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Auswahl der wissenschaftlichen Literatur zum Thema „Interferometry“
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Zeitschriftenartikel zum Thema "Interferometry"
Chesneau, O., K. Rousselet-Perraut und F. Vakili. „Interferometry and Stellar Magnetism“. International Astronomical Union Colloquium 175 (2000): 174–77. http://dx.doi.org/10.1017/s0252921100055792.
Der volle Inhalt der QuelleMcAlister, Harold A. „Overview of Multiple–Aperture Interferometry Binary Star Results from the Northern Hemisphere“. Proceedings of the International Astronomical Union 2, S240 (August 2006): 35–44. http://dx.doi.org/10.1017/s1743921307003778.
Der volle Inhalt der QuelleJankov, S. „Astronomical optical interferometry, I: Methods and instrumentation“. Serbian Astronomical Journal, Nr. 181 (2010): 1–17. http://dx.doi.org/10.2298/saj1081001j.
Der volle Inhalt der QuelleTrolinger, James D., Amit Lal, Joshua Jo und Stephen Kupiec. „Programmable Holographic Optical Elements as Adaptive Optics in Optical Diagnostics Devices“. Key Engineering Materials 437 (Mai 2010): 108–12. http://dx.doi.org/10.4028/www.scientific.net/kem.437.108.
Der volle Inhalt der QuelleCavedo, Federico, Parisa Esmaili, Alessandro Pesatori und Michele Norgia. „Self-mixing Interferometer: Frequency Modulation Noise Dependence on Laser Source“. Journal of Physics: Conference Series 2698, Nr. 1 (01.02.2024): 012019. http://dx.doi.org/10.1088/1742-6596/2698/1/012019.
Der volle Inhalt der QuelleYankelev, Dimitry, Chen Avinadav, Nir Davidson und Ofer Firstenberg. „Atom interferometry with thousand-fold increase in dynamic range“. Science Advances 6, Nr. 45 (November 2020): eabd0650. http://dx.doi.org/10.1126/sciadv.abd0650.
Der volle Inhalt der QuelleStee, Ph, D. Bonneau, F. Morand, D. Mourard und F. Vakili. „Current studies and future prospects in stellar-structure imaging with the GI2T“. Symposium - International Astronomical Union 176 (1996): 191–98. http://dx.doi.org/10.1017/s0074180900083224.
Der volle Inhalt der QuelleNoordam, J. E. „European Space Interferometry“. Symposium - International Astronomical Union 166 (1995): 345. http://dx.doi.org/10.1017/s0074180900228349.
Der volle Inhalt der QuellePushin, D. A., M. G. Huber, M. Arif, C. B. Shahi, J. Nsofini, C. J. Wood, D. Sarenac und D. G. Cory. „Neutron Interferometry at the National Institute of Standards and Technology“. Advances in High Energy Physics 2015 (2015): 1–7. http://dx.doi.org/10.1155/2015/687480.
Der volle Inhalt der QuelleMonnier, John D. „Infrared interferometry of circumstellar envelopes“. Symposium - International Astronomical Union 191 (1999): 321–30. http://dx.doi.org/10.1017/s0074180900203239.
Der volle Inhalt der QuelleDissertationen zum Thema "Interferometry"
Ho, Lap. „High precision short-baseline pointing system using GPS interferometry“. Ohio : Ohio University, 1995. http://www.ohiolink.edu/etd/view.cgi?ohiou1179435242.
Der volle Inhalt der QuelleLemes, Andryos da Silva [UNESP]. „Novas configurações de interferômetros de quadratura e de técnicas de detecção de fase óptica baseadas em phase unwrapping“. Universidade Estadual Paulista (UNESP), 2014. http://hdl.handle.net/11449/111112.
