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Journal articles on the topic 'Stokes polarimetry'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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1

Leiber, Th, and K. Reif. "First Observations by the Bonn Wide-Field Photometer and Polarimeter (WWFPP): Surface Polarimetry of the Crab Nebula." Symposium - International Astronomical Union 161 (1994): 481–83. http://dx.doi.org/10.1017/s0074180900047926.

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To test the performance of the WWFPP in polarimetric mode, we performed surface polarimetry of the Crab nebula in February 1993 using the Asiago 1.82 m telescope of the ‘Osservatorio Astronomico di Padova’. The polarimeter is a new design and enables us to do simultaneous wide-field polarimetry (15 × 15 arcmin field with 0.43 arcsec/pixel) of four polarization angles using a twin Wollaston prism or simultaneous polarimetry of two angles using a double wedge plate with orthogonal sheet polarizers in combination with an achromatic half wave plate. For the observations described here we used the

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2

Espinosa-Soria, Alba, Francisco J. Rodríguez-Fortuño, Amadeu Griol, and Alejandro Martínez. "Full Measurement of the Stokes Parameters Using a Subwavelength Silicon On-Chip Polarimeter." Advances in Science and Technology 98 (October 2016): 103–8. http://dx.doi.org/10.4028/www.scientific.net/ast.98.103.

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Polarimetry enables to measure the state of polarization (SoP) of a light beam, which is essential in many disciplines. Typical polarimeters use bulky and expensive optical elements such as half-wave plates and grid polarizers. Plasmonic nanostructures may help to transform such bulky components into subwavelength metallic elements showing similar performance. Based on the concept of spin-orbit coupling, here we demonstrate a nanophotonic polarimeter that measures the Stokes parameters of a light beam over an ultrabroad bandwidth in a less than a square wavelength active region. Furthermore, t

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3

Guo, Jing, Deqing Ren, Yongtian Zhu, and Xi Zhang. "A high-speed and high-efficiency imaging polarimeter based on ferroelectric liquid crystal retarders: Design and test." Publications of the Astronomical Society of Japan 73, no. 2 (2021): 405–16. http://dx.doi.org/10.1093/pasj/psab007.

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Abstract Polarimeters play a key role in investigating solar magnetic fields. In this paper, a High speed and high efficiency Imaging POlarimeter (HIPO) is proposed based on a pair of ferroelectric liquid crystal retarders (FLCs), with the ultimate goal of measuring magnetic fields of prominences and filaments from the ground. A unique feature of the HIPO is that it enables high cadence polarization measurements covering a wide field of view (FOV); the modulation frequency of the HIPO is able to achieve ∼100 Hz, which greatly suppresses the seeing-induced crosstalk, and the maximum FOV can rea

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4

Hannonen, Antti, Bernhard J. Hoenders, Wolfgang Elsässer, Ari T. Friberg, and Tero Setälä. "Ghost polarimetry using Stokes correlations." Journal of the Optical Society of America A 37, no. 5 (2020): 714. http://dx.doi.org/10.1364/josaa.385851.

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5

Eshaghi, Mahdi, and Aristide Dogariu. "Single-shot omnidirectional Stokes polarimetry." Optics Letters 45, no. 15 (2020): 4340. http://dx.doi.org/10.1364/ol.396528.

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6

Raney, R. Keith. "Hybrid Dual-Polarization Synthetic Aperture Radar." Remote Sensing 11, no. 13 (2019): 1521. http://dx.doi.org/10.3390/rs11131521.

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Compact polarimetry for a synthetic aperture radar (SAR) system is reviewed. Compact polarimetry (CP) is intended to provide useful polarimetric image classifications while avoiding the disadvantages of space-based quadrature-polarimetric (quad-pol) SARs. Two CP approaches are briefly described, π/4 and circular. A third form, hybrid compact polarimetry (HCP) has emerged as the preferred embodiment of compact polarimetry. HCP transmits circular polarization and receives on two orthogonal linear polarizations. When seen through its associated data processing and image classification algorithms,

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7

Krouglov, Serguei, and Virginijus Barzda. "Three-dimensional nonlinear Stokes–Mueller polarimetry." Journal of the Optical Society of America B 36, no. 2 (2019): 541. http://dx.doi.org/10.1364/josab.36.000541.

