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Magnetic island formation between large-scale flow vortices at an undulating postnoon magnetopause for northward interplanetary magnetic field
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2009 (English)In: Journal of Geophysical Research, ISSN 0148-0227, Vol. 114, no 2, A00C17- p.Article in journal (Refereed) Published
Abstract [en]

Time History of Events and Macroscale Interactions during Substorms multispacecraft observations are presented for a similar to 2-h-long postnoon magnetopause event on 8 June 2007 that for the first time indicate that the trailing (sunward) edges of Kelvin-Helmholtz (KH) waves are commonly related to small-scale < 0.56 R-E magnetic islands or flux transfer events (FTE) during the growth phase of these surface waves. The FTEs typically show a characteristic bipolar B-N structure with enhanced total pressure at their center. Most of the small-scale FTEs are not related to any major plasma acceleration. TH-A observations of one small FTE at a transition from the low-latitude boundary layer (LLBL) into a magnetosheath plasma depletion layer were reconstructed using separate techniques that together confirm the presence of a magnetic island within the LLBL adjacent to the magnetopause. The island was associated with a small plasma vortex and both features appeared between two large-scale (similar to 1 R-E long and 2000 km wide) plasma vortices. We propose that the observed magnetic islands may have been generated from a time-varying reconnection process in a low ion plasma beta (beta(i) < 0.2) and low 8.3 degrees field shear environment at the sunward edge of the growing KH waves where the local magnetopause current sheet may be compressed by the converging flow of the large-scale plasma vortices as suggested by numerical simulations of the KH instability.

Place, publisher, year, edition, pages
2009. Vol. 114, no 2, A00C17- p.
National Category
Physical Sciences
URN: urn:nbn:se:uu:diva-148776DOI: 10.1029/2008JA013505ISI: 000263615000007OAI: oai:DiVA.org:uu-148776DiVA: diva2:402974
Available from: 2011-03-10 Created: 2011-03-10 Last updated: 2011-03-10Bibliographically approved

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Swedish Institute of Space Physics, Uppsala Division
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