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1.
Article | IMSEAR | ID: sea-198303

ABSTRACT

Background: The anatomical boundaries of the orbit are defined and the contribution of various bones in makingup the orbital margins is determined .Associated with this, orbital dimensions like length, breadth and theorbital index are determined along with the associated dimorphic and bilateral variations. The findings of theseterritorial specimens are analyzed and compared with similar findings from other vernacular territories. Thebilateral craniofacial structures are studied and they are dimensionally classified and characterized.Comprehensive documentation thus promulgated functions to prove vital in the conquest of dexterity in the fieldof surgery and forensic anthropometry alike. The evaluated parameters also serve as an empirical guide indiscerning tenuous sites that are susceptible to impaction and in defining the safe limits of orbital explorationResults: The study has returned an average value of 81.47 as the orbital index of the scrutinized dry skullspecimens thus placing them under the category of microseme. The average values of orbital length and breadthwere found to be 31.26mm and 38.37mm respectively. The superior margin formed exclusively by the frontalbone measured 32.7mm on average with the supraorbital notch/foramen being displaced 5.92mm from themedial limit of the superior margin. For 25.88mm, which was the average length of medial margin, maxilla stoodthe dominant contributor (13.81mm) with the frontal bone chipping in to contribute to the rest. The inferiormargin paints a contrary picture of maxilla being the secondary contributor (16.13mm) whilst here it is thezygoma which makes a greater contribution (17.29mm).Conclusion: This study hereby establishes Microseme to be the predominant orbital index of the scrutinized skullspecimens in addition to quantifying the contributions of various bones towards making up the margins.Comparative analysis with confluent such studies from other provinces of the Indian subcontinent has confirmedthe latitude variation associated with orbital index. The results thus established will be unerringly essential inthe field of surgery and forensic anthropometry

2.
Article in English | IMSEAR | ID: sea-175426

ABSTRACT

Background: The moderator band has the right bundle of His within the right ventricle. It also is known to prevent the over dilatation of RV. It is important because of its involvement in RV infarcts, in differentiating RV from LV in congenital anomalies, in VPDs & VTs and in VSDs. The present literature is very much lacking in its morphometry. Materials and Methods: Moderator band was looked for in 50 hearts and only in this study did we find it in all the hearts. The length, the thickness, the distance from the tricuspid valve along with the presence of any trabeculations in the septal end or in the papillary muscle end were looked for and recorded. Results: The average length was 14.71±4.99mm, the average thickness was 4.97±1.64 mm, the average distance from the tricuspid orifice was 19.85±5.92 mm. The attachment to the anterior papillary muscle was found to be branched in 8 hearts that is having an incidence of 14% . The septal end were branched and separated as two in only two specimens. Only one specimen had branched attachments on both the apical and septal ends. Conclusion: The distance from tricuspid valve and knowledge of branching are important in corrective surgeries of the VSDs. An awareness of length and thickness helps the clinician to differentiate moderator band from the other structures, which may result in misdiagnosis during echocardiography. Its presence may in fact be of significance in preventing over distension of the heart in RV myocardial ischaemia.

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