SUMMARY
Collisionless plasmas are characterized by weak coupling among particles, where collisions are negligible compared to long-range collective interactions. A large mean free path and low particle density are critical factors that determine whether a plasma is collisionless. The electromagnetic perspective emphasizes that charged particles are primarily influenced by net charge distribution and magnetic fields. For further insights, refer to the discussions in "The Sun as a Guide to Stellar Physics" by E.R. Priest, 2019.
PREREQUISITES
- Understanding of plasma physics concepts
- Familiarity with mean free path and particle density
- Knowledge of electromagnetic interactions in plasmas
- Basic principles of magnetohydrodynamics
NEXT STEPS
- Research the role of mean free path in plasma behavior
- Study electromagnetic interactions in collisionless plasmas
- Explore magnetohydrodynamics and its applications
- Read "The Sun as a Guide to Stellar Physics" by E.R. Priest for advanced insights
USEFUL FOR
Researchers, physicists, and students interested in plasma physics, particularly those focusing on the dynamics of collisionless plasmas and their electromagnetic properties.