- •Preface
- •Imaging Microscopic Features
- •Measuring the Crystal Structure
- •References
- •Contents
- •1.4 Simulating the Effects of Elastic Scattering: Monte Carlo Calculations
- •What Are the Main Features of the Beam Electron Interaction Volume?
- •How Does the Interaction Volume Change with Composition?
- •How Does the Interaction Volume Change with Incident Beam Energy?
- •How Does the Interaction Volume Change with Specimen Tilt?
- •1.5 A Range Equation To Estimate the Size of the Interaction Volume
- •References
- •2: Backscattered Electrons
- •2.1 Origin
- •2.2.1 BSE Response to Specimen Composition (η vs. Atomic Number, Z)
- •SEM Image Contrast with BSE: “Atomic Number Contrast”
- •SEM Image Contrast: “BSE Topographic Contrast—Number Effects”
- •2.2.3 Angular Distribution of Backscattering
- •Beam Incident at an Acute Angle to the Specimen Surface (Specimen Tilt > 0°)
- •SEM Image Contrast: “BSE Topographic Contrast—Trajectory Effects”
- •2.2.4 Spatial Distribution of Backscattering
- •Depth Distribution of Backscattering
- •Radial Distribution of Backscattered Electrons
- •2.3 Summary
- •References
- •3: Secondary Electrons
- •3.1 Origin
- •3.2 Energy Distribution
- •3.3 Escape Depth of Secondary Electrons
- •3.8 Spatial Characteristics of Secondary Electrons
- •References
- •4: X-Rays
- •4.1 Overview
- •4.2 Characteristic X-Rays
- •4.2.1 Origin
- •4.2.2 Fluorescence Yield
- •4.2.3 X-Ray Families
- •4.2.4 X-Ray Nomenclature
- •4.2.6 Characteristic X-Ray Intensity
- •Isolated Atoms
- •X-Ray Production in Thin Foils
- •X-Ray Intensity Emitted from Thick, Solid Specimens
- •4.3 X-Ray Continuum (bremsstrahlung)
- •4.3.1 X-Ray Continuum Intensity
- •4.3.3 Range of X-ray Production
- •4.4 X-Ray Absorption
- •4.5 X-Ray Fluorescence
- •References
- •5.1 Electron Beam Parameters
- •5.2 Electron Optical Parameters
- •5.2.1 Beam Energy
- •Landing Energy
- •5.2.2 Beam Diameter
- •5.2.3 Beam Current
- •5.2.4 Beam Current Density
- •5.2.5 Beam Convergence Angle, α
- •5.2.6 Beam Solid Angle
- •5.2.7 Electron Optical Brightness, β
- •Brightness Equation
- •5.2.8 Focus
- •Astigmatism
- •5.3 SEM Imaging Modes
- •5.3.1 High Depth-of-Field Mode
- •5.3.2 High-Current Mode
- •5.3.3 Resolution Mode
- •5.3.4 Low-Voltage Mode
- •5.4 Electron Detectors
- •5.4.1 Important Properties of BSE and SE for Detector Design and Operation
- •Abundance
- •Angular Distribution
- •Kinetic Energy Response
- •5.4.2 Detector Characteristics
- •Angular Measures for Electron Detectors
- •Elevation (Take-Off) Angle, ψ, and Azimuthal Angle, ζ
- •Solid Angle, Ω
- •Energy Response
- •Bandwidth
- •5.4.3 Common Types of Electron Detectors
- •Backscattered Electrons
- •Passive Detectors
- •Scintillation Detectors
- •Semiconductor BSE Detectors
- •5.4.4 Secondary Electron Detectors
- •Everhart–Thornley Detector
- •Through-the-Lens (TTL) Electron Detectors
- •TTL SE Detector
- •TTL BSE Detector
- •Measuring the DQE: BSE Semiconductor Detector
- •References
- •6: Image Formation
- •6.1 Image Construction by Scanning Action
- •6.2 Magnification
- •6.3 Making Dimensional Measurements With the SEM: How Big Is That Feature?
