As depicted above, by about 2014 the international Afternoon Constellation should include OCO-2, GCOM-W1, Aqua, CloudSat, CALIPSO, and Aura. (Glory was lost in a launch vehicle failure on March 4, 2011.) In December 2009, PARASOL began to leave the constellation; it will exit completely by 2012. The instruments on these precisely engineered satellites make almost simultaneous measurements of clouds, aerosols, atmospheric chemistry, and other elements critical to understanding Earth’s changing climate. The footprint of each of the A-Train’s instruments is shown: active instruments aboard CALIPSO/CALIOP and CloudSat/CPR are indicated with dashed lines. This illustration color-codes instrument swaths—the area of Earth’s surface, or the surface of its atmosphere, over which data is collected—based on observed wavelength ranges. Microwaves (observed by both AMSRs, AMSU-A, CPR, MLS) are represented by red-purple to deep purple colors; solar wavelengths (POLDER, OMI, OCO-2), yellow; solar and infrared wavelengths (MODIS, CERES), gray; other infrared wavelengths (IIR, AIRS, TES, HIRDLS) are represented by reds.
NASA and its international partners operate several Earth observing satellites that closely follow one after another along the same orbital “track.” This coordinated group of satellites, constituting a significant subset of NASA’s current operating major satellite missions, is called the Afternoon Constellation, or the A-Train, for short. The satellites are in a polar orbit, crossing the equator at about 1:30 p.m. local time, within seconds to minutes of each other. This allows near-simultaneous observations of a wide variety of parameters to aid the scientific community in advancing our knowledge of Earth System Science and applying this knowledge for the benefit of society. Four satellites currently fly in the A-Train: Aqua, CloudSat, CALIPSO, and Aura. GCOM-W1 and OCO-2 are scheduled to join the configuration in 2012 and 2013, respectively. Glory was lost in a launch vehicle failure on March 4, 2011.
Please use the tabbed menu above to learn more about the individual satellite missions involved with the A-Train Constellation.
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Launch Date: May 4, 2002
Launch Location: Vandenberg Air Force Base, California
Aqua is a major international Earth Science satellite mission centered at NASA. Launched on May 4, 2002, the satellite has six differrent Earth-observing instruments on board and is named for the large amount of information it collects about water in the Earth system. Aqua gathers this information from its stream of approximately 89 Gigabytes of data a day! The water variables being measured include almost all elements of the water cycle and involve water in its liquid, solid, and vapor forms. Additional variables being measured include radiative energy fluxes, aerosols, vegetation cover on the land, phytoplankton and dissolved organic matter in the oceans, and air, land, and water temperatures.
To learn more see Aqua's excerpt from the Earth Science Reference Handbook.
Aqua (EOS PM) Project Scientist: Claire L. Parkinson
Enhanced understanding of water in the Earth's climate system and the global water cycle.
Enhanced understanding of additional components of the Earth's climate system and their interactions.
Improved weather forecasting.
Launch Date: July 15, 2004
Launch Location: Vandenberg Air Force Base, California
Aura's four instruments study the atmosphere's chemistry and dynamics. Aura's measurements enable us to investigate questions about ozone trends, air-quality changes and their linkage to climate change. Aura's measurements also provide accurate data for predictive models and useful information for local and national agency decision-support systems.
To learn more see Aura's excerpt from the Earth Science Reference Handbook.
Aura Project Scientist: Anne Douglass
The Aura mission seeks to answer three main science questions:
Is the stratospheric ozone layer recovering?
What are the processes controlling air quality?
How is Earth's climate changing?
Launch Date: December 2004
Launch Location: Kourou, French Guiana
The French Space Agency CNES launched PARASOL into the A-Train orbit in December 2004. Originally designed to be a 2-year mission, PARASOL flew within ~30 seconds of the CALIPSO and CloudSat satellites. In early December 2009, the PARASOL satellite orbit was lowered under the A-train, which will enable it to keep on sharing data periodically with the A-train members, while gradually leaving the A-Train neighborhood. Based on a typical decay of its orbit, it is expected to be completely out of the A-train neighborhood at the end of 2012.
Launch Date: April 28, 2006
Launch Location: Vandenberg Air Force Base, California
CALIPSO is a joint U.S. (NASA) / French (Centre National d'Etudes Spatiales/CNES) mission. Observations from spaceborne lidar, combined with passive imagery, will lead to improved understanding of the role aerosols and clouds play in regulating the Earth's climate, in particular, how aerosols and clouds interact with one another.
To learn more see Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO)'s excerpt from the Earth Science Reference Handbook.
