Sound vs EM Key Differences Applications │ Elastic Wave Types Creating Waves Snell's Law Impedance │ What Is Ultrasound? Acoustic Spectrum UT Principle Generating UT │ A-scan B-scan C-scan Material Props │ Advanced Topics ↓

Sound Waves vs Electromagnetic (EM) Waves

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.

🌏 Sound — longitudinal pressure wave / elastic wave

Blue bands = compression   Orange bands = rarefaction.   Medium particles push & pull along the propagation direction — requires a medium.

⚡ EM wave — oscillating E & B fields (3D view)

Red = Electric field (E)   Blue = Magnetic field (B).   E ⊥ B ⊥ propagation — no medium needed; travels in vacuum at c.

Key Differences — Speed, Medium & Energy Loss

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.

Property
🔊 Sound Wave
⚡ EM Wave (light / radio / microwave)
Needs a medium?
✓ Yes — solid, liquid, or gas
✗ No — propagates freely in vacuum
Speed in Vacuum
✗ Cannot travelno medium → no wave
3 × 108 m/sconstant — the speed of light, c
Speed in Air
343 m/s
3 × 108 m/s876,000× faster than sound in air
Speed in Water
1,480 m/s
2.25 × 108 m/sslows slightly (n ≈ 1.33)
Speed in Steel
5,900 m/sfaster in solids than in liquids or gases
✗ Cannot penetrateabsorbed / reflected at the metal surface
Energy Loss
as the wave travels
Attenuates with distance & frequency
α ≈ 0.5–2 dB/(mm·MHz) in steel — higher frequency loses energy faster
Zero loss in vacuum or transparent media
Fully absorbed or reflected at any metal surface — cannot inspect inside metals
Why sound wins for metal inspection: EM waves (radio, microwave, visible light) are stopped dead at any metal surface — the free electrons reflect them completely. Sound travels freely through steel at 5,900 m/s, and the round-trip travel time for a 50 mm thick part (≈17 µs) is easily measured with standard electronics. Flaw depth follows directly from d = c × t / 2.

Where Each Wave Is Used

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.

🔊 Sound Wave — Applications
  • Ultrasonic NDT/NDE — flaw detection in metals, welds, and composites; the core use case for this toolkit
  • Medical ultrasound — prenatal imaging, cardiac echocardiography, abdominal scans (soft-tissue B-mode)
  • Sonar — underwater mapping, submarine detection, fish-finding, seafloor bathymetry
  • Acoustic emission (AE) — real-time monitoring of crack growth and structural damage
  • Ultrasonic cleaning — cavitation removes surface contamination from precision parts and surgical instruments
⚡ EM Wave — Applications
  • X-ray radiography & CT — imaging internal casting defects, bone fractures, and security screening
  • Radar & GPS — aircraft navigation, weather detection, speed enforcement, autonomous vehicles
  • WiFi, 5G & satellite — wireless communications and global positioning across any environment
  • Infrared thermography (IRT) — surface hot-spot detection in electronics, composites, and building envelopes
  • Optical fiber — high-bandwidth data transmission via light pulses in glass fiber

Types of Elastic Waves

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.

Bulk wave

1. Longitudinal (L)

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.

Bulk wave

2. Shear (S): SH & SV

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.

Surface wave

3. Rayleigh (R)

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.

Parallel motionL-wave: particle motion ∥ travel
Perpendicular motionS-wave: particle motion ⟂ travel
Elliptical motionRayleigh: surface-localized rolling

How Are Different Elastic Waves Created?

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.

θᵢ = 0°

1. Normal incidence

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.

θᵢ > 0°

2. Oblique incidence

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.

Critical θᵢ

3. Rayleigh critical angle

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.

Incident L Reflected L Transmitted L Transmitted SV Rayleigh
The control knob is angle: Snell’s law links every refracted mode to its wave speed. Increasing the incident angle first changes the L and SV directions, then drives bulk modes to their critical conditions; tuning to the Rayleigh condition concentrates energy at the surface. In practice, wedges are often used instead of water to set these angles precisely.

