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On the profile of intense high-altitude auroral electric fields at magnetospheric boundaries
KTH, Skolan för elektro- och systemteknik (EES), Rymd- och plasmafysik.
KTH, Skolan för elektro- och systemteknik (EES), Rymd- och plasmafysik.ORCID-id: 0000-0002-1594-1861
KTH, Skolan för elektro- och systemteknik (EES), Rymd- och plasmafysik.ORCID-id: 0000-0003-1270-1616
KTH, Skolan för elektro- och systemteknik (EES), Rymd- och plasmafysik.
Visa övriga samt affilieringar
2006 (Engelska)Ingår i: Annales Geophysicae, ISSN 0992-7689, E-ISSN 1432-0576, Vol. 24, nr 6, s. 1713-1723Artikel i tidskrift (Refereegranskat) Published
Abstract [en]

The profile of intense high-altitude electric fields on auroral field lines has been studied using Cluster data. A total of 41 events with mapped electric field magnitudes in the range between 0.5-1 V/m were examined, 27 of which were co-located with a plasma boundary, defined by gradients in particle flux, plasma density and plasma temperature. Monopolar electric field profiles were observed in 11 and bipolar electric field profiles in 16 of these boundary-associated electric field events. Of the monopolar fields, all but one occurred at the polar cap boundary in the late evening and midnight sectors, and the electric fields were typically directed equatorward, whereas the bipolar fields all occurred at plasma boundaries clearly within the plasma sheet. These results support the prediction by Marklund et al. (2004), that the electric field profile depends on whether plasma populations, able to support intense field-aligned currents and closure by Pedersen currents, exist on both sides, or one side only, of the boundary.

Ort, förlag, år, upplaga, sidor
2006. Vol. 24, nr 6, s. 1713-1723
Nyckelord [en]
aurora; boundary layer; electric field; magnetosphere; plasma
Nationell ämneskategori
Fusion, plasma och rymdfysik
Identifikatorer
URN: urn:nbn:se:kth:diva-7558DOI: 10.5194/angeo-24-1713-2006ISI: 000239724500020Scopus ID: 2-s2.0-33751071835OAI: oai:DiVA.org:kth-7558DiVA, id: diva2:12621
Anmärkning
QC 20100730Tillgänglig från: 2007-10-22 Skapad: 2007-10-22 Senast uppdaterad: 2017-12-14Bibliografiskt granskad
Ingår i avhandling
1. Investigations of auroral electric fields and currents
Öppna denna publikation i ny flik eller fönster >>Investigations of auroral electric fields and currents
2007 (Engelska)Doktorsavhandling, sammanläggning (Övrigt vetenskapligt)
Abstract [en]

The Cluster spacecraft have been used to investigate auroral electric fields and field-aligned currents (FACs) at geocentric distances between 4 and 7 Re. The electric fields have been measured by the EFW instrument, consisting of two pairs of spherical probes, and the FACs have been calculated from measurements of the magnetic field by the FGM fluxgate magnetometer. CIS ion and PEACE electron measurements have also been used. Event studies as well as statistical studies have been used to determine the characteristics of the auroral electric fields. In two events where regions of both spatial and temporal electric field variations could be identified, the quasi-static electric fields were, compared to the Alfvén waves, found to be more intense and contribute more to the downward Poynting flux. With the use of the four Cluster spacecraft, the quasi-static electric field structures were found to be relatively stable on the time scale of at least half a minute. Quasi-static electric fields were found throughout the altitude range covered by Cluster in the auroral region. The electric field structures were found both in the upward and downward current regions. Bipolar and monopolar electric fields, corresponding to U- and S-shaped potential structures, have been found at different plasma boundaries, consistent with the view that the plasma conditions and the geometry of the current system are related to the shape of the electric field. The type of the bipolar electric field structures (convergent or divergent) was further found to be consistent with the FAC direction. The typical scale sizes of the electric field structures have been determined to be between 4 and 5 km, when mapped to ionospheric altitude. The most intense FACs associated with intense electric fields were found for small FAC widths. The widths of upward and downward FACs were similar.

Ort, förlag, år, upplaga, sidor
Stockholm: KTH, 2007. s. vii, 48
Serie
Trita-EE, ISSN 1653-5146 ; 2007:056
Nyckelord
auroral physics, auroral electric fields, auroral potential structures, auroral particle acceleration
Nationell ämneskategori
Fusion, plasma och rymdfysik
Identifikatorer
urn:nbn:se:kth:diva-4512 (URN)978-91-7178-761-3 (ISBN)
Disputation
2007-11-09, F3, Lindstedsvägen 26, Stockholm, 10:00
Opponent
Handledare
Anmärkning
QC 20100730Tillgänglig från: 2007-10-22 Skapad: 2007-10-22 Senast uppdaterad: 2010-07-30Bibliografiskt granskad

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Marklund, GöranKarlsson, TomasLindqvist, Per-Arne

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