The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT
Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new ob...
Ausführliche Beschreibung
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| Autor*in: |
Konovalenko, A. [verfasserIn] Sodin, L. [verfasserIn] Zakharenko, V. [verfasserIn] Zarka, P. [verfasserIn] Ulyanov, O. [verfasserIn] Sidorchuk, M. [verfasserIn] Stepkin, S. [verfasserIn] Tokarsky, P. [verfasserIn] Melnik, V. [verfasserIn] Kalinichenko, N. [verfasserIn] Stanislavsky, A. [verfasserIn] Koliadin, V. [verfasserIn] Shepelev, V. [verfasserIn] Dorovskyy, V. [verfasserIn] Ryabov, V. [verfasserIn] Koval, A. [verfasserIn] Bubnov, I. [verfasserIn] Yerin, S. [verfasserIn] Gridin, A. [verfasserIn] Kulishenko, V. [verfasserIn] Reznichenko, A. [verfasserIn] Bortsov, V. [verfasserIn] Lisachenko, V. [verfasserIn] Reznik, A. [verfasserIn] Kvasov, G. [verfasserIn] Mukha, D. [verfasserIn] Litvinenko, G. [verfasserIn] Khristenko, A. [verfasserIn] Shevchenko, V. V. [verfasserIn] Shevchenko, V. A. [verfasserIn] Belov, A. [verfasserIn] Rudavin, E. [verfasserIn] Vasylieva, I. [verfasserIn] Miroshnichenko, A. [verfasserIn] Vasilenko, N. [verfasserIn] Olyak, M. [verfasserIn] Mylostna, K. [verfasserIn] Skoryk, A. [verfasserIn] Shevtsova, A. [verfasserIn] Plakhov, M. [verfasserIn] Kravtsov, I. [verfasserIn] Volvach, Y. [verfasserIn] Lytvinenko, O. [verfasserIn] Shevchuk, N. [verfasserIn] Zhouk, I. [verfasserIn] Bovkun, V. [verfasserIn] Antonov, A. [verfasserIn] Vavriv, D. [verfasserIn] Vinogradov, V. [verfasserIn] Kozhin, R. [verfasserIn] Kravtsov, A. [verfasserIn] Bulakh, E. [verfasserIn] Kuzin, A. [verfasserIn] Vasilyev, A. [verfasserIn] Brazhenko, A. [verfasserIn] Vashchishin, R. [verfasserIn] Pylaev, O. [verfasserIn] Koshovyy, V. [verfasserIn] Lozinsky, A. [verfasserIn] Ivantyshin, O. [verfasserIn] Rucker, H. O. [verfasserIn] Panchenko, M. [verfasserIn] Fischer, G. [verfasserIn] Lecacheux, A. [verfasserIn] Denis, L. [verfasserIn] Coffre, A. [verfasserIn] Grieβmeier, J.-M. [verfasserIn] Tagger, M. [verfasserIn] Girard, J. [verfasserIn] Charrier, D. [verfasserIn] Briand, C. [verfasserIn] Mann, G. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Experimental astronomy - Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989, 42(2016), 1 vom: 28. Apr., Seite 11-48 |
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| Übergeordnetes Werk: |
volume:42 ; year:2016 ; number:1 ; day:28 ; month:04 ; pages:11-48 |
| Links: |
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| DOI / URN: |
10.1007/s10686-016-9498-x |
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| Katalog-ID: |
SPR012459429 |
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| 024 | 7 | |a 10.1007/s10686-016-9498-x |2 doi | |
| 035 | |a (DE-627)SPR012459429 | ||
| 035 | |a (SPR)s10686-016-9498-x-e | ||
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| 082 | 0 | 4 | |a 520 |q ASE |
| 084 | |a 39.00 |2 bkl | ||
| 100 | 1 | |a Konovalenko, A. |e verfasserin |4 aut | |
| 245 | 1 | 4 | |a The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT |
| 264 | 1 | |c 2016 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
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| 520 | |a Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. | ||
| 650 | 4 | |a Radio astronomy |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Radio telescope |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Antenna arrays |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Space research |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Sodin, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Zakharenko, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Zarka, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Ulyanov, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Sidorchuk, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Stepkin, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Tokarsky, P. |e verfasserin |4 aut | |
