Solar Wind Data
Solar Wind data has been propagated to the front of the magnetosphere (courtesy Dr. James Weygand) using the pseudo-minimum variance technique of Dan Weimer et al. [2003; 2004]. Data are included in both line plots and polar plots. ASCII data can be downloaded through the Line Plots page by making a plot for time interval of interest.
References:
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Weimer, D.R., D.M. Ober, N.C. Maynard, M.R. Collier, D.J. McComas, N.F. Ness, C.W. Smith, and J. Watermann, Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique, J. Geophys. Res., 108, 10.1029/2002JA009405, 2003.
- Weimer, D. R. (2004), Correction to ''Predicting interplanetary magnetic field (IMF) propagation delay times using the minimum variance technique,'' J. Geophys. Res., 109, A12104, doi:10.1029/2004JA010691.
