• 한국해양학회지:바다
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• 제24권2호
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• pp.208-225
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• 2019

동해의 평균 표층 순환과 표층 해류의 변동성을 이해하기 위하여 1991년부터 2017년까지 동해를 지나간 표층 뜰개들의 궤적을 분석하였다. 표층 뜰개 자료를 분석하여 동해 표층 해류들을 그 주경로 별로 분류하고, 이들 해류의 변동을 조사하였다. 동한난류는 한국 동해안을 따라 북쪽으로 흐르며 $36{\sim}38^{\circ}N$에서 이안한 후 동해 중앙($131{\sim}137^{\circ}E$)에서 동쪽으로 흐른다. 이때 해류 경로의 평균 위도는 $36{\sim}40^{\circ}N$의 범위를 가지며, 남북으로 큰 진폭을 갖고 사행한다. 표층 뜰개 경로의 평균 위도가 $37.5^{\circ}N$ 이남(이북)일 때 사행진폭이 상대적으로 크며(작으며) 진폭은 약 100 (50) km이다. 동해 중앙에서 표층 뜰개들은 $37.5{\sim}38.5^{\circ}N$를 따라 동쪽으로 흐르는 경로를 가장 빈번하게 지나간다. 동해 북부 블라디보스토크 연안에 투하된 표층 뜰개들은 연안을 따라 남서쪽으로 이동하다가 일본분지 서쪽에서 반시계방향 순환을 따라 남동쪽으로 이동한 후 $39{\sim}40^{\circ}N$에서 동쪽으로 사행하여 이동한다. 다음으로 동해를 $0.25^{\circ}$ 간격으로 격자를 나누어 각 격자를 통과하는 표층 뜰개들의 이동 속도 벡터 자료로 동해 평균 표층 해류 벡터장과 속력장을 구하였다. 그리고 $0.5^{\circ}$ 격자 간격으로 해류장의 분산타원을 계산하였다. 울릉분지 서쪽에서는 동한난류의 경로가 매년 변화하고, 야마토분지에서는 해류의 사행과 소용돌이가 많아 해류의 변동성(분산)이 크다. 표층 뜰개의 주 이동 경로, 평균 해류 벡터장, 분산을 모두 반영하여 표층 뜰개 자료에 근거한 동해 표층 해류 모식도를 제시하였다. 이 연구는 그동안 인공위성 고도계 자료를 이용하여 구한 표층 지형류와 해양수치모델로 모의한 해류를 중심으로 연구해 왔던 동해 표층 순환을 라그랑지 관측 자료를 통해 정리했다는 데 의의가 있다.

• 대기
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• 제23권2호
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• pp.205-220
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• 2013

Upper ocean response to typhoon Ewiniar (0603) and its impact on the following typhoon Bilis (0604) are investigated using observational data and numerical experiments. Data used in this study are obtained from the Ieodo Ocean Research Station (IORS), ARGO, and satellite. Numerical simulations are conducted using 3-dimensional Princeton Ocean Model. Results show that when Ewiniar passes over the western North Pacific, unique oceanic responses are found at two places, One is in East China Sea near Taiwan and another is in the vicinity of IORS. The latter are characterized by a strong sea surface cooling (SSC), $6^{\circ}C$ and $11^{\circ}C$ in simulation and observation, under the condition of typhoon with a fast translation speed (8m $s^{-1}$) and lowering intensity (970 hPa). The record-breaking strong SSC is caused by the Yellow Sea Bottom Cold Water, which produces a strong vertical temperature gradient within a shallow depth of Yellow Sea. The former are also characterized by a strong SSC, $7.5^{\circ}C$ in simulation, with a additional cooling of $4.5^{\circ}C$ after a storm's passage mainly due to enhanced and maintained upwelling process by the resonance coupling of storm translation speed and the gravest mode internal wave phase speed. The numerical simulation reveals that the Ewiniar produced a unfavorable upper-ocean thermal condition, which eventually inhibited the intensification of the following typhoon Bilis. Statistics show that 9% of the typhoons in western North Pacific are influenced by cold wakes produced by a proceeding typhoon. These overall results demonstrate that upper ocean response to a typhoon even after the passage is also important factor to be considered for an accurate intensity prediction of a following typhoon with similar track.

• 대기
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• 제15권4호
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• pp.229-239
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• 2005

The effect of inversion layer on the land and sea breeze near the Gangneung city was investigated. The land and sea breeze occurrence days were selected, and the height and the intensity of inversion layer were calculated with the upper air observational data of the Sokcho Station. The relationships between the temperature variation near the Gangneung and the inflow time, inland penetration and the inflow depth of the land and sea breeze were also analyzed. And the Gangwon Short-range prediction system was verified with the comparison of surface stream line by the Gangwon short-range prediction system with the AWS wind vector data. It was revealed that the inversion layer tended to block the sea breeze, shorten the inland penetration distance and lower the inflow depth, causing the temperature rise. The comparison and analysis of surface steam line by the Gangwon short-range prediction system and the AWS wind vector showed that the system quite well simulated the sea breeze, thus the system could be well utilized in the prediction of land and sea breeze.

