The MODIS thermal emissive bands (TEB) radiometric calibration uses a quadratic function for the instrument response, and the calibration coefficients look-up tables (LUTs) are updated using the response of an on-board blackbody (BB). After more than 21 and 19 years on-orbit, the TEB performances for Terra and Aqua MODIS have been generally stable. However, contamination from electronic crosstalk, a known issue since prelaunch, has affected the L1B image quality and measurement accuracy. In addition to the photovoltaic (PV) longwave infrared (LWIR) bands crosstalk correction included in Terra MODIS Collection 6.1 (C6.1), a crosstalk correction for select detectors in the Terra and Aqua mid-wave infrared (MWIR) and Aqua PV LWIR bands are applied in C7. The mission-long crosstalk coefficients for the selected detectors are derived and populated in the form of LUTs. The crosstalk correction is applied to both on-orbit calibration and the algorithm used to generate Earth-view L1B products. Among these detectors, the Aqua MODIS band 24 detector 1 crosstalk has the largest impact on image quality, with striping observed over cold scenes for both Terra and Aqua MODIS. The images of C7 L1B and C6.1 are compared to assess the impact of the correction. Additional assessments using Earthview measurements and inter-comparison also revealed the need for improvement of calibration stability and consistence for select bands. Additional improvements for long-term stability and mirror side consistence were developed using quasideep convective clouds (qDCC), Dome-C, ocean, desert, and inter-comparison with other instruments.
The Moderate Resolution Imaging Spectroradiometer (MODIS) is a key instrument aboard the Terra and Aqua satellites, launched in 1999 and 2002, respectively. Relying on a two-sided paddle-wheel cross-track scanning mirror, the sensor provides Earth view measurements in 36 spectral bands from 0.4 to 14.4 μm. The swath of data collected by MODIS is over 2300 km wide and covers the entire surface of the Earth every one to two days. A set of onboard calibrators include a solar diffuser (SD) and a solar diffuser stability monitor, a v-grooved flat panel blackbody (BB), and a spectro-radiometric calibration assembly. A deep space view (SV) is used as a background reference. The thermal emissive bands (TEBs) on‐orbit calibration is performed using a quadratic algorithm by reference to a temperature controlled BB on a scan-by-scan basis. This study examines the consistency of the Terra MODIS TEB responses between the two mirror sides for measurements from the BB, SV, SD, and Earth view sectors. It was found that there is a mirror side correlated noise (MSCN) during the early mission of Terra MODIS, particularly after the electronic configuration changes or instrument resets. In this work, the impact of MSCN on radiometric calibration is assessed using measured brightness temperatures obtained from the deep convective clouds, ice/snow surface at Dome C, Antarctica and the Atlantic Ocean. Results of this study provide a further assessment of the newly implemented Collection 7 calibration algorithm in reducing the MSCN induced striping in the MODIS L1B imagery.
The Moderate-resolution Imaging Spectroradiometer (MODIS) instruments are on-board the Aqua and Terra spacecraft, launched in 2002 and 1999, respectively. Since beginning operation, they have continued to collect valuable remote sensing data of the Earth in 36 spectral bands ranging in wavelengths from 0.41 to 14.5 μm. The Level 1B (L1B) algorithm produces calibrated top of the atmosphere (TOA) radiances for each Earth-view (EV) pixel and calibrated TOA reflectances for the reflective solar bands using geo-located, uncalibrated instrument data and calibration look up tables (LUTs) produced regularly by the MODIS Characterization Support Team (MCST). The L1B algorithm also calculates an uncertainty value for each EV pixel. The calibrated radiance and reflectance products are used to generate higher-level science products. A separate L1B code version is maintained for both MODIS instruments so that sensor specific issues can be handled individually. The current L1B algorithm version produces the Collection 6.1 (C6.1) products and was released in 2017. An overview of the C6.1 algorithm is provided together with improvements made since its release. Also discussed briefly are the planned improvements in the Collection 7 L1B algorithm.
