We report results of initial space mission simulation studies for a laser-based, atmospheric CO2 sounder, which are based on real-time carbon cycle process modelling and data analysis. The mission concept corresponds to the Active Sensing of CO2 Emissions over Nights, Days and Seasons (ASCENDS) recommended by the US National Academy of Sciences’ Decadal Survey. As a pre-requisite for meaningful quantitative evaluation, we employ a CO2 model that has representative spatial and temporal gradients across a wide range of scales. In addition, a relatively complete description of the atmospheric and surface state is obtained from meteorological data assimilation and satellite measurements. We use radiative transfer calculations, an instrument model with representative errors and a simple retrieval approach to quantify errors in ‘measured’ CO2 distributions, which are a function of mission and instrument design specifications along with the atmospheric/surface state. Uncertainty estimates based on the current instrument design point indicate that a CO2 laser sounder can provide data consistent with ASCENDS requirements and will significantly enhance our ability to address carbon cycle science questions. Test of a dawn/dusk orbit deployment, however, shows that diurnal differences in CO2 column abundance, indicative of plant photosynthesis and respiration fluxes, will be difficult to detect.
Carbon dioxide (CO2) is the largest known anthropogenic forcing of climate change, yet substantial uncertainty is attached to the current atmospheric CO2 budget. Global, decadal budgets infer a large residual sink for atmospheric CO2 with attached uncertainty of 50–100% or more (IPCC, 2007; SOCCR, 2007). Several lines of evidence suggest that the Northern Hemisphere terrestrial biosphere is responsible, but the magnitude, location and mechanisms producing the sink are not well determined (Tans et al., 1990; Bousquet et al., 2000; Stephens et al., 2007). Furthermore, interannual variability in the increase of atmospheric CO2, and hence variation in the terrestrial sink (and to a lesser extent ocean), is large, but the forcing/response mechanisms and connection to decadal processes are not quantitatively resolved (Langenfelds et al., 2002; Nemani et al., 2003; Baker et al., 2006). As a result, carbon–climate interaction is among the leading sources of uncertainty in prediction of future climate (Cox et al., 2000; Dufresne et al., 2002, Friedlingstein et al., 2006). To a large extent, our ability to quantify CO2 sources and sinks using diagnostic models is hampered by sparse data limitations (Gurney et al., 2002).
New global remote sensing data from satellites hold great promise to reduce CO2 source/sink uncertainties (e.g. Rayner and O’Brien, 2001). The CO2 measurement precision and accuracy requirements, however, are unprecedented for atmospheric constituents from space. High precision, dedicated measurements of CO2 from space are just now becoming available from the Greenhouse gases Observing SATellite (GOSAT aka IBUKI) (Yokota et al., 2004). GOSAT, and those planned from the Orbiting Carbon Observatory (OCO) (Crisp et al., 2004), uses passive spectroscopy of reflected near-infrared sunlight to retrieve total column CO2 abundances. Passive instruments such as these, however, have inherent sampling limitations related to sun angle, surface reflectance and cloud cover (Miller et al., 2007; Chevallier et al., 2009). In addition, potential errors resulting from uncertainty in the impact of cloud and aerosol scattering can be significant (Dufour and Breon, 2003; Mao and Kawa, 2004).
Many of the shortcomings of passive CO2 detection can be overcome with active CO2 lidar measurements. For this reason, the US National Academy of Sciences Decadal Survey of Earth Science and Applications from Space recommended the Active Sensing of CO2 Emissions over Nights, Days and Seasons (ASCENDS) mission for NASA launch in about 2016 (NRC, 2007). The key characteristics of ASCENDS would be highly precise global CO2 measurements without seasonal, latitudinal or diurnal bias. The target precision for measuring CO2 is 0.5% at 100–200 km spatial scales over land and ocean, respectively, leading to surface flux quantification on 1° grids at weekly time resolution. Analysis of possible lidar techniques and performance indicates that such sensors are feasible (Menzies and Tratt, 2003; Ehret et al., 2008). Both ground-based and airborne CO2 measuring lidar have been developed and demonstrated (see Dobbs et al., 2002; Koch et al., 2004; Gibert et al., 2006; Abshire et al., 2007, 2009; Kameyama et al., 2009).
