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자료유형
학술저널
저자정보
지건화 (한국해양과학기술원 부설 극지연구소) 김정한 (한국해양과학기술원 부설 극지연구소) 김용하 (충남대학교)
저널정보
한국우주과학회 Journal of Astronomy and Space Sciences Journal of Astronomy and Space Sciences 제31권 제2호
발행연도
2014.6
수록면
169 - 176 (8page)
DOI
http://dx.doi.org/10.5140/JASS.2014.31.2.169

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Since the operation of the King Sejong Station (KSS) started in Antarctic Peninsula in 1989, there have been continuousefforts to perform the observation for the upper atmosphere. The observations during the initial period of the stationinclude Fabry-Perot Interferometer (FPI) and Michelson Interferometer for the mesosphere and thermosphere, which areno longer in operation. In 2002, in collaboration with York University, Canada, the Spectral Airglow Temperature Imager(SATI) was installed to observe the temperature in the mesosphere and lower thermosphere (MLT) region and it has stillbeen producing the mesopause temperature data until present. The observation was extended by installing the meteorradar in 2007 to observe the neutral winds and temperature in the MLT region during the day and night in collaborationwith Chungnam National University. We also installed the all sky camera in 2008 to observe the wave structures in the MLTregion. All these observations are utilized to study on the physical characteristics of the MLT region and also on the wavephenomena such as the tide and gravity wave in the upper atmosphere over KSS that is well known for the strong gravitywave activity. In this article, brief introductions for the currently operating instruments at KSS will be presented with theirapplications for the study of the upper atmosphere.

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