KEYWORDS: MODIS, Calibration, Sensors, Long wavelength infrared, Space operations, Photovoltaics, Mirrors, Contamination, Clouds, Temperature metrology
Terra and Aqua MODIS have successfully operated for more than 20 and 18 years, respectively, and far exceeded their designed lifetimes of 6 years. MODIS has 36 spectral bands, among which 16 are the thermal emissive bands (TEB) covering a wavelength range from 3.75 to 14.24 μm. Observations from the MODIS TEB have been used to generate a number of data products, such as surface/cloud/atmospheric temperatures, cloud top altitude, and water vapor properties. To a large extent, the quality of the MODIS L1B radiance product has been maintained through the entirety of each mission via extensive on-orbit calibration and validation efforts. MODIS TEB calibration uses a quadratic algorithm and is referenced to an on-board blackbody with its temperature measurements traceable to the NIST standard. We provide an overview of the MODIS instrument operations, key TEB calibration activities, and algorithms used in the latest L1B data Collection 6.1 (C6.1) and describe the TEB on-orbit performance for both Terra and Aqua MODIS. The TEB gain trends have been stable to within 5% over the Terra mission after 2003 under the same electronic configuration, except for bands 27 to 30, and within 3% over the Aqua mission. The Terra MODIS optical crosstalk correction implemented right after launch has been very effective in removing the ghost images in its photoconductive detector bands 32 to 36. Starting from C6.1, an electronic crosstalk correction algorithm has also been applied to the Terra MODIS photovoltaic detector long-wave infrared bands 27 to 30. The noise characterization performance remains stable with most TEB detectors continuously meeting their design requirements. A gradual loss of the Aqua MODIS radiative cooler margin reached its maximum in 2013 and has been slowly recovering since then. On-orbit changes in TEB response versus scan angle are extremely small based on pitch maneuver observations and assessments using vicarious approaches. The remaining challenges in TEB calibration and proposed improvements for the upcoming data collection with L1B data production and reprocessing are discussed.
Terra and Aqua MODIS have provided continuous global observations for scientific applications for more than 20 and 18 years, respectively. The radiometric calibration of the MODIS thermal emissive bands (TEB) is based on a quadratic approximation of the instrument response. The calibration coefficients look-up tables (LUTs) are updated using the response of the MODIS on-board blackbody (BB) with the response background subtracted by space view. The quarterly on-board BB warm-up and cool-down activity temperature ranges from 270 K to 315 K, and the derived offset has a relatively large uncertainty. Electronic cross-talk, an artifact that affects both instrument calibration and Earth view (EV) radiance retrievals, is corrected based on lunar observations. Calibration assessments using EV observations (e.g. ocean, desert, Antarctic Dome Concordia, and deep convective clouds) provide useful information to evaluate the impact of the Terra safe mode (February 2016) and Aqua MODIS formatter reset (January 2018) events on both MODIS instruments. This study focuses on the TEB radiometric calibration algorithm improvements for future collections based on calibration assessments using EV measurements and analytical modeling. Measurement stability and consistency over specific Earth scenes with a wide temperature range, as well as their brightness temperature (BT) dependency, are used for bias estimations in the calibration coefficients. Calibration coefficients are derived and updated after adjusting the current fitting algorithm. Thereafter, using the test LUTs, their impact on the Level 1B (L1B) data for different EV scenes is analyzed.
