[PDF] Top 20 Sobre una nueva especie catalana del género Hieracium L. (Asteraceae)
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Cosmic rays in the knee energy range
... the energy range of the so called ‘knee’ be- tween 100 TeV and 1 EeV one expects to identify the end of the galactic origin of cosmic ...high- energy particles are performed indirectly ... See full document
80
Ankle Phenomenon in the Cosmic Ray Energy Spectrum
... the knee energy range (at 3 PeV) may not be stable, as in the case of the standard ...the knee energy phenomenon is observed when cosmic rays are emitted from ... See full document
28
Ultra-high energy cosmic rays and the strongest AGN flares
... simple approach does not distinguish between source and background photons, therefore the flux is inevitably overestimated, especially at low galactic latitudes. Also, at the energies ∼ 100 MeV the point spread function ... See full document
13
Cosmic rays measurements around the knee of the primary spectrum
... the knee was widely studied, a break- through was recently obtained by the EAS experiments supplying the detection of di ff erent EAS components on an event by event basis with a resolution lower than the EAS ... See full document
6
The ATLAS Hadronic Physics Program and High Energy Cosmic Rays
... Inclusive charged-particle distributions have been previously measured in p.p and p.pbar collisions at a range of different centre-of-mass energies [11]. These measurements provide insight into the strong ... See full document
5
Interactions of Cosmic Rays in the primary energy range (0.1-1) PeV studied by the ARGO-YBJ Experiment
... the cosmic ray flux in an energy range hardly accessed by direct ...an energy region up to ∼ 100 TeV where the primary cosmic ray composition is sufficiently well known for that measure ... See full document
82
Ultimate precision in cosmic-ray radio detection — the SKA
... Abstract. As of 2023, the low-frequency part of the Square Kilometre Array will go online in Australia. It will constitute the largest and most powerful low-frequency radio- astronomical observatory to date, and will ... See full document
23
TeV Blazars as the Sources of Ultra High Energy Cosmic Rays
... high energy gamma rays, and they show variability in flux at all wavelengths as well as spectral shape on time scales ranging from months to a few ...gamma rays from Mkn 421 with the Whipple imaging ... See full document
11
Measurement of Ultra High Energy Cosmic Rays with CHICOS
... Clocks at widely separated locations are kept synchronized by the GPS signal. When the GPS receiver is used set in “stationary” mode (i.e., assuming fixed location), the accuracy of the timing pulse used to resynchronize ... See full document
22
Experimental Summary: Very High Energy Cosmic Rays and their Interactions
... High Energy Cosmic Ray Interactions, held in August of 2012 in Berlin, was the first one in the history of the Symposium, where a plethora of high precision LHC data with relevance for cosmic ray ... See full document
29
Observations of nitrogen and oxygen isotopes in the low energy cosmic rays
... The curves represent the smoothed isotope response used to obtain a new range correction for helium.. electron pickup, which reduces the relative stopping power[r] ... See full document
5
The GRAND project and GRANDProto300 experiment
... Ultra-high energy neutrinos could be an extremely valuable tool to answer this question: thanks to their very low interaction probabil- ity and neutral charge, these particles indeed travel unim- peded from their ... See full document
26
Measurement of ultra-high energy cosmic rays: An experimental summary and prospects
... Multi-Composition Model. On the other hand, Auger, with its measured composition changing from proton to heavier nuclei in this energy range, has not associated the observed spectral features with a ... See full document
19
Neutrinos from colliding wind binaries: future prospects for PINGU and ORCA
... ray energy spectra from stellar environments are believed to be of too low energy in order to explain the total flux of cosmic rays up to the knee: the observed cosmic ray ... See full document
6
Ionization and heating by X-rays and cosmic rays
... their energy into a larger volume, thus not contributing much to the disk surface heating (Ercolano et ...large range of radii, from 1–70 AU, with ... See full document
9
Exploring cosmic rays at the highest-energy frontier with the Pierre Auger Observatory
... given energy bin the value in the template is weighted according to the fraction of each ...whole energy range for all three interaction ...whole energy range, dropping to near zero ... See full document
22
Tunka Advanced Instrument for cosmic rays and Gamma Astronomy (TAIGA): Status, results and perspectives
... The energy distribution for the events close to the array threshold is shown in ...simulated energy distribution for the different rates is shown in ...shower energy is ...peak energy of the ... See full document
11
Observation of ultra-high energy cosmic rays with the Telescope Array experiment
... of cosmic rays follows power law distribution, and due to low flux, the origin of UHECR is ...primary cosmic rays with atmo- spheric particles, which are called air ...the energy and ... See full document
78
Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum
... neutrinos and gamma rays. A pure proton composition is, theoretically, a natural possibility. Proton is the most abundant element in the universe and several di ff erent astrophysical objects, at present and past ... See full document
21
Recent results from ANTARES
... detect cosmic high-energy neutrinos we are now at the verge of opening a neutrino era in high-energy astrophysics thanks to the results of the IceCube neutrino telescope in Antarctica that show ... See full document
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