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Long‐Term Monitoring of Energetic Protons at the Bottom of Earth’s Radiation Belt
Published 2021-01-01“…It is also found that the influence of galactic cosmic ray fluctuations becomes smaller as the L‐value moves closer to 1.…”
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82
Galactic Cosmic Radiation in the Interplanetary Space Through a Modern Secular Minimum
Published 2020-09-01“…During such periods of low solar activity, the fluxes of galactic cosmic rays (GCRs) increase remarkably, presenting a hazard for long‐term crewed space missions. …”
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83
Study on Test‐Mass Charging for Taiji Gravitational Wave Observatory
Published 2024-01-01“…This study aims to model the charging of TMs during Galactic cosmic rays and solar proton events (SPEs) using the Monte Carlo simulation toolkit meanwhile with constructing the sophisticated 3D spacecraft. …”
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84
Relativistic Electron Acceleration and the “Ankle” Spectral Feature in Earth’s Magnetotail Reconnection
Published 2025-01-01“…Spectral analysis showed that these relativistic electrons deviated from the main plasma sheet population and exhibited an “ankle” feature similar to that observed in galactic cosmic rays. The contribution of “ankle” electrons to the total electron energy density increased from 0.1% to 1% in the separatrix layer though the spectral slopes did not exhibit clear variations. …”
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The Pierre Auger Observatory open data
Published 2025-01-01“…In 2023, a catalog of the highest-energy cosmic-ray events examined in depth has been included. …”
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87
Status and New Data of the Geochemical Determination of the pp-Neutrino Flux by LOREX
Published 2012-01-01“…The ratio of 205Pb/205Tl atoms in the Tl-bearing mineral lorandite provides, if corrected for the cosmic-ray induced background, the product of the flux of solar neutrinos and their capture probability by 205Tl, averaged over the age of lorandite. …”
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88
The Badhwar‐O'Neill 2020 GCR Model
Published 2020-06-01“…Abstract The Badhwar‐O'Neill (BON) model has been used for some time to describe the galactic cosmic ray (GCR) environment encountered in deep space by astronauts and sensitive electronics. …”
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89
Performance simulation study of plastic scintillator arrays for stability monitoring applications
Published 2025-01-01“…The characteristics of high energy cosmic-ray muons make them strongly penetrative in materials. …”
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90
Quasi-random numbers in some statistical systems
Published 2000-12-01“…Some methods include making hardware devices that generate noise, observing cosmic ray flux and etc. Pseudo-random numbers come from mathematical functions and algorithms that provides such numbers called pseudo-random generators. …”
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91
Model for the curvature response of the CDF II drift chamber
Published 2025-02-01“…Constraints on the model parameters are obtained from cosmic-ray data and from information published by CDF in the context of the W boson mass measurement. …”
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92
Virtual Joint Field Campaign: a framework of synthetic landscapes to assess multiscale measurement methods of water storage
Published 2025-02-01“…<p>Various methods are available to measure water storage across different landscape compartments, e.g. cosmic-ray neutron sensing, remote sensing, or hydrogravimetry. …”
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Rapidity dependence of antideuteron coalescence in pp collisions at s=13 TeV with ALICE
Published 2025-01-01“…Such measurements are of interest to the astrophysics community, since they can be used for the calculation of the flux of antinuclei from cosmic rays, in combination with coalescence models.…”
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95
A Model for Cosmic Magnetic Field Amplification: Effects of Pressure Anisotropy Perturbations
Published 2024-12-01“…By considering the balance between isotropization through magnetic field amplification and anisotropy generation by external sources such as turbulence and anisotropic cosmic-ray scattering, it is reasonable to assume that the system evolves around an equilibrium anisotropy value. …”
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96
Dark photon pair production via off-shell dark Higgs at FASER
Published 2024-12-01Get full text
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97
Modeling of the Near-Earth Low-Energy Antiproton Fluxes
Published 2011-01-01“…Simulated flux of the trapped antiprotons in the inner magnetosphere due to galactic cosmic ray (GCR) interactions with the atmospheric constituents exceeds the galactic antiproton flux up to several orders. …”
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98
Analysis of the Ground Level Enhancement GLE 60 on 15 April 2001, and Its Space Weather Effects: Comparison With Dosimetric Measurements
Published 2023-08-01“…Subsequently, employing the updated and verified by balloon measurements dosimetric model: Oulu CRAC:DOMO (Cosmic Ray Atmospheric Cascade: Dosimetric Model) we computed the dose rates throughout the event at several altitudes using the obtained spectra as an input. …”
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99
Recent results from NA61/SHINE
Published 2025-01-01“…Its research program includes studies of strong interactions as well as reference measurements for neutrino and cosmic-ray physics. A significant advantage of NA61/SHINE over collider experiments is its extended coverage of phase space available for hadron production. …”
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Kinematic Approach to the 24th Solar Cycle Prediction
Published 2012-01-01“…Time series of solar and cosmic ray monthly mean indices were received from web resources of international data centers. …”
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