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Orbiting Carbon Observatory-2 (OCO-2) cloud screening algorithms: validation against collocated MODIS and CALIOP data

Taylor, Thomas E. and O'Dell, Christopher W. and Frankenberg, Christian and Partain, Philip T. and Cronk, Heather Q. and Savtchenko, Andrey and Nelson, Robert R. and Rosenthal, Emily J. and Chang, Albert Y. and Fisher, Brenden and Osterman, Gregory B. and Pollock, Randy H. and Crisp, David and Eldering, Annmarie and Gunson, Michael R. (2016) Orbiting Carbon Observatory-2 (OCO-2) cloud screening algorithms: validation against collocated MODIS and CALIOP data. Atmospheric Measurement Techniques, 9 (3). pp. 973-989. ISSN 1867-8548. https://resolver.caltech.edu/CaltechAUTHORS:20200529-093433107

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Abstract

The objective of the National Aeronautics and Space Administration's (NASA) Orbiting Carbon Observatory-2 (OCO-2) mission is to retrieve the column-averaged carbon dioxide (CO₂) dry air mole fraction (XCO2) from satellite measurements of reflected sunlight in the near-infrared. These estimates can be biased by clouds and aerosols, i.e., contamination, within the instrument's field of view. Screening of the most contaminated soundings minimizes unnecessary calls to the computationally expensive Level 2 (L2) X_(CO₂) retrieval algorithm. Hence, robust cloud screening methods have been an important focus of the OCO-2 algorithm development team. Two distinct, computationally inexpensive cloud screening algorithms have been developed for this application. The A-Band Preprocessor (ABP) retrieves the surface pressure using measurements in the 0.76 µm O₂ A band, neglecting scattering by clouds and aerosols, which introduce photon path-length differences that can cause large deviations between the expected and retrieved surface pressure. The Iterative Maximum A Posteriori (IMAP) Differential Optical Absorption Spectroscopy (DOAS) Preprocessor (IDP) retrieves independent estimates of the CO₂ and H₂O column abundances using observations taken at 1.61 µm (weak CO₂ band) and 2.06 µm (strong CO₂ band), while neglecting atmospheric scattering. The CO₂ and H₂O column abundances retrieved in these two spectral regions differ significantly in the presence of cloud and scattering aerosols. The combination of these two algorithms, which are sensitive to different features in the spectra, provides the basis for cloud screening of the OCO-2 data set. To validate the OCO-2 cloud screening approach, collocated measurements from NASA's Moderate Resolution Imaging Spectrometer (MODIS), aboard the Aqua platform, were compared to results from the two OCO-2 cloud screening algorithms. With tuning of algorithmic threshold parameters that allows for processing of  ≃ 20–25 % of all OCO-2 soundings, agreement between the OCO-2 and MODIS cloud screening methods is found to be  ≃ 85 % over four 16-day orbit repeat cycles in both the winter (December) and spring (April–May) for OCO-2 nadir-land, glint-land and glint-water observations. No major, systematic, spatial or temporal dependencies were found, although slight differences in the seasonal data sets do exist and validation is more problematic with increasing solar zenith angle and when surfaces are covered in snow and ice and have complex topography. To further analyze the performance of the cloud screening algorithms, an initial comparison of OCO-2 observations was made to collocated measurements from the Cloud-Aerosol Lidar with Orthogonal Polarization (CALIOP) aboard the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO). These comparisons highlight the strength of the OCO-2 cloud screening algorithms in identifying high, thin clouds but suggest some difficulty in identifying some clouds near the surface, even when the optical thicknesses are greater than 1.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.5194/amt-9-973-2016DOIArticle
ORCID:
AuthorORCID
Taylor, Thomas E.0000-0002-1650-4882
Frankenberg, Christian0000-0002-0546-5857
Nelson, Robert R.0000-0002-3471-5683
Crisp, David0000-0002-4573-9998
Eldering, Annmarie0000-0003-1080-9922
Additional Information:© Author(s) 2016. This work is distributed under the Creative Commons Attribution 3.0 License. Received: 22 Oct 2015 – Discussion started: 04 Dec 2015 – Revised: 02 Feb 2016 – Accepted: 03 Feb 2016 – Published: 08 Mar 2016. The CSU contribution to this work was supported by JPL subcontract 1439002. A portion of the research described in this paper was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. We would like to acknowledge the hard work of those individuals on the OCO-2 algorithm and data processing teams whose efforts helped make this work possible. The list (in alphabetical order) includes (but is not limited to) Charlie Avis, Lars Chapsky, Lan Dang, Robert Granat, Richard Lee, Lukas Mandrake, James McDuffie, Vijay Natraj, Fabian Oyafuso, Vivienne Payne, Rob Rosenberg, Mike Smyth, Paul Wennberg, Debra Wunch and Jia Zong, all at JPL. We would also like to acknowledge the contributions made by the GOSAT JAXA and NIES teams that made this research possible. In addition we thank the computer support staff at CSU, Natalie Tourville and Michael Hiatt. Finally, we thank the two anonymous reviewers and the journal editor and staff who provided useful comments and helped typeset the manuscript. Edited by: A. Kokhanovsky
Funders:
Funding AgencyGrant Number
JPL1439002
NASA/JPL/CaltechUNSPECIFIED
Issue or Number:3
Record Number:CaltechAUTHORS:20200529-093433107
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200529-093433107
Official Citation:Taylor, T. E., O'Dell, C. W., Frankenberg, C., Partain, P. T., Cronk, H. Q., Savtchenko, A., Nelson, R. R., Rosenthal, E. J., Chang, A. Y., Fisher, B., Osterman, G. B., Pollock, R. H., Crisp, D., Eldering, A., and Gunson, M. R.: Orbiting Carbon Observatory-2 (OCO-2) cloud screening algorithms: validation against collocated MODIS and CALIOP data, Atmos. Meas. Tech., 9, 973–989, https://doi.org/10.5194/amt-9-973-2016, 2016.
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103554
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:01 Jun 2020 14:30
Last Modified:01 Jun 2020 14:30

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