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海洋暮光带碳收支的调和。

Reconciliation of the carbon budget in the ocean's twilight zone.

机构信息

1] National Oceanography Centre, University of Southampton, Waterfront Campus, European Way, Southampton SO14 3ZH, UK [2] Ocean and Earth Sciences, University of Southampton, European Way, Southampton SO14 3ZH, UK [3] Institute of Biological and Environmental Sciences, Oceanlab, University of Aberdeen, Newburgh AB41 6AA, UK.

National Oceanography Centre, University of Southampton, Waterfront Campus, European Way, Southampton SO14 3ZH, UK.

出版信息

Nature. 2014 Mar 27;507(7493):480-3. doi: 10.1038/nature13123. Epub 2014 Mar 19.

Abstract

Photosynthesis in the surface ocean produces approximately 100 gigatonnes of organic carbon per year, of which 5 to 15 per cent is exported to the deep ocean. The rate at which the sinking carbon is converted into carbon dioxide by heterotrophic organisms at depth is important in controlling oceanic carbon storage. It remains uncertain, however, to what extent surface ocean carbon supply meets the demand of water-column biota; the discrepancy between known carbon sources and sinks is as much as two orders of magnitude. Here we present field measurements, respiration rate estimates and a steady-state model that allow us to balance carbon sources and sinks to within observational uncertainties at the Porcupine Abyssal Plain site in the eastern North Atlantic Ocean. We find that prokaryotes are responsible for 70 to 92 per cent of the estimated remineralization in the twilight zone (depths of 50 to 1,000 metres) despite the fact that much of the organic carbon is exported in the form of large, fast-sinking particles accessible to larger zooplankton. We suggest that this occurs because zooplankton fragment and ingest half of the fast-sinking particles, of which more than 30 per cent may be released as suspended and slowly sinking matter, stimulating the deep-ocean microbial loop. The synergy between microbes and zooplankton in the twilight zone is important to our understanding of the processes controlling the oceanic carbon sink.

摘要

海洋表层光合作用每年产生约 100 亿吨有机碳,其中 5%至 15%被输出到深海。下沉碳在深海中被异养生物转化为二氧化碳的速度对控制海洋碳储存至关重要。然而,目前仍不确定海洋表层碳供应在多大程度上满足水柱生物群的需求;已知的碳源和汇之间的差异高达两个数量级。在这里,我们通过现场测量、呼吸速率估算和稳态模型,在北大西洋东部的豪猪深海平原站点,使碳源和汇在观测不确定性范围内达到平衡。我们发现,尽管大部分有机碳是以大型、快速下沉颗粒的形式输出的,这些颗粒可供大型浮游动物获取,但在黄昏带(水深 50 至 1000 米)中,原核生物负责估计再矿化作用的 70%至 92%。我们认为,这是因为浮游动物将快速下沉的颗粒破碎并摄入其中的一半,其中超过 30%可能作为悬浮和缓慢下沉的物质释放出来,刺激了深海微生物环。黄昏带中微生物和浮游动物之间的协同作用对于我们理解控制海洋碳汇的过程非常重要。

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