Variations of electron density based on long‐term incoherent scatter radar and ionosonde measurements over Millstone Hill

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Observations and simulations of the ionospheric and thermospheric response to the December 2006 geomagnetic storm : Initial phase (2007, background): “For a given NO+, @NOþ @z in the topside ionosphere can be considered as the inverse of the effective vertical scale height [Lei et al., 2005; Liu et al., 2007].”
Comparison of COSMIC ionospheric measurements with ground-based observations and model predictions : Preliminary results (2007, methodology): “A least-squares fitting of the RO electron density profile at the F2 layer to a two-layer Chapman function [ Lei et al., 2004, 2005 ] is performed:”
Automated GPS processing for global total electron content data (2006, methodology): “The Madrigal database has been an invaluable tool for many long-term scientific studies using incoherent scatter data ( Lei et al. 2004, 2005; Zhang et al. 2004, 2005).”
Solar activity variations of nighttime ionospheric peak electron density (2006, background): “Previous works about the solar activity dependence of the ionosphere mainly pay attention to the daytime ionosphere, which show complicated solar activity variations of the ionosphere [e.g., Adler et al., 1997; Balan et al., 1994a, 1994b, 1996; Bilitza et al., 2007; Gupta and Singh, 2001; Huang and ”