To be published in the proceeding of "Waves and Instabilities in Space and Astrophysical Plasmas" (WISAP) Eilat, Israel, June 19th - June 24th, 2011 "The acceleration of electrons at 1-10 keV energies is the cause of the polar aurora displays, and an important factor of magnetic energy transfer from the solar wind to the Earth. Two main families of acceleration processes are observed: those based on coherent quasi-static structures called double layers, and those based of the propagation of Alfvén Waves (AW). This paper is a review of the Alfvénic acceleration processes, and of their role in the global dynamics of the auroral zone
International audienceWith the help of a 2.5-D particle-in-cell simulation code, we investigate the ...
International audienceThe Alfvén mission will explore particle acceleration processes and their cons...
[1] In a recent work [Wu, 2003a, 2003b], a dissipative nonlinear inertial Alfvén wave (DNIAW) were ...
To be published in the proceeding of "Waves and Instabilities in Space and Astrophysical Plasmas" (W...
To be published in the proceeding of "Waves and Instabilities in Space and Astrophysical Plasmas" (W...
Abstract. The acceleration of electrons at 1-10 keV energies is the cause of the polar aurora displa...
Proceeding of the SF2A conference in Nice, 2012.In the Earth auroral zone, the electron acceleration...
Proceeding of the SF2A conference in Nice, 2012.In the Earth auroral zone, the electron acceleration...
The aurorae are dynamic, luminous displays that grace the night skies of Earth’s high latitude regio...
The aurorae are dynamic, luminous displays that grace the night skies of Earth’s high latitude regio...
International audienceDispersive Alfvén wave activity is identified in four dayside auroral oval eve...
International audienceIt is shown that two circularly polarised Alfvén waves that propagate along th...
International audienceWith the help of a 2.5-D particle-in-cell simulation code, we investigate the ...
International audienceIt is shown that two circularly polarised Alfvén waves that propagate along th...
Abstract. In the Earth auroral zone, the electron acceleration by Alfvén waves is sometimes a precu...
International audienceWith the help of a 2.5-D particle-in-cell simulation code, we investigate the ...
International audienceThe Alfvén mission will explore particle acceleration processes and their cons...
[1] In a recent work [Wu, 2003a, 2003b], a dissipative nonlinear inertial Alfvén wave (DNIAW) were ...
To be published in the proceeding of "Waves and Instabilities in Space and Astrophysical Plasmas" (W...
To be published in the proceeding of "Waves and Instabilities in Space and Astrophysical Plasmas" (W...
Abstract. The acceleration of electrons at 1-10 keV energies is the cause of the polar aurora displa...
Proceeding of the SF2A conference in Nice, 2012.In the Earth auroral zone, the electron acceleration...
Proceeding of the SF2A conference in Nice, 2012.In the Earth auroral zone, the electron acceleration...
The aurorae are dynamic, luminous displays that grace the night skies of Earth’s high latitude regio...
The aurorae are dynamic, luminous displays that grace the night skies of Earth’s high latitude regio...
International audienceDispersive Alfvén wave activity is identified in four dayside auroral oval eve...
International audienceIt is shown that two circularly polarised Alfvén waves that propagate along th...
International audienceWith the help of a 2.5-D particle-in-cell simulation code, we investigate the ...
International audienceIt is shown that two circularly polarised Alfvén waves that propagate along th...
Abstract. In the Earth auroral zone, the electron acceleration by Alfvén waves is sometimes a precu...
International audienceWith the help of a 2.5-D particle-in-cell simulation code, we investigate the ...
International audienceThe Alfvén mission will explore particle acceleration processes and their cons...
[1] In a recent work [Wu, 2003a, 2003b], a dissipative nonlinear inertial Alfvén wave (DNIAW) were ...