Lin,Chih-Hsun / Senior Research Scientist

Research Interest

• High energy experiments, Radiation hard electronics and testing, detectors for radiotherapy

獎項及殊榮

Experience

• 10/1999 – 07/2003Postdoctoral Associate at National Central University
• 08/2003 – 08/2005Assistant Research Scientist of National Science Council
• 09/2005 – 07/2009Associate Researcher at National Space Organization

Publication

Journal Papers

• [1]     AMS Collaboration, 2021, “Properties of Heavy Secondary Fluorine Cosmic Rays: Results from the Alpha Magnetic Spectrometer”, PHYSICAL REVIEW LETTERS, 126, 081102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [2]     AMS Collaboration, 2021, “The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II - Results from the first seven years”, PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 891, 1-116. (SCIE) (IF: 25.809; SCI ranking: 2.4%)
  
  
• [3]     Chien-Ying Yang, Yi-Chi Chang, Hung-Hsiang Liang, Che-Yen Chu, Jr-Yue Hsiang, Jeng-Lun Chiu, Chih-Hsun Lin,Philippe Laurent,Jerome Rodriguez, Hsiang-Kuang Chang, 2020, “Feasibility of Observing Gamma-Ray Polarization from Cygnus X-1 Using a CubeSat”, ASTRONOMICAL JOURNAL, 160:54. (SCIE) (IF: 5.84; SCI ranking: 13.2%)
  
  
• [4]     AMS Collaboration, 2020, “Properties of Neon, Magnesium, and Silicon Primary Cosmic Rays Results from the Alpha Magnetic Spectrometer”, PHYSICAL REVIEW LETTERS, 124, 211102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [5]     AMS Collaboration, 2019, “Properties of Cosmic Helium Isotopes Measured by the Alpha Magnetic Spectrometer”, PHYSICAL REVIEW LETTERS, 123,181102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [6]     AMS Collaboration, 2019, “Towards Understanding the Origin of Cosmic-Ray Electrons”, PHYSICAL REVIEW LETTERS, 122.101101. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [7]     AMS Collaboration, 2019, “Towards Understanding the Origin of Cosmic-Ray Positrons”, PHYSICAL REVIEW LETTERS, 122.041102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [8]     AMS Collaboration, 2018, “Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 121, 051102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [9]     AMS Collaboration, 2018, “Observation of Fine Time Structures in the Cosmic Proton and Helium Fluxes with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 121, 051101. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [10]     AMS Collaboration, 2018, “Precision Measurement of Cosmic-Ray Nitrogen and its Primary and Secondary Components with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 121, 051103. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [11]     AMS Collaboration, 2018, “Observation of New Properties of Secondary Cosmic Rays Lithium, Beryllium, and Boron by the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 120,021101. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [12]     AMS Collaboration, 2017, “Observation of the Identical Rigidity Dependence of He, C, and O Cosmic Rays at High Rigidities by the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 119, 251101. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [13]     Yi-Chun Lin, C.Y. Pan, K.J. Chiang, M.C. Yuan, C.H. Chu, Y.W. Tsai, P.K. Teng, C.H. Lin, T.C. Chao, C.C. Lee, C.J. Tung, A.E. Chen, 2017, “Monte Carlo simulations for angular and spatial distributions in therapeutic-energy proton beams”, RADIATION PHYSICS AND CHEMISTRY, 140, 217-224. (SCIE) (IF: 2.226; SCI ranking: 48.6%,62.3%,11.8%)
  
  
• [14]     AW Lowell et al., 2017, “Maximum Likelihood Compton Polarimetry with the Compton Spectrometer and Imager”, ASTROPHYSICAL JOURNAL, 848(2), 120. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
  
  
• [15]     AW Lowell et al., 2017, “Polarimetric Analysis of the Long Duration Gamma-Ray Burst GRB 160530A With the Balloon Borne Compton Spectrometer and Imager”, ASTROPHYSICAL JOURNAL, 848(2), 119. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
  
