Three‐dimensional MHD simulation of a flux rope driven CME

By W. Manchester IV, Tamas I. Gombosi, Ilia I. Roussev, D. D. De Zeeuw, Igor M. Sokolov, Kenneth G. Powell, G. T'oth, Merav Opher. 2004

137 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/3b671570fd3e8d70ab002b1a30f9abb7e0a027ef

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Citations in the corpus

Modeling a space weather event from the Sun to the Earth: CME generation and interplanetary propagation (2004, methodology): “In the CME simulation presented by Manchester et al. [2004], this thermal absorption was prevented.”
MAGNETOHYDRODYNAMIC WAVES AND CORONAL HEATING: UNIFYING EMPIRICAL AND MHD TURBULENCE MODELS (2012, background): “…solar wind (Roussev et al. 2003b; Cohen et al. 2007, 2008), as well as the initiation (Roussev et al. 2003a; Jacobs et al. 2009) and propagation of idealized (Manchester et al. 2004a,b) and not-so-idealized (Roussev et al. 2004, 2007) solar eruptions and associated SEP events (Sokolov et al. 2004).”
Coronal Mass Ejection Shock and Sheath Structures Relevant to Particle Acceleration (2005, unknown): “…al. 2000; Riley et al. 2002; Manchester 2003; Roussev et al. 2004; Manchester et al. 2004a), some of which (e.g., Wu et al. 1999; Riley et al. 2002; Roussev et al. 2004; Manchester et al. 2004a) are global models that 1225 include a solar wind and hence can address shock formation and propagation.”
Numerical Simulation of the Interaction of Two Coronal Mass Ejections from Sun to Earth (2005, methodology): “The flux rope’s properties are identical to those of the rope extensively studied in Manchester et al. (2004b).”
The Calm before the Storm: The Link between Quiescent Cavities and Coronal Mass Ejections (2006, background): “The idea of the erupting CME as a magnetic flux rope has gained acceptance over the years (Amari et al. 2003; Chen&Krall 2003; Roussev et al. 2003; MacNeice et al. 2004; Manchester et al. 2004).”
The Physical Processes of CME/ICME Evolution (2017, background): “…8–24 hours, (iii) the CME speeds can change significantly, even at large distances from the Sun, due to their interaction with the solar wind (Manchester et al. 2004a; Temmer et al. 2011; Liu et al. 2013), (iv) CME-CME interaction is inherently a three-dimensional process, and the changes…”