Zobrazeno 1 - 10
of 284
pro vyhledávání: '"Mazelle , Christian"'
Autor:
Andrés, Nahuel, Romanelli, Norberto, Mazelle, Christian, Chen, Li-Jen, Gruesbeck, Jacob R., Espley, Jared R.
Using Mars Atmosphere and Volatile EvolutioN Magnetometer observations, we report the first statistical study of ultra-low frequency (ULF) waves at the Martian foreshock. The analyzed foreshock ULF wave events are observed in the 0.008-0.086 Hz frequ
Externí odkaz:
http://arxiv.org/abs/2408.09003
Autor:
Chian, Abraham, Miranda, Rodrigo, Bertucci, Cesar, Blanco-Cano, Xóchitl, Borovsky, Joe, Dasso, Sergio, Echer, Ezequiel, Franco, Adriane, Girgis, Kirolosse M., González-Esparza, J. Américo, Hada, Tohru, Hasegawa, Hiroshi, Hsieh, Syau-Yun, Kajdič, Primoz, Mazelle, Christian, Rempel, Erico, Rojas-Castillo, Diana, Sánchez-Cano, Beatriz, Sibeck, David, Stepanova, Marina, Valdés-Galicia, José, Valdivia, Juan
Publikováno v:
In Journal of Atmospheric and Solar-Terrestrial Physics June 2024 259
Autor:
Wedlund, Cyril Simon, Volwerk, Martin, Mazelle, Christian, Halekas, Jasper, Rojas-Castillo, Diana, Espley, Jared, Möstl, Christian
Publikováno v:
J. Geophys. Res. Space Phys. 127 (2022) 1-28
We present an in-depth analysis of a time interval when quasi-linear mirror mode structures were detected by magnetic field and plasma measurements as observed by the NASA/Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft. We employ ion and e
Externí odkaz:
http://arxiv.org/abs/2107.11223
Autor:
Sánchez-Cano, Beatriz, Lester, Mark, Andrews, David J., Opgenoorth, Hermann, Lillis, Robert, Leblanc, François, Fowler, Christopher M., Fang, Xiaohua, Vaisberg, Oleg, Mayyasi, Majd, Holmberg, Mika, Guo, Jingnan, Hamrin, Maria, Mazelle, Christian, Peter, Kerstin, Pätzold, Martin, Stergiopoulou, Katerina, Goetz, Charlotte, Ermakov, Vladimir Nikolaevich, Shuvalov, Sergei, Wild, James, Blelly, Pierre-Louis, Mendillo, Michael, Bertucci, Cesar, Cartacci, Marco, Orosei, Roberto, Chu, Feng, Kopf, Andrew J., Girazian, Zachary R., Roman, Michael T.
The objective of this White Paper submitted to ESA's Voyage 2050 call is to get a more holistic knowledge of the dynamics of the Martian plasma system from its surface up to the undisturbed solar wind outside of the induced magnetosphere. This can on
Externí odkaz:
http://arxiv.org/abs/1908.05497
Autor:
Götz, Charlotte, Gunell, Herber, Volwerk, Martin, Beth, Arnaud, Eriksson, Anders, Galand, Marina, Henri, Pierre, Nilsson, Hans, Wedlund, Cyril Simon, Alho, Markku, Andersson, Laila, Andre, Nicolas, De Keyser, Johan, Deca, Jan, Ge, Yasong, Glaßmeier, Karl-Heinz, Hajra, Rajkumar, Karlsson, Tomas, Kasahara, Satoshi, Kolmasova, Ivana, LLera, Kristie, Madanian, Hadi, Mann, Ingrid, Mazelle, Christian, Odelstad, Elias, Plaschke, Ferdinand, Rubin, Martin, Sanchez-Cano, Beatriz, Snodgrass, Colin, Vigren, Erik
Comets hold the key to the understanding of our solar system, its formation and its evolution, and to the fundamental plasma processes at work both in it and beyond it. A comet nucleus emits gas as it is heated by the sunlight. The gas forms the coma
Externí odkaz:
http://arxiv.org/abs/1908.00377
Akademický článek
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Collisionless shocks are efficient particle accelerators. At Earth, ions with energies exceeding 100 keV are seen upstream of the bow shock when the magnetic geometry is quasi-parallel, and large-scale supernova remnant shocks can accelerate ions int
Externí odkaz:
http://arxiv.org/abs/1511.02077
The planetary exospheres are poorly known in their outer parts, since the neutral densities are low compared with the instruments detection capabilities. The exospheric models are thus often the main source of information at such high altitudes. We p
Externí odkaz:
http://arxiv.org/abs/1508.00426
Publikováno v:
Icarus, Volume 266, 1 March 2016, Pages 410-422
The planetary exospheres are poorly known in their outer parts, since the neutral densities are low compared with the instruments detection capabilities. The exospheric models are thus often the main source of information at such high altitudes. We p
Externí odkaz:
http://arxiv.org/abs/1503.08122
Publikováno v:
Icarus, Volume 266, 1 March 2016, Pages 410-422
The planetary exospheres are poorly known in their outer parts, since the neutral densities are low compared with the instruments detection capabilities. The exospheric models are thus often the main source of information at such high altitudes. We p
Externí odkaz:
http://arxiv.org/abs/1502.06701