EGU26-20038, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-20038
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Tuesday, 05 May, 08:30–10:15 (CEST), Display time Tuesday, 05 May, 08:30–12:30
 
Hall X4, X4.181
Ionospheric traces of plasmaspheric plumes
Balázs Heilig1,2 and Máté Tomasik1,2
Balázs Heilig and Máté Tomasik
  • 1HUN-REN Insitute of Earth Physics and Space Science, Sopron, Hungary (heilig.balazs@epss.hun-ren.hu)
  • 2Space Lab/Institute of Electrophysics, Obuda University, Budapest, Hungary

The plasmasphere is a torus of cold plasma ‘frozen’ into the Earth’s magnetic field, sourced from the ionosphere. Drainage channels, called plumes are formed during disturbed periods by the modified electric field. While plumes have been primarily observed near the equator, the electric field driving then acts along the entire geomagnetic field line, setting the plasma within a complete drift shell into motion. Ionospheric evidence of this process is found in the so-called Storm-Enhanced-Density plumes, which also exhibit density surplus compared to the background. These findings led to the establishment of the geospace plume concept. However, this same process creates other features in the ionosphere, like the midlatitude trough, a zone of depleted plasma density. The relationship between plasmaspheric plumes and the ionospheric trough has been neglected in previous studies. Our findings challenge the current understanding of the geospace plume concept and underscore the need for its refinement.

How to cite: Heilig, B. and Tomasik, M.: Ionospheric traces of plasmaspheric plumes, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-20038, https://doi.org/10.5194/egusphere-egu26-20038, 2026.