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      KCI등재 SCOPUS

      Korea Pathfinder Lunar Orbiter Magnetometer Instrument and Initial Data Processing

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      https://www.riss.kr/link?id=A108884887

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      다국어 초록 (Multilingual Abstract)

      The Korea Pathfinder Lunar Orbiter (KPLO), the first South Korea lunar exploration probe, successfully arrived at the Moon on December, 2022 (UTC), following a 4.5-month ballistic lunar transfer (BLT) trajectory. Since the launch (4 August, 2022), the KPLO magnetometer (KMAG) has carried out various observations during the trans-lunar cruise phase and a 100 km altitude lunar polar orbit. KMAG consists of three fluxgate magnetometers capable of measuring magnetic fields within a ± 1,000 nT range with a resolution of 0.2 nT. The sampling rate is 10 Hz. During the originally planned lifetime of one year, KMAG has been operating successfully while performing observations of lunar crustal magnetic fields, magnetic fields induced in the lunar interior, and various solar wind events. The calibration and offset processes were performed during the TLC phase.
      In addition, reliabilities of the KMAG lunar magnetic field observations have been verified by comparing them with the surface vector mapping (SVM) data. If the KPLO’s mission orbit during the extended mission phase is close enough to the lunar surface, KMAG will contribute to updating the lunar surface magnetic field map and will provide insights into the lunar interior structure and lunar space environment.
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      The Korea Pathfinder Lunar Orbiter (KPLO), the first South Korea lunar exploration probe, successfully arrived at the Moon on December, 2022 (UTC), following a 4.5-month ballistic lunar transfer (BLT) trajectory. Since the launch (4 August, 2022), the...

      The Korea Pathfinder Lunar Orbiter (KPLO), the first South Korea lunar exploration probe, successfully arrived at the Moon on December, 2022 (UTC), following a 4.5-month ballistic lunar transfer (BLT) trajectory. Since the launch (4 August, 2022), the KPLO magnetometer (KMAG) has carried out various observations during the trans-lunar cruise phase and a 100 km altitude lunar polar orbit. KMAG consists of three fluxgate magnetometers capable of measuring magnetic fields within a ± 1,000 nT range with a resolution of 0.2 nT. The sampling rate is 10 Hz. During the originally planned lifetime of one year, KMAG has been operating successfully while performing observations of lunar crustal magnetic fields, magnetic fields induced in the lunar interior, and various solar wind events. The calibration and offset processes were performed during the TLC phase.
      In addition, reliabilities of the KMAG lunar magnetic field observations have been verified by comparing them with the surface vector mapping (SVM) data. If the KPLO’s mission orbit during the extended mission phase is close enough to the lunar surface, KMAG will contribute to updating the lunar surface magnetic field map and will provide insights into the lunar interior structure and lunar space environment.

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      참고문헌 (Reference)

      1 손대락, "피드백형 플럭스게이트 마그네토미터 제작" 한국자기학회 22 (22): 45-48, 2012

      2 Haviland HF, "Time-dependent hybrid plasma simulations of lunar electromagnetic induction in the solar wind" 46 : 4151-4160, 2019

      3 Davis L Jr, "The in-flight determination of spacecraft magnetic field zeros" 49 : 257-, 1968

      4 Maggiolo R, "The delayed time response of geomagnetic activity to the solar wind" 122 : 11109-11127, 2017

      5 Auster HU, "The THEMIS fluxgate magnetometer" 141 : 235-264, 2008

      6 Hood LL, "The Moon : sources of the crustal magnetic anomalies" 204 : 53-57, 1979

      7 Kato M, "The Kaguya mission overview" 154 : 3-19, 2010

      8 Dyal P, "The Apollo 12 magnetometer experiment:internal lunar properties from transient and steady magnetic field measurements" 1971

      9 Dyal P, "Structure of the lunar interior from magnetic field measurements" 1976

      10 Magnes W, "Space weather magnetometer aboard GEO-KOMPSAT2A" 216 : 119-, 2020

      1 손대락, "피드백형 플럭스게이트 마그네토미터 제작" 한국자기학회 22 (22): 45-48, 2012

      2 Haviland HF, "Time-dependent hybrid plasma simulations of lunar electromagnetic induction in the solar wind" 46 : 4151-4160, 2019

