论文标题
在太阳能颗粒中添加氢气的元素丰度模式的优点
Virtues of Including Hydrogen in the Patterns of Element Abundances in Solar Energetic Particles
论文作者
论文摘要
我们在2012年1月23日的事件中重新审视了太阳能颗粒（SEP）元素丰度（SEP）的多空间研究，其中增强的幂律模式与FE元素C的质量与电荷比A/Q的质量A/Q在MED接近MG的突破中部分中断了，这是不幸的分散分散的。在当前的文章中，我们发现将最小二乘适合C -Fe的最小二乘在A/Q = 1时将其扩展到H，即使H本身并未包含在拟合中，也可以对Power Laws有更多的信任。在此事件中，我们还研究了冲击波后面磁性颗粒的绝热“储层”的程度。
We revisit a multi-spacecraft study of the element abundances of solar energetic particles (SEPs) in the 23 January 2012 event, where the power-law pattern of enhancements versus the mass-to-charge ratio A/Q for the elements C through Fe was partly disrupted by a break near Mg, which turned out to be an unfortunate distraction. In the current article we find that extending that least-squares fits for C - Fe down to H at A/Q = 1 lends much more credence to the power laws, even though H itself was not included in the fits. We also investigate the extent of an adiabatically invariant "reservoir" of magnetically-trapped particles behind the shock wave in this event.
