Estimate plasma oscillations for any charged species. Choose units, solve frequency or density accurately fast. Download tables, share outputs, and verify your setups easily.
The plasma angular frequency for a single species is: ωp = √( n q² / (ε₀ εᵣ m) ).
Convert to ordinary frequency using fp = ωp / (2π). When solving for density, rearrange to n = (ε₀ εᵣ m / q²) (2πf)².
Examples below assume electrons and εᵣ = 1.
| n (cm⁻³) | n (m⁻³) | fp (Hz) | fp (GHz) |
|---|---|---|---|
| 1.00000 × 10^6 | 1.00000 × 10^12 | 5.19767 × 10^-9 | 0.00000000000000000519767 |
| 1.00000 × 10^8 | 1.00000 × 10^14 | 5.19767 × 10^-8 | 0.0000000000000000519767 |
| 1.00000 × 10^10 | 1.00000 × 10^16 | 5.19767 × 10^-7 | 0.000000000000000519767 |
| 1.00000 × 10^12 | 1.00000 × 10^18 | 5.19767 × 10^-6 | 0.00000000000000519767 |
Plasma frequency is the natural oscillation rate of free charge carriers after a small displacement. In an electron plasma, electrons slosh against an almost stationary ion background. The characteristic angular frequency is ωp, and the ordinary frequency is fp = ωp/(2π).
If a wave’s frequency is below fp, the plasma tends to reflect it; above fp, waves can propagate with modified dispersion. This helps explain radio reflection in the ionosphere, shielding in dense discharges, and cutoff behavior in plasma‑filled devices. It is a cornerstone parameter in plasma diagnostics.
Because ωp ∝ 1/√m, electrons dominate the high‑frequency response. Ion plasma frequencies are far lower due to larger ion mass, but you can explore ion cases by changing the particle mass input and comparing how fp scales.
Electron density varies widely. The ionosphere can be about 1010–1012 m⁻³, giving plasma frequencies from tens of kilohertz to a few megahertz. Laboratory plasmas may reach 1014–1016 m⁻³, pushing fp into the megahertz to hundreds‑of‑megahertz range. Dense fusion plasmas can exceed 1019 m⁻³, where fp can reach tens of gigahertz.
The model uses ε = ε0εr. Many low‑pressure plasmas are close to εr ≈ 1, but an increased εr lowers ωp by √εr. That shift changes the effective cutoff frequency for a given density.
Density is often reported in cm⁻³. Use 1 cm⁻³ = 106 m⁻³. Doubling density increases fp by √2, not by 2. The calculator also reports ωp in rad/s, which is useful for dispersion relations and time‑domain simulations.
For HF radio (3–30 MHz), a layer with fp near 10 MHz can reflect signals at or below that frequency. In microwave probes and reflectometry, selecting a frequency above expected fp avoids cutoff, improves penetration, and reduces measurement ambiguity.
The basic plasma frequency assumes a uniform, collisionless, unmagnetized plasma with small perturbations. Collisions, gradients, and magnetic fields add damping and extra resonances (for example, cyclotron effects), so treat fp as a baseline parameter for cutoff and response scale.
ωp is the angular plasma frequency in rad/s. fp is the ordinary frequency in hertz. They are related by fp = ωp/(2π). Use ωp for differential equations and fp for cutoff comparisons in Hz.
You may enter density in m⁻³ or cm⁻³. If you have cm⁻³ values, multiply by 10⁶ to convert to m⁻³. The calculator also provides both representations in the results for quick verification.
A larger carrier density strengthens the restoring electric field when charges are displaced. Stronger restoring force makes the oscillation faster, so ωp and fp scale with √n rather than linearly with n.
Plasma frequency is inversely proportional to √m. Electrons give much higher frequencies than ions. If you switch to a heavier ion mass, the plasma frequency drops sharply, often by orders of magnitude.
εr increases the permittivity of the medium. A larger εr lowers ωp by a factor of √εr, which reduces the cutoff frequency for the same density and mass.
No. Plasma frequency comes from electrostatic restoring forces in a neutralizing background. Cyclotron frequency is the rotation rate of charges in a magnetic field. In magnetized plasmas, both can appear together in wave behavior.
If collisions are strong, temperature is high, density varies sharply, or magnetic fields are significant, simple cutoff reasoning can fail. Use fp as a starting point, then apply the relevant dispersion relation for your geometry and conditions.
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