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Extremely large-scale antenna arrays (ELAAs) have emerged as a pivotal technology for addressing the unprecedented performance demands of next-generation wireless communication systems. To enhance their practicality, we propose…

信号处理 · 电气工程与系统科学 2026-01-21 Zhengyu Wang , Tiebin Mi , Gui Zhou , Robert C. Qiu

This paper describes the system architecture of a newly constructed radio telescope - the Boolardy Engineering Test Array, which is a prototype of the Australian Square Kilometre Array Pathfinder telescope. Phased array feed technology is…

The ARIANNA collaboration completed the installation of the hexagonal radio array (HRA) in December 2014, serving as a pilot program for a planned high energy neutrino telescope located about 110 km south of McMurdo Station on the Ross Ice…

The workhorse instruments of the 8-10m class observatories have become their multi-object spectrographs (MOS), providing comprehensive follow-up to both ground-based and space-borne imaging. With the advent of deeper imaging surveys from,…

An extended aperture has the potential to greatly improve ultrasound imaging performance. This work extends the effective aperture size by coherently compounding the received radio frequency data from multiple transducers. A framework is…

Very long baseline interferometry at millimetre/submillimetre wavelengths (mmVLBI) offers the highest achievable spatial resolution at any wavelength in astronomy. The anticipated inclusion of ALMA as a phased array into a global VLBI…

天体物理仪器与方法 · 物理学 2014-07-02 R. P. J. Tilanus , T. P. Krichbaum , J. A. Zensus , A. Baudry , M. Bremer , H. Falcke , G. Giovannini , R. Laing , H. J. van Langevelde , W. Vlemmings , Z. Abraham , J. Afonso , I. Agudo , A. Alberdi , J. Alcolea , D. Altamirano , S. Asadi , K. Assaf , P. Augusto , A-K. Baczko , M. Boeck , T. Boller , M. Bondi , F. Boone , G. Bourda , R. Brajsa , J. Brand , S. Britzen , V. Bujarrabal , S. Cales , C. Casadio , V. Casasola , P. Castangia , J. Cernicharo , P. Charlot , L. Chemin , Y. Clenet , F. Colomer , F. Combes , J. Cordes , M. Coriat , N. Cross , F. D'Ammando , D. Dallacasa , J-F. Desmurs , R. Eatough , A. Eckart , D. Eisenacher , S. Etoka , M. Felix , R. Fender , M. Ferreira , E. Freeland , S. Frey , C. Fromm , L. Fuhrmann , K. Gabanyi , R. Galvan-Madrid , M. Giroletti , C. Goddi , J. Gomez , E. Gourgoulhon , M. Gray , I. di Gregorio , R. Greimel , N. Grosso , J. Guirado , K. Hada , A. Hanslmeier , C. Henkel , F. Herpin , P. Hess , J. Hodgson , D. Horns , E. Humphreys , B. Hutawarakorn Kramer , V. Ilyushin , V. Impellizzeri , V. Ivanov , M. Julião , M. Kadler , E. Kerins , P. Klaassen , K. van 't Klooster , E. Kording , M. Kozlov , M. Kramer , A. Kreikenbohm , O. Kurtanidze , J. Lazio , A. Leite , M. Leitzinger , J. Lepine , S. Levshakov , R. Lico , M. Lindqvist , E. Liuzzo , A. Lobanov , P. Lucas , K. Mannheim , J. Marcaide , S. Markoff , I. Martí-Vidal , C. Martins , N. Masetti , M. Massardi , K. Menten , H. Messias , S. Migliari , A. Mignano , J. Miller-Jones , D. Minniti , P. Molaro , S. Molina , A. Monteiro , L. Moscadelli , C. Mueller , A. Müller , S. Muller , F. Niederhofer , P. Odert , H. Olofsson , M. Orienti , R. Paladino , F. Panessa , Z. Paragi , T. Paumard , P. Pedrosa , M. Pérez-Torres , G. Perrin , M. Perucho , D. Porquet , I. Prandoni , S. Ransom , D. Reimers , M. Rejkuba , L. Rezzolla , A. Richards , E. Ros , A. Roy , A. Rushton , T. Savolainen , R. Schulz , M. Silva , G. Sivakoff , R. Soria-Ruiz , R. Soria , M. Spaans , R. Spencer , B. Stappers , G. Surcis , A. Tarchi , M. Temmer , M. Thompson , J. Torrelles , J. Truestedt , V. Tudose , T. Venturi , J. Verbiest , J. Vieira , P. Vielzeuf , F. Vincent , N. Wex , K. Wiik , T. Wiklind , J. Wilms , E. Zackrisson , H. Zechlin

