Skip to main content

CORRECTION article

Front. Astron. Space Sci.
Sec. Planetary Science
Volume 11 - 2024 | doi: 10.3389/fspas.2024.1503779
This article is part of the Research Topic Remote Sensing and Modelling of Planetary and Moon Surfaces View all articles

Corrigendum: The temporal variability of Io's hotspots

Provisionally accepted
Alessandro Mura Alessandro Mura 1*Francesca Zambon Francesca Zambon 1Federico Tosi Federico Tosi 1Rosaly Lopes Rosaly Lopes 2Julie Rathbun Julie Rathbun 3Madeline Pettine Madeline Pettine 3Alberto Adriani Alberto Adriani 1Francesca Altieri Francesca Altieri 1Mauro Ciarniello Mauro Ciarniello 1Andrea Cicchetti Andrea Cicchetti 1Gianrico Filacchione Gianrico Filacchione 1Davide Grassi Davide Grassi 1Raffaella Noschese Raffaella Noschese 1Alessandra Migliorini Alessandra Migliorini 1Giuseppe Piccioni Giuseppe Piccioni 1Christina Plainaki Christina Plainaki 4Roberto Sordini Roberto Sordini 1Giuseppe Sindoni Giuseppe Sindoni 4Diego Turrini Diego Turrini 1
  • 1 Institute for Space Astrophysics and Planetology (INAF), Rome, Italy
  • 2 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, United States
  • 3 Cornell University, Ithaca, NY, United States, Itacha, United States
  • 4 Italian Space Agency (ASI), Rome, Lazio, Italy

The final, formatted version of the article will be published soon.

    Keywords: io, Galilean moons of Jupiter, Volcanism, infrared-IR, Juno

    Received: 29 Sep 2024; Accepted: 02 Oct 2024.

    Copyright: © 2024 Mura, Zambon, Tosi, Lopes, Rathbun, Pettine, Adriani, Altieri, Ciarniello, Cicchetti, Filacchione, Grassi, Noschese, Migliorini, Piccioni, Plainaki, Sordini, Sindoni and Turrini. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

    * Correspondence: Alessandro Mura, Institute for Space Astrophysics and Planetology (INAF), Rome, Italy

    Disclaimer: All claims expressed in this article are solely those of the authors and do not necessarily represent those of their affiliated organizations, or those of the publisher, the editors and the reviewers. Any product that may be evaluated in this article or claim that may be made by its manufacturer is not guaranteed or endorsed by the publisher.