October 1995 Storm Event:
On October 18, 1995, an interplanetary magnetic cloud encountered the Earth and consequently induced a major magnetic storm as well as massive substorms (with the maximum magnitude of Dst reaching 120 nT and AE reaching 1600 nT). The realistic time-dependent high-latitude ionospheric convection and auroral precipitation patterns derived from the AMIE procedure was used as inputs to the NCAR-TIEGCM to simulate the ionospheric/thermospheric response to the storm. The TIEGCM ran in a 5-min time step, and the TIEGCM history volumes were recorded every 10 mins. For the period of October 18-19, 1995, the 2-day average solar radiation index Sa was 80x10^-22 W/m^2Hz.

Modeled difference in total electron content (TEC) with respect to quiet-day background for October 18, 1995, in the northern hemisphere. The color scale is in TEC units (or 10^16 electrons/m^2).

Modeled difference in total electron content (TEC) with respect to quiet-day background for October 18, 1995, in the southern hemisphere. The color scale is in TEC units (or 10^16 electrons/m^2).

Modeled difference in total electron content (TEC) with respect to quiet-day background for October 19, 1995, in the northern hemisphere. The color scale is in TEC units (or 10^16 electrons/m^2).

Modeled difference in total electron content (TEC) with respect to quiet-day background for October 19, 1995, in the southern hemisphere. The color scale is in TEC units (or 10^16 electrons/m^2).

Modeled difference in total electron content (TEC) with respect to quiet-day background for October 18-19, 1995. Global cylindrical equidistant map projection. The color scale is in TEC units (or 10^16 electrons/m^2).
Tiegcm runs by Gang Lu: ganglu@ucar.edu.
Web page by Ben Foster: foster@ucar.edu.