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从电离层观测推断夏季正午条件下热层参数的纵向变化:与经验模型的比较。

Longitudinal variations in thermospheric parameters under summer noontime conditions inferred from ionospheric observations: A comparison with empirical models.

作者信息

Mikhailov Andrey V, Perrone Loredana

机构信息

Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radio Wave Propagation (IZMIRAN), Moscow, Russia.

Istituto Nazionale di Geofisica e Vulcanologia (INGV), Rome, Italy.

出版信息

Sci Rep. 2019 Sep 4;9(1):12763. doi: 10.1038/s41598-019-49255-1.

Abstract

Longitudinal variations in the thermospheric neutral composition ([O] and [N]) and exospheric temperature Tex have been inferred from June monthly median noontime fF and fF observations at mid-latitudes to check for consistency with empirical MSIS models. In general, a similarity in longitudinal variations has been demonstrated, and this is interesting, as similar variations were obtained with very different methods and different data sources. Both inferred and MSISE-00 modelled height-integrated O/N ratios are comparable to TIMED/GUVI observations only under solar minimum conditions but differ substantially under high solar activity. The retrieved height-integrated O/N ratio longitudinal variations are small (∼15%) in comparison to the observed NF variations under high solar activity. The height-integrated O/N ratio cannot be incorporated into the F-layer formation mechanism; therefore, such observations cannot be used for any quantitative interpretation of NF variations.

摘要

已从中纬度地区6月的月中值正午fF和fF观测数据推断出热层中性成分([O]和[N])以及外逸层温度Tex的纵向变化,以检验其与经验性MSIS模型的一致性。总体而言,已证明纵向变化具有相似性,这很有意思,因为通过非常不同的方法和不同的数据来源获得了相似的变化。仅在太阳活动极小期条件下,推断出的和MSISE - 00模拟的高度积分O/N比才与TIMED/GUVI观测结果相当,但在高太阳活动期间则有很大差异。与高太阳活动期间观测到的NF变化相比,反演得到的高度积分O/N比纵向变化较小(约15%)。高度积分O/N比无法纳入F层形成机制;因此,此类观测不能用于对NF变化进行任何定量解释。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/63d1/6726631/e5d41329609e/41598_2019_49255_Fig1_HTML.jpg

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