging and flaw detection rather than just hearing.
Acoustic waves span the full frequency range from infrasound, through audible sound, to ultrasound. Inspection methods occupy several parts of this spectrum; conventional industrial ultrasonic NDE most often uses 0.1 MHz to 50 MHz, trading penetration at low frequency against resolution at high frequency.
| Frequency Range | Wavelength in Steel | Best for |
|---|---|---|
| 0.1 – 0.5 MHz | 12 – 59 mm | Coarse-grained castings, concrete, rough surfaces; high penetration |
| 1 – 5 MHz | 1.2 – 5.9 mm | Most common NDE range — good balance of penetration and resolution |
| 5 – 15 MHz | 0.4 – 1.2 mm | Small defects, thin sections, fine-grained metals, composites |
| 15 – 50 MHz | 0.12 – 0.4 mm | High-resolution imaging, microelectronics, thin coatings |
In pulse-echo UT, a transducer fires a short burst of ultrasound into the part and listens for returning echoes. The time it takes each echo to arrive directly encodes depth — flaws appear as early echoes, the back wall gives total thickness. Everything flows from d = c × t / 2.
Cyan arcs = transmitted pulse & back-wall echo. Red arcs = flaw echo reflected from the void.
IP = initial pulse • Flaw Echo = void reflection • BW = back-wall echo. Trace builds as pulse travels.
Ultrasound for inspection is generated by a transducer — a device that converts electrical energy into mechanical vibration (and back again). The key mechanism is the piezoelectric effect.
Certain crystals (quartz, PZT ceramic) have a special property: squeeze them and they produce a voltage; apply a voltage and they squeeze themselves. When a short electrical pulse is applied to a piezoelectric element, it vibrates rapidly — generating a burst of ultrasound. When a returning echo hits the element, it produces a tiny voltage that the instrument records. The same element transmits and receives.
In most NDE setups, the transducer fires a short burst of ultrasound and then listens for echoes. Reflections return from the front surface (initial pulse / entry echo), any internal flaws (defect echo), and the back wall. Time-of-flight is converted to depth via d = c × t / 2 — dividing by 2 because the wave travels the path twice (down and back).
Every transducer is characterised by its centre frequency fc and fractional −6 dB bandwidth (BW / fc). Because the transmitted burst is finite, pulse duration sets a hard limit on axial (depth) resolution — the minimum separation at which two reflectors produce distinct echoes:
Wide bandwidth (high backing impedance → short ring-down) gives fine axial resolution. Low damping lets the element ring for many cycles, merging echoes from closely spaced interfaces. The diagram below contrasts the two regimes for two reflectors at identical depth separation:
A laser powder-bed fusion (LPBF) Ti-6Al-4V build, 30 mm thick, must be screened for lack-of-fusion (LoF) voids in the build direction. Target flaw size: 0.1–0.5 mm axial extent. Material properties: cL = 6 100 m/s, attenuation α ≈ 0.5 dB/(mm · MHz) (columnar prior-β grain structure).
| Parameter | 10 MHz probe | 5 MHz probe |
|---|---|---|
| Wavelength λ = c/f | 0.61 mm | 1.22 mm |
| Near field N (D = 6 mm) | ~15 mm | ~7.4 mm |
| Two-way attenuation at 30 mm | ~30 dB | ~15 dB |
| Min. resolvable flaw size (∼λ/2) | ~0.3 mm ← meets target | ~0.6 mm — misses <0.5 mm LoF |
The 10 MHz probe meets the resolution target but accumulates ~30 dB two-way attenuation across the 30 mm build — approaching the dynamic range limit of most pulser-receivers and leaving little margin for a DAC correction. The practical solution is a 10 MHz focused immersion probe (focal depth F = 20 mm, water-path corrected via WP = F − d × cw/cs) with TCG applied to restore uniform sensitivity across depth. Sensitivity is validated against a reference coupon of the same build orientation containing calibrated 0.5 mm flat-bottom holes at 10, 20, and 30 mm depths.
