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Choosing A Light Source For Your Spectrometer

Choosing A Light Source For Your Spectrometer

Depending on your spectrometer application, you will probably need at least one illumination or excitation source. For electroluminescence measurements will require of some sort of testing board connected to an external voltage source. However, most characterisation of optical materials require some sort of incident light.

The light source you will need depends on the measurements you are doing. For photoluminescence measurements, you will need a monochromatic light source with a higher energy than the transition you wish to measure. Often a UV light source is chosen due to its high energy. Additionally, you may also need a monochromatic light source if you are using absorbance spectroscopy to measure optical density. However, to find an absorbance spectrum for your material over a significant wavelength range, you will need a broadband illumination source.

There are many things to consider when you are choosing light sources for your optical spectroscopy lab. The best light source for you will depend on:

  • The type of measurements you are doing
  • The specifications of your USB spectrometer
  • Your budget
  • The safety restrictions of your lab.
  • The time needed to set-up and maintain your light source

One important thing to note is that you will need different light sources for different optical measurements. Therefore, it is quite likely that you will need more than one light source in order to fully characterise your organic electronic materials.

Comparing Different Spectroscopy Light Sources


In the table below, we have done a brief comparison of different light sources. Here, we have outlined their ideal applications, costs and other important information.

 

White Light LED Tungsten Halogen + Deuterium Light Sources Monochromatic LED Light Source Lasers
Type Broadband Monochromatic
What measurement is this for?
  • Absorbance measurements
  • Transmission measurements
  • Reflectivity measurements
  • Photoluminescence
  • Optical Density
  • Measuring concentration of certain molecule
    • Photoluminescence
    • ASE
    • Time-resolved spectroscopy (for pulsed laser systems)
    Advantages Long bulb lifetimes Wide spectral range Long bulb lifetimes
    • High power (for weak fluorescence)
    • Can emit short pulses for TRPL
    Cost Low price and low running costs High ($4000-$5000) Low High ($1000 – $6500)
    Emission Spectra Broad spectrum (360 nm – 900 nm for Ossila Broadband White Light) Very broad spectrum (190 nm – 2200 nm) Well-defined narrowband emission (e.g. 370 nm for Ossila UV light source- 700 nm for the Ossila Infrared Light Source) Well-defined emissions (can be tunable depending on the laser)
    Warm-Up Time Minimal 30 minutes – 1 hour Minimal 5–60 minutes (will vary depending on laser material and mode)
    Temperature Control Needed? No Yes – to stop overheating No Most likely – but depends on the laser
    Set Up and Calibration Time Low Low Low High
    Safety Considerations Low Low Low–Medium High

    In order to take the broadest range of general spectroscopy measurements, you will need multiple light sources, such as can be found in our LED Light Source Set.

    Ossila Light Sources


    Ossila sell many low-cost light sources which are compatible with the Ossila USB Spectrometer, but also with other spectroscopy equipment via the use of standard optical fibers. This will enable you to take a range of spectroscopy measurements quickly and easily.

    UV Light Source

    UV Light Source

    Our USB-C powered UV Light Source emits light at 370 nm. It will not be as powerful as laser excitation but is considerably safer.

    Suitable for:

    • Optical excitation in visible fluorescence spectroscopy measurements.
    Infrared Light Source

    Infrared Light Source

    This USB-C powered Infrared Light Source emits light at specific infrared wanvelengths. Infrared radiation is lower intensity than other excitation sources so will minimize damage to more senstive samples. You can choose from range of wavelengths betwee 700 - 980 nm. It will not be as powerful as laser excitation but is considerably safer and less expensive.

    Suitable for:

  • Studying biological samples
  • Molecular Identification
    • Studying functional groups and chemical bonds
    Broadband White Light Source

    Broadband White Light Source

    Our LED Broadband White Light Source outputs light over the entire visible spectrum (360 nm - 900 nm). This white light source is considerably smaller than tungsten/deuterium sources.

    Suitable for:

  • Absorbance measurements
  • Transmission measurements
  • Reflectivity measurements
  • UV Light Source

    LED Light Source

    Our range of USB-C powered LED Light Sources emit light centred around a single wavelength for specific excitation. You can choose from a range of specific wavelengths between 375-980 nm. This can be useful for

    Suitable for:

    • Fluorescence excitation sources
    • Measuring specific moleculular concentrations
    Represented output of Ossila LED Light Sources
    Normalized spectra of our various LED light sources

    In combination, these two light sources will provide you with everything you need to take basic spectroscopy measurements. These are compatible with standard spectroscopy fittings (SMA 905 fiber connections, M6 optical breadboard holes) so that they can be easily integrated with any spectroscopy system.

    LED Light Sources Set

    LED Light Sources Set
    Sample Preparation for UV-Vis Spectroscopy Sample Preparation for UV-Vis Spectroscopy

    When done correctly, UV-Vis (or optical) spectroscopy can be a powerful technique which can reveal intricate details about the molecular structure and optical properties of a sample. However, without well prepared samples, the results can be not only challenging to interpret but also potentially deceptive.

    Read more...
    Spectrometer Optics Spectrometer Optics

    A spectrometer can be designed and built with a variety of optical configurations. These include the Littrow configuration, the Ebert-Fastie configuration, the Czerny-Turner configuration, and the concave aberration-corrected holographic grating configuration. Careful choice of components and configuration can avoid aberrations, which result in distorted or blurred spectra.

    Read more...

    Contributing Authors


    Written by

    Dr. Mary O'Kane

    Application Scientist

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