The jovian moon Io disperses about 1 ton/s of material in the planetary magnetosphere, mainly by sublimation of SO2 from the surface and by its intense volcanic activity. The ejected material supplies the plasma cloud surrounding Jupiter known as Io Plasma Torus (IPT). The radio communication between Juno and the Earth DSN station crosses the IPT near the closest approach. Being a dispersive medium, the IPT introduces a path delay in the signal, which can be analyzed to retrieve the density distribution of electrons. We used radio tracking data from the first 25 orbits to investigate the morphology of the IPT and its variability. We adopted a static and axisymmetric model for the electron density and we updated it including temporal and longitudinal variability. We found that our best fit model must include both variabilities, even though on average the morphology of the IPT agrees with previous analyses. Our results suggest that the density of the outer region of the IPT fluctuates over 50% the average value over a typical time scale of about 420 days.

Morphology of the Io Plasma Torus From Juno Radio Occultations / Moirano, A.; Gomez Casajus, L.; Zannoni, M.; Durante, D.; Tortora, P.. - In: JOURNAL OF GEOPHYSICAL RESEARCH. SPACE PHYSICS. - ISSN 2169-9380. - 126:10(2021), pp. 1-25. [10.1029/2021JA029190]

Morphology of the Io Plasma Torus From Juno Radio Occultations

Moirano A.
Primo
;
Durante D.;
2021

Abstract

The jovian moon Io disperses about 1 ton/s of material in the planetary magnetosphere, mainly by sublimation of SO2 from the surface and by its intense volcanic activity. The ejected material supplies the plasma cloud surrounding Jupiter known as Io Plasma Torus (IPT). The radio communication between Juno and the Earth DSN station crosses the IPT near the closest approach. Being a dispersive medium, the IPT introduces a path delay in the signal, which can be analyzed to retrieve the density distribution of electrons. We used radio tracking data from the first 25 orbits to investigate the morphology of the IPT and its variability. We adopted a static and axisymmetric model for the electron density and we updated it including temporal and longitudinal variability. We found that our best fit model must include both variabilities, even though on average the morphology of the IPT agrees with previous analyses. Our results suggest that the density of the outer region of the IPT fluctuates over 50% the average value over a typical time scale of about 420 days.
2021
Juno; Io Plasma Torus; Radio Occultations
01 Pubblicazione su rivista::01a Articolo in rivista
Morphology of the Io Plasma Torus From Juno Radio Occultations / Moirano, A.; Gomez Casajus, L.; Zannoni, M.; Durante, D.; Tortora, P.. - In: JOURNAL OF GEOPHYSICAL RESEARCH. SPACE PHYSICS. - ISSN 2169-9380. - 126:10(2021), pp. 1-25. [10.1029/2021JA029190]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1605347
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