Zobrazeno 1 - 10
of 110
pro vyhledávání: '"Ronan Modolo"'
Autor:
Lina Z. Hadid, Dominique Delcourt, Yuki Harada, Mathias Rojo, Sae Aizawa, Yoshifumi Saito, Nicolas André, Austin N. Glass, Jim M. Raines, Shoichiro Yokota, Markus Fränz, Bruno Katra, Christophe Verdeil, Björn Fiethe, Francois Leblanc, Ronan Modolo, Dominique Fontaine, Norbert Krupp, Harald Krüger, Frédéric Leblanc, Henning Fischer, Jean-Jacques Berthelier, Jean-André Sauvaud, Go Murakami, Shoya Matsuda
Publikováno v:
Communications Physics, Vol 7, Iss 1, Pp 1-7 (2024)
Abstract Understanding Mercury’s magnetosphere is crucial for advancing our comprehension of how the solar wind interacts with the planetary magnetospheres. Despite previous missions, several gaps remain in our knowledge of Mercury’s plasma envir
Externí odkaz:
https://doaj.org/article/a09aa15cc285492fa093e28710b3ebd3
Autor:
Clément Moissard, Axel Bernal, Philippe Savoini, Dominique Fontaine, Ronan Modolo, Vincent David, Bayane Michotte de Welle
Interplanetary shocks are some of the main drivers of geomagnetic storms. Before they can impact the geomagnetic environment, they propagate through the magnetosheath where their properties and geometry can be modified. What is the velocity of interp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::64375c4e6092543d11d7a4271ceae3d4
https://doi.org/10.5194/egusphere-egu23-9423
https://doi.org/10.5194/egusphere-egu23-9423
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:
Jean-Yves Chaufray, Francisco Gonzalez-Galindo, Margaux Vals, Loic Rossi, Franck Montmessin, Franck Lefevre, François Leblanc, Ronan Modolo, François Forget, Ehouarn Millour, Gabriella Gilli, Miguel Lopez-Valverde, Majd Mayyasi
The D/H ratio is a key parameter to understand the atmospheric evolution of a planet. On Mars a D/H ~ 5 times larger than the ratio on Earth is measured. This large ratio can be explained by a preferential escape of the hydrogen compared to the deute
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5af03b5e6a02833b14f6d6a1434ec643
https://doi.org/10.5194/epsc2022-568
https://doi.org/10.5194/epsc2022-568
Autor:
Claire Vallat, Nicolas Altobelli, Rosario Lorente, Claudio Munoz, Olivier Witasse, Thibault Cavalié, Leigh Fletcher, Adam Masters, Ronan Modolo, Thomas Roatsch, Gabriel Tobie, Federico Tosi, Tim Van Hoolst
JUICE is the first large mission chosen in the framework of ESA’s Cosmic Vision 2015-2025 program. The focus of JUICE is to characterize the conditions that might have led to the emergence of habitable environments among the Jovian icy satellites,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b65a8a0a435c146b74ec5bdf9d3e4f16
https://doi.org/10.5194/epsc2022-1236
https://doi.org/10.5194/epsc2022-1236
Autor:
Erwan Jariel, Sae Aizawa, Ronan Modolo, Ludivine Leclercq, Claire Baskevitch, Nicolas Andre, Moa Persson
Unlike Earth, Venus doesn’t have an intrinsic magnetic field shielding it from the solar wind. However, an inducedmagnetic field is generated from the interaction of solar wind and the dense atmosphere of the planet. RecentVenus flybys by the BepiC
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dfd1a390ea18469418a2d9860774147b
https://doi.org/10.5194/epsc2022-417
https://doi.org/10.5194/epsc2022-417
Publikováno v:
EPSC Abstracts
Europlanet Science Congress 2022
Europlanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-469
Europlanet Science Congress 2022
Europlanet Science Congress 2022, Sep 2022, Granada, Spain. pp.EPSC2022-469
Venus lacks an intrinsic magnetic filed, as a result, the incoming solar wind interacts directly with its atmosphere, creating an induced magnetosphere. Venus is believed to have once held a significant amount of water, which has since then disappear
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9c13417756564fe3d53105bde1921dd8
https://doi.org/10.5194/epsc2022-469
https://doi.org/10.5194/epsc2022-469
Autor:
Ronan Modolo, Francois Leblanc, Jean-Yves Chaufray, Norberto Romanelli, Eduard Dubinin, Vincent Génot, Claire Baskevitch, David Brain, Shannon Curry, Robert Lillis
Publikováno v:
EGU General Assembly 2022
EGU General Assembly 2022, May 2022, Online, Austria. ⟨10.5194/egusphere-egu22-7665⟩
EGU General Assembly 2022, May 2022, Online, Austria. ⟨10.5194/egusphere-egu22-7665⟩
During the last decade, MAVEN space mission have emphasized a widespread spatial distribution of escaping O+ ions (Brain et al., 2015; Dong et al., 2015; Curry et al., 2015). Statistical studies have demonstrated that such structure is constant and p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3706e4004bacf9670bb15e351ebdedb5
https://doi.org/10.5194/egusphere-egu22-7665
https://doi.org/10.5194/egusphere-egu22-7665
Autor:
Sae Aizawa, Moa Persson, Thibault Menez, Nicolas Andre, Ronan Modolo, Alain Barthe, Emmanuel Penou, Andrei Fedorov, Jean-Andre Sauvaud, Francois Leblanc, Jean-Yves Chaufray, Yoshifumi Saito, Shoichiro Yokota, Go Murakami, Vincent Genot, Beatriz Sanchez-Cano, Daniel Heyner, Tim Horbury, Philippe Louarn, Christopher Owen
The 2nd Venus flyby of BepiColombo has been examined and compared by the newly developed global hybrid simulation LatHyS for the Venusian environment. The LatHyS has been first validated by comparison with Venus Express observations, then using the o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::afa2479e12794284a70b5b299320a969
https://doi.org/10.5194/egusphere-egu22-4175
https://doi.org/10.5194/egusphere-egu22-4175