首页> 外文期刊>Danishgah-i Ulum-i Pizishki va Khadamat-i Bihdashti-Darmani Shahid Sadugi Yazd. Majallah >Comparing Eruption Space of the Lower Third Molar in Unerupted and Erupted Teeth via Digital Anoramic Radiography in Patients Referring to Yazd Dental College during 2011-13
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Comparing Eruption Space of the Lower Third Molar in Unerupted and Erupted Teeth via Digital Anoramic Radiography in Patients Referring to Yazd Dental College during 2011-13

机译:通过数字全景射线照相比较2011-13年间亚兹德牙科学院的患者下颌磨牙和未萌出和萌出的牙齿中第三磨牙的萌发空间

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Introduction: The aim of this study is to determine and compare the eruption space of unerupted and erupted third molars by the means of digital panoramic radiography in patients referring to Yazd dental college during 2011-2013.Methods: In this cross-sectional descriptive study, 150 archived digital panoramic radiographies in radiology department were evaluated with Romexis software under the standard circumstances. The radiographic pictures belonged to 73 men and 77 women with the average age of 21.18±1.67 years. In patients with erupted third molars as well as unerupted third molars (mesio-angular and vertical), several parameters were examined including: angle of the tooth axis of second and third molar, Gonial angle, the width of third molar, retro-molar space and its ratio to the width of third molar, the development stage of third molar root as well as the distance between the center of ramus and the most distal point of second molar. The data related to age, sex and the eruption situation of lower third molar- unerupted or erupted- were extracted from the patient’s log. The data were analyzed by SPSS (ver.17) via applying descriptive tests and T-test.Results: A statistically significant difference was observed between the two groups in regard with the average angle between second and third molar, the mean space of retro-molar and its ratio to the width of third molar as well as the mean distance between centers of ramus and second molar (P=0.0001). Moreover, no significant difference was observed in Gonial angle mean (P=0.213) and the width of third molar (P.value=0.348).Conclusion: Increasing the angle between second and third molar as well as inadequate space of retro-molar can lead to impaction of lower third molar, but the width of third molar and the Gonial angle size did not reveal any significant role in determination of impaction or eruption of third molar.
机译:简介:本研究的目的是通过数字全景射线照相术确定和比较Yazd牙科学院在2011-2013年期间患者的未磨牙和第三磨牙的萌出空间。方法:在该横断面描述性研究中,在标准情况下,使用Romexis软件评估了放射科的150份存档的数字全景放射照相。放射线照片属于73名男性和77名女性,平均年龄为21.18±1.67岁。在患有第三磨牙和未磨牙的第三磨牙(中角和垂直)患者中,检查了几个参数,包括:第二和第三磨牙的牙齿轴角度,基准角,第三磨牙的宽度,后磨牙空间其与第三磨牙的宽度之比,第三磨牙根的发育阶段以及支心的中心与第二磨牙的最远点之间的距离。从患者的日志中提取出与年龄,性别和下颌第三磨牙未发或发过的爆发状况有关的数据。应用描述性检验和T检验,通过SPSS(版本17)对数据进行分析。结果:两组之间在第二和第三磨牙之间的平均角度,后牙的平均间隔方面存在统计学差异。臼齿及其与第三臼齿宽度的比值以及支齿与第二臼齿中心之间的平均距离(P = 0.0001)。此外,在角向角均值(P = 0.213)和第三磨牙宽度(P.value = 0.348)上没有观察到显着差异。结论:增大第二磨牙与第三磨牙之间的夹角以及后磨牙罐的空间不足导致较低的第三臼齿的撞击,但第三臼齿的宽度和Gonial角尺寸在确定第三臼齿的撞击或爆发方面没有显示任何重要作用。

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