Origin and Dynamics of Cosmic Rays
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Publication:3267352
DOI10.1103/PHYSREV.109.1328zbMath0091.45403WikidataQ129661902 ScholiaQ129661902MaRDI QIDQ3267352
Publication date: 1958
Published in: Physical Review (Search for Journal in Brave)
Related Items (5)
On the production of suprathermal grains ⋮ Suprathermal Particles ⋮ Acceleration of Cosmic Radiation ⋮ On the propagation of hydromagnetic waves in a plasma of thermal and suprathermal components ⋮ Quasilongitudinal propagation of Narrow beams of nonlinear magnetohydrodynamic waves
Cites Work
- The Boltzmann equation an d the one-fluid hydromagnetic equations in the absence of particle collisions
- Use of the Boltzmann Equation for the Study of Ionized Gases of Low Density. I
- Use of the Boltzmann Equation for the Study of Ionized Gases of Low Density. II
- On the Origin of the Cosmic Radiation
- Magneto-Hydrodynamic Shocks
- Cosmic Radiation and Cosmic Magnetic Fields. I. Origin and Propagation of Cosmic Rays in our Galaxy
- The Origin of Cosmic Rays
- Dimensional Relations in Magnetohydrodynamics
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