[PDF] Top 20 Modulation of high energy cosmic rays in the heliosphere
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Modulation of high energy cosmic rays in the heliosphere
... 2 DATA AND METHODS OF ANALYSES 2.1 Cosmic ray observing stations 2.2 Atmospheric effects 2.2.1 Correcting for the pressure effect 2.2.2 Correcting for the temperature effects 2.3 Fourier[r] ... See full document
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Cosmic ray modulation in the heliosphere
... 1 fi+1,j,kfi-1,j,k gri,j,k = f tj,k rt+i ri-1 The integral value of the radial gradient between two rigidity values was calculated using the same central difference approximation, except[r] ... See full document
199
Ankle Phenomenon in the Cosmic Ray Energy Spectrum
... knee energy is the split between radiation- dominated expansion and matter-dominated expansion of an expanding heat bath of a black ...of high energy cosmic rays and the loca- tion of ... See full document
5
Ultra-high energy cosmic rays: 40 years retrospective of continuous observations at the Yakutsk array: Part 2. Mass composition of cosmic rays at ultra high energies
... metagalactic cosmic rays recently developed nonlinear kinetic theories of CR acceleration in supernova remnants has allowed not only to achieve agreement in the shape of the CR spectrum up to energies ∼ 10 ... See full document
5
Tunka Advanced Instrument for cosmic rays and Gamma Astronomy (TAIGA): Status, results and perspectives
... The energy spectrum obtained by above described procedure is shown in ...The energy threshold of almost 100% efficiency of registration is about 250 ... See full document
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Status and perspectives of the radio detection of highenergy cosmic rays
... Figure 3. Left: Conceptional illustration of an upgraded station of the Surface Detector array of the Pierre Auger observatory, comprised of (from bottom to top) a water- ˇ Cerenkov detector, a layer of scintillators, ... See full document
7
INFN - LNS
... Radio detection of ultra high energy cosmic rays with the Auger Engineering Radio Array. 10:00 - 10:30 Abigail Vieregg[r] ... See full document
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Observation of ultra-high energy cosmic rays with the Telescope Array experiment
... m) [18]. The left panel of figure 5 shows the ratio of the SD signal of the experimental data to the MC prediction as a function of a lateral distance R [18]. The result on the high muon purity condition described ... See full document
9
Measurement of ultra-high energy cosmic rays: An experimental summary and prospects
... ln A is statistically not consistent with a constant value of ln A, whereas the same plots by other experiments are statistically consistent with both constant and changing values of ln A with respect to log(E) (see Fig. ... See full document
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Cosmic rays in the knee energy range
... the cosmic ray spectra obtained by direct measurements for the different ...solar modulation affects the spectral shape) is used as argu- ment that the galactic cosmic rays originated from a ... See full document
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The highest-energy cosmic-rays – the past, the present and the future
... highest-energy cosmic- rays relies almost entirely on concepts, both analytical and technical, that were proposed more than 40 years ago and by a handful of ...in cosmic rays tended, in ... See full document
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Highlights from the Telescope Array
... ultra high energy cosmic ray induced extensive air ...the energy spectrum and chemical composition of the primary ...of cosmic rays and ...ultra high energy ... See full document
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General overview of recent results from the Pierre Auger Observatory
... in high energy cosmic ray physics using the powerful hybrid technique: joined use of fluorescence telescopes and surface stations to achieve high performances and unprecedented ...(million ... See full document
7
Studies of Cosmic Rays at the Highest Energies with the Pierre Auger Observatory
... sequence of the deeper development and the reduced number of muons, photon showers are expected to have a smaller size at the ground, a steeper lateral distribution of secondary particles, a sparser distribution of ... See full document
12
Numerical Study of the Electron Lateral Distribution in Atmospheric Showers of High Energy Cosmic Rays
... and energy corresponding to a specific interaction model. The CORSIKA (COsmic Ray SImulations for KAscade) is a Monte Carlo simulation program for the physics of cosmic rays, used by many ... See full document
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DEFLECTION ANGLE OF HIGH ENERGY COSMIC RAYS IN THE PROPAGATION THROUGH THE GALACTIC AND EXTRAGALACTIC MAGNETIC FIELDS AND THE GZK (GREISEN-ZATSEPIN-KUZMIN) CUTOFF
... the energy spectrum of the cosmic rays is expected due to the energy degradation of the cosmic rays through their interaction with photons of the microwave background ... See full document
11
Measurement of Ultra High Energy Cosmic Rays with CHICOS
... Angeles-area high schools for the dual purposes of education outreach and UHECR ...solid-scintillator cosmic ray detectors spread throughout the San Gabriel and San Fernando ...a high school (or in ... See full document
178
Experimental Summary: Very High Energy Cosmic Rays and their Interactions
... large high energy cosmic neutrino telescopes are now quite ...neutrino energy spectrum (see also Fe- dynitch and ...where high en- ergy muons and neutrinos may provide a link to ... See full document
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The ATLAS Hadronic Physics Program and High Energy Cosmic Rays
... A fast timing system that can precisely measure the time difference between outgoing scattered protons is a key component of the AFP detector. The time difference is equivalent to a constraint on the event vertex, thus ... See full document
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Ultra-high energy cosmic rays: Setting the stage
... of energy loss by protons traveling through the microwave background due to e + e- pair production, or the transition between the termination of a galactic spectrum and a harder extragalactic ...the cosmic ... See full document
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