Results 111 to 120 of about 69,000 (198)
Small-scale Cosmic-Ray Anisotropy Observed by the GRAPES-3 Experiment at TeV Energies
GRAPES-3 is a mid-altitude (2200 m) and near-equatorial (11.°4N) air shower array, overlapping in its field of view for cosmic-ray observations with experiments that are located in the Northern and Southern Hemispheres. We analyze a sample of 3.7 × 10 ^9
M. Chakraborty +37 more
doaj +1 more source
Este texto sintetiza a modulação pelas partículas do fluxo de raios cósmicos galáticos durante seu transporte na heliosfera, fornecendo algumas referências necessárias para a compreensão do assunto aos interessados no tema.
A.G. Izzo de Oliveira +2 more
doaj +1 more source
Extra-Galactic Cosmic Rays [PDF]
Yoichi Fujimoto +2 more
openaire +1 more source
Cosmic ray albedo gamma rays from the quiet sun [PDF]
We estimate the flux of gamma-rays that result from collisions of high energy galactic cosmic rays with the solar atmosphere. An important aspect of our model is the propagation of cosmic rays through the magnetic fields of the inner solar systems.
Gaisser, T. K., Seckel, D., Stanev, T.
core +1 more source
Galactic Cosmic-Rays after AMS02
Presentation given at the "Anti-deuteron 2019" conference at UCLA (Los Angeles) on March 27, 2019. Abstract: The current generation of cosmic-ray (CR) experiments in the GeV-TeV range has reached an unprecedented level of precision, unveiling fine-details of the energy spectra. The interpretation of these measurements could require a profound revision
openaire +1 more source
The Correspondence between Leaky-box and Diffusion Models of Cosmic-Ray Propagation
The leaky-box model and the attendant concept of path-length distribution of cosmic rays were invented in the mid-1960s. Even though versatile computational packages such as GALPROP and DRAGON with the diffusion approach are now available for analyzing ...
Ramanath Cowsik, Dawson Huth
doaj +1 more source
Impact of Anisotropic Cosmic-Ray Transport on the Gamma-Ray Signatures in the Galactic Center
The very high energy (VHE) emission of the central molecular zone (CMZ) is rarely modeled in 3D. Most approaches describe the morphology in 1D or simplify the diffusion to the isotropic case.
J. Dörner +5 more
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Galactic Cosmic-Ray Background Deduction Method Based on Empirical Mode Decomposition
The inversion of the relative content and spatial distribution characteristics of radioactive elements on the lunar surface, as inferred from gamma-ray spectrometer data, holds substantial importance for forecasting lunar surface compositions. During the
Yitong Cui +7 more
doaj +1 more source
Recurrent variations of anomalous oxygen in association with a corotating interaction region
The fluxes of anomalous oxygen (<i>E</i> ranging from 3.5-6.8 MeV/amu), as measured by the EPAC instrument on ULYSSES, show a recurrent variation with the solar rotation period, which is anticorrelated with the fluxes of particles accelerated
M. K. Reuss, M. Fränz, E. Keppler
doaj
Search for Galactic Cosmic Ray Sources with H.E.S.S
Supernova remnants (SNRs) are the prime candidates for the acceleration of the Galactic Cosmic Rays. Tracers for interactions of Cosmic Rays with ambient material are gamma rays at TeV energies, which can be observed with ground based Cherenkov ...
Komin, Nukri
core +1 more source

