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    Optics and Lasers in Engineering 37 (2002) 101114

    Near- and mid-infrared laser-optical sensors for

    gas analysis

    Peter Werlea,*, Franz Slemra, Karl Maurera, Robert Kormannb,

    Robert M.ucke

    c

    , Bernd J.anker

    d

    aFraunhofer Institut, D-82467 Garmisch-Partenkirchen, GermanybMax-Planck Institut f.ur Chemie, D-55128 Mainz, Germany

    c Infineon Technologies, D-93049 Regensburg, GermanydCarl Zeiss, D-73446 Oberkochen, Germany

    Received 15 April 2001; accepted 12 July 2001

    Abstract

    Semiconductor diode lasers were first developed in the mid-1960s and found immediateapplication as much needed tunable sources for high-resolution laser spectroscopy commonly

    referred to as tunable diode laser absorption spectroscopy (TDLAS). In this paper, currently

    available semiconductor lasers for spectroscopy in the near- and mid-infrared spectral region

    based upon gallium arsenide, indium phosphite, antimonides and lead-salt containing com-

    pounds will be reviewed together with the main features of TDLAS. Room-temperature

    measurements of atmospheric carbon dioxide near 2 mm will be discussed and recent results

    obtained with a fast chemical sensor for methane flux measurements based on lead-salt diode

    lasers operating near 7.8mm will be presented.r 2002 Elsevier Science Ltd. All rights reserved.

    Keywords: Semiconductor lasers; Diode laser spectroscopy; Trace gas analysis; Carbon dioxide; Methane

    1. Introduction

    Laser-optical sensors are now at the threshold of routine applications in air

    pollution monitoring and industrial process and gas analysis. The development of

    this technology has been driven mainly by scientific questions, but increasingly these

    sensors are transferred to industrial and other applications whenever sensitive,

    selective and fast analysis is required. With the increasing complexity of processes,

    *Corresponding author. Haidestr. 4, D-82438 Eschenlohe, Germany.

    E-mail address: [email protected] (P. Werle).

    0143-8166/02/$ - see front matter r 2002 Elsevier Science Ltd. All rights reserved.

    PII: S 0 1 4 3 - 8 1 6 6 ( 0 1 ) 0 0 0 9 2 - 6

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    online gas analysis is becoming a key issue in automated control of various industrial

    applications, in combustion diagnostics, for investigations of aeroengines and

    automobile exhaust measurements. Other challenges are online analysis of high-

    purity process gases, medical diagnostics and monitoring of agricultural andindustrial emissions. The need to meet increasingly stringent environmental and

    legislative requirements has also led to the development of analyzers to measure the

    concentrations of a variety of gases [1] based on near- and mid-infrared absorption

    spectroscopy. After a brief review of currently available diode lasers for different

    spectral regions we will describe a near-infrared trace-gas sensor for carbon dioxide

    based on a room-temperature diode laser and a fast chemical mid-infrared sensor for

    methane based on a lead-salt diode laser.

    2. Semiconductor lasers

    Semiconductor diode lasers play an important role in telecommunications and

    consumer electronics in applications such as fiber optical communications, laser

    printers and CD players because of their small size, high reliability and ease of use.

    As it can be seen from Fig. 1, the whole spectral range from the visible to the infrared

    can be covered by semiconductor lasers of various compounds, which mainly are

    gallium arsenide, indium phosphite, antimonides and lead salts. A drawback for

    industrial applications of spectrometers based on semiconductor lasers is the lack of

    high-quality, high-power laser diodes for many spectral regions of interest.Gallium arsenide and indium phosphite lasers are commercially made from the III

    V group of semiconductor materials. These diode lasers emit from the visible to near-

    infrared wavelengths from 0.63 to 1.55 mm including the InGaAsP/InP 1.31.55 mm

    optical communication lasers, as well as the GaAs/AlGaAs 0.78 and 0.83 mm lasers

    found in compact disk players. The technology of near-IR 1.3 and 1.55mm

    InGaAsP/InP diode lasers developed for fiber-optic communication can be extended

    to fabricate lasers that emit anywhere in the wavelength interval of about 1.22 mm.

