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: 2020
Subjects:
Online Access:http://hdl.handle.net/10852/82775
http://urn.nb.no/URN:NBN:no-85606
https://doi.org/10.1029/2019JA027734
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spelling ftoslouniv:oai:www.duo.uio.no:10852/82775 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 2020-07-22T14:50:06Z http://hdl.handle.net/10852/82775 http://urn.nb.no/URN:NBN:no-85606 https://doi.org/10.1029/2019JA027734 EN eng NFR/275653 NFR/223252 http://urn.nb.no/URN:NBN:no-85606 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. Journal of Geophysical Research (JGR): Space Physics. 2020, 125(6) http://hdl.handle.net/10852/82775 1820203 info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Journal of Geophysical Research (JGR): Space Physics&rft.volume=125&rft.spage=&rft.date=2020 Journal of Geophysical Research (JGR): Space Physics 125 6 0 https://doi.org/10.1029/2019JA027734 URN:NBN:no-85606 Fulltext https://www.duo.uio.no/bitstream/handle/10852/82775/2/Spicher_2019JA027734.pdf Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/ CC-BY 2169-9380 Journal article Tidsskriftartikkel Peer reviewed PublishedVersion 2020 ftoslouniv https://doi.org/10.1029/2019JA027734 2021-02-03T23:30:59Z 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. Article in Journal/Newspaper Svalbard Universitet i Oslo: Digitale utgivelser ved UiO (DUO) Svalbard Journal of Geophysical Research: Space Physics 125 6
institution Open Polar
collection Universitet i Oslo: Digitale utgivelser ved UiO (DUO)
op_collection_id ftoslouniv
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.
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
publishDate 2020
url http://hdl.handle.net/10852/82775
http://urn.nb.no/URN:NBN:no-85606
https://doi.org/10.1029/2019JA027734
geographic Svalbard
geographic_facet Svalbard
genre Svalbard
genre_facet Svalbard
op_source 2169-9380
op_relation NFR/275653
NFR/223252
http://urn.nb.no/URN:NBN:no-85606
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. Journal of Geophysical Research (JGR): Space Physics. 2020, 125(6)
http://hdl.handle.net/10852/82775
1820203
info:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Journal of Geophysical Research (JGR): Space Physics&rft.volume=125&rft.spage=&rft.date=2020
Journal of Geophysical Research (JGR): Space Physics
125
6
0
https://doi.org/10.1029/2019JA027734
URN:NBN:no-85606
Fulltext https://www.duo.uio.no/bitstream/handle/10852/82775/2/Spicher_2019JA027734.pdf
op_rights Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/
op_rightsnorm CC-BY
op_doi https://doi.org/10.1029/2019JA027734
container_title Journal of Geophysical Research: Space Physics
container_volume 125
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