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8

Arbabi, Ehsan, Seyedeh Mahsa Kamali, Amir Arbabi, and Andrei Faraon. "Full-Stokes Imaging Polarimetry Using Dielectric Metasurfaces." ACS Photonics 5, no. 8 (2018): 3132–40. http://dx.doi.org/10.1021/acsphotonics.8b00362.

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9

Tomczyk, Steven, Roberto Casini, Alfred G. de Wijn, and Peter G. Nelson. "Wavelength-diverse polarization modulators for Stokes polarimetry." Applied Optics 49, no. 18 (2010): 3580. http://dx.doi.org/10.1364/ao.49.003580.

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10

Azzam, R. M. A. "Stokes-vector and Mueller-matrix polarimetry [Invited]." Journal of the Optical Society of America A 33, no. 7 (2016): 1396. http://dx.doi.org/10.1364/josaa.33.001396.

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11

Myserlis, I., E. Angelakis, A. Kraus, et al. "Full-Stokes polarimetry with circularly polarized feeds." Astronomy & Astrophysics 609 (January 2018): A68. http://dx.doi.org/10.1051/0004-6361/201630301.

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We present an analysis pipeline that enables the recovery of reliable information for all four Stokes parameters with high accuracy. Its novelty relies on the effective treatment of the instrumental effects even before the computation of the Stokes parameters, contrary to conventionally used methods such as that based on the Müller matrix. For instance, instrumental linear polarization is corrected across the whole telescope beam and significant Stokes Q and U can be recovered even when the recorded signals are severely corrupted by instrumental effects. The accuracy we reach in terms of polar

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12

O’Connor, Eoin G. P., Andrew Shearer, Christian Gouiffes, and Philippe Laurent. "High Time Resolution Astronomical Polarimetry with GASP." Proceedings of the International Astronomical Union 13, S337 (2017): 384–85. http://dx.doi.org/10.1017/s1743921317010626.

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AbstractThe Galway Astronomical Stokes Polarimeter (GASP) is a high time resolution, full-Stokes imaging polarimeter which utilises a Fresnel rhomb prism as a beam-splitter and quarter wave retarder. The ability to perform optical photometry and polarimetry at high frame rates enables more detailed studies of a multitude of compact objects including; optical pulsars, magnetars and Active Galactic Nuclei (AGN). We present a brief discussion of the instruments’ current capabilities and hardware design. GASP is currently configured with two Electron Multiplying Charge-Coupled Devices (EMCCDs), wh

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13

Bains, I., J. Caswell, A. M. S. Richards, et al. "VLBI OH maser polarimetry with the Australian Long Baseline Array: the star-forming region G340.054–0.244." Proceedings of the International Astronomical Union 3, S242 (2007): 64–65. http://dx.doi.org/10.1017/s1743921307012574.

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AbstractUntil recently, high spatial resolution full Stokes maser polarimetry was the sole domain of northern interferometers and a wealth of sources in the far south remained unexplored due to a lack of suitable instrumentation having both high spatial and high velocity resolution. The Australia Telescope Long Baseline Array (LBA) has now switched to disk-based software correlation, permitting full Stokes observing in spectral line mode with velocity channels which are sufficiently narrow to sample usefully the polarization structure. To illustrate the utility of this valuable addition to rad

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14

Brugés Martelo, Javier, Jan Lundgren, and Mattias Andersson. "Paperboard Coating Detection Based on Full-Stokes Imaging Polarimetry." Sensors 21, no. 1 (2020): 208. http://dx.doi.org/10.3390/s21010208.