Der volle Inhalt der QuelleInterferômetros ópticos de saída única são muito sensíveis quando operam nas proximidades do ponto de quadratura de fase da sua curva característica de entrada e saída. Entretanto, as flutuações ambientais de baixa frequência produzem derivas aleatórias entre os caminhos ópticos do interferômetro que desviam o ponto quiescente da quadratura, levando ao fenômeno de desvanecimento de sinal. Através de processamento eletrônico de dois sinais interferométricos de saída, defasados a 90º entre si, consegue-se demodular o sinal independentemente das derivas ambientais. Esses interferômetros chamados de interferômetros de quadratura são amplamente utilizados em laboratórios de metrologia, porém, devido à grande quantidade de componentes ópticos normalmente envolvidos, são de difícil alinhamento e de elevado custo. Neste trabalho estuda-se a interferometria homódina de dois feixes em quadratura e as suas complexidades inerentes. Propõe-se uma nova arquitetura, baseada na configuração de Michelson, de alinhamento mais simples e de baixo custo. Descreve-se matematicamente o processo de obtenção dos sinais em quadratura deste arranjo. Também, se explora uma técnica capaz de obter dois sinais interferométricos em quadratura através da configuração tradicional de Michelson explorando-se a distribuição espacial do padrão de franjas. Desenvolve-se, ainda, um novo algoritmo de phase unwrapping aplicável como método de detecção de fase óptica, capaz de reconstruir a forma de onda de sinais de modulação e fornecer a diferença de fase estática entre os braços do interferômetro, quando o sinal de modulação possui valor médio nulo. Testes computacionais são realizados para corroborar na tarefa de evidenciar o potencial da técnica. Por meio do método de demodulação apresentado, em adição com o interferômetro proposto e da técnica explorada, realiza-se testes experimentais em um atuador piezoelétrico ...
Optical interferometers with single outputs are very sensitive when operating close to the phase quadrature point of their input-output characteristic curves. However, low frequency environmental fluctuations generate random drifts between the optical paths of the interferometer that deviate the quiescent point from the quadrature condition. This problem causes the phenomenon called signal fading. By electronically processing these two interferometry output signals, shifted by 90º, it is possible to demodulate the signal regardless of environmental drift. These kinds of interferometers, known as quadrature interferometers, are widely used in metrology laboratories, but, due to the large amount of optical components, they are expensive and difficult to design. In this work a low cost homodyne interferometer with two output quadrature beams based on the Michelson configuration is studied, and the procedure to achieve the quadrature signals is mathematically described. Also, a recent technique, not widely known in the literature and that is able to obtain two quadrature signals by using the standard configuration of the Michelson interferometer is explored, exploiting the spatial distribution of the fringe pattern. A new method for optical phase shift demodulation based on phase unwrapping is developed. This approach is able to recover not only the modulation signal waveform, but can also calculate the static phase shift between the interferometer arms when the modulation signal has an average value equal to zero. The method also has the ability to demodulate signals which vary arbitrarily in time. Computational test were done aiming to demonstrate the technique potential. By using this new optical phase shift demodulation method, combined with the proposed interferometer and exploiting the spatial distribution of the fringe pattern, a piezoelectric flextensional actuator is characterized. Displacement versus drive voltage and frequency ...
Lemes, Andryos da Silva. „Novas configurações de interferômetros de quadratura e de técnicas de detecção de fase óptica baseadas em phase unwrapping /“. Ilha Solteira, 2014. http://hdl.handle.net/11449/111112.
Der volle Inhalt der QuelleBanca: Ricardo Tokio Higuti
Banca: Ronny Calixto Carbonari
Resumo: Interferômetros ópticos de saída única são muito sensíveis quando operam nas proximidades do ponto de quadratura de fase da sua curva característica de entrada e saída. Entretanto, as flutuações ambientais de baixa frequência produzem derivas aleatórias entre os caminhos ópticos do interferômetro que desviam o ponto quiescente da quadratura, levando ao fenômeno de desvanecimento de sinal. Através de processamento eletrônico de dois sinais interferométricos de saída, defasados a 90º entre si, consegue-se demodular o sinal independentemente das derivas ambientais. Esses interferômetros chamados de interferômetros de quadratura são amplamente utilizados em laboratórios de metrologia, porém, devido à grande quantidade de componentes ópticos normalmente envolvidos, são de difícil alinhamento e de elevado custo. Neste trabalho estuda-se a interferometria homódina de dois feixes em quadratura e as suas complexidades inerentes. Propõe-se uma nova arquitetura, baseada na configuração de Michelson, de alinhamento mais simples e de baixo custo. Descreve-se matematicamente o processo de obtenção dos sinais em quadratura deste arranjo. Também, se explora uma técnica capaz de obter dois sinais interferométricos em quadratura através da configuração tradicional de Michelson explorando-se a distribuição espacial do padrão de franjas. Desenvolve-se, ainda, um novo algoritmo de phase unwrapping aplicável como método de detecção de fase óptica, capaz de reconstruir a forma de onda de sinais de modulação e fornecer a diferença de fase estática entre os braços do interferômetro, quando o sinal de modulação possui valor médio nulo. Testes computacionais são realizados para corroborar na tarefa de evidenciar o potencial da técnica. Por meio do método de demodulação apresentado, em adição com o interferômetro proposto e da técnica explorada, realiza-se testes experimentais em um atuador piezoelétrico...
