Ultra-high sensitivity NDIR gas sensors

Abstract
A compact and long path-length sample cell that is a hollow waveguide with a plurality of bends that are collectively greater than 180 degrees in three dimensions, a focusing device for quasi-focusing radiation into a beam with an angle of incidence between greater than approximately 0° and approximately 10° relative to a longitudinal axis of a first linear segment of the waveguide proximate a source of infrared radiation and a second focusing device for focusing infrared radiation after it has traveled through substantially all of the waveguide as it approaches a detector chamber. The sample cell can be used with two or more detectors to detect the concentrations of one or more gasses, to levels less than 100 ppm, after correction for water vapor.
Description

BRIEF DESCRIPTION OF THE DRAWINGS


FIG. 1 is a schematic layout drawing for the present Super Tube invention showing a bending angle of 540° from the original orientation with three U (180°) turns.



FIG. 2 is a schematic layout drawing for the present Super Tube invention showing a bending angle of 900° from the original orientation with five U (180°) turns.



FIG. 3 shows the use of a conical mirror installed in front of the infrared source in order to limit the launching angle of the radiation emanating from it to <20° with respect to the longitudinal axis of the Super Tube.



FIG. 4 shows the use of a parabolic mirror in front of the infrared source in order to limit the launching angle of the radiation emanating from it to <20° with respect to the longitudinal axis of the Super Tube.



FIG. 5 shows the use of a conical mirror installed just in front of the infrared detector serving as a radiation concentrator in order to condense the radiation from the source onto the detector.



FIG. 6 shows the optical arrangement installed within the Super Tube near the detector end for creating two in-line detectors one of which is used to measure water vapor in order to provide real time in-situ correction for water vapor interference.



FIG. 7 shows an optical arrangement installed within the Super Tube near the detector end for creating two or more in-line detectors that will provide the sensor with a multi-gas detection capability.



FIG. 8 shows a packaging scheme for mounting four standard infrared sources onto a special TO8 header.





DETAILED DESCRIPTION OF THE PREFERRED EMBODIMENT

For over two decades, the present inventor diligently worked on simple, rugged and low-cost NDIR gas sample chambers culminating in the so-called “wave-guide” sample chamber invention disclosed in U.S. Pat. No. 5,163,332 (1992). Indeed, for gases with moderate to strong absorption bands in the mid-infrared spectral region like CO2 (4.26 μm), H2O (2.7 μm), CH4 (3.4 μm) etc., the optimum and simplest gas sample chamber is a hollow straight metallic tube with arbitrary cross-section but speculatively reflective inner walls very much likened to a standard microwave wave-guide. Today after over a decade has gone by since the advent of the “wave-guide” gas sample chamber (a.k.a., “The Tube”), most of the reliable, rugged, sensitive and low-cost CO2 sensors use this design, rendering a host of new applications, including faster and false-alarm resistant fire detectors and Demand Control Ventilation (DCV) strategies for saving energy in high-rise office and commercial buildings, many of which were not practical earlier because of high CO2 sensor costs.


The present invention discloses a new sample chamber that, like the prior “wave-guide” or The Tube, will create a host of new applications because it overcomes a number of technical impediments that have prevented the extension of such an approach into the arena of achieving compact, low-cost and long path-length NDIR and TDLAS gas sample chambers.


In U.S. Pat. No. 5,696,379 issued to Burkhard Stock in 1997, a two-dimensional configuration for a waveguide type NDIR gas sample chamber aimed at reducing the size of the subsequent gas sensor was disclosed. In this disclosure, a configuration utilizing two 90° bends and one with one 90° bend followed by a U-shape in one plane were described for achieving the overall size reduction for the designed NDIR gas sensors. Without an explicit description or reasoning, the author of this patent also claimed that his 2-dimensional configuration can also be extended to the third dimension with equal benefits. However, he emphasized with a detailed explanation that his teaching only worked for guiding the radiation through a maximum of a 180° bend such as two right angle (90°) bends or a U (180°) bend. Also, standard radiation sources (quasi blackbody) were used but no method teaching how to guide the emitted radiation down the two-dimensional hollow waveguide was advanced. There is no doubt that the use of curved hollow waveguides with speculatively reflective inner walls will render the design of an NDIR gas sensor more compact than the use of a straight hollow waveguide having the same path length. However, the gain in compactness for the designed gas sensor using either a 2- or 3-dimensionnal hollow waveguide configuration is severely limited by not being able to guide the radiation through a bend that is greater than 180°.


