The present invention relates generally to methods and devices for trace gas detection. More specifically, it relates to improvements of the detection of trace gasses such as NO2 using laser induced fluorescence.
Laser induced fluorescence (LIF) is a common spectroscopic technique for trace gas detection in atmospheric monitoring and combustion sciences. One important application of LW is to the detection of nitrogen dioxide (NO2) which is an important chemical species in the atmosphere and in combustion processes. Concerns about the harmful health effects of NO2 and its role in forming deleterious atmospheric species have made it desirable to have sensitive measurements of NO2. Fluorescence assay with gas expansion (FAGE) is one type of LW technique used to measure NO2 in the atmosphere. Although FAGE achieves excellent sensitivities at short averaging times, it has the disadvantage that its sensitivity requires an expensive pumping system to lower the pressure of the air below ambient atmospheric pressure. The low pressure extends the fluorescence lifetime of the excited NO2, and time-gated electronics are then used to discriminate against the scattered laser photons. The low pressure reduces the background “noise” arising from scattered photons resulting from the laser light interacting with air molecules, allowing the system to achieve sensitivities of less than 1 part per billion (ppb). When the main source of background noise is described by a Poisson distribution, the limit of detection (LOD), [NO2]min, is given by the following equation:
where SNR is the signal to noise ratio (typically SNR=2), C is the sensitivity of the LW instrument (counts s−1 ppb−1) Sbg is the background signal (counts s−1), and t is the integration time (s). The LOD improves as the square root of the background noise which goes down linearly with pressure. More importantly, a reduction in pressure decreases the number density of “bath” molecules which act to quench the excited molecule, thereby increasing the fluorescence lifetime, τNO2, which is given by
where kr is the radiative rate constant, kqi, are the species dependent collisional quenching rate constants and Miq are the number density of potential quenching molecules (e.g., O2, N2). The FAGE technique exploits this increase in fluorescence lifetime to avoid detecting scattered laser photons which arrive relatively instantaneously, by waiting sometime after the laser pulse to turn on the detector. Thus, using low pressure and time-gating, the fluorescence photons are measured against a very low background (e.g. 1.5 counts s−1). However, to obtain this low background and high sensitivity, FAGE requires bulky pumping systems which increase instrument energy use, cost, and complexity. Further complexity is added by the time-gated electronics that are needed to discriminate the fluorescence signal from the background. It would be a significant advance in the art of LIF to overcome this and other limitations of known techniques.
In one aspect, the present invention provides a high sensitivity LIF instrument for detecting an amount of a component in a sample gas at atmospheric pressure. Advantageously, the instrument does not need to operate at low pressure to achieve high sensitivity and thus does not require an expensive pump. In addition, the instrument is able to operate in continuous mode and does not require time gating circuitry to discriminate the fluorescence signal from the background.
In one embodiment, the invention provides a method of detecting an amount of a component in a sample gas. An excitation light is passed through the sample gas at atmospheric pressure to produce fluorescence light from the component. The fluorescence light is discriminated using a sequence of multiple long pass interference filters to filter out the excitation light. The discriminated fluorescence light is then detected to produce a signal representative of the amount of the component in the sample gas. The excitation light may be generated using a laser diode or light emitting diode. When applied to the detection of nitrogen dioxide, in some embodiments the excitation light preferably has a wavelength of less than 410 nm, more preferably a wavelength 403 nm to 409 nm, or most preferably a wavelength of 406.3 nm, while in other embodiments the excitation light preferably has a wavelength 398 nm to 450 nm, more preferably a wavelength 410 nm to 440 nm, or most preferably a wavelength of 413 or 435 nm. The fluorescence light from the nitrogen dioxide preferably has a lifetime less than 80 μS. The long pass filters each preferably achieve an optical density of 5 for wavelengths shorter than 440 nm and a transmittance greater than 90% for wavelengths in the range 448 to 900 nm. Preferably, the excitation light is continuously passed through the sample gas. In one embodiment, the gas flows through a cell having a parabolic reflector as an interior surface and a source of the excitation light at a focus of the parabolic reflector. In other embodiments, multiple components are detected in parallel using multiple sample cells and a fiber optic multiplexer to sequentially filter and detect the fluorescence light from each of the multiple sample cells.
