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General

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KBr is almost universally used as a substrate material in FTIR beamsplitters ... So they are referred to as Ge on KBr beamsplitters ... – PowerPoint PPT presentation

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Title: General


1
General
  • This is the subtitle

2
Introduction to Fourier Transform Infrared
Spectroscopy
3
What is FTIR?
  • FTIR stands for Fourier Transform Infra Red, the
    preferred method of infrared spectroscopy.
  • A method for measuring all of the infrared
    frequencies simultaneously, rather than
    individually as with dispersive instruments

4
Why Infrared Spectroscopy ?
  • An Infrared spectrum represents a fingerprint of
    a sample with absorption peaks which correspond
    to the frequencies of vibrations between the
    bonds of the atoms making up the material-Because
    each different material is a unique combination
    of atoms, no two compounds produce the exact same
    spectrum, therefore IR can result in a unique
    identification of every different kind of
    material!

FingerPrint
5
Infrared Spectroscopy is simply the study of the
interaction of Infrared light with matter!!
  • Most powerful aspect is the ability to identify
    complete unknowns
  • direct correlation between the wavenumbers at
    which a molecule absorbs infrared radiation and
    its chemical structure

6
Infrared Spectroscopy
UV
VIS
NIR
IR
Far IR
Microwave
10-5
10-5
10-4
10-3
10-2
10-1
Wavelength (cm)
Energy (Frequency)
Light, or more properly, electromagnetic
radiation, can be described in terms of
frequency ? or wavelength ? . Energy of
radiation increases with increasing frequency
and decreases with increasing wavelength
7
Wavenumbers (cm-1) - standard


IR spectral units
  • Modern infrared instruments record the absorption
    of energy as a function of decreasing frequency
    (decreasing energy) from left to right
  • W ( cm-1) 1/?
  • A frequency-related unit known as a wavenumber
    is expressed as reciprocal centimeters- number
    of vibrations occurring over 1 cm


8
WAVENUMBER SCALE
9
Origins of Infrared Absorptions
  • All atoms within molecules are in constant
    vibration
  • all bonds with a permanent dipole (slightly
    electronegative charge) will absorb infrared
    radiation at the appropriate vibrational
    frequency (??/ ?X ? 0 )
  • the vibrational frequency will depend on the
    atoms associated with the bond as well as the
    bond strength

10
Symmetric stretching
In-plane bending
Antisymmetric stretching
Out-of-plane bending
When the molecule is irradiated with IR
electromagnetic radiation, the vibrating bond
will absorb energy if the frequencies of the
light and the vibration are identical
11
Nature of Molecular Vibrations Normal Modes
STRETCHING
VIBRATING BONDS
CONTRACTING
When a molecule absorbs IR radiation, its
chemical bonds vibrate. The bonds can
stretch, contract, and bend. Vibrational motion
can be broken down into a number of constituent
vibrations called normal modes (Rough Guide-
of atoms in a molecule helps

determine of vibrations a molecule
possesses)
12
Factors affecting frequency of
molecular vibrations
  • Mass of the atoms - heavier molecules will result
    in slower movement and result in lower
    frequencies
  • Elasticity of the spring (force constant) - a
    stronger spring (bond) will cause the vibration
    to be more rapid than a weaker one- HIGHER
    FREQUENCY
  • Bond Strength - increasing of bonds increases
    frequency of vibration

13
Dispersive IR Instruments
  • Infrared light from the source passes through the
    sample, then goes through a slit into a grating
    to disperse the light into a spectrum of its
    component wavenumbers.
  • The grating is rotated so that different
    wavenumber slices pass through the slit and are
    sampled by the detector

14
A Dispersive Infrared Spectrophotometer
Shimadzu IR-470
15
Older Technology- limitations
  • Slow Measurements Because dispersive
    instruments measure each frequency individually,
    a single measurement may take as long as 15
    minutes
  • Relatively Insensitive Older instruments
    employed detectors which required a large amount
    of sample. Today we can detect as little as 0.01
    of a compound in a particular matrix with FTIR
  • Mechanically Complex- Because dispersive
    instruments have lots of moving parts, they are
    susceptible to mechanical failure increasing
    possible instrument down time and the slits throw
    most of the sample beam away at any one time
    anyhow

16
Advantages of FTIR (technique)
  • Universal technique
  • sensitivity 10-6 grams
  • fast and easy
  • relatively inexpensive
  • rich information
  • sensitive to molecules-anything that contains
    chemical bonds
  • vast majority of molecules in the universe absorb
    mid-infrared light, making it a highly useful
    tool