In this paper, we present a modelling and data analysis framework developed to test the ability of a prospective lidar mission to measure known (modelled) atmospheric CO2 distributions, to calculate the uncertainties associated with the measurements and to examine the sensitivity of the ‘measured’ CO2 distributions and errors to varying environmental, mission and instrument design parameters. Figure 1 shows a schematic of the mission simulation process. Our approach is to constrain the simulation as closely as possible to real-world conditions using analysed meteorological fields, a model CO2 atmosphere that represents observed gradients across a wide range of spatial/temporal scales, and collocated, contemporaneous observations of key environmental state variables. Because the CO2 fluxes and transport are driven by real-time analysed weather fields, meteorologically driven covariances (e.g. synoptic weather–cloudiness–vegetation flux–CO2 transport) and attendant potential biases are explicitly included in the simulations. The methodology is generally applicable to other measurement approaches including passive sensors.
The instrument radiance detection errors are derived from radiative transfer calculations and an instrument model that has been developed for the ASCENDS CO2 lidar (Abshire et al., 2007). We use the resulting pseudo-data fields to estimate the performance of the current instrument design point in measuring global column CO2 and to explore how this performance scales with several instrument and mission design options. We also use the pseudo data to address questions of how best to aggregate data to minimize uncertainties and maximize information content for carbon cycle science applications including a dawn/dusk versus midday/midnight orbit. Here, we use forward simulations to test the sensitivity of the inferred CO2 distributions to design parameters for the CO2 sounder concept. In the future, we plan to use an inverse model to evaluate the impacts on inferring surface sources and sinks of CO2 (e.g. Rayner et al., 2002).
2. CO2 flux and transport modelling
The CO2 fields used for the simulation are taken from an updated version of the atmospheric flux and transport modelling of Kawa et al. (2004). Real-time, analysed meteorological fields from the Goddard Global Modelling and Assimilation Office, version GEOS-4, are used to drive both the biospheric flux and CO2 transport models. Monthly global biosphere fluxes at 1° × 1° are produced from the Carnegie-Ames-Stanford Approach (CASA) model using mean GEOS-4 meteorology and monthly Normalized Difference Vegetation Index (NDVI) data (Tucker et al., 2005). Three-hourly net ecosystem exchange and respiration are generated from the monthly values using 3-h GEOS-4 radiation and temperature in the method of Olsen and Randerson (2004). Biomass burning from GFED2 (van der Werf et al., 2006) is included in the CASA monthly fluxes. Fossil fuel and ocean fluxes are adopted from TransCom-C (Law et al., 2008). The transport model grid used here is 1°× 1.25°× 28 levels with output hourly. The model CO2 output has been extensively compared to in situ and remote sensing observations at a wide variety of sites. In most cases, the model simulates diurnal to synoptic to seasonal variability with a high degree of fidelity (Kawa et al., 2004; Bian et al., 2006; Law et al., 2008; Parazoo et al., 2008).
3. Orbit sampling
We use CALIPSO data (Winker et al., 2007) as the model for the CO2 laser sounder orbital sampling. CALIPSO travels in the so-called ‘A-train’ orbit, which is a 705-km sun-synchronous polar orbit with an equator-crossing time of about 1:30 a.m./p.m. local solar time, and a 16-day repeat cycle. The orbit inclination of 98.2° provides global coverage between 82°N and 82°S. The 5-km CALIPSO orbit data are sampled according to the nominal averaging time of the CO2 laser sounder, 10 s in this case. This produces samples approximately every 70 km along the orbit, which is a reasonable match to the resolution of the global CO2 model. Model CO2 profiles at the nearest output time are interpolated to the sample locations along with temperature and water vapour from the assimilation data for input to the radiative transfer calculations.
Surface reflectivity over land is interpolated from MODIS (Terra + Aqua) 5-km, 16-d composite nadir BRDF-adjusted reflectance data at 1.64 μm (band 6), which are available every 8 days (Schaaf et al., 2002). Recent analysis of POLDER, MODIS and expected lidar ‘hot spot’ reflectivity (Disney et al., 2009) suggests that the 1.64-μm nadir reflectance product should be reasonably accurate for the laser wavelengths (1572 nm) used here; a decrease in reflectance of 15–20% in going from 1.64 to 1.57 μm is compensated for by an enhancement factor of similar magnitude in viewing the nadir hot spot within 2°. Over ocean, nadir glint reflectance is calculated from GEOS-4 10-m wind speeds (Lancaster et al., 2005). Figure 2 shows the global surface reflectance for 2006-07-26 (using the MODIS composite from 2006-07-28 over land) and that interpolated to the orbit track for the day. Because the laser return signal is inversely proportional to reflectivity, the measurement uncertainty depends strongly on this variable, which varies widely around the globe (Fig. 2b). Reflectivity at these wavelengths is generally lower over ice and water than land, but the difference for the laser sounder is not as large as for passive sensors since the lidar continually views the glint point at nadir.
