Characterization Method Finder

This page helps you decide which instrument to use when you have a sample and a question. Choose what you want to know and the constraints of your sample; suitable methods are listed in order, and methods that do not fit are set aside with the reason. Pick two to four methods to compare side by side, including preparation before measuring and pitfalls in reading the results.

Values are typical values from the sources and vary greatly with instrument, conditions and material. Use them as a guide for comparing methods and narrowing down candidates, and check with the instrument manager or service lab before measuring. Standards are listed by name, number and scope only (see the standards themselves for specimen dimensions and conditions).

Microstructure and shape 11

Look at a polished and etched section to see grain size, phase distribution, inclusions and layer thickness. The first step in examining a microstructure.

Principle Metals are viewed in reflected light. An etchant attacks grain boundaries and phases at different rates, which turns them into light and dark contrast.

Used for Microstructure on a section Grain size, orientation and texture Thickness of films and layers Precipitates Fracture surface Internal defects Surface shape and roughness Phase identification and crystal structure

Typical figures

Lateral resolution
About 0.2 µm (limit set by the wavelength of light)
Depth resolution / information depth
Image of the polished plane (no depth information)
Detection limit
— (no elemental analysis)
Analyzed depth / volume
Surface of the polished section
Elements
None (phases are inferred from color, shape and etching response)
Quantitative accuracy
Area fractions and grain size can be quantified by image analysis

Sample and effort

Size
Powders and small pieces can be mounted in resin; large parts must be sectioned
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Cut or polish The sectioned and polished part is destroyed
Preparation
Moderate Cut → mount in resin → polish → etch. Half a day to a day, depending on material and etchant
Time
Short Minutes to tens of minutes once the sample is ready
Cost
Low Usually cheap on a shared university instrument

Pitfalls

  • Polishing scratches and smeared layers are highlighted by etching and can be mistaken for microstructure. Etching does not remove earlier damage
  • Resolution is about 0.2 µm, so fine precipitates and the inside of martensite laths are not resolved (go to SEM or TEM)
  • A section is a 2-D cut, so grain shape and size look different depending on the cutting direction. For rolled material, examine several sections in defined directions

Often combined with SEM · EBSD · HV/HR/HBW

Standards ASTM E3 (guide to preparing metallographic specimens) / ASTM E407 (microetching metals and alloys) / JIS G 0551 / ASTM E112 (determining grain size) / ISO 3887 (determining the depth of decarburization of steels)

Terms Pearlite Martensite Hall–Petch relationship

Sources: MyScope SEM; Metkon (ASTM E407); ISO 3887

Image surface topography (SE) and differences in mean atomic number (BSE) with far better resolution and depth of field than an optical microscope. The workhorse for fracture surfaces and fine microstructure.

Principle A finely focused electron beam is scanned over the surface, and the number of secondary electrons (SE) and backscattered electrons (BSE) coming out sets the brightness of each pixel.

Used for Surface shape and roughness Fracture surface Microstructure on a section Thickness of films and layers Precipitates Internal defects Grain size, orientation and texture

Typical figures

Lateral resolution
About 1–5 nm (around 1 nm with a field-emission gun, about 5 nm on a typical instrument)
Depth resolution / information depth
SE from the top ~15 nm; BSE from deeper (depends on accelerating voltage)
Detection limit
— (use EDS for composition)
Analyzed depth / volume
SE: the very surface; BSE: the upper part of the electron interaction volume
Elements
Not from the image (BSE brightness is only a guide to mean atomic number)
Quantitative accuracy
Calibrate the magnification with a standard before measuring sizes

Sample and effort

Size
Whatever fits the chamber (instrument dependent); large parts must be cut
Conductivity
Insulators need a ~10 nm conductive coating or low-vacuum imaging
Vacuum
Normally high vacuum; wet samples must be dried or imaged in low vacuum
Destructive?
Non-destructive for surfaces; sections must be cut and polished
Preparation
Minimal Little for surfaces; polishing for sections; coating for insulators
Time
Short Tens of minutes to a few hours per sample
Cost
Low Usually cheap on a shared university instrument

Pitfalls

  • Reading BSE contrast as composition. Topography and crystal orientation (channeling) also change the brightness, so check on a flat polished surface together with EDS
  • Mistaking charging artifacts (bright, smeared areas) on insulators, or the grain of a coating, for microstructure
  • Trusting the on-screen scale as is. Calibrate the magnification with a standard before measuring sizes

Often combined with EDS (EDX) · EBSD · FIB

Terms SEM (scanning electron microscope) Fatigue striations

Sources: MyScope SEM; EAG technique chart

Map the orientation of every grain to obtain grain size, texture, grain-boundary misorientation, phase distribution (by crystal structure) and a guide to local strain.

Principle In the SEM the sample is tilted to 70°, the diffraction pattern of backscattered electrons (Kikuchi pattern) is recorded, and the crystal orientation is solved point by point.

Used for Grain size, orientation and texture Phase identification and crystal structure Microstructure on a section

Typical figures

Lateral resolution
20–80 nm (material dependent). Grains smaller than 50 nm are difficult (TKD on a thin foil reaches 2–20 nm)
Depth resolution / information depth
Top ~10 nm of the surface
Detection limit
— (no elemental analysis)
Analyzed depth / volume
Top ~10 nm layer
Elements
None (combine with simultaneous EDS to separate phases)
Quantitative accuracy
Orientation precision about 0.2° (about 0.001° with cross-correlation analysis for strain)

Sample and effort

Size
Whatever fits the SEM chamber
Conductivity
A conductive coating weakens the patterns, so low-vacuum imaging is preferred for insulators
Vacuum
Normally vacuum (low-vacuum instruments exist)
Destructive?
Cut or polish Needs a flat polished surface, so that part is cut and polished
Preparation
Extensive Mechanical polishing followed by a strain-free finish (chemical or electrolytic polishing). Laborious
Time
Moderate Tens of minutes to hours per map (fast detectors exceed 3000 points per second)
Cost
Moderate Medium (fewer SEMs carry EBSD)

Pitfalls

  • Polishing damage left at the surface kills the patterns and leaves many points unindexed. Mechanical polishing alone is often not enough
  • Grain size depends on the misorientation threshold used to define a boundary and on the step size. State them when comparing
  • The mapped area is small (hundreds of µm to mm). Check the texture of the whole sheet with XRD pole figures

Often combined with SEM · XRD (sin²ψ, pole figures) · OM

Terms Recrystallization Hall–Petch relationship

Sources: DTU Nanolab EBSD; SERC (Carleton College); EAG technique chart; ASM EDFAS (EBSD detector)

Image dislocations, precipitates and interfaces down to atomic columns using electrons transmitted through a specimen thinner than 100 nm. With electron diffraction and EDS/EELS, structure and composition come from the same spot.

Principle Bright- and dark-field contrast comes from differences in diffracted intensity, and HRTEM forms lattice images by interference of transmitted and diffracted waves. STEM-HAADF collects electrons scattered to high angles, so heavier atoms look brighter (Z contrast).

Used for Precipitates Microstructure on a section Phase identification and crystal structure Thickness of films and layers Local composition and element maps Internal defects Grain size, orientation and texture Chemical state (oxidation state, bonding)

Typical figures

Lateral resolution
0.1–0.3 nm (TEM point resolution 0.14 nm, 0.1 nm in an aberration-corrected STEM; about 0.2–0.25 nm without correction)
Depth resolution / information depth
Projection through the whole specimen thickness (<100 nm)
Detection limit
EDS about 0.5 wt% (0.01–0.1 wt% under good conditions)
Analyzed depth / volume
A region of µm size or less in a foil thinner than 100 nm
Elements
EDS from B upwards (poor sensitivity to light elements); EELS down to Li
Quantitative accuracy
EDS is semi-quantitative to a few percent

Sample and effort

Size
Disks about 3 mm across, particles on a grid, or FIB lamellae
Conductivity
Not needed (thinning is what matters)
Vacuum
Required (dry, beam-tolerant specimens)
Destructive?
Cut or polish Destroys the part that is thinned
Preparation
Extensive Thin by electropolishing, ion milling, FIB or ultramicrotomy. Needs skill and time
Time
Long Days to weeks including preparation
Cost
High (often outsourced)

Pitfalls

  • The volume examined is tiny (<100 nm thick, µm across). One field may not represent the sample, so survey with SEM first and then choose the site
  • Preparation damage mistaken for microstructure. FIB lamellae carry a Ga-damaged layer on both faces; milling at 30 kV alone leaves about 20 nm per side in Si
  • Bright- and dark-field contrast mainly reflects diffraction. Check whether it is compositional with HAADF (brightness set by atomic number) or EDS

Often combined with FIB · SAED/CBED · APT

Terms Dislocation Burgers vector Precipitation hardening

Sources: Univ. Duisburg-Essen ICAN; Microscopy Australia TechFi; EAG technique chart; MyScope EDS

Mill a chosen site with µm precision to expose a cross-section or to make TEM lamellae and APT needles. Combined with an SEM, repeated slice-and-image gives 3-D microstructure.

Principle Ga ions focused below 10 nm sputter atoms from the surface. The milled face is imaged with the electron beam (SEM).

Used for Thickness of films and layers Microstructure on a section Internal defects

Typical figures

Lateral resolution
Beam below 10 nm; imaging at SEM resolution (about 1 nm)
Depth resolution / information depth
Serial sectioning gives 3-D data on regions 100 nm–10 µm in size
Detection limit
— (combine with EDS etc.)
Analyzed depth / volume
A local region of µm to tens of µm
Elements
—
Quantitative accuracy
—

Sample and effort

Size
Whatever fits the SEM chamber
Conductivity
Insulators charge and should be coated
Vacuum
Required
Destructive?
Cut or polish Destroys the milled spot (locally)
Preparation
Moderate Decide the site first; deposit a protective layer before milling
Time
Moderate Hours per cross-section; half a day to a day per TEM lamella
Cost
Moderate Medium to high (instrument time is expensive)

Pitfalls

  • The milled face carries a Ga-damaged layer (about 20 nm per side in Si at 30 kV). Finish TEM lamellae at low voltage (3–7 nm at 2 kV)
  • The accessible area is small, so locate the feature with SEM or optical microscopy before milling

Often combined with SEM · TEM/STEM · APT

Sources: Microscopy Australia TechFi; Univ. Twente NanoLab; EAG technique chart

Trace the surface with a sharp tip and build a height map at nm scale. Measures roughness, steps and particle heights without vacuum, on insulators too.

Principle A laser reads the deflection of the cantilever carrying the tip, and the height is followed so that the tip–surface force stays constant.

Used for Surface shape and roughness Thickness of films and layers

Typical figures

Lateral resolution
2–150 nm (set by the tip radius)
Depth resolution / information depth
Height resolution 0.01 nm
Detection limit
—
Analyzed depth / volume
Surface only (scan up to about 90 µm square and 5 µm in height)
Elements
None
Quantitative accuracy
Height values depend on tip shape and scan conditions

Sample and effort

Size
Small pieces to wafers (some stages take 300 mm)
Conductivity
Not needed (insulators are fine)
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Minimal Almost none (keep the surface clean)
Time
Short Minutes to tens of minutes per site
Cost
Low Usually cheap on a shared university instrument

Pitfalls

  • The tip shape is convolved into the image: a blunt tip makes narrow trenches look shallower and narrower and bumps look wider
  • The field of view is small (up to about 90 µm). Survey with an optical microscope and pick a representative site
  • Steps above a few µm and very rough surfaces are a problem (use a laser confocal microscope or white-light interferometer)

Often combined with Laser confocal microscopy and white-light interferometry · SEM · Nanoindentation

Sources: EAG AFM; EAG technique chart; Penn State AFM

Measure the 3-D shape of a surface optically and without contact, and turn roughness, steps, wear-scar depth and indent shape into numbers.

