Planetary Radio Emissions Vii 2011
DOI: 10.1553/pre7s521
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Abstract: According to the special Program of the National Academy of Sciences of Ukraine, creation of the new giant Ukrainian radio telescope (GURT) was started a few years ago on the UTR-2 radio telescope observatory. The main goal is to reach maximum band at the lowest frequencies (10-70 MHz), effective area (step-by-step up to 100,000 sq.m), and high interference immunity for resolving many astrophysical tasks when the sensitivity is less limited by the confusion effects. These tasks include stellar radio astronomy … Show more

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Cited by 8 publications
(4 citation statements)
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“…Many astrophysical phenomena and types of radio sources were studied using these receivers. The Digital spectro-polarimeter was used for a broadband study of Solar and Jovian radio emissions (Konovalenko et al, 2001) and helped to discover the anomalously intense pulses of pulsars in the LF range (Ulyanov et al, 2006(Ulyanov et al, , 2007. The Portable Pulsar Receiver permitted the detection of giant pulses of the pulsar in the Crab Nebula at 23 MHz (Popov et al, 2006).…”
Section: Previous Generations Of Digital Receivers With Frequency Con...mentioning
confidence: 99%
“…Many astrophysical phenomena and types of radio sources were studied using these receivers. The Digital spectro-polarimeter was used for a broadband study of Solar and Jovian radio emissions (Konovalenko et al, 2001) and helped to discover the anomalously intense pulses of pulsars in the LF range (Ulyanov et al, 2006(Ulyanov et al, , 2007. The Portable Pulsar Receiver permitted the detection of giant pulses of the pulsar in the Crab Nebula at 23 MHz (Popov et al, 2006).…”
Section: Previous Generations Of Digital Receivers With Frequency Con...mentioning
confidence: 99%
“…Additional searches have been reported by Bastian et al (2000) using the VLA (Very Large Array), as well as George and Stevens (2007) using the GMRT. The currently most sensitive radio array at decametric frequencies is the UTR-2 (Konovalenko et al, 2001) carried out between 1997 and 2001 , but also without positive detection of exoplanetary radio emission.…”
Section: Exoplanetary Radio Emissionmentioning
confidence: 99%
“…allows to analyze the specific Sburst features from the microscopic to macroscopic scale [Litvinenko et al, 2009]. With this aim several observational campaigns were performed in November 2009 using the UTR-2 radio telescope (Kharkov, Ukraine) and effective registration systems possessing high frequency and temporal resolutions (antenna effective area is close to 100,000 m 2 , the frequency resolution is 4 kHz, the temporal resolution is 0.25 ms, the dynamic range is 70 dB) [Konovalenko et al, 2001]. The main goal of…”
mentioning
confidence: 99%
“…A huge amount of wide-band data of the radiation from different Io-dependent sources taken for the present analysis has been obtained using the high frequency and temporal resolution digital receiver (DSP) [Kozhin et al, 2007] installed into the Ukrainian world's largest decameter band radio telescope UTR-2 [Konovalenko et al, 2001]. It is a fully digital baseband device which satisfies all modern requirements for the Jovian decameter emission investigations.…”
mentioning
confidence: 99%