CALIPSO Principal Investigator: Dave Winker
Launch Date: April 28, 2006
Launch Location: Vandenberg Air Force Base, California
CloudSat is studying clouds in detail to better characterize the role they play in regulating Earth's climate. CloudSat is providing the first direct, global survey of the vertical structure and overlap of cloud systems and their liquid and ice-water contents.Data returned should lead to improved cloud representations in atmospheric models, which should help improve the accuracy of weather forecasts and climate predictions made using these models.
To learn more see CloudSat's excerpt from the Earth Science Reference Handbook.
CloudSat Principal Investigator: Graeme Stephens
Profile the vertical structure of clouds: Understanding the vertical structure of clouds is fundamentally important to improving our understanding of how clouds affect both the local and large-scale environment.
Measure the profiles of cloud liquid water and ice water content: These two quantities-predicted by cloud process and global scale models alike-determine practically all other cloud properties, including precipitation and cloud optical properties.
Measure profiles of cloud optical properties: These measurements, when combined with water and ice content information, provide critical tests of key cloud process parameterizations and enable the estimation of flux profiles and radiative heating rates through the atmospheric column.
Launch Date: 2012
The "Global Change Observation Mission" (GCOM) aims to construct, use, and verify systems that enable continuous global-scale observations (for 10 to 15 years) of effective geophysical parameters for elucidating global climate change and water circulation mechanisms.
Water circulation changes will be observed by a microwave radiometer onboard the GCOM-W (Water) satellite (scheduled to be launched in Japan Fiscal Year 2012). The GCOM-W will observe precipitation, vapor amounts, wind velocity above the ocean, sea water temperatures, water levels on land areas and snow depths.
Enhanced understanding of water in the Earth's climate system and the global water cycle.
Enhanced understanding of additional components of the Earth's climate system and their interactions.
Improved weather forecasting.
Launch Date: December 2014
Launch Location: Vandenberg Air Force Base, California
OCO-2 is designed to provide space-based global measurements of atmospheric carbon dioxide (CO2) with the precision and resolution needed to identify and characterize the processes that regulate this important greenhouse gas. With its three high-resolution grating spectrometers, data collected by OCO-2 could be combined with meteorological observations and ground-based CO2 measurement to help characterize CO2 sources and sinks on regional scales at monthly intervals for 2 years.
To learn more see Orbiting Carbon Observatory 2 (OCO-2)'s excerpt from the Earth Science Reference Handbook.
OCO-2 Project Scientist: Mike Gunson
Improve our understanding of the geographic distribution of CO2 sources and sinks (surface fluxes) and the processes controlling their variability on seasonal time scales.
Validate a passive spectroscopic measurement approach and analysis concept that is well suited for future systematic CO2 monitoring missions.
Launch Date: March 4, 2011
Launch Location: Vandenberg Air Force Base, California
The Glory satellite consists of a spacecraft bus and three instruments and will be launched from the Vandenberg Air Force Base aboard a Taurus 2110 launch vehicle. Glory's remote sensing mission is designed to:
1) collect data on the optical, microphysical, and chemical properties, and spatial and temporal distributions of aerosols and clouds; and 2) continue the long-term total solar irradiance climate record.
NASA's Glory spacecraft failed to reach orbit after its 5:09:45 a.m. EST liftoff Friday March 4, 2011 from California's Vandenberg Air Force Base. The fairing on the Taurus XL launch vehicle failed to separate.
The image below reveals where Glory would have flown as part of the A-Train constellation, one minute behind CALIPSO.
To learn more about Glory, see Glory's excerpt from the Earth Science Reference Handbook.
Glory Project Scientist: Michael Mishchenko
Use data collected on the optical, microphysical, and chemical properties of aerosols and clouds to analyze aerosols and aerosol-cloud interactions.
Measure total solar irradiance for long-term climate studies.
New A-Train poster available at: http://atrain.nasa.gov/publications/A-TrainPoster.pdf
Due to a bus undervoltage caused by the emergence of one or more weak battery cells, the CloudSat spacecraft entered emergency mode on April 18, 2011. Through fault protection, the radar was turned off, as were all non-essential spacecraft systems, and the spacecraft was commanded by fault protection into a spinning configuration with solar arrays canted +/-40°. On June 18, CloudSat was able to perform a maneuver to lower its orbit to avoid conjunction with the Aqua satellite. At this time, CloudSat is orbiting below the A-Train. Studies are underway to determine when, if, and in what location CloudSat will return to the A- Train once radar operations are restored.
Aura is NASA’s third large Earth Observing System mission and is dedicated to understanding the changing chemistry of our atmosphere. View the latest brochure highlighting some of the discoveries from the Aura Mission.
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