• Title/Summary/Keyword: space technology

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ALMA OBSERVATIONS OF W HYDRAE: IMPACT OF MISSING BASELINES

  • Do, Thi Hoai;Pham, Tuan Anh;Pham, Tuyet Nhung;Darriulat, Pierre;Pham, Ngoc Diep;Nguyen, Bich Ngoc;Tran, Thi Thai
    • Journal of The Korean Astronomical Society
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    • v.54 no.6
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    • pp.171-182
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    • 2021
  • The lack of short baselines, referred to as the short-spacing problem (SSP), is a well-known limitation of the performance of radio interferometers, causing a reduction of the flux detected from source structure on large angular scales. The very large number of antennas operated in the Atacama Large Millimeter/sub-millimeter Array (ALMA) generates situations for which the impact of the SSP takes a complex form, not simply measurable by a single number, such as the maximal recoverable scale. In particular, extended antenna configurations, complemented by a small group of closeby antennas at the centre of the array, may result in a double-humped baseline distribution with a significant gap between the two groups. In such cases one should adopt as the effective maximal recoverable scale the one associated with the extended array and use only the central array to recover missing flux, as one would do with single dish or ACA (Atacama Compact Array) observations. The impact of the missing baselines can be very important and may easily be underestimated, or even overlooked. The present study uses ALMA archival data of the 29SiO(8-7) line emission of the AGB star W Hydrae for a demonstration. A critical discussion of the reliability of the observations away from the star is presented together with comments of a broader scope. Properties of the circumstellar envelope of W Hya within ~15 au from the star, many of which are not mentioned in the published literature, are briefly described and compared with R Doradus, an AGB star having properties very similar to W Hya.

Development and International Collaborations on Quantum Noise Reduction Technology for Gravitational Wave Detectors (중력파 검출기 양자잡음 저감기술 개발 및 국제협력)

  • Lee, Sungho;Kim, Chang-Hee;Park, June Gyu;Kim, Yunjong;Seong, Hyeon Cheol;Jeong, Ueejeong;Je, Soonkyu;Ra, Young-Sik;Gwak, Geunhee;Yoon, Youngdo;Go, Byeong Yoon;Kim, Hyunjin;Roh, Chan
    • The Bulletin of The Korean Astronomical Society
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    • v.46 no.2
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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.

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OVERVIEW OF KITSAT-1/2 MICROSATELLITE SYSTEMS (우리별 1, 2호 위성 시스템 개요)

  • 박성동;성단근;최순달
    • Journal of Astronomy and Space Sciences
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    • v.13 no.2
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    • pp.1-19
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    • 1996
  • Satellite Technology Research Center(SaTReC) of Korean Advanced Institute of Science and Technology(KAIST) has started a collaborative research, development, and training program in the field of space technology. As the result of that, SaTReC has successfully developed and operated the KISTAT-1, which is the first Korean satellite system. From the experience gained. SaTReC has developed the KITSAT-2 with its own technology and man-power and acquired the capability to design and to manufacture small satellite systems. In this paper, an overview of KITSAT-1/2 microsatellite systems and operational results are introduced.

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Analysis of the Adaptability and Methods of Public space in media - Focused on new-media and HCI theory - (공공공간에서 나타나는 미디어 특성에 관한 연구 - 뉴 미디어와 HCI 이론을 중심으로 -)

  • Koh, Gwi-Han;Kang, Seon-Gyung
    • Korean Institute of Interior Design Journal
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    • v.22 no.1
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    • pp.203-210
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    • 2013
  • With digital technology, space design is developing in a new direction with the changing paradigm. The space creates an interactive environment by motivating the User's active participation through the digital madia. In this social stream, it is very important to think about how this new paradigm affects the spatial design and the interactions between social changes and spatial design paradigm, so that we can understand design paradigm of our time. Hence, in this research, we will think about social characteristic and design paradigm of digital age by questioning how spatial design is changing in the digital age and how digital technology is affecting spatial design. this study analyzed about the space form, digital media setting, user interactivity of the examples of experience space using digital media. fields of our society, interactive space with the concept of HCI became a big issue in environmental design field. In this interactive space, various types of informative factors of the given space are sent using sensor and computer networking technology to the main system, and the main computer system sends manipulated output media to interactive devices. So, a user's movement in the space is more than just a movement itself user's movement now forms a important spatial structure that leads the narrative of the space. Researcher will analyze the characteristic of a public space and progress this research supposing that space needs this interactive design.

