Martian Water(火星水)研究综述
Martian Water 火星水 - The proposed resurfacing event creating the Borealis basin could have been important for the loss of a significant part of the early Martian water inventory. [1] Until now, meteoric smoke has been neglected in general circulation model studies of the formation of Martian water ice clouds. [2] Up to now, all attempts to retrieve martian water vapor from nadir observations have focused their analysis on a single spectral domain and comparison between the results of various experiments showed the difficulty to reconcile the water vapor datasets together. [3] This study constrains the lower bound of the scattering phase function of Martian water ice clouds (WICs) through the implementation of a new observation aboard the Mars Science Laboratory (MSL). [4] Additionally, we will discuss lessons learned from the implementation and validation of PAWES to guide further development of Martian water extraction systems. [5]提议的重新表面事件创建北极星盆地可能对早期火星水库存的重要部分损失很重要。 [1] 迄今为止，在火星水冰云形成的一般环流模型研究中，大气烟雾一直被忽略。 [2] 到目前为止，所有从最低点观测中检索火星水汽的尝试都将他们的分析集中在单个光谱域上，并且各种实验结果之间的比较表明很难将水汽数据集协调在一起。 [3] 本研究通过在火星科学实验室 (MSL) 上实施一项新观测，限制了火星水冰云 (WIC) 散射相函数的下限。 [4] 此外，我们将讨论从 PAWES 的实施和验证中吸取的经验教训，以指导火星水提取系统的进一步发展。 [5]
martian water ice 火星水冰
Until now, meteoric smoke has been neglected in general circulation model studies of the formation of Martian water ice clouds. [1] This study constrains the lower bound of the scattering phase function of Martian water ice clouds (WICs) through the implementation of a new observation aboard the Mars Science Laboratory (MSL). [2]迄今为止，在火星水冰云形成的一般环流模型研究中，大气烟雾一直被忽略。 [1] 本研究通过在火星科学实验室 (MSL) 上实施一项新观测，限制了火星水冰云 (WIC) 散射相函数的下限。 [2]