[PDF] Top 20 Cosmic rays measurements around the knee of the primary spectrum
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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
Interactions of Cosmic Rays around the Universe. Models for UHECR data interpretation
... energy spectrum measurements from the TA collaboration [3] and the upper bound on the flux of cosmogenic neutrinos from the IceCube collaboration [16], as done in ...TA spectrum is performed (and it ... See full document
6
Precision measurements of cosmic rays up to the highest energies with a large radio array at the Pierre Auger Observatory
... the cosmic microwave background (CMB), the light elements could then be fragments of heavier nuclei that disintegrated during ...the spectrum, and are of extragalactic ... See full document
9
Ankle Phenomenon in the Cosmic Ray Energy Spectrum
... the knee energy by a series of nuclear components of cosmic rays which respond to the galactic magnetic field, each having an anti-Gaussian energy spectrum at different peak positions ...of ... See full document
5
Galactic cosmic rays
... of cosmic rays (CRs) is no exception to this rule: generally speaking it is fair to say that at present there is little doubt in the Physics community at large, that the bulk of CRs are produced in the ... See full document
6
Study of muons in extensive air showers from ultra-high energy cosmic rays measured with the Telescope Array experiment
... energy cosmic rays (UHECRs) has been a long-standing ...of primary cosmic ...energy spectrum, mass composition and anisotropy of cosmic rays by utilizing an array of ... See full document
6
Studies of Cosmic Rays at the Highest Energies with the Pierre Auger Observatory
... key measurements of the highest-energy cosmic ...The spectrum suppression is well established. The measurements of the large scale anisotropy provides upper limits in the dipole amplitude that ... See full document
12
The GRAND project and GRANDProto300 experiment
... the primary particles informations will be applied to the selected events in order to build the sky distribution, energy spectrum and elongation rate of the candidate ...to cosmic rays in the ... See full document
7
Ultra High Energy Cosmic Rays: Origin, Composition and Spectrum
... The measurements carried out by the Auger observatory [6] have shown that the mass composition, from prevalently light at ∼ 10 18 eV, becomes increasingly heavier towards higher ... See full document
6
Multiplicity spectrum of muon bundles and primary CR composition in the range 1 – 10000 TeV
... Despite of a number of experiments the study of muon bundles underground is an unappreciated method of in- vestigation of the primary CR spectrum and composition. However, this method has a particular ... See full document
5
Cosmic ray physics with the ARGO-YBJ experiment
... and cosmic ray physics below and around the knee of the primary energy spectrum (10 12 − 10 16 eV), where the transition from direct to indirect measurement techniques takes ...of ... See full document
6
A JOURNEY THROUGH RESEARCHES ON COSMIC RAYS
... Cosmic rays are high energy charged particles consisting of electrons, positrons, protons and atomic nuclei ranging from lightest to transuranic ...energy spectrum from 100Mev to 10Gev within the ... See full document
12
Estimation of index of power law rigidity spectrum of cosmic rays using effective rigidity of multidirectional muon detector
... increases with γ are S30, W30, and SW39. These three channels are closest to the vertical channel in terms of measured fluxes and the shape of the coupling functions and are characterized by low cutoff rigidities. The ... See full document
6
Measurements of He isotopic ratio in cosmic rays in the 100 MeV – 1 GeV range with the PAMELA experiment
... To select the primary (galactic) component we evaluated the local geomagnetic cutoff G in the St¨ormer approxima- tion (Shea et al., 1987). The value of G = 14.9/L 2 - valid for vertically incident particles - is ... See full document
5
Cosmic-ray energy spectrum around the knee observed with the Tibet air-shower experiment
... the primary mass and models of hadronic interactions in the energy range over PeV because of the observation of the shower size at nearly maximum development irrespective of the primary ...on primary ... See full document
6
Cosmic rays in the knee energy range
... the cosmic ray spectra obtained by direct measurements for the different ...galactic cosmic rays originated from a single acceleration and propagation process within our Milky Way which is ... See full document
7
Neutrinos from colliding wind binaries: future prospects for PINGU and ORCA
... of cosmic rays up to the knee: the observed cosmic ray energy spectrum is believed to be produced by one dominant source class up to the first, most prominent change in the spectral ... See full document
5
New look on the origin of cosmic rays
... of cosmic rays by supernova explosions this suggests that the shock wave is both strong enough and slightly loaded by cosmic ...of cosmic rays by supernova explosions less attractive ... See full document
8
Mesons in NA61/SHINE
... (1) measurements of hadron spectra in hadron-nucleus collisions for neutrino and cosmic rays experiments; and (2) study of strongly interacting matter via a two-dimensional beam momentum and system ... See full document
6
Böhm, Vanessa (2017): Cosmic lensing of galaxies and the cosmic microwave background beyond the linear regime. Dissertation, LMU München: Fakultät für Physik
... power spectrum implies the abundance of many hot and cold spots with a size correspond- ing to this ...power spectrum, which is almost featureless due to the imperfect coupling of photons to ...power ... See full document
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