模拟火星火山大气热循环的模拟,使用中等尺度数值模型
Scot C R Rafkin1, Magdalena R V Sta Maria, Timothy I Michaels
1Department of Meteorology, San José State University, One Washington Square, San José, California 95117, USA. rafkin@metsun1.met.sjsu.edu
Nature
|October 18, 2002
概括
火星上的中层大气现象,如尘埃云,使用新的中层大气模型可以更好地理解. 这些模型揭示了大量的热循环,将尘埃运送到很远的距离.
科学领域:
- 行星科学 行星科学
- 大气动力学 大气动力学
- 火星气象学 火星气象学
背景情况:
- 在火星上,中尺度 (<100公里) 的大气现象是常见的.
- 有限的数据需要对火星大气动态进行数值建模.
- 一般的循环模型缺乏对中大尺度现象的分辨率.
研究的目的:
- 为了研究火星中层大气现象.
- 模拟Arsia Mons上方的螺旋尘埃云,使用一个中等尺度模型.
- 为了了解火星尘埃运输的动态.
主要方法:
- 使用了火星区域大气建模系统 (MRAMS).
- 采用了嵌套模型的层次结构,网格尺寸从240公里到3公里.
- 模拟中层层级尘埃云的形成和运输.
主要成果:
- 阿西亚山上空的尘埃云显示出一个更大,光学上更薄的热循环.
- 这种循环达到高达30公里的高度.
- 显著的水平尘埃传输发生在数千公里内.
结论:
- 中等尺度模型对于解决火星大气现象至关重要.
- 阿西亚山的尘埃云是深层热循环的可见体现.
- 火星的热循环在全球尘埃运输中发挥着重要作用.
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