scholarly journals Analytic model for electromagnetic fields in the bubble regime of plasma wakefield in non-uniform plasmas

2017 ◽  
Vol 24 (10) ◽  
pp. 103104 ◽  
Author(s):  
A. A. Golovanov ◽  
I. Yu. Kostyukov ◽  
J. Thomas ◽  
A. Pukhov
2014 ◽  
Vol 32 (2) ◽  
pp. 277-284 ◽  
Author(s):  
J. Thomas ◽  
A. Pukhov ◽  
I.Yu. Kostyukov

AbstractAn extended analytical model for particle dynamics in fields of a highly-nonlinear plasma wakefield (the bubble or blow out regime) is derived. A recently proposed piecewise model is generalized to include a time dependent bubble radius and full field solution in the acceleration direction. Incorporation of the cavity dynamics in the model is required to simulate the particle trapping properly. On the other hand, it is shown that the previously reported piecewise model does not reproduce the formation of a mono energetic peak in the particle spectrum. The mono energetic electron beams are recovered only when the full longitudinal field gradient is included in the model.


2019 ◽  
Author(s):  
Roberto Manuzzo ◽  
Francesco Califano ◽  
Gerard Belmont ◽  
Laurence Rezeau

Abstract. Observation of the solar wind – magnetosphere boundary provides a unique opportunity to investigate the physics underlying the interaction between two collisionless magnetized plasmas with different temperature, density and magnetic field topology. Their mixing across the interface as well as the boundary dynamics are affected by the development of fluid (and kinetic) instabilities driven by large scale inhomogeneities in particle and electromagnetic fields. Building up a realistic initial equilibrium state of the magnetopause according to observations is still a challenge nowadays. In this paper we address the modeling of the particles and electromagnetic fields configuration across the Earth's magnetopause by means of a three-fluid analytic model. The model relies on one hot and one cold ion population and on a neutralizing electron population. The goal is to build up an analytic model able to reproduce as closely as possible the observations. Some parameters of the model are set by using a fit procedure aiming at minimizing their difference with respect to experimental data provided by the Magnetospheric MultiScale mission. All the other profiles, concerning the electron pressure and the relative densities of the cold and hot ion populations, are calculated in order to satisfy the fluid equilibrium equations. Finally, by means of a new tri-fluid code, we have checked the stability of the large-scale equilibrium model for a given experimental case and given the proof that the system is unstable to reconnection. This model could be of interest for the interpretation of satellite results and for the study of the dynamics at the boundary between the Magnetosphere and the solar wind.


2018 ◽  
Vol 25 (10) ◽  
pp. 103107 ◽  
Author(s):  
A. A. Golovanov ◽  
I. Yu. Kostyukov

Author(s):  
Vadim Khudiakov ◽  
Konstantin V Lotov ◽  
Mike Downer

Abstract In plasma wakefield accelerators, the wave excited in the plasma eventually breaks and leaves behind slowly changing fields and currents that perturb the ion density background. We study this process numerically using the example of a FACET experiment where the wave is excited by an electron bunch in the bubble regime in a radially bounded plasma. Four physical effects underlie the dynamics of ions: (1) attraction of ions toward the axis by the fields of the driver and the wave, resulting in formation of a density peak, (2) generation of ion-acoustic solitons following the decay of the density peak, (3) positive plasma charging after wave breaking, leading to acceleration of some ions in the radial direction, and (4) plasma pinching by the current generated during the wavebreaking. Interplay of these effects result in formation of various radial density profiles, which are difficult to produce in any other way.


2013 ◽  
Vol 20 (1) ◽  
pp. 013108 ◽  
Author(s):  
S. A. Yi ◽  
V. Khudik ◽  
C. Siemon ◽  
G. Shvets

2007 ◽  
Vol 14 (7) ◽  
pp. 073103 ◽  
Author(s):  
Bai-Song Xie ◽  
Hai-Cheng Wu ◽  
Hongyu Wang ◽  
Nai-Yan Wang ◽  
M. Y. Yu

2005 ◽  
Vol 24 (1) ◽  
pp. 2-10 ◽  
Author(s):  
Kenneth F. Taylor ◽  
Nozumu Inoue ◽  
Bahman Rafiee ◽  
John E. Tis ◽  
Kathleen A. McHale ◽  
...  

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