论文标题
$4π$透视的科学案例：研究太阳风和太阳瞬变的演变和传播的极地/全球视图
The Science Case for the $4π$ Perspective: A Polar/Global View for Studying the Evolution & Propagation of the Solar Wind and Solar Transients
论文作者
论文摘要
To make progress on the open questions on CME/CIR propagation, their interactions and the role and nature of the ambient solar wind, we need spatially resolved coverage of the inner heliosphere -- both in-situ and (critically) imaging -- at temporal scales matching the evolutionary timescales of these phenomena (tens of minutes to hours), and from multiple vantage points.由于其提供了广泛的覆盖范围和独特的观点，因此极地有利是独特的。最终目标是到2050年实现太阳表面和气氛的全额$4π$。
To make progress on the open questions on CME/CIR propagation, their interactions and the role and nature of the ambient solar wind, we need spatially resolved coverage of the inner heliosphere -- both in-situ and (critically) imaging -- at temporal scales matching the evolutionary timescales of these phenomena (tens of minutes to hours), and from multiple vantage points. The polar vantage is uniquely beneficial because of the wide coverage and unique perspective it provides. The ultimate goal is to achieve full $4π$ coverage of the solar surface and atmosphere by 2050.
