Academic literature on the topic 'Radar telescopes'

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Journal articles on the topic "Radar telescopes"

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Ruf, K., E. Fürst, K. Grypstra, J. Neidhöfer, and M. Schumacher. "Response of the Effelsberg 100m radio telescope to signals in the near-field at 24 GHz." Advances in Radio Science 1 (May 5, 2003): 329–33. http://dx.doi.org/10.5194/ars-1-329-2003.

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Abstract. Short range radar (SRR) for cars has been proposed to operate over 5 GHz of bandwidth at the 24 GHz ISM band. To estimate the level of interference from these devices on radio telescopes, the near-field antenna pattern has to be known. We report on new measurements with the Effelsberg 100 m radio telescope. These measurements were performed with a transmitter set up at a distance of 1.7 km from the telescope. The strength of the signal picked up by the telescope sidelobes shows that the proposed SRR would interfere with sensitive radio astronomical observations.
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Huyan, Zongbo, Yu Jiang, Hengnian Li, Pengbin Ma, and Dapeng Zhang. "Bistatic Radar Observations Correlation of LEO Satellites Considering J2 Perturbation." Mathematics 10, no. 13 (2022): 2197. http://dx.doi.org/10.3390/math10132197.

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Space debris near Earth severely interferes with the development of space, and cataloging space objects is increasingly important. Since optical telescopes and radars used to detect space debris only provide short-arc observations, mathematical algorithms are needed to solve problems in the correlation of observations. In this work, an efficient mathematical algorithm based on J2 analytic solutions is put forward. Initial orbit determination (IOD) serves as the starter and orbit determination (OD) with the weighted least-squares method (WLSM) is used to improve the accuracy of the estimated or
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Sobirin, Farhan Fatwa, Satia Nugraha, Fauzia Haz, and Peberlin Sitompul. "Study of Cassegrain-type antenna for radio telescope." Journal of Physics: Conference Series 2214, no. 1 (2022): 012028. http://dx.doi.org/10.1088/1742-6596/2214/1/012028.

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Abstract There are many critical parameters in the design of a radio telescope, such as antenna gain and antenna resolution. In telecommunications, radar, and radio telescopes, an antenna is a very important component. There are many designs of the antenna, such as dipole array and parabolic antenna. Parabolic antennas also have many sub-reflector and antenna methods that control the radio wave, such as the Cassegrain type. A Cassegrain-type antenna is a parabolic antenna in which the feed antenna is mounted at or behind the surface of the main parabolic reflector dish. For the transmitter sys
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Sun, Jing, Jinsong Ping, Yuri Bondarenko, et al. "Promoting Earth-Based Radar Astronomical Observations of the Moon." Sensors 20, no. 7 (2020): 1874. http://dx.doi.org/10.3390/s20071874.

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Earth-based radar astronomical observations provide information on surface characteristics, orbits, and rotations for a wide variety of solar system objects. Based on compound radio telescopes, both the Chinese VLBI (Very Long Baseline Interferometry) network (CVN) and the Russian VLBI network (Quasar), in cooperation with the Chinese radar transmitters, we present the current ground radar astronomical observations of the moon. The spectrum of the reflected radio signals was obtained and the Doppler frequency shift in bi-static radar mode was measured. Radar albedo of the observed region and p
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Kłos, Julia, Konrad Jędrzejewski, Aleksander Droszcz, Krzysztof Kulpa, Mariusz Pożoga, and Jacek Misiurewicz. "Experimental Verification of the Concept of Using LOFAR Radio-Telescopes as Receivers in Passive Radiolocation Systems." Sensors 21, no. 6 (2021): 2043. http://dx.doi.org/10.3390/s21062043.

