Plasma Heating and Energy Transport During Solar Flares of Max '91

摘要：本研究旨在建立一个耀斑模型，该模型自洽地包含准静态场、电流和波粒相互作用，这对确定粒子动力学很重要。该模型将以早期研究微波和软、硬x射线发射的一些特征的工作为基础。该模型将能够预测基本的耀斑过程，包括耀斑发生的必要条件（例如磁场结构），耀斑电流系统和各种波长的耀斑发射的演变，包括微波和x射线。这些预测将根据观测结果进行检验，从而对观测结果进行更详细的分析，并更好地了解潜在的物理现象。＊＊＊

Abstract This proposed work seeks to develop a flare model which self-consistently incorporates the quasi-static fields, currents, and wave-particle interactions important in determining the particle dynamics. The model will be based on earlier work which has investigated some of the characteristics of microwave and soft and hard X-ray emissions. The model will be able to make predictions on basic flare processes, including the necessary conditions for flare onset (e.g. magnetic field configuration), the flare current system and the evolution of flare emissions at a variety of wavelengths, including microwaves and X-rays. These predictions will be tested against observations, allowing more detailed analysis of the observations and better insight into the underlying physics. ***