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The manufacturing of high-quality extruded low-density polyethylene (PE) paperboard intended for the food packaging industry relies on manual, intrusive, and destructive off-line inspection by the process operators to assess the overall quality and functionality of the product. Defects such as cracks, pinholes, and local thickness variations in the coating can occur at any location in the reel, affecting the sealable property of the product. To detect these defects locally, imaging systems must discriminate between the substrate and the coating. We propose an active full-Stokes imaging polarim

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15

Sankarasubramanian, K., G. Srinivasulu, A. V. Ananth, and P. Venkatakrishnan. "Stokes Polarimetry at the Kodaikanal Tower Tunnel Telescope." International Astronomical Union Colloquium 179 (2000): 241–44. http://dx.doi.org/10.1017/s0252921100064575.

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AbstractA Stokes polarimeter has been developed using a masked CCD arrangement for the measurement of the vector magnetic field of sunspots. Charge shifting within the CCD is used to record near simultaneous orthogonal polarisation. The testing of the Stokes polarimeter and the behavior of the integrated system combined with the Kodaikanal tower tunnel telescope will be discussed.

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16

Loktev, Vladislav, Tuomo Salmi, Joonas Nättilä, and Juri Poutanen. "Oblate Schwarzschild approximation for polarized radiation from rapidly rotating neutron stars." Astronomy & Astrophysics 643 (November 2020): A84. http://dx.doi.org/10.1051/0004-6361/202039134.

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We have developed a complete theory for the calculation of the observed Stokes parameters for radiation emitted from the surface of a rapidly rotating neutron star (NS) using the oblate Schwarzschild approximation. We accounted for the rotation of the polarization plane due to relativistic effects along the path from the stellar surface to the observer. The results were shown to agree with those obtained by performing full numerical general relativistic ray-tracing with the ARCMANCER code. We showed that the obtained polarization angle profiles may differ substantially from those derived for a

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17

Phan, Quoc-Hung, and Yu-Lung Lo. "Stokes-Mueller matrix polarimetry system for glucose sensing." Optics and Lasers in Engineering 92 (May 2017): 120–28. http://dx.doi.org/10.1016/j.optlaseng.2016.08.017.

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18

Liu, Yeng-Cheng, Yu-Lung Lo, Chang-Ye Li, and Chia-Chi Liao. "Spectroscopic Stokes polarimetry based on Fourier transform spectrometer." Optics Communications 336 (February 2015): 295–300. http://dx.doi.org/10.1016/j.optcom.2014.09.023.

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19

Zhang, Yaxin, Jinjin Jin, Mingbo Pu, et al. "Full Stokes Polarimetry for Wide‐Angle Incident Light." physica status solidi (RRL) – Rapid Research Letters 14, no. 5 (2020): 2000044. http://dx.doi.org/10.1002/pssr.202000044.

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20

Yu, Mingxuan, Tiegen Liu, Hesong Huang, Haofeng Hu, and Bingjing Huang. "Multispectral Stokes Imaging Polarimetry Based on Color CCD." IEEE Photonics Journal 8, no. 5 (2016): 1–10. http://dx.doi.org/10.1109/jphot.2016.2599006.

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21

Cook, P. J., J. Zhang, Y. Liu, et al. "Magneto-Optical Stokes Polarimetry and Nanostructured Magnetic Materials." Journal of Nanoscience and Nanotechnology 12, no. 2 (2012): 1067–73. http://dx.doi.org/10.1166/jnn.2012.4258.

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22

Sankarasubramanian, K., G. Srinivasulu, A. V. Ananth, and P. Venkatakrishnan. "Stokes polarimetry at the Kodaikanal tower tunnel telescope." Journal of Astrophysics and Astronomy 21, no. 3-4 (2000): 241–44. http://dx.doi.org/10.1007/bf02702399.

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23

Volkmer, Reiner. "3-Dimensional High-Resolution Solar Spectro-Polarimetry." International Astronomical Union Colloquium 149 (1995): 193–94. http://dx.doi.org/10.1017/s0252921100022934.