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The paper presents a new idea of using a low-frequency radio-telescope belonging to the LOFAR network as a receiver in a passive radar system. The structure of a LOFAR radio-telescope station is described in the context of applying this radio-telescope for detection of aerial (airplanes) and space (satellite) targets. The theoretical considerations and description of the proposed signal processing schema for the passive radar based on a LOFAR radio-telescope are outlined in the paper. The results of initial experiments verifying the concept of a LOFAR station use as a receiver and a commercial
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Virkki, Anne, Catherine Neish, Edgard Rivera-Valentín, et al. "Planetary Radar—State-of-the-Art Review." Remote Sensing 15, no. 23 (2023): 5605. http://dx.doi.org/10.3390/rs15235605.

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Planetary radar observations have provided invaluable information on the solar system through both ground-based and space-based observations. In this overview article, we summarize how radar observations have contributed in planetary science, how the radar technology as a remote-sensing method for planetary exploration and the methods to interpret the radar data have advanced in the eight decades of increasing use, where the field stands in the early 2020s, and what are the future prospects of the ground-based facilities conducting planetary radar observations and the planned spacecraft missio
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Gallardo-Alvarado, Jaime, Horacio Orozco-Mendoza, and José M. Rico-Martínez. "A novel five-degrees-of-freedom decoupled robot." Robotica 28, no. 6 (2009): 909–17. http://dx.doi.org/10.1017/s0263574709990749.

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SUMMARYIn this work a new nonoverconstrained redundant decoupled robot, free of compound joints, formed from three parallel manipulators, with two moving platforms and provided with six active limbs connected to the fixed platform, called LinceJJP, is presented. Interesting applications such as multi-axis machine tools with parallel kinematic architectures, solar panels, radar antennas, and telescopes are available for this novel spatial mechanism.
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Ostro, Steven J. "Radar Astrometry of Asteroids, Comets and Planetary Satellites." Symposium - International Astronomical Union 172 (1996): 365–72. http://dx.doi.org/10.1017/s0074180900127706.

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Groundbased radar has considerable astrometric potential for asteroids, comets and natural satellites that enter the detectability windows of available telescopes. For very closely approaching asteroids and comets, measurements of the distribution of echo power in time delay (range) and Doppler frequency (radial velocity) can achieve a fractional precision between 10−5 and 10−9, and consequently are invaluable for refining orbits and prediction ephemerides. Even for mainbelt asteroids and the more readily detectable planetary satellites whose orbits are very well known, radar can collapse rang
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Lister, Tim A., S. Greenstreet, E. Gomez, E. Christensen, and S. Larson. "The LCOGT NEO Follow-up Network." Proceedings of the International Astronomical Union 10, S318 (2015): 321–23. http://dx.doi.org/10.1017/s1743921315006778.

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AbstractLas Cumbres Observatory Global Telescope Network (LCOGT) has deployed a homogeneous telescope network of nine 1-meter telescopes to four locations in the northern and southern hemispheres, with a planned network size of twelve 1-meter telescopes at 6 locations. This network is very versatile and is designed to respond rapidly to target of opportunity events and also to perform long term monitoring of slowly changing astronomical phenomena. The global coverage of the network and the apertures of telescope available make LCOGT ideal for follow-up and characterization of Solar System obje
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McMillan, Robert S., Jeffrey A. Larsen, Terrence H. Bressi, James V. Scotti, Ronald A. Mastaler, and Andrew F. Tubbiolo. "Spacewatch Astrometry and Photometry of Near-Earth Objects." Proceedings of the International Astronomical Union 10, S318 (2015): 317–18. http://dx.doi.org/10.1017/s1743921315006766.

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AbstractThe Spacewatch Project uses four telescopes of apertures 0.9-m, 1.8-m, 2.3-m, and 4-m on Kitt Peak mountain in Arizona for followup astrometry of priority NEOs. Objects as faint as V=23 on the MPC's NEO Confirmation Page, targets of radar, potential impactors, targets of spacecraft observations or visits, and PHAs with future close approaches to Earth receive priority for astrometry.
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Dissertations / Theses on the topic "Radar telescopes"

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Dituri, Joseph. "Ballistic missile trajectory estimation." Thesis, Monterey, Calif. : Naval Postgraduate School, 2006. http://bosun.nps.edu/uhtbin/hyperion.exe/06Dec%5FDituri.pdf.

