All Figures

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{4502f1.eps} \end{figure}$ Figure 1: Stokes V ripple wavelet power spectrum, obtained using the spectrum of $\alpha$ Lyr. Note the evident power at scales 0.015-0.022 pixel $^{\rm -1}$ due to polarimetric ripples.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8cm,clip]{4502f2a.eps}\par\vspace{0.25cm} \includegraphics[width=8cm,clip]{4502f2b.eps} \end{figure}$ Figure 2: Ripple removal from spectra of $\alpha$ And using Vega as a template. Lower frame - Vega, upper frame - $\alpha$ And. In both frames, raw and corrected Stokes V, as well as the fringe pattern, have been scaled and shifted for display purposes.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{4502f3.eps} \end{figure}$ Figure 3: Example MuSiCoS (9 Jul. 03) and ESPaDOnS (21 Feb. 05) LSD profiles. Note the residual ripples in the MuSiCoS Stokes V profile, which extend well outside the range of the Stokes I profile.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{4502f4.eps} \end{figure}$ Figure 4: Longitudinal magnetic field measurements (epoch 3) as a function of rotational phase.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=8.3cm,clip]{4502f5a.eps}\par... ...e{2mm} \includegraphics[angle=-90,width=8.3cm,clip]{4502f5b.eps} \end{figure}$ Figure 5: Reduced $\chi ^2$ of the Stokes V model/data comparison for dipole fields, as a function of the polar field strength $B_{\rm p}$ and the obliquity between the rotational axis and the magnetic field symmetry axis $\beta$ . A rotational axis inclination of $i=74^\circ$ has been assumed for all models. Dark regions correspond to models consistent with the observations, while white regions correspond to models incompatible with the observations at more than 99% confidence. Upper frame - ESPaDOnS data ( $\phi _0=0.00$ ). Lower frame - MuSiCoS data ( $\phi _0=0.00$ ).
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{4502f6a.eps}\hspace*{4mm}\includegraphics[angle=-90,width=7.5cm,clip]{4502f6b.eps} \end{figure}$ Figure 6: Variability of Hg II 3984 and Hg II 5677 in ESPaDOnS spectra of $\alpha$ And.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=7.5cm,clip]{4502f1.eps} \end{figure}$	Figure 1: Stokes V ripple wavelet power spectrum, obtained using the spectrum of $\alpha$ Lyr. Note the evident power at scales 0.015-0.022 pixel $^{\rm -1}$ due to polarimetric ripples.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8cm,clip]{4502f2a.eps}\par\vspace{0.25cm} \includegraphics[width=8cm,clip]{4502f2b.eps} \end{figure}$	Figure 2: Ripple removal from spectra of $\alpha$ And using Vega as a template. Lower frame - Vega, upper frame - $\alpha$ And. In both frames, raw and corrected Stokes V, as well as the fringe pattern, have been scaled and shifted for display purposes.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{4502f3.eps} \end{figure}$	Figure 3: Example MuSiCoS (9 Jul. 03) and ESPaDOnS (21 Feb. 05) LSD profiles. Note the residual ripples in the MuSiCoS Stokes V profile, which extend well outside the range of the Stokes I profile.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{4502f4.eps} \end{figure}$	Figure 4: Longitudinal magnetic field measurements (epoch 3) as a function of rotational phase.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{4502f6a.eps}\hspace*{4mm}\includegraphics[angle=-90,width=7.5cm,clip]{4502f6b.eps} \end{figure}$	Figure 6: Variability of Hg II 3984 and Hg II 5677 in ESPaDOnS spectra of $\alpha$ And.
Open with DEXTER