论文标题
下太阳大气中的高分辨率波动力学
High-resolution wave dynamics in the lower solar atmosphere
论文作者
论文摘要
太阳光球的磁性和对流性提供了一个独特的平台，可以从该平台上建模，观察和解释生成的波，并在空间和时间尺度的广度上进行建模。随着振荡是在原位产生的或通过光晶层出现的，迅速发展的密度，温度和磁场强度之间的相互作用可提供嵌入式波模式的动态演化，因为它们将它们传播到近似的太阳能层中。组装了一个重点的科学团队，以讨论较低太阳大气中波浪研究中当前面临的挑战，包括与光光学计和光学较厚区域中的辐射转移相关的挑战。在2020年2月在Chicheley Hall举行的Theo Murphy国际科学会议之后，该科学团队合作为当前的特刊提供了15个独立出版物，并在此处介绍。根据即将到来的下一代观察和高性能计算设施的含义，讨论了当前研究工作的含义。
The magnetic and convective nature of the Sun's photosphere provides a unique platform from which generated waves can be modelled, observed, and interpreted across a wide breadth of spatial and temporal scales. As oscillations are generated in-situ or emerge through the photospheric layers, the interplay between the rapidly evolving densities, temperatures, and magnetic field strengths provides dynamic evolution of the embedded wave modes as they propagate into the tenuous solar chromosphere. A focused science team was assembled to discuss the current challenges faced in wave studies in the lower solar atmosphere, including those related to spectropolarimetry and radiative transfer in the optically thick regions. Following the Theo Murphy international scientific meeting held at Chicheley Hall during February 2020, the scientific team worked collaboratively to produce 15 independent publications for the current Special Issue, which are introduced here. Implications from the current research efforts are discussed in terms of upcoming next-generation observing and high performance computing facilities.
