Gotowa bibliografia na temat „Spectro-Polarimetric”
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Artykuły w czasopismach na temat "Spectro-Polarimetric"
Rousselet-Perraut, K., C. Stehlé, J. B. Le Bouquin, S. Jankov i F. Vakili. "Stellar polarimetry with SPIN (Spectro-Polarimetric INterferometry)". EAS Publications Series 9 (2003): 123. http://dx.doi.org/10.1051/eas:2003094.
Pełny tekst źródłaSmith, Craig H., Christopher M. Wright, David K. Aitken i Patrick F. Roche. "Mid-infrared Observations of Magnetic Fields in the Disks of Bi-Polar Outflow Sources". International Astronomical Union Colloquium 163 (1997): 799–800. http://dx.doi.org/10.1017/s0252921100044067.
Pełny tekst źródłavan Noort, M. "Spatially coupled inversion of spectro-polarimetric image data". Astronomy & Astrophysics 548 (12.11.2012): A5. http://dx.doi.org/10.1051/0004-6361/201220220.
Pełny tekst źródłaBoccaletti, Anthony, Anne-Lise Maire, Raphaël Galicher, Pierre Baudoz, Dimitri Mawet, John Trauger, Jean Schneider i in. "SPICES: A Mission Concept to Characterize Long Period Planets from Giants to Super-Earths". Proceedings of the International Astronomical Union 8, S293 (sierpień 2012): 429–34. http://dx.doi.org/10.1017/s1743921313013331.
Pełny tekst źródłaJordan, Stefan. "Magnetic fields in White Dwarfs and their direct progenitors". Proceedings of the International Astronomical Union 4, S259 (listopad 2008): 369–78. http://dx.doi.org/10.1017/s1743921309030749.
Pełny tekst źródłaGAN Shi-qi, 甘世奇, 陈向宁 CHEN Xiang-ning, 刘鹏 LIU Peng i 孙健 SUN Jian. "Transmittance spectrum in the liquid crystal spectro-polarimetric system". Chinese Journal of Liquid Crystals and Displays 32, nr 2 (2017): 97–103. http://dx.doi.org/10.3788/yjyxs20173202.0097.
Pełny tekst źródłaLepera, E., C. Provenzano, P. Pagliusi i G. Cipparrone. "Liquid Crystal Based Polarization Gratings for Spectro-Polarimetric Applications". Molecular Crystals and Liquid Crystals 558, nr 1 (30.05.2012): 109–19. http://dx.doi.org/10.1080/15421406.2011.653716.
Pełny tekst źródłaBommier, V., E. Landi Degl'Innocenti, M. Landolfi i G. Molodij. "UNNOFIT inversion of spectro-polarimetric maps observed with THEMIS". Astronomy & Astrophysics 464, nr 1 (14.12.2006): 323–39. http://dx.doi.org/10.1051/0004-6361:20054576.
Pełny tekst źródłaBoccaletti, Anthony, Jean Schneider, Wes Traub, Pierre-Olivier Lagage, Daphne Stam, Raffaele Gratton, John Trauger i in. "SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems". Experimental Astronomy 34, nr 2 (29.02.2012): 355–84. http://dx.doi.org/10.1007/s10686-012-9290-5.
Pełny tekst źródłaLibbrecht, Tine, Jaime de la Cruz Rodríguez, Sanja Danilovic, Jorrit Leenaarts i Hiva Pazira. "Chromospheric condensations and magnetic field in a C3.6-class flare studied via He I D3 spectro-polarimetry". Astronomy & Astrophysics 621 (styczeń 2019): A35. http://dx.doi.org/10.1051/0004-6361/201833610.
Pełny tekst źródłaRozprawy doktorskie na temat "Spectro-Polarimetric"
Aleau, Killian. "Développement d’un diffusiomètre supercontinuum pour la caractérisation spectro-polarimétrique des aérosols : application au problème de l’inversion des données lidar". Electronic Thesis or Diss., Toulouse, ISAE, 2024. http://www.theses.fr/2024ESAE0022.
