一旦天文学家知道一个太阳系外行星的大小，并对它的位置了解的足够精确的话，他们就可以求助于气候模型师，他们可以创造虚拟的大气，并且观察它是如何运转的。
Once astronomers know an exoplanet's size and location with reasonable accuracy, they can turn it over to climate modelers who can create a virtual atmosphere and see how it might behave.
而多数行星模型均假设它们和我们太阳系的类地行星相似，即在大气中碳含量是氧含量的一半左右。
Most models of planets assume that they are similar to the terrestrial planets in our own Solar System, with about half as much carbon as oxygen in the atmosphere.
模型成功重现了在太阳辐射变化时，科学家已经在高层大气观测到的状况。
The model successfully reproduced what scientists have observed happening in the upper atmosphere during changes in solar radiation.
在建立动力学模型中，计及了地球扁球形的摄动、大气阻力、太阳辐射压的效应以及日月引力摄动。
The dynamical model included the effects of the earth non-spherical shape, atmospheric drag, solar radiation pressure as well as lunar and solar perturbations.
提出了地球大气太阳能—风能转换的双热机并联模型。
The twin engine model for the wind system of the earths atmosphere is presented.
提出了地球大气太阳能—风能转换的双热机并联模型。
The twin engine model for the wind system of the earths atmosphere is presented.
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