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    A.E. Gunns MENA3100 V10

    Sample preparation for TEM Crushing

    Cutting

    saw, diamond pen, ultrasonic drill, FIB

    Mechanical thinning

    Grinding, dimpling

    Electrochemical thinning

    Ion milling

    Coating

    Replica methods

    FIB

    Plane view or cross section sample?

    Is your material brittle or ductile?

    Is it a conductor or insulator?

    Is it a multi layered material?

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    A.E. Gunns MENA3100 V10

    Grind down/

    dimple

    TEM sample preparation: Thin films

    Top view

    Cross section

    or

    Cut out a cylinder

    and glue it in a Cu-tube

    Grind down and

    glue on Cu-rings

    Cut a slice of the

    cylinder and grind

    it down / dimple

    Ione beam thinning

    Cut out cylinder

    Ione beam thinning

    Cut out slices

    Glue the interface

    of interest face toface together with

    support material

    Cut off excess

    material

    Focused Ion Beam

    (FIB)

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    A.E. Gunns MENA3100 V10

    Basic principles, first TEM

    Wave length:

    = h/(2meV)0.5 (NB non rel. expr.)

    = h/(2m0eV(1+eV)/2m0c2)0.5(relativistic expression)

    200kV: = 0.00251 nm (v/c= 0.6953, m/m0= 1.3914)

    Electrons are deflected by bothelectrostatic and magnetic fields

    Force from an electrostatic field (in the gun)

    F= -e E

    Force from amagnetic field (in the lenses)

    F= -e (v x B)

    Nobel prize lecture: http://ernst.ruska.de/daten_e/library/documents/999.nobellecture/lecture.html

    a) The first electron microscope built by Knoll

    and Ruska in 1933, b) The first commercial

    electron Microscope built by Siemens in 1939.

    http://ernst.ruska.de/daten_e/library/documents/999.nobellecture/lecture.htmlhttp://ernst.ruska.de/daten_e/library/documents/999.nobellecture/lecture.htmlhttp://ernst.ruska.de/daten_e/library/documents/999.nobellecture/lecture.html
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    A.E. Gunns MENA3100 V10

    Basic TEM

    Electron source:

    Tungsten, W

    LaB6

    FEG

    Electron gun

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    A.E. Gunns MENA3100 V10

    Electron guns

    Thermionic gunField emission gun (FEG)

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    A.E. Gunns MENA3100 V10

    Technical data of different sourcesTungsten LaB6 Cold

    FEG

    Schottky Heated

    FEG

    Brightness

    (A/m2/sr)

    (0.3-2)109 (0.3-2)109 1011-1014 1011-1014 1011-1014

    Temperature

    (K)

    2500-3000 1400-2000 300 1800 1800

    Work function

    (eV)

    4.6 2.7 4.6 2.8 4.6

    Source size

    (m)

    20-50 10-20

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    A.E. Gunns MENA3100 V10

    Basic TEM

    Electron gun

    Vacuum requirements:

    - Avoid scattering from residual gas inthe column.

    - Thermal and chemical stability of the

    gun during operation.

    - Reduce beam-induced contamination

    of the sample.

    LaB6: 10-7torr

    FEG: 10-10torr

    Electron source:

    Tungsten, W

    LaB6

    FEGCold trap

    Sample position

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    A.E. Gunns MENA3100 V10

    The lenses in a TEM

    Sample

    Filament

    Anode

    1. and 2. condenser lenses

    Objective lens

    Intermediate lenses

    Projector lens

    Compared to the lenses in an

    optical microscope they are verypoor!

    The point resolution in a TEM is

    limited by the aberrations of the

    lenses.

    The diffraction limit on resolution

    is given by the Raleigh criterion:

    d=0.61/sin, =1, sin~

    -Spherical

    - Chromatic

    -Astigmatism

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    A.E. Gunns MENA3100 V10

    Spherical aberrations

    Spherical aberration coefficient

    ds= 0.5MCs3

    M: magnification

    Cs:Spherical aberration coefficient

    : angular aperture/

    angular deviation from optical axis

    2000FX: Cs= 2.3 mm

    2010F: Cs= 0.5 nm

    r1

    r2

    Disk of least confusion

    Cscorrected TEMs are now available

    The diffraction and the spherical aberration limits on resolution

    have an opposite dependence on the angular aperture of the objective.