Principle A laser confocal microscope picks up only in-focus light to find the height; a white-light interferometer finds the height where the interference fringes are strongest.

Used for Surface shape and roughness Thickness of films and layers Fracture surface

Typical figures

Lateral resolution
About 0.3–0.5 µm (lateral resolution is diffraction-limited, 0.61λ/NA: about 0.26 µm at 405 nm and NA 0.95; 0.5 µm in a white-light interferometer example)
Depth resolution / information depth
White-light interferometry 0.1 nm (phase mode) to 6 nm (scanning mode)
Detection limit
—
Analyzed depth / volume
Surface only (one field is mm-sized, stitched up to several cm)
Elements
None
Quantitative accuracy
Data drop out or go wrong on steep slopes and under transparent films

Sample and effort

Size
Small pieces to parts tens of cm across (depends on the stage)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Minimal Almost none
Time
Short Minutes per site
Cost
Low Usually cheap on a shared university instrument

Pitfalls

  • On steep or rough surfaces light does not return, leaving gaps or noise in the data
  • Under a transparent film, light returns from both the film surface and the interface, distorting the shape. Film thickness can be measured only for transparent films of known refractive index
  • Roughness values depend on the evaluation length or area and on the filter (cut-off). Use the same conditions when comparing

Often combined with AFM · OM · HV/HR/HBW

Sources: Evident laser microscope principles; EAG optical profilometry

Trace the surface with a diamond stylus to measure step heights (film thickness) and surface roughness, over long distances in one scan (up to 150 mm on one instrument).

Principle A stylus pressed on with a small force is moved across the surface, and its vertical motion is recorded as a surface profile.

Used for Surface shape and roughness Thickness of films and layers

Typical figures

Lateral resolution
Set by the stylus tip radius (2 µm for a standard stylus)
Depth resolution / information depth
Heights down to the ångström level (instrument example)
Detection limit
—
Analyzed depth / volume
The traced line
Elements
—
Quantitative accuracy
Valleys narrower than the stylus and steep slopes are rounded off by the stylus shape

Sample and effort

Size
Small pieces to plates on the stage; portable units measure on large parts (scan lengths up to 150 mm on one instrument)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive The stylus touches the surface (the force can be set low)
Preparation
Minimal Almost none (film thickness is measured at a step)
Time
Short
Cost
Low Cheap

Pitfalls

  • Features finer than the stylus tip (for example 2 µm) are not resolved; valleys come out shallow and peaks broad
  • Only one line is measured, so check variation by measuring several lines
  • Film thickness is measured as a step, so part of the film has to be removed to make one

Often combined with Laser confocal microscopy and white-light interferometry · AFM · Spectroscopic ellipsometry

Sources: Rochester profilometer

Shine X-rays at grazing angles on a thin film on a flat substrate and use the change of reflectivity with angle to obtain film thickness, density and interface width (roughness). For single and multilayer films about 1 nm to 1 µm thick.

Principle Reflectivity is measured from near the critical angle of total reflection upward, and thickness, density and interface width are found by fitting a curve calculated from a layer model.

Used for Thickness of films and layers Surface shape and roughness

Typical figures

Lateral resolution
— (average over the X-ray footprint, which must be laterally uniform)
Depth resolution / information depth
Films about 1 nm to 1 µm thick
Detection limit
—
Analyzed depth / volume
X-ray footprint × film
Elements
Elements are not measured directly (no chemical information)
Quantitative accuracy
A layer model (number and order of layers) is assumed for fitting, so a different model gives different values

Sample and effort

Size
Films on flat substrates (wafers, plates)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive (the film must not change during the measurement)
Preparation
Minimal Almost none (keep the surface clean)
Time
Moderate Measurement and model fitting take time
Cost
Moderate

Pitfalls

  • A substrate that is not flat, or a film that is laterally non-uniform within the footprint, cannot be analyzed
  • Surface contamination or reacted layers act as extra layers. Keep the surface clean before measuring
  • XRR alone gives no elements or chemical states. Combine with XPS or similar for composition

Often combined with Spectroscopic ellipsometry · XRD · XPS (ESCA)

Standards ISO 16413 (thickness, density and interface width of thin films by X-ray reflectometry)

Sources: ISO 16413; Diamond Light Source XRR

Measure the change in polarization of reflected light (Ψ and Δ) at many wavelengths to obtain thin-film thickness and optical constants such as refractive index, without contact or damage. Sensitive to sub-monolayer changes, and up to tens of µm for transparent films.

Principle Polarized light is reflected at an oblique angle and the change in polarization is measured. The data do not give thickness directly; a layer model with optical-constant dispersion formulas is fitted to them.

Used for Thickness of films and layers

Typical figures

Lateral resolution
— (average over the illuminated spot)
Depth resolution / information depth
Sensitive to sub-monolayer changes; about 0.5 nm to 20 µm for transparent films (instrument example)
Detection limit
—
Analyzed depth / volume
Illuminated spot × film
Elements
Elements are not measured (optical constants are)
Quantitative accuracy
A layer model and dispersion formulas are assumed for fitting, so a different model gives different values

Sample and effort

Size
Flat, reflective samples (wafers, glass plates, etc.)
Conductivity
Not needed (dielectric, organic, semiconductor and metal films)
Vacuum
Not needed
Destructive?
Non-destructive (no contact)
Preparation
Minimal Clean and dry the surface
Time
Short Each point is quick, but model fitting can take time
Cost
Moderate

Pitfalls

  • Thickness comes from fitting a model to Ψ and Δ, so wrong assumptions about the layers or optical constants give wrong values
  • Surfaces that are not flat or do not reflect light cannot be measured
  • Compare with XRR or cross-sections to check that the model is reasonable

Often combined with XRR · Stylus profilometer (roughness and step height) · SEM

Sources: Vanderbilt ellipsometer; J.C. Bose Univ. ellipsometer

Record X-ray radiographs while rotating the sample to see internal pores, cracks, inclusions and fiber orientation in 3-D without cutting.

Principle The X-ray attenuation at each point (set by density and atomic number) is reconstructed by computation from projections taken in many directions.

Used for Internal defects Microstructure on a section Thickness of films and layers Density and porosity

Typical figures

Lateral resolution
About 1/1000–1/2000 of the sample width (finer for smaller samples: µm for mm-sized samples; instruments reaching 0.1 µm exist)
Depth resolution / information depth
Same as lateral (3-D voxels)
Detection limit
— (small density differences are hard to see)
Analyzed depth / volume
The whole sample (mm to tens of cm, as far as X-rays penetrate)
Elements
None (attenuation contrast only)
Quantitative accuracy
Porosity and defect volume depend on how the image threshold is set

Sample and effort

Size
From a pellet of powder to large parts (resolution drops as size grows)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Minimal Almost none
Time
Moderate Hours to a day for scanning and reconstruction
Cost
Moderate Medium (instruments are less common)

Pitfalls

  • Resolution is set by sample size. A large part scanned whole will not show fine cracks; cut out a smaller piece if needed
  • Artifacts such as beam hardening (bright rim, dark center) mistaken for density differences
  • Closed cracks and phases of similar density are hard to distinguish

Often combined with RT · UT · SEM

Sources: SERC (Carleton College); EAG technique chart

Composition 12

Find out quickly which elements are present, and roughly how much, at a point, line or area hit by the electron beam in an SEM or TEM. Good for element maps.

Principle The beam knocks out inner-shell electrons, and a semiconductor detector sorts and counts the characteristic X-rays by energy.

Used for Local composition and element maps Average composition Precipitates Thickness of films and layers Composition versus depth

Typical figures

Lateral resolution
1 to a few µm in the SEM (set by the interaction volume); a few nm in a thin TEM foil
Depth resolution / information depth
1 to a few µm in the SEM
Detection limit
0.1–0.5 wt% (0.02–0.05 wt% reported under good conditions)
Analyzed depth / volume
µm-sized volume
Elements
Be–U (Be–F can be detected but are hard to quantify; H, He and Li cannot be measured)
Quantitative accuracy
A few percent relative for major elements on a flat polished surface against standards; standardless results carry larger errors and are semi-quantitative

Sample and effort

Size
Whatever fits the SEM chamber
Conductivity
Insulators need a carbon (or other) coating or low vacuum (semi-quantitative in low vacuum)
Vacuum
Normally vacuum
Destructive?
Non-destructive Surfaces can be measured as they are (quantification needs a polished surface; depth or layer thickness needs a cut section)
Preparation
Moderate Almost none for qualitative work; a flat polished surface for quantification
Time
Short Seconds to minutes per point; tens of minutes to hours per map
Cost
Low Cheap; usually fitted to the SEM

Pitfalls

  • Trusting quantified C, N and O. Light-element X-rays are strongly absorbed and their peaks change shape between compounds. C cannot be measured on carbon-coated samples, and O is often calculated rather than measured
  • Peak overlaps (S, Mo and Pb near 2.3 keV; Ti and Ba; Ti and V) lead to reporting elements that are not there
  • Spot analysis of particles or layers smaller than 1–2 µm also picks up the surroundings and the substrate
  • Rough fracture surfaces and loose powders do not give correct quantitative values (quantify on flat polished surfaces)

Often combined with WDS/EPMA · SEM · XPS (ESCA)

Standards ISO 22309 (quantitative EDS analysis of elements from Na upwards)

Terms EDS (energy-dispersive X-ray spectroscopy)

Sources: MyScope EDS; Newbury & Ritchie 2013; Microscopy Australia TechFi; Oxford Instruments (EDS vs WDS)

With about ten times the spectral resolution of EDS, quantify trace elements down to ~100 ppm and elements with overlapping peaks accurately against standards. Also used for line scans such as carbon profiles across case-hardened layers.

Principle Characteristic X-rays are Bragg-reflected by an analyzing crystal and counted wavelength by wavelength; each spectrometer measures one wavelength at a time.