| 700 | 1 | |a Melnik, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Kalinichenko, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Stanislavsky, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Koliadin, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Shepelev, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Dorovskyy, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Ryabov, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Koval, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Bubnov, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Yerin, S. |e verfasserin |4 aut | |
| 700 | 1 | |a Gridin, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Kulishenko, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Reznichenko, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Bortsov, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Lisachenko, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Reznik, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Kvasov, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Mukha, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Litvinenko, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Khristenko, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Shevchenko, V. V. |e verfasserin |4 aut | |
| 700 | 1 | |a Shevchenko, V. A. |e verfasserin |4 aut | |
| 700 | 1 | |a Belov, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Rudavin, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Vasylieva, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Miroshnichenko, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vasilenko, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Olyak, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Mylostna, K. |e verfasserin |4 aut | |
| 700 | 1 | |a Skoryk, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Shevtsova, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Plakhov, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Kravtsov, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Volvach, Y. |e verfasserin |4 aut | |
| 700 | 1 | |a Lytvinenko, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Shevchuk, N. |e verfasserin |4 aut | |
| 700 | 1 | |a Zhouk, I. |e verfasserin |4 aut | |
| 700 | 1 | |a Bovkun, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Antonov, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vavriv, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Vinogradov, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Kozhin, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Kravtsov, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Bulakh, E. |e verfasserin |4 aut | |
| 700 | 1 | |a Kuzin, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vasilyev, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Brazhenko, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Vashchishin, R. |e verfasserin |4 aut | |
| 700 | 1 | |a Pylaev, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Koshovyy, V. |e verfasserin |4 aut | |
| 700 | 1 | |a Lozinsky, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Ivantyshin, O. |e verfasserin |4 aut | |
| 700 | 1 | |a Rucker, H. O. |e verfasserin |4 aut | |
| 700 | 1 | |a Panchenko, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Fischer, G. |e verfasserin |4 aut | |
| 700 | 1 | |a Lecacheux, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Denis, L. |e verfasserin |4 aut | |
| 700 | 1 | |a Coffre, A. |e verfasserin |4 aut | |
| 700 | 1 | |a Grieβmeier, J.-M. |e verfasserin |4 aut | |
