Solar Particle Transport in a Dynamical Quasi‐linear Theory
- 1 June 2003
- journal article
- Published by American Astronomical Society in The Astrophysical Journal
- Vol. 589 (2) , 1027-1039
- https://doi.org/10.1086/374812
Abstract
No abstract availableKeywords
This publication has 18 references indexed in Scilit:
- Energetic Particle Observations during the 2000 July 14 Solar EventThe Astrophysical Journal, 2002
- The Rigidity Dependence of Solar Particle Scattering Mean Free PathsThe Astrophysical Journal, 2000
- Observational constraints on the dynamics of the interplanetary magnetic field dissipation rangeJournal of Geophysical Research, 1998
- Dominant two‐dimensional solar wind turbulence with implications for cosmic ray transportJournal of Geophysical Research, 1996
- Proton and electron mean free paths: The Palmer consensus revisitedThe Astrophysical Journal, 1994
- Interplanetary transport of solar electrons and protons: Effect of dissipative processes in the magnetic field power spectrumJournal of Geophysical Research, 1993
- Evidence for the presence of quasi‐two‐dimensional nearly incompressible fluctuations in the solar windJournal of Geophysical Research, 1990
- Cosmic-ray pitch-angle scattering in isotropic turbulenceThe Astrophysical Journal, 1988
- Large-amplitude Alfvén waves in the interplanetary medium, 2Journal of Geophysical Research, 1971
- Cosmic-Ray Propagation. I. Charged Particles in a Random Magnetic FieldThe Astrophysical Journal, 1966