Xie Yuan, Fu Yingdi, Shao Yaqi, Qu Lina, Yang Jiangang, Yang Chengjia, Zhou Kun, Li Kai, Xu Zi, Xu Dong, Cao Kai, Tian Ning, Lv Ke, Wang Linjie, Wang Yaping, Wang Ningli, Li Yinghui
Beijing Tongren Eye Center, Beijing Tongren Hospital, Capital Medical University, Beijing Ophthalmology and Visual Sciences Key Laboratory, Beijing, 100730, China.
Beijing Institute of Ophthalmology, Beijing Tongren Hospital, Capital Medical University, Beijing, 100005, China.
NPJ Microgravity. 2024 Jan 17;10(1):9. doi: 10.1038/s41526-024-00347-x.
The elevation in the optic nerve sheath (ONS) pressure (ONSP) due to microgravity-induced headward fluid shift is the primary hypothesized contributor to SANS. This longitudinal study aims to quantify the axial plane of the optic nerve subarachnoid space area (ONSSA), which is filled with cerebrospinal fluid (CSF) and expands with elevated ONSP during and after head-down tilt (HDT) bed rest (BR). 36 healthy male volunteers (72 eyes) underwent a 90-day strict 6° HDT BR. Without obtaining the pre-HDT data, measurements were performed on days 30, 60, and 90 during HDT and at 6 recovery time points extended to 180-days (R + 180) in a supine position. Portable B-scan ultrasound was performed using the 12 MHz linear array probe binocularly. The measurements of the ONS and the calculation of the ONSSA were performed with ImageJ 1.51 analysis software by two experienced observers in a masked manner. Compared to R + 180, the ONSSA on HDT30, HDT60, and HDT90 exhibited a consistently significant distention of 0.44 mm (95% CI: 0.13 to 0.76 mm, P = 0.001), 0.45 mm (95% CI: 0.15 to 0.75 mm, P = 0.001), and 0.46 mm (95% CI: 0.15 to 0.76 mm, P < 0.001), respectively, and recovered immediately after HDT on R + 2. Such small changes in the ONSSA were below the lateral resolution limit of ultrasound (0.4 mm) and may not be clinically relevant, possibly due to ONS hysteresis causing persistent ONS distension. Future research can explore advanced quantitative portable ultrasound-based techniques and establish comparisons containing the pre-HDT measurements to deepen our understanding of SANS.
由于微重力引起的头部液体上移导致的视神经鞘(ONS)压力(ONSP)升高是太空飞行相关性神经眼科综合征(SANS)的主要假设成因。这项纵向研究旨在量化视神经蛛网膜下腔面积(ONSSA)的轴向平面,该区域充满脑脊液(CSF),并在头低位倾斜(HDT)卧床休息(BR)期间及之后随着ONSP升高而扩大。36名健康男性志愿者(72只眼)接受了为期90天的严格6°HDT BR。在未获取HDT前数据的情况下,于HDT期间的第30天、60天和90天以及仰卧位恢复至180天(R + 180)的6个时间点进行测量。使用12 MHz线性阵列探头双眼进行便携式B超检查。ONS的测量以及ONSSA的计算由两名经验丰富的观察者使用ImageJ 1.51分析软件以盲法进行。与R + 180相比,HDT30、HDT60和HDT90时的ONSSA分别持续显著扩张0.44 mm(95%CI:0.13至0.76 mm,P = 0.001)、0.45 mm(95%CI:0.15至0.75 mm,P = 0.001)和0.46 mm(95%CI:0.15至0.76 mm,P < 0.001),并在HDT后于R + 2时立即恢复。ONSSA的这种微小变化低于超声的横向分辨率极限(0.4 mm),可能与临床无关,这可能是由于ONS滞后导致ONS持续扩张。未来的研究可以探索先进的基于便携式超声的定量技术,并建立包含HDT前测量值的比较,以加深我们对SANS的理解。