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SOHO CTOF Observations of Interstellar He~+ Pickup Ion Enhancements in Solar Wind Compression Regions

机译:SOHO CTOF INTERTELLAR HE〜+拾取离子增强在太阳风压缩区域

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We present a recent analysis with 1996 SOHO CELIAS CTOF data, which reveals correlations of He~+ pickup ion fluxes and spectra with the magnetic field strength and solar wind density. The motivation is to better understand the ubiquitous large variations in both pickup ion fluxes and their velocity distributions found in interstellar pickup ion datasetts. We concentrate on time periods of that can be associated with compression regions in the solar wind. Along with enhancements of the overall pickup ion fluxes, adiabatic heating and acceleration of the pickup ions are also observed in these regions. Transport processes that lead to the observed compressions and related heating or acceleration are discussed. A shift in velocity space associated with traveling interplanetary compression regions is observed, and a simple model presented to explain this phenomenon based on the conserved magnetic adiabatic moment.
机译:我们最近展示了1996年SOHO Celias CTOF数据的分析,揭示了He〜+拾取离子通量和光谱与磁场强度和太阳能密度的相关性。动机是更好地了解拾取离子助焊剂的无处不在的大变化及其在星际拾取离子数据素中发现的速度分布。我们专注于时间段,可以与太阳风中的压缩区域相关联。随着整体拾取离子助熔剂的增强,在这些区域中也观察到拾取离子的绝热加热和加速度。讨论了导致观察到的按压和相关加热或加速度的运输过程。观察到与行驶截然型压缩区域相关联的速度空间的换档,并且提出了一种基于保守的磁绝热时刻来解释这种现象的简单模型。

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