Before describing embodiments of the present invention in detail, it is helpful to discuss some of the principles which allow high sensitivity at ambient pressures to be attained. The pressure dependence of a fluorescence signal may be calculated using the governing equations for an LIF signal (SNO2) which is equal to the product of the excitation rate (ENO2), the fluorescence efficiency (φNO2), and the collection efficiency (CNO2) of the detection system:
S
NO2
=C
NO2
*E
NO2*φNO2. (3)
While excited NO2 emits light over a wide spectrum (i.e., greater than 1000 nm), only a fraction of that light falls within the spectral window of a typical detector (200-900 nm). CNO2 represents the efficiency involved with collecting the fluorescence signal,
C
NO2=Ω*F*T, (4)
where Ω(0.038) is the solid angle intercepted by the collection optics for a typical off-axis design, F (0.7) is the fraction of fluorescence occurring within the spectral window of the detector and T (0.8) is the fraction of transmitted fluorescence through the optics (lens and filters). ENO2 is the rate at which NO2 is excited with units of molecules s−1, and can be expressed by:
E
NO2
=c·l·∫φ(v)σ(v,temp,pressure)dv, (5)
where c is the number density of NO2 (molecules cm−3), l (1 cm) is the length through which laser light interacts with the gas which is within the detector's view, φ(3×1015 photons s−1 cm−2) is the laser flux and σ(about 6×10−19 cm2 molecule−1) is the absorption cross section of NO2. φNO2 is a function radiative rate constant for electronically excited NO2 and the quenching rates:
For high pressures (i.e., ΣkqiMi>>kr) equation 6 simplifies to
where KQ is a weighted average of the quenching rates which for dry air is ˜6×10−11 cm3 molecule−1 s−1 and M is the total number density of air molecules (in molecules cm−3). The radiative rate constant for the fluorescence transition at λexcitation=406.3 is kr=2.6×104 s−1 so that approximation in equation 7 can be made for pressures greater than 10 torr (i.e., M>3.26×1017 molecules cm−3). The number density of NO2, c, and the total number density M from equation 7 are combined to yield
This result shows that the fluorescence signal is proportional to the mixing ratio of NO2 and does not depend on the absolute number density of NO2 for high pressures.
Surprisingly, the analysis above indicates that the fluorescence yield is higher at atmospheric pressure, is pressure-independent and the yield is even higher for transitions that have short lifetimes. In contrast, existing techniques of low-pressure LW, such as FAGE, succeed by using temporal gating to discriminate against laser photons and reduce background and desire a longer fluorescence lifetime. Embodiments of the present invention discriminate through the use of optical filters instead of temporal gating and prefer a shorter fluorescence lifetime.
Based on equation 4, the expected fluorescence signal is approximately 40 counts s−1 ppb−1. To achieve a LOD of 1 ppb NO2 for a 60 second averaging time and a SNR of 2, the background is preferably less than 24,000 counts s−1 (equation 1). Background reduction (Sbg≈10 000 counts s−1) may be achieved through the use of high quality long-pass filters (e.g., O.D. >5 for λ=300-431 nm and % T>90 for λ=448-900 nm).
The zero pressure fluorescence lifetime, τ0, and the radiative rate constant are reciprocal so that equation 7 may be rewritten as:
Therefore, a fluorescence transition with a shorter lifetime yields a greater fluorescence signal. NO2 is spectroscopically complex leading to long lifetimes (˜100 μs) for most fluorescence transitions. The fluorescence lifetime is in the range of 28 to 42 μs for the 400-410 nm range as opposed to more than 80 μs for wavelengths used in other LIF instrumentation. Consequently, a factor of 2 increase in radiative rate constant may be obtained by exciting in the blue. Therefore, embodiments of the present invention use an excitation wavelength further into the blue, which also allows more of the red-shifted fluorescence to be within a detector spectral window of 200-900 nm.
An apparatus according to one embodiment of the invention is shown in
Laser 10 may be, for example, a temperature and current controlled 35 mW continuous-wave GaN semiconductor laser diode (Sanyo, DL 5146-152). This compact and relatively inexpensive laser diode is capable of being tuned over the range of 395-415 nm. In some embodiments of the invention designed for the detection of NO2, the excitation light preferably has a wavelength less than 410 nm, more preferably between 403 nm and 409 nm, and most preferably tuned to 406.3 nm. In other embodiments of the invention designed for the detection of NO2, the excitation light preferably has a wavelength 398 nm to 450 nm, more preferably a wavelength 410 nm to 440 nm, or most preferably a wavelength of 413 or 435 nm. Light 32 from laser 10 is directed by steering mirrors 14, 16 into sample cell 22 where it excites sample gas present in the cell. The beam exits cell 22 and is directed by mirror 18 into beam dump 20. Sample gas enters cell 22 after passing through polytetrafluoroethylene (PTFE) filter 42 and is drawn out of cell 22 by diaphram pump 40.
Fluorescence cell 200 is not required to be vacuum tight in order to make measurements. However, the cell is preferably air tight to facilitate gas sampling and constructed to shield extraneous environmental light. The fluorescence cell is preferably a cubic (4×4×4 cm) cell with two side arms 210, 212 for shielding extraneous light from entering the cell. Side arms 210, 212 preferably end with windows held at Brewster's angle where the excitation light enters and exits. The fluorescence signal 216 exits the cell 200 orthogonal to the excitation beam 214. Cell 200 also has two 0.635 cm diameter stainless steel gas ports (not shown) to which 0.635 cm PTFE tubing is connected for sample gas delivery and removal. Preferably these two ports are positioned on two opposite faces aligned on an axis orthogonal to the plane of the figure.
