[PDF] Top 20 Observations of the anisotropy of cosmic rays at TeV–PeV
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Observations of the anisotropy of cosmic rays at TeV–PeV
... of cosmic rays from nearby sources in the ...large-scale anisotropy at the 10 −3 level can easily arise from cosmic rays diffusing from nearby supernova ...the anisotropy we ... See full document
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A solution to the cosmic ray anisotropy problem
... Abstract. Observations of the cosmic ray (CR) anisotropy are widely advertised as a means of finding nearby ...the anisotropy observed for hadronic CRs is not understood, in the sense that ... See full document
5
TeV Cosmic Ray Anisotropy and the Heliospheric Magnetic Field
... scale anisotropy can be qualitatively explained on the basis of diffusive propagation of cosmic rays in the Milky Way from stochastically distributed ...the anisotropy amplitude, although for ... See full document
7
Cosmic rays in the knee energy range
... 100 TeV and 1 EeV one expects to identify the end of the galactic origin of cosmic ...primary cosmic rays at few PeV and an increasing dominance of heavy ones towards higher ener- ... See full document
7
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 ...100 TeV where the primary cosmic ray composition is sufficiently well known for that measure to be ...∼ PeV energies in the ... See full document
5
The CALorimetric Electron Telescope (CALET) on the International Space Station: Results from the First Two Years of Operation
... galactic cosmic-ray acceleration and propagation, and search for dark matter ...of cosmic-ray electrons (including positrons) up to 20 TeV, gamma-rays to 10 TeV, and nuclei up to 1,000 ... See full document
8
A Consistent Scenario for the IBEX Ribbon, Anisotropies in TeV Cosmic Rays, and the Local Interstellar Medium
... global TeV anisotropy, there are also features in TeV cosmic ray maps that may be directly related to heliospheric struc- ...anisotropic cosmic rays in the 10’s TeV en- ... See full document
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TeV Blazars as the Sources of Ultra High Energy Cosmic Rays
... energy cosmic rays (UHECRs) were defined as those cosmic rays with energies above 10 18 eV ...a cosmic ray primary with energy of 10 20 eV was reported [12], a succession of de- ... See full document
12
Galactic cosmic rays
... 200 TeV [5–7], while energies as high as ∼ PeV might be reachable in type II SN explosions in the dense winds of their red giant parent stars, if the spectrum of accelerated particles is relatively hard (∝ ... See full document
6
The Anisotropy of Cosmic Rays and the Global Anisotropy of Physical Space
... the anisotropy of CR with the energy of 10 TeV that were measured with the use of the Super-Kamiokande detector ...the anisotropy found in this experiment ( = 75˚ 7˚, = –5˚ 7˚) is in ... See full document
5
The origin of cosmic rays and TeV gamma-ray astronomy
... of observations at all wavelengths and theoretical work established SNRs as main sources of cos- mic ...of cosmic ray acceleration in SNR as described above, but also the search for the sources of ... See full document
6
Fermi bubbles as sources of cosmic rays above 1 PeV
... Such objects should not be unique phenomena observed only in our Galaxy. However, Fermi bubbles are too faint and it is impossible to detect exactly the same structures elsewhere. Yet some much more powerful objects with ... See full document
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Research of Global Anisotropy of Physical Space on Investigation Base of Changes in and α-decay Rate of Radioactive Elements. Motion of Pulsars and Anisotropy of Cosmic Rays
... global anisotropy (10 -15 – free physical space; 10 -5 – intrinsic physical space of elementary particles), as distinct from all basic isotropic models with the same properties in various ...said anisotropy ... See full document
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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
... In this review, we used the work of the Yakutsk group in which was introduced an estimation of the mass composition of cosmic rays at ultrahigh energies [1–5]. In these studies we analyzed the ... See full document
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Tunka Advanced Instrument for cosmic rays and Gamma Astronomy (TAIGA): Status, results and perspectives
... flux at the four stations closest to the core. The energy distribution for the events close to the array threshold is shown in Fig. 11. The distributions measured in October 2015 and January 2016 are shown separately ... See full document
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New look on the origin of cosmic rays
... together cosmic rays originating from different supernova, and forms the unique particle spectrum, extending from energies in a few units of GeV to energies 10 18 ...of cosmic rays in the ... See full document
8
Effects of Mobile Radiations and its Prevention
... atoms/molecules and creates ions. Examples include ultraviolet rays, X-rays, gamma rays, cosmic rays, etc. Non-ionizing radiations: These waves do not carry high energy per qua[r] ... See full document
7
International Year of Astronomy (IYA-2009) and its significance
... sources, we need spececraft, baloons or satel- lites as these are mostly absorbed by Earth’s at- mosphere. The large scale IR observations were first done by IRAS (Infra Red Astronomical Sat- ellite) launched in ... See full document
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Results from Tunka-133 (5 years observation) and from the Tunka-HiSCORE prototype
... To expand the measurement range to lower energies the new array Tunka-HiSCORE [2] data has been used. The HiSCORE concept has been described in [3] and [4]. The preliminary primary energy spectrum in the range 200 ... See full document
6
Neutrinos from colliding wind binaries: future prospects for PINGU and ORCA
... ical view, the atmospheric muon neutrino flux is reduced to zero at these energies. This would, again theoretically, reduce the background to zero, such that a single signal event would become significant. Of course, ... See full document
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