High-resolution mapping of secondary cosmic rays with miniaturised stacked pixel telescope

Authors

  • Carlos Granja Advacam, U Pergamenky 12, 170 00 Prague, Czech Republic; VSB – Technical University of Ostrava, Faculty of Electrical Engineering and Computer Science, Department of Physics, 17. listopadu 2172/15, 708 00 Ostrava, Czech Republic
  • Herve Chanal Université Clermont Auvergne, CNRS/IN2P3, Laboratoire de Physique de Clermont-Ferrand, 4 avenue Blaise Pascal, Aubière, F-63000 Clermont-Ferrand, France
  • Václav Zach Nuclear Physics Institute, Czech Academy of Sciences, Husinec – Řež 130, 250 68 Řež, Czech Republic
  • David Chvátil Nuclear Physics Institute, Czech Academy of Sciences, Husinec – Řež 130, 250 68 Řež, Czech Republic
  • Cristina Oancea Advacam, U Pergamenky 12, 170 00 Prague, Czech Republic
  • Dušan Poklop VSB – Technical University of Ostrava, Faculty of Electrical Engineering and Computer Science, Department of Physics, 17. listopadu 2172/15, 708 00 Ostrava, Czech Republic; Nuclear Physics Institute, Czech Academy of Sciences, Husinec – Řež 130, 250 68 Řež, Czech Republic
  • Václav Olšanský Nuclear Physics Institute, Czech Academy of Sciences, Husinec – Řež 130, 250 68 Řež, Czech Republic
  • Jan Jakůbek Advacam, U Pergamenky 12, 170 00 Prague, Czech Republic

DOI:

https://doi.org/10.14311/AP.2025.65.0016

Keywords:

cosmic rays, particle tracking, radiation imaging, particle telescope, pixel detectors

Abstract

We performed detailed measurements of the secondary cosmic ray field in the lower atmosphere (at 200 m). We use a miniaturised particle telescope consisting of two closely stacked synchronised Timepix3 detectors. Position-, spectral-, and time-sensitive particle tracking provides enhanced particle-type resolving power and high angular resolution mapping of charged particles. Evaluation and calibration of the telescope synchronised tracking and directional response was performed with proton and electron beams. The telescope architecture, modeled angular response and developed data analysis provide accurate composition characterisation and high-angular resolution directional mapping of the charged particle component. In particular, the muon component can be resolved to a high degree over the photon and electron components in the lower atmosphere. The muon angular flux is measured in a wide field of view with enhanced discrimination.

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References

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Published

2025-03-06

How to Cite

Granja, C., Chanal, H. ., Zach, V. ., Chvátil, D. ., Oancea, C. ., Poklop, D. ., Olšanský, V. ., & Jakůbek, J. . (2025). High-resolution mapping of secondary cosmic rays with miniaturised stacked pixel telescope. Acta Polytechnica, 65(1), 16-24. https://doi.org/10.14311/AP.2025.65.0016