Contact, immersion, EMAT, phased array, dual-element — designs, selection guides, and links to manufacturers.
The A-scan (Amplitude scan) is the most fundamental display in ultrasonic testing. It shows amplitude vs. time for a single transducer position — essentially what the transducer "hears" after it fires a pulse.
The time axis is converted to depth using d = c × t / 2 (round-trip). Three key features appear:
A-scans can be displayed as RF (raw bipolar), full rectified (both halves folded positive), or envelope (smooth amplitude via Hilbert transform). Most field instruments default to rectified RF.
A B-scan (Brightness scan) builds a 2D cross-section image by moving the transducer linearly across the surface and stacking A-scans side by side. The horizontal axis is scan position; the vertical axis is depth.
B-scans are excellent for showing flaw depth and through-thickness extent. They are commonly used for corrosion mapping, weld root inspection, and in-service thickness profiling. Each column of the B-scan image is one rectified or envelope-detected A-scan, with the time axis converted to depth and mapped to pixel brightness. A strong echo (high amplitude) produces a bright vertical stripe at that scan position.
Two independent length scales govern what a B-scan can resolve:
Here BW is the −6 dB bandwidth of the pulse, τp is the pulse duration, and the lateral expression is the focal spot diameter for a focused transducer at depth F (same as for C-scan). Axial resolution is governed by pulse length — higher bandwidth (shorter pulse, higher damping on the pulser) gives finer depth discrimination. Lateral resolution degrades away from focus, because the beam expands in the far field at half-angle sin θ ≈ 0.514λ/D. In unfocused contact scanning, two vertical flaws separated by less than the −6 dB beam diameter at their depth will appear as a single blurred column in the B-scan — an artefact misread as a single large reflector.
A common application is in-service corrosion mapping of oil and gas pipelines. A 5 MHz, 25 mm diameter contact transducer is scanned longitudinally along a steel pipe section (nominal wall thickness T = 12 mm, cL = 5 900 m/s, λ = 1.18 mm). The B-scan is recorded at a 0.5 mm index step.
| Parameter | Value | Physical meaning |
|---|---|---|
| Axial resolution δz | ≈ 0.6 mm | Distinguishes FW from BW echoes in this 12 mm wall (TOF difference = 4.1 µs ≫ pulse length ≈ 0.2 µs — no issue here; limit matters for thin-wall < 3 mm) |
| Lateral resolution δx | ≈ 10–15 mm at 12 mm depth | Unfocused beam in the far field (N = D²f/4c = 25² × 5×10⁶ / (4 × 5900) ≈ 132 mm; 12 mm is well in near field — beam stays collimated ≈ 25 mm diameter) |
| What the B-scan shows | BW echo arrival time vs. scan position | Local BW arrival early → wall thinned by corrosion. A 3 mm pit appears as a region where the BW echo rises from 4.1 µs (12 mm) to 3.1 µs (9 mm), visible as an upward bulge in the BW line |
| Minimum detectable wall loss | ≈ δz/2 ≈ 0.3 mm | Set by the axial resolution (pulse bandwidth); confirmed on a step-machined reference block |
The primary output from this scan is a TOF B-scan: the back-wall echo arrival time at each scan position is converted to remaining wall thickness via \(t_\text{BW} = 2d/c\). Regions of corrosion appear as bright upward-displaced BW-echo columns — a direct map of wall thinning without sectioning the pipe. For a pipe under internal pressure, the minimum remaining wall thickness (MWT) read from the B-scan feeds directly into fitness-for-service calculations per API 579-1 / ASME FFS-1 Level 1 assessment.
A C-scan (Plan view scan) produces a top-down 2D map of the part. The transducer is raster-scanned in X–Y, and at each position a single scalar value extracted from the A-scan within a user-defined depth gate is recorded as one pixel. The result is a spatially registered image of the internal structure projected onto the scan plane.
The gate is a time window set on the A-scan. Only echoes arriving within the gate contribute to the C-scan pixel. This depth selectivity is the key distinction from a simple reflectivity map: placing the gate at a specific depth range lets the operator image one layer at a time while suppressing reflectors above and below it.
