[P-EM18] Dynamics of Magnetosphere and Ionosphere

[PEM18-P10] Statistical characteristics of the Jovian Io-related and auroral S-bursts from the Long Wavelength Array Juno-supporting high-resolution ground-based radio observatories

*Adam Boudouma¹, Masafumi Imai¹, Emilie Mauduit², Philippe Zarka², Laurent Lamy^2,3,4, Alain Lecacheux², Tracy Ellen Clarke⁵, Chuck Higgins⁶ (1. Institute of Atmospheric Physics Czech Academy of Sciences, Prague, Czechia, 2. Laboratory for Instrumentation and Research in Astrophysics, Observatoire de Paris, Meudon, France, 3. Laboratory of Astrophysics of Marseille, Marseille, France, 4. Nançay Radioastronomic Observatory, Nançay, France, 5. Naval Research Laboratory, Washington D.C, USA, 6. Department of Physics and Astronomy, Middle Tennessee State University, USA)

Keywords:Jupiter, Radio, Auroral, Maser-cyclotron, S-burst, Ground-based