How Much Flux Does a Flux Transfer Event Transfer?
Flux transfer events are bursts of reconnection at the dayside magnetopause, which give rise to characteristic signatures observed by a range of magnetospheric/ionospheric instrumentation. One outstanding problem is that there is a fundamental mismatch between space-based and ionospheric estimates o...
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American Geophysical Union (AGU), Wiley
2018
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ftleicester:oai:lra.le.ac.uk:2381/40998 2023-05-15T13:31:55+02:00 How Much Flux Does a Flux Transfer Event Transfer? Fear, R. C. Trenchi, L. Coxon, J. C. Milan, S. E. 2018-01-24T14:21:45Z http://onlinelibrary.wiley.com/doi/10.1002/2017JA024730/abstract http://hdl.handle.net/2381/40998 https://doi.org/10.1002/2017JA024730 en eng American Geophysical Union (AGU), Wiley Journal of Geophysical Research: Space Physics, 2017, 122, 12, 310–12, 327. 2169-9380 http://onlinelibrary.wiley.com/doi/10.1002/2017JA024730/abstract http://hdl.handle.net/2381/40998 doi:10.1002/2017JA024730 2169-9402 Copyright © the authors, 2017. This is an open-access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited. CC-BY reconnection magnetopause flux transfer event Journal Article Article in Press 2018 ftleicester https://doi.org/10.1002/2017JA024730 2019-03-22T20:24:34Z Flux transfer events are bursts of reconnection at the dayside magnetopause, which give rise to characteristic signatures observed by a range of magnetospheric/ionospheric instrumentation. One outstanding problem is that there is a fundamental mismatch between space-based and ionospheric estimates of the flux that is opened by each flux transfer event-in other words, their overall significance in the Dungey cycle. Spacecraft-based estimates of the flux content of individual flux transfer events (FTEs) correspond to each event transferring flux equivalent to approximately 1% of the open flux in the magnetosphere, whereas studies based on global-scale radar and auroral observations suggest this figure could be of the order of 10%. In the former case, flux transfer events would be a minor detail in the Dungey cycle, but in the latter they could be its main driver. We present observations of two conjunctions between flux transfer events observed by the Cluster spacecraft and pulsed ionospheric flows observed by the Super Dual Auroral Radar Network (SuperDARN) network. In both cases, a similar number of FTE signatures were observed by Cluster and one of the SuperDARN radars, but the conjunctions differ in the azimuthal separation of the spacecraft and ionospheric observations (i.e., the distance of the spacecraft from the cusp throat). We argue that the reason for the existing mismatch in flux estimates is due to implicit assumptions made about FTE structure, which tacitly ignore the majority of flux opened in mechanisms based on longer reconnection lines. If the effects of such mechanisms are considered, a much better match is found. R. C. F. was supported by the UK's Science and Technology Facilities Council (STFC) Ernest Rutherford Fellowship ST/K004298/2; L. T. and J. C. C. were supported by STFC Ernest Rutherford grant ST/L002809/1, and S. E. M. was supported by STFC consolidated grant ST/N000749/1. SuperDARN is a collection of radars funded by national scientific funding agencies of Australia, Canada, China, France, Japan, South Africa, United Kingdom, and the United States of America. Data were obtained from the British Antarctic Survey SuperDARN data hub and processed with RST v4.0 and FITACF v3.0. Cluster data were obtained from the Cluster Science Archive (https://www.cosmos.esa.int/web/csa). We are grateful to Paul Breen, Pasha Ponomarenko, Kevin Sterne, and Keith Kotyk for their assistance with the SuperDARN data hub, RST, and FITACF. Peer-reviewed Publisher Version Article in Journal/Newspaper Antarc* Antarctic British Antarctic Survey University of Leicester: Leicester Research Archive (LRA) Antarctic Canada Breen ENVELOPE(13.338,13.338,66.778,66.778) Journal of Geophysical Research: Space Physics 122 12 12,310 12,327 |
institution |
Open Polar |
collection |
University of Leicester: Leicester Research Archive (LRA) |
op_collection_id |
ftleicester |
language |
English |
topic |
reconnection magnetopause flux transfer event |
spellingShingle |
