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Detailed Reference Information |
Frank, L.A., Paterson, W.R., Ackerson, K.L., Kokubun, S., Yamamoto, T., Fairfield, D.H. and Lepping, R.P. (1994). Observations of plasmas associated with the magnetic signature of a plasmoid in the distant magnetotail. Geophysical Research Letters 21: doi: 10.1029/94GL01604. issn: 0094-8276. |
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The three-dimensional electron and positive ion velocity distributions were examined for four events for which the magnetic signature of plasmoids occurred at the Geotail spacecraft position in Earth's distant magnetotail. The proton bulk parameters and the electron velocity distributions for one of the events are presented in order to characterize the qualitative character of the set of events. The north-to-south turnings of the magnetic field that were taken for evidence of the passage of a plasmoid were often accompanied by a significant strong core of By that was centered on the transition of Bz from north to south. The magnetic signatures thus appeared to be more indicative of flux ropes than of classical plasmoids with weak core fields. The proton and electron bulk velocities in these magnetic structures are not equal, a situation that provides an earthward current. The plasma &bgr; was typically one or greater. Counterstreaming of low-energy electrons was often found on the magnetic field lines around the central magnetic core and suggested the existence of a closed field line topology in these regions. These events appeared to be the tailward flowing debris from acceleration processes occurring in the vicinity of a separator positioned nearer to Earth. ¿American Geophysical Union 1994 |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Magnetospheric Physics, Magnetotail, Magnetospheric Physics, Magnetotail boundary layers, Magnetospheric Physics, Plasma convection, Magnetospheric Physics, Plasma sheet |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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