Solar system radio emissions studies with the largest low-frequency radio telescopes

Zakharenko, V.; Konovalenko, A.; Mylostna, Krystyna; Litvinenko, G.; Kolyadin, V.; Griessmeier, J.-M.; Zarka, P.; Sidorchuk, M.; Rucker, H.; Vasylieva, I.; Fischer, G.; Cecconi, B.; Coffre, A.; Denis, L.; Shevchenko,; Al, E. T.; Nikolaenko,

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Solar system radio emissions studies with the largest low-frequency radio telescopes

Journal article published in 2014 by V. Zakharenko, A. Konovalenko, Krystyna Mylostna, G. Litvinenko, V. Kolyadin, J.-M. Griessmeier, P. Zarka, M. Sidorchuk, H. Rucker, I. Vasylieva, G. Fischer, B. Cecconi

, A. Coffre, L. Denis, Shevchenko and other authors.

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Abstract

We describe the trends and tasks in the field of low-frequency studies of radio emission from the Solar system's objects. The world's largest decameter radio telescopes UTR-2 and URAN have a unique combination of sensitivity and time/frequency resolution parameters, providing the capability of the most detailed studies of various types of solar and planetary emissions.