Rayleigh-Taylor Instability Development in the Equatorial Ionosphere and a Geometry of an Initial Irregularity
- Authors: Kashchenko N.M.1, Ishanov S.A.1, Matsievsky S.V.1
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Affiliations:
- Kant Baltic Federal University
- Issue: Vol 11, No 3 (2019)
- Pages: 341-348
- Section: Article
- URL: https://journals.rcsi.science/2070-0482/article/view/203188
- DOI: https://doi.org/10.1134/S2070048219030116
- ID: 203188
Cite item
Abstract
In this paper, we performed a numerical simulation for the conditions of the equatorial F‑region of the Earth’s ionosphere using the two-dimensional electrodynamically consistent mathematical MI2 model. The development time of ionospheric bubbles is shown to depend sufficiently strongly on the vertical scale and less strongly on the horizontal scale of the initial irregularity. Ionospheric bubbles developed more slowly at the generation of instability by increasing the plasma concentration than by depleting a plasma. On increasing the initial irregularity scale, three metric thresholds are experimentally found.
About the authors
N. M. Kashchenko
Kant Baltic Federal University
Author for correspondence.
Email: kaschtschenko@mail.ru
Russian Federation, Kaliningrad, 236041
S. A. Ishanov
Kant Baltic Federal University
Author for correspondence.
Email: sergey.ishanov@ya.ru
Russian Federation, Kaliningrad, 236041
S. V. Matsievsky
Kant Baltic Federal University
Author for correspondence.
Email: sergei.matsievsky@yandex.ru
Russian Federation, Kaliningrad, 236041