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首页> 外文期刊>Marine ecology progress series >Abundance, oxygen consumption and carbon demand of brittle stars in Young Sound and the NE Greenland shelf
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Abundance, oxygen consumption and carbon demand of brittle stars in Young Sound and the NE Greenland shelf

机译:Young Sound和东北格陵兰大陆架的脆性恒星的丰度,耗氧量和碳需求

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ABSTRACT: We used sea floor photography to estimate brittle star abundance in Young Sound, NE Greenland and the adjacent shelf. From photos covering a total area of 78 m2 and spanning a depth range from 20 to 310 m we found maximum average densities of 400 ind. m–2 at 40 to 80 m depth. Ophiocten sericeum was the dominant species. However, gradual changes in species and size composition with depth were observed. Average biomass was ~600 mg C m–2 with highest values at sites dominated by the large Ophiopleura borealis (up to 2190 mg C m–2). We measured average individual oxygen consumption of 3 dominant species at ambient temperature (–1.0°C) and salinity in incubation chambers using a fiber-optic oxygen sensor enabling continuous measurements. We established a general relation between individual disc diameter (D, mm) and oxygen consumption (R, µmol O2 h–1 ind.–1): R = 6.0 × 10–4 × D2.60 (R2 = 0.96, n = 33), which facilitated the estimation of community respiration and carbon demand from sea floor images. Peaks in total carbon demand were found in the fjord at 30 m (14 mg C m–2 d–1) and 160 m depth (13 mg C m–2 d–1), resulting from high densities of medium sized (10 to 15 mm disc diameter) O. sericeum, and the presence of the very large (20 to 35 mm disc diameter) O. borealis, respectively. At the other stations values ranged from 0.5 to 8 mg C m–2 d–1. Overall, our results demonstrate that brittle stars, despite very low individual energy requirements, contribute significantly to marine carbon cycling in Young Sound as well as in the shelf areas off NE Greenland.
机译:摘要:我们使用海床摄影技术来估算扬德湾,格陵兰东北部和邻近大陆架的脆性恒星丰度。从覆盖总面积为78 m 2 且深度范围为20到310 m的照片中,我们发现最大平均密度> 400 ind。 m –2 在40至80 m深度处。 Ophiocten sericeum 是优势种。然而,观察到物种和大小组成随深度的逐渐变化。平均生物量为〜600 mg C m –2 ,在以 Ophiopleura northalis 为主的部位最高(最高至2190 mg C m –2 )。我们使用能够连续测量的光纤氧气传感器,测量了环境温度(–1.0°C)和温育箱中盐度的三种主要物种的平均个体氧气消耗量。我们建立了单个椎间盘直径( D ,mm)和耗氧量( R ,µmol O 2 h –1之间的一般关系 ind。 –1 ): R = 6.0×10 –4 × D 2.60 (R 2 = 0.96,n = 33),这有助于根据海床图像估算群落呼吸和碳需求。峡湾的总碳需求峰值在30 m(14 mg C m –2 d –1 )和160 m深度(13 mg C m –2 d –1 ),是由于中等尺寸(圆盘直径10至15 mm) O的密度高所致。并有很大的(直径为20至35毫米的椎间盘) O。北极在其他站点,值范围从0.5到8 mg C m –2 d –1 。总体而言,我们的结果表明,尽管单个恒星的能量消耗非常低,但脆性星还是对Young Sound以及东北格陵兰岛的陆架碳循环起了重要作用。

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