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Thesis (M.S. in Astronautical Engineering)--Naval Postgraduate School, December 2006.<br>Thesis Advisor(s): Kyle T. Alfriend, Don A. Danielson. "December 2006." Includes bibliographical references (p. 57). Also available in print.
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Plante, Julien. "Technologies habilitantes pour l’acquisition et le traitement en temps-réel de gros volumes de données et leurs applications aux télescopes astronomiques géants et aux systèmes radars." Electronic Thesis or Diss., Université Paris sciences et lettres, 2023. http://www.theses.fr/2023UPSLO015.

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Les systèmes de notre monde sont en croissance constante en termes de précision, rapidité et consommation énergetique. Cette croissance passe par la production de volumes de données toujours plus importants, qui deviennent difficiles à traiter avec les technologies standard actuelles. Dans le cadre de cette thèse, nous nous sommes intéressé à des technologies émergentes, telles que le calcul sur GPU, le réseau en espace utilisateur, DPDK et GPUDirect, permettant de répondre à ce besoin, et les avons appliquées à plusieurs projets concrets (acquisition de front d’ondes pour optique adaptative,
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Brundage, William D. "VLA X-Band Preparation for Voyager 2 at Neptune." International Foundation for Telemetering, 1987. http://hdl.handle.net/10150/615320.

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International Telemetering Conference Proceedings / October 26-29, 1987 / Town and Country Hotel, San Diego, California<br>The Very Large Array (VLA) radio telescope, located in west-central New Mexico, obtains high-resolution radio images of astronomical objects by using Fourier aperture synthesis with 27 antennas. With the addition of X-band to its receiving capabilities by 1989, and when arrayed with the Goldstone Deep Space Communications Complex (GDSCC), the VLA will double the Deep Space Network (DSN) receiving aperture in the U. S. longitude for signals from Voyager 2 at Neptune. This p
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Books on the topic "Radar telescopes"

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United States. National Aeronautics and Space Administration., ed. Lidar analyses: Contract period 7/01/93 - 10/30/94. Center for Applied Optics, University of Alabama in Huntsville, 1995.

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Meeting, COSPAR Plenary. Ionospheric incoherent scatter results: Proceedings of Workshop V of the COSPAR twenty-seventh Plenary Meeting held in Espoo, Finland, 18-29 July 1988. Published for the Committee on Space Research by Pergamon Press, 1989.

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Mar, James W., and Harold Liebowitz. Structures Technology for Large Radio and Radar Telescope Systems. MIT Press, 2003.

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Analyzing the Physics of Radio Telescopes and Radio Astronomy. IGI Global, 2020.

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Yeap, Kim Ho, and Kazuhiro Hirasawa. Analyzing the Physics of Radio Telescopes and Radio Astronomy. IGI Global, 2020.

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Yeap, Kim Ho, and Kazuhiro Hirasawa. Analyzing the Physics of Radio Telescopes and Radio Astronomy. IGI Global, 2020.

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Yeap, Kim Ho, and Kazuhiro Hirasawa. Analyzing the Physics of Radio Telescopes and Radio Astronomy. IGI Global, 2020.

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Yeap, Kim Ho, and Kazuhiro Hirasawa. Analyzing the Physics of Radio Telescopes and Radio Astronomy. IGI Global, 2020.

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Gordon, M. A. Recollections of "Tucson Operations": The Millimeter-Wave Observatory of the National Radio Astronomy Observatory. Springer, 2011.

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Cospar. Ionospheric Incoherent Scatter Results: Proceedings of Workshop V of the Cospar 27th Plenary Meeting Held in Espoo, Finland, 18-29 July, 1988 (Ionospheric Incoherent Scatter Results). Elsevier Science Pub Co, 1989.

