Relevant bibliographies by topics / Satellites en Rotation

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Satellites en Rotation'

Author: Grafiati
Published: 8 February 2025
Last updated: 31 July 2025

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Journal articles on the topic "Satellites en Rotation"

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Agrusa, Harrison F., Yun Zhang, Derek C. Richardson, et al. "Direct N-body Simulations of Satellite Formation around Small Asteroids: Insights from DART’s Encounter with the Didymos System." Planetary Science Journal 5, no. 2 (2024): 54. http://dx.doi.org/10.3847/psj/ad206b.

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Abstract We explore binary asteroid formation by spin-up and rotational disruption considering the NASA DART mission's encounter with the Didymos–Dimorphos binary, which was the first small binary visited by a spacecraft. Using a suite of N-body simulations, we follow the gravitational accumulation of a satellite from meter-sized particles following a mass-shedding event from a rapidly rotating primary. The satellite’s formation is chaotic, as it undergoes a series of collisions, mergers, and close gravitational encounters with other moonlets, leading to a wide range of outcomes in terms of th
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Raghuprasad, Puthalath Koroth. "Synchronous, Nonsynchronous and Negative Rotations: How Spin and Gravity Orchestrate Planetary Motions." Applied Physics Research 12, no. 2 (2020): 1. http://dx.doi.org/10.5539/apr.v12n2p1.

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This study identifies the unique features accompanying the phenomenon of synchronous rotation of the major (proximal) satellites of the gas giants and the earth’s moon, and the special features leading to the ‘negative’ rotation of Venus, Uranus and Pluto, as well as the most peripheral small satellites of the gas giants. Such features help us understand how these phenomena occur but also, by combining all of the observations help explain other (regular) planetary motions as well. In the synchronously rotating satellites, the salient features are the satellites&am
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Lieske, J. H. "IAU North Poles and Rotation Parameters for Natural Satellites." Symposium - International Astronomical Union 156 (1993): 351–56. http://dx.doi.org/10.1017/s0074180900173498.

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In 1970 the IAU defined any object'snorthpole to be that axis of rotation which lies north of the solar system's invariable plane. A competing definition in widespread use at some institutions followed the “right hand rule” whereby the “north” axis of rotation was generally said to be that that of the rotational angular momentum.A Working Group has periodically updated the recommended values of planet and satellite poles and rotation rates in accordance with the IAU definition of north and the IAU definition of prime meridian.In this paper we review the IAU definitions ofnorthand of the locati
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Van Hoolst, Tim. "The libration and interior structure of large icy satellites and Mercury." Proceedings of the International Astronomical Union 9, S310 (2014): 1–8. http://dx.doi.org/10.1017/s1743921314007698.

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AbstractLongitudinal librations are periodic changes in the rotation angle of a planet or satellite. Their observation and subsequent interpretation have profoundly increased our understanding of the interior structure of Mercury. Likewise, libration is thought to provide important constraints on the interior structure of icy satellites. Here we study the libration of Mercury and large icy satellites rotating synchronously with their orbital motion and explain how it depends on the interior structure.
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Pashkevich, Vladimir V., and Andrey N. Vershkov. "Geodetic Precession of the Sun, Solar System Planets, and their Satellites." Artificial Satellites 57, no. 1 (2022): 77–109. http://dx.doi.org/10.2478/arsa-2022-0005.

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Abstract The effect of the geodetic precession is the most significant relativistic effect in the rotation of celestial bodies. In this article, the new geodetic precession values for the Sun, the Moon, and the Solar System planets have been improved over the previous version by using more accurate rotational element values. For the first time, the relativistic effect of the geodetic precession for some planetary satellites (J1–J4, S1–S6, S8–S18, U1–U15, N1, and N3–N8) with known quantities of the rotational elements was studied in this research. The calculations of the values of this relativi
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Pashkevich, Vladimir V., and Andrey N. Vershkov. "Geodetic Precession of the Sun, Solar System Planets, and their Satellites." Artificial Satellites 57, no. 1 (2022): 77–109. http://dx.doi.org/10.2478/arsa-2022-0005.

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Abstract The effect of the geodetic precession is the most significant relativistic effect in the rotation of celestial bodies. In this article, the new geodetic precession values for the Sun, the Moon, and the Solar System planets have been improved over the previous version by using more accurate rotational element values. For the first time, the relativistic effect of the geodetic precession for some planetary satellites (J1–J4, S1–S6, S8–S18, U1–U15, N1, and N3–N8) with known quantities of the rotational elements was studied in this research. The calculations of the values of this relativi
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Velgas, Lev Borisovich, and Liia Lvovna Iavolinskaia. "Seven main discoveries, rigorously proven." Interactive science, no. 6 (40) (June 21, 2019): 103–5. http://dx.doi.org/10.21661/r-496981.