    Near-infrared multiple-quantum-well distributed-feedback (DFB) lasers have the

    advantages of single-mode outputs at milliwatt power and near-room-temperature

    operation [2]. A drawback of these devices is that they are available only in narrowspectral regions and only a limited number of molecular species have absorption

    features in the spectral region covered by these lasers. Furthermore, near-IR

    absorptions are overtone or combination bands that are typically one to several

    orders of magnitude weaker than the IR-fundamental band, while many molecules

    of interest have near-IR absorption bands that are strong enough for detection at

    parts-per-million (ppm) and, in some cases, even parts-per-billion (ppb) levels [25].

    Especially, the lasers for the visible/blue spectral range are of increasing importance

    for element analysis based on atom absorption spectroscopy [6].

    Antimonide lasers can be used for wavelengths longer than 1.8 mm and are based

    on IIIV compounds such as AlGaAsSb, InGaAsSb, and InAsSbP. Roomtemperature lasing from 2 to 2.4mm has been reported from simple double

    heterostructure antimonide diode lasers. As wavelength increases up to 3.7 mm, the

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    maximum operating temperature decreases as a result of increasing optical and

    electrical losses. Laser devices based on InAsSb/ InAsSbP double heterostructure

    devices were grown by liquid-phase epitaxy on InAs substrate and cover the spectral

    range from 3 to 4 mm at LN2temperatures. These devices are well suited, e.g. for the

    detection of HCHO at 3.6 mm and CH4 at 3.26 mm [7]. For this spectral range also

    spectroscopic sources based on frequency mixing techniques have been designed,

    which allow room-temperature operation [8].

    Lead-salt diode lasers are made from IVVI semiconductor materials and operate

    in the 330 mm spectral region [9]. Therefore, they cover the IR fundamental bands

    with strong absorption for the most atmospheric trace gases [1]. They are usedalmost exclusively for spectroscopic applications [1014]. Since IVVI lasers and

    their associated detectors operate at cryogenic temperatures, they are more expensive

    Fig. 1. Spectral coverage of the visible to infrared region by different semiconductor laser materials: While

    for pn-junction lasers room-temperature operation is only possible up to 23mm for IIIV materials,

    Quantum cascade lasers become a promising alternative to the cryogenic cooled IVVI lead-salt diode

    lasers. Also shown are absorption cross sections for methane and interfering water vapor.

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    and more cumbersome to use than IIIV devices [15]. In trace gas monitoring

    applications, lead-salt laser instruments have routinely achieved parts-per-billion

    detection levels of a number of important molecular species [1]. For unattended

    industrial routine applications, however, the use of lead-salt diode lasers is limited bythe need of cryogenic cooling by LN2or Stirling coolers (typ. 78120 K), occurrence

    of multimode emission and power levels which are typically only several hundred

    microwatts. Compared to GaAs lasers, lead-salt semiconductor lasers are at a

    relatively early stage of their development due to a much smaller market.

    Until recently, all semiconductor lasers, regardless of their operating wavelength,

    relied upon direct band-to-band transitions in bulk material as shown in Fig. 1 (top

    left). Rapid progress has been reported in mid-IR lasers based on new types of

    transitions. The most notable example is the Quantum cascade (QC) lasers.

    Although the basic concept was proposed as early as 1971, it took more than 20

    years before an actual device was demonstrated in 1994 [16]. Quantum cascade lasers

    are based on a completely different approach than the lasers described so far. In a

    QC laser, electrons make transitions between bound states created by quantum

    confinement in ultra-thin alternating layers of semiconductor materials. Since these

    ultra-thin layers, called quantum wells, have a size comparable to the electrons de

    Broglie wavelength, they restrict the electron motion perpendicular to the plane of

    the layer. Due to this effect called quantum confinement, the electron can only jump

    from one state to the other by discrete steps, emitting photons of light (Fig. 1 top

    right). The spacing between the steps depends on the width of the well, and increases

    as the well size is decreased. In a pictorial way, this laser is freed from bandgapslavery, i.e. the emission wavelength depends now on the layer thickness and not on

    the bandgap of the constituent materials. This has allowed, using the same base

    semiconductors (InGaAs and AlInAs grown on InP), the manufacture of lasers with

    an emission wavelength from 3.5 to 11.5 mm (recent work in Bell labs at Lucent

    Technologies has pushed this limit to 17 mm). Compared to conventional (interband)

    lasers, the quantum cascade laser has the following advantages: The same

    semiconductor material whose technology is very well mastered can be used to

    manufacture lasers operating across the whole mid-infrared (and potentially even

    farther in the far-infrared). It is based on a cascade of identical stages (typically 20

