JpGU-AGU Joint Meeting 2020

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-EM18] 太陽地球系結合過程の研究基盤形成

コンビーナ:山本 衛(京都大学生存圏研究所)、小川 泰信(国立極地研究所)、野澤 悟徳(名古屋大学宇宙地球環境研究所)、吉川 顕正(九州大学大学院理学研究院地球惑星科学部門)

[PEM18-06] Statistical study of Sporadic Sodium Layers (SSLs) above Tromsø (2)

*野澤 悟徳1津田 卓雄2斎藤 徳人3川原 琢也4和田 智之3小川 泰信5藤原 均6高橋 透7川端 哲也1ホール クリス8ブレッケ アスゲイル8 (1.名古屋大学宇宙地球環境研究所、2.電気通信大学、3.理学研究所光量子工学研究センター、4.信州大学工学部、5.国立極地研究所、6.成蹊大学工学部、7.オスロ大学物理学科、8.ノルウェー北極大学)

キーワード:SSL、Tromsoe、プラズマー中性大気結合、ナトリウムライダー

This study is the first statistical study of SSLs differentiating in-situ generated SSLs from advected SSLs at high latitudes, and evaluates necessary conditions for generating a SSL. Based on about 3000 hours of sodium density data obtained with the Tromsø sodium LIDAR over 7 year seasons (October-March) between 2012 and 2018, we have identified 36 events of Sporadic Sodium Layer (SSL) in the polar mesosphere and lower thermosphere (MLT) region. A SSL is a thin sodium layer (about 1-2 km) with high sodium density (usually factor of 2 or more higher than that of a normal layer), and its life time is said to be about a few minutes to a few hours. Observational results of SSLs are summarized as follows: (1) SSLs appeared for shorter than 5 % of the overall observational time, confirming it is a rare event at high latitude. (2) The advent altitude distributed from 94 km to 106 km; no clear trend is found. (3) The advent time distributed from 18 LT to 1 UT: no events are found before 18 LT or later 1 LT. (4) No relationship is found between advent time and altitude. (5) The peak density tends to be lower as height increasing. (6) Lifetimes do not show a clear relationship with advent altitudes. We have investigated necessary conditions for a SSL to form in the polar MLT region. Auroral electron precipitation as well as appearance of a sporadic E layer would be one of necessary conditions to form a SSL.



By using an advantage of five directional measurements, we have derived movement velocities of SSLs using detection times (i.e., advent times) at five positions by assuming a SSL has a linear front perpendicular to the movement direction, and have compared wind velocity. The movement directions are dominantly from south-eastward to south westward except for 3 events: most SSLs moved southward in the meridional direction. Based on comparison of the velocities, we have found that 29 out of 36 events (81%) are likely classified to be advection events, while 7 events are left for candidates of in-situ generation events. We will discuss difference of “advection” and “in-situ” events in terms of height/horizontal structures of sodium densities.