• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2008년도 한국우주과학회보 제17권2호
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• pp.32.2-32.2
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• 2008

A major solar radio burst can disturb many kinds of radio instruments, including cellular phone, GPS, and radar. Korea Astronomy and Space Science Institute (KASI) is developing Korean Solar Radio Burst Locator (KSRBL) in collaboration with New Jersey Institute of Technology. KSRBL is a single dish radio spectrograph, which records the spectra of microwave (0.5 - 18 GHz) bursts with 1 MHz spectral resolution and 1 s time cadence, and locates their positions on the solar disk within 2 arcmin. Hardware manufacturing is almost completed including 4-channel digitizer/FPGA. The system is currently installed at Owens Valley Radio Observatory (OVRO), and test of the operation is in progress. It will be installed at KASI in 2009. We report current status and test results of KSRBL.

• Journal of the Optical Society of Korea
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• 제16권2호
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• pp.141-144
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• 2012

A mobile Rayleigh Doppler wind LIDAR at an eye-safe wavelength of 355 nm incorporating double-edge technique with triple-channel Fabry-Perot etalon is developed for wind measurement from 5 to 40km. The structure of this LIDAR system is described. An intercomparsion experiment with rawinsonde is made, showing good agreement with expected measurement accuracy. A continuous observation of stratosphere wind field for several days with temporal resolution of 15 min and spatial resolution of 200 m from 5 to 40 km is presented, demonstrating the stability and robustness of the LIDAR. A stratospheric quasi-zero wind layer can be found at around 20 km with a direction change from east to west evident in the continuous observation.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2001년도 한국우주과학회보 제10권2호
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• pp.43-43
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• 2001

• 천문학회보
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• 제46권2호
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• pp.60.2-60.2
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• 2021

중력파 관측은 2015년에 사상 최초로 검출에 성공한 이래, 불과 5년 만에 주 1 회 이상 안정적으로 검출되고 있으며 검출기들의 성능이 계속 향상됨에 따라 관측 범위와 빈도가 급격히 확대되는 추세에 있다. 이제 중력파는 전자기파 외에 우주를 보는 새로운 창으로서 확고한 지위를 구축하고 있으며 향후 무궁무진한 발전의 잠재력을 보여주고 있다. 이러한 가능성을 일찌감치 내다본 미국과 유럽의 선도 국가들은 현재 운영 중인 LIGO와 Virgo 검출기의 지속적인 업그레이드는 물론 Cosmic Explorer, Einstein Telescope 등 차세대 거대 검출기 개발을 병행해서 진행하고 있으며, 일본, 인도, 중국, 호주 등 후발주자들도 제각기 다양한 중력파 검출기 계획들을 추진하고 있다. 이에 한국천문연구원에서도 2019년부터 중력파 검출기술 연구를 시작하였으며, 특히 한국과학기술원 물리학과와 협력하여 차세대 핵심기술인 양자잡음 저감기술을 중점적으로 개발하고 있다. 이 발표에서는 본 연구팀의 최근 연구 진행상황을 요약하고 국제 중력파 검출기 공동개발 참여 현황을 소개한다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 1996년도 한국우주과학회보 제5권2호
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• pp.22-22
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• 1996

No Abstract, See Full Text

• 천문학회보
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• 제32권1호
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• pp.35.1-35.1
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• 2007

• 천문학회보
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• 제34권1호
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• pp.78.2-78.2
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• 2009

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2006년도 한국우주과학회보 제15권1호
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• pp.30-30
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• 2006

• 천문학회보
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• 제44권2호
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• pp.42.2-42.2
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• 2019

Korea Astronomy and Space Science Institute (KASI) has been developing a next-generation coronagraph (NGC) in cooperation with NASA to measure the coronal electron density, temperature, and speed using four different filters around 400 nm. To demonstrate technology for the measurement through the 2017 total solar eclipse across the USA, KASI organized an expedition team to demonstrate the coronagraph measurement scheme and the instrumental technology. The observation site was in Jackson Hole, Wyoming, USA. We built an eclipse observation system, so-called Diagnostic Coronal Experiment (DICE), which is composed of two identical telescopes to improve a signal to noise ratio. The observation was conducted with 4 wavelengths and 3 linear polarization directions according to the planned schedule in a limited total eclipse time of about 140 seconds.Polarization information of corona from the data was successfully obtained but we failed to get the coronal electron temperature and speed information due to a low signal-to-noise ratio of the optical system. In this study, we report the development of DICE and observation results. TSE observation and analysis by using our own developed instrument gave an important lesson that a coronagraph should be carefully designed to archive the scientific purpose. This experience through TSE observation will be very useful for a success of NASA-KASI joint missions called the Balloon-borne Investigation of the Temperature and Speed of Electrons in the Corona (BITSE) and COronal Diagnostic EXperiment (CODEX).

• International Journal of Aeronautical and Space Sciences
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• 제12권3호
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• pp.283-287
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• 2011

Science and Technology Satellite-3 (STSAT-3) is a 150 kg class micro satellite based with the national space program. The STSAT-3 system consists of a space segment, ground segment, launch service segment, and various external interfaces including additional ground stations to support launch and early operation phases. The major ground segment is the ground station at the Satellite Technology Research Center, Korea Advanced Institute of Science and Technology site. The ground station provides the capability to monitor and control STSAT-3, conduct STSAT-3 mission planning, and receive, process, and distribute STSAT-3 payload data to satisfy the overall missions of STSAT-3. The ground station consists of the mission control element and the data receiving element. This ground station is designed with the concept of low cost and high efficiency. In this paper, the requirements and design of the ground station that has been developed are examined.