The advent of Extremely Large Telescopes ELTs, ground-based optical or infrared observatories with primary mirrors exceeding 20 m heralds a transformative epoch in observational astronomy. This article examines the dawn of this new era and…

科普物理 · 物理学 2026-05-22 Priya Hasan

3GPP is finalising the first release of the 5G New Radio physical layer. To cope with the demanding 5G requirements on global connectivity and large throughput, Satellite Communications might be a valuable resource to extend and complement…

网络与互联网体系结构 · 计算机科学 2017-09-19 Alessandro Guidotti , Alessandro Vanelli-Coralli , Oltjon Kodheli , Giulio Colavolpe , Tommaso Foggi

The Auger Engineering Radio Array (AERA) complements the Pierre Auger Observatory with 150 radio-antenna stations measuring in the frequency range from 30 to 80 MHz. With an instrumented area of 17 km$^2$, the array constitutes the largest…

天体物理仪器与方法 · 物理学 2019-06-12 Tim Huege

Extremely large antenna array (ELAA) is a common feature of several key candidate technologies for sixth-generation mobile networks (6G), such as ultra-massive multiple-input-multiple-output (UM-MIMO), cell-free massive MIMO, reconfigurable…

信息论 · 计算机科学 2024-10-28 Mingyao Cui , Zidong Wu , Yu Lu , Xiuhong Wei , Linglong Dai

This paper introduces a novel beam tracking scheme for full-duplex ground user terminals aiming to transmit uplink and receive downlink from two low Earth orbit (LEO) satellites at the same time and same frequency. Our proposed technique…

信号处理 · 电气工程与系统科学 2024-11-15 Chaeyeon Kim , Joohyun Son , Daesik Hong , Ian P. Roberts

Digital radio arrays are widely used for the low-frequency radio astronomy as well as for detection of air-showers induced by high-energy cosmic rays and neutrinos. Since the radio emission from air-showers forms short broadband pulses with…

The World Space Observatory Project is a new space mission concept, grown out the needs of the Astronomical community to have access to the part of the electromagnetic spectrum where all known physics can be studied on all possible time…

This paper introduces a new instrument enabling a novel combination of Earth measuring techniques: direct observations with the radio astronomical instruments to satellites of the global navigation satellite systems. Inter-technique biases…

地球物理 · 物理学 2025-03-26 Lucia McCallum , David Schunck , Jamie McCallum , Tiege McCarthy

The light produced by parametric down-conversion shows strong spatial entanglement that leads to violations of EPR criteria for separability. Historically, such studies have been performed by scanning a single-element, single-photon…

The low-frequency sky below $\sim$15 MHz (20 m) is obscured by the Earth's ionosphere, the layer of charged particles above the neutral atmosphere. Single spacecraft have made measurements in this band, but cannot achieve high or even…

天体物理仪器与方法 · 物理学 2024-04-15 Mary Knapp , Lenny Paritsky , Ekaterina Kononov , Melodie M. Kao

The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that comprises millimeter- and submillimeter-wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating…

天体物理仪器与方法 · 物理学 2019-07-08 The Event Horizon Telescope Collaboration

A new generation of telescopes with mirror diameters of 20 m or more, called extremely large telescopes (ELTs) has the potential to provide unprecedented imaging and spectroscopy of exo-planetary systems, if the difficulties in achieving…

天体物理仪器与方法 · 物理学 2016-04-20 Richard A. Frazin

Antenna arrays are beginning to make important contributions to high energy astroparticle physics supported by recent progress in the radio technique for air showers. This article provides an update to my more extensive review published in…

天体物理仪器与方法 · 物理学 2019-05-17 Frank G. Schröder