Gotowe bibliografie tematyczne / Radiophysics Laboratory

Gotowa bibliografia na temat „Radiophysics Laboratory”

Autor: Grafiati
Data publikacji: 25 lipca 2024

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Artykuły w czasopismach na temat "Radiophysics Laboratory"

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Pereslegin, V. S., N. G. Kozhelupova, D. V. Ivonin i S. A. Sviridov. "TO THE 95th ANNIVERSARY OF THE BIRTH OF SERGEI VLADIMIROVICH PERESLEGIN (01.10.1928–31.07.2023)". Journal of Oceanological Research 51, nr 3 (9.11.2023): 267–80. http://dx.doi.org/10.29006/1564-2291.jor-2023.51(3).18.

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The article is dedicated to the 95th anniversary of the birth of Sergei Vladimirovich Pereslegin – radiophysicist – oceanologist, Candidate of Technical Sciences (1977), Doctor of Physical and Mathematical Sciences (2000), Chief Researcher of the Laboratory of Nonlinear Wave Processes of the Shirshov Institute of Oceanology of RAS. Dr. Pereslegin is the creator of a new direction at the Institute of Oceanology at the intersection of theoretical and experimental radiophysics and oceanology – the development of radar methods for ocean research. Sergei Pereslegin left us on July 31, 2023, leaving behind many ideas, projects and inventions.
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Minnett, H. "The Radiophysics Laboratory at the University of Sydney." Historical Records of Australian Science 12, nr 4 (1998): 419. http://dx.doi.org/10.1071/hr9991240419.

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Davies, Jenny. "Resource Sharing in the CSIRO Division of Radiophysics Library". International Astronomical Union Colloquium 110 (1989): 196–97. http://dx.doi.org/10.1017/s0252921100003390.

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The CSIRO Divison of Radiophysics was established as the CSIRO Radiophysics Laboratory in 1939 to conduct radar research. After World War 2 experimental radar instruments were applied to the developing field of radio astronomy. Current areas of research for the Division, which is host to the new Australia Telescope (AT), are radio astronomy, antenna technology, satellite communications, signal processing and microelectronics.The AT has three observatory sites, all in New South Wales: six antennas near Narrabri, over 500 km from Sydney, the 27-year-old Parkes observatory, 350 km from Sydney, and one antenna near Coonabarabran, between Parkes and Narrabri. Most staff are located at the Division’s headquarters in Sydney, where the main library is also located, and small collections are maintained at the Parkes and Narrabri observatories.
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Gubsky, Dmitry, Irina Ivanova i Anatoly Kleschenkov. "Developing of computer models of modern measuring instruments for a remote virtual laboratory". ITM Web of Conferences 30 (2019): 11001. http://dx.doi.org/10.1051/itmconf/20193011001.

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The study introduces the approach of creating a virtual laboratory for performing laboratory works with remote access. The proposed virtual lab can be used for distance learning and is an extension of the functionality of the previously created virtual workshop. This virtual laboratory with remote access is an alternative to laboratory works performed with real experimental equipment and provides an opportunity to gain skills in operation with measuring microwave equipment without giving classes in educational laboratories. The results of testing virtual lab works with remote access in educational radiophysics laboratories are presented.
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Robertson, Peter, Glen Cozens, Wayne Orchiston, Bruce Slee i Harry Wendt. "Early Australian Optical and Radio Observations of Centaurus A". Publications of the Astronomical Society of Australia 27, nr 4 (2010): 402–30. http://dx.doi.org/10.1071/as09071.

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AbstractThe discovery of the radio source Centaurus A and its optical counterpart NGC 5128 were important landmarks in the history of Australian astronomy. NGC 5128 was first observed in August 1826 by James Dunlop during a survey of southern objects at the Parramatta Observatory, west of the settlement at Sydney Cove. The observatory had been founded a few years earlier by Thomas Brisbane, the new governor of the British colony of New South Wales. Just over 120 years later, John Bolton, Gordon Stanley and Bruce Slee discovered the radio source Centaurus A at the Dover Heights field station in Sydney, operated by CSIRO's Radiophysics Laboratory (the forerunner to CSIRO Astronomy and Space Sciences). This paper will describe this early historical work and summarize further studies of Centaurus A by other Radiophysics groups up to 1960.
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Sullivan, Woodruff T. "Some Highlights of Interferometry in early Radio Astronomy". International Astronomical Union Colloquium 131 (1991): 132–49. http://dx.doi.org/10.1017/s025292110001321x.

