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-P12] トロムソナトリウムライダーを用いた北極域SSLの統計解析

*小川 洋平1野澤 悟徳1津田 卓雄2川原 琢也3小川 泰信4藤原 均5斎藤 徳人6和田 智之5高橋 透4堤 雅基4川端 哲也1Hall Chris7Brekke Asgeir7 (1.名古屋大学、2.電気通信大学、3.信州大学、4.NIPR、5.成蹊大学、6.理化学研究所、7.ノルウェー北極大学)

We will present statisitical results about sporadic sodium layers (SSLs) appearing in the polar lower thermosphere/upper mesosphere during winter (November – January). The sodium LIDAR at Tromsø (69.6N, 19.2E) has made simultaneous five directional (vertical postion, plus 4 horizontal positions with zenith angale = 30 deg or 12.5 deg and azimuth = 0, 90, 180, 270 deg) observations, and has obtained about 2100 hours of temperature, sodium density, and wind data beteween October 2012 and March 2016. Analyzing these datasets, we have identified twenty-four SSL events over the four winter seasons, and have investigated charactristics of the SSLs.

We have addressed the following questions about SSLs: (1) in-situ generation or advection, (2) ionization of aurora is needed, (3) role of Es layers and temperature, and (4) local time dependence and advent height. Concerning (1), it is important to distinguish events if they were in-situ generated or just adveceted into the views of the LIDAR, since so far no proposed mechanisms can explain well the rapid increase of the sodium density found in the begging of SSL events. Based on investigation of timmings of detection at each beam direction, it is found that SSLs of the 10 events seemed to be in-situ generated, while those of 14 events were advected. Concerning (2), auroras would play an important role for generation of SSLs at high latitudes, but their role is not yet well understood. At Tromsø, several instruments monitor the aurora activity. These data showed that auroras appeared in 17 events. Concerning (3), exisitence of sporadic E layaer would be imporntat for generation (in particular, for providing sodium atoms), but its role is not well understood quantatively. Concerning (4), local time dependence and height of advent of SSLs are also keys to understand generation mechanisms of SSLs, in particular relationship with tide, planetary, and gravity waves. out of the 24 events, SSLs of 9 events appeared above 100 km before 21 UT, while SSLs of the 11 events showed up below 100 km after 21 UT.