Is there a plasma density gradient role on the generation of short-scale Farley-Buneman waves?

C. Haldoupis (1) , T. Ogawa (2) , K. Schlegel (3) , J. A. Koehler (4) , T. Ono (5)

1 Department of Physics [Heraklion]
2 STEL - Solar-Terrestrial Environment Laboratory [Nagoya]
3 MPS - Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research
4 Department of Physics and Engineering Physics
5 Department of Geophysics [Kyoto]

The physics of the unstable E-region plasma is based on the modified two stream, or Farley-Buneman, and the gradient drift instabilities. The theory combines both mechanisms into a single dispersion relation which applies for the directly generated short-scale plasma waves, known as type 1 irregularities. In the absence of a plasma gradient it is only the two stream mechanism acting which favors wave excitation if E×B electron drifts relative to the ions exceed a threshold slightly above the ion acoustic speed. On the other hand, the theory also predicts that a destabilizing (stabilizing) electron density gradient acts to decrease (increase) the ion acoustic threshold, and hence the wave phase velocities at threshold, depending on the gradient strength and the wavelength. Given a destabilizing plasma gradient, the threshold reduction is larger at longer than shorter wavelengths and thus the best way to test the gradient role is by simultaneous observations of type 1 waves at two or more radio backscatter frequencies. The present paper relies on dual frequency backscatter observations of 1.1 m and 3.1 m type 1 irregularities made simultaneously at 144 MHz and 50 MHz, respectively, in mid-latitude sporadic E-layers. Using as typical plasma gradient scale lengths for destabilized sporadic E-layers those that are obtained from rocket electron density profiles, the radar observations are compared with the predictions of kinetic theory. The results suggest that the plasma density gradient effect on meter scale Farley-Buneman waves is not important. This is reinforced further by the analysis of backscatter from destabilized meteor trail plasma when very steep gradients are expected in electron density. The present findings, and more from past studies, question the electron density gradient role in the generation of short-scale plasma waves as predicted by the linear instability theory. This deserves attention and more study.

Domaines: Océan, Atmosphère; Sciences de la Terre

C. Haldoupis, T. Ogawa, K. Schlegel, J. A. Koehler, T. Ono. Is there a plasma density gradient role on the generation of short-scale Farley-Buneman waves?. Annales Geophysicae, 2005, 23 (10), pp.3323-3337. ⟨hal-00318037⟩