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We are striving to prove that all planets rotate around their axis due to their satellites. Rotation of the collateral gravitation is analogous for all the planets, for the Sun as well. The Sun, as well as every single planet, can have multiple satellites. Satellite and planet’s collateral gravitation, if it moves because of satellite’s movement around the orbit, rotates the planet or the Sun. The article proves that collateral gravitation of the Moon and the Earth, that moves around the Earth due to Moon’s movement around the Earth, rotates the Earth around it’s axis.
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Zhang, Xiaozhen, Yao Kong, Xiaochun Lu, and Decai Zou. "Contribution of Etalon Observation to Earth Rotation Parameters under a New Observation Scenario." Applied Sciences 12, no. 10 (2022): 4936. http://dx.doi.org/10.3390/app12104936.

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The standard products of the International Laser Ranging Service (ILRS) are mainly based on the two laser geodynamics satellites (LAGEOS) due to the sparse observations of the Etalon satellites. With improvements in the ability to track high-altitude satellites, ILRS conducted a 3-month Etalon tracking campaign. In this paper, we study the contribution of more Etalon observations in the new observation scenario to weekly ILRS products, such as station coordinates, Earth rotation parameters (ERPs) and satellite orbit. We compare the ILRS products estimated from LAGEOS-only solutions and LAGEOS+
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Pashkevich, V. V., and A. N. Vershkov. "Secular geodetic rotation of celestial bodies in the system of Jupiter’s moons." Publications of the Pulkovo Observatory 235 (December 2024): 51–68. https://doi.org/10.31725/0367-7966-2024-235-51-68.

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This article studies the relativistic effect of geodetic precession in the rotation around their axes of Jupiter and its 94 satellites for which ephemerides are known. As a result, the most significant secular terms of the geodetic rotation of these celestial bodies were determined for the first time: 1. for Jupiter relative to the barycenter of the Solar System and the plane of the mean orbit of Jupiter at the epoch J2000.0 in Euler angles, in the perturbing terms of physical libration and in the absolute value of the vector of angular rotation of the geodetic rotation of the body under study
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Schildknecht, T., I. Bauersima, U. Hugentobler, A. Verdun, and G. Beutler. "CQSSP: A New Technique for Establishing the Tie Between the Stellar and Quasar Celestial Reference Frames." International Astronomical Union Colloquium 127 (1991): 341–47. http://dx.doi.org/10.1017/s0252921100064174.

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AbstractUsing artificial satellites as transfer objects the project “Coupled Quasar-Satellite-Star Positioning” represents an independent method for linking quasar and stellar reference frames. Optical observations of close approaches between reference stars and satellites yield satellite positions in the stellar reference frame. On the other hand high precision satellite orbits in the International Earth Rotation Service (IERS) terrestrial reference frame are obtained from laser or radiometric observations. Using IERS earth rotation parameters and adopted transformation models the satellite a
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Dissertations / Theses on the topic "Satellites en Rotation"

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Cottereau, Laure. "Etude complète de la rotation d'un corps triaxial : application à Vénus et à Phoebe." Paris 6, 2011. http://www.theses.fr/2011PA066261.

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Cette thèse a pour sujet l'étude des mouvements de rotation des corps dits triaxiaux, qui ne sont pas seulement aplatis comme la Terre, mais qui s'écartent aussi de la symétrie axiale. Nous commençons par construire une théorie analytique fondée sur un formalisme Hamiltonien, que nous appliquons ensuite à deux corps triaxiaux : la planète Vénus et le neuvième satellite de Saturne, Phoebe. Ceci nous permet de déterminer pour la première fois leurs coefficients de précession-nutation en longitude et en obliquité. On présente aussi les caractéristiques du mouvement libre de Vénus. Puis nous rééva
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Robertson, Michael James. "Command Generation for Tethered Satellite Systems." Diss., Georgia Institute of Technology, 2005. http://hdl.handle.net/1853/6921.