Extinction of the laser signal by clouds and aerosols is derived from CALIPSO measured optical depths. We use the CALIPSO level-2, version 2.01 cloud and aerosol optical depth profile products, which are reported every 5-km along track (see http://eosweb.larc.nasa.gov/PRODOCS/calipso/Quality_Summaries/CALIOP_L2LayerProducts_2.01.html). Although this is a beta CALIPSO product with known large uncertainties, we feel its use is justified because we only use the data at relatively low optical depths where the retrieval is best constrained, and because the data closely represent the cloud and aerosol distributions that the CO2 laser would encounter. Cloud optical depths are reported for the 532 nm laser only presuming that cloud extinction is largely independent of wavelength. Aerosol optical depths are reported at 532 and 1064 nm. We use the 1064 nm product for completeness, but for our application the contribution of aerosol to the total attenuation is nearly negligible. Up to 10 layer optical depths are reported for each profile. We simply sum them all in the vertical to obtain a total cloud+aerosol optical depth (τc). This method underestimates actual optical depth in opaque clouds, but we only use the data in thin cloud/aerosol cases. Profile samples with τc greater than 1.0 are masked out in this analysis. The cut-off value of τc= 1.0 was chosen as a qualitative compromise between minimizing the random error produced at high optical depth (low SNR) and maximizing the number of accepted samples. We examined use of a cut-off from 0.1 to 1.6 and selected 1.0 for the optimum ratio of sample number to SNR. This number will be optimized for the space instrument depending on actual performance. We decided to sample the CALIPSO 5-km fields rather than average along-track to represent optical depth for our 10-s (70-km) CO2 sample profiles to retain the full probability distribution (PDF) of total optical depth. The τc data are highly variable so along-track averaging narrows the PDF (fewer high and low values), which results in fewer accepted samples at a given τc cutoff and thus greater overall CO2 measurement uncertainty. We do not, however, expect the CO2 space instrument to operate in a simple time averaging mode. Cloud-clearing will likely be done at a sample frequency greater than 1 Hz (roughly equivalent to the 5-km CALIPSO granule), producing a conditionally sampled average measurement with optical depth significantly less than the 10-s average.
For the dawn/dusk orbit test shown below, we shift the CALIPSO orbit points in time to a 0600/1800 hours equator crossing and sample the CO2 and meteorological fields accordingly. CALIPSO cloud and aerosol fields are used as measured. Note also that the baseline radiance error calculations below are done for a 450-km orbit height, which is not fully consistent with the CALIPSO track, but this approximation will not significantly affect the sensitivity and uncertainty results.
4. Radiative transfer
For each orbit sample point, spectral atmospheric transmission for the laser target CO2 line is calculated from the model sampled profiles (P, T, CO2, H2O) using the Line-By-Line Radiative Transfer Model (Clough et al., 1992; Clough and Iacono, 1995) and the HIgh-resolution TRANsmission molecular absorption (HITRAN) database 2008 version (Rothman et al., 2009). The measured cloud and aerosol optical depths are not explicitly included in the transmission calculations, but the transmission at all wavelengths in the CO2 band centred at 1575 nm is diminished by a factor of EXP(-τc) (Fig. 3a). As stated earlier, only profiles with total cloud and aerosol optical depth less than 1.0 are retained for further analysis. In the test cases for July and December, 2006, this results in about 37–40% of the profiles being used. Retrievals from cloud top reflection may be possible in some cases, but we neglect those opportunities for now. Most variability in Fig. 3(a) results from cloud attenuation; aerosol optical depths are relatively small. Although cloud optical depths will in general be somewhat wavelength dependent, that difference between the CO2 laser and CALIPSO wavelengths is expected to be about 30% (Warren, 1984), which is comparable to the overall uncertainty in measured τc.
