When electromagnetic radiation is emitted, scattered,
or reflected from an object moving toward or away from an observer, the
observed wavelength is shifted (the Doppler effect). The molecules of a
gas will scatter electromagnetic radiation (Rayleigh scattering). Thus,
radiation that is Rayleigh-scattered from a gas may be shifted in wavelength
because of the velocity of the scattering molecules.
The distribution of velocities will vary with the composition of
the gas, so when light of a single frequency is scattered from
a gas, the frequency
spectrum of the scattered light is broadened (Doppler broadening).
The degree of broadening will depend upon the velocities of the
molecules,
which in turn depend upon the composition of the gas. Therefore, it
is possible to determine the composition of a gas by measuring
the Doppler
broadening of Rayleigh-scattered light.
A theoretical model was developed that predicts the spectrum of the
Doppler-broadened light and the signal-to-noise ratio for this
technique as a function of
the key design parameters. This model includes both direct detection
and heterodyne detection approaches. An example of predicted
spectrum is shown
in figure 1.
Five approaches to implementation of this technique were considered
singly and in combination as candidates for a proof-of-principle
experiment:
- Homodyne detection.
- Offset homodyne
detection.
- Heterodyne detection.
- Vapor absorption
filter.
- Fabry Perot interferometer.
A survey of the key technologies for the laser, detector, modulator,
filter, and frequency discriminator indicated that two approaches
may be currently
feasible for a proof-of-principle experiment: homodyne and a combination
of vapor absorption filter and Fabry Perot. Analyses using the model
developed in this phase indicate that both of these techniques
are expected to provide
signal-to-noise ratios suitable for proof-of-principle experiments.
Designs for these two experiments are outlined in figures 2 and
3. The next step
in development after proof of principle will be to add a scanning system
to enable acquisition of a two-dimensional image of the distribution
of the leaking gas.
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Figure 1. Predicted Doppler Spectrum Scattered From a Mixture of Oxygen,
Nitrogen, and Helium With Flux in Watts and Angular
Frequency in Radians/Second
Contacts:
C.K. Davis (Christopher.Davis-1@ksc.nasa.gov),
YA-E2, (321) 867-8801; R.E. Rhodes, YA-C, (321) 867-6298; and Dr.
R.C. Youngquist, YA-C3-E, (321) 867-1829
Participating Organization: Florida Space Institute (G. Sellar)
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