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Command generation is a process by which input commands are constructed or modified such that the system's response adheres to a set of desired performance specifications. Previously, a variety of command generation techniques such as input shaping have been used to reduce residual vibration, limit transient deflection, conserve fuel or adhere to numerous other performance specifications or performance measures. This dissertation addresses key issues regarding the application of command generation techniques to tethered satellite systems. The three primary objectives of this research are as
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Evans, Joshua L. "SMALL SATELLITE NONCOMMUTATIVE ROTATION SEQUENCE ATTITUDE CONTROL USING PIEZOELECTRIC ACTUATORS." UKnowledge, 2016. http://uknowledge.uky.edu/ece_etds/91.

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Attitude control remains one of the top engineering challenges faced by small satellite mission planning and design. Conventional methods for attitude control include propulsion, reaction wheels, magnetic torque coils, and passive stabilization mechanisms, such as permanent magnets that align with planetary magnetic fields. Drawbacks of these conventional attitude control methods for small satellites include size, power consumption, dependence on external magnetic fields, and lack of full control authority. This research investigates an alternative, novel approach to attitude-control method fo
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Debes, John H., Charles A. Poteet, Hannah Jang-Condell, et al. "Chasing Shadows: Rotation of the Azimuthal Asymmetry in the TW Hya Disk." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/623947.

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We have obtained new images of the protoplanetary disk orbiting TW Hya in visible, total intensity light with the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST), using the newly commissioned BAR5 occulter. These HST/STIS observations achieved an inner working angle of similar to 0."2, or 11.7 au, probing the system at angular radii coincident with recent images of the disk obtained by ALMA and in polarized intensity near-infrared light. By comparing our new STIS images to those taken with STIS in 2000 and with NICMOS in 1998, 2004, and 2005, we demonstrate that
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Ning, Zuoli. "Roles of plate locking and block rotation in the tectonics of the Pacific Northwest /." Thesis, Connect to this title online; UW restricted, 2003. http://hdl.handle.net/1773/6833.

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Astoul, Aurélie. "Impact du magnétisme et de la rotation différentielle sur les marées dans les étoiles de faible masse et les planètes géantes gazeuses." Thesis, Université de Paris (2019-....), 2020. http://www.theses.fr/2020UNIP7073.

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Plus de 4000 exoplanètes ont été découvertes au cours de ces 25 dernières années, pour la plupart en orbite autour d’étoiles de faible masse. Dans les systèmes planétaires à très courte période orbitale, les interactions de marée étoile-planète sont connues pour gouverner l’évolution tardive de l’architecture orbitale des systèmes et de la rotation de leur étoile hôte, comme c’est aussi le cas dans les systèmes serrés planète-satellite(s) de notre système solaire tels que les systèmes jovien et saturnien. Les temps caractéristiques de variation des paramètres orbitaux et de rotation des corps,
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Kulick, Wayne J. "Development of a Control Moment Gyroscope controlled, three axis satellite simulator, with active balancing for the bifocal relay mirror initiative." Thesis, Monterey, Calif. : Springfield, Va. : Naval Postgraduate School ; Available from National Technical Information Service, 2004. http://library.nps.navy.mil/uhtbin/hyperion/04Dec%5FKulick.pdf.

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LOYER, SYLVAIN. "Techniques dynamiques d'observation de la rotation de la terre mesures satellites et apports des gravimetres et des gyroscopes." Toulouse 3, 1997. http://www.theses.fr/1997TOU30269.

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Les variations de l'orientation de la terre dans l'espace sont aujourd'hui mesurees par differentes techniques astrometriques ; radio-interferometrie a tres longue base, tirs lasers sur la lune, et mesures de positionnement des satellites artificiels. Les parametres de rotation de la terre, utilises pour decrire les variations d'orientation sont determines avec une precision inferieure a 1 milliseconde de degre, et une resolution temporelle de 1 jour. Nous presentons les resultats de mesure des variations a courte periode de l'orientation (variations diurnes et subdiurnes) et nous montrons com
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Coulot, David. "Télémétrie laser sur satellites et combinaison de techniques géodésiques : contributions aux systèmes de référence terrestres et applications." Phd thesis, Observatoire de Paris, 2005. http://tel.archives-ouvertes.fr/tel-00069016.

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La qualité actuelle des techniques de Géodésie Spatiale permet d'estimer des séries temporelles de produits géodésiques tels que les paramètres de rotation et les positions de stations terrestres. Ces nouveaux produits doivent être utilisés dans la matérialisation des Systèmes de Référence Terrestres, en constantes évolution et amélioration. Ils doivent aussi mettre en évidence les phénomènes, globaux ou locaux, régissant la rotation terrestre et les mouvements de la croûte. C'est dans ce contexte riche d'enjeux divers que s'inscrivent ces travaux. Leur but premier a été l'élaboration et l'app
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Coulot, David. "Télémétrie laser sur satellites et combinaison de techniques géodésiques : contributions aux systèmes de référence terrestres et applications." Phd thesis, Observatoire de Paris (1667-....), 2005. https://theses.hal.science/tel-00069016.