| 700 | 1 | |a Tagger, M. |e verfasserin |4 aut | |
| 700 | 1 | |a Girard, J. |e verfasserin |4 aut | |
| 700 | 1 | |a Charrier, D. |e verfasserin |4 aut | |
| 700 | 1 | |a Briand, C. |e verfasserin |4 aut | |
| 700 | 1 | |a Mann, G. |e verfasserin |4 aut | |
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10.1007/s10686-016-9498-x doi (DE-627)SPR012459429 (SPR)s10686-016-9498-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.00 bkl Konovalenko, A. verfasserin aut The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. Radio astronomy (dpeaa)DE-He213 Radio telescope (dpeaa)DE-He213 Antenna arrays (dpeaa)DE-He213 Space research (dpeaa)DE-He213 Sodin, L. verfasserin aut Zakharenko, V. verfasserin aut Zarka, P. verfasserin aut Ulyanov, O. verfasserin aut Sidorchuk, M. verfasserin aut Stepkin, S. verfasserin aut Tokarsky, P. verfasserin aut Melnik, V. verfasserin aut Kalinichenko, N. verfasserin aut Stanislavsky, A. verfasserin aut Koliadin, V. verfasserin aut Shepelev, V. verfasserin aut Dorovskyy, V. verfasserin aut Ryabov, V. verfasserin aut Koval, A. verfasserin aut Bubnov, I. verfasserin aut Yerin, S. verfasserin aut Gridin, A. verfasserin aut Kulishenko, V. verfasserin aut Reznichenko, A. verfasserin aut Bortsov, V. verfasserin aut Lisachenko, V. verfasserin aut Reznik, A. verfasserin aut Kvasov, G. verfasserin aut Mukha, D. verfasserin aut Litvinenko, G. verfasserin aut Khristenko, A. verfasserin aut Shevchenko, V. V. verfasserin aut Shevchenko, V. A. verfasserin aut Belov, A. verfasserin aut Rudavin, E. verfasserin aut Vasylieva, I. verfasserin aut Miroshnichenko, A. verfasserin aut Vasilenko, N. verfasserin aut Olyak, M. verfasserin aut Mylostna, K. verfasserin aut Skoryk, A. verfasserin aut Shevtsova, A. verfasserin aut Plakhov, M. verfasserin aut Kravtsov, I. verfasserin aut Volvach, Y. verfasserin aut Lytvinenko, O. verfasserin aut Shevchuk, N. verfasserin aut Zhouk, I. verfasserin aut Bovkun, V. verfasserin aut Antonov, A. verfasserin aut Vavriv, D. verfasserin aut Vinogradov, V. verfasserin aut Kozhin, R. verfasserin aut Kravtsov, A. verfasserin aut Bulakh, E. verfasserin aut Kuzin, A. verfasserin aut Vasilyev, A. verfasserin aut Brazhenko, A. verfasserin aut Vashchishin, R. verfasserin aut Pylaev, O. verfasserin aut Koshovyy, V. verfasserin aut Lozinsky, A. verfasserin aut Ivantyshin, O. verfasserin aut Rucker, H. O. verfasserin aut Panchenko, M. verfasserin aut Fischer, G. verfasserin aut Lecacheux, A. verfasserin aut Denis, L. verfasserin aut Coffre, A. verfasserin aut Grieβmeier, J.-M. verfasserin aut Tagger, M. verfasserin aut Girard, J. verfasserin aut Charrier, D. verfasserin aut Briand, C. verfasserin aut Mann, G. verfasserin aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 42(2016), 1 vom: 28. Apr., Seite 11-48 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:42 year:2016 number:1 day:28 month:04 pages:11-48 https://dx.doi.org/10.1007/s10686-016-9498-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 42 2016 1 28 04 11-48 |
| spelling |
10.1007/s10686-016-9498-x doi (DE-627)SPR012459429 (SPR)s10686-016-9498-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.00 bkl Konovalenko, A. verfasserin aut The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. Radio astronomy (dpeaa)DE-He213 Radio telescope (dpeaa)DE-He213 Antenna arrays (dpeaa)DE-He213 Space research (dpeaa)DE-He213 Sodin, L. verfasserin aut Zakharenko, V. verfasserin aut Zarka, P. verfasserin aut Ulyanov, O. verfasserin aut Sidorchuk, M. verfasserin aut Stepkin, S. verfasserin aut Tokarsky, P. verfasserin aut Melnik, V. verfasserin aut Kalinichenko, N. verfasserin aut Stanislavsky, A. verfasserin aut Koliadin, V. verfasserin aut Shepelev, V. verfasserin aut