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How much flux does a flux transfer event transfer?

How much flux does a flux transfer event transfer?
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 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 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 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.
2169-9380
12,310-12,327
Fear, R.C.
8755b9ed-c7dc-4cbb-ac9b-56235a0431ab
Trenchi, L.
565a6c2f-9b87-4a3a-a453-ff7cfecbb266
Coxon, J.C.
566baea5-6a30-4855-bde3-a09c115efde4
Milan, S. E.
4495fdee-b600-43e5-99f7-6193a849b7f5
Fear, R.C.
8755b9ed-c7dc-4cbb-ac9b-56235a0431ab
Trenchi, L.
565a6c2f-9b87-4a3a-a453-ff7cfecbb266
Coxon, J.C.
566baea5-6a30-4855-bde3-a09c115efde4
Milan, S. E.
4495fdee-b600-43e5-99f7-6193a849b7f5

Fear, R.C., Trenchi, L., Coxon, J.C. and Milan, S. E. (2017) How much flux does a flux transfer event transfer? Journal of Geophysical Research: Space Physics, 122, 12,310-12,327. (doi:10.1002/2017JA024730).

Record type: Article

Abstract

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 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 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.

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Accepted/In Press date: 15 November 2017
e-pub ahead of print date: 26 December 2017

Identifiers

Local EPrints ID: 416736
URI: https://eprints.soton.ac.uk/id/eprint/416736
ISSN: 2169-9380
PURE UUID: 54ba979e-4826-4275-bc99-06fda09f7b28
ORCID for R.C. Fear: ORCID iD orcid.org/0000-0003-0589-7147
ORCID for J.C. Coxon: ORCID iD orcid.org/0000-0002-0166-6854

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Date deposited: 05 Jan 2018 17:30
Last modified: 03 Dec 2019 01:35

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Contributors

Author: R.C. Fear ORCID iD
Author: L. Trenchi
Author: J.C. Coxon ORCID iD
Author: S. E. Milan

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