论文标题
CME加速度作为冠状磁场的探针
CME Acceleration as a Probe of the Coronal Magnetic Field
论文作者
论文摘要
到2050年，我们预计CME模型将准确地描述并理想地预测，观察到的太阳喷发和CME通过电晕传播。我们描述了在观察和模型中需要解决的一些已知未知数，以实现这一目标。我们还描述了如何为一些肯定会成为挑战的未知未知数做准备。
By 2050, we expect that CME models will accurately describe, and ideally predict, observed solar eruptions and the propagation of the CMEs through the corona. We describe some of the present known unknowns in observations and models that would need to be addressed in order to reach this goal. We also describe how we might prepare for some of the unknown unknowns that will surely become challenges.