- •Using a Calibrated Structure in ImageJ-Fiji
- •6.4 Image Defects
- •6.4.1 Projection Distortion (Foreshortening)
- •6.4.2 Image Defocusing (Blurring)
- •6.5 Making Measurements on Surfaces With Arbitrary Topography: Stereomicroscopy
- •6.5.1 Qualitative Stereomicroscopy
- •Fixed beam, Specimen Position Altered
- •Fixed Specimen, Beam Incidence Angle Changed
- •6.5.2 Quantitative Stereomicroscopy
- •Measuring a Simple Vertical Displacement
- •References
- •7: SEM Image Interpretation
- •7.1 Information in SEM Images
- •7.2.2 Calculating Atomic Number Contrast
- •Establishing a Robust Light-Optical Analogy
- •Getting It Wrong: Breaking the Light-Optical Analogy of the Everhart–Thornley (Positive Bias) Detector
- •Deconstructing the SEM/E–T Image of Topography
- •SUM Mode (A + B)
- •DIFFERENCE Mode (A−B)
- •References
- •References
- •9: Image Defects
- •9.1 Charging
- •9.1.1 What Is Specimen Charging?
- •9.1.3 Techniques to Control Charging Artifacts (High Vacuum Instruments)
- •Observing Uncoated Specimens
- •Coating an Insulating Specimen for Charge Dissipation
- •Choosing the Coating for Imaging Morphology
- •9.2 Radiation Damage
- •9.3 Contamination
- •References
- •10: High Resolution Imaging
- •10.2 Instrumentation Considerations
- •10.4.1 SE Range Effects Produce Bright Edges (Isolated Edges)
- •10.4.4 Too Much of a Good Thing: The Bright Edge Effect Hinders Locating the True Position of an Edge for Critical Dimension Metrology
- •10.5.1 Beam Energy Strategies
- •Low Beam Energy Strategy
- •High Beam Energy Strategy
- •Making More SE1: Apply a Thin High-δ Metal Coating
- •Making Fewer BSEs, SE2, and SE3 by Eliminating Bulk Scattering From the Substrate
- •10.6 Factors That Hinder Achieving High Resolution
- •10.6.2 Pathological Specimen Behavior
- •Contamination
- •Instabilities
- •References
- •11: Low Beam Energy SEM
- •11.3 Selecting the Beam Energy to Control the Spatial Sampling of Imaging Signals
- •11.3.1 Low Beam Energy for High Lateral Resolution SEM
- •11.3.2 Low Beam Energy for High Depth Resolution SEM
- •11.3.3 Extremely Low Beam Energy Imaging
- •References
- •12.1.1 Stable Electron Source Operation
- •12.1.2 Maintaining Beam Integrity
- •12.1.4 Minimizing Contamination
- •12.3.1 Control of Specimen Charging
- •12.5 VPSEM Image Resolution
- •References
- •13: ImageJ and Fiji
- •13.1 The ImageJ Universe
- •13.2 Fiji
- •13.3 Plugins
- •13.4 Where to Learn More
- •References
- •14: SEM Imaging Checklist
- •14.1.1 Conducting or Semiconducting Specimens
- •14.1.2 Insulating Specimens
- •14.2 Electron Signals Available
- •14.2.1 Beam Electron Range
- •14.2.2 Backscattered Electrons
- •14.2.3 Secondary Electrons
- •14.3 Selecting the Electron Detector
- •14.3.2 Backscattered Electron Detectors
- •14.3.3 “Through-the-Lens” Detectors
- •14.4 Selecting the Beam Energy for SEM Imaging
- •14.4.4 High Resolution SEM Imaging
- •Strategy 1
- •Strategy 2
- •14.5 Selecting the Beam Current
- •14.5.1 High Resolution Imaging
- •14.5.2 Low Contrast Features Require High Beam Current and/or Long Frame Time to Establish Visibility
- •14.6 Image Presentation
- •14.6.1 “Live” Display Adjustments
- •14.6.2 Post-Collection Processing
- •14.7 Image Interpretation
- •14.7.1 Observer’s Point of View
- •14.7.3 Contrast Encoding
- •14.8.1 VPSEM Advantages
- •14.8.2 VPSEM Disadvantages
- •15: SEM Case Studies
- •15.1 Case Study: How High Is That Feature Relative to Another?
