The Clouds and the Earth's Radiant Energy System (CERES) is the only program currently measuring the global
Earth Radiation Budget (ERB) from space. Two CERES units are located on the EOS Terra platform and two more
are placed on the EOS Aqua satellite. Each of the four operational CERES instruments uses three broadband
radiometric scanning telescopes: the shortwave (SW 0.3 - 5μ), total (0.3 - >100μ), and window (8 - 12μ) channels.
Rigorous pre-launch ground calibration and in-flight calibration is performed on each CERES unit to achieve an
accuracy goal of 1% for SW flux and 0.5% for outgoing LW flux.
The CERES Flight Model-1 and -2 instruments flew aboard the Terra into orbit in December 1999 and the FM-3 and -4 instruments flew on the Aqua spacecraft in May 2002. To date these instruments have provided seven years of measurements on Terra and five years on Aqua. The accuracy requirement for CERES is 0.5% for longwave radiances and 1.0% for shortwave. Achieving this objective is possible by using experience from the ERBE instrument to evolve the CERES design and the methods for analyzing the data. In order to achieve and maintain this accuracy, an internal calibration system and an attenuated view of the Sun are used. Subsequently, to validate that this accuracy has been achieved, a number of techniques have been developed which cover a range of temporal and spatial scales. This ensemble of methods provides a protocol which assures that the CERES measurements are of climate quality. In addition to retrieving fluxes at the top of the atmosphere, the CERES program uses data from other instruments aboard the spacecraft to compute the radiation balance at the surface and at levels through the atmosphere. Finally, the CERES data products are upgraded as higher-level data products show the need for revisions. The calibration stability is better than 0.2% and traceability from ground to in-flight calibration is 0.25%
Clouds and the Earth's Radiant Energy System (CERES) instruments were designed to measure the reflected
shortwave and emitted longwave radiances of the Earth's radiation budget and to investigate the cloud interactions
with global radiances for the long-term monitoring of Earth's climate. The CERES instrument with the three
scanning thermistor bolometers measure broadband radiances in the shortwave (0.3 to 5.0 micrometer), total (0.3 to
>100 micrometer) and 8 - 12 micrometer water vapor window regions. The four CERES instruments (Flight Models
1 through 4) aboard Earth Observing System (EOS) Terra and Aqua platforms were instrumental in conducting
lunar radiance measurement on a regular basis. Moon-reflected solar radiances were measured with the shortwave
sensor while both moon-reflected solar and moon-emitted longwave radiances were measured using the total sensor.
The CERES sensors performed lunar measurements at various phase angles ranging from four to ten degrees before
and after each full moon phase. Additional measurements were also conducted during the lunar eclipse events. The
resulting filtered radiances were normalized to the mean sun-moon distance and the mean earth-moon distance. The
lunar radiances measured by the sensors from all CERES instruments for a period of January 2001 to June 2007
were analyzed and compared. The CERES total sensor results showed a variation of about +/- 0.5 percent, while a
+/- 2.0 percent variation was seen in shortwave sensor results.
The Clouds and the Earth's Radiant Energy System (CERES) is the only project currently measuring the global
Earth Radiation Budget (ERB) from space. Two CERES instruments are located on the EOS Terra platform and
two more are placed on the EOS Aqua satellite. One more CERES unit provided 8 months of ERB data in 1998
from the TRMM platform. Each of the CERES devices uses three broadband radiometric scanning telescopes:
the shortwave (SW 0.3 → 5μm), Total (0.3 → 100μm), and window (8 → 12μm) channels. Rigorous pre-launch
ground calibration is performed on each CERES unit to achieve an accuracy goal of 1% for Short Wave (SW) and
0.5% for outgoing Long Wave (LW) radiance. Any ground to flight or in-flight changes in radiometer response is
monitored using onboard calibration sources. For the total and window channels these take the form of concentric
groove blackbodies, while the SW channels use stable tungsten lamps. Recent studies have shown that the SW
response of space based broadband radiometers can change dramatically due to optical contamination. With
these changes having most impact on optical response to blue-UV radiance, where tungsten lamps are largely
devoid of output, such changes are hard to monitor accurately using existing on-board sources. This study
details an attempt to use the vicarious stability metric of deep convective clouds (DCC), nighttime LW scenes
and a newly developed SW optical darkening model to place all CERES instrument measurements on the same
radiometric scale. The results show that scene dependant dispersion in nadir comparisons between instruments
on the same satellite are significantly reduced. Also the suggestion is that the pre-flight contamination of the
CERES instruments may require an increase in Terra and Aqua measured SW flux. A larger necessary increase
in Aqua SW flux is believed to be due to greater pre-flight contamination of the CERES Aqua optics.
