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A non-equilibrium Alfvénic state of the Langevin system for single particles reproduces the linear relation between the cross helicity and the residual energy in the solar wind

机译:单颗粒的Langevin系统的非平衡alfvénic状态再现了太阳风中的十字螺旋和残余能量之间的线性关系

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As a minimal phenomenological model of unidirectional Alfvénic fluctuations in the solar wind, a non-equilibrium Alfvénic state (NAS) in the Langevin system for single particles is studied. The NAS is a nonequilibrium steady state of the Langevin system including both friction force and random force. It is shown that the overdamped Langevin system gives the NAS without the assumption of the monochromatic wave. The resultant NAS gives the relationship between the energy dissipation rate, the cross-helicity, and the residual energy with a single phenomenological parameter. It is shown that the energy dissipation rate can be evaluated using the non-equilibrium work, which satisfies the fluctuation dissipation-like relation.
机译:作为太阳风中的单向Alfvénic波动的最小现象学模型,研究了单颗粒的Langevin系统中的非平衡Alfvénic状态(NAS)。 NAS是Langevin系统的非QuibiRimibrium稳定状态,包括摩擦力和随机力。 结果表明,覆盖的Langevin系统给出了没有假设单色波的NAS。 所得NAS具有单一现象学参数的能量耗散速率,交叉螺旋性和残余能之间的关系。 结果表明,可以使用不平衡工作来评估能量耗散速率,这满足了波动耗散的关系。

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