  
• [16]     AMS Collaboration, 2016, “Precision Measurement of the Boron to Carbon Flux Ratio in Cosmic Rays from 1.9 GV to 2.6 TV with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 117, 231102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [17]     AMS Collaboration, 2016, “Antiproton Flux, Antiproton-to-Proton Flux Ratio, and Properties of Elementary Particle Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station ”, PHYSICAL REVIEW LETTERS, 117,091103. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [18]     AMS Collaboration, 2015, “Precision Measurement of the Helium Flux in Primary Cosmic Rays of Rigidities 1.9 GV”, PHYSICAL REVIEW LETTERS, 115, 211101. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [19]     J.-L. Chiu et al. COSI collaboration, 2015, “The upcoming balloon campaign of the Compton Spectrometer and Imager (COSI)”, NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT, 784, 359-363. (SCIE) (IF: 1.265; SCI ranking: 76.6%,86.2%,52.9%,84.2%)
  
  
• [20]     M. Aguilar et al. AMS Collaboration, 2015, “ Precision Measurement of the Proton Flux in Primary Cosmic Rays from Rigidity 1 GV to 1.8 TV with the Alpha Magnetic Spectrometer on the International Space Station ”, PHYSICAL REVIEW LETTERS, 114, 171103. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [21]     AMS collaboration, 2014, “Precision Measurement of the (e(+) + e(-)) Flux in Primary Cosmic Rays from 0.5 GeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 113, 221102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [22]     M. Aguilar et al. AMS Collaboration, 2014, “Electron and Positron Fluxes in Primary Cosmic Rays Measured with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 113, 121102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [23]     L. Accardo et al. AMS Collaboration, 2014, “High Statistics Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–500 GeV with the Alpha Magnetic Spectrometer on the International Space Station”, PHYSICAL REVIEW LETTERS, 113, 121101. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [24]     ALEPH Collaboration ; DELPHI Collaboration ; L3 Collaboration ; OPAL Collaboration ; LEP Electroweak Working Grp, 2013, “Electroweak measurements in electron positron collisions at W-boson-pair energies at LEP”, PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 532(4), 119-244. (SCIE) (IF: 25.809; SCI ranking: 2.4%)
  
  
• [25]     ALEPH and DELPHI and L3 and OPAL and LEP Electroweak Working Group Collaborations, 2013, “Search for Charged Higgs bosons: Combined Results Using LEP Data ”, EUROPEAN PHYSICAL JOURNAL C, 73:2463. (SCIE) (IF: 4.389; SCI ranking: 24.1%)
  
  
• [26]     M. Aguilar et al. AMS Collaboration , 2013, “First Result from the Alpha Magnetic Spectrometer on the International Space Station: Precision Measurement of the Positron Fraction in Primary Cosmic Rays of 0.5–350 GeV”, PHYSICAL REVIEW LETTERS, 110, 141102. (SCIE) (IF: 8.385; SCI ranking: 7.1%)
  
  
• [27]     L3 collaboration, 2011, “Generalized event shape and energy flow studies in e+e− annihilation at √s=91.2−208.0 GeV”, JOURNAL OF HIGH ENERGY PHYSICS, 143. (SCIE) (IF: 5.875; SCI ranking: 13.8%)
  
  
• [28]     M. S. Bandstra, E. C. Bellm, S. E. Boggs, D. Perez-Becker, A. Zoglauer, H.-K. Chang, J.-L. Chiu, J.-S. Liang, Y.-H. Chang, Z.-K. Liu, W.-C. Hung, M.-H. A. Huang, S. J. Chiang, R.-S. Run, C.-H. Lin, M. Amman, P. N. Luke,P. Jean, P. von Ballmoos, and C. B. Wunderer, 2011, “DETECTION AND IMAGING OF THE CRAB NEBULA WITH THE NUCLEAR COMPTON TELESCOPE”, ASTROPHYSICAL JOURNAL, 738(1), 8. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
  
  
• [29]     M. Aguilar et al., 2011, “ISOTOPIC COMPOSITION OF LIGHT NUCLEI IN COSMIC RAYS: RESULTS FROM AMS-01”, ASTROPHYSICAL JOURNAL, 736(2),105. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
  
  
• [30]     The L3 Collaboration, 2011, “Test of the τ-model of Bose–Einstein correlations and reconstruction of the source function in hadronic Z-boson decay at LEP”, EUROPEAN PHYSICAL JOURNAL C, 71(5), 1648. (SCIE) (IF: 4.389; SCI ranking: 24.1%)
  
  
• [31]     M. Aguilar et al., 2010, “RELATIVE COMPOSITION AND ENERGY SPECTRA OF LIGHT NUCLEI IN COSMIC RAYS:”, ASTROPHYSICAL JOURNAL, 724,329-340. (SCIE) (IF: 5.746; SCI ranking: 14.7%)
  
