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Moseley Plot and Absorption Edges

Powder or single crystal

Where an element’s characteristic X-ray lines fall, from the one relation that connects them all: the square root of the line energy is linear in atomic number. The straight line is fitted to this site’s own six anodes, so you can see what it is worth before you use it.

You supply
An element symbol (Ni) or an atomic number (28). Nothing else — a characteristic line is a property of the element alone.
Reading it
A predicted line is not a measured one: the fit is good to about a per cent from roughly Z = 20 to 50 and drifts several per cent by tungsten. Where this site holds the measurement it is printed beside the prediction. Moseley’s law fits the characteristic lines and predicts no absorption edge: the edge energies here are tabulated, and the bracket between two elements is a check on them rather than a substitute for them.

Worked examples: nickel, the filter for copper · zirconium, the filter for molybdenum · tungsten, far outside the fit

Earlier on the path: X-ray Tube Spectrum Next on the path: Absorption Coefficient Calculator On Choosing the radiation, step 2 of 4

See also: X-ray Tube Spectrum · Absorption Coefficient Calculator

Teaching with this page
Objective
After this page a learner can name the filter for an anode and say what makes that element and no other the right one.
Start from
this worked example
Ask first
Nickel is the filter for a copper tube. Would nickel also filter a molybdenum tube?
Watch for
“Yes — nickel absorbs X-rays whatever produced them”
Then
Absorption Coefficient Calculator
Check yourself: Nickel is the filter for a copper tube. Would nickel also filter a molybdenum tube?

No — a filter is chosen for one anode, not for X-rays in general Yes — nickel absorbs X-rays whatever produced them

A filter works because its K absorption edge falls between the anode’s two lines. Nickel’s edge is at 8.33 keV, which sits between copper’s Kβ at 8.91 and Kα at 8.04 — so Kβ is on the strongly absorbed side and Kα is not. Molybdenum’s lines are at 19.61 and 17.44 keV, both far above nickel’s edge, where nickel absorbs the two almost equally and improves nothing. Molybdenum’s filter is zirconium, edge 18.00 keV.

Input

Element

Either form: Ni or 28. The six elements this site carries as anodes — Cr, Fe, Co, Cu, Mo, Ag — also print their measured wavelengths, so you can see what the fit is worth.

Predicted lines for Zr (Z = 40)

Lines predicted for this element, against the wavelength measured for it. CSV
Line E / keV λ / Å measured λ / Å difference
Kα 15.7980 0.784810 — —
Kα1 15.8307 0.783190 — —
Kα2 15.7331 0.788048 — —
Kβ 17.7348 0.699099 — —

The straight line is fitted to this site’s own six anodes, Z = 24 to 47, and reproduces all of their measured wavelengths to better than 0.16% in E. It stays inside about 1% from roughly Z = 20 to Z = 50. Further out it is an extrapolation and the error grows: E against Z is not exactly straight, because screening is incomplete and relativistic corrections rise as Z4, so by tungsten (Z = 74) the predicted Kα is several per cent low. A predicted line is not a measured one; where this site has the measurement it is printed beside the prediction.

Moseley’s law

12340Cr24Fe26Co27Cu29Mo42Ag47Cr Z=24, √E = 2.3263 √keVFe Z=26, √E = 2.5298 √keVCo Z=27, √E = 2.6316 √keVCu Z=29, √E = 2.8357 √keVMo Z=42, √E = 4.1767 √keVAg Z=47, √E = 4.7017 √keVZ=40, predicted √E = 3.9747 √keVatomic number Z√(E / keV)

Filled points are the measured Kα energies of the six anodes; the dashed line is the least-squares fit through them. The open ring is Zr where the fit puts it.

