对于Vogt-Koyanagi-Harada疾病中的夕阳光底的初次访问时的预测因素
Tetsuya Muto1,2,3, Masaaki Sakamoto4, Shigeki Machida4
1Department of Ophthalmology, Dokkyo Medical University Saitama Medical Center, Koshigaya, 343-8555, Japan. ueda.castle@gmail.com.
Scientific reports
|July 7, 2025
概括
在Vogt-Koyanagi-Harada (VKH) 疾病中的日落发光 (SGF) 与吸烟史,视力敏度和前段特征等初次访问因素有关. 早期识别这些风险因素对于管理VKH疾病至关重要.
科学领域:
- 眼科医生 眼科 眼科
- 免疫学 免疫学 免疫学
- 医学诊断 医学诊断 医学诊断
背景情况:
- 沃格特-科亚纳吉-哈拉达病 (VKH) 是一种影响眼组织的全身性炎症状况.
- 夕阳发光底部 (Sunset glow fundus,SGF) 是VKH疾病中发现的一种特征性底部,通常与视力障碍有关.
- 识别SGF的早期预测因素对于及时干预和改善患者结果至关重要.
研究的目的:
- 确定与未经治疗的VKH疾病患者中SGF发展相关的初次诊断临床和人口因素.
- 为了确定与SGF发展相关的关键风险因素的预测截止值.
主要方法:
- 从70名从未接受过治疗的VKH患者的139只眼睛进行了回顾性分析.
- 根据脉冲类固醇治疗后12个月的底部外观,将其分为SGF和非SGF组.
- 多变量后勤回归用于识别SGF的显著预测因素.
主要成果:
- 与SGF相关的因素包括脑膜炎,不完整/可能的VKH类型,吸烟史,高对数最佳校正视敏度 (BCVA),高球体等价值 (SE),浅的外周前腔深度 (ACD),狭窄的前腔角 (ACA),瞳孔直径增加,角膜变厚.
- 确定了对逻辑BCVA (>0.261),SE (>-2.813 D),外围ACD (<2.138 mm),ACA (<40.55°),瞳孔直径 (>3.040 mm) 和角膜厚度 (>579.500 μm) 的最佳切线值.
结论:
- 最初的访问发现,如特定的VKH诊断标准,吸烟状态,视敏度,折射误差和前段参数预测SGF的发展.
- 患有已确定的风险因素的患者需要迅速和警的管理,以减轻VKH疾病中SGF进展.
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