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    A.E. Gunns MENA3100 V10

    Aberrations in a nutshell

    Core of the M100 galaxy seen through

    Hubble (source: NASA)

    Before Cscorrection

    After Cscorrection

    Q.M. Ramasse

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    A.E. Gunns MENA3100 V10

    Resolution limit

    Year Resolution1940s ~10nm1950s ~0.5-2nm1960s 0.3nm (transmission)

    ~15-20nm (scanning)1970s 0.2nm (transmission)

    7nm (standard scanning)

    1980s 0.15nm (transmission)5nm (scanning at 1kV)

    1990s 0.1nm (transmission)3nm (scanning at 1kV)

    2000s

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    A.E. Gunns MENA3100 V10

    Chromatic aberration

    v

    v -vdc= Cc((U/U)

    2+ (2I/I)2+ (E/E)2)0.5

    Cc: Chromatic aberration coefficient

    : angular divergence of the beam

    U: acceleration voltage

    I: Current in the windings of the objective lens

    E: Energy of the electrons

    2000FX: Cc= 2.2 mm

    2010F: Cc= 1.0 mm

    Chromatic aberration coefficient:

    Thermally emitted electrons:E/E=KT/eV

    Force from amagnetic field:F= -e (v x B)

    Disk of least confusion

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    A.E. Gunns MENA3100 V10

    Lens aberrations

    Lens astigmatismLoss of axial asymmetry

    y-focus

    x-focusy

    xThis astigmatism can not be

    prevented, but it can be

    corrected!

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    A.E. Gunns MENA3100 V10

    Operating modes

    Convergent beam Parallel beam

    Can be scanned

    (STEM mode)

    Specimen

    Imaging mode

    orDiffraction mode

    Spectroscopy and mapping

    (EDS and EELS)

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    A.E. Gunns MENA3100 V10

    Image or diffraction mode

    1. and 2. condenser

    lenses

    Objective lens

    Intermediate lenses

    Projector lens

    Spesimen

    Filament

    Anode

    Diffraction plane

    Image plane

    Objective aperture

    Selected area aperture

    Image or diffraction patternSTEM detectors (BF and HAADF)

    Bi-prism

    Viewing screen

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    A.E. Gunns MENA3100 V10

    Advanced nanotool

    JEOL 2010F FEGTEMUltra high resolution version with analytical possibilities

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    A.E. Gunns MENA3100 V10

    Imaging / microscopy

    200 nm

    Si

    SiO2

    TiO2

    Pt

    BiFeO3

    Glue

    TEM

    - High resolution (HREM)- Bright field (BF)

    - Dark field (DF)

    - Shadow imaging

    (SAD+DF+BF)

    STEM

    - Z-contrast (HAADF)

    - Elemental mapping

    (EDS and EELS)

    GIF

    - Energy filtering

    Holography

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    A.E. Gunns MENA3100 V10

    Simplified ray diagram

    Objective lense

    Diffraction plane

    (back focal plane)

    Image plane

    Sample

    Parallel incoming electron beamSi

    c

    ow

    erCell2.0

    1,1 nm

    3,8

    Objective aperture

    Selected area

    aperture

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    A.E. Gunns MENA3100 V10

    Apertures

    Selected area aperture

    Condenser aperture

    Objective aperture

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    A.E. Gunns MENA3100 V10

    Use of apertures

    Condenser aperture:Limits the number of electrons hitting the sample (reducing the intensity),

    Reducing the diameter of the discs in the convergent electron diffraction pattern.

    Selected area aperture:Allows only electrons going through an area on the sample that is limited by the SAD aperture

    to contribute to the diffraction pattern (SAD pattern).

    Objective aperture:Allows certain reflections to contribute to the image. Increases the contrast in the image.

    Bright field imaging (central beam, 000), Dark field imaging (one reflection, g), High resolution

    Images (several reflections from a zone axis).

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    A.E. Gunns MENA3100 V10

    Objective aperture: Contrast enhancement

    All electrons contributes to the image. A small aperture allows only electrons in the

    central spot in the back focal plane to contribute

    to the image.Intensity: Thickness and density

    dependence

    Mass-thickness contrast

    Si Ag and Pb

    glue(light elements)

    hole

    50 nmOne grain seen along a

    low index zone axis.

    Diffraction contrast(Amplitude contrast)

    Diffraction contrast: B i ht fi ld (BF)

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    A.E. Gunns MENA3100 V10

    Diffraction contrast: Bright field (BF),dark field (DF) and weak-beam (WB)

    BF image

    Objective

    aperture

    DF image Weak-beam

    Dissociation of pure screw dislocation

    In Ni3Al, Meng and Preston, J.

    Mater. Scicence, 35, p. 821-828, 2000.

