Canadian scientific instrument aboard NASA's Terra satellite
MOPITT 2000 global carbon monoxide.
MOPITT (Measurements of Pollution in the Troposphere) is an ongoing astronomical instrument aboardNASA'sTerra satellite that measures globaltropospheric carbon monoxide levels. It is part of NASA'sEarth Observing System (EOS), and combined with the otherpayload remote sensors on the Terra satellite, the spacecraft monitors the Earth's environment and climate changes. Following its construction in Canada, MOPITT was launched into Earth's orbit in 1999 and utilizes gas correlationspectroscopy to measure the presence of different gases in the troposphere. The fundamental operations occur in its optical system composed of twooptical tables holding the bulk of the apparatus. Results from the MOPITT enable scientists to better understand carbon monoxide's effects on a global scale, and various studies have been conducted based on MOPITT's measurements.[1][2][3]
TheNational Research Council Canada founded the MOPITT project following its initial proposal in 1989. After the establishment of theCanadian Space Agency (CSA), MOPITT shifted into the agency where it received financial support from the Space Science Division of CSA. It was successfully launched from theVandenberg Air Force Base on December 18, 1999, and began scientific measurements in March 2000. Before its execution, the only existing global carbon monoxide dataset was measured by the MAPS instrument aboard space shuttles. MOPITT is the first tool to measure globalconcentrations and variations in carbon monoxide. It is part of a series of five payloads on the Terra satellite that oversees global environmental changes:[1][4]
ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer)
MODIS (Moderate Resolution Imaging Spectroradiometer)
MOPITT (Measurements of Pollution in the Troposphere)[5]
Despite the initial five-year term plan, the satellite has continued to operate for over 20 years, and researchers expect all five of these instruments to maintain their functionality and transmit information and data past 2026.[5][6]
MOPITT is a nadir-sounding (vertically downward pointing) instrument that measures upwellinginfrared radiation and utilizes correlationspectroscopy (comparison ofwavelengths or absorption between a known and unknown sample) to measure concentrations of carbon monoxide. Essentially, MOPITT takes carbon monoxide as anoptical filter to measure the signal of the same gas in the troposphere. The sensor quantifiesradiance emitted and reflected from Earth through threespectral bands:
4.7 μm channels are referred to as the carbon monoxide thermal channels because the signals stem from the thermal emissions from Earth's surface and the atmosphere
The 2.3 μm channels are termed the carbon monoxide solar channel because they absorb the dominant signal from reflected sunlight
2.2 μm channels refer to the methane solar channels because reflected sunlight is the major signal, similar to the 2.3 μm channels[6]
These channels absorb different amounts of energy, leading to differences in the resulting signals that correlate to the spectral sample of carbon monoxide. To further analyze carbon monoxide levels, MOPITT adjusts the path length or gaseouspressure of the gas sample, causing the frequency of thesespectral lines to vary, which will give a difference and an average transmission. The difference specifies the gases measured, whereas the average signal indicates the overall radiation minus the initial gas measured.[2]
MOPITT's spatial resolution is 22 km horizontally and about 5 km vertically and scans Earth at a broad area of 640 km wide. The carbon monoxide measurement profiles are created through theupwelling ofthermal radiance in 4.6-μm absorption. MOPITT can view different layers of the troposphere by varying modulated cells: Pressure-modulated cells (PMCs) are used to observe upper layers while length-modulated cells (LMCs) can view lower layers of the troposphere.[7]
At the heart of MOPITT lies the optical system, which is composed of two identical "mirror imaged"optical tables that include the calibration sources, scan mirrors,choppers, LMCs, PMCs, modulators, anddewar cooler assemblies containing cold optics and thermal and solar detectors. A pair of low-vibrationStirling Cycle coolers chill the dewar. Considerable heat-emitting units like the cooler are placed intentionally on the coldplate, and other critical electronic pieces are placed near it as well. The coldplate, located under MOPITT's baseplate, provides a stable thermal environment for the instrument. It utilizescapillary action withammonia as itsworking fluid.[6][7]
In the two optical systems referred to above, eight channels measure carbon monoxide or methane. Channels one, two, three, five, six, and seven focus on carbon monoxide. The six channels for carbon monoxide vary in cell pressures from 25 to 800 mb, and their cell lengths range from 2 to 10 mm. Their centerwavelength also differs between channels, and the modulator types are either LMCs or PMCs. In contrast, channels four and eight measure methane, and their only difference is the different LMCs used. All channels operate at 300 K.[8]
Before MOPITT's release, data on carbon monoxide was limited. With MOPITT's comprehensive measurements of carbon monoxide throughout the past two decades, scientists are better equipped to predict the potential consequences of carbon monoxide pollution. Its applications include:
A better understanding of the increase inozone concentration in the troposphere allows scientists to perform interim pollution methods
^abDrummond, James R.; Bailey, Paul L.; Brasseur, Guy; Davis, Gary R.; Gille, John C.; Peskett, Guy D.; Reichle, Henry K.; Roulet, N.; Mand, Gurpreet S.; Mcconnell, Jack C. (1999-10-01).Early mission planning for the MOPITT instrument. SPIE's International Symposium on Optical Science, Engineering, and Instrumentation. Vol. 3756. pp. 396–402.Bibcode:1999SPIE.3756..396D.doi:10.1117/12.366395.