In order to best detect real changes in the Earth's climate system, it is estimated that in space based instrumentation
measuring the Earth Radiation Budget (ERB) must remain calibrated with a stability of 0.3Wm−2
per decade and reach an absolute accuracy of 1Wm−2. Such stability is beyond that specified by existing ERB
programs such as the Clouds and the Earth's Radiant Energy System (CERES, using three broadband radiometric
scanning channels: the shortwave (SW 0.3−5um), Total (0.3− > 100um), and window (8−12um)).
The CERES measurement of daytime outgoing longwave radiance (OLR) is obtained using subtraction of the
SW channel signal from that of the co-aligned Total channel telescope. This requires precise balancing of the
estimated response of the Total channel optics with those of the SW only channel when viewing daytime Earth
scenes. Any post ground calibration contamination of Total channel optics that reduces its response to SW radiance
can therefore upset this balancing process, introducing biases and trends in measurements of daytime LW
radiance. This paper presents a new methodology used for balancing Total and SW channel spectral responses
for all daytime Earth scenes using a model of contaminant spectral darkening. The results of the technique when
applied to both CERES units on Terra are shown to remove significant trends and biases in measurements of
daytime LW radiance.
Clouds and the Earth's Radiant Energy System (CERES) instruments were designed to measure the reflected
shortwave and emitted longwave radiances of the Earth's radiation budget and to investigate the cloud interactions
with global radiances for the long-term monitoring of Earth's climate. CERES instrument has three scanning
thermistor bolometers that measure broadband radiances in the shortwave (0.3 to 5.0 micrometer), total (0.3 to >100
micrometer) and 8 - 12 micrometer water vapor window regions. Four CERES instruments (Flight Models1 through
4) are flying aboard EOS Terra and Aqua platforms with two instruments aboard each spacecraft. The pre-launch
accuracy requirements for CERES were 1.0% in the shortwave and 0.5% in longwave regions.
The in-flight calibration of CERES sensors are carried out using the internal calibration module (ICM) comprising
of blackbody sources and tungsten lamp, and a solar diffuser plate known as the Mirror Attenuator Mosaic (MAM).
The ICM and MAM calibration results are instrumental in understanding the ground to flight shift and in-flight drifts
in CERES sensors' gains. Inter and intra instrument validation studies are conducted on the CERES measurements
to monitor the behavior of the sensors in various spectral regions. Targets such as deep convective clouds and
tropical ocean are used to evaluate the sensors' stability within an instrument. With two CERES instruments on
same platform, inter comparison of similar sensor measurements viewing the same geolocation are also conducted.
The results from these individual studies have collectively given an understanding of each CERES sensor's behavior
in different spectral regions. This paper discusses the results from each of these studies which facilitated the
correction of CERES data products with a calibration stability better than 0.2%.
Keywords: CERES, EOS Instrument, Radiometry, Calibration, Validationt
It is estimated that in order to best detect real changes in the Earth's climate system, space based instrumentation
measuring the Earth Radiation Budget (ERB) needs to remain calibrated with a stability of 0.3% per decade.
This stability is beyond the specification of existing ERB programs such as the Clouds and the Earth's Radiant
Energy System (CERES, using three broadband radiometric scanning channels: the shortwave 0.3 - 5μm, total
0.3- > 100μm, and window 8 - 12μm). It is known that when in low earth orbit, optical response to blue/UV
radiance can be reduced significantly due to UV hardened contaminants deposited on the surface of the optics.