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AbstractIn order to obtain information on the magnetic field on the sun in two spatial dimensions, a spectro-polarimeter of high spatial, spectral, and temporal resolution was built in the German Vacuum Tower Telescope (VTT) at the Observatorio del Teide/Tenerife. The two-dimensional spectrometer in the VTT, using a Universal Birefringent Filter (UBF) and a Fabry-Perot Interferometer (FPI) to obtain narrow-band nltergrams with a spectral resolution of the order of 3.105 (approx. 22 mÅ at CE5; at 6303 Å) and a spatial resolution of 0.2 arcsec/pixel (Bendlin et al. 1992, Bendlin and Volkmer 1993

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24

Karachevtsev, A. O. "Fourier-Stokes polarimetry of fields corresponding to linearly and circularly polarized birefringent protein networks." Semiconductor Physics Quantum Electronics and Optoelectronics 15, no. 3 (2012): 252–60. http://dx.doi.org/10.15407/spqeo15.03.252.

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25

Dubolazov, O. V., M. Yu Sakhnovsky, O. V. Olar, P. M. Grigorishin, and Yu O. Ushenko. "Fourier-Stokes polarimetry system of biological tissues polycrystalline networks." Optoelectronic Information-Power Technologies 35, no. 1 (2019): 36–44. http://dx.doi.org/10.31649/1681-7893-2019-35-1-36-44.

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26

Yampolskiy, A., O. Makarenko, V. Lendel, V. Prorok, A. Sharapa, and L. Poperenko. "Stokes-polarimetry of ultrathin Au and Sn island films." Bulletin of Taras Shevchenko National University of Kyiv. Series: Physics and Mathematics, no. 4 (2018): 122–29. http://dx.doi.org/10.17721/1812-5409.2018/4.18.

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The optical properties of ultrathin Au and Sn islet films, obtained by the methods of magnetron sputtering and thermal evaporation, respectively, are considered in this paper. By measuring the Stokes vector of the beam reflected from the samples, polarized and depolarized radiation components were separated. The conditions of the polarization degree dependence on the surface structure for a series of islet films with different morphologies are analyzed. To determine the morphological structure of the metal layer, methods of atomic force microscopy and resistivity measurement were also employed

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27

Foreman, Matthew R., and François Goudail. "On the equivalence of optimization metrics in Stokes polarimetry." Optical Engineering 58, no. 08 (2019): 1. http://dx.doi.org/10.1117/1.oe.58.8.082410.

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28

Cheng, Bo, Yuxiao Zou, Hanxiao Shao, Tong Li, and Guofeng Song. "Full-Stokes imaging polarimetry based on a metallic metasurface." Optics Express 28, no. 19 (2020): 27324. http://dx.doi.org/10.1364/oe.400622.

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29

Faugeras, Blaise, and Francesco Orsitto. "Equilibrium reconstruction at JET using Stokes model for polarimetry." Nuclear Fusion 58, no. 10 (2018): 106032. http://dx.doi.org/10.1088/1741-4326/aad751.

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30

Liu, Jiamin, Chuanwei Zhang, Zhicheng Zhong, et al. "Measurement configuration optimization for dynamic metrology using Stokes polarimetry." Measurement Science and Technology 29, no. 5 (2018): 054010. http://dx.doi.org/10.1088/1361-6501/aaaeeb.

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31

Manthalkar, Amogh, Isaac Nape, Najmeh Tabe Bordbar, et al. "All-digital Stokes polarimetry with a digital micromirror device." Optics Letters 45, no. 8 (2020): 2319. http://dx.doi.org/10.1364/ol.389346.

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32

Sutinjo, A., J. O'Sullivan, E. Lenc, et al. "Understanding instrumental Stokes leakage in Murchison Widefield Array polarimetry." Radio Science 50, no. 1 (2015): 52–65. http://dx.doi.org/10.1002/2014rs005517.