Long-Term Science Goals with In Situ Observations at the Sun-Earth Lagrange Point L4

  • Dae-Young Lee;Rok-Soon Kim;Kyung-Eun Choi;Jungjoon Seough;Junga Hwang;Dooyoung Choi;Ji-Hyeon Yoo;Seunguk Lee;Sung Jun Noh;Jongho Seon;Kyung-Suk Cho;Kwangsun Ryu;Khan-Hyuk Kim;Jong-Dae Sohn;Jae-Young Kwak;Peter H. Yoon
    • Journal of Astronomy and Space Sciences
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    • v.41 no.1
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    • pp.1-15
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    • 2024
  • The Korean heliospheric community, led by the Korea Astronomy and Space Science Institute (KASI), is currently assessing the viability of deploying a spacecraft at the Sun-Earth Lagrange Point L4 in collaboration with National Aeronautics and Space Administration (NASA). The aim of this mission is to utilize a combination of remote sensing and in situ instruments for comprehensive observations, complementing the capabilities of the L1 and L5 observatories. The paper outlines longterm scientific objectives, underscoring the significance of multi-point in-situ observations to better understand critical heliospheric phenomena. These include coronal mass ejections, magnetic flux ropes, heliospheric current sheets, kinetic waves and instabilities, suprathermal electrons and solar energetic particle events, as well as remote detection of solar radiation phenomena. Furthermore, the mission's significance in advancing space weather prediction and space radiation exposure assessment models through the integration of L4 observations is discussed. This article is concluded with an emphasis on the potential of L4 observations to propel advancements in heliospheric science.

Ground Station Design for STSAT-3

  • Kim, Kyung-Hee;Bang, Hyo-Choong;Chae, Jang-Soo;Park, Hong-Young;Lee, Sang-Hyun
    • International Journal of Aeronautical and Space Sciences
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    • v.12 no.3
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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.

Space Telescope Pre-study of KASI for the Next Decades (2030년대 우주망원경 운영을 대비한 한국천문연구원의 우주망원경 사전 연구)

  • Moon, Bongkon;Lee, Dae-Hee;Choi, Young-Jun;Han, Wonyong;Nam, Ukwon;Park, Youngsik;Park, Won-Kee;Lee, Duk-hang;Kim, Woojin;Han, Jeong-Yeol;Choi, Seonghwan;Kim, Jihun;Ko, Jongwan;Kim, Il-joong;Moon, Hong-Kyu
    • The Bulletin of The Korean Astronomical Society
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    • v.46 no.2
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    • pp.77.1-77.1
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    • 2021
  • 한국천문연구원은 천문우주분야의 과학임무 탑재체 개발을 주도적으로 수행해오고 있다. 과학기술위성1호 주탑재체 원자외선영상분광기 FIMS 개발, 과학기술위성3호 주탑재체 다목적적외선영상시스템 MIRIS 개발, 차세대소 형위성1호 주탑재체 근적외선영상분광기 NISS 개발을 수행하였고, 현재는 NASA와 국제협력으로 SPHEREx 우주 망원경을 개발하고 있다. 이러한 개발 과정을 거치면서 주경 20cm 이하의 소형 탑재체 과학임무 한계와 더불어 연구 현장에서 더 큰 우주망원경의 수요가 제기되었고, 현재의 국가우주개발 중장기계획에도 2030년대 한국형 우주망원경을 포함하게 되었다. 이러한 일정에 발맞추어 한국천문연구원은 2030년대 한국형 우주망원경 독자 운영을 대비하기 위해서 2020년 1월부터 주요 사업으로 한국형 우주망원경 개발을 위한 기획연구를 시작하였다. 이 기획연구는 2021년 말까지 2년 동안 수행하고 있으며, 이 기획연구를 통해서 학계의 과학임무 요구사항을 종합 수렴하였고, 관련 컨설팅 업체와 협업하여 사전 기획연구 활동들을 수행하였으며, 향후 우주망원경 개발에 대한 전략을 제안하고 보고서를 마무리하는 단계에 와 있다. 이 발표에서는 이러한 기획연구의 세부 활동을 공유하고 보고하고자 한다.

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