CarbonSat is a proposed Earth observation mission, which was selected in 2010 as one of two candidates for becoming the European Space Agency’s (ESA) eighth Earth Explorer (EE8). It is currently undergoing parallel feasibility studies (phase A) performed by two industrial consortia. CarbonSat aims at a better understanding of the natural and anthropogenic sources and sinks of the two most important anthropogenic greenhouse gases CO2 and CH4, which will contribute to a better understanding of climate feedback and forcing mechanisms. To achieve these objectives the instrument will quantify and monitor the spatial distribution of carbon dioxide (CO2) and methane (CH4). It will deliver global data sets of dry air column-averaged mixing ratios of these gases with high precision (1 - 3 ppm for CO2 and 6 - 12 ppb for CH4) and accuracy (0.5 ppm for CO2 and 5 ppb for CH4). The measurements will provide global coverage every 12 days above 40 degrees latitude at a spatial resolution of 2 x 3 km2. The retrieval products are inferred from observations of Earth radiance and solar irradiance at high to medium spectral resolution (0.1-0.55 nm) in the Near Infrared (747-773 nm) and Short Wave Infrared (1590- 1675 nm and 1925-2095 nm) spectral regions. The combination of high spatial resolution and global coverage requires a swath width larger than 180 km for three spatially co-aligned push-broom imaging spectrometers. The targeted product accuracy translates into stringent radiometric, spectral and geometric requirements for the instrument. This paper presents the system requirements derived from the demanding mission objectives and reports preliminary results of the feasibility studies. It highlights the key components of the instrument, focusing on the optical conceptual design, and addresses the identified critical performance aspects.
The Scanning Imaging Absorption spectroMeter for Atmospheric CHartographY (SCIAMACHY) is a contribution to the ENVISAT-1 satellite, which has been launched in March 2002. The SCIAMACHY instrument measures sunlight transmitted, reflected and scattered by the Earth's atmosphere or surface simultaneously from the UV to the SWIR spectral region (214 - 2380 nm) in nadir, limb, and occultation viewing geometry. SCIAMACHY allows the characterisation of the composition of the Earth atmosphere from the ground to the mesosphere. This paper gives an overview of the SCIAMACHY instrument and its in-flight detector, spectral and radiometric performance. Furthermore first results on trace gas retrieval from limb and nadir measurement mode will be summarised.
SCIAMACHY is a UV/visible/near-infrared grating spectrometer on board the European environmental satellite ENVISAT that observes the atmosphere in nadir, limb, and solar and lunar occultation viewing geometries with moderate spectral resolution (0.2-1.5 nm). At the University of Bremen a modified DOAS algorithm (WFM-DOAS) is being developed primarily for the retrieval of CH4, CO, CO2, H2O, N2O, and O2 total columns from SCIAMACHY near-infrared and visible nadir spectra. A first version of this algorithm has been implemented based on a fast look-up table approach. The algorithm and the look-up table is described along with an initial error analysis. Weighting functions and averaging kernels indicate that the SCIAMACHY near-infrared nadir measurements are highly sensitive to trace gas concentration changes even in the lowest kilometer of the atmosphere. The results presented have been obtained by applying WFM-DOAS to small spectral fitting windows focusing on CH4, CO2, CO, and O2 column retrieval and CH4 and CO2 to O2 column ratios (denoted XCH4 and XCO2, respectively). These type of data products are planned to be used within the EU research project EVERGREEN to constrain surface sources and sinks of CH4 and CO2 using inverse modeling techniques. This study discussed the first set of WFM-DOAS products generated for and to be further improved within EVERGREEN. Although no detailed validation has been performed yet we found that the retrieved columns have the right order of magnitude and show (at least qualitatively) the expected correlation of the well mixed gases CO2 and CH4 with O2 and surface topography. The standard deviation of the dry air column averaged mixing ration XCO2 within 10° latitude bands is ±10 ppmv or 2.7% (XCH4: ±50 ppbv or ±2.8%) for measurements over land (over ocean the scatter is a factor of 2-4 larger). These values have been determined from ~25% of the ground pixels of one orbit which fulfill the following requirements: (nearly) cloud free, solar zenith angle <75°, XCO2 error < 4% (XCH4 error < 6%). It has not been assessed how much of this variability can be attricuted to real column changes. The observed variability is about three times larger than expected from (single spectra) signal-to-noise considerations but might be affected by limitations of the current implementation of the retrieval algorithm (e.g., sensitivity to surface reflectivity) and calibrations issues (e.g., not yet considered ADC non-linearity correction). Especially the CO retrieval needs further study and improvement. The CO fit errors are 20-40% over land but typically significantly larger over the ocean. A clear identification of the weak CO lines is difficult as the CO fit residuals are dominated by relatively stable systematic artifacts (also observed in the CO2 and CH4 fitting windows) on the order of the weak CO absorption lines. This might be explained by the still preliminary calibration of the SCIAMACHY spectra and/or errors of the spectroscopic data.
GOMETRAN/SCIATRAN is a radiative transfer forward model developed for retrieval of atmospheric trace gas concentrations, aerosol and cloud parameters, and surface reflectance from the spectral radiance measurements of the SCIAMACHY/ENVISAT-1 and GOME/ERS-2 UV-Vis-NIR multichannel spectrometers. For radiative transfer modeling of the line absorptions of O2, H2O, CO2, CH4, N2O, and CO, tow different schemes are under development: an accurate but rather slow line-by-line (LBL) implementation and a significantly faster correlated-k (c-k) distribution scheme. The c-k scheme has been matched to the resolution of the instruments, which is channel dependent. In spectral regions free of overlapping line-absorbers the multiply scattered radiance calculated with both, the LBL and the c-k scheme, agrees within 1-2 percent. Calculations in c-k mode are a factor of 25-800 faster depending on spectral interval. Good agreement has been found with the MODTRAN/DISORT radiative transfer model. First results concerning a new method are presented indicating that overlapping line-absorbers can be modeled with similar accuracy and speed as single line-absorbers.
The atmospheric spectrometer SCIAMACHY to be launched on board ESA's Envisat satellite in 2000 will measure UV, visible and IR spectra from nadir, limb and occultation with spectral resolution between 0.2 and 1.4 nm. SCHIAMACHY's channel 8 covering the wavelength range 2265-2380 nm will allow the global determination of concentrations of methane, carbon monoxide and nitrous oxide. Sensitivity studies using the most recent values for the instrument parameters show that the minimum values for the accuracies for total vertical columns are of order 5 Dobson units (DU) for carbon monoxide, 3 DU for methane, and 6 DU for nitrous oxide, for a 1 s SCIAMACHY nadir observation. The detection of the IR spectra features novel InGaAs detectors, specially developed for the SCIAMACHY project. While providing the required sensitivity in this wavelength domain, these detectors are limited by noise levels that vary strongly from pixel to pixel. This poses special challenges to the retrieval of molecule concentrations from the measured detector signals. Ways to overcome this problem are discussed.
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