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33

Barrett, P. "Multicolour 'Stokes' polarimetry of SN 1987A in the LMC." Monthly Notices of the Royal Astronomical Society 234, no. 4 (1988): 937–56. http://dx.doi.org/10.1093/mnras/234.4.937.

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34

Zhao, Bo, Xiao-Bo Hu, Valeria Rodríguez-Fajardo, et al. "Real-time Stokes polarimetry using a digital micromirror device." Optics Express 27, no. 21 (2019): 31087. http://dx.doi.org/10.1364/oe.27.031087.

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35

Elias, Nicholas M. II, Stanislav S. Edel, Carol E. Jones, et al. "Imaging Stars by Performing Full-Stokes Optical Interferometric Polarimetry." Journal of Astronomy and Space Sciences 29, no. 1 (2012): 85–91. http://dx.doi.org/10.5140/jass.2012.29.1.085.

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36

Samim, Masood, Serguei Krouglov, Daniel F. James, and Virginijus Barzda. "Characterization of heterogeneous media using nonlinear Stokes–Mueller polarimetry." Journal of the Optical Society of America B 33, no. 12 (2016): 2617. http://dx.doi.org/10.1364/josab.33.002617.

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37

Scholiers, W., and E. Wiehr. "Stokes-spectro-polarimetry with a two-dimensional diode array." Solar Physics 99, no. 1-2 (1985): 349–63. http://dx.doi.org/10.1007/bf00157318.

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38

Code, A. D., K. H. Nordsieck, and C. M. Anderson. "Ultraviolet Polarimetry." International Astronomical Union Colloquium 123 (1990): 291. http://dx.doi.org/10.1017/s0252921100077162.

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AbstractInterstellar polarization and polarization of the sky background is predicted to be significantly smaller in the ultraviolet than in the optical region of the spectrum; while intrinsic polarization is expected to be greater. For these reasons alone ultraviolet polarimetry should provide a powerful diagnostic tool. To date such polarization measurements have not been undertaken. The Wisconsin Ultraviolet Photopolarimeter Experiment (WUPPE) will be the first to carry out a program of UV spectropolarimetry. WUPPE is one of the four ASTRO-1 payloads. It consists of a half meter aperture Ca

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39

Jayasri, P. V., H. S. V. Usha Sundari, E. V. S. Sita Kumari, and A. V. V. Prasad. "Study of Oil spill in Norwegian area using Decomposition Techniques on RISAT-1 Hybrid Polarimetric Data." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XL-8 (November 28, 2014): 1043–48. http://dx.doi.org/10.5194/isprsarchives-xl-8-1043-2014.

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Over past few years Synthetic Aperture Radar(SAR) has received a considerable attention for monitoring and detection of oil spill due to its unique capabilities to provide wide-area surveillance and day and night measurements, almost independently from atmospheric conditions. The critical part of the oil spill detection is to distinguish oil spills from other natural phenomena. Stokes vector analysis of the image data is studied to estimate the polarized circular and linear components of the backscatter signal which essentially utilize the degree of polarization(m) and relative phase (&del

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40

Srivastava, H. S., and T. Sivasankar. "POTENTIAL OF C-BAND HYBRID POLARIMETRIC RISAT-1 SAR DATA FOR WHEAT CROP HEIGHT ESTIMATION." ISPRS - International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences XLII-3/W6 (July 26, 2019): 637–41. http://dx.doi.org/10.5194/isprs-archives-xlii-3-w6-637-2019.

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<p><strong>Abstract.</strong> The advancement of hybrid polarimetry and the launch of Radar Imaging SATellite-1 (RISAT-1), the first Earth observing satellite with capability to acquire hybrid polarimetric SAR data, have given opportunity to explore the potentials of this data for various geo-spatial applications. Among these, crop growth monitoring and soil moisture estimation is one of the important application for proper irrigation management, yield forecasting and crop insurance systems. The objective of this paper is to provide a better understanding of the sensitivity o

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41

Dubolazov, O. V., M. Yu Sakhnovsky, O. V. Olar, P. M. Grigorishin, and Yu O. Ushenko. "Fourier-Stokes-polarimetry system of polycrystalline networks of biological tissues." Optoelectronic Information-Power Technologies 1, no. 35 (2019): 36–44. http://dx.doi.org/10.31649/1681-7893-2018-35-1-36-44.

