Sensitivity of solar-induced fluorescence to spectral stray light in high resolution imaging spectroscopy

Loren P. Albert, K. C. Cushman, Yuqin Zong, David W. Allen, Luis Alonso, James R. Kellner

Research output: Contribution to journalArticlepeer-review

6 Scopus citations

Abstract

Remote sensing of solar-induced chlorophyll fluorescence (SIF) advances our ability to monitor gross primary productivity. Because SIF is usually <5% of recorded canopy radiance, sources of measurement error must be reduced for accurate SIF retrieval. Here we quantify the impact of spectral stray light on SIF retrieval using a high-resolution imaging spectrometer. We first derived the FLD retrieval solution in the presence of stray light under the simplifying assumptions that SIF, reflectance, and stray light are constant across the region of the spectrum used in the retrieval. We show that stray light contributions from the canopy and reference spectra could cancel out if obtained from the same instrument. In practice however, the simplifying assumptions are unlikely to hold because SIF and reflectance vary across regions of the spectrum commonly exploited by the FLD retrieval, and stray light can also vary across the spectrum, as we demonstrate with an empirical example. To quantify the impact of spectral stray light on SIF retrievals in more realistic scenarios, we performed a sensitivity analysis. We used a stray light signal distribution function and measurements of spectral radiance and SIF to generate spectra with known quantities of SIF and stray light over four orders of magnitude of stray light. We then quantified the bias in retrieved SIF using four SIF retrieval approaches—standard FLD, 3FLD, a spectral fitting method (SFM), and a method based on singular value decomposition (SVD)—applied to the red and/or far-red spectral domains. We found that spectral stray light can cause either a positive or negative bias in SIF estimates. In the highest stray light scenario, with spectral stray light one order of magnitude smaller than the radiance signal, the stray light error ranged from < ± 1% of SIF (for O2-A band retrievals with FLD, 3FLD, and SFM methods, and for far-red retrievals in the 748 nm to 756 nm domain with SVD-based and 3FLD methods applied to Fraunhofer lines) to >30% of SIF (O2-B band retrieval with SFM, and 3FLD applied to Fraunhofer lines in the red domain). For context, a bias of 27% of SIF is a comparable magnitude to seasonal variation in SIF observed in the Amazon basin, and to SIF differences among plant functional types. However, when spectral stray light was three orders of magnitude smaller than the radiance signal, mean bias was < ± 2% for all retrieval methods. Our analysis informs when spectral stray light corrections must be performed for SIF remote sensing.

Original languageEnglish
Article number113313
JournalRemote Sensing of Environment
Volume285
DOIs
StatePublished - Feb 1 2023
Externally publishedYes

Funding

We are grateful to Christian Frankenberg and Philipp Köhler for sharing Matlab code for SIF retrieval, and to Pablo Morcillo Pallarés for SFM retrieval with our stray light scenarios with the FLUORT toolbox ( https://www.researchgate.net/publication/333245562_FLUORT_a_GUI_FLUOresence_Retrieval_Toolbox_for_automating_and_optimizing_sun-induced_chlorophyll_fluorescence_retrieval_from_spectroscopy_data) under the supervision of Jochem Verrelst and Jose Moreno. The fluorescence imaging spectrometer was acquired using funds provided to JRK by the Institute at Brown for Environment and Society. LPA was supported by a Voss Postdoctoral Fellowship from the Institute at Brown for Environment and Society, with partial support from NASA Award 80NSSC21K1707. We thank Henry Johnson for computational and mechanical support. We thank Stephen Porder and two anonymous NIST reviewers for feedback on the manuscript. The Keck/NASA RELAB at Brown University ( www.planetary.brown.edu/relab/) characterized reflectance of the Spectralon panel used in this study. Part of the imaging spectroscopy data processing was conducted using computational resources and services at the Center for Computation and Visualization, Brown University. We are grateful to Christian Frankenberg and Philipp Köhler for sharing Matlab code for SIF retrieval, and to Pablo Morcillo Pallarés for SFM retrieval with our stray light scenarios with the FLUORT toolbox ( https://www.researchgate.net/publication/333245562_FLUORT_a_GUI_FLUOresence_Retrieval_Toolbox_for_automating_and_optimizing_sun-induced_chlorophyll_fluorescence_retrieval_from_spectroscopy_data ) under the supervision of Jochem Verrelst and Jose Moreno. The fluorescence imaging spectrometer was acquired using funds provided to JRK by the Institute at Brown for Environment and Society. LPA was supported by a Voss Postdoctoral Fellowship from the Institute at Brown for Environment and Society, with partial support from NASA Award 80NSSC21K1707. We thank Henry Johnson for computational and mechanical support. We thank Stephen Porder and two anonymous NIST reviewers for feedback on the manuscript. The Keck/NASA RELAB at Brown University ( www.planetary.brown.edu/relab/ ) characterized reflectance of the Spectralon panel used in this study. Part of the imaging spectroscopy data processing was conducted using computational resources and services at the Center for Computation and Visualization, Brown University.

FundersFunder number
National Aeronautics and Space Administration80NSSC21K1707
Brown University

    Keywords

    • Chlorophyll fluorescence
    • Near-surface remote sensing
    • Sensor characterization
    • Spectral imaging
    • Stray light

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