- •15.2 Revealing Shallow Surface Relief
- •16.1.2 Minor Artifacts: The Si-Escape Peak
- •16.1.3 Minor Artifacts: Coincidence Peaks
- •16.1.4 Minor Artifacts: Si Absorption Edge and Si Internal Fluorescence Peak
- •16.2 “Best Practices” for Electron-Excited EDS Operation
- •16.2.1 Operation of the EDS System
- •Choosing the EDS Time Constant (Resolution and Throughput)
- •Choosing the Solid Angle of the EDS
- •Selecting a Beam Current for an Acceptable Level of System Dead-Time
- •16.3.1 Detector Geometry
- •16.3.2 Process Time
- •16.3.3 Optimal Working Distance
- •16.3.4 Detector Orientation
- •16.3.5 Count Rate Linearity
- •16.3.6 Energy Calibration Linearity
- •16.3.7 Other Items
- •16.3.8 Setting Up a Quality Control Program
- •Using the QC Tools Within DTSA-II
- •Creating a QC Project
- •Linearity of Output Count Rate with Live-Time Dose
- •Resolution and Peak Position Stability with Count Rate
- •Solid Angle for Low X-ray Flux
- •Maximizing Throughput at Moderate Resolution
- •References
- •17: DTSA-II EDS Software
- •17.1 Getting Started With NIST DTSA-II
- •17.1.1 Motivation
- •17.1.2 Platform
- •17.1.3 Overview
- •17.1.4 Design
- •Simulation
- •Quantification
- •Experiment Design
- •Modeled Detectors (. Fig. 17.1)
- •Window Type (. Fig. 17.2)
- •The Optimal Working Distance (. Figs. 17.3 and 17.4)
- •Elevation Angle
- •Sample-to-Detector Distance
- •Detector Area
- •Crystal Thickness
- •Number of Channels, Energy Scale, and Zero Offset
- •Resolution at Mn Kα (Approximate)
- •Azimuthal Angle
- •Gold Layer, Aluminum Layer, Nickel Layer
- •Dead Layer
- •Zero Strobe Discriminator (. Figs. 17.7 and 17.8)
- •Material Editor Dialog (. Figs. 17.9, 17.10, 17.11, 17.12, 17.13, and 17.14)
- •17.2.1 Introduction
- •17.2.2 Monte Carlo Simulation
- •17.2.4 Optional Tables
- •References
- •18: Qualitative Elemental Analysis by Energy Dispersive X-Ray Spectrometry
- •18.1 Quality Assurance Issues for Qualitative Analysis: EDS Calibration
- •18.2 Principles of Qualitative EDS Analysis
- •Exciting Characteristic X-Rays
- •Fluorescence Yield
- •X-ray Absorption
- •Si Escape Peak
- •Coincidence Peaks
- •18.3 Performing Manual Qualitative Analysis
- •Beam Energy
- •Choosing the EDS Resolution (Detector Time Constant)
- •Obtaining Adequate Counts
- •18.4.1 Employ the Available Software Tools
- •18.4.3 Lower Photon Energy Region
- •18.4.5 Checking Your Work
- •18.5 A Worked Example of Manual Peak Identification
- •References
- •19.1 What Is a k-ratio?