reconnection magnetopause flux transfer event Fear, R. C. Trenchi, L. Coxon, J. C. Milan, S. E. How Much Flux Does a Flux Transfer Event Transfer? |
topic_facet |
reconnection magnetopause flux transfer event |
description |
Flux transfer events are bursts of reconnection at the dayside magnetopause, which give rise to characteristic signatures observed by a range of magnetospheric/ionospheric instrumentation. One outstanding problem is that there is a fundamental mismatch between space-based and ionospheric estimates of the flux that is opened by each flux transfer event-in other words, their overall significance in the Dungey cycle. Spacecraft-based estimates of the flux content of individual flux transfer events (FTEs) correspond to each event transferring flux equivalent to approximately 1% of the open flux in the magnetosphere, whereas studies based on global-scale radar and auroral observations suggest this figure could be of the order of 10%. In the former case, flux transfer events would be a minor detail in the Dungey cycle, but in the latter they could be its main driver. We present observations of two conjunctions between flux transfer events observed by the Cluster spacecraft and pulsed ionospheric flows observed by the Super Dual Auroral Radar Network (SuperDARN) network. In both cases, a similar number of FTE signatures were observed by Cluster and one of the SuperDARN radars, but the conjunctions differ in the azimuthal separation of the spacecraft and ionospheric observations (i.e., the distance of the spacecraft from the cusp throat). We argue that the reason for the existing mismatch in flux estimates is due to implicit assumptions made about FTE structure, which tacitly ignore the majority of flux opened in mechanisms based on longer reconnection lines. If the effects of such mechanisms are considered, a much better match is found. R. C. F. was supported by the UK's Science and Technology Facilities Council (STFC) Ernest Rutherford Fellowship ST/K004298/2; L. T. and J. C. C. were supported by STFC Ernest Rutherford grant ST/L002809/1, and S. E. M. was supported by STFC consolidated grant ST/N000749/1. SuperDARN is a collection of radars funded by national scientific funding agencies of Australia, Canada, China, France, Japan, South Africa, United Kingdom, and the United States of America. Data were obtained from the British Antarctic Survey SuperDARN data hub and processed with RST v4.0 and FITACF v3.0. Cluster data were obtained from the Cluster Science Archive (https://www.cosmos.esa.int/web/csa). We are grateful to Paul Breen, Pasha Ponomarenko, Kevin Sterne, and Keith Kotyk for their assistance with the SuperDARN data hub, RST, and FITACF. Peer-reviewed Publisher Version |
format |
Article in Journal/Newspaper |
author |
Fear, R. C. Trenchi, L. Coxon, J. C. Milan, S. E. |
author_facet |
Fear, R. C. Trenchi, L. Coxon, J. C. Milan, S. E. |
author_sort |
Fear, R. C. |
title |
How Much Flux Does a Flux Transfer Event Transfer? |
title_short |
How Much Flux Does a Flux Transfer Event Transfer? |
title_full |
How Much Flux Does a Flux Transfer Event Transfer? |
title_fullStr |
How Much Flux Does a Flux Transfer Event Transfer? |
title_full_unstemmed |
How Much Flux Does a Flux Transfer Event Transfer? |
title_sort |
how much flux does a flux transfer event transfer? |
publisher |
American Geophysical Union (AGU), Wiley |
publishDate |
2018 |
url |
http://onlinelibrary.wiley.com/doi/10.1002/2017JA024730/abstract http://hdl.handle.net/2381/40998 https://doi.org/10.1002/2017JA024730 |
long_lat |
ENVELOPE(13.338,13.338,66.778,66.778) |
geographic |
Antarctic Canada Breen |
geographic_facet |
Antarctic Canada Breen |
genre |
Antarc* Antarctic British Antarctic Survey |
genre_facet |
Antarc* Antarctic British Antarctic Survey |
op_relation |
Journal of Geophysical Research: Space Physics, 2017, 122, 12, 310–12, 327. 2169-9380 http://onlinelibrary.wiley.com/doi/10.1002/2017JA024730/abstract http://hdl.handle.net/2381/40998 doi:10.1002/2017JA024730 2169-9402 |
op_rights |
Copyright © the authors, 2017. This is an open-access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0/), 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/10.1002/2017JA024730 |
container_title |
Journal of Geophysical Research: Space Physics |
container_volume |
122 |
container_issue |
12 |
container_start_page |
12,310 |
op_container_end_page |
12,327 |
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1766022423771086848 |