Notes
Slide Show
Outline
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Skoog – Chapter 7
Components of Optical Instruments
  • General Design of Optical Instruments
  • Sources of Radiation
  • Wavelength Selectors
  • Sample Containers
  • Radiation Transducers (Detectors)
  • Signal Processors and Readouts
  • Fiber Optics
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Ultraviolet – Visible – Infrared Instrumentation
  • Focus our attention on measurements in the UV-vis region of the EM spectrum
  • Good instrumentation available
  • Very widely used techniques
  • Longstanding and proven methods
  • IR instrumentation will be considered from time to time particularly when there are similarities to UV-vis
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"Absorption measurements require:"
  • Absorption measurements require:
  • 1) source of radiation
  • 2) device for dispersing radiation into component wavelengths
  • 3) a means of putting sample into the optical path, i.e., cell
  • 4) Detector to convert the EM to an electrical signal
  • 5) readout device or circuitry, i.e., meter, computer, recorder, integrator, etc.
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"Block diagram of instrument for..."
  •  Block diagram of instrument for absorption
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"Block diagram of instrument for..."
  •  Block diagram of instrument for absorption
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"Emission measurements require:"
  • Emission measurements require:
  • 1) means of exciting emission i.e., way of populating upper energy level which spontaneously emits
  • 2) device for dispersing radiation into component wavelengths
  • 3) a means of putting sample into the optical path, i.e., cell
  • 4) Detector to convert the EM to an electrical signal
  • 5) readout device or circuitry, i.e., meter, computer, recorder, integrator, etc.
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"Block diagram of instrument for..."
  •  Block diagram of instrument for emission    i.e.,
  •                                                           &  fluorescence
  •                                                          phosphorescence
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"The requirements for the various..."
  • The requirements for the various components used in different instruments change with the type of spectroscopy as well as for different kinds of measurements within a type of spectroscopy
  • We will consider the components separately then combine them to make the overall instrument
  • And finally look at the measurements with regard to theory and practice
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"Sources – important characteristics"
  • Sources – important characteristics
  • 1) Spectral distribution i.e., intensity vs. λ                              (continuum vs. line sources)
  • 2) Intensity
  • 3) Stability – short term fluctuations (noise), long term drift
  • 4) Cost
  • 5) Lifetime
  • 6) Geometry – match to dispersion device
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"CONTINUUM SOURCES"
  • CONTINUUM SOURCES
      • Thermal radiation (incandescence) – heated solid emits radiation close to the theoretical “Black Body” radiation i.e., perfect emitter, perfect absorber

    • Behavior of Black Body
    • - Total power ~ T4  therefore need constant temperature for stability when using incandescent sources
    • - Spectral distribution follows Planck’s radiation law
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"Spectral Distribution Curves of a..."
  • Spectral Distribution Curves of a Tungsten (Black Body) Lamp
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"IR Region thermal sources (..."
  • IR Region thermal sources (Black Body) are:
  • Nernst Glower – fused mixture of ZrO2, Y2O3, and ThO2 normally operated at 1900 oC – better for shorter IR λ’s (near IR)
  • Globar – silicon carbide normally operated at 1200 to 1400 oC – better at longer IR λ’s (doesn’t approach Black Body)
  • Incandescent Wire – e.g., nichrome wire – cheapest way
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"All operated at relatively low..."
  • All operated at relatively low temperature.
  • Good for IR and give some visible emission.
  • Operated in air so will burn up if temp goes too high
  • Advantages
  • Nernst Glower – low power consumption, operates in air, long lifetime
  • Globar – more stable than Nernst Glower, requires more power & must be cooled.  Long lifetime, but resistance changes with use
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"Visible Region sources are:"
  • Visible Region sources are:
  • Glass enclosed Tungsten (W) filament - normally operated at ~3000 oK with inert atmosphere to prevent oxidation.  Useful from 350 nm to 2000 nm, below 350 nm glass envelope absorbs & emission weak
  • Tungsten-Halogen lamps - can be operated as high as 3500 oK.  More intense (high flux).  Function of halogen is to form volatile tungsten-halide which redeposits W on filament, i.e., keeps filament from burning out.  Requires quartz envelope to withstand high temps (which also transmits down to shorter wavelengths).  Fingerprints are a problem – also car headlights
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"Gas Discharge Lamps – two..."
  • Gas Discharge Lamps – two electrodes with a current between them in a gas filled tube.  Excitation results from electrons moving through gas.  Electrons collide with gas ΰ excitation ΰ emission
  • At high pressure ΰ “smearing” of energy levels ΰ spectrum approaches continuum
  • The higher the pressure, the greater the probability that any given molecule or atom will be perturbed by its neighbor at the moment of emission.
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"Hydrogen Lamp - most common..."
  • Hydrogen Lamp - most common source for UV absorption measurements
  • H2 emission is from
  • 180 nm to 370 nm
  • limited by jacket


  • Line spectrum from ΰ
  • 100 watt Hydrogen
  • Lamp at low pressure in
  • Pyrex
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"Deuterium Lamp – same λ..."
  • Deuterium Lamp – same λ distribution as H2 but with higher intensity (3 to 5 times) -
  • D2 is a heavier
  • molecule & moves
  • slower so there is
  • less loss of energy
  • by collisions


