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Journal articles on the topic 'Michelson interferometer'

Author: Grafiati

Published: 4 June 2021

Last updated: 25 July 2025

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1

Mamadjanov, A. I., A. Turgunov, and M. Umaraliyev. "INVESTIGATE THE DEPENDENCE OF THE LIGHT REFRACTIVE INDEX OF AN IDEAL GAS ON ITS PRESSURE USING INTERFEROMETERS." International Journal of Advanced Research 8, no. 12 (2020): 272–79. http://dx.doi.org/10.21474/ijar01/12147.

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This article analyzes the working principle of the Michelson interferometer and the ability to measure some physical quantities. Using the Michelson Interferometer, the ability to detect not only the light wave but also the full wavelength of radio waves was analyzed. Using the Mach-Zehnder and Michelson interferometers, it was determined that the refractive index of air depends on its pressure. The results obtained in two different interferometers were compared comparatively in the graphs.

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Shyu, Lih Horng, Yung Cheng Wang, and Jui Cheng Lin. "A Compact Signal Processing with Position Sensitive Detectors Utilized for Michelson Interferometer." Key Engineering Materials 437 (May 2010): 98–102. http://dx.doi.org/10.4028/www.scientific.net/kem.437.98.

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Interferometric signals of a homodyne Michelson interferometer appear in sinusoidal forms. In this investigation, new concepts for signal processing of Michelson interferometer are demonstrated. With the utilization of detection of position sensitive detector (PSD) and by the procedure of differential signals and the characteristic of symmetric waveform, a compact signal processing for homodyne Michelson interferometer has been developed. Its advantages include simplified procedure, fast processing and few electronic hardware. For experiment tests of the signal processing, a conventional homod

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3

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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Kravets, Е., and E. Semenova. "A Research of Intermodulation Components in Laser Vibrometers for Precise Measurement of Oscillations." Proceedings of Telecommunication Universities 10, no. 2 (2024): 57–66. http://dx.doi.org/10.31854/1813-324x-2024-10-2-57-66.

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This paper presents the results of theoretical research of signals of laser vibrometers, with the surface of the object of interest orthogonal to the direction of the beam. The article shows that the Michelson interferometer based vibrometer may yield erroneous results when measuring the amplitude of oscillations. The errors arise due to the phase shift between the interfering beams, which affects the measurement of the absolute value of surface shift. The article presents theoretical analysis of the spectra of the output signals of interferometers of various designs. For the Michelson interfe

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5

Giacomo, Pierre. "The Michelson interferometer." Mikrochimica Acta 93, no. 1-6 (1987): 19–31. http://dx.doi.org/10.1007/bf01201680.

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6

Ahmedov, Haci, Mehnet Celik, Recep Orhan, Beste Korutlu, Sahin Ersoy, and Ramiz Hamid. "A UME Kibble balance displacement measurement procedure." ACTA IMEKO 9, no. 3 (2020): 11. http://dx.doi.org/10.21014/acta_imeko.v9i3.766.

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<p>The redefinition of the kilogram in terms of Planck constant came into effect on 20 May 2019. The National Metrology Institute of Turkey (UME) realised the new definition by means of the oscillating magnet Kibble balance. The novel dynamical measurement procedure developed for Kibble balance in Turkey has the advantage of being less sensitive to environmental disturbances compared to the traditional Kibble balance experiments. Precise displacement measurements are performed either with Michelson or Fabry-Perot interferometers in worldwide Kibble balances. Moreover, most of them operat

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Lin, Xu Ling, Huan Li, Jian Bing Zhang, and Zhi Min Dai. "Design a Modified Michelson Interferometer for THz Spectrum Measurement." Advanced Materials Research 760-762 (September 2013): 1335–38. http://dx.doi.org/10.4028/www.scientific.net/amr.760-762.1335.

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In this paper, a modified Michelson interferometer is designed to measure Terahertz spectrum. Compared with normal Michelson interferometer, hollow retroreflectors are used instead of flat mirrors as reflective mirrors. The theory analysis and some measurement are given.

