Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements
We present a new technique for the upcoming tri-static incoherent scatter radar system EISCAT 3D (E3D) to perform a volumetric reconstruction of the 3D ionospheric electric current density vector field, focusing on the feasibility of the E3D system. The input to our volumetric reconstruction techniq...
Published in: | Journal of Geophysical Research: Space Physics |
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Main Authors: | , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
AGU
2024
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Subjects: | |
Online Access: | https://hdl.handle.net/11250/3180230 https://doi.org/10.1029/2024JA032744 |
_version_ | 1828058751064604672 |
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author | Reistad, Jone Peter Hatch, Spencer Mark Laundal, Karl Magnus Oksavik, Kjellmar Zettergren, M. Vanhamäki, Heikki Virtanen, Ilkka |
author_facet | Reistad, Jone Peter Hatch, Spencer Mark Laundal, Karl Magnus Oksavik, Kjellmar Zettergren, M. Vanhamäki, Heikki Virtanen, Ilkka |
author_sort | Reistad, Jone Peter |
collection | University of Bergen: Bergen Open Research Archive (BORA-UiB) |
container_issue | 8 |
container_title | Journal of Geophysical Research: Space Physics |
container_volume | 129 |
description | We present a new technique for the upcoming tri-static incoherent scatter radar system EISCAT 3D (E3D) to perform a volumetric reconstruction of the 3D ionospheric electric current density vector field, focusing on the feasibility of the E3D system. The input to our volumetric reconstruction technique are estimates of the 3D current density perpendicular to the main magnetic field, j⊥, and its covariance, to be obtained from E3D observations based on two main assumptions: (a) Ions fully magnetized above the E region, set to 200 km here. (b) Electrons fully magnetized above the base of our domain, set to 90 km. In this way, j⊥ estimates are obtained without assumptions about the neutral wind field, allowing it to be subsequently determined. The volumetric reconstruction of the full 3D current density is implemented as vertically coupled horizontal layers represented by Spherical Elementary Current Systems with a built-in current continuity constraint. We demonstrate that our technique is able to retrieve the three dimensional nature of the currents in our idealized setup, taken from a simulation of an active auroral ionosphere using the Geospace Environment Model of Ion-Neutral Interactions (GEMINI). The vertical current is typically less constrained than the horizontal, but we outline strategies for improvement by utilizing additional data sources in the inversion. The ability to reconstruct the neutral wind field perpendicular to the magnetic field in the E region is demonstrated to mostly be within ±50 m/s in a limited region above the radar system in our setup. publishedVersion |
format | Article in Journal/Newspaper |
genre | EISCAT |
genre_facet | EISCAT |
geographic | Gemini |
geographic_facet | Gemini |
id | ftunivbergen:oai:bora.uib.no:11250/3180230 |
institution | Open Polar |
language | English |
long_lat | ENVELOPE(-62.500,-62.500,-66.133,-66.133) |
op_collection_id | ftunivbergen |
op_doi | https://doi.org/10.1029/2024JA032744 |
op_relation | Norges forskningsråd: 300844 https://hdl.handle.net/11250/3180230 https://doi.org/10.1029/2024JA032744 cristin:2288442 Journal of Geophysical Research (JGR): Space Physics. 129 (8), e2024JA032744. |
op_rights | Navngivelse 4.0 Internasjonal http://creativecommons.org/licenses/by/4.0/deed.no Copyright 2024 The Author(s) |
op_source | e2024JA032744 Journal of Geophysical Research (JGR): Space Physics 129 8 |
publishDate | 2024 |
publisher | AGU |
record_format | openpolar |
spelling | ftunivbergen:oai:bora.uib.no:11250/3180230 2025-03-30T15:10:34+00:00 Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements Reistad, Jone Peter Hatch, Spencer Mark Laundal, Karl Magnus Oksavik, Kjellmar Zettergren, M. Vanhamäki, Heikki Virtanen, Ilkka 2024 application/pdf https://hdl.handle.net/11250/3180230 https://doi.org/10.1029/2024JA032744 eng eng AGU Norges forskningsråd: 300844 https://hdl.handle.net/11250/3180230 https://doi.org/10.1029/2024JA032744 cristin:2288442 Journal of Geophysical Research (JGR): Space Physics. 129 (8), e2024JA032744. Navngivelse 4.0 Internasjonal http://creativecommons.org/licenses/by/4.0/deed.no Copyright 2024 The Author(s) e2024JA032744 Journal of Geophysical Research (JGR): Space Physics 129 8 Journal article Peer reviewed 2024 ftunivbergen https://doi.org/10.1029/2024JA032744 2025-03-04T00:50:00Z We present a new technique for the upcoming tri-static incoherent scatter radar system EISCAT 3D (E3D) to perform a volumetric reconstruction of the 3D ionospheric electric current density vector field, focusing on the feasibility of the E3D system. The input to our volumetric reconstruction technique are estimates of the 3D current density perpendicular to the main magnetic field, j⊥, and its covariance, to be obtained from E3D observations based on two main assumptions: (a) Ions fully magnetized above the E region, set to 200 km here. (b) Electrons fully magnetized above the base of our domain, set to 90 km. In this way, j⊥ estimates are obtained without assumptions about the neutral wind field, allowing it to be subsequently determined. The volumetric reconstruction of the full 3D current density is implemented as vertically coupled horizontal layers represented by Spherical Elementary Current Systems with a built-in current continuity constraint. We demonstrate that our technique is able to retrieve the three dimensional nature of the currents in our idealized setup, taken from a simulation of an active auroral ionosphere using the Geospace Environment Model of Ion-Neutral Interactions (GEMINI). The vertical current is typically less constrained than the horizontal, but we outline strategies for improvement by utilizing additional data sources in the inversion. The ability to reconstruct the neutral wind field perpendicular to the magnetic field in the E region is demonstrated to mostly be within ±50 m/s in a limited region above the radar system in our setup. publishedVersion Article in Journal/Newspaper EISCAT University of Bergen: Bergen Open Research Archive (BORA-UiB) Gemini ENVELOPE(-62.500,-62.500,-66.133,-66.133) Journal of Geophysical Research: Space Physics 129 8 |
spellingShingle | Reistad, Jone Peter Hatch, Spencer Mark Laundal, Karl Magnus Oksavik, Kjellmar Zettergren, M. Vanhamäki, Heikki Virtanen, Ilkka Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements |
title | Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements |
title_full | Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements |
title_fullStr | Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements |
title_full_unstemmed | Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements |
title_short | Volumetric Reconstruction of Ionospheric Electric Currents From Tri-Static Incoherent Scatter Radar Measurements |
title_sort | volumetric reconstruction of ionospheric electric currents from tri-static incoherent scatter radar measurements |
url | https://hdl.handle.net/11250/3180230 https://doi.org/10.1029/2024JA032744 |