📈 Snell's Law & Mode Conversion

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:

$$\frac{\sin\theta_i}{c_{L1}} = \frac{\sin\theta_L}{c_{L2}} = \frac{\sin\theta_S}{c_{S2}}$$

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.

Water / Couplant c₁ = 1480 m/s Steel cL = 5900 m/s   cS = 3200 m/s P-wave: total internal reflection θᵢ = 20° > θc1 = 14.5° — no P enters the steel Interface normal Incident P θᵢ = 20° θᵢ Reflected P θᵣ = θᵢ = 20° Mode-converted S θS ≈ 47.7° θS

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.

Incident P Reflected P (TIR) Mode-converted S

Critical Angles

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°
NDE example — 45° shear weld probe (Perspex–steel):
Required wedge angle: sin(θwedge) = sin(45°) × cPerspex / cS-steel = 0.707 × 2730 / 3200 = 0.603 → θwedge ≈ 37°.
The wide Perspex–steel window (27.6° – 58.5°) means a single wedge material covers 45°, 60°, and 70° shear angles — each cut at a different face angle. For a 25 mm thick plate, one half-skip leg covers a surface distance of T × tan(45°) = 25 mm; a full V-path spans 50 mm, directly constraining probe placement during weld-root inspection.

🔄 Acoustic Impedance

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.

$$Z = \rho\,c \qquad [\text{Pa·s/m} = \text{Rayl}]$$
Medium 1 (Z₁) Medium 2 (Z₂) Interface Incident (I) Transmitted (T) Reflected (R) R = [(Z₂−Z₁)/(Z₂+Z₁)]² T = 1 − R

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.

Incident Reflected Transmitted

Reflection & Transmission Coefficients (Normal Incidence)

For a wave striking an interface at normal incidence, the intensity reflection and transmission coefficients are:

$$R = \left(\frac{Z_2 - Z_1}{Z_2 + Z_1}\right)^{\!2} \quad (\text{intensity reflection}) \qquad T = 1 - R \quad (\text{intensity transmission})$$

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.

Acoustic Impedance of NDE-Relevant Materials

Material ρ (kg/m³) cL (m/s) Z (MRayl) NDE relevance
Steel (low-alloy)7 8005 90046.0Primary inspection target
Aluminium2 7006 32017.1Aerospace structures, AM Ti parts
Titanium4 5106 10027.5Additive-manufactured components
CFRP (through-thickness)~1 600~2 800~4.5Low Z → large mismatch with steel tooling
Water (20 °C)9981 4801.48Immersion couplant
Ultrasonic gel~1 000~1 500~1.5Contact couplant — closely matches water
Air1.23430.0004Near-total reflection at any solid–air gap

Worked NDE Example — Immersion Inspection of Aluminium

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):

$$R = \left(\frac{17.1 - 1.48}{17.1 + 1.48}\right)^{\!2} = \left(\frac{15.62}{18.58}\right)^{\!2} \approx 0.71 \quad (71\,\% \text{ of intensity reflected})$$

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.

Importance of Couplant

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.

Phase inversion diagnostic: In RF mode, a reflection from a lower-Z material (e.g. the far face of a steel plate into water, or a gas pore within metal) appears as a polarity-inverted echo relative to the entry surface. This sign flip is a direct consequence of r < 0 and can distinguish an open crack (gas-filled, soft reflection) from a bonded inclusion (hard reflection) — a technique used in diffusion-bonded and brazed-joint inspection.

What Is Ultrasound?

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.

🏥
Medical imaging
Obstetric & cardiac ultrasound — 1–15 MHz
🏭
Industrial NDT
Flaw detection & thickness gauging — 0.5–25 MHz — this toolkit's focus
🐋
Sonar & bio-sonar
Navigation & echolocation — 20–200 kHz

The Acoustic Spectrum for Inspection

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.

