在引力和姿势变化下的视网膜血液动力学计算模型
Michele Nigro1,2, Andrea Montanino1,3, Eduardo Soudah1,2
1International Center for Numerical Methods in Engineering (CIMNE), Barcelona, Spain.
The Journal of physiology
|February 25, 2026
概括
与太空飞行相关的神经眼综合征 (SANS) 的风险可以通过新模型更好地理解. 这个工具模拟了太空飞行期间的眼睛变化,揭示了液体变化如何影响视网膜血流和眼内压力.
科学领域:
- 眼科医生 眼科 眼科
- 航空航天医学 航空航天医学
- 生物医学工程 生物医学工程
背景情况:
- 太空飞行相关的神经眼综合征 (SANS) 给宇航员带来了风险,原因是人们对视网膜变化的了解不足.
- 眼球循环和眼内压力 (IOP) 受到微重力和姿势变化的显著影响.
研究的目的:
- 开发和验证一个计算模型模拟视网膜血液动力学在改变的引力条件下.
- 调查与SANS相关的连接液态变化,内压变化和视网膜血流变化的机制.
主要方法:
- 创建了一个块式参数模型,将五个分区的视网膜血管网络与动态IOP模块集成在一起.
- 模拟了向下倾斜的实验,以模拟微重力诱导的头部液体移动.
- 模型输出与内压,眼 perfusion 压力和视网膜血流的实验数据进行了验证.
主要成果:
- 在头向下倾斜时,模拟的内血压增加了81%,而眼球 perfusion 压力保持稳定.
- 视网膜血流预测与体内多普勒测量结果一致.
- 中央视网膜动脉和动脉分段被确定为最容易受到机械应力的影响.
结论:
- 经过验证的模型通过整合视网膜和眼睛生物力学,提供了对SANS病原学的机制性见解.
- 它建立了对抗措施的定量门,并有助于了解陆地眼部疾病.
- 该模型作为研究眼和高血压视网膜病变的可转移工具.
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