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The evolution of flux pileup regions in the plasma sheet : Cluster observations

Hamrin, Maria (author)
Umeå universitet,Institutionen för fysik
Norqvist, Patrik (author)
Umeå universitet,Institutionen för fysik
Karlsson, Tomas (author)
KTH,Rymd- och plasmafysik
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Nilsson, H. (author)
Fu, H. S. (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Buchert, Stephan (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
André, Mats (author)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Marghitu, O. (author)
Pitkänen, Timo, 1979- (author)
Umeå universitet,Institutionen för fysik
Klecker, B. (author)
Kistler, L. M. (author)
Dandouras, I. (author)
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 (creator_code:org_t)
2013-10-09
2013
English.
In: Journal of Geophysical Research. - : American Geophysical Union (AGU). - 0148-0227 .- 2156-2202 .- 2169-9380 .- 2169-9402. ; 118:10, s. 6279-6290
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • Bursty bulk flows (BBFs) play an important role for the mass, energy, and magnetic flux transport in the plasma sheet, and the flow pattern in and around a BBF has important consequences for the localized energy conversion between the electromagnetic and plasma mechanical energy forms. The plasma flow signature in and around BBFs is often rather complicated. Return flows and plasma vortices are expected to exist at the flanks of the main flow channel, especially near the inner plasma sheet boundary, but also farther down-tail. A dipolarization front (DF) is often observed at the leading edge of a BBF, and a flux pileup region (FPR) behind the DF. Here we present Cluster data of three FPRs associated with vortex flows observed in the midtail plasma sheet on 15 August 2001. According to the principles of Fu et al. (2011, 2012c), two of the FPRs are considered to be in an early stage of evolution (growing FPRs). The third FPR is in a later stage of evolution (decaying FPR). For the first time, the detailed energy conversion properties during various stages of the FPR evolution have been measured. We show that the later stage FPR has a more complex vortex pattern than the two earlier stage FPRs. The two early stage FPR correspond to generators, EJ<0, while the later stage FPR only shows weak generator characteristics and is instead dominated by load signatures at the DF, EJ>0. Moreover, to our knowledge, this is one of the first times BBF-related plasma vortices have been observed to propagate over the spacecraft in the midtail plasma sheet at geocentric distances of about 18R(E). Our observations are compared to recent simulation results and previous observations.

Subject headings

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

dipolarization front
energy conversion
flow vortices
flux pileup region
generator
load

Publication and Content Type

ref (subject category)
art (subject category)

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