Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Nastaran Farhang"'
Publikováno v:
Scientific Reports, Vol 12, Iss 1, Pp 1-12 (2022)
Abstract Determination of self-organized criticality (SOC) is crucial in evaluating the dynamical behavior of a time series. Here, we apply the complex network approach to assess the SOC characteristics in synthesis and real-world data sets. For this
Externí odkaz:
https://doaj.org/article/dee727d196df42c4bd991c7bd49be395
Publikováno v:
The Astrophysical Journal Supplement Series, Vol 273, Iss 1, p 1 (2024)
Solar and stellar magnetic patches (i.e., magnetic fluxes that reach the surface from the interior) are believed to be the primary sources of a star’s atmospheric conditions. Here, we apply the complex network approach and investigate its efficacy
Externí odkaz:
https://doaj.org/article/5c380d82bcdb4dbc992e72bc31b1dc18
Publikováno v:
The Astrophysical Journal. 936:87
Quasi-periodic pulsations (QPPs) with various periods that originate in the underlying magnetohydrodynamic processes of flaring structures are detected repeatedly in solar flare emissions. We apply a 2D cellular automaton (CA) avalanche model to simu
The distributions of solar flare energies and waiting times have not been described simultaneously by a single physical model, yet. In this research, we investigate whether recent avalanche models can describe the distributions for both the released
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::efec769b3c21c582eb20a53ce4b6ddf0
http://arxiv.org/abs/1909.00195
http://arxiv.org/abs/1909.00195
Publikováno v:
The Astrophysical Journal. 894:66
A constructive approach is developed to build the solar flare complex network by utilizing a visibility graph condition alongside the Abe–Suzuki method. Solar flare information such as position, start time, and peak flux is used for this purpose. T
Solar flares are an abrupt release of magnetic energy in the Sun's atmosphere due to reconnection of the coronal magnetic field. This occurs in response to turbulent flows at the photosphere which twist the coronal field. Similar to earthquakes, sola
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fad63a9a7d58f35c82fcffbff85c7cfc