• 천문학회지
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• 제54권2호
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• pp.49-60
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• 2021

Observations of line of sight (LOS) Doppler velocity and non-thermal line width in the off-limb solar corona are often used for investigating the Alfvén wave signatures in the corona. In this study, we compare LOS Doppler velocities and non-thermal line widths obtained simultaneously from two different instruments, Coronal Multichannel Polarimeter (CoMP) and Hinode/EUV Imaging Spectrometer (EIS), on various off-limb coronal regions: flaring and quiescent active regions, equatorial quiet region, and polar prominence and plume regions observed in 2012-2014. CoMP provides the polarization at the Fe xiii 10747 Å coronal forbidden lines which allows their spectral line intensity, LOS Doppler velocity, and line width to be measured with a low spectral resolution of 1.2 Å in 2-D off limb corona between 1.05 and 1.40 RSun, while Hinode/EIS gives us the EUV spectral information with a high spectral resolution (0.025 Å) in a limited field of view raster scan. In order to compare them, we make pseudo raster scan CoMP maps using information of each EIS scan slit time and position. We compare the CoMP and EIS spectroscopic maps by visual inspection, and examine their pixel to pixel correlations and percentages of pixel numbers satisfying the condition that the differences between CoMP and EIS spectroscopic quantities are within the EIS measurement accuracy: ±3 km s-1 for LOS Doppler velocity and ±9 km s-1 for non-thermal width. The main results are summarized as follows. By comparing CoMP and EIS Doppler velocity distributions, we find that they are consistent with each other overall in the active regions and equatorial quiet region (0.25 ≤ CC ≤ 0.7), while they are partially similar to each other in the overlying loops of prominences and near the bottom of the polar plume (0.02 ≤ CC ≤ 0.18). CoMP Doppler velocities are consistent with the EIS ones within the EIS measurement accuracy in most regions (≥ 87% of pixels) except for the polar region (45% of pixels). We find that CoMP and EIS non-thermal width distributions are similar overall in the active regions (0.06 ≤ CC ≤ 0.61), while they seem to be different in the others (-0.1 ≤ CC ≤ 0.00). CoMP non-thermal widths are similar to EIS ones within the EIS measurement accuracy in a quiescent active region (79% of pixels), while they do not match in the other regions (≤ 61% of pixels); the CoMP observations tend to underestimate the widths by about 20% to 40% compared to the EIS ones. Our results demonstrate that CoMP observations can provide reliable 2-D LOS Doppler velocity distributions on active regions and might provide their non-thermal width distributions.

• 한국작물학회지
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• 제42권3호
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• pp.255-262
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• 1997

벼 군락에서 건물생산량을 태양광의 반사스펙트럼 특성을 이용하여 추정하고자 1993년 4월부터 10월까지 경기도 소재 수원기상대 구내 포장에서 조생종 진부벼와 중만생종 대청벼, 일품벼를 공시 품종으로 하고 생육시기별 태양광 반사스펙트럼과 건물중을 조사한 결과 다음과 같다. 1. 출수전에 근적외광 파장대(720∼l,100nm)의 반사율을 가시광 파장대 (400∼700nm)의 반사율로 나눈 비율이 건물생산량과 상관이 높았으며, 가시광 파장대 중에서도 녹색, 적색파장보다 청색파장(400∼500nm)의 반사율로 나눈 비율이 건물생산량과의 상관이 높았다. 2. 적외광 파장의 반사율을 청색파장의 반사율로 나눈 비율 중에서 특히 R910 /R460 비율이 건물생산량과 가장 높은 정의 상관을 보였다. 3. 출수이전에 R910/R460 비율과 건물생산과의 회귀식을 이용한 추정식 Y=21.24284 X-212.734는 실측치와의 상관관계는 매우 높았다. 4. 출수이후엔 근적외광 파장(720∼l,100nm)의 반사율을 적색파장(600∼700nm)의 반사율로 나눈 비율이 청색이나 녹색파장의 반사율로 나눈 비율보다 건물생산량과의 상관이 더 높았다.

• 한국환경농학회지
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• 제3권1호
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• pp.71-78
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• 1984

약 500nm 이하의 파장영역(청색광)이 차단된 태양광은 고추의 생장에 괄목할만한 효과를 보였다. 영양생장기의 여러가지 생장지표들은 전반적으로 생육상태가 향상 내지 촉진되고 있음을 보여주었다. 한편, chlorophyll a, ${\beta}-carotene$, 및 다섯가지 성분의 xanthophyll을 주성분으로 하는 것으로 밟혀진 고추의 광합성색소계의 수준은 광질처리구의 잎에서 백색광 대조구에 비하여 높게 나타났다. 특히 carotenoid들의 함량증가가 보다 현저하였다. 광질 처리효과로 생긴 왕성한 생장력은 숙과의 수량형성에도 반영되어 대조구대비 35%의 증수를 보였다. 또한 청색광을 차단한 광질처리가 식품으로서의 숙과의 품질들 저하시키는 일이 없음도 아울러 확인하였다. 본 연구에 사용한 광질을 선택한 논리적 근거와 실험결과들을 여러 가지 광생물학적 측면에서 토의하였다.

