Statistical Distributions of Plasma Density and Pressure in the Jovian Plasma Sheet

Abstract

The Jovian plasma sheet is a key region of the Jovian magnetosphere populated by a mix of warm and hot plasma. It is the main channel for radial transport of mass and energy in the Jovian magnetosphere and provides a favorable environment for magnetic reconnection and wave–particle interactions although the understanding of its plasma properties is incomplete. This study combines observations from the Jovian Auroral Distributions Experiment and Juno Energetic Particle Detector Instrument on board the Juno spacecraft during its first 31 orbits to analyze the plasma properties of the Jovian plasma sheet from 20 R _J to 100 R _J . Our results indicate that the plasma number density decreases from 1 cm ^−3 at 20 R _J to 0.005 cm ^−3 at 100 R _J , while the plasma pressure decreases from 2 nPa at 20 R _J to 0.02 nPa at 100 R _J . The plasma pressure inside the plasma sheet is comparable to the magnetic pressure in the lobe region, suggesting a rough balance between the two. In the plasma sheet with r > 70 R _J , the H ^+ density and pressure remain relatively constant, likely due to other plasma sources such as the solar wind. Additionally, we find that the pressure (density) ratios for heavy ions between the center and the edge of the plasma sheet are generally an order of magnitude, while that for H ^+ decreases with radial distance. These findings contribute to a more comprehensive understanding of the plasma properties of the Jovian plasma sheet.

Keywords

• Planetary magnetospheres
• Planetary science
• Planetary-disk interactions