Titlebook: Cosmic Radiation in Contemporary Astrophysics; Maurice M. Shapiro Book 1986 D. Reidel Publishing Company, Dordrecht, Holland 1986 Populati

Antagonism

Particle Acceleration by PulsarsIt is argued that the winds from fast-rotating magnets — like pulsars — consist primarily of (relativistic) electrons and positrons with Lorentz factors in excess of 10.. The particle energies are likely distributed according to a power law, with Lorentz factors reaching and exceeding γ = 10..

Asymptomatic

Nato Science Series C:http://image.papertrans.cn/c/image/238887.jpg

擁擠前

Particle Acceleration by Magnetic Reconnectionnergy gain is directly proportional to the product of the strength of the pre-merging magnetic field and the plasma resistivity. Particle acceleration to relativistic energies is possible provided that plasma turbulence or some form of instability leads to a drastic reduction of the classical (Coulomb) conductivity.

gerrymander

X-Ray Burst Sourcess perhaps a black hole) and a low-mass (?0.7 M.) companion filling its critical Roche lobe. Consequently, most orbital periods of these very “tight” binaries are about 1–10 hours. The objects are concentrated towards the galactic center and about ten of them are located in globular clusters; they are an old population.

Airtight

Cosmic Radiation in Contemporary Astrophysics978-94-009-5488-5Series ISSN 1389-2185

偏見

reaching

聯(lián)想記憶

PALSY

Digital Work: An Organizational Perspectiver a description of the cosmic ray pre-history. Subsequently other channels of information are drawn in, and it is shown that it is very difficult to formulate a unified picture of the origin of GeV-energy cosmic rays which encompasses both the heavy nuclei and the proton-helium component.

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