用密度分布确定太阳的内部结构
The determination of the internal structure of the sun by the density distribution
摘要：
本文考察了几种能描述太阳引力稳定聚变反应堆的解析模型。一个分析多参数模型再现各种结构参数，如密度，质量，压力和温度在整个太阳能核心，这已经通过数值求解太阳能结构系统的微分方程。为了简单起见，数值和分析结果进行了详细讨论的两个参数模型。
英文摘要：
This paper examines a number of analytic models which can describe the gravitationally stabilized fusion reactor of the Sun. An analytical multiparameter model is shown to reproduce various structure parameters such as density, mass, pressure and temperature throughout the solar core, which have been obtained by solving numerically the system of solar structure differential equations. For simplicity, numerical and analytical results are discussed in detail for a two-parameter model.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
