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Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances
The Ionospheric Data Assimilation Four‐Dimensional (IDA4D) technique has been coupled to Sami3, which is another model of the ionosphere (SAMI3). In this application, ground‐based and space‐based GPS total electron content (TEC) data have been assimilated into SAMI3, while in‐situ electron densities...
Autores principales: | , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
John Wiley and Sons Inc.
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9285011/ https://www.ncbi.nlm.nih.gov/pubmed/35846730 http://dx.doi.org/10.1029/2021JA029324 |
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author | Chartier, A. T. Datta‐Barua, S. McDonald, S. E. Bust, G. S. Tate, J. Goncharenko, L. P. Romeo, G. Schaefer, R. K. |
author_facet | Chartier, A. T. Datta‐Barua, S. McDonald, S. E. Bust, G. S. Tate, J. Goncharenko, L. P. Romeo, G. Schaefer, R. K. |
author_sort | Chartier, A. T. |
collection | PubMed |
description | The Ionospheric Data Assimilation Four‐Dimensional (IDA4D) technique has been coupled to Sami3, which is another model of the ionosphere (SAMI3). In this application, ground‐based and space‐based GPS total electron content (TEC) data have been assimilated into SAMI3, while in‐situ electron densities, autoscaled ionosonde NmF2, and reference GPS stations have been used for validation. IDA4D/SAMI3 shows that night‐time ionospheric localized enhancements (NILE) are formed following geomagnetic storms in November 2003 and August 2018. The NILE phenomenon appears as a moderate, longitudinally extended enhancement of NmF2 at 30°–40°N MLAT, occurring in the late evening (20–24 LT) following much larger enhancements of the equatorial anomaly crests in the main phase of the storms. The NILE appears to be caused by upward and northward plasma transport around the dusk terminator, which is consistent with eastward polarization electric fields. Independent validation confirms the presence of the NILE, and indicates that IDA4D is effective in correcting random errors and systematic biases in SAMI3. In all cases, biases and root‐mean‐square errors are reduced by the data assimilation, typically by a factor of 2 or more. During the most severe part of the November 2003 storm, the uncorrected ionospheric error on a GPS 3D position at 1LSU (Louisiana) is estimated to exceed 34 m. The IDA4D/SAMI3 specification is effective in correcting this down to 10 m. |
format | Online Article Text |
id | pubmed-9285011 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | John Wiley and Sons Inc. |
record_format | MEDLINE/PubMed |
spelling | pubmed-92850112022-07-15 Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances Chartier, A. T. Datta‐Barua, S. McDonald, S. E. Bust, G. S. Tate, J. Goncharenko, L. P. Romeo, G. Schaefer, R. K. J Geophys Res Space Phys Research Article The Ionospheric Data Assimilation Four‐Dimensional (IDA4D) technique has been coupled to Sami3, which is another model of the ionosphere (SAMI3). In this application, ground‐based and space‐based GPS total electron content (TEC) data have been assimilated into SAMI3, while in‐situ electron densities, autoscaled ionosonde NmF2, and reference GPS stations have been used for validation. IDA4D/SAMI3 shows that night‐time ionospheric localized enhancements (NILE) are formed following geomagnetic storms in November 2003 and August 2018. The NILE phenomenon appears as a moderate, longitudinally extended enhancement of NmF2 at 30°–40°N MLAT, occurring in the late evening (20–24 LT) following much larger enhancements of the equatorial anomaly crests in the main phase of the storms. The NILE appears to be caused by upward and northward plasma transport around the dusk terminator, which is consistent with eastward polarization electric fields. Independent validation confirms the presence of the NILE, and indicates that IDA4D is effective in correcting random errors and systematic biases in SAMI3. In all cases, biases and root‐mean‐square errors are reduced by the data assimilation, typically by a factor of 2 or more. During the most severe part of the November 2003 storm, the uncorrected ionospheric error on a GPS 3D position at 1LSU (Louisiana) is estimated to exceed 34 m. The IDA4D/SAMI3 specification is effective in correcting this down to 10 m. John Wiley and Sons Inc. 2021-09-13 2021-09 /pmc/articles/PMC9285011/ /pubmed/35846730 http://dx.doi.org/10.1029/2021JA029324 Text en © 2021. The Authors. https://creativecommons.org/licenses/by-nc-nd/4.0/This is an open access article under the terms of the http://creativecommons.org/licenses/by-nc-nd/4.0/ (https://creativecommons.org/licenses/by-nc-nd/4.0/) License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non‐commercial and no modifications or adaptations are made. |
spellingShingle | Research Article Chartier, A. T. Datta‐Barua, S. McDonald, S. E. Bust, G. S. Tate, J. Goncharenko, L. P. Romeo, G. Schaefer, R. K. Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances |
title | Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances |
title_full | Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances |
title_fullStr | Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances |
title_full_unstemmed | Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances |
title_short | Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances |
title_sort | night‐time ionospheric localized enhancements (nile) observed in north america following geomagnetic disturbances |
topic | Research Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9285011/ https://www.ncbi.nlm.nih.gov/pubmed/35846730 http://dx.doi.org/10.1029/2021JA029324 |
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