Dust modification of the plasma conductivity in the mesosphere
B. P. Pandey, S. V. Vladimirov

TL;DR
This paper investigates how dust particles influence the plasma conductivity in Earth's mesosphere, affecting the Hall effect and the propagation of ultra-low frequency waves, with implications for mesospheric and ionospheric dynamics.
Contribution
It introduces the concept that dust charge and size alter the sign and magnitude of Hall conductivity, impacting wave damping and propagation in the mesosphere.
Findings
Hall conductivity sign depends on dust charge and size.
Ultra-low frequency waves cannot originate below 80 km due to damping.
Above 80 km, Hall effect enables wave propagation with minimal damping.
Abstract
Relative transverse drift (with respect to the ambient magnetic field) between the weakly magnetized electrons and the unmagnetized ions at the lower altitude (80 km) and between the weakly magnetized ions and unmagnetized dust at the higher altitude (90 km) gives rise to the finite Hall conductivity in the Earth's mesosphere. If, on the other hand, the number of free electrons is sparse in the mesosphere and most of the negative charge resides on the weakly magnetized, fine, nanometre sized dust powder and positive charge on the more massive, micron sized, unmagnetized dust, the sign of the Hall conductivity due to their relative transverse drift will be opposite to the previous case. Thus the sign of the Hall effect not only depends on the direction of the local magnetic field but also on the nature of the charge carrier in the partially ionized dusty medium. As the Hall and the Ohm…
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