A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary

The aim of this paper is to advance the current understanding of the spectral width parameter observed by coherent high frequency (HF) radars. In particular, we address the relationship of a frequently observed gradient, between low ( < 200 m/s) and high ( > 200 m/s) spectral width, to magneto...

Full description

Bibliographic Details
Published in:Annales Geophysicae
Main Authors: Woodfield, Emma E., Davies, J. A., Eglitis, P., Lester, M.
Format: Article in Journal/Newspaper
Language:English
Published: European Geosciences Union (EGU) 2013
Subjects:
Online Access:http://www.ann-geophys.net/20/501/2002/angeo-20-501-2002.html
http://hdl.handle.net/2381/28304
https://doi.org/10.5194/angeo-20-501-2002
id ftleicester:oai:lra.le.ac.uk:2381/28304
record_format openpolar
spelling ftleicester:oai:lra.le.ac.uk:2381/28304 2023-05-15T16:04:47+02:00 A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary Woodfield, Emma E. Davies, J. A. Eglitis, P. Lester, M. 2013-10-17T11:20:49Z http://www.ann-geophys.net/20/501/2002/angeo-20-501-2002.html http://hdl.handle.net/2381/28304 https://doi.org/10.5194/angeo-20-501-2002 en eng European Geosciences Union (EGU) ANNALES GEOPHYSICAE, 2002, 20 (4), pp. 501-509 0992-7689 http://www.ann-geophys.net/20/501/2002/angeo-20-501-2002.html http://hdl.handle.net/2381/28304 doi:10.5194/angeo-20-501-2002 1432-0576 Copyright © 2002 The authors. This is an open-access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/3.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. CC-BY Science & Technology Physical Sciences Astronomy & Astrophysics Geosciences Multidisciplinary Meteorology & Atmospheric Sciences Geology ionosphere auroral ionosphere ionospheric irregularities AURORAL EMISSION EISCAT SVALBARD F-REGION CUSP SUPERDARN SYSTEM PRECIPITATION SIGNATURES DYNAMICS Journal Article Article;Journal 2013 ftleicester https://doi.org/10.5194/angeo-20-501-2002 2019-03-22T20:19:10Z The aim of this paper is to advance the current understanding of the spectral width parameter observed by coherent high frequency (HF) radars. In particular, we address the relationship of a frequently observed gradient, between low ( < 200 m/s) and high ( > 200 m/s) spectral width, to magnetospheric boundaries. Previous work has linked this gradient in the spectral width, in the nightside sector of magnetic local time, to the Polar Cap Boundary (PCB), and also to the boundary between the Central Plasma Sheet (CPS) and the Plasma Sheet Boundary Layer (PSBL). The present case study investigates the former by comparison with the 630.0 nm optical emission. No suitable data were available to test the second of the two hypotheses. It is found that during the interval in question the spectral width gradient is within the region of the 630.0 nm optical emission. A comparison of coherent and incoherent scatter radar data is also conducted, which indicates that values of high spectral width are typically collocated with elevated F-region electron temperatures. We conclude that the high spectral width region in the interval under study is associated with particle precipitation and also that the spectral width gradient is not a reliable method for locating the PCB. Peer-reviewed Publisher Version Article in Journal/Newspaper EISCAT Svalbard University of Leicester: Leicester Research Archive (LRA) Svalbard Annales Geophysicae 20 4 501 509
institution Open Polar
collection University of Leicester: Leicester Research Archive (LRA)
op_collection_id ftleicester
language English
topic Science & Technology
Physical Sciences
Astronomy & Astrophysics
Geosciences
Multidisciplinary
Meteorology & Atmospheric Sciences
Geology
ionosphere
auroral ionosphere
ionospheric irregularities
AURORAL EMISSION
EISCAT SVALBARD
F-REGION
CUSP
SUPERDARN
SYSTEM
PRECIPITATION
SIGNATURES
DYNAMICS
spellingShingle Science & Technology
Physical Sciences
Astronomy & Astrophysics
Geosciences
Multidisciplinary
Meteorology & Atmospheric Sciences
Geology
ionosphere
auroral ionosphere
ionospheric irregularities
AURORAL EMISSION
EISCAT SVALBARD
F-REGION
CUSP
SUPERDARN
SYSTEM
PRECIPITATION
SIGNATURES
DYNAMICS
Woodfield, Emma E.
Davies, J. A.
Eglitis, P.
Lester, M.
A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary
topic_facet Science & Technology
Physical Sciences
Astronomy & Astrophysics
Geosciences
Multidisciplinary
Meteorology & Atmospheric Sciences
Geology
ionosphere
auroral ionosphere
ionospheric irregularities
AURORAL EMISSION
EISCAT SVALBARD
F-REGION
CUSP
SUPERDARN
SYSTEM
PRECIPITATION
SIGNATURES
DYNAMICS
description The aim of this paper is to advance the current understanding of the spectral width parameter observed by coherent high frequency (HF) radars. In particular, we address the relationship of a frequently observed gradient, between low ( < 200 m/s) and high ( > 200 m/s) spectral width, to magnetospheric boundaries. Previous work has linked this gradient in the spectral width, in the nightside sector of magnetic local time, to the Polar Cap Boundary (PCB), and also to the boundary between the Central Plasma Sheet (CPS) and the Plasma Sheet Boundary Layer (PSBL). The present case study investigates the former by comparison with the 630.0 nm optical emission. No suitable data were available to test the second of the two hypotheses. It is found that during the interval in question the spectral width gradient is within the region of the 630.0 nm optical emission. A comparison of coherent and incoherent scatter radar data is also conducted, which indicates that values of high spectral width are typically collocated with elevated F-region electron temperatures. We conclude that the high spectral width region in the interval under study is associated with particle precipitation and also that the spectral width gradient is not a reliable method for locating the PCB. Peer-reviewed Publisher Version
format Article in Journal/Newspaper
author Woodfield, Emma E.
Davies, J. A.
Eglitis, P.
Lester, M.
author_facet Woodfield, Emma E.
Davies, J. A.
Eglitis, P.
Lester, M.
author_sort Woodfield, Emma E.
title A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary
title_short A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary
title_full A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary
title_fullStr A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary
title_full_unstemmed A case study of HF radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary
title_sort case study of hf radar spectral width in the post midnight magnetic local time sector and its relationship to the polar cap boundary
publisher European Geosciences Union (EGU)
publishDate 2013
url http://www.ann-geophys.net/20/501/2002/angeo-20-501-2002.html
http://hdl.handle.net/2381/28304
https://doi.org/10.5194/angeo-20-501-2002
geographic Svalbard
geographic_facet Svalbard
genre EISCAT
Svalbard
genre_facet EISCAT
Svalbard
op_relation ANNALES GEOPHYSICAE, 2002, 20 (4), pp. 501-509
0992-7689
http://www.ann-geophys.net/20/501/2002/angeo-20-501-2002.html
http://hdl.handle.net/2381/28304
doi:10.5194/angeo-20-501-2002
1432-0576
op_rights Copyright © 2002 The authors. This is an open-access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/3.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
op_rightsnorm CC-BY
op_doi https://doi.org/10.5194/angeo-20-501-2002
container_title Annales Geophysicae
container_volume 20
container_issue 4
container_start_page 501
op_container_end_page 509
_version_ 1766400410184056832