The VLF model suggests that there is a good chance of detecting a radio 'afterglow' as a rise in VLF recorded voltage when solar plasma crosses the F, E and D layers. A description of the magnetosphere of the earth by T. Phan suggests that the solar plasma enter the polar region through a perpendicular jet. Figure 4 shows how ions might enter the ionosphere. Three-dimensional cutaway view of the magnetosphere. These values are normalized to give a ratio for kT .
Units are in centimeters per steradians per second.
All quantum values are measured in the same units and expressed as coupled non-linear equations dependent on the voltage as detected from the VLF teles cope. Results of these three equations represent the EUV emissions of the halo regions in the Virgo and Coma Galaxy Clusters. 1997 Measurements of the cosmic ray positron fraction with the HEAT spectrometer , unplished. Challenges to Relativistic Astrophysics, Proc. The VLF readings were in excess of 5 volts.