This paper discusses the development of an open-path millimeter-wave (mm-wave) spectroscopy system in the 225--315 GHz atmospheric window. The new system is primarily a monostatic swept-frequency radar consisting of a mm-wave sweeper, hot-electron-bolometer or Schottky detector, and trihedral reflector. The heart of the system is a Russian backward-wave oscillator (BWO) tube that is tunable over 225--350 GHz. A mm-wave sweeper has been built with the BWO tube to sweep the entire frequency range within 1 s. The chemical plume to be detected is situated between the transmitter/receiver and the reflector. Millimeter-wave absorption spectra of chemicals in the plume are determined by measuring swept-frequency radar signals with and without the plume in the beam path. Because of power supply noise and thermal instabilities within the BWO structure over time, the BWO frequencies fluctuate between sweeps and thus cause errors in baseline subtraction. To reduce this frequency-jitter problem, a quasi-optical Fabry-Perot cavity is used in conjunction with the radar for on-line calibration of sweep traces, allowing excellent baseline subtraction and signal averaging. Initial results of the new system are given for open-path detection of chemicals

Bakhtiari, S.

Gopalsami, N.

Raptis, A. C.

UNT Digital Library

OPEN-PATH MILLIMETER-WAVE SPECTROSCOPY IN THE 225-315 GHz RANGE* b y  N. Gopalsami, S. Bakhtiari, and A. C. Energy Technology Division Argonne National Laboratory Argonne, Illinois 60439 Raptis The submitted manuscript has been authored by a contractor of the U.S. Government unde r  contract No. W-3 1-1 09-ENG-3 8. According 1 y , the U.S. Government retains a nonexclusive, royalty-free license to publish or reproduce the published form of this contribution, o r  allow others to do so, for U.S. Government purposes .  To appear in Proceedings of SPIE'96 Intl. Conference on Millimeter and Submillimeter Waves and Applications 111, August 4-9, 1996, Denver, CO *Work supported by U. S. Department of Energy, Office of Nonproliferation and National Security, Office of Research and Development, under Contract W-3 1-109-ENG-38 DISCLAIMER Portions of this document may be illegible in electronic image products. Images are produced from the best available original document c Open-Path blillimeter-Wave Spectroscopy in the 225-3 I5 GHz Range N. Gopalsami. S. Bakhtiari. and A. C. Raptis Energy Technology Division hgonne National Laboratory, Argonne, Illinois 60439 ABSTRACT This paper discusses the development of an open-path millimeter-wave (mm-wave) spectroscopy system in the 225-3 15 GHz atmospheric window. The new system is primarily a monostatic swept- frequency radar consisting of a nun-wave sweeper, hot-electron-bolometer or Schottky detector, and trihedral reflector. The heart of the system is a Russian backward-wave oscillator (BWO) tube that is tunable over 225-350 GHz. A mm-wave sweeper has been built with the BWO tube to sweep the entire frequency range within 1 s. The chemical plume to be detected is situated between the transmitterh-eceiver and the reflector. Millimeter-wave absorption spectra of chemicals in the plume are determined by measuring swept-frequency radar signals with and without the plume in the beam path. Because of power supply noise and thermal instabilities within the BWO structure over time, the BWO frequencies fluctuate between sweeps and thus cause errors in baseline subtraction. To reduce this frequency-jitter problem, a quasi-optical Fabry-Perot cavity is used in conjunction with the radar for on- line calibration of sweep traces, allowing excellent baseline subtraction and signal averaging. Initial results of the new system are given for open-path detection of chemicals. Key Words: Millimeter waves, backward-wave oscillator, molecular spectroscopy, open-path monitoring. 1. INTRODUCTION Under the 1990 Clean Air Act Amendments, industry is required to demonstrate environmental compliance by enhanced (continuous) monitoring of its emissions or of parameters correlated to its emissions.' The continuous monitoring devices (CEMs) available to date are mostly species-specific and use sampling techniques. Standoff or open-path monitoring of stack emissions is attractive because it is nonintrusive and obviates the need for sampling. Electromagnetic radiation utilizing broadband sources in the infrared (IR), visible, and ultraviolet (UV) regions has been investigated for remote sensing of chemicak2 In addition, laser techniques known as LIDAR (light detection and ranging) are g M g  importance for remote   en sing.