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出生季节、光照周期与婴儿期屈光状态

Birth season, photoperiod, and infancy refraction.

作者信息

Deng Li, Gwiazda Jane

机构信息

Department of Vision Science, New England College of Optometry, Boston, Massachusetts 02115, USA.

出版信息

Optom Vis Sci. 2011 Mar;88(3):383-7. doi: 10.1097/OPX.0b013e31820b0517.

Abstract

PURPOSE

To investigate the association between birth month/photoperiod and refraction in infancy.

METHODS

Seven hundred twenty-two children with refractions measured between 1 and 3 months were included in this analysis. Non-cycloplegic near retinoscopy was performed by three experienced optometrists over a 32-year period. Photoperiod hours were calculated as the mean daylight hours 30 days after each infant's birth and then grouped into quartiles between 9.12 and 15.25 hours. Two classifications for birth season were considered: regular season (Spring: March-May, Summer: June-August, Fall: September-November, and Winter: December-February) and alternate season (Spring: February-April, Summer: May-July, Fall: August-October, and Winter: November-January).

RESULTS

The mean infant age was 2.11 ± 0.55 months. The mean spherical equivalent refraction (SER) was 0.61 ± 1.56 diopters (D). Children born in the photoperiod group with the most daylight hours had slightly lower refractions than those in the shortest photoperiod group (0.43 ± 1.60 D vs. 0.87 ± 1.43 D, p < 0.05). In the longest photoperiod group, the percentage of infants with SER ≤-0.25 D was significantly higher (51/179 = 28.49%) than in the shortest photoperiod group (31/177 = 17.51%) (p = 0.02). Similar patterns were observed using the alternate season classification, with (1) lower mean SER in infants born in the summer vs. the winter and (2) a higher percentage of SER ≤-0.25 D in infants born in the summer vs. the winter. However, by regular seasons, the mean SERs were similar between summer and winter.

CONCLUSIONS

A small, statistically significant lower refraction was found in infants with the most vs. the least daylight soon after birth, suggesting that light might play a small role in the refractive error of newborns.

摘要

目的

探讨出生月份/光照周期与婴儿屈光不正之间的关联。

方法

本分析纳入了722名在1至3个月时进行屈光测量的儿童。由三位经验丰富的验光师在32年的时间里进行非散瞳近检影验光。光照时长计算为每个婴儿出生后30天的平均日照时长,然后分为9.12至15.25小时的四分位数。考虑了两种出生季节分类:常规季节(春季:3月至5月,夏季:6月至8月,秋季:9月至11月,冬季:12月至2月)和交替季节(春季:2月至4月,夏季:5月至7月,秋季:8月至10月,冬季:11月至1月)。

结果

婴儿的平均年龄为2.11±0.55个月。平均球镜等效屈光力(SER)为0.61±1.56屈光度(D)。出生在日照时长最长的光照周期组的儿童屈光不正程度略低于日照时长最短的组(0.43±1.60 D对0.87±1.43 D,p<0.05)。在日照时长最长的组中,SER≤ -0.25 D的婴儿百分比显著高于日照时长最短的组(51/179 = 28.49%对31/177 = 17.51%)(p = 0.02)。使用交替季节分类观察到类似模式,即(1)夏季出生的婴儿与冬季出生的婴儿相比,平均SER较低;(2)夏季出生的婴儿与冬季出生的婴儿相比,SER≤ -0.25 D的百分比更高。然而,按照常规季节分类,夏季和冬季之间的平均SER相似。

结论

出生后日照时长最多与最少的婴儿相比,发现屈光不正程度有统计学意义的轻微降低,这表明光线可能在新生儿屈光不正中起小作用。

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