Contrary to the disclosure of U.S. Pat. No. 5,696,379 issued to Stock (1997), the current invention is a 3-dimensional configuration such as the shape of a many-turn circular coil (>360°) or a number of paper clip-shaped tubes stacked together to create a column by deforming the shape of the circular tube forming the coil into an elongated ellipse. The current invention called the “Super Tube” exploits the curved hollow waveguide concept in three dimensions by advancing methods to allow radiation to readily propagate through bends that are >180° thereby achieving a very long path length sample chamber that occupies the minimum of a 3-dimensional space, even though Stock teaches away from such a result.


The first problem that the present invention addresses is to make sure that the incident radiation entering a long waveguide sample chamber having many curves (such as a coil) or U-bends (in the form of a stack of paper clips) be able to “turn” corners inside with relative ease and thereby exiting without significant loss in radiation intensity. The present invention solves this first problem by reducing the angles of incidence for radiations emanating from a quasi-blackbody infrared source.


The second problem that the present invention addresses is to restore some of the inevitable losses that the radiation suffers as it traverses the 3-dimensioanl curved hollow tube or the “Super Tube.” The current invention addresses this problem with simple internal focusing elements installed inside the Super Tube. This is unique only to the innate structure of the current invention.


The third problem that the present invention addresses is the interference of the measurement by ubiquitous water vapor that can be present in the atmosphere in relatively small amounts (e.g. 5,000 ppm) on a dry day or in significantly larger quantities (>45,000 ppm) on a humid day. The current invention addresses this problem with a novel technique of in-situ water vapor correction.


The main drawback for the present invention is the fact that the path-length of the sample chamber is no longer adjustable but depends only upon the actual length of the Super Tube. Comparing with the White and the Herriott cells, the present invention does not require any meticulous adjustments of the optical components prior to its use. It does not require any expensive component like the Pockels cell in the Wong cell which also limits its use by virtue of available electro-optical crystals for its construction. Furthermore, the Super Tube is very easy to build and at a significantly lesser cost. Finally, it is rugged enough for use outside of laboratories in both NDIR and TDLAS type transportable gas analyzers.


The Super Tube of the present invention is a hollow metallic tube, preferably made out of aluminum, brass or stainless steel with specularly reflective inner walls. The typical outside diameter for the Super Tube is not critical and a convenient value is 0.500″ with a typical wall thickness of ˜0.050″. FIG. 1 depicts the schematic layout for the present Super Tube 1 invention having a bending radius of “R” and a section length of “L”. The total path length for the Super Tube is equal to [(N×π×R)+(N+1)×L] where N is the number of “U” (180°) bends forming the Super Tube. The bending radius R typically should be >1.00″ otherwise it would be very difficult to form. The sectional length L can be of any value that fits a particular dimensional requirement. As shown in FIG. 1 the path length has a value equal to (3πR+4L). For example, when R=1.25″ and L=12″, the path length of the Super Tube will be approximately 2 meters or six feet.


Depending upon the path length requirement together with an overall dimensional restriction for a particular sensor, the number of U bends forming the Super Tube can be increased to meet a particular demand. FIG. 2 shows a Super Tube 2 that possesses a total of 5 U bends. In this case for the same R=1.25″ and L=12″ as before, the path length of the Super Tube 2 as depicted in FIG. 2 is close to 3 meters or nine feet. It is especially preferred, for ease of manufacture, that the two ends of the Super Tube are in roughly the same plane and that the bends be U bends (i.e., 180° bends), but this is not required. With reference to FIG. 3, for the Super Tube to work as designed, radiation 3 radiating into this long sample chamber 4 from infrared source 5 having many U (180°) bends must be able to “turn” corners inside with relative ease to thereby propagate inside it without any significant losses in intensity.