Audible & Below
Low UT
Medical
NDE Main Range
High-Res NDE
20 Hz 20 kHz 100 kHz 1 MHz 10 MHz 50 MHz
Audible & Below < 20 kHz
  • Human hearing range
  • Seismic monitoring
  • SONAR (low-freq)
Low UT 20–100 kHz
  • Ultrasonic cleaning
  • Welding / bonding
  • Thickness gauging
Medical 100 kHz – 1 MHz
  • Prenatal imaging
  • Cardiac echocardiography
  • Abdominal scans
NDE Main Range ★ 1 – 10 MHz
  • Weld inspection & flaw detection
  • Plate & pipe thickness measurement
  • Composite laminate scanning
  • Corrosion mapping
  • Forgings & castings
High-Res NDE 10 – 50 MHz
  • Microelectronics inspection
  • Thin coating & bond testing
  • Fine-grained metal imaging
  • High-resolution C-scan

Choosing the Right 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
The fundamental trade-off: Resolution is limited to approximately one wavelength (λ = c / f). Higher frequency → shorter wavelength → finer resolution. But higher frequency also means more attenuation — the wave dies out sooner. A 5 MHz probe in steel gives λ ≈ 1.2 mm; at 1 MHz, λ ≈ 5.9 mm. Choose frequency based on the smallest flaw you need to detect vs. the depth you need to reach.

Fundamental Principle of Ultrasonic NDT

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.

🔊 Pulse-Echo Schematic

Cyan arcs = transmitted pulse & back-wall echo.   Red arcs = flaw echo reflected from the void.

📈 A-scan — Amplitude vs Time

IP = initial pulse  •  Flaw Echo = void reflection  •  BW = back-wall echo.   Trace builds as pulse travels.

How is Ultrasound Generated?

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.

The Piezoelectric Effect — Simply Put

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.

Backing Material absorbs rearward energy, shortens pulse Piezoelectric Crystal (PZT) Matching Layer Wear Plate couplant (water / gel) Test Material Backing damps reverb Crystal vibrates at MHz Matching layer improves coupling Voltage pulse in 🔊 Ultrasound pulses propagate into the material

The Pulse-Echo Principle

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).

Pulse Bandwidth & Axial Resolution

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:

$$\delta z \;=\; \frac{c}{2\,\Delta f_{-6\,\text{dB}}} \;\approx\; \frac{c\,\tau_p}{2}$$

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:

Wideband (high damping) Short pulse · fine axial resolution gap δz resolved ✓ Resolved Time of flight → Narrowband (low damping) Long ring-down · poor axial resolution ✗ Cannot resolve same δz — merged Time of flight →
Bandwidth rule of thumb: A broadband element (>60 % fractional BW, e.g., a 5 MHz probe with −6 dB bandwidth spanning 3–7 MHz) delivers τp < 0.5 µs — resolving reflectors separated by ≥ ~1.5 mm in steel. An underdamped element (<20 % BW) can ring for 2–5 µs, merging echoes from reflectors up to 6–15 mm apart. Specify backing impedance and fractional bandwidth explicitly when thin-section or fine-defect axial resolution is the primary inspection requirement.

Worked NDE Example — Probe Selection for LPBF Ti-6Al-4V

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).

Parameter10 MHz probe5 MHz probe
Wavelength λ = c/f0.61 mm1.22 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.

🔌

Learn More: Transducer Types, Designs & Resources

Contact, immersion, EMAT, phased array, dual-element — designs, selection guides, and links to manufacturers.

→

Scanning Methods — A-scan

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.

flaw Transducer top bottom Part cross-section 0 Time (proportional to depth) Amplitude IP Flaw Echo BW depth to flaw part thickness A-scan display (amplitude vs. time)

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-scan formula: d = c × t / 2    where d = depth, c = wave speed (material-specific), t = measured time-of-flight. The factor of 2 accounts for the round-trip path (down and back).

Scanning Methods — B-scan

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.

Scan direction 0 Depth ↓ T Scan position (X) flaw Part cross-section B-scan image

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.