- •19.3 Sets of k-ratios
- •19.5 The Analytical Total
- •19.6 Normalization
- •19.7.1 Oxygen by Assumed Stoichiometry
- •19.7.3 Element by Difference
- •19.8 Ways of Reporting Composition
- •19.8.1 Mass Fraction
- •19.8.2 Atomic Fraction
- •19.8.3 Stoichiometry
- •19.8.4 Oxide Fractions
- •Example Calculations
- •19.9 The Accuracy of Quantitative Electron-Excited X-ray Microanalysis
- •19.9.1 Standards-Based k-ratio Protocol
- •19.9.2 “Standardless Analysis”
- •19.10 Appendix
- •19.10.1 The Need for Matrix Corrections To Achieve Quantitative Analysis
- •19.10.2 The Physical Origin of Matrix Effects
- •19.10.3 ZAF Factors in Microanalysis
- •X-ray Generation With Depth, φ(ρz)
- •X-ray Absorption Effect, A
- •X-ray Fluorescence, F
- •References
- •20.2 Instrumentation Requirements
- •20.2.1 Choosing the EDS Parameters
- •EDS Spectrum Channel Energy Width and Spectrum Energy Span
- •EDS Time Constant (Resolution and Throughput)
- •EDS Calibration
- •EDS Solid Angle
- •20.2.2 Choosing the Beam Energy, E0
- •20.2.3 Measuring the Beam Current
- •20.2.4 Choosing the Beam Current
- •Optimizing Analysis Strategy
- •20.3.4 Ba-Ti Interference in BaTiSi3O9
- •20.4 The Need for an Iterative Qualitative and Quantitative Analysis Strategy
- •20.4.2 Analysis of a Stainless Steel
- •20.5 Is the Specimen Homogeneous?
- •20.6 Beam-Sensitive Specimens
- •20.6.1 Alkali Element Migration
- •20.6.2 Materials Subject to Mass Loss During Electron Bombardment—the Marshall-Hall Method
- •Thin Section Analysis
- •Bulk Biological and Organic Specimens
- •References
- •21: Trace Analysis by SEM/EDS
- •21.1 Limits of Detection for SEM/EDS Microanalysis
- •21.2.1 Estimating CDL from a Trace or Minor Constituent from Measuring a Known Standard
- •21.2.2 Estimating CDL After Determination of a Minor or Trace Constituent with Severe Peak Interference from a Major Constituent
- •21.3 Measurements of Trace Constituents by Electron-Excited Energy Dispersive X-ray Spectrometry
- •The Inevitable Physics of Remote Excitation Within the Specimen: Secondary Fluorescence Beyond the Electron Interaction Volume
- •Simulation of Long-Range Secondary X-ray Fluorescence
- •NIST DTSA II Simulation: Vertical Interface Between Two Regions of Different Composition in a Flat Bulk Target
- •NIST DTSA II Simulation: Cubic Particle Embedded in a Bulk Matrix
- •21.5 Summary
- •References
- •22.1.2 Low Beam Energy Analysis Range
- •22.2 Advantage of Low Beam Energy X-Ray Microanalysis
- •22.2.1 Improved Spatial Resolution
- •22.3 Challenges and Limitations of Low Beam Energy X-Ray Microanalysis
- •22.3.1 Reduced Access to Elements
- •22.3.3 At Low Beam Energy, Almost Everything Is Found To Be Layered
- •Analysis of Surface Contamination
- •References
- •23: Analysis of Specimens with Special Geometry: Irregular Bulk Objects and Particles
- •23.2.1 No Chemical Etching
- •23.3 Consequences of Attempting Analysis of Bulk Materials With Rough Surfaces
- •23.4.1 The Raw Analytical Total
- •23.4.2 The Shape of the EDS Spectrum
- •23.5 Best Practices for Analysis of Rough Bulk Samples
- •23.6 Particle Analysis
- •Particle Sample Preparation: Bulk Substrate
- •The Importance of Beam Placement
- •Overscanning
- •“Particle Mass Effect”
- •“Particle Absorption Effect”
- •The Analytical Total Reveals the Impact of Particle Effects
- •Does Overscanning Help?
