Mathematical modelling of solar plasma jets

学生i)我将把对更大的，所谓的宏观针状射流的分析推广到更普遍的小射流（称为针状）和更大的射流（称为涌流），以便对这些现象有更广泛的能谱。研究人员将调查这些太阳喷流是否遵循柯尔莫哥洛夫分布。关于太阳喷射能谱性质的结论性陈述将是该领域的一次飞跃，具有更广泛的影响。Ii)还将建立旋转磁性龙卷风（即旋转射流）的数学（分析）模型，并用收集到的数据验证该模型。Iii)最后，学生将进行旋转射流的稳定性分析，这是太阳和一般等离子体天体物理学领域的一个活跃研究领域。我们预计目前被广泛接受的不稳定性阈值将被修订，使学生在该领域产生另一个引人注目的（更理论化的）影响。

The Student i) I will generalise the analyses of larger, so-called macro-spicule, jets to the much more ubiquitous small jets (called spicules) and much larger jets (called surges) i order to have a wide range of energy spectrums of these phenomena. Study will be conducted to investigate whether these solar jets follow a Kolmogorov distributions. A conclusive statement on the nature of the solar jet energy spectrum would be a leap in the field with wider impacts. ii) will also build a mathematical (analytical) model of rotating magnetic tornadoes (i.e rotating jets) and validate the modelling with the gathered data. Iii) Finally, the student will carry out stability analysis of rotating jets that is an active area of research in the field of solar and general plasma astrophysics. We anticipate that the currently widely accepted instability threshold will be revised enabling the student to have another high-profile (more theoretical) impact in the field.