How A-scans are stacked to form a B-scan column Amplitude Position x₁ (no flaw) FW BW flaw Position x₂ (flaw present) Position x₃ (no flaw) stack & encode B-scan FW flaw BW 0 T Depth Scan position X x₁ x₂ x₃

Axial and Lateral Resolution in B-scan

Two independent length scales govern what a B-scan can resolve:

$$\delta_z = \frac{c}{2\,\text{BW}} \approx \frac{c\,\tau_p}{2} \quad \text{(axial)} \qquad \delta_x \approx \frac{1.02\,\lambda F}{D} \quad \text{(lateral, at focus)}$$

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.

NDE Example — Pipeline Corrosion Mapping with B-scan

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.

ParameterValuePhysical 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.

Limitation — acoustic shadowing: A large near-surface reflector (e.g. a delamination) can shadow smaller, deeper reflectors in the same beam path. Multiply-reflected "ghost" echoes between two parallel reflectors also produce spurious B-scan columns at multiples of the true depth — visible in thick-walled parts at high PRF or gain. For complex geometries, multiple scan directions or phased-array volumetric methods are preferred over a single-angle B-scan.

Scanning Methods — C-scan

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.

X Y Raster scan pattern (top view) High Low C-scan amplitude map X Y

Depth Gating — How One Pixel Is Formed

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.

A-scan at one X–Y position DEPTH GATE (d₁ to d₂) FW Flaw peak A = 68% FSH → pixel value BW Time-of-flight (∝ depth) Amp. d₁ d₂ gate peak C-scan map (X–Y plane) 68% FSH 100% 50% 0% X position (mm) Y

Two distinct C-scan modes extract different information from the gated A-scan:

Scan Resolution and Lateral Resolution Limits

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.

NDE Example — Immersion C-scan of an L-PBF Ti-6Al-4V Coupon

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:

ParameterValueRationale
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).

Summary of the three scanning methods:
A-scan = what echoes exist at this one spot (amplitude vs. time).   B-scan = how deep is the flaw along a line (cross-section view).   C-scan = where is the flaw across the whole surface (map view).   A C-scan is a stack of gated A-scans reduced to one scalar per pixel; the gate definition is the operator’s primary tool for targeting a specific depth layer.

What Does Ultrasound Actually Measure?

Three distinct material properties are encoded in a single pulse-echo A-scan — each read from a different feature of the returned waveform.

01

Wave Speed

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.

c = 2d / Δt

d = known thickness  ·  Δt = FW-to-BW time difference
Steel ≈ 5 920 m/s  ·  Aluminium ≈ 6 320 m/s

📊 A-scan — Time of Flight

FW = front-wall echo  ·  BW = back-wall echo  ·  Δt = round-trip transit time

02

Attenuation

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.

α = (1/2d) · ln(AFW / ABW)

Units: Np/m or dB/mm  ·  Higher α → shorter inspection range
Typical: 0.1–5 dB/mm at 5 MHz in metals

📊 A-scan — Amplitude Loss

ABW is smaller than AFW due to material attenuation — the decay is exponential with depth

03

Backscatter

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.

BSC ∝ f⁴ · d³

Rayleigh regime (grain size d « λ)  ·  Coarser grains + higher frequency → stronger noise

🎗 Material — Grain Microstructure

Orange flashes = grain boundary scatter events as wave pulse traverses the material

📊 A-scan — Grain Noise

Random grain noise fills the region between FW and BW — amplitude ∝ grain size × f⁴

Advanced Topics

🔴 Attenuation — Detailed

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.

$$\alpha_\text{total}(f) = \underbrace{\alpha_\text{abs} \cdot f}_{\text{absorption}} + \underbrace{\alpha_R \cdot f^4 \cdot d^3}_{\text{Rayleigh}} + \underbrace{\alpha_S \cdot f^2 \cdot d}_{\text{stochastic}}$$

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:

Three Scattering Regimes

Frequency (log scale) α (dB/mm) — log scale 0.5 1 2 5 10 MHz kd ≈ 1 (d≈200 µm) Absorption (∝ f) Stochastic (∝ f²) Rayleigh (∝ f⁴) Rayleigh regime (kd ≪ 1) Stochastic regime (kd ~ 1)

Schematic log–log attenuation vs. frequency for a polycrystalline metal. Regime boundary shifts left for coarser grains (larger d).