Excitation light 214 interacts with the sample gas in cell 200 to produce fluorescence light 216. The wavelength of the excitation light preferably is selected so that the fluorescence lifetime of the species being detected in the sample gas is less than 80 μs, thereby producing a stronger fluorescence signal than with longer lifetimes. The fluorescence signal 216 exits the cell 200 and is directed by lens 204 through long pass filter 206 and then focused upon photomultiplier 208 by lens 202. The two lenses 202, 204 are preferably 25 mm achromatic lenses with anti-reflection coatings and 30 mm focal lengths (Edmunds Optics, ACH 25×30 VIS-NIR). Positioned between the two lenses is long pass filter 206 preferably composed of four long-pass interference filters with cut-on wavelengths at 440 nm (Chroma tech., HQ440LP). These filters reject scattered photons from the excitation light and transmit photons from the fluorescence light. These filters each achieve an optical density of 5 for wavelengths shorter than 431 nm and a transmittance greater than 90% for wavelengths in the range 448 to 900 nm The focal point of the first lens 204 intersects the excitation beam 214 so that the rays of the fluorescence light 216 propagate along parallel paths through the long-pass filters and are focused by the second lens 202 onto the active surface of the photodetector 208.
Returning to
A small inexpensive diaphragm pump (Rietschel Thomas, Model 2107 capable of 46 lpm at 760 torr) 40 may be used to produce flow of ambient pressure sample gas through the tubing from an ambient rooftop intake manifold and through the sample cell 22. Prior to entering the chamber 22 the sample gas may be passed through a polytetrafluoroethylene filter (SKC, 47 mm) 42 with a 2 μm pore size to remove light-scattering particles. For background measurements, nitrogen dioxide can be removed from the gas flow by passing the sample gas through ferrous sulfate or by reducing nitrogen dioxide photolytically. Calibration of the LW instrument may be performed using standard gas calibration techniques using National Institute of Standards and Technology (NIST) gas standards or permeation tubes and dilution systems.
By operating the excitation light in continuous wave mode this system has the advantage of very low photon density, thereby significantly reducing the likelihood of two photon inferences. Other species which can photodissociate to NO2 include HNO3, N2O5, HNO4, PAN and ClNOX. However, because they have absorption cross sections 10 to 100,000 times smaller than that of NO2, they will not interfere significantly at concentrations typically found in the atmosphere.
This embodiment provides a continuous-wave laser-diode LW-based approach for NO2 detection that can be operated at atmospheric pressure. The use of high quality optical filters provides substantial discrimination against scattered laser photons without the use of time-gated electronics or expensive pumps to produce low pressure, thereby avoiding complexity and cost to conventional LIF instrumentation. This improvement allows operation at atmospheric pressure with a low-cost diaphragm sampling pump. The LIF instrument for NO2 detection operates at atmospheric pressure and has a sensitivity of 2 ppb (SNR=2) with an averaging interval of 60 s. Those skilled in the art can appreciate that many variations may be made to the specific embodiment described. For example, the optical train may be optimized to potentially achieve sub-ppb sensitivities. Fiber optics can be used for the delivery of excitation light to the cell, and for the delivery of fluorescence light from the cell to the filters and photomultiplier. Tuning of the laser to move the wavelength of the excitation light in and out of the NO2 absorption feature can be used to eliminate the need for FeSO4 for background measurements. In addition to environmental applications, this system also has potential application for other fields where direct and non-intrusive measurements of NO2 are needed, such as flame, combustion and surface chemistry.
Embodiments of the invention can be utilized as a “backend” detector of an NOy ambient monitor. Since this NO2 detection technique does not require an expensive high-capacity pump, separate cells for each constituent of NOy can be employed, thereby eliminating the complexity and potential chemical artifacts associated with switching between NOy modes. For example,
Multiplexer 434 will now be described in detail in relation to
fluorescence signal
NO2
NO2
NO2
NO2
fluorescence signal
fluorescence signal
fluorescence signal
fluorescence signal
Although the above embodiments have been described with reference to the measurement of NO2 in the atmosphere, those skilled in the art will appreciate from the above description that the principles of the invention are not limited to NO2 measurements. Any atmospheric gas species which is excited in the visible and fluoresces in the visible is a candidate for the ambient pressure fluorimeter designs in accordance with the teachings of the present invention. It is only a matter of selecting the appropriate excitation source wavelength and interference filters.
This application claims priority from U.S. Provisional Patent Application 61/216,897 filed May 22, 2009, which is incorporated herein by reference.
Number | Date | Country | |
---|---|---|---|
61216897 | May 2009 | US |