MODIS is a cross-track, whisk-broom scanning imaging radiometer with a double-sided scan mirror that collects data in 36 spectral bands. Sixteen of the 36 MODIS spectral bands are Thermal Emissive Bands (TEBs) whose spectral wavelengths range from 3.5 μm to 14.4 μm. The TEB detectors are calibrated on a scan-by-scan basis using a quadratic calibration algorithm by observing both the MODIS on-board blackbody (BB) and a background space view reference. Blackbody warm-up/cool-down (WUCD) events are performed quarterly to track on-orbit changes associated with the TEB detectors' non-linearity. Following each WUCD, the calibration coefficients in the quadratic algorithm, and their associated contributions to the total uncertainty, are updated and delivered through separate look-up tables (LUTs) when all update criteria are met. Afterwards, the LUTs are incorporated into the Level 1B (L1B) product. Since the Terra MODIS mission began, a steady increase in electronic cross-talk has been observed for TEBs 27{30. Starting from Collection 6.1, an algorithm has been applied using correction coefficients derived from regularly-scheduled lunar observations, with the correction LUT update dependent on its impact on the current L1B product. The MODIS Characterization Support Team (MCST) has established a comprehensive set of procedures to assure timely and accurate LUT updates, and maintain the quality and accuracy of the L1B and science products. This paper provides an overview of the current calibration and LUT delivery process for the MODIS TEBs in Collections 6 and 6.1.
KEYWORDS: MODIS, Sensors, Calibration, Photovoltaics, Long wavelength infrared, Signal processing, Analog electronics, Staring arrays, Earth observing sensors, Signal detection
The Electronic Calibration (Ecal) tests are performed during various stages of instrument development to examine the linearity of the instrument electronics. During this process, charges with stepwise increments are injected in the analog electronics circuitry to generate a ramp signal that can be used to characterize any nonlinearities in the electronics. The prelaunch characterization of MODIS (on the Terra and Aqua platforms) and VIIRS (on SNPP, JPSS-1 and JPSS-2) involved a regular evaluation of the electronics linearity using the Ecal tests. On orbit, the Ecal tests have been regularly performed over the mission for both the MODIS instruments to derive the electronics gain and linearity. Unlike MODIS, the Ecal tests on the VIIRS instruments are performed on an as-needed basis. To date, no Ecal tests were performed for S-NPP VIIRS on orbit. The VIIRS instrument on JPSS-1 (now NOAA 20) was launched on November 18, 2017. An Ecal test was performed to support the instruments initial post-launch performance assessment. Shortly after the
Terra MODIS has provided continuous global observations for science research and applications for more than 18 years. The MODIS Thermal emissive bands (TEB) radiometric calibration uses a quadratic function for instrument response. The calibration coefficients are updated using the response of an on-board blackbody (BB) in quarterly warm-up and cool-down (WUCD) events. As instrument degradation and electronic crosstalk of long-wave infrared (LWIR) bands 27 to 30 developed substantial issues, accurate calibration is crucial for a high-quality L1B product. The on-board BB WUCD temperature ranges from 270 K to 315 K and the derived nonlinear response has a relatively large uncertainty for the offset, especially for these LWIR bands, which affects the measurements of low brightness temperature (BT) scenes. In this study, the TEB radiometric calibration impact on the L1B product is assessed using selected cold targets and the measurements during regular lunar rolls. The cold targets include Antarctic Dome Concordia (Dome-C) and deep convective clouds (DCC) for the calibration assessment, focusing on bands 27 to 30. Dome-C area is covered with uniformly-distributed permanent snow, and the atmospheric effect is small and relatively constant. Usually the DCC is treated as an invariant earth target to evaluate the reflective solar band calibration. The DCC can also be treated as a stable target to assess the performance of TEB calibration. During a scheduled lunar observation event with a spacecraft roll maneuver to view the moon through the space view port, the instrument cavity provides a stable reference for calibration assessment. The long-term trending of BT measurements and the relative difference between scan mirror sides and detectors are used for the assessment of the calibration consistency and stability. The comparison of L1B products over the selected targets before and after the calibration coefficients update can be used to assess the impact of a calibration look-up table (LUT) update. This assessment is beneficial for future calibration algorithm and LUT update procedure improvements for enhancing the L1B product quality.
The Moderate Resolution Imaging Spectroradiometer (MODIS) is a key scientific instrument that was launched into
Earth orbit by NASA in 1999 on board the Terra (EOS AM) satellite and in 2002 on board the Aqua (EOS PM) satellite.