Typical onboard calibration lamps do not emit sufficient energy in the blue/UV region, hence this darkening
is not directly measurable using standard internal calibration techniques. This paper details a study using a
model of contaminant deposition and darkening, in conjunction with in-flight vicarious calibration techniques, to
derive the spectral shape of darkening to which a broadband instrument is subjected. The model ultimately uses
the reflectivity of Deep Convective Clouds as a stability metric. The results of the model when applied to the
CERES instruments on board the EOS Terra satellite are shown. Given comprehensive validation of the model,
these results will allow the CERES spectral responses to be updated accordingly prior to any forthcoming data
release in an attempt to reach the optimum stability target that the climate community requires.
Clouds and the Earth's Radiant Energy system (CERES) sensors provide accurate measurements for the long-term monitoring of the Earth's radiation budget components. The three scanning thermistor bolometer sensors on CERES measure broadband radiances in the shortwave (0.3 to 5.0 micrometer), total (0.3 to >100 micrometer) and in 8 - 12 micrometer water vapor window regions. Currently four of the CERES instruments (Flight Models 1 through 4 [FM1 - FM4]) are flying aboard EOS Terra and Aqua platforms with two instruments aboard each spacecraft. The sensor calibrations are performed with onboard blackbody sources and a tungsten lamp as well as a solar diffuser plate known as the Mirror Attenuator Mosaic (MAM). The calibration results collectively depict the ground to orbit shifts and the on-orbit drifts in the sensor reponses. Deep convective clouds and tropical ocean are used as validation targets to understand the sensors' stability on-orbit. With two CERES instruments on the same platform, comparison of measurements from similar sensors viewing the same geolocation are performed. The different calibration and validation studies performed on CERES bring to light the radiometric gain and spectral variation of the sensors from pre and post launch. This paper discusses briefly the contribution of each calibration and validation study in understanding CERES sensors' behavior. It also shows the results from these studies which enabled to correct the data products with a calibration stability of better than 0.2%.
It is estimated that in order to best detect real changes in the Earth's climate system, space based instrumentation measuring the Earth Radiation Budget (ERB) must remain calibrated with a stability of 0.3% per decade. Such stability is beyond the specified accuracy of existing ERB programs such as the Clouds and the Earth's Radiant Energy System (CERES, using three broadband radiometric scanning channels: the shortwave 0.3 - 5μm, total 0.3- > 100μm, and window 8 - 12μm). It has been shown that when in low earth orbit, optical response to blue/UV radiance can be reduced significantly due to UV hardened contaminants deposited on the surface of the optics. Since typical onboard calibration lamps do not emit sufficient energy in the blue/UV region, this darkening is not directly measurable using standard internal calibration techniques. This paper describes a study using a model of contaminant deposition and darkening, in conjunction with in-flight vicarious calibration techniques, to derive the spectral shape of darkening to which a broadband instrument is subjected. Ultimately the model uses the reflectivity of Deep Convective Clouds as a stability metric. The results of the model when applied to the CERES instruments on board the EOS Terra satellite are shown. Given comprehensive validation of the model, these results will allow the CERES spectral responses to be updated accordingly prior to any forthcoming data release in an attempt to reach the optimum stability target that the climate community requires.
