June 2015
Volume 56, Issue 7
Free
ARVO Annual Meeting Abstract  |   June 2015
Corneal strains induced by ocular pulse and larger IOP elevations
Author Affiliations & Notes
  • Elias Pavlatos
    Department of Biomedical Engineering, Ohio State University, Columbus, OH
  • Hong Chen
    Department of Biomedical Engineering, Ohio State University, Columbus, OH
  • Xueliang Pan
    Center For Biostatistics, Ohio State University, Columbus, OH
  • Jun Liu
    Department of Biomedical Engineering, Ohio State University, Columbus, OH
    Department of Ophthalmology, Ohio State University, Columbus, OH
  • Footnotes
    Commercial Relationships Elias Pavlatos, None; Hong Chen, Ohio State University (P); Xueliang Pan, None; Jun Liu, Ohio State University (P)
  • Footnotes
    Support None
Investigative Ophthalmology & Visual Science June 2015, Vol.56, 1100. doi:
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      Elias Pavlatos, Hong Chen, Xueliang Pan, Jun Liu; Corneal strains induced by ocular pulse and larger IOP elevations. Invest. Ophthalmol. Vis. Sci. 2015;56(7 ):1100.

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      © ARVO (1962-2015); The Authors (2016-present)

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Abstract
 
Purpose
 

To compare corneal strains induced by an ocular pulse of a few mmHg with those during inflation from 5 to 30 mmHg in the same eye to evaluate whether the ocular pulse associated strains could predict the outcome of a standard mechanical testing, i.e., inflation.

 
Methods
 

Seventeen porcine globes were tested within 48 hours postmortem. Whole globes were secured using a custom-built holder and immersed in 0.9% saline. A 20G needle was inserted into the anterior chamber and connected to a pressure sensor (P75, Harvard Apparatus) to monitor the intraocular pressure (IOP). Another 20G needle was connected to a programmable syringe pump (PHD Ultra, Harvard Apparatus) to control IOP. The globes were preconditioned with 5 pressure cycles from 5 to 30 mmHg and then equilibrated at 16.5 mmHg for 15 minutes. The ocular pulse was simulated by oscillating IOP between 15 and 18 mmHg at 1 Hz for 25 cycles, and ultrasonic scans (radiofrequency data) were saved for the last 5 cycles. After equilibration at 5 mmHg for 15 minutes, the globe was inflated from 5 to 30 mmHg with 0.5 mmHg steps every 15 seconds. Ultrasonic scans were performed at each step. Corneal radial strains were determined using an ultrasound speckle tracking technique (Tang & Liu, J Biomech Eng 2012, 134(9)). For both the ocular pulse and inflation tests, a stiffness index “b” was calculated by fitting the nonlinear relationship between IOP and strain.

 
Results
 

For all seventeen globes, the average peak radial strain induced by ocular pulse was 0.13 ± 0.03%. The average radial strain at 30 mmHg in the inflation tests was 3.10 ± 0.72%. The correlation between these peak strains was significant (R=0.671, p=0.003; Figure 1). A representative strain map obtained from ocular pulse is shown in Figure 2. The b-values, more representative of the overall nonlinear relationship, were also significantly correlated (R=0.570, p=0.017).

 
Conclusions
 

The strong positive correlation in maximum strain magnitudes and b-values between ocular pulse and inflation tests suggested that these two methods generated correlative biomechanical evaluation of the cornea. While the inflation across a large range of IOPs is difficult to implement in vivo, the naturally occurring ocular pulse could be a feasible alternative to evaluate corneal biomechanics in vivo.  

 
Fig 1. Comparison of inflation and ocular pulse maximum strains.
 
Fig 1. Comparison of inflation and ocular pulse maximum strains.
 
 
Fig 2. Corneal strain map at peak pressure of ocular pulse.
 
Fig 2. Corneal strain map at peak pressure of ocular pulse.

 
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