Mathematics
Scientific paper
Jun 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jgr....98.9249k&link_type=abstract
Journal of Geophysical Research (ISSN 0148-0227), vol. 98, no. A6, p. 9249-9258.
Mathematics
32
Geomagnetic Tail, Geomagnetism, Magnetic Field Configurations, Plasma Layers, Plasma Pressure, Magnetic Storms, Pressure Distribution, Superposition (Mathematics)
Scientific paper
Using data from 41 substorm events in the near-Earth magnetotail, we have combined plasma, energetic ion, and magnetic field data from the AMPTE/IRM spacecraft to perform a superposed epoch analysis of changes in the total pressure and in the magnetic field configuration as a function of time relative to substorm onset. Unloading is evident in the total pressure profile; the pressure decreases by about 20 percent. Pressure changes during the growth phase are not as uniform for the different substorms as the pressure changes during the expansion phase. To study changes in the magnetic field configuration, we have determined the development of the plasma pressure profiles in z for an average of data from 15 to 19 R(E). At substorm onset, the field line dipolarization begins on the innermost field lines and then progresses to the outer field lines. The field lines map the closest to the Earth about 45 min after substorm onset, and then begin to stretch out again during the recovery phase of the substorm.
Baumjohann Wolfgang
Kistler Lynn M.
Möbius Eberhard
Nagai Takaya
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