Bingham, R. and Bamford, R. and Kellett, B. J. and Shapiro, V. D. (2010) Electron energization in lunar magnetospheres. Journal of Plasma Physics, 76 (6). pp. 915-918. ISSN 0022-3778Full text not available in this repository. (Request a copy from the Strathclyde author)
The interaction of the solar wind with lunar surface magnetic fields produces a bow shock and a magnetosphere-like structure. In front of the shock wave energetic electrons up to keV energies are produced. This paper describes how resonant interactions between plasma turbulence in the form of lower-hybrid waves and electrons can result in field aligned electron acceleration. The turbulent wave fields close to the lower-hybrid resonant frequency are excited most probably by the modified two-stream instability, driven by the solar wind ions that are reflected and deflected by the low shock.
|Keywords:||plasma turbulence, lower-hybrid waves, electrons, field aligned electron acceleration, turbulent wave fields, solar wind ions, frequency, Plasma physics. Ionized gases, Condensed Matter Physics|
|Subjects:||Science > Physics > Plasma physics. Ionized gases|
|Department:||Faculty of Science > Physics|
|Depositing user:||Pure Administrator|
|Date Deposited:||07 Mar 2011 23:21|
|Last modified:||22 Mar 2017 11:15|