Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity
We present observations from the Falkland Islands Super Dual Auroral Radar Network radar of the propagation of HF radio waves via the Weddell Sea Ionospheric Anomaly (WSA), a region of enhanced austral summer nighttime ionospheric electron densities covering the southern Pacific and South Americas re...
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ftleicesterunfig:oai:figshare.com:article/10176056 2023-05-15T18:43:16+02:00 Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity Steve Milan Adrian Grocott S. de Larquier Mark Lester Tim Yeoman M. P. Freeman G. Chisham 2013-10-01T00:00:00Z https://figshare.com/articles/journal_contribution/Traveling_ionospheric_disturbances_in_the_Weddell_Sea_Anomaly_associated_with_geomagnetic_activity/10176056 unknown 2381/28729 https://figshare.com/articles/journal_contribution/Traveling_ionospheric_disturbances_in_the_Weddell_Sea_Anomaly_associated_with_geomagnetic_activity/10176056 All Rights Reserved Uncategorized Science & Technology Physical Sciences Astronomy & Astrophysics GEOSCIENCES MULTIDISCIPLINARY ionosphere anomaly waves SuperDARN ATMOSPHERIC GRAVITY-WAVES HF RADARS Text Journal contribution 2013 ftleicesterunfig 2021-11-11T20:01:12Z We present observations from the Falkland Islands Super Dual Auroral Radar Network radar of the propagation of HF radio waves via the Weddell Sea Ionospheric Anomaly (WSA), a region of enhanced austral summer nighttime ionospheric electron densities covering the southern Pacific and South Americas region. This anomaly is thought to be produced by uplift of the ionosphere by prevailing equatorward thermospheric winds. Of particular interest are perturbations of the WSA-supported propagation, which suggest that during periods of geomagnetic disturbance, the ionospheric layer can be lowered by several tens of kilometers and subsequently recover over a period of 1 to 2 h. Perturbations can appear singly or as a train of two to three events. We discuss possible causes of the perturbations and conclude that they are associated with equatorward propagating large-scale atmospheric waves produced by magnetospheric energy deposition in the auroral or subauroral ionosphere. Changes in high/ middle latitude electrodynamics during geomagnetic storms may also account for the perturbations, but further modeling is required to fully understand their cause. Other Non-Article Part of Journal/Newspaper Weddell Sea University of Leicester: Figshare Weddell Sea Austral Weddell |
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Open Polar |
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University of Leicester: Figshare |
op_collection_id |
ftleicesterunfig |
language |
unknown |
topic |
Uncategorized Science & Technology Physical Sciences Astronomy & Astrophysics GEOSCIENCES MULTIDISCIPLINARY ionosphere anomaly waves SuperDARN ATMOSPHERIC GRAVITY-WAVES HF RADARS |
spellingShingle |
Uncategorized Science & Technology Physical Sciences Astronomy & Astrophysics GEOSCIENCES MULTIDISCIPLINARY ionosphere anomaly waves SuperDARN ATMOSPHERIC GRAVITY-WAVES HF RADARS Steve Milan Adrian Grocott S. de Larquier Mark Lester Tim Yeoman M. P. Freeman G. Chisham Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity |
topic_facet |
Uncategorized Science & Technology Physical Sciences Astronomy & Astrophysics GEOSCIENCES MULTIDISCIPLINARY ionosphere anomaly waves SuperDARN ATMOSPHERIC GRAVITY-WAVES HF RADARS |
description |
We present observations from the Falkland Islands Super Dual Auroral Radar Network radar of the propagation of HF radio waves via the Weddell Sea Ionospheric Anomaly (WSA), a region of enhanced austral summer nighttime ionospheric electron densities covering the southern Pacific and South Americas region. This anomaly is thought to be produced by uplift of the ionosphere by prevailing equatorward thermospheric winds. Of particular interest are perturbations of the WSA-supported propagation, which suggest that during periods of geomagnetic disturbance, the ionospheric layer can be lowered by several tens of kilometers and subsequently recover over a period of 1 to 2 h. Perturbations can appear singly or as a train of two to three events. We discuss possible causes of the perturbations and conclude that they are associated with equatorward propagating large-scale atmospheric waves produced by magnetospheric energy deposition in the auroral or subauroral ionosphere. Changes in high/ middle latitude electrodynamics during geomagnetic storms may also account for the perturbations, but further modeling is required to fully understand their cause. |
format |
Other Non-Article Part of Journal/Newspaper |
author |
Steve Milan Adrian Grocott S. de Larquier Mark Lester Tim Yeoman M. P. Freeman G. Chisham |
author_facet |
Steve Milan Adrian Grocott S. de Larquier Mark Lester Tim Yeoman M. P. Freeman G. Chisham |
author_sort |
Steve Milan |
title |
Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity |
title_short |
Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity |
title_full |
Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity |
title_fullStr |
Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity |
title_full_unstemmed |
Traveling ionospheric disturbances in the Weddell Sea Anomaly associated with geomagnetic activity |
title_sort |
traveling ionospheric disturbances in the weddell sea anomaly associated with geomagnetic activity |
publishDate |
2013 |
url |
https://figshare.com/articles/journal_contribution/Traveling_ionospheric_disturbances_in_the_Weddell_Sea_Anomaly_associated_with_geomagnetic_activity/10176056 |
geographic |
Weddell Sea Austral Weddell |
geographic_facet |
Weddell Sea Austral Weddell |
genre |
Weddell Sea |
genre_facet |
Weddell Sea |
op_relation |
2381/28729 https://figshare.com/articles/journal_contribution/Traveling_ionospheric_disturbances_in_the_Weddell_Sea_Anomaly_associated_with_geomagnetic_activity/10176056 |
op_rights |
All Rights Reserved |
_version_ |
1766233546586849280 |