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Otolith microstructural and microchemical changes associated with settlement in the diadromous fish Galaxias maculatus

机译:溢水鱼类银耳的沉降相关的耳石微结构和微化学变化

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摘要

The presence of a settlement mark in the otoliths of the common galaxid Galaxias maculatus was validated by examining the relationship between changes in otolith microstructure and otolith microchemistry. Two methods were used to examine the microchemistry of otoliths: (1) laser-ablation multi-collector inductively-coupled plasma mass spectrometry (LA-MC-ICPMS) to examine changes in Sr isotope ratios, and (2) laser-ablation inductively-coupled-plasma mass spectrometry (LA-ICPMS) to examine changes in Ba/Ca and Sr/Ca. Both analytical techniques detected changes in otolith microchemistry consistent with movement from oceans into rivers (settlement). There was a strong correlation between the timing of settlement as indicated by otolith microstructure and both Sr-based methods; however, Ba/Ca was a less reliable marker of settlement for this species. These results support the use of this settlement mark for further otolith based studies of age, growth and the reconstruction of settlement histories in C. maculatus and demonstrate the potential utility of otolith microchemistry as a method for validating settlement marks in other diadromous fish.
机译:通过检查耳石微结构变化与耳石微化学之间的关系,验证了常见星系Galaxias maculatus耳石中是否存在沉降标记。两种方法被用来检验耳石的微化学:(1)激光烧蚀多收集器电感耦合等离子体质谱法(LA-MC-ICPMS)来检测Sr同位素比的变化,以及(2)激光烧蚀感应法耦合等离子体质谱(LA-ICPMS)来检查Ba / Ca和Sr / Ca的变化。两种分析技术都检测到耳石微化学的变化,这与从海洋向河流的迁移(沉降)一致。耳石微结构表明的沉降时间与两种基于Sr的方法之间都有很强的相关性。但是,Ba / Ca并不是该物种定居的可靠标志。这些结果支持该沉降标记用于进一步基于耳石的年龄,生长和定居史的重建研究中的使用,并证明了耳石微化学作为一种验证其他过缺鱼类中的沉降标志的方法的潜在用途。

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