Terra and Aqua MODIS collect the entire Earth’s images every 1 to 2 days in 36 spectral bands. MODIS band 1 (0.620-
0.670 μm) and band 2 (0.841-0.876 μm) have nadir spatial resolution of 250 m and their measurements are crucial to
derive key land surface products. This study evaluates the performance of the Collection 6 (C6, and C6.1) L1B of both
Terra and Aqua MODIS bands 1 and 2 using Simultaneous Nadir Overpass (SNO) data to compare with AVHRR/3
sensors. We examine the relative stability between Terra and Aqua MODIS in reference to NOAA N15 and N19 the
Advanced Very High Resolution Radiometer (AVHRR/3). The comparisons for MODIS to AVHRR/3 are over a fifteenyear
period from 2002 to 2017. Results from this study provide a quantitative assessment of Terra and Aqua MODIS
band 1 and band 2 calibration stability and the relative differences through the NOAA N15 and N19 AVHRR/3 sensors.
KEYWORDS: MODIS, Calibration, Photovoltaics, Sensors, Signal detection, Signal to noise ratio, Space operations, Long wavelength infrared, Mirrors, Staring arrays
MODIS has 36 spectral bands located on four focal plane assemblies (FPAs), covering wavelengths from 0.41 to 14.4 μm. MODIS bands 1-30 collect data using photovoltaic (PV) detectors and, therefore, are referred to as the PV bands. Similarly, bands 31-36 using photoconductive (PC) detectors are referred to as the PC bands. The MODIS instrument was built with a set of on-board calibrators (OBCs) in order to track on-orbit changes of its radiometric, spatial, and spectral characteristics. In addition, an electronic calibration (ECAL) function can be used to monitor on-orbit changes of its electronic responses (gains). This is accomplished via a series of stair step signals generated by the ECAL function. These signals, in place of the FPA detector signals, are amplified and digitized just like the detector signals. Over the entire mission of both Terra and Aqua MODIS, the ECAL has been performed for the PV bands and used to assess their on-orbit performance. This paper provides an overview of MODIS on-orbit calibration activities with a focus on the PV ECAL, including its calibration process and approaches used to monitor the electronic performance. It presents the results derived and lessons learned from Terra and Aqua MODIS on-orbit ECAL. Also discussed are some of the applications performed with the information provided by the ECAL data.
MODIS is a key instrument of NASA’s Earth Observing System. It has successfully operated for 16+ years on the Terra satellite and 14+ years on the Aqua satellite, respectively. MODIS has 36 spectral bands at three different nadir spatial resolutions, 250m (bands 1-2), 500m (bands 3-7), and 1km (bands 8-36). MODIS subframe measurement is designed for bands 1-7 to match their spatial resolution in the scan direction to that of the track direction. Within each 1 km frame, the MODIS 250 m resolution bands sample four subframes and the 500 m resolution bands sample two subframes. The detector gains are calibrated at a subframe level. Due to calibration differences between subframes, noticeable subframe striping is observed in the Level 1B (L1B) products, which exhibit a predominant radiance-level dependence. This paper presents results of subframe differences from various onboard and earth-view data sources (e.g. solar diffuser, electronic calibration, spectro-radiometric calibration assembly, Earth view, etc.). A subframe bias correction algorithm is proposed to minimize the subframe striping in MODIS L1B image. The algorithm has been tested using sample L1B images and the vertical striping at lower radiance value is mitigated after applying the corrections. The subframe bias correction approach will be considered for implementation in future versions of the calibration algorithm.