Dorovskyy, V. verfasserin aut Ryabov, V. verfasserin aut Koval, A. verfasserin aut Bubnov, I. verfasserin aut Yerin, S. verfasserin aut Gridin, A. verfasserin aut Kulishenko, V. verfasserin aut Reznichenko, A. verfasserin aut Bortsov, V. verfasserin aut Lisachenko, V. verfasserin aut Reznik, A. verfasserin aut Kvasov, G. verfasserin aut Mukha, D. verfasserin aut Litvinenko, G. verfasserin aut Khristenko, A. verfasserin aut Shevchenko, V. V. verfasserin aut Shevchenko, V. A. verfasserin aut Belov, A. verfasserin aut Rudavin, E. verfasserin aut Vasylieva, I. verfasserin aut Miroshnichenko, A. verfasserin aut Vasilenko, N. verfasserin aut Olyak, M. verfasserin aut Mylostna, K. verfasserin aut Skoryk, A. verfasserin aut Shevtsova, A. verfasserin aut Plakhov, M. verfasserin aut Kravtsov, I. verfasserin aut Volvach, Y. verfasserin aut Lytvinenko, O. verfasserin aut Shevchuk, N. verfasserin aut Zhouk, I. verfasserin aut Bovkun, V. verfasserin aut Antonov, A. verfasserin aut Vavriv, D. verfasserin aut Vinogradov, V. verfasserin aut Kozhin, R. verfasserin aut Kravtsov, A. verfasserin aut Bulakh, E. verfasserin aut Kuzin, A. verfasserin aut Vasilyev, A. verfasserin aut Brazhenko, A. verfasserin aut Vashchishin, R. verfasserin aut Pylaev, O. verfasserin aut Koshovyy, V. verfasserin aut Lozinsky, A. verfasserin aut Ivantyshin, O. verfasserin aut Rucker, H. O. verfasserin aut Panchenko, M. verfasserin aut Fischer, G. verfasserin aut Lecacheux, A. verfasserin aut Denis, L. verfasserin aut Coffre, A. verfasserin aut Grieβmeier, J.-M. verfasserin aut Tagger, M. verfasserin aut Girard, J. verfasserin aut Charrier, D. verfasserin aut Briand, C. verfasserin aut Mann, G. verfasserin aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 42(2016), 1 vom: 28. Apr., Seite 11-48 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:42 year:2016 number:1 day:28 month:04 pages:11-48 https://dx.doi.org/10.1007/s10686-016-9498-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 42 2016 1 28 04 11-48 |
| allfields_unstemmed |
10.1007/s10686-016-9498-x doi (DE-627)SPR012459429 (SPR)s10686-016-9498-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.00 bkl Konovalenko, A. verfasserin aut The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. Radio astronomy (dpeaa)DE-He213 Radio telescope (dpeaa)DE-He213 Antenna arrays (dpeaa)DE-He213 Space research (dpeaa)DE-He213 Sodin, L. verfasserin aut Zakharenko, V. verfasserin aut Zarka, P. verfasserin aut Ulyanov, O. verfasserin aut Sidorchuk, M. verfasserin aut Stepkin, S. verfasserin aut Tokarsky, P. verfasserin aut Melnik, V. verfasserin aut Kalinichenko, N. verfasserin aut Stanislavsky, A. verfasserin aut Koliadin, V. verfasserin aut Shepelev, V. verfasserin aut Dorovskyy, V. verfasserin aut Ryabov, V. verfasserin aut Koval, A. verfasserin aut Bubnov, I. verfasserin aut Yerin, S. verfasserin aut Gridin, A. verfasserin aut Kulishenko, V. verfasserin aut Reznichenko, A. verfasserin aut Bortsov, V. verfasserin aut Lisachenko, V. verfasserin aut Reznik, A. verfasserin aut Kvasov, G. verfasserin aut Mukha, D. verfasserin aut Litvinenko, G. verfasserin aut Khristenko, A. verfasserin aut Shevchenko, V. V. verfasserin aut Shevchenko, V. A. verfasserin aut Belov, A. verfasserin aut Rudavin, E. verfasserin aut Vasylieva, I. verfasserin aut Miroshnichenko, A. verfasserin aut Vasilenko, N. verfasserin aut Olyak, M. verfasserin aut Mylostna, K. verfasserin aut Skoryk, A. verfasserin aut Shevtsova, A. verfasserin aut Plakhov, M. verfasserin aut Kravtsov, I. verfasserin aut Volvach, Y. verfasserin aut Lytvinenko, O. verfasserin aut Shevchuk, N. verfasserin aut Zhouk, I. verfasserin aut Bovkun, V. verfasserin aut Antonov, A. verfasserin aut Vavriv, D. verfasserin aut Vinogradov, V. verfasserin aut Kozhin, R. verfasserin aut Kravtsov, A. verfasserin aut Bulakh, E. verfasserin aut Kuzin, A. verfasserin aut Vasilyev, A. verfasserin aut Brazhenko, A. verfasserin aut Vashchishin, R. verfasserin aut Pylaev, O. verfasserin aut Koshovyy, V. verfasserin aut Lozinsky, A. verfasserin aut Ivantyshin, O. verfasserin aut Rucker, H. O. verfasserin aut Panchenko, M. verfasserin aut Fischer, G. verfasserin aut Lecacheux, A. verfasserin aut Denis, L. verfasserin aut Coffre, A. verfasserin aut Grieβmeier, J.