• 한국해안해양공학회지
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• 제18권3호
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• pp.189-197
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• 2006

수치해석을 통하여 이어도 종합해양과학기지 구조물이 대기 유동에 미치는 영향을 분석하였고, 이 결과를 바탕으로 과학기지에 설치된 풍속센서에서의 측정값 오차를 평가하는 연구를 수행하였다. 과학기지 형상을 3차원으로 모델링하였고 수치해석을 위한 격자를 생성하여, Navier-Stokes 방정식 및 난류모델을 적용하여 수치해석을 수행하였다. 선정된 자유류의 풍속과 풍향 조건에 대하여 과학기지 구조물에 의해 변화된 유동장을 계산하고, 실제 풍속센서가 설치된 위치에서의 풍속/풍향 정보와 자유류를 비교하였다. 이를 통하여 자유류 방향 및 측정 위치에 따른 데이터의 정확도와 신뢰할 수 있는 데이터 범위를 알아보았다. 본 연구 결과로 관측된 해상풍 데이터의 구조물 간섭에 의한 오차 범위를 정량적으로 파악할 수 있었으며, 과학기지가 위치한 지점의 정확한 해상풍 데이터 제공을 위한 기초 자료로 활용될 것으로 기대된다.

• 대한원격탐사학회지
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• 제39권5_1호
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• pp.467-479
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• 2023

위성 고도계는 30년 동안 지속적으로 전 지구 대양에서 해수면고도를 관측하고 있으며, 전 지구 평균 해수면의 상승에 대한 명확한 근거를 제시하였다. 지역적인 해역에서 해수면고도의 시공간 변동성을 연구하기 위해서는 정확한 관측 자료가 필수적으로 요구된다. 본 연구에서는 외해에 위치한 이어도 해양과학기지 관측자료를 활용하여 인공위성(Envisat, Jason-1, Jason-2, SARAL, Jason-3, Sentinel-3A/B) 고도계 관측 해수면고도를 비교 검증하였다. 위성별 해수면고도 편차와 평균제곱근오차는 각각 1.58-4.69 cm와 6.33-9.67 cm를 나타냈다. 위성-이어도 일치점 거리가 멀어질수록 위성 해수면고도 관측 오차가 현저히 증폭되었다. 이어도 해양과학기지 관측 해수면고도를 조석 주기에 대해 조화분해 하였으며 대기압 자료를 활용하여 역기압효과를 계산하여 위성 고도계 자료의 조석 및 대기 효과 보정을 검증하였다. 한반도 주변 해역에서 위성 해수면고도 자료의 정확한 조석 보정을 위해서는 위성에 활용되는 조석 자료의 정확도 향상이 필요함을 확인하였다.

• 천문학회보
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• 제37권1호
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• pp.32.1-32.1
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• 2012

Radial color gradient of disk galaxies has been a key tool for diagnosing the ages and metallicities of the stars and gas of these galaxies, and thus, the formation process of these disks. In many cases, observational data support the 'inside-out' picture of disk galaxy formation proposed by Larson (1976). In this scenario, gas within dark matter halos cools and accretes on to the outer disk while enhancing star formation in the disk. Recent discoveries of "extended ultra-viloet" (XUV) disks also show that majority of disk galaxy experience active star formation within out disks where gas surface density is quite low (Thilker et al. 2007; Gil de Paz et al. 2007). However, neither gas, nor stars stay put within galaxies. They rather migrate into bulges, disperse throughout galaxies, or flow into and out of galaxies via various mechanisms. There have been a few notable studies to investigate how radial star formation and metal abundance gradients vary across populations of disk galaxies systematically. However, the mechanisms driving gas transport are still poorly understood. Cross-matching various galaxy catalogs including KVAGC and UKIDSS, we are investigating if color gradients of late-type galaxies depend on their physical properties, especially on environmental properties. We will present the result from the pilot study on Karachentsev isolated galaxy catalog.

