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ORIGINAL RESEARCH article

Front. Astron. Space Sci.
Sec. Space Physics
Volume 11 - 2024 | doi: 10.3389/fspas.2024.1347048

Experimental Modeling of Atmospheric Discharge Phenomena and Charged Dust Particle Interactions Provisionally Accepted

 Mohamad E. Abdelaal1, 2* Alexander V. Zakharov2* Igor V. Dokuchaev2 Sergey A. Bednyakov2
  • 1Moscow Institute of Physics and Technology, Russia
  • 2Space Research Institute (RAS), Russia

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The upper atmosphere, comprising the mesosphere and thermosphere, is intricately influenced by various atmospheric and magnetospheric impacts. Various atmospheric waves excited in the troposphere can propagate into the mesosphere-thermosphere (M-T) region, altering its dynamics. Additionally, large-scale disturbances in the middle atmosphere, such as sudden stratospheric warming and geomagnetic disturbances induced by solar activity, affect the upper atmosphere. To better understand these complex processes, observations from multiple platforms and instruments, along with modeling studies, are necessary. This study presents experimental investigations into the electromagnetic signatures generated by atmospheric discharge conditions, including breakdown events and interactions of charged dust particles. A vacuum chamber was used to simulate upper atmospheric conditions. An electromagnetic signal analyzer (EMA) registered signals generated from the atmospheric discharge and the electromagnetic signature of charged dust particles. The results provide crucial insights into the distinctive electromagnetic processes occurring during breakdown events and charged particle interactions within Earth's atmosphere.

Keywords: Electromagnetic Phenomena, Charged dust particles, Upper atmosphere, Highvoltage discharges, Atmospheric phenomena, Electromagnetic analyzer

Received: 30 Nov 2023; Accepted: 27 Mar 2024.

Copyright: © 2024 Abdelaal, Zakharov, Dokuchaev and Bednyakov. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

* Correspondence:
Mx. Mohamad E. Abdelaal, Moscow Institute of Physics and Technology, Dolgoprudny, Russia
Prof. Alexander V. Zakharov, Space Research Institute (RAS), Moscow, Moscow Oblast, Russia