-M. verfasserin aut Tagger, M. verfasserin aut Girard, J. verfasserin aut Charrier, D. verfasserin aut Briand, C. verfasserin aut Mann, G. verfasserin aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 42(2016), 1 vom: 28. Apr., Seite 11-48 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:42 year:2016 number:1 day:28 month:04 pages:11-48 https://dx.doi.org/10.1007/s10686-016-9498-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 42 2016 1 28 04 11-48 |
| allfieldsGer |
10.1007/s10686-016-9498-x doi (DE-627)SPR012459429 (SPR)s10686-016-9498-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.00 bkl Konovalenko, A. verfasserin aut The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. Radio astronomy (dpeaa)DE-He213 Radio telescope (dpeaa)DE-He213 Antenna arrays (dpeaa)DE-He213 Space research (dpeaa)DE-He213 Sodin, L. verfasserin aut Zakharenko, V. verfasserin aut Zarka, P. verfasserin aut Ulyanov, O. verfasserin aut Sidorchuk, M. verfasserin aut Stepkin, S. verfasserin aut Tokarsky, P. verfasserin aut Melnik, V. verfasserin aut Kalinichenko, N. verfasserin aut Stanislavsky, A. verfasserin aut Koliadin, V. verfasserin aut Shepelev, V. verfasserin aut Dorovskyy, V. verfasserin aut Ryabov, V. verfasserin aut Koval, A. verfasserin aut Bubnov, I. verfasserin aut Yerin, S. verfasserin aut Gridin, A. verfasserin aut Kulishenko, V. verfasserin aut Reznichenko, A. verfasserin aut Bortsov, V. verfasserin aut Lisachenko, V. verfasserin aut Reznik, A. verfasserin aut Kvasov, G. verfasserin aut Mukha, D. verfasserin aut Litvinenko, G. verfasserin aut Khristenko, A. verfasserin aut Shevchenko, V. V. verfasserin aut Shevchenko, V. A. verfasserin aut Belov, A. verfasserin aut Rudavin, E. verfasserin aut Vasylieva, I. verfasserin aut Miroshnichenko, A. verfasserin aut Vasilenko, N. verfasserin aut Olyak, M. verfasserin aut Mylostna, K. verfasserin aut Skoryk, A. verfasserin aut Shevtsova, A. verfasserin aut Plakhov, M. verfasserin aut Kravtsov, I. verfasserin aut Volvach, Y. verfasserin aut Lytvinenko, O. verfasserin aut Shevchuk, N. verfasserin aut Zhouk, I. verfasserin aut Bovkun, V. verfasserin aut Antonov, A. verfasserin aut Vavriv, D. verfasserin aut Vinogradov, V. verfasserin aut Kozhin, R. verfasserin aut Kravtsov, A. verfasserin aut Bulakh, E. verfasserin aut Kuzin, A. verfasserin aut Vasilyev, A. verfasserin aut Brazhenko, A. verfasserin aut Vashchishin, R. verfasserin aut Pylaev, O. verfasserin aut Koshovyy, V. verfasserin aut Lozinsky, A. verfasserin aut Ivantyshin, O. verfasserin aut Rucker, H. O. verfasserin aut Panchenko, M. verfasserin aut Fischer, G. verfasserin aut Lecacheux, A. verfasserin aut Denis, L. verfasserin aut Coffre, A. verfasserin aut Grieβmeier, J.-M. verfasserin aut Tagger, M. verfasserin aut Girard, J. verfasserin aut Charrier, D. verfasserin aut Briand, C. verfasserin aut Mann, G. verfasserin aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 42(2016), 1 vom: 28. Apr., Seite 11-48 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:42 year:2016 number:1 day:28 month:04 pages:11-48 https://dx.doi.org/10.1007/s10686-016-9498-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 42 2016 1 28 04 11-48 |
