@InProceedings{ZarkaMLRLECHCD:2017:RaEmGa,
author = "Zarka, Philippe and Marques, Manilo Soares and Louis, Corentin and
Ryabov, Vladimir and Lamy, Laurent and Echer, Ezequiel and
Cecconi, Baptiste and Hess, S{\'e}bastien and Coffre, Andr{\'e}
and Denis, Laurent",
affiliation = "{Observatoire de Paris} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {} and {} and {} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Radio emission from the Ganymede-Jupiter interaction and
consequence for radio emissions from exoplanets",
year = "2017",
organization = "Magnetospheres of the Outer Planets (MOP)",
abstract = "Analysis of a catalog of 26 years of radio decameter observations
from Jupiter in Nan{\c{c}}ay (France) allowed us to detect
unambiguously the radio emissions resulting from the
Ganymede-Jupiter interaction. The duration and power of the 189
events detected suggest sporadic reconnection with an average
radio power released in the Ganymede-Jupiter decameter emission 15
times smaller than in the Io-Jupiter one. This compares well with
the ratio of the magnetic power (Poynting flux) dissipated at the
Ganymede-Jupiter and Io-Jupiter interactions, confirming the
radio-magnetic Bodes law of Zarka et al. (2001), that serves as a
basis for predicting exoplanetary radio emissions. Constraints
imposed by the Ganymede-Jupiter radio emission on Jovian magnetic
field models are also discussed.",
conference-location = "Uppsala, Sweden",
conference-year = "12-16 june",
language = "en",
urlaccessdate = "28 abr. 2024"
}