Two distinct C-scan modes extract different information from the gated A-scan:
C-scan image fidelity is governed by two independent factors. The scan step (Δx, Δy) is the mechanical indexing pitch — analogous to pixel pitch in digital imaging. Nyquist-equivalent spatial sampling requires Δx ≤ dspot/2, where \(d_\text{spot} \approx 1.02\,\lambda F/D\) is the −6 dB focal spot diameter. Undersampling misses flaws smaller than the step pitch even if the beam could resolve them.
The beam lateral resolution is the hard physical limit: two adjacent reflectors separated by less than dspot cannot be distinguished regardless of step size. In the far field of an unfocused transducer, lateral resolution degrades linearly with depth, making focused immersion setups necessary for thin-section or high-resolution work.
Laser powder-bed fusion (L-PBF) parts contain sub-surface porosity and lack-of-fusion voids whose spatial distribution governs fatigue life. A representative immersion C-scan protocol for a 10 × 10 × 5 mm coupon:
| Parameter | Value | Rationale |
|---|---|---|
| Transducer | 25 MHz, 6 mm diam., F = 25 mm (f/4) | λ = 6320 / 25×10⁶ ≈ 0.25 mm in Ti; dspot ≈ 1.07 mm at focus |
| Scan step | 0.1 mm × 0.1 mm | Well below dspot/2 ≈ 0.54 mm; oversampled for lateral position accuracy |
| Gate | 0.3 – 4.7 mm depth | Excludes the front-wall dead zone (<0.3 mm) and back-wall reflection (>4.7 mm) |
| C-scan mode | Amplitude + TOF (dual output) | Amplitude locates voids; TOF estimates void depth and part-thickness deviation |
| Min. detectable void | ∼0.1 mm (from SDH reference at 3 mm depth) | 25 MHz gives λ/2 ≈ 0.13 mm axial; lateral mapping resolution limited to ∼1 mm by spot size |
Voids appear as amplitude drops in through-transmission or amplitude peaks in pulse-echo. Through-transmission eliminates the front-wall dead zone but discards all depth information; pulse-echo retains TOF depth at the cost of a near-surface blind region equal to approximately one pulse length (∼λ/2 per cycle in the burst).
Three distinct material properties are encoded in a single pulse-echo A-scan — each read from a different feature of the returned waveform.
Sound travels at a characteristic speed set by the material's elastic stiffness and density. Measuring the round-trip time between the front-wall (FW) and back-wall (BW) echo gives wave speed directly — no destructive contact needed beyond the transducer.
d = known thickness · Δt = FW-to-BW time difference
Steel ≈ 5 920 m/s · Aluminium ≈ 6 320 m/s
FW = front-wall echo · BW = back-wall echo · Δt = round-trip transit time
Sound loses energy to absorption (heat) and scattering as it propagates. The back-wall echo arrives weaker than the transmitted pulse — the amplitude ratio over the round-trip path gives the attenuation coefficient α.
Units: Np/m or dB/mm · Higher α → shorter inspection range
Typical: 0.1–5 dB/mm at 5 MHz in metals
ABW is smaller than AFW due to material attenuation — the decay is exponential with depth
In polycrystalline metals, grain boundaries scatter sound in all directions. A fraction returns to the transducer as random “grain noise” filling the A-scan between FW and BW. Its intensity is a direct measure of grain size and microstructure.
