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Polar OH-Airglow Temperature Variations in the 87/88 Winter

机译:87/88冬季的极性OH-气辉温度变化

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Measurements of OH-airglow spectra from Nord-lysstasjonen in Adventdalen, Svalbard (15°E, 78°N) from the period 1980-2000 have been done. The temperature at 87 km height was iterated by fitting synthetic spectra to the measured spectra using the vibrational band (6-2). As a first results of the analysis of the time series mesospheric coolings, strong diurnal and semidiurnal tides and a planetary wave have been found in the temperatures in the winter of 1987/1988. At the time of the extraordinarily early stratospheric warming in December a cooling of 30 K was observed. The strength of the diurnal and semidiurnal tides were 30 K and 15 K respectively. The observation of the planetary wave confirms various models that have shown that mesospheric planetary waves can be generated indirectly by planetary waves in the stratosphere, due to an uneven distribution of the propagation of orographic planetary waves into the mesosphere.
机译:从1980年至2000年,对斯瓦尔巴特群岛Adventdalen的Nord-lysstasjonen的OH-气辉光谱进行了测量(15°E,78°N)。通过使用振动带(6-2)将合成光谱拟合到测得的光谱,来迭代87 km高度的温度。作为对时间序列中层冷却的分析的初步结果,在1987/1988年冬季的温度中发现了强烈的昼夜和半昼间潮汐和行星波。在12月,平流层特别早期变暖时,观测到30 K的降温。日潮和半日潮的强度分别为30 K和15K。行星波的观测证实了各种模型,这些模型表明平流层中的行星波可以间接产生中层行星波,这是由于地形行星波向中层的传播分布不均匀所致。

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