- •23.6.6 Peak-to-Background (P/B) Method
- •Specimen Geometry Severely Affects the k-ratio, but Not the P/B
- •Using the P/B Correspondence
- •23.7 Summary
- •References
- •24: Compositional Mapping
- •24.2 X-Ray Spectrum Imaging
- •24.2.1 Utilizing XSI Datacubes
- •24.2.2 Derived Spectra
- •SUM Spectrum
- •MAXIMUM PIXEL Spectrum
- •24.3 Quantitative Compositional Mapping
- •24.4 Strategy for XSI Elemental Mapping Data Collection
- •24.4.1 Choosing the EDS Dead-Time
- •24.4.2 Choosing the Pixel Density
- •24.4.3 Choosing the Pixel Dwell Time
- •“Flash Mapping”
- •High Count Mapping
- •References
- •25.1 Gas Scattering Effects in the VPSEM
- •25.1.1 Why Doesn’t the EDS Collimator Exclude the Remote Skirt X-Rays?
- •25.2 What Can Be Done To Minimize gas Scattering in VPSEM?
- •25.2.2 Favorable Sample Characteristics
- •Particle Analysis
- •25.2.3 Unfavorable Sample Characteristics
- •References
- •26.1 Instrumentation
- •26.1.2 EDS Detector
- •26.1.3 Probe Current Measurement Device
- •Direct Measurement: Using a Faraday Cup and Picoammeter
- •A Faraday Cup
- •Electrically Isolated Stage
- •Indirect Measurement: Using a Calibration Spectrum
- •26.1.4 Conductive Coating
- •26.2 Sample Preparation
- •26.2.1 Standard Materials
- •26.2.2 Peak Reference Materials
- •26.3 Initial Set-Up
- •26.3.1 Calibrating the EDS Detector
- •Selecting a Pulse Process Time Constant
- •Energy Calibration
- •Quality Control
- •Sample Orientation
- •Detector Position
- •Probe Current
- •26.4 Collecting Data
- •26.4.1 Exploratory Spectrum
- •26.4.2 Experiment Optimization
- •26.4.3 Selecting Standards
- •26.4.4 Reference Spectra
- •26.4.5 Collecting Standards
- •26.4.6 Collecting Peak-Fitting References
- •26.5 Data Analysis
- •26.5.2 Quantification
- •26.6 Quality Check
- •Reference
- •27.2 Case Study: Aluminum Wire Failures in Residential Wiring
- •References
- •28: Cathodoluminescence
- •28.1 Origin
- •28.2 Measuring Cathodoluminescence
- •28.3 Applications of CL
- •28.3.1 Geology
- •Carbonado Diamond
- •Ancient Impact Zircons
- •28.3.2 Materials Science
- •Semiconductors
- •Lead-Acid Battery Plate Reactions
- •28.3.3 Organic Compounds
- •References
- •29.1.1 Single Crystals
- •29.1.2 Polycrystalline Materials
- •29.1.3 Conditions for Detecting Electron Channeling Contrast
- •Specimen Preparation
- •Instrument Conditions
- •29.2.1 Origin of EBSD Patterns
- •29.2.2 Cameras for EBSD Pattern Detection
- •29.2.3 EBSD Spatial Resolution
- •29.2.5 Steps in Typical EBSD Measurements
- •Sample Preparation for EBSD
- •Align Sample in the SEM
- •Check for EBSD Patterns
- •Adjust SEM and Select EBSD Map Parameters
- •Run the Automated Map
- •29.2.6 Display of the Acquired Data
- •29.2.7 Other Map Components
- •29.2.10 Application Example
- •Application of EBSD To Understand Meteorite Formation
- •29.2.11 Summary
- •Specimen Considerations
- •EBSD Detector
- •Selection of Candidate Crystallographic Phases
- •Microscope Operating Conditions and Pattern Optimization
- •Selection of EBSD Acquisition Parameters
- •Collect the Orientation Map
- •References
- •30.1 Introduction
- •30.2 Ion–Solid Interactions
- •30.3 Focused Ion Beam Systems
- •30.5 Preparation of Samples for SEM
- •30.5.1 Cross-Section Preparation
- •30.5.2 FIB Sample Preparation for 3D Techniques and Imaging
- •30.6 Summary
- •References
- •31: Ion Beam Microscopy
- •31.1 What Is So Useful About Ions?