MODerate resolution Imaging Spectroradiometer (MODIS), a leading heritage sensor in the fleet of Earth Observing System for the National Aeronautics and Space Administration (NASA) is in space orbit on two spacecrafts. They are the Terra (T) and Aqua (A) platforms. Both instruments have successfully continued to operate beyond the 6 year design life time, with the T-MODIS currently functional beyond 15 years and the A-MODIS operating beyond 13 years respectively. The MODIS sensor characteristics include a spectral coverage from 0.41 μm – 14.4 μm, of which wavelengths ranging from 3.7 μm – 14. 4 μm cover the thermal infrared region also referred to as the Thermal Emissive Bands (TEBs). The TEBs is calibrated using a v-grooved BlackBody (BB) whose temperature measurements are traceable to the National Institute of Standards and Technology temperature scales. The TEBs calibration based on the onboard BB is extremely important for its high radiometric fidelity. In this paper, we provide a complete characterization of the lifetime instrument performance of both MODIS instruments in terms of the sensor gain, the Noise Equivalent difference Temperature, key instrument telemetry such as the BB lifetime trends, the instrument temperature trends, the Cold Focal Plane telemetry and finally, the total assessed calibration uncertainty of the TEBs.
The MODerate-resolution Imaging Spectroradiometer (MODIS) is one of the primary instruments in the fleet of NASA’s Earth Observing Systems (EOS) in space. Terra MODIS has completed 15 years of operation far exceeding its design lifetime of 6 years. The MODIS Level 1B (L1B) processing is the first in the process chain for deriving various higher level science products. These products are used mainly in understanding the geophysical changes occurring in the Earth’s land, ocean, and atmosphere. The L1B code is designed to carefully calibrate the responses of all the detectors of the 36 spectral bands of MODIS and provide accurate L1B radiances (also reflectances in the case of Reflective Solar Bands). To fulfill this purpose, Look Up Tables (LUTs), that contain calibration coefficients derived from both on-board calibrators and Earth-view characterized responses, are used in the L1B processing. In this paper, we present the implementation mechanism of the electronic crosstalk correction in the Photo Voltaic (PV) Long Wave InfraRed (LWIR) bands (Bands 27-30). The crosstalk correction involves two vital components. First, a crosstalk correction modular is implemented in the L1B code to correct the on-board Blackbody and Earth-View (EV) digital number (dn) responses using a linear correction model. Second, the correction coefficients, derived from the EV observations, are supplied in the form of LUTs. Further, the LUTs contain time stamps reflecting to the change in the coefficients assessed using the Noise Equivalent difference Temperature (NEdT) trending. With the algorithms applied in the MODIS L1B processing it is demonstrated that these corrections indeed restore the radiometric balance for each of the affected bands and substantially reduce the striping noise in the processed images.
Radiometric calibration is important for continuity and reliability of any optical sensor data. The Moderate Resolution Imaging Spectroradiometer (MODIS) onboard NASA EOS (Earth Observing System) Aqua satellite has been nominally operating since its launch on May 4, 2002. The MODIS thermal emissive bands (TEB) are calibrated using a quadratic calibration algorithm and the dominant gain term is determined every scan by reference to a temperature-controlled blackbody (BB) with known emissivity. On a quarterly basis, a BB warm-up and cool-down (WUCD) process is scheduled to provide measurements to determine the offset and nonlinear coefficients used in the TEB calibration algorithm. For Aqua MODIS, the offset and nonlinear terms are based on the results from prelaunch thermal vacuum tests. However, on-orbit trending results show that they have small but noticeable drifts. To maintain data quality and consistency, an iterative approach is applied to adjust the prelaunch based nonlinear terms, which are currently used to produce Aqua MODIS Collection-6 L1B. This paper provides details on how to use an iterative solution to determine these calibration coefficients based on BB WUCD measurements. Validation is performed using simultaneous nadir overpasses (SNO) of Aqua MODIS and the Infrared Atmospheric Sounding Interferometer (IASI) onboard the Metop-A satellite and near surface temperature measurements at Dome C on the Antarctic Plateau.