Abstract: Optical interferometers with single outputs are very sensitive when operating close to the phase quadrature point of their input-output characteristic curves. However, low frequency environmental fluctuations generate random drifts between the optical paths of the interferometer that deviate the quiescent point from the quadrature condition. This problem causes the phenomenon called signal fading. By electronically processing these two interferometry output signals, shifted by 90º, it is possible to demodulate the signal regardless of environmental drift. These kinds of interferometers, known as quadrature interferometers, are widely used in metrology laboratories, but, due to the large amount of optical components, they are expensive and difficult to design. In this work a low cost homodyne interferometer with two output quadrature beams based on the Michelson configuration is studied, and the procedure to achieve the quadrature signals is mathematically described. Also, a recent technique, not widely known in the literature and that is able to obtain two quadrature signals by using the standard configuration of the Michelson interferometer is explored, exploiting the spatial distribution of the fringe pattern. A new method for optical phase shift demodulation based on phase unwrapping is developed. This approach is able to recover not only the modulation signal waveform, but can also calculate the static phase shift between the interferometer arms when the modulation signal has an average value equal to zero. The method also has the ability to demodulate signals which vary arbitrarily in time. Computational test were done aiming to demonstrate the technique potential. By using this new optical phase shift demodulation method, combined with the proposed interferometer and exploiting the spatial distribution of the fringe pattern, a piezoelectric flextensional actuator is characterized. Displacement versus drive voltage and frequency ...
Mestre
Nečesal, Daniel. „Fázové zobrazování pod difrakčním limitem“. Master's thesis, Vysoké učení technické v Brně. Fakulta strojního inženýrství, 2020. http://www.nusl.cz/ntk/nusl-417067.
Der volle Inhalt der QuelleGuo, Yifan. „Developments in moire interferometry: carrier pattern technique and vibration insensitive interferometers“. Diss., Virginia Polytechnic Institute and State University, 1989. http://hdl.handle.net/10919/54181.
Der volle Inhalt der QuellePh. D.
Iacchetta, Alexander S. „Spatio-Spectral Interferometric Imaging and the Wide-Field Imaging Interferometry Testbed“. Thesis, University of Rochester, 2018. http://pqdtopen.proquest.com/#viewpdf?dispub=10936092.
Der volle Inhalt der QuelleThe light collecting apertures of space telescopes are currently limited in part by the size and weight restrictions of launch vehicles, ultimately limiting the spatial resolution that can be achieved by the observatory. A technique that can overcome these limitations and provide superior spatial resolution is interferometric imaging, whereby multiple small telescopes can be combined to produce a spatial resolution comparable to a much larger monolithic telescope. In astronomy, the spectrum of the sources in the scene are crucial to understanding the material composition of the sources. So, the ultimate goal is to have high-spatial-resolution imagery and obtain sufficient spectral resolution for all points in the scene. This goal can be accomplished through spatio-spectral interferometric imaging, which combines the aperture synthesis aspects of a Michelson stellar interferometer with the spectral capabilities of Fourier transform spectroscopy.
Spatio-spectral interferometric imaging can be extended to a wide-field imaging modality, which increases the collecting efficiency of the technique. This is the basis for NASA’s Wide-field Imaging Interferometry Testbed (WIIT). For such an interferometer, there are two light collecting apertures separated by a variable distance known as the baseline length. The optical path in one of the arms of the interferometer is variable, while the other path delay is fixed. The beams from both apertures are subsequently combined and imaged onto a detector. For a fixed baseline length, the result is many low-spatial-resolution images at a slew of optical path differences, and the process is repeated for many different baseline lengths and orientations. Image processing and synthesis techniques are required to reduce the large dataset into a single high-spatial-resolution hyperspectral image.
