Inferring Photosynthetic Light-Use Efficiency of Terrestrial Ecosystems from Multi-angular Satellite Observations.
Thomas
Hilker, UMBC /NASA GSFC, thomas.hilker@nasa.gov
(Presenter)
Terrestrial ecosystems absorb about 2.8 Gt C yr-1 which is estimated to be about a quarter of the carbon emitted from fossil fuel combustion. However, the uncertainties of this sink are large, in the order of +- 40%, with spatial and temporal variations largely unknown. One of the largest factors contributing to the uncertainty is photosynthesis, the process by which plants absorb carbon from the atmosphere. Currently, photosynthesis – as related by gross primary productivity (GPP) – can only be observed from flux-towers measuring the exchange of CO2 in the surrounding air column, and, consequently, existing carbon models suffer from a lack of spatial coverage of accurate GPP observations. Here, we show that photosynthetic light-use efficiency (ε) and hence photosynthesis can be directly measured in a spatially continuous mode from space. We demonstrate that the differential between spectral wavebands associated with the vegetation xanthophyll cycle and estimates of canopy shading obtained from multi-angular satellite observations allows direct and accurate measurements of plant photosynthesis, independently of vegetation type and structure. This is a significant advance over previous approaches seeking to model global scale photosynthesis indirectly from a combination of growth limiting factors, most notably pressure deficit and temperature. Direct observations of ε and GPP can be used in a data assimilation mode to provide regularly timed calibration points for continuous modeling of plant photosynthesis at a global scale. Presentation: 2011_Poster_Hilker_35_296.pdf (2072k) Presentation Type: Poster Session: Coupled Processes at Land-Atmosphere-Ocean Interfaces (Mon 4:00 PM) Associated Project(s):
Poster Location ID: 35
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