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  4. Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances

Night‐Time Ionospheric Localized Enhancements (NILE) Observed in North America Following Geomagnetic Disturbances

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JGR Space Physics - 2021 - Chartier - Night‐Time Ionospheric Localized Enhancements NILE Observed in North America.pdf

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Author(s)
Chartier, AT
•
Datta‐Barua, S
•
McDonald, SE
•
Bust, GS
•
Tate, J
•
Goncharenko, LP
•
Romeo, G
•
Schaefer, RK
Date Issued
August 24, 2021
Journal
Journal of Geophysical Research: Space Physics
Publisher
American Geophysical Union
Citation
Chartier, A. T., Datta-Barua, S., McDonald, S. E., Bust, G. S., Tate, J., Goncharenko, L. P., et al. (2021). Night-time ionospheric localized enhancements (NILE) observed in North America following geomagnetic disturbances. Journal of Geophysical Research: Space Physics, 126, e2021JA029324.
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Final published version
Abstract
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.
MIT Department
Haystack Observatory
Terms of Use
Creative Commons Attribution-NonCommercial-NoDerivatives
https://creativecommons.org/licenses/by-nc-nd/4.0/
Persistent DSpace Link
https://dspace.mit.edu/handle/1721.1/176372
DOI of Published Version
https://doi.org/10.1029/2021ja029324
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