MODIS Collection 6.1 (C6.1) is the current official version of its NASA Level-1B (L1B) product, while the Collection (C7) production is presently underway. Amongst the various improvements from its preceding Collections, the most impactful development in C6.1 was the application of a correction to reduce the crosstalk contamination between the MODIS photovoltaic longwave infrared (PV LWIR) bands. In the case of Terra MODIS, such correction was applied via reprocessing to the long-term record, whereas for Aqua MODIS, it was implemented starting March 2022 after the spacecraft and MODIS entered into a safe mode state that significantly increased the crosstalk contamination between the instrument’s PV LWIR bands. In MODIS C7, such correction is applied from mission beginning. Over recent years, both MODIS sensors have seen a gradual crosstalk increase, this in turn has caused drifts across different Earth view scenes despite the correction application, since it can’t completely remove the crosstalk contamination. These drifts are most critical for Aqua band 29 (vastly used by the science community) and Terra band 30. In the case of Aqua MODIS band 29, this is true for both C6.1 and C7, whereas for Terra MODIS band 30, the downward trend is most significant in C6.1 and overcorrected in C7. This led the MODIS Characterization Support Team (MCST) to assess and develop a strategy to reduce these drifts in C7. The methodology involves updating the algorithm used to generate the on-orbit derived calibration coefficients and scaling the crosstalk correction coefficients. However, after several discussions with science teams whose higher-level products ingest the MODIS Level-1B products, the latter was dispensed. The original and revised strategies are discussed. Overall, the agreed upon approach successfully reduces the long-term drifts for all the MODIS PV LWIR bands whose algorithm was updated. Close to pushing the quarter century mark, the Terra and Aqua MODIS legacy instruments will be essential to perpetuate long-term environmental data records after these are superseded by more novel sensors such as VIIRS. Hence the need for the algorithm updates presented in this work to maintain stable data archives.
The MODIS instruments onboard the Terra and Aqua satellites have provided continuous global observations for science research and applications. The calibration accuracy and product quality have been maintained via routine monitoring and characterization of the instrument behavior. Electronic crosstalk in the thermal emissive bands (TEB) is a known issue, and its impact on the calibrated imagery has been mitigated via corrections derived from scheduled lunar observations. Mission-long crosstalk corrections for the Terra MODIS photovoltaic (PV) longwave infrared (LWIR) bands have been applied in Collection 6.1 (C6.1). In recent years, the electronic crosstalk between the Aqua PV LWIR bands has exhibited an increasing downward trend in the crosstalk coefficients. Just like Terra MODIS, this affects the Level-1B (L1B) product’s measurement accuracy and image quality. These artifacts were further amplified after the safe mode event in March 2022. Starting in April 2022, crosstalk corrections have been applied to the Aqua MODIS PV LWIR bands in the Level-1B product. However, due to the uncertainty associated with these crosstalk coefficients, an over- or under-correction was observed in the EV imagery in the form of residual striping. With the development of an Earth image assessment tool, the image striping has been quantified, and a subsequent correction was developed. The crosstalk coefficients for each receiving detector are additionally corrected to maintain the product’s image quality. Lastly, a crosstalk correction for select detectors in the MWIR bands is also applied to both MODIS missions in Collection 7.
The MODIS instrument onboard the Terra and Aqua satellites provides key measurements of various environmental parameters such as the land, ocean, and atmosphere. After over two decades of successful operations, both sensors experienced anomalies in the year 2022. In March, the Aqua spacecraft and, subsequently, the MODIS instrument entered a safe mode, and Terra MODIS experienced a Command Processor and Format Processor (CP/FP) reset. Separately, the Terra constellation exit maneuver (CEM) was performed in October, which included the transition of the MODIS instrument into a safe configuration as well. While MODIS has 16 infrared channels referred to as the thermal emissive bands (TEB), only the longwave infrared bands (27-30) were significantly impacted due to an increase in electronic crosstalk contamination after the Aqua MODIS sensor entered into safe mode. Crosstalk corrections have been applied to these bands to maintain the Level 1B product quality. Although to a lesser extent, the same MODIS bands were affected due to a slight increase in electronic crosstalk contamination after the Terra CEM was completed. Lastly, the Terra MODIS CP/FP reset had an effect on the digital output that transferred onto its photovoltaic bands due to their calibration algorithm. This paper presents the impacts of these events on the instruments’ TEB performance, and the subsequent changes made to their respective calibration algorithms.
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.