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8

Shepherd, G. G., W. A. Gault, and R. A. Koehler. "The development of wide-angle Michelson interferometers in Canada." Canadian Journal of Physics 69, no. 8-9 (1991): 1175–83. http://dx.doi.org/10.1139/p91-178.

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The history of wide-angle Michelson interferometers in Canada began in 1961, in Paris. This will culminate with the launch of the WINDII (WIND Imaging Interferometer) instrument in 1991, precisely 30 years later. The intervening developments are reviewed, and possible future directions are described.

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Volkov, Petr, Andrey Lukyanov, Alexander Goryunov, Daniil Semikov, and Oleg Vyazankin. "Low-Coherence Homodyne Interferometer for Sub-Megahertz Fiber Optic Sensor Readout." Sensors 24, no. 2 (2024): 552. http://dx.doi.org/10.3390/s24020552.

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This study proposes a method for interferometric fiber optic sensor readouts. The method utilizes the advantages of the active homodyne demodulation technique and low-coherence interferometry. The usage of the tandem low-coherence interferometer enables modulating the reference interferometer without any changes to the sensor. This achieves high sensitivity, high stability, and a wide frequency band. A sensitivity of up to 0.1 nm (RMS) in the frequency range of 5 kHz is demonstrated by detecting acoustic signals with a fiber Michelson interferometer as a sensor.

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10

Quirrenbach, A. "Stellar Diameters, Limb Darkening, Extended Atmospheres, and Shells: Observations with the MKIII Interferometer." Symposium - International Astronomical Union 158 (1994): 407–9. http://dx.doi.org/10.1017/s007418090010806x.

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The resolution of close binaries and direct measurements of stellar angular diameters were the first achievements of astronomical interferometry (Michelson and Pease 1921). Fringe tracking interferometers are now capable of producing visibility measurements which are sufficiently sensitive and well-calibrated to make more sophisticated measurements possible. Results from current instruments include measurements of limb darkening, of the wavelength-dependence of stellar diameters, and of non-spherical stars, and observations with narrow spectral bands. This paper summarizes recent results from

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11

Stávek, Jiří. "The Descartes Code (Spin Orbital Rotation of Photons)–I. The Fourth-Order Effects in the Michelson Interferometer." European Journal of Applied Physics 5, no. 6 (2023): 25–30. http://dx.doi.org/10.24018/ejphysics.2023.5.6.291.

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In 1887 Michelson and Morley published their very important paper with the null result in the Michelson interferometer. Since that time there were published several hundred papers with various ad hoc hypotheses to interpret this unexpected result but none of these attempts was accepted to offer an alternative to Einstein’s 1905 theory. In order to avoid this trap with ad hoc models we have combined knowledge of Old Masters and derived a new description of the longitudinal and transverse arms of the Michelson interferometer. In this model the fourth-order effect of (v/c)4 was derived where v is

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12

Sullivan, Woodruff T. "Some Highlights of Interferometry in early Radio Astronomy." International Astronomical Union Colloquium 131 (1991): 132–49. http://dx.doi.org/10.1017/s025292110001321x.

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AbstractTwo important episodes in the early development of interferometry in radio astronomy are traced in detail. The first is the use of the sea-cliff interferometer at the Radiophysics Laboratory in Sydney, first by Pawsey for solar observations and later by Bolton for radio star surveys. The second is the development of the Michelson interferometer and the phase switch by Ryle in Cambridge. This also was employed for important observations of the sun and radio stars.

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Gryaznov, N. A., D. А. Goryachkin, V. I. Kuprenyuk, Е. N. Sosnov, and V. L. Alekseev. "PASSIVE STABILISATION OF MICHELSON INTERFEROMETER." NAUCHNOE PRIBOROSTROENIE 30, no. 4 (2020): 63–74. http://dx.doi.org/10.18358/np-30-4-i6374.

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In some applications of a Michelson interferometer, in particular, when it is used in a laser resonator, the phase difference of radiation beams passing the interferometer optical branches must be stabilized with high accuracy. The proposed paper is devoted to experimental studying the long-term stability of several interferometer designs and choosing the optimal version for applying as a compound resonator mirror with the controllable reflection for generation of ultrashort laser pulses.