The mechanism and efficiency of radiation propagating along a curved tube such as a circle, a U (180°) or right angle (90°) or a combination thereof is quite different from those propagating along a straight section of a tube. In both cases, radiation has to reflect repeatedly forward within the smooth inner walls of the tube in order to reach the detector, its intended target. For radiation propagating along a straight section of a tube, the result is simple and deterministic. However, for radiation propagating along a curved tubing, the result can be haphazard and unpredictable. In this case, the angle of incidence of the impinging radiation upon the inner wall surface plays a crucial role in determining whether the radiation will continue to go forwards, trapped into stationery resonant reflections or reversing its reflection direction going backwards altogether. Depending upon the size of the tube, there exists a critical angle of incidence for the impinging radiation above which the reflecting and forward-going radiation will reverse its direction along the tube and go backwards. Thus, in order to ensure that the radiation introduced into a waveguide sample chamber having a structure other than a simple straight section, the entrance angle of incidence, which depends upon the tube diameter, must be correctly designed and taken into consideration.


The present invention addresses this problem by reducing the angle of incidence 6 for radiations emanating from a quasi-blackbody infrared source 5 with a reflecting conical surface 7 having an inclined angle 8 to the longitudinal axis 9 of the Super Tube of ˜10° as depicted in FIG. 3. In order to provide this symmetrical conical reflecting surface 7, a hollow conical mirror 10 (see FIG. 3) is installed very closely to emitting surface 11 of infrared source 5. This hollow conical mirror 10 has a polished inner surface 7 to provide a high reflectivity for incident radiation 3 emanating from infrared source 5. Aperture 12 of conical mirror 10 facing infrared source 5 virtually accepts all radiations from it. The opposite aperture 13 of conical mirror 10 matches the inner diameter R of the Super Tube.


Since most infrared sources are quasi-blackbodies, the radiation pattern in a hemisphere follows closely to that of the Lambertian distribution. The Lambertian distribution of an infrared source specifies the magnitude of its spectral radiant emittance radiating into an hemisphere at any point in space as a function of the Euler angles subtended by the point at the geometrical center of the source. From the consideration of their subtended solid angles at the source, both obtuse (grazing) and normal (perpendicular to the source surface) direction radiations are much weaker than those radiating at angles between 30-60° as measured from the normal to the source's surface. Thus, a significant amount of radiation from an infrared source entering the “wave-guide” sample chamber or the Super Tube will normally have incident angles ranging from 30 to over 60°. Radiations traveling in a tube having this range of incident angles will not be able to turn circular corners having a relatively small radius (<2.0″) efficiently. The same holds true for traversing a 180° U turn. However, the installation of the hollow conical mirror 10 (see FIG. 3) effectively reduces the magnitude of the “bouncing angle” for radiation emanating from the source to approximately <20° thereby greatly increasing its throughput as the radiation traverses the bending curves of the Super Tube.


Another approach to limit the launching angle for radiations emanating from an infrared source for the Super Tube is to install a parabolic mirror in front of the source as shown schematically in FIG. 4. In FIG. 4, source 5 will be located very close to the focus of parabolic mirror 14 so that most of the radiation from source 5 will be quasi-focused into an approximately parallel beam hugging longitudinal axis 9 of the Super Tube 4; however, such radiation must not be a beam that is parallel, such as what might be obtained through use of a laser, because such a beam would hit the wall of the first bend and bounce back out of the Super Tube, not propagate within the Super Tube. Accordingly, the “bouncing angle” for radiation emanating from the source should ideally be greater than 0° and less than approximately 20°.


Contrary to the disclosure of the U.S. Pat. No. 5,696,379 issued to Stock (1997), the current invention is a 3-dimensional configuration such as stacking a number of U-bends upon themselves much like forming a column of paper clips with one on top of the other as exemplified in FIGS. 1 and 2 as examples. For the current Super Tube invention to work, another problem that needs to be addressed is how to restore some of the inevitable losses that the radiation, emanating from the infrared source, suffers as it traverses the 3-dimensional Super Tube. Since the sensitive area of the infrared detector is smaller than the internal diameter of the Super Tube, another hollow conical mirror can be used to focus down the extent of the incoming radiation to match the sensitive area of the detector as illustrated in FIG. 5. Unlike the situation described earlier in the use of a conical mirror to limit the launching angle of radiations emanating from the infrared source 5 (see FIG. 3), aperture 15 of conical mirror 10 (see FIG. 5) is only slightly larger than the sensitive area 11 of infrared detector 12. It is important to point out that the vertical angle 13 of conical mirror 10 with respect to the longitudinal axis 9 of the Super Tube must not be more than ˜10° otherwise the incident radiation might reverse itself in direction and miss the detector altogether.