Our contributions to spatio-spectral interferometry include various aspects of theory, simulation, image synthesis, and processing of experimental data, with the end goal of better understanding the nature of the technique. We present the theory behind the measurement model for spatio-spectral interferometry, as well as the direct approach to image synthesis. We have developed a pipeline to preprocess experimental data to remove unwanted signatures in the data and register all image measurements to a single orientation, which leverages information about the optical system’s point spread function. In an experimental setup, such as WIIT, the reference frame for the path difference measured for each baseline is unknown and must be accounted for. To overcome this obstacle, we created a phase referencing technique that leverages point sources within the scene of known separation in order to recover unknown information regarding the measurements in a laboratory setting. We also provide a method that allows for the measurement of spatially and spectrally complicated scenes with WIIT by decomposing them prior to scene projection.
Vieira, Marcio Alexandre Pinto. „Analise vibracional de viga engastada utilizando a tecnica de moire : um estudo de caso“. [s.n.], 2005. http://repositorio.unicamp.br/jspui/handle/REPOSIP/257093.
Der volle Inhalt der QuelleDissertação (mestrado) - Universidade Estadual de Campinas, Faculdade de Engenharia Agricola
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Resumo: O fenômeno de vibração é de ocorrência comum na mecânica, geralmente associado à membros estruturais assim como elementos de maquinas. Particularmente, no campo da engenharia agrícola, vibração vem associada à ferimentos em vegetais nas operações de campo, que claramente inclui colheita, transporte e processamento. A escolha de membros estruturais simples, como as viga engastada, para validar o método, quando uma estrutura mais complexa for ser considerada. O nome moiré tem sua origem na língua francesa, referindo-se ao padrão de onda formado. O fenômeno é gerado quando telas são sobrepostas, produzindo padrões de ondas ou franjas, que se movem quando suas posições relativas são alteradas. O método selecionado é chamado método geométrico de moiré, que consiste em projetar uma grade sobre a superfície do objeto em estudo e superpor a foto original e a grade deformada. Software's especificos são empregados na análise de imagens. O objetivo do presente trabalho é determinar o deslocamento transversal da linha elástica na Teoria da viga engastada de Euler-Bernoulli, excitada por um excitador eletromagnético, utilizado em analise modal, utilizando a técnica de moiré descrita acima
Abstract: Vibration phenomena are of common occurrence in mechanics, generally associated to structural members as well as to machine elements. Particularly, in the field of agricultural engineering, vibration comes also associated to vegetable bruising during field operations, which clearly includes harvesting, transportation and processing. The selection of a simple structural member as a cantilever beam to support the utility of a moiré technique in studying vibration analysis is to validate the method when more complex structures are being considered. Vibration modes of a cantilever beam are easily determined by analytical methods. The name moiré has its origin in the French language, referring to wave like pattern. The phenomenon is generated when screens superposed, producing wave like patterns or fringes, which move when its relative positions are displaced. The selected method is named geometric moiré, which consists in projecting a grid onto the object in study and superposing both, the original and the deformed grid. Specific software's were employed in the image analysis. The objective of the present work is to determine the transversal displacement of the elastic line of Euler-Bernoulli cantilever beam being excited by an electromagnetic varying field using the moiré technique described above. Keywords: vibration, geometric moiré
Mestrado
Projetos, Desenvolvimento e Otimização de Maquinas Agricolas
Mestre em Engenharia Agrícola
Bins, Leonardo Sant'Anna 1961. „Estimação de fase absoluta e de linha de base em radar interferométrico de abertura sintética com múltiplas antenas“. [s.n.], 2014. http://repositorio.unicamp.br/jspui/handle/REPOSIP/261023.
