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Examining marine particulate or ganic matter at sub-micron scales using scanning transmission X-ray microscopy and carbon X-ray absorption near edge structure spectroscopy

机译:使用扫描透射X射线显微镜和碳X射线吸收近边缘结构光谱法检查亚微米级的海洋微粒或有机物

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Marine sinking particulate organic matter (POM) represents the link between surface primary production and burial of organic matter in marine sediments. As such, the nature of this material has been the subject of numerous studies attempting to characterize its composition. The results of these studies have shown that a significant proportion of POM is not recognizable as known compounds, and that the proportion of uncharacterized material increases with age/depth/diagenesis. However, few studies have examined the spatial heterogeneity of this material. This study uses a new tool, scanning transmission X-ray microscopy (STXM), together with carbon X-ray absorption near edge structure (C-XANES), to examine POM collected from sediment traps deployed at one location in the Arabian Sea as part of the JGOFS program. The results indicate that POM is composed primarily of four distinct phases: protein, an aliphatic rich phase, a carboxylic-acid-rich phase, and a phase with complex unsaturated and quinone character. This last phase may be a condensation product between carbohydrates and proteins, or from degraded plant pigments. Many particles consisted of a single chemical phase; however, in particles with mixed compositions, individual domains retained distinctive chemical signatures at the instrument's resolution limit (50 nm). All major chemical phases were observed in sediment trap particles from 531 to 3369 m depth, supporting the hypothesis that non-selective degradation dominates particle remineralization, and that overall particle compositions are determined by near surface processes. Only one particle, out of more than 60 examined, exhibited soot-like composition. The lack of a significant black carbon/soot component may be attributable to sampling during the winter monsoon period.
机译:海洋下沉的颗粒有机物(POM)代表了海洋沉积物中地表初生与埋藏有机物之间的联系。因此,这种材料的性质已成为试图表征其成分的众多研究的主题。这些研究的结果表明,不可识别的POM中有很大一部分是已知化合物,未表征物质的比例随年龄/深度/成岩作用而增加。但是,很少有研究检查这种材料的空间异质性。这项研究使用了一种新的工具,即扫描透射X射线显微镜(STXM)和边缘结构附近的碳X射线吸收(C-XANES),来检查从部署在阿拉伯海一个地点的沉积物捕集器收集的POM JGOFS程序。结果表明POM主要由四个不同的相组成:蛋白质,富含脂肪族的相,富含羧酸的相和具有复杂的不饱和和醌特征的相。最后一个阶段可能是碳水化合物和蛋白质之间的缩合产物,或来自降解的植物色素。许多颗粒是由一个化学相组成的。但是,在具有混合成分的颗粒中,单个域在仪器的分辨率极限(50 nm)处保留了独特的化学特征。在531至3369 m深度的沉积物捕集颗粒中观察到所有主要化学相,支持以下假设:非选择性降解在颗粒再矿化中占主导地位,并且总体颗粒组成由近地表过程决定。在检查的60多个颗粒中,只有一个颗粒显示出类似烟灰的成分。缺乏大量的黑碳/烟灰成分可能是由于冬季季风期间的采样。

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