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Plasma parameters

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The complex self-constricting magnetic field lines and current paths in a Birkeland current that may develop in a plasma (Evolution of the Solar System, 1976)

Plasma parameters define various characteristics of a plasma, an electrically conductive collection of charged particles that responds collectively to electromagnetic forces. Plasma typically takes the form of neutral gas-like clouds or charged ion beams, but may also include dust and grains.[1] The behaviour of such particle systems can be studied statistically.[2]

Fundamental plasma parameters

All quantities are in Gaussian (cgs) units except energy and temperature expressed in eV and ion mass expressed in units of the proton mass ; is charge state; is Boltzmann's constant; is wavenumber; is the Coulomb logarithm.

Frequencies

  • electron gyrofrequency, the angular frequency of the circular motion of an electron in the plane perpendicular to the magnetic field:
  • ion gyrofrequency, the angular frequency of the circular motion of an ion in the plane perpendicular to the magnetic field:
  • electron plasma frequency, the frequency with which electrons oscillate (plasma oscillation):
  • ion plasma frequency:
  • electron trapping rate:
  • ion trapping rate:
  • electron collision rate in completely ionized plasmas:
  • ion collision rate in completely ionized plasmas:
  • electron (ion) collision rate in slightly ionized plasmas:

where is a collision crossection of the electron (ion) on the operating gas atoms (molecules), is the electron (ion)

distribution function in plasma, and is an operating gas concentration.

Lengths

  • classical distance of closest approach, the closest that two particles with the elementary charge come to each other if they approach head-on and

each have a velocity typical of the temperature, ignoring quantum-mechanical effects:

  • electron gyroradius, the radius of the circular motion of an electron in the plane perpendicular to the magnetic field:
  • ion gyroradius, the radius of the circular motion of an ion in the plane perpendicular to the magnetic field:
  • plasma skin depth, the depth in a plasma to which electromagnetic radiation can penetrate:
  • Debye length, the scale over which electric fields are screened out by a redistribution of the electrons:
  • Ion inertial length, the scale at which ions decouple from electrons and the magnetic field becomes frozen into the electron fluid rather than the bulk plasma:
  • Free path is the average distance between two subsequent collisions of the electron (ion) with plasma components:

where is an average velocity of the electron (ion), and is the electron or ion collision rate.

Velocities

  • ion sound velocity, the speed of the longitudinal waves resulting from the mass of the ions and the pressure of the electrons:
,

where is the adiabatic index, and here is the number of degrees of freedom

  • Alfvén velocity, the speed of the waves resulting from the mass of the ions and the restoring force of the magnetic field:

Dimensionless

A 'sun in a test tube'. The Farnsworth-Hirsch Fusor during operation in so called "star mode" characterized by "rays" of glowing plasma which appear to emanate from the gaps in the inner grid.
  • square root of electron/proton mass ratio
  • number of particles in a Debye sphere
  • Alfvén velocity/speed of light
  • electron plasma/gyrofrequency ratio
  • ion plasma/gyrofrequency ratio
  • thermal/magnetic pressure ratio ("beta")
  • magnetic/ion rest energy ratio
  • Coulomb logarithm is an average coefficient taking into account far Coulomb interactions of charged particles in plasma.

Its value is evaluated in the nonrelativistic case approximately for electrons ,

for ions

See also

References

Footnotes

  1. ^ Peratt, Anthony, Physics of the Plasma Universe (1992);
  2. ^ Parks, George K., Physics of Space Plasmas (2004, 2nd Ed.)