Kinematic Treatment of Coronal Mass Ejection Evolution in the Solar Wind

By Pete Riley, N. Crooker. 2004

167 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/7d71c03186bd591c159631c9c01c1fe63bb53b58

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In Astronomy and Astrophysics

1. N. Lugaz
2. M. Temmer
3. Pete Riley
4. B. Vršnak
5. W. Manchester IV
6. J. Davies
7. A. Thernisien
8. A. Vourlidas

Citations in the corpus

• The association of coronal mass ejections with their effects near the Earth (2005, background): “The statement by Riley and Crooker (2004) describes the present status quite well: " These models include a rich variety of physics and have been quite successful in reproducing a wide range of observational signatures.”
• Constraints on the global structure of magnetic clouds: Transverse size and curvature (2006, background): “The distortion of MCs, resulting from the interaction with the ambient solar wind, is mainly a kinematic effect since magnetic forces are dominated by the flow momentum [ Riley and Crooker, 2004 ].”
• IMPLEMENTATION OF THE GRADUATED CYLINDRICAL SHELL MODEL FOR THE THREE-DIMENSIONAL RECONSTRUCTION OF CORONAL MASS EJECTIONS (2011, background): “Above 30 R , observational evidences (Kahler & Webb 2007) as well as theoretical models (Riley & Crooker 2004) seem to show that the front of flux rope CMEs get distorted because of interactions with the ambient solar wind.”
• Fitting Flux Ropes to a Global MHD Solution: A Comparison of Techniques. Appendix 1 (2004, background): “We have shown (Riley and Crooker, 2004) that the fundamental cross-section of flux ropes in the solar wind is neither circular nor elliptical, but rather a convexoutward, ‘‘pancake’’ shape.”
• The Plasma and Suprathermal Ion Composition (PLASTIC) Investigation on the STEREO Observatories (2008, methodology): “, based on the GradShafranov equation (Hu and Sonnerup 2002), and using kinematic expansions of the clouds (Riley and Crooker 2004).”
• The Physical Processes of CME/ICME Evolution (2017, background): “Simulations also illustrate the deformation of CMEs by bimodal ambient solar wind typical of solar minimum (e.g., Gosling 1999; Odstrčil and Pizzo 1999b; Riley and Crooker 2004; Manchester et al. 2004a).”
• RECONSTRUCTING CORONAL MASS EJECTIONS WITH COORDINATED IMAGING AND IN SITU OBSERVATIONS: GLOBAL STRUCTURE, KINEMATICS, AND IMPLICATIONS FOR SPACE WEATHER FORECASTING (2010, background): “CMEs can be significantly distorted by ambient coronal and solar wind structures (Liu et al. 2006a, 2008a, 2009b); even a uniform solar wind can easily flatten the cross section with its radial flow (Riley & Crooker 2004; Liu et al. 2006a).”