论文标题
部分可观测时空混沌系统的无模型预测
Solar rotation elements $i, Ω$ and period determined using sunspot observations by Ruđer Bošković in 1777
论文作者
论文摘要
RuelerBošković开发了确定太阳旋转元件的方法：太阳赤道倾斜度I，节点ω的经度和太阳旋转周期。 1785年出版的《 Optionia et opticam et opertinia》在他的最后一部作品中，于1785年发表，在《 OpuScule II》一章中描述了他的方法，他的方法，具有图形描述的公式，以及用于计算太阳旋转元素的示例，并使用他自己的观察值在1777年9月进行了详细的数值解释。在目前的工作中，我们对R.Bošković的原始结果进行了描述，并将其与我们的重新计算值进行了比较。
Ruđer Bošković developed methods for determination of solar rotation elements: the solar equator inclination i, the longitude of the node Ω and the period of solar rotation. In his last work Opera pertinentia ad opticam et astronomiam, published in 1785, in the chapter Opuscule II he described his methods, the formulae with figure descriptions and an example for calculation of the solar rotation elements with detailed numerical explanation using his own observations performed in September 1777. The original numerical procedure was performed using logarithmic formulae. In present work we give a description of the original results of R. Bošković and compare them with our recalculated values.
