Table 6: Slopes of the linear fits to the logarithm of the PWTs of the solar series for 480 days of data.
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) $-0.165 \pm 0.012$ $-1.291 \pm 0.017$

B (Min) $-0.129 \pm 0.014$ $-1.278 \pm 0.013$

G (Max) $-0.163 \pm 0.012$ $-1.290 \pm 0.016$

G (Min) $-0.124 \pm 0.015$ $-1.277 \pm 0.014$

R (Max) $-0.188 \pm 0.013$ $-1.319 \pm 0.059$

R (Min) $-0.152 \pm 0.015$ $-1.306 \pm 0.022$

**Table 6:** Slopes of the linear fits to the logarithm of the PWTs of the solar series for 480 days of data.
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)	$-0.165 \pm 0.012$	$-1.291 \pm 0.017$
B (Min)	$-0.129 \pm 0.014$	$-1.278 \pm 0.013$
G (Max)	$-0.163 \pm 0.012$	$-1.290 \pm 0.016$
G (Min)	$-0.124 \pm 0.015$	$-1.277 \pm 0.014$
R (Max)	$-0.188 \pm 0.013$	$-1.319 \pm 0.059$
R (Min)	$-0.152 \pm 0.015$	$-1.306 \pm 0.022$

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