The final and extraordinarily difficult problem facing the Super Tube is a problem whose existence to date has not even been identified nor properly addressed by the NDIR gas sensor community, namely, the interference of the measurement of very weak absorbing gases, or gases that need to be detected down to very low levels (e.g. ppm-ppb ranges) or both by the presence of an unpredictable quantity of water vapor in the ambient air.


Let us briefly explain why water vapor interference is such a nasty problem for making very low concentration measurements for weakly absorbing gases when using the NDIR gas detection technique. First of all, apart from its prominent infrared absorption bands at 1.87μ, 2.67μ, 3.2μ and 6.27μ, water vapor has numerous weaker absorptions literally everywhere throughout the middle infrared spectrum (2.0μ-16 μ). For measurement of gas concentrations such as CO2, methane etc. in the hundreds of ppm range using the NDIR technique, such weak absorptions of water vapor can be ignored because its interference, even within the absorption band of the gas in question, is equivalent to only a few ppm's and hence relatively small. However, for the measurement of very low concentration of gas species (ppb-ppm ranges) such as ethylene (C2H4), the interference of these weak but fluctuating water vapor absorptions within the pass band of C2H4 on the actual gas measurement is nevertheless significant. Even though its effect is also equivalent to just a few ppm's, its magnitude is comparable to the level of the gas measurement itself. For this reason, the water vapor interference must be corrected or compensated for. The current invention uses what is called an “in-situ” water vapor interference correction methodology to overcome this problem. Such a method actually measures the amount of water vapor present in the sample chamber with the use of a separate and in-situ calibrated detector so that the interference effect can be quantitatively deducted from the measured signal. As will be expounded below, such a methodology is feasible only with the advent of the current Super Tube sample chamber configuration and is therefore uniquely complementary to the current invention.


Apart from some very strong infrared absorbing bands, water vapor also has very weakly absorbing bands throughout the entire infrared region (2-16μ). In fact, that is the reason why water vapor is such a bother, but only in very special situations when very low concentration of gases need to be detected as mentioned above. However, there is a silver lining behind it. Because of the fact that the absorption is so weak in the regions other than its own strong absorbing bands, the concentration of water vapor can be measured almost anywhere provided that there are no known absorption bands for other gases (including the gas in question) present. In other words, whereas the spectral filter for the gas measurement has to be carefully selected, the spectral filter for the water measurement can be readily chosen as long as the filter band does not coincide with any known absorption bands of gases in the atmosphere. Thus it is possible to detect the actual presence of water vapor within a particular absorption band designed to measure gas X by providing a second detector that will simultaneously measure only water vapor and nothing else. Since the absorbing band for gas X also measures water vapor, the measurement of only water vapor by another detector could be used to subtract out the contribution of water vapor in the gas X measurement channel.


The Super Tube's unique sample chamber configuration provides a very convenient way to set up an optical arrangement for installing a second detector in line with the main “gas” detector for the measurement of water vapor as illustrated in FIG. 6. As shown in FIG. 6, both the gas detector 16 and the second water vapor detector 17 are housed behind an infrared window 18 in a detector chamber. Window 18 is used to eliminate any thermal influence from the flowing gas sample on the performance of the detectors during operation. As shown in FIG. 6, the front or “gas” detector 16 is structurally suspended in the middle of the Super Tube but does not totally obscure the second or back detector 17 from the incident radiation of the infrared source. To improve the collection efficiency of radiation for the back detector 17, a suitably designed conical mirror 19 can be installed in front of it as shown in FIG. 6. Despite the functionally negligible difference in radiation collection efficiency for the two detectors, both of them share substantially the same sample chamber environment as far as gas measurement is concerned. While the ambient gas sample entering the sensor contains both the “gas” to be measured and also a certain unknown amount of water vapor, the front detector will measure the influence of both gas species on its output whereas the back detector measures only the influence of the water vapor present in the entering gas sample. Thus, if the output influence of the second detector is subtracted from that of the first, the interference of water vapor on the “gas” measurement is effectively taken into consideration or eliminated. (Or, of course, the order of the detectors could be reversed and the first detector could be used to measure the influence of water vapor while the second detector could be used to measure the influence of the gas species to be detected.)


