Results of calculations describing secondary-electron production and other inelastic processes in collisions of 1 to 25,000 keV/u S${}^{q+}$ ($q=-1\text{–}16$) with H${}_2$ are presented. These data complement previous results for the same processes in O${}^{q+}$ ($q=-1\text{–}8$) + H${}_2$ (Schultz et al. 2017, 2019) and for H${}^{q+}$ ($q=-\text{1,0,1}$) (Schultz et al. 2020). Used in ion-transport and secondary-electron simulations, these data provide a description of the atomic processes driven by these principal ions precipitating into the upper atmosphere of Jupiter, enabling better understanding the coupling of the Jovian magnetosphere, ionosphere, and atmosphere.

描述 1 到 25,000 keV/u S 碰撞中二次电子产生和其他非弹性过程的计算结果${}^{q+}$ ($q=-1\text{——}16$) 与 H${}_2$被提出。这些数据补充了 O 中相同过程的先前结果${}^{q+}$ ($q=-1\text{——}8$) + H${}_2$ (Schultz et al. 2017, 2019) 和 H${}^{q+}$ ($q=-\text{1,0,1}$)（舒尔茨等人，2020 年）。这些数据用于离子传输和二次电子模拟，描述了由这些主要离子沉淀到木星高层大气中驱动的原子过程，从而能够更好地了解木星磁层、电离层和大气的耦合。