• 제목/요약/키워드: upper atmosphere

검색결과 234건 처리시간 0.026초

대기요소 고려를 통한 무인항공기 비행시험계획 수립에 대한 연구 (A study on the Unmanned Aerial Vehicle(UAV) Flight Test Planning Establishment through Atmospheric Considerations)

  • 김영래;이정숙;이상철;고상호;강자영;최종욱;성덕용
    • 한국항공운항학회지
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    • 제18권4호
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    • pp.73-79
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    • 2010
  • Flight test is the final and a mandatory process for the development of unmanned aerial vehicles(UAVs) as well as manned. Since most UAVs fly in a low speed and are prone to adverse weather conditions such as air turbulence, atmospheric weather environment around flight test regions will be a critical item to be considered for a flight test planning for UAVs. In this paper, we suggest a decision method for a UAV flight test schedule based on weather conditions of surface and upper atmospheres and also introduce a program for an effective flight test planning through weather forecasts.

도심지의 온열성상에 관한 연구 -제1보 도심지 온열환경 예측모델을 위한 실측조사- (Study on Thermal Property in Urban Area - Part 1 : Experimental Analysis for Predicting Methodology of Thermal Property in Urban Area -)

  • 손원득;이성
    • 설비공학논문집
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    • 제16권10호
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    • pp.984-989
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    • 2004
  • Significant air temperature increases in urban areas is well known as the heat island phenomenon in a global scale. Therefore, we propose numerical model in order to analyze quantitative effects of building environmental factors on the heat island phenomenon in urban area. In this paper, thermal property of upper atmosphere is experimentally investigated for Sakae, Nagoya Japan. In conclusion, it was confirmed that the boundary layer of a urban canopy existed near the altitude of 139 m.

서해 중부 해상 대기의 연직구조 분석 (Analysis of Vertical Structure of Atmosphere on the Middle Part of the Yellow Sea)

  • 윤용훈;임주연;김백조;김태희;서장원;조하만
    • 한국지구과학회지
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    • 제21권1호
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    • pp.22-22
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    • 2000
  • 상층과 하층의 대기구조 특성을 알아내기 위하여, 해양의 특성을 잘 표현한다고 사료되는 섬(충남 보령시 오천면 외연도리)을 관측지점으로 선택하여 라디오존데를 이용하여 대기의 연직구조를 관측하였다. 관측결과를 이용하여, 저 고기압이 통과할 때의 상대습도, 기온과 바람의 변화를 분석하였으며 각각의 경우에 대해 결과치들을 비교하였다. 해양과 육상에서의 대기구조를 비교하기 위하여 오산의 관측 결과를 분석하였다. 그 결과, 상대습도가 고 · 저기압의 통과에 따라 변화함을 알 수 있었다. 즉, 저기압이 다가올 때는 상대습도는 하층보다 상층에서 먼저 증가하였으나 고기압이 다가올 때는 상층에서 10%까지 급격하게 감소하였다. 또, 상대습도는 변화폭이 육상에서보다 큰 것으로 분석되었다. 앞으로 해양과 육상에서의 수증기간의 관계를 계절별, 그리고 일별로 동시간 관측을 통해 찾고자 한다. 가하였으나 고기압이 다가올 때는 상층에서 10%까지 급격하게 감소하였다. 또, 상대습도는 변화폭이 육상에서보다 큰 것으로 분석되었다. 앞으로 해양과 육상에서의 수증기간의 관계를 계절별, 그리고 일별로 동시간 관측을 통해 찾고자 한다.

