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THE SPECTRO-PAEDIA

click on any item in the list for its wikipedia entry if available.


absorbance
adsorption
Atomization
bandwidth
Beamsplitters
bioluminescence
chemiluminescence
chromatography
electroluminescence
electromagnetic
emission
Emissivity
Fluorescence
luminescence
Michelson
monochromators
photo-multiplier
Phosphorescence
photodiodes
photoelectric
photoluminescence
Rayleigh
Raman
spectrofluorometer
spectrometer
spectrophotometer
Spectrum
Transmittance
ultraviolet
Visible
wavelength
Wavenumber
UV Light
Beer's Law
Diode Array
Deuterium Discharge Lamp
Low Pressure Zinc Discharge Lamp
High Pressure Mercury Discharge Lamp
Low Pressure Cadmium Lamp
Tungsten Halogen Lamp
Lens and Window Material in Spectrometers
Cuvettes
Luminescence
Photoluminescence
Fluorescence
Phosphorescence
Bioluminescence
Radioluminescence
Electroluminescence
Fluorescence Reagents
Spectrum
Diffraction Grating
Interferogram
Fourier Transform IR Spectrometer
FT-IR
Halide Disks
Mull Samples
Film Samples for IR Spectroscopy
Light Pipes
Attenuated Total Reflectance Spectroscopy
Multiple Internal Reflectance
External Reflectance
Specular Reflectance
Diffuse Reflectance
Photoacoustic Spectroscopy
Beam Splitter
Raman Scattering
Rayleigh Scattering
Raman Spectroscopy
Atomic Spectroscopy
Atomic Emission Spectroscopy
Atomic Absorption Spectroscopy
The Inductively Coupled Plasma Torch
The Helium Plasma Torch
Emission Spectrometer
Atomic Absorption Spectrometry
Flame Atomic Absorption Spectrometer
Flame AA
Hollow Cathode Lamp
Electrothermal Atomization
Graphite Furnace
L’vov Platform
Electron Paramagnetic Resonance
Zeeman Effect
Continuous Wave
Electron Paramagnetic Resonance
Pulsed EPR
Electron Spin Echo
Multple Resonance Spectroscopy
Magnetic Resonance Spectroscopy
NMR
Precessing
Nucleus Spin Decoupling in NMR
Superconducting Magnets
NMR Microcells
Electron Impact Ionisation
Chemical Ionization
Inductively Coupled Plasma Ionization
Secondary Ion Mass Spectrometry
Fast Atom Bombardment
Plasma Desorption Mass Spectrometry
Laser Desorption Mass Spectrometry
Matrix Assisted Desorption mass Spectrometry
Field Desorption Ionization
Thermospray Ionization
Electrospray Ionization
Atmospheric Pressure Ionization
Particle Beam Interface
Permeable Membrane Interface
Sector Mass Spectrometer
Quadrupole Mass Spectrometer
Ion Trap Mass Spectrometer
Time of Flight Mass Spectrometer
Optical RotationCircular Dichroism
Circularly Polarized Light
Verdet Constant
Faraday Effect
 

Introduction to Spectroscopy

Spectroscopy is the study of the absorption and emission of electromagnetic radiation by matter. The electromagnetic radiation of analytical interest ranges from γ rays that have a frequency of about 3x1018 and wavelength of about 10 pm, to the radio waves used in NMR having a frequency of about of 3x106 and a wavelength of about10 m. This range encompasses UV and visible spectroscopy, Fluorescence spectroscopy, infrared spectroscopy, Raman Spectroscopy, ESR (electron spin resonance spectroscopy) and NMR (nuclear magnetic resonance spectroscopy). There is another very important, so- called analytical spectroscopic technique, called mass spectroscopy (MS), which is somewhat an anomaly, as it does not deal with the adsorption or emission of electromagnetic radiation but the separation of ions of different masses. In its early development, the resolution of different ion masses was included as a spectroscopic technique largely because the curves relating ion intensity to ion mass bore some graphical similarities to true electromagnetic wave absorption spectra.

An electromagnetic wave consists of a sinusoidal electrostatic field acting at right angles to, and in phase with, a sinusoidal magnetic field. A diagram of an electromagnetic wave is shown in figure 1.

Figure 1 An electromagnetic Wave

It is the electric vector that has the major effect on matter; it is the electric vector that activates the cells in the retina of the eye and provides sight; it is the same vector that activates the light sensitive surface of a photoelectric cell, which then responds to the intensity of light falling on it. All electromagnetic radiation travels at the same velocity (c) viz., 2.997925 x 108 ms-1 which can be approximated to 3 x 108 m/s. electromagnetic radiation has two characteristics, its frequency and its wavelength which are related by the following equation,

(1)

where ((λ) is the wavelength of the electromagnetic wave, and ((ν) is the frequency of the electromagnetic wave.

The relationship between wavelength and frequency for the different regions is shown in figure 2.

