Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1777053 | Journal of Atmospheric and Solar-Terrestrial Physics | 2012 | 5 Pages |
It is generally assumed that negatively charged icy dust particles in the mesosphere are charged by the collection of thermal plasma particles. However, there are some indications that there may be a population of hyperthermal electrons in the D-region under auroral activity under certain conditions (e.g. Margot-Chaker and McNamara, Planetary and Space Science 32, 391, 1984). In this brief communication, we speculate on the effect of a hyperthermal distribution of electrons on dust charging, and how this might affect prevailing turbulence scattering theory for polar summer mesophere echoes.
► We speculate on how hyperthermal electrons that may occur in the D-region under auroral activity could affect dust charging. ► If the dust density is smaller than the density of hyperthermal electrons, the dust negative charge could be enhanced. ► Enhancement of the dust negative charge may lead to increases in the Schmidt numbers by factors of about 2–4.