Reference : The auroral and ionospheric flow signatures of dual lobe reconnection
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Earth sciences & physical geography
Physical, chemical, mathematical & earth Sciences : Multidisciplinary, general & others
http://hdl.handle.net/2268/61239
The auroral and ionospheric flow signatures of dual lobe reconnection
English
Imber, S. M. [> > > >]
Milan, S. E. [> > > >]
Hubert, Benoît mailto [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP) >]
2006
Annales Geophysicae
European Geosciences Union
24
11
3115-3129
Yes (verified by ORBi)
International
0992-7689
Katlenburg-Lindau
[en] magnetospheric physics (magnetospherie configuration and dynamics ; plasma convection ; solar windmagnetosphere interactions)
[en] We present the first substantial evidence for the occurrence of dual lobe reconnection from ionospheric flows and auroral signatures. The process of dual lobe reconnection refers to an interplanetary magnetic field line reconnecting with lobe field lines in both the northern and southern hemispheres. Two bursts of sunward plasma flow across the noon portion of the open/closed field line boundary (OCB), indicating magnetic flux closure at the dayside, were observed in SuperDARN radar data during a period of strongly northward IMF. The OCB is identified from spacecraft, radar backscatter, and auroral observations. In order for dual lobe reconnection to take place, we estimate that the interplanetary magnetic field clock angle must be within +/- 10 degrees of zero (North). The total flux crossing the OCB during each burst is small (1.8% and 0.6% of the flux contained within the polar cap for the two flows). A brightening of the noon portion of the northern auroral oval was observed as the clock angle passed through zero, and is thought to be due to enhanced precipitating particle fluxes due to the occurrence of reconnection at two locations along the field line. The number of solar wind protons captured by the flux closure process was estimated to be similar to 2.5 x 10(30) (4 tonnes by mass), sufficient to populate the cold, dense plasma sheet observed following this interval.
Researchers ; Professionals
http://hdl.handle.net/2268/61239
10.1029/2001JA011400

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