  • High pressure D2 ΰ
  • with quartz jacket
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"For higher intensity"
  • For higher intensity
  • Xenon Lamp – Xe at high pressure (10-20 atm)
  • - high pressure needed
  • to get lots of collisions
  • for broadening
  • leading to continuum
  • - short life relatively
  • - arc wander (stabilize)
  • - need jolt to start
  • - output = f(time)
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"d)"
  • d) High Pressure Mercury Lamp – can’t completely eliminate bands associated with particular electronic transitions even at very high pressures (e.g., 100 atm)
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"For UV-vis absorption spectrophotometry usually..."
  • For UV-vis absorption spectrophotometry usually use H2 for UV and tungsten for visible region (switching mid scan)
  • Sometimes use D2 instead of H2
  • For fluorescence spectrophotometry use xenon arc lamp in scanning instruments
  • Can use He below 200 nm
  • Hg at low pressure is used in fixed wavelength (non scanning) fluorometers
  • Can use mixture of Hg and Xe
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"LINE SOURCES"
  • LINE SOURCES
    • Gas (Vapor) Discharge Lamps at low pressure (i.e., few torr) – minimize collisional interaction so get line spectrum
    • - most common are Hg and Na
    • - often used for λ calibration
    • - Hg pen lamp
    • - fluorescent lights are another example
    • - also used UV detectors for HPLC
    • Hollow Cathode Lamps (HCL) – for AA
    • Electrodeless Discharge Lamps (EDL) - AA
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"4)"
  • 4) Lasers (Light Amplification by Stimulated Emission of Radiation) – start with material that will exhibit stimulated emission and populate upper states typically using another light source
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"Stimulated Emission – photon strikes..."
  • Stimulated Emission – photon strikes excited state causing it to emit a burst of photons
  • Pumping source used to populate upper states can be flashlamp, another laser or electrical
  • Often use prism to select pumping wavelength


  • Advantages of lasers
  • 1) Intense
  • 2) Monochromatic – very narrow band
  • 3) Coherent – all radiation at same phase
  • angle
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"4)"
  • 4) Directional – full intensity emitted as beam


  • Limitations of lasers
  • High cost in many cases
  • Wavelength range is somewhat limited
  • Many operate in pulsed mode – some are continuous wave (CW)


  • Pulsed mode lasers are not always problematic as light sources, can use pulse frequency with gated detection
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"Types of Lasers:"
  • Types of Lasers:
  • 1) Solid State Lasers
  • a) Ruby laser – Al2O3 + Cr(III) - 694.3 nm pumped with Xe arc flashlamp – pulsed (can be continuous)
  • b) Nd/YAG laser – yittrium aluminum garnet + Nd - 1064 nm
  • 2) Gas Lasers
  • a) Neutral atom – He-Ne – 632.8 nm continuous
  • b) Ion lasers – Ar+ or Kr+ 514.5 nm
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"c)"
    • c) Molecular lasers – CO2 (10,000 nm = 1000 cm-1) or N2 (337.1 nm) pulsed
    • d) Eximer lasers – inert gas + fluorine creates eximers ArF+ (193 nm), KrF+ (248 nm), XeF+ (351) pulsed
    • Dye Lasers – tunable over 20 – 50 nm many dyes available for wide range of λ’s
    • Semiconductor Diode Lasers – wide range of λ’s available, continuous
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Wavelength Selection
  • Three main approaches:
  • 1) Block off unwanted radiation – optical filters
  • 2) Disperse radiation & select desired band – monochromator
  • 3) Modulate wavelengths at different frequencies - interferometer
  • FILTERS
  • 1) Absorption – colored glass, colored film, colored solutions – cheapest way
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"Absorption filters are also known..."
  • Absorption filters are also known as bandpass filters
  • Usually exhibit low peak transmittance
  • Typically have a broad peak profile
  • Can use two or more absorption filters together to produce desired transmittance characteristics
  • Generic filters are 2 x 2 inch glass or quartz
  • Relatively inexpensive
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"2)"
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"Condition for constructive interference"
  • Condition for constructive interference


  •                                   mλ
  •                          2d = ------
  •                                     η




  • If distance (d) is multiple (m) of wavelength (λ) then it won’t be interfered with
  • Concept of Order – constructive & destructive interference causes waves with different phase angles to be eliminated except if they are multiples of each other
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"Transmittance vs."
  • Transmittance vs. wavelength for typical Fabrey-Perot Interference filter showing first and second order λ’s (m = 1 & m = 2)
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"3)"
  • 3) Neutral density filters – reduces intensity without any λ discrimination
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"MONOCHROMATORS"
  • MONOCHROMATORS


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"Optical Materials – need optically..."
  • Optical Materials – need optically transparent materials for lenses, prisms & sample cells
  • In visible region – can use glass down to 350 nm
  • In the UV region – quartz is material of choice
  • In the IR region – NaCl, KBr, etc. The heavier the atoms of the salt, the farther into the IR region (i.e., longer λ) before significant absorption occurs
  • Problem – sensitivity to moisture