Clouds and the Earth's Radiant Energy System

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Artist representation of CERES instruments scanning Earth in Rotating Azimuth Plane mode.

Clouds and the Earth's Radiant Energy System (CERES) is on-going NASA climatological experiment from Earth orbit.[1][2] The CERES are scientific satellite instruments, part of the NASA's Earth Observing System (EOS), designed to measure both solar-reflected and Earth-emitted radiation from the top of the atmosphere (TOA) to the Earth's surface. Cloud properties are determined using simultaneous measurements by other EOS instruments such as the Moderate Resolution Imaging Spectroradiometer (MODIS).[3] Results from the CERES and other NASA missions, such as the Earth Radiation Budget Experiment (ERBE),[4] could lead to a better understanding of the role of clouds and the energy cycle in global climate change. [1][5]

Incoming, top-of-atmosphere (TOA) shortwave flux radiation, shows energy received from the sun (Jan 26-27, 2012).
Outgoing, longwave flux radiation at the top-of-atmosphere (Jan 26-27, 2012). Heat energy radiated from Earth (in watts per square meter) is shown in shades of yellow, red, blue and white. The brightest-yellow areas are the hottest and are emitting the most energy out to space, while the dark blue areas and the bright white clouds are much colder, emitting the least energy.

Scientific goals[edit]

CERES experiment has four main objectives:

  • Continuation of the ERBE record of radiative fluxes at the top of the atmosphere (TOA) for climate change analysis.
  • Doubling the accuracy of estimates of radiative fluxes at TOA and the Earth's surface.
  • Provide the first long-term global estimates of the radiative fluxes within the Earth's atmosphere.
  • Provide cloud property estimates that are consistent with the radiative fluxes from surface to TOA.

Each CERES instrument is a radiometer which has three channels - a shortwave (SW) channel to measure reflected sunlight in 0.2 - 5 µm region, a channel to measure Earth-emitted thermal radiation in the 8-12 µm "window" or "WN" region, and a Total channel to measure entire spectrum of outgoing Earth's radiation (>0.2 µm). The CERES instrument was based on the successful Earth Radiation Budget Experiment which used three satellites to provide global energy budget measurements from 1984 to 1993.[6]

Ground Absolute Calibration[edit]

For a Climate Data Record (CDR) mission like CERES, accuracy is of high importance and achieved for pure Infra-Red nighttime measurements by use of a ground laboratory SI traceable blackbody to determine Total and WN channel radiometric gains. This however was not the case for CERES solar channels such as SW and solar portion of the Total telescope, which have no direct un-broken chain to SI traceability. This is because CERES solar responses were measured on ground using lamps whose output energy were estimated by a cryo-cavity reference detector, which used a silver Cassegrain telescope identical to CERES devices to match the satellite instrument Field of View. The reflectivity of this telescope built and used since the mid-1990s was never actually measured, estimated[7] only based on witness samples (see slide 9 of Priestley et al (2014)[8]). Such difficulties in ground calibration, combined with suspected on-ground contamination events[9] have resulted in the need to make un-explained ground to flight changes in SW detector gains as big as 8%[10], simply to make the ERB data seem somewhat reasonable to climate science (note that CERES currently claims[11] a one sigma SW absolute accuracy of 0.9%).

In-flight Calibration[edit]

CERES spatial resolution at nadir view (equivalent diameter of the footprint) is 10 km for CERES on TRMM, and 20 km for CERES on Terra and Aqua satellites. Perhaps of greater importance for missions such as CERES is calibration stability, or the ability to track and partition instrumental changes from Earth data so it tracks true climate change with confidence. CERES onboard calibration sources intended to achieve this for channels measuring reflected sunlight include solar diffusers and tungsten lamps. However the lamps have very little output in the important Ultra-Violet wavelength region where degradation is greatest and they have been seen to drift in energy by over 1.4% in ground tests, without a capability to monitor them on-orbit (Priestley et al (2001)[12]). The solar diffusers have also degraded greatly in orbit such that they have been declared un-usable by Priestley et al (2011)[13]. A pair of blackbody cavities that can be controlled at different temperatures are used for the Total and WN channels, but these have not been proved stable to better than 0.5%/decade[9]. Cold space observations and internal calibration are performed during normal Earth scans.

Missions[edit]

First Launch[edit]

The first CERES instrument Proto-Flight Module (PFM) was launched aboard the NASA Tropical Rainfall Measuring Mission (TRMM) in November 1997 from Japan. However, this instrument failed to operate after 8 months due to an on-board circuit failure.

