E. T. Cuadros

ORCID: 0000-0002-6718-6837
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About
Contact & Profiles
Research Areas
  • Advanced Optical Sensing Technologies
  • Gamma-ray bursts and supernovae
  • Ionosphere and magnetosphere dynamics
  • Electrical Fault Detection and Protection
  • Astrophysics and Cosmic Phenomena
  • Solar and Space Plasma Dynamics
  • Lightning and Electromagnetic Phenomena
  • Planetary Science and Exploration
  • Fire effects on ecosystems

National Institute for Space Research
2019-2022

Abstract This work presents the first simultaneous X‐ray measurement and high‐speed video observation of propagation a lightning leader producing X‐rays. As result, three‐dimensional distance from and, for time, conditions preexisting channel during were observed. Although four leaders in this seven‐stroke flash followed same path to ground, X‐rays only observed before return stroke with highest peak current. The fact that other three following ground did not produce detectable confirms...

10.1029/2019ja027247 article EN Journal of Geophysical Research Space Physics 2019-11-07

Abstract High‐energetic charged particles, such as solar protons, and phenomena Forbush decreases are eligible candidates to affect the global electric circuit. These effects have been studied by analyzing disturbances of potential gradient in ground‐based measurements fair weather regions. In this paper, we investigate deviations diurnal curve, during proton events, decreases, from mean values obtained conditions. each situation, select only events which not accompanied or followed other....

10.1029/2021sw002944 article EN cc-by-nc-nd Space Weather 2022-02-26

Abstract The Large Aperture GRBs Observatory is a continental-wide observatory devised to detect high energy (around 100 GeV) component of Gamma Ray Bursts (GRBs), by using the single particle technique in arrays Water Cherenkov Detectors (WCDs) at mountain sites Argentina, Bolivia, Colombia, Guatemala, Mexico, Venezuela and Peru. Details instalation operation detectors Marcapomacocha Peru 4550 m.a.s.l. are given. detector calibration method will also be shown.

10.1017/s1743921312005248 article EN Proceedings of the International Astronomical Union 2011-10-01
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