首页> 外文期刊>Annales Geophysicae >Five-day planetary waves in the middle atmosphere from Odin satellite data and ground-based instruments in Northern Hemisphere summer 2003, 2004, 2005 and 2007
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Five-day planetary waves in the middle atmosphere from Odin satellite data and ground-based instruments in Northern Hemisphere summer 2003, 2004, 2005 and 2007

机译:来自奥丁卫星数据和北半球2003年,2004年,2005年和2007年夏季的地面仪器在中层大气中的五天行星波

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A number of studies have shown that 5-day planetary waves modulatenoctilucent clouds and the closely related Polar Mesosphere Summer Echoes(PMSE) at the summer mesopause. Summer stratospheric winds should inhibitwave propagation through the stratosphere and, although some numericalmodels (Geisler and Dickinson, 1976) do show a possibility for upward wavepropagation, it has also been suggested that the upward propagation may inpractice be confined to the winter hemisphere with horizontal propagation ofthe wave from the winter to the summer hemisphere at mesosphere heightscausing the effects observed at the summer mesopause. It has further beenproposed (Garcia et al., 2005) that 5-day planetary waves observed in thesummer mesosphere could be excited in-situ by baroclinic instability in theupper mesosphere. In this study, we first extract and analyze 5-dayplanetary wave characteristics on a global scale in the middle atmosphere(up to 54 km in temperature, and up to 68 km in ozone concentration) usingmeasurements by the Odin satellite for selected days during northernhemisphere summer from 2003, 2004, 2005 and 2007. Second, we show that 5-daytemperature fluctuations consistent with westward-traveling 5-day waves arepresent at the summer mesopause, using local ground-based meteor-radarobservations. Finally we examine whether any of three possible sources ofthe detected temperature fluctuations at the summer mesopause can beexcluded: upward propagation from the stratosphere in the summer-hemisphere,horizontal propagation from the winter-hemisphere or in-situ excitation as aresult of the baroclinic instability. We find that in one case, far fromsolstice, the baroclinic instability is unlikely to be involved. In onefurther case, close to solstice, upward propagation in the same hemisphereseems to be ruled out. In all other cases, all or any of the three proposedmechanisms are consistent with the observations.
机译:大量研究表明,在中绝经期,为期5天的行星波会调制夜光云和与之密切相关的极地中层夏季回波(PMSE)。夏季平流层的风会抑制波在平流层中的传播,尽管一些数值模型(Geisler和Dickinson,1976)确实显示了向上传播的可能性,但也有人提出,向上传播可能不限于冬季半球的水平传播。从冬季到夏季半球在中层高度发生波动,造成夏季中段停滞。进一步提出(Garcia等,2005),在夏季中球层观测到的5天行星波可被上部中层球体的斜压不稳定原位激发。在这项研究中,我们首先使用奥丁卫星在北半球夏季的特定日子进行的测量,首先在中层大气(温度高达54 km,臭氧浓度高达68 km)的全球范围内提取并分析了5天行星波特征分别从2003年,2004年,2005年和2007年开始。第二,我们使用当地的地面流星雷达观测资料,在夏季更年期出现了与西行5天波一致的5天温度波动。最后,我们检查是否可以排除夏季中绝经期检测到的温度波动的三个可能来源中的任何一个:夏季半球的平流层向上传播,冬季半球的水平传播或由于斜压不稳定导致的原位激发。我们发现,在距夏至很远的情况下,不太可能涉及斜压不稳定。在另一种情况下,接近至冬,似乎排除了在同一半球内向上传播的可能性。在所有其他情况下,提出的三种机制中的全部或任何一种都与观察结果一致。

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