Title: EDS Energy Dispersive Spectroscopy
1EDSEnergy Dispersive Spectroscopy
2Background Theory
- Introduction to the EDS System
- Hardware Software
- X-Ray Signal Generation
- Signal Origin, Spatial Resolution, Direction of
Signal, Sample Surface - EDS Instrumentation Signal Generation
- Detector and geometry efficiency, Signal
processing, Energy Resolution, Collimation
3Introduction to the EDS System
4Hardware Schematic
SEM Column
Monitor (MCA Display)
Dewar
FET
Preamp
Chamber
Pole Piece
HP Computer
Detector
EDAM III
Window
PCI
Sample Stage
Collimator
5Processing Schematic
Spectrum Interpretation
Electron Beam
Signal Processing
Beam- Specimen Interaction
Signal Detection
X-Ray Signal
6X-Ray Signal Generation
- Signal Origin
- Spatial Resolution
- Directionality of Signals
- Analysis of Rough Surfaces or Particles
7Bohr Model of the Atom (a simplified view)
---where X rays come from
La
Lb
Ka
Kb
Ma
Real life spectra are more complex because there
are multiple orbitals (esp. for the L, M and N
orbitals). L-series spectra in EDS can have 6 or
7 peaks.
Nucleus
8Atomic Number Order for the K Series Peaks
9Chart of Lines visible 0-10 kV
- K Lines - Be (Z4) to Ga (Z31)
- L Lines - S (Z16) to Au (Z79)
- M Lines - Zr (Z40) to the highest occurring
atomic numbers.
Every element (Zgt3) will have at least one line
viewable between 0.1 and 10 keV. In some overlap
conditions it might be necessary to examine the
area between 10 and 20 keV.
10Interaction Volume Regions
primary beam
sample surface
se
bse
This diagram is somewhat misleading. High-energy
and low-energy x rays behave very differently
(just like e-).
x-rays
High energy x rays can not be excited at great
depths. Low energy x rays can be excited at
great depths, but will most likely be absorbed
and will not escape.
11SE vs BSE Images
SE -- Edge effect, charge sensitive, very
little Z contrast.
BSE --Z contrast dominates, no edge
effect, no charging seen.
12X-Ray Spatial Resolution
Low Z
Spot size does not determine the reso-lution but
kV and Z are more significant.
High Z
Low kV
High kV
13Signal Resolution
- Signal resolution (se) is determined by the width
of the electron beam (spot size) and is
proportional to the signal depth.
x-ray
se
bse
sample surface
se
bse
x-rays
14Directionality of Signals
- SE Signal - attracted to positive voltage on wire
mesh network in front of detector. - BSE Signal - Detector is arranged to collect
signals from a large, symmetrical area. - X-ray Signal - most directional of all signals,
only one detector with no way to influence the
trajectory of x-rays
15Spectrum Anomalies
Detector
Electron Beam
Backscatter electrons
Fluorescence
X-rays
Specimen Matrix
Interaction volume
Absorption of x-rays
16Directionality of X-ray Signal
Detector Direction
A B C
stage/mount
sample
Topography has a significant effect on spectrum
count rate and on composition (take-off angle
and absorption effects)
17B
A Lower low end peaks B Normal C Higher low
end peaks
C
A
3 different spectra at 3 locations on the same
particle with a uniform composition.
Take-off angle is highest at C and lowest at A.
18Effects of Tilt (FeCO3)
Peaks are autoscaled to the O K peak. Q What if
they were scaled to the background area? A FeK
same height, C K, O K and FeL would be higher at
30 degrees.
19EDS Instrumentation Signal Detection
- X-Ray Detectors
- The Detector Efficiency
- Geometrical Efficiency
- Signal Processing
- The Signal Processor
- Energy Resolution
- Collimation
20X-section of window crystal (sapphire)
-500 to 1000 volts
,- charges
x-ray (photon) microscope vacuum
to preamplifier (FET)
Detector Vacuum
Detector
SiLi
Detector Window 8u Be or 0.3u Polymer
Metallization Layer,(85 angstroms) plus the Si
dead layer
21Detector EfficiencyWindow Transmission
Capabilities
- I / Io e -(mr t)
- Where
- I Final Intensity
- Io Initial Intensity
- m mass absorption coefficient
- r density
- t thickness
22Transmission of K x-rays through various windows
23Mass Absorption Coefficient
N Ka Energy
Absorption edge or critical excita- tion energy
Absorption
(Kab)
C
C Ka Energy
0.284
X-ray Energy (keV)
24Absorption evidence in Spectra
The background is lower on the high-energy side
due to absorption in the sample.
25Solid Angle
- W A/d 2
- Where
- A detector area, mm 2
- d the sample to detector distance
- The solid angle (omega) is in steradians. Count
rate at 70 mm scale setting 1/4 that at 50 mm.
26The Preamplifier
50 ns/x-ray event
C
Output
FET
Ultimate peak measurement time will be about 50
us (1000x 50 ns)
Reset
Detector
27Output signal of an X-Ray Event (or 3 events)
Higher dead time (all rejected)
Voltage (mv)
Lower dead time
v
Time
Multiple x-ray events too close to each other
will be rejected.
28Throughput Curves
Lesson High count rates and high dead times
actually give fewer counts and poorer spectra.
You might consider a faster time constant.
29Multichannel Analyzer
30Resolution Equation
- FWHM SQRT(FWHM)noise2 (2.35 FEe)2
-
- Where
- F fano factor 0.11
- E energy of the x-ray, ev
- e 3.8 ev/charge pair (Si), 2.96
ev/charge pair (Ge)
31Resolution vs Energy for 70ev noise
Mn
32Collimators
Be Window with no magnets (BSE do not penetrate)
SUTW or UTW Window with magnets (shown in yellow)
to deflect BSE
If BSE reach the detector they will
produce background anomalies --a hump in
the background at high energies.