KEYWORDS: MODIS, Calibration, Sensors, Long wavelength infrared, Space operations, Mirrors, Diffusers, Electronics, Signal to noise ratio, Near infrared
Since launch in December 1999, Terra MODIS has successfully operated for nearly 15 years, making continuous observations. Data products derived from MODIS observations have significantly contributed to a wide range of studies of key geophysical parameters of the earth’s eco-system of land, ocean, and atmosphere, and their changes over time. The quality of MODIS data products relies on the dedicated effort to monitor and sustain instrument health and operation, to calibrate and update sensor parameters and properties, and to improve calibration algorithms. MODIS observations are made in 36 spectral bands, covering wavelengths from visible to long-wave infrared. The reflective solar bands (1-19 and 26) are primarily calibrated by a solar diffuser (SD) panel and regularly scheduled lunar observations. The thermal emissive bands (20-25 and 27- 36) calibration is referenced to an on-board blackbody (BB) source. On-orbit changes in the sensor spectral and spatial characteristics are monitored by a spectroradiometric calibration assembly (SRCA). This paper provides an overview of Terra MODIS on-orbit operation and calibration activities and implementation strategies. It presents and summarizes sensor on-orbit performance using nearly 15 years of data from its telemetry, on-board calibrators, and lunar observations. Also discussed in this paper are changes in sensor characteristics, corrections applied to maintain MODIS level 1B (L1B) data quality, and efforts for future improvements.
KEYWORDS: Calibration, MODIS, Sensors, Algorithm development, Staring arrays, Mirrors, Long wavelength infrared, Black bodies, Detection and tracking algorithms, Temperature metrology
The MODerate Resolution Imaging Spectroradiometer (MODIS) is a heritage sensor operating on both the Terra and
Aqua platforms, and has collected remotely sensed data for a combined mission time of twenty plus years. The
instrument robustness and performance over their lifetimes has been very satisfactory and is well calibrated using the onboard
calibrators (OBC). The radiometric fidelity of the MODIS instruments has ensured the high quality of science
products derived from the Level 1B (L1B) imagery. MODIS Thermal Emissive Bands (TEB) are calibrated on-orbit
using an on-board blackbody (BB) and through the space-view (SV) port. The MODIS BB is nominally controlled at
290K for Terra and at 285K for Aqua. Periodically, a BB warm-up and cool-down (WUCD) process is implemented,
during which the BB temperatures vary from instrument ambient (approximately 272K) to 315K. The calibration
coefficients for the 16 TEB bands are characterized using the above mentioned on-board BB operations (i.e. using
nominal and WUCD operations). This paper will focus on the calibration algorithms of the TEB developed for collection
6 (C6) processing, its impact on the Level 1B (L1B) product in comparison to collection 5 (C5), and the methodology
for issuing a Look Up Table (LUT) update for L1B processing.
KEYWORDS: MODIS, Sensors, Calibration, Algorithm development, Mirrors, Detection and tracking algorithms, Space operations, Temperature metrology, Data processing, Reflectivity
The Moderate Resolution Imaging Spectroradiometer (MODIS) has been operating on both the Terra and Aqua
spacecraft for over 10.5 and 8 years, respectively. Over 40 science products are generated routinely from MODIS Earth
images and used extensively by the global science community for a wide variety of land, ocean, and atmosphere
applications. Over the mission lifetime, several versions of the MODIS data set have been in use as the calibration and
data processing algorithms evolved. Currently Version 5 MODIS data is the baseline Level-1B calibrated science
product. The MODIS Characterization Support Team (MCST), with input from the MODIS Science Team, developed
and delivered a number of improvements and enhancements to the calibration algorithms, Level-1B processing code and
Look-up Tables for the Version 6 Level-1B MODIS data. Version 6 implements a number of changes in the calibration
methodology for both the Reflective Solar Bands (RSB) and Thermal Emissive Bands (TEB). This paper describes the
improvements introduced in Collection 6 to the RSB and TEB calibration and detector Quality Assurance (QA)
handling.
