Modeling a space weather event from the Sun to the Earth: CME generation and interplanetary propagation

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

244 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/d6fa2d88bcd7063172f405f2b849c62a8e759472

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In Astronomy and Astrophysics

Citations in the corpus

The Physical Processes of CME/ICME Evolution (2017, methodology): “…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…”
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).”
Deriving the radial distances of wide coronal mass ejections from elongation measurements in the heliosphere - application to CME-CME interaction (2009, methodology): “This has been shown by multiple-spacecraft observations (e.g. Möstl et al., 2009) and from simulations (Riley et al., 2003; Manchester et al., 2004; Odstrcil et al., 2005).”
Constraints on the global structure of magnetic clouds: Transverse size and curvature (2006, background): “, 2003] and structured solar wind [e.g., Groth et al., 2000; Odstrcil et al., 2004; Manchester et al., 2004].”
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).”
Adaptive numerical algorithms in space weather modeling (2012, methodology): “Currently the physics-based EE model only works in a stand-alone mode [30,31], and we use the empirical models to generate CMEs in the SWMF [32,33].”
Properties of Interplanetary Coronal Mass Ejections at One AU During 1995 – 2004 (2006, background): “…some of which include launching CMEs and following them to Earth (e.g., Odstrcil and Pizzo, 1999a,b,c; Linker et al., 2003; Riley et al., 2003; Manchester et al., 2004), there is no thorough understanding of key aspects of CMEs, specifically, how they are initiated in the solar corona, and…”
The association of coronal mass ejections with their effects near the Earth (2005, methodology): “The work by Plunkett et al. (1998) made use of the observation that the outer boundaries of most limb CMEs form a cone of constant spread with a median angular extent of about 50. This was confirmed for many more limb CMEs by St.Cyr et al. (2000). Adopting this value and knowing the projection speed”