JpGU-AGU Joint Meeting 2017

講演情報

[EE]Eveningポスター発表

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-EM15] [EE] 太陽地球系結合過程の研究基盤形成

2017年5月25日(木) 15:30 〜 16:45 ポスター会場 (国際展示場 7ホール)

[PEM15-P13] Vertical motion of the neutral atmosphere above Tromsoe

*野澤 悟徳1小川 泰信2藤原 均3川原 琢也4津田 卓雄5斎藤 徳人6和田 智之6高橋 透2堤 雅基2川端 哲也1Hall Chris7Brekke Asgeir7 (1.名古屋大学宇宙地球環境研究所、2.国立極地研究所、3.成蹊大学理工学部、4.信州大学工学部、5.電気通信大学情報理工学部、6.理化学研究所光量子工学研究領域、7.UiT ノルウェー北極大学)

キーワード:Vertical wind, Mesosphere and lower Thermosphere, LIDAR, Tromsoe, EISCAT

We will present results of vertical motion above Tromsoe (69.6 deg. N, 19.2 deg. E) mainly based on sodium LIDAR data. Vertical motion of the neutral gases in the upper mesosphere and lower thermosphere (MLT) is a peculiar issue, and its understanding is important in terms of substance transport as well as thermal structures. Observations of the vertical wind in the MLT region are rather difficult, because vertical velocities are generally thought to be about two orders smaller than horizontal wind velocities. It is believed that the cold summer mesopause is set up by upward wind with strength of a few cm/s in the mesosphere. During high auroral activity intervals, some observations conducted by Fabry-Perot Interferometer (FPI) reported about 10 m/s or larger vertical wind velocity in the polar lower thermosphere. FPI measurements, however, suffer from a serious weakness of passive measurements: no information on the height observed. On the other hand, observations of vertical winds by radars are also difficult. Thus, our understanding of the vertical motion in the polar MLT region is still limited. The sodium LIDAR operated at Tromsoe is capable of simultaneous measurements of wind velocities with five directions with a good accuracy (1-2 m/s). By using the LIDAR data (about 2100 hr data) obtained from October 2012 to March 2016 together with EISCAT, MF, and meteor radar data as well as auroral image data, we will discuss the characteristics of the vertical motion in the polar MLT.

We have found some events where the vertical wind blew with strength of about 10 m/s. In the case of January 14, 2015, the upward vertical wind with an amplitude of 10 m/s was found between 92 and 101 km over a few hours. During the night, the semidiurnal tide was strong with an amplitude of 100 m/s. This would confirm that strong vertical motion exists when such waves pass by the MLT region. In another event found in February 8, 2013, upward flows were observed between 94 and 96 km at the same time for 15 min, while no vertical flows were found at and above 97 km and at and below 93 km. Of particular interest in both cases is that a sporadic sodium layer (SSL) appeared nearby the height region where the upward vertical wind was observed at the same time (in the case of January 14, 2015) or 15 min later (in the case of February 8, 2013). In this presentation, we will address what conditions are needed for the vertical motion occurring, and also discuss possible relationship with the advent of SSLs.