Rayleigh regime (grain size d « λ) · Coarser grains + higher frequency → stronger noise
Orange flashes = grain boundary scatter events as wave pulse traverses the material
Random grain noise fills the region between FW and BW — amplitude ∝ grain size × f⁴
Total attenuation in a polycrystalline metal has two physically distinct contributions: absorption (thermoelastic and viscous energy conversion to heat) and scattering (energy redirected by grain boundaries, pores, and inclusions). Their frequency scalings differ, so the dominant mechanism — and the optimal inspection frequency — depends on grain size relative to wavelength.
where d is mean grain diameter, f is frequency, and αR, αS are material constants. The active regime is determined by the dimensionless parameter kd = 2πfd/c:
Schematic log–log attenuation vs. frequency for a polycrystalline metal. Regime boundary shifts left for coarser grains (larger d).
| Regime | Condition | α scaling | Dominant in |
|---|---|---|---|
| Rayleigh | kd ≪ 1 (d ≪ λ/6) | α ∝ f⁴ · d³ | Fine-grained wrought steel / Al at 1–5 MHz |
| Stochastic | kd ~ 1 | α ∝ f² · d | Coarse-grained castings, austenitic welds, AM metals |
| Geometric | kd ≫ 1 | α → frequency-independent | Very coarse grains; rarely used in practice |
| Absorption | All regimes | α ∝ f | Polymers, viscous media; minor in metals |
Austenitic SS weld metal solidifies as columnar dendritic grains, with effective grain diameters of 50–500 µm and strong crystallographic texture. At a typical 5 MHz inspection frequency in steel (cL ≈ 5 900 m/s, λ ≈ 1.2 mm), a 200 µm grain gives kd ≈ 0.7 — squarely in the stochastic regime. The consequence is severe coherent grain noise (often called backwall grass) that can mask crack tip signals. The standard engineering response is to drop to 1–2 MHz, accepting lower axial resolution, to push kd back into the Rayleigh regime and recover signal-to-noise. The trade-off is quantified by the figure of merit:
FOM is approximately constant within the stochastic regime and is used as a material characterisation parameter for phased-array inspection qualification. For fine-grained carbon steel (d ~ 20 µm), FOM ≈ 0.005–0.02 dB/(mm·MHz²); for coarse austenitic weld metal it can reach 0.1–0.5 — an order-of-magnitude degradation in inspectability.
Sound speed is not a universal constant — it depends on the elastic stiffness and density of the host material. For isotropic solids the two fundamental velocities are:
where E is Young's modulus, G the shear modulus, ν Poisson's ratio, and ρ density. Because steel has ν ≈ 0.29, the ratio cS/cL ≈ 0.55 — shear waves travel at roughly half the longitudinal speed, directly explaining the critical-angle geometry in Snell's law.
| Material | E (GPa) | ν | ρ (kg/m³) | cL (m/s) | cS (m/s) |
|---|---|---|---|---|---|
| Steel (low-alloy) | 207 | 0.29 | 7 800 | 5 900 | 3 200 |
| Aluminium | 70 | 0.33 | 2 700 | 6 320 | 3 130 |
| Titanium | 116 | 0.32 | 4 510 | 6 100 | 3 120 |
| Copper | 130 | 0.34 | 8 960 | 4 700 | 2 260 |
| CFRP (0° ply) | ~140 | ~0.30 | ~1 600 | ~7 000–9 000 | ~2 500–3 500 |
Within the near field, wavefronts emitted from different regions of the aperture arrive with varying phase at any on-axis point, producing a standing interference pattern. Axial pressure oscillates between maxima and nulls — the last axial maximum occurs right at N, after which pressure decays smoothly. Amplitude-based flaw sizing in the near field is unreliable without calibration on a reference reflector at the same depth, because a lateral shift of even a few millimetres can swing the echo amplitude by >6 dB without any change in reflector size. The boundary is the Rayleigh distance:
Beyond N, beam pressure decays as 1/r and the −6 dB beam edge expands at a fixed half-angle determined by aperture and wavelength:
A larger aperture D narrows the far-field cone but pushes N deeper — there is no free parameter that simultaneously minimises near-field length and far-field spread. Frequency is the only independent lever: increasing f shrinks λ, tightening both near-field axial resolution and far-field divergence at the cost of higher attenuation.
A spherically curved element or acoustic lens concentrates energy at geometric focal depth F, yielding a diffraction-limited lateral spot:
A phased array transducer replaces a single piezoelectric element with a linear (or matrix) array of small elements — typically 16 to 128 — each fired with an independently programmed time delay. By controlling those delays, a single probe can steer the beam to any angle, focus at any depth, and reconstruct a full cross-sectional image without moving the probe. This is electronic scanning rather than mechanical scanning.
