A comprehensive set of calculations of the radiative losses of solar coronal plasmas is presented. The Los Alamos suite of atomic structure and collision codes is used to generate collisional data for 15 coronal elements. These data are used in the Los Alamos plasma kinetics code ATOMIC to compute the radiative power loss as a function of electron temperature. We investigate the sensitivity of the loss curves to the quality of the atomic data and changes in the coronal elemental abundances, and we compare our results with previous work.
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机译：提出了一套完整的太阳日冕等离子体辐射损失的计算方法。 Los Alamos的原子结构和碰撞代码套件用于生成15个冠状元素的碰撞数据。这些数据用于洛斯阿拉莫斯等离子体动力学代码ATOMIC中，以计算作为电子温度的函数的辐射功率损耗。我们研究了损耗曲线对原子数据质量和日冕元素丰度变化的敏感性，并将我们的结果与以前的工作进行了比较。
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