17
Disadvantages of FTIR
  • Cannot detect atoms or monoatomic ions - single
    atomic entities contain no chemical bonds
  • Cannot detect molecules comprised of two
    identical atomS symmetric-such as N2 or O2.
  • Aqueous solutions are very difficult to analyze-
    water is a strong IR absorber
  • Complex mixtures - samples give rise to complex
    spectra

18
Michelson Interferometer
IR radiation from the source is separated by the
beamsplitter into two beams that travel different
pathlengths.When these two separated beams are
recombined, an interference pattern is generated
and passed through the sample. The FTIR relies on
a mathematical (Fourier Transform) reconstruction
of the spectrum from this interference pattern
19
Constructive Interference
? n? Constructive Interference will take
place for any value of ?
when the two beams are in phase
n0,1,2,3,..
20
Destructive Interference
Fixed Mirror
Moving Mirror
? ( n 1/2 ) ? Totally destructive
interference takes place when optical path
difference is 1/2 ? or some multiple of it-beams
are completely out of phase
21
At all path differences other than ZPD (zero path
difference), a variation of constructive and
destructiveinterference takes place - this
modulated radiation is denoted by how many
times a wave may switch between being light and
dark known as the frequency
22
where Fv Modulation
frequency Fv 2VW V moving
mirror velocity in cm/sec
W wavenumber passing
through interferometer -Both of these
wavenumbers are distinguished by the detector as
a cosine wave, but their frequencies
are different as expected from the equation above
23
Interferogram of a Broadband Source
A plot of light intensity versus optical path
difference is an Interferogram These are the
fundamental measurements obtained by an FTIR
24
Relationship between Interferogram and Power
Spectrum
25
FTIR HhOWHHrinciples
How an Interferogram becomes a Spectrum!
26
Fourier Transform of an Interferogram
  • The wavelength and intensity data at each point
    in the scanned spectrum are encoded so that all
    of the spectral information is acquired at once
    it is mathematically decoded through Fourier
    Transform.
  • Essentially, wavelength and intensity are related
    mathematically to mirror position and velocity.

27
What is Apodization?????? (comes from
Greek word a podi or no feet)
  • Calculating A Fourier Transform involves
    performing a mathematical integral on the IFG.
    Ideally the limits of this integral should be /-
    infinity (infinity for OPD and of data points
    collected to Fourier Transform properly) - This
    is impossible, so the IFG and the integral must
    be truncated at some point, the limits being 0
    OPD and the maximum OPD
  • An unfortunate outcome of truncating the signal
    is the lineshapes become distorted causing
    sidelobes which are sinusoidal undulations in
    the baseline. These lobes, or feet are
    suppressed by multiplying the IFG by an
    Apodization Function

28
Main Side-Effect of Apodization!!
  • - Spectral Resolution Will be Reduced - AFs
    vary in how well they suppress sidelobes, and how
    much they degrade resolution
  • AF that provides the highest resolution, and does
    the worst job of suppressing sidelobes, is the
    boxcar apodization (only use with gases or where
    utmost resolution is required)
  • AF recommended for Condensed Phase samples is
    Happ-Genzel or Medium Beer-Norton

29
Relationship between the Interferogram and the
Spectrum
30
Multiplex (Fellgett) Advantage
All wavelengths measured all the time-because all
data is measured simultaneously, measurements are
made in seconds rather than several minutes

31
Jacquinot ( Throughput) Advantage
'
All infrared radiation passes through the sample
and strikes the detector at once-there are no
slits to restrict the energy increased
sensitivity and reduced noise automatically
32
Connes (Frequency Calibration) Advantage
Because the He-Ne laser emission occurs at
exactly 632.8nm, it is used to set the exact
wavenumber(cm-1) scale in the IR spectrum
Spectrum of high wavenumber accuracy is obtained
and you never have to calibrate
33
The Signal-Averaging Advantage
  • Fast scans with an FTIR enable the coaddition of
    many scans in order to reduce the random
    measurement noise-use the computer to do this
    quite easily
  • The positive and negative fluctuations in the
    random noise level cancel themselves out as more
    scans are added together

34
FTIR 8300/8400/8700/8900 SOURCE
  • Purpose provide radiant energy in the infrared
    region of the electromagnetic spectrum
  • Ceramic Source/Globar- bright and very intense -
    inert solid is heated electrically to 1500-2000 K
    -guaranteed for 5000 hours