Every anode in the fit, measured against what the law predicts. CSV
Anode Z measured λ / Å E/keV fitted E residual
Cr 24 2.29100 2.32633 2.32268 0.157%
Fe 26 1.937355 2.52976 2.52918 0.023%
Co 27 1.790260 2.63163 2.63243 0.030%
Cu 29 1.541838 2.83572 2.83893 0.113%
Mo 42 0.710730 4.17668 4.18117 0.108%
Ag 47 0.560868 4.70168 4.69741 0.091%

Bohr’s model predicts m = R∞⁢h⁢c×3/4 = 0.10102 keV and σ = 1 for Kα — one 1s electron screening the other. Fitted over the four light anodes alone (Cr to Cu), Kα gives m = 0.10188 and σ = 1.17, which is Moseley’s result. Including Mo and Ag bends the line and pulls σ to 1.50 — the value the fit above this table used. Nothing is wrong with either fit: the law is an excellent approximation over a limited span of Z, not an identity, and Moseley worked from aluminium to zinc.

How this is calculated

Moseley’s law: the square root of the photon energy of a characteristic line is linear in atomic number.E=m⁢(Z−σ)

Fitted by least squares to the six anodes this site carries, for the Kα line:m=0.103249keV,σ=1.50417

E=0.103249⁢(40−1.50417)=3.97467keV

E=(3.97467)2=15.7980keV

λ=h⁢cE=12.3984keVÅ15.7980keV=0.784810Å

The K absorption edge

Walk up the periodic table at a fixed wavelength and μ/ρ climbs steadily — more electrons, more absorption. At each of these six wavelengths it does that everywhere except at one place, where it falls by a factor near seven between neighbouring elements. That is the K absorption edge, and the direction is worth stating in the variable that is moving. Walking up Z at a fixed wavelength: for the lighter element the edge lies below the photon’s energy, so the photon can eject a 1s electron and the K shell contributes; one element heavier the edge has risen past it, the photon can no longer reach the 1s electron, and the K shell stops absorbing altogether. Said in energy at a fixed element, which is how an edge is usually quoted, that is the same fact the other way round: a photon above the edge energy ionises the K shell and one below it cannot.

Each radiation, and the two K edges its energy falls between. CSV
Radiation Z Kα / Å E / keV edge lies between their K edges / keV μ/ρ either side drop
Ag Kα 47 0.560868 22.106 Tc (43) and Ru (44) 21.044 < 22.106 < 22.117 66.3348 → 11.1094 ×6.0
Mo Kα 42 0.710730 17.445 Y (39) and Zr (40) 17.038 < 17.445 < 17.998 97.9348 → 15.5573 ×6.3
Cu Kα 29 1.541838 8.041 Co (27) and Ni (28) 7.709 < 8.041 < 8.333 324.234 → 46.8312 ×6.9
Co Kα 27 1.790260 6.925 Mn (25) and Fe (26) 6.539 < 6.925 < 7.112 393.149 → 53.6275 ×7.3
Fe Kα 26 1.937355 6.400 Cr (24) and Mn (25) 5.989 < 6.400 < 6.539 445.428 → 57.1066 ×7.8
Cr Kα 24 2.29100 5.412 Ti (22) and V (23) 4.966 < 5.412 < 5.465 558.513 → 68.5299 ×8.1

The drop is found in the coefficients and the edge energies are tabulated separately, so the last two columns are a check rather than a restatement: the photon energy has to fall between the two edges named, and it does, on every row. Nothing here is predicted — the Moseley fit above is over emission lines, and it is not continued to an absorption edge.

A Kβ filter is a foil whose own K edge lies between the anode’s Kα and Kβ: Kβ is the more energetic, so it is absorbed by ejecting the foil’s 1s electrons, while Kα falls just short of the edge and passes almost untouched. The jump above names the lightest element that clears the Kα side. The conventional filter is that element or one or two heavier — nickel for copper, zirconium for molybdenum, palladium for silver — because a filter whose edge sits only just above Kα leaves no margin. Silver is the extreme case, and the margin is now a number rather than a phrase: Ag Kα is 0.05% below the K edge of ruthenium, which is why nobody uses ruthenium.

Where this comes from