^ These techniques are generally based on molecular vibrational energy transitions in the IR region, electronic energy transitions in the W and visible regions, and Raman scattering in the UV region. Millimeter-wave (mm-wave) spectroscopy based on rotational energy transitions is a complementary technique to the optical and laser approaches. Because of their longer wavelengths compared to those optics, mm-wave techniques can be used in smoky and dusty environments, are less affected by cloud conditions, and can provide longer detection ranges. Additionally, interference fiom water vapor and other common atmospheric species such as CO2 and methane is reduced when using mm wavcs. Polar molecules selectively absorb electromagnetic radiation of specific wavelengths in the centimeter and millimeter regions in accordance with their rotational energy transitions.' Millimeter- wave spectral lines are narrow and highly resolvable under low pressures (<1 torr). As the pressure increases, however, the spectral lines are broadened due to molecular collisions, and also the peaks of the lines are reduced. As a result, detection sensitivity and chemical selectivity suffer at higher pressures. The pressure-broadening problems inherent with open-path monitoring (e.g., in the atmosphere) can be mitigated by using high-frequency mm-wave sources with wide sweep-width capability. Detection sensitivity increases in general with the square of the frequency, and the number of resolution lines (chemical selectivity) increases with the sweep width. Recently, feasibility of the mm-wave technique was shown for environmental monitoring in open air by using a monostatic swept-frequency radar system in the 225-3 15 GHz range.' The mm waves were generated by employing a low-frequency sweeper and frequency triplers. Because the triplers, which are based on harmonic generation are not efficient, the radiation power obtained was low in the microwatt range. The narrow bandwidth of the triplers also limited the tuning range to within 50 GHz. The proof- of-principle was tested with this system by detecting D20 in open air. In additon, the chemical selectivity of the technique was demonstrated by employing a special deconvolution procedure; individual chemicals in a multicomponent mixture were determined with both simulated and experimental spectra.6 This paper describes the development of a prototype radar system based on a Russian backward- wave-oscillator (BWO) tube (Model OB-30) that can sweep the entire frequency range within 1 s and generates up to 10 mW of power. This higher power allows longer detection range and the wider tuning range improves spectral line resolution and molecular selectivity. Because of power supply noise and thermal instabilities in the B WO structure over time, the BWO frequencies fluctuate between sweeps and cause poor baseline subtraction. To mitigate the frequency jitter problem, part of the mm-wave beam is coupled to a quasi-optical Fabry-Perot cavity that produces a sequence of frequency markers during the sweep. These cavity markers are used in software to produce on-the-fly calibration of the sweep traces, which then allows excellent baseline subtraction and signal averaging. Initial results of the new mm-wave system are given for open-path detection of chemicals. 2. DEVELOPMENT OF MONOSTATIC RADAR SYSTEM Figure 1 is a schematic diagram of the monostatic radar system built for open-path chemical measurements in the frequency range of 225-3 15 GHz. It consists of a free-running mm-wave sweeper that generates and transmits mm waves through a plume of chemicals to be measured. A retroreflector is used on the far side of the plume to return the radiation to the transmitter. A liquid-helium-cooled bolometer or ambient-temperature Schottky detector is used to measure return signals. Absorption spectra of the plume gases are determined by comparing the return signals with and without the plume in the beam path. 2. t Millimeter-wave sweeper sweeper. The tube, as shown in Fig. 2(a), is 25 mm in diameter and 35 mm Long, and water cooled. It requires an AC filament power supply (6.4 V, 1.35 A) to heat the cathode, a high-voltage (HV) power supply (1 000-4000 V, 40 mA) between the cathode and slow-wave structure to accelerate the electrons, and a DC magnetic field of 7000 G between cathode and collector to steer the electron beam over the slow-wave structure. A permanent magnet made of cobalt-samarium alloy produces the magnetic field. To generate mm-wave oscillations, the tube must be properly aligned with respect to the DC magnetic field and is mounted in the pole gap of the magnet with a three-axis alignment fixture, see Fig. 2(b); the radiation is coupled to a scalar horn through an over-moded rectangular wave guide attached to the tube structure. The tube is tunable from 225 to 350 GHz by varying the HV from 1000 to 4000 V and provides average of 10 mW. A 5-kV Bertan power supply (Model 210-05R) that can be swept by a 0-5 V remote control input is used to sweep the HV. A backward-wave oscillator tube (OB-30 from the Istok Company, Russia) is the heart ofmm-wave I ~ Plume Fabry-Perot Cavity Fig. 1. Schematic diagram of mm-wave radar system in 225-3 15 GHz range. The BWO tube generates monochromatic radiation, but its frequency stability depends on (a) power supply