서해 중부 해상 대기의 연직구조 분척 (Analysis of Vertical Structure of Atmosphere on the Middle Part of the Yellow Sea)

  • 윤용훈;임주연;김백조;김태희;서장원;조하만
    • 한국지구과학회지
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    • 제21권1호
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    • pp.23-39
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    • 2000
  • 상층과 하층의 대기구조 특성을 알아내기 위하여, 해양의 특성을 잘 표현한다고 사료되는 섬(충남 보령시 오천면 외연도리)을 관측지점으로 선택하여 라디오존데를 이용하여 대기의 연직구조를 관측하였다. 관측결과를 이용하여, 저 고기압이 통과할 때의 상대습도, 기온과 바람의 변화를 분석하였으며 각각의 경우에 대해 결과치들을 비교하였다. 해양과 육상에서의 대기구조를 비교하기 위하여 오산의 관측 결과를 분석하였다. 그 결과, 상대습도가 고 저기압의 통과에 따라 변화함을 알 수 있었다. 즉, 저기압이 다가올 때는 상대습도는 하층보다 상층에서 먼저 증가하였으나 고기압이 다가올 때는 상층에서 10%까지 급격하게 감소하였다. 또, 상대습도 변화폭이 육상에서보다 큰 것으로 분석되었다. 앞으로 해양과 육상에서의 수증기간의 관계를 계절별, 그리고 일별로 동시간 관측을 통해 찾고자 한다.

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A SIGNATURE OF CHROMOSPHERIC ACTIVITY IN BROWN DWARFS: A RECENT RESULT FROM NIRLT MISSION PROGRAM

  • Sorahana, Satoko;Suzuki, Takeru K.;Yamamura, Issei
    • 천문학논총
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    • 제32권1호
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    • pp.131-133
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    • 2017
  • We present the latest results from the Mission Program NIRLT (PI: I.Yamamura), the near-infrared spectroscopy of brown dwarfs using the AKARI/IRC grism mode with the spectral resolution of ~ 120. The near-infrared spectra in the wavelength range between 2.5 and $5.0{\mu}m$ are especially important to study the brown dwarf atmospheres because of the presence of major molecular bands, including $CH_4$ at $3.3{\mu}m$, $CO_2$ at $4.2{\mu}m$, CO at $4.6{\mu}m$, and $H_2O$ around $2.7{\mu}m$. We observed 27 sources, and obtained 16 good spectra. Our model fitting reveals deviations between theoretical model and observed spectra in this wavelength range, which may be attributed to the physical condition of the upper atmosphere. The deviations indicate additional heating, which we hypothesize to be due to chromospheric activity. We test this effect by modifying the brown dwarf atmosphere model to artificially increase the temperature of the upper atmosphere, and compare the revised model with observed spectra of early- to mid-L type objects with $H{\alpha}$ emission. We find that the chemical structure of the atmosphere changes dramatically, and the heating model spectra of early-type brown dwarfs can be considerably improved to match the observed spectra. Our result suggests that chromospheric activity is essential to understand early-type brown dwarf atmospheres.

A Case Study of Tsukuba Tornado in Japan on 6 May 2012

  • Choo, Seonhee;Min, Ki-Hong;Kim, Kyung-Eak;Lee, Gyuwon
    • 한국지구과학회지
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    • 제39권5호
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    • pp.403-418
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    • 2018
  • This study conducted synoptic and mesoscale analyses to understand the cause of Japan Tsukuba tornado development, which occurred at 0340 UTC 6 May 2012. Prior to the tornado occurrence, there was a circular jet stream over Japan, and the surface was moist due to overnight precipitation. The circular jet stream brought cold and dry air to the upper-level atmosphere which let strong solar radiation heat the ground with clearing of sky cover. A tornadic supercell developed in the area of potentially unstable atmosphere. Sounding data at Tateno showed a capping inversion at 900 hPa at 0000 UTC 6 May. Strong insolation in early morning hours and removal of the inversion instigated vigorous updraft with rotation due to vertical shear in the upper-level atmosphere. This caused multiple tornadoes to occur from 0220 to 0340 UTC 6 May 2012. When comparing Tateno's climatological temperature and dew-point temperature profile on the day of event, the mid-level atmosphere was moister than typical sounding in the region. This study showed that tornado development in Tsukuba was caused by a combination of (a) topography and potential vorticity anomaly, which increased vorticity over the Kanto Plain; (b) vertical shear, which produced horizontal vortex line; and c) thermal instability, which triggered supercell and tilted the vortex line in the vertical.

