Role of Coulomb collisions in the equatorial F-region plasma instabilities
Abstract
The effect of collisions on electrostatic instabilities driven by gravity and density gradients perpendicular to the ambient magnetic field is studied. Electron collisions tend to stabilize the short wavelength ( kyϱi ≫ 1, where ky is the perpendicular wavenumber of the instability and ϱi is the ion Larmor radius) kinetic interchange mode. In the presence of weak ion-ion collisions, this mode gets converted into an unmagnetized ion interchange mode which has maximum growth rate one order smaller than that of the collisionless mode. On the other hand, electron collisions can excite a long wavelength resistive interchange mode in a wide wavenumber regime ( 10 -3 ⩽ k y ϱ i ⋍ 0.3 ) with growth rates comparable to that of the collisional Rayleigh-Taylor mode. The results may be relevant to some of the spread F irregularities.
- Publication:
-
Planetary and Space Science
- Pub Date:
- May 1984
- DOI:
- 10.1016/0032-0633(84)90114-4
- Bibcode:
- 1984P&SS...32..635B
- Keywords:
-
- Coulomb Collisions;
- Equatorial Atmosphere;
- F Region;
- Ionospheric Disturbances;
- Magnetohydrodynamic Stability;
- Space Plasmas;
- Collisional Plasmas;
- Electron Scattering;
- Electrostatics;
- Ionic Collisions;
- Modal Response;
- Geophysics