Used for Local composition and element maps Average composition Trace elements and impurities Precipitates Thickness of films and layers Composition versus depth

Typical figures

Lateral resolution
1 to a few µm (set by the interaction volume)
Depth resolution / information depth
1 to a few µm
Detection limit
100–300 ppm (a few ppm under favourable conditions)
Analyzed depth / volume
µm-sized volume
Elements
Be (B on some instruments) to U. H, He and Li cannot be measured; errors grow for Be–O
Quantitative accuracy
0.5–1.5% relative for major elements (>1 wt%); standards are essential

Sample and effort

Size
Flat samples from a few hundred µm to about 50 mm (one facility's example)
Conductivity
Insulators are carbon coated
Vacuum
Required
Destructive?
Cut or polish Needs a flat polished surface
Preparation
Moderate Polish to a flat mirror finish and carbon coat
Time
Moderate Minutes per point; longer with many elements
Cost
Moderate Medium (fewer instruments)

Pitfalls

  • Without standards there is no accuracy. Calibrate with standards of similar composition
  • Oxidation states such as Fe²⁺ versus Fe³⁺ cannot be distinguished
  • Spectrometers scan one wavelength at a time, so many elements take long. Screen the elements with EDS first

Often combined with EDS (EDX) · XRF · XPS (ESCA)

Standards ISO 3887 (determining the depth of decarburization of steels)

Terms Carburizing

Sources: SERC (Carleton College); Univ. Arizona EPMA; Oxford Instruments (EDS vs WDS); ISO 3887

Determine elements from Na to U nondestructively and quickly from the fluorescent X-rays excited by an X-ray beam. Used for alloy sorting, plating composition and thickness, and powders or liquids.

Principle Primary X-rays eject inner-shell electrons, and the element-specific fluorescent X-rays emitted as the atoms relax are sorted by energy (ED) or wavelength (WD).

Used for Average composition Trace elements and impurities Thickness of films and layers Local composition and element maps

Typical figures

Lateral resolution
Usually an average over a mm-sized area (tens of µm with micro-XRF)
Depth resolution / information depth
A few µm to several mm (strongly dependent on the X-ray line and the matrix)
Detection limit
Around ppm (instrument and element dependent; worse for light elements)
Analyzed depth / volume
Irradiated area × information depth
Elements
Usually Na–U. WDXRF with multilayer analyzers also reaches Be–O (including C, N and O), but sensitivity and accuracy drop for elements lighter than Na (H and Li cannot be measured; handheld units cannot measure elements lighter than Mg)
Quantitative accuracy
Accurate when calibrated with standards of similar composition; standardless fundamental-parameter results are convenient but can carry large errors in some matrices

Sample and effort

Size
Powders and liquids to large parts (large parts with a handheld unit on site)
Conductivity
Not needed
Vacuum
Not needed (vacuum or helium improves light-element sensitivity)
Destructive?
Non-destructive
Preparation
Minimal Measured as is; fused beads or pressed pellets for better accuracy
Time
Short Minutes
Cost
Low Cheap

Pitfalls

  • Reading the composition of plating, oxide, paint or dirt as that of the base metal. The information depth ranges from a few µm to several mm depending on the element
  • Matrix effects change the intensities, so values are off unless calibrated with standards of similar composition
  • Light elements (lighter than Na) lose sensitivity and accuracy even with WDXRF and are not measured by ED or handheld units. Use combustion analysis for C in steel

Often combined with ICP-OES / ICP-MS · EDS (EDX) · GD-OES

Standards ISO 3497 (coating thickness by X-ray spectrometry)

Sources: SERC (Carleton College); HORIBA XRF; Evident handheld XRF; EAG technique chart; Rigaku multilayer analyzers

Dissolve the sample in acid and feed the solution into a hot plasma to quantify about 70 elements: down to ppm in the solid with ICP-OES and ppb with ICP-MS. The standard route to average composition and trace impurities.

Principle A hot argon plasma excites and ionizes the atoms; elements are sorted by emission wavelength (OES) or ion mass (MS).

Used for Average composition Trace elements and impurities

Typical figures

Lateral resolution
— (average of all the dissolved material)
Depth resolution / information depth
—
Detection limit
About 1 ppm in the solid for ICP-OES and 10 ppb for ICP-MS (solution limits multiplied by the dissolution and dilution factor; interferences make them an order of magnitude worse or more)
Analyzed depth / volume
All the dissolved material (one facility asks for at least 1 g of solid)
Elements
About 70 elements. ICP-OES cannot measure C, N, O, halogens, noble gases or H (one facility's list)
Quantitative accuracy
Uncertainty of 5% or less (20% or less near the limit) in one facility's example

Sample and effort

Size
Powder, chips or small pieces (cut from large parts)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Destroys the sample Consumed by dissolution
Preparation
Extensive Dissolve completely in acid (HF or fusion for refractory materials). Laborious
Time
Moderate Hours to a day to dissolve; weeks to a month if outsourced
Cost
Moderate Medium (often outsourced)

Pitfalls

  • Losing elements through undissolved residue or volatilization. Complete dissolution is assumed
  • Spectral overlaps (OES) and polyatomic ions (MS) produce false or inflated results
  • Taking the solution detection limit as the limit in the solid (multiply by the dilution factor)
  • No information on spatial distribution (segregation, surface layers)

Often combined with XRF · Combustion and inert gas fusion analysis (C, S, O, N, H) · GD-OES

Sources: PSI ICP-OES; EAG ICP; EAG technique chart

Quantify C and S (combustion) and O, N and H (inert gas fusion) in metals quickly, down to ppm levels. Used for carbon in steel, oxygen and hydrogen in titanium, hydrogen in weld metal and so on.

Principle Combustion burns the sample in oxygen and measures the CO₂ and SO₂ by infrared absorption. Inert gas fusion melts the sample in a graphite crucible and measures the CO (from O), N₂ and H₂ by infrared absorption or thermal conductivity.

Used for Average composition Trace elements and impurities

Typical figures

Lateral resolution
— (average of the whole sample)
Depth resolution / information depth
—
Detection limit
From about 0.1 ppm (element and instrument dependent)
Analyzed depth / volume
The whole sample burned or fused
Elements
C, S, O, N and H only
Quantitative accuracy
Calibrated with reference materials

Sample and effort

Size
Chips or small pieces (cut from large parts)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Destroys the sample Consumed by burning or fusion
Preparation
Moderate Cut to a set size and remove surface contamination
Time
Short Minutes per sample
Cost
Moderate Medium (fewer instruments, but analysis is fast)

Pitfalls

  • Diffusible hydrogen escapes quickly even at room temperature. In weld metal the value falls the longer the delay (about 20% between 20 s and 300 s before quenching in liquid nitrogen in one study), so keep samples cold
  • Total hydrogen (fusion) and diffusible hydrogen released on heating are different quantities. State which was measured
  • No spatial information (segregation, decarburized or carburized layers). Use EPMA, GD-OES or hardness profiles on a section

Often combined with Spark OES · ICP-OES / ICP-MS · GD-OES

Standards ASTM E1019 (C, S, N and O in steel, iron, Ni and Co alloys) / ASTM E1447 (H in reactive metals such as Ti and Zr) / ISO 3690 (diffusible hydrogen in weld metal)

Sources: ASTM E1019; ASTM E1447; Klett et al. 2020; EAG technique chart

Fire a spark between a metal sample and an electrode and use the emitted light to determine many elements at once, including C, N, P, S and B. Used for composition control of steels, cast irons and nonferrous metals.

Principle A spark discharge in argon vaporizes and excites the sample surface, and the intensities of element-specific emission lines are measured. Lines of C, N, P and S lie in the vacuum ultraviolet, which air absorbs, so the spectrometer is evacuated.

Used for Average composition Trace elements and impurities

Typical figures

Lateral resolution
— (average over the spark spot)
Depth resolution / information depth
—
Detection limit
Below 10 ppm for some elements (instrument examples: below 10 ppm for B and Pb, below 1 ppm for Zn)
Analyzed depth / volume
Spark spot × surface layer
Elements
Many elements in metals, including C, N, P, S and B. N needs a capable instrument; use gas analysis for O and H (some instruments handle O in copper and H in titanium alloys)
Quantitative accuracy
Calibrated with standards of similar composition (prepared the same way)

Sample and effort

Size
Metal pieces that can be ground flat and cover the spark stand opening
Conductivity
Conductive metals only (the sample is an electrode)
Vacuum
Not needed (the sample is in argon; the spectrometer is evacuated)
Destructive?
Cut or polish Leaves a spark mark; the surface is ground
Preparation
Moderate Grind the surface flat and keep it clean; spark on sound metal without pores or pits
Time
Short Each measurement is quick
Cost
Low Cheap

Pitfalls

  • Sparking on pores or pits changes the discharge and gives wrong values. Grind and measure sound metal
  • Touching or contaminating the ground surface changes the result. Keep it clean after grinding
  • If standards are not prepared the same way as samples, the calibration does not match

Often combined with Combustion and inert gas fusion analysis (C, S, O, N, H) · XRF · ICP-OES / ICP-MS

Standards ASTM E415 (spark atomic emission analysis of carbon and low-alloy steel)

Sources: ASTM E415; Hitachi High-Tech OES

Sputter the surface with a glow discharge while recording the emitted light to obtain composition depth profiles from nm to about 100 µm (plating, nitrided layers, oxides, paint) for almost all elements including H, in a short time.

Principle An argon glow discharge with the sample as cathode sputters surface atoms; their emission in the plasma is dispersed and recorded element by element against time (= depth).

Used for Composition versus depth Thickness of films and layers Average composition Trace elements and impurities

Typical figures

Lateral resolution
— (average over a circle a few mm across; no lateral mapping)
Depth resolution / information depth
About 10% of the depth (for layers thicker than 10 nm)
Detection limit
1–100 ppm (element and matrix dependent)
Analyzed depth / volume
Sputtered circle × depth (nm to about 100 µm; over 150 µm reported)
Elements
Almost all elements including H, C, N and O
Quantitative accuracy
Calibrated with standards (matrix-independent calibration is possible)

Sample and effort

Size
Pieces or sheets with a flat area larger than 4 mm across
Conductivity
Not needed (RF discharge for insulators)
Vacuum
No high vacuum, but the sample face is exposed to low-pressure argon
Destructive?
Cut or polish Leaves a sputter crater
Preparation
Minimal None if there is a flat surface
Time
Short Minutes per measurement
Cost
Moderate Medium (fewer instruments)

Pitfalls

  • Depth resolution is about 10% of the depth, so deeper interfaces look broader. Do not mistake the interface width for a diffusion width
  • Laterally everything is averaged: islands, local precipitates or non-uniform layers are not seen (laterally uniform layers are assumed)
  • Converting time to depth needs the sputter rate (material dependent) and a measured crater depth

Often combined with XPS (ESCA) · SIMS · ICP-OES / ICP-MS

Standards ISO 3887 (determining the depth of decarburization of steels)

Terms Nitriding Carburizing

Sources: IFW Dresden GD-OES; HORIBA GD-OES; ISO 3887

Heat the sample at a constant rate and measure the hydrogen released at each temperature. Used to find how much hydrogen a steel contains and where (in which traps) it is held.

Principle The sample is heated and the released hydrogen is measured, either with a mass spectrometer in vacuum (TDS) or carried by argon to a gas chromatograph (TDA). Changing the heating rate shifts the desorption peak temperatures, and the shift gives the binding energy of each trap.