• 천문학논총
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• 제10권1호
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• pp.91-108
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• 1995

We have intensively examined the structure of photospheric magnetic fields obtained from the calculation of the polarized radiation transfer for the model atmosphere. To determine more reliable magnetic field in the photospheric region composed of umbra, penumbra and quite area, we have calculated the polarized radiative transfer for a magnetically sensitive spectral line, FeI $6302.5{\AA}$, using our composite model representing three kinds of the atmospheric area distinguished by the pixel value of the Stokes I image over the region. Polarization data of the full Stokes parameters, used in this paper had been obtained from the vector magnetograph on Solar Flare Telescope of National Astronomical Observatory at Mitaka(MTK) in Japan. According to our investigation on the active region in the photosphere, it has been found that the large current density(${\geq}8{\times}10^2A/km^2$) and shear angle(${\geq}85^{\circ}$) should be distributed along the magnetic neutral line. To be compared with the results of MTK, our results in transverse magnetic field strength and direction are similar with those of MTK, however our longitudinal field strength at the center of the spot is somewhat(${\sim}1000$ Gauss) larger than MTK.

• 대기
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• 제20권4호
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• pp.519-530
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• 2010

In this paper we review current research on Atmospheric Brown Clouds (ABCs) with lightweight Unmanned Aerial Vehicles (UAVs) and miniaturized instruments. The UAV technology for in-situ measurements, including aerosol concentration, aerosol size distribution, aerosol absorption, cloud drop size distribution, solar radiation fluxes (visible and broadband), and spectral radiative fluxes, is a leading-edge technology for cost-effective atmospheric sounding, which can fill the gap between the ground measurement and satellite observation. The first experimental observation with UAVs in Korea, Cheju ABC Plume Monsoon Experiment (CAPMEX), conducted during summer 2008 revealed that the Beijing plumes exerted a strong positive influence on the net warming and fossil-fuel-dominated black-carbon plumes were approximately 100% more efficient warming agents than biomass-burning-dominated plumes. Long-term sustainable routine UAV measurements will eventually provide truly three-dimensional data of ABCs, which is necessary for the better understanding of their climate impacts and for the improvement of numerical models for air pollution, weather forecast and climate change.

• 대한원격탐사학회:학술대회논문집
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• 대한원격탐사학회 2006년도 Proceedings of ISRS 2006 PORSEC Volume I
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• pp.446-449
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• 2006

It is backscattering of solar radiation by water body that makes ocean color observable from above, either by airplanes or satellites. Given the very low direct contribution to backscattering by phytoplankton cells, it is curious why the retrieval of phytoplankton concentration from remotely observed ocean color is evidently successful. From semianalytical bio-optical models, a dataset is created of spectral absorption, scattering and backscattering coefficients as a function of chlorophyll concentration. Four scenarios are considered, 1) only molecular and no particle scattering, 2) random particle backscattering uncorrelated with chlorophyll concentration, 3) constrained random particle scattering with known backscattering ratio, and 4) constrained random scattering with random backscattering ratio. Scenario 1 only introduces moderate errors of -20% - 90%. And for scenarios 3 and 4, the errors are largely within 30% and 100%. Scenario 2 introduces the largest errors, with the retrieved chlorophyll concentration virtually uncorrelated with the true values, implying the backscattering must somehow be related to the trophic state. The results of the study suggested These 3 cases confirmed that while it is the absorption by phytoplankton that in large part decides the accuracy of chlorophyll concentration retrieval, for the success of monitoring of global ocean primary productivity we have to improve our knowledge on particle backscattering.

• 천문학논총
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• 제30권2호
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• pp.761-763
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• 2015

Colors have been derived from the observed optical spectrum of Mars and Jupiter. It is known that the planets and the Moon emit reflected sunlight and thus their spectra are similar to the spectrum of solar radiation. The question was then why is the color of Mars different from that of other planets, i.e. red, although it would share the same spectrum of reflected sunlight. Can one derive color from the spectrum? Therefore, we observed the optical spectra of the scattered sunlight in day time for the Moon and Mars using a 1-D array spectrograph on the 12-inch reflecting telescope in the Korea Science Academy of KAIST in Busan, Korea. We adopted the International Commission on Illumination (CIE) in 1931 of three spectral sensitivity peaks for the human eye in short, medium and long wavelengths in visible light. The observed spectra were imposed on CIE sensitivities and the color detected by the human eye was derived. The Mars spectrum represents red color and the Moon white. It is a similar color to that which a human would see. This result means that color is easily derived from astronomical spectra. The appearance of the planets surface can be determined for Mars, which is the result of iron oxide.

