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:2003年,2004年,2005年和2007年夏季从北半球的Odin卫星数据和地基仪器获得的中天五天行星波

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A number of studies have shown that 5-day planetary waves modulate noctilucent clouds and the closely related Polar Mesosphere Summer Echoes (PMSE) at the summer mesopause. Summer stratospheric winds should inhibit wave propagation through the stratosphere and, although some numerical models (Geisler and Dickinson, 1976) do show a possibility for upward wave propagation, it has also been suggested that the upward propagation may in practice be confined to the winter hemisphere with horizontal propagation of the wave from the winter to the summer hemisphere at mesosphere heights causing the effects observed at the summer mesopause. It has further been proposed (Garcia et al., 2005) that 5-day planetary waves observed in the summer mesosphere could be excited in-situ by baroclinic instability in the upper mesosphere. In this study, we first extract and analyze 5-day planetary wave characteristics on a global scale in the middle atmosphere (up to 54 km in temperature, and up to 68 km in ozone concentration) using measurements by the Odin satellite for selected days during northern hemisphere summer from 2003, 2004, 2005 and 2007. Second, we show that 5-day temperature fluctuations consistent with westward-traveling 5-day waves are present at the summer mesopause, using local ground-based meteor-radar observations. Finally we examine whether any of three possible sources of the detected temperature fluctuations at the summer mesopause can be excluded: upward propagation from the stratosphere in the summer-hemisphere, horizontal propagation from the winter-hemisphere or in-situ excitation as a result of the baroclinic instability. We find that in one case, far from solstice, the baroclinic instability is unlikely to be involved. In one further case, close to solstice, upward prop- agation in the same hemisphere seems to be ruled out. In al other cases, all or any of the three proposed mechanisms are consistent with the observations.
机译:大量研究表明,在夏季中绝经期,为期5天的行星波会调制夜光云和密切相关的极地中层夏季回波(PMSE)。夏季平流层的风应抑制波在平流层中的传播,尽管一些数值模型(Geisler和Dickinson,1976)确实显示了向上波传播的可能性,但也有人建议,向上传播实际上可能限于冬季半球。从冬季到夏季半球的波在中层高度的水平传播会引起夏季中更年期的影响。有人进一步提出(Garcia等,2005),夏季中层大气中观察到的5天行星波可被中高层中层的斜压不稳定性原位激发。在这项研究中,我们首先使用Odin卫星在测量期间的选定天数中的测量值,在全球范围内提取和分析全球大气中5天的行星波特征(温度高达54 km,臭氧浓度高达68 km)。北半球从2003年,2004年,2005年和2007年开始的夏季。其次,我们使用当地的地面流星雷达观测结果,发现夏季中隔存在与西行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途探测到的三个温度波动的可能来源中的任何一个:夏季半球平流层的向上传播,冬季半球的水平传播或由于原位激发而引起的原地激发。斜压不稳定。我们发现,在距夏至很远的情况下,不太可能涉及斜斜不稳定。在另一种情况下,接近冬至时,似乎排除了在同一半球的向上传播。在其他情况下,三个或所有提议的机制都与观察结果一致。

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