      3 Davis L Jr, "The in-flight determination of spacecraft magnetic field zeros" 49 : 257-, 1968

      4 Maggiolo R, "The delayed time response of geomagnetic activity to the solar wind" 122 : 11109-11127, 2017

      5 Auster HU, "The THEMIS fluxgate magnetometer" 141 : 235-264, 2008

      6 Hood LL, "The Moon : sources of the crustal magnetic anomalies" 204 : 53-57, 1979

      7 Kato M, "The Kaguya mission overview" 154 : 3-19, 2010

      8 Dyal P, "The Apollo 12 magnetometer experiment:internal lunar properties from transient and steady magnetic field measurements" 1971

      9 Dyal P, "Structure of the lunar interior from magnetic field measurements" 1976

      10 Magnes W, "Space weather magnetometer aboard GEO-KOMPSAT2A" 216 : 119-, 2020

      11 Garrick-Bethell I, "Reiner gamma : a magnetized elliptical disk on the Moon" 46 : 5065-5074, 2019

      12 Song YJ, "Overview of the flight dynamics subsystem for Korea Pathfinder Lunar Orbiter mission" 8 : 222-, 2021

      13 Russell CT, "Measurements of the lunar induced magnetic moment in the geomagnetic tail:evidence for a lunar core?" 1981

      14 Shue JH, "Magnetopause location under extreme solar wind conditions" 103 : 17691-17700, 1998

      15 Tsunakawa H, "Lunar magnetic field observation and initial global mapping of lunar magnetic anomalies by MAP-LMAG onboard SELENE (Kaguya)" 154 : 219-251, 2010

      16 Binder AB, "Lunar Prospector : overview" 281 : 1475-1476, 1998

      17 Belcher JW, "Large-amplitude Alfvén waves in the interplanetary medium, 2" 76 : 3534-3563, 1971

      18 Lee H, "KMAG : KPLO magnetometer payload" 133 : 034506-, 2021

      19 Song YJ, "KARI and NASA JSC collaborative endeavors for joint Korea Pathfinder Lunar Orbiter flight dynamics operations: architecture, challenges, successes, and lessons learned" 10 : 664-, 2023

      20 Ness NF, "Initial results of the Imp 1 magnetic field experiment" 69 : 3531-3569, 1964

      21 Hood LL, "Initial measurements of the lunar induced magnetic dipole moment using Lunar Prospector magnetometer data" 26 : 2327-2330, 1999

      22 Takahashi F, "In-orbit calibration of the lunar magnetometer onboard SELENE(KAGUYA)" 61 : 1269-1274, 2009

      23 Kim JH, "Development of KPLO science data archive for public release" 2017

      24 Baek SM, "Detailed study of the Mare Crisium northern magnetic anomaly" 122 : 411-430, 2017

      25 Fairfield DH, "Average and unusual locations of the Earth’s magnetopause and bow shock" 76 : 6700-6716, 1971

      26 Park HH, "Analysis of the KPLO magnetic cleanliness for the KMAG instrument" 69 : 1198-1204, 2022

      27 Leinweber HK, "An advanced approach to finding magnetometer zero levels in the interplanetary magnetic field" 19 : 055104-, 2008

      28 Kepko EL, "Accurate determination of magnetic field gradients from four point vector measurements. I. Use of natural constraints on vector data obtained from a single spinning spacecraft" 32 : 377-385, 1996

      29 Belcher JW, "A variation of the Davis-Smith method for in-flight determination of spacecraft magnetic fields" 78 : 6480-6490, 1973

      30 Richmond NC, "A preliminary global map of the vector lunar crustal magnetic field based on Lunar Prospector magnetometer data" 113 : E02010-, 2008

      31 Farrell WM, "A method of calibrating magnetometers on a spinning spacecraft" 31 : 966-972, 1995

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