Active region NOAA 13842 produced two successive solar flares: an X7.1-class flare on 2024 October 1, and an X9.0-class flare on 2024 October 3. This study continues our previous simulation work that successfully reproduced the X7.1-class solar flare. In
Keitarou Matsumoto +7 more
doaj +1 more source
Magnetic Reconnection In Solar, Space, And Laboratory Plasmas
Magnetic reconnection is a ubiquitous process in space, astrophysical, and laboratory plasmas. Observations of reconnection in the solar corona, such as those by the X-Ray Telescope on Hinode and the Atmospheric Imaging Assembly on the Solar Dynamics Observatory, allow us to study the large-scale consequences and dynamics of reconnection but provide ...
openaire +1 more source
Properties of Magnetic Switchbacks in the Near-Sun Solar Wind. [PDF]
Badman ST +26 more
europepmc +1 more source
Perpendicular ion heating in turbulence and reconnection: magnetic moment breaking by coherent fluctuations. [PDF]
Mallet A +4 more
europepmc +1 more source
Day-to-Day Boundary Fluctuations in Coronal Holes: Causes and Consequences. [PDF]
Ugarte-Urra I +3 more
europepmc +1 more source
Simulation Models for Exploring Magnetic Reconnection. [PDF]
Shay M +24 more
europepmc +1 more source
Numerical Modeling of Prominences and Coronal Rain with the MPI-AMRVAC Code. [PDF]
Liakh V, Jenkins J.
europepmc +1 more source
Energetic spectra from semi-implicit particle-in-cell simulations of magnetic reconnection. [PDF]
Schoeffler KM +4 more
europepmc +1 more source
Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Veronig AM +12 more
europepmc +1 more source
Evaluating Solar Wind Forecast Using Magnetic Maps That Include Helioseismic Far-Side Information. [PDF]
Heinemann SG +7 more
europepmc +1 more source

