ICME Structure and Evolution in the Inner Heliosphere

Adam Szabo, George C. Ho, Lan K. Jian, David Lario, Teresa Nieves-Chinchilla
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Abstract

Synapsys : Interplanetary Coronal Mass Ejections (ICMEs) have been studied for decades using various methods and observational tools; however, their internal structure, transport and evolution in the inner heliosphere remains poorly understood. Similarly, the transport and diffusion of solar energetic particles on their way to 1 AU is surrounded by controversy. This white paper outlines possible next research objectives and a possible multi-spacecraft mission concept (HELIIX) that would provide the measurements to achieve these objectives.
内日球层ICME结构与演化
行星际日冕物质抛射(ICMEs)已经用各种方法和观测工具研究了几十年;然而,它们的内部结构、内部日球层的运输和演化仍然知之甚少。类似地,太阳高能粒子向1天文单位运动的输运和扩散也存在争议。这份白皮书概述了可能的下一个研究目标和一个可能的多航天器任务概念(HELIIX),它将为实现这些目标提供测量。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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