Used for Average composition

Typical figures

Lateral resolution
— (whole sample)
Depth resolution / information depth
—
Detection limit
About 1 wt ppm (about 50 atomic ppm) in steel with one instrument
Analyzed depth / volume
The whole sample
Elements
Hydrogen
Quantitative accuracy
Hydrogen held in different ways is separated by the desorption curve (peaks) versus temperature

Sample and effort

Size
Small pieces (cut out)
Conductivity
Not needed
Vacuum
Depends on the setup (TDS in vacuum; gas-chromatograph TDA in a furnace with flowing argon)
Destructive?
Cut or polish Cut out; heating drives the hydrogen out
Preparation
Extensive Keep hydrogen-charged samples in liquid nitrogen until measurement so the hydrogen stays in
Time
Moderate (longer with slow heating)
Cost
Moderate (few instruments)

Pitfalls

  • Water adsorbed on the surface also gives a hydrogen peak (a peak near 350 °C after about a minute in laboratory air was reported). Decide how samples are handled
  • Diffusible hydrogen escapes even at room temperature. Keep samples cold between charging and measurement
  • In thin cut samples, surface working and condition shift the peak temperatures (cutting reduced the measured hydrogen in one report)

Often combined with Combustion and inert gas fusion analysis (C, S, O, N, H) · SIMS · SEM

Sources: Tapia-Bastidas et al. (TDS); AIST HYDROGENIUS (TDS); Enomoto & Hirakami 2015 (ISIJ Int.)

Identify the elements within a few nm of the surface and their chemical state (metal or oxide, bonding partner). The standard tool for passive films, contamination and plating adhesion failures.

Principle The kinetic energy of photoelectrons ejected by X-rays gives their binding energy, which identifies the element and shifts slightly with chemical state (chemical shift).

Used for Chemical state (oxidation state, bonding) Composition versus depth Thickness of films and layers Organics, polymers and contamination

Typical figures

Lateral resolution
10 µm to 2 mm (instrument dependent; smallest analysis areas of about 30–100 µm reported)
Depth resolution / information depth
Top 1–10 nm
Detection limit
About 0.1 at% (0.1–1 at%)
Analyzed depth / volume
Tens of µm to mm across × a few nm
Elements
Li–U (H and He cannot be measured)
Quantitative accuracy
Mostly semi-quantitative with sensitivity factors. In sputter depth profiles, sputtering can change the chemical state

Sample and effort

Size
Small pieces that fit the instrument (some take wafers)
Conductivity
Not needed (insulators are fine)
Vacuum
Required (ultra-high vacuum compatible)
Destructive?
Non-destructive for surface analysis; depth profiling sputters
Preparation
Minimal Almost none (do not touch or contaminate the surface)
Time
Moderate Hours per sample
Cost
Moderate Medium (fewer instruments)

Pitfalls

  • It sees only the top few nm, so adventitious carbon and native oxide from air are easily mistaken for the composition of the material
  • Ion sputtering during depth profiling changes chemical states (for example by reduction). Do not over-trust states deep in the profile
  • Elements below about 0.1 at% are not seen

Often combined with AES · SIMS · GD-OES

Terms XPS (X-ray photoelectron spectroscopy) Passivity

Sources: EAG XPS; VUB SURF XPS

Analyze the elements in the top few nm at a chosen spot with an electron beam focused to 10–20 nm. Used for tiny particles, grain-boundary segregation and depth profiles of thin films.

Principle Elements are identified by the energy of Auger electrons emitted by atoms excited by the beam. Auger electrons can escape only from the top few nm.

Used for Composition versus depth Local composition and element maps Precipitates

Typical figures

Lateral resolution
10 nm and above (beam can be focused to 10–20 nm)
Depth resolution / information depth
Top 3–10 nm; 2–20 nm in depth profiles
Detection limit
0.1–5 at% (element and instrument dependent)
Analyzed depth / volume
A ~10 nm spot × a few nm
Elements
All except H and He
Quantitative accuracy
Semi-quantitative with sensitivity factors (better against samples of known composition)

Sample and effort

Size
Small pieces that fit the instrument (some take 300 mm wafers)
Conductivity
Insulators charge and are difficult
Vacuum
Required
Destructive?
Non-destructive for surface analysis; depth profiling sputters
Preparation
Minimal Almost none
Time
Moderate Hours per sample
Cost
Moderate Medium (fewer instruments)

Pitfalls

  • Insulators charge and are hard to analyze (use XPS for chemical states of insulating surfaces)
  • Little chemical-state information (use XPS if you need the state)
  • Elements below 0.1–1 at% are not seen

Often combined with XPS (ESCA) · SEM · SIMS

Sources: EAG AES; KIT KNMFi AES

Sputter the surface with ions and mass-analyze the secondary ions to obtain depth profiles of dopants and impurities below ppm levels (10¹⁰–10¹⁶ atoms/cm³).

Principle A primary ion beam (O₂⁺, Cs⁺ etc.) erodes the sample and the ejected ions are counted isotope by isotope in a mass spectrometer.

Used for Composition versus depth Trace elements and impurities Local composition and element maps

Typical figures

Lateral resolution
Depth profiles over areas of 10 µm and above; about 1 µm in imaging
Depth resolution / information depth
From about 0.5 nm (a few Å)
Detection limit
10¹⁰–10¹⁶ atoms/cm³ (ppm and below)
Analyzed depth / volume
µm to hundreds of µm across × depth (a few Å to tens of µm)
Elements
H–U including isotopes (adsorbed water and hydrocarbons give a hydrogen background, suppressed by ultra-high vacuum and cryogenic trapping)
Quantitative accuracy
Concentrations require standards (for example ion-implanted samples)

Sample and effort

Size
Small pieces that fit the instrument
Conductivity
Insulators charge up, so charge compensation with an electron beam is needed (instrument dependent)
Vacuum
Required (vacuum-compatible solids)
Destructive?
Cut or polish Leaves a crater (destructive)
Preparation
Minimal Almost none
Time
Moderate Hours per sample
Cost
High (often outsourced)

Pitfalls

  • Without standards there are no concentrations. Calibrate with standards in the same matrix (ion-implanted samples etc.)
  • Destructive: the crater remains and the spot cannot be reused
  • No chemical bonding information (use XPS for bonding)

Often combined with XPS (ESCA) · APT · GD-OES

Terms SIMS (secondary ion mass spectrometry)

Sources: EAG SIMS; CAMECA SIMS on insulators; CAMECA hydrogen by SIMS

Field-evaporate atoms one by one from a needle-shaped specimen and reconstruct in 3-D which atom was where. Used for the composition of nm-sized precipitates, clusters and grain-boundary segregation.

Principle A needle cooled to 25–80 K is held at high voltage, and voltage or laser pulses ionize surface atoms; time of flight gives the mass and the detector position gives the original location.

Used for Precipitates Local composition and element maps Trace elements and impurities

Typical figures

Lateral resolution
0.5 nm lateral and 0.3 nm in depth in metals (about 1 nm in semiconductors and insulators)
Depth resolution / information depth
0.3 nm
Detection limit
About 10 ppm
Analyzed depth / volume
About 50 nm square × 100–500 nm deep
Elements
H–U (residual hydrogen in the analysis chamber gives a background, so deuterium is sometimes used to tell them apart)
Quantitative accuracy
Accuracy drops for elements with overlapping mass peaks

Sample and effort

Size
A needle with apex radius below 100 nm (made by FIB etc.)
Conductivity
Voltage pulsing for conductors, laser pulsing for semiconductors and insulators
Vacuum
Required (cryogenic, ultra-high vacuum)
Destructive?
Cut or polish The part made into a needle is destroyed
Preparation
Extensive Needles made by FIB etc. (hours each). Needs skill
Time
Long Days to weeks including preparation
Cost
High (few instruments)

Pitfalls

  • The analyzed volume is tiny (50 nm square × a few hundred nm). Choose the site with TEM or SEM before making the needle
  • Needles can fracture in the high field before the run is finished (material dependent)
  • Position and composition accuracy degrade at interfaces and in complex geometries

Often combined with TEM/STEM · FIB · SIMS

Terms Precipitation hardening

Sources: EAG APT; Khanchandani et al. (H in APT)

Crystal structure 4

Identify crystalline phases and measure lattice parameters, crystallite size, strain and crystallinity on powders, plates and thin films as they are, in a short time.

Principle The positions and intensities of the diffracted beams that satisfy the Bragg condition (2d sinθ = λ) are matched against database (ICDD) patterns.

Used for Phase identification and crystal structure Grain size, orientation and texture Precipitates

Typical figures

Lateral resolution
Usually an average over 0.1 to several mm (20–25 µm with micro-diffraction)
Depth resolution / information depth
The 1/e attenuation depth of Cu Kα X-rays is about 4 µm in iron, 70 µm in Al and 3 mm in polyethylene (calculated from NIST attenuation coefficients); a few nm at grazing incidence
Detection limit
A minor phase from about 1%
Analyzed depth / volume
Irradiated area × X-ray penetration depth (varies greatly with material)
Elements
Elements are not measured directly (seen as crystalline phases)
Quantitative accuracy
Phase fractions are approximate (phases below about 1% are missed)

Sample and effort

Size
Sub-milligram powders to plates and parts that fit the stage
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Minimal Almost none (pack powders flat)
Time
Short Minutes to an hour per sample
Cost
Low Cheap (common in universities)

Pitfalls

  • Confusing Scherrer "crystallite size" with grain or particle size. One particle can contain many crystallites. Above about 100 nm the estimate is unreliable, and instrumental broadening must be corrected and strain broadening separated
  • Amorphous phases give no peaks and cannot be identified
  • Phases below about 1% are missed
  • Powder packing or rolling texture changes intensity ratios so that patterns do not match the database

Often combined with XRD (sin²ψ, pole figures) · SAED/CBED · TEM/STEM

Terms XRD (X-ray diffraction) Bragg's law Scherrer equation Extinction rules

Sources: EAG XRD; Rigaku crystallite size; NIST X-ray attenuation

Measure near-surface residual stress from the shift of a diffraction peak (lattice spacing) while tilting the sample, and texture (pole figures) from the diffracted intensity as the orientation is changed.

Principle In the sin²ψ method the spacing d is measured at several tilts ψ; stress follows from the slope of d against sin²ψ and the elastic constants of the measured plane.

Used for Residual stress Grain size, orientation and texture

Typical figures

Lateral resolution
Average over the irradiated area (0.1 to several mm)
Depth resolution / information depth
Average over a few to tens of µm from the surface (5–50 µm in most materials; Cr Kα is used for steel). Deeper levels are measured after removing layers by electropolishing
Detection limit
—
Analyzed depth / volume
Irradiated area × a few to tens of µm
Elements
—
Quantitative accuracy
Coarse grains mean few diffracting grains and poorer precision (10–100 µm grains are fine)

Sample and effort

Size
Pieces to parts that fit the stage (portable instruments for large structures)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive (layers are removed by electropolishing for depth profiles)
Preparation
Minimal Measure the as-received surface; do not grind or polish
Time
Moderate Tens of minutes to hours per point
Cost
Moderate Medium

Pitfalls

  • Grinding, machining or wire brushing adds surface stress. Measure as received, and remove layers only by electropolishing or chemical attack
  • It gives the stress within a few to tens of µm of the surface, not in the interior (use neutron diffraction for the interior)
  • Texture or coarse grains make d versus sin²ψ non-linear; taking a slope regardless gives wrong values
  • Use the elastic constants of the measured plane (X-ray elastic constants), not bulk values

Often combined with ND · XRD · EBSD

Standards ASTM E2860 (residual stress by XRD in bearing steels) / ASTM E81 (preparing quantitative pole figures)

Sources: NPL GPG 52; EAG XRD

Determine crystal structure, orientation and orientation relationships from a selected region of nm to a few hundred nm inside the TEM. Identifies the phase of a single precipitate.