CERES on the EOS Mission Satellites[edit]

An additional four CERES instruments were launched on the Earth Observing System, with the Terra satellite, launched in December 1999, carrying two (Flight Module 1 (FM1) and FM2) and the Aqua satellite, launched in May 2002, carrying the other two (FM3 and FM4). A fifth instrument is on the Suomi NPP satellite (FM5) launched in October 2011. Four of the CERES Flight Modules are fully operational as of 2017, with the failure of PFM on TRMM and the 2005 loss of the SW channel of FM4 on Aqua. The FM6 instrument is to be launched on the JPSS-1 spacecraft in 2017.[14][15]

Radiation Budget Instruments[edit]

The measurements of the CERES instruments will be furthered by the Radiation Budget Instrument (RBI) to be launched on Joint Polar Satellite System-2 (JPSS-2) in 2021, JPSS-3 in 2026, and JPSS-4 in 2031.[15]. The Trump administration however seems set to cancel the RBI project, despite most of the money for it already having been spent.

Operating modes[edit]

CERES operates in three scanning modes: across the satellite ground track (cross-track), along the direction of the satellite ground track (along-track), and in a Rotating Azimuth Plane (RAP). In RAP mode, the radiometers scan in elevation as they rotate in azimuth, thus acquiring radiance measurement from a wide range of viewing angles. Until February 2005, on Terra and Aqua satellites one of CERES instruments scanned in cross-track mode while the other was in RAP or along-track mode. The instrument operating in RAP scanning mode took two days of along-track data every month. However the multi-angular CERES data allowed to derive new models which account for anisotropy of the viewed scene, and allow TOA radiative flux retrieval with enhanced precision.[16]

See also[edit]

References[edit]

  1. ^ a b B. A. Wielicki; Harrison, Edwin F.; Cess, Robert D.; King, Michael D.; Randall, David A.; et al. (1995). "Mission to Planet Earth: Role of Clouds and Radiation in Climate". Bull. Amer. Meteorol. Soc. pp. 2125–2152. Bibcode:1995BAMS...76.2125W. doi:10.1175/1520-0477(1995)076<2125:MTPERO>2.0.CO;2. 
  2. ^ Wielicki; et al. (1996). "Clouds and the Earth's Radiant Energy System (CERES): An Earth Observing System Experiment". Bull. Amer. Meteor. Soc. 
  3. ^ P. Minnis; et al. (September 2003). "CERES Cloud Property Retrievals from Imager on TRMM, Terra and Aqua" (PDF). Spain. pp. 37–48. 
  4. ^ Barkstrom, Bruce R. (1984). "The Earth Radiation Budget Experiment". Bulletin of the American Meteorological Society. pp. 1170–1186. Bibcode:1984BAMS...65.1170B. doi:10.1175/1520-0477(1984)065<1170:TERBE>2.0.CO;2. 
  5. ^ "Surface and Atmospheric Remote Sensing: Technologies, Data Analysis and Interpretation., International". Geoscience and Remote Sensing Symposium IGARSS '94. 1994. 
  6. ^ NASA, Clouds and the Earth's Radiant Energy System (CERES) (accessed Sept. 9, 2014)
  7. ^ M. Folkman et al., "Calibration of a shortwave reference standard by transfer from a blackbody standard using a cryogenic active cavity radiometer," IEEE Geoscience and Remote Sensing Symposium, pp. 2298-2300, 1994.
  8. ^ Priestley, Kory; et al. (August 5, 2014). "CERES CALCON Talk". 
  9. ^ a b Matthews (2009). "In-Flight Spectral Characterization and Calibration Stability Estimates for the Clouds and the Earth's Radiant Energy System (CERES)". Journal of Atmospheric and Oceanic Technology. 
  10. ^ Priestley, Kory : (July 1, 2002). "CERES Gain Changes". 
  11. ^ Wielicki; et al. (2013). "Achieving Climate Change Absolute Accuracy". Bull. Amer. Meteor. Soc. 
  12. ^ Priestley; et al. (2001). "Postlaunch Radiometric Validation of the Clouds and the Earth's Radiant Energy System (CERES) Proto-Flight Model on the Tropical Rainfall Measuring Mission (TRMM) Spacecraft through 1999". Journal of Applied Meteorology. 
  13. ^ Priestley; et al. (2011). "Radiometric Performance of the CERES Earth Radiation Budget Climate Record Sensors on the EOS Aqua and Terra Spacecraft through April 2007". Journal of Atmospheric and Oceanic Technology. 
  14. ^ "Joint Polar Satellite System - Launch Schedule". www.jpss.noaa.gov. Retrieved 23 January 2017. 
  15. ^ a b "Joint Polar Satellite System: Mission and Instruments". NASA. Retrieved 14 November 2017. 
  16. ^ N. G. Loeb; Kato, Seiji; Loukachine, Konstantin; Manalo-Smith, Natividad; et al. (2005). "Angular distribution models for top-of-atmosphere radiative flux estimation from the Clouds and the Earth's Radiant Energy System instrument on the Terra Satellite. Part I: Methodology". J. Atmos. Ocean. Tech. pp. 338–351. Bibcode:2005JAtOT..22..338L. doi:10.1175/JTECH1712.1. 

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