Abstract <![CDATA[Long-term trends in the <ce:italic> <ce:small-caps>D</ce:small-caps> </ce:italic>- and <ce:italic>E</ce:italic>-region based on rocket-borne measurements]]>
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D - and E-region based on rocket-borne measurements]]>

机译:<![cdata [ d - 和 e - 基于火箭型测量的原理]]>

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AbstractElectron densities obtained from rocket borne measurements are compared to an empirical, steady state model built from these data. The ratios between each measured value and its corresponding model valuevs. time yield trends which significantly vary with altitude. Notably above 120–130km the electron densities generally increase, whereas between 95 and 120km the ionosphere appears stable. Somewhere below 80–90km - depending on the investigated data subset - there is again a positive trend down to below 70km. Tentative explanations such as cooling of the mesosphere are suggested and may be confirmed by comprehensive theoretical models of the upper atmosphere.Highlights?Electron densities measuredin-situby sounding rockets over 50 years reveal trends which appear to support both theoretical models as well as ground-based and satellite data.?More than 50 years of rocket measurements.?Three height regions of long-term trends.?
机译:<![cdata [ 抽象 从火箭传播的电子密度与这些数据构建的经验,稳态模型进行了比较。每个测量值与其相应的模型值之间的比率。时间收益率趋势明显随高度而变化。特别高于120-130km的电子密度通常增加,而在95到120km之间,电离层出现稳定。在80-90km以下的某个地方 - 取决于调查的数据子集 - 再次趋势下降到70公里以下。提出了若干诸如冷却介质的解释,并且可以通过上层大气的综合理论模型来证实。 突出显示 电子密度测量 In-situ 通过50年来探测火箭揭示似乎支持理论模型以及地面和地面的趋势卫星数据。 超过50年的火箭测量。 长期趋势的三个高度区域。

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