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Page 1: 1_electron_microscopy.pdf

David Muller 2008

Introduction to Electron MicroscopyIntroduction to Electron MicroscopyProf. David Muller, [email protected] 274 Clark Hall, 255-4065

Ernst Ruska and Max Knoll builtthe first electron microscope in 1931

(Nobel Prize to Ruska in 1986)T4 Bacteriophage

Electron Microscopy bridges the 1 nm – 1 μm gap between x-ray diffraction and optical microscopy

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David Muller 2008

Tools of the TradeTools of the Trade

Transmission Electron Microscope

Scanned Probe Microscope(includes Atomic Force Microscope)

AFM MFM

Scanning Electron Microscope

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David Muller 2008

Biological and Electronic Component Dimensions

Electronic ComponentsBiological Tool

Siz

e (m

)

10-10

10-8

10-6

10-4

10-2

1

Mammalian cell

Bacterial cell

Virus

GeneProtein

Atom

Logic Board

Computer chip

Transistor

Gate Oxide

OpticalMicroscope

TEM

AFM/STM

SEM

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David Muller 2008

Comparison of Optical and Electron MicroscopesComparison of Optical and Electron Microscopes

• Electron microscopes are operated in vacuum because the mean free path of electrons is air is short – this mean biological samples should not degas – they can either be dehydrated or frozen – pathology, not in-vivo.

•Electron microscopes have higher resolution than optical microscopes –atomic resolution is possible.

•Chemical imaging and spectroscopy – mapping π and σ bonds at 1nm resolution can be done.

•Radiation damage is severe and limits the image quality and resolution (not as bad as x-rays or neutrons though! – see R. Henderson, Quarterly Reviews of Biophysics 28 (1995) 171-193.)

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David Muller 2008

Comparison of Optical and Electron MicroscopesComparison of Optical and Electron Microscopes

TEMLight Microscopesource

1st condenser

CA condenser apertureOA objective aperture

SA selected area aperture

2nd condenser

Objectivelens

Projectorlenses

Viewing screenOr CCD

Viewing screenOr CCD

specimen

SEM or STEM

Image formed by scanning a small spot

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David Muller 2008

Inside a Transmission Electron Microscope

High tension cable(100-200 kV)

Filament

Double condenser lenscondenser aperture

Viewing chamber

Sample sits hereobjective aperture

Selected areaaperture

Accelerating stack

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David Muller 2008

An Electron Lens

Page 8: 1_electron_microscopy.pdf

David Muller 2008

An Electron Lens

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David Muller 2008

Geometric Optics Geometric Optics –– A Simple LensA Simple Lens

x x

Objectplane

imageplane

Backfocalplane

frontfocalplane

Lensat z=0

θ

Focusing: angular deflection of ray α distance from optic axis

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David Muller 2008

Geometric Optics Geometric Optics –– A Simple LensA Simple Lens

x x

Objectplane

imageplane

Backfocalplane

frontfocalplane

Lensat z=0

θ1

θ1

Wavefronts in focal plane are the Fourier Transform of the Image/Object

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David Muller 2008

X-ray and Electron Diffraction from a Silicon Crystal

λ=0.0251Å

200 keV Electrons

λ=1.54 Å

10 keV x-rays

θλ sindn =

In Si d220 = 1.92 Å

Bragg’s Law:

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David Muller 2008

Electron Velocity and Wavelength

De Broglie Wavelength:ph

=λ Where h is Planck’s constantAnd p=mv are the momentum, mass and velocity of the electron

If an electron is accelerated through a potential eV, it gains kinetic energy

eVmv =2

21

So the momentum is meVmv 2=

Vnm

meVh 23.1

2

2

==λElectron wavelength

( relativistically correct form: )2( 2

0

22

eVcmeVch

+=λ )

(V in Volts)

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David Muller 2008

Electron Wavelength vs. Accelerating Voltage

0.00871890.813521 MeV

0.0196870.77653300 keV

0.0250780.69531200 keV

0.0370130.54822100 keV

0.122040.01919410 keV

0.387630.0624691 keV

1.22630.0062560100 V

12.2640.00197841 V

λ (Ǻ)v/cAccelerating Voltage

0

0.01

0.02

0.03

0.04

0.05

0 200 400 600 800 1000

RelativisticNon-relativistic

λ (A

ngst

rom

s)

Electron Kinetic Energy (keV)

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David Muller 2008

Resolution Limits Imposed by Spherical Aberration, Cs(Or why we can’t do subatomic imaging with a 100 keV electron)

Lens

3min 2

1 αsCd =

Plane ofLeast Confusion

Gaussian image plane

Cs=0

Cs>0

For Cs>0, rays far from the axis are bent too strongly and come to a crossover before the gaussian image plane.

