日本地球惑星科学連合2023年大会

講演情報

[E] 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-EM12] Coupling Processes in the Atmosphere-Ionosphere System

2023年5月21日(日) 15:30 〜 16:45 101 (幕張メッセ国際会議場)

コンビーナ: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)、大塚 雄一(名古屋大学宇宙地球環境研究所)、Chang Loren(Institute of Space Science, National Central University)、Yue Deng(University of Texas at Arlington)、Chairperson:Yosuke Yamazaki(Leibniz Institute of Atmospheric Physics)、齊藤 昭則(京都大学大学院理学研究科地球物理学教室)


15:30 〜 15:45

[PEM12-16] Equatorial Sporadic E layers as seen from GNSS radio occultations

★Invited Papers

*Christina Arras1,2、Laysa Resende3、Jens Wickert1,2 (1.TU Berlin, Germany、2.GFZ Potsdam, Germany、3.INPE, Sao José dos Campos, Brazil)

キーワード:Ionosphere, sporadic E layer, GNSS radio occultation

The GNSS radio occultation (RO) technique has been established successfully during the previous two decades. It evolved into a valuable observation tool for precise atmospheric and ionospheric vertical profiling. Radio occultation measurements provide globally distributed precise profiles of the refractivity of the Earth’s atmosphere that can be converted into profiles of temperature, pressure, and water vapor in the lower neutral atmosphere and into electron density values in the ionosphere. The main advantage of this technique is that it provides the profiles in a very high vertical resolution covering the whole globe. Until today, there are about 14 million RO recordings available.

GNSS RO signals are very sensitive to vertical electron density gradients in the Earth’s ionosphere. This becomes visible as strong fluctuations in, e.g., signal-to-noise ratio recordings, which allow detecting ionospheric disturbances like sporadic E (Es) layers in the lower ionospheric E region. Due to the geometry of the GNSS RO technique, it enables for the first time receiving a global and comprehensive picture of the occurrence and the properties of Es layers in a high spatial resolution.

In this presentation, we like to focus on the difference between midlatitude and low-latitude sporadic E properties. We observed that the Es occurrence rate shows a pronounced depression directly at the magnetic equator. Further, the equatorial Es altitudes show a strong longitudinal variability which is not the case at midlatitudes. We will give and explanation attempt for the observed features in the equatorial region using equatorial electric field data provided by the Swarm satellites.