Title: Advantages of Fourier Transform Spectroscopy
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25Advantages of Fourier Transform Spectroscopy
26Advantages of Fourier Transform Spectroscopy
- Fig. 7-40, pg. 185 "Illustrations of time doamin
plots (a) and (b) frequency domain plots (c),
(d), and (e)."
27Advantages of Fourier Transform Spectroscopy
- Fig. 7-41, pg. 186 "Time domain spectrum of a
source made up of several wavelengths."
28Advantages of Fourier Transform Spectroscopy
- Michelson Interferometer
- Fig. 7-42, pg. 186 "Schematic of a Michelson
interferometer illuminated by a monochromatic
source."
29Advantages of Fourier Transform Spectroscopy
- Fig. 7-43, pg. 188 Comparison of interferograms
and optical spectra.
30FT-IR
31Advantages of Fourier Transform Spectroscopy
- Throughput no slits or gratings. Full power of
source reaches detector - Resolution depends on length of mirror scan,
can be very high - Rapid data collection
32Scan Times, Frequency Domain
- Resolution elements spectral width/resolution
- IR spectrum, 500 cm-1 to 4500 cm-1
- For 3 cm-1 resolution, 4500/3 1500 elements
- For 1 cm-1 resolution, 4500/1 4500 elements
- Scan at 0.5 sec/element,1500 elements,12.5min
- Scan at 0.5 sec/element,4500 elements,37.5min
- Signal/Noise S/N
- S/N improvement n1/2 where n time per element
- To improve S/N by 3, n 9. 9 X 0.5 s 4.5 sec
- Scan time goes to 9 x 37.5 min 5.6 hrs for high
resolution scan.
33Scan Times, Time Domain
- About 0.5 sec per scan required
- Entire spectrum collected with each scan
- Assume short data collection, 12.5 min
- 750 sec/0.5 sec per scan 1500 spectra
- S/N improvement is 15001/2 39
- Multiplex advantage due to short scan time in
time domain spectroscopy
34Measurements in the time domain
- Light moves fast, c 3 x 108 m/s
- Consider infrared, ? 3 x 10-6 m
- 3 x 10-6 m/3 x 108 m/s 10-14 s for one
wavelength of light to pass by a detector - To resolve 3 x 10-6 m from 4 x 10-6 m in
frequency domain requires time resolution of less
than 10-14 s - too fast for any known photo
detector!
35Measuring time versus intensity
- P(t) kcos(2p?1t) kcos(2 p?2t)
- After this is measured, P(?) is given by a
Fourier transform of P(t). - How do you measure P(t) when c3 x 108m/s?
- Answer Interferometry
- P(t) P(t)/k, k is called modulation factor
- f frequency at detector 2 vm/?
- vm mirror velocity, ? wavelength of light
36Retardation
Retardation d 2(M-F) dmax 0 dmin ½ ? dmin
dmax ½ ? ? 2(dmin dmax) At M F, d
0 At M F ½ ?, d - ?
37Optical frequency and detector frequency
- Detector frequency f 2vm/?
- c ??photon
- f 2vm/? (2vm/c)?photon k?photon
- Since c is large, k is small and f is an easily
measured frequency for a simple detector
38Optical frequency and detector frequency
- detector frequency (observed) is given by f
2vm/?. This is the frequency for observing
fringes in the interference pattern. - Example vm 3 cm/s, ? 3 x 10-4 cm
- f104 s-1 and 1/f 10-4 s
- For ? 3 x 10-4 cm, ?photon c/?
- ?photon (3 x 1010 cm/s)/(3 x 10-4 cm) 1014
s-1 and 1/? 10-14 s - Conclusion Detector needs to detect signals
with a time resolution of about 10-4 s to
reproduce the optical signal that would require
time resolution of about 10-14 s
39Resolution with interferometry
- Principle one complete beat pattern must be
scanned to fully resolve all components - Closely spaced features have smaller differences
in frequencies, so a long cycle is needed to see
a full beat - To resolve 2 features separated by ??, the length
of the scan distance is given by
L 1/2?? - Example For resolution of 0.1 cm-1,
L 1/(2)(0.1 cm) 5 cm