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Book chapters on the topic "Radar telescopes"

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Orchiston, Wayne, Peter Robertson, and Woodruff T. Sullivan III. "From Radar to Radio Astronomy." In Golden Years of Australian Radio Astronomy. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-319-91843-3_1.

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AbstractToday’s astronomers study the sky at a wide range of wavelengths, spread across the electromagnetic spectrum, from radio through microwave, infrared, the optical range, the ultraviolet, X-rays and gamma rays (Fig. 1.1). They also use cosmic rays and neutrinos, and the newest field is gravitational wave astronomy. Some of these types of radiation can be observed from the Earth’s surface, others rely on space telescopes. Some are comparatively recent innovations, while optical astronomy – in various guises – dates back many millennia.
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Sánchez, Francisco. "Telescopes Versus Military Radars (1977–1978)." In Astronomers' Universe. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-66426-8_11.

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Cottrell, Geoff. "7. The radio sky." In Telescopes: A Very Short Introduction. Oxford University Press, 2016. http://dx.doi.org/10.1093/actrade/9780198745860.003.0007.

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‘The radio sky’ considers radio telescopes that can see much longer wavelengths. Cosmic radio waves were first discovered in 1932 by Karl Jansky, with the first radio telescope built in 1937. Technology for radar systems advanced during World War II and then after the war scientists, such as Bernard Lovell and Martin Ryle, made use of the advances in electronics, radio technology, and digital computers, to found radio astronomy. Single-dish antennas—including the Lovell Telescope at Jodrell Bank Observatory—continue to play important roles. To improve angular resolution two antennas need to be operated as an interferometer. These are described along with the discovery of quasars, supermassive black holes, pulsars, and neutron stars.
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"Homologous Deformation of Tiltable Telescopes." In Structures Technology for Large Radio and Radar Telescope Systems. The MIT Press, 2003. http://dx.doi.org/10.7551/mitpress/6523.003.0020.

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"Maintaining Surface Accuracy of Large Radio Telescopes by Active Compensation." In Structures Technology for Large Radio and Radar Telescope Systems. The MIT Press, 2003. http://dx.doi.org/10.7551/mitpress/6523.003.0018.

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"Application of the NASA General Purpose Structural Analysis Program to Large Radio Telescopes." In Structures Technology for Large Radio and Radar Telescope Systems. The MIT Press, 2003. http://dx.doi.org/10.7551/mitpress/6523.003.0027.

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"The Nançay Radio Telescope." In Structures Technology for Large Radio and Radar Telescope Systems. The MIT Press, 2003. http://dx.doi.org/10.7551/mitpress/6523.003.0006.

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"Preface." In Structures Technology for Large Radio and Radar Telescope Systems. The MIT Press, 2003. http://dx.doi.org/10.7551/mitpress/6523.003.0001.

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"The Role of the Giant Steerable Telescope in Radio Astronomy." In Structures Technology for Large Radio and Radar Telescope Systems. The MIT Press, 2003. http://dx.doi.org/10.7551/mitpress/6523.003.0002.

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"The Design of a 300-ft Research Antenna." In Structures Technology for Large Radio and Radar Telescope Systems. The MIT Press, 2003. http://dx.doi.org/10.7551/mitpress/6523.003.0003.

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Conference papers on the topic "Radar telescopes"

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Clark, S. E., and L. F. Desandre. "Laser Radar Imaging with a Sparse Random Array Receiver." In Adaptive Optics for Large Telescopes. Optica Publishing Group, 1992. http://dx.doi.org/10.1364/aolt.1992.afa10.

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Over the last few years, there has been considerable interest1-4 in using multiple aperture receiver arrays in laser radar systems where low cost lightweight sensor systems of low power consumption and high angular resolution for tracking and imaging are required. As has been previously demonstrated2-4, the problem of determining the target phase from the measured phase which is corrupted by positional and reference wavefront errors can be overcome in an adaptive way prior to using the array for imaging.
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Cappellen, W. a., S. J. Wijnholds, and J. D. Bregman. "Sparse antenna array configurations in large aperture synthesis radio telescopes." In 2006 European Radar Conference. IEEE, 2006. http://dx.doi.org/10.1109/eurad.2006.280277.