Measurement of Radiative Loss from the Multi-layer Spectral Inversion of the Ha line and Ca II 8542 line taken by the FISS

  • Kang, Soo Sang;Chae, Jongchul
    • 천문학회보
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    • 제46권2호
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    • pp.77.3-78
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    • 2021
  • Measuring radiative loss from the solar chromospheric lines like Ha line, Ca II 8542 line helps to infer the exact amount of non-thermal heating in the solar atmosphere. By courtesy of the multi-layer spectral inversion, it is able to determine the radiative loss in the upper and lower chromosphere. Consequently, we found that the radiative loss is around 10 kW/m2, which is consistent with previous studies. Comparing the radiative loss at the upper and lower chromosphere, the loss at the lower chromosphere is larger than that of upper chromosphere and tends to spread all over the field of view while the loss in the upper chromosphere tends to be localized. We hope to find a hint for specific non-thermal heating process to explain the chromospheric radiative loss.

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해풍 효과에 의한 저층대기구조 변화의 측정 (Observation on Structural Change of Low Level Atmosphere due to Effect of Sea Breeze)

  • 전병일;김유근
    • 한국환경과학회지
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    • 제5권4호
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    • pp.441-451
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    • 1996
  • The surface meteorological and upper layer meteorological observation carried out to investigate influences of sea breeze effect on lower layer atmosphere at Gori nuclear power plant for 29∼30 July, 1996. According to surface meteorological data, the inflow of sea breeze was occurred 11:30 on 29 July, 10:30-on 30 July, respectively, at observation site. And the meteorological tower data showed that wind direction of sea breeze was identified as south-westerly, and wind speed of 58 m was 2 times stronger than that of 10 m. It is notworthy that surface inversion layer which built from the night time to daybreak of next day was not broken off by seab reeze's inflow for daytime, and strong inversion layer observed at 47∼243 m with moderately stable class (F) by URC. It was found that strong stable layer of potential temperature appeared at that layer, maximum relative humidity observed at the bottom of inversion layer and maximum mixing ratio observed in the low of inversion layer.

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MHD WAVES IN A STRATIFIED VISCOUS SOLAR ATMOSPHERE

  • KUMAR, NAGENDRA;KUMAR, ANIL;MURAWSKI, K.
    • 천문학논총
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    • 제30권2호
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    • pp.53-55
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    • 2015
  • We study MHD wave propagation in a gravitationally stratified isothermal viscous atmosphere of the Sun, permeated by a uniform magentic field. We perform numerical simulations by launching a slow wave on the upper boundary. The driven slow wave propagates down from low-${\beta}$ to high-${\beta}$ plasma across the region where the plasma ${\beta}$ is unity. It is found that mode conversion takes place at $z{\approx}-1.8$ in the layer ${\beta}{\approx}1$. The amplitudes of horizontal and vertical velocites are smaller than those obtained in the absence of viscosity.

한국형모델의 신규 GNSS RO 자료 활용과 품질검사 개선에 관한 연구 (A Study on Improvement of the Use and Quality Control for New GNSS RO Satellite Data in Korean Integrated Model)

  • 김은희;조영순;이은희;이용희
    • 대기
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    • 제31권3호
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    • pp.251-265
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    • 2021
  • This study examined the impact of assimilating the bending angle (BA) obtained via the global navigation satellite system radio occultation (GNSS RO) of the three new satellites (KOMPSAT-5, FY-3C, and FY-3D) on analyses and forecasts of a numerical weather prediction model. Numerical data assimilation experiments were performed using a three-dimensional variational data assimilation system in the Korean Integrated Model (KIM) at a 25-km horizontal resolution for August 2019. Three experiments were designed to select the height and quality control thresholds using the data. A comparison of the data with an analysis of the European Centre for Medium-Range Weather Forecasts (ECMWF) integrated forecast system showed a clear positive impact of BA assimilation in the Southern Hemisphere tropospheric temperature and stratospheric wind compared with that without the assimilation of the three new satellites. The impact of new data in the upper atmosphere was compared with observations using the infrared atmospheric sounding interferometer (IASI). Overall, high volume GNSS RO data helps reduce the RMSE quantitatively in analytical and predictive fields. The analysis and forecasting performance of the upper temperature and wind were improved in the Southern and Northern Hemispheres.