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终点变化不是眼跳适应中的噪声。

End-point variability is not noise in saccade adaptation.

机构信息

Department of Biology, The City College of New York, New York, New York, United States of America.

出版信息

PLoS One. 2013;8(3):e59731. doi: 10.1371/journal.pone.0059731. Epub 2013 Mar 21.

DOI:10.1371/journal.pone.0059731
PMID:23555763
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC3605199/
Abstract

When each of many saccades is made to overshoot its target, amplitude gradually decreases in a form of motor learning called saccade adaptation. Overshoot is induced experimentally by a secondary, backwards intrasaccadic target step (ISS) triggered by the primary saccade. Surprisingly, however, no study has compared the effectiveness of different sizes of ISS in driving adaptation by systematically varying ISS amplitude across different sessions. Additionally, very few studies have examined the feasibility of adaptation with relatively small ISSs. In order to best understand saccade adaptation at a fundamental level, we addressed these two points in an experiment using a range of small, fixed ISS values (from 0° to 1° after a 10° primary target step). We found that significant adaptation occurred across subjects with an ISS as small as 0.25°. Interestingly, though only adaptation in response to 0.25° ISSs appeared to be complete (the magnitude of change in saccade amplitude was comparable to size of the ISS), further analysis revealed that a comparable proportion of the ISS was compensated for across conditions. Finally, we found that ISS size alone was sufficient to explain the magnitude of adaptation we observed; additional factors did not significantly improve explanatory power. Overall, our findings suggest that current assumptions regarding the computation of saccadic error may need to be revisited.

摘要

当许多扫视中的每一次扫视都超过目标时,幅度会逐渐减小,这种现象被称为扫视适应。超调是通过次要的、向后的扫视内目标步(ISS)实验诱导的,该步由主要扫视触发。然而,令人惊讶的是,没有研究比较不同大小的 ISS 在通过系统地在不同的会话中改变 ISS 幅度来驱动适应方面的有效性。此外,很少有研究检验相对较小的 ISS 适应的可行性。为了在基本层面上最好地理解扫视适应,我们在一个实验中使用一系列小的固定 ISS 值(在 10°主要目标步之后为 0°至 1°)来解决这两个问题。我们发现,即使 ISS 小至 0.25°,在受试者中也会发生显著的适应。有趣的是,尽管只有对 0.25° ISS 的适应似乎是完全的(扫视幅度的变化幅度与 ISS 的大小相当),但进一步的分析表明,在不同条件下,ISS 被补偿的比例相当。最后,我们发现,ISS 大小本身足以解释我们观察到的适应幅度;其他因素并没有显著提高解释能力。总的来说,我们的发现表明,当前关于扫视误差计算的假设可能需要重新考虑。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/d8ae4c383624/pone.0059731.g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/87739c52ae5e/pone.0059731.g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/98287096ed85/pone.0059731.g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/50d7dce763d6/pone.0059731.g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/748930fe6f6a/pone.0059731.g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/d8ae4c383624/pone.0059731.g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/87739c52ae5e/pone.0059731.g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/98287096ed85/pone.0059731.g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/50d7dce763d6/pone.0059731.g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/748930fe6f6a/pone.0059731.g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/11fa/3605199/d8ae4c383624/pone.0059731.g005.jpg

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