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Monteiro, Catarina S., Margarida Ferreira, João P. Mendes, Luís C. C. Coelho, Susana Silva, and Orlando Frazão. "Optical Fiber Flowmeter Based on a Michelson Interferometer." EPJ Web of Conferences 287 (2023): 09040. http://dx.doi.org/10.1051/epjconf/202328709040.

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In this work, an optical fiber flowmeter based on a Michelson interferometer is presented. The Michelson interferometer uses a long period fiber grating (LPFG) to couple light to the cladding modes followed by a section of a GO-coated single mode fiber (SMF). By radiating the GO thin film, it will increase its temperature changing the effective refractive index of the optical cavity of the Michelson interferometer. By placing the sensor on a gas flow, its temperature surface will decrease in a proportional manner to the flow rate. The sensor was studied in both static and dynamic dry nitrogen

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15

Trávníček, Z., A. B. Wang, V. Lédl, T. Vít, Y. C. Chen, and F. Maršík. "Holographic-Interferometric and Thermoanemometric Study of a Thermoacoustic Prime Mover." Journal of Mechanics 29, no. 1 (2012): 59–66. http://dx.doi.org/10.1017/jmech.2012.110.

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AbstractA thermoacoustic standing-wave prime mover with a quarter-wave resonator has been investigated experimentally. The working fluid is air at the barometric pressure. The holographic interferometry and hot-wire anemometry have been used. A special optical setup, based on a Michelson interferometer, has been developed and used. The setup exhibits a double sensitivity, in comparison with a common Mach-Zehnder holographic interferometer. The results have confirmed a proper function of the prime mover, and advantages of the present optical setup.

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Gryaznov, N. A., D. А. Goryachkin, V. I. Kuprenyuk, Е. N. Sosnov, and V. L. Alekseev. "Controllable Michelson interferometer of refractive type." NAUCHNOE PRIBOROSTROENIE 31, no. 1 (2021): 59–65. http://dx.doi.org/10.18358/np-31-1-i5965.

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In some applications of a Michelson interferometer, in particular, when it is used in a laser resonator, the high stability of its phases is necessary. The proposed paper contains the comparison of two interferometer configurations. The first of them uses a classical schematic interferometer, the second one is designed with the use of a refractive schematic one, which is typical of enhanced stability against misalignments and occasional fluctuations of surrounding air. The possibility is discussed of applying the controllable refractive interferometer inside the resonator for generation of ult

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Tsuji, Takashi. "Warm Molecular Sphere around Red Supergiant Stars—A Missing Link between the Photosphere and Masering Water Clouds in the Circumstellar Envelope." Symposium - International Astronomical Union 205 (2001): 316–17. http://dx.doi.org/10.1017/s0074180900221347.

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Interferometry of red supergiants before 2000: The M2 supergiant Betelgeuse (α Ori) is the first star whose angular diameter was measured by the Michelson stellar interferometer (Michelson & Pease 1921). Since then, however, we had to wait half a century before we witnessed the renaissance of interferometric observations in optical astronomy with novel methods such as speckle interferometry (Laberie 1970). Michelson's classical method was also extended to the infrared regime (e.g. McCarthy et al. 1977). The initial results served not only to compare stellar temperature scale with the measu

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Mendoza-Figueroa, Virginia, and Jesús de la Cruz-Alejo. "Michelson Interferometer for near Infrared Wavelengths." Advanced Materials Research 677 (March 2013): 79–84. http://dx.doi.org/10.4028/www.scientific.net/amr.677.79.

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This paper presents an architecture to simplify a Michelson Interferometer, designed with MEMS technology in order to obtain the near infrared wavelengths in the range of [1620-1800 nm], which will be used in a non-invasive micro sensor of glucose. The input interferometer is fed with a white light source. The poli-silicon, superficial and bulk processes are utilized to design the architecture. The interferometer is based on dividing the design into three parts formed by two gears, a zipper and two mirrors at 90° each of one, for achieving resolution improvement without decreasing mechanical r

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Rahnama, Peyman, Yves J. Rochon, Ian C. McDade, Gordon G. Shepherd, William A. Gault, and Alan Scott. "Satellite Measurement of Stratospheric Winds and Ozone Using Doppler Michelson Interferometry. Part I: Instrument Model and Measurement Simulation." Journal of Atmospheric and Oceanic Technology 23, no. 6 (2006): 753–69. http://dx.doi.org/10.1175/jtech1880.1.

