Plasma Effects in Dust Devils near the Martian Surface


Citar

Texto integral

Acesso aberto Acesso aberto
Acesso é fechado Acesso está concedido
Acesso é fechado Somente assinantes

Resumo

Plasma−dust effects in the martian atmosphere are discussed. A specific feature of the martian atmosphere is the presence of dust grains in a wide range of altitudes. Taking into account the presence of the martian ionosphere and the high conductivity of the medium at lower altitudes, the appearance of plasma systems in the martian atmosphere can be considered quite a common phenomenon. Special attention is paid to dust devils that frequently form in the martian atmosphere and can efficiently lift dust grains. The processes of dust grain charging as a result of triboelectric effect and generation of electric fields in a dust devil are discussed. The dynamics of dust grains in such a vortex is simulated with allowance for their charging and the generated electric field.

Sobre autores

Yu. Izvekova

Space Research Institute; Moscow Institute of Physics and Technology

Email: popel@iki.rssi.ru
Rússia, Moscow, 117997; Dolgoprudnyi, Moscow oblast, 141700

S. Popel

Space Research Institute; Moscow Institute of Physics and Technology; National Research University Higher School of Economics

Autor responsável pela correspondência
Email: popel@iki.rssi.ru
Rússia, Moscow, 117997; Dolgoprudnyi, Moscow oblast, 141700; Moscow, 101000


Declaração de direitos autorais © Pleiades Publishing, Ltd., 2017

Este site utiliza cookies

Ao continuar usando nosso site, você concorda com o procedimento de cookies que mantêm o site funcionando normalmente.

Informação sobre cookies