5. Instrument and error model
The measurement radiance error model is based on the CO2 laser sounder approach developed at NASA Goddard Space Flight Center (GSFC) for ASCENDS (Abshire at al., 2007). The technique is integrated path differential absorption laser spectroscopy. The space instrument concept uses several tunable fibre laser transmitters for simultaneous measurement of the absorption from a CO2 line in the 1575 nm band, O2 extinction in the oxygen A-band, and surface height and aerosol backscatter in the same path. One tunable laser is stepped across a single line for the CO2 column measurement, whereas another laser is stepped across a pair of lines near 765 nm for the O2 measurement (Stephen et al., 2007). The instrument directs the narrow, co-aligned laser beams toward nadir, and measures the energy of the laser echoes reflected from land and water surfaces. Narrow-linewidth lasers are stepped across the selected bands at a frequency of ∼8 kHz. The receiver uses a 1.5-m-diameter telescope and photon counting detectors (Table 1). The detected signal includes background light and laser echoes from the surface along with scattering from any clouds or aerosols in the path. After suitable averaging the gas extinction and column densities for CO2 and O2 are estimated via differential absorption lidar (DIAL) techniques.
Table 1. Lidar instrument model specifications
Orbital altitude (km)
Laser peak power (W)
Laser pulse width (μs)
Laser pulse rate (each wavelength) (Hz)
CO2 line centre wavelength (nm)
Receiver telescope diameter (m)
Telescope and receiver transmission
Receiver optical bandwidth (nm)
Detector photon counting efficiency (%)
Detector dark count rate (Hz)
5 × 105
Measurement integration time (s)
The CO2 sounder approach uses pulsed lasers, a photon counting receiver, and time gating in the receiver to time (height) resolve the laser backscatter profile (Table 1). This allows signal processing to isolate the arrival time and energy in the laser return from the Earth's surface, and to exclude laser photons scattered from clouds and aerosols that generally arrive earlier. Hence, the technique allows isolating the full column CO2 measurement from potential bias errors caused by atmospheric scattering, which is major advantage of this technique. Time gating centred around the ground echo pulse also substantially reduces solar background noise. Recent airborne experiments show that with 1-μs transmitter pulses, the height of the laser reflecting layers, and hence the length of atmospheric path, can be determined to about 4 m.
Table 1 lists key instrument design parameters used to calculate the laser radiance random measurement errors. The lidar configuration and error model are similar to that evaluated by Ehret et al. (2008), and the sensitivities to atmospheric and instrument variables (e.g. telescope size, transmitter energy, detector efficiency) are generally the same. For a given instrument design the returned pulse power, and hence signal-to-noise ratio (SNR), depends most strongly on the atmospheric transmission and surface reflectivity. These values are drawn from the model samples, measurements and radiative transfer calculations as discussed earlier. The contribution of solar irradiance background noise is computed from the solar zenith angle at the sample point and the instrument optical parameters. The random relative error in the on-line/off-line radiance ratio (more below) for each profile of one test day is shown in Fig. 3(b). Random error varies by more than a factor of 10 among profiles around the globe depending on the atmospheric state. The root mean square (RMS) error is 0.0024, which corresponds to about 0.9 ppmv on a global background CO2 of 375 ppmv. Calculations can be done at this level for any variety of instrument/mission specifications (as listed in Table 1) to determine the global sensitivity of the random error to these design choices. In general, the global mean error calculated in this way for a given instrument design is substantially different (larger) than that calculated using a global mean reflectance and/or uniform transmission estimate.
An additional error source of ±2 mbar (uncorrelated with radiance error) is imposed for the surface pressure uncertainty in converting column CO2 density to column average mixing ratio (<CO2>). It is expected that surface pressure data will be available with this uncertainty either from the collocated laser measurements of O2 column or from weather data assimilation. Additional errors induced by uncertainty in atmospheric variables (T, H2O, aerosol) are expected to be small relative to a surface pressure error of this magnitude (Ehret et al., 2008). We include a 0.05%‘representation error’ globally to account for the ability of the narrow (∼70 m wide) laser sample stripe to measure mean <CO2> in a grid sample volume of about (70 km)2 (Miller et al., 2007; Corbin et al., 2008). Another 0.1% uncorrelated error is introduced over land surfaces to account for noise produced by changes in surface reflectance and non-simultaneity of the laser footprints at the pulsed laser sample wavelengths (Amediek et al., 2009) along with other pointing/timing errors (Ehret et al., 2008). We have not included spectroscopy, a priori and retrieval fitting, or other systematic instrument errors at this time.
