JpGU-AGU Joint Meeting 2017

講演情報

[EE] 口頭発表

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM11] [EE] Mesosphere-Thermosphere-Ionosphere Coupling in the Earth's Atmosphere

2017年5月23日(火) 15:30 〜 17:00 A01 (東京ベイ幕張ホール)

コンビーナ:Chang Loren(Institute of Space Science, National Central University)、Liu Huixin(九州大学理学研究院地球惑星科学専攻 九州大学宙空環境研究センター)、齊藤 昭則(京都大学大学院理学研究科地球物理学教室)、Tzu-Wei Fang、座長:Fang Tzu-Wei(University of Colorado, USA)

16:10 〜 16:30

[PEM11-03] Observations of the thermal structure, composition, and energy budget of the mesosphere and thermosphere from 15 years of data from SABER

★招待講演

*Martin G Mlynczak1Linda A Hunt2James M Russell3Thomas Marshall4 (1.NASA Langley Research Center、2.Science Systems and Applications, Inc. 、3.Hampton University、4.GATS, Inc. )

キーワード:Mesosphere-Thermosphere, Solar-Terrestrial Coupling, Global Change

The Sounding of the Atmosphere using Broadband Emission Radiometry (SABER) instrument has been observing the thermal structure, chemical composition, and energy budget of the Earth’s mesosphere and thermosphere for over 15 years. The instrument is on the NASA Thermosphere-Ionosphere-Mesosphere-Energetics and Dynamics (TIMED) satellite and continues to operate nominally, routinely collecting over 1500 profiles of limb radiance daily in each of its 10 channels. These measurements produce over 30 unique data products. The length of the SABER dataset continues to enable scientific discovery on topics ranging from solar-terrestrial connections to global change due to carbon dioxide increases. In this talk we will review in particular the influence of solar variability on the energy balance, composition, and thermal structure of the upper atmosphere. A specific focus will be on the current state of the Sun as it progresses towards the next solar minimum, and the corresponding effects seen in Earth’s atmosphere. We also will examine the effects of recent high speed solar wind stream events that are now becoming more common in this phase of solar activity, searching for evidence of previously-observed harmonics of the solar rotation period in the infrared cooling budget of the thermosphere. Prospects and requirements for new observations of the ionosphere-thermosphere-mesosphere will also be presented.