Model

We used the KEMPO1 [Omura and Matsumoto, 1993], which is a one-dimensional electromagnetic particle code. To make the essential physics clear, we further simplify the simulation model by eliminating electromagnetic part of the simulation code. Namely, we only solve Poisson's equation to obtain electrostatic fields the spatial profile of the charge density. We assume a one-dimensional space with the x-axis along which the static magnetic field is taken.

We assume three species of charged particles. Two electron beams and one ion beam. We assume these beams take densities n1, n2 and ni, respectively. The first electron beam with n1 take a drift velocity Vd/2, and the second electron beam with n2 and the ion beam with ni take a drift velocity -Vd/2. We take this frame of reference so that the maximum particle velocity in the simulation system becomes minimum, which gives a better numerical accuracy for a fixed time step \Delta t. It is noted that the frame of reference does not change the physics. We also assume these beams take shifted-Maxwellian velocity distributions with thermal velocities Ve for the electron beams and Vi for the ion beam, respectively.

The charge neutrality condition of the plasma gives, n1 + n2 = ni . In the following simulation runs, we varies the density n1 and n2 keeping ni constant. We define a density ratio R = n1/ni, and indicate it as a parameter of each simulation runs. Another parameter to be varied is the thermal velocity of the ion beam Vi, which control the Landau damping of the ion acoustic waves in the simulation system.

We list the fixed parameters for the simulation runs. Physical parameters are normalized to the initial electron thermal velocity and the electron plasma frequency.

The simulation system has a spatial scale of 1024 \lambdaD, where \lambdaD is the initial Debye length. We assume the periodic bounary condition for the simulation system. Since we assume a relatively warm ion beam, the thermal kinetic energy of the ion beam is the major energy in the system. To suppress the thermal fluctuations of the ion beam, we have to assign a much larger number of superparticles in the system. Otherwise, the thermal fluctuation due to a small number of superparticles may distroy the ESW. We varied the density ratio R from 0.1 to 1.0. When R=1.0, the model is reduced electron-ion stream model where Buneman instability is expected. For the thermal velocity of ions, we assume Vi = 0.1 and 2.0.