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Physical and ecological factors explain the distribution of Ross Sea Weddell seals during the breeding season

机译:物理和生态因素解释了繁殖季节Ross Sea Weddell海豹的分布

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Weddell seal Leptonychotes weddellii populations can potentially serve as indicators of change in Southern Ocean food web structure, but tracking populations at regional to continental scales has so far been impossible. Here, we combined citizen science with remote sensing to learn about environmental and biological factors that explain fine-scale distribution of Weddell seal haul-outs in the Ross Sea, Antarctica. We employed the crowd-sourcing platform Tomnod (DigitalGlobe) to host high-resolution (similar to 0.5-0.6 m) satellite imagery of the Antarctic fast ice during November in 2010 and 2011 and asked volunteers to identify seals on images. We created a 5 km x 5 km grid of seal presence per year, and modeled habitat suitability for seals using a generalized linear model. The top Ross Sea-wide model that best explained seal presence included proximity to fast-ice cracks, deep water, and emperor penguin Aptenodytes forsteri colonies. This model also revealed that seal presence decreased with proximity to Adelie penguin Pygoscelis adeliae colonies and size of the nearest emperor penguin colony, suggesting the potential for trophic competitive exclusion by large penguin colonies. With respect to 3 sub-regions within the Ross Sea (North and South Victoria Land in the western Ross Sea, and Marie Byrd Land in the east), we found that 3 habitat variables differed in their effects among sub-regions: proximity to emperor penguin colonies, proximity to deep water, and relative ice width. Our results represent a step toward effectively monitoring Weddell seal population trends, and disentangling biological and environmental factors influencing locations of Weddell seal haul-outs around Antarctica.
机译:Weddell海豹Leptonychotes weddellii种群有可能成为南部海洋食物网结构变化的指标,但迄今为止,不可能在区域到大陆范围内追踪种群。在这里,我们将公民科学与遥感相结合,以了解环境和生物因素,这些因素解释了南极罗斯海的韦德尔海豹捕捞活动的精细分布。我们利用众包平台Tomnod(DigitalGlobe)于2010年和2011年11月托管了南极快冰的高分辨率(约0.5-0.6 m)卫星图像,并请志愿者在图像上标识海豹。我们每年创建一个5 km x 5 km的海豹存在网格,并使用广义线性模型对海豹的栖息地适应性进行建模。能够最好地解释海豹存在的顶级罗斯海宽模型包括靠近速冻裂缝,深水和帝企鹅Aptenodytes forsteri殖民地。该模型还显示,海豹的存在随着靠近阿德利企鹅Pygoscelis adeliae菌落和最近的帝王企鹅菌落的大小而减少,这表明大企鹅菌落有可能被营养性竞争排斥。关于罗斯海中的3个子区域(西部罗斯海的北部和南部维多利亚州土地,以及东部的玛丽·伯德土地),我们发现3个栖息地变量在这些子区域中的影响有所不同:接近皇帝企鹅殖民地,靠近深水的地方以及相对的冰宽。我们的结果代表了朝着有效监测Weddell海豹种群趋势迈出的一步,并解开了影响南极洲Weddell海豹出没地点的生物学和环境因素。

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