[논문]CHARACTERISTICS OF ATMOSPHERIC WAVES OBSERVED FROM AIRGLOW MEASUREMENTS IN THE NORTHERN HIGH-LATITUDE

Won, Yong-In; Lee, Bang-Yong; Kwon, Soon-Chul

doi:10.5140/jass.2004.21.2.101

CHARACTERISTICS OF ATMOSPHERIC WAVES OBSERVED FROM AIRGLOW MEASUREMENTS IN THE NORTHERN HIGH-LATITUDE 원문보기

韓國宇宙科學會誌 = Journal of astronomy & space sciences, v.21 no.2, 2004년, pp.101 - 108

Won, Yong-In (Polar Research Institute, Korea Ocean R＆D Institute) , Lee, Bang-Yong (Polar Research Institute, Korea Ocean R＆D Institut) , Kwon, Soon-Chul (MIS Team, Korea Ocean R＆D Institute)

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The terrestrial nightglow emission in near infrared region were obtained using a Fourier Transform Spectrometer(FTS) at Esrange, Sweden ($67.90^{\circ}$N, $21.10^{\circ}$E) and the OH(4- 2) bands were used to derive temperature and airglow emission rate of the upper mesosphere. For this study, we analyzed data taken during winter of 2001/2002 and performed spectral analysis to retrieve wave information. From the Lomb-Scargle spectral analysis to the measured temperatures, dominant oscillations at various periods near tidal frequency are found. Most commonly observed waves are 4, 6, and 8 hour oscillations. Because of periods and persistence, the observed oscillations are most likely of tidal origin, i.e. zonally symmetric tides which are known to have their maximum amplitudes at the pole.

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waves in the high-latitude thermosphere and upper mesosphere region. In this report, we present our preliminary results taken at Esrange, Sweden during the winter of 2001, with emphasis on the characteristics of the observed oscillations.
Later, however, Oznovich & McEwen (1997) raised a question on the gravity wave explanation because of the persistence of the observed 8 hour oscillations. The frequently observed nature of the 8 hour oscillation, and the consistent negative phases for Krassovsky's ratio, resulted in a conflict for the explanation of the origin of the fluctuations and they suggested a further detailed inspection of the model with respect to various parameters such as lapse rate and minor constituent concentrations.

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The FTS is housed in a hut on KEOPS (Kiruna Esrange Optical Platform System), located on top of a hill in Esrange (European Sounding Rocket Launching Range) near Kiruna, Sweden. The system is fully automated and has been in continuous operation since its installation in late October 2001.
2001). The instrument employs a thermoelectrically cooled InGaAs detector with maximum sensitivity in the wavelength region 1.0 to 1.7 ㎛.The system provides 5 choices of spectral resolution that can be selected manually.

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CHARACTERISTICS OF ATMOSPHERIC WAVES OBSERVED FROM AIRGLOW MEASUREMENTS IN THE NORTHERN HIGH-LATITUDE 원문보기

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CHARACTERISTICS OF ATMOSPHERIC WAVES OBSERVED FROM AIRGLOW MEASUREMENTS IN THE NORTHERN HIGH-LATITUDE 원문보기

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