Regime Summary

RegimeConditionα scalingDominant 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

NDE Example: Austenitic Stainless Steel Welds

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:

$$\text{FOM} = \frac{\alpha}{f^2}$$

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.

Practical rule: For carbon steel, α ≈ 0.5–2 dB/(mm·MHz) at 5 MHz depending on grain size. Coarse-grained castings can be 10× worse, and austenitic weld metal 20–50× worse than fine-grained wrought steel. Always measure α on a representative coupon — never assume handbook values for cast or additively manufactured microstructures.

🔭 Beam Physics

Wave Velocity from Material Properties

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:

$$c_L = \sqrt{\frac{E\,(1-\nu)}{\rho\,(1+\nu)(1-2\nu)}} \qquad c_S = \sqrt{\frac{G}{\rho}} = \sqrt{\frac{E}{2\rho\,(1+\nu)}}$$

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.

MaterialE (GPa)νρ (kg/m³)cL (m/s)cS (m/s)
Steel (low-alloy)2070.297 8005 9003 200
Aluminium700.332 7006 3203 130
Titanium1160.324 5106 1003 120
Copper1300.348 9604 7002 260
CFRP (0° ply)~140~0.30~1 600~7 000–9 000~2 500–3 500
Why this matters for inspection design: A higher cL shortens the wavelength at a given frequency (λ = c/f), improving axial resolution. Conversely, CFRP composites have directional velocities that vary with fibre orientation — a constant velocity assumption introduces depth errors that can exceed 10 % in multi-ply layups. Always verify velocity on a reference block of the same material and lay-up.

Near Field (Fresnel Zone)

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:

$$N = \frac{D^2}{4\lambda} = \frac{D^2 f}{4c}$$
D Xdcr Near Field irregular amplitude N = D²f / 4c N θ Far Field smooth divergence sin θ ≈ 0.514λ/D (−6 dB)
Worked example — 5 MHz, 12.7 mm probe in steel (cL = 5 900 m/s): λ = 5 900 / 5 × 106 = 1.18 mm  •  N = (12.7)2 / (4 × 1.18) ≈ 34 mm. Inspecting a 20 mm thick weld means the back-wall echo arrives at ∼0.59 N — deep in the near field. Echo amplitude can vary >6 dB with lateral position without any reflector change, making amplitude-based DAC unreliable. Remedies: focus the probe at mid-thickness (immersion or delay-line lens), reduce diameter, or lower frequency to push N below the part thickness.

Far-Field Divergence

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:

$$\sin\!\left(\theta_{1/2}\right) \approx \frac{0.514\,\lambda}{D} \quad (-6\,\text{dB half-angle}) \qquad \sin\theta \approx \frac{1.2\,\lambda}{D} \quad (\text{Rayleigh criterion})$$

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.

Focused Transducers

A spherically curved element or acoustic lens concentrates energy at geometric focal depth F, yielding a diffraction-limited lateral spot:

$$d_{\text{spot}} \approx \frac{1.02\,\lambda F}{D} = \frac{1.02\,F}{f\text{-number}}$$
Design trade-off: A tighter focus (smaller f-number) improves lateral resolution but compresses the depth of field to ∼±(dspot)2/λ. For thick welds (>50 mm) an unfocused or weakly focused beam maintains sensitivity throughout the volume; for thin composites or additively manufactured parts with fine porosity, a focus at mid-thickness maximises lateral resolution where it matters most.

🔋 Phased Arrays & Advanced Imaging

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.

Delay-Law Beam Steering

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:

$$\tau_n = \frac{(n-1)\,p\,\sin\theta}{c}$$

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:

$$\tau_n^{\text{focus}} = \frac{1}{c}\!\left(F - \sqrt{F^2 + \left[(n - \tfrac{N+1}{2})\,p\right]^2}\right)$$
Test piece Water path / gel couplant 1 10 ← τ₁ (fires first) ··· τ₁₀ (fires last) — steers beam right → θ = 30° Focal spot S-scan coverage sector (electronically swept) T Active beam (30°, focused) Other S-scan angles Focal spot / indication

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.

