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      Amplitude and phase recovering from a micro-digital hologram using angular spectrum

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          Abstract

          In this paper we present a method to get the complex amplitude of a digital hologram obtained through phase shifting transmission digital holographic microscopy. This is based on the angular spectrum method as a reconstruction algorithm employing an in-line experimental setup. The reconstruction technique automatically eliminates the zero order and the twin images from the digital hologram. By means of a reference hologram reconstruction method, a temporal averaging procedure and a focus distance averaging of the reconstructed complex amplitude, we extend an already efficient methodology to obtain high precision phase images with a reduced amount of aberrations caused by the microscope objective, and at the same time, we reduce the optical noise of the reconstructed complex amplitude. Using a homemade micro-thin film step surface, our system was calibrated and made traceable to an atomic force microscope (AFM). It is shown that our experimental results, compared to those given by the AFM, reach an axial accuracy of 9.7 nm from a typical phase sample.

          Translated abstract

          En este trabajo presentamos una metodología para la obtencion de la amplitud compleja de un holograma digital por medio de un microscopio holográfico digital en transmisión usando corrimiento de fase. Como método de reconstrucción se usa el algoritmo de propagación del espectro angular, empleando un arreglo experimental en eje. Esta técnica de reconstrucción elimina de manera automática el orden cero y la imagen gemela del holograma digital. Por medio del método de reconstruccion del holograma de referencia, el metodo del promediado temporal y el metodo de promediado de la distancia focal de la amplitud compleja reconstruida ampliamos una metodología eficiente para obtener imágenes de fase de alta precisión con una cantidad reducida de aberraciones provocadas por el objetivo de microscopio, así como la reduccion de ruido óptico de la amplitud compleja reconstruida. Usando una micro película delgada superficial en forma de escalon hecha en casa como primera muestra, nuestro sistema fue calibrado y con los resultados de un microscopio de fuerza atómica como medio de trazabilidad de la misma muestra. Se muestra que nuestros resultados experimentales comparados con los del microscopio de fuerza atómica alcanzan una precisión axial de 9.7 nm de una muestra típica de fase.

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          Introduction to Fourier optics

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            Status of the UC-Berkeley SETI Efforts

            We summarize radio and optical SETI programs based at the University of California, Berkeley. The SEVENDIP optical pulse search looks for ns time scale pulses at visible wavelengths using an automated 30 inch telescope. The ongoing SERENDIP V.v sky survey searches for radio signals at the 300 meter Arecibo Observatory. The currently installed configuration supports 128 million channels over a 200 MHz bandwidth with ~1.6 Hz spectral resolution. SETI@home uses the desktop computers of volunteers to analyze over 160 TB of data at taken at Arecibo looking for two types of continuous wave signals and two types of pulsed signals. A version to be released this summer adds autocorrelation analysis to look for complex wave forms that have been repeated (and overlayed) after a short delay. SETI@home will soon be processing data of Kepler exoplanet systems collected at the GBT. The Astropulse project is the first SETI search for \(\mu\)s time scale dispersed pulses in the radio spectrum. We recently reobserved 114 sky locations where microsecond pulses were detected. This data is in process of being transferred to Berkeley for analysis.
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                Author and article information

                Journal
                rmf
                Revista mexicana de física
                Rev. mex. fis.
                Sociedad Mexicana de Física (México, DF, Mexico )
                0035-001X
                August 2011
                : 57
                : 4
                : 315-321
                Affiliations
                [01] León Guanajuato orgnameCentro de investigaciones en óptica, A.C. México migue@ 123456cio.mx
                Article
                S0035-001X2011000400004 S0035-001X(11)05700400004
                eae1de88-2b31-4df1-8956-97586f4960d0

                This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.

                History
                : 31 May 2011
                : 25 November 2010
                Page count
                Figures: 0, Tables: 0, Equations: 0, References: 36, Pages: 7
                Product

                SciELO Mexico

                Categories
                Research

                phase measurement,phase retrieval,surface measurements,rugosidad,medición superficial,medicion de fase,técnicas de reconstrucción de imagen,microscopia,image reconstruction techniques,recuperación de fase,Digital holography,holografía por computadora,compensación de aberraciones,aberration compensation,microscopy,computer holography,Holografía digital,roughness

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