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

摘要 这项拟议的工作旨在开发一个耀斑模型， 自洽地结合了准静态场，电流， 以及波粒相互作用对确定 粒子动力学 该模型将基于早期的工作， 研究了微波的一些特性， 软X射线和硬X射线发射。 这个模型将能够 对基本耀斑过程的预测，包括必要的 耀斑爆发的条件（如磁场配置）， 耀斑电流系统和耀斑排放的演变. 包括微波和X射线。 这些 预测将根据观察进行测试，允许更多 详细分析观察结果，更好地了解 基础物理学***

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. ***