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Development of Laser, Detector, and Receiver Systems for an Atmospheric CO2 Lidar Profiling System

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Development of Laser, Detector, and Receiver Systems for an Atmospheric CO2 Lidar Profiling System Development of Laser, Detector, and Receiver Systems for an Atmospheric CO2 lidar profiling System Syed Ismail1, Grady Koch2, Nurul Abedin3, Tamer Refaat4, Manuel Rubio5, and Upendra Singh6 1,2, 3,5,6NASA Langley Research Center, Hampton, VA 23681 1757-864-2719; [email protected] 2757-864-3850; [email protected] 3757-864-4814;m.n.abedin@ nasa.gov 5757-864-2338; [email protected] 6757-864-1570;[email protected] 4Old Dominion University, Norfolk, VA 23529 4 757-218-0608; [email protected] Abstract- A ground-based Differential Absorption Lidar configuration. The detector has been characterized in the (DIAL) is being developed with the capability to laboratory and by conducting atmospheric tests at measure range-resolved and column amounts of NCAR, Boulder. The receiver uses an F2.2 all atmospheric CO2. This system is also capable of aluminum 16”diameter telescope and the system is providing high-resolution aerosol profiles and cloud designed to focus light onto a 200 micron size detector. distributions. It is being developed as part of the NASA Subsystem level integration and testing has been Earth Science Technology Office’s Instrument Incubator completed in the second year. System level testing is Program. This three year program involves the design, planned in the third year along with validation in the late development, evaluation, and fielding of a ground-based spring of 2008 that involves comparisons with ground- CO2 profiling system. At the end of a three-year based and aircraft in situ CO2 sensors. development this instrument is expected to be capable of making measurements in the lower troposphere and TABLE OF CONTENTS boundary layer where the sources and sinks of CO2 are 1. INTRODUCTION....ERROR! BOOKMARK NOT DEFINED. located. It will be a valuable tool in the validation of 2. THE CO DIAL PROFILING SYSTEM……….2 NASA Orbiting Carbon Observatory (OCO) 2 3. LASER DEVELOPMENT AND TESTING....…2 measurements of column CO and suitable for 2 4. DETECTOR SYSTEM INTEGRATION AND deployment in the North American Carbon Program ATMOSPHERIC TESTS…………………..………4 (NACP) regional intensive field campaigns. The system 5. RECEIVER SYSTEM……………………...……5 can also be used as a test-bed for the evaluation of lidar REFERENCES………………………………...……6 technologies for space-application. BIOGRPHY…………………………...…………….6 This DIAL system leverages 2-micron laser technology developed under a number of NASA programs to develop new solid-state laser technology that provides 1. INTRODUCTION high pulse energy, tunable, wavelength-stabilized, and double-pulsed lasers that are operable over pre-selected The atmospheric burden of CO2 is increasing in response temperature insensitive strong CO2 absorption lines to widespread anthropogenic combustion of fossil fuels. suitable for profiling of lower tropospheric CO2. It also Roughly half of the emitted CO2 is absorbed by the incorporates new high quantum efficiency, high gain, Earth’s oceans and terrestrial ecosystems [1]. This and relatively low noise phototransistors, and a new uptake [2] varies annually from 1 to 6 PgC yr-1. receiver/signal processor system to achieve high Understanding source/sink processes and the geographic precision DIAL measurements. patterns of carbon fluxes are primary goals of carbon cycle science. Uncertainty in predictions of the carbon Atmospheric tests of the laser have been conducted by cycle is one of the leading sources of uncertainty in operating it locked to the CO2 absorption line center, projections of future climate [3]. A double-pulsed DIAL with off-set locking in the side-line mode, and in the off- system operating in the 2.05-micron band of CO2 is line position. The reference laser is locked to center of being developed for profiling CO2 in the low-to-mid absorption line within 390 kHz. This improves the level troposphere. There are several advantages of this system of stabilization by factor of 10 compared to earlier over passive remote sensing systems including day/night operation, reduction or elimination of interference from tunable laser is configured to operate at the 2053.204 nm clouds and aerosols, and direct and straight forward CO2 absorption line and later on the laser is planned to inversion that leads to better quality data and faster operate on the more temperature in sensitive line [8] at retrievals with few assumptions. A ground-based lidar 2050.967 nm using the Ho:Tm:YLF configuration. The profiling system with ability to delineate atmospheric CO2 line will be fully characterized using a tunable high- boundary layer (ABL) CO2 from the free tropospheric resolution (New Focus Model #6335) laser diode at the CO2 is needed that can operate during day or night. CO2 Jet Propulsion Laboratory [9]. Accurate spectroscopic distributions in the troposphere