KEYWORDS: MODIS, Temperature metrology, Calibration, Sensors, Long wavelength infrared, Mid-IR, Infrared radiation, Space operations, Mirrors, Black bodies
MODIS is a major instrument for the NASA EOS Terra and Aqua missions, launched in December 1999 and May 2002
respectively. MODIS has 16 thermal emissive bands and they are calibrated using an onboard blackbody (BB) based on
a nonlinear second order relationship. While the gains of the MODIS thermal bands are calibrated on a scan-by-scan
basis, the offset and non-linear terms are determined either from prelaunch or on-orbit measurements during scheduled
BB warm-up and cool-down cycles. A major concern on determination of the offset and non-linear terms from on-orbit
BB measurements is that the controlled BB temperature range is relative small compared to the temperature range used
in prelaunch tests, which could have impacts on the retrieval of brightness temperatures (BT) well outside the calibration
range. In this study, the stability of offset and non-linear terms obtained from BB warm-up/cool-down cycles is
presented. Several approaches to derive the on-orbit offset and non-linear terms are used and their impacts on the Earth
scene BT estimates are examined. By comparison with BT derived using prelaunch offset and nonlinear terms under the
same electronic configuration, it is shown that the current approach of deriving on-orbit offset and nonlinear terms
applied in L1B radiance products causes positive BT biases of exceeding 1K at low temperatures for middle- to longwave
IR bands. Comparison of MODIS and AIRS (The Atmospheric Infrared Sounder), both on-board Aqua spacecraft,
for cold temperature scenes at Antarctica for two long-wave IR bands also indicates that there are temperature-dependent
positive BT biases for about the same magnitudes. Results of this study have a significant impact on improving the current approach of setting a0 and a2 used to produce MODIS L1B data products.
KEYWORDS: Calibration, MODIS, Sensors, Mirrors, Temperature metrology, Electronics, Space operations, Staring arrays, Long wavelength infrared, Black bodies
The Moderate Resolution Imaging Spectroradiometer (MODIS) is a major instrument for NASA's Earth Observing
System (EOS), currently operating on-board the EOS Terra spacecraft, launched in December 1999, and Aqua
spacecraft, launched in May 2002. MODIS is a whiskbroom scanning radiometer using a double-sided paddle wheel
scan mirror. It makes measurements in 36 spectral bands with wavelengths from visible (VIS) to long-wave infrared
(LWIR). Bands 20-25 and 27-36 are the thermal emissive bands (TEB) covering wavelengths from 3.5 to 14.4μm.
During pre-launch thermal vacuum measurements, a laboratory blackbody calibration source (BCS) was used as the
primary calibration source for the TEB. For on-orbit operation, an on-board blackbody (BB) source and a space view
(SV) port are used together for the TEB calibration on a scan-by-scan basis. This paper provides an overview of Terra
and Aqua MODIS pre-launch and on-orbit calibration and characterization activities, methodologies, data analysis
results, and lessons learned for the thermal emissive bands. It focuses on major issues that could impact MODIS TEB
calibration and data quality. Results presented in this paper include detector noise characterization, response versus scan
angle (RVS), and response versus instrument and focal plane temperatures. Similar discussions for the MODIS reflective
solar bands (RSB) are presented in a separate paper in these proceedings (Xiong et. al).
The Moderate Resolution Imaging Spectroradiometer (MODIS) has 36 spectral bands covering wavelengths from 0.41 to 14.4_m. It is a cross-track scanning radiometer that uses a two-sided paddle-wheel scan mirror to make observations over a wide field-of-view (FOV). Each scan of 1.478 seconds, it produces a swath of 10km along-track (at nadir) by 2330km along-scan. Bands 1-19 and 26 are the reflective solar bands (RSB) and bands 20-25 and 27-36 are the thermal emissive bands (TEB). There are a total of 160 detectors (10 detectors per band) for the thermal emissive bands that are calibrated on-orbit by a blackbody (BB) on a scan-by-scan basis. The spectral radiance of each individual TEB detector is calculated every scan from the BB source temperature. The temperature of the BB is measured by a set of 12 thermistors. On-orbit performance of the BB, such as its temperature stability and uncertainty, directly impacts the TEB calibration and data product quality. Excluding a few spacecraft and instrument related anomalies or safe hold events, the Terra MODIS (launched in December 1999) BB has operated continuously on-orbit for more than five years. Using its on-orbit calibration data, this paper examines the Terra MODIS BB performance and its impact on the TEB calibration uncertainty. The results show that the Terra MODIS BB has been performing extremely well in terms of its reliability and stability. Under the same operating configuration, the average BB temperature drift per year (long-term stability) is less than 0.005K. The scan-to-scan temperature variation (short-term stability) is within ±0.03K. Also illustrated in this paper are examples of the TEB detectors' responses to the on-board BB and the detectors' noise characterization results at different BB temperatures.
