Magnetohydrodynamic Simulation of a Solar Flare with Chromospheric Evaporation Effect Based on the Magnetic Reconnection Model

By T. Yokoyama, Kazunari Shibata. 2001

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View Paper: https://www.semanticscholar.org/paper/affafc058197d5b4557720087f7e60eaefea7498

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In Astronomy and Astrophysics

Citations in the corpus

On Solving the Coronal Heating Problem (2005, methodology): “Some existing MHD models do include field-aligned thermal conduction (e.g., Lionello, Linker, and Mikić, 2001; Yokoyama and Shibata, 2001; Gudiksen and Nordlund, 2002, 2005a,b), but they do not yet adequately resolve the transition region.”
Hot Jupiters and Hot Spots: The Short- and Long-Term Chromospheric Activity on Stars with Giant Planets (2004, background): “Yohkoh solar X-ray observations (e.g. Yokoyama & Shibata 2001) have shown that the energy release at the site of magnetic reconnection during a solar flare generates a burst of X-ray emitting gas.”
On the Star-Magnetosphere Interaction of Close-in Exoplanets (2004, background): “…reconnection site at the loop top will create a burst of X-ray–emitting gas; the funneling of the hot plasma, along the magnetic field lines down to the footpoints, in turn produces anomalous heating at the chromospheric layer (Tsuneta 1997; Masuda, Kosugi, & Hudson 2001; Yokoyama & Shibata 2001).”
Solar Flares: Magnetohydrodynamic Processes (2011, methodology): “Those features mentioned above have been reproduced by recent MHD simulations (Yokoyama and Shibata, 1997, 1998, 2001), which are discussed in Section 5.”
Modelling Quasi-Periodic Pulsations in Solar and Stellar Flares (2018, result): “12a), which is different from the previous expectations based on a standard flare model and previous simulations (Yokoyama and Shibata 2001).”
Investigation of the Neupert effect in solar flares. I. Statistical properties and the evaporation model (2002, methodology): “Recently, extensive simulations of chromospheric evaporation driven by thermal conduction have been performed by Yokoyama & Shibata (1998, 2001).”