Principle The diffraction pattern of electrons transmitted through the specimen is recorded. Selected-area diffraction (SAED) chooses the region with an aperture; convergent-beam diffraction (CBED) takes the pattern from a finely focused probe.

Used for Phase identification and crystal structure Precipitates Grain size, orientation and texture

Typical figures

Lateral resolution
SAED about 250 nm (set by the aperture); CBED a few nm
Depth resolution / information depth
The whole specimen thickness (<100 nm)
Detection limit
—
Analyzed depth / volume
A small region of a thin foil
Elements
— (use EDS or EELS for composition)
Quantitative accuracy
Lattice spacings are usually accurate to 1–3% (0.1% with careful calibration), poorer than XRD

Sample and effort

Size
TEM foils
Conductivity
Not needed (thinning is what matters)
Vacuum
Required
Destructive?
Cut or polish Destroys the part made into a foil
Preparation
Extensive As for TEM (make a foil)
Time
Long Days to weeks including preparation
Cost
High (often outsourced)

Pitfalls

  • Spacings are good to about 1–3%. Use XRD for precise lattice parameters
  • Errors in camera length (which changes with specimen height) shift d. Calibrate with a standard
  • The selected region is small, so phase fractions of the whole sample are unknown

Often combined with TEM/STEM · XRD · EBSD

Terms Extinction rules

Sources: Univ. Duisburg-Essen ICAN; Czigány & Kis 2023

Because neutrons penetrate deep into metals, map residual stress inside components and study crystal structures containing light elements such as H and Li, and magnetic structures.

Principle Neutrons are scattered by nuclei. Scattering strength does not follow atomic number, so light elements that X-rays barely see, and isotopes of the same element, can be distinguished.

Used for Residual stress Phase identification and crystal structure Grain size, orientation and texture

Typical figures

Lateral resolution
Gauge volume about 1–10 mm³
Depth resolution / information depth
Same (mm scale)
Detection limit
—
Analyzed depth / volume
Total path length up to about 60 mm in steel and 100 mm in Al
Elements
Light elements (H) and isotopes are easy to distinguish
Quantitative accuracy
Stress accuracy about 10 MPa in Al and 30 MPa in steel in one example

Sample and effort

Size
Small pieces to large parts
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive (a stress-free reference may be cut out)
Preparation
Minimal Prepare a stress-free reference (d₀)
Time
Long Months from beam-time proposal; days of measurement
Cost
High (reactor or spallation facilities)

Pitfalls

  • A stress-free reference (d₀) is required, and how it is prepared changes the result a lot
  • Only possible at large facilities (reactors, accelerators), with long lead times from proposal to measurement
  • The near-surface region (tens of µm) is hard to resolve with mm-sized gauge volumes (use XRD for the surface)

Often combined with XRD (sin²ψ, pole figures) · CT

Standards ISO 21432 (residual stress by neutron diffraction)

Sources: NIST NCNR; Veqter neutron diffraction

Thermal 5

Measure the temperatures and heats of melting, crystallization, glass transition, precipitation and phase transformations while heating or cooling at a constant rate. Used for glass transitions and crystallinity of polymers and transformation temperatures of alloys.

Principle DTA records the temperature difference between sample and reference, DSC the difference in heat flow. After calibration, DSC peak areas give heats.

Used for Transition temperatures and reactions Organics, polymers and contamination Precipitates

Typical figures

Lateral resolution
— (whole sample)
Depth resolution / information depth
—
Detection limit
DSC is more sensitive than DTA, so weak events such as glass transitions are easier to see
Analyzed depth / volume
All of a small sample
Elements
—
Quantitative accuracy
Quantitative heats with DSC; DTA suits high temperatures (above 800 °C) and mainly gives temperatures

Sample and effort

Size
Small pieces or powder that fit the pan (cut from larger items)
Conductivity
Not needed
Vacuum
Not needed (usually under flowing inert gas)
Destructive?
Destroys the sample A small piece is cut and altered by heating
Preparation
Moderate Cut a small piece and seal it in a pan
Time
Short One to a few hours per run
Cost
Low Cheap (common in universities)

Pitfalls

  • Transition temperatures shift with heating rate. Compare samples at the same rate, and go slower for accurate values
  • Decomposition or evaporation overlapping a transition spoils the heat (use only while the sample mass is constant)
  • Solid-state transformations in metals can release little heat and be missed (combine with dilatometry)

Often combined with TGA · Dilatometry · DMA

Terms Glass transition temperature Crystallinity Precipitation hardening

Sources: EAG DSC; Bhadeshia (Cambridge); Labcompare (DSC vs DTA)

Record the change in sample mass on heating to find moisture and volatiles, decomposition temperatures, filler content and weight gain from oxidation.

Principle The sample sits on a balance in a furnace and its mass is logged in inert or oxidizing gas.

Used for Decomposition, moisture and filler content (mass change on heating) Transition temperatures and reactions Organics, polymers and contamination

Typical figures

Lateral resolution
— (whole sample)
Depth resolution / information depth
—
Detection limit
Mass changes below a microgram (instrument example; samples of about 1–150 mg)
Analyzed depth / volume
The whole sample (up to about 1 g in one example)
Elements
—
Quantitative accuracy
Weighing precision ±0.01% in one example

Sample and effort

Size
Small pieces or powder that fit the pan
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Destroys the sample A small piece is cut and altered by heating
Preparation
Moderate Cut a small piece and place it in the pan
Time
Short One to a few hours per run
Cost
Low Cheap

Pitfalls

  • It does not say what was lost. Identify evolved gases with TGA-MS or TGA-FTIR
  • Results depend on the atmosphere (inert or air); weight gain by oxidation and loss by decomposition can overlap

Often combined with DSC/DTA · FTIR

Terms Parabolic rate law

Sources: EAG TGA; UW–Madison WCNT TGA

Record the change in length while changing temperature to obtain the thermal expansion coefficient, transformation temperatures of steels (Ac₁, Ac₃, Ms etc.) and sintering shrinkage.

Principle The extension of a rod specimen is transmitted by a push rod to a displacement sensor outside the furnace. Phase transformations change the volume, so the curve bends.

Used for Transition temperatures and reactions Thermal expansion and conduction

Typical figures

Lateral resolution
— (whole sample)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
The whole rod specimen
Elements
—
Quantitative accuracy
Transformation temperatures and fractions are fixed by combining the curve with metallography

Sample and effort

Size
Rods mm to cm long (machined)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Cut or polish A specimen is machined out
Preparation
Moderate Machine a rod of set shape
Time
Moderate A few hours per run (depends on the thermal cycle)
Cost
Moderate Medium

Pitfalls

  • Transformation temperatures change with heating and cooling rates (and differ between continuous cooling and isothermal holding). State the conditions when comparing
  • Do not identify phases from kinks in the curve alone. Confirm with metallography
  • Rolled and composite materials expand differently in different directions. Record the specimen orientation

Often combined with DSC/DTA · OM · LFA

Standards ASTM E228 (linear thermal expansion with a push-rod dilatometer) / ASTM A1033 (phase transformations of hypoeutectoid carbon and low-alloy steels)

Terms Coefficient of linear thermal expansion Martensite

Sources: ASTM A1033

Heat the front of a thin disk with a light pulse and obtain thermal diffusivity from how fast the rear face warms up; multiply by specific heat and density for thermal conductivity.

Principle An infrared detector records the rear-face temperature rise, and diffusivity is calculated from the thickness and the time to reach a set fraction of the maximum rise.

Used for Thermal expansion and conduction

Typical figures

Lateral resolution
— (through-thickness value of the whole disk)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
The whole disk
Elements
—
Quantitative accuracy
Conductivity is diffusivity times specific heat and density, so it carries their errors too

Sample and effort

Size
Small pieces that can be machined into disks
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Cut or polish Machined into a disk
Preparation
Moderate Machine a disk; usually spray with graphite
Time
Moderate Minutes per temperature; hours for a temperature series
Cost
Moderate Medium

Pitfalls

  • Translucent polymers and glasses, and shiny metals, need a graphite coating to be measured correctly. Too much graphite lowers the value for highly conductive Cu and Al (4% with a ~5 µm layer in one example)
  • Homogeneous, isotropic, opaque samples are assumed. Analyze layered or anisotropic materials with their orientation and structure in mind
  • Conductivity = diffusivity × specific heat × density, so errors in specific heat and density go straight into it

Often combined with Dilatometry · DSC/DTA

Standards ASTM E1461 (thermal diffusivity by the flash method)

Terms Thermal diffusivity

Sources: ASTM E1461; NETZSCH AN 066

Apply a small oscillating deformation while changing temperature to measure storage modulus, loss modulus and tan δ. Detects the glass transition of polymers more sensitively than DSC.

Principle The phase lag between oscillating force and deformation separates the elastic (E′) and viscous (E″) components. Tg is taken as the onset of the E′ drop, the E″ peak or the tan δ peak.

Used for Transition temperatures and reactions

Typical figures

Lateral resolution
— (whole specimen)
Depth resolution / information depth
—
Detection limit
— (transitions hard to see by DSC are often clearer)
Analyzed depth / volume
The whole specimen
Elements
—
Quantitative accuracy
Tg depends on the definition (E′ onset < E″ peak < tan δ peak) and on frequency. Use the same definition and frequency when comparing

Sample and effort

Size
Bars or strips (held in clamps)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Cut or polish A specimen is cut
Preparation
Moderate Cut flat, untwisted bars or strips
Time
Moderate (longer with slow heating)
Cost
Moderate

Pitfalls

  • Tg differs between definitions (E′ onset, E″ peak, tan δ peak). State which was used
  • Higher frequencies give higher Tg. Compare at the same frequency
  • Heating thick specimens fast makes the specimen temperature lag. Heat thick specimens slowly

Often combined with DSC/DTA · TGA · Tensile testing

Standards ASTM E1640 (assignment of the glass transition temperature by DMA)

Terms Glass transition temperature Thermosetting resin

Sources: TA Instruments DMA

Mechanical 6

Pull a specimen to measure Young's modulus, the yield point or 0.2% proof stress, tensile strength, elongation and reduction of area. The basic strength values of a material.

Principle The specimen is pulled at a constant rate while force and extension (extensometer) are recorded to give the engineering stress–strain curve.

Used for Hardness, strength and ductility

Typical figures

Lateral resolution
— (whole gauge length)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
The gauge section
Elements
—
Quantitative accuracy
Elongation depends on specimen shape and gauge length, so compare like specimens

Sample and effort

Size
Enough material to machine a standard specimen (small specimens exist)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Destroys the sample Broken
Preparation
Extensive Machine a specimen of standard shape
Time
Moderate Minutes to tens of minutes per specimen (days to machine specimens)
Cost
Low Cheap (common in universities)

Pitfalls

  • Confusing the (upper) yield point with the 0.2% proof stress. Use proof stress when there is no distinct yield point
  • Reading the fall in engineering stress after necking as weakening of the material (the cross-section is shrinking; look at true stress)
  • Elongation depends on specimen shape and gauge length. Do not compare elongations of different specimen types directly

Often combined with HV/HR/HBW · Charpy impact testing · SEM

Standards JIS Z 2241 (tensile testing of metallic materials) / ISO 6892-1 (tensile testing of metallic materials at room temperature)

Terms 0.2% offset yield strength Young's modulus Work hardening

Sources: TWI tensile testing; Princeton MAE 324 necking

Measure hardness from the size or depth of an indent. Quick, possible on finished parts, and used for hardness profiles through heat treatments, case-hardened layers and welds.