are linked to transport parameters will be derived that are critical to realizing and dynamical processes in the atmosphere and are ground-based CO2 lidar detection strategy. The low- associated with near-surface sources and sinks. Annually pressure line position is known to an uncertainty less averaged, inter-hemispheric, and continental to marine than 6×10-5 cm-1 [9]. The ambient temperature line boundary layer CO2 mixing ratio differences are on the strength will be determined to 2%, the line width to 3%, order of 1 to 3 ppm [4]. Thus 0.2 ppm has long been a and the atmospheric pressure shift to 5×10-4 cm-1 using a benchmark for required instrumental precision. multispectral fitting technique. Achieving this level of precision is difficult with remote sensors. Much larger mixing ratio differences emerge, TABLE I: LIDAR PARAMETERS however, at smaller spatial and temporal scales. In many Parameters Value Unit instances exchange of ABL CO with the free 2 Pulse Energy 90 mJ troposphere takes place through convective activity and Pulse width 180 ns passage of weather fronts. Hurwitz et al. [5], describe several synoptic passages and document 10 to 20 ppm Pulse repetition rate 5 Hz, doublets mixing ratio changes that result from frontal passages. Spectrum Single frequency ….. Thouret et al. [6], have shown that there is a high On-line wavelength 2050.967 nm probability of observing more than one layered structure Off-line wavelength 2051.017 nm above the boundary layer at any time. Airborne Beam quality < 1.3 time diffraction limit ….. sampling shows that the majority of the vertical structures in CO mixing ratios are found within the Long term (one hour) < 2 MHz 2 stability lowest 5 km of the troposphere [4]. Thus, the Telescope Diameter 16 inch requirements of this DIAL system development are: 0.5% (1.5 ppm) precision for vertical differences in the Detector AlGaAsSb/InGaAsSb ….. Phototransistor 30 minute mean mixing ratio resolved every 1 km from 0.5 to 5 km above ground. Progress during the last two years in the design, 3. LASER DEVELOPMENT AND TESTING development, atmospheric testing, and performance modeling associated with the development of this DIAL Recent improvements in performance of the laser system is presented in this paper. Field evaluation of the transmitter include double-pulse operation as DIAL will be conducted in year 3 of the project in demonstrated in the past with other DIAL systems. The coordination with field observations of the North double-pulse is injection seeded with different on-off American Carbon Plan (NACP) and OCO pre-validation wavelength for each pulse of the doublet. The activities. wavelength switching is accomplished by having two injection seed lasers that can be rapidly (in under 1 μs) 2. THE CO2 DIAL PROFILING SYSTEM switched by an electro-optic device controlled by a simple logic signal. One of the seed lasers is tuned to the The DIAL system incorporates a high pulse energy, CO2 line and the second is tuned to off line. The on-line tunable, wavelength-stabilized, and double-pulsed laser laser is referenced to a CO2 absorption cell at low that operates over a pre-selected temperature insensitive pressure, and recent work has improved the performance strong CO2 absorption line in the 2.05-μm band. It of the wavelength locking to a level within 390 kHz incorporates a newly developed low noise and high gain standard deviation over hour-long time periods. This InGaAsSb/AlGaAsSb (AstroPower) infrared level of stabilization to line center reflects a factor of 10 heterojunction phototransistor (HPT) with a 200 μm improvements over our previous implementation, sensitive area diameter. It is planned to operate it in the realized by converting to an external frequency direct detection mode by taking advantage of a large 16” modulation technique rather than wavelength dithering diameter telescope, which increases the photons of the laser cavity length. An option now exists for collection at the detector by a factor of 16 over our tuning the on-line laser to the side of the line rather than previous system [7] in order to make CO2 measurements the center of the line. By using the side of the absorption above the boundary layer. The key lidar system line, the optical depth of the DIAL measurement can be parameters are given in Table 1. The Ho:Tm:LuLF tailored for optimal performance. The side line reference is made by locking one seed laser onto line center and 38 pm from line center. These results indicate ability to referencing a second laser to the center-line laser by operate the laser in the sideline mode to optimize monitoring the heterodyne beat signal between the two. performance by tuning the sideline to desired absorption. A feedback loop, with results shown in Figure. 1, has More quantitative CO2 measurements in the atmosphere been implemented to lock the side-line laser to the were made in March, 2007 in the boundary layer using center-line laser. the Ho:Tm:LuLF laser and the existing heterodyne detection system.
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