    70), allowing one electron to emit many photons, emitting more optical power. It isintrinsically more robust (no interface recombination) and since the dominant non-

    radiative recombination mechanism is optical phonon emission and not Auger effect

    (as it is the case in narrow-gap materials), it allows intrinsically higher operating

    temperature. While these new types of lasers are still in the experimental stage, they

    appear to offer the prospect of more robust construction and higher temperature

    operation than is possible with the materials which have been used up to this point.

    These devices are operated in pulsed mode at room temperature and allow

    continuous wave operation only at lower temperatures. In the 58 mm wavelength

    region, continuous wave operation at temperatures above 120 K generates

    remarkable output powers of 220 mW and about 200 mW at 80 K [17], while incomparison lead-salt diode lasers deliver only 200 mW at liquid nitrogen temperature.

    With quantum cascade lasers already first spectroscopic measurements have been

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    reported [1820]. The commercial availability of these lasers might promote the

    development of new operational systems that allow highly sensitive measurements

    based on the strong fundamental IR transitions.

    3. Diode laser spectroscopy

    Semiconductor lasers were first introduced in the mid-1960s and found immediate

    application as much needed tunable sources for high-resolution infrared laser

    absorption spectroscopy. The principal setup of an optical absorption spectrometer

    is shown in Fig. 2a. All designs contain a radiation source, a detector and the species

    under investigation in a closed absorption cell for the determination of gas

    concentrations according to Beers law. Most systems also provide a modulation unit

    to generate an AC signal. As a prerequisite to obtain the required specific

    wavelength, selective elements have to be inserted into the optical path. Gasfilter-

    Correlator systems require a reference cell with a high concentration of the gas under

    investigation. While for DOAS systems a monochromator is used, FTIR instruments

    apply a Michelson interferometer as the selective element. Non-dispersive infrared

    systems (NDIR) are based on gas selective devices. All instruments based on these

    technologies meanwhile reached a high degree of complexity and sophistication. An

    alternative approach is to insert the selective element directly into the radiation

    sourceFthe laser. In principle, laser spectrometers allow less complex optomecha-

    nical designs than the current analytical instrumentation and with semiconductor

    Fig. 2. (a) Principle setup of optical absorption spectroscopy, (b) direct absorption spectroscopy using a

    tunable diode laser, (c) conventional wavelength modulation (kHz) spectroscopy and (d) high-frequency

    modulation spectroscopy (MHz).

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    lasers even the required modulation can be implemented electronically. Therefore,

    diode laser spectroscopy is an attractive and promising technique for analytical

    instrumentation. The most important research applications of TDLs in atmospheric

    field measurements required long-path absorption cells to provide high-sensitivitylocal measurements. In spectroscopy a single narrow laser line usually scans over an

    isolated absorption line of the species under investigation (Fig. 2b). To achieve the

    highest selectivity, analysis is made at low pressure, where the absorption lines are

    not substantially broadened by pressure. This type of measurements has developed

    into a very sensitive and general technique for monitoring most atmospheric trace

    species [1]. The main requirement is that the molecule should have an infrared line-

    spectrum which is resolvable at the Doppler limit, which in practice includes most

    molecules with up to five atoms together with some larger molecules. Since TDLAS

    operates at reduced pressure it is not restricted in wavelength to the atmospheric

    windows such as 3.45 and 813 mm.

    Direct absorption measurements have to resolve small changes in a large signal. In

    comparison with direct spectroscopy, the benefits of modulation spectroscopy in

    TDLAS are twofold. Firstly, it produces a difference signal which is directly

    proportional to the species concentration (zero baseline technique) and, secondly, it

    allows the signal to be detected at a frequency at which the laser noise is significantly

    reduced. Wavelength modulation spectroscopy (WMS) has been used with tunable

    diode laser sources since the early 1970s. The earliest TDL systems used a

    modulation frequency in the lower kHz regime and second harmonic detection.