Pełny tekst źródłaThe radiative properties of particles like aerosols are a crucial area of study for optical remote sensing, especially for techniques like elastic backscatter lidar. Radiative backscatter properties, such as the depolarization ratio, are particularly important for inverting the lidar equation and deriving physical products from a lidar measurement. The goal of this doctoral work aims to develop laboratory instrumentation dedicated to the spectropolarimetric measurement of the radiative parameters of aerosols, such as desert or volcanic dust. The instrument, named SOPHOS for Spectro-Polarimetric and HOlographic Scatterometer, allows for the measurement of scattering properties, including backscatter, as a function of wavelength in the visible to near-infrared spectrum, based on polarization states. These spectropolarimetric scattering measurements are coupled with a digital holography imaging technique to simultaneously measure microphysical properties, such as the size and shape of aerosols. Indeed, the backscatter phenomenon is particularly sensitive to the microphysical properties of aerosols. Following a validation of the measurement concept, the SOPHOS instrument was calibrated using spherical particles of known size and then used to measure the spectropolarimetric radiative properties of atmospheric aerosols, such as volcanic and desert dust, but also of interest for space, such as lunar regoliths. The contribution of these measurements will ultimately establish a link between their microphysical and radiative properties, particularly in backscatter for lidar applications. This study will focus on the analysis of depolarization as a function of particle size and shape factor at a multitude of wavelengths, to observe the effect of particle asphericity and wavelength on depolarization. In perspective, a portable version of the SOPHOS instrument was developed during the thesis. The HALO instrument is a portable holographic measurement device dedicated to the analysis of aerosols in the air. This device allows determining the size and shape distribution as well as a measurement of the aerosol extinction with the aim of providing a complementary analysis to remote lidar measurements
Perrot, Clément. "Imagerie directe de systèmes planétaires avec SPHERE et prédiction des performances de MICADO sur l’E-ELT". Thesis, Sorbonne Paris Cité, 2017. http://www.theses.fr/2017USPCC212/document.
Pełny tekst źródłaThis thesis is performed in the context of the study of the formation and evolution of planetary systems using high contrast imaging, also known as direct imaging in contrast to so-called "indirect" detection methods. The work I present in this manuscript is divided into two distinct parts.The first part concerns the observational component of my thesis, using the SPHERE instrument installed at Very LargeTelescope. This work was done as part of the consortium of the same name. The purpose of the SPHERE instrument is to detect and characterize young and massive exoplanets, but also circumstellar disks ranging from very young protoplanetary disks to older debris disks. In this manuscript, I present my contribution to the program SHINE, a large survey with an integration time of 200 nights' worth of observation, the goal of which is the detection of new exoplanets and the spectral and orbital characterization of some previously-known companions. I also present the two studies of circumstellar disks that I made, around the stars HD 141569 and HIP 86598. The first study allowed the discovery of concentric rings at about ten AU of the star along with an unusual flux asymmetry in the disk. The second study is about the discovery of a debris disk that also has an unusual flux asymmetry. The second part concerns the instrumental component of my thesis work done within the MICADO consortium, in charge of the design of the camera of the same name which will be one of the first light instruments of the European Extremely Large Telescope (ELT). In this manuscript, I present the study in which I define the design of some components of the coronagraphic mode of MICADO while taking into account the constraints of the instrument - which is not dedicated to high contrast imaging, unlike SPHERE
Książki na temat "Spectro-Polarimetric"
Hyperspectral and Spectro-Polarimetric Pixel-Level Classification Using Genetic Programming. Storming Media, 2001.
Znajdź pełny tekst źródłaCzęści książek na temat "Spectro-Polarimetric"
Ceolato, Romain, i Nicolas Riviere. "Advances in Spectro-Polarimetric Light-Scattering by Particulate Media". W Springer Series in Light Scattering, 55–107. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-70808-9_2.
Pełny tekst źródłaMukhopadhyay, Nilanjan, i Arijit Saha. "Design of Super-Achromatic Phase Controlling Assemblies for THz Spectro-Polarimetric Imaging System Using Metaheuristic Optimization Technique". W Progress in Optical Science and Photonics, 17–28. Singapore: Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-99-0228-6_2.