KEYWORDS: Sensors, Calibration, MODIS, Black bodies, Long wavelength infrared, Near infrared, Mirrors, Electronics, Signal to noise ratio, Spatial resolution
The MODerate Resolution Imaging Spectroradiometer (MODIS) is one of the key instruments for the NASA’s Earth Observing System (EOS). The MODIS ProtoFlight Model (PFM) was launched on-board the EOS Terra spacecraft on December 18, 1999. The science data acquisition started on February 24, 2000. Since then it has been providing the science community and public users unprecedented amount of data sets for the global monitoring of the Earth’s land, oceans, and atmosphere. MODIS has 36 spectral bands with wavelengths ranging from 0.41 micrometer to 14.5 micrometers. Its 16 thermal emissive bands (TEB) range from 3.7 to 14.2 micrometers and have a total of 160 individual detectors (10 detectors per band). The thermal emissive bands are calibrated on-orbit by an on-board calibrator blackbody (OBC BB) on a scan by scan basis. The detectors responses to the BB source track their operational stability and therefore their noise characteristics as well. In this paper, we provide a brief review of the MODIS TEB on-orbit calibration algorithm with a focus on detector stability using over three years of on-orbit calibration data sets. The on-orbit changes in detectors responses from one operational configuration to another, the changes within the same operational condition, and the impact of these changes on the calibration and on the Earth scene observations are carefully examined. Except for a few detectors that were identified from pre-launch or became noisy on-orbit, the overall performance of MODIS TEB detectors is very satisfactory according to the design specifications.
KEYWORDS: Sensors, MODIS, Calibration, Mirrors, Black bodies, Space operations, Imaging systems, Algorithm development, Space mirrors, Detection and tracking algorithms
The MODerate Resolution Imaging Spectroradiometer (MODIS) Flight Model (FM1) was launched on-board the NASA Earth Observing System (EOS)Aqua spacecraft on May 4, 2002. Following initial instrument outgas, focal plane cooling, and functional testing, Aqua MODIS opened its nadir aperture door (NAD) on June 24, 2002 and acquired the first on-orbit image. Modis has 36 spectral bands with wavelengths ranging from 0.412μ to 14.5μ. The 16 thermal emissive bands (B20-25 and 27-36) with wavelengths above 3.5μ are calibrated on-orbit by an on-board calibrator blackbody (OBC BB) on a scan by scan basis. In this paper, we provide a brief review of MODIS thermal emissive bands (TEB) calibration algorithm and present early results from Aqua MODIS on-orbit calibration and characterization, including sensor's response stability, noise assessment, and the response versus scan angle (RVS) difference between the two sides of the scan mirror. In general, the on-orbit performance of Aqua MODIS TEB has been consistent with the instrument pre-launch calibration and characterization. Compared to its Protoflight Model (PFM), or the Terra MODIS, launched on December 18, 1999, a number of improvements have been achieved. During instrument on-orbit operation, the BB can be operated from 270 - 315 K (during scheduled warm-up/cool-down cycle). When the BB temperature is above certain limits, three thermal emissive bands (33, 35, and 36) saturate when directly viewing the calibration source. We have developed an algorithm of using the Look-Up Table (LUT) gain coefficients for these three bands to keep the Earth view data calibrated under this situation. An illustration of on-orbit performance of this approach is provided.
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