• 한국환경생태학회지
• /
• 제32권3호
• /
• pp.342-350
• /
• 2018

본 연구는 한국 중부 도심지에서 우점하는 참매미와 말매미를 대상으로 울음 시작 및 종료에 영향을 미치는 환경요인을 규명하는데 그 목적이 있다. 연구대상지는 서울시 반포아파트였고. 연구기간은 2015년 7월 말부터 8월 말까지 2개월이었다. 매미 울음의 시작 및 종료시각 분석 결과 참매미는 평균 5시 21분에, 말매미는 7시 40분에 울음을 시작하였다. 울음 종료는 참매미는 평균 18시 31분, 말매미는 평균 19시 51분에 울음을 종료하였다. 산점도와 상자도표 작성 결과, 참매미는 05시에 규칙적으로 울음을 시작하였고, 말매미는 20시에 참매미와 비교해서 규칙적으로 울음을 그치는 패턴을 보였다. 매미 울음 시작 및 종료시각과 환경요인 간 다중회귀분석 결과, 참매미 울음 시작은 일출시각만이 영향을 미치는 요인으로 선택되었다. 참매미 울음 종료시각은 일몰시각과 전운량이 영향을 미치는 것으로 나타났다. 말매미 울음 시작 시각은 주로 기온과 일출시각에 영향을 받는 것으로 나타났는데, 이 중 기온요인의 영향력이 더 큰 것으로 나타났다. 말매미 울음 종료 시각은 일몰시각에 의해 강하게 영향을 받으며, 이외에 최고기온이 영향을 미치는 것으로 나타났다. 이상의 내용을 종합해보면 참매미의 울음 시작 및 종료에 영향을 미치는 핵심 요인은 일출과 일몰로 판단된다. 이로 인해 일출과 동시에 울음을 시작하고, 종료 시각 또한 일몰에 영향을 받는 것으로 보인다. 말매미는 울음 시작 원인요인은 기온이고, 울음 종료 요인은 일몰로 판단되었다. 이로 인해 말매미 울음 시작은 당일 기온 변화에 따라 편차가 발생하지만, 울음 종료 요인은 일몰과 동시에 일제히 울음을 종료하는 것으로 나타났다.

• Journal of Astronomy and Space Sciences
• /
• 제30권4호
• /
• pp.327-334
• /
• 2013

The purpose of this study is to develop an observation program for obtaining effective flat images that are necessary for photometric observation. The development of the program was achieved by improving the existing method for obtaining twilight flat images. The existing method for obtaining twilight flat images acquires flat images by observing the sky light after sunset or light before sunrise. The decision of when to observe flat images at each night is solely dependent on the judgment of an observer, and thus the obtained flat images for particular nights may not be clean. Especially, in the case of the observatories where an automated observation system is in operation, there is a difficulty that an observer should pay attention during sunrise and sunset in order to obtain flat images. In this study, a computer program is developed to improve this inconvenience and to efficiently perform photometric observation in the observatories where an automated observation system is applied. This program can obtain flat images by calculating the time for obtaining flat images automatically and the exposure time using a numerically calculated function. When obtaining twilight flat images at dusk and at dawn, the developed program performs automated observation and provides effective flat images by acquiring appropriate exposure time considering the sunrise and sunset times that vary depending on the day of observation. The code for performing this task was added to Obs Tool II (Yoon et al. 2006), which is the automated observation system of the Chungbuk National University Observatory, and the usefulness of the developed program was examined by performing an actual automated observation. If this program is applied to other observatories where automated observation is in operation, it is expected that stable and high-quality flat images could be obtained, which can be used for the pre-processing of photometric observation data.

• 한국환경농학회지
• /
• 제30권4호
• /
• pp.382-389
• /
• 2011

BACKGROUND: Light-emitting diodes (LEDs) with lower electric cost and the specific wavelength have been considering as a novel light source for plant production in greenhouse conditions as well as in a closed culture system. Supplementary lighting for day-length extension was considered as light intensity, light quality, and/or photoperiod control on plant growth and development. Effects of supplementary blue or red LED radiation with lower light intensity on growth of Ageratum (Ageratum houstonianum Mill., cv. Blue Field), African marigold (Tagetes erecta L., cv. Orange Boy), and Salvia (Salvia splendens F. Sello ex Ruem & Schult., cv. Red Vista) were discussed during sunrise and sunset twilight in the experiment. METHODS AND RESULTS: Supplementary lighting by blue and red LEDs for 30 (Treatment B30; R30) or 60 (Treatment B60; R60) min. per day were established in greenhouse conditions. Photosynthetic photon flux for supplementary radiation was kept at $15{\mu}mol\;m^{-2}\;s^{-1}$ on the culture bed. Natural condition without supplementary light was considered as a control. The highest shoot and root dry weights were shown in African marigold exposed by red light for 60 min. per day. Supplementary blue and red lighting regardless of the radiation time significantly stimulated development of lateral branches in African marigold. Stem growth in Ageratum and Salvia seedlings was significantly promoted by red radiation as well as natural light. CONCLUSIONS: Extending of the radiation time at sunrise and sunset twilight using LEDs stimulated reproductive growth of flowering plant species. Different characteristics on growth under supplementary blue or red lighting conditions were also observed in the seedlings during supplementary radiation.

