A photo-acoustic spectrometer (PAS) is an instrument to measure trace gases, which operates by illuminating the gas with modulated light resonant with the species of interest in a small chamber. The light energy is absorbed, usually exciting molecular vibrational modes. Via collisional exchange, the vibrational energy is transferred to increased molecular kinetic energy, equivalent to a local rise in macroscopic temperature. The local temperature increase induces a pressure wave, which propagates throughout the small chamber and is measured by a microphone.
In a non-resonant chamber the acoustic pressure is P=K(Cp/Cv−1)I/f; where K is a constant depending on the cell geometry and gas; Cp and Cv are the gas specific heats at constant pressure and volume, respectively; I is the light intensity; and f is the light modulation frequency. That the acoustic pressure depends on the period of the light modulation implies there is no well definable acoustic wave front, but rather the entire volume of gas is being heated over a time T/2 where T is f1. Typically f ˜25 Hz. Physically, the pressure inside the chamber is increasing and decreasing at that frequency. At atmospheric pressure and typical chamber length scales of 1 cm the corresponding acoustic frequency would be 33 kHz.
In a resonant photo-acoustic spectrometer, the light is modulated at a frequency equal to a natural resonant frequency of the chamber. For a cube chamber geometry this would be a standing wave mode, with the lowest frequency mode having a wavelength twice the cube's linear dimension. Typical modulation frequencies for resonant chambers are in the kilohertz range. Resonant chambers pump up the standing wave in a coherent fashion, resulting in higher pressure levels and larger microphone signals. Resonant chamber spectrometers can have signal-to-noise ratios orders of magnitude higher than their non-resonant counterparts.
A problem is that for a non-resonant case the modulation frequencies must be low to provide a chamber pressure level detectable by the microphone. At low frequencies, external vibrational noise amplitudes are higher. Secondly, the wave nature of pressure propagation is not capitalized on. For a traveling sine wave, instantaneous nodes of zero pressure amplitude must be balanced by antinodes with a much higher pressure amplitude to maintain average energy density. The resulting larger amplitude provides a larger microphone signal, which is absent in the non-resonant case.
The details of one or more embodiments of the invention are set forth in the accompanying drawings and the description below. Other features, objects, and advantages of the invention will be apparent from the description and drawings, and from the claims.
Like reference symbols in the various drawings indicate like elements.
With respect to the resonant case, resonant chamber geometries have been simple in design; cylindrical is a common choice. That makes exciting a single mode optimized for detector placement difficult if not impossible. Current designs typically place the pick-up microphone at the halfway point along the cylinder z-axis and are sensitive to whatever amount of amplitude is present in the fundamental longitudinal mode and possibly its odd harmonics.
The Photo-Acoustic chamber is a gas volume enclosed by a high rigidity material to have minimal deformation by surface pressure. This results in maximal reflection of an acoustic pressure wave from each surface, giving the chamber a high Q factor. Any cell geometry will have an infinite series of resonant modes and a corresponding resonant frequency. Optimal cell design insures that the resonant mode of intended operation will be well separated in frequency from any neighboring modes to avoid energy loss to modes with frequencies outside the phase detection bandwidth. The chamber windows may have 100% transmission at the excitation light wavelength to prevent absorptive heating and subsequent acoustic excitation at the chamber resonant frequency. Acoustic excitation from absorptive window loss would mimic a desired gas detection signal and reduce the real signal-to-noise ratio.
The Light Source provides excitation light at a resonant optical absorption frequency of the trace gas species of interest. It is narrow band to minimize excitation of interfering gas species with overlapping absorption spectral lines. Multi-frequency light may be provided by using broadband light sources and appropriate filters or narrow band tunable light sources. The excitation light is modulated by the Light Modulator, typically in an on-off fashion using a chopper wheel or an electro-optic modulator deriving its signal from the Modulator Reference. The frequency of the on-off light modulation is chosen to match the acoustic resonance mode that the Photo-Acoustic Chamber is designed for. When the light modulation frequency is matched with the chamber acoustic resonant frequency, the acoustic resonant mode is pumped up in amplitude until the input absorptive light energy equals the dissipative energy losses of the Photo-Acoustic Chamber. A high Q (low energy loss per acoustic cycle) chamber is thus desired to maximize the pressure amplitude of the acoustic resonant mode. The pressure amplitude of the acoustic resonant mode is then sensed by the Microphone coupled to the acoustic chamber. The Microphone signal and the Modulator Reference signal are processed together using a Phase Sensitive Detector to extract the acoustic resonant amplitude resulting from the optical absorption resonance of the trace gas species of interest. The Phase Sensitive Detector Output Signal is then proportional to the trace gas species concentration.
