Engineering-Level Model Atmospheres for Titan and Neptune
Engineering-Level Model Atmospheres for Titan and Neptune
复制标题
泰坦和海王星的工程级模型大气
DOI：
10.2514/6.2003-4803
复制
发表时间：
2003
期刊：
影响因子：
--
通讯作者：
Dale L. Johnson
中科院分区：
文献类型：
--
作者：
C. Justus;A. Duvall;Dale L. Johnson
泰坦和海王星的工程级大气模型已经开发出来，用于NASA对外行星飞行任务中的航空捕获应用的系统分析研究。类似于非常成功的地球全球参考大气模型（Jesus，Justus等人，2000）和Mars（Mars-Mars，Justus和约翰逊，2001，Justus等人，和Mars-Bronze一样，Titan-Bronze和Neptune-Bronze的一个重要特征是它们能够模拟准随机扰动，用于开发制导、导航和控制算法以及热系统设计中的蒙特卡罗分析。
Engineering-level atmospheric models for Titan and Neptune have been developed for use in NASA s systems analysis studies of aerocapture applications in missions to the outer planets. Analogous to highly successful Global Reference Atmospheric Models for Earth (GRAM, Justus et al., 2000) and Mars (Mars-GRAM, Justus and Johnson, 2001, Justus et al., 2002) the new models are called Titan-GRAM and Neptune-GRAM. Like GRAM and Mars-GRAM, an important feature of Titan-GRAM and Neptune-GRAM is their ability to simulate quasi-random perturbations for Monte- Carlo analyses in developing guidance, navigation and control algorithms, and for thermal systems design.