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眼眶间质液:颅外脑脊液吸收潜在途径的证据

Orbital Interstitial Fluid: Evidence of a Potential Pathway for Extracranial Cerebrospinal Fluid Absorption.

作者信息

Sachs Jeffrey R, Zapadka Michael E, Elster Allen D

机构信息

From the Department of Radiology, Wake Forest School of Medicine, Wake Forest Baptist Health, Winston-Salem, NC.

出版信息

J Comput Assist Tomogr. 2018 Jul/Aug;42(4):497-501. doi: 10.1097/RCT.0000000000000716.

DOI:10.1097/RCT.0000000000000716
PMID:29489593
Abstract

BACKGROUND AND PURPOSE

The aim of the study was to describe the prevalence and characteristics of orbital interstitial fluid seen on magnetic resonance (MR) images of infants and young children.

MATERIALS AND METHODS

Fat-suppressed axial T2-weighted MR images of 100 consecutive infants and young children (<6 years) without orbital pathology were retrospectively reviewed by 2 neuroradiologists. The presence, location, and extent of high-signal orbital interstitial fluid were characterized and tabulated as a function of age.

RESULTS

Orbital interstitial fluid was detected in 90 (90%) of the 100 subjects overall, present in 100% (75/75) of infants and children younger than 3 years, 75% (12/16) of those aged 3 to 5 years, and 33% (3/9) of those aged 5 to 6 years. The fluid was bilateral and symmetric in all cases. Two morphologic patterns were distinguished, which often co-existed: (1) a focal discrete curvilinear band of fluid in the posterior-lateral orbit, more common in younger patients, and (2) an ill-defined, lace-like pattern primarily in the superior orbit seen in subjects of all ages.

CONCLUSIONS

Orbital interstitial fluid as detected by fat-suppressed T2-weighted MR imaging is a nearly universal finding in infants and young children and should not be considered pathologic. It may have either a focal or lace-like pattern or both. Orbital interstitial fluid decreases in size and prevalence as a function of age but is still present in nearly half of children aged 4 to 6 years. Possible explanations concerning the nature and origin of this fluid are presented, including the fascinating possibility that the fluid represents an extracranial pathway for outflow of cerebrospinal fluid.

摘要

背景与目的

本研究旨在描述婴幼儿磁共振(MR)图像上眼眶间质液的患病率及特征。

材料与方法

2名神经放射科医生对100例连续的无眼眶病变的婴幼儿(<6岁)的脂肪抑制轴向T2加权MR图像进行回顾性分析。眼眶高信号间质液的存在、位置及范围按年龄进行特征描述并制成表格。

结果

100名受试者中,90名(90%)检测到眼眶间质液,3岁以下婴幼儿中100%(75/75)存在,3至5岁儿童中75%(12/16)存在,5至6岁儿童中33%(3/9)存在。所有病例中液体均为双侧且对称。区分出两种形态学模式,且常同时存在:(1)眼眶后外侧局限性离散曲线状液带,在较年幼患者中更常见;(2)所有年龄段受试者中主要位于眼眶上部的边界不清的花边样模式。

结论

脂肪抑制T2加权MR成像检测到的眼眶间质液在婴幼儿中几乎普遍存在,不应视为病理性的。它可能呈局限性或花边样模式,或两者皆有。眼眶间质液的大小和患病率随年龄增长而降低,但在4至6岁儿童中仍近半数存在。文中提出了关于这种液体的性质和来源的可能解释,包括这种液体代表脑脊液颅外流出途径这一引人入胜的可能性。

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