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康曼德雷拉巴西站的气辉观测历史:温度测量和重力波研究。

Historical line of airglow observations at Comandante Ferraz Brazilian Station: measurements of temperature and studies on gravity waves.

机构信息

Instituto Nacional de Pesquisas Espaciais (INPE), Coordenação Espacial do Sul (COESU), Av. Roraima, 1000, Camobi, 97105-970 Santa Maria, RS, Brazil.

Instituto Nacional de Pesquisas Espaciais (INPE), Divisão de Clima Espacial, Av. dos Astronautas, 1758, Jardim da Granja, 12227-010 São José dos Campos, SP, Brazil.

出版信息

An Acad Bras Cienc. 2023 Nov 3;95(suppl 3):e20210836. doi: 10.1590/0001-3765202320210836. eCollection 2023.

Abstract

The thermal dynamics of the upper atmosphere, especially in the mesosphere, have been improving our understanding about the effects of climate change, as well as how the dynamics and general circulation in the upper atmosphere are driven by different types of waves, such as the atmospheric gravity waves, planetary waves and atmospheric tides. In order to study the upper atmospheric temperature variability and gravity waves, several research groups have been employing the remote technique of observing the airglow emissions originated in the upper mesosphere and lower thermosphere, besides emissions from the ionosphere. INPE's airglow group started the studies on emissions from the upper atmosphere to investigate temperature and dynamics in the mesosphere, thermosphere/ionosphere at the end of 70's. However, only in 2001 this group sent the first airglow experiment to the Brazilian Antarctic Station Comandante Ferraz (EACF) to measure the OH (8-3) emission and temperature. From that year to 2014, several other experiments were carried out at EACF, not only to measure the temperature and airglow intensities, but also to observe gravity waves, winds and other related phenomena. This paper presents airglow experiments at EACF from 2001 to the present, including illustrations, examples of already published results, and unpublished data.

摘要

高层大气的热力学,特别是中层大气的热力学,提高了我们对气候变化影响的认识,以及不同类型的波动(如大气重力波、行星波和大气潮汐)如何驱动高层大气的动力学和整体环流。为了研究高层大气温度变化和重力波,一些研究小组一直在利用远程技术观测高层中层和低层热层中源自气辉的发射,以及电离层中的发射。INPE 的气辉小组在 70 年代末开始研究高层大气的发射,以调查中层、热层/电离层中的温度和动力学。然而,直到 2001 年,该小组才首次向巴西南极站指挥官费拉兹(EACF)发送气辉实验,以测量 OH(8-3)发射和温度。从那年到 2014 年,EACF 进行了其他几次实验,不仅测量了温度和气辉强度,还观察了重力波、风等相关现象。本文介绍了 2001 年至今在 EACF 进行的气辉实验,包括说明、已经发表的结果示例和未发表的数据。

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