Solar Flare and Solar-Interplanetary Phenomena Investigated with High-Energy Charged Particles

这项研究旨在继续实验和 大尺度动力学现象的分析研究 太阳极区磁场产生的日球层 极性反转，并研究太阳耀斑带电粒子 在当前的太阳周期中加速。 第一个目标 将把重点放在带电粒子上， 磁场，其起源是太阳磁场携带 在日光层中被太阳风吹走第二 目标将包括太阳能的实验研究 利用能量测量的耀斑粒子加速 太阳光谱和元素及同位素组成 从航天器数据中获得的耀斑。 这两个目标将 需要广泛使用中子监测器和来自 几个航天器上的仪器网络。拟议 因此，研究将包括持续运作和 维持Climax、CO和 秘鲁万卡约，可能在 毛伊岛，夏威夷。后一个站最终将取代 在秘鲁。

This investigation is designed to continue experimental and analytical studies of the large scale dynamical phenomena in the heliosphere resulting from the solar polar magnetic field polarity reversals , and to study solar flare charged particle acceleration in the present solar cycle. The first objective will focus on charged particles as probes of heliospheric magnetic fields, whose origin is the solar magnetic field carried throughout the heliosphere by the solar wind. The second objective will consist of experimental investigations for solar flare particle acceleration using measurements of the energy spectrum and elemental and isotopic composition of the solar flares obtained from spacecraft data. Both objectives will require extensive use of neutron monitors and of data from a network of instruments aboard several spacecraft. The proposed research will therefore include continued operation and maintenance of neutron monitoring stations at Climax, CO and Huancayo, Peru, with the possible addition of a new station in Maui, Hawaii. This latter station will eventually replace the one in Peru.