HR: 08:45h
AN: SM41B-04    [Abstracts]
TI: Measures of Geo-effectiveness in Storms
AU: * Mitchell, E J
EM: mitchell@uta.edu
AF: Department of Physics, University of Texas at Arlington, Arlington, TX 76019, United States
AU: Lopez, R
EM: relopez@uta.edu
AF: Department of Physics, University of Texas at Arlington, Arlington, TX 76019, United States
AB: Geomagnetic storms are produced by solar wind disturbances causing large currents to flow throughout the magnetosphere. These currents are the magnetosphere's response to the solar wind electric field and the rate of the interplanetary magnetic field's reconnection with the magnetosphere. To gauge the geo-effectiveness of a storm, or the magnetosphere's response to the storm, we consider the ratio of the ring current injection rate (RCIR) to measures of the solar wind input. Burton et al. [1975] called this parameter α, using VB_s as the solar wind input. We calculate three versions of α: α₁ is the Burton et al. [1975] parameter, α₂ is the ratio of the RCIR to the Newell et al. [2007] universal coupling function, α₃ is the ratio of the RCIR to a measure of the dayside reconnection rate recently proposed by Borovsky. Using each of these values of α, we rank 100 storms with Dst < -75 nT, between 1995 and 2005. The top 10% and lowest 10% of storms are examined in detail to determine what characteristics they might have in common.
DE: 2784 Solar wind/magnetosphere interactions
DE: 2788 Magnetic storms and substorms (7954)
SC: SPA-Magnetospheric Physics [SM]
MN: 2007 Fall Meeting