    Today 50 kHz modulation with 100 kHz detection is quite usual and, consequently, itis convenient to regard 100 kHz as a limit of conventional wavelength-modulated

    TDLAS. Modulation spectroscopy is based on the ease with which diode lasers can

    be modulated. In WMS with diode lasers, the injection current is modulated as the

    laser wavelength is tuned repeatedly at about 100 Hz over the selected absorption

    line and a computer-controlled signal-averager is used to accumulate the signal from

    a lock-in amplifier (Fig. 2c or d). This produces a harmonic spectrum of the line,

    with an amplitude proportional to the species concentration. Scanning over the line

    gives increased confidence in the measurement because the characteristic feature of

    the measured species is clearly seen and unwanted spectral features due to interfering

    species or !etalon fringes can easily be identified.While mid-infrared lasers operated at cryogenic temperatures cover the funda-

    mental absorption bands required for ultra-sensitive gas analysis, near-infrared

    room-temperature diode lasers give access mainly to significantly weaker overtone

    and combination bands. Therefore, the selection of the optimum operating

    conditions for a gas analyzer is always a tradeoff between the required sensitivity

    and an operational system. By averaging over periods longer than 1 s or by using

    longer path length the detection limits can be improved. While the predicted

    sensitivities are based on known line strengths and the performance of a typical

    TDLAS system, it is in the nature of field measurements that optimum performance

    is not always achieved due to drift effects and other interfering disturbances [21]. Tocope with these problems different approaches based upon signal processing [22] and

    double modulation techniques [23] have been proposed and successfully applied.

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    To illustrate the performance and operation of state-of-the-art near- and mid-

    infrared spectrometers based on tunable diode lasers in the next section an example

    of a near-infrared trace gas sensor for carbon dioxide based on a room-temperature

    2mm indium-phosphite-DFB-laser will be presented. Finally, a typical mid-infraredspectrometer for methane detection based on a lead-salt diode laser operating at

    7.8mm at liquid nitrogen temperature will be described.

    4. Near-infrared trace-gas sensor for carbon dioxide based on a room-temperature

    diode laser

    For many field measurements or industrial applications the use of liquid nitrogen

    must be avoided, only temperature stabilization by thermoelectrical elements is

    acceptable. Therefore, in a fast CO2 sensor (Fig. 3a) we implemented InP-DFB-

    Fig. 3. (a) Optical layout of a near-infrared spectrometer using an optical multipass cell (Herriott), (b)

    typical mode map of an indium-phosphite-DFB-laser at 2 mm with 12 mW power, (c) measurements of12CO2in ambient air at a pressure of 100 mbar and 100 m optical path length, (d) time series data recorded

    from a 358 ppm 12CO2calibration gas mixture and (e) identification of 12CO2and

    13CO2absorption lines

    around 2001.3 nm.

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    lasers from Sensors Unlimited Inc. (Princeton, NJ) with room-temperature single-

    mode emission at lE2mm as shown in Fig. 3b. The components are mounted on a

    60cm 110 cm optical breadboard on top of a double 19 in rack. The DFB laser is

    held inside a Peltier-cooled mount which is fixed on an xyz-stage. The laser beam iscollimated by an off-axis parabola (OAP) with 10 mm diameter and 12 mm focal

    length. The beam is focused by a spherical mirror (f 1m) to the center of a

    Herriott-type measurement cell. After 181 reflections, corresponding to 100 m, the

    beam exits the cell and is focused onto a temperature-stabilized extended InGaAs

    detector (sensors unlimited) by another OAP. About 8% of the laser beam is coupled

    off by a beam-splitter and directed through the 28 cm reference cell onto another

    InGaAs detector. The whole system is pre-aligned by a visible diode laser, coupled

    into the setup by a pellicle beam-splitter which has to be removed during the

    measurements. In order to provide static as well as flux measurements at defined cell

    pressures, the measurement cell is equipped with a pressure sensor and on/off-valves

    (at inlet and outlet) as well as with a needle valve at the inlet and a throttle valve at

    the outlet. The reference cellFfilled with a high-concentration CO2 mixture and

    sealed offFis connected to the measurement cell by a temperature bridge and a

    differential pressure sensor. With adjusted laser power and the right concentration in

    the reference cell the signals from both detectors have identical shape and amplitude

    and after system calibration using certified gas mixtures the reference signal can be

    used as a secondary calibration standard. The signal processing schemes for single-

    tone and two-tone FM spectroscopy can be found in detail in a recent review of

    advances in semiconductor laser-based gas monitors [1].The NIR system shown above has been applied for the detection of atmospheric

