# Maxwellian_speed_3D

plasmapy.formulary.distribution.Maxwellian_speed_3D(v, T, particle='e', v_drift=0, vTh=nan, units='units')

Probability distribution function of speed for a Maxwellian distribution in 3D.

Return the probability density function for finding a particle with speed components vx, vy, and vz in m/s in an equilibrium plasma of temperature T which follows the 3D Maxwellian distribution function. This function assumes Cartesian coordinates.

Parameters
• v (Quantity) – The speed in units convertible to m/s.

• T (Quantity) – The temperature, preferably in kelvin.

• particle (str, optional) – Representation of the particle species(e.g., 'p' for protons, 'D+' for deuterium, or 'He-4 +1' for $$He_4^{+1}$$ (singly ionized helium-4)), which defaults to electrons.

• v_drift (Quantity) – The drift speed in units convertible to m/s.

• vTh (Quantity, optional) – Thermal velocity (most probable) in m/s. This is used for optimization purposes to avoid re-calculating vTh, for example when integrating over velocity-space.

• units (str, optional) – Selects whether to run function with units and unit checks (when equal to “units”) or to run as unitless (when equal to “unitless”). The unitless version is substantially faster for intensive computations.

Returns

f – Probability density in speed-1, normalized so that: $$\iiint_0^∞ f(\vec{v}) d\vec{v} = 1$$.

Return type

Quantity

Raises

Notes

In 3D, the Maxwellian speed distribution function describing the distribution of particles with speed $$v$$ in a plasma with temperature $$T$$ is given by:

$f = 4 π v^{2} (π v_{Th}^2)^{-3/2} \exp(-v^{2} / v_{Th}^2)$

where $$v_{Th} = \sqrt{2 k_B T / m}$$ is the thermal speed.

Examples

>>> from astropy import units as u
>>> v=1 * u.m / u.s
>>> Maxwellian_speed_3D(v=v, T=30000*u.K, particle='e', v_drift=0 * u.m / u.s)
<Quantity 2.60235...e-18 s / m>