CROSS-MODALITY VALIDATION OF ACETABULAR SURFACE MODELS USING 3-D ULTRASOUND VERSUS MAGNETIC RESONANCE IMAGING IN NORMAL AND DYSPLASTIC INFANT HIPS

被引:6
作者
Diederichs, Chad [1 ]
Heath, Alana [1 ]
Hareendranathan, Abhilash R. [1 ]
Zonoobi, Dornoosh [1 ]
Kuntze, Gregor [3 ]
Dulai, Sukhdeep [2 ]
Mabee, Ymyles G. [1 ]
Ronsky, Janet L. [3 ]
Jaremko, Jacob L. [1 ]
机构
[1] Univ Alberta, Dept Radiol & Diagnost Imaging, 2 A2-41WC Mackenzie Hlth Sci Ctr,8440-112 St, Edmonton, AB T6G 2B7, Canada
[2] Univ Alberta, Div Orthopaed Surg, Edmonton, AB, Canada
[3] Univ Calgary, Dept Mech Engn, Calgary, AB, Canada
关键词
Developmental dysplasia of the hip; 3-D ultrasound; Pediatrics; Magnetic resonance imaging; DEVELOPMENTAL DYSPLASIA; DIAGNOSIS;
D O I
10.1016/j.ultrasmedbio.2016.04.006
中图分类号
O42 [声学];
学科分类号
070206 [声学];
摘要
Current imaging diagnosis of developmental dysplasia of the hip (DDH) in infancy relies on 2-D ultrasound (US), which is highly operator-dependent. 3-D US offers more complete, and potentially more reliable, imaging of infant hip geometry. We sought to validate the fidelity of acetabular surface models obtained by 3-D US against those obtained concurrently by magnetic resonance imaging (MRI). 3-D US and MRI scans were performed on the same d in 20 infants with normal to severely dysplastic hips (mean age, 57 d; range 13-181 d). 3-D US was performed by two observers using a Philips VL13-5 probe. Coronal 3-D multi-echo data image combination (MEDIC) magnetic resonance (MR) images (1-mm slice thickness) were obtained, usually without sedation, in a 1.5 T Siemens unit. Acetabular surface models were generated for 40 hips from 3-D US and MRI using semi-automated tracing software, separately by three observers. For each hip, the 3-D US and MRI models were co-registered to overlap as closely as possible using Amira software, and the root mean square (RMS) distances between points on the models were computed. 3-D US scans took 3.2 s each. Inter-modality variability was visually minimal. Mean RMS distance between corresponding points on the acetabular surface at 3-D US and MRI was 0.4 +/- 0.3 mm, with 95% confidence interval <1 mm. Mean RMS errors for inter-observer and intra-observer comparisons were significantly less for 3-D US than for MRI, while inter-scan and inter-modality comparisons showed no significant difference. Acetabular geometry was reproduced by 3-D US surface models within 1 mm of the corresponding 3-D MRI surface model, and the 3-D US models were more reliable. This validates the fidelity of 3-D US modeling and encourages future use of 3-D US in assessing infant acetabulum anatomy, which may be useful to detect and monitor treatment of hip dysplasia. (C) 2016 World Federation for Ultrasound in Medicine & Biology.
引用
收藏
页码:2308 / 2314
页数:7
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