35
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36
BEAMSPLITTER
  • KBr is almost universally used as a substrate
    material in FTIR beamsplitters-this material does
    not split the beam since it transmits in the IR
  • Instead, a thin coating of Germanium is
    sandwiched between two pieces (disks) of KBr, and
    it is this Ge coating that splits the beam. So
    they are referred to as Ge on KBr beamsplitters
  • Disadvantage KBrs natural tendency to absorb
    moisture-fogging

37
FTIR 83/84/87/8900 Interferometer
Mirror is the only
moving part
  • FJS -Flexible Joint Support-
    unique-patented
  • Shimadzu system
  • Swing system with smooth film support
    system.
  • Base plate swings while keeping parallel against
    the
  • top plate.
  • Mirror is mounted in front of the base.
  • Mirror runs parallel with theTop plate
  • Advantage
  • Long endurance and precision because of
    noncontact
  • free from wear


  • High linearity and precision almost equal to an
    air
  • bearing system

38
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39
Friction-less Mirror Drive Requires No
Maintenance
  • Unique, patented Shimadzu design employs a
    friction-less electro-magnetic moving mirror
    drive supported by two tough, durable polyimide
    sheets (a flexible joint support system).
  • Stability and linearity of response is equivalent
    to the Air-bearing Drive without the need for
    pure, dry air

40
FTIR83/84/87/8900 DETECTORS
  • DLATGS (deuterated L-Alanine doped tri-glycine
    Sulfate) - Shimadzu patented design
  • pyroelectric bolometer - changes in the amount of
    infrared radiation striking the detector cause
    the temperature of the DTGS element to change,
    measured as a voltage change
  • -Temperature controlled high sensitivity
    detector-better sensitivity than traditional DTGS
    detector
  • MCT Detector (optional) - AIM Microscope required
  • ----mercury cadmium telluride (HgCdTe)- consists
    of an alloy of 3 elements, and it is a
    semi-conductor. Energy is detected by use of a
    bandgap (photons exceeding the energy bandgap
    will be detected)

41
He-Ne Laser
  • Laser acts as an internal wavenumber standard. -
    He-Ne gives off light at precisely 15,798.637
    cm-1. All infrared frequencies are measured
    relative to it.
  • Laser is used to track the position of the moving
    mirror. - so the optical path difference can be
    measured precisely and any adjustments will be
    made instantaneously to the fixed mirror
    positioning

42
Dynamic Alignment System
43
Dynamic Auto-Alignment for Maximum Reproducibility
  • Dynamic feedback loop - maintains the optimum
    alignment conditions during measurement, a
    consistently stable and reproducible spectrum is
    obtained.
  • Continuous laser referencing - operates
    continuously at 5,000 to 10,000 Hz
  • Auto-Adjust Function - provides quick and easy
    fine tuning of the interferometer. It eliminates
    the need for tedious mechanical adjustments

44
Dynamic Auto-Alignment (contd)
  • Recalls last position at power-down
  • Minimizes start-up time
  • 5 min or less for Qualitative Analysis
  • 30 min for Quantitative Analysis
  • Eliminates the need to keep the FTIR on
    continuously

45
Triple Protection of the Interferometer
46
Interferometer Optical Component Protection
features
  • A high-tech proprietary anti-moisture coating is
    applied directly to the KBr beamsplitter surface
  • Optical compartment is sealed and desiccated with
    Calcium Oxide - will not re-release moisture back
    into the optical compartment
  • KRS-5 Exit Window does not react with water, it
    is impervious to moisture and will never fog-
    Disadvantage only 70 transmissivity

47
Common Causes of Instrument Problems?
  • Beam blocked by something
  • Low throughput accessory
  • Poor (vibration,humidity) operational environment
  • Failing Source
  • Fogged Beamsplitter
  • Poorly Aligned (tuned) moving mirror
  • Failing detector
  • Electronic Failures

48
Initial Suggestions to Follow
  • Follow infra red beam (Are laser spots in the
    sample compartment visible on your hand?) - Make
    sure no obstructionsin light path/ Does problem
    exist with Accessories removed?
  • Turn power on/off - Look for laser lights. If not
    present, replace laser tube/laser power supply

49
More Suggestions !
  • Inspect beamsplitter for fogging, and replace if
    necessary
  • Check the Moving Mirror in Hayato 105 (Service
    Mode) and see if it moves freely-it should since
    we are forcing it to move- If it does not then
    inspect with different scanning speeds to observe
    movement- if none- replace the CPU boards- FTIR
    Main/Digital II

50
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