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Mathematical model describes planetary weather pattern

机译:数学模型描述了行星的天气模式

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摘要

An anomalous weather pattern that occurs in 40- to 50-day cycles, the Madden-Julian Oscillation (MJO) enhances and suppresses tropical rainfall over a wide swath of the planet; it begins over the Indian Ocean and propagates eastward across the Pacific Ocean. Although the MJO affects monsoon development, intraseasonal weather in the midlatitudes, and the formation of El Nino, the oscillation's mechanism has not been well understood despite decades of research since its discovery in 1971. Andrew Majda and Samuel Stechmann developed a mathematical model that captures the fundamental physical features of this complex weather pattern. Whereas previous MJO models emphasized instability on the planetary scale, the authors suggest that the intraseasonal oscillation arises from stable climate interactions between equatorial moisture in the lower troposphere and synoptic scale atmospheric wave activity, which produces the system's dominant eastward propagation.
机译:Madden-Julian涛动(MJO)以40到50天为周期的异常天气模式,增强并抑制了整个地球上的热带降雨;它开始于印度洋,并向东跨太平洋传播。尽管MJO影响季风发展,中纬度的季节内天气以及厄尔尼诺现象的形成,但自1971年被发现以来,尽管进行了数十年的研究,但对振荡的机理仍不甚了解。Andrew Majda和Samuel Stechmann开发了一个数学模型来捕获这种复杂天气模式的基本物理特征。尽管先前的MJO模型强调了行星尺度的不稳定性,但作者认为,季节内振荡起因于对流层低层的赤道湿度与天气尺度的大气波活动之间的稳定气候相互作用,从而形成了该系统的主要向东传播。

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