    CO2. The DC current of the temperature-stabilized DFB laser is adjusted to the

    selected absorption line. The laser is scanned over this line by a 1 kHz ramp and

    additionally modulated by high frequency. In order to optimize the signal-to-noise

    ratio and the system stability two different FM techniques (single-tone and two-tone)

    have been implemented. Due to the limited detector bandwidth, frequencies up to

    300 MHz are applied, corresponding to the line width of CO2 at a pressure of

    100 mbar. Some FM signals from a near-infrared InP diode laser operating around

    2mm are shown in Fig. 3c when outdoor air has been pumped through the Herriott

    cell and the ambient CO2 signal of 350 ppm was recorded at 2.004 mm. From theweaker absorption lines of CO2and H2O under high amplification a precision of up

    to 104 has been estimated for 256 averages in less than 1 s. It is obvious that this

    spectral region has a significant advantage versus the 1.573 mm absorption band in

    the NIR, where the line strength is about 2 orders of magnitude weaker. At 2 mm the

    line strength is still weaker than in the fundamental band, but room-temperature

    operation of diode lasers is still possible for cw applications [2]. Recording of

    averaged spectra and calibration lead to time series data as shown in Fig. 3d for a

    358 ppm CO2 calibration gas mixture. Besides ambient measurements another

    possible application could be isotopic ratio measurements for medical diagnosis, e.g.

    breath test.1 Therefore, 13CO2/12CO2 line pairs within the operation range of the

    1 E.g. IRIS-infrared 13C stable isotope analyser, www.wagner-bremen.de.

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    tested 2mm laser have been analyzed in the vicinity of 2000.8 and 2001.3 nm. The

    latter line pair is partly influenced by water vapor as displayed in Fig. 3e but one has

    to consider that the CO2 absorption in expiration air is by a factor of 2030 higher

    than the displayed ones. For medical applications the measuring instrument shouldbe able to determine the ratio of 13CO2 and

    12CO2 with a resolution of at least 1%

    [2], while the absolute CO2 concentration in human expiration air is 35%, with

    100% relative humidity at body temperature. The natural ratio 13CO2 :12CO2 is

    1.09570.003%. Therefore, the instrument must be able to detect both isotopes with

    a resolution ofo103 unaffected by water vapor. The measurement of the 13CO2content in expiration air using the lines at 2000.8 and 2001.3 nm generates about the

    same signal as 12CO2 in ambient atmospheric air masses at 2004 nm. Therefore,

    equivalent detection limits are expected. For a typical required reproducibility of less

    than 0.3 delta per mille for the determination of the 13C/12C ratio, the neighboring12CO2 lines, which are weaker by a factor of 4, dominate the sensitivity, but even at

    absorption path lengths of less than 10 m clear signals are expected. The main

    problem of accuracy is connected with temperature: the ratio of the line strength

    must be kept constant, which means here that the temperature during the analysis

    including calibration must be stable within 0.01 K, because the involved line

    strengths show opposite temperature dependencies (at 2001.3 nm the ratio of the line

    strengths changes from 5.4655 at 290 K to 4.081 at 300 K). A reliable measurement

    of the 13CO2 :12CO2ratio using the 2000.8 and 2001.3 nm spectral regions is not easy

    to perform, but feasible when using a small multipass cell. Nevertheless, the

    utilization of line pairs with reduced sensitivity to temperature changes isrecommended. Therefore, the line pairs must be chosen in such a way that their

    temperature coefficients are low but also as close as possible to each other. However,

    this measurement illustrates the principle and feasibility of isotopic measurements

    using tunable diode laser absorption spectroscopy, but especially for 13CO2/12CO2

    isotopic ratio analysis already commercially available competitive systems based on

    non-dispersive infrared analyzers exist, which meet the requirements in terms of

    sensitivity and time resolution (see footnote 1).

