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

用高能带电粒子研究太阳耀斑和太阳行星际现象

• 批准号: 9420790
• 负责人: John Simpson
• 金额: $ 26.5万
• 依托单位: University of Chicago
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1995
• 资助国家: 美国
• 起止时间: 1995-03-01 至 1997-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9420790&HistoricalAwards=false
• 关键词: Solar; Flare; Interplanetary; Phenomena; Investigated

This proposal is composed of both research and continued operations of the neutron monitors at Climax, Colorado and Haleakala, Hawaii. The motivation for research is to understand the physics of the electrodynamical processes in three dimensions in the inner heliosphere, with special emphasis on the solar-terrestrial region. In addition, the PIs will continue their long-term studies of the apparent bimodal character of cosmic ray modulation through the next solar minimum. Finally, the PIs wish to implement the continuation of the Climax and Haleakala neutron monitors extending into the solar minimum period with the same level of precision maintained over successive solar activity cycles.

这项建议包括科罗拉多的Climax和夏威夷的Haleakala的中子监测器的研究和继续运行。 研究的动机是了解日光层内部三维电动过程的物理学，特别强调日地区域。 此外，研究所将继续长期研究宇宙线调制在下一个太阳活动极小期期间的明显双峰特征。 最后，研究所希望继续使用Climax和Haleakala中子监测器，将其延伸到太阳活动极小期，并在连续的太阳活动周期中保持同样的精度。