High-order aberrations (HOAs) are optical defects that degrade the image quality. They change with factors such as pupil diameter, age, and accommodation. The changes in optical aberrations during accommodation are mainly due to lens shape and position changes. Primary spherical aberration (Z(4.0)) is closely related to accommodation and some studies suggested that it plays an important role in the control of accommodation. Furthermore, central and peripheral HOAs vary with refractive error and seem to influence eye growth and the onset and progression of myopia. The variations of central and peripheral HOAs during accommodation also appear to be different
depending on the refractive error. Central and peripheral high-order aberrations are closely related to accommodation and influence the accuracy of the accommodative response and the progression of refractive errors, especially myopia.
Author (Year) | Eyes | Age (Years) | Refractive State (D) | Accommodative Stimulus (D) | Accommodation Stimulation Method | Measurement Method |
---|---|---|---|---|---|---|
Atchison et al. (1995) [13] | 15 | 0D, 1.5D and 3.00D | Aberroscope | |||
He et al. (2000) [8] | 8 | 24–38 | SEQ: −2.00D–−5.56D | Between 0 and 6.00D in steps of 1.00D | Spatially resolved refractometer | |
Ninomiya et al. (2002) [14] | 33 | 28.7 ± 4.4 | 0 and 3.00D | TDV | S-H | |
He et al. (2003) [15] | 12 | 23–32 | SEQ: 0–−3.00D; Cil ≤ 0.25D | 0.25D and 5.00D | TDV | CTS |
Hazel et al. (2003) [16] | 30 | 18–27 | SEQ: +0.50D–−6.00D; Cil < 0.50D | Between 0 and 4.00D in steps of 1.00D | NSL | S-H |
Cheng et al. (2004) [9] | 76 | 21–40 | Sphere: +1.25D–−8.25D; Cil: −0.25D–−2.75D | 0, 3.00D and 6.00D | TDV | S-H |
Gicquel et al. (2005) [17] | 28 | 20–25 | SEQ: −2.00D–+1.00D | Between 1.00D and 5.00D in steps of 0.50D | TDV | S-H |
Plainis et al. (2005) [6] | 7 | 23–33 | Emmetropes; Myopes with sphere: −2.00D–−2.50D | Between 0D and 8.00D in steps of 1.00D | TDV | S-H |
Buehren et al. (2006) [10] | 10 | 22–36 | Sphere: emmetropes +0.05D ± 0.19D; myopes −2.25D ± 0.85D Cil for both: −0.30D ± 0.45D |
0.17D, 1.00D, 2.00D, 3.00D, 4.00D and 5.00D | TDV | S-H |
Wang et. al (2007) [18] | 20 | 18–32 | Sphere: −6.00D–+3.00D | Between 0 and −4.00D in steps of 1.00D | TDV | S-H |
López-Gil et al. (2008) [19] | 24 | 19–29 | Sphere: −3.00D–+3.00D; Cil <1.00D | Between 0 and 5.00D in steps of 0.50D | TDV | S-H |
López-Gil et al. (2010) [20] | 15 | 20–38 | Sphere: 0.38D–−3.06D; Cil: −0.38D ± 0.25D | Between 0.50D and 9.50D in steps of 0.50D | Badal | S-H |
Fritzsch et. al (2011) [21] | 25 | 15–27 | Emmetropes | 0.22D and 5.00D | TDV | S-H |
Yuan et al. (2013) [22] | 35 | 20–33 | SEQ: +0.50D–−2.38D; Cil <0.75D | 0.25D and 3.00D | TDV | S-H |
Zhou et al. (2015) [12] | 22 | 18–28 | Sphere: 0D–−1.00D; Cil: −0.75D and 0D | Between 1.00D and 6.00D in steps of 1.00D | NSL | S-H |
Wang et al. (2015) [11] | 10 | 0 and 3.00D | TDV | S-H |