@InProceedings{FerreiraDoMeMaCeEcVi:2016:DiCoWa,
author = "Ferreira, Maria Teodora and Domingues, Margarete Oliveira and
Mendes, Odim and Macau, Elbert Einstein Nehrer and Cecatto,
Jos{\'e} Roberto and Echer, Ezequiel and Vieira, Luis Eduardo
Antunes",
affiliation = "{Universidade do Vale do Para{\'{\i}}ba (UNIVAP)} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Instituto Nacional de
Pesquisas Espaciais (INPE)} and {Instituto Nacional de Pesquisas
Espaciais (INPE)} and {Instituto Nacional de Pesquisas Espaciais
(INPE)} and {Instituto Nacional de Pesquisas Espaciais (INPE)} and
{Instituto Nacional de Pesquisas Espaciais (INPE)}",
title = "Discrete complex wavelet approach applied to phase synchronization
on solar parameters",
year = "2016",
organization = "International Conference on Nonlinear Science and Complexity, 6.",
keywords = "Analysis and Control of Nonlinear Dynamical Systems with Practical
Applications, Fluidodynamics, Plasma and Turbulence,
Synchronization in Nonlinear Systems, Phase Synchronization, Solar
Parameters.",
abstract = "In general for the space science, and in particular for the solar
physics, the development of new nonlinear analysis methods is
always interesting and a promising initiative, because most of the
time dynamical aspects may be unraveled from the physical records.
Much effort has been done to survey the dynamical behavior of the
Sun described by physical parameters connected to complex
non-linear mechanisms responsible for the energy release on the
solar atmosphere. Discrete Complex Wavelet Approach (DCWA) is
based on the phase assignment from complex wavelet coefficients
obtained by using a dual-tree complex wavelet transform. Can DCWA
be validate for phase assignment, and subsequently in the
calculation of phase difference of solar parameters? For
validation tests, two time series of important solar parameters
are chosen: (1) the daily sunspot number, and (2) the daily total
radio flux at 10.7cm, from 1999 till 2002, which corresponds to
the maximum phase of the previous solar cycle. Initially, the DCWA
allows us to find the frequencies that are present in those
signals. The implemented method allows us to identify the
preservation of synchronism along the time and the intervals
related to phase-slips among them. The result indicates that both
series are under synchronization almost all the time. This result
is consistent with what we expect according with the physics of
that problem. Indeed, the recorded daily sunspot number (of
sunspots) is well related with the daily measured radio flux at
10.7 cm. The result found confirms what is well known from the
literature that both parameters can be used as proxies for the
solar activity. Also, this DCWA method is validated as a tool to
analyze in a complete way the synchronization of a wider set of
solar parameters.",
conference-location = "S{\~a}o Jos{\'e} dos Campos, SP",
conference-year = "16-20 May",
language = "en",
urlaccessdate = "27 abr. 2024"
}