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La qualité actuelle des techniques de géodésie spatiale permet d'estimer des séries temporelles de produits géodésiques tels que les paramètres de rotation et les positions de stations terrestres. Ces nouveaux produits doivent être utilisés dans la matérialisation des systèmes de référence terrestres, en constantes évolution et amélioration. Ils doivent aussi mettre en évidence les phénomènes, globaux ou locaux, régissant la rotation terrestre et les mouvements de la croûte. C’est dans ce contexte riche d’enjeux divers que s’inscrivent ces travaux. Leur but premier a été l’élaboration et l’app
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Books on the topic "Satellites en Rotation"

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A, Arnold David, Grossi Mario D, Gullahorn Gordon E, and United States. National Aeronautics and Space Administration, eds. The investigation of tethered satellite system dynamics: Quarterly report, #7 for the period 15 February 1986 through 14 May 1986. Smithsonian Institution, Astrophysical Observatory, 1986.

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Belet͡skiĭ, V. V. Vrashchatelʹnoe dvizhenie namagnichennogo sputnika. "Nauka," Glav. red. fiziko-matematicheskoĭ lit-ry, 1985.

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United States. National Aeronautics and Space Administration., ed. Ocean tide models for satellite geodesy and earth rotation: Final technical report. National Aeronautics and Space Administration, 1991.

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Grazzini, Francesca. Sun, where do you go? Kane/Miller Book Publishers, 1996.

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Stewart, Melissa. Why do seasons change? Marshall Cavendish Benchmark, 2006.

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Langel, R. A. The magnetic field of the Earth's lithosphere: The satellite perspective. Cambridge University Press, 1998.

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Slade, Suzanne. Seasonal cycles. Rosen Pub. Group's PowerKids Press, 2007.

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Rau, Dana Meachen. El tiempo y el espacio. Marshall Cavendish Benchmark, 2009.

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Rau, Dana Meachen. Space and time. Marshall Cavendish Benchmark, 2008.

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E, Davies Merton, Rogers Patricia G, and United States. National Aeronautics and Space Administration., eds. Phoebe: Preliminary control network and rotational elements. Rand, 1990.

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Book chapters on the topic "Satellites en Rotation"

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Lieske, J. H. "IAU North Poles and Rotation Parameters for Natural Satellites." In Developments in Astrometry and Their Impact on Astrophysics and Geodynamics. Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1711-1_65.

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Lainey, V., and A. Vienne. "Rotation of Natural Shaped Satellites and Their Orbital Motion." In Modern Celestial Mechanics: From Theory to Applications. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-2304-6_31.

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Hussmann, Hauke, Gaël Choblet, Valéry Lainey, et al. "Implications of Rotation, Orbital States, Energy Sources, and Heat Transport for Internal Processes in Icy Satellites." In Satellites of the Outer Solar System. Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-7439-6_12.

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Moon, Wooil M., Roger Tang, and B. H. Choi. "Study of fluid-solid earth coupling process using satellite altimeter data." In Variations in Earth Rotation. American Geophysical Union, 1990. http://dx.doi.org/10.1029/gm059p0085.

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Zhang, Jiahao, Ming Zhang, Zuoliang Yin, Zhian Deng, and Weijian Si. "WiFi CSI Fingerprinting Positioning Based on User Rotation." In Wireless and Satellite Systems. Springer International Publishing, 2019. http://dx.doi.org/10.1007/978-3-030-19153-5_27.

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Svehla, Drazen. "Insight into the Earth’s Interior from Geometrical Rotations in Temporal Gravity Field Maps and Earth’s Rotation." In Geometrical Theory of Satellite Orbits and Gravity Field. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-76873-1_28.

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Svehla, Drazen. "A Geometrical Approach to Model Circular Rotations." In Geometrical Theory of Satellite Orbits and Gravity Field. Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-76873-1_23.

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Bois, E. "Analytical Theory of the Rotation of an Artificial Satellite." In Long-Term Dynamical Behaviour of Natural and Artificial N-Body Systems. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-3053-7_11.

