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Article: Patterns of coronal and sagittal deformities in adolescent idiopathic scoliosis

TitlePatterns of coronal and sagittal deformities in adolescent idiopathic scoliosis
Authors
KeywordsAdolescent idiopathic scoliosis
Pelvic incidence
Pelvic tilt
Sacral slope
Lumbar lordosis
Thoracic kyphosis
Issue Date2021
PublisherBioMed Central Ltd. The Journal's web site is located at http://www.biomedcentral.com/bmcmusculoskeletdisord/
Citation
BMC Musculoskeletal Disorders, 2021, v. 22 n. 1, article no. 44 How to Cite?
AbstractBackground: Thoracic scoliosis has been shown to be associated with hypokyphosis in adolescent idiopathic scoliosis (AIS). However, the relationship of sagittal spino-pelvic parameters with different coronal curve patterns and their influence on patient-perceived quality of life is unknown. This study aims to determine the association between coronal and sagittal malalignment in patients with AIS and to determine their effects on SRS-22r scores. Methods: A cross-sectional study was conducted on 1054 consecutive patients with AIS. The coronal Cobb angle, thoracic kyphosis (TK), lumbar lordosis (LL), pelvic incidence (PI), PI-LL mismatch (PI-LL), pelvic tilt (PT), and sacral slope (SS) were measured on standing radiographs. The coronal Cobb angle (mild: 10-20 degrees; moderate: >20-40 degrees; severe: >40 degrees) and PI (low: <35; average: 35-50 degrees; high: >50 degrees) were divided into 3 sub-groups for comparison. Relationship between coronal curve magnitudes and sagittal parameters was studied as was their association with SRS-22r scores. Results: Low PI had smaller SS (30.18.3 degrees vs 44.8 +/- 7.7 degrees; p<0.001), PT (-0.38.1 degrees vs 14.4 +/- 7.5 degrees; p<0.001), and LL (42.013.2 degrees vs 55.1 +/- 10.6 degrees; p<0.001), negative PI-LL mismatch (-12.113.1 degrees vs 4.1 +/- 10.5 degrees; p<0.001) as compared to large PI. There were no significant relationships with PI and TK (p=0.905) or curve magnitude (p=0.431). No differences in sagittal parameters were observed for mild, moderate or severe coronal Cobb angles. SRS-22r scores only correlated with coronal Cobb angle and larger Cobb angles were negatively correlated with the function, appearance and pain domains. Conclusions: The sagittal profile for AIS is associated with the pelvic parameters especially PI but not with the coronal curve pattern. All patients have a similar TK regardless of coronal curve type. However, it appears that the coronal deformity is a greater influence on quality of life outcomes especially those >40 degrees.
Persistent Identifierhttp://hdl.handle.net/10722/295736
ISSN
2021 Impact Factor: 2.562
2020 SCImago Journal Rankings: 0.837
PubMed Central ID
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorMak, T-
dc.contributor.authorCheung, PWH-
dc.contributor.authorZhang, T-
dc.contributor.authorCheung, JPY-
dc.date.accessioned2021-02-08T08:13:16Z-
dc.date.available2021-02-08T08:13:16Z-
dc.date.issued2021-
dc.identifier.citationBMC Musculoskeletal Disorders, 2021, v. 22 n. 1, article no. 44-
dc.identifier.issn1471-2474-
dc.identifier.urihttp://hdl.handle.net/10722/295736-
dc.description.abstractBackground: Thoracic scoliosis has been shown to be associated with hypokyphosis in adolescent idiopathic scoliosis (AIS). However, the relationship of sagittal spino-pelvic parameters with different coronal curve patterns and their influence on patient-perceived quality of life is unknown. This study aims to determine the association between coronal and sagittal malalignment in patients with AIS and to determine their effects on SRS-22r scores. Methods: A cross-sectional study was conducted on 1054 consecutive patients with AIS. The coronal Cobb angle, thoracic kyphosis (TK), lumbar lordosis (LL), pelvic incidence (PI), PI-LL mismatch (PI-LL), pelvic tilt (PT), and sacral slope (SS) were measured on standing radiographs. The coronal Cobb angle (mild: 10-20 degrees; moderate: >20-40 degrees; severe: >40 degrees) and PI (low: <35<degrees>; average: 35-50 degrees; high: >50 degrees) were divided into 3 sub-groups for comparison. Relationship between coronal curve magnitudes and sagittal parameters was studied as was their association with SRS-22r scores. Results: Low PI had smaller SS (30.18.3 degrees vs 44.8 +/- 7.7 degrees; p<0.001), PT (-0.3<plus/minus>8.1 degrees vs 14.4 +/- 7.5 degrees; p<0.001), and LL (42.0<plus/minus>13.2 degrees vs 55.1 +/- 10.6 degrees; p<0.001), negative PI-LL mismatch (-12.1<plus/minus>13.1 degrees vs 4.1 +/- 10.5 degrees; p<0.001) as compared to large PI. There were no significant relationships with PI and TK (p=0.905) or curve magnitude (p=0.431). No differences in sagittal parameters were observed for mild, moderate or severe coronal Cobb angles. SRS-22r scores only correlated with coronal Cobb angle and larger Cobb angles were negatively correlated with the function, appearance and pain domains. Conclusions: The sagittal profile for AIS is associated with the pelvic parameters especially PI but not with the coronal curve pattern. All patients have a similar TK regardless of coronal curve type. However, it appears that the coronal deformity is a greater influence on quality of life outcomes especially those >40 degrees.-
dc.languageeng-
dc.publisherBioMed Central Ltd. The Journal's web site is located at http://www.biomedcentral.com/bmcmusculoskeletdisord/-
dc.relation.ispartofBMC Musculoskeletal Disorders-
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.subjectAdolescent idiopathic scoliosis-
dc.subjectPelvic incidence-
dc.subjectPelvic tilt-
dc.subjectSacral slope-
dc.subjectLumbar lordosis-
dc.subjectThoracic kyphosis-
dc.titlePatterns of coronal and sagittal deformities in adolescent idiopathic scoliosis-
dc.typeArticle-
dc.identifier.emailCheung, PWH: gnuehcp6@hku.hk-
dc.identifier.emailZhang, T: tgzhang@hku.hk-
dc.identifier.emailCheung, JPY: cheungjp@hku.hk-
dc.identifier.authorityCheung, JPY=rp01685-
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1186/s12891-020-03937-4-
dc.identifier.pmid33419438-
dc.identifier.pmcidPMC7791682-
dc.identifier.scopuseid_2-s2.0-85099003841-
dc.identifier.hkuros321139-
dc.identifier.volume22-
dc.identifier.issue1-
dc.identifier.spagearticle no. 44-
dc.identifier.epagearticle no. 44-
dc.identifier.isiWOS:000608282900001-
dc.publisher.placeUnited Kingdom-

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