• 제목/요약/키워드: Space Astronomy

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Current Status and Future Prospects of Korean VLBI Network (KVN)

  • Jung, Taehyun;Sohn, Bong Won;So, Byunghwa;Oh, Chungsik;Je, Do-Heung;Byun, Do-Young;Jung, Dong-Kyu;Roh, Duk Gyoo;Lee, Euikyum;Kim, Hyo Ryoung;Kim, Hyun-Goo;Byun, Hyungkyu;Chung, Hyunsoo;Yim, In Sung;Kim, Jae-Young;Kim, Jaeheon;Yeom, Jaehwan;Shin, Jaesik;Park, Jeong-Je;Kim, Jeong-Sook;Hwang, Jungwook;Wajima, Kiyoaki;Song, Min-Gyu;Chung, Moon-Hee;Sakai, Nobuyuki;Lee, Sang-Hyun;Lee, Sang-Sung;Oh, Sej-Jin;Wi, Seog Oh;Kim, Seungrae;Kim, Soon-Wook;Lee, Sung-Mo;Kang, Yong-Woo;Minh, Young Chol;Kim, Young-Sik;Yun, Youngjoo
    • 천문학회보
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    • 제46권1호
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    • pp.60.3-61
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    • 2021
  • The Korean VLBI Network (KVN) consists of three 21m radio telescopes installed in Seoul, Ulsan, and Jeju Island with the world's first 4-channel receiver that can observe four different frequencies (e.g., 22, 43, 86, 129 GHz) simultaneously. This receiving system of KVN is particularly effective in millimeter-wavelength VLBI (mm-VLBI) observations by compensating fast atmospheric fluctuations effectively. This technology is now being enhanced with a compact triple-band receiver, becoming the world standard for a mm-VLBI system. In 2020, KVN supported 54 observing programs (KVN: 28, EAVN: 26) including the 2nd KVN Key Science Program (KSP) which supports 8Gbps data recording rate and the East Asian VLBI Network (EAVN) programs. KVN also participated in the European VLBI Network (EVN) and GMVA (Global Millimeter VLBI Array) sessions regularly. Here, we report current status and future propsects of KVN.

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Efficiency of DRAO Radio Telescope

  • Jung, Jae-Hoon;Auh, Byung-Ryul;Cho, Se-Hyung;Kim, Hyun-Goo;Kim, Bong-Gyu;Park, Yong-Sun;Roh, Duk-Gyoo;Hong, Jung-Ho;Lee, Chang-Hoon;Yim, In-Sung;Choi, Moon-Hang
    • 천문학회보
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    • 제14권
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    • pp.8.1-8.1
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    • 1989
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Thermal Analysis of MIRIS Space Observation Camera for Verification of Passive Cooling

  • Lee, Duk-Hang;Han, Won-Yong;Moon, Bong-Kon;Park, Young-Sik;Jeong, Woong-Seob;Park, Kwi-Jong;Lee, Dae-Hee;Pyo, Jeong-Hyun;Kim, Il-Joong;Kim, Min-Gyu;Matsumoto, Toshio
    • Journal of Astronomy and Space Sciences
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    • 제29권3호
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    • pp.305-313
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    • 2012
  • We conducted thermal analyses and cooling tests of the space observation camera (SOC) of the multi-purpose infrared imaging system (MIRIS) to verify passive cooling. The thermal analyses were conducted with NX 7.0 TMG for two cases of attitude of the MIRIS: for the worst hot case and normal case. Through the thermal analyses of the flight model, it was found that even in the worst case the telescope could be cooled to less than $206^{\circ}K$. This is similar to the results of the passive cooling test (${\sim}200.2^{\circ}K$). For the normal attitude case of the analysis, on the other hand, the SOC telescope was cooled to about $160^{\circ}K$ in 10 days. Based on the results of these analyses and the test, it was determined that the telescope of the MIRIS SOC could be successfully cooled to below $200^{\circ}K$ with passive cooling. The SOC is, therefore, expected to have optimal performance under cooled conditions in orbit.

Test Observations of 14m Radio Telescope(I)

  • Cho, Se-Hyung;Auh, Byung-Ryul;Jung, Jae-Hoon;Lee, Chang-Hoon;Kim, Hyun-Goo;Park, Yong-Sun;Roh, Duk-Gyoo;Yim, In-Sung;Kim, Bong-Gyu;Kim, Tu-Hwan
    • 천문학회보
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    • 제12권
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    • pp.11.1-11.1
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    • 1987
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Introduction of Space Weather Monitoring Lab at KASI

  • Moon, Yong-Jae;Choi, Seong-Hwan;Baek, Ji-Hye;Park, Young-Deuk;Cho, Kyung-Suk;Kim, Khan-Hyuk;Park, Hyung-Min;Kim, Yeon-Han;Bong, Su-Chan;Kim, Su-Jin;Park, Jin-Young;Hwang, Jung-A
    • 한국우주과학회:학술대회논문집(한국우주과학회보)
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    • 한국우주과학회 2007년도 한국우주과학회보 제16권1호
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    • pp.36-36
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    • 2007
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The Vibration Test Result of MIRIS

  • 정웅섭;문봉곤;차상목;박영식;이대희;이창희;남욱원;이미현;박성준;가능현;이덕행;박장현;;한원용
    • 천문학회보
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    • 제34권2호
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    • pp.64.2-64.2
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    • 2009
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