論文

査読有り
2014年10月

Program of the Antarctic Syowa MST/IS radar (PANSY)

JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS
  • Kaoru Sato
  • ,
  • Masaki Tsutsumi
  • ,
  • Toru Sato
  • ,
  • Takuji Nakamura
  • ,
  • Akinori Saito
  • ,
  • Yoshihiro Tomikawa
  • ,
  • Koji Nishimura
  • ,
  • Masashi Kohma
  • ,
  • Hisao Yamagishi
  • ,
  • Takashi Yamanouchi

118
1
開始ページ
2
終了ページ
15
記述言語
英語
掲載種別
研究論文(学術雑誌)
DOI
10.1016/j.jastp.2013.08.022
出版者・発行元
PERGAMON-ELSEVIER SCIENCE LTD

The PANSY radar is the first Mesosphere-Stratosphere-Troposphere/Incoherent Scatter (MST/IS) radar in the Antarctic region. It is a large VHF monostatic pulse Doppler radar operating at 47 MHz, consisting of an active phased array of 1045 Yagi antennas and an equivalent number of transmit-receive (TR) modules with a total peak output power of 500 kW. The first stage of the radar was installed at Syowa Station (69 degrees 00'S, 39 degrees 35'E) in early 2011, and is currently operating with 228 antennas and modules. 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 clouds (PMC) and polar stratospheric clouds (PSC). 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, light weight and tough antenna elements, and versatile antenna arrangements. Although the radar is currently operating with only about a quarter of its full designed system components, we have already obtained interesting results on the Antarctic troposphere, stratosphere and mesosphere, such as gravity waves, multiple tropopauses associated with a severe snow storm in the troposphere and stratosphere, and polar mesosphere summer echoes (PMSE). (C) 2013 Elsevier Ltd. All rights reserved.

リンク情報
DOI
https://doi.org/10.1016/j.jastp.2013.08.022
Web of Science
https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000340332800002&DestApp=WOS_CPL
ID情報
  • DOI : 10.1016/j.jastp.2013.08.022
  • ISSN : 1364-6826
  • eISSN : 1879-1824
  • Web of Science ID : WOS:000340332800002

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