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Heterodyne Instrument for the Far Infrared (HIFI)

HIFI will advance our understanding of interstellar chemistry. With its high spectroscopic resolution and sensitivity, the instrument can detect and analyze emissions from a variety of molecules. It uses far-infrared and submillimetre wavebands to observe molecules in various chemical processes and astrophysical environments.

How it works

The instrument uses a local oscillator to produce its reference signal. This is mixed with the signal from the source object, and the result is a signal frequency much lower than the original and much easier to process with electronic circuits.

Musicians will recognize the heterodyne principle, since it's what they use when they tune their instruments, as they listen for the beat frequency. For HIFI, the reference signal must be extremely stable and pure. The advanced local oscillator source unit being contributed by Canada has unprecedented precision and stability.


Canadian scientists developed the “tuner” (above) for Herschel’s HIFI instrument, which will explore the chemistry of our galaxy.
(Source: Michel Fich)

The Principal Investigator for HIFI in Canada is Professor Michel Fich of the University of Waterloo. For technical information on HIFI, please visit the Herschel-HIFI website of the University of Waterloo.

 

 

 

 

 

 

Updated: 2007/03/19 Important Notices