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Abstract This paper presents an instrument model and observation simulations for the measurement of stratospheric winds and ozone concentration using a satellite instrument employing imaging and the Doppler Michelson interferometery technique. The measurement technique and instrument concept are described. The instrument model and simulations are based on initial design characteristics of the Canadian Stratospheric Wind Interferometer for Transport Studies (SWIFT) satellite instrument. SWIFT employs an imaging array and a field-widened Michelson interferometer. It will measure stratospheric wi

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Badie Younis, Raya, Suha Mousa Khorsheed, and Ziad Tarik AlDahan. "Modified Michelson Interferometer Design for Ear Measurement." International Journal of Scientific Engineering and Research 6, no. 12 (2018): 36–41. https://doi.org/10.70729/ijser18394.

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Oosterbeek, Johan W., Neha Chaudhary, Matthias Hirsch, Udo Höfel, and Robert C. Wolf. "Assessment of ECH stray radiation levels at the W7-X Michelson Interferometer and Profile Reflectometer." EPJ Web of Conferences 203 (2019): 03010. http://dx.doi.org/10.1051/epjconf/201920303010.

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Electron Cyclotron Heating and Electron Cyclotron Current Drive are key components for heating and control in magnetically confined fusion plasmas. The high power microwaves are not always completely absorbed leading to stray radiation [1], [2]. At W7-X, the total injected microwave power can be up to 7.5 MW @140 GHz while the entire Electron Cyclotron Emission picked-up by an observer at the edge of the plasma is a fraction of a mW. In the situation of a Michelson Interferometer, the principle measurement is the entire ECE spectrum. Thus, any stray radiation is bound to enter the spectrum. In

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Zuo Xiao-Jie, Sun Ying-Rong, Yan Zhi-Hui, and Jia Xiao-Jun. "High sensitivity quantum Michelson interferometer." Acta Physica Sinica 67, no. 13 (2018): 134202. http://dx.doi.org/10.7498/aps.67.20172563.

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Chhaniwal, Vani K. "Beamsplitter testing with Michelson interferometer." Optical Engineering 44, no. 7 (2005): 079701. http://dx.doi.org/10.1117/1.1951775.

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Sánchez-de-la-Llave, David. "Multiple beam Michelson-based interferometer." Optical Engineering 48, no. 8 (2009): 085601. http://dx.doi.org/10.1117/1.3192784.

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Zhang, Chunmin, Baohui Zhu, Huachun Zhu, Wenfeng Zeng, and Wenyi Ren. "Novel polarization atmosphere Michelson interferometer." Optical Engineering 51, no. 10 (2012): 101714–1. http://dx.doi.org/10.1117/1.oe.51.10.101714.

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Pathare, Shirish, and Vikrant Kurmude. "Low cost Michelson–Morley interferometer." Physics Education 51, no. 6 (2016): 063001. http://dx.doi.org/10.1088/0031-9120/51/6/063001.

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Xie, Dong, Chunling Xu, and An Min Wang. "Michelson interferometer for measuring temperature." Physics Letters A 381, no. 36 (2017): 3038–42. http://dx.doi.org/10.1016/j.physleta.2017.07.036.

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Yuan, Libo, Jun Yang, Zhihai Liu, and Jiaxing Sun. "In-fiber integrated Michelson interferometer." Optics Letters 31, no. 18 (2006): 2692. http://dx.doi.org/10.1364/ol.31.002692.

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Yu, Wenlei, Lei Jiang, Kehao Zeng, Xinyuan Jing, and Yunfeng Jiang. "Michelson interferometer with Bessel beams." Optics and Lasers in Engineering 177 (June 2024): 108146. http://dx.doi.org/10.1016/j.optlaseng.2024.108146.

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Filipescu, Filip Dambi. "Opposing hypotheses of the reflection of light applied to the Michelson interferometer with a particular geometry." Physics Essays 34, no. 3 (2021): 268–73. http://dx.doi.org/10.4006/0836-1398-34.3.268.