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AbstractTwo important episodes in the early development of interferometry in radio astronomy are traced in detail. The first is the use of the sea-cliff interferometer at the Radiophysics Laboratory in Sydney, first by Pawsey for solar observations and later by Bolton for radio star surveys. The second is the development of the Michelson interferometer and the phase switch by Ryle in Cambridge. This also was employed for important observations of the sun and radio stars.
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Thomas, Bruce MacA, i Brian J. Robinson. "Harry Clive Minnett 1917 - 2003". Historical Records of Australian Science 16, nr 2 (2005): 199. http://dx.doi.org/10.1071/hr05011.

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In April 1940, Harry Minnett joined the Council for Scientific and Industrial Research (CSIR, renamed CSIRO in May 1949), soon after the establishment of the Radiophysics Laboratory for research into advanced radar systems. He remained with the organization until his retirement in 1981. Harry's ability as a meticulous engineer with a thorough understanding of the related underlying scientific principles was recognized by his being appointed to leading roles in a number of significant projects. These were to have a long-term impact on Australian science and technology. Among the most important was his role in guiding the design of the Parkes 64-m radio telescope to successful completion, and the establishment of a world-recognized research group on antenna design to support radio telescope design and upgrades. He also had considerable impact on the construction of the 3.9-m Anglo-Australian optical telescope at Siding Spring Mountain, New South Wales, and the 'Interscan' aircraft Microwave Landing System being developed by the Division of Radiophysics in collaboration with industry. He was Chief of the Division from 1978 to 1981. Harry died on 20 December 2003 after a short period of illness.
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Koribalski, Bärbel. "Millimetre-wave Astronomy: Abstracts from a One-day Workshop held on 19 April 1995 at the Australia Telescope National Facility". Publications of the Astronomical Society of Australia 13, nr 2 (maj 1996): 179–81. http://dx.doi.org/10.1017/s1323358000020750.

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SummaryA Millimetre-wave Astronomy Workshop was held at the CSIRO Radiophysics Laboratory in Marsfield, Sydney, on 19 April 1995. The workshop, sponsored by the Australia Telescope National Facility (ATNF), was a meeting of mm-wave specialists as well as astronomers and students interested in the field, and attracted about 80 participants from 13 institutions. The program consisted of 23 oral contributions (5–45 min) followed by lively discussions. Abstracts of most of the contributions are presented here, arranged by groups dealing with subjects such as ‘A Basic Introduction’, ‘Astronomy in the mm-range with Mopra’ and ‘Projects: Galactic and Extragalactic 3 mm-wave astronomy’.
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Koribalski, Bärbel. "Dark Matter: Abstracts from a Two-day Workshop held in February 1994 by the Australia Telescope National Facility". Publications of the Astronomical Society of Australia 12, nr 1 (kwiecień 1995): 117–38. http://dx.doi.org/10.1017/s1323358000020142.

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Summary A Dark Matter Workshop was held at the CSIRO Radiophysics Laboratory in Marsfield, Sydney, on 24–25 February 1994. The workshop, sponsored by the Australia Telescope National Facility (ATNF), was a meeting of dark matter (DM) specialists as well as astronomers interested in the field, and attracted about 80 participants from nine institutions. The program consisted of 22 oral contributions (15–45 minutes), followed by lively discussions, as well as podium discussions at the end of each day. Abstracts of most of the contributions are presented here, arranged by subject groups which range from ‘Gravitational Lensing and DM in Clusters’, ‘DM in Elliptical Galaxies’, ‘The Nature of DM’, and ‘The Shapes of Dark Halos’ to ‘Alternatives to DM’.
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Ekers, RD. "John Bolton's Variable-baseline Interferometer and the Structure of Radio Galaxies". Australian Journal of Physics 47, nr 5 (1994): 569. http://dx.doi.org/10.1071/ph940569.