Part of a solution is to excite a single resonant mode with a correspondingly optimized detector placement. The result of doing that, in conjunction with a small chamber, will impose a second part of the solution: higher frequency operation. These goals may be accomplished via the following embodiments.
Elliptical Chamber Design
In one embodiment, the path lengths are arranged from the excitation region to the pick-up microphone to be the same. This is accomplished by using an elliptical chamber with the light excitation path oriented along one focus and the pick-up microphone oriented along the other focus. Such an elliptical chamber will replace the cylindrical one in
A single constant, the eccentricity e, defines the shape of the ellipse and is the ratio of the semi-major axis a to the ellipse-center-to-focus length. The path length F1-ellipse-F2 is 2a, so if the speed of sound in the chamber gas is c, after a time 2a/c a delta function excitation at F1 will converge at F2, and after 4a/c will reconverge on F1 again. The delta function excitation and reconvergence of the line pressure pulse is actually a superposition of all transverse modes for the elliptical cavity. For a small resonator chamber with semi-major axis a=1 cm, and atmospheric sound velocity of 330 m/s, the round trip time for a signal generated at F1 to reconverge on F1 is 60.6 μs, or a rate of 16.5 kHz. That leads to the following embodiment.
Fast Resonant Light Pulsing
If a short light pulse is repeated at the above resonant rate along focus F1, the approximately delta function pulse will gain in amplitude until the cavity energy loss per cycle equals the light energy absorbed by the gas. That is the rise time to reach maximal amplitude of the 16.5 kHz traveling wave pulse, and will produce maximal pressure levels alternatingly at foci F1 and F2. Now the pressure level at F2 needs to be sensed, which may be performed in accordance with any of the following embodiments.
Sensing a Line-Like Pressure
A number of embodiments of the invention have been described. Nevertheless, it will be understood that various modifications may be made without departing from the spirit and scope of the invention. Accordingly, other embodiments are within the scope of the following claims.
This application claims priority to U.S. Application Ser. No. 60/867,361, filed on Nov. 27, 2006.
Number | Name | Date | Kind |
---|---|---|---|
3179898 | Meltzer | Apr 1965 | A |
3266313 | Litterst | Aug 1966 | A |
3588739 | Yoshikawa et al. | Jun 1971 | A |
3745325 | Harvey | Jul 1973 | A |
3946239 | Salzman et al. | Mar 1976 | A |
4188543 | Brunsting et al. | Feb 1980 | A |
4457162 | Rush et al. | Jul 1984 | A |
4557603 | Oehler et al. | Dec 1985 | A |
4657397 | Oehler et al. | Apr 1987 | A |
4740086 | Oehler et al. | Apr 1988 | A |
4771629 | Carlson et al. | Sep 1988 | A |
4818882 | Nexo et al. | Apr 1989 | A |
5170064 | Howe | Dec 1992 | A |
5753797 | Forster et al. | May 1998 | A |
5973326 | Parry et al. | Oct 1999 | A |
6006585 | Forster | Dec 1999 | A |
6694799 | Small | Feb 2004 | B2 |
6843102 | Shulga et al. | Jan 2005 | B1 |
6897960 | DiMeo et al. | May 2005 | B2 |
7069769 | Kung | Jul 2006 | B2 |
7213444 | Baraket et al. | May 2007 | B2 |
7263871 | Selker et al. | Sep 2007 | B2 |
7488942 | Hopkins et al. | Feb 2009 | B2 |
Number | Date | Country | |
---|---|---|---|
20080121018 A1 | May 2008 | US |
Number | Date | Country | |
---|---|---|---|
60867361 | Nov 2006 | US |