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The Observational Aspects of the Three Largest Solar-Energetic Particle Fluxes:19-20/10/1989,14/7/2000 and 9/11/2000

机译:三大太阳能粒子通量的观察方面:19-20 / 10 / 1989,14 / 7/2000和9/11/2000

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摘要

The study of the largest solar energetic particle (SEP) events gives important information about the physical process in the solar corona and in the heliosphere.The hourly solar energetic particles and interplanetary (IP) and geomagnetic measurements of the three largest SEP events have been compared.The results indicate that there is a quite different in IP and geomagnetic disturbances and in turn,the mechanism of particle accelerations among the three events.The acceleration of fluxes was not a function of the IP shock's efficiency.The IP shock was hardly deteriorated in its path to the Earth.Different dynamics structures in the heliosphere during the considered events,have been found.
机译:最大的太阳能粒子(SEP)事件的研究为太阳能电晕和幽光圈​​的物理过程提供了重要信息。每小时的太阳能粒子和星际(IP)和地磁测量的三个最大的SEP事件进行了比较。结果表明,IP和地磁干扰的存在非常不同,又有三种事件中的粒子加速机制。势倍的加速不是IP休克效率的函数。IP休克几乎没有恶化它已经找到了它的地球的路径。已经发现了在考虑的事件中的氦圈中的不同动态结构。

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