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Electron temperature, electron heat flux and corresponding charge density. (a) Case 2B (m i =m e ¼ 100) at x pe0 t ¼ 200. (b) Case 2B (m i =m e ¼ 100) at x pe0 t ¼ 400.

Electron temperature, electron heat flux and corresponding charge density. (a) Case 2B (m i =m e ¼ 100) at x pe0 t ¼ 200. (b) Case 2B (m i =m e ¼ 100) at x pe0 t ¼ 400.

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Article
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Grid-based Vlasov simulations are carried out to re-evaluate the one-dimensional collisionless plasma expansion into vacuum. The grid-based method eliminates the inherent statistical noise in particle-based methods and allows us to extend the solution beyond the self-similar expansion region and resolve small electron timescale wave perturbations....

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Context 1
... w ¼ v x À hv x i is the random electron velocity and ~ w ¼ w=v te0 . Figure 7 further correlates ~ T e ð~ xÞ, with the local electron heat flux ~ Q e ð~ xÞ, and the space charge density ~ n i ð~ xÞ À ~ n e ð~ xÞ for case 2B. Here, the electron heat flux ~ Q e ð~ xÞ is calculated from ...
Context 2
... the left-side boundary of region B propagates toward the upstream at the same speed as the group velocity of the electron Langmuir wave, ~ v ele g . Thus, the left boundary of region B coincides with that of the electron Langmuir wave front given by Eq. (25), ~ x ele À ð ~ tÞ ¼ À~ v ele g Á ~ t, and the location of region B is defined by À~ v ele Fig. 7 also shows that, while the plasma is overall quasi-neutral during the expansion process, there are small density oscillations on the electron timescale upstream of the expansion front. These small density oscillations correspond to the perturbations caused by the electron Langmuir wave. In region B, the electron temperature decreases ...
Context 3
... front does not affect those electrons that leave the bulk plasma at the start of the expansion but attracts some of the electrons to backflow during subsequent expansion. The stream of the backflow electrons creates the peak in the electron VDF in region D. This peak corresponds to the temperature enhancement shown in the ~ T e ð~ xÞ profile in Fig. 7. As the electron VDF at the expansion front does not spread out but has a non-Maxwellian component, the electron temperature will be estimated high from Eq. ...
Context 4
... The energy lost by the electrons sustains the propagation of the electron Langmuir wave. This resonant wave-particle interaction depletes the number of electrons with a velocity at ~ v $ À~ v ele g . Behind the wave front, the void in the electron VDF is gradually refilled. This leads to the slight decrease in ~ T e in region B as observed in Fig. 7. Previously, Medvedev 42 showed that an ion "cooling" wave with a spatial size much longer than the rarefaction wave perturbed region exists in the ion-ion plasma expansion. It was also speculated that the cooling observed should also exist FIG. 8. Local electron velocity distribution functions (VDFs) at selected locations for case 2B ...

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