Plasma Pressure Calculator

Find total plasma pressure, p = neTee + niTie, allowing electron and ion temperatures to differ, as they often do in real plasmas.

🌡️ Plasma Pressure Calculator
m⁻³
eV
m⁻³
eV
Total pressure
In atmospheres
Electron pressure
Ion pressure
Step-by-step working

🌡️ What is the Plasma Pressure Calculator?

This plasma pressure calculator finds the total kinetic pressure of a plasma from separate electron and ion densities and temperatures. Enter each species' density and temperature, and it returns the total pressure along with each species' individual contribution.

Total plasma pressure is simply the sum of each species' own ideal-gas pressure, p = neTee + niTie, the exact same p = nkT relationship that governs ordinary gases, applied separately to electrons and ions and then added together.

Unlike simplified formulas that assume electrons and ions share a single temperature, this calculator handles the common real-world case where Te and Ti differ, since collisional energy exchange between the two species is often too slow to fully equalize their temperatures.

This calculator is useful for plasma physics and fusion engineering students computing plasma beta or studying energy balance, and anyone curious how much pressure a hot, dense plasma actually exerts.

📐 Formula

p  =  ne Te e  +  ni Ti e
ne, ni = electron and ion number densities
Te, Ti = electron and ion temperatures, in eV
e = elementary charge
Example: tokamak (ne=ni=10²⁰ m⁻³, Te=Ti=10 keV): p ≈ 3.20 × 10⁵ Pa.

📖 How to Use This Calculator

Steps

1
Enter the electron density and temperature.
2
Enter the ion density and temperature, these can differ from the electron values.
3
Read the total pressure and each species' contribution.

💡 Example Calculations

Example 1 - Tokamak plasma with Te = Ti

1
ne=ni=10²⁰ m⁻³, Te=Ti=10,000 eV
2
pe = pi = 1.6022 × 10⁵ Pa
3
ptotal = 3.2044 × 105 Pa (about 3.16 atmospheres)
ptotal = 3.2044 × 105 Pa
Try this example →

Example 2 - Tokamak plasma with Te ≠ Ti

1
ne=ni=10²⁰ m⁻³, Te=10,000 eV, Ti=5,000 eV
2
ptotal = 2.4033 × 105 Pa, lower than Example 1
3
A cooler ion population contributes less pressure even at the same density
ptotal = 2.4033 × 105 Pa
Try this example →

Example 3 - Solar corona

1
ne=ni=10¹⁴ m⁻³, Te=Ti=100 eV
2
ptotal = 3.2044 × 10-3 Pa
3
Far lower than the tokamak despite comparable temperature, reflecting the corona's much lower density
ptotal = 3.2044 × 10-3 Pa
Try this example →

❓ Frequently Asked Questions

What is plasma pressure?+
Plasma pressure is the total kinetic (thermal) pressure exerted by all charged particle species in a plasma, arising from their random thermal motion, exactly like the pressure of an ordinary ideal gas. Since a plasma contains both electrons and ions, its total pressure is the sum of the pressure each species contributes on its own.
What is the formula for plasma pressure?+
p = neTee + niTie, where ne and ni are the electron and ion number densities, Te and Ti are their respective temperatures in electronvolts, and e is the elementary charge (which converts the eV-density product into pascals). Each term is simply that species' own ideal-gas pressure, nTe.
Why does this calculator allow Te to differ from Ti?+
In many real plasmas, especially those heated rapidly or with relatively low collision rates, energy exchange between electrons and ions is slow enough that the two species settle into different temperatures. This calculator handles that general case directly, rather than assuming Te = Ti as some simplified formulas do.
Why might electrons and ions have different temperatures?+
Heating mechanisms often couple more directly to one species (for example, ohmic heating and electron-cyclotron heating primarily heat electrons, while neutral beam injection primarily heats ions), and the electron-ion collisional energy exchange time can be much longer than the heating or confinement timescale, letting a temperature difference persist.
How is plasma pressure related to plasma beta?+
Plasma beta is exactly the ratio of this total plasma pressure to the magnetic pressure, β = p/(B²/2μ₀). This calculator computes the numerator (or its Te=Ti special case) that the Plasma Beta Parameter Calculator compares against the magnetic pressure.
Why does electron density often equal ion density?+
Plasmas are quasi-neutral overall, so for a plasma with only singly-charged ions (Z=1), electron density must equal ion density (ne=ni) to keep the total charge density near zero. For multiply-charged ions (charge state Z), quasi-neutrality instead requires ne = Z·ni.
Is this the same as the pressure in the ideal gas law?+
Yes, exactly, each species obeys the same p = nkT (or p = nTe in electronvolt units) relationship as an ordinary ideal gas, since the derivation from kinetic theory does not depend on whether the particles are neutral molecules or charged plasma particles. The only difference for a plasma is that there are typically two or more species contributing pressure simultaneously.
Does this formula include magnetic pressure?+
No, this calculator computes only the kinetic (thermal) pressure from particle motion. Magnetic pressure, B²/2μ₀, is a separate quantity computed by the Plasma Beta Parameter Calculator, which compares the two.
Why is plasma pressure important for fusion confinement?+
A magnetically confined plasma's thermal pressure must be balanced by the confining magnetic pressure, or the plasma will expand and lose confinement. Higher achievable pressure at a given magnetic field (higher plasma beta) directly translates into more fusion power for the same, expensive superconducting magnet system.
How does pressure differ between the solar corona and a tokamak?+
A tokamak achieves comparable or higher pressure than the solar corona despite the corona having a vastly larger volume, because the tokamak's density and temperature are both far higher, illustrating just how extreme laboratory fusion conditions are compared to a natural stellar atmosphere.

