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

ATM9912341调查人员将使用Ulysses和IMP-8航天器上的中子监测器和其他仪器的数据进行研究，并继续由Topax和环卡约山宇宙辐射中子站进行精确观测。这项研究将集中在三维日球层中带电粒子的传播模式，以及太阳耀斑和日冕物质抛射中的带电粒子加速现象。利用尤利西斯的数据，研究人员将研究在高太阳纬度观测到的宇宙线强度的26天周期性调制。他们还将展示太阳粒子事件期间的直接太阳中子探测如何提供有关粒子加速机制的信息。这项支持将使地面站47年来的宇宙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.