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Li, Guiming, Zhihui Li, Rui Liu, Jianfu Zhang, Yushuang Wang, and Ao Chen. "Layout Design of Satellite Star Sensor Fixed to Rotation Platform." In Lecture Notes in Electrical Engineering. Springer Nature Singapore, 2023. http://dx.doi.org/10.1007/978-981-19-6613-2_664.

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Lara, Martin. "Collinear Point Dynamics of a Dumbbell Satellite in Fast Rotation." In NODYCON Conference Proceedings Series. Springer Nature Switzerland, 2024. http://dx.doi.org/10.1007/978-3-031-50631-4_44.

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Conference papers on the topic "Satellites en Rotation"

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He, Jie, Jianjun Yi, and Lelun Xu. "Non-cooperative Satellite Rotation Estimation Based on Monocular Vision." In 2024 4th Asia-Pacific Conference on Communications Technology and Computer Science (ACCTCS). IEEE, 2024. http://dx.doi.org/10.1109/acctcs61748.2024.00056.

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Liu, Yangfan, Yanan Guo, Huanyu Bian, et al. "Rotation correction-based neural radiance fields for multiview satellite images." In Optoelectronic Imaging and Multimedia Technology XI, edited by Zhenrong Zheng and Jinli Suo. SPIE, 2024. http://dx.doi.org/10.1117/12.3037382.

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Lohit, Suhas, and Tim K. Marks. "Rotation-Equivariant Neural Networks for Cloud Removal from Satellite Images." In 2024 58th Asilomar Conference on Signals, Systems, and Computers. IEEE, 2024. https://doi.org/10.1109/ieeeconf60004.2024.10942613.

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Faieta, Matteo, Federico Masiero, Alessandro Niccolai, and Riccardo Zich. "Evolutionary Optimization of Reflectarrays with Steering Beam by Feeder Rotation for Satellite Antennas." In IAF Space Communications and Navigation Symposium, Held at the 75th International Astronautical Congress (IAC 2024). International Astronautical Federation (IAF), 2024. https://doi.org/10.52202/078363-0063.

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Ali, Muhammad Moazzam, Shaiful Jahari Hashim, Zaid Ahmad, Guillaume Ferré, Fakhrul Zaman Rokhani, and Muhammad Akmal Chaudhary. "Frequency Dependent RSSI Behavior of Rotating Polarization Waves in Diverse Environmental Conditions." In 2024 IEEE International Conference on Communication, Networks and Satellite (COMNETSAT). IEEE, 2024. https://doi.org/10.1109/comnetsat63286.2024.10862054.

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Zhang, Jiahao, Hui Zhao, Mingyang Yang, and Xuewu Fan. "High-resolution rotating pupil optical imaging for satellite remote sensing." In Optoelectronic Imaging and Multimedia Technology XI, edited by Zhenrong Zheng and Jinli Suo. SPIE, 2024. http://dx.doi.org/10.1117/12.3036296.

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Zhang, Yuchen, Yang Zheng, Yuhuan Zhang, Shijie Liu, and Shangrong Ouyang. "Design of QV-Band Rotating Joint Apply in Satellite Communication System." In 2025 IEEE 5th International Conference on Power, Electronics and Computer Applications (ICPECA). IEEE, 2025. https://doi.org/10.1109/icpeca63937.2025.10928801.

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Kang, Jingyi, Wenlai Ma, and Shengyu Lin. "Adaptive Attitude Control of a Satellite with Bilateral Rotating Solar Arrays." In 2024 2nd Asian Aerospace and Astronautics Conference (AAAC). IEEE, 2024. https://doi.org/10.1109/aaac63570.2024.11027360.

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Lukaschek, Leon, Vijay Nagalingesh, Lisa Elsner, Alexander Kleinschrodt, Marco Schmidt, and Klaus Schilling. "Algorithmic Center of Rotation to Center of Mass Offset Estimation of a Spherical Air-Breaing Attitude Simulator." In 31st IAA Symposium on Small Satellite Missions, Held at the 75th International Astronautical Congress (IAC 2024). International Astronautical Federation (IAF), 2024. https://doi.org/10.52202/078365-0187.

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Yang, Wenhui, Yong Li, Jianfeng Wang, and Daifang Huang. "Observability of INS/OD Integration with Rotating MEMS IMU: A Global Perspective." In 37th International Technical Meeting of the Satellite Division of The Institute of Navigation (ION GNSS+ 2024). Institute of Navigation, 2024. http://dx.doi.org/10.33012/2024.19775.

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