Principle Vickers uses the diagonals of the indent of a square diamond pyramid, Brinell the diameter of a ball indent, and Rockwell the depth of a cone or ball indent.

Used for Hardness, strength and ductility Thickness of films and layers

Typical figures

Lateral resolution
Set by the indent size (for example, about 30 µm diagonal at 0.98 N in a 200 HV steel)
Depth resolution / information depth
Indent depth and its surroundings
Detection limit
—
Analyzed depth / volume
A small volume around the indent
Elements
—
Quantitative accuracy
Conversions between scales and to tensile strength are approximate and limited to tables for specific materials

Sample and effort

Size
Small pieces to parts (Rockwell or portable testers on finished parts)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive Leaves a small indent (portable testers measure parts as they are). Hardness profiles through layers need a cut section
Preparation
Moderate A polished surface for micro-Vickers; a flat surface for Rockwell and Brinell
Time
Short Tens of seconds to minutes per indent
Cost
Low Cheap

Pitfalls

  • Indents too close to each other or to an edge give wrong values because of work hardening around earlier indents or lack of support. Keep the spacings set by the standard
  • On thin samples or thin layers the anvil or substrate shows through. Respect the minimum thickness in the standard, and use nanoindentation for thin films
  • Conversions between HV, HRC and HB and to tensile strength are approximate; use only tables matching the material and heat treatment

Often combined with Tensile testing · Nanoindentation · OM

Standards JIS Z 2244-1 (Vickers hardness test) / JIS Z 2245 (Rockwell hardness test) / JIS Z 2243-1 (Brinell hardness test) / ASTM E92 (Vickers and Knoop hardness) / ASTM E110 (Rockwell and Brinell hardness by portable testers) / ASTM E140 (hardness conversion tables) / ISO 3887 (determining the depth of decarburization of steels)

Terms Work hardening Hardenability Carburizing Nitriding

Sources: Instron TechNotes 35; ASTM E140; ISO 3887; ASTM E110

Record force and depth continuously while indenting to nm–µm depths, and obtain hardness and Young's modulus of thin films, small phases and surface layers.

Principle From the load–depth curves on loading and unloading, the contact area and the initial unloading slope (contact stiffness) are found and hardness and modulus are calculated.

Used for Hardness, strength and ductility

Typical figures

Lateral resolution
Positioning below 50 nm (indents need µm spacing)
Depth resolution / information depth
Displacement noise below 0.1 nm, up to about 20 µm
Detection limit
—
Analyzed depth / volume
A small volume around the indent
Elements
—
Quantitative accuracy
Indenting shallower than 10–20% of the film thickness is the usual rule, but for a hard film on a soft substrate the substrate shows through even at 5%

Sample and effort

Size
Small pieces to wafers
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Cut or polish Leaves a small indent
Preparation
Moderate Flat, smooth surface (roughness scatters the values)
Time
Short Minutes per indent; hours for a map
Cost
Moderate Medium

Pitfalls

  • Substrate properties mix into the film value. For a hard film on a soft substrate the substrate shows through even at shallow depths
  • Rough surfaces and films thinner than 10 nm give semi-quantitative values only
  • Indentation hardness (instrumented) and Vickers hardness are defined differently. Do not compare the numbers directly

Often combined with HV/HR/HBW · AFM · SEM

Standards ISO 14577-1 (instrumented indentation test for hardness and materials parameters)

Terms Young's modulus

Sources: EAG nanoindentation; Chen & Vlassak 2000

Break a notched specimen with one swing of a pendulum and compare toughness (whether it fails in a brittle way) by the absorbed energy. Tests at several temperatures reveal the ductile–brittle transition.

Principle The energy used to break the specimen is found from the difference between the height the pendulum is raised to and the height it swings up to afterwards.

Used for Toughness, fatigue and creep

Typical figures

Lateral resolution
— (whole specimen)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
Around the notch
Elements
—
Quantitative accuracy
Values scatter even at one temperature, so several specimens are averaged. Values are for comparison with specifications and cannot be converted into fracture toughness

Sample and effort

Size
Enough material to machine a standard specimen
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Destroys the sample Broken
Preparation
Extensive Machine to standard shape, cut the notch, condition to temperature
Time
Moderate Minutes per specimen (days to machine and condition specimens)
Cost
Low Cheap

Pitfalls

  • Using absorbed energy as a fracture toughness for design. Results are for comparison with each other or with a specification
  • Comparing at one temperature only. In the transition region small temperature differences change the value greatly, so test at several temperatures and draw the curve
  • Also record the crystalline (brittle) versus fibrous (ductile) fraction of the fracture and the lateral expansion

Often combined with Tensile testing · SEM

Standards JIS Z 2242 (Charpy impact test of metallic materials) / ISO 148-1 (Charpy pendulum impact test) / ASTM E23 (notched bar impact testing)

Terms Fracture toughness

Sources: TWI (impact testing)

Apply cyclic loading and count cycles to failure to obtain the S–N curve and the fatigue limit (fatigue strength). Crack growth rate (da/dN) tests are another form.

Principle Several specimens at different stress amplitudes are cycled until they fail or reach a set number of cycles (run-out).

Used for Toughness, fatigue and creep

Typical figures

Lateral resolution
— (whole specimen)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
The gauge section
Elements
—
Quantitative accuracy
Lives scatter widely (log life is close to normally distributed), so test enough specimens and treat the data statistically

Sample and effort

Size
Material for several standard specimens
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Destroys the sample Broken
Preparation
Extensive Machine specimens and finish their surfaces
Time
Long 10⁷ cycles take about 12 days at 10 Hz; weeks to months overall
Cost
High (long use of the test machine)

Pitfalls

  • Deriving a design curve (mean minus two standard deviations) from few data. Small samples underestimate the standard deviation, which is unconservative
  • Putting run-outs (unbroken specimens) into the regression as if they had failed
  • Striation spacing on the fracture surface is a guide to crack advance per cycle. Read it together with SEM fractography

Often combined with SEM · XRD (sin²ψ, pole figures) · Tensile testing

Standards ASTM E466 (force-controlled constant-amplitude axial fatigue tests)

Terms Fatigue limit Fatigue striations Paris law Miner's rule Modified Goodman diagram

Sources: TWI (fatigue statistics); NIMS (STAM feature)

Hold a constant load at high temperature and record strain against time (creep curve) and time to rupture. The basis of life assessment for high-temperature components.

Principle A specimen in a furnace carries a constant load while its extension is logged for a long time. Rupture times are organized by temperature and stress (Larson–Miller parameter etc.).

Used for Toughness, fatigue and creep

Typical figures

Lateral resolution
— (whole specimen)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
The gauge section
Elements
—
Quantitative accuracy
Some programmes aim at the stress that causes rupture in 100,000 hours (about 11 years)

Sample and effort

Size
Material for several standard specimens
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Destroys the sample Broken (or deformed for a long time)
Preparation
Extensive Machine specimens
Time
Long Hundreds to tens of thousands of hours
Cost
High (long use of furnaces and machines)

Pitfalls

  • Extrapolating short-term results too far. Check the assumptions of parameter methods (no change of mechanism) and state the extrapolation range
  • Small temperature differences change rupture life greatly. Verify temperature control and measurement

Often combined with Tensile testing · SEM · TEM/STEM

Standards ASTM E139 (creep and creep-rupture tests of metallic materials)

Terms Creep Power-law creep Larson–Miller parameter Deformation mechanism map

Sources: NIMS (STAM feature)

Bonding and other 4

Measure molecular and lattice vibrations from tiny wavelength shifts in scattered laser light to identify carbon forms (diamond, graphite, amorphous), oxides and polymers, and stress in semiconductors, at a 1 µm spot. No vacuum and nondestructive.

Principle Scattered light whose wavelength has changed by exchanging energy with molecular or lattice vibrations (Raman scattering) is dispersed and recorded.

Used for Organics, polymers and contamination Phase identification and crystal structure Chemical state (oxidation state, bonding) Residual stress

Typical figures

Lateral resolution
1 µm and above
Depth resolution / information depth
1–5 µm in confocal mode
Detection limit
1 wt% and above
Analyzed depth / volume
A spot about 1 µm across
Elements
Sees bonds and crystal types, not elements (pure metals give no peaks; oxides and rust can be measured)
Quantitative accuracy
Quantification needs standards

Sample and effort

Size
Particles to small pieces
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive Usually non-destructive
Preparation
Minimal Almost none
Time
Short Minutes per spot
Cost
Low Cheap

Pitfalls

  • Strong fluorescence swamps the much weaker Raman signal (try another excitation wavelength)
  • Quantification is difficult without standards
  • Each spectrum comes from a ~1 µm spot. Measure many spots on inhomogeneous samples

Often combined with FTIR · XRD · XPS (ESCA)

Terms Graphene Carbon nanotube

Sources: EAG Raman; Shimadzu rust analysis

Identify polymers, organics, contamination and coatings from infrared absorption by functional groups. With ATR, simply pressing a solid onto the crystal probes roughly the top 0.1–2 µm.

Principle Infrared light at the frequencies of molecular vibrations is absorbed; an interferometer and Fourier transform record all wavelengths at once.

Used for Organics, polymers and contamination Chemical state (oxidation state, bonding)

Typical figures

Lateral resolution
15–50 µm (FTIR microscope)
Depth resolution / information depth
About 0.1–2 µm with ATR
Detection limit
1–10 wt% for quantifying known components; 5–20% for identifying unknowns
Analyzed depth / volume
Illuminated area × penetration depth
Elements
Sees functional groups, not elements
Quantitative accuracy
Quantification needs standards and uniform thickness

Sample and effort

Size
Particles visible by eye to small pieces
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive Usually non-destructive
Preparation
Minimal None with ATR; KBr pellets or extraction are sometimes used
Time
Short Minutes per sample
Cost
Low Cheap

Pitfalls

  • Metals themselves cannot be measured (only contamination or films on them)
  • Water absorbs strongly, so dry wet samples first
  • Contamination films thinner than about 100 nm are hard to see (use XPS for the outermost surface)

Often combined with Raman spectroscopy · TGA · XPS (ESCA)

Terms Thermosetting resin

Sources: EAG FTIR; Innsbruck ATR-FTIR

Sweep the potential in solution and measure the current to obtain corrosion potential, corrosion rate, the passive range and pitting potential. AC impedance (EIS) follows the resistance of films and coatings and how it changes.

Principle A potentiostat sweeps the potential in a three-electrode cell (working electrode = sample, counter and reference electrodes). Corrosion current comes from Tafel extrapolation, or from polarization resistance and Tafel slopes (Stern–Geary equation).

