@InProceedings{MagalhãesZarEchEchGon:2018:LoFrVa,
author = "Magalh{\~a}es, Fab{\'{\i}}ola Pinho and Zarka, P. and Echer,
Ezequiel and Echer, Mariza Pereira de Souza and Gonzalez Alarcon,
Walter Dem{\'e}trio",
affiliation = "{Instituto Nacional de Pesquisas Espaciais (INPE)} and {} and
{Instituto Nacional de Pesquisas Espaciais (INPE)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)}",
title = "Low frequency variations of Jovian radio emissions observed by
Cassini",
year = "2018",
organization = "Latin American Conference on Space Geophysics, 11. (COLAGE)",
abstract = "Since the 1950s, Jupiter is known to be a major source of radio
emissions. First, ground-based antennas obtained radio
observations. Later the knowledge about plasma sources on Jupiters
magnetosphere were based on in-situ and remote sensing
measurements onboard spacecrafts. The radio spectrum of Jupiter
spanning the frequency range from 10 kHz to 3 GHz is dominated by
strong non-thermal radiation. Jupiters giant magnetosphere is
mostly determined by internal interactions, primarily due to
activity in Ios volcanoes, affecting the supply of plasma to all
other regions. However, the Jovian magnetosphere dynamics is
believed to be in part responsive changes in Solar Wind
conditions. In the end of the year 2000, Cassini-Huygens
spacecraft performed its closest approach to Jupiter, reaching a
distance of ten million kilometers of the planet. During Cassinis
flyby at the Jovian system, the Radio and Plasma Wave Science (the
acronym RPWS) instrument measured Jovians radio emissions during
the inbound and outbound trajectories. The present work aims to
investigate Jupiters radio emissions long term variation (¿ 1
Jupiter rotation), analyzing the behaviour of the 10- hour
integrated fluxes to the DAM, HOM, nKOM and bKOM bands. The data
period used goes from October 2000 to March 2001. Averaged fluxes
are compared for inbound and outbound orbits Correlation and
Lomb-Scargle periodogram analyses were applied to RPWS data to
investigate the correlation among different spectral ranges and
the major periodicities.",
conference-location = "Buenos Aires, Argentina",
conference-year = "16-20 abr.",
language = "en",
urlaccessdate = "28 abr. 2024"
}