The European Space Agency (ESA), in collaboration with the European Commission (EC) and EUMETSAT, is developing a space-borne observing system for quantification of anthropogenic carbon dioxide (CO2) emissions. Forming part of the EC's Copernicus programme, the CO2 monitoring (CO2M) mission will be implemented as a constellation of identical satellites, to be operated over a period > 7 years and measuring CO2 concentration in terms of column-averaged mole fraction (denoted as XCO2). Each satellite will continuously image XCO2 along the satellite track on the sun-illuminated part of the orbit, with a swath width of >250 km. Observations will be provided at a spatial resolution < 2 x 2 km2 near the swath center, with high precision (<0.7 ppm) and accuracy (bias <0.5 ppm). To this end, the payload comprises a suite of instruments addressing the various aspects of the challenging observation requirements: A push-broom imaging spectrometer will perform co-located measurements of top-of-atmosphere radiances in the Near Infrared (NIR) and Short-Wave Infrared (SWIR) at high to moderate spectral resolution (NIR: 747-773nm@0.1nm, SWIR-1: 1595-1675nm@0.3nm, SWIR-2: 1990-2095nm@0.35nm). These observations are complemented by measurements in the visible spectral range (405-490 nm@0.6nm), providing vertical column measurements of nitrogen dioxide (NO2) that serve as a tracer to assist the detection of fossil-fuel emission plumes (e.g. from coal-fired power plants and cities). High quality retrievals of XCO2 will be ensured even over polluted industrial regions, thanks to co-located measurements of aerosols performed by a Multiple-Angle Polarimeter (MAP). Finally, measurements of a three-band Cloud Imager, co-registered with the CO2 observations, will provide the required cloud-flagging capacity at sub-sample level (<200m resolution).
The presentation will review the results of the Phase A/B1 instrument studies carried out in 2018-2019, including technology pre-development activities, and highlight the identified engineering challenges. The preliminary design of the CO2M mission’s instruments at the beginning of the implementation phase will be presented, along with an outlook on the development activities under the Phase B2CD programme.
As part of the European Copernicus Programme, the European Commission (EC) and the European Space Agency (ESA) together with the support of Eumetsat and the European Centre for Medium-Range Weather Forecasts (ECMWF) are initiating the development of operational satellites for measurements of anthropogenic carbon dioxide (CO2) emissions. The CO2 Monitoring (CO2M) mission shall provide atmospheric CO2 measurements at 4 km2 spatial resolution and a precision and systematic error better than 0.7 ppm and 0.5 ppm respectively in column-average dry-air mole fractions of CO2 (XCO2). The demanding requirements necessitate a payload composed of several instruments, which simultaneously perform co-located measurements. The main CO2 instrument is a 250 km swath pushbroom imaging spectrometer allowing to retrieve XCO2 from reflectance measurements in the Near-Infrared (747-773 nm) and Short-Wave Infrared spectral regions (1590-1675 nm and 1990-2095 nm). The observations for CO2 concentration will be complemented by measurements of nitrogen dioxide (NO2) columns over the same area. The NO2 measurements from the visible region (405-490 nm) will serve as a tracer for plumes of CO2 emission resulting from high temperature combustion, which will facilitate plume identification and mapping from (fossil fuel) power plants and large cities. The third component of the payload is a multiple-angle polarimeter, performing high-precision measurements of aerosol (and cloud) properties. Its measurements of polarized radiance under various observation angles will allow a precise light path correction. The resulting improved knowledge of the effective optical path due to scattering will reduce XCO2 bias error. Retrievals will be successful not only under clear sky conditions, but also under moderate aerosols loading and hence significantly increase the yield of useful XCO2 retrievals. The strong sensitivity of the XCO2 retrieval to cloud contamination calls also for a cloud-imager capable of detecting small tropospheric clouds and cirrus cover with an accuracy of 1% to 5% and with a sampling better than 400 m.
This paper, “The ENVISAT Michelson interferometar for passive atmospheric sounding: MIPAS," was presented as part of International Conference on Space Optics—ICSO 1997, held in Toulouse, France.
A low-noise 625-650 GHz receiver has been developed for trace gas measurements in the stratosphere. The instrument isdesigned for single-sideband operation allowing the detection of a variety of weak emission lines in both receiver sidebands.During several measurement campaigns over northern Europe, in the winters 1991/92 and 1992/93, the radiometer wasoperated on board the research aircraft FALCON. We report on receiver performance and present recent results of the flightexperiments.
As one of three ENVISAT instruments dedicated for atmospheric chemistry research, the Michelson Interferometer for Passive Atmospheric Sounding (MIPAS), a high-resolution Fourier Transform Infrared (FTIR) limb sounding spectrometer, will measure the Earth's limb emission in the infrared range (685 - 2410 cm-1, 14.6 - 4.15 micrometers ) on a global scale over a period of several years. The systematic processing of MIPAS scene and calibration data up to fully calibrated, geo-located limb radiance data and vertical profiles of atomospheric pressure, temperature and volume- mixing-ratios (VMR) of several atmospheric species requires a stable data acquisition and ground processing scenario and a number of calibration and characterization activities prior and after launch. After completion of the Flight Model FM test campaign and subsequent integration and test on the ENVISAT platform, MIPAS is now ready for launch by an ARIANE-5 launcher into an 800 km polar orbit. This paper gives an overview of the MIPAS instrument design, recalls the performance as measured in the instrument ground test campaigns and presents the preparations for the commissioning phase, comprising of an initial switch-on and data acquisition phase (SODAP) and a subsequent calibration/validation (CAL/VAL) phase preparing MIPAS for routine operation.
Recent progress in the development of submillimeter-wave instrumentation has provided access to a new spectral range (v = 625-655 GHz) to study upper atmospheric chemistry. A number of strong emission features, in particular of HCl, ClO and O3 have been measured in this frequency band with the SUMAS (Submillimeter-wave Atmospheric Sounder) experiment. The instrument has been operated successfully during the European Arctic Stratospheric Ozone Experiment (EASOE), in the period December 1991 to March 1992. We give a description of the SUMAS experiment and report on fast results obtained during EASOE.
A heterodyne receiver has been developed for operation in the frequency range 625-650 GHz. The goal of the ongoing project is to provide an effective tool to study upper atmospheric trace gases. The receiver is designed to operate on the research aircraft FALCON at flight altitudes of 10-12 km. Receiver performance and tuning capability were tested during a first flight campaign in April '91, with measurements of stratospheric ozone (647.8 GHz) and HCl (625.9 GHz).
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