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Institut d'Astrophysique et
de Géophysique (Bât. B5c)
Quartier Agora
Allée du 6 août, 19C
B-4000 Liège 1 (Sart-Tilman)
Belgique
Tel.: 04.366.9779
Fax: 04.366.9729
de Géophysique (Bât. B5c)
Quartier Agora
Allée du 6 août, 19C
B-4000 Liège 1 (Sart-Tilman)
Belgique
Tel.: 04.366.9779
Fax: 04.366.9729
Seminars
Seminars are regularly held to enable department's researchers as well as external scientists to present the latest findings in their fields. You are most welcome to join us:
07/12/2023 : 16h00 | Electro-dynamic moon-magnetosphere interactions in our Solar System Bertrand BONFOND |
14/12/2023 : 16h00 | TBA Camilla Pezzotti |
25/01/2024 : 16h00 | TBA Sophie Rosu |
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Electro-dynamic moon-magnetosphere interactions in our Solar System
Bertrand BONFOND (University of Liège)
Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)
The electro-dynamic interactions between moons and the magnetosphere of their host planets have been investigated since the mid-20th century and the implication of the Alfvén waves was recognized right away. However, in the first models, Alfvén waves were only considered as current carriers. It is only after the Voyager missions that the possibility of complex reflection patterns was considered and their ability to accelerate particles became fully appreciated only recently. For this seminar, I will review the history of our understanding of the various cases of moon-magnetosphere interactions in our Solar System. The presence of the largest of these moons in the stream of the magnetospheric plasma generates powerful large-scale Alfvén waves, which can break up into smaller scales, reflect off density gradients and accelerate particles, ultimately impacting the atmosphere of the planet to generate auroras and trigger radio emissions. The best-known case is the Io-Jupiter interaction, since its observational signatures are the richest and most obvious. As our means of investigation improved, signatures of similar interactions have also been discovered for the other Galilean moons, as well as for moons orbiting Saturn. Interestingly, similar interactions can occur on rare occasions between the planets themselves and the solar wind and most likely take place in exo-planetary systems as well.
Bertrand BONFOND (University of Liège)
Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)
The electro-dynamic interactions between moons and the magnetosphere of their host planets have been investigated since the mid-20th century and the implication of the Alfvén waves was recognized right away. However, in the first models, Alfvén waves were only considered as current carriers. It is only after the Voyager missions that the possibility of complex reflection patterns was considered and their ability to accelerate particles became fully appreciated only recently. For this seminar, I will review the history of our understanding of the various cases of moon-magnetosphere interactions in our Solar System. The presence of the largest of these moons in the stream of the magnetospheric plasma generates powerful large-scale Alfvén waves, which can break up into smaller scales, reflect off density gradients and accelerate particles, ultimately impacting the atmosphere of the planet to generate auroras and trigger radio emissions. The best-known case is the Io-Jupiter interaction, since its observational signatures are the richest and most obvious. As our means of investigation improved, signatures of similar interactions have also been discovered for the other Galilean moons, as well as for moons orbiting Saturn. Interestingly, similar interactions can occur on rare occasions between the planets themselves and the solar wind and most likely take place in exo-planetary systems as well.
TBA
Camilla Pezzotti (AGO)
Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)
Camilla Pezzotti (AGO)
Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)

TBA
Sophie Rosu (KTH Royal Institute of Technology, Stockholm, Sweden)
Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)
Sophie Rosu (KTH Royal Institute of Technology, Stockholm, Sweden)
Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)
University of Liège >
Faculty of Sciences >
Department of Astrophysics, Geophysics and Oceanography :
CoWebAGO, June 2009.