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Sandbox Physics

E04 · Electron microscopy / foundations

Electron Resolution & Aberration Budget

Open or close the aperture and switch on spherical, chromatic, source, drift, vibration and astigmatism terms. Compare the pupil phase, Gaussian sample response and weak-phase contrast-transfer curve. Tune the aperture within ten percent of the best probe in this budget, then turn on correction and inspect the remaining floor.

Interactive modelElectron Resolution & Aberration Budget
Total probe scale0 nm0\,\mathrm{nm}
Diffraction contribution0 nm0\,\mathrm{nm}
Spherical contribution0 nm0\,\mathrm{nm}
Chromatic contribution0 nm0\,\mathrm{nm}
Source and mechanical floor0 nm0\,\mathrm{nm}
Fifth-order residual0 nm0\,\mathrm{nm}
Best semi-angle in scan0 mrad0\,\mathrm{mrad}
Best probe in scan0 nm0\,\mathrm{nm}
Largest contribution—\text{—}
Experiment task—\text{—}

Physics tutorial

What limits the probe after spherical correction?

BackgroundOpen or close the aperture and switch on spherical, chromatic, source, drift, vibration and astigmatism terms. Compare the pupil phase, Gaussian sample response and weak-phase contrast-transfer curve. Tune the aperture within ten percent of the best probe in this budget, then turn on correction and inspect the remaining floor.

Why it mattersExplore how the electron source, column and specimen constrain an instrument before interpreting an image.

Start with the essentials

Focus question
What limits the probe after spherical correction?
One-sentence intuition
Correcting one aberration moves the optimum aperture and exposes the next largest contribution. A blur budget and a signed CTF answer different imaging questions.

Core mathematical model

Quadrature blur budget

d2=ddiff2+dsph2+dchr2+ds2+ddrift2+dv2+da2+d52d^2=d_{\mathrm{diff}}^2+d_{\mathrm{sph}}^2+d_{\mathrm{chr}}^2+d_s^2+d_{\mathrm{drift}}^2+d_v^2+d_a^2+d_5^2

The terms use characteristic diameter conventions; adding them in quadrature is an engineering approximation.

Competing aperture terms

ddiff=0.61λ/α,dsph=Csα3/2,dchr=CcαΔE/Ed_{\mathrm{diff}}=0.61\lambda/\alpha,\quad d_{\mathrm{sph}}=C_s\alpha^3/2,\quad d_{\mathrm{chr}}=C_c\alpha\Delta E/E

Diffraction falls with aperture angle while the aberration terms rise.

Residual correction

Cs,res=0.01Cs,d5=C5α5,C5=10 mmC_{s,\mathrm{res}}=0.01C_s,\qquad d_5=C_5\alpha^5,\quad C_5=10\,\mathrm{mm}

These residual settings are illustrative, not a commercial corrector performance claim.

Separate weak-phase transfer

CTF(q)=−sin⁡ ⁣[π(12Csλ3q4−Δfλq2)]exp⁡(−2π2σ2q2)\mathrm{CTF}(q)=-\sin\!\left[\pi\left(\frac12C_s\lambda^3q^4-\Delta f\lambda q^2\right)\right]\exp(-2\pi^2\sigma^2q^2)

The Gaussian envelope includes source, drift and vibration. The zero-frequency transfer vanishes for a weak phase object.

Common difficulties

Keep the model boundary explicit

Typical misconceptionTurning on a corrector eliminates every resolution limit.

Better mental modelSource size, energy spread, drift, vibration and higher-order residuals remain.

Run the experiment

  1. 01

    Bracket the optimum

    Compare narrow and wide presets, predict the best angle, then tune within ten percent of the best budget and Check target.

    What to observe: An intermediate aperture balances diffraction and aberrations.
  2. 02

    Expose the floor

    Enable correction, then separately disable chromatic, drift and source terms.

    What to observe: Residual terms can limit the corrected probe even when spherical blur is small.
  3. 03

    Read contrast reversal

    Keep the blur budget fixed and change CTF defocus through positive and negative values.

    What to observe: The signed transfer changes; the independent diameter budget stays fixed.