ISS as a Platform for Optical Remote Sensing of Ecosystem Carbon Fluxes: A Case Study Using HICO

dc.contributor.authorHuemmrich, Karl
dc.contributor.authorCampbell, Petya Entcheva
dc.contributor.authorGao, Bo-Cai
dc.contributor.authorFlanagan, Larry B.
dc.contributor.authorGoulden, Michael
dc.date.accessioned2023-07-11T13:53:22Z
dc.date.available2023-07-11T13:53:22Z
dc.date.issued2017-09-26
dc.description.abstractData from the hyperspectral imager for coastal ocean (HICO), mounted on the International Space Station (ISS), were used to develop and test algorithms for remotely retrieving ecosystem productivity. Twenty-six HICO images were used from four study sites representing different vegetation types: grasslands, shrubland, and forest. Gross ecosystem production (GEP) data from eddy covariance were matched with HICO-derived spectra. Multiple algorithms were successful relating spectral reflectance with GEP, including: spectral vegetation indices (SVI), SVI in a light-use efficiency model framework, spectral shape characteristics through spectral derivatives and absorption feature analysis, and statistical models leading to multiband hyperspectral indices from stepwise regressions and partial least squares regression. Successful algorithms were able to achieve r ² better than 0.7 for both GEP at the overpass time and daily GEP. These algorithms were successful using a diverse set of observations combining data from multiple years, multiple times during growing season, different times of day, with different view angles, and different vegetation types. The demonstrated robustness of the algorithms presented in this study over these conditions provides some confidence in mapping spatial patterns of GEP, describing variability within fields, as well as the regional patterns. The ISS orbit provides periods with multiple observations collected at different times of the day within a period of a few days. Diurnal GEP patterns were estimated comparing the half-hourly average GEP from the flux tower against HICO estimates of GEP (r ² = 0.87) if morning, midday, and afternoon observations were available.en_US
dc.description.sponsorshipThe authors would like to thank the HICO Mission Office, D. MacKenzie for the ISS orbital calculations using STK, and D. Landis for graphics help. They would also like to thank B. Law's research team for providing the Marys River AmeriFlux site data, which was supported by the U.S. Department of Energy, Office of Science, under BER Contract DE-FG02-06ER64318.en_US
dc.description.urihttps://ieeexplore.ieee.org/document/8051041en_US
dc.format.extent16 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2l092-igo1
dc.identifier.citationK. F. Huemmrich, P. K. E. Campbell, B.-C. Gao, L. B. Flanagan and M. Goulden, "ISS as a Platform for Optical Remote Sensing of Ecosystem Carbon Fluxes: A Case Study Using HICO," in IEEE Journal of Selected Topics in Applied Earth Observations and Remote Sensing, vol. 10, no. 10, pp. 4360-4375, Oct. 2017, doi: 10.1109/JSTARS.2017.2725825.en_US
dc.identifier.urihttps://doi.org/10.1109/JSTARS.2017.2725825
dc.identifier.urihttp://hdl.handle.net/11603/28571
dc.language.isoen_USen_US
dc.publisherIEEEen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Joint Center for Earth Systems Technology
dc.relation.ispartofUMBC Faculty Collection
dc.relation.ispartofUMBC Geography and Environmental Systems Department
dc.relation.ispartofUMBC GESTAR II
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleISS as a Platform for Optical Remote Sensing of Ecosystem Carbon Fluxes: A Case Study Using HICOen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-4148-9108en_US
dcterms.creatorhttps://orcid.org/0000-0002-0505-4951en_US

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