= m
= eV
= Hz


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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
Fluorescence Reagents
Diffraction Grating
Fourier Transform IR Spectrometer
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
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

The Basic UV and Visible Spectrometer

Electromagnetic radiation can be dispersed into a band of radiation composed of progressively increasing (or decreasing) wavelength in two ways, either by means of a suitable prism or by a Diffraction Grating. A prism consists of a triangular section of material that is transparent to the light being examined (e.g. glass for the Visible range of radiation). An example of the dispersion of white light by a prism is shown in figure 3. A narrow beam of white light (containing all Visible wavelengths) is made to strike one surface of the prism at an angle and, on entering the medium is refracted away from the normal. The refractive index of the medium differs for light of different wavelength and, thus, the extent of the light beam bending (the refraction) increases as the wavelength of the light decreases. Thus, the violet light will be deflected most and the red light least. As a result the emerging light will be dispersed into a broad band of colours. Prism have a larger bandwidth than gratings but gratings are the more popular as it is easier to obtain high resolution from a grating.
A diagram of the optical system of a UV/Visible Dispersive Spectrometer (spectrophotometer). is shown in Figure 8. The components of the light system through which the light will pass must be made from quartz or pure silica . In addition, surfaces from which the light is to be reflected must also have special surface treatment. If very short wavelengths are to be used then extremely pure silica must be used for any lens, windows or dispersive units. The deuterium lamp is used to provide UV Light between 180 and 350 nm and a tungsten-halogen lamp to provide Visible light between 350 and 800nm. Light from the source lamp is collimated by two curved mirrors and focused onto the dispersion unit Diffraction Grating. Originally the light was dispersed using a quartz prism but all modern instruments employ a holographic Diffraction Grating. Light of the required wavelength is selected by adjusting the angle of the grating. The dispersed light is then focused, by means of a curved mirror, onto a plane mirror and then focused by means of a lens through the sample cell. The sample cell must be sufficiently long to provide adequate light absorption and wide enough to provide enough light to activate the photocell of the sensor. A micro-cell 1 cm long and 1 mm in diameter will have a volume of about 8 μl and a sensitivity of about 1 x 10-8 g/ml (cf toluene at 254 nm). The exit beam from the sample cell is focused onto a photo-cell which gives a response that is some function of the intensity of the light falling on it. The original sensors that were used took the form of a photo-cell consisting of a electron emissive surface on which the light was focused situated in a evacuated bulb fitted with a second electrode, the anode.

Figure 8. The Multi-wavelength Dispersive Spectrometer

A voltage was applied cross the electrode system and the electrons emitted by the light collected and amplified. These devices had limited sensitivity and were replaced by photo-multipliers, which were similar in form but contained a staircase of electrodes, the emitted electrons being amplified at each stage. Modern photocells are usually semiconductor devices (photodiodes or phototransistors) fitted with pure fused silica windows. The output from the photocells is not linearly related to the intensity of the light falling on it and, thus, either an analogue-modifying amplifier must be used or the response corrected digitally by a computer.
The wavelength of the light passing through the sample is selected or scanned by rotating the grating. The output from the sensor amplifier is presented on a chart recorder or computer printer as an adsorption curve relating adsorption to wavelength (or frequency or wave numbers). The adsorption curve is known as the adsorption Spectrum and its shape will be characteristic for the substance being examined.
The Diode Array UV/Visible Spectrometer
The Diode Array spectrometer functions in an entirely different way to that of the dispersive instrument. A diagram of a Diode Array detector is shown in Figure 7. In the diode array spectrometer the sample is subjected to light of all wavelengths generated by the lamp. Light from a deuterium lamp is collimated by an achromatic lens system so that the total light of all wavelengths passes through the sample cell onto a holographic grating. The dispersed light from the grating is then focused onto a Diode Array. The array may contain many hundreds of diodes and the output from each diode is regularly sampled by a computer and stored on disk. The Spectrum of the sample can be obtained by recalling from memory the output of each of the diodes, i.e. a curve relating adsorption to wavelength. The only disadvantage of this type of spectrometer is that the number of diodes in the array limits its resolution.

Figure 7. The Diode Array Detector

If the resolution of the detector is (Δλ) will the number of diodes in the array (n), and the range of wavelengths covered by the array is (λ2 - λ1),


It is seen that the ultimate resolving power of the Diode Array detector will depend on the semi-conductor manufacturer and on how narrow the individual photo cells can be commercially fabricated. As a result of considerable research in diode sensors, the size of the diodes are continually being reduced and consequently the resolution is now very high and still improving.
Although, the two spectroscopic systems described appear to be satisfactory, both suffer from certain disadvantages due to second-order effects. When light having a narrow band wavelengths is passed through the cell (as in the dispersive spectrometer) and the whole of the transmitted light allowed to fall on the sensor, then the light received will not only be that light of the same wavelength that was transmitted through the cell, but also any fluorescent light that the incident light may have excited. Thus, the light measured may not be solely transmitted light of the selected wavelength but will also contain any fluorescent light that was generated by the incident light passing through the sample.
In a similar way, when light containing the whole range of wavelengths is passed through the cell (as in the Diode Array spectrometer), then the light sensed at a selected wavelength will not only contain the transmitted light of that wavelength but also any fluorescent light of the same wavelength that may have been excited by incident light of other wavelengths.
It is seen that neither spectrometer system can be certain of measuring true light absorption at a specific wavelength. In fact, true light absorption can only be measured by first selecting the incident wavelength and then allowing the transmitted light to be resolved on another monochromator. The second monochromator selects the same wavelength as the incident light and in this way any fluorescent light is eliminated and only the transmitted light measured.


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.

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