What is plasma pressure?

Plasma pressure is the total kinetic (thermal) pressure exerted by all charged particle species in a plasma, arising from their random thermal motion, exactly like the pressure of an ordinary ideal gas. Since a plasma contains both electrons and ions, its total pressure is the sum of the pressure each species contributes on its own.

What is the formula for plasma pressure?

p = neTee + niTie, where ne and ni are the electron and ion number densities, Te and Ti are their respective temperatures in electronvolts, and e is the elementary charge (which converts the eV-density product into pascals). Each term is simply that species' own ideal-gas pressure, nTe.

Why does this calculator allow Te to differ from Ti?

In many real plasmas, especially those heated rapidly or with relatively low collision rates, energy exchange between electrons and ions is slow enough that the two species settle into different temperatures. This calculator handles that general case directly, rather than assuming Te = Ti as some simplified formulas do.

Why might electrons and ions have different temperatures?

Heating mechanisms often couple more directly to one species (for example, ohmic heating and electron-cyclotron heating primarily heat electrons, while neutral beam injection primarily heats ions), and the electron-ion collisional energy exchange time can be much longer than the heating or confinement timescale, letting a temperature difference persist.

How is plasma pressure related to plasma beta?

Plasma beta is exactly the ratio of this total plasma pressure to the magnetic pressure, β = p/(B²/2μ₀). This calculator computes the numerator (or its Te=Ti special case) that the <a href="/science/plasma-physics/plasma-beta-parameter-calculator/">Plasma Beta Parameter Calculator</a> compares against the magnetic pressure.

Why does electron density often equal ion density?

Plasmas are quasi-neutral overall, so for a plasma with only singly-charged ions (Z=1), electron density must equal ion density (ne=ni) to keep the total charge density near zero. For multiply-charged ions (charge state Z), quasi-neutrality instead requires ne = Z·ni.

Is this the same as the pressure in the ideal gas law?

Yes, exactly, each species obeys the same p = nkT (or p = nTe in electronvolt units) relationship as an ordinary ideal gas, since the derivation from kinetic theory does not depend on whether the particles are neutral molecules or charged plasma particles. The only difference for a plasma is that there are typically two or more species contributing pressure simultaneously.

Does this formula include magnetic pressure?

No, this calculator computes only the kinetic (thermal) pressure from particle motion. Magnetic pressure, B²/2μ₀, is a separate quantity computed by the <a href="/science/plasma-physics/plasma-beta-parameter-calculator/">Plasma Beta Parameter Calculator</a>, which compares the two.

Why is plasma pressure important for fusion confinement?

A magnetically confined plasma's thermal pressure must be balanced by the confining magnetic pressure, or the plasma will expand and lose confinement. Higher achievable pressure at a given magnetic field (higher plasma beta) directly translates into more fusion power for the same, expensive superconducting magnet system.

How does pressure differ between the solar corona and a tokamak?

A tokamak achieves comparable or higher pressure than the solar corona despite the corona having a vastly larger volume, because the tokamak's density and temperature are both far higher, illustrating just how extreme laboratory fusion conditions are compared to a natural stellar atmosphere.