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The derivation of light paths in the Michelson interferometer is based on the hypothesis that the incident speed and reflected speed of the wavefront of a ray of light are equal in the frame at absolute rest. In this case, the Michelson‐Morley experiment predicts a fringe shift of <mml:math display="inline"> <mml:mrow> <mml:mo> </mml:mo> <mml:mn>0.40</mml:mn> </mml:mrow> </mml:math> . With the hypothesis that the incident speed and reflected speed of the wavefront of a ray of light are equal in the inertial frame of a mirror at the instance of co

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Wang, Weitao, Chen Wang, Shuai Qu, et al. "Research on the Linear Demodulation Range and Background Noise of Fiber-Optic Interferometer System." Photonics 10, no. 3 (2023): 283. http://dx.doi.org/10.3390/photonics10030283.

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The linear demodulation range and background noise of the Michelson interferometer system are investigated with a laser phase noise measurement system. We have theoretically and experimentally analyzed the performance of the interferometer system by changing the frequency modulation amplitude of the laser and the optical path difference (OPD) of the interferometer, respectively. It is shown that the linear demodulation range of the Michelson interferometer system is finite, which depends on the parameters of the system, such as the sample frequency, the delay time between two interferometer ar

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Klinaku, Shukri. "Michelson-Morley experiment explained by means of five methods." Journal of Physics: Conference Series 2197, no. 1 (2022): 012018. http://dx.doi.org/10.1088/1742-6596/2197/1/012018.

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Abstract The Michelson-Morley experiment (MME) is still important to physics, and not just to the history of physics. The hypothesis of contraction of bodies in the direction of their motion arose as an ad hoc hypothesis about the “contraction” of the Michelson’s interferometer arm in the direction of its motion. Even today this experiment is the “strongest argument” of this hypothesis, and of time dilation too. This work will present the explanation of the MME through five methods. The first method can be called the traditional method, which was applied by Michelson, but not correctly. The ot

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Jiang, Tong, Yungui Gong, and Xuchen Lu. "Sky localization of space-based detectors with time-delay interferometry." Journal of Cosmology and Astroparticle Physics 2024, no. 10 (2024): 067. http://dx.doi.org/10.1088/1475-7516/2024/10/067.

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Abstract The accurate sky localization of gravitational wave (GW) sources is an important scientific goal for space-based GW detectors. The main differences between future space-based GW detectors, such as Laser Interferometer Space Antenna (LISA), Taiji, and TianQin, include the time-changing orientation of the detector plane, the arm length, the orbital period of the spacecraft and the noise curve. Because of the effects of gravity on three spacecraft, it is impossible to maintain the equality of the arm length, so the time-delay interferometry (TDI) method is needed to cancel out the laser

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Rapport, Nathan. "Classical Doppler shift explains the Michelson‐Morley null result." Physics Essays 35, no. 4 (2022): 326–44. http://dx.doi.org/10.4006/0836-1398-35.4.326.

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Here we review Michelson‐Morley's original analysis of their interferometer experiment and discuss its use of optical distance. We derive a formula for transverse Doppler shift from geometric considerations, apply this to the Michelson‐Morley interferometer, and present a phase analysis for the experiment. Furthermore, we present an equation for Doppler shift at a general angle and use this to derive the null phase shift result for round-trip interferometer paths at any arbitrary angle. We do not dispute the validity of the null result, nor the prediction of an arrival-time difference for the

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Okishev, Konstantin N., Grigory A. Anikeev, Polina S. Goncharova, Alexander Vjacheslavovich Syuy, and Alena V. Popova. "Michelson Interferometer Mirror Shift Method for Femtosecond Pulse Studies." Key Engineering Materials 806 (June 2019): 180–85. http://dx.doi.org/10.4028/www.scientific.net/kem.806.180.

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In this paper is considered the autocorrelator of ultrashort pulses based a Michelson interferometer, his schemes and operating principles. The method of measuring ultrashort pulses is given. The schemes and principles of operation of the main nodes of the autocorrelation receiver are presented: the optical-mechanical part (the construction of the Michelson interferometer) and the electronic part, which includes a photodetector module, a control and data processing unit with a speaker amplifier, and a personal computer.

