Abstract
The results of a study on the relationship of ion upflow occurrence with upstream solar wind plasma parameters and terrestrial magnetic activity are presented.
| Original language | English |
|---|---|
| Article number | JASR19414 |
| Pages (from-to) | 9617-9632 |
| Journal | Advances in Space Research |
| Volume | 77 |
| Issue number | 9 |
| DOIs | |
| Publication status | Published - 13 Apr 2026 |
Bibliographical note
The authors acknowledge the EISCAT Scientific Association for easy access to the Madrigal database. The international community is equally applauded for the 2007 international polar year campaign that generated such a high level of robust data. The authors also acknowledge the OMNIWeb data team for providing the data. This research used the SPECTRE High Performance Computing Facility at the University of Leicester.© 2026 COSPAR. Published by Elsevier B.V. All rights are reserved, including those for text and data mining, AI training, and similar technologies.
Data Access Statement
The EISCAT data used in this paper can be obtained via the schedule pages of the EISCAT website ( https://www.eiscat.se/) and the Madrigal database. The OMNI Web data used in this paper can be accessed from ( https://omniweb.gsfc.nasa.gov/).Keywords
- Electron precipitation
- Ambipolar electric field
- Joule heating
- Upflow
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