fourier transform infrared spectroscopy (1)

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    Fourier TransformInfrared Spectroscopy

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    ABOUTFTIR

    BACKGROUND

    MECHANISMPROCESS

    USESADVANTAGES

    DISADVANTAGES

    OPERATIONPRINCIPLE

    SAMPLE PREPARATION

    DATAANALYSIS

    TYPES

    DEVICE

    TRANSMISSIONTECHNIQUES

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    ABOUTFTIR

    FT-IR stands forFourier TransformInfraRed.

    Named afterJ.B.J. Fourier

    Includes the absorption, reflection,emission, or photoacousticspectrum obtained by Fourier

    transform of an opticalinterferogram.

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    ABOUTFTIR

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    ABOUTFTIR

    Identification of unknown materials

    Determination of the quality orconsistency of a sample

    Determination of the amount ofcomponents in a mixture

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    DEVELOPMENTALBACKGROUND

    late 1880sAlbert A. Michelson invented the

    Michelson Interferometer.

    Performed the experiment to determine the

    speed of light. (Michelson Morleyexperiment).

    1907 Michelson received the Nobel Prize in

    Physics

    Michelson could not take advantage of the

    field ofFourier Transform Spectroscopy (FTS).

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    SCHEMATIC DIAGRAMMICHELSONINTERFEROMETER

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    DEVELOPMENTALBACKGROUND

    1940s Practical Fourier Transform

    Spectroscopy

    Used to measure light from celestial bodies.

    1949 first Fourier transform spectrum

    Different types of interferometers had been

    developed

    Lamellar gratingFabry-Perot interferometers

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    DEVELOPMENTALBACKGROUND

    1960 growing interest in

    interferometric spectroscopy

    J. W. Cooley and John Turkey

    fast Fourier Transform (FFT)

    algorithmAllowed Fourier transforms to be

    computed easily on computers

    available.

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    DEVELOPMENTALBACKGROUND

    1966 the first near infrared

    planetary spectra was recorded

    1969 high resolution and high

    quality spectra of the planets

    first commercial FT-IR

    spectrometer was sold byDigilab.

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    DEVELOPMENTALBACKGROUND

    1970 commercial fourier transform

    spectometers became widely accessible.

    The first FT-IR spectrometers were large

    and expensive.

    1981 Robert Z. Muggli adapted a

    microscope to a FT-IR spectrometer.

    1983 Digilab and Spectra-Techdeveloped the first commercial FT-IR

    microspectrophotometer.

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    DEVELOPMENTALBACKGROUND

    First low-cost spectrophotometer capable

    of recording an infrared spectrum was the

    Perkin-Elmer Infracord in 1957.

    Covered the wavelength range from

    2.5 m to 15 m

    Lower wavelength limit - highest

    vibration frequency due to a

    fundamental molecular vibration.

    Upper wavelength limit - spectral

    region or rock-salt region.

    Later instruments used potassium bromide

    prisms and caesium iodide.

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    DEVELOPMENTALBACKGROUND

    Region beyond 50 m is the far-infrared region

    Merges into the microwaveregion.

    diffraction gratings replacedprisms as dispersing elements.

    More sensitive detectors detect lowenergy radiation.

    Electronic computer needed toperform the required Fouriertransform.

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    USES&APPLICATIONS

    Identify unknown materials

    Determine the quality or consistency of a

    sample

    Determine the amount of components in amixture

    Analysis of liquid chromatography fractions.

    Acquire spectrum of light emitted by the

    sample.

    Photocurrent spectra.

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    USES&APPLICATIONS

    Functional Group Analysis

    Surface Molecular Composition

    Chromatographic Effluents

    Mixture Compound Determination

    Stereochemistry

    Molecular Orientation

    Fingerprinting

    Identification of Reaction components

    Identification of Polymer, Resins, and Plastics

    Formulation of Insecticides and Polymers

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    USES&APPLICATIONS

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    ADVANTAGES

    Non-destructive technique

    Provides a precise measurement method

    which requires no external calibration

    Increase speed, collecting multiple scans

    simultaneously

    Little Sample Preparation

    Identifies structural isomers

    Increase sensitivity and wavelength

    accuracy

    Has greater optical throughput and

    resolution

    Mechanically simple

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    DISADVANTAGES

    FTIR do not measure spectra, only

    interferograms which are difficult to

    interpret.

    Cannot use advanced electronic filteringtechniques (lower S-N Ratio than

    Dispersive)

    Noise sensitive - affects the radiation from

    infrared source

    Uses a single beam changes in infrared

    absorbing gas can affect results

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    TYPESofFTIR

    FAR-INFRARED FTIR

    developed for far-infrared range for

    mechanical tolerance needed for good

    optical performance.

    A typical instrument was the cube

    interferometer developed at the NPL and

    marketed by Grubb Parsons.

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    TYPESofFTIR

    NEAR-INFRARED FTIR

    The near-infrared region spans the

    wavelength range between the rock-salt

    region and the start of the visible region at

    about 750 nm.

