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

ATM 9912341 abs研究人员将使用中子监测器和IMP-8航天器上的其他仪器的数据进行研究，并继续由Climax和Huancayo山宇宙辐射中子站进行精确观测。 研究重点将是三维日光层中的带电粒子传播模式，以及太阳耀斑和日冕物质抛射中的带电粒子加速现象。 研究人员将利用这些数据，研究在太阳高纬度地区观测到的宇宙射线强度的周期性26天调制。 他们还将展示在太阳粒子事件期间如何直接探测太阳中子，以提供有关粒子加速机制的信息。 这一支持将使地面台站47年来的宇宙射线观测记录得以延续。

ATM9912341absThe investigators will conduct research using data from neutron monitors and other instruments on the Ulysses and IMP-8 spacecraft, and continue precision observations by the Climax and Huancayo Mountain cosmic radiation neutron stations. The research will focus on charged particle modes of propagation in the three-dimensional heliosphere, and charged particle acceleration phenomena in solar flares and coronal mass ejections. Using the Ulysses data, the investigators will study the recurrent 26-day modulation in cosmic ray intensity observed at high solar latitudes. They will also show how direct solar neutron detection during solar particle events provide information about particle acceleration mechanisms. The support will allow continuation of the 47 year record of cosmic ray observations from ground-based stations.