Results 281 to 290 of about 263,873 (299)
Energetic Radiation From Galactic Cosmic Ray Interactions With Saturn's Main Rings. [PDF]
J Geophys Res Space Phys, 2018 Cooper JF, Sturner SJ.
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The Behaviour of Galactic Cosmic-Ray Intensity During Solar Activity Cycle 24. [PDF]
Sol Phys, 2019 Ross E, Chaplin WJ.
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Bedrock sculpting under an active alpine glacier revealed from cosmic-ray muon radiography. [PDF]
Sci Rep, 2019 Nishiyama R +10 more
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Cosmic γ rays and cosmic-ray particles [PDF]
Nature, 1983 Recent 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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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).
Tadeus Wibig +3 more
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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).
Tadeus Wibig +3 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.
Benjamin J. McCall, Nick Indriolo
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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.
Benjamin J. McCall, Nick Indriolo
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Il Nuovo Cimento, 1952
Cosmic rays undergound are treated as entirely caused by the electromagnetic interactions of μ-mesons. Simple approximations are given for the underground spectra of μ-mesons, virtual photons, soft showers, and nucleons. Comparison with experimental data is satisfactory on the absolute rate of slow neutron and nuclear star production, and on the charge
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Cosmic rays undergound are treated as entirely caused by the electromagnetic interactions of μ-mesons. Simple approximations are given for the underground spectra of μ-mesons, virtual photons, soft showers, and nucleons. Comparison with experimental data is satisfactory on the absolute rate of slow neutron and nuclear star production, and on the charge
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2010
This book is not a book on high energy physics and particle interactions. We have, however, to give the reader some information on the structure of matter and the interactions between its building blocks, because these are necessary for the understanding of the phenomena of cosmic ray acceleration, propagation in the Universe, and detection.
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This book is not a book on high energy physics and particle interactions. We have, however, to give the reader some information on the structure of matter and the interactions between its building blocks, because these are necessary for the understanding of the phenomena of cosmic ray acceleration, propagation in the Universe, and detection.
openaire +2 more sources