Stallinga Sjoerd
Philips Research Laboratories, Professor Holstlaan 4, Eindhoven 5656AA, The Netherlands.
Appl Opt. 2005 Feb 20;44(6):849-58. doi: 10.1364/ao.44.000849.
Optical disks are read out by focusing a beam of high numerical aperture (NA) through the substrate. Deviations of the thickness from the nominal value result in spherical aberration; tilting the substrate results in coma. Exact analytical expressions for the rms aberration per micrometer thickness mismatch (for spherical aberration) and per degree tilt (for coma) are derived. The paraxial estimates for these sensitivities proportional to NA4 (spherical aberration) and NA3 (coma) underestimate the exact values by a factor of approximately 2 for the value NA = 0.85, corresponding to the new Blu-ray disk format. Expansion of the aberration function in Zernike aberrations shows that the exact aberration functions are well described by the lowest-order Zernike spherical aberration (A40) and coma (A31) term for all but the very highest NA values.
通过将高数值孔径(NA)光束聚焦穿过基板来读取光盘。厚度与标称值的偏差会导致球差;基板倾斜会导致彗差。推导了每微米厚度失配(球差)和每度倾斜(彗差)的均方根像差的精确解析表达式。对于数值孔径NA = 0.85(对应于新的蓝光光盘格式),这些与NA4(球差)和NA3(彗差)成比例的灵敏度的傍轴估计值比精确值低约2倍。像差函数在泽尼克像差中的展开表明,除了非常高的NA值外,对于所有情况,精确的像差函数都可以由最低阶的泽尼克球差(A40)和彗差(A31)项很好地描述。