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    A.E. Gunns MENA3100 V10

    Bending contours

    BF image

    DF image

    DF image

    Obj. aperture

    Obj. lens

    sample

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    A.E. Gunns MENA3100 V10

    Thickness fringes/contours

    Sample (side view)

    e

    000 g

    t

    Ig=1- Io

    In the two-beam situation the intensity

    of the diffracted and direct beamis periodic with thickness (Ig=1- Io)

    Ig=(t/g)2(sin2(tseff)/(tseff)

    2))

    t = distance traveled by the diffracted beam.

    g= extinction distance

    Sample (top view)Hole

    Positions with max

    Intensity in Ig

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    A.E. Gunns MENA3100 V10

    Thickness fringes,bright and dark field images

    Sample Sample

    DF imageBF image

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    A.E. Gunns MENA3100 V10

    Phase contrast: HREM and Moire fringes

    2 nm

    http://www.mathematik.com/Moire/

    A Moir patternis an interferencepattern created, for example, when

    two grids are overlaid at an angle, or

    when they have slightly different mesh

    sizes (rotational and parallel Moire

    patterns).HREM image

    Long-Wei Yin et al., Materials Letters, 52, p.187-191

    200-400 kV TEMs are mostcommonly used for HREM

    Interference pattern

    http://www.mathematik.com/Moire/http://www.mathematik.com/Moire/
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    A.E. Gunns MENA3100 V10

    Moire fringe spacing

    Parallel Moire spacingdmoire= 1 / IgI = 1 / Ig1-g2I = d1d2/Id1-d2I

    Rotational Moire spacing

    dmoire= 1 / IgI = 1 / Ig1-g2I ~1/g= d/

    Parallel and rotational Moire spacing

    dmoire= d1d2/((d1-d2)2+ d1d2

    2)0.5

    g1

    g2

    g

    g1g2 g

    Simulating HREM images

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    A.E. Gunns MENA3100 V10

    Simulating HREM imagesContrast transfer function (CTF)

    CTF (Contrast Transfer Function) is the function which

    modulates the amplitudes and phases of the electron

    diffraction pattern formed in the back focal plane of theobjective lens. It can be represented as:

    k = u

    The curve depend on:

    Cs (the quality of objective lens)l(wave-length defined by accelerating voltage)

    Df(the defocus value)

    u(spatial frequency)

    In order to take into account the effect of the

    objective lens when calculating HREM images, the

    wave function (u) in reciprocal space has to be

    multiplied by a transfer function T(u).

    In general we have:

    (r)= (u) T(u) exp (2iu.r)

    T(u)= A(u) exp(i), A(u): aperture function 1 or 0

    (u)= fu2+1/2Cs3u4 : coherent transfer function

    Si l ti HREM i

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    A.E. Gunns MENA3100 V10

    Simulating HREM images

    Contrast transfer function (CTF)

    Effect of the envelope functions can be represented as:

    where Ecis the temporal coherency envelope(caused by

    chromatic aberrations, focal and energy spread,instabilities in thehigh tension and objective lens current), and Eais spatial

    coherencyenvelope(caused by the finite incident beam

    convergence).

    http://www.maxsidorov.com/ctfexplorer/webhelp/background.htm

    http://www.maxsidorov.com/ctfexplorer/webhelp/spatial_coherency.htmhttp://www.maxsidorov.com/ctfexplorer/webhelp/spatial_coherency.htmhttp://www.maxsidorov.com/ctfexplorer/webhelp/background.htmhttp://www.maxsidorov.com/ctfexplorer/webhelp/background.htmhttp://www.maxsidorov.com/ctfexplorer/webhelp/spatial_coherency.htmhttp://www.maxsidorov.com/ctfexplorer/webhelp/spatial_coherency.htm
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    A.E. Gunns MENA3100 V10

    Scherzer defocus

    http://www.maxsidorov.com/ctfexplorer/webhelp/effect_of_defocus.htm

    f = - (Cs)1/2

    f = -1.2(Cs)1/2

    Scherzer condition Extended Scherzer condition

    http://www.maxsidorov.com/ctfexplorer/webhelp/effect_of_defocus.htmhttp://www.maxsidorov.com/ctfexplorer/webhelp/effect_of_defocus.htm
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    A.E. Gunns MENA3100 V10

    HREM simulations

    One possible model for which the simulated HREM images match rectangular region I

    HREM simulation along [0 0 1] based on the above structures. The numbers before and after the slash

    symbol / represent the defocus and thickness (nm), respectively

    The assessment of GPB2/S structures in AlCuMg alloys

    Wang and Starink, Mater. Sci. and Eng. A, 386, p 156-163, 2004.

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    A.E. Gunns MENA3100 V10

    HAADF image of an icosahedral FePt particle (false colors): thanks to the small

    probe size, it is possible to probe precisely the chemical structure of samples atthe atomic level, revealing here a small crystalline layer of iron oxide

    surrounding the outermost shell of the particle.

    Combined HAADF and EELS

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    A.E. Gunns MENA3100 V10

    Energy filtering

    A. Thgersen et al., Collaboration with Prof. T. Finnstad, UiO, S. Diplas, SINTEF and

    UniS, UK and NIMS, Japan