Astron. Astrophys. 328, 670-681 (1997)
Appendix
The most popular canonical example (see e.g. Farge, 1992) is a
frequency doubling in a harmonic signal. Here, we present the Morlet
wavelet transform of a harmonic (11-y period) signal with a relatively
small frequency change ( ) at
(Figs. 12 and
13).
We also examine the Morlet wavelet transform
for a harmonic (11-y period) signal exhibiting a 1-y phase shift
( ) (Figs. 14 and
(15).
![[FIGURE]](img55.gif) |
Fig. 12. Canonical example of a Morlet wavelet transform: the sinusoidal period increases from 11 to 12 years. Modulus
|
![[FIGURE]](img77.gif) |
Fig. 13. Canonical example of a Morlet wavelet transform: the sinusoidal period increases from 11 to 12 years. Phase
|
![[FIGURE]](img75.gif) |
Fig. 14. Canonical example of a Morlet wavelet transform: the sinusoidal phase is shifted by . Modulus
|
![[FIGURE]](img79.gif) |
Fig. 15. Canonical example of a Morlet wavelet transform: the sinusoidal phase is shifted by . Phase.
|
The third canonical example aims at illustrating Maunder
minimum-type events. For that, we examine the modulus of a periodic
signal that contains a gap of two oscillations (Figs. 16 and
17).
![[FIGURE]](img81.gif) |
Fig. 16. Morlet wavelet transform for an artificial example: modulus of sinusoidal with a gap of two oscillations; modulus of wavelet coefficients.
|
![[FIGURE]](img83.gif) |
Fig. 17. Morlet wavelet transform for an artificial example: a sinusoidal with a gap of two oscillations; phase.
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© European Southern Observatory (ESO) 1997
Online publication: March 26, 1998
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