Beyond the visible: Accounting for ultraviolet and far‐red radiation in vegetation productivity and surface energy budgets
Abstract
Photosynthetically active radiation (PAR) is typically defined as light with a wavelength within 400–700 nm. However, ultra-violet (UV) radiation within 280–400 nm and far-red (FR) radiation within 700–750 nm can also excite photosystems, though not as efficiently as PAR. Vegetation and land surface models (LSMs) typically do not explicitly account for UV's contribution to energy budgets or photosynthesis, nor FR's contribution to photosynthesis. However, whether neglecting UV and FR has significant impacts remains unknown. We explored how canopy radiative transfer (RT) and photosynthesis are impacted when explicitly implementing UV in the canopy RT model and accounting for UV and FR in the photosynthesis models within a next-generation LSM that can simulate hyperspectral canopy RT. We validated our improvements using photosynthesis measurements from plants under different light sources and intensities and surface reflection from an eddy-covariance tower. Our model simulations suggested that at the whole plant level, after accounting for UV and FR explicitly, chlorophyll content, leaf area index (LAI), clumping index, and solar radiation all impact the modeling of gross primary productivity (GPP). At the global scale, mean annual GPP within a grid would increase by up to 7.3% and the increase is proportional to LAI; globally integrated GPP increases by 4.6 PgC year−1 (3.8% of the GPP without accounting for UV + FR). Further, using PAR to proxy UV could overestimate surface albedo by more than 0.1, particularly in the boreal forests. Our results highlight the importance of improving UV and FR in canopy RT and photosynthesis modeling and the necessity to implement hyperspectral or multispectral canopy RT schemes in future vegetation and LSMs.
Copyright and License
© 2024 John Wiley & Sons.
Copyright and License
This research has been supported by the National Aeronautics and Space Administration (NASA) Carbon Cycle Science grant 80NSSC21K1712 and OCO2/3 Science Team 80NSSC21K1075 awarded to CF. CF acknowledges support from Schmidt Sciences, LLC. This research was partially carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. This material is based on the MOFLUX site supported by the U.S. Department of Energy, Office of Science, Office of Biological and Environmental Research Program, Climate and Environmental Sciences Division through Oak Ridge National Laboratory's Terrestrial Ecosystem Science Scientific Focus Area. We appreciate the constructive suggestions provided by the anonymous reviewers. California Institute of Technology. Government sponsorship acknowledged (Copyright 2024. All rights reserved).
Data Availability
The version of CliMA Land used to run global simulations (simulation tag “a12”) is openly available in Zenodo at https://doi.org/10.5281/zenodo.10652942 (CliMA Land Team, 2024a). The data that support the findings of this study are available in Zenodo at https://doi.org/10.5281/zenodo.10652972 (CliMA Land Team, 2024b). Global datasets used to feed to CliMA Land and perform the analysis can be accessed at https://data.caltech.edu/records/mwhhr-0rq03 and https://doi.org/10.5281/zenodo.8345558 or by using GriddingMachine (https://github.com/CliMA/GriddingMachine.jl).
Conflict of Interest
The authors declare no conflict of interest.
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Additional details
- ISSN
- 1365-2486
- National Aeronautics and Space Administration
- 80NSSC21K1712
- National Aeronautics and Space Administration
- 80NSSC21K1075
- Schmidt Family Foundation
- Jet Propulsion Laboratory
- United States Department of Energy
- Caltech groups
- Division of Geological and Planetary Sciences