用电感耦合等离子体炬研究火星和土卫六大气的理论方法的第一步
First Step in Theoretical Approach in Study of Mars and Titan Atmospheres with an Inductively Coupled Plasma Torch
摘要：
为了获得可以用作测试案例的ICP炬的建模，我们必须确定所有的热力学性质和传输系数。为了计算数据，我们必须首先确定所有物种的组成和碰撞积分，以计算输运系数。我们将计算应用于火星和土卫六的大气成分。测定谱线的强度与温度的关系。
英文摘要：
To obtain the modelling of an ICP torch that can be used as a test case, we have to determine all the thermodynamic properties and transport coefficients. To calculate the data we have first to determine the composition and the collisions integrals for all the species in the purpose to calculate the transport coefficients. We apply the calculation to the Mars and to the Titan atmosphere compositions. The intensities of the spectral lines are determined versus temperature.
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。