Figure 2 The Relationship between wavelength and Frequency and the Different Regions of the electromagnetic Spectrum

The regions given in figure 2 does not help the analytical chemist much as it does not indicate how the different frequencies or wavelengths are related to the physical chemical processes with which they are associated. This relationship can be explained as follows.

γ Rays-These rays, that have frequencies lying between ca 3x1018 and 3x1020 Herz (100pm-1pm wavelength), are capable of exciting atomic nuclei. γ Ray spectroscopy is not normally used in general analytical work and the energies involved amount to 109-1011 joules per gram atom.
X-Rays - These rays, having frequencies lying between ca 3x1016 and 3x1018 Herz (10nm-100pm wavelength), can excite inner electronic transitions in an atom and are used extensively in X-ray crystallography. Inner electronic transitions involve energies that may be as great as ten thousand joules per gram atom
Ultra Violet and Visible Radiation - Ultra violet and Visible radiation, having frequencies lying between ca 3x1014 and 3x1016 Herz (1μ-10nm wavelength), can excite outer electronic vibrations (valence electrons) in atoms and absorption or emission of light of this wavelength range is commonly used in analytical techniques to identify aromatic compounds, olefins and substances having one or more double bonds and unshared electrons. The excitation of a valence electron involves the movement of electronic charges in the molecule from one energy level to another. The energies involved in such transitions amount to some hundreds of kilojoules per mole. Absorption of radiation in this frequency range is also used in certain types of sensing devices that are employed in chromatographic detectors.
Infrared and Microwave Radiation - Infrared and part of the microwave band, having frequencies lying between ca 3x1010 and 3x1014 Herz (100μm-1μm wavelength), can excite molecular vibrations and rotations. Absorption of electromagnetic radiation in this wavelength range can be used to confirm the identity of specific compounds and to identify explicit chemical groups in a molecular structure.
Short Wave Radio Radiation -Short wave radio radiation, having frequencies lying between ca 3x108 and 3x1010 Herz is employed in electron spin resonance studies.
Medium Wave Radio Radiation - Medium wave radio radiation, having frequencies lying between ca 3x106 and 3x108 Herz is used in nuclear magnetic resonance studies.


Einstein, Planck and Bohr suggested that electromagnetic radiation could also be considered as a stream of particles in discrete energy packets called quanta and the energy (E) of each particle of frequency (n) was given by,
E = hν (2)
where (h) is Planck’s Constant = 6.62 x 10-34 Js = 6.62 x10-27 ergs/sec

Using equation (2), the energy associated with any transition whether electronic, rotational or vibrational, induced by radiation of a specific frequency can be calculated.

 

About the Author
RAYMOND PETER WILLIAM SCOTT was born on June 20 1924 in Erith, Kent, UK. He studied at the University of London, obtaining his B.Sc. degree in 1946 and his D.Sc. degree in 1960. After spending more than a decade at Benzole Producers, Ltd. Where he became head of the Physical Chemistry Laboratory, he moved to Unilever Research Laboratories as Manager of their Physical Chemistry department. In 1969 he became Director of Physical Chemistry at Hoffmann-La Roche, Nutley, NJ, U.S.A. and subsequently accepted the position of Director of the Applied Research Department at the Perkin-Elmer Corporation, Norwalk, CT, U.S.A.
In 1986 he became an independent consultant and was appointed Visiting Professor at Georgetown
University, Washington, DC, U.S.A. and at Berkbeck College of the University of London; in 1986 he retired but continues to write technical books dealing with various aspects of physical chemistry and physical chemical techniques. Dr. Scott has authored or co-authored over 200 peer reviewed scientific papers and authored, co-authored or edited over thirty books on various aspects of physical and analytical chemistry. Dr. Scott was a founding member of the British chromatography Society and received the American Chemical society Award in chromatography (1977), the M. S. Tswett chromatography Medal (1978), the Tswett chromatography Medal U.S.S.R., (1979), the A. J. P. Martin chromatography Award (1982) and the Royal Society of Chemistry Award in Analysis and Instrumentation (1988).
Dr. Scott’s activities in gas chromatography started at the inception of the technique, inventing the Heat of Combustion Detector (the precursor of the Flame Ionization Detector), pioneered work on high sensitivity detectors, high efficiency columns and presented fundamental treatments of the relationship between the theory and practice of the technique. He established the viability of the moving bed continuous preparative gas chromatography, examined both theoretically and experimentally those factors that controlled dispersion in packed beds and helped establish the gas chromatograph as a process monitoring instrument. Dr. Scott took and active part in the renaissance of liquid chromatography, was involved in the development of high performance liquid chromatography and invented the wire transport detector. He invented the liquid chromatography mass spectrometry transport interface, introduced micro-bore liquid chromatography columns and used them to provide columns of 750,000 theoretical plates and liquid chromatography separations in less than a second. Dr. Scott has always been a “hands-on” scientist with a remarkable record of accomplishments in chromatography ranging from hardware design to the development of fundamental theory. He has never shied away from questioning “conventional wisdom” and his original approach to problems has often produced significant breakthroughs.

gamma rays