On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels

We present a multi‐instrument multiscale study of a channel of enhanced, inhomogeneous flow in the cusp ionosphere occurring on November 30, 2014. We provide evidence that strong Global Navigation Satellite System (GNSS) phase scintillations indices (σϕ>0.5 rad) can arise from such events, indica...

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Published in:Journal of Geophysical Research: Space Physics
Main Authors: Spicher, Andres, Deshpande, Kshitija, Jin, Yaqi, Oksavik, Kjellmar, Zettergren, Matthew D., Clausen, Lasse Boy Novock, Moen, Jøran Idar, Hairston, Marc R., Baddeley, Lisa
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 2020
Subjects:
Online Access:https://hdl.handle.net/11250/2740332
https://doi.org/10.1029/2019JA027734
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spelling ftunivbergen:oai:bora.uib.no:11250/2740332 2023-05-15T18:29:44+02:00 On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels Spicher, Andres Deshpande, Kshitija Jin, Yaqi Oksavik, Kjellmar Zettergren, Matthew D. Clausen, Lasse Boy Novock Moen, Jøran Idar Hairston, Marc R. Baddeley, Lisa 2020 application/pdf https://hdl.handle.net/11250/2740332 https://doi.org/10.1029/2019JA027734 eng eng Wiley Norges forskningsråd: 275653 urn:issn:2169-9380 https://hdl.handle.net/11250/2740332 https://doi.org/10.1029/2019JA027734 cristin:1820203 Journal of Geophysical Research: Space Physics. 2020, 125 (6), e2019JA027734. Navngivelse 4.0 Internasjonal http://creativecommons.org/licenses/by/4.0/deed.no Copyright 2020. The Authors. e2019JA027734 Journal of Geophysical Research (JGR): Space Physics 125 6 Journal article Peer reviewed 2020 ftunivbergen https://doi.org/10.1029/2019JA027734 2023-03-14T17:41:15Z We present a multi‐instrument multiscale study of a channel of enhanced, inhomogeneous flow in the cusp ionosphere occurring on November 30, 2014. We provide evidence that strong Global Navigation Satellite System (GNSS) phase scintillations indices (σϕ>0.5 rad) can arise from such events, indicating that they are important in the context of space weather impacts on technology. We compare in detail two‐dimensional maps of ionospheric density, velocity, and temperatures obtained by the European Incoherent Scatter Scientific Association Svalbard Radar with scintillation indices detected from a network of four GNSS receivers around Svalbard and examine the different sources of free energy for irregularity creation. We observe that the strongest phase scintillations occur on the poleward side of the flow channel in a region of sheared plasma motion and structured low‐energy particle precipitation. As inhomogeneous plasma flows are evident in our observations, we perform a quantitative, nonlinear analysis of the Kelvin–Helmholtz instability (KHI) and its impact on phase scintillations using numerical simulations from the first principles‐based Geospace Environment Model of Ion‐Neutral Interactions and Satellite‐beacon Ionospheric‐scintillation Global Model of the upper Atmosphere. Using representative values consistent with the radar data, we show that KHI can efficiently create density structures along with considerable scintillations and is thus likely to contribute significantly under similar conditions, which are frequent in the cusp. publishedVersion Article in Journal/Newspaper Svalbard University of Bergen: Bergen Open Research Archive (BORA-UiB) Svalbard Journal of Geophysical Research: Space Physics 125 6
institution Open Polar
collection University of Bergen: Bergen Open Research Archive (BORA-UiB)
op_collection_id ftunivbergen
language English
description We present a multi‐instrument multiscale study of a channel of enhanced, inhomogeneous flow in the cusp ionosphere occurring on November 30, 2014. We provide evidence that strong Global Navigation Satellite System (GNSS) phase scintillations indices (σϕ>0.5 rad) can arise from such events, indicating that they are important in the context of space weather impacts on technology. We compare in detail two‐dimensional maps of ionospheric density, velocity, and temperatures obtained by the European Incoherent Scatter Scientific Association Svalbard Radar with scintillation indices detected from a network of four GNSS receivers around Svalbard and examine the different sources of free energy for irregularity creation. We observe that the strongest phase scintillations occur on the poleward side of the flow channel in a region of sheared plasma motion and structured low‐energy particle precipitation. As inhomogeneous plasma flows are evident in our observations, we perform a quantitative, nonlinear analysis of the Kelvin–Helmholtz instability (KHI) and its impact on phase scintillations using numerical simulations from the first principles‐based Geospace Environment Model of Ion‐Neutral Interactions and Satellite‐beacon Ionospheric‐scintillation Global Model of the upper Atmosphere. Using representative values consistent with the radar data, we show that KHI can efficiently create density structures along with considerable scintillations and is thus likely to contribute significantly under similar conditions, which are frequent in the cusp. publishedVersion
format Article in Journal/Newspaper
author Spicher, Andres
Deshpande, Kshitija
Jin, Yaqi
Oksavik, Kjellmar
Zettergren, Matthew D.
Clausen, Lasse Boy Novock
Moen, Jøran Idar
Hairston, Marc R.
Baddeley, Lisa
spellingShingle Spicher, Andres
Deshpande, Kshitija
Jin, Yaqi
Oksavik, Kjellmar
Zettergren, Matthew D.
Clausen, Lasse Boy Novock
Moen, Jøran Idar
Hairston, Marc R.
Baddeley, Lisa
On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels
author_facet Spicher, Andres
Deshpande, Kshitija
Jin, Yaqi
Oksavik, Kjellmar
Zettergren, Matthew D.
Clausen, Lasse Boy Novock
Moen, Jøran Idar
Hairston, Marc R.
Baddeley, Lisa
author_sort Spicher, Andres
title On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels
title_short On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels
title_full On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels
title_fullStr On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels
title_full_unstemmed On the Production of Ionospheric Irregularities Via Kelvin-Helmholtz Instability Associated with Cusp Flow Channels
title_sort on the production of ionospheric irregularities via kelvin-helmholtz instability associated with cusp flow channels
publisher Wiley
publishDate 2020
url https://hdl.handle.net/11250/2740332
https://doi.org/10.1029/2019JA027734
geographic Svalbard
geographic_facet Svalbard
genre Svalbard
genre_facet Svalbard
op_source e2019JA027734
Journal of Geophysical Research (JGR): Space Physics
125
6
op_relation Norges forskningsråd: 275653
urn:issn:2169-9380
https://hdl.handle.net/11250/2740332
https://doi.org/10.1029/2019JA027734
cristin:1820203
Journal of Geophysical Research: Space Physics. 2020, 125 (6), e2019JA027734.
op_rights Navngivelse 4.0 Internasjonal
http://creativecommons.org/licenses/by/4.0/deed.no
Copyright 2020. The Authors.
op_doi https://doi.org/10.1029/2019JA027734
container_title Journal of Geophysical Research: Space Physics
container_volume 125
container_issue 6
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