  
• [32]     Wei-Che Hung; Yuan-Hann Chang; "Chih-Hsun Lin"; Boggs, S.E.; Hsiang-Kuang Chang; Bandstra, M.S.; Bellm, E.C.; Jeng-Lun Chiu; Jau-Shian Liang; Zong-Kai Liu; Perez-Becker, D.; Wunderer, C.B.; Zoglauer, A.; Ming-Huey Huang; Amman, M.; Luke, P.N.;, 2009, “The Data Readout System of the Nuclear Compton Telescope (NCT)”, IEEE TRANSACTIONS ON NUCLEAR SCIENCE, 56(04), 2303-2308. (SCIE) (IF: 1.575; SCI ranking: 65.8%,26.5%)
  
  
• [33]     Zong-Kai Liu, Yuan-Hann Chang, Boggs S.E., Bandstra M.S., Bellm E.C., Bowen J.D., Perez-Becker D., Wunderer C.B., Zoglauer A., Amman M., Luke P.N., Hsiang-Kuang Chang, Jeng-Lun Chiu, Jau-Shian Liang, "Chih-Hsun Lin", Wei-Che Hung, 2009, “Characterizing and Correcting the Cross-Talk Effect on Depth Measurement in the NCT Detectors”, IEEE TRANSACTIONS ON NUCLEAR SCIENCE, Volume 56, Issue 3, Part 2, 1210-1214. (SCIE) (IF: 1.575; SCI ranking: 65.8%,26.5%)
  
  
• [34]     Bellm, E.C., Boggs, S.E., Bandstra, M.S., Bowen, J.D., Perez-Becker, D., Wunderer, C.B., Zoglauer, A., Amman, M., Luke, P.N., Hsiang-Kuang Chang, Jeng-Lun Chiu, Jau-Shian Liang, Yuan-Hann Chang, Zong-Kai Liu, Wei-Che Hung, "Chih-Hsun Lin", Huang, M.A.,Jean, P., 2009, “Overview of the Nuclear Compton Telescope”, IEEE TRANSACTIONS ON NUCLEAR SCIENCE, Volume 56, Issue 3, Part 2, 1250-1256. (SCIE) (IF: 1.575; SCI ranking: 65.8%,26.5%)
  
  

發現與突破

• [1]     西元年：2015
  研究人員(中)：林志勳、陳鎰鋒、李宗其、 鄧炳坤、朱明禮、謝奇文、葉健一
  研究人員(英)：LIN, CHIH-HSUN, A.E. Chen, C.C. Lee, P.K. Teng, M. Chu, CW Hsieh, J.Y. Yi
  研究成果名稱(中)：適用於放射治療筆型掃描離子束量測的偵測器及其在每日品保之應用
  研究成果名稱(英)：Detector for measurements of scanning beam in radiotherapy and its application in daily QA
  簡要記述(中)：李世昌院士領軍的中央研究院物理研究所實驗高能物理團隊成員(林志勳、朱明禮、鄧炳坤)與中央大學、長庚大學及嘉義大學合作，應用高能物理探測器的技術，研發出適用於掃瞄式筆型質子束品保的偵測器。此偵測器具備高速及高解析功能，可在極短時間內驗證質子束特性(位置、大小、掃瞄速度及能量)，立即反應任何異常，而達到每日品保目的。
  現今全世界質子癌症治療中心數目快速成長，其中新穎的筆形掃瞄技術將成主流。此偵測器可在極短時間內完成精確的質子束特性驗證，頗具市場競爭力。此一成果獲得第十二屆國家新創獎 - 臨床新創獎的肯定。
  
  簡要記述(英)：The experimental high energy group (Drs. Lin C.H., Chu M. and Teng P.K.) of Institute of Physics, Academia Sinica, led by Academician Lee S.C., has been collaborating with National Central University, Chang Gung University and National Chiayi University to develop a high speed and fine spatial resolution ionization detector, “Cross”, to measure the characteristics of proton scanning pencil beam. The detector can determine the position, shape, scanning speed and energy of the proton beam in a very short time.
  Proton therapy using pencil beam scanning (PBS) system allows precision dose delivery to target and minimizes the overall exposure. The Cross detector is highly competitive with its great performance for the PBS daily QA.