It appears you don't have support to open PDFs in this web browser. To view this file, Open with your PDF reader
Abstract
When light propagates through opaque material, the spatial information it holds becomes scrambled, but not necessarily lost. Two classes of techniques have emerged to recover this information: methods relying on optical memory effects, and transmission matrix (TM) approaches. Here we develop a general framework describing the nature of memory effects in structures of arbitrary geometry. We show how this framework, when combined with wavefront shaping driven by feedback from a guide-star, enables estimation of the TM of any such system. This highlights that guide-star assisted imaging is possible regardless of the type of memory effect a scatterer exhibits. We apply this concept to multimode fibres (MMFs) and identify a ‘quasi-radial’ memory effect. This allows the TM of an MMF to be approximated from only one end - an important step for micro-endoscopy. Our work broadens the applications of memory effects to a range of novel imaging and optical communication scenarios.
Imaging through scattering media is possible using a transmission matrix or the memory effect. Here, the authors describe the nature of optical memory effects in structures of arbitrary geometry and use this framework to estimate the transmission matrix of an optical fibre from just one end.
You have requested "on-the-fly" machine translation of selected content from our databases. This functionality is provided solely for your convenience and is in no way intended to replace human translation. Show full disclaimer
Neither ProQuest nor its licensors make any representations or warranties with respect to the translations. The translations are automatically generated "AS IS" and "AS AVAILABLE" and are not retained in our systems. PROQUEST AND ITS LICENSORS SPECIFICALLY DISCLAIM ANY AND ALL EXPRESS OR IMPLIED WARRANTIES, INCLUDING WITHOUT LIMITATION, ANY WARRANTIES FOR AVAILABILITY, ACCURACY, TIMELINESS, COMPLETENESS, NON-INFRINGMENT, MERCHANTABILITY OR FITNESS FOR A PARTICULAR PURPOSE. Your use of the translations is subject to all use restrictions contained in your Electronic Products License Agreement and by using the translation functionality you agree to forgo any and all claims against ProQuest or its licensors for your use of the translation functionality and any output derived there from. Hide full disclaimer
Details




1 University of Exeter, Physics and Astronomy, Exeter, UK (GRID:grid.8391.3) (ISNI:0000 0004 1936 8024); Huazhong University of Science and Technology, Wuhan National Laboratory for Optoelectronics, School of Optical and Electronic Information, Wuhan, China (GRID:grid.33199.31) (ISNI:0000 0004 0368 7223)
2 University of Exeter, Physics and Astronomy, Exeter, UK (GRID:grid.8391.3) (ISNI:0000 0004 1936 8024)
3 Faculty of Science, Masaryk University, Department of Theoretical Physics and Astrophysics, Brno, Czech Republic (GRID:grid.10267.32) (ISNI:0000 0001 2194 0956); Institute of Scientific Instruments of CAS, Brno, Czech Republic (GRID:grid.438850.2) (ISNI:0000 0004 0428 7459)
4 Institute of Scientific Instruments of CAS, Brno, Czech Republic (GRID:grid.438850.2) (ISNI:0000 0004 0428 7459); Leibniz Institute of Photonic Technology, Jena, Germany (GRID:grid.418907.3) (ISNI:0000 0004 0563 7158)