For a lens with aperture angle α, the minimum blur is

mind

Typical TEM numbers: Cs= 1 mm, α=10 mrad → dmin= 0.5 nm

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David Muller 2008

Resolution Limits Imposed by the Diffraction Limit(Less diffraction with a large aperture – must be balanced against Cs)

Lens

000

61.0sin61.0

αλ

αλ

≈=n

d

Gaussian image plane

The image of a point transferred through a lens with a circular aperture of

semiangle α0 is an Airy Disk of diameter

0d

(for electrons, n~1, and the angles are small)

α0

(0.61 for incoherent imaging e.g. ADF-STEM, 1.22 for coherent or phase contrast,. E.g TEM)

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David Muller 2008

Balancing Spherical Aberration against the Diffraction Limit(Less diffraction with a large aperture – must be balanced against Cs)

230

2

0

220

2

2161.0

⎟⎠⎞

⎜⎝⎛+⎟⎟

⎞⎜⎜⎝

⎛=+≈ α

αλ

sstot Cddd

For a rough estimate of the optimum aperture size, convolve blurring terms-If the point spreads were gaussian, we could add in quadrature:

1

10

100

1 10

Prob

e Si

ze (A

ngst

rom

s)

α (mrad)

ds

d0

Optimal apertureAnd minimum

Spot size

4/34/1min 66.0 λsCd =

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David Muller 2008

Balancing Spherical Aberration against the Diffraction Limit(Less diffraction with a large aperture – must be balanced against Cs)

4/34/1min 43.0 λsCd =

A more accurate wave-optical treatment, allowing less than λ/4 of phase shift across the lens gives

Minimum Spot size:

4/14

⎟⎟⎠

⎞⎜⎜⎝

⎛=

sopt C

λαOptimal aperture:

At 200 kV, λ=0.0257 Ǻ, dmin = 1.53Ǻ and αopt = 10 mrad

At 1 kV, λ=0.38 Ǻ, dmin = 12 Ǻ and αopt = 20 mrad

4/34/1min 61.0 λsCd =

(Incoherent image - e.g. STEM)

(coherent image - e.g. TEM)

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David Muller 2008

Electron Diffraction and Imaging a [100] Silicon Crystal

λ=0.0251Å

Diffraction Pattern

In Si d220 = 1.92 Å

Image

220

400

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David Muller 2008

Depth of Field, Depth of Focus

00 tanα

dD =

For d=3nm, α=10 mrad, D0= 300 nm For d=200nm, α=0.1 mrad, D0= 2 mm!

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David Muller 2008

Lenses in a Transmission Microscope(and deflection coils to correct their alignment)

http://www.rodenburg.org/RODENBURG.pdf

Condensor: uniformly illuminate the sampleIf misaligned, you will lose the beam when changing magnification

Gun: electron sourceIf misaligned, low intensity & other alignments may also be out

Objective: image sample – determines resolution. If misaligned, the image will be distorted, blurry.

projector: magnifies image/ forms diffraction pattern – should not alter resolution. If misaligned, the image will be distorted, diffraction pattern may be blurry.

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David Muller 2008

Caustics in a Lens

http://www-optics.unine.ch/education/optics_tutorials/aspherical_surface.html

On-axis

Tilted

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David Muller 2008

Caustics(remove extreme rays and caustics by putting in an aperture)

From “Natural Focusing and Fine Structure of Light: Caustics and Wave Dislocations” by J. F. Nye

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David Muller 2008

Common AberrationsAstigmatism Coma

Bad

Good

-Δf +ΔfΔf=0

-x&y focus at different planes-fix by adjusting stigmators

Check lens alignment by going through focus (change lens strength)

Bad

Good

-beam is tilted off axis-fix by centering aperture

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David Muller 2008

Lens AlignmentCorrecting for a gun shift misalignment

Step 1:Strongly excite C1(small spot size)cross-over movesto lens & optic axis.

Use beam shift D2to bring spot toto axis below C2

Step 2:Weaken C1(large spot size)cross-over movesaway from optic axis

Use gun shift D1to bring spot toto axis below C2.

Iterate until spotstops moving

How do we align one lens, when all lenses are misaligned?

http://www.rodenburg.org/RODENBURG.pdf

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David Muller 2008

Focusing using Fresnel Fringes

Check lens alignment by going through focus (change lens strength)

In focus

Minimum contrast

2 μm underfocus 2 μm overfocus

bright fringe dark fringe

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David Muller 2008

Correcting Objective Astigmatism using Fresnel Fringes

Stigmated& focused

bright fringedark fringe

Astigmatic & best focus

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Duffield: John Grazul150 Duffield(TEM+STEM)

Clark: Mick ThomasF3 Clark (STEM+EDX)

•1 nm (polymers) –> atomic resolution of crystals in thin samples•X-ray mapping at 1 nm•EELS at < 1 nm•Requires sample thinning (except for nanoparticles)

Transmission Electron Microscopy

•Clark: Mick ThomasF3 Clark Hall

•Bard/Snee:John Hunt SB56 Bard/1149 Snee

•Dr. Jonathan ShuD-22 Clark Hall

•Prof. Kit UmbachSB-60C Bard Hall

•CNF Clean Room

Location•Topographic Imaging on wafers•Accurate height measurements on flat surfaces (~ 0.5 nm vertical)•Lateral Resolution 10-20 nm•In-situ – no vacuum required

Atomic Force Microscopy

•Imaging of complex structures at 1-20 nm resolution•X-ray mapping at 100-500 nm •In-vacuum•Clark: High spatial resolution•Snee/Bard: best x-ray mapping, OIM

Scanning Electron Microscopy

ApplicationsType

Materials Microscopy Resources on Campus(http://www.ccmr.cornell.edu/facilities/)