• 한국수산과학회지
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• 제50권2호
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• pp.207-218
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• 2017

Seawater with salinity of 32.5 psu or less is observed in the southern Japan/East Sea (JES) every autumn. It is confined to a surface layer 30-45 m in depth that expands to cover the entire JES in October. Two sources of "autumn low-salinity water" have been identified from historical hydrographic data in the western JES: East China Sea (ECS) water mixed with fresh water discharge from the Yangtze River (Changjiang) and seawater diluted with melted sea ice in the northern JES. Low-salinity water inflow from the ECS begins in June and reaches its peak in September. Low-salinity water from the northern JES expands southward along the coast, and its horizontal distribution varies among years. A rare observational study of the entire JES in October 1969 indicated that water with salinity less than 33.0 psu covered the southwestern JES; the lowest salinity water was found near the Ulleung Basin. In October 1995, the vertical distribution of salinity observed in a meridional section revealed that water with salinity of 33.6 psu or less was present in the area north of the subpolar front.

• 천문학회보
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• 제39권1호
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• pp.52.1-52.1
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• 2014

Radio pulsars are highly magnetized, rapidly rotating neutron stars that emit synchrotron radiation along the magnetic axes at their spin frequencies. Traditionally, pulsar observations have been done at low frequencies (MHz up to a few GHz), since radio pulsar spectrum is known to a power-law with a steep negative spectral index. More recently, high-frequency pulsar observations (several GHz and above) have been made as a broadband spectrometer and fast computers became available. High-frequency pulsar observations will provide information on radio emission mechanism of pulsars in the vicinity of the neutron star surface. There is also huge interest from gravitational-wave and astrophysics community to find a pulsar in the center of our Galaxy. The Korean VLBI Network has three 21-m single dishes in the Korean peninsula. Using KVN's lowest observational frequency of 22-GHz, we performed test observations with the KVN targeting a few selected known, bright pulsars. In addition, we have been developing pulsar pipelines that can be utilized with a VLBI facility using Mark-V. We present a brief introduction of radio pulsars and show data obtained with the KVN.

• 대기
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• 제18권3호
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• pp.171-182
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• 2008

In this study, we analyzed the spatial and temporal distribution of wind resources over Korea based on hourly observational data recorded over a period of 5 years from 457 stations belonging to Korea Meteorological Administration (KMA). The surface and 850 hPa wind data obtained from the Korea Local Analysis and Prediction System (KLAPS) and the Regional Data Assimilation and Prediction System (RDAPS) over a period of 1 year are used as supplementary data sources. Wind speed is generally high over seashores, mountains, and islands. In 62 (13.5%) stations, mean wind speeds for 5 years are greater than $3ms^{-1}$. The effects of seasonal wind, land-sea breeze, and mountain-valley winds on wind resources over Korea are evaluated as follows: First, wind is weak during summer, particularly over the Sobaek Mountains. However, over the coastal region of the Gyeongnam-province, strong southwesterly winds are observed during summer owing to monsoon currents. Second, the wind speed decreases during night-time, particularly over the west coast, where the direction of the land breeze is opposite to that of the large-scale westerlies. Third, winds are not always strong over seashores and highly elevated areas. The wind speed is weaker over the seashore of the Gyeonggi-province than over the other seashores. High wind speed has been observed only at 5 stations out of the 22 high-altitude stations. Detailed information on the wind resources conditions at the 21 stations (15 inland stations and 6 island stations) with high wind speed in Korea, such as the mean wind speed, frequency of wind speed available (WSA) for electricity generation, shape and scale parameters of Weibull distribution, constancy of wind direction, and wind power density (WPD), have also been provided. Among total stations in Korea, the best possible wind resources for electricity generation are available at Gosan in Jeju Island (mean wind speed: $7.77ms^{-1}$, WSA: 92.6%, WPD: $683.9Wm^{-2}$) and at Mt. Gudeok in Busan (mean wind speed: $5.66ms^{-1}$, WSA: 91.0%, WPD: $215.7Wm^{-2}$).

• 천문학회보
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• 제40권1호
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• pp.56.3-57
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• 2015

As of early 2015, more than 12,000 Near-Earth Objects (NEOs) have been catalogued by the Minor Planet Center, however their observational properties such as broadband colors and rotational periods are known only for a small fraction of the population. Thanks to time series observations with the KMTNet, orbits, optical sizes (and albedo), spin states and three dimensional shapes of asteroids and comets including NEOs will be systematically investigated and archived for the first time. Based on SDSS and BVRI colors, their approximate surface mineralogy will also be characterized. This so-called DEEP-South (Deep Ecliptic Patrol of the Southern Sky) project will provide a prompt solution to the demand from the scientific community to bridge the gaps in global sky coverage with a coordinated use of the network of ground-based telescopes in the southern hemisphere. We will soon finish implementing dedicated software subsystem consisted of automated observation scheduler and data pipeline for the sake of increased discovery rate, rapid follow-up, timely phase coverage, and efficient data analysis. We will give a brief introduction to test runs conducted at CTIO with the first KMTNet telescope in February and March 2015 and experimental data processing. Preliminary scientific results will also be presented.