Survey of Juno Observations in Jupiter's Plasma Disk: Density

The jovian plasma density data provided here was used in the following
peer review publication, and contains the raw data analysed and values
for some figures:

Huscher, E., Bagenal, F., Wilson, R. J., Allegrini, F., Ebert, R. W.,
Valek, P. W., et al. (2021). Survey of Juno Observations in Jupiter's
Plasma Disk: Density. Journal of Geophysical Research: Space Physics,
126, e2021JA029446. https://doi.org/10.1029/2021JA029446

This paper has the abstract:

We explore the variation in plasma conditions through the middle
magnetosphere of Jupiter with latitude and radial distance using
Juno-JADE measurements of plasma density (electrons, protons, sulfur and
oxygen ions) surveyed on orbits 5 to 26 between March 2017 and April
2020. On most orbits the densities exhibit regular behavior, mapping out
a disk between 10-50 RJ (jovian radii). In the disk the heavy ions are
confined close to the centrifugal equator which oscillates relative to
the spacecraft due to the ∼10° tilt of Jupiter's magnetic dipole.
Exploring each crossing of the plasma disk shows there are some
occasions where the density profiles are smooth and well-defined. At
other times, small-scale structures suggest temporal and/or spatial
variabilities. There are some exceptional orbits where the outer regions
(30-50 RJ) of the plasma disk show uniform depletion, perhaps due to
enhanced ejection of plasmoids down the magnetotail, possibly triggered
by solar wind compression events.

We encourage people to read the paper, and then use this dataset if they
wish to verify the results, or overlay this paper's results in their own
figures.