Using 180° field-of-view (full-sky) imaging polarimetry, we measured the spatiotemporal change of the polarization of skylight during the total solar eclipse on 29 March 2006 in Turkey. We present our observations here on the temporal variation of the celestial patterns of the degree p and angle α of linear polarization of the eclipsed sky measured in the red \left(650\text{\hspace{0.17em} nm}\right) , green \left(550\text{\hspace{0.17em} nm}\right) , and blue \left(450\text{\hspace{0.17em} nm}\right) parts of the spectrum. We also report on the temporal and spectral change of the positions of neutral (unpolarized, p=0 ) points, and points with local minima or maxima of p of the eclipsed sky. Our results are compared with the observations performed by the same polarimetric technique during the total solar eclipse on 11 August 1999 in Hungary. Practically the same characteristics of celestial polarization were encountered during both eclipses. This shows that the observed polarization phenomena of the eclipsed sky may be general.