- Astrophysics and Cosmic Phenomena
- Dark Matter and Cosmic Phenomena
- Particle Detector Development and Performance
- Neutrino Physics Research
- Nuclear physics research studies
- Tropical and Extratropical Cyclones Research
- Particle Accelerators and Free-Electron Lasers
- Quantum chaos and dynamical systems
- Quantum Chromodynamics and Particle Interactions
- Radiation Detection and Scintillator Technologies
- Methane Hydrates and Related Phenomena
- Radio Astronomy Observations and Technology
- Photocathodes and Microchannel Plates
- Aeroelasticity and Vibration Control
- Remote Sensing in Agriculture
- Vibration Control and Rheological Fluids
- Oceanographic and Atmospheric Processes
- solar cell performance optimization
- Wind and Air Flow Studies
- Radio, Podcasts, and Digital Media
- Scientific Research and Discoveries
- CCD and CMOS Imaging Sensors
- Atomic and Subatomic Physics Research
- Astro and Planetary Science
- Gamma-ray bursts and supernovae
Associazione Calabrese di Epatologia
2023
Université Paris-Sud
2018
Centre National de la Recherche Scientifique
2011-2018
Istituto Nazionale di Fisica Nucleare, Sezione di Bari
2018
Institute of Space Science - INFLPR Subsidiary
1999-2018
Sofia University "St. Kliment Ohridski"
2018
Institut National de Physique Nucléaire et de Physique des Particules
2018
University of Rome Tor Vergata
2018
Centre de Développement des Technologies Avancées
2018
Karlsruhe Institute of Technology
2016
We describe a new measurement of the intensities heavy primary cosmic-ray nuclei O, Ne, Mg, Si, and Fe from 10 GeV amu-1 to energies beyond 1 TeV amu-1. The was conducted in 1999 during day test flight Transition Radiation Array for Cosmic Energetic (TRACER), telescope designed long-duration balloon flights. TRACER uses an array thin-walled single-wire proportional tubes determine particle Lorentz factor measurements specific ionization transition radiation. nuclear charge is obtained with...
This paper presents an astroclimatological study of meteorological data on relative humidity, dew-point temperature, air wind speed and barometric pressure recorded at four Romanian locations (Baisoara, Rosia Montana, Semenic, Ceahlau) the Nordic Optical Telescope (NOT) located Observatorio del Roque de Los Muchachos (ORM), island La Palma, Canary Islands, Spain.
The instability of the aircraft's flexible control surfaces caused by uncontrolled vibrations represents a challenging issue aviation security. Flutter is violent vibration whose amplitude grows strongly in short time. Once flutter reached, plane destabilized and it can no longer be controlled. This paper proposes specially designed demonstrator intended to extend flight envelope raising speed limit at which occurs. anti-flutter an intelligent airplane wing model made from longeron covered...
We analyze on a classical 2D version of the "nuclear billiard" onset chaotic behaviour three-dimensional nucleonic trajectories in different dynamical states axially symmetric deformed nuclei. The coupling between single-particle and collective degrees freedom presence dissipation for several multipolarities is taken into account. examine order-to-chaos transition by studying Shannon entropies, which quantify time rate information production during certain motion. For monopole dipole...
strumento idoneo ai fini di aumentare la sicurezza delle cure.L'obiettivo questo lavoro è realizzazione e introduzione una scheda infermieristica che permetta rilevazione lo scambio informazioni puntuali accurate per garantire un'assistenza personalizzata l'appropriatezza cure erogate con decisioni cliniche basate sulle evidenze scientifiche.
Experimental data on the pion-nucleus total cross sections are analyzed in terms of optimal resonances predictions (OR). The OR-predictions found a good agreement with actual experimental region corresponding to Delta(1236) resonance elementary pi-N scattering. essential signatures experimentally verified high accuracy.
The WILLI detector, installed in the National Institute of Physics and Nuclear Engineering — Horia Hulubei Bucharest has been devised for studies atmospheric muons, particular muon charge ratio. We report on results various energies (pμ < 1 GeV/c). are compared with Monte‐Carlo simulations performed CORSIKA GEANT codes. exploring potential a small detector array to be set up nearby actual triggering ratio measurements by Extended Air Shower (EAS) events.
The Solar Two Gamma-Ray Observatory is a ground-based instrument designed to detect 20-300 GeV gamma rays by sampling the Cherenkov light generated as and cosmic interact with atmosphere. observatory utilizes solar two pilot power plant in Barstow, California which has largest heliostat mirror area world. It over 2,000 heliostats each about 41 m<SUP>2</SUP> are. total active are 75,000 m<SUP>2</SUP>. Thus, potential be most sensitive gamma-ray detector between GeV. secondary system, capable...