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Barbosa, Francisco de Assis Andrade, Gilder Nader, Ricardo Tokio Higuti, Cláudio Kitano, and Emílio Carlos Nelli Silva. "A simple interferometric method to measure the calibration factor and displacement amplification in piezoelectric flextensional actuators." Sba: Controle & Automação Sociedade Brasileira de Automatica 21, no. 6 (2010): 577–87. http://dx.doi.org/10.1590/s0103-17592010000600003.

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Laser interferometry is a well-established technique for the characterization of piezoelectric actuators. In this work, by using a low cost Michelson interferometer, the measurement of the calibration factor and the displacement amplification of a novel piezoelectric flextensional actuator (PFA), designed by using the topology optimization method, is performed. A simple method, based on small phase modulation depth when the PFA is driven by a triangular waveform, allows the absolute interferometer calibration. The free-displacement of the PFA for various drive voltages is measured and the disp

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Grizbil, B. A., L. A. Maksimova, and V. P. Ryabukho. "Diffraction model of a laser speckle interferometer for measuring micro-displacements of objects with scattering surface." Computer Optics 44, no. 4 (2020): 568–77. http://dx.doi.org/10.18287/2412-6179-co-702.

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On the basis of diffraction transformations of an optical wave field a mathematical model for the formation of speckle modulated interference patterns and signals at the output of a speckle interferometer is developed, which allows us to identify their properties and quantitative parameters. Speckle interferometers based on a Michelson arrangement are considered, where objects with scattering surfaces are used instead of mirrors in the reference and object arms. Results of numerical simulation of speckle modulated interference patterns on the basis of diffraction transformations of wave fields

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RATNA PURI, TASA. "Menentukan Panjang Gelombang Laser He-Ne." Jurnal Penelitian Fisika dan Terapannya (JUPITER) 5, no. 2 (2024): 52–56. http://dx.doi.org/10.31851/jupiter.v5i2.12138.

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Interferometer Michelson adalah alat eksperimen yang berlandaskan pada interferensi dari gabungan dua gelombang cahaya dengan lintasan optik yang berbeda. Pola interferensi yang terbentuk pada interferometer Michelson lebih tajam, lebih jelas, dan jarak antar frinji lebih sempit dibandingkan dengan interferometer lainnya. Prinsip interferensi menyatakan bahwa perbedaan lintasan optik (d) akan membentuk suatu frinji. Frinji ini digunakan untuk menentukan besaran fisis, salah satunya adalah panjang gelombang. Untuk menentukan panjang gelombang sumber cahaya laser He-Ne, dapat digunakan persamaan

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Shvets, Viacheslav A., Grigory I. Dolgikh, Aleksandr A. Plotnikov, and Sergey V. Yakovenko. "Development and research of a system for monitoring the state of instruments of a laser-interference geophysical complex." Izmeritel`naya Tekhnika, no. 3 (2021): 22–28. http://dx.doi.org/10.32446/0368-1025it.2021-3-22-28.

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This article gives an overview of results achieved in process of design, developing and using of data acquisition and control systems for LSM (long-base strainmeters) and other devices based on Michelson laser interferometer. Such control systems are also used in other types of laser-interference instruments that provide the study of geodynamic processes in a broad frequency range. It’s shown that the effective means for control of external factors in geophysical measurements using LSMs are the same-type laser-interference instruments. The geophysical laser-interference complex is described in

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Fikadu, Boka, Bulcha Bekele, Leta Tesfaye Jule, Anatol Degefa, N. Nagaprasad, and Krishnaraj Ramaswamy. "Investigation of Light Parameters on Image Quality and Optical Coherence Tomography." International Journal of Optics 2021 (November 26, 2021): 1–6. http://dx.doi.org/10.1155/2021/2322858.

