The structure of Venus' middle atmosphere and ionosphere
The structure of Venus' middle atmosphere and ionosphere
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DOI：
10.1038/nature06239
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发表时间：
2007-11-29
期刊：
影响因子：
64.8
通讯作者：
Tyler, G. L.
中科院分区：
文献类型：
--
作者：
Paetzold, M.;Haeusler, B.;Tyler, G. L.
金星的大气层和电离层过去曾通过航天器遥感（1-4）或原位技术（3,4）进行过研究。然而，这些早期的任务给我们留下了一些问题，例如，从对流层上层到中间层下层（50-90公里）过渡区域的大气结构，以及电离层的显著变化结构。在全球云层内和云层下的观测变得越来越困难(
The atmosphere and ionosphere of Venus have been studied in the past by spacecraft with remote sensing(1-4) or in situ techniques(3,4). These early missions, however, have left us with questions about, for example, the atmospheric structure in the transition region from the upper troposphere to the lower mesosphere (50-90 km) and the remarkably variable structure of the ionosphere. Observations become increasingly difficult within and below the global cloud deck (