Der volle Inhalt der QuelleTese (doutorado) - Universidade Estadual de Campinas, Faculdade de Engenharia Elétrica e de Computação
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Resumo: Dois problemas importantes na interferometria SAR (Synthetic Aperture Radar) são a estimação da fase absoluta e das linhas de base. O conhecimento preciso da fase absoluta e das linhas de base são fundamentais para a geração de modelos digitais de superfície ou terreno com alta precisão planimétrica e altimétrica. A estimação de fase absoluta consiste de duas etapas. A primeira etapa efetua o desdobramento da fase, o qual recupera a fase absoluta com os correspondentes múltiplos de 2?. A segunda etapa consiste na estimação do deslocamento de fase, causada pela combinação de erros de sincronização no sistema de aquisição de dados com erros de processamento da Interferometria SAR (InSAR). A estimação de linha de base consiste na determinação da posição da antena escrava relativa à posição da antena mestre (ou antena de referência). As contribuições desta tese consistem na concepção e na implementação de três métodos que se valem de múltiplas antenas (múltiplos interferogramas) para resolver esses dois problemas, como se segue. O primeiro método efetua o método de desdobramento de fase pontual, através do desdobramento de fase iterativo dos interferogramas, seguido da fusão dos mesmos, usando máxima verossimilhança. O segundo método refina a estimação de fase absoluta através da estimação do deslocamento de fase usando múltiplas antenas não colineares. O método se baseia na minimização da distorção geométrica (ou erro relativo) induzida pelo processamento com a presença de deslocamentos de fase com valores diferentes do verdadeiro. Uma das vantagens do método é que ele dispensa a instalação de refletores de canto na região imageada. Por último, um algoritmo do tipo Monte Carlo foi desenvolvido para a determinação das posições relativas das antenas escravas em relação à antena mestre. O método utiliza refletores de canto, cujas posições em campo são conhecidas, para reduzir o erro quadrático médio
Abstract: Two important issues in SAR interferometry (InSAR) are absolute phase and baseline estimation. The precise knowledge of these parameters is essential for the production of digital elevation models with high accuracy. The absolute phase estimation can be done in two steps. The first step performs the unwrapping of the phase, which retrieves the 2? multiples of the phase. The second step estimates the phase offset caused by a combination of errors in the acquisition system and in SAR interferometry (InSAR) processing. The baseline estimation determines the relative position of the slave antenna with respect to the master antenna (reference antenna). The contributions of this thesis consist in the design and implementation of three methods that use multiple antennas to address the above issues. The first method performs the unwrapping of the phase in a pixel based fashion, by iteratively unfolding the phase corresponding to each interferograma, followed by maximum likelihood fusion of the unwrapped phases. The second method refines the absolute phase estimation of the first step by incorporating a phase offset estimation based on multiple, noncollinear, antennas. This is achieved by minimizing the geometrical distortion (relative error) in the reconstructed digital elevation model induced by erroneous phase offsets in the interferograms. One advantage of this method is that it does not require the deployment of corner reflector in the area to be imaged. Lastly, the third method deals with baselines estimation. A baseline is determined by the relative positions of the slave and master antennas. The estimation is performed with a greedy stochastic algorithm of Monte Carlo type which uses corner reflectors with precisely known positions. A new position for the slave antenna is accepted when the mean square error of the corner reflector positions is reduced
Doutorado
Telecomunicações e Telemática
Doutor em Engenharia Elétrica
Ramasubramanian, Srikanth. „Design and development of a portable Moiré interferometer“. Morgantown, W. Va. : [West Virginia University Libraries], 2004. https://etd.wvu.edu/etd/controller.jsp?moduleName=documentdata&jsp%5FetdId=3460.
Der volle Inhalt der QuelleTitle from document title page. Document formatted into pages; contains x, 132 p. : ill. (some col.). Vita. Includes abstract. Includes bibliographical references (p. 131).
Featonby, Paul. „Atom interferometry“. Thesis, University of Oxford, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.390459.
Der volle Inhalt der QuelleBücher zum Thema "Interferometry"
R, Thompson A. Interferometry and synthesis in radio astronomy. Malabar, Fla: Krieger Pub., 1991.
Den vollen Inhalt der Quelle findenMałgorzata, Kujawińska, Pryputniewicz Ryszard J, Takeda Mitsuo 1946-, Society of Photo-optical Instrumentation Engineers. und Society for Experimental Stress Analysis (U.S.), Hrsg. Laser interferometry VIII--techniques and analysis: 6-7 August, 1996, Denver Colorado. Bellingham, Wash: SPIE--the International Society for Optical Engineering, 1996.
Den vollen Inhalt der Quelle findenP, Hariharan, und Malacara Daniel 1937-, Hrsg. Selected papers on interference, interferometry, and interferometric metrology. Bellingham, Wash: SPIE Optical Engineering Press, 1995.
Den vollen Inhalt der Quelle findenHanssen, Ramon F. Radar Interferometry. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/0-306-47633-9.
Der volle Inhalt der QuelleRastogi, Pramod K., Hrsg. Holographic Interferometry. Berlin, Heidelberg: Springer Berlin Heidelberg, 1994. http://dx.doi.org/10.1007/978-3-540-48078-5.
