Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Quentin Nenon"'
Publikováno v:
Geophysical Research Letters, Vol 51, Iss 10, Pp n/a-n/a (2024)
Abstract This study presents evidence of stably trapped electrons at Jupiter's moon Ganymede. We model energetic electron pitch angle distributions and compare them to observations from the Galileo Energetic Particle Detector to identify signatures o
Externí odkaz:
https://doaj.org/article/217798c886c94f1ebfb2fe0d4a98692e
Autor:
Sae Aizawa, Yuki Harada, Nicolas André, Yoshifumi Saito, Stas Barabash, Dominique Delcourt, Jean-André Sauvaud, Alain Barthe, Andréi Fedorov, Emmanuel Penou, Shoichiro Yokota, Wataru Miyake, Moa Persson, Quentin Nénon, Mathias Rojo, Yoshifumi Futaana, Kazushi Asamura, Manabu Shimoyama, Lina Z. Hadid, Dominique Fontaine, Bruno Katra, Markus Fraenz, Norbert Krupp, Shoya Matsuda, Go Murakami
Publikováno v:
Nature Communications, Vol 14, Iss 1, Pp 1-7 (2023)
Abstract Mercury’s magnetosphere is known to involve fundamental processes releasing particles and energy like at Earth due to the solar wind interaction. The resulting cycle is however much faster and involves acceleration, transport, loss, and re
Externí odkaz:
https://doaj.org/article/5f4eaef0a1544ca1bb59720e7a1aa757
Autor:
Sae Aizawa, Nicolas Andre, Moa Persson, Ronan Modolo, Jim Raines, Francois Leblanc, Jean-Yves Chaufray, Quentin Nenon
The escape and precipitation of planetary ions at Mercury under different solar wind conditions have been examined using a global hybrid simulation. The combination of Mercury’s weak intrinsic magnetic field and solar wind conditions at Mercury’s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1ef7d86f7adb6032ef7167df2237b6f4
https://doi.org/10.5194/epsc2022-902
https://doi.org/10.5194/epsc2022-902
Autor:
Jamey Szalay, Todd Smith, Eric Zirnstein, David McComas, Luke Begley, Fran Bagenal, Peter Delamere, Robert Wilson, Phil Valek, Andrew Poppe, Quentin Nenon, Frederic Allegrini, Robert Ebert, Scott Bolton
Water-group gas continuously escapes from Jupiter’s icy moons to form co-orbiting populations of particles, or neutral toroidal clouds. We report the first observations of H2+ pickup ions in Jupiter’s magnetosphere from 13-18 Jovian radii, confir
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ace86ee478b7e544785192adca64be03
https://doi.org/10.5194/epsc2022-702
https://doi.org/10.5194/epsc2022-702
Jupiter’s moon Callisto is exposed to a highly dynamic magnetospheric environment. During a full synodic period, properties of the local magnetospheric field and thermal plasma environment change by an order of magnitude, and Callisto’s resulting
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::557c19a8db830d712e3842d8b1acf9c6
https://doi.org/10.5194/epsc2022-282
https://doi.org/10.5194/epsc2022-282