MOPITT

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MOPITT 2000 global carbon monoxide. Mopitt first year carbon monoxide.jpg
MOPITT 2000 global carbon monoxide.

MOPITT (Measurements of Pollution in the Troposphere) is an ongoing astronomical instrument aboard NASA's Terra satellite that measures global tropospheric carbon monoxide levels. It is part of NASA's Earth Observing System (EOS), and combined with the other payload 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 correlation spectroscopy to measure the presence of different gases in the troposphere. The fundamental operations occur in its optical system composed of two optical 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]

Contents

Background

The National Research Council Canada founded the MOPITT project following its initial proposal in 1989. After the establishment of the Canadian 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 the Vandenberg 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 global concentrations 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]

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]

Technology

Instrument Methodology

MOPITT is a nadir-sounding (vertically downward pointing) instrument that measures upwelling infrared radiation and utilizes correlation spectroscopy (comparison of wavelengths or absorption between a known and unknown sample) to measure concentrations of carbon monoxide. Essentially, MOPITT takes carbon monoxide as an optical filter to measure the signal of the same gas in the troposphere. The sensor quantifies radiance emitted and reflected from Earth through three spectral bands:

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 gaseous pressure of the gas sample, causing the frequency of these spectral 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 the upwelling of thermal 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]

Instrument Description

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, and dewar cooler assemblies containing cold optics and thermal and solar detectors. A pair of low-vibration Stirling 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 utilizes capillary action with ammonia as its working 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 center wavelength 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]

Applications

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:

Studies

Many studies utilizing MOPITT's data have been completed. Notable ones include:

In the year 2022 alone, more than 250 studies have used measurements from MOPITT. [6]

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References

  1. 1 2 "Measurements Of Pollution In The Troposphere (MOPITT) | Atmospheric Chemistry Observations & Modeling". www2.acom.ucar.edu. Retrieved 2023-10-24.
  2. 1 2 Thome, Kurtis. "MOPITT | Terra". terra.nasa.gov. Retrieved 2023-10-24.
  3. "Terra (satellite)", Wikipedia, 2023-09-18, retrieved 2023-10-24
  4. "ASDC | MOP03JM_8". asdc.larc.nasa.gov. Retrieved 2023-10-24.
  5. 1 2 3 SCMO, CMOS Bulletin (2019-12-21). "MOPITT - 20 Years of Measuring Atmospheric Pollution - CMOS Bulletin". CMOS BULLETIN SCMO. Retrieved 2023-10-24.
  6. 1 2 3 4 "Measurements Of Pollution In The Troposphere". mopitt.physics.utoronto.ca. Retrieved 2023-10-24.
  7. 1 2 Drummond, 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. doi:10.1117/12.366395.
  8. "Instrument Concepts | Atmospheric Chemistry Observations & Modeling". www2.acom.ucar.edu. Retrieved 2023-11-07.
  9. Agency, Canadian Space (2007-03-12). "Measuring atmospheric pollutants". Canadian Space Agency. Retrieved 2023-10-24.