Der volle Inhalt der QuelleK, Rastogi P., Hrsg. Holographic interferometry. Berlin: Springer, 1994.
Den vollen Inhalt der Quelle finden1937-, Malacara Daniel, Hrsg. Selected papers on optical shop metrology. Bellingham, Wash., USA: SPIE Optical Engineering Press, 1990.
Den vollen Inhalt der Quelle findenUnited States. National Aeronautics and Space Administration., Hrsg. Solid state laser systems for space application: NASA grant NAG5-1319 : fo[u]rth semi-annual report, Summer '93. [Washington, DC: National Aeronautics and Space Administration, 1993.
Den vollen Inhalt der Quelle finden1937-, Malacara Daniel, Hrsg. Optical Shop Testing. New York: Wiley, 1992.
Den vollen Inhalt der Quelle findenUnited States. National Aeronautics and Space Administration., Hrsg. Solid state laser systems for space application. [Washington, DC]: National Aeronautics and Space Administration, 1994.
Den vollen Inhalt der Quelle findenBuchteile zum Thema "Interferometry"
Evans, Christopher J. „Interferometry“. In CIRP Encyclopedia of Production Engineering, 1–8. Berlin, Heidelberg: Springer Berlin Heidelberg, 2016. http://dx.doi.org/10.1007/978-3-642-35950-7_16700-3.
Der volle Inhalt der QuelleNolte, David D. „Interferometry“. In Optical Interferometry for Biology and Medicine, 3–48. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0890-1_1.
Der volle Inhalt der QuelleKervella, Pierre. „Interferometry“. In Encyclopedia of Astrobiology, 1–6. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_792-5.
Der volle Inhalt der QuelleIizuka, Keigo. „Interferometry“. In Engineering Optics, 651–82. Cham: Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-319-69251-7_21.
Der volle Inhalt der QuelleEvans, Christopher J. „Interferometry“. In CIRP Encyclopedia of Production Engineering, 710–17. Berlin, Heidelberg: Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-20617-7_16700.
Der volle Inhalt der QuelleKervella, Pierre. „Interferometry“. In Encyclopedia of Astrobiology, 1212–17. Berlin, Heidelberg: Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_792.
Der volle Inhalt der QuelleGross, Herbert, Bernd Dörband und Henriette Müller. „Interferometry“. In Handbook of Optical Systems, 1–180. Weinheim, Germany: Wiley-VCH Verlag GmbH & Co. KGaA, 2015. http://dx.doi.org/10.1002/9783527699230.ch1.
Der volle Inhalt der QuelleTotzeck, Michael. „Interferometry“. In Springer Handbook of Lasers and Optics, 1255–83. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-19409-2_16.
Der volle Inhalt der QuelleMertz, Lawrence. „Interferometry“. In Excursions in Astronomical Optics, 47–77. New York, NY: Springer New York, 1996. http://dx.doi.org/10.1007/978-1-4612-2386-3_3.
Der volle Inhalt der QuelleEvans, Christopher J. „Interferometry“. In CIRP Encyclopedia of Production Engineering, 966–73. Berlin, Heidelberg: Springer Berlin Heidelberg, 2019. http://dx.doi.org/10.1007/978-3-662-53120-4_16700.
Der volle Inhalt der QuelleKonferenzberichte zum Thema "Interferometry"
Dowling, Jonathan P., und Marian O. Scully. „Quantum-noise limits to matter-wave interferometry“. In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1993. http://dx.doi.org/10.1364/oam.1993.thoo.4.
Der volle Inhalt der QuelleCampbell, Gene, Gary E. Sommargren und Bruce E. Truax. „Image Acquisition for High Accuracy Interferometry“. In Optical Fabrication and Testing. Washington, D.C.: Optica Publishing Group, 1998. http://dx.doi.org/10.1364/oft.1998.owc.2.
Der volle Inhalt der QuelleReasenberg, Robert D. „POINTS Optics: Challenges and Options“. In Space Optics for Astrophysics and Earth and Planetary Remote Sensing. Washington, D.C.: Optica Publishing Group, 1991. http://dx.doi.org/10.1364/soa.1991.tuc2.
Der volle Inhalt der QuelleRiza, Nabeel A. „In-Line Acousto-Optic Architectures for Holographic Interferometry and Sensing“. In Holography. Washington, D.C.: Optica Publishing Group, 1996. http://dx.doi.org/10.1364/holography.1996.hma.4.
Der volle Inhalt der QuelleDevoe, R. G., C. Fabre, K. Jungmann, J. Hoffnagle und R. G. Brewer. „Precision interferometry with stabilized lasers“. In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1987. http://dx.doi.org/10.1364/oam.1987.wm3.
Der volle Inhalt der QuelleStahl, H. Phil. „Performance of an Infrared Phase-Shifting Interferometric System“. In Optical Fabrication and Testing. Washington, D.C.: Optica Publishing Group, 1985. http://dx.doi.org/10.1364/oft.1985.thcc1.
Der volle Inhalt der QuelleDevoe, R. G., C. Fabre, K. Jungmann, J. Hoffnagle und R. G. Brewer. „Optical heterodyne interferometry“. In OSA Annual Meeting. Washington, D.C.: Optica Publishing Group, 1986. http://dx.doi.org/10.1364/oam.1986.mw1.
Der volle Inhalt der QuelleBen-Chorin, Moshe, Silvia Chuartzman und Yehiam Prior. „Absolute distance measurements using a noisy interferometer“. In The European Conference on Lasers and Electro-Optics. Washington, D.C.: Optica Publishing Group, 1998. http://dx.doi.org/10.1364/cleo_europe.1998.cfd4.
Der volle Inhalt der QuelleWilliams, Rick A., und Osuk Y. Kwon. „Subaperture Interferometric Testing of Aspheric Optics“. In Optical Fabrication and Testing. Washington, D.C.: Optica Publishing Group, 1987. http://dx.doi.org/10.1364/oft.1987.thaa3.
Der volle Inhalt der QuelleReynaud, Francois, J. J. Alleman und H. Lagorceix. „Interferometric fiber arms for stellar interferometry“. In Garmisch - DL tentative, herausgegeben von Guy Cerutti-Maori und Philippe Roussel. SPIE, 1994. http://dx.doi.org/10.1117/12.185277.
Der volle Inhalt der QuelleBerichte der Organisationen zum Thema "Interferometry"
Pritchard, David E. Atom Interferometry. Fort Belvoir, VA: Defense Technical Information Center, Dezember 2001. http://dx.doi.org/10.21236/ada397658.
Der volle Inhalt der QuelleEichel, P. H., D. C. Ghiglia und C. V. Jr Jakowatz. Spotlight SAR interferometry for terrain elevation mapping and interferometric change detection. Office of Scientific and Technical Information (OSTI), Februar 1996. http://dx.doi.org/10.2172/211364.
Der volle Inhalt der QuelleFitch, J. P. Single antenna interferometry. Office of Scientific and Technical Information (OSTI), Dezember 1989. http://dx.doi.org/10.2172/7247425.
Der volle Inhalt der QuelleGoldberg, Kenneth A. Extreme ultraviolet interferometry. Office of Scientific and Technical Information (OSTI), Dezember 1997. http://dx.doi.org/10.2172/658173.
Der volle Inhalt der QuelleErskine, D. Techniques in Broadband Interferometry. Office of Scientific and Technical Information (OSTI), Januar 2004. http://dx.doi.org/10.2172/15009760.
Der volle Inhalt der QuelleTringe, J. W., M. C. Converse und R. J. Kane. Develop Prototype Microwave Interferometry Diagnostic. Office of Scientific and Technical Information (OSTI), November 2016. http://dx.doi.org/10.2172/1335776.
Der volle Inhalt der QuelleFriedman. Adaptive Optics, LLLFT Interferometry, Astronomy. Fort Belvoir, VA: Defense Technical Information Center, März 2002. http://dx.doi.org/10.21236/ada415904.
Der volle Inhalt der QuellePritchard, David E. New Developments in Atom Interferometry. Fort Belvoir, VA: Defense Technical Information Center, Juli 1992. http://dx.doi.org/10.21236/ada254094.
Der volle Inhalt der QuelleTownes, Charles H. Support of Infrared Spatial Interferometry. Fort Belvoir, VA: Defense Technical Information Center, Mai 1996. http://dx.doi.org/10.21236/ada310085.
Der volle Inhalt der QuelleDainty, J. C. High Annular Resolution Stellar Interferometry. Fort Belvoir, VA: Defense Technical Information Center, Juli 1985. http://dx.doi.org/10.21236/ada168755.
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