• 대기
• /
• 제24권1호
• /
• pp.17-27
• /
• 2014

In this study, the observational environment for sunshine duration at Seoul and Daegu Automated Synoptic Observing Systems (ASOSs) was analyzed using a numerical model. In order to analyze the effects of topography and buildings on observational environment for sunshine duration, the model domains including the elevated building and mountainous areas around Seoul and Daegu ASOSs were considered. Three dimensional topography and buildings used as input data for the numerical model were constructed using a geographic information system (GIS) data. Solar azimuth and altitude angles calculated for the analysis period (one-week for each season in 2008) in this study were validated against those by Korea Astronomy and Space Science Institute (KASI). The starting and ending times of sunshine duration observed at ASOSs largely differed from the respective sunrise and sunset times simply calculated using solar angles and information of ASOSs' latitude and longitude, because uneven topography and elevated buildings around ASOSs cut off sunshine duration right after the sunrise and right before the sunset. The model produced the sunshine indices for Seoul and Daegu ASOSs with the time interval of one minute and the period of one week for each season and we compared the hourly averaged indices with those observed at the ASOSs. One week of which the cloudiness is lowest for each season is selected for analysis. Not only the adjacent buildings but also distant buildings and mountain cut off sunshine duration right after the sunrise and right before the sunset. The buildings and topography cutting off sunshine duration were found for each analyzing date. It was suggested that, in order to evaluate the observational environment for sunshine duration, we need to consider even the information of topography and/or building far away from ASOSs. This study also showed that the analyzing method considering the GIS data is very useful for evaluation of observational environment for sunshine duration.

• 수산해양기술연구
• /
• 제58권4호
• /
• pp.317-325
• /
• 2022

Korean tuna purse seine fishery in the Western and Central Pacific Ocean (WCPO) began to operate in earnest in the early 1980s. Since then, the total catch has shown an increasing trend and the target species are skipjack tuna (Katsuwonus pelamis), yellowfin tuna (Thunnus albacare) and bigeye tuna (Thunnus obesus). Based on the operational data of Korean tuna purse seine fishery from 2016 to 2020, the catch rates of target species (skipjack and yellowfin tunas) were analyzed by operation time for set types (free school and FAD sets). In the case of the free school sets, they were usually made from sunrise to sunset, and the catch rate was high before and after sunrise for skipjack tuna and before sunset for yellowfin tuna. On the other hand, for the FAD sets, more than 90% of them were made just before sunrise, and there were few operations during the daytime. The purpose of this study is to examine whether there are differences in the catch rate of skipjack and yellowfin tunas by operation time and by school type for Korean tuna purse seine fishery in the WCPO, which could be helpful in understanding its fishing characteristics and providing useful information for developing the stock indices of the target species.

• 한국환경복원기술학회지
• /
• 제13권1호
• /
• pp.40-46
• /
• 2010

In urban area, inversion layer prevents air pollutants from being dispersed. To determine nocturnal inversion characteristics at SookMyung Girls' High School near high-rise residential commercial complex buildings in Seoul, air temperature and humidity data were observed at 10minute interval from December 1st, 2007 to May 2nd, 2008. Temperature-Humidity (T-H) sensors were installed at SMG (SookMyung_Ground) and SMR (SookMyung_Roof), and then these two data were compared, analyzed and examined to illustrate air temperature differences of SMG and SMR. After the analysis, the maximum nocturnal inversion was observed by $3.3^{\circ}C$ at 18:10 on December 26th 2007, at that time the weather condition was clear and weak wind. Nocturnal inversions began 2-3 hours before sunset and it reached maximum inversion just after sunset and continued through nighttime until sunrise or 1-2 hours after sunrise. In terms of seasonal variation nocturnal inversions occurred dominantly in March and April rather than winter season.