voltage fluctuations, (b) alignment of the tube in the magnetic field, and (c) temperature of the tube structure. The frequency of the tube is controlled mainly by the HV power supply. On the average, the tube has a sensitivity of 70 W. Because the BWO tube has extremely low internal capacitance, all Hv noise, including 60-Hz ripple and switching power-supply noise (20 kHz), are converted into frequency variation. Three types of instabilities (blinking effect, mode breaks, and mode switching) may occur while tuning the tube,but in most cases can be eliminated by proper alignment. To control the temperature of the tube structure and thus ensure long-term stability of the radiation, a temperature-controlled closed-cycle water pump circulates coolant through the tube. 35 mm I- Cooling tubes ’ 1 I Slow- Waveguide with antenna wave structure T :  254mm I Support Structure *F mm Filaments 1 11 Cathode / (a) Backward-wave oscillator (BWO) tube 189 mm $ Magnet A (b) BWO tube positioned inside magnet, with alignment fixture Fig. 2. Backward wave oscillator: (a) internal structure of tube, (b) support and alignment furture inside the permanent magnet. Despite of all the precautions one may take to control BWO stability, it is nearly impossible to achieve the frequency stability required for baseline subtraction and signal averaging. Hence, one often resorts to phase-locked control of the BWO in high-resolution spectroscopy, but this is rather slow for cavity markers. Because the cavity markers correspond to the actual frequencies during a sweep, the cavity markers and the corresponding samples of radar data are aligned or matched with each other by sof'tware between data traces. The radar data between the cavity markers are interpolated linearly. Figure 4 shows subtraction of two B WO swept-frequency traces, with and without the use of cavity markers. Because of transients associated with the return ramp of the sweep, the first 5000 points of 25,000 points of the sweep trace are ignored. Further improvement is possible by increasing the cavity length, which in turn decreases the spacing between frequency markers. Thus, the use of an F-P cavity enables us to calibrate on-the-fly the frequencies of a fiee-running oscillator, providing excellent baseline subtraction and signal averaging. Dirwt...wbtractjon ........................................................... ............................... .- ICI 0 ....- (P - ction after alignment with cavity markers 8 -100 ' .. -200' ' " I '  " ' I " " I " ' I '  " ' 5000 I 104 1.5 104 2 104 2.5 104 3 io4 Sample Numbers Fig. 4. Baseline subtraction with and without cavity markers. To test the spectral line detection, 200 mtorr of CH3CN was pumped into a 1.4-m-long gas cell. The BWO was swept linearly between 1500 to 2700 V in 1 s. Three groups of CH3CN lines around 276, 294, and 3 12 GHz were covered in the sweep range. Figure 5 gives the percent absorption of the gas determined by measuring the detected power (with a bolometer) with and without the gas in the cell. The small spikes along the baseline correspond to those cavity lines not totally subtracted out. The sweep trace was calibrated in terms of frequency by using the known CH3CN lines and appropriate interpolation based on the BWO voltage-to-fkequency static tuning curve. Resolution and sensitivity of the system can be determined by examining (zooming) a narrow frequency range ofthe fast sweep data. Figure 6 is a replot of the data in Fig. 5 over a 5 GHz range near the 276 GHz line. We see not only the rotational lines of the ground state but also those of excited vibrational states. The system provides a resolution of about 4 MHz and a sensitivity of the fast-sweep mode for low-pressure lines. cm-' in S 0 .- CI L n n 0 v) Q S Q) CI P a Fig. 5 .  Low-pressure spectra of CH3CN. - 3. Open-path measurements The monostatic mm-wave radar system in Fig. 1 was tested for open-path detection of chemicals in the laboratory, with a distance of 5 m between the transmitter and reflector. The same sweep parameters (sweep range and sweep rate) used for the CH3CN tests (Fig. 5) were adopted for this test, so that the calibration of the sweep trace is known with respect to frequency. A plume was created by heating D20 in a beaker and releasing the vapor in the path of the rmn-wave beam. To improve the pathlength, we contained the plume in a 46-cm-long T-shaped glass pipe with open ends. Figure 7 shows the absorption peak of DzO around 3 18 GHz. Fluctuation in the baseline is due to changes in the pattern of the standing waves that arise fiom reflections at the detector, reflector, and transmitter. ....................................................................................... _.._..._ 274 275 276 277 278 279 Frequency (GHt)  Fig. 6.  Replot of Fig. 5 over a narrow frequency range. 