The optical arrangement concept disclosed above in the use of two in-line detectors for correcting the interference of water vapor in “gas” measurement can readily be extended to render the sensor into one that can detect multiple gas species. Such an optical arrangement is depicted in FIG. 7. With the exception of the front-most detector 16 and the rear-most detector 17 one or more detectors can be mounted off-axis so as not to impede the incident radiation from reaching the rear-most detector 17 but allowing some radiation to incident on itself. (Also, the other detectors could also be mounted off-axis, but this is not preferable because such an arrangement would be less efficient.) As shown in FIG. 7, a third detector 20 with an appropriate spectral filter 21 for detecting gas species Y, represents another gas detection means when it is mounted off the axis 10 and behind the front-most detector 16. Similarly, more detectors with appropriate filters can be mounted off-axis in front of the rear-most detector 17. Thus, this optical arrangement, which is unique to the current Super Tube sample chamber, is capable of rendering the sensor with multiple gas species detection capability.


The optics of the current Super Tube invention provide yet another very important sensor performance enhancement characteristic. Because the sensor optics comprises only a reflective hollow tube and radiation from the infrared source is made to travel forwards from one end of the tube to reach one or more detectors at the other end, there is no inherent restriction as to how much incident power from the source can be “pumped” into the Super Tube provided adequate heat-sinking means is available. In other words, the Super Tube allows, at least in principle, as much radiation as is needed to be used for the detection of one or more gases. Since the detectivities of the sensor detectors are not affected, the overall signal-to-noise (S/N) can be boosted at will. The only limitation appears to be the added implementation cost for the sensor.



FIG. 8 shows one packaging scheme for the Super Tube infrared source that houses four regular blackbody sources thus boosting the incident radiation by a factor close to four. With reference to FIG. 8, four blackbody sources 22 are die-attached on to one single TO8 header 23 with a protective can (not shown). The special TO8 header 23 allows the extra heat generated by the sources to be adequately dissipated to a heat sink (not shown) and its surroundings. It can readily be seen that any reasonable number of similar blackbody sources (>4) can be packaged to a custom header if more power is required.


It can be seen from the discussion above that the current Super Tube invention is capable of providing long path lengths for the detection of trace gases having a very weak infrared absorption band or required to be detected down to ppb-ppm ranges within a relatively compact space. Furthermore, the current invention offers great robustness and a low-cost implementation when applied to either NDIR or TDLAS type transportable gas analyzers.


While the invention has been described herein with reference to certain examples, those examples have been presented for illustration and explanation only, and not to limit the scope of the invention. Additional modifications and examples thereof will be obvious to those skilled in the art having the benefit of this detailed description. For example, while the Super Tube has been depicted in the drawings and discussed above as having a circular cross-section, it need not only have such geometry; instead, the Super Tube can have a cross section in many different geometries, such as a square, so long as it functions as a hollow waveguide. In addition, several detectors can be combined in one physical package and the Super Tube will also be useful in certain applications where only one detector is required. Further modifications are also possible in alternative embodiments without departing from the inventive concept.


Accordingly, it will be apparent to those skilled in the art that still further changes and modifications in the actual concepts described herein can readily be made without departing from the spirit and scope of the disclosed inventions as defined by the following claims.

