Bohm Diffusion Calculator
Our plasma physics calculator computes bohm diffusion accurately. Enter measurements for results with formulas and error analysis.
Formula
D_B = kT_e / (16eB)
Where D_B = Bohm diffusion coefficient (m^2/s), k = Boltzmann constant, T_e = electron temperature (in eV multiply by e to get Joules), e = electron charge (1.602e-19 C), and B = magnetic field strength (Tesla). The confinement time is tau_B = L^2 / D_B.
Worked Examples
Example 1: Tokamak Edge Plasma
Problem: Calculate the Bohm diffusion coefficient and confinement time for a tokamak edge plasma with Te = 100 eV, B = 2 Tesla, plasma size L = 0.5 m, and density n = 1e19 m^-3.
Solution: Te = 100 eV = 100 * 1.602e-19 J = 1.602e-17 J\nD_B = kT_e / (16eB) = 1.602e-17 / (16 * 1.602e-19 * 2) = 1.602e-17 / 5.126e-18 = 3.125 m^2/s\ntau_B = L^2 / D_B = 0.25 / 3.125 = 0.08 seconds = 80 ms\nParticle flux: Gamma = D_B * n / L = 3.125 * 1e19 / 0.5 = 6.25e19 m^-2 s^-1\nn * tau_B = 1e19 * 0.08 = 8e17 m^-3 s
Result: D_B = 3.125 m^2/s | Bohm time = 80 ms | n*tau = 8e17 (below Lawson criterion of ~1e20)
Example 2: Hall Thruster Discharge
Problem: A Hall effect thruster operates with Te = 20 eV, B = 0.02 Tesla, channel width L = 0.025 m, and density n = 1e18 m^-3. Find the Bohm diffusion rate.
Solution: Te = 20 eV = 3.204e-18 J\nD_B = kT_e / (16eB) = 3.204e-18 / (16 * 1.602e-19 * 0.02) = 3.204e-18 / 5.126e-20 = 62.5 m^2/s\ntau_B = L^2 / D_B = 6.25e-4 / 62.5 = 1e-5 s = 10 microseconds\nElectron Larmor radius: rho = sqrt(m_e kT_e) / (eB) = sqrt(9.109e-31 * 3.204e-18) / (1.602e-19 * 0.02)\n= 1.708e-24^0.5 / 3.204e-21 = 5.41e-13 / ... = 0.848 mm\nParticle flux = 62.5 * 1e18 / 0.025 = 2.5e21 m^-2 s^-1
Result: D_B = 62.5 m^2/s | Transit time = 10 microseconds | High cross-field transport as expected
Frequently Asked Questions
What is Bohm diffusion and why is it important?
Bohm diffusion is an anomalous cross-field plasma transport mechanism that was first observed by David Bohm during the Manhattan Project in the 1940s. It describes the rate at which charged particles diffuse across magnetic field lines in a magnetized plasma, and it is typically much faster than the classically predicted diffusion rate. The Bohm diffusion coefficient is D_B = kT_e / (16eB), where T_e is the electron temperature and B is the magnetic field strength. This scaling with 1/B (rather than the classical 1/B^2) means magnetic confinement is far less effective than classical theory predicts. Bohm diffusion remains one of the central challenges in achieving controlled nuclear fusion, as it causes plasma to leak out of magnetic confinement devices much faster than desired.
How does the Bohm diffusion coefficient compare to classical diffusion?
Classical cross-field diffusion (described by Braginskii transport theory) scales as 1/B^2 and depends on the collision frequency between particles. The Bohm diffusion coefficient scales as 1/B and is independent of collision frequency, making it an anomalous transport process driven by plasma instabilities and turbulence rather than binary collisions. In typical laboratory plasmas, Bohm diffusion is 10 to 1000 times faster than classical diffusion predictions. The ratio of Bohm to classical diffusion is roughly D_B/D_cl = omega_ce * tau_e / 16, where omega_ce is the electron cyclotron frequency and tau_e is the electron collision time. In hot fusion plasmas where collisions are rare, this ratio can be enormous, making Bohm diffusion the dominant loss mechanism.
What causes Bohm diffusion in plasmas?
Bohm diffusion is driven by microscopic plasma turbulence and instabilities rather than particle-particle collisions. Low-frequency electrostatic fluctuations create random electric fields that cause E cross B drift of particles across magnetic field lines. These fluctuations arise from various plasma instabilities including drift waves, interchange modes, and gradient-driven turbulence. The turbulent electric fields have typical amplitudes that satisfy the so-called Bohm criterion, where the correlation between density fluctuations and potential fluctuations maximizes transport. Modern understanding shows that Bohm diffusion is not a universal law but rather represents an upper bound on anomalous transport that many plasmas happen to approach. Some plasmas exhibit transport below the Bohm level, while others can exceed it.
What is the Bohm confinement time?
The Bohm confinement time is the characteristic time for plasma to escape a magnetic confinement region of size L due to Bohm diffusion, given by tau_B = L^2 / D_B = 16eBL^2 / (kT_e). This time determines how long a plasma can be magnetically confined before diffusive losses drain it. For a fusion reactor to work, the confinement time must be long enough that the fusion energy produced exceeds the energy lost through transport. The Lawson criterion requires n * tau_E > 10^20 m^-3 s for deuterium-tritium fusion, where tau_E is the energy confinement time. Bohm diffusion typically gives confinement times that fall short of this requirement, which is why modern tokamaks work hard to suppress turbulent transport through techniques like plasma shaping, magnetic shear, and transport barriers.
How does Bohm diffusion affect fusion reactor design?
Bohm diffusion has profoundly influenced fusion reactor design since the earliest magnetic confinement experiments. In the 1950s and 1960s, most confinement devices showed transport losses consistent with Bohm scaling, which seemed to doom magnetic fusion to impossibility. The breakthrough came with the development of the tokamak configuration, which achieved confinement significantly better than Bohm scaling. Modern tokamaks operate with transport between classical and Bohm levels, and understanding and reducing anomalous transport remains the central challenge. Techniques including plasma elongation, triangularity, reversed magnetic shear, and H-mode operation have progressively improved confinement. The ITER reactor is designed with sufficient margin above Bohm scaling to achieve net fusion energy production.
What is the Larmor radius and how does it relate to Bohm diffusion?
The Larmor radius (also called cyclotron or gyroradius) is the radius of the circular orbit a charged particle traces around a magnetic field line, given by rho = mv_perp / (qB), where m is the particle mass, v_perp is the perpendicular velocity, q is the charge, and B is the magnetic field. For thermal particles, rho = sqrt(kT/m) / (qB/m) = sqrt(mkT) / (qB). The Bohm diffusion coefficient can be rewritten as D_B = rho_e * v_thermal / 16, showing it represents a random walk with step size equal to the electron Larmor radius and step frequency equal to the inverse of the cyclotron period divided by 16. Classical diffusion has a much smaller step size determined by the Larmor radius times the ratio of collision frequency to cyclotron frequency, which is typically a very small number in hot plasmas.