    5. Fast chemical mid-infrared sensor for methane based on a lead-salt diode laser

    A fast laser-optical sensor is the key issue for trace gas flux measurements based

    on the so-called eddy correlation technique [1214]. As high time resolution and high

    chemical resolution were the prerequisites for the success of the measurements, high-

    frequency modulation (FM) spectroscopy has been selected. In FM spectroscopy,

    the laser is modulated at higher frequencies, typically in the radio frequency (rf)

    region, thus allowing selective and fast scanning over an absorption line of a

    molecule [1]. The layout of the detection electronics is shown in Fig. 4a. The system

    can be run in either single-tone or two-tone mode and the optimum method can be

    selected by the system operator from case to case depending on the experimentalconditions. The modulation section provides the required rf-modulation for the

    laser. The laser beam is split into a sample and a reference path. Detector signals are

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    fed into a phase-sensitive detection electronics, which can be regarded as a high-

    frequency lock-in amplifier. Both signals (sample and reference) are then digitized

    and further processed by digital filters, line locking, normalization and calibration

    procedures [22]. The reference beam goes through a reference cell, which provides a

    high signal-to-noise ratio signal from the spectral feature under investigation. This

    channel is used for line locking and online drift correction. A line locking proceduremonitors the deviation of the signal position from a given set-point and decides

    whether a change in temperature or current has to be made to compensate for drifts.

    Fig. 4. (a) Setup of a mid-infrared (7.8mm) high-frequency modulation spectrometer with a sample and a

    reference cell, high-bandwidth HgCdTe detectors and subsequent phase-sensitive detection electronics, (b)

    optical layout of the system with a small volume (0.3 l) Herriott cell, (c) photo of the fast chemical sensor

    for eddy correlation trace gas flux measurements during a field campaign in Italy [14], (d) typical modemap of a lead-salt diode laser, (e) time series data of ambient methane concentrations with 10 Hz time

    resolution to calculate the (f) methane flux from rice paddy fields over several days. Each point is based

    upon 18,000 individual concentration measurements as shown in (e).

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    In order to compensate for fast and small fluctuations the signals are online shifted

    prior to signal averaging. These corrected signals are then fed into a digital filter

    routine which removes the background and references the signal to a previously

    stored calibration signal. All algorithms and procedures were implemented in a real-time parallel multi-processor system. The optical layout together with the external

    control units of the system based on the detection scheme described above is shown

    in Fig. 4b/c. For typical line strengths an ambient concentration of 1 ppbv produces

    an absorption of only 1 part in 107 over a 10 cm path length. Conventional

    absorption spectroscopy would not be able to measure such small absorptions.

    TDLAS overcomes this problem by using a (White or Herriott) multi-pass cell with

    effective path lengths of 100 m or more. All optomechanical components of the

    spectrometer are mounted on a 50 cm 90 cm optical breadboard. The lead-salt

    diode laser is mounted on a cold head within an LN2 dewar (Laser Photonics, Inc.,

    Analytics Division, Andover, MA, Model L5736 Laser Dewar). The diverging laser

    beam is collimated to a nearly parallel beam (1) by an off-axis parabola (OAP) and

    passes through the beam steering optics, which focuses the beam at the center of a

    commercial astigmatic Herriott cell (New Focus, Inc., Santa Clara, CA, Model 5611

    Multipass cell) with a total path length of 18 m. This cell has a very small internal

    volume of 0.3 l and is especially designed for applications requiring high time

    resolution. The outcoming thin and nearly parallel beam (3) is then focused onto a

    broadband HgCdTe measurement detector using a BaF2 planoconvex lens. The

    reflex of the cell inlet window is used as reference (2) after passing a small cell

    containing pure methane gas. This reference beam is used, on the one hand, for thereliable identification of the absorption features of the trace gas of interest, and, on

    the other hand, for the active stabilization (line locking) of the spectrometer. A

    visible (680 nm) diode laser is used to align the system. The beam splitter, which sets

    the alignment beam onto the main light path, is removed during the measurement. A

    rotary vacuum pump (Leybold AG, K .oln, Germany, Model SOGEVAC SV 65)

    provides the gas flow of about 18 slm through the Herriott cell at a pressure of about

    50 hPa. A dust filter is mounted at the inlet point of the measurement head to protect

    the gas system and especially the mirrors of the Herriott cell from pollution. A newly

    developed calibration system allowed programmed sequences of measurements of

    background signals (N2), calibration gas and ambient air. The calibration system isbased on a dilution system and high-concentration calibration gas from steel

    cylinders is diluted to ambient concentrations.