Sectorial Scan (S-scan)

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.

Full Matrix Capture & Total Focusing Method (FMC/TFM)

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):

$$I(x,z) = \left|\sum_{t=1}^{N}\sum_{r=1}^{N} s_{tr}\!\left(\frac{\sqrt{(x-x_t)^2+z^2}+\sqrt{(x-x_r)^2+z^2}}{c}\right)\right|^2$$

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.

NDE Example — Inspection of Metal Additive Manufactured Parts

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
Grating lobe criterion: Element pitch p must satisfy p ≤ λ/2 to avoid grating lobes — spurious off-axis beams at angles where element-to-element path differences equal whole wavelengths. For 5 MHz in steel (λ = 1.18 mm), p ≤ 0.6 mm. Active aperture D = N·p governs near-field length and far-field divergence identically to a single-element probe of the same diameter.

📏 Calibration & Reference Levels

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.

Decibel Scale

UT amplitudes span several orders of magnitude, so all gain and sensitivity comparisons are expressed logarithmically:

$$\Delta\,(\text{dB}) = 20\log_{10}\!\!\left(\frac{A_2}{A_1}\right)$$

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.

Quick conversions: +6 dB = ×2 amplitude  |  +20 dB = ×10  |  −6 dB = ×0.5  |  −20 dB = ×0.1  |  −40 dB = ×0.01

Distance Amplitude Correction (DAC)

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.

100% 80% 60% 40% 20% 0% 25 50 75 100 Reflector depth (mm) Amplitude (% FSH) ▲ Indication exceeds DAC → Record & evaluate per code Below –6 dB → not recorded DAC curve –6 dB evaluation line Reference SDH echoes Recordable indication

Worked Example — Contact UT on Steel Pressure Vessel

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 DepthRecorded Peak Amp.Amplitude Drop from #1Implied Decay
25 mm (SDH #1)82 % FSH (gain set here)——
50 mm (SDH #2)55 % FSH−3.5 dBGeometric 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).

Time-Corrected Gain (TCG) — the Digital Equivalent

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.

Reference Blocks & Standards

⚡ Pulser-Receiver & the Signal Chain

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.

Pulser Settings

SettingTypical RangeEffect 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).

Receiver Settings

SettingFunction
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 ModeSelects 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.

Rectification Modes — Animated

The raw A-scan is a bipolar RF voltage. Rectification converts it for easier visual interpretation:

Which mode to use? RF is essential for TOFD and precise pulse-width measurement. Full-wave is the most common field choice — it preserves symmetry and is easiest to gate. Half-wave modes are occasionally used to distinguish the polarity of a reflection (positive → hard reflection from higher-Z material; negative → soft reflection from lower-Z material).

🖐 TOFD — Time-of-Flight Diffraction

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.

Test Piece (thickness T) — separation 2S between probe centres Crack tip Crack base a TX RX 2S lateral wave (surface) tip signal — shorter path, earlier arrival base signal — longer path, later arrival θ

From the geometry of the two pitch-catch propagation paths:

$$a = \cos\theta \times \frac{(t_{\text{base}} - t_{\text{tip}})\, v}{2}$$

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.

Reading a TOFD B-Scan

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:

DEAD ZONE (lateral wave masks near-surface region) Lateral wave (tlat) crack position Tip diffraction (hyperbola, same phase as lateral wave) Base diffraction (hyperbola, phase-inverted relative to tip) Backwall (tbw) Δt → crack height a Scan position along weld → Time-of-flight (depth) ↓

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.

Worked Example — Weld Root Crack Sizing

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.

$$a = 0.447 \times \frac{2.1\!\times\!10^{-6}\;\text{s} \;\times\; 5\,900\;\text{m/s}}{2} = 0.447 \times 6.195\;\text{mm} \approx \mathbf{2.8\;mm}$$

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.

