Dependence of the large-scale, inner magnetospheric electric field on geomagnetic activity

Measurements made with the University of California, Berkeley/Air Force Geophysics Laboratory electric field instrument on the CRRES spacecraft are examined to determine the average structure of the inner magnetospheric electric field for different geomagnetic activity levels. Data were gathered between L=2.5 and L=8.5 over the period from January to October 1991 in the local time sector between 1200 and 0400 magnetic local time. The average dawn-dusk component of the electric field was nearly always duskward, scaling in magnitude from 0.05 mV/m to 1.5 mV/m as Kp increased from 0 to 9-. The data indicate that the electric field is shielded out of the inner magnetosphere, with the shielding distance starting at about L=5.0 for Kp=1 and moving 0.5 RE earthward for every unit increase in Kp. There is evidence that the electric field penetrates below L=2.5 for Kp ≥ 5. The most interesting aspect of this statistical study is the development for moderate to high Kp of a region of enhanced electric field between L=3.5 and L=6. For moderately active conditions the electric field does not decrease monotonically as one moves earthward. Instead, it increases to a broad local maximum near the position where the ring current is typically observed to be the strongest, falling off earthward of that position. The electric field magnitude can be a factor of 2 or more larger at this location than at higher L values. These results are discussed in the context of large-scale flows and the effects of hot plasma in the inner magnetosphere.

[1]  A. Pedersen,et al.  Solar wind and magnetosphere plasma diagnostics by spacecraft electrostatic potential measurements , 1995 .

[2]  Wolfgang Baumjohann,et al.  Magnetospheric convection observed between 0600 and 2100 LT: solar wind and IMF dependence , 1985 .

[3]  N. Maynard,et al.  The plasmaspheric electric field as measured by ISEE 1 , 1983 .

[4]  W. J. Burke,et al.  Quantitative simulation of a magnetospheric substorm 2. Comparison with observations , 1981 .

[5]  N. Maynard,et al.  Magnetospheric observation of large sub-auroral electric fields , 1980 .

[6]  R. Heelis,et al.  Rapid subauroral ion drifts observed by Atmosphere Explorer C , 1979 .

[7]  H. Volland A model of the magnetospheric electric convection field , 1978 .

[8]  D. Southwood The role of hot plasma in magnetospheric convection , 1977 .

[9]  F. Mozer,et al.  The average auroral zone electric field , 1974 .

[10]  Richard A. Wolf,et al.  Self‐consistent calculation of the motion of a sheet of ions in the magnetosphere , 1973 .

[11]  F. Mozer Analyses of techniques for measuring DC and AC electric fields in the magnetosphere , 1973 .

[12]  F. Mozer,et al.  Electric field mapping in the ionosphere at the equatorial plane , 1970 .

[13]  D. L. Carpenter Relations between the dawn minimum in the equatorial radius of the plasmapause and Dst, Kp , and local K at Byrd Station , 1967 .

[14]  F. Mozer,et al.  CRRES electric field/langmuir probe instrument , 1992 .

[15]  John R Wygant,et al.  Fluxgate magnetometer instrument on the CRRES , 1992 .

[16]  Wolfgang Baumjohann,et al.  Magnetospheric convection observed between 0600 and 2100 LT: Variations with Kp , 1985 .

[17]  V. Vasyliūnas,et al.  Mathematical models of magnetospheric convection and its coupling to the ionosphere , 1970 .