• 한국농림기상학회지
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• 제23권1호
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• pp.82-88
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• 2021

원격탐사 기법을 이용하여 산출된 태양 유도 엽록소 형광(Sun-Induced Fluorescence, SIF)을 통해 식생의 광합성 효율 및 스트레스 상태를 이해하기 위한 노력이 세계적으로 진행되고 있다. 최근 SIF 관측을 위한 광학 기기 개발과 SIF 산출 방법론이 정립되고 있으나 아직 국내에서는 SIF 관측이 드물며 관측 자료의 수도 적다. 본고에서는 나주에서 2020년 6월 10일부터 2020년 10월 5일까지 벼 생육기간 동안 광학 기기를 이용하여 관측된 SIF 자료를 공개하였다. SFM 방법과 iFLD 방법으로 O2A과 O2B 흡수 대역의 SIF를 산출하였으며, 광합성 유효 복사량에 대한 정보도 제공하였다. 또한, 태양천정각, 센서의 광 포화상태, 관측 순간의 태양광의 급격한 변화, 태양광 정반사 영향 등을 고려하여 품질이 낮은 SIF 자료를 필터링하였다. 본 자료를 통해 연구자들이 SIF에 대한 이해를 높이고, 제안된 SIF 자료 필터링 방법으로 SIF 산출물 품질관리에 도움이 될 것으로 기대한다.

• 한국작물학회지
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• 제42권2호
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• pp.173-181
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• 1997

태양복사 스펙트럼을 이용하여 벼 군락의 엽면적지수를 비파괴적인 방법으로 추정하고자 1993년 경기도 수원기상대 포장에서 조생종 진부벼와 중만생종 대청벼, 일품벼를 공시하여 벼 군락의 태양광 반사특성과 엽면적지수의 시기별 변화를 조사한 결과는 다음과 같다. 1. 출수이전의 생육기간동안에 태양광의 파장별 반사율은 가시광 파장대에서는 0.1이하로 낮았고, 근적외광 파장대에서는 0.1∼0.5 이상이었다. 가시광 파장대에서는 LAI가 증가할수록 반사율이 감소하였고, 근적외광 파장대는 LAI가 증가할수록 반사율도 증가하였다. 2. 출수전에 근적외광 파장대(720∼1,100nm)의 반사율을 가시광 파장대 (400∼700nm)의 반사율로 나눈 비율이 LAI와 높은 상관을 보였으며, 가시광 파장대중에서는 녹색, 적색파장보다 청색파장(400∼500nm)의 반사율로 나눈 비율이 높은 상관을 보였다. 3. 근적외광 파장의 반사율을 청색파장의 반사율로 나눈 비율중에서 특히 R910/R460 비율이 LAI와 가장 높은 정의 상관을 보였다. 4. 출수이전의 R910/R460과 LAI의 회귀식을 이용한 추정식 Y=0.160799-X0.79776는 실측치와의 상관관계가 매우 높았다. 5. 출수이후엔 근적외광 파장(720∼1,100nm)의 반사율을 적색파장(600∼700nm)의 반사율로 나눈 비율이 청색이나 녹색파장의 반사율로 나눈 것보다 LAI와의 상관이 높았다.

• 한국환경과학회:학술대회논문집
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• 한국환경과학회 2003년도 International Symposium on Clean Environment
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• pp.232-235
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• 2003

In general, the parameters of climate change include aerosol chemical compounds, aerosol optical depth, greenhouse gases(carbon dioxide, CFCs, methane, nitrous oxide, tropospheric ozone), ozone distribution, precipitation acidity and chemical compounds, persistent organic pollutants and heavy metals, radioactivity, solar radiation including ultra-violet and standard meteorological parameters. Over the last ten years, the monitoring activities of Korea regarding to the climate change have been progressed within the WMO GAW and ACE-Asia IOP programs centered at the observation sites of Anmyeon and Jeju Gosan islands respectively. The Greenhouse gases were pointed out that standard air quality monitoring techniques are required to enhance data comparability and that data presentation formats need to be harmonized and easily understood. Especially, the impact of atmospheric aerosols on climate depends on their optical properties, which, in turn, are a function of aerosol size distribution and the spectral reflective indices. Aerosol optical depth and single scattering albedo in the visible are used as the two basic parameters in the atmospheric temperature variation studies. The former parameter is an indicator of the attenuation power of aerosols, while the latter represents the relative strength of scattering and absorption by aerosols. For aerosols with weak absorption, surface temperature decreases as the optical depth increases because of the domination of backscattering. For aerosols with strong absorption, however, warming could occur as the optical depth increases. The objective of the study is to characterize the means, variability, and trends of Greenhouse gases and aerosol properties on a regional basis using data from its baseline observatories in Korea peninsula. A further goal is to understand the factors that control radiative forcing of the greenhouse and aerosol.