L. Conti

ORCID: 0000-0003-2966-2000
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About
Contact & Profiles
Research Areas
  • Astrophysics and Cosmic Phenomena
  • Dark Matter and Cosmic Phenomena
  • Earthquake Detection and Analysis
  • Particle Detector Development and Performance
  • Ionosphere and magnetosphere dynamics
  • Solar and Space Plasma Dynamics
  • earthquake and tectonic studies
  • Neutrino Physics Research
  • Geomagnetism and Paleomagnetism Studies
  • Particle physics theoretical and experimental studies
  • Gamma-ray bursts and supernovae
  • Seismic Waves and Analysis
  • Atmospheric Ozone and Climate
  • Astro and Planetary Science
  • Photocathodes and Microchannel Plates
  • Quantum Chromodynamics and Particle Interactions
  • Neural dynamics and brain function
  • EEG and Brain-Computer Interfaces
  • Functional Brain Connectivity Studies
  • Seismology and Earthquake Studies
  • Planetary Science and Exploration
  • Space Satellite Systems and Control
  • Particle Accelerators and Free-Electron Lasers
  • Stellar, planetary, and galactic studies
  • High-Energy Particle Collisions Research

Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata
1999-2025

UniNettuno University
2016-2025

Engineering (Italy)
2019-2025

University of Rome Tor Vergata
2019-2024

Uninett (Norway)
2024

Istituto Nazionale di Fisica Nucleare, Sezione di Torino
2018-2023

Istituto Nazionale di Fisica Nucleare, Sezione di Roma I
1998-2023

Sapienza University of Rome
1996-2023

University of Turin
2019-2023

Institute of Experimental Physics of the Slovak Academy of Sciences
2023

The Extreme Universe Space Observatory on a Super Pressure Balloon 1 (EUSO-SPB1) was launched in 2017 April from Wanaka, New Zealand. plan of this mission opportunity NASA super pressure balloon test flight to circle the southern hemisphere. primary scientific goal make first observations ultra-high-energy cosmic-ray extensive air showers (EASs) by looking down atmosphere with an ultraviolet (UV) fluorescence telescope suborbital altitude (33~km). After 12~days and 4~hours aloft, terminated...

10.1016/j.astropartphys.2023.102891 article EN cc-by Astroparticle Physics 2023-09-04

Abstract The China Seismo-Electromagnetic Satellite ( CSES ) aims to monitor electromagnetic, particle, and plasma perturbations in the iono-magnetosphere inner Van Allen radiation belts originated by electromagnetic sources external internal geomagnetic cavity, cosmic rays, solar events. In particular, objective of space mission is investigate lithosphere–atmosphere–ionosphere coupling mechanisms (including effects lightning, earthquakes, volcanoes, artificial emissions) that induce top...

10.3847/1538-4365/ab276c article EN The Astrophysical Journal Supplement Series 2019-07-01

10.1016/j.astropartphys.2018.05.007 article EN Astroparticle Physics 2018-05-23

Abstract High-energy, long gamma-ray bursts (GRBs) can be generated by the core collapse of massive stars at end their lives. When they happen in close-by universe exceptionally bright, as seen from Earth case recent, giant, long-lasting GRB221009A. GRB221009A was produced a collapsing star with redshift 0.152: this event observed many space experiments, which also detected an extraordinary afterglow. The large fluence prompt emission about 0.013 erg cm −2 illuminated geographical region...

10.3847/2041-8213/acc247 article EN cc-by The Astrophysical Journal Letters 2023-03-01

Abstract The High-energy Particle Detector (HEPD) on board the China Seismo-Electromagnetic Satellite (CSES-01)—launched 2018 February 2—is a light and compact payload suitable for measuring electrons (3–100 MeV), protons (30–250 nuclei (up to few hundreds of MeV). Sun-synchronous orbit large acceptance allow HEPD measure cosmic-ray particles near ±65° latitude limit fair amount time per day. In this work, three semiannual galactic hydrogen energy spectra between ∼40 250 MeV are presented,...

10.3847/1538-4357/abad3e article EN cc-by The Astrophysical Journal 2020-09-01

Abstract In this work we present the High‐Energy Particle Detector (HEPD‐01) observations of proton fluxes from space during 28 October 2021 solar energetic particle event, which produced a ground‐level enhancement on Earth. The event was associated with major, long‐duration X1‐class flare and concomitant coronal mass ejection (CME) that erupted Active Region 12887. This is first direct measurement particles emitted current cycle, recorded by single instrument in energy range ∼50 MeV/n up to...

10.1029/2022sw003191 article EN cc-by Space Weather 2022-10-11

Abstract Time-dependent energy spectra of galactic cosmic rays (GCRs) carry crucial information regarding their origin and propagation throughout the interstellar environment. When observed at Earth, after traversing interplanetary medium, such are heavily affected by solar wind embedded magnetic field permeating inner sectors heliosphere. The activity Sun changes significantly over an 11 yr cycle—and so does effect on particles; this translates into a phenomenon called modulation. Moreover,...

10.3847/2041-8213/acbea7 article EN cc-by The Astrophysical Journal Letters 2023-03-01

10.1007/978-3-031-47606-8_33 article EN Advances in neurobiology 2024-01-01

Understanding human cortical neurodynamics is increasingly important, as highlighted by the European Innovation Council, which prioritises tools for measuring and stimulating brain activity. Unravelling how cytoarchitecture, morphology, connectivity shape essential developing technologies that target specific regions. Given dynamic non-stationary nature of neural interactions, there an urgent need non-linear signal analysis methods, in addition to linear ones, track local differentiate...

10.3390/fractalfract9050278 article EN cc-by Fractal and Fractional 2025-04-25
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