Profiles of ionospheric storm‐enhanced density during the 17 March 2015 great storm

• Published in: Journal of geophysical research. Space physics 2016-01, Vol.121 (1), p.727-744
• Main Authors: Liu, Jing, Wang, Wenbin, Burns, Alan, Yue, Xinan, Zhang, Shunrong, Zhang, Yongliang, Huang, Chaosong
• Format: Article
• Language: English
• Subjects: Conduction heating; Conductive heat transfer; Correlation; Daytime; Density; Depletion; Dipping; Electron density; Electron density profiles; Electron temperature; Electron temperatures; Electrons; F 2 region; Geophysics; Heat; Ionosphere; Ionospheric electron density; Ionospheric electron density profiles; Ionospheric electrons; ionospheric storm‐enhanced density; Ionospherics; Plasmasphere; Scale height; Storm effects; Storms; Total Electron Content; Trapping
• ISSN: 2169-9380; 2169-9402
• DOI: 10.1002/2015JA021832

Ionospheric F2 region peak densities (NmF2) are expected to have a positive correlation with total electron content (TEC), and electron densities usually show an anticorrelation with electron temperatures near the ionospheric F2 peak. However, during the 17 March 2015 great storm, the observed TEC, NmF2, and electron temperatures of the storm‐enhanced density (SED) over Millstone Hill (42.6°N, 71.5°W, 72° dip angle) show a quiet different picture. Compared with the quiet time ionosphere, TEC, the F2 region electron density peak height (hmF2), and electron temperatures above ~220 km increased, but NmF2 decreased significantly within the SED. This SED occurred where there was a negative ionospheric storm effect near the F2 peak and below it, but a positive storm effect in the topside ionosphere. Thus, this SED event was a SED in TEC but not in NmF2. The very low ionospheric densities below the F2 peak resulted in a much reduced downward heat conduction for the electrons, trapping the heat in the topside in the presence of heat source above. This, in turn, increased the topside scale height so that even though electron densities at the F2 peak were depleted, TEC increased in the SED. The depletion in NmF2 was probably caused by an increase in the density of the molecular neutrals, resulting in enhanced recombination. In addition, the storm time topside ionospheric electron density profiles were much closer to diffusive equilibrium than the nonstorm time profiles, indicating less daytime plasma flow between the ionosphere and the plasmasphere. Key Points A SED in TEC but not in NmF2 Storm time topside ionospheric electron density profiles were in diffusive equilibrium Increase in the topside but decrease in bottom side ionosphere