Global thermospheric neutral density and wind response to the severe 2003 geomagnetic storms from CHAMP accelerometer data

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Rotating solar coronal holes and periodic modulation of the upper atmosphere (2008, methodology): “[4] The satellite drag data that we present are in the form of thermosphere densities, obtained from accelerometer measurements of non-gravitational accelerations on the Challenging Minisatellite Payload (CHAMP) satellite [Reigber et al., 2002] using standard methods [Sutton et al., 2005, 2007].”
Thermospheric Density and Wind Determination from Satellite Dynamics (2012, background): “, Jacchia and Slowey [35] led to the development of the first thermosphere models by Harris and Priester [30] and Jacchia [33].”
Thermosphere density response to the 20-21 November 2003 solar and geomagnetic storm from CHAMP and GRACE accelerometer data (2006, methodology): “The global thermosphere density response to the intense storms of 29 October to 1 November 2003, as revealed by CHAMP measurements, were presented by Liu and L}hr [2005] and Sutton et al. [2005] .”