Morphology of the Auroral Tail of Io, Europa, and Ganymede From JIRAM L‐Band Imager

Autor: Federico Tosi, Vincent Hue, Bianca Maria Dinelli, Raffaella Noschese, Roberto Sordini, Giuseppe Sindoni, Francesca Altieri, Stavro Ivanovski, Vincent Dols, Alessandro Moirano, Jamey Szalay, Christina Plainaki, Gianrico Filacchione, Scott Bolton, Jack H. Waite, Ali Sulaiman, Davide Grassi, Stefano Massetti, Alberto Adriani, Andrea Cicchetti, Alessandro Mura, Robert L. Lysak, Maria Luisa Moriconi, Bertrand Bonfond, Giuseppe Piccioni, Diego Turrini, Alessandra Migliorini

Publikováno v: Journal of geophysical research. Space physics
(2021): e2021JA029450. doi:10.1029/2021JA029450
info:cnr-pdr/source/autori:Alessandro Moirano1, Alessandro Mura1, Alberto Adriani1, Vincent Dols2, Bertrand Bonfond3, Jack H. Waite4,5, Vincent Hue4, Jamey R. Szalay6, Ali H. Sulaiman7, Bianca M. Dinelli8, Federico Tosi1, Francesca Altieri1, Andrea Cicchetti1, Gianrico Filacchione1, Davide Grassi1, Alessandra Migliorini1, Maria L. Moriconi8, Raffaella Noschese1, Giuseppe Piccioni1, Roberto Sordini1, Diego Turrini1, Christina Plainaki9, Giuseppe Sindoni9, Stefano Massetti1, Robert L. Lysak10, Stavro L. Ivanovski11, and Scott J. Bolton4/titolo:Morphology of the Auroral Tail of Io, Europa, and Ganymede From JIRAM L-Band Imager/doi:10.1029%2F2021JA029450/rivista:Journal of geophysical research. Space physics (Print)/anno:2021/pagina_da:/pagina_a:e2021JA029450/intervallo_pagine:e2021JA029450/volume

Jupiter hosts intense auroral activity associated with charged particles precipitating into the planet's atmosphere. The Galilean moons orbiting within the magnetosphere are swept by the magnetic field: the resulting perturbation travels along field

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6bdd56ce64e8ff43e3fa8869c0f8addb
https://doi.org/10.1029/2021ja029450