Determination of the characteristics of interstellar turbulence from data on the diffusion coefficient of cosmic rays
- 1 January 1987
- journal article
- research article
- Published by Springer Nature in Astrophysics
- Vol. 26 (2) , 175-184
- https://doi.org/10.1007/bf01005556
Abstract
No abstract availableKeywords
This publication has 11 references indexed in Scilit:
- Hydromagnetic waves in high Beta plasmasThe Astrophysical Journal, 1979
- Particle streaming - Is the Alfven velocity the ultimate speed limitThe Astrophysical Journal, 1979
- A theory of the interstellar medium - Three components regulated by supernova explosions in an inhomogeneous substrateThe Astrophysical Journal, 1977
- On the origin of cosmic rays: Some problems in high-energy astrophysicsReviews of Modern Physics, 1976
- Nonlinear perturbation theory for cosmic ray propagation in random magnetic fieldsAstrophysics and Space Science, 1973
- Role of Hydromagnetic Waves in Cosmic-Ray Confinement in the Disk. Theory of Behavior in General Wave SpectraThe Astrophysical Journal, 1973
- On the role of plasma effects in the cosmic ray propagation and isotropization in the GalaxyAstrophysics and Space Science, 1973
- Взаимодействие Быстрых частиц с магнито-гидродинамической турБулентностьюAstrophysics and Space Science, 1973
- Interaction Between Cosmic-Ray Electrons and Cosmic-Ray ProtonsThe Astrophysical Journal, 1970
- The Effect of Wave-Particle Interactions on the Propagation of Cosmic RaysThe Astrophysical Journal, 1969