Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.iki.rssi.ru/magbase/REFMAN/SPPHTEXT/coldwave.html
Дата изменения: Unknown
Дата индексирования: Fri Dec 21 22:03:17 2007
Кодировка:
Поисковые слова: п п п п п п п п п
Space Physics Group of Oulu

Waves in cold plasma

SpaceWeb@SkyNet.oulu.fi - last update: 28 May 1995, 0800 UT
As discussed in context of plasma theories, the thermal kinetic energy of plasma particles is ignored in cold plasmas. In practice this means neglection of the pressure terms in the equations. In the theory of waves, this approximation is justified if the particle thermal velocity is small when compared with the wave phase velocity. Accordingly, for waves with very small phase velocities, warm plasma theory must be used.

Another often used approximation is to consider only electron motion. The theory of wave propagation in a cold homogenous electron gas immersed in a magnetic field (B) is known as magnetoionic theory. The neglection of ions is valid only for high frequency waves, i.e., for frequencies large compared to the ion cyclotron frequency. To go on to the next level of approximation, the theory of high-frequency small-amplitude plane waves propagating in an arbitrary direction with respect to B is called the Appleton-Hartree theory. This was first developed to study wave propagation in the Earth's ionosphere. The restriction of small-amplitude waves makes it possible to use linear perturbation theory, where the wave related variations in the plasma parameters are small when compared to the undisturbed parameters. The use of plane waves makes the equations easier, but implyes no loss of generality, since any wave motion can always be synthesized in terms of plane waves. The hydromagnetic extension of magnetoionic theory deals with multicomponent cold plasma.

In the cold electron gas, important variables are the electron number density and the average electron velocity. They must satisfy

The wave modes are found from the dispersion relation calculated using the above equations. We start investigating the results from a non-magnetized (isotropic) plasma, before including the external magnetic field so important for space physics. Ion motion is not included (but some remarks about ion effects are given).

Non-magnetized cold plasma

There are one oscillation mode and one real wave mode in cold isotropic electron plasma:
  1. electron plasma oscillations
  2. transverse waves

Frequency dependence of the phase and group velocities for the transverse waves in a collisionless isotropic cold electron plasma.

Magnetized cold plasma

Things get quite a bit more complicated when external magnetic field B is taken into account (even with the Appleton-Hartree approximation):
Propagation parallel to B (three wave modes)
  1. longitudinal electron plasma oscillations (as for isotropic plasma)
  2. transverse right-hand circularly polarized waves, RCP
  3. transverse left-hand circularly polarized waves, LCP

Frequency dependence of the phase and group velocities for the transverse RCP and LCP waves propagating along magnetostatic field in a collisionless cold electron plasma.

An important point is that, in the very low frequency limit, the phase velocities of the RCP and LCP waves (if ion motion is included) go to zero. This means that in order to get Alfven waves (see MHD waves) one has to use warm plasma theory, where the low frequency phase velocity is, approximately, Alfven velocity.

Propagation perpendicular to B (two wave modes)
  1. ordinary waves
  2. extraordinary waves
Propagation at arbitrary directions
We are not going into details here (perhaps later)!

A phenomenon known as Faraday rotation occurs in the frequency range of RCP and LCP waves, and can be used as a plasma diagnostic tool.

See also: