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Готові списки джерел за темами / Interferometry

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Добірка наукової літератури з теми "Interferometry"

Автор: Grafiati

Опубліковано: 4 червня 2021

Оновлено: 25 липня 2025

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Статті в журналах з теми "Interferometry"

1

Chesneau, O., K. Rousselet-Perraut, and F. Vakili. "Interferometry and Stellar Magnetism." International Astronomical Union Colloquium 175 (2000): 174–77. http://dx.doi.org/10.1017/s0252921100055792.

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AbstractThe classical detection of magnetic fields in Be stars remains a challenge due to the sensitivity threshold and geometrical cancelation of the field effects. We propose to study the Zeeman effect using Spectro-Polarimetric INterferometry (SPIN) which consists of the simultaneous use of polarimetry and very high angular resolution provided by long baseline interferometers. As monitoring of the instrumental polarisation is mandatory in order to calibrate interferometric observations in any case, the polarised signal is a natural by-product of interferometers. This method will be tested o

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2

McAlister, Harold A. "Overview of Multiple–Aperture Interferometry Binary Star Results from the Northern Hemisphere." Proceedings of the International Astronomical Union 2, S240 (2006): 35–44. http://dx.doi.org/10.1017/s1743921307003778.

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AbstractLong-baseline optical interferometry (LBI) can nearly close the gap in selection space between astrometric and spectroscopic detection of binary star systems, bringing the complementary powers of astrometry and spectroscopy to bear on a complete dynamical understanding of such systems, particularly including the determination of the masses of the individual stellar components. In the case of double-lined spectroscopic systems, their resolution by long-baseline interferometry also yields the orbital parallax and hence the luminosities of the individual stars. In some of these cases, the

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3

Jankov, S. "Astronomical optical interferometry, I: Methods and instrumentation." Serbian Astronomical Journal, no. 181 (2010): 1–17. http://dx.doi.org/10.2298/saj1081001j.

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Previous decade has seen an achievement of large interferometric projects including 8-10m telescopes and 100m class baselines. Modern computer and control technology has enabled the interferometric combination of light from separate telescopes also in the visible and infrared regimes. Imaging with milli-arcsecond (mas) resolution and astrometry with micro-arcsecond (?as) precision have thus become reality. Here, I review the methods and instrumentation corresponding to the current state in the field of astronomical optical interferometry. First, this review summarizes the development from the

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4

Trolinger, James D., Amit Lal, Joshua Jo, and Stephen Kupiec. "Programmable Holographic Optical Elements as Adaptive Optics in Optical Diagnostics Devices." Key Engineering Materials 437 (May 2010): 108–12. http://dx.doi.org/10.4028/www.scientific.net/kem.437.108.

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This paper reports a combined, Hartmann/Digital Holographic interferometry inspection system for inspecting optical components that do not easily lend themselves to conventional interferometric or Hartmann inspection. A programmable holographic optical element (HOE) preconditions wavefronts to extend the dynamic range of interferometry measurements and also transforms the same system into a scanning Hartmann operation, which has lower resolution but higher dynamic range. Inspecting aspherical surfaces with existing interferometers requires special, computer generated holographic optical elemen

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5

Cavedo, Federico, Parisa Esmaili, Alessandro Pesatori, and Michele Norgia. "Self-mixing Interferometer: Frequency Modulation Noise Dependence on Laser Source." Journal of Physics: Conference Series 2698, no. 1 (2024): 012019. http://dx.doi.org/10.1088/1742-6596/2698/1/012019.

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Abstract The acquisition of frequency modulation in self-mixing interferometry opens the way to a new generation of instruments, with significantly superior performance compared to traditional self-mixing interferometers. In this work, we experimentally confirm the noise limit dependence of this kind of interferometer on the laser source linewidth. The obtained results confirm the theoretical prediction, opening the way for a deeper improvement in sensitivity, by employing narrow-line lasers in this interferometric configuration.

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6

Yankelev, Dimitry, Chen Avinadav, Nir Davidson, and Ofer Firstenberg. "Atom interferometry with thousand-fold increase in dynamic range." Science Advances 6, no. 45 (2020): eabd0650. http://dx.doi.org/10.1126/sciadv.abd0650.

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The periodicity inherent to any interferometric signal entails a fundamental trade-off between sensitivity and dynamic range of interferometry-based sensors. Here, we develop a methodology for substantially extending the dynamic range of such sensors without compromising their sensitivity, stability, and bandwidth. The scheme is based on simultaneous operation of two nearly identical interferometers, providing a moiré-like period much larger than 2π and benefiting from close-to-maximal sensitivity and from suppression of common-mode noise. The methodology is highly suited to atom interferomete

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7

Stee, Ph, D. Bonneau, F. Morand, D. Mourard, and 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.

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The capability of optical long baseline interferometry for measuring the angular diameter of stars or binary separation is now well established. However, for the imaging of photospheric disk structures one needs very long baseline interferometers operated in the multi-telescope phase-closure technique. In this paper we will stress the capability of spectro-interferometric measurements to constrain the physics of hot stars. We will report our study of the interacting binary, β Lyrae, and the mass-losing Be star γ Cassiopeiae. We will look at the interpretation of both the modulus and phase data

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8

Pushin, D. A., M. G. Huber, M. Arif, et al. "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.

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Neutron interferometry has proved to be a very precise technique for measuring the quantum mechanical phase of a neutron caused by a potential energy difference between two spatially separated neutron paths inside interferometer. The path length inside the interferometer can be many centimeters (and many centimeters apart) making it very practical to study a variety of samples, fields, potentials, and other macroscopic medium and quantum effects. The precision of neutron interferometry comes at a cost; neutron interferometers are very susceptible to environmental noise that is typically mitiga

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9

Naeem, Muddasir, and Tayyab Imran. "ZEMAX Simulations and Experimental Validation of Laser Interferometers." Photonics 12, no. 3 (2025): 206. https://doi.org/10.3390/photonics12030206.

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This study presents the design, simulation, and experimental validation of six fundamental laser interferometer types: Sagnac, Mach–Zehnder, Michelson, Twyman–Green, Fizeau, and Fabry–Pérot. Using ZEMAX OpticStudio in non-sequential mode with the physical optics propagation (POP) algorithm, the simulations provide detailed insights into the optical performance of these interferometers. A direct comparison is made between the simulated and experimental fringe patterns, coherent irradiance distributions, and phase plots, demonstrating strong agreement and validating the accuracy of computational

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10

Noordam, J. E. "European Space Interferometry." Symposium - International Astronomical Union 166 (1995): 345. http://dx.doi.org/10.1017/s0074180900228349.

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Optical interferometry is ensconced as an ‘area of future interest’ (a socalled Green Dream) in Horizon 2000, the long-term scientific plan of ESA. Over the years, there have been three large ESA workshops on Space interferometry, where many different concepts and designs were proposed, and several ESA committees have studied the possibilities. These committees were also involved, in an advisory role, in a modest technological research program (TRP) by ESTEC. In 1990, the Space Interferometry Study Team (SIST) recommended building an optical interferometer, consisting of 10-15 small telescopes

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Дисертації з теми "Interferometry"

1

Ho, Lap. "High precision short-baseline pointing system using GPS interferometry." Ohio : Ohio University, 1995. http://www.ohiolink.edu/etd/view.cgi?ohiou1179435242.

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2

Lemes, 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.

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Made available in DSpace on 2014-12-02T11:16:55Z (GMT). No. of bitstreams: 0 Previous issue date: 2014-03-27Bitstream added on 2014-12-02T11:20:53Z : No. of bitstreams: 1 000795995.pdf: 2794066 bytes, checksum: f46bd6b9d4e609f70fa6e80ae87f6cae (MD5)<br>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, l

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3

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.

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Orientador: Cláudio Kitano<br>Banca: Ricardo Tokio Higuti<br>Banca: Ronny Calixto Carbonari<br>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,

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4

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.

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Tato diplomová práce se zabývá konstrukcí interferenčních zařízení pro výzkum měření fáze světla na mikro-strukturách a fáze plazmonů na nano-strukturách. V první kapitole je vybudován teoretický základ pro optiku a nano-fotoniku používané v budoucích kapitolách. Následně je popsána interference vln a jejich praktické použití pro prolomení difrakčního limitu pomocí holografie plazmonů. Prvním experimentální sestavou je Machův-Zehnderův holografický mikroskop. Je popsán způsob, jak ho sestavit z běžně dostupných součástek a jak je navržen ovládací software k jeho používání. Následně jsou popsán

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5

Guo, 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.

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Due to the rapid expansion of applications of composite materials, investigations of their properties have greatly increased. Since theoretical and numerical methods have many limitations for anisotropic materials, experimental methods are sometimes the only way to answer the questions. It has been proved that moire interferometry is a powerful technique in the study of composite materials. The high sensitivity and resolution of a measurement technique is the key to determining the properties of a material which has a fine and complicated structure such as fiber reinforced composite lamina

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6

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.

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<p> The 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

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7

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.

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Orientador: Inacio Maria Dal Fabbro<br>Dissertação (mestrado) - Universidade Estadual de Campinas, Faculdade de Engenharia Agricola<br>Made available in DSpace on 2018-08-08T06:46:24Z (GMT). No. of bitstreams: 1 Vieira_MarcioAlexandrePinto_M.pdf: 3890763 bytes, checksum: ec176daee99c277e022ce62c1efe297e (MD5) Previous issue date: 2005<br>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

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8

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.

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Orientador: Max Henrique Machado Costa<br>Tese (doutorado) - Universidade Estadual de Campinas, Faculdade de Engenharia Elétrica e de Computação<br>Made available in DSpace on 2018-08-24T13:29:51Z (GMT). No. of bitstreams: 1 Bins_LeonardoSant'Anna_D.pdf: 7799361 bytes, checksum: 9e2474fa080f4e6f30dd2971af9cd670 (MD5) Previous issue date: 2014<br>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 digita

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9

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.

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Thesis (M.S.)--West Virginia University, 2004.<br>Title from document title page. Document formatted into pages; contains x, 132 p. : ill. (some col.). Vita. Includes abstract. Includes bibliographical references (p. 131).

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10

Featonby, Paul. "Atom interferometry." Thesis, University of Oxford, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.390459.

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Книги з теми "Interferometry"

1

R, Thompson A. Interferometry and synthesis in radio astronomy. Krieger Pub., 1991.

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2

Małgorzata, Kujawińska, Pryputniewicz Ryszard J, Takeda Mitsuo 1946-, Society of Photo-optical Instrumentation Engineers., and Society for Experimental Stress Analysis (U.S.), eds. Laser interferometry VIII--techniques and analysis: 6-7 August, 1996, Denver Colorado. SPIE--the International Society for Optical Engineering, 1996.

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3

P, Hariharan, and Malacara Daniel 1937-, eds. Selected papers on interference, interferometry, and interferometric metrology. SPIE Optical Engineering Press, 1995.

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4

Hanssen, Ramon F. Radar Interferometry. Springer Netherlands, 2001. http://dx.doi.org/10.1007/0-306-47633-9.

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5

Rastogi, Pramod K., ed. Holographic Interferometry. Springer Berlin Heidelberg, 1994. http://dx.doi.org/10.1007/978-3-540-48078-5.

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6

K, Rastogi P., ed. Holographic interferometry. Springer, 1994.

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7

1937-, Malacara Daniel, ed. Selected papers on optical shop metrology. SPIE Optical Engineering Press, 1990.

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8

United States. National Aeronautics and Space Administration., ed. Solid state laser systems for space application: NASA grant NAG5-1319 : fo[u]rth semi-annual report, Summer '93. National Aeronautics and Space Administration, 1993.

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9

1937-, Malacara Daniel, ed. Optical Shop Testing. Wiley, 1992.

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10

United States. National Aeronautics and Space Administration., ed. Solid state laser systems for space application. National Aeronautics and Space Administration, 1994.

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Частини книг з теми "Interferometry"

1

Evans, Christopher J. "Interferometry." In CIRP Encyclopedia of Production Engineering. Springer Berlin Heidelberg, 2016. http://dx.doi.org/10.1007/978-3-642-35950-7_16700-3.

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2

Nolte, David D. "Interferometry." In Optical Interferometry for Biology and Medicine. Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0890-1_1.

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3

Kervella, Pierre. "Interferometry." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-27833-4_792-5.

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4

Iizuka, Keigo. "Interferometry." In Engineering Optics. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-319-69251-7_21.

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5

Evans, Christopher J. "Interferometry." In CIRP Encyclopedia of Production Engineering. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-642-20617-7_16700.

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6

Kervella, Pierre. "Interferometry." In Encyclopedia of Astrobiology. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-44185-5_792.

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7

Gross, Herbert, Bernd Dörband, and Henriette Müller. "Interferometry." In Handbook of Optical Systems. Wiley-VCH Verlag GmbH & Co. KGaA, 2015. http://dx.doi.org/10.1002/9783527699230.ch1.

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Totzeck, Michael. "Interferometry." In Springer Handbook of Lasers and Optics. Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-19409-2_16.

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Mertz, Lawrence. "Interferometry." In Excursions in Astronomical Optics. Springer New York, 1996. http://dx.doi.org/10.1007/978-1-4612-2386-3_3.

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Evans, Christopher J. "Interferometry." In CIRP Encyclopedia of Production Engineering. Springer Berlin Heidelberg, 2019. http://dx.doi.org/10.1007/978-3-662-53120-4_16700.

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Тези доповідей конференцій з теми "Interferometry"

1

Habib, K., and F. Al-Sabti. "3D-Interferometric Microscopy of Pitting Corrosion." In CORROSION 1997. NACE International, 1997. https://doi.org/10.5006/c1997-97289.

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Abstract An optical corrosion-meter has been developed for materials testing and evaluation of different corrosion phenomena. The idea of the optical corrosion-meter was established based on principles of 3D-holographic interferometry for measuring microsurface dissolution, i.e. mass loss, and on those of electrochemistry for measuring the bulk electronic current, i.e. corrosion current of metallic samples in aqueous solutions. An early stage of pitting corrosion of aluminium and copper in seawater was monitored in situ by the optical corrosion-meter during the cyclic polarization test. The ob

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2

Habib, K. "Detection of Crevice Corrosion of Metallic Alloys by Optical Interferometry." In CORROSION 1999. NACE International, 1999. https://doi.org/10.5006/c1999-99218.

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Abstract In the present investigation, an optical corrosion-meter has been developed for materials testing and evaluation of different corrosion phenomena. The idea of the optical corrosion-meter was established based on principles of 3D-holographic interferometry for measuring microsurface dissolution,i.e. mass loss, and on those of electrochemistry for measuring the bulk electronic current, i.e. corrosion current of metallic samples in aqueous solutions. In the present work, an early stage of crevice corrosion of a titanium alloy, a carbon steel and a pure aluminum in seawater was monitored

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3

Dowling, Jonathan P., and Marian O. Scully. "Quantum-noise limits to matter-wave interferometry." In OSA Annual Meeting. Optica Publishing Group, 1993. http://dx.doi.org/10.1364/oam.1993.thoo.4.

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The field of atom interferometry1 is interesting since the potential sensitivity of matter-wave interferometers far exceeds that of their light-wave antecedents.2 As was emphasized at the recent Solvay conference on quantum optics, there is at present no paradigm available for calculating the quantum noise limits to matter-wave interferometers.3 We show that the phase uncertainty is inversely proportional to the square root of the total number, rather than the mean number, of atoms in the interferometert.4 We find that a matter-wave interferometer used as a gyroscope can be expected to be more

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4

Reasenberg, Robert D. "POINTS Optics: Challenges and Options." In Space Optics for Astrophysics and Earth and Planetary Remote Sensing. Optica Publishing Group, 1991. http://dx.doi.org/10.1364/soa.1991.tuc2.

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It has been widely recognized for several years that interferometric instruments will play a major role in many aspects of space-based optical astronomy. More recently, optical interferometry received very favorable treatment in the AASC (Bahcall Committee) report and the POINTS mission is a close match to the Astrometric Interferometry Mission that the report lists as a moderate space-based program. In the next century, milliarcsecond-and submilliarcsecond-resolution images will likely be obtained from interferometric instruments deployed in space. An important precursor to such imaging instr

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5

Campbell, Gene, Gary E. Sommargren, and Bruce E. Truax. "Image Acquisition for High Accuracy Interferometry." In Optical Fabrication and Testing. Optica Publishing Group, 1998. http://dx.doi.org/10.1364/oft.1998.owc.2.

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In phase shifting interferometry, the image acquisition electronics have largely been ignored, because the overall measurement accuracy has generally been limited by the quality of the reference wave. A recently developed interferometer, the phase shifting diffraction interferometer,[1] provides a high quality reference wave, which has been measured to be better than λ/8000 rms. With such a reference wave, the interferometer accuracy then becomes limited by systematic errors in the image acquisition electronics. This paper presents a variety of issues that arise when using image acquisition el

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6

Riza, Nabeel A. "In-Line Acousto-Optic Architectures for Holographic Interferometry and Sensing." In Holography. Optica Publishing Group, 1996. http://dx.doi.org/10.1364/holography.1996.hma.4.

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Novel two Bragg cell and one Bragg cell acousto-optic (AO) interferometers are introduced in this paper. These interferometers can be used as a variety of optical instruments such as holographic interferometers, interferometric sensors, material characterization tools, and diagnostic measurement systems such as turbulence and flow/temperature assessment. To this date, to the best of the author’s knowledge, no such optical systems have been proposed for interferometric sensing and measurement tools that offer high optical power (e.g., 1 W CW), high speed scanning (e.g., < 50 μs per scan spot

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7

Devoe, R. G., C. Fabre, K. Jungmann, J. Hoffnagle, and R. G. Brewer. "Precision interferometry with stabilized lasers." In OSA Annual Meeting. Optica Publishing Group, 1987. http://dx.doi.org/10.1364/oam.1987.wm3.

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Interferometers are essential tools for measuring optical wavelengths and frequencies. We demonstrate a new form of interferometry that is both simpler and more precise than conventional methods. Stable laser and electrooptic FM sideband techniques make a direct electronic measurement of the mode spacing of an ultrahigh finesse cavity with subhertz precision (0.4-Hz rms) over a 50-THz region. A new interferometer equation is derived in which all variables can be measured directly in situ. Experiments indicate errors below 10−10 over a 50-THz bandwidth and that the technique can be improved to

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8

Stahl, H. Phil. "Performance of an Infrared Phase-Shifting Interferometric System." In Optical Fabrication and Testing. Optica Publishing Group, 1985. http://dx.doi.org/10.1364/oft.1985.thcc1.

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An infrared phase-shifting interferometric system has been developed at the University of Arizona Optical Sciences Center. It is a compact, self-contained, easy to align and operate, next generation optical shop instrument. The principle applications for an infrared interferometer are: 1) inspection of infrared materials in transmission for index homogeneity and internal defects, 2) interferometry of surfaces, such as an asphere, whose slopes are too steep for the fringes to be resolved by a visible interferometer, and 3) interferometry of surfaces that are too rough to be tested at visible wa

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9

Devoe, R. G., C. Fabre, K. Jungmann, J. Hoffnagle, and R. G. Brewer. "Optical heterodyne interferometry." In OSA Annual Meeting. Optica Publishing Group, 1986. http://dx.doi.org/10.1364/oam.1986.mw1.

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We describe a new approach to precision interferometry that is in principle different from previous techniques in that it is free from the systematic errors usually associated with interferometry. Optical heterodyne techniques are used to directly measure the empirical mode spacing of an interferometer over a broad (10%) frequency range. The frequency difference between any two modes can then be computed by summing the spacing of the modes that lie between them, in this way optical frequency differences of up to 50 THz can be measured without the usual corrections for mirror phase shift or dif

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10

Ben-Chorin, Moshe, Silvia Chuartzman, and Yehiam Prior. "Absolute distance measurements using a noisy interferometer." In The European Conference on Lasers and Electro-Optics. Optica Publishing Group, 1998. http://dx.doi.org/10.1364/cleo_europe.1998.cfd4.

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The spectrum of white light passing through a Michelson interferometer develops a sinusoidal modulation, the frequency of which is determined by the path difference between the interferometer arms. Dispersive white light interferometry is capable of measuring relatively large distances (hundreds of µm) with high precision, and without moving parts. However, as with all interferometric methods, it is very sensitive to phase noise arising from such factors as vibrations or air turbulence. The random phase jumps reduce the visibility of the white light fringes. This limitation imposes stringent c

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Звіти організацій з теми "Interferometry"

1

Pritchard, David E. Atom Interferometry. Defense Technical Information Center, 2001. http://dx.doi.org/10.21236/ada397658.

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Eichel, P. H., D. C. Ghiglia, and C. V. Jr Jakowatz. Spotlight SAR interferometry for terrain elevation mapping and interferometric change detection. Office of Scientific and Technical Information (OSTI), 1996. http://dx.doi.org/10.2172/211364.

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3

Fitch, J. P. Single antenna interferometry. Office of Scientific and Technical Information (OSTI), 1989. http://dx.doi.org/10.2172/7247425.

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4

Goldberg, Kenneth A. Extreme ultraviolet interferometry. Office of Scientific and Technical Information (OSTI), 1997. http://dx.doi.org/10.2172/658173.

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5

Erskine, D. Techniques in Broadband Interferometry. Office of Scientific and Technical Information (OSTI), 2004. http://dx.doi.org/10.2172/15009760.

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Tringe, J. W., M. C. Converse, and R. J. Kane. Develop Prototype Microwave Interferometry Diagnostic. Office of Scientific and Technical Information (OSTI), 2016. http://dx.doi.org/10.2172/1335776.

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Friedman. Adaptive Optics, LLLFT Interferometry, Astronomy. Defense Technical Information Center, 2002. http://dx.doi.org/10.21236/ada415904.

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Pritchard, David E. New Developments in Atom Interferometry. Defense Technical Information Center, 1992. http://dx.doi.org/10.21236/ada254094.

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9

Townes, Charles H. Support of Infrared Spatial Interferometry. Defense Technical Information Center, 1996. http://dx.doi.org/10.21236/ada310085.

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Dainty, J. C. High Annular Resolution Stellar Interferometry. Defense Technical Information Center, 1985. http://dx.doi.org/10.21236/ada168755.

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