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

V. Zakharenko , A. Konovalenko , G. Litvinenko , V. Kolyadin , P. Zarka (1) , K. Mylostna , I. Vasylieva (1) , Jean-Mathias Griessmeier (2) , M. Sidorchuk , H. Rucker , G. Fischer , B. Cecconi (1) , A. Coffre (3) , L. Denis (3) , V. Shevchenko , V. Nikolaenko

1 LESIA (UMR_8109) - Laboratoire d'études spatiales et d'instrumentation en astrophysique
2 LPC2E - Laboratoire de Physique et Chimie de l'Environnement et de l'Espace
3 USN - Unité Scientifique de la Station de Nançay

We describe the trends and tasks in the field of lowfrequency 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.

Domains: Sciences of the Universe [physics]

V. Zakharenko, A. Konovalenko, G. Litvinenko, V. Kolyadin, P. Zarka, et al.. Solar system radio emissions studies with the largest low-frequency radio telescopes. European Planetary Science Congress 2014, Sep 2014, Cascais, Portugal. pp.2581-2650. ⟨insu-03577344⟩