Space Plasma Characteristics
Space plasma pioneers Hannes Alfvén and Carl-Gunne Fälthammar divided the plasmas in the solar system into three different categories:
Classification of Magnetic Cosmic Plasmas
Characteristic | Space plasma density categories (Note that density does not refer to only particle density) |
Ideal comparison | ||
High density | Medium Density | Low Density | ||
Criterion | λ << ρ | λ << ρ << lc | lc << λ | lc << λD |
Examples | Stellar interior Solar photosphere |
Solar chromosphere/corona Interstellar/intergalactic space Ionosphere above 70 km |
Magnetosphere during magnetic disturbance. Interplanetary space |
Single charges in a high vacuum |
Diffusion | Isotropic | Anisotropic | Anisotropic and small | No diffusion |
Conductivity | Isotropic | Anisotropic | Not defined | Not defined |
Electric field parallel to B in completely ionized gas |
Small | Small | Any value | Any value |
Particle motion in plane perpendicular to B |
Almost straight path between collisions |
Circle between collisions |
Circle | Circle |
Path of guiding centre parallel to B |
Straight path between collisions |
Straight path between collisions |
Oscillations (e.g. between mirror points) |
Oscillations (e.g. between mirror points) |
Debye Distance λD | λD << lc | λD << lc | λD << lc | λD >> lc |
Magnetohydrodynamics suitability |
Yes | Approximately | No | No |
λ=Mean free path. ρ= Larmor radius (gyroradius) of electron. λD=Debye length. lc=Characteristic length
Read more about this topic: Astrophysical Plasma
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