For a linear array with element pitch p (centre-to-centre spacing), the delay applied to the n-th element to steer the beam to angle θ is:
Element 1 fires first; each successive element fires later by an increment p sinθ /c. The wavefronts from all elements constructively interfere along the chosen steering direction, forming a coherent beam at angle θ. Applying a parabolic delay profile on top of the steering ramp simultaneously focuses the beam at depth F:
Ten-element array with staggered transmit delays (blue bars, proportional to τn) steering a focused beam to 30°. Purple dashed rays represent the full S-scan sector swept electronically without moving the probe.
In an S-scan, the delay law is updated in real time to sweep the beam through a preset angular range — typically 40° to 70° for shear-wave weld inspection — while simultaneously adjusting the focus depth at each angle. Each angular position yields one A-scan; stacking them produces a cross-sectional image where steering angle maps to lateral position and time-of-flight to depth. A single probe placed beside the weld delivers the full volumetric image that conventional UT would require three separate angle-wedge setups to achieve.
FMC is an acquisition mode in which every transmit–receive pair is recorded independently: element 1 transmits while all N elements receive; then element 2 transmits; and so on. For an N-element array, FMC yields N² A-scans. TFM then reconstructs an image by coherent delay-and-sum over every pixel (x, z):
Because each pixel is reconstructed with its own exact delay law, TFM achieves diffraction-limited focusing uniformly across the image — not only at the single depth a conventional focused probe can target. The N² summation also suppresses incoherent grain noise by approximately √N² = N relative to a coherent flaw signal, improving SNR by ~20 log10(N) dB; for N = 64 that is 36 dB. The computational cost is substantial — a 64-element, 10 MHz array over a 50×50 mm image at 0.1 mm pixel pitch requires O(109) multiply-accumulate operations per frame, typically handled by GPU or FPGA.
Laser powder-bed fusion (LPBF) components present a demanding inspection scenario: sub-millimetre lack-of-fusion (LOF) voids and keyhole pores (10–200 µm diameter), columnar grain texture aligned with the build direction, and near-net-shape surfaces. Conventional pulse-echo at 5–10 MHz detects pores > ~0.5 mm in diameter reasonably well, but planar LOF defects oriented parallel to the build layers — the highest-risk flaw type in fatigue-critical components — return amplitudes well below a standard DAC curve because their specular reflection is directed away from the transducer.
Multi-mode TFM (LL, LT, TT propagation paths) addresses both limitations. Longitudinal– Longitudinal (LL) mode at near-normal incidence minimises mode-conversion noise from the textured grains; Longitudinal–Transverse (LT) and TT modes illuminate LOF faces at oblique incidence, returning an amplitude that is far less sensitive to defect tilt angle. For an LPBF IN718 coupon (cL ≈ 5 700 m/s, α ≈ 0.3 dB/mm at 10 MHz), a 64-element, 10 MHz, 0.6 mm-pitch immersion array achieves a focal spot dspot = 1.02λF/D ≈ 0.35 mm at 15 mm depth — resolving individual 250 µm LOF defects invisible to conventional single-element UT. Qualification per ASTM E2700 and ASME Code Case 2541 requires demonstrating detection of 0.8 mm FBH equivalents at T/4, T/2, and 3T/4 across the inspection volume.
| Parameter | Conventional UT | PA S-scan | FMC/TFM |
|---|---|---|---|
| Beam steering | Mechanical (swap wedge) | Electronic (delay law) | Post-processing (all angles) |
| Focusing | Fixed depth (lens) | Dynamic per angle | Optimal at every pixel |
| Data per position | 1 A-scan | Nangles A-scans | N² A-scans |
| Lateral resolution | Beam width at one focus | Varies with depth | Diffraction-limited everywhere |
| Grain-noise suppression | Baseline | Moderate | +20 log10(N) dB |
Calibration establishes a quantitative reference so that any indication can be evaluated consistently regardless of depth or scan position. The core problem it solves is that echo amplitude from an identical flaw decreases with depth due to beam spreading and attenuation — without a depth-corrected baseline, a deep 3 mm crack looks weaker than a shallow 1 mm pore.