PropertyPulse-EchoTOFD
Sizing principleEcho amplitude (qualitative)Time difference (quantitative)
Probes needed12 (TX and RX straddle weld)
Near-surface dead zoneSmall (with delay line)Larger — lateral wave masks near-surface region
Sizing accuracy±2–4 mm (orientation dependent)±0.5–1 mm (geometry based)
StandardsASME, AWS, EN 1712EN 583-6, ASME Code Case 2235
Practical note: TOFD provides accurate crack height but cannot locate the crack laterally (it only knows the probe is somewhere in the scan range when Δt is maximum). Pairing TOFD with phased-array pulse-echo — now standard in nuclear and pressure-vessel inspections per ASME Section V — gives height (TOFD) and lateral position (PA) simultaneously from a single encoded scan pass.

🔧 Application — Weld Inspection

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.

Stage 1 — Straight-Beam Lamination Scan

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.

Stage 2 — Angle-Beam Weld Volume Scan

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:

$$S_{1/2} = 2T \tan\theta$$

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.

0° L-wave Stage 1 lamination check 45° SV 45° S½ = 2T·tanθ = 270 mm (20 mm wall, 45°) Weld cap HAZ HAZ fusion line Weld root Leg 1 — root Leg 2 — crown T Base metal

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.

Worked NDE Example — Pipeline Girth Weld

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.

Common Weld Defects Detectable by UT

DefectLocationBest Detection Angle
Porosity (gas pores)Throughout weld beadNormal or 45° (cluster detection; single pores near resolution limit)
Slag inclusionsBetween weld passes45°–70°
Lack of sidewall fusion (LOF)Fusion boundary60°–70° aimed perpendicular to fusion line
Lack of root penetration (LRP)Root region45° from both sides (S¼ position)
Longitudinal cracksCrown, root, or bead centrelineTransverse scan at 45°
Transverse cracksAcross weld, often hydrogen-inducedParallel scan along weld axis
UndercuttingWeld toes (HAZ boundary)Straight beam or 70° with probe close to weld edge
Stainless steel and coarse-grained alloys: Austenitic stainless and nickel-alloy welds have columnar grains (1–5 mm) aligned with the solidification direction. These act as scatterers with Rayleigh-regime attenuation scaling as f4, making standard 2–5 MHz shear waves essentially unusable — grain noise overwhelms real flaw signals. The practical fix is refracted longitudinal waves at 1–2.5 MHz (longer wavelength, sub-Rayleigh regime) or phased-array TFM with a grain-noise model to separate coherent flaw signals from incoherent scattering. Low-frequency arrays (0.5–2 MHz) purpose-built for austenitic inspection are commercially available and specified in ENIQ Procedure 009.

Angle Beam Geometry

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:

$$\text{Depth} = \ell\cos\theta_R \qquad \text{Surface dist. from entry} = \ell\sin\theta_R$$

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:

Weld cap Weld 45° SV ¼S ½S ¾S Full S Full skip = 2T·tanθ θR T Near-surface Mid-thickness Root zone Backwall (B/W) ¼S: beam at T/2 depth (upper region) ½S: backwall (root) ¾S: T/2 depth (return leg) Full S: crown zone

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
NDE example — full volumetric coverage of API 5L X65 girth weld (T = 20 mm):
Per ASME Section V and API 1104, every volume element must be illuminated from at least two directions. A 45° SV probe placed at S½ = 20 mm from the weld centreline puts the first-leg beam at the weld root; shifting to 2S½ = 40 mm sweeps the cap interior. A 70° SV probe at S½ ≈ 55 mm then covers the sidewalls and near-crown region that the 45° beam strikes at an unfavourable angle. The two-probe combination satisfies the geometric coverage requirement without repositioning the scanner assembly — the 45° probe handles root/cap and the 70° handles sidewalls, making the pair complementary rather than redundant. Sensitivity at each stand-off is set by calibrating on 1.6 mm (1/16") SDH at T/4, T/2, and 3T/4 in an ASTM E1158 block of matching material.