• 한국환경과학회지
• /
• 제8권5호
• /
• pp.633-637
• /
• 1999

A series of meterological observation using automation weather station(AWS) carried out to investigate characteristics of nocturnal meteorological parameters for 16~17 June 1998 at Buljeongdong mountain slope, Kyungbuk. Dry temperature at valley was lower than mountain because of high lapse rate at valley, so the strong inversion layer occurrenced at mountain slope for nighttime. Contrary of dry temperature, relative humidity of valley was higher than mountain for nighttime. Wind speed at valley from sunset to next day morning was lower than mountain, but that of valley after sunrise was higher than mountain. Wind direction at valley for all observation time were southeasterlies(SE), that of mountain for nighttime were northeasterlies(NE) or northnorthwesterlies(NNW), and that of mountain after sunrise were irregular. Vapor pressure at valley for all observation time was higher mountain, particularly the difference was high for nighttime.

• Journal of Astronomy and Space Sciences
• /
• 제28권3호
• /
• pp.173-181
• /
• 2011

Korea Astronomy and Space Science Institute researchers have installed and operated magnetometers at Mt. Bohyun Observatory to measure the Earth's magnetic field variations in South Korea. We, in 2007, installed a fluxgate magnetometer (RFP-523C) to measure H, D, and Z components of the geomagnetic field. In addition, in 2009, we installed a Overhauser proton sensor to measure the absolute total magnetic field F and a three-axis magneto-impedance sensor for spectrum analysis. Currently three types of magnetometer data have been accumulated. In this paper, we provide the preliminary and the first statistical analysis using the BOH magnetometer installed at Mt. Bohyun Observatory. By superposed analysis, we find that daily variations of H, D, and Z shows similar tendency, that is, about 30 minutes before the meridian (11:28) a minimum appears and the time after about 3 hours and 30 minutes (15:28) a maximum appears. Also, a quiet interval start time (19:06) is near the sunset time, and a quiet interval end time (06:40) is near the sunrise time. From the sunset to the sunrise, the value of H has a nearly constant interval, that is, the sun affects the changes in H values. Seasonal variations show similar dependences to the sun. Local time variations show that noon region has the biggest variations and midnight region has the smallest variations. We compare the correlations between geomagnetic variations and activity indices as we expect the geomagnetic variation would contain the effects of geomagnetic activity variations. As a result, the correlation coefficient between H and Dst is the highest (r = 0.947), and other AL, AE, AU index and showed a high correlation. Therefore, the effects of geomagnetic storms and geomagnetic substorms might contribute to the geomagnetic changes significantly.

• 에너지공학
• /
• 제19권2호
• /
• pp.128-135
• /
• 2010

본 연구에서는 LabVIEW를 활용한 임베디드 태양추적장치가 개발되었다. 이 시스템은 LabVIEW로 작성된 소프트웨어, CompactRIO, C-계열의 모션 인터페이스 모듈, 아날로그 수집 모듈(DAQ:Data Acquisition), 스텝 드라이브, 스텝 모터, 피드백디바이스 그리고 기타 부품들로 구성되어져 있다. CompactRIO는 내부에 리얼타임 프로세서를 내장하고 있으며 이는 태양추적장치가 외부 제어없이도 자동으로 작동이 가능하게 한다. 태양 추적장치의 정확도를 높이기 위하여 천문학적인 방법과 광학적인 방법을 통합하여 개발하였다. 광학적인 방법에서는 피드백디바이스가 사용되었는데 4개의 CdS를 사용하여 지속적으로 피드백 신호를 컨트롤러로 공급하여 문제 발생시에도 태양을 지속적으로 추적한다. 태양의 고도 및 방위각의 데이터베이스는 미국의 Naval Observatory의 데이터와 비교하였다.

• 에너지공학
• /
• 제20권4호
• /
• pp.353-357
• /
• 2011

본 연구에서는 AVR 마이크로 컨트롤러를 사용하여 임베디드 태양추적장치를 개발하였다. 본 시스템은 Atmega128 마이크로 컨트롤러, 스텝 모터, 스텝 드라이브 모듈, CdS 센서 그리고 GPS 모듈 및 기타 부품들로 구성되어 있다. 태양추적장치는 광학적 방법과 천문학적인 방법에 의해 작동된다. 최초 태양추적은 천문학적인 계산방법에 의해 얻어진 결과에 따라 이루어지고 CdS에 의해 미세 조정이 이루어진다. 태양추적장치가 설치된 지점에서 GPS는 UTC(Universal Time Coordinated)와 위도 및 경도 데이터를 마이크로 컨트롤러에 전송한다. 전송되어진 데이터에 의해 실시간으로 태양위치, 일출 및 일몰시간이 계산되어 진다. 태양 추적에 필요한 데이터들은 범용 비동기화 송수신기(UART)를 통하여 컴퓨터로 전송 받을 수 있다.