Space Weather: Numerical Magnetohydrodynamics (MHD) Study of Coronal Mass Ejections (CMEs): Initiation and Propagation

一个为期三年的研究计划，追求的目标是使用数值磁流体动力学（MHD）模型和观测，以加强太阳日冕物质抛射（CME）的启动和传播。 这项活动有两个组成部分：㈠研究太阳喷发现象的基本物理学，特别是日冕物质抛射的起始过程和传播，㈡预测对太阳-行星际-磁层耦合研究很重要的扰动太阳风参数。 这项工作的总体目标是为开发基于科学的空间气象预测模型奠定基础。

A three-year research program is pursued with the goal of using numerical magnetohydro-dynamic (MHD) models and observations to sturdy the initiation and propagation of solar coronal mass ejections (CMEs). There are two components to this activity, (i) to study the fundamental physics of solar eruptive phenomena, specifically the CME initiation process and propagation, and (ii) to predict the disturbed solar wind parameters which are important to solar-interplanetary-magnetosphere coupling studies. The overarching objective of this work is to lay the foundation for the development of a science-based space weather predictive model.