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Heliospheric Pickup Ions and Favored Acceleration Locations at the Termination Shock (FALTS): Are Voyager observations really inconsistent?

机译:终止休克(Falts)的终极拾取离子和有利的加速位置:航行员观察真的不一致吗?

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Pickup ions (PUIs) are created from a number of neutral sources both inside and outside the heiosphere. The combination of recent observational and theoretical work has completed the catalog of at least the major sources of Heliospheric PUIs. These PUIs are the seed population for anomalous cosmic rays (ACRs), which are accelerated to high energies at the termination shock (TS). Recently, Voyager 1 (V1) encountered strong intensity enhancements in the energy range where pickup ions are energized into ACRs. These observations may indicate that V1 has already passed beyond the TS into the bath of accelerated pickup ions in the inner heliosheath. However, opposing this conclusion, V1 magnetic field and higher energy particle observations appear very typical. Here, we advance the concept that V1 was in a special region in the heliosphere where the magnetic field is highly distorted due to solar wind shearing and footpoint motions at the Sun. These Favored Acceleration Locations at the Termination Shock (FALTS) efficiently inject pickup ions into diffusive shock acceleration due to slightly increased radial field components in the FALTS field regions. Such regions provide much more direct field-line connection to the TS than along strongly wound Parker field lines found outside of FALTS. Inside the TS, FALTS naturally enhance fluxes of accelerated pickup ions. Thus, FALTS may be responsible for the V1 observations of energetic particle enhancements. Further, FALTS provide a conduit for an inward electron heat flux from hot electrons beyond the TS, thereby heating the plasma and increasing the electron impact ionization rate. This additional ionization causes mass loading that locally weakens the TS and draws it in toward the Sun. Thus, FALTS can cause both energetic particle intensity enhancements and a weaker, locally drawn in TS; these effects may help explain the otherwise contradictory V1 observations.
机译:拾取离子(PUIS)是由机器内外的许多中性来源创建的。最近的观察和理论作品的结合已经完成了至少主要的Heliospheric Puis来源的目录。这些PUI是用于异常宇宙射线(ACRS)的种子群,其在终止冲击(TS)处加速到高能量。最近,Voyager 1(V1)在拾取离子通电的能量范围内遇到强度强度增强。这些观察结果可以表明V1已经超越TS进入内部Heliosheath中加速拾取离子的浴。然而,反对这一结论,V1磁场和更高的能量粒子观测非常典型。在这里,我们推进了V1在氦圈中的特殊区域中的概念,其中由于太阳风剪切和太阳的足部运动,磁场非常扭曲。这些有利于终止冲击(FALT)的加速位置有效地将拾取离子注入扩散离子,因为FALTS场区域中的径向场部件略微增加。这些区域提供了与TS的更直接的场线连接,而不是沿着Falts之外的强烈缠绕的帕克场线。在TS内部,生长自然增强加速拾取离子的助熔剂。因此,FALTS可能负责高能粒子增强的V1观察。此外,Falts为来自TS之外的热电子的向内电子热量提供了一种导管,从而加热等离子体并增加电子冲击电离率。这种额外的电离导致质量加载,局部削弱TS并将其朝向太阳落入太阳。因此,FALTS会导致能量粒子强度增强和较弱,在TS中征地;这些效果可能有助于解释其他矛盾的V1观察结果。

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