What are the greenhouse gas observing system requirements for reducing fundamental biogeochemical process uncertainty? Amazon wetland CH4 emissions as a case study
Item
Title (Dublin Core)
What are the greenhouse gas observing system requirements for reducing fundamental biogeochemical process uncertainty? Amazon wetland CH4 emissions as a case study
Description (Dublin Core)
Understanding the processes controlling terrestrial carbon fluxes is one of the grand challenges of climate science. Carbon cycle process controls are readily studied at local scales, but integrating local knowledge across extremely heterogeneous biota, landforms and climate space has proven to be extraordinarily challenging. Consequently, top-down or integral flux constraints at process-relevant scales are essential to reducing process uncertainty. Future satellite-based estimates of greenhouse gas fluxes – such as CO<sub>2</sub> and CH<sub>4</sub> – could potentially provide the constraints needed to resolve biogeochemical process controls at the required scales. Our analysis is focused on Amazon wetland CH<sub>4</sub> emissions, which amount to a scientifically crucial and methodologically challenging case study. We quantitatively derive the observing system (OS) requirements for testing wetland CH<sub>4</sub> emission hypotheses at a process-relevant scale. To distinguish between hypothesized hydrological and carbon controls on Amazon wetland CH<sub>4</sub> production, a satellite mission will need to resolve monthly CH<sub>4</sub> fluxes at a ∼ 333 km resolution and with a ≤ 10 mg CH<sub>4</sub> m<sup>−2</sup> day<sup>−1</sup> flux precision. We simulate a range of low-earth orbit (LEO) and geostationary orbit (GEO) CH<sub>4</sub> OS configurations to evaluate the ability of these approaches to meet the CH<sub>4</sub> flux requirements. Conventional LEO and GEO missions resolve monthly ∼ 333 km Amazon wetland fluxes at a 17.0 and 2.7 mg CH<sub>4</sub> m<sup>−2</sup> day<sup>−1</sup> median uncertainty level. Improving LEO CH<sub>4</sub> measurement precision by <msqrt>2</msqrt> would only reduce the median CH<sub>4</sub> flux uncertainty to 11.9 mg CH<sub>4</sub> m<sup>−2</sup> day<sup>−1</sup>. A GEO mission with targeted observing capability could resolve fluxes at a 2.0–2.4 mg CH<sub>4</sub> m<sup>−2</sup> day<sup>−1</sup> median precision by increasing the observation density in high cloud-cover regions at the expense of other parts of the domain. We find that residual CH<sub>4</sub> concentration biases can potentially reduce the ∼ 5-fold flux CH<sub>4</sub> precision advantage of a GEO mission to a ∼ 2-fold advantage (relative to a LEO mission). For residual CH<sub>4</sub> bias correlation lengths of 100 km, the GEO can nonetheless meet the ≤ 10 mg CH<sub>4</sub> m<sup>−2</sup> day<sup>−1</sup> requirements for systematic biases ≤ 10 ppb. Our study demonstrates that process-driven greenhouse gas OS simulations can enhance conventional uncertainty reduction assessments by quantifying the OS characteristics required for testing biogeochemical process hypotheses.
Creator (Dublin Core)
Bloom, A. Anthony
Lauvaux, Thomas
Worden, John
Yadav, Vineet
Duren, Riley
Sander, Stanley P.
Schimel, David S.
Date (Dublin Core)
2018-09-19
Type (Dublin Core)
Text
Format (Dublin Core)
application/pdf
Identifier (Dublin Core)
10.5194/acp-16-15199-2016
https://acp.copernicus.org/articles/16/15199/2016/
Source (Dublin Core)
eISSN: 1680-7324
Language (Dublin Core)
eng



