Radial Transport of Io Plasma From the Inner Magnetosphere to the Tail
Published in Journal of Geophysical Research: Space Physics, 2023
Around 10–15 Rj in the equatorial plane, precession effect overwhelms interchange for the outward transport of Io plasma
Io plasma is interchange unstable around 15–20 Rj and here diffuses outward while being mixed with H+ from the ionosphere
The equatorial diffuse emission is projected with the low-speed polar wind to the outer shell of the Io torus around 15–20 Rj in the equatorial plane
Recommended citation: Tanaka, T., Ebihara, Y., Watanabe, M., Fujita, S., & Kataoka, R. (2023). "Radial Transport of Io Plasma From the Inner Magnetosphere to the Tail" Journal of Geophysical Research: Space Physics. 128, e2022JA030891 https://doi.org/10.1029/2022JA030891