Line-widths, line-bottom intensities, and wavelength shifts of reconstructed profiles for the strong (solid curves) and weak lines (dashed) at eight successive positions during the planetary transit, obtained from Gaussian fits to the data. The error bars denote one standard deviation to these fits but judgments of any apparent dependences should also examine the reconstructed profiles to which these fits were made. The various transit epochs, with their center-to-limb locations shown at bottom, correspond to those in Fig. 1.