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논문 기본 정보

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학술저널
저자정보
Dae-Young Lee (Department of Astronomy and Space Science, Chungbuk National University) 김록순 (한국천문연구원) Kyung-Eun Choi (Space Sciences Laboratory, University of California) 서정준 (한국천문연구원) Junga Hwang (Korea Astronomy and Space Science Institute) Dooyoung Choi (Chungbuk National University) 유지현 (충북대학교) 이승욱 (충북대학교) Sung Jun Noh (ISR-1: Space Science and Applications, Los Alamos National Laboratory, Los Alamos) Jongho Seon (Kyung Hee University) Kyung-Suk Cho (Korea Astronomy and Space Science Institute) Kwangsun Ryu (Korea Advanced Institute of Science and Technology) 김관혁 (경희대학교) Jongdae Sohn (Korea Astronomy and Space Science Institute) Jaeyoung Kwak (Korea Astronomy and Space Science Institute) Peter H. Yoon (University of Maryland)
저널정보
한국우주과학회 Journal of Astronomy and Space Sciences Journal of Astronomy and Space Sciences Vol.41 No.1
발행연도
2024.3
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1 - 15 (15page)

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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.

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