Used for Corrosion behavior

Typical figures

Lateral resolution
— (average over the electrode area)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
The surface in contact with the solution
Elements
—
Quantitative accuracy
Polarization resistance is taken from the linear range around the corrosion potential (about 10 mV or less). Scan rate and solution resistance change the value

Sample and effort

Size
Small pieces with a defined exposed area
Conductivity
A conductive sample (electrode) is required
Vacuum
Not needed
Destructive?
Cut or polish The surface is corroded
Preparation
Moderate Mask all but the measured area; polish to a consistent finish
Time
Short Tens of minutes to hours per run (including stabilization)
Cost
Low Cheap

Pitfalls

  • Fast scans mix in charging current (slow scans such as 0.1 mV/s are used)
  • Not correcting the potential error from solution resistance (IR drop)
  • Not stating the reference electrode (SCE, Ag/AgCl, SHE), so results cannot be compared
  • Results depend on test solution and temperature. Use conditions close to service

Often combined with SEM · XPS (ESCA) · EDS (EDX)

Standards JIS G 0577 (pitting potential of stainless steels) / ASTM G59 (potentiodynamic polarization resistance) / ASTM G61 (cyclic potentiodynamic polarization for localized corrosion)

Terms Standard electrode potential Passivity Pitting corrosion Galvanic corrosion Stress corrosion cracking

Sources: Metrohm AN-COR-003

Weigh the sample dry, saturated with water and suspended in water to obtain bulk density and the fraction of pores connected to the surface (open porosity). A basic measure of how dense a sintered body is.

Principle The difference between saturated and suspended weights gives the sample volume, and the weight of absorbed water gives the open-pore volume.

Used for Density and porosity Internal defects

Typical figures

Lateral resolution
— (whole sample)
Depth resolution / information depth
—
Detection limit
—
Analyzed depth / volume
The whole sample
Elements
—
Quantitative accuracy
Pores not connected to the surface (closed pores) are not counted

Sample and effort

Size
Small pieces to parts that fit the balance
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive (the sample is soaked in water)
Preparation
Moderate Weigh dry, weigh saturated, weigh suspended in water
Time
Short (excluding drying and soaking)
Cost
Low Cheap

Pitfalls

  • Closed pores are not counted, so do not judge density from open porosity alone (use sections or X-ray CT for closed pores)
  • Incomplete saturation underestimates open porosity
  • Materials that react with or dissolve in water cannot be measured as they are

Often combined with CT · OM · SEM

Standards ISO 18754 (density and apparent porosity of fine ceramics)

Sources: Muğla Univ. Archimedes method; ISO 18754

Nondestructive testing 5

Send ultrasound into a part and receive reflections from internal flaws (cracks, voids, inclusions, weld defects) to estimate their position and size. Also measures wall thickness.

Principle A probe sends ultrasound at about 1–25 MHz through a couplant (water, oil etc.), and the arrival time and height of echoes from flaws and the back wall are read.

Used for Internal defects Thickness of films and layers

Typical figures

Lateral resolution
— (higher frequency is more sensitive to small flaws)
Depth resolution / information depth
Depth from the echo time
Detection limit
—
Analyzed depth / volume
The full thickness of the part
Elements
—
Quantitative accuracy
Echo heights are compared with reference blocks to estimate flaw size

Sample and effort

Size
Small pieces to large structures (on site)
Conductivity
Not needed (sound must pass)
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Minimal Smooth the contact surface and apply couplant
Time
Short Minutes per location and up
Cost
Low Cheap

Pitfalls

  • Coarse-grained materials (austenitic welds, castings) attenuate the sound and give high noise
  • Without calibration on reference blocks, flaw sizes are misjudged. Needs skilled operators
  • Without couplant the sound does not get in

Often combined with RT · CT · ET

Standards JIS Z 2344 (general rules for pulse-echo ultrasonic testing of metals) / JIS Z 2355-1 (ultrasonic thickness measurement: method)

Terms Heat-affected zone

Sources: Istanbul Tech. Univ. (NDT); JSNDI

Reveal surface-breaking cracks and pinholes as colored or fluorescent indications using a penetrant and developer. Works on any non-porous material: metals, ceramics, plastics.

Principle The penetrant seeps into flaws; after the surface excess is removed, the developer draws it out to form an indication.

Used for Surface cracks (nondestructively)

Typical figures

Lateral resolution
—
Depth resolution / information depth
Surface-breaking flaws only
Detection limit
—
Analyzed depth / volume
Surface
Elements
—
Quantitative accuracy
The indication is larger than the flaw (it bleeds)

Sample and effort

Size
Small pieces to large parts (on site)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive (liquids are applied)
Preparation
Moderate Clean off oil, paint and dirt thoroughly and dry
Time
Short Tens of minutes (including dwell and development)
Cost
Low Cheap

Pitfalls

  • Flaws that do not break the surface (internal or subsurface) are not found
  • Porous materials retain penetrant everywhere and cannot be tested
  • Insufficient pre-cleaning leaves oil or paint plugging the flaw mouths, so flaws are missed

Often combined with MT · ET · SEM

Standards JIS Z 2343-1 (penetrant testing: general principles)

Sources: Istanbul Tech. Univ. (NDT); JSNDI

Magnetize steel or another ferromagnetic material and collect magnetic particles where flux leaks out at surface and near-surface cracks.

Principle Flux leaks out at a flaw and the particles (fluorescent ones exist) gather there to form an indication. Sensitivity is best when the flux is perpendicular to the flaw.

Used for Surface cracks (nondestructively) Internal defects

Typical figures

Lateral resolution
—
Depth resolution / information depth
Surface and just below
Detection limit
—
Analyzed depth / volume
Near-surface
Elements
—
Quantitative accuracy
The indication length gives a guide to crack length

Sample and effort

Size
Small pieces to large parts (on site)
Conductivity
Ferromagnetic materials only (steel, cast iron, Ni, Co…)
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Moderate Remove dirt and thick coatings
Time
Short Minutes to tens of minutes
Cost
Low Cheap

Pitfalls

  • It does not work on non-ferromagnetic materials (austenitic stainless steel, Al, Cu…); use penetrant or eddy current testing
  • Cracks parallel to the flux are hard to see. Magnetize in two directions

Often combined with PT · ET · UT

Standards JIS Z 2320-1 (magnetic particle testing: general principles)

Sources: Istanbul Tech. Univ. (NDT); JSNDI

Induce eddy currents in a conductor with a coil to find surface and near-surface cracks, differences in material (conductivity) and plating or coating thickness, quickly and without contact. Used for 100% inspection of tubes and wire.

Principle Flaws or material changes disturb the eddy currents and change the coil impedance. Higher frequencies see only shallower depths (skin effect).

Used for Surface cracks (nondestructively) Thickness of films and layers Internal defects

Typical figures

Lateral resolution
—
Depth resolution / information depth
Penetration depends on frequency, conductivity and permeability (the standard depth of penetration is where intensity falls to 37%)
Detection limit
—
Analyzed depth / volume
Near-surface
Elements
—
Quantitative accuracy
Signal size is judged against reference standards

Sample and effort

Size
Small pieces to large parts, tubes and wire
Conductivity
Conductors only
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Minimal Almost none (surface condition affects the signal)
Time
Short Minutes (high speed on production lines)
Cost
Low Cheap

Pitfalls

  • Only conductors can be tested
  • Deep flaws are not seen; penetration is set by frequency, conductivity and permeability
  • Flaws parallel to the coil winding or the scan direction are easily missed
  • Without reference standards, signal size cannot be related to flaw size

Often combined with PT · MT · UT

Standards JIS Z 2316-1 (eddy current testing: general principles)

Terms Eddy-current loss

Sources: Istanbul Tech. Univ. (NDT); TWI (eddy current depth); JSNDI

Pass X-rays or gamma rays through a weld or casting onto film or a detector to find internal porosity, lack of fusion and cracks. Leaves a permanent record.

Principle Voids and low-density regions let more radiation through and appear darker on the image.

Used for Internal defects

Typical figures

Lateral resolution
— (as a guide, voids about 2% of the thickness are visible: about 0.5 mm in 25 mm of steel)
Depth resolution / information depth
The thickness is projected (no depth information)
Detection limit
—
Analyzed depth / volume
The whole penetrated thickness
Elements
—
Quantitative accuracy
Judged from density differences on the image (image quality checked with IQIs)

Sample and effort

Size
Small pieces to large structures (on site)
Conductivity
Not needed
Vacuum
Not needed
Destructive?
Non-destructive
Preparation
Minimal Almost none (film or detector must fit behind)
Time
Short Minutes to expose; hours including processing and evaluation
Cost
Moderate Medium (radiation control required)

Pitfalls

  • Thin cracks show only when the beam is parallel to the crack plane. Shoot from several directions
  • Radiation protection (controlled areas, qualified staff) is required
  • The image is a projection, so the depth of a flaw is unknown (use UT or CT)

Often combined with UT · CT

Standards JIS Z 3104 (radiographic testing of steel welds)

Terms Heat-affected zone Shrinkage cavity

Sources: Istanbul Tech. Univ. (NDT)

Overview table

Resolution, detection limit, and whether the sample is destroyed, preparation, time and cost for every method in one table. Figures are typical ranges and vary with the instrument and conditions. Preparation, time and cost are rough three-level comparisons between methods; actual prices and turnaround depend on the laboratory.