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John Bolton was a pioneer in the study of extragalactic radio sources, first at the CSIRO Radiophysics Laboratory and then at the California Institute of Technology's Owens Valley interferometer. I became his Ph.D. student after he returned to the Parkes Observatory from California, and I helped in the construction of the Parkes interferometer. This consisted of a 60-ft dish connected to the existing 210-ft dish by a flexible cable trailing from the 60-footer. The interferometer was used to observe continuously at 467 and 1401 MHz while the 60-ft dish was pulled along a track. The wisdom of the design is illustrated by comparing observations of Pictor A made at Parkes and at Owens Valley.
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Książki na temat "Radiophysics Laboratory"

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G, Bowen E. Textbook of Radar: A Collective Work by the Staff of the Radiophysics Laboratory C. S. I. R. o Australia. Cambridge University Press, 2016.

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Abrahamyan, Tigran, i Henrik Parsamyan. Automation of a Scientific Experiment in the LabVIEW environment. YSU press, 2023. http://dx.doi.org/10.46991/ysuph/9785808426139.

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The textbook “Automation of a Scientific Experiment in the LabVIEW environment” is devoted to a series of descriptions of laboratory work, which, in accordance with the curriculum of the Faculty of Radiophysics, are intended as a part of the laboratory classes of the courses “Automation of a scientific experiment” and “Practice of automation of a scientific experiment”. The tools of the LabVIEW software environment and the operating features of the packages used in laboratory work are presented. Descriptions of laboratory work are provided with the equipment for conducting them and the step-bystep description of the experiment itself. The manual presents the data import and processing in the computer. The characteristics of data output from a computer, and the automation of the process of controlling equipment and conducting experiments using the LabVIEW software environment are introduced.
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Części książek na temat "Radiophysics Laboratory"

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Orchiston, Wayne, Peter Robertson i Woodruff T. Sullivan III. "Where did it all Lead?" W Golden Years of Australian Radio Astronomy, 205–49. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-319-91843-3_5.

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AbstractAt the end of World War II it would have been impossible to have foreseen the rapid growth of radio astronomy at the Radiophysics Lab. In the space of about five years radio astronomy not only became the dominant research program, but the RP group was easily the largest and most generously funded in the world. The two main rivals to Radiophysics were the Jodrell Bank group at the University of Manchester led by Bernard Lovell and the Cavendish Laboratory at Cambridge University led by Martin Ryle. However, both these English groups were relatively small sections within their University’s physics departments and, with the post-war austerity in England, both groups operated on shoestring budgets. Around 1950, the combined budgets of the Jodrell Bank and Cambridge groups were only a small fraction of the RP radio astronomy budget (see e.g. Robertson, 1992: 131; Sullivan, 2009: 153).
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Goss, W. M. "Wartime Research by Ruby Payne-Scott at the Radiophysics Laboratory". W Astronomers' Universe, 67–86. Berlin, Heidelberg: Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-35752-7_5.

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Goss, W. M. "1949–1951: Radio Astronomy Blossoms as a Field, but Ruby Must Resign from the Radiophysics Laboratory". W Astronomers' Universe, 167–99. Berlin, Heidelberg: Springer Berlin Heidelberg, 2013. http://dx.doi.org/10.1007/978-3-642-35752-7_10.

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Orchiston, Wayne, Peter Robertson i Woodruff T. Sullivan III. "Expanding Horizons – The Milky Way and Beyond". W Golden Years of Australian Radio Astronomy, 149–204. Cham: Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-319-91843-3_4.

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AbstractNon-solar research at the Radiophysics Laboratory (RP) was launched in September 1946 when Joe Pawsey (1908–1962) tried unsuccessfully to observe the enigmatic ‘radio star’ in Cygnus that the British team of Stanley Hey (1909–2000, Fig. 4.1), John Parsons and James Phillips (1946) had announced in the 17 August issue of Nature. Two months later, John Bolton (1922–1993; Fig. 4.2) and research assistant Bruce Slee (1924–2016) were at Dover Heights trying to observe the Sun at 60 MHz. When it insisted on remaining inactive they decided to use their 2-Yagi antenna in sea interferometer mode to search for radio emission from other types of objects. Neither had a background in astronomy, and their astronomical knowledge and resources were virtually non-existent. Bolton (1982: 349) later described how they used the Russell, Duggan and Stewart book Astronomy to “… hazard guesses as to which types of objects might emit copious amounts of radio emission …” and Norton’s Star Atlas “… to find the position of the brightest candidate in each class.”
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