6. Simplified retrieval algorithm
For this work, we use a notional DIAL retrieval algorithm, which assumes that the sampled CO2 column density is proportional to the logarithm of the on-line/off-line transmission ratio at selected wavelength points. The off-line wavelength is chosen to be where the sample-average absorption in the band is the minimum (Fig. 3a, red symbol). For on-line, we use the wavelength at which the average absorption is 50% (Fig. 3a, green symbol). The CO2 error is then proportional to the relative uncertainty in the log of the on-line/off-line radiance ratio measurement, which is a function of the SNR at these wavelengths (e.g. Ehret et al., 2008). In the two-wavelength case, the relative error is the minimum for 50% absorption. In practice, an optimization algorithm using laser absorption at several wavelengths along the absorption line can be used to retrieve CO2 column with varying vertical weighting functions. The current GSFC design allows for up to eight sample wavelengths distributed across the line. Measurement using multiple wavelengths also allows for reducing possible instrumental effects and more tightly controlling potential bias errors. The simple retrieval assumption used here can be viewed as a minimum-capability instrument case. The method is, however, quantitative for estimating the relative CO2 measurement uncertainty and its sensitivity to changing conditions and instrument design parameters.
A uniform vertical weighting function is used to extract total column CO2 from the model. Again, depending on the lidar design, a CO2 vertical weighting function with multiple degrees of freedom will likely be possible with multiple laser wavelengths. This will result in improved sensitivity to variations of CO2 in the lower atmosphere, which occur in response to surface sources and sinks—the ultimate objective of ASCENDS. For the cases studied here, we use error in total column as a conservative metric for the measurement error. Note that different weighting functions are simple to apply in the modelling framework and these can be tested in future studies.
7. Design point data error estimate
Figure 4(a) shows the full model <CO2> field at midday on 2006-07-26. Gradients of several ppmv/1000 km are seen in the northern hemisphere and tropics resulting from weather systems that transport air masses along and across surface flux gradients. In particular, low CO2 downwind of regions with large vegetation uptake in summer is seen in the North. High CO2 from fossil fuel emission is associated with population centres as well as biomass burning in the tropics. The sampled, cloud-screened, error-containing ‘data’ representation over the entire day is seen in Fig. 4(b). Comparison of the pseudo data with the original sampled values (Fig. 4c) shows errors as large as several ppmv locally, but the global RMS error is 1.21 ppmv. RMS errors for other days in July range from 1.12 to 1.30 ppmv. Sample days from December 2006 are also in the same range. This demonstrates that a space instrument designed to the specifications of Table 1 would be able to achieve the performance requirements of ASCENDS assuming no other significant unmodelled errors. Global <CO2> measurements at this level of precision are expected to significantly reduce the uncertainty in inferred surface fluxes of CO2 (Rayner et al., 2002). Note also that, by way of consistency check, the magnitude of the <CO2> error is close to the root sum of squares of the errors enumerated in Section 5, which is to be expected for uncorrelated error sources.
8. Pseudo-data examples
Depending on the application, it is likely that some averaging or compositing of the data would be done to reduce random errors. Using example pseudodata we can begin to address questions of how to optimally aggregate the data for maximum information content and minimum error. Figure 5 shows the sampled pseudo data for 2006-07-26 averaged into 10°× 10° latitude–longitude regions and the difference from the ‘true’ average in space and time for that day. Although there are many grid elements without sampling, the total RMS error is reduced globally to about 0.7 ppmv. The sample RMS error alone (i.e. ‘perfect instrument’ averages constructed by sampling and averaging the original field without any measurement error) is about 0.4 ppmv. Slightly smaller sample errors are found in Northern winter (December, not shown) cases (∼0.3 ppmv) when the global <CO2> gradients are smaller.
All ‘measured’ samples from a 16-d orbit repeat cycle and the corresponding 16-d average model <CO2> field are shown in Fig. 6. Comparing the averaged full field to the instantaneous in Fig. 4, we see many details are smoothed by averaging the evolving field. The ‘measured’ field now, however, presents a fairly complete spatial representation. Spatial averaging of the 16-d accumulated data on varying grids is shown in Fig. 7. The total errors continue to decline with increasing averaging scale, although regional details of the <CO2> distribution are averaged out. Errors (‘true’—‘measured’) are largest where they might be expected: in regions of large gradients that are evolving in time, for example Northern mid to high latitudes. The best way to use the ‘data’ will depend on the application. For example, some inverse model methods are limited to coarse observation grids by computational constraints, whereas other methods may be able to ingest individual soundings over several weeks or more. The pseudo data and errors that we have generated will be available for further analysis.
