EGU24-9328, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-9328
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Study of Martian Ionospheric Plasma Depletion Events using MAVEN and Mars Express Spacecraft

Praveen Basuvaraj1, František Němec1, Christopher Fowler2, Leonardo Regoli3, Zdeněk Němeček1, and Jana Šafránková1
Praveen Basuvaraj et al.
  • 1Faculty of Mathematics and Physics, Charles University, Prague, Czechia (praveen.basuvaraj@matfyz.cuni.cz)
  • 2Department of Physics and Astronomy, West Virginia University, Morgantown, WV, USA
  • 3Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA

Plasma Depletion Events (PDEs), characterized by a significant reduction (at least tenfold) in ion number density, are known to occur in the Martian ionosphere. Since its launch in September 2014, the MAVEN spacecraft has spotted around 1000 PDEs, primarily located in the nightside ionosphere and regions with strong crustal magnetic fields. We show that dayside PDEs are associated with an increased level of electrostatic fluctuations and suggest their formation through ambipolar diffusion triggered by the sudden escape of suprathermal electrons. We further investigate possible concurrent detections of PDEs by MAVEN and Mars Express. For this purpose, local electron density measurements from Mars Express near the MAVEN-identified PDEs are systematically checked. We present the first multi-spacecraft observations of PDEs, and we use them to discuss their spatio-temporal extents.

How to cite: Basuvaraj, P., Němec, F., Fowler, C., Regoli, L., Němeček, Z., and Šafránková, J.: Study of Martian Ionospheric Plasma Depletion Events using MAVEN and Mars Express Spacecraft, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-9328, https://doi.org/10.5194/egusphere-egu24-9328, 2024.