Hui Shen , Xianhui S. Wan , Wenbin Zou , Mingming Chen , Zhendong Hu , Senwei Tong , Kuanbo Zhou , Zong-Pei Jiang , Yao Zhang , Minhan Dai , Shuh-Ji Kao
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引用次数: 0
Abstract
Nitrogen fixation is a vital new nitrogen source in the oligotrophic ocean. Although our knowledge of the controlling factors of marine nitrogen fixation have increased rapidly, the physical controls, particularly eddies-induced upwelling and light intensity, remain elusive. In this study, conducted in the Subtropical Northwestern Pacific, we measured nitrogen fixation rates (NFR) in two cyclonic eddies (CEs). Our observations in one CE revealed that depth-integrated NFR (INFR) in core stations were significantly higher than in edge stations, indicating that CEs-induced upwelling might enhance nitrogen fixation. However, more intense upwelling in another CE resulted in lower INFR in core stations compared to edge stations. The INFR distributions in CEs were driven by the upwelling intensity, showing a unimodal response, i.e., the maximum INFR appeared at optimal upwelling intensity. This finding reconciles the debate about whether CEs inhibit nitrogen fixation. Additionally, results from light manipulation incubations proved that light intensity is a key driver for the vertically unimodal pattern of NFR, i.e., peaks at the subsurface layer with an optimum light intensity of 20% to 50% of surface PAR. Furthermore, molecular evidence showed that UCYN-A dominated in the upwelling area, while UCYN-B dominated in the non-upwelling area, indicating that CEs-induced physical perturbation regulates the niches of diazotrophs. Taken together, these results suggest that physical dynamics exert profound controls on the spatial heterogeneity of diazotrophic distribution and activity in the Subtropical Northwestern Pacific, providing new insights into the physical drivers of nitrogen fixation on mesoscale hydrodynamics..
固氮是寡营养海洋中一个重要的新氮源。虽然我们对海洋固氮控制因素的了解迅速增加,但物理控制因素,特别是漩涡引起的上升流和光照强度,仍然难以捉摸。本研究在亚热带西北太平洋进行,我们测量了两个气旋漩涡(CEs)的固氮率(NFR)。我们在一个气旋漩涡中的观测结果表明,核心站的深度整合固氮率(INFR)明显高于边缘站,这表明气旋漩涡引起的上升流可能会促进固氮作用。然而,在另一个 CE 中,更强烈的上升流导致核心站的 INFR 低于边缘站。CE中的INFR分布受上升流强度的影响,呈现单峰响应,即在最佳上升流强度时INFR最大。这一发现调和了 CE 是否抑制固氮作用的争论。此外,光照操作培养的结果证明,光照强度是 NFR 垂直单峰模式的关键驱动因素,即在地表层下出现峰值,最佳光照强度为地表 PAR 的 20% 至 50%。此外,分子证据表明,UCYN-A 在上升流区占优势,而 UCYN-B 在非上升流区占优势,这表明 CEs 诱导的物理扰动调节了重氮营养盐的龛位。总之,这些结果表明,物理动力学对西北太平洋亚热带重氮营养体分布和活动的空间异质性具有深刻的控制作用,为中尺度水动力固氮的物理驱动因素提供了新的见解。
期刊介绍:
Progress in Oceanography publishes the longer, more comprehensive papers that most oceanographers feel are necessary, on occasion, to do justice to their work. Contributions are generally either a review of an aspect of oceanography or a treatise on an expanding oceanographic subject. The articles cover the entire spectrum of disciplines within the science of oceanography. Occasionally volumes are devoted to collections of papers and conference proceedings of exceptional interest. Essential reading for all oceanographers.