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Delay in Onset Times of Solar Energetic Particles

机译:太阳高能粒子起效时间的延迟

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Onset analysis is a commonly used method in studying Solar Energetic Particles (SEPs). One can use the linear dispersion relation between the onset time and the reciprocal of particle speed to determine the length of the connecting magnetic field line or time of injection. This is true if the SEP have travelled nearly scatter free at nearly zero pitch angle along the path it travelled. It is important to determine the the time of injection and location of the SEP release at the Sun. Using a particle transport model we study the effect of scattering in the determination of SEP onsets. Using different levels of scattering we find the delays of energetic particles as they arrive at Earth. These delays will affect the correct determination of time of injection and distance travelled.
机译:发作分析是研究太阳高能粒子(SEPs)的常用方法。可以使用开始时间与粒子速度的倒数之间的线性色散关系来确定连接磁场线的长度或注入时间。如果SEP沿其行进路径几乎以零螺距角自由行进,则情况如此。确定注射时间和SEP在太阳上释放的位置非常重要。使用粒子传输模型,我们研究了散射在SEP发作确定中的作用。使用不同程度的散射,我们发现了高能粒子到达地球时的延迟。这些延迟将影响对喷射时间和行进距离的正确确定。

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