    Fundamental vibrations can be observed

    in this region.

    It is used mainly in industrial applications

    such as process control and chemical

    imaging.

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    OPERATIONPRINCIPLE

    I is the constant level with no modulation present.

    The second term - spectrum.

    The lower integration limit can be set to - sinceB() = 0 for all negative .

    I(x) is defined as the modulated part of the

    interferogram.

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    OPERATIONPRINCIPLE

    I() is the light source intensity distribution

    B() is the modified source function.

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    DEVICE

    Three basic spectrometer components in an

    FT system:

    Radiation source

    Interferometer

    Detector

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    DEVICE

    IMV-4000 The newest most rapid FTIRArray micrscope.

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    DEVICE

    PARTS OF MICHELSON Interferometer

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    DEVICE

    Interferometerproduces a unique signal which contains

    infrared frequencies encoded into it

    Mirrorsreflects the beam transmitted

    Beam Splittertakes the incoming infrared beam and

    divides it into two optical beamsDetector

    where all radiation incident on the

    interferometer is registered.

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    DEVICE

    Spectrometer Layout

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    DEVICE

    Spectrometer Layout

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    SPECTROMETERDESIGN

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    SPECTROMETERDESIGN

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    SPECTROMETERDESIGN

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    MECHANISM

    1. The Source: Infrared energy is emitted

    from a glowing black-body source. This

    beam passes

    through an aperture which controlsthe amount of energy presented to the

    sample

    2. The Interferometer: The beam enters the

    interferometer where the spectralencoding takes place.

    The resulting interferogram signal

    then exits the interferometer.

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    MECHANISM

    3. The Sample: The beam enters the sample

    compartment where it is transmitted through

    or reflected off of the surface of the sample,

    depending on the type of analysis beingaccomplished.

    This is where specific frequencies of

    energy are absorbed.

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    MECHANISM

    4. The Detector: The beam finally passes to

    the detector for final measurement. The

    detectors used are specially designed to

    measure the special interferogram signal.

    5. The Computer: The measured signal is

    digitized and sent to the computer where

    the Fourier transformation takes place.

    The final infrared spectrum is thenpresented to the user for

    interpretation and any further

    manipulation.

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    MECHANISM

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    MECHANISMPROCESS

    A collimator is irradiated with monochromatic

    light yielding a parallel ray of light.

    The ray is split into two components in the

    beam splitter.

    Following reflection in the mirrors another

    passage through the beam splitter occurs

    Rays are added on the detector.

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    TRANSMISSIONTECHNIQUES

    Solid Samples:

    KBr Disk Technique

    Quantitative analysis of organic or

    inorganic substances in powder form.

    Thin-Film Technique

    Polymeric qualitative and quantitative

    analysis for substances in film form.

    Solution Technique

    Primarily qualitative analysis of substances

    dissolved in solvent. Uses liquid cells

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    TRANSMISSIONTECHNIQUES

    Liquid Samples:

    Liquid Film Technique

    Qualitative analysis of viscous and

    nonvolatile substances

    Solution Technique

    Qualitative analysis of liquids that dissolve

    in solvent and nonvolatile substances

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    RELATEDTECHNIQUES

    Nuclear magnetic resonance

    Additional information on detailed

    molecular structure

    Mass spectrometry

    Molecular mass information andadditional structural information

    Raman spectroscopy

    Complementary information on molecular

    vibration.

    Facilitates analysis of aqueous samples.

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    SAMPLEPREPARATION

    SamplesState

    Any solid, liquid or gas sample

    Amount Solids:50 to 200 mg is desirable, but 10 g

    ground with transparent matrix

    1 to 10 g minimum is required if solid issoluble in suitable solvent.

    Liquids: 0.5 L is needed if neat, less ifpure.

    Gases: 50 ppb is needed

    Preparation Little or no preparation is required;suitable solvent

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    SAMPLEPREPARATION

    Analysis TimeEstimated time: 1 to 10 min depending on the

    type of instrument and the resolution required.

    Samples are prepared 1 to 5 min.

    DATAANALYSIS

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    DATAANALYSIS

    Emission Spectrum

    from a light source

    obtained by passing the light

    through a monochromator,

    Intensity of remaining light is

    measured.

    Intensity that was directly measured.

    DATAANALYSIS

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    DATAANALYSIS

    Absorption spectrum Light source with continuous spectrum

    in a broad wavelength range.

    Gas sample placed between the beam

    splitter and the detector.

    Measurement

    Background acquired without the

    sample cell

    Measurement done with the cellplace in sample compartment.

    Difference of the measurements -

    measure of the absorption.

    DATAANALYSIS

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    DATAANALYSIS

    The spectrum of light of blue flame of butane torch.

    Horizontal axis is the wavelength of light

    Vertical axis represents amount of light emitted

    DATAANALYSIS

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    DATAANALYSIS

    DATAANALYSIS

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    DATAANALYSIS