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In this work, image quality and optical coherence tomography were studied. The results of the study show that there is a very significant difference between ultrasound and optical coherence tomography to produce an image with a different wave. To understand this, we studied the basic principle of optical coherence tomography in the Michelson interferometer using monochromatic and broadband sources. Time-domain and spectral-domain measurements, which exist at the detector level, are briefly described using a glass sample. The time-domain signal strength of the Michelson interferometer using a b

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Zeng, Jiazhong, and Xiaoqi Zeng. "Measuring the central wavelength and bandwidth of an LED with the Michelson interferometer." Physics Education 58, no. 1 (2022): 015015. http://dx.doi.org/10.1088/1361-6552/ac9efa.

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Abstract A method for measuring the central wavelength and bandwidth of a light emitting diode (LED) using the Michelson interferometer is proposed. It is easy to see the interference fringes on the screen by setting the optical path properly. Based on it, the central wavelength and bandwidth of LEDs with three different colours are measured, and the experimental results are consistent with the results from a spectrometer. The experiment will be helpful for students to understand the spectral and coherence characteristics of LEDs. It can also be an extended content of Michelson interferometer.

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Fisher, Philip C., Joseph B. Houston, and Tilman W. Stuhlinger. "Infrared Interferometers for Observing Extra-Solar Planets." International Astronomical Union Colloquium 161 (January 1997): 367–73. http://dx.doi.org/10.1017/s0252921100014871.

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AbstractConcepts are outlined for ground - and space-based interferometers for observing nearby extra-solar earth-like planets (in the 8-20 μ range). The collecting elements are special coronagraphs, two of which constitute part of a Michelson interferometer. Performance characteristics are compared to those inferred for several competing systems. One conclusion is that one could construct a groundbased instrument that seems superior to the Keck interferometer system («superior» meaning up to a tenfold increase in angular resolution in each of two orthogonal directions, up to a tenfold increas

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Haschberger, Peter. "Impact of the Sinusoidal Drive on the Instrumental Line Shape Function of a Michelson Interferometer with Rotating Retroreflector." Applied Spectroscopy 48, no. 3 (1994): 307–15. http://dx.doi.org/10.1366/0003702944028236.

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In Fourier spectrometers using the classical Michelson setup, conventionally a plane mirror travels with constant speed to generate an optical pathlength alteration. Recently, different types of Michelson interferometers have been developed that use one or more rotating retroreflectors for pathlength variation. They all exhibit a sinusoidal dependence of the pathlength on time. This paper discusses the effects of the nonlinear mirror motion on the interferogram and the calculated spectrum. The requirements necessary for the acquisition system are deduced, and distortions due to nonideal analog

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Lukens, Joseph M., Nicholas A. Peters, and Raphael C. Pooser. "Naturally stable Sagnac–Michelson nonlinear interferometer." Optics Letters 41, no. 23 (2016): 5438. http://dx.doi.org/10.1364/ol.41.005438.

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Li, Xianyao, Xi Xiao, Hao Xu, et al. "Highly Efficient Silicon Michelson Interferometer Modulators." IEEE Photonics Technology Letters 25, no. 5 (2013): 407–9. http://dx.doi.org/10.1109/lpt.2013.2238625.

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Lebedev, M. V., O. V. Misochko, and A. A. Driomin. "Michelson interferometer with multichannel interferogram recording." Optics and Spectroscopy 107, no. 5 (2009): 826–29. http://dx.doi.org/10.1134/s0030400x09110228.

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Ikram, Masroor, and Ghazanfar Hussain. "Michelson interferometer for precision angle measurement." Applied Optics 38, no. 1 (1999): 113. http://dx.doi.org/10.1364/ao.38.000113.

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Barone, F., L. Di Fiore, L. Milano, G. Russo, and S. Solimeno. "Automatic alignment of a Michelson interferometer." IEEE Transactions on Nuclear Science 39, no. 2 (1992): 232–37. http://dx.doi.org/10.1109/23.277488.

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Sutter, John P., Tetsuya Ishikawa, Ulrich Kuetgens, et al. "An X-ray BBB Michelson interferometer." Journal of Synchrotron Radiation 11, no. 5 (2004): 378–85. http://dx.doi.org/10.1107/s0909049504015468.

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Vollmer, M., and K. P. Möllmann. "Michelson Interferometer for Your Kitchen Table." Physics Teacher 46, no. 2 (2008): 114–17. http://dx.doi.org/10.1119/1.2834535.

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