As a further test of data aggregation and sampling methods, we used a dawn/dusk orbit sampling rather than the near-midday/midnight orbit model of CALIPSO. The ‘data’ over the 16-d repeat cycle at approximately 0600 and 1800 local solar time are shown in Figs 8(a) and (b) using the same instrument model as earlier. Note that the individual sample errors are lower here than for the daytime samples above because the solar background radiance is small near dawn/dusk. The aggregate 16-d, 5-degree averaged difference between the dusk and dawn <CO2> fields is shown in Fig. 8(c). A 0600/1800 local time equator-crossing orbit was chosen because globally the maximum average 12-h <CO2> difference in the model occurs for these times. The full model (1° × 1.25°) dusk–dawn (1800–0600 local solar time) difference averaged over 16 days (not shown) has maximum values for <CO2> of 0.5–1.5 ppmv over actively photosynthesizing vegetation, that is tropical forest in equatorial South America and Africa, and northern temperate and boreal forests in North America and Eurasia. Maximum differences are less than 1 ppmv when averaged up to 5° bins. Some semblance of this distribution can be seen in Fig. 8(c), but the errors (noise) are larger than the expected signal in most areas. The global RMS error in the ‘true’ versus ‘measured’ diurnal difference is 0.9 ppmv and the correlation coefficient (r) is about 0.3. Much of this error is due to sampling error (RMS = 0.6 ppmv) in trying to extract a diurnal difference from the relatively large, evolving synoptic <CO2> variations. Note, however, that measurements with a strong near-surface weighting function would likely improve detection of the diurnal difference more than proportionately because almost the entire signal arises from CO2 change at the vegetation canopy level.
9. Summary and future applications
Simulation studies are presented for a laser-based CO2 space mission that generally corresponds to the ASCENDS (NRC, 2007). CO2 pseudo-data distributions and uncertainties are quantified using a realistic description of the atmosphere and surface state with a representative model of the instrument capabilities. This framework provides a comprehensive test bed to examine many potential implementation options and sensitivity to environmental conditions. Most of the expected major measurement error sources are included in detail (random radiance noise, surface pressure uncertainty, representation error, ground reflectance/wavelength shift error). Some additional potential error sources such as sub-grid scale variability will be explored further and incorporated when quantified. Also, more sophisticated multi-wavelength retrieval approaches will be included when available.
The error characteristics estimated for the CO2 laser sounder's present design (i.e. orbit height, sample time, laser power, detector efficiency, etc.) indicate that such a mission can meet the ASCENDS measurement requirements and provide important new insights into carbon cycle science. Data precision on the order of 0.5% RMS appears possible with existing technologies on a single 10-s (70-km) sample basis. Random error reduction is quantified for several examples of space–time averaging.
Detecting perturbations in the diurnal balance between photosynthesis and respiration fluxes of CO2 to inform the status and health of underlying vegetation will not be readily attainable from <CO2> measurements. This measurement requirement for ASCENDS (NRC, 2007) should be revisited in comparison to a midday/midnight orbit, which is near the time of the local daily mean <CO2> over vegetation, that is sampling is unbiased diurnally with respect to the mean (cf. Rayner et al., 2002).
An important next step will be to input the pseudo data into a CO2 source/sink inversion model(s) and calculate the resulting uncertainty in regional to global surface flux estimates. Because flux results will depend on the specifics of the inverse model and methodology, perhaps several models will be used to compare between inverse applications and among a targeted set of mission options. Meanwhile, there is much that can be learned from further application of our framework with the forward model. We plan to fill out an annual cycle of pseudo data to determine measurement precisions for the global distribution of the CO2 seasonal cycle, which provides a powerful constraint on our representation of source/sink processes and their response to environmental forcing. In addition, we can quantitatively test mission, instrument and retrieval approaches for their ability to measure CO2 and address key carbon science hypotheses.
We acknowledge the support of the NASA Earth Science Technology Office's Advanced Instrument Technology and Instrument Incubator Programs, the NASA Carbon Cycle Science Program and Goddard Internal Research and Development. CALIPSO data were obtained from the NASA Langley Research Center Atmospheric Science Data Center and MODIS data were obtained from the Land Processes Distributed Active Archive Center (LP DAAC).