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All Figures

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f1.eps}\end{figure}$ Figure 1: Temporal variation in rotational kinetic energy throughout the convection zone. The continuous lines join values of the total kinetic energy (in units of the temporal mean) in the convection zone at different epochs; the dashed and dotted lines respectively join corresponding contributions from the low-latitude ( $\le$ $\pi /4$ ) and high-latitude ( $\ge$ $\pi /4$ ) regions. For clarity, only a few representative error bars are shown. The values in the upper panel were obtained from the MDI data, the values in the lower panel from the GONG data.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f2.eps}\end{figure}$ Figure 2: Relative variation with time of the rotational kinetic energy in different regions (indicated in each panel) of the Sun, obtained from the GONG data. The continuous lines indicate the variation over entire spherical shells, and the dashed and dotted lines respectively indicate the variation in the low- ( $\le$ $\pi /4$ ) and high-latitude ( $\ge$ $\pi /4$ ) regions. For clarity, only a few representative error bars are shown. The lowest panel depicts the variation in solar activity as measured by the 10.7 cm radio flux over the same time interval.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f3.eps}\end{figure}$ Figure 3: Correlation coefficients between the temporal variation in kinetic energy of rotation obtained using GONG data and the 10.7 cm radio flux, plotted as a function of radius. The continuous curve is the coefficient for an entire spherical shell; the dashed and dotted curves are respectively the correlation coefficients for the low-latitude ( $\le$ $\pi /4$ ) and high-latitude ( $\ge$ $\pi /4$ ) regions.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f4.eps}\end{figure}$ Figure 4: Amplitude of relative variation in rotational kinetic energy, plotted against radius, obtained by fitting a sinusoid with a period of 11 years to the inferences from GONG data. The continuous curve represents the entire spherical shell, the dashed and dotted curves respectively represent the low- ( $\le$ $\pi /4$ ) and high- ( $\ge$ $\pi /4$ ) latitude regions.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f5.eps}\end{figure}$ Figure 5: Correlation coefficient between the the 10.7 cm radio flux and the kinetic energy and angular momentum, integrated over entire spherical shells, plotted against radius. The solid and long-dashed curves are kinetic energy and angular momentum inferred from GONG data, the dotted and short-dashed curves are from MDI data.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f6.eps}\end{figure}$ Figure 6: Power spectrum of temporal variation in rotational kinetic energy in different depth ranges (as marked in each panel). The solid lines represent the entire spherical shell, the dashed and dotted lines represent the low- ( $\le$ $\pi /4$ ) and high- ( $\ge$ $\pi /4$ ) latitude regions, respectively. The seismic data were obtained from GONG; the results from MDI are similar, and have been omitted for concision.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f7.eps}\end{figure}$ Figure 7: Temporal variation in rotational kinetic energy and angular momentum in the low-latitude region with $0.70~R_\odot\le r\le0.74~R_\odot$ . The continuous lines are the result of using GONG data, the dotted lines are from using MDI data. For clarity, only a few representative error bars are shown.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f8.eps}\end{figure}$ Figure 8: Temporal variation in (even) multipole moments J₂ - J₁₂. The solid lines are the results from using GONG data, dashed lines from using MDI data. In all cases a sinusoidal fit, with a period of 11 years, is also shown.
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In the text

$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f4.eps}\end{figure}$	Figure 4: Amplitude of relative variation in rotational kinetic energy, plotted against radius, obtained by fitting a sinusoid with a period of 11 years to the inferences from GONG data. The continuous curve represents the entire spherical shell, the dashed and dotted curves respectively represent the low- ( $\le$ $\pi /4$ ) and high- ( $\ge$ $\pi /4$ ) latitude regions.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f5.eps}\end{figure}$	Figure 5: Correlation coefficient between the the 10.7 cm radio flux and the kinetic energy and angular momentum, integrated over entire spherical shells, plotted against radius. The solid and long-dashed curves are kinetic energy and angular momentum inferred from GONG data, the dotted and short-dashed curves are from MDI data.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f7.eps}\end{figure}$	Figure 7: Temporal variation in rotational kinetic energy and angular momentum in the low-latitude region with $0.70~R_\odot\le r\le0.74~R_\odot$ . The continuous lines are the result of using GONG data, the dotted lines are from using MDI data. For clarity, only a few representative error bars are shown.
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$\begin{figure} \par\includegraphics[width=8.2cm,clip]{8209f8.eps}\end{figure}$	Figure 8: Temporal variation in (even) multipole moments J₂ - J₁₂. The solid lines are the results from using GONG data, dashed lines from using MDI data. In all cases a sinusoidal fit, with a period of 11 years, is also shown.
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