UT amplitudes span several orders of magnitude, so all gain and sensitivity comparisons are expressed logarithmically:
The factor of 20 (not 10) arises because acoustic intensity scales as amplitude squared; \(20\log_{10}(A_2/A_1) = 10\log_{10}(A_2^2/A_1^2)\). This means the dB scale is the same whether you express it in terms of pressure amplitude or intensity.
DAC is constructed by scanning reference reflectors of identical size (side-drilled holes, SDH, or flat-bottom holes, FBH) at multiple depths in a calibration block made of the same material as the part under inspection. At each depth the gain is held fixed and the peak echo is marked on the A-scan screen. Connecting these peaks traces the DAC curve — a direct empirical map of how amplitude from an equal-area reflector decays with path length under the combined effects of beam divergence (\(\propto 1/r^2\) in the far field) and material attenuation (\(\propto e^{-2\alpha r}\)). Any indication reaching the DAC curve is flagged for evaluation; most codes add sub-DAC evaluation lines at −6 dB (50 % of DAC amplitude) and −14 dB.
Setup: 5 MHz, 12.7 mm diameter contact transducer on low-alloy steel (cL = 5 900 m/s). Near field N = D²f / 4c = 12.7² × 5×10⁶ / (4 × 5 900) ≈ 34 mm, so reflectors at 25, 50, and 75 mm are all in the far field. An ASTM E1158 block with 2.4 mm (3/32") SDH at those three depths is used.
| SDH Depth | Recorded Peak Amp. | Amplitude Drop from #1 | Implied Decay |
|---|---|---|---|
| 25 mm (SDH #1) | 82 % FSH (gain set here) | — | — |
| 50 mm (SDH #2) | 55 % FSH | −3.5 dB | Geometric spreading + ~0.04 dB/mm attenuation |
| 75 mm (SDH #3) | 36 % FSH | −7.1 dB (from #1) | Consistent; no anomalous grain scattering |
During the scan an indication appears at 60 mm depth, peaking at 73 % FSH. The DAC curve interpolated at 60 mm reads ≈ 47 % FSH. Because 73 % > 47 %, the indication exceeds DAC and must be recorded and evaluated per the applicable code (e.g., ASME Sec. VIII, AWS D1.1).
Modern digital instruments implement DAC in hardware as TCG: instead of drawing a reference curve on the A-scan, the instrument dynamically increases amplifier gain with time-of-flight so that the reference echo from any depth appears at the same screen height (typically 80 % FSH). This linearises the display — every point on the A-scan can be compared against a flat 100 % reference line. TCG is mandatory for phased-array instruments and encoded scanning where the gain must track to sub-millimetre depth increments.
Every UT system revolves around a pulser-receiver: the instrument that fires the transducer and amplifies the returning echoes. Understanding its settings is essential for optimising sensitivity, resolution, and noise rejection.