Pełny tekst źródłaStreszczenia konferencji na temat "Spectro-Polarimetric"
Kim, Youngchan, Wonjoon Jin, Sunghyun Cho i Seung-Hwan Baek. "Neural Spectro-polarimetric Fields". W SA '23: SIGGRAPH Asia 2023. New York, NY, USA: ACM, 2023. http://dx.doi.org/10.1145/3610548.3618172.
Pełny tekst źródłaGerini, G., L. P. Stoevelaar i T. Ceccotti. "Metamaterial Based Spectro-polarimetric Systems". W 2020 Fourteenth International Congress on Artificial Materials for Novel Wave Phenomena (Metamaterials). IEEE, 2020. http://dx.doi.org/10.1109/metamaterials49557.2020.9285133.
Pełny tekst źródłaKnitter, S., M. Kues i C. Fallnich. "Spectro-polarimetric Measurements on Random Lasers". W CLEO: Science and Innovations. Washington, D.C.: OSA, 2012. http://dx.doi.org/10.1364/cleo_si.2012.cth4d.5.
Pełny tekst źródłaWang, Xueji, Ziyi Yang i Zubin Jacob. "Spinning Meta-Cam: Spectro-Polarimetric Long-wave Infrared Thermal Imaging based on Spinning Metasurfaces". W CLEO: Fundamental Science. Washington, D.C.: Optica Publishing Group, 2023. http://dx.doi.org/10.1364/cleo_fs.2023.fth4d.2.
Pełny tekst źródłaHuber, Daniel F., Louis J. Denes, Martial Hebert, Milton S. Gottlieb, Boris Kaminsky i Peter Metes. "Spectro-polarimetric imager for intelligent transportation systems". W Intelligent Systems & Advanced Manufacturing, redaktorzy Marten J. de Vries, Pushkin Kachroo, Kaan Ozbay i Alan C. Chachich. SPIE, 1998. http://dx.doi.org/10.1117/12.300844.
Pełny tekst źródłaLevesque, Martin P., Maria Dissanska i Jean-Pierre Ardouin. "Polarization artefacts correction procedure for a spectro-polarimetric goniometer". W IGARSS 2014 - 2014 IEEE International Geoscience and Remote Sensing Symposium. IEEE, 2014. http://dx.doi.org/10.1109/igarss.2014.6947108.
Pełny tekst źródłaPlemmons, Robert J., Sudhakar Prasad i Qiang Zhang. "Deblurring Compressive Spectro-Polarimetric Images Taken Trough Atmospheric Turbulence". W Signal Recovery and Synthesis. Washington, D.C.: OSA, 2014. http://dx.doi.org/10.1364/srs.2014.stu3f.1.
Pełny tekst źródłaJones, A. M., S. A. Kemme, D. A. Scrymgeour i R. A. Norwood. "Single layer spectro-polarimetric filter for advanced LWIR FPAs". W SPIE Defense, Security, and Sensing, redaktorzy Bjørn F. Andresen, Gabor F. Fulop i Paul R. Norton. SPIE, 2012. http://dx.doi.org/10.1117/12.919313.
Pełny tekst źródłaRodenhuis, M., B. Sprenger i C. U. Keller. "A spectro-polarimetric integral field spectrograph for EPICS-EPOL". W SPIE Astronomical Telescopes + Instrumentation, redaktorzy Ian S. McLean, Suzanne K. Ramsay i Hideki Takami. SPIE, 2012. http://dx.doi.org/10.1117/12.927206.
Pełny tekst źródłaLozi, Julien, Olivier Guyon, Tomoyuki Kudo, Jin Zhang, Nemanja Jovanovic, Barnaby Norris, Marc-Antoine Martinod i in. "New NIR spectro-polarimetric modes for the SCExAO instrument". W Adaptive Optics Systems VII, redaktorzy Dirk Schmidt, Laura Schreiber i Elise Vernet. SPIE, 2020. http://dx.doi.org/10.1117/12.2562792.
Pełny tekst źródłaRaporty organizacyjne na temat "Spectro-Polarimetric"
Rauss, Patrick. Hyperspectral and Spectro-Polarimetric Pixel-Level Classification Using Genetic Programming. Fort Belvoir, VA: Defense Technical Information Center, listopad 2001. http://dx.doi.org/10.21236/ada397832.
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