The Square Kilometre Array: Paving the way for the new 21st century radio astronomy paradigm | Proceedings of Symposium 7 of JENAM 2010
Lingua: inglese
Editore: Springer, 2014
Serie: Libro 11 di 41 - Astrophysics and Space Science Proceedings
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The Square Kilometre Array: Paving the way for the new 21st century radio astronomy paradigm | Proceedings of Symposium 7 of JENAM 2010 | Domingos Barbosa (u. a.) | Taschenbuch | Astrophysics and Space Science Proceedings | x | Englisch | 2014 | Springer | EAN 9783642445323 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu.
Codice articolo 105432894
- Titolo
- The Square Kilometre Array: Paving the way for the new 21st century radio astronomy paradigm | Proceedings of Symposium 7 of JENAM 2010
- Autore
- Domingos Barbosa (u. a.)
- Editore
- Springer
- Anno di pubblicazione
- 2014
- Condizione
- Neu
- Rilegatura
- Taschenbuch
- Lingua
- inglese
- ISBN 10
- 3642445322
- ISBN 13
- 9783642445323
- Peso dell'articolo
- 207 grammi
- Dimensioni
- 235 x 155 x 8 mm
- Serie
- Libro 11 di 41: Astrophysics and Space Science Proceedings
- Cataloghi dei venditori
- Bücher
: The Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telescope over a wavelength range of several hundred to one, from decametric to microwave wavelengths. It will revolutionize the study of the most abundant element in the Universe, hydrogen, from the epoch of reionisation to the present-day, probing the onset formation period of the very first stars, will closely scan proto-planets and, through the precision timing of pulsars, will detect the distortions of space-time due to gravitational radiation. The SKA is a sensing network spanning 3000 km from its centre and with a collecting area of more than 1 square kilometre, using technologies of the 21st century. The SKA will make the study of a wide range of phenomena initially studied at other wavelengths possible at radio wavelengths, as well as opening a new discovery window on new phenomena at radio wavelengths.
Symposium 7 of the JENAM 2010 aimed at bringing these diverse opportunities to the attention of both theoretical and observational astronomers working at all wavelengths, including the potential for synergies with other facilities. The meeting highlighted the scientific potential of the SKA, discussed scientific priorities and their impact on the design of the SKA, explored the synergies between the SKA and other next-generation astronomical facilities in different wavelength domains such as the ALMA, ELTs, LSST, JWST, GRE, IXO, Gaia and Euclid, and high-energy facilities (Auger), explored the cyberinfrastructure that may become available for the distribution and distributed analysis of SKA data.
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Dalla quarta di copertina
The Square Kilometre Array (SKA) will provide more than one order of magnitude improvement in sensitivity compared with any existing radio telescope over a wavelength range of several hundred to one, from decametric to microwave wavelengths. It will revolutionize the study of the most abundant element in the Universe, hydrogen, from the epoch of reionisation to the present-day, probing the onset formation period of the very first stars, will closely scan proto-planets and, through the precision timing of pulsars, will detect the distortions of space-time due to gravitational radiation. The SKA is a sensing network spanning 3000 km from its centre and with a collecting area of more than 1 square kilometre, using technologies of the 21st century. The SKA will make the study of a wide range of phenomena initially studied at other wavelengths possible at radio wavelengths, as well as opening a new discovery window on new phenomena at radio wavelengths.
Symposium 7 of the JENAM 2010 aimed at bringing these diverse opportunities to the attention of both theoretical and observational astronomers working at all wavelengths, including the potential for synergies with other facilities. The meeting
· highlighted the scientific potential of the SKA
· discussed scientific priorities and their impact on the design of the SKA
· explored the synergies between the SKA and other next-generation astronomical facilities in different wavelength domains such as the ALMA, ELTs, LSST, JWST, GRE, IXO, Gaia and Euclid, and high-energy facilities (Auger)
· explored the cyber infrastructure that may become available for the distribution and distributed analysis of SKA data
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