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Kassim, Namir E., and William C. Erickson. "Meter- and decameter-wavelength array for astrophysics and solar radar." In Astronomical Telescopes & Instrumentation, edited by Thomas G. Phillips. SPIE, 1998. http://dx.doi.org/10.1117/12.317406.

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Pisanu, T., R. Concu, F. Gaudiomonte, et al. "SRT as a receiver in a bistatic radar space debris configuration." In SPIE Astronomical Telescopes + Instrumentation, edited by Helen J. Hall, Roberto Gilmozzi, and Heather K. Marshall. SPIE, 2016. http://dx.doi.org/10.1117/12.2231753.

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Zhao, Qi, Hongying Fan, Shaoyun Hu, Min Zhong, and Lü Baida. "Effect of optical aberration of telescopes to the laser radar." In 5th International Symposium on Advanced Optical Manufacturing and Testing Technologies, edited by Yudong Zhang, José Sasián, Libin Xiang, and Sandy To. SPIE, 2010. http://dx.doi.org/10.1117/12.867716.

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Konovalenko, Oleksandr O., and Vyacheslav V. Zakharenko. "Study of the space by low-frequency radio telescopes." In 2014 20th International Conference on Microwaves, Radar, and Wireless Communications (MIKON). IEEE, 2014. http://dx.doi.org/10.1109/mikon.2014.6899827.

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Pisanu, Tonino, Luca Schirru, Enrico Urru, and Paolo Maxia. "Status of the Sardinia Radio Telescope as a receiver of the BIRALET bi-static radar for space debris observations." In Ground-based and Airborne Telescopes VIII, edited by Heather K. Marshall, Jason Spyromilio, and Tomonori Usuda. SPIE, 2020. http://dx.doi.org/10.1117/12.2576249.

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Bondarenko, Yu, D. Marshalov, D. Vavilov, and Y. Medvedev. "International Radar Observations of Near-Earth Asteroids on Radio Telescopes of the Quasar VLBI Network." In Groud-Based Astronomy in Russia. 21st Century. Специальная астрофизическая обсерватория РАН, 2020. http://dx.doi.org/10.26119/978-5-6045062-0-2_2020_455.

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Johann, U. A., F. Safa, and P. M. Schwarzenberger. "Aladin: Mission and Instrument Concept for a European Space-borne CO2-Laser Doppler Wind Lidar." In Coherent Laser Radar. Optica Publishing Group, 1995. http://dx.doi.org/10.1364/clr.1995.mc2.

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The main features of the proposed instrument are a fixed nadir-oriented telescope with an oversized primary mirror and an array of off-axis secondary mirrors, addressing shot azimuth positions on a 30° nadir-angle cone. Step scanning is performed by a small focal plane stepper, avoiding lag-angle and torque compensation problems encountered in scanning telescope concepts. Hence, the concept is insensitive to misalignment and employs a minimum of internal alignment control at full scanning capability.
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Bianchi, G. "The new transmitting antenna for BIRALES." In Aeronautics and Astronautics. Materials Research Forum LLC, 2023. http://dx.doi.org/10.21741/9781644902813-104.

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Abstract. In the last decades the increasing Resident Space Objects (RSOs) population is fostering many Space Surveillance and Tracking (SST) initiatives, which are currently based on the use of ground sensors. These can be distinguished in optical, laser and radar and categorized in tracking and survey sensors. In particular, the survey radars allow to determine the orbit of both catalogued and uncatalogued objects. Italy contributes to the European SST (EUSST) activities with the BIstatic RAdar for LEo Survey (BIRALES), whose transmitter is the Radio Frequency Transmitter (TRF), located at t
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