- •31.2 Generating Ion Beams
- •31.3 Signal Generation in the HIM
- •31.5 Patterning with Ion Beams
- •31.7 Chemical Microanalysis with Ion Beams
- •References
- •Appendix
- •A Database of Electron–Solid Interactions
- •A Database of Electron–Solid Interactions
- •Introduction
- •Backscattered Electrons
- •Secondary Yields
- •Stopping Powers
- •X-ray Ionization Cross Sections
- •Conclusions
- •References
- •Index
- •Reference List
- •Index
30.5 · Preparation of Samples for SEM
a
b
. Fig. 30.5 Images of a tungsten wire (left) and a human hair (right). a Secondary electron image induced by 5-kV electrons. b Ion induced secondary ion images with 30-kV Ga ions. Note the reduced charging in the ISE image and the increased surface detail visible in the secondary ion image
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. Fig. 30.6 Electron beam (5-kV) induced secondary electron imaging of a free-machining brass (Cu-Zn alloy) that has been coated with layers of Cu, Ni and Au. Note that the various layers are faintly visible and that the contrast is as expected with the highest atomic number region (Pb) brighter than the brass or the Cu and Ni. Au also appears bright
bright relative to the brass as in . Fig. 30.6. . Figure 30.7 demonstrates that the iSE yield is not a simple function of the target atomic number (Joy and Michael 2014). Also,
. Fig. 30.7 demonstrates the very strong grain contrast that can be observed in many crystalline materials. This grain contrast is due to the way that the crystallography of the sample impacts the penetration depth of the primary beam ions and therefore the iSE yield. Small changes in the ion beam incident angle can change the grain contrast that is observed. Thus, if you are trying to determine the nature of the contrast that is observed in a crystalline sample it is a simple matter to tilt the sample 2–4° and observe how the contrast changes. If the contrast is due to ion channeling then the contrast between grains should change (Giannuzzi and Michael 2013).
. Fig. 30.7 Ion beam (30-kV) induced secondary electron imaging of a free-machining brass (Cu-Zn alloy) that has been coated with layers of Cu, Ni and Au. Note that the various layers are much more easily visualized due to the high contrast crystallographic contrast. Also, note that the brightness of the phases can no longer be interpreted strictly by atomic number. Here the Pb and the Au regions appear with lower signal levels than does the brass or the Cu and Ni layers
30.5\ Preparation of Samples for SEM
FIB–based sample preparation for SEM is a large field due to the versatility of modern SEMs and the many techniques that are utilized. One of the most common uses of FIB is for subtractive processing of the sample in that the FIB is used to
\522 Chapter 30 · Focused Ion Beam Applications in the SEM Laboratory
sputter site specific regions of the sample to produce cross sections. It is also common to produce samples that are manipulated from the bulk for study. One example is the extraction and production of thin samples for transmission Kikuchi diffraction as discussed in module 29 on electron backscatter diffraction. FIB has become an indispensable tool in the production of electron transparent samples for STEM/TEM and now the FIB can produce samples that are sufficiently thin for transmission imaging in the SEM at 30 keV using the STEM-in-SEM technique. FIB sample preparation is applicable to many materials classes that are imaged in the SEM including polymers, metal, semiconductors, and
30 ceramics.
30.5.1\ Cross-Section Preparation
In materials characterization it is often of interest to image a section of the sample that is not visible from a planar section. In this case, the FIB is used to mill away material to expose a cross sectional view of the sample, as shown schematically in
. Fig. 30.8. There are many ways to accomplish this and in many modern FIB tools this process is fully automated and the user must simply indicate where the cross section is to be made. The following example will show the steps that are needed for a cross section to be produced.