MethodLateral resolutionDepth resolution / information depthDetection limitDestructive?PreparationTimeCost
Microstructure and shape
OMAbout 0.2 µm (limit set by the wavelength of light)Image of the polished plane (no depth information)— (no elemental analysis)Cut or polishModerateShortLow
SEMAbout 1–5 nm (around 1 nm with a field-emission gun, about 5 nm on a typical instrument)SE from the top ~15 nm; BSE from deeper (depends on accelerating voltage)— (use EDS for composition)Non-destructiveMinimalShortLow
EBSD20–80 nm (material dependent). Grains smaller than 50 nm are difficult (TKD on a thin foil reaches 2–20 nm)Top ~10 nm of the surface— (no elemental analysis)Cut or polishExtensiveModerateModerate
TEM/STEM0.1–0.3 nm (TEM point resolution 0.14 nm, 0.1 nm in an aberration-corrected STEM; about 0.2–0.25 nm without correction)Projection through the whole specimen thickness (<100 nm)EDS about 0.5 wt% (0.01–0.1 wt% under good conditions)Cut or polishExtensiveLongHigh
FIBBeam below 10 nm; imaging at SEM resolution (about 1 nm)Serial sectioning gives 3-D data on regions 100 nm–10 µm in size— (combine with EDS etc.)Cut or polishModerateModerateModerate
AFM2–150 nm (set by the tip radius)Height resolution 0.01 nm—Non-destructiveMinimalShortLow
Laser confocal microscopy and white-light interferometryAbout 0.3–0.5 µm (lateral resolution is diffraction-limited, 0.61λ/NA: about 0.26 µm at 405 nm and NA 0.95; 0.5 µm in a white-light interferometer example)White-light interferometry 0.1 nm (phase mode) to 6 nm (scanning mode)—Non-destructiveMinimalShortLow
Stylus profilometer (roughness and step height)Set by the stylus tip radius (2 µm for a standard stylus)Heights down to the ångström level (instrument example)—Non-destructiveMinimalShortLow
XRR— (average over the X-ray footprint, which must be laterally uniform)Films about 1 nm to 1 µm thick—Non-destructiveMinimalModerateModerate
Spectroscopic ellipsometry— (average over the illuminated spot)Sensitive to sub-monolayer changes; about 0.5 nm to 20 µm for transparent films (instrument example)—Non-destructiveMinimalShortModerate
CTAbout 1/1000–1/2000 of the sample width (finer for smaller samples: µm for mm-sized samples; instruments reaching 0.1 µm exist)Same as lateral (3-D voxels)— (small density differences are hard to see)Non-destructiveMinimalModerateModerate
Composition
EDS (EDX)1 to a few µm in the SEM (set by the interaction volume); a few nm in a thin TEM foil1 to a few µm in the SEM0.1–0.5 wt% (0.02–0.05 wt% reported under good conditions)Non-destructiveModerateShortLow
WDS/EPMA1 to a few µm (set by the interaction volume)1 to a few µm100–300 ppm (a few ppm under favourable conditions)Cut or polishModerateModerateModerate
XRFUsually an average over a mm-sized area (tens of µm with micro-XRF)A few µm to several mm (strongly dependent on the X-ray line and the matrix)Around ppm (instrument and element dependent; worse for light elements)Non-destructiveMinimalShortLow
ICP-OES / ICP-MS— (average of all the dissolved material)—About 1 ppm in the solid for ICP-OES and 10 ppb for ICP-MS (solution limits multiplied by the dissolution and dilution factor; interferences make them an order of magnitude worse or more)Destroys the sampleExtensiveModerateModerate
Combustion and inert gas fusion analysis (C, S, O, N, H)— (average of the whole sample)—From about 0.1 ppm (element and instrument dependent)Destroys the sampleModerateShortModerate
Spark OES— (average over the spark spot)—Below 10 ppm for some elements (instrument examples: below 10 ppm for B and Pb, below 1 ppm for Zn)Cut or polishModerateShortLow
GD-OES— (average over a circle a few mm across; no lateral mapping)About 10% of the depth (for layers thicker than 10 nm)1–100 ppm (element and matrix dependent)Cut or polishMinimalShortModerate
TDS/TDA— (whole sample)—About 1 wt ppm (about 50 atomic ppm) in steel with one instrumentCut or polishExtensiveModerateModerate
XPS (ESCA)10 µm to 2 mm (instrument dependent; smallest analysis areas of about 30–100 µm reported)Top 1–10 nmAbout 0.1 at% (0.1–1 at%)Non-destructiveMinimalModerateModerate
AES10 nm and above (beam can be focused to 10–20 nm)Top 3–10 nm; 2–20 nm in depth profiles0.1–5 at% (element and instrument dependent)Non-destructiveMinimalModerateModerate
SIMSDepth profiles over areas of 10 µm and above; about 1 µm in imagingFrom about 0.5 nm (a few Å)10¹⁰–10¹⁶ atoms/cm³ (ppm and below)Cut or polishMinimalModerateHigh
APT0.5 nm lateral and 0.3 nm in depth in metals (about 1 nm in semiconductors and insulators)0.3 nmAbout 10 ppmCut or polishExtensiveLongHigh
Crystal structure
XRDUsually an average over 0.1 to several mm (20–25 µm with micro-diffraction)The 1/e attenuation depth of Cu Kα X-rays is about 4 µm in iron, 70 µm in Al and 3 mm in polyethylene (calculated from NIST attenuation coefficients); a few nm at grazing incidenceA minor phase from about 1%Non-destructiveMinimalShortLow
XRD (sin²ψ, pole figures)Average over the irradiated area (0.1 to several mm)Average over a few to tens of µm from the surface (5–50 µm in most materials; Cr Kα is used for steel). Deeper levels are measured after removing layers by electropolishing—Non-destructiveMinimalModerateModerate
SAED/CBEDSAED about 250 nm (set by the aperture); CBED a few nmThe whole specimen thickness (<100 nm)—Cut or polishExtensiveLongHigh
NDGauge volume about 1–10 mm³Same (mm scale)—Non-destructiveMinimalLongHigh
Thermal
DSC/DTA— (whole sample)—DSC is more sensitive than DTA, so weak events such as glass transitions are easier to seeDestroys the sampleModerateShortLow
TGA— (whole sample)—Mass changes below a microgram (instrument example; samples of about 1–150 mg)Destroys the sampleModerateShortLow
Dilatometry— (whole sample)——Cut or polishModerateModerateModerate
LFA— (through-thickness value of the whole disk)——Cut or polishModerateModerateModerate
DMA— (whole specimen)—— (transitions hard to see by DSC are often clearer)Cut or polishModerateModerateModerate
Mechanical
Tensile testing— (whole gauge length)——Destroys the sampleExtensiveModerateLow
HV/HR/HBWSet by the indent size (for example, about 30 µm diagonal at 0.98 N in a 200 HV steel)Indent depth and its surroundings—Non-destructiveModerateShortLow
NanoindentationPositioning below 50 nm (indents need µm spacing)Displacement noise below 0.1 nm, up to about 20 µm—Cut or polishModerateShortModerate
Charpy impact testing— (whole specimen)——Destroys the sampleExtensiveModerateLow
Fatigue testing— (whole specimen)——Destroys the sampleExtensiveLongHigh
Creep testing— (whole specimen)——Destroys the sampleExtensiveLongHigh
Bonding and other
Raman spectroscopy1 µm and above1–5 µm in confocal mode1 wt% and aboveNon-destructiveMinimalShortLow
FTIR15–50 µm (FTIR microscope)About 0.1–2 µm with ATR1–10 wt% for quantifying known components; 5–20% for identifying unknownsNon-destructiveMinimalShortLow
Electrochemical measurements (polarization curves, EIS)— (average over the electrode area)——Cut or polishModerateShortLow
Archimedes method (density and open porosity)— (whole sample)——Non-destructiveModerateShortLow
Nondestructive testing
UT— (higher frequency is more sensitive to small flaws)Depth from the echo time—Non-destructiveMinimalShortLow
PT—Surface-breaking flaws only—Non-destructiveModerateShortLow
MT—Surface and just below—Non-destructiveModerateShortLow
ET—Penetration depends on frequency, conductivity and permeability (the standard depth of penetration is where intensity falls to 37%)—Non-destructiveMinimalShortLow
RT— (as a guide, voids about 2% of the thickness are visible: about 0.5 mm in 25 mm of steel)The thickness is projected (no depth information)—Non-destructiveMinimalShortModerate

How to think about resolution, detection limit and analyzed volume

Method numbers differ by orders of magnitude because what you probe with and what you collect fixes the size of the region the signal comes from. SEM secondary electrons escape only from the top ~15 nm, so images are sharp, while X-rays from the same beam (EDS) come from the whole 1–few µm interaction volume, so composition maps are µm-scale. XPS and AES see a few nm, XRD a few to tens of µm, and neutrons several cm into steel.

The detection limit is set by the ratio of signal to background. EDS peaks are broad (tens of eV up to about 250 eV) and sit on the continuum, so about 0.1 wt% is the limit; WDS separates wavelengths with a crystal, giving narrow peaks (a few to tens of eV) and limits around 100 ppm. ICP-MS, which dissolves the sample and counts ions one by one, reaches ppb levels in the solid.

Resolution and detection limit tend to trade off. A smaller volume contains fewer atoms, so minor elements become harder to see: APT gives about 10 ppm at 0.3 nm resolution, TEM-EDS about 0.5 wt% at a nm spot, and ICP reaches ppb by giving up spatial information. Decide both where and down to what level you need to know before choosing.

The values in the tables are typical values from the sources. They vary a lot with instrument generation, conditions and material, so ask the instrument manager or service lab for the value on your sample.

Qualitative versus quantitative, and which analyzes need standards

"What is there" (qualitative) and "how much" (quantitative) are different questions. EDS spot analysis is qualitative within seconds, but it becomes quantitative to a few percent relative for major elements only on a flat polished sample compared against standards of known composition. Treat standardless results as semi-quantitative, not as quantitative values for a paper.

Standards are essentially required for WDS (EPMA), SIMS (ion-implanted standards), XRF (similar-composition standards), ICP (solution calibration), combustion and fusion analysis (certified reference materials) and GD-OES. XPS and AES are mostly semi-quantitative with sensitivity factors, and XRD has difficulty seeing phases below about 1%.

Standards should have a similar matrix, because the signal from the same amount of an element changes with absorption and excitation by the surrounding elements (matrix effects). When outsourcing, ask for the standards used for calibration together with the results.

What to decide before measuring

Write the aim in one sentence. If it is "find why hardness dropped after heat treatment", what you need is the change in microstructure (optical microscopy, SEM), the precipitates (TEM) and the hardness profile (hardness testing), perhaps not precise composition.

Decide what to compare with. Measuring only the failed part shows no difference without a good part. Measure good, failed and untreated samples side by side with the same method and conditions.

Decide numbers and statistics: how many hardness indents, how many fields for grain size, how many fatigue specimens, and report the scatter (standard deviation). One microscope field or one APT needle may not represent the whole sample.

Assume that preparation changes the result. Record preparation and storage: polishing scratches, FIB damage, coatings, grinding stresses, hydrogen loss during storage and so on.

What to tell a service lab

What you want to know (the aim) and what decision the result will feed. Giving the aim, not just a method name, lets the lab suggest a better method or conditions.

About the sample: material type and expected composition, heat-treatment and processing history, size and number, conductivity, magnetism, whether it may go into vacuum, presence of moisture, oil or organics, and whether it contains toxic or radioactive substances.

Where to measure: which face, depth or region (mark it on a photo), and whether to compare with a good part.

The form of the result: required detection limit, resolution and precision, candidate elements or phases, a statement of standards and calibration, whether raw data are needed, deadline and budget. Say in advance whether the sample must come back (destructive or not).

Main sources

FAQ

Can I report C or O amounts from EDS?

Light elements such as C, N and O are strongly absorbed and their peaks change shape between compounds, so EDS quantification can be far off. C cannot be measured on carbon-coated samples, and O is often calculated. Use EDS only as a guide to presence; measure amounts with WDS (with standards) or, for C in steel, combustion analysis.

Why does XRD crystallite size differ from the grain size I see in the microscope?

The Scherrer crystallite size is the average size of coherently diffracting domains, and one particle or grain may contain many of them. Above about 100 nm the estimate is unreliable, and strain broadening also mixes in. Measure grain size with optical microscopy, SEM or EBSD.

Are bright areas in a BSE image heavy elements?

On a flat polished surface BSE brightness is set mainly by mean atomic number, so bright areas tend to be heavier on average. But topography and crystal orientation (channeling) also change brightness, so on fracture surfaces or poorly polished samples confirm with EDS rather than reading contrast as composition.

For internal flaws without cutting, how do I choose between UT, radiography and CT?

UT suits thick parts and structures on site and gives flaw depth, but needs couplant and skill and struggles with coarse grains. Radiography leaves a record and is strong on volumetric flaws such as porosity, but cracks may not show depending on orientation and depth is unknown. CT gives 3-D shape and position, but resolution falls as samples get larger and the sample must fit the instrument.

Do the values in the tables apply to my instrument?

They are typical values from the sources and vary a lot with instrument generation, conditions and sample. Use them to compare methods and narrow down candidates, and check the values for your sample with the instrument manager or service lab before measuring.

Practice questions in related topics