Results 231 to 240 of about 46,447 (277)
On the Search for Potentially Anomalous Traces of Cosmic Ray Particles in Images Acquired by Cmos Detectors for a Continuous Stream of Emerging Observational Data. [PDF]
Sensors (Basel)Piekarczyk M, Hachaj T.
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Galactic cosmic ray effects on iron and nickel isotopes in iron meteorites. [PDF]
Meteorit Planet Sci, 2020 Cook DL, Leya I, Schönbächler M.
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Inference of the Local Interstellar Spectra of Cosmic-Ray Nuclei Z ⩽ 28 with the GalProp-HelMod Framework. [PDF]
Astrophys J Suppl Ser, 2020 Boschini MJ +13 more
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Cosmic-Ray Propagation in Light of the Recent Observation of Geminga. [PDF]
Astrophys J, 2019 Jóhannesson G +2 more
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Chemical Society Reviews, 2013
Gas-phase chemistry in the interstellar medium is driven by fast ion-molecule reactions. This, of course, demands a mechanism for ionization, and cosmic rays are the ideal candidate as they can operate throughout the majority of both diffuse and dense interstellar clouds.
Nick, Indriolo, Benjamin J, McCall
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Gas-phase chemistry in the interstellar medium is driven by fast ion-molecule reactions. This, of course, demands a mechanism for ionization, and cosmic rays are the ideal candidate as they can operate throughout the majority of both diffuse and dense interstellar clouds.
Nick, Indriolo, Benjamin J, McCall
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Cosmic γ rays and cosmic-ray particles
Nature, 1983Recent experiments using extensive air shower techniques1–5 have given evidence for the presence of significant fluxes of cosmic γ rays, in the energy range 1015–1016 eV, from specific cosmic sources. We argue here that the flux from these sources, and others as yet unresolved, is probably sufficient to allow the explanation of a number of previously ...
J. Wdowczyk, A. W. Wolfendale
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IBM Journal of Research and Development, 1996
This paper reviews the basic physics of those cosmic rays which can affect terrestrial electronics. Cosmic rays at sea level consist mostly of neutrons, protons, pions, muons, electrons, and photons. The particles which cause significant soft fails in electronics are those particles with the strong interaction: neutrons, protons, and pions.
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This paper reviews the basic physics of those cosmic rays which can affect terrestrial electronics. Cosmic rays at sea level consist mostly of neutrons, protons, pions, muons, electrons, and photons. The particles which cause significant soft fails in electronics are those particles with the strong interaction: neutrons, protons, and pions.
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Physical Review, 1950
The original idea of Menzel and Salisbury concerning the origin of cosmic rays has been extended and some of its possible consequences worked out in more detail. It is concluded that low frequency electromagnetic waves (a few cycles per second) may exist in limited regions near the outer edge of the solar corona, and could accelerate ions to cosmic-ray
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The original idea of Menzel and Salisbury concerning the origin of cosmic rays has been extended and some of its possible consequences worked out in more detail. It is concluded that low frequency electromagnetic waves (a few cycles per second) may exist in limited regions near the outer edge of the solar corona, and could accelerate ions to cosmic-ray
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Physical Review, 1954
For more than a generation cosmic rays have been studied primarily as a natural beam of high-energy particles. It is unnecessary to detail here how fruitful that “laboratory” has been, how much of our knowledge about fundamental particles and their interactions, from the cascade process of electromagnetic radiation through the nature of hyperons and ...
Morrison, Philip +2 more
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For more than a generation cosmic rays have been studied primarily as a natural beam of high-energy particles. It is unnecessary to detail here how fruitful that “laboratory” has been, how much of our knowledge about fundamental particles and their interactions, from the cascade process of electromagnetic radiation through the nature of hyperons and ...
Morrison, Philip +2 more
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Nuclear Physics B - Proceedings Supplements, 2004
Two aspects of cosmic rays and cosmology are considered here. Firstly, the relevance of extragalactic cosmic rays to the radiation – and magnetic – fields in the Universe and secondly the contribution of Galactic cosmic rays (or other entities allied to them) to the 'foreground' in analysis of the cosmic microwave background (CMB).
TADEUSZ WIBIG, ARNOLD W. WOLFENDALE
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Two aspects of cosmic rays and cosmology are considered here. Firstly, the relevance of extragalactic cosmic rays to the radiation – and magnetic – fields in the Universe and secondly the contribution of Galactic cosmic rays (or other entities allied to them) to the 'foreground' in analysis of the cosmic microwave background (CMB).
TADEUSZ WIBIG, ARNOLD W. WOLFENDALE
openaire +1 more source