A Model of Double Coronal Hard X-Ray Sources in Solar Flares

@article{Kong2022AMO,
  title={A Model of Double Coronal Hard X-Ray Sources in Solar Flares},
  author={Xiangliang Kong and Jing Ye and Bin Chen and Fan Guo and Chengcai Shen and Xiaocan Li and Sijie Yu and Yao Chen and Joe Giacalone},
  journal={The Astrophysical Journal},
  year={2022},
  volume={933}
}
A number of double coronal X-ray sources have been observed during solar flares by RHESSI, where the two sources reside at different sides of the inferred reconnection site. However, where and how these X-ray-emitting electrons are accelerated remains unclear. Here we present the first model of the double coronal hard X-ray (HXR) sources, where electrons are accelerated by a pair of termination shocks driven by bidirectional fast reconnection outflows. We model the acceleration and transport of… 

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