This is the supporting data set for the paper by the same title published in AGU JGR Space Physics, 10.1029/2021JA029195 Abstract We present Jovian electron densities measured by the Juno Waves instrument at high-latitudes on magnetic field lines threading the Io torus using the first 29 orbits of the Juno mission. We infer electron densities from characteristic frequency cutoffs and resonances in plasma wave spectra. There are often times when more than one of the characteristic frequency of the plasma can be identified, whose consistency provides more credibility to the plasma density estimates. The majority of density measurements are on magnetic field lines threading the Io torus and intersecting Jupiter's ionosphere between Io's M-sh...
peer reviewedThe Juno spacecraft crossed flux tubes connected to the Io footprint tail at low Jovian...
Recent observations by the Juno spacecraft have shown that electrons contributing to Jupiter's main ...
The relationship between electron energy flux and the characteristic energy of electron distribution...
International audienceWe present a survey of electron partial densities (i.e., the portion of the to...
We present a survey of electron partial densities (i.e., the portion of the total density measured b...
Jupiter hosts very intense auroral emissions, which originates from various magnetospheric processes...
The Juno spacecraft crossed flux tubes connected to the Io footprint tail at low Jovian altitudes on...
The jovian moon Io disperses about 1 ton/s of material in the planetary magnetosphere, mainly b...
[1] Recent observations of auroral arcs on Jupiter suggest that electrons are being accelerated down...
This is the supporting data set for the paper by the same title published in AGU JGR Space Physics. ...
Io is the primary source of plasma in the Jovian magnetosphere, continuously releasing approximately...
International audienceJupiter's main auroral oval provides a window into the complex magnetospheric ...
peer reviewedThe Juno spacecraft crossed flux tubes connected to the Io footprint tail at low Jovian...
Recent observations by the Juno spacecraft have shown that electrons contributing to Jupiter's main ...
The relationship between electron energy flux and the characteristic energy of electron distribution...
International audienceWe present a survey of electron partial densities (i.e., the portion of the to...
We present a survey of electron partial densities (i.e., the portion of the total density measured b...
Jupiter hosts very intense auroral emissions, which originates from various magnetospheric processes...
The Juno spacecraft crossed flux tubes connected to the Io footprint tail at low Jovian altitudes on...
The jovian moon Io disperses about 1 ton/s of material in the planetary magnetosphere, mainly b...
[1] Recent observations of auroral arcs on Jupiter suggest that electrons are being accelerated down...
This is the supporting data set for the paper by the same title published in AGU JGR Space Physics. ...
Io is the primary source of plasma in the Jovian magnetosphere, continuously releasing approximately...
International audienceJupiter's main auroral oval provides a window into the complex magnetospheric ...
peer reviewedThe Juno spacecraft crossed flux tubes connected to the Io footprint tail at low Jovian...
Recent observations by the Juno spacecraft have shown that electrons contributing to Jupiter's main ...
The relationship between electron energy flux and the characteristic energy of electron distribution...