Cloud's and the Earth's Radiant Energy System (CERES) is an investigation into the role of clouds and radiation in the Earth's climate system. Four CERES scanning thermistor bolometer instruments are currently in orbit. Flight model 1 (FM1) and 2 (FM2) are aboard the Earth Observing System (EOS) Terra satellite and FM3 and FM4 are aboard the EOS Aqua satellite. Each CERES instrument measures in three broadband radiometric regions: the shortwave (SW 0.3-5μm), total (0.3- > 100μm), and window (8-12μm). It has been found that both CERES instruments on the Terra platform imply that the SW flux scattered from the Earth had dropped by up to 2% from 2000 to 2004. No climatological explanation for this drop could be found, suggesting the cause was a drift in both the Terra instruments. However, the onboard calibration lamps for the SW channels do not show a change in gain of this magnitude. Experience from other satellite missions has shown that optics in the orbital environment can become contaminated, severely reducing their transmission of ultra-violet (UV) radiation. Since the calibration lamps emit little radiance in the UV spectral region it was suggested that contaminates could be responsible for an undetectable 'spectral darkening' of the CERES SW channel optics and hence the apparent drop in SW flux. Further evidence for this was found by looking at the comparison between simultaneous measurements made by FM1 and FM2. The proposed mechanisms for contaminant build up would not apply to a CERES instrument operating in the normal cross track scan mode. Indeed it was found from the comparison between CERES instruments on Terra that the response of the instrument operating in rotating azimuth plane (RAPS) mode consistently dropped relative to the other cross track instrument. Since at all times one of the instruments operates in cross track mode, where it is not subject to spectral darkening, it allowed that unit to be used as a calibration standard from which the darkening of the other RAPS instrument can be measured. A table of adjustment coefficients to compensate for this spectral darkening are therefore derived in this paper. These figures are designed to be multiplied by SW fluxes or radiances produced in the climate community using Edition 2 CERES data. SW CERES measurements that have been revised using these coeffcients are therefore to be referred to as ERBE-like Edition2_Rev1 or SSF Edition2B_Rev1 data in future literature. Current work to fully characterize the effect of spectral darkening on the instrument spectral response before the release of Edition 3 data is also described.
It is important to maintain measurements of Earth Radiation Budget parameters from orbit. Such measurements require broadband radiance detectors such as bolometers or thermopiles that rely on the conversion of radiant energy into heat. This heat conversion/conduction results in a thermal detector typically having an exponential time lag of a few milliseconds. However, it is found that there is often a far slower 'slow mode transient' response of around 300ms because the detector mounting material tends to rise in temperature as heat flows out of the detector to its surroundings. Hence this can cause the detector response to a constant input of radiance to continue increasing by a further 1%, for up to half a second after initial exposure. Using analysis of the heat flow out from a bolometer and through its mounting, the Laplace domain impulse response of the detector is derived that includes both first and second time constant effects. Transformation to the Z domain then allows design of a numerical filter to remove the second time constant effect while retaining that of the first time constant. Restoration of the ideal detector response is shown to be advantageous when applied to the output of thermistor bolometers onboard the Cloud's and the Earth's Radiant Energy System (CERES). It also allows more complete characterization of the response of such detectors using general calibration data. The design and use of such a filter is therefore highly applicable to any scanning bolometer or thermopile instrument with spurious slow mode effects.
Resolving uncertainties surrounding the nature of future climate change is currently one of the greatest challenges facing mankind. Validating climate model predictions of the currently much miss-represented cloud radiative feedback requires measurements made from orbit of the Earth Radiation Budget (ERB), specifically targeted at clouds. The ERB parameters for measure are the scattered solar or short wave (SW, 0.3-5μm) and the emitted thermal or long wave radiance (LW, 5-100μm). The Clouds and the Earth's Radiant Energy System (CERES), as part of NASA's Earth observing System, uses thermistor bolometer detectors to provide global high spatial resolution ERB measurements from polar orbiting space platforms. The Geostationary Earth Radiation Budget (GERB) experiment is a European Space Agency (ESA) project on board the spin stabilized Meteosat second Generation (MSG) platform. Location in geostationary orbit and the use of an array of thermopile detectors enables sampling of ERB radiances from the entire Earth disc at an optimum 5 minute temporal resolution. Taking full advantage of both GERB's time resolution and CERES's global coverage for climate science requires a radiometric cross calibration and validation between the two satellite programs. This study quantifies the instantaneous sampling errors incurred by the GERB instrument due to geo-location uncertainties and orbit spin axis miss-alignment. The results can therefore be characterized as a function of scene contrast, allowing an appropriate statistical weighting to be employed when making a radiometric comparison between the GERB and CERES instruments.
Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks.
You are receiving this notice because your organization may not have SPIE eBooks access.*
*Shibboleth/Open Athens users─please
sign in
to access your institution's subscriptions.
To obtain this item, you may purchase the complete book in print or electronic format on
SPIE.org.
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.