On the Question of Calculating the Parameters of Vortices in the Near-Surface Atmosphere of Mars
- Authors: Izvekova Y.N.1,2, Popel’ S.I.1,2, Izvekov O.Y.2
-
Affiliations:
- Space Research Institute, Russian Academy of Sciences
- Moscow Institute of Physics and Technology
- Issue: Vol 53, No 6 (2019)
- Pages: 423-430
- Section: Article
- URL: https://journal-vniispk.ru/0038-0946/article/view/171401
- DOI: https://doi.org/10.1134/S0038094619050058
- ID: 171401
Cite item
Abstract
The paper is dedicated to the study of dust vortices on the Earth and Mars. The hydrodynamic similarity of convective vortices is considered, and the similarity criteria are determined. The motion of dust particles in a vortex is modeled. The conditions for the similarity of dust particle trajectories in a vortex in the terrestrial and Martian atmospheres are determined. It is shown that there is a similarity between terrestrial and Martian vortices. This fact can be useful for the study of the Martian atmosphere, given that there are proven methods for measuring the parameters of vortices on the Earth, while such measurements on Mars are difficult.
About the authors
Yu. N. Izvekova
Space Research Institute, Russian Academy of Sciences; Moscow Institute of Physics and Technology
Author for correspondence.
Email: besedina_yn@mail.ru
Russian Federation, Moscow; Dolgoprudny
S. I. Popel’
Space Research Institute, Russian Academy of Sciences; Moscow Institute of Physics and Technology
Email: besedina_yn@mail.ru
Russian Federation, Moscow; Dolgoprudny
O. Ya. Izvekov
Moscow Institute of Physics and Technology
Email: besedina_yn@mail.ru
Russian Federation, Dolgoprudny
Supplementary files
