Abstract
The distribution function of cosmic rays streaming perpendicular to the mean magnetic field in a turbulent medium is re-examined. Urch's (1977) discovery that, in quasilinear theory, the flux is due to particles at 90° pitch angle is discussed and shown to be consistent with previous formulations of the theory. We point out that this flux of particles at 90° cannot be arbitrarily set equal to zero, and hence we dismiss the alternative theory which proceeds from this premise. A further, basic inconsistency in Urch's new transport equation is demonstrated, and the connection between quasilinear theory and compound diffusion is discussed.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 507-513 |
| Number of pages | 7 |
| Journal | Astrophysics and Space Science |
| Volume | 53 |
| Issue number | 2 |
| DOIs | |
| State | Published - Feb 1978 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science