日本地球惑星科学連合2014年大会

講演情報

インターナショナルセッション(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-EM06_1AM2] Study of coupling processes in Sun-Earth system with large radars and large-area observations

2014年5月1日(木) 11:00 〜 12:45 312 (3F)

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(名古屋大学太陽地球環境研究所)、橋口 浩之(京都大学生存圏研究所)、座長:McCrea Ian(RAL Space, STFC Rutherford Appleton Laboratory)

11:00 〜 11:30

[PEM06-23] 南極昭和基地大型大気レーダー計画の現状

*佐藤 薫1堤 雅基2佐藤 亨3中村 卓司2齊藤 昭則3冨川 喜弘2西村 耕司2高麗 正史1山岸 久雄2山内 恭2 (1.東京大学大学院理学系研究科地球惑星科学専攻、2.国立極地研究所、3.京都大学)

キーワード:大型大気レーダー, 極域大気, 中層大気, 重力波, 大気大循環

The PANSY radar is the first Mesosphere-Stratosphere-Troposphere/Incoherent Scatter (MST/IS) radar in the Antarctic. It is a VHF monostatic pulse Doppler radar operating at 47 MHz, consisting of an active phased array of 1,045 Yagi antennas and an equivalent number of transmit-receiver modules with a total peak output power of 500 kW. The first stage of the radar was installed at Syowa Station (69o00'S, 39o35'E) in early 2011, and is continuously operating with 228 antennas and modules since April 2012. The full radar system operation will start in 2015. This paper reports the project's scientific objectives, technical descriptions, and the preliminary results of observations made to date. The radar is designed to clarify the role of atmospheric gravity waves at high latitudes in the momentum budget of the global circulation in the troposphere, stratosphere and mesosphere, and to explore the dynamical aspects of unique polar phenomena such as polar mesospheric/stratospheric clouds. The katabatic winds as a branch of Antarctic tropospheric circulation and as an important source of gravity waves are also of special interest. Moreover, strong and sporadic energy inputs from the magnetosphere by energetic particles and field-aligned currents can be quantitatively assessed by the broad height coverage of the radar which extends from the lower troposphere to the upper ionosphere. From engineering points of view, the radar had to overcome restrictions related to the severe environments of Antarctic research, such as very strong winds, limited power availability, short construction periods, and limited manpower availability. We resolved these problems through the adoption of specially designed class-E amplifiers, lightweight and tough antenna elements, and versatile antenna arrangements. We will show highlights of several interesting results from the radar observations regarding severe snow storms, gravity waves, multiple tropopauses, and polar mesosphere summer/winter echoes.ReferenceSato, K., et al., J. Atmos. Solar-Terr. Phys., doi:10.1016/j.jastp.2013.08.022, 2013.