    The key element of the fast chemical sensor is the laser diode. In the lower part of

    Fig. 1 the absorption spectrum of methane is plotted together with atmospheric

    water absorption versus wavelength. The near-IR absorption consists of overtone or

    combination bands that are typically one to several orders of magnitude weaker than

    the IR-fundamental band. Antimonide lasers [7] can be used for the detection of CH4at 3.26mm (n3) and for the 7.8 mm (n4) spectral region lead-salt diode lasers are the

    optimum choice, as they cover the IR fundamental bands with strong absorption for

    the most atmospheric trace gases. In trace gas monitoring applications, lead-saltlaser instruments have routinely achieved parts-per-billion detection levels of a

    number of important molecular species. When starting to select a laser, the first task

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    is to select from mode maps a combination of base temperature and drive current at

    which the laser produces a strong, preferably single-mode emission, tuned to the

    absorption line being monitored. After investigation of several antimonide and lead-

    salt diode lasers, the lead-salt device with the characteristics shown in Fig. 4d hasbeen selected. For injection currents between 400 and 600 mA at temperatures

    ranging from 85 to 95 K single-mode operation with an average power level of

    200mW was ensured and isolated methane absorption lines could be reproducibly

    selected for the measurements even after repetitive thermal cycling, which was an

    important criterion for the planned field measurements.

    With this spectrometer ambient methane concentrations around 2 ppm can be

    detected with a precision of about 1% at a 10 Hz repetition rate and a typical data set

    of 18,000 individual concentration values is shown in Fig 4e. The data have been

    collected during about half an hour of sampling at 10 Hz. Each concentration value

    has been obtained by averaging individual spectra followed by a background

    correction. Such fast response measurements of state variables generate time series of

    data that can be statistically analyzed. As a result a set of flux data has been

    obtained, which is shown in Fig 4f. Each data point shown represents a 30 min

    average obtained from time series data as shown in Fig. 4e. From an intercompar-

    ison of these data with several other independent measurements based on gas

    chromatography it was found that there is a bias of up to 70% between different flux

    measurement methods [14]. This finding is important for atmospheric chemistry

    research in the context of greenhouse gases. Such simultaneously fast and highly

    sensitive measurements would not be possible with near-infrared systems due to thelack of sensitivity and the results shown here demonstrate that tunable diode laser

    absorption spectroscopy can be a valuable tool for quality assurance and quality

    control.

    6. Conclusion

    The features of diode laser spectroscopy rendering it such a valuable technique for

    gas analysis are given below. It is specific and as a high resolution spectroscopic

    technique it is virtually immune to interference by other speciesFa problem thatplagues most competing methods. This ability to provide unambiguous measure-

    ments leads to the use of TDLAS as a reference technique against which other

    methods are often compared. It is a technique universally applicable to all smaller

    infrared active molecules and the same instrument can easily be converted from one

    species to another by changing the laser and calibration gases. The time resolution of

    TDLAS measurements can be traded off against sensitivity and this allows very fast

    measurements with millisecond time resolution. In order to improve sensitivity

    various types of modulation spectroscopy have been employed in which the diode

    laser wavelength is modulated while being scanned across an absorption line. These

    modulation techniques allow absorption as low as 1 part in 106 to be measuredwithin a 1 Hz bandwidth. In combination with optical multi-pass cells, this is

    equivalent to detection limits of around 20 pptv for the most strongly absorbing

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    species and better than 1 ppbv for almost all species of interest [1]. TDLAS has made

    the transition from a technique mainly of interest to instrument developers into one

    which produces results of real value to trace gas analysis and atmospheric chemistry

    studies. However, it has yet to become an instrument suited to routine use by non-expert operators, mainly due to the complex and sometimes unreproducible behavior

    of the lasers. Further laser development is underway to remedy this and

    semiconductor lasers are available meanwhile from the visible to the mid-infrared

    and hopefully the spectral coverage is continuously increasing. Strong effort is

    underway to further improve quantum cascade lasers as an alternative source of

    infrared tunable radiation. Anyway, the near- and mid-infrared spectral regions will

    provide complementary systems. For a certain limited number of species, where

    ultrahigh sensitivity is not required, the near-infrared systems will provide

    advantages of size, simplicity and cost. For other species requiring a more universal

    and sensitive system, the mid-infrared diodes will continue to provide a superior and

    highly specific measurement device.

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