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Science, 1960
New and more powerful methods for eliminating background intensity are needed in order to make possible the development of neutrino astronomy into a new, far-reaching branch of science.
G, Marx, N, Menyhárd
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New and more powerful methods for eliminating background intensity are needed in order to make possible the development of neutrino astronomy into a new, far-reaching branch of science.
G, Marx, N, Menyhárd
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РАДИАЦИОННАТА БЕЗОПАСНОСТ В СЪВРЕМЕННИЯ СВЯТ
Cosmic radiation is a form of energy that travels through space from all directions of the universe. In this paper we look at what cosmic radiation is, its types and penetrating power, and what fraction of all radiation it is. How it affects us - irradiation, dose. Can we protect ourselves from it.
Dimitrova, A. +2 more
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Cosmic radiation is a form of energy that travels through space from all directions of the universe. In this paper we look at what cosmic radiation is, its types and penetrating power, and what fraction of all radiation it is. How it affects us - irradiation, dose. Can we protect ourselves from it.
Dimitrova, A. +2 more
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Cosmic Microwave Background Radiation
Reviews of Modern Physics, 1999Most astronomers and physicists now believe that we live in an expanding universe that evolved from an early state of extremely high density and temperature. Measurements of the spectrum and anisotropy of the cosmic microwave background radiation (CMBR) provide strong evidence supporting this picture. Today, the spectrum of the CMBR matches that of a 2.
Lyman Page, David Wilkinson
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Acceleration of Cosmic Radiation
Physical Review, 1958Alfven's model of discontinuous magnetic field variations for the acceleration of cosmic rays by the betatron mechanism was generalized to continuous field variations. with special reference to sinusoidal fields. It is shown that the efflciency of this model is maximum when the "rate of randomization'' is equal to the frequency of oscillation of the ...
Murty, G. S., Varma, R. K.
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Radiation transport calculations for cosmic radiation
Annals of the ICRP, 2012The radiation environment inside and near spacecraft consists of various components of primary radiation in space and secondary radiation produced by the interaction of the primary radiation with the walls and equipment of the spacecraft. Radiation fields inside astronauts are different from those outside them, because of the body's self-shielding as ...
A, Endo, T, Sato
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1976 International Conference on Submillimeter Waves and Their Applications, 1976
The existence of essentially isotropic homogeneous cosmic background radiation with the spectrum of a 3 K blackbody places important limits on cosmological speculations. This radiation has been the subject of intensive experimental investigation for more than a decade.
P. L. Richards, D. P. Woody
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The existence of essentially isotropic homogeneous cosmic background radiation with the spectrum of a 3 K blackbody places important limits on cosmological speculations. This radiation has been the subject of intensive experimental investigation for more than a decade.
P. L. Richards, D. P. Woody
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American Journal of Physics, 1960
The paper gives some general information about cosmic rays, especially with regard to the properties of the primary flux: charge composition, energy spectrum, and time variations. The experimental evidence for these properties of the cosmic rays is outlined briefly and possible origins of the radiation are discussed.
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The paper gives some general information about cosmic rays, especially with regard to the properties of the primary flux: charge composition, energy spectrum, and time variations. The experimental evidence for these properties of the cosmic rays is outlined briefly and possible origins of the radiation are discussed.
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The cosmic microwave background radiation
Reviews of Modern Physics, 1979Radio Astronomy has added greatly to our understanding of the structure and dynamics of the universe. The cosmic microwave background radiation, considered a relic of the explosion at the beginning of the universe some 18 billion years ago, is one of the most powerful aids in determining these features of the universe. This paper is about the discovery
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