Plasma Parameters
Characterizing plasmas through dimensionless quantities
4.1 Temperature and Density
Plasma state is characterized by two fundamental quantities: temperature T anddensity n. These span enormous ranges across different plasmas.
Temperature
In plasma physics, temperature is often expressed in electron volts (eV):
Electrons and ions can have different temperatures: Te ≠ Ti. Equilibration occurs through collisions on timescale:
Density Ranges
- • Interstellar medium: n ∼ 106 m−3, T ∼ 1 eV
- • Solar wind: n ∼ 107 m−3, T ∼ 10 eV
- • Ionosphere: n ∼ 1012 m−3, T ∼ 0.1 eV
- • Tokamak core: n ∼ 1020 m−3, T ∼ 10 keV
- • Laser fusion: n ∼ 1031 m−3, T ∼ 10 keV
4.2 Beta Parameter
The plasma beta is the ratio of thermal to magnetic pressure:
Beta determines the relative importance of thermal vs. magnetic forces:
- • β << 1: Magnetic field dominates, particles gyrate freely
- • β ∼ 1: Thermal and magnetic pressures comparable
- • β >> 1: Thermal pressure dominates, field can be expelled
Beta in Different Plasmas
- • Solar corona: β ∼ 10−4 – 10−2 (magnetically dominated)
- • Solar wind at 1 AU: β ∼ 1 (pressure balance)
- • Tokamak: β ∼ 0.05 (must keep low for MHD stability)
- • Reverse field pinch: β ∼ 0.1 – 0.2
In fusion, achieving high β is crucial for reactor economics (higher β means less magnetic field needed for confinement).
4.3 Coupling Parameter
The coupling parameter Γ compares potential to kinetic energy:
where a = (3/4πn)1/3 is the mean inter-particle spacing (Wigner-Seitz radius).
Plasma Regimes
- • Γ << 1 (weakly coupled): Ideal gas, kinetic theory applies
- • Γ ∼ 1 (intermediate): Correlations important
- • Γ >> 1 (strongly coupled): Liquid-like or crystalline
Examples
- • Fusion plasmas: Γ ∼ 10−3 (weakly coupled)
- • White dwarf interior: Γ ∼ 1 – 100 (strongly coupled)
- • Dusty plasma crystals: Γ ∼ 100 – 1000 (Coulomb crystal)
- • Warm dense matter: Γ ∼ 1 (emerging field)
Relation to plasma parameter:
4.4 Magnetization Parameter
In magnetized plasmas, the key parameter is the ratio of gyroradius to system size:
Equivalently, compare cyclotron frequency to collision frequency:
- • ωc/ν >> 1: Magnetized plasma (particles complete many gyro-orbits between collisions)
- • ωc/ν ∼ 1: Weakly magnetized
- • ωc/ν << 1: Unmagnetized (collisions dominate)
For electrons in a tokamak: ωce/νei ∼ 105, highly magnetized!
4.5 Classification of Plasmas
Plasmas can be classified along several axes:
By Temperature
- • Cold: T < 1 eV (fluorescent lamps, ionosphere)
- • Thermal: T ∼ 1 – 100 eV (arcs, processing plasmas)
- • Hot: T > 1 keV (fusion, astrophysical)
By Density
- • Low density: n < 1016 m−3 (space, laboratory)
- • Medium: n ∼ 1018 – 1020 m−3 (fusion)
- • High density: n > 1026 m−3 (ICF, stellar)
By Generation Method
- • DC discharge: Glow discharge, arc
- • RF discharge: Inductively coupled, capacitively coupled
- • Magnetic confinement: Tokamak, stellarator
- • Inertial confinement: Laser-driven, Z-pinch
- • Natural: Solar, magnetospheric, astrophysical
4.6 The n-T Diagram
Plasmas span 20+ orders of magnitude in density and temperature. Key boundaries:
The fusion triple product criterion:
defines the region where fusion power exceeds input power (ignition).