Hydrodynamics of core-collapse supernovae and their progenitors
B Müller - Living Reviews in Computational Astrophysics, 2020 - Springer
Multi-dimensional fluid flow plays a paramount role in the explosions of massive stars as
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …
core-collapse supernovae. In recent years, three-dimensional (3D) simulations of these …
The physical processes of CME/ICME evolution
W Manchester, EKJ Kilpua, YD Liu, N Lugaz… - Space Science …, 2017 - Springer
As observed in Thomson-scattered white light, coronal mass ejections (CMEs) are manifest
as large-scale expulsions of plasma magnetically driven from the corona in the most …
as large-scale expulsions of plasma magnetically driven from the corona in the most …
Magnetohydrodynamic simulation of interplanetary propagation of multiple coronal mass ejections with internal magnetic flux rope (SUSANOO‐CME)
D Shiota, R Kataoka - Space Weather, 2016 - Wiley Online Library
Coronal mass ejections (CMEs) are the most important drivers of various types of space
weather disturbance. Here we report a newly developed magnetohydrodynamic (MHD) …
weather disturbance. Here we report a newly developed magnetohydrodynamic (MHD) …
Electric currents in flare ribbons: observations and three-dimensional standard model
M Janvier, G Aulanier, V Bommier… - The Astrophysical …, 2014 - iopscience.iop.org
We present for the first time the evolution of the photospheric electric currents during an
eruptive X-class flare, accurately predicted by the standard three-dimensional (3D) flare …
eruptive X-class flare, accurately predicted by the standard three-dimensional (3D) flare …
Forecasting the structure and orientation of earthbound coronal mass ejections
Abstract Coronal Mass Ejections (CMEs) are the key drivers of strong to extreme space
weather storms at the Earth that can have drastic consequences for technological systems in …
weather storms at the Earth that can have drastic consequences for technological systems in …
Magnetic flux ropes in the solar corona: structure and evolution toward eruption
R Liu - Research in Astronomy and Astrophysics, 2020 - iopscience.iop.org
Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …
Quantitative analysis of CME deflections in the corona
In this paper, ten CME events viewed by the STEREO twin spacecraft are analyzed to study
the deflections of CMEs during their propagation in the corona. Based on the three …
the deflections of CMEs during their propagation in the corona. Based on the three …
The first observation of a rapidly rotating coronal mass ejection in the middle corona
A Vourlidas, R Colaninno… - The Astrophysical …, 2011 - iopscience.iop.org
In this Letter, we present the first direct detection of a rotating coronal mass ejection (CME) in
the middle corona (5–15 R☉). The CME rotation rate is 60 day–1, which is the highest rate …
the middle corona (5–15 R☉). The CME rotation rate is 60 day–1, which is the highest rate …
Flare-CME models: an observational perspective (invited review)
B Schmieder, G Aulanier, B Vršnak - Solar physics, 2015 - Springer
Eruptions, flares, and coronal mass ejection (CMEs) are due to physical phenomena mainly
driven by an initially force-free current-carrying magnetic field. We review some key …
driven by an initially force-free current-carrying magnetic field. We review some key …
Inner heliosphere MHD modeling system applicable to space weather forecasting for the other planets
We developed a magnetohydrodynamic (MHD) solar wind model which can be used for
practical use in real‐time space weather forecasting at Earth's orbit and those of other …
practical use in real‐time space weather forecasting at Earth's orbit and those of other …