A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements

Accurately measuring the location and motion of the polar cap boundary (PCB) in the high-latitude ionosphere can be crucial for studies concerned with the dynamics of the polar cap, e.g. the measurement of reconnection rates. The Doppler spectral width characteristics of backscatter received by the...

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Published in:Annales Geophysicae
Main Authors: Chisham, G., Freeman, M. P.
Format: Text
Language:English
Published: 2018
Subjects:
Online Access:https://doi.org/10.5194/angeo-21-983-2003
https://angeo.copernicus.org/articles/21/983/2003/
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spelling ftcopernicus:oai:publications.copernicus.org:angeo34891 2023-05-15T13:36:36+02:00 A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements Chisham, G. Freeman, M. P. 2018-09-27 application/pdf https://doi.org/10.5194/angeo-21-983-2003 https://angeo.copernicus.org/articles/21/983/2003/ eng eng doi:10.5194/angeo-21-983-2003 https://angeo.copernicus.org/articles/21/983/2003/ eISSN: 1432-0576 Text 2018 ftcopernicus https://doi.org/10.5194/angeo-21-983-2003 2020-07-20T16:27:44Z Accurately measuring the location and motion of the polar cap boundary (PCB) in the high-latitude ionosphere can be crucial for studies concerned with the dynamics of the polar cap, e.g. the measurement of reconnection rates. The Doppler spectral width characteristics of backscatter received by the SuperDARN HF radars have been previously used for locating and tracking the PCB in the cusp region. The boundary is generally observed in meridional beams of the SuperDARN radars and appears as a distinct change between low spectral width values observed equatorward of the cusp region, and high, but variable spectral width values observed within the cusp region. To identify the spectral width boundary (SWB) between these two regions, a simple algorithm employing a spectral width threshold has often been applied to the data. However, there is not, as yet, a standard algorithm, or spectral width threshold, which is universally applied. Nor has there been any rigorous assessment of the accuracy of this method of boundary determination. This study applies a series of threshold algorithms to a simulated cusp-region spectral width data set, to assess the accuracy of different algorithms. This shows that simple threshold algorithms correctly identify the boundary location in, at the most, 50% of the cases and that the average boundary error is at least ~ 1–2 range gates (~ 1° latitude). It transpires that spatial and temporal smoothing of the spectral width data (e.g. by median filtering), before application of a threshold algorithm can increase the boundary determination accuracy to over 95% and the average boundary error to much less than a range gate. However, this is sometimes at the cost of temporal resolution in the motion of the boundary location. The algorithms are also applied to a year’s worth of spectral width data from the cusp ionosphere, measured by the Halley SuperDARN radar in Antarctica. This analysis highlights the increased accuracy of the enhanced boundary determination algorithm in the cusp region. Away from the cusp, the resulting SWB locations are often dependent on the choice of threshold. This suggests that there is not a sharp latitudinal SWB in regions of the dayside ionosphere away from the cusp, but that there is a shallower latitudinal gradient in spectral width near the boundary location. Key words. Ionosphere (instruments and techniques) – Magnetospheric physics (magnetopause, cusp and boundary layers; magnetosphere-ionosphere interactions) Text Antarc* Antarctica Copernicus Publications: E-Journals Annales Geophysicae 21 4 983 996
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description Accurately measuring the location and motion of the polar cap boundary (PCB) in the high-latitude ionosphere can be crucial for studies concerned with the dynamics of the polar cap, e.g. the measurement of reconnection rates. The Doppler spectral width characteristics of backscatter received by the SuperDARN HF radars have been previously used for locating and tracking the PCB in the cusp region. The boundary is generally observed in meridional beams of the SuperDARN radars and appears as a distinct change between low spectral width values observed equatorward of the cusp region, and high, but variable spectral width values observed within the cusp region. To identify the spectral width boundary (SWB) between these two regions, a simple algorithm employing a spectral width threshold has often been applied to the data. However, there is not, as yet, a standard algorithm, or spectral width threshold, which is universally applied. Nor has there been any rigorous assessment of the accuracy of this method of boundary determination. This study applies a series of threshold algorithms to a simulated cusp-region spectral width data set, to assess the accuracy of different algorithms. This shows that simple threshold algorithms correctly identify the boundary location in, at the most, 50% of the cases and that the average boundary error is at least ~ 1–2 range gates (~ 1° latitude). It transpires that spatial and temporal smoothing of the spectral width data (e.g. by median filtering), before application of a threshold algorithm can increase the boundary determination accuracy to over 95% and the average boundary error to much less than a range gate. However, this is sometimes at the cost of temporal resolution in the motion of the boundary location. The algorithms are also applied to a year’s worth of spectral width data from the cusp ionosphere, measured by the Halley SuperDARN radar in Antarctica. This analysis highlights the increased accuracy of the enhanced boundary determination algorithm in the cusp region. Away from the cusp, the resulting SWB locations are often dependent on the choice of threshold. This suggests that there is not a sharp latitudinal SWB in regions of the dayside ionosphere away from the cusp, but that there is a shallower latitudinal gradient in spectral width near the boundary location. Key words. Ionosphere (instruments and techniques) – Magnetospheric physics (magnetopause, cusp and boundary layers; magnetosphere-ionosphere interactions)
format Text
author Chisham, G.
Freeman, M. P.
spellingShingle Chisham, G.
Freeman, M. P.
A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements
author_facet Chisham, G.
Freeman, M. P.
author_sort Chisham, G.
title A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements
title_short A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements
title_full A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements
title_fullStr A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements
title_full_unstemmed A technique for accurately determining the cusp-region polar cap boundary using SuperDARN HF radar measurements
title_sort technique for accurately determining the cusp-region polar cap boundary using superdarn hf radar measurements
publishDate 2018
url https://doi.org/10.5194/angeo-21-983-2003
https://angeo.copernicus.org/articles/21/983/2003/
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source eISSN: 1432-0576
op_relation doi:10.5194/angeo-21-983-2003
https://angeo.copernicus.org/articles/21/983/2003/
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