F. Monterde-Andrade

ORCID: 0000-0002-9618-702X
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About
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Research Areas
  • Ionosphere and magnetosphere dynamics
  • Astrophysics and Cosmic Phenomena
  • Solar and Space Plasma Dynamics
  • Radiation Therapy and Dosimetry
  • Particle Detector Development and Performance
  • Earthquake Detection and Analysis
  • Dark Matter and Cosmic Phenomena
  • Gamma-ray bursts and supernovae
  • Lightning and Electromagnetic Phenomena

Universidad Nacional Autónoma de México
2022-2023

The University of Tokyo
2023

Nagoya University
2023

Institute for Cosmic Ray Research
2023

The effects of Space Weather events on cosmic rays detected by the Solar Neutron Telescope (SNT) at Sierra Negra, Mexico, were studied. SNT is part Negra Cosmic Ray Observatory (SN-CRO), located 4580 m a.s.l. We analyzed data recorded six channels (C2, C3, C4, N2, N3, and N4) during geomagnetic storms from December 2015 to 2022. Using Dst Kp indices, 30 moderate (Dst < -50 nT, ≥ 5) intense -100 7) selected. C2, N3 N4 detect charged neutral particles, respectively, with energy deposition...

10.22323/1.444.1272 article EN cc-by-nc-nd Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 2023-07-29

The Scibar Cosmic-Ray Telescope (SciCRT) is a brand new detector of the Sierra Negra Cosmic Rays Observatory (SN-CRO). It designed to observe solar neutrons and muon background produced by galactic cosmic rays. In this work we present Geant4-based simulation detection efficiency SciCRT; for purpose injected 10$^{5}$ muons, in an energy range from 100 1000 MeV, impinging SciCRT array. Our results provide information about performance may be used study variations low

10.22323/1.444.1273 article EN cc-by-nc-nd Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019) 2023-07-25

Abstract The Scibar Cosmic-Ray Telescope (SciCRT) is the most promising detector of Sierra Negra Cosmic Rays Observatory (SN-CRO). At this location, being a target and tracker secondary cosmic rays, SciCRT offers high probability observing solar energetic particles lower energy galactic rays (LEGCR); also, it allows identification incoming by measuring their deposition. In work we present Geant4-based simulation deposited neutrons, $$\gamma $$ <mml:math...

10.1140/epjc/s10052-024-13325-0 article EN cc-by The European Physical Journal C 2024-09-27
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