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THEORETICAL MODEL IMAGES AND SPECTRA FOR COMPARISON WITH RHESSI AND MICROWAVE OBSERVATIONS OF SOLAR FLARES

机译:与rhesi和太阳耀斑的微波观测相比的理论模型图像和光谱

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We have computed bremsstrahlung and gyrosynchrotron images and spectra from a model flare loop. Electrons with a power-law energy distribution are continuously injected at the top of a semicircular magnetic loop. The Fokker-Planck equation is integrated to obtain the steady-state electron distribution throughout the loop. Coulomb scattering and energy losses and magnetic mirroring are included in the model. The resulting electron distributions are used to compute the radiative emissions. Sample images and spectra are presented here. We are developing these models for the interpretation of RHESSI x-ray/gamma-ray data and coordinated microwave observations.
机译:我们从模型闪光环中计算了Bremsstrahlung和Gyrosynchrotron图像和光谱。具有动力 - 法能量分布的电子在半圆形磁环顶部连续注入。集成了Fokker-Planck方程以获得整个环路的稳态电子分布。模型中包含库仑散射和能量损失和磁性镜像。所得到的电子分布用于计算辐射发射。此处提出了样本图像和光谱。我们正在开发这些模型,以解释RhesiSi X射线/伽马射线数据和协调的微波观察。

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