As was discussed earlier, any time the sample is exposed to the ion beam damage will occur. It is necessary to image the sample during preparation so the easiest way to eliminate the damage to the sample from the beam is to place a protective layer over the area to be cross sectioned. FIB tools come
Ion beam
Electron beam
Stair step cut
. Fig. 30.8 Schematic of an FIB-prepared cross section. A stair-step is milled using the ion beam and then the exposed section that is perpendicular to the original sample surface is polished with a series of lower current ion beams. The cross section can be immediately imaged with the SEM beam that is at some inclined angle with respect to the ion beam
equipped with gas injectors that can be used during sample preparation. Common precursor gasses used can deposit tungsten, platinum, or carbon. Each of these materials works quite well to protect the region of interest from the ion beam. The precursor gasses are delivered to the sample surface through a small needle that is placed in very close proximity to the area of interest. Either the ion beam or the electron beam can be scanned over the area of interest. Some of the gas molecules that are delivered through the needle absorb on to the sample surface where combined action of the primary beam (electron or ion) and the secondary electrons produced by the interaction of the beam with the sample decomposes the absorbed gas. This leaves behind a deposit that contains the desired material but also includes the ion beam species (if ions were used) and some residual organics from the precursor. Due to the short range of ions in materials, the protective layer need not be very thick; but typically most applications use about 1 μm to provide protection and for ease of subsequent milling of the sample. . Figure 30.9 shows a cross section produced in a sulfide copper test coupon where the objective of the experiment was to measure the rate of sulfide growth in accelerated aging conditions. The first step (. Fig. 30.9a) is to deposit the protective platinum layer on the area to be sectioned. The goal is to have the completed cross section positioned under the platinum protective layer. A coarse first cut is made with a large current ion beam, the result of which is shown in . Fig. 30.9b. Although the cross section is relatively clean at this point it is not adequate for quality SEM imaging. Further polishing of the cross section is completed with lower current ion beams in this case . Fig. 30.9c was completed with a 1-nA ion beam and
. Fig. 30.9d is the cross section after final polishing with a 300-pA ion beam. The total time to produce this cross section is about 20 min. The completed cross section imaged at higher resolution is shown in . Fig. 30.10. Note that all of the important microstructural features are easily observed in this very smooth polished cross section.
FIB prepared surfaces can be very smooth and nearly featureless. The relative brightness between different materials can often provide sufficient image contrast. Materials contrast by itself may be insufficient and a method to enhance the contrast may be needed. One way to do this is to introduce gasses near the sample that react with the ion beam and the sample surface to etch the FIB polished surface. One chemical that does this for semiconductor devices is trifluoracetic acid (TFA) that etches oxides and nitrides preferentially to silicon and metals. . Figure 30.11 demonstrates the use of TFA for enhancing the contrast in FIB milled surfaces. The sample was prepared using standard cross sectioning procedures in the FIB. After cross sectioning the sample was rotated and tilted so that the milled surface was normal to the ion beam. A low beam current is selected and then the gas is introduced through a fine needle while the ion beam is scanned over the milled surface. While milling, the sample image provides an etching progress monitor so that the etching progress can be terminated when the correct degree of etching has been achieved.
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30.5 · Preparation of Samples for SEM
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5 mm
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5 mm
. Fig. 30.9 Required steps to making a quality cross section of the surface of a corroded copper test coupon in the FIB. a Deposition of platinum protective layer. b Coarse milling of the cross section with a
. Fig. 30.10 High resolution image of the sulfide layer on the top of the test coupon sectioned in . Fig. 30.9. Note the surface smoothness and the feature sizes that can be observed on the ion milled section
200 nm
7-nA Ga ion beam. c Further polishing with a 1-nA Ga ion beam d Final polishing with a 300-pA Ga ion beam to produce the completed cross section
Ion beam pt
Electron beam pt
Copper sulfide
Au marker layer Copper sulfide copper
524\ Chapter 30 · Focused Ion Beam Applications in the SEM Laboratory
a
30
b
Once the sample was attached to the support structure, final sample polishing was performed and the sample was ready for analysis. EBSD results obtained from the sample shown in
. Fig. 30.12 are shown in . Fig. 30.13. Note that the sample surface is nearly ideal for EBSD as the number of mis-indexed or not indexed pixels is quite low.
