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pro vyhledávání: '"Farhang, Nastaran"'
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. Hence, detecting and identifying these features (also known as magnetic ele
Externí odkaz:
http://arxiv.org/abs/2307.15523
Quasi-periodic pulsations (QPPs) with various periods that originate in the underlying magnetohydrodynamic processes of the flaring structures are detected repeatedly in the solar flare emissions. We apply a 2D cellular automaton (CA) avalanche model
Externí odkaz:
http://arxiv.org/abs/2208.02493
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:
http://arxiv.org/abs/1909.00195
Solar coronal loops represent the variety of fast, intermediate, and slow normal mode oscillations. In this study, the transverse oscillations of the loops with a few-minutes period and also with damping caused by the resonant absorption were analyze
Externí odkaz:
http://arxiv.org/abs/1902.09649
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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:
http://arxiv.org/abs/1804.10356
Autor:
Kaki, Bardia1 (AUTHOR) bardia.kaki@znu.ac.ir, Farhang, Nastaran2 (AUTHOR), Safari, Hossein1 (AUTHOR) safari@znu.ac.ir
Publikováno v:
Scientific Reports. 10/7/2022, Vol. 12 Issue 1, p1-12. 12p.
Akademický článek
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