Thoracoscopic anterior instrumented fusion for adolescent idiopathic scoliosis with emphasis on the sagittal plane

2009 ◽  
Vol 9 (7) ◽  
pp. 523-529 ◽  
Author(s):  
Baron S. Lonner ◽  
Joshua D. Auerbach ◽  
Rafael Levin ◽  
David Matusz ◽  
Carrie L. Scharf ◽  
...  
2009 ◽  
Vol 9 (10) ◽  
pp. 202S-203S
Author(s):  
Yongjung Kim ◽  
Lawrence Lenke ◽  
Keith Bridwell ◽  
Oheneba Boachie-Adjei ◽  
Jean-Luc Clement ◽  
...  

2016 ◽  
Vol 25 (10) ◽  
pp. 3095-3103 ◽  
Author(s):  
Javier Pizones ◽  
Alberto Núñez-Medina ◽  
Felisa Sánchez-Mariscal ◽  
Lorenzo Zúñiga ◽  
Enrique Izquierdo

2016 ◽  
Vol 55 (4) ◽  
pp. 561-572 ◽  
Author(s):  
Nicolas Newell ◽  
Caroline A. Grant ◽  
Bethany E. Keenan ◽  
Maree T. Izatt ◽  
Mark J. Pearcy ◽  
...  

2021 ◽  
Author(s):  
Kepeng Li ◽  
Jun Miao ◽  
Jingan Zhang ◽  
Xijie Wang ◽  
Ye Han

Abstract Background: This study aims to evaluate the effects of bracing on the Cobb’s angle (CA) and spinopelvic parameters in adolescent idiopathic scoliosis (AIS) patients. Methods: A total of 51 AIS patients who received bracing treatment between January 2018 and August 2019 were retrospectively analyzed. The pro-bracing and in-bracing radiographs were analyzed with regard to the spinopelvic parameters. The CA, pelvic coronal obliquity angle (PCOA), thoracolumbar kyphosis (TK), lumbar lordosis (LL), pelvic incidence (PI), pelvic tilt (PT), sacral slope (SS), sagittal vertical angle (SVA) and coronal vertical angle (CVA) were measured. Results: The mean age at the initiation of bracing was 13.6 ± 1.5 years. The mean pro-bracing CA was 24.0° ± 6.3°. There were no statistically significant differences between pro-bracing and in-bracing measurements of SVA and CVA. However, there were statistically significant differences between the pro-bracing and in-bracing measurements of the CA, PCOA, TLK, LL, PT and SS. A significant correlation was observed between PT variation and TLK variation in the sagittal plane. In the coronal plane, the PCOA variation was correlated to pro-bracing PCOA. Conclusion: Bracing effects of AIS can be extended to the pelvis. The pelvis should retro-rotate correspondingly to TLK hypokyphosis on sagittal plane, whereas in coronal plane, pelvic obliquity was improved independently.


2021 ◽  
Author(s):  
Gökhan Karademir ◽  
Kerim Sarıyılmaz ◽  
Okan Özkunt ◽  
Mehmet Demirel ◽  
Fatih Dikici ◽  
...  

Abstract BackgroundAlthough Lenke classification analyses the sagittal plane as (+), N, and (-), it does not consider it in the choice of treatment, and it has limitations with overall thoracic kyphosis (TK). To investigate the importance of TK for treatment preference in patients with Lenke 5C adolescent idiopathic scoliosis (AIS) by comparing radiological outcomes of the patients who underwent selective fusion (SF) or nonselective fusion (NSF). MethodsThirty-two patients with Lenke type 5C AIS were included and then divided into two groups as per the fusion procedure used in the surgical treatment. SF group including 17 patients (15 females; mean age = 16 years, age range, 14–21) with normal TK and NSF group including 15 patients (11 females; mean age = 17 years, age range, 13–26) with thoracic hyper-kyphosis. Thorocolumbar/lumbar (TL/L) Cobb, thoracic (T) Cobb, TK and lumbar lordosis (LL) were measured on standing spine radiographs preoperatively and at the final follow-up. The correction rates (CR) of each radiographic parameter were calculated.ResultsNo significant differences were observed in the mean CR of all radiographic parameters, except TK and LL correction rates. The mean CR of TK was significantly higher in NSF group (-17% [range, -100–69]) than in SF group (67% [range, 9–100]) (p = 0.000). Likewise, the mean CR of LL was found significantly higher in NSF group (12.47% [range, -100–51]) than in SF group (-2.41% [range, -75–47]) (p = 0.036).ConclusionIn patients in whom Lenke's sagittal modifier is N, SF can be performed efficiently. NSF should be preferred in those with Lenke's sagittal modifiers (+) as TK can be better controlled with NSF.Level of Evidence: 3


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