Table 7: Slopes of the linear fits to the logarithm of the PWTs of the solar series for 54 days of data analysed as the stellar data, including its observed window function.
Filters and Slope from $1.0 \times 10^{-4}$ Slope from $0.7 \times 10^{-3}$

activity to $0.6 \times 10^{-3}$ Hz to $2.5 \times 10^{-3}$ Hz

B (Max) $-0.117 \pm0.061$ $-1.155 \pm 0.037$

B (Min) $-0.063 \pm0.039$ $-1.221 \pm 0.040$

G (Max) $-0.137 \pm0.069$ $-1.166 \pm 0.034$

G (Min) $-0.019 \pm0.042$ $-1.217 \pm 0.038$

R (Max) $-0.131 \pm0.071$ $-1.191 \pm 0.025$

R (Min) $-0.084 \pm0.050$ $-1.231 \pm 0.030$

**Table 7:** Slopes of the linear fits to the logarithm of the PWTs of the solar series for 54 days of data analysed as the stellar data, including its observed window function.
Filters and	Slope from $1.0 \times 10^{-4}$	Slope from $0.7 \times 10^{-3}$
activity	to $0.6 \times 10^{-3}$ Hz	to $2.5 \times 10^{-3}$ Hz
B (Max)	$-0.117 \pm0.061$	$-1.155 \pm 0.037$
B (Min)	$-0.063 \pm0.039$	$-1.221 \pm 0.040$
G (Max)	$-0.137 \pm0.069$	$-1.166 \pm 0.034$
G (Min)	$-0.019 \pm0.042$	$-1.217 \pm 0.038$
R (Max)	$-0.131 \pm0.071$	$-1.191 \pm 0.025$
R (Min)	$-0.084 \pm0.050$	$-1.231 \pm 0.030$

Source LaTeX | All tables | In the text

	1 Introduction
	2 Stellar data analysis
	3 Stellar acoustic Power Wavelet Transforms
	4 Analysis of a G type star: the Sun
	5 Discussion and conclusions
	References