𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Improvement of optical resolution in far-field imaging by optical multiplication

✍ Scribed by I. Leizerson; S.G. Lipson; V. Sarafis


Publisher
Elsevier Science
Year
2003
Tongue
English
Weight
361 KB
Volume
34
Category
Article
ISSN
0968-4328

No coin nor oath required. For personal study only.

✦ Synopsis


Based on the idea of the complex filters suggested by Toraldo di Francia in 1952, super-resolved imaging has been achieved by using interferometric image multiplication. The question of whether super-resolution implies a limited field of view is discussed, and an analytical criterion to decide this question is obtained. Three different imaging configurations are investigated, all of which gave a spatial resolution exceeding that corresponding to the full open aperture of the optical system. A resolution limit 55% of the Rayleigh limit was achieved for incoherently illuminated objects. One price that must be paid for the super-resolution is inefficient use of the light source. A second price is a limitation to the usable field of view.


πŸ“œ SIMILAR VOLUMES


The precision improvement of the scanner
✍ Jiying Xiang; Zhen Wu; Ping Zhang; Dexiu Huang; Gaoshang Wei πŸ“‚ Article πŸ“… 1998 πŸ› Elsevier Science 🌐 English βš– 242 KB

A disadvantage of using a galvanometer as the horizontal scanner in CSOM and OCT is its nonlinear distortion caused by the rotational inertial. This is inevitable even if a closed loop is equipped. Here, a second closed loop is introduced to provide pixel clocks to reduce the pincushion distortion o

Optical Image of Stars in the Camera Fie
✍ P. D. Tschobanoff; N. S. Nikolov πŸ“‚ Article πŸ“… 1979 πŸ› John Wiley and Sons 🌐 English βš– 259 KB πŸ‘ 1 views

The possibility the turbulent atmosphere to act as a cause for an amplification of the optical star images is considered. This is made on introducing the turbulent atmosphere a an optical collimator set. Some considerations about the modelling and formalization of this effect are made. Finally some