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Samuel C.C. Ting

Samuel C.C. Ting

Verified

Massachusetts Institute of Technology · Physics

Active 1966–2024

h-index68
Citations26.3k
Papers52222 last 5y
Funding
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Research topics

  • Astrophysics
  • Physics
  • Astronomy
  • Nuclear physics
  • Optics

Selected publications

  • Properties of Iron Primary Cosmic Rays: Results from the Alpha Magnetic Spectrometer

    Physical Review Letters · 2021 · 111 citations

    • Physics
    • Nuclear physics
    • Astrophysics

    We report the observation of new properties of primary iron (Fe) cosmic rays in the rigidity range 2.65 GV to 3.0 TV with 0.62×10^{6} iron nuclei collected by the Alpha Magnetic Spectrometer experiment on the International Space Station. Above 80.5 GV the rigidity dependence of the cosmic ray Fe flux is identical to the rigidity dependence of the primary cosmic ray He, C, and O fluxes, with the Fe/O flux ratio being constant at 0.155±0.006. This shows that unexpectedly Fe and He, C, and O belong to the same class of primary cosmic rays which is different from the primary cosmic rays Ne, Mg, and Si class.

  • The Alpha Magnetic Spectrometer (AMS) on the international space station: Part II — Results from the first seven years

    Physics Reports · 2020 · 421 citations

    • Physics
    • Nuclear physics
    • Astrophysics

    The Alpha Magnetic Spectrometer (AMS) is a precision particle physics detector on the International Space Station (ISS) conducting a unique, long-duration mission of fundamental physics research in space. The physics objectives include the precise studies of the origin of dark matter, antimatter, and cosmic rays as well as the exploration of new phenomena. Following a 16-year period of construction and testing, and a precursor flight on the Space Shuttle, AMS was installed on the ISS on May 19, 2011. In this report we present results based on 120 billion charged cosmic ray events up to multi-TeV energies. This includes the fluxes of positrons, electrons, antiprotons, protons, and nuclei. These results provide unexpected information, which cannot be explained by the current theoretical models. The accuracy and characteristics of the data, simultaneously from many different types of cosmic rays, provide unique input to the understanding of origins, acceleration, and propagation of cosmic rays.

Frequent coauthors

  • K.L. Tung

    801 shared
  • A.A. Vorobyov

    775 shared
  • U. Becker

    European Organization for Nuclear Research

    771 shared
  • G.G.G. Massaro

    FHNW University of Applied Sciences and Arts

    677 shared
  • W. Krenz

    676 shared
  • R. Y. Zhu

    646 shared
  • J.D. Burger

    Massachusetts Institute of Technology

    633 shared
  • W. Lohmann

    615 shared
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