This technique of sample lift-out is applicable to all imaging and analysis modes in the SEM. Once the sample is mounted flat on a surface or a support structure it is in an
2 mm ideal sample orientation for imaging with secondary electrons of backscattered electrons. Lift-out samples also provide ideal sample orientations for EDS, WDS, or EBSD analysis. This is not true of cross sections that are milled into the bulk and not lifted out as access to the sample for some imaging and analysis techniques is not close to ideal depending on the particular FIB/SEM platform chosen (Giannuzzi 2006).
2 mm
. Fig. 30.11 This figure demonstrates the enhancement of image contrast using a TFA as a beam assisted etchant. a As-milled cross section of a semiconductor device. Note the surface smoothness and the low contrast. b Same surface after beam assisted etching with TFA. Note that process adds a small amount of topography to the milled surface allowing the different materials to be more easily imaged
SEM applications of FIB sample preparation can also utilize samples that have been removed from the bulk material. This is generally done when the research requires EDS, EBSD, or STEM-in-SEM to be conducted as each of these techniques will not work optimally with standard cross sections (Prasad et al. 2003). Lift-out samples are made by milling trenches on both sides of the area of interest after a protective layer was deposited. The FIB beam is used to cut the sample free from the bulk material and then it can either be polished in the trench or lifted out to a support grid for subsequent polishing and if needed thinning to an acceptable thickness. Figure 30.12 shows some of the steps required to lift-out a 150-μm-wide sample. This was accomplished with a Xe plasma FIB but the steps are the same for a Ga FIB. Ex situ lift-out was used to remove the sample from the bulk followed by attachment to the Cu support structure to allow safe handling of the sample.
30.5.2\ FIB Sample Preparation for 3D Techniques and Imaging
One of the truly important advances in FIB applications is the ability to automate the FIB operation and coordinate it with the SEM imaging or analysis using EDS or EBSD. This coordination allows the FIB column to be used to mill specified volumes from a sample face and then allow that same slice to be imaged or an analytical technique applied and then the process can be repeated. This is often referred to as serial sectioning. In this way a direct reconstruction (direct tomograph) of a 3D volume can be developed. One must always remember though that in this sort of work there is no ability to go back and start over unless a second suitable region is available. It is also important to remember the length scales that are practically reached with FIB methods. The typical area that can be accessed with LMIS-based FIB columns is 50 μm wide by 10 μm deep. The number of slices is limited by the operator’s patience and the stability of the FIB/SEM being utilized.
The first step is to deposit a protective layer over the entire region that is to be milled. This step is necessary, as discussed for single sections, to protect the sample region from damage by the ion beam. The larger the area to be sectioned, the larger the protective layer has to be and this deposition may be quite time consuming. Once the protective layer has been deposited, there are two ways to proceed with serial sectioning and imaging. The easiest method is to simply produce a cross section of the sample, as described previously. The polished face is then used as the starting point of the sectioning. One must be very careful when doing this to ensure that the
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30.5 · Preparation of Samples for SEM
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. Fig. 30.12 Gibeon meteorite sample produced by the lift-out method to produce large area samples suitable for EBSD, TKD, EDS, or STEM imaging. a Milled sample ready for ex situ lift-out. b Lift-out sample on the end of the micromanipulator needle. c Cu support for the sample. It was
placed across the large gap in the middle and epoxied in place. d Sample after final milling of the surface. e Sample arranged on a pre-tilted sample holder for EBSD