Lesson 5 of 15

Plasma Beta

Plasma Beta

Plasma beta (β\beta) is one of the most important dimensionless parameters in plasma physics. It is the ratio of the thermal pressure to the magnetic pressure:

β=pthermalpmagnetic=nkBTB2/(2μ0)\beta = \frac{p_{thermal}}{p_{magnetic}} = \frac{n k_B T}{B^2 / (2\mu_0)}

Where:

  • nn = number density (m⁻³)
  • kB=1.381×1023k_B = 1.381 \times 10^{-23} J/K
  • TT = temperature (K)
  • BB = magnetic field strength (T)
  • μ0=4π×107\mu_0 = 4\pi \times 10^{-7} H/m (permeability of free space)

Pressure Components

Thermal pressure (kinetic pressure of the plasma): pthermal=nkBTp_{thermal} = n k_B T

Magnetic pressure (energy density of the magnetic field): pmagnetic=B22μ0p_{magnetic} = \frac{B^2}{2\mu_0}

Physical Significance

β\beta tells us which pressure dominates the plasma dynamics:

β\beta valueRegimeExample
β1\beta \ll 1Magnetically dominatedFusion tokamaks (β0.1\beta \sim 0.1)
β1\beta \sim 1Comparable pressuresSolar corona
β1\beta \gg 1Thermally dominatedAccretion disks
  • Low-β\beta plasmas: magnetic field controls particle motion; good confinement
  • High-β\beta plasmas: particles can distort or escape the field

In tokamak fusion reactors, achieving higher β\beta means more plasma pressure (and thus more fusion power) for a given magnetic field — a key engineering goal.

Implement the three pressure functions below. Keep all constants (kBk_B, μ0\mu_0) inside the function bodies.

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