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10.1007/s10686-016-9498-x doi (DE-627)SPR012459429 (SPR)s10686-016-9498-x-e DE-627 ger DE-627 rakwb eng 520 ASE 39.00 bkl Konovalenko, A. verfasserin aut The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT 2016 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. Radio astronomy (dpeaa)DE-He213 Radio telescope (dpeaa)DE-He213 Antenna arrays (dpeaa)DE-He213 Space research (dpeaa)DE-He213 Sodin, L. verfasserin aut Zakharenko, V. verfasserin aut Zarka, P. verfasserin aut Ulyanov, O. verfasserin aut Sidorchuk, M. verfasserin aut Stepkin, S. verfasserin aut Tokarsky, P. verfasserin aut Melnik, V. verfasserin aut Kalinichenko, N. verfasserin aut Stanislavsky, A. verfasserin aut Koliadin, V. verfasserin aut Shepelev, V. verfasserin aut Dorovskyy, V. verfasserin aut Ryabov, V. verfasserin aut Koval, A. verfasserin aut Bubnov, I. verfasserin aut Yerin, S. verfasserin aut Gridin, A. verfasserin aut Kulishenko, V. verfasserin aut Reznichenko, A. verfasserin aut Bortsov, V. verfasserin aut Lisachenko, V. verfasserin aut Reznik, A. verfasserin aut Kvasov, G. verfasserin aut Mukha, D. verfasserin aut Litvinenko, G. verfasserin aut Khristenko, A. verfasserin aut Shevchenko, V. V. verfasserin aut Shevchenko, V. A. verfasserin aut Belov, A. verfasserin aut Rudavin, E. verfasserin aut Vasylieva, I. verfasserin aut Miroshnichenko, A. verfasserin aut Vasilenko, N. verfasserin aut Olyak, M. verfasserin aut Mylostna, K. verfasserin aut Skoryk, A. verfasserin aut Shevtsova, A. verfasserin aut Plakhov, M. verfasserin aut Kravtsov, I. verfasserin aut Volvach, Y. verfasserin aut Lytvinenko, O. verfasserin aut Shevchuk, N. verfasserin aut Zhouk, I. verfasserin aut Bovkun, V. verfasserin aut Antonov, A. verfasserin aut Vavriv, D. verfasserin aut Vinogradov, V. verfasserin aut Kozhin, R. verfasserin aut Kravtsov, A. verfasserin aut Bulakh, E. verfasserin aut Kuzin, A. verfasserin aut Vasilyev, A. verfasserin aut Brazhenko, A. verfasserin aut Vashchishin, R. verfasserin aut Pylaev, O. verfasserin aut Koshovyy, V. verfasserin aut Lozinsky, A. verfasserin aut Ivantyshin, O. verfasserin aut Rucker, H. O. verfasserin aut Panchenko, M. verfasserin aut Fischer, G. verfasserin aut Lecacheux, A. verfasserin aut Denis, L. verfasserin aut Coffre, A. verfasserin aut Grieβmeier, J.-M. verfasserin aut Tagger, M. verfasserin aut Girard, J. verfasserin aut Charrier, D. verfasserin aut Briand, C. verfasserin aut Mann, G. verfasserin aut Enthalten in Experimental astronomy Dordrecht [u.a.] : Springer Science + Business Media B.V., 1989 42(2016), 1 vom: 28. Apr., Seite 11-48 (DE-627)312841116 (DE-600)2012330-9 1572-9508 nnns volume:42 year:2016 number:1 day:28 month:04 pages:11-48 https://dx.doi.org/10.1007/s10686-016-9498-x lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 39.00 ASE AR 42 2016 1 28 04 11-48 |
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Konovalenko, A. @@aut@@ Sodin, L. @@aut@@ Zakharenko, V. @@aut@@ Zarka, P. @@aut@@ Ulyanov, O. @@aut@@ Sidorchuk, M. @@aut@@ Stepkin, S. @@aut@@ Tokarsky, P. @@aut@@ Melnik, V. @@aut@@ Kalinichenko, N. @@aut@@ Stanislavsky, A. @@aut@@ Koliadin, V. @@aut@@ Shepelev, V. @@aut@@ Dorovskyy, V. @@aut@@ Ryabov, V. @@aut@@ Koval, A. @@aut@@ Bubnov, I. @@aut@@ Yerin, S. @@aut@@ Gridin, A. @@aut@@ Kulishenko, V. @@aut@@ Reznichenko, A. @@aut@@ Bortsov, V. @@aut@@ Lisachenko, V. @@aut@@ Reznik, A. @@aut@@ Kvasov, G. @@aut@@ Mukha, D. @@aut@@ Litvinenko, G. @@aut@@ Khristenko, A. @@aut@@ Shevchenko, V. V. @@aut@@ Shevchenko, V. A. @@aut@@ Belov, A. @@aut@@ Rudavin, E. @@aut@@ Vasylieva, I. @@aut@@ Miroshnichenko, A. @@aut@@ Vasilenko, N. @@aut@@ Olyak, M. @@aut@@ Mylostna, K. @@aut@@ Skoryk, A. @@aut@@ Shevtsova, A. @@aut@@ Plakhov, M. @@aut@@ Kravtsov, I. @@aut@@ Volvach, Y. @@aut@@ Lytvinenko, O. @@aut@@ Shevchuk, N. @@aut@@ Zhouk, I. @@aut@@ Bovkun, V. @@aut@@ Antonov, A. @@aut@@ Vavriv, D. @@aut@@ Vinogradov, V. @@aut@@ Kozhin, R. @@aut@@ Kravtsov, A. @@aut@@ Bulakh, E. @@aut@@ Kuzin, A. @@aut@@ Vasilyev, A. @@aut@@ Brazhenko, A. @@aut@@ Vashchishin, R. @@aut@@ Pylaev, O. @@aut@@ Koshovyy, V. @@aut@@ Lozinsky, A. @@aut@@ Ivantyshin, O. @@aut@@ Rucker, H. O. @@aut@@ Panchenko, M. @@aut@@ Fischer, G. @@aut@@ Lecacheux, A. @@aut@@ Denis, L. @@aut@@ Coffre, A. @@aut@@ Grieβmeier, J.