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Updated: Jul 12, 2026

High Speed Sub-GHz Spectrometer for Brillouin Scattering Analysis
Published on: December 22, 2015
Cascaded interferometric imaging spectrometer.
1Space Science and Technology Department, Rutherford Appleton Laboratory, Chilton, Didcot, Oxon, UK OX11 0QX. B.M.Swinyard@rl.ac.uk
We developed a new method for order sorting a Fabry-Perot interferometer with a Fourier transform spectrometer (FTS). This novel technique enhances imaging spectroscopy for astronomical mapping, offering significant speed advantages over existing instruments.
Area of Science:
- Optical instrumentation
- Spectroscopy
- Astrophysical observation
Background:
- Fabry-Perot interferometers are crucial for spectral analysis.
- Order sorting is essential for unambiguous spectral data.
- Existing Fourier transform spectrometer (FTS) and grating instruments have limitations in speed and field of view.
Purpose of the Study:
- To introduce a novel method for order sorting a Fabry-Perot interferometer.
- To demonstrate the applicability of this method across various wavelengths, specifically in the 5-25 micrometer band.
- To evaluate the performance and advantages of this new instrument concept for imaging spectroscopy.
Main Methods:
- Utilizing a Fourier transform spectrometer (FTS) in tandem with a Fabry-Perot interferometer for order sorting.
- Developing a model instrument response to demonstrate the order-sorting mechanism.
- Comparing the performance against grating and standard FTS instruments under noise-limited conditions.
Main Results:
- The proposed method achieves effective order sorting for Fabry-Perot interferometers.
- The instrument concept allows for a large bandwidth, wide field of view, and high transmission efficiency.
- The new system demonstrates a speed advantage over standard FTS instruments and grating instruments under specific conditions.
Conclusions:
- The novel tandem FTS-Fabry-Perot interferometer offers a powerful technique for imaging spectroscopy.
- Its attributes are particularly beneficial for mapping large astronomical sources.
- The instrument provides a significant speed improvement, making it valuable for background and detector noise-limited observations.
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