| Setting | Typical Range | Effect on Signal |
|---|---|---|
| Pulse Energy (Voltage) | 100 – 800 V | Higher voltage → greater acoustic energy transmitted → deeper penetration, but also more ringing (longer pulse) and potential saturation on strong reflectors. |
| Damping (Impedance) | 50 Ω – 1 kΩ | Higher damping shortens the pulse, improving axial resolution at the cost of lower amplitude. Low damping = high energy, longer ring-down. Match to application: thin-wall = high damping; deep penetration = low damping. |
| Pulse Repetition Frequency (PRF) | 10 Hz – 20 kHz | Must be low enough that all echoes return before the next pulse fires. Too high a PRF causes "ghost echoes" from the previous pulse. Rule: PRF < c / (2 × max depth). |
| Setting | Function |
|---|---|
| Gain / Amplification (dB) | Scales the entire A-scan. Every +6 dB doubles the displayed amplitude. Used to bring the reference echo to a standard level (e.g., 80% full-screen height). |
| Rectification Mode | Selects how the bipolar RF signal is processed before display — see animation below. |
| Filter (Bandpass) | Removes out-of-band electronic noise. Centre frequency should match the transducer's centre frequency; narrow bandwidth improves SNR but can broaden the pulse in time. |
| Reject (Suppression) | Clips all signals below a threshold level. Removes grass/noise floor but can hide real low-amplitude indications — use with caution. |
The raw A-scan is a bipolar RF voltage. Rectification converts it for easier visual interpretation:
Conventional pulse-echo sizes flaws by amplitude — but amplitude depends on crack orientation, surface roughness, and coupling, none of which correlate reliably with crack height. TOFD sidesteps amplitude entirely: it measures the time difference between diffracted signals from the crack tip and crack base, yielding a geometry-based crack height that is independent of reflectivity and orientation. Sizing accuracy of ±0.5–1 mm is routinely achieved on welds where pulse-echo would give ±2–4 mm.
From the geometry of the two pitch-catch propagation paths:
where θ = arctan(S/d) is the beam half-angle (half the probe separation S divided by the reflector depth d), v is the longitudinal wave velocity, and Δt = tbase − ttip is measured directly from the TOFD B-scan. Division by 2 is correct here — unlike pulse-echo, TOFD uses a pitch-catch geometry so the measured time is a one-way path, not a round-trip; the factor of 2 in the denominator converts one-way path length to crack height via the cosine projection.
As the TX/RX pair translates along the weld, four characteristic signal traces build up in the time-position (B-scan) display. Recognising all four — and understanding why three of them are hyperbolic — is essential for correct interpretation:
The two diffraction hyperbolas are phase-inverted relative to each other: the tip signal leads with the same polarity as the lateral wave (compression arriving first), while the base signal is inverted (rarefaction arriving first). This phase reversal is a direct consequence of diffraction geometry — the wavefront wraps around opposite edges of the crack — and serves as an internal consistency check. If both signals show the same phase, one is likely a geometric artefact rather than a true tip/base pair.
Butt weld in low-alloy steel (cL = 5 900 m/s), probe separation 2S = 100 mm. An indication is observed near the weld root at estimated depth d ≈ 25 mm. Beam half-angle: θ = arctan(50 mm / 25 mm) = 63.4°, cos θ = 0.447. Measured separation between tip and base hyperbola apices: Δt = 2.1 μs.
For a pipe wall of 12.7 mm nominal thickness, 2.8 mm represents ~22 % through-wall — above the typical ASME Code Case 2235 accept/reject threshold (∼14 % for this geometry), triggering disposition. A supplementary PA or TOFD scan at finer index pitch would then characterise the axial extent before fitness-for-service (FFS) assessment.
| Property | Pulse-Echo | TOFD |
|---|---|---|
| Sizing principle | Echo amplitude (qualitative) | Time difference (quantitative) |
| Probes needed | 1 | 2 (TX and RX straddle weld) |
| Near-surface dead zone | Small (with delay line) | Larger — lateral wave masks near-surface region |
| Sizing accuracy | ±2–4 mm (orientation dependent) | ±0.5–1 mm (geometry based) |
| Standards | ASME, AWS, EN 1712 | EN 583-6, ASME Code Case 2235 |
Weld inspection is the dominant contact UT application, and the one that most directly motivates the beam physics covered earlier. A complete weld examination follows a two-stage procedure mandated by AWS D1.1 and ASME Section V: first a straight-beam lamination check of the base metal, then an angle-beam volume scan of the weld itself.
A 0° longitudinal probe scans the base metal on both sides of the weld — specifically the heat-affected zone (HAZ), the region where thermal cycling has altered the grain structure. The goal is to detect pre-existing laminations or delaminations in the plate stock. An undetected lamination lying parallel to the surface will shadow the angle beam in Stage 2, creating a false "clean" weld — the most dangerous miss in contact UT.