Claims
  • 1. A measuring apparatus for measuring the concentration of a gas by infrared absorption, the measuring apparatus comprising: a radiation source for emitting infrared radiation;a hollow waveguide defining a measuring length and an interior for receiving the gas to be measured;a focusing device for quasi-focusing said radiation into a beam with an angle of incidence between greater than approximately 0° and approximately 10° relative to a longitudinal axis of a first linear segment of the waveguide proximate the source;a first radiation detector for converting said infrared radiation into a first measurement quantity; anda second radiation detector for converting said infrared radiation into a second measurement quantity;wherein the measuring length of said waveguide has a plurality of bends that are collectively greater than 180 degrees in three dimensions, andwherein one of the first and second signals is based upon a first absorption band for gas species X while the other of said signals is based upon a second absorption band chosen to detect water which does not coincide with any known absorption bands of gases in the sample cell.
  • 2. The measuring apparatus of claim 1, further comprising: a window impermeable to said gas and mounted in said hollow waveguide for partitioning the detector chamber with the first and second radiation detectors from said gas.
  • 3. The measuring apparatus of claim 1, wherein the focusing device is located in the hollow waveguide.
  • 4. The measuring apparatus of claim 3, wherein the focusing device is a conical reflective surface having an inclined angle to the longitudinal axis of approximately 10 degrees and the conical reflective surface is installed proximate an emitting surface of the infrared source.
  • 5. The measuring apparatus of claim 3, wherein the focusing device is a parabolic mirror.
  • 6. The measuring apparatus of claim 1, further comprising: a second focusing device for focusing said infrared radiation after it has traveled through substantially all of the waveguide and as it approaches the first detector.
  • 7. The measuring apparatus of claim 6, wherein the second focusing device is a conical mirror with a vertical angle with respect to the longitudinal axis of the detector chamber of not more than approximately 10 degrees.
  • 8. The measuring apparatus of claim 7, further comprising: a third focusing device for focusing said infrared radiation between said first and said detectors.
  • 9. The measuring apparatus of claim 6, wherein the third focusing device is a conical mirror with a vertical angle with respect to the longitudinal axis of the detector chamber of not more than approximately 10 degrees.
  • 10. The measuring apparatus of claim 6, wherein one of the first and second detectors are offset relative to the other of said detectors in a detector chamber and said first and second detectors are positioned in-line on a single detector axis.
  • 11. The measuring apparatus of claim 6, further comprising: a third radiation detector located in the detector chamber for converting said infrared radiation into a third measurement quantity based upon a third absorption band for a gas species Y.
  • 12. The measuring apparatus of claim 11, wherein the third detector is mounted off a single detector axis in which said first and second detectors are positioned.
  • 13. The measuring apparatus of claim 11, further comprising: third and fourth focusing devices for focusing said infrared radiation between each of said first, second and third detectors.
  • 14. The measuring apparatus of claim 13, wherein said third and fourth focusing devices are conical mirrors with a vertical angle with respect to the longitudinal axis of the detector chamber of not more than approximately 10 degrees.
  • 15. The measuring apparatus of claim 14, wherein the concentration of gas species X detected is less than 100 parts per million (“ppm”).
  • 16. The measuring apparatus of claim 15, wherein the plurality of bends are collectively greater than 360 degrees in three dimensions.
  • 17. The measuring apparatus of claim 1, wherein the radiation source is comprised of a plurality of infrared sources with a heat sink.
  • 18. A measuring apparatus for measuring the concentration of a gas by infrared absorption with a correction for water vapor, the measuring apparatus comprising: a radiation source for emitting infrared radiation;a hollow waveguide defining a measuring length and an interior for receiving the gas to be measured;a focusing device for quasi-focusing said radiation into a beam with an angle of incidence between greater than approximately 0° and approximately 20° relative to a longitudinal axis of a first linear segment of the waveguide proximate the source;a first radiation detector for converting said infrared radiation into a first measurement quantity;a second radiation detector for converting said infrared radiation into a second measurement quantity;a second focusing device for focusing said infrared radiation after it has traveled through substantially all of the waveguide and as it approaches the first detector; anda third focusing device for focusing said infrared radiation between said first and said detectors;wherein the measuring length of said waveguide has a plurality of bends that are collectively greater than 360 degrees in three dimensions, andwherein one of the first and second detectors are offset relative to the other of said detectors in a detector chamber; and
  • 19. The measuring apparatus of claim 18, further comprising: a third radiation detector located in the detector chamber for converting said infrared radiation into a third measurement quantity based upon a third absorption band for a gas species Y.
  • 20. A compact and long path-length sample cell for use in measuring very small concentrations of a gas based upon the absorption of infrared radiation as it passes through the gas within the sample cell, comprising: a hollow waveguide defining a measuring length and an interior for receiving the gas to be measured;a focusing device for quasi-focusing said radiation into a beam with an angle of incidence between greater than approximately 0° and approximately 10° relative to a longitudinal axis of a first linear segment of the waveguide proximate a source of infrared radiation; anda second focusing device for focusing said infrared radiation after it has traveled through substantially all of the waveguide as it approaches a detector chamber;wherein the measuring length of said waveguide has a plurality of bends that are collectively greater than 180 degrees in three dimensions.