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42

Angelsky, P. O., L. B. Bodnar, M. P. Gorskii, and L. Ya Kushnerick. "Fourier-Stokes polarimetry of fields scattered by birefringent biological networks." Optical Memory and Neural Networks 21, no. 4 (2012): 233–41. http://dx.doi.org/10.3103/s1060992x12040029.

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43

Hall, Shaun A., Marc-André Hoyle, Joshua S. Post, and Dennis K. Hore. "Combined Stokes Vector and Mueller Matrix Polarimetry for Materials Characterization." Analytical Chemistry 85, no. 15 (2013): 7613–19. http://dx.doi.org/10.1021/ac401864g.

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44

Singh, Keshaan, Najmeh Tabebordbar, Andrew Forbes, and Angela Dudley. "Digital Stokes polarimetry and its application to structured light: tutorial." Journal of the Optical Society of America A 37, no. 11 (2020): C33. http://dx.doi.org/10.1364/josaa.397912.

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45

Shen, Qun, S. Shastri, and K. D. Finkelstein. "Stokes polarimetry for x rays using multiple‐beam diffraction (invited)." Review of Scientific Instruments 66, no. 2 (1995): 1610–13. http://dx.doi.org/10.1063/1.1145857.

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46

Adhiya, Asha, Ankur Pandya, and Rajwinder Kaur. "Determination of Mueller Matrix for Metal Substrates by Stokes Polarimetry." IEEE Transactions on Instrumentation and Measurement 70 (2021): 1–7. http://dx.doi.org/10.1109/tim.2021.3097863.

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47

Cenacchi, Elena, A. Kraus, and K. H. Mack. "Deriving AGN properties from circular and linear radio polarimetry." Proceedings of the International Astronomical Union 4, S259 (2008): 561–62. http://dx.doi.org/10.1017/s1743921309031330.

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AbstractWe report multi-frequency circular polarization measurements for the radio source 0056-00 taken at the Effelsberg 100-m radio telescope. The data reduction is based on a new calibration procedure that allows the contemporary measurement of the four Stokes parameters with single-dish radio telescopes.

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48

Goto, Motoshi, Ryohko Ishikawa, Yusuke Iida, and Saku Tsuneta. "Analytical Solution of the Hanle Effect in View of CLASP and Future Polarimetric Solar Studies." Atoms 7, no. 2 (2019): 55. http://dx.doi.org/10.3390/atoms7020055.

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We have solved a problem of the Hanle effect for the hydrogen Lyman- α line in an intuitive and straightforward way. The Stokes parameters amid an anisotropic radiation field and a magnetic field are derived as an analytical formula which enables us to conduct immediate analyses of observation data taken by spectro-polarimetry. The derived formula is, in particular, supposed to be used for the analysis of the data taken by CLASP (Chromospheric Lyman-Alpha Spectro-Polarimeter), which has aimed at measuring the linear polarization in the hydrogen Lyman- α line (121.6 nm) and then evaluating the

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49

Li, Xiaobo, Tiegen Liu, Bingjing Huang, Zhanjie Song, and Haofeng Hu. "Optimal distribution of integration time for intensity measurements in Stokes polarimetry." Optics Express 23, no. 21 (2015): 27690. http://dx.doi.org/10.1364/oe.23.027690.

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50

Hore, Dennis K., Almeria L. Natansohn, and Paul L. Rochon. "Optical Anisotropy as a Probe of Structural Order by Stokes Polarimetry." Journal of Physical Chemistry B 106, no. 35 (2002): 9004–12. http://dx.doi.org/10.1021/jp025877u.

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