Estimation of Vegetation Photosynthetic Capacity from Space-Based Measurements of Chlorophyll Fluorescence for Terrestrial Biosphere Models.

摘要

Photosynthesis simulations by terrestrial biosphere models are usually based on the Farquhar's model, in which the maximum rate of carboxylation V (sub CMAX) is a key control parameter of photosynthetic capacity. Even though V (sub CMAX) is known to vary substantially in space and time in response to environmental controls, it is typically parameterized in models with tabulated values associated to plant functional types. Remote sensing can be used to produce a spatially continuous and temporally resolved view on photosynthetic efficiency, but traditional vegetation observations based on spectral reflectance lack a direct link to plant photochemical processes. Alternatively, recent space-borne measurements of sun-induced chlorophyll fluorescence (SIF) can offer an observational constraint on photosynthesis simulations. Here, we show that top-of-canopy SIF measurements from space are sensitive to V (sub CMAX) at the ecosystem level, and present an approach to invert V (sub CMAX) from SIF data. We use the Soil-Canopy Observation of Photosynthesis and Energy (SCOPE) balance model to derive empirical relationships between seasonal Vcmax and SIF which are used to solve the inverse problem. We evaluate our V (sub CMAX) method at six agricultural flux tower sites in the midwestern US using spaced-based SIF retrievals. Our V (sub CMAX) estimates agree well with literature values for corn and soybean plants (average values of 37 and 101 micron mol m (exp-2)s(exp-1), respectively) and show plausible seasonal patterns. The effect of the updated seasonally varying V (sub CMAX) parameterization on simulated gross primary productivity (GPP) is tested by comparing to simulations with fixed V (sub CMAX) values. Validation against flux tower observations demonstrate that simulations of GPP and light use efficiency improve significantly when our time-resolved V (sub CMAX) estimates from SIF are used, with R2 for GPP comparisons increasing from 0.85 to 0.93, and for light use efficiency from 0.44 to 0.83. Our results support the use of space-based SIF data as a proxy for photosynthetic capacity and suggest the potential for global, time-resolved estimates of V (sub CMAX).