Refracted shear waves (typically 45°, 60°, or 70°) are directed through the weld cross-section using a wedge probe. Because the weld cap blocks direct access, the beam must travel an oblique V-path. The probe is indexed to place the beam at the root (first leg — direct downward path) and at the crown interior (second leg — beam reflected off the backwall), then progressively shifted to sweep the full volume.
The half-skip distance — the surface distance from probe exit to where the beam completes one V-path and returns to the top surface — is:
where T is wall thickness and θ is the refraction angle in the material. For a 20 mm wall at 45°: S½ = 40 mm; at 70°: S½ = 110 mm. The large change in index distance is why 70° is preferred for thin plate and 45° for thick sections — the probe simply cannot be placed close enough to the weld for a 70° beam to reach the root in thick material without standing on the weld cap.
Cross-section view. Blue = 45° SV-wave, first leg sweeping the root region. Purple dashed = second (reflected) leg sweeping the weld interior and cap. Stage 1 straight-beam probe (left) pre-clears the HAZ for laminations before the angle scan.
Consider inspection of an API 5L X65 pipeline girth weld: wall thickness T = 20 mm, V-groove butt joint, material cS = 3250 m/s. Per ASME B31.3 / API 1104, two refraction angles are required for full volumetric coverage.
For a 45° shear-wave probe: S½ = 2 × 20 × tan(45°) = 40 mm. Place the probe so its index point is 40 mm from the weld centreline — the beam then completes one V-path and illuminates the weld cap interior on the far side. Shift the probe to index point + 20 mm (i.e. S¼ = T × tanθ) and the first leg terminates at the root — the most fracture-critical location.
A 70° probe gives S½ = 2 × 20 × tan(70°) ≈ 110 mm. This covers the weld sidewalls and upper-bead region that the 45° beam illuminates at an unfavorable angle. The combination — 45° for root/cap, 70° for sidewalls — satisfies the ASME requirement that every volume element be interrogated from at least two directions. Sensitivity is set by calibrating on a 1.5 mm side-drilled hole (SDH) at T/4, T/2, and 3T/4 depths in the reference block.
| Defect | Location | Best Detection Angle |
|---|---|---|
| Porosity (gas pores) | Throughout weld bead | Normal or 45° (cluster detection; single pores near resolution limit) |
| Slag inclusions | Between weld passes | 45°–70° |
| Lack of sidewall fusion (LOF) | Fusion boundary | 60°–70° aimed perpendicular to fusion line |
| Lack of root penetration (LRP) | Root region | 45° from both sides (S¼ position) |
| Longitudinal cracks | Crown, root, or bead centreline | Transverse scan at 45° |
| Transverse cracks | Across weld, often hydrogen-induced | Parallel scan along weld axis |
| Undercutting | Weld toes (HAZ boundary) | Straight beam or 70° with probe close to weld edge |
For a shear wave refracted at angle θR in a plate of wall thickness T, the depth and surface distance from the probe entry point to any point at beam path length ℓ are:
The half-skip distance S½ = T tanθR is the surface distance at which the beam terminates at the backwall — the critical stand-off for root inspection. After one reflection the beam returns to the scanning surface at the full-skip distance 2S½ = 2T tanθR. The four canonical probe positions and the weld zones they illuminate are:
45° SV-wave V-path in a plate of thickness T. Coloured markers show the four standard probe stand-off positions used for full weld-volume coverage.
| Refraction angle | tan θR | ½-skip S½ (T = 20 mm) | Full skip 2S½ | Typical application |
|---|---|---|---|---|
| 45° | 1.000 | 20 mm | 40 mm | Thick sections (>25 mm); root and cap, good weld-root access |
| 60° | 1.732 | 35 mm | 69 mm | General purpose; sidewalls and mid-bead passes |
| 70° | 2.747 | 55 mm | 110 mm | Thin sections (<15 mm); near-surface/crown region; detects steep-sided cracks |