-M. @@aut@@ Tagger, M. @@aut@@ Girard, J. @@aut@@ Charrier, D. @@aut@@ Briand, C. @@aut@@ Mann, G. @@aut@@ |
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Konovalenko, A. Sodin, L. Zakharenko, V. Zarka, P. Ulyanov, O. Sidorchuk, M. Stepkin, S. Tokarsky, P. Melnik, V. Kalinichenko, N. Stanislavsky, A. Koliadin, V. Shepelev, V. Dorovskyy, V. Ryabov, V. Koval, A. Bubnov, I. Yerin, S. Gridin, A. Kulishenko, V. Reznichenko, A. Bortsov, V. Lisachenko, V. Reznik, A. Kvasov, G. Mukha, D. Litvinenko, G. Khristenko, A. Shevchenko, V. V. Shevchenko, V. A. Belov, A. Rudavin, E. Vasylieva, I. Miroshnichenko, A. Vasilenko, N. Olyak, M. Mylostna, K. Skoryk, A. Shevtsova, A. Plakhov, M. Kravtsov, I. Volvach, Y. Lytvinenko, O. Shevchuk, N. Zhouk, I. Bovkun, V. Antonov, A. Vavriv, D. Vinogradov, V. Kozhin, R. Kravtsov, A. Bulakh, E. Kuzin, A. Vasilyev, A. Brazhenko, A. Vashchishin, R. Pylaev, O. Koshovyy, V. Lozinsky, A. Ivantyshin, O. Rucker, H. O. Panchenko, M. Fischer, G. Lecacheux, A. Denis, L. Coffre, A. Grieβmeier, J.-M. Tagger, M. Girard, J. Charrier, D. Briand, C. Mann, G. |
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The modern radio astronomy network in Ukraine: UTR-2, URAN and GURT |
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Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. |
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Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. |
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Abstract The current status of the large decameter radio telescope UTR-2 (Ukrainian T-shaped Radio telescope) together with its VLBI system called URAN is described in detail. By modernization of these instruments through implementation of novel versatile analog and digital devices as well as new observation techniques, the observational capabilities of UTR-2 have been substantially enhanced. The total effective area of UTR-2 and URAN arrays reaches 200 000 $ m^{2} $, with 24 MHz observational bandwidth (within the 8–32 MHz frequency range), spectral and temporal resolutions down to 4 kHz and 0.5 msec in dynamic spectrum mode or virtually unlimited in waveform mode. Depending on the spectral and temporal resolutions and confusion effects, the sensitivity of UTR-2 varies from a few Jy to a few mJy, and the angular resolution ranges from ~ 30 arcminutes (with a single antenna array) to a few arcseconds (in VLBI mode). In the framework of national and international research projects conducted in recent years, many new results on Solar system objects, the Galaxy and Metagalaxy have been obtained. In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. The radio telescope systems described herein can be used in synergy with other existing low-frequency arrays such as LOFAR, LWA, NenuFAR, as well as provide ground-based support for space-based instruments. |
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In order to extend the observation frequency range to 8–80 MHz and enlarge the dimensions of the UTR-2 array, a new instrument – GURT (Giant Ukrainian Radio Telescope) – is now under construction. 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| score |
7.4000835 |