4. CONCLUSIONS We have developed a swept-frequency monostatic radar system in the range of 225-3 15 GHz for open-path detection of chemicals. As a part of the system, a mm-wave sweeper has been built using a Russian backward-wave oscillator (BWO) tube; it can be swept over the entire frequency range in 1 s and provides an average power of 10 mW. While a free-running BWO sweeper is inherently unstable in - terms of repeatability of frequencies during a sweep, this frequency instability problem was solved by using a Fabry-Perot cavity that provides on-the-fly calibration of frequencies. The BWO sweeper was tested by measuring low-pressure CH3CN lines in a gas cell. A comparison of baseline subtraction with and without the cavity markers showed the superiority of the cavity approach. The system showed a frequency resolution of 4 MHz and a detection sensitivity of cm-' in a fast scan of low-pressure lines. The new system offers a major improvement in power, sweep range, and detection sensitivity over the previous system which used frequency triplers on the output of a low-frequency ~weeper.~ Open-path detection capability of the monostatic swept-frequency radar system was tested by releasing D20 in open air. Initially, the system was tested in the laboratory over a short range (5-m distance between the transmitter and reflector). The tests showed the detection of D20 absorption line . .  at 3 18 GHz. Further work is underway to test the system at longer distances and against different chemicals by sampling chemicals into a plastic (Tedlar) bag and palcing it in the beam path. ..................................................................................................................................................................... BF A i ............................................................ - ............................... -2 I 1 , , 1 , , , , 1 , , , , 1 , , , , ~ , , , ,  280 290 300 31 0 320 330 Frequency (GHz) Fig. 7. Detection of D20 plume released in open air. 5. ACKNOWLEDGMENTS The authors thank Dr. M. Yu. Tretyakov for helpful suggestions on the characterization of BWO - instabilities. The BWO alignment structure and power supply were built by The Ohio State University, and the Fabry-Perot cavity was built by the Institute of Applied Physics, N i d i  Novgorod, Russia, under subcontracts from Argonne National Laboratory. This work is supported by the U.S. Departrnent of Energy, Ofice of Nonproliferation and National Security, Office of Research and Development, under Contract W-3 1 - 109-ENG-3 8. 6. REFERENCES 1. P. G. McCoy, S .  Boone, T. Dincer, and C. Mijares, "Statistical review of U.S. EPA Region 5's CEM database," Roc. AWMA Cod. on Continuous Compliance Monitoring under the Clean Air act Amendments, Chicago, Oct. 25-27,1995. Air Waste Manage. Assoc., vol. 42, pp. 18-30, 1992. 2. W. B. Grant, R €3. Kagann, and W. A. McClenny, "Optical remote measurement of toxic gases, J. 3.  J. V. Cernius, D. A. Elser, and J. Fox, “Remote active spectrometer,” SPIE laser applications in 4. W. Gordy and R. L. Cook, Microwave Molecular Spectra, John Wiley, New York, 1984. 5.  N. Gopalsami, S .  Bakhtiari, A. C. Raptis, S. L. Dieckman, and F. C .  De Lucia, ”Millimeter-wave measurements of molecular spectra with application to environmental monitoring,” IEEE Transactions on Instrumentation and Measurement, vo1.45, pp. 225-230, 1996. 6. N. Gopalsami, S .  Bakhtiari, and A. C.  Raptis, “Development of a millimeter-wave sensor for environmental monitoring,” Proc. International Conf. on Millimeter and Submillimeter Waves and Applications 11, SPIE, vol. 2558, pp. 189-200, 1995. 7. Y. A. Dryagin, V. V. Parshin, A. F. Krupnov, N. Gopalsami, and A. C .  Raptis, ”Precision broadband wavemeter for millimeter and submillimeter range,” To appear in IEEE Transactions on Microwave Theory and Techniques, vol. 44, Sept. 1996. metrology and earth and atmospheric remote sensing, vol. 1062, pp. 164- 17 1 , 1989. DISCLAIMER This report was prepared as an account of work sponsored by an agency of the United States Government. Neither the United States Government nor any agency thereof, nor any of their employees, makes any warranty, express or implied, or assumes any legal liability or responsi- bility for the accuracy, completeness, or usefulness of any information, apparatus, product, or process disclosed, or represents that its use would not infringe privately owned rights. Refer- ence herein to any specific commefcial product, process, or service by trade name, trademark, manufacturer, or oth rwise does not necessarily c nstitute or imply its endorsement, recom- mendation, or favoring by the United States Government or any agency thereof. The views and orinions of authors expressed herein do not necessarily state or reflect those of the -~~ United States Government or any agency thereof. 

Open-path millimeter-wave spectroscopy in the 225--315 GHz range

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Open-path millimeter-wave spectroscopy in the 225--315 GHz range

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