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首页> 外文期刊>Astronomy and astrophysics >Suprathermal helium in corotating interaction regions: combined observations from SOHO/CELIAS/STOF and ACE/SWICS
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Suprathermal helium in corotating interaction regions: combined observations from SOHO/CELIAS/STOF and ACE/SWICS

机译:在卡切相互作用区域中的同龄氦气:来自SOHO / Celias / Stof和ACE / SWIC的组合观察

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Context. Energetic particle enhancements that are associated with corotating interaction regions (CIRs) are typically believed to arise from the sunward propagation of particles that are accelerated by CIR-driven shocks beyond 1 AU. It is expected that these sunward-travelling particles will lose energy and scatter, resulting in a turnover of the energy spectra below ~ 0.5 MeV/nuc. However, the turnover has not been observed so far, suggesting that the CIR-associated low-energy suprathermal ions are accelerated locally close to the observer. Aims. We investigate the variability of suprathermal particle spectra from CIR to CIR as well as their evolution and variation as the observer moves away from the rear shock or wave. Methods. Helium data in the suprathermal energy range from the Solar and Heliospheric Observatory/Charge, Element, and Isotope Analysis System/Suprathermal Time-of-Flight (SOHO/CELIAS/STOF) were used for the spectral analysis and were combined with data from the Advanced Composition Explorer/ Solar Wind Ion Composition Spectrometer (ACE/SWICS) in the solar wind energies. Results. We investigated sixteen events: nine clean CIR events, three CIR events with possible contamination from upstream ion events or solar energetic particles (SEPs), and four events that occurred during CIR periods that were dominated by SEPs. Six of the nine clean CIR events showed possible signs of a turnover between ~ 10 ? 40 keV/nuc in the fast solar wind that trails the compression regions. Three of them even showed this behaviour inside the compressed fast wind. The turnover part of the spectra became flatter and shifted from lower to higher energies with increasing connection distance to the reverse shock. The remaining three clean events showed continuous power-law spectra in both the compressed fast wind and fast wind regions, that is, the same behaviour as reported from previous observations. The spectra of the seven remaining events are more variable, that is, they show power law, turnover, and a superposition of these two shapes.
机译:语境。与卡托基相互作区(CIR)相关联的能量粒子增强通常被认为是从通过CIR驱动的冲击超出1 AU加速的颗粒的向阳传播而产生。预计这些阳光行驶颗粒将失去能量和散射,导致能量光谱的换档低于约0.5mev / nuc。然而,到目前为止尚未观察到营业额,表明Cir相关的低能量上班子离子在局部接近观察者局部地加速。目标。我们调查来自CIR的Suprathermal粒子光谱的可变性以及它们的进化和变化,因为观察者远离后冲击或波浪。方法。 Suprathermal能量范围内的氦气数据从太阳能和光纤观测所/电荷,元素和同位素分析系统/上班牙飞行时间(SOHO / Celias / stof)用于光谱分析,并与先进的数据相结合在太阳风能中的组成探险器/太阳能管离子组成光谱仪(ACE / SWICS)。结果。我们调查了十六次活动:九个清洁赛事件,三个CIR事件,来自上游离子事件或太阳能粒子(SEP)的可能污染,以及在SEPS主导的CIR期间发生的四个事件。六个九个干净的事件中的六个事件显示了〜10之间的成交量的迹象?快速太阳风中的40 kev / nuc,落后压缩区域。其中三个甚至在压缩的快速风中展示了这种行为。光谱的周转部分变得更平坦,从较低的能量转移到更高的能量,随着与反向冲击的增加。剩下的三种清洁事件在压缩的快风和快速风区域中显示出连续的功率法谱,即与先前观察结果报告的相同行为。七个剩余事件的光谱是更具变量,即它们显示电力法,周转,以及这两个形状的叠加。

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