More Frequent Spaceborne Sampling of XCO2 Improves Detectability of Carbon Cycle Seasonal Transitions in Arctic-Boreal Ecosystems

Nicholas C Parazoo, Gretchen Keppel-Aleks, Stanley Sander, Brendan Byrne, Vijay Natraj, Mingzhao Luo, Jean-Francois Blavier, Leonard Dorsky, Ray Nassar
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Abstract

Surface, aircraft, and satellite measurements indicate pervasive cold season CO2 emissions across Arctic regions, consistent with a hyperactive biosphere and increased metabolism in plants and soils. A key remaining question is whether cold season sources will become large enough to permanently shift the Arctic into a net carbon source. Polar orbiting GHG satellites provide robust estimation of regional carbon budgets but lack sufficient spatial coverage and repeat frequency to track sink-to-source transitions in the early cold season. Mission concepts such as the Arctic Observing Mission (AOM) advocate for flying imaging spectrometers in highly elliptical orbits (HEO) over the Arctic to address sampling limitations. We perform retrieval and flux inversion simulation experiments using the AURORA mission concept, leveraging a Panchromatic imaging Fourier Transform Spectrometer (PanFTS) in HEO. AURORA simulations demonstrate the benefits of increased CO2 sampling for detecting spatial gradients in cold season efflux and improved monitoring of rapid Arctic change.
更频繁的XCO2星载采样提高了北极-北方生态系统碳循环季节转换的可探测性
地面、飞机和卫星测量表明,北极地区普遍存在寒冷季节的二氧化碳排放,这与生物圈过度活跃以及植物和土壤代谢增加相一致。剩下的一个关键问题是,寒冷季节的碳源是否会变得足够大,从而永久地将北极变成一个净碳源。极轨温室气体卫星提供了对区域碳收支的可靠估计,但缺乏足够的空间覆盖和重复频率来跟踪冷季早期的汇源转换。像北极观测任务(AOM)这样的任务概念提倡在北极上空的高椭圆轨道(HEO)上飞行成像光谱仪,以解决采样限制。利用HEO中的全色成像傅立叶变换光谱仪(PanFTS),利用AURORA任务概念进行检索和通量反演模拟实验。AURORA模拟表明,增加CO2采样对于探测寒冷季节外排的空间梯度和改进对北极快速变化的监测是有益的。
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