Boltzmann-Kinetic studies of MHD-plasma properties near the solar wind termination shock and the heliosheath

为了描述等离子体-等离子体相互作用的情况下，像日光层界面在迄今为止的文献中，只有经典的磁流体动力学方法被使用。然而，这些，在许多方面失败，因为非理想的磁场行为和电荷交换引起的偏离假设的平衡分布函数不能考虑在这些磁流体的方法。在这个项目中，我们的目标是玻尔兹曼动力学控制目前讨论的日光层界面结构的MHD解决方案。我们计算动力学引起的非理想的介电常数和它们的违反所采用的理想冻结场的概念。我们还研究了等离子体粒子的动力学特性，在其弓激波或终止激波transition产生高度非弛豫，不稳定的分布函数，其中包含大量的自由能，它们驱动冲击产生的recipences。在这些研究中，我们还考虑到冲击等离子体物种的抗磁作用，在减少冲击后的磁场感应强度，这很可能可以解释最近观察到的令人惊讶的等离子体特性与遥远的太空探测器VOYAGER-1。我们还表明，电荷交换引起的非平衡分布函数实际上将与即将到来的空间任务，如IBEX观察，然后将给出非常有价值的提示，实际上正在进行的物理学在日光层界面。

To describe plasma-plasma interaction scenarios like the heliospheric interface in the up-to-now literature only classical magneto-hydrodynamic approaches are used. These, however, fail in many respects, since non-idealities in the magnetic field behaviour and charge-exchange induced deviations from the hypothesized equilibrium distribution functions cannot be taken into account in these magneto-fluid approaches. In this project we aim at a Boltzmann-kinetic controle on presently discussed MHD solutions for the heliospheric interface structures. We calculate kinetically induced non-ideal resistivities and their violation of the adopted ideal frozen-in field concept. We also study kinetic properties of plasma panicles at their bowshock or termination shock transititon producing highly non-relaxated, unstable distribution functions which contain substantial amounts of free energy by which they drive shock-generated turbulences. In these studies we also take into account the diamagnetic action of shocked plasma species in reducing the postshock magnitude of the magnetic field induction which most likely may explain the surprising plasma properties recently observed with the distant spaceprobe VOYAGER-1. We also show that charge-exchange induced non-equilibrium distribution functions will in fact be observable with upcoming space missions like IBEX and then will give extremely valuable hints to the actually ongoing physics in the heliospheric interface.