Modeling the Sun-to-Earth propagation of a very fast CME

Advances in Space Research

Volumn 38, Issue 2, 2006, Pages 253-262

  Manchester IV, W B ^a   Ridley, A J ^a   Gombosi, T I ^a   DeZeeuw, D L ^a  

^a UNIVERSITY OF MICHIGAN   (United States)

Author keywords

Coronal mass ejection; Magnetohydrodynamics; Shock

Indexed keywords

ASTRONOMY; COMPUTER SIMULATION; EARTH (PLANET); MAGNETIC FIELDS; MATHEMATICAL MODELS; SOLAR SYSTEM; TOPOLOGY;

BLOCK ADAPTIVE TREE SOLARWIND ROE UPWIND SCHEME; CORONAL HOLES; CORONAL MASS EJECTION; GIBSON-LOW;

MAGNETOHYDRODYNAMICS;

EID: 33749539712     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.asr.2005.09.044     Document Type: Article

References (24)

1. Amari T., Luciani J.F., Mikić Z., and Linker J. A twisted flux rope model for coronal mass ejections and two-ribbon flares. ApJ 529 (2000) L49-L52
2. Antiochos S.K., DeVore C.R., and Klimchuk J.A. A model for coronal mass ejections. ApJ 510 (1999) 485-493
3. Forbes T.G., and Priest E.R. Photospheric magnetic field evolution and eruptive flares. ApJ 446 (1995) 377-389
4. Gibson S., and Low B.C. A time-dependent three-dimensional magnetohydrodynamic model of the coronal mass ejection. ApJ 493 (1998) 460-473
5. Gosling J.T. The solar flare myth. J. Geophys. Res. 98 (1993) 18937-18950
6. Gosling J.T., Bame S.J., McComas D.J., Phillips J.L., Scime E.E., Pizzo V.J., Goldstein B.E., and Balogh A. A forward-reverse shock pair in the solar wind driven by over-expansion of a conral mass ejection: ulysses observations. Geophys. Res. Lett. 21 (1994) 237-240
7. Groth C.P.T., DeZeeuw D.L., Gombosi T.I., and Powell K.G. Global three-dimensional MHD simulation of a space weather event: CME formation, interplanetary propagation, and interaction with the magnetosphere. J. Geophys. Res. 105 (2000) 25053-25078
8. Hundhausen, A.J. Solar wind six, in: Pizzo, V.J., Holzer, T.E., Sime, D.G. (Eds.), NCAR/TN-306+Proc, Natl. Cent. for Atmos. Res., Boulder, Colorado, pp. 181-214, 1987.
9. Hundhausen A.J. Sizes and locations of coronal mass ejections: SMM observations from 1980 and 1094-1989. J. Geophys. Res. 98 (1993) 13177-13200
10. Kennel C.F., Edmiston J.P., and Hada T. A quarter century of collisionless shock research. In: Robert Stone, and Bruce Tsurutani (Eds). Geophysical Monograph34, Collisionless Shocks in the Heliosphere: A Tutorial Review (1985), American Geophysical Union (AGU), Washington, DC 1-36
11. Low B.C. Coronal mass ejections, magnetic flux ropes, and solar magnetism. J. Geophys. Res. 106 (2001) 25141-25163
12. Manchester IV W.B. Buoyant disruption of magnetic arcades with self-induced shearing. J. Geophys. Res. 108 A4 (2003) 1162
13. Manchester IV W.B., Gombosi T.I., Roussev I., DeZeeuw D.L., Sokolov I.V., Powell K.G., Tóth G., and Opher M. Three-dimensional MHD simulation of a flux rope driven CME. J. Geophys. Res. 109 (2004) A01102
14. Manchester IV W.B., Gombosi T.I., Roussev I., Ridley A.J., DeZeeuw D.L., Sokolov I.V., Powell K.G., and Tóth G. Modeling a space weather event from the Sun to the Earth: CME generation and propagation. J. Geophys. Res. 109 (2004) A02107
15. Manchester IV W., Gombosi T.I., DeZeeuw D.L., Sokolov I.V., Roussev I.I., Powell K., Toth G., and Zurbuchen T.H. CME shock and sheath structures relevant to particle acceleration. ApJ 622 (2005) 1225-1239
16. Parker E.N. Interplanetary Dynamical Processes (1963), Wiley-Interscience, New York
17. Pneuman G.W., and Kopp R.A. Gas-magnetic field interactions in the solar corona. Sol. Phys. 18 (1971) 258-270
18. Powell K.G., Roe P.L., Linde T.J., Gombosi T.I., and DeZeeuw D.L. A solution-adaptive upwind scheme for ideal magnetohydrodynamics. J. Comput. Phys. 154 (1999) 284-309
19. Riley P., Linker J.A., Mikić Z., Odstrcil D., Pizzo V.J., and Webb D.F. Evidence of posteruption reconnection associated with coronal mass ejections in the solar wind. ApJ 578 (2002) 972-978
20. Roussev I.I., Sokolov I.V., Forbes T.G., Gombosi T.I., Lee M.A., and Sakai J.I. A numerical model of a coronal mass ejection: shock development with implications for the acceleration of GeV protons. ApJ 605 (2004) L73-L76
21. Tsurutani B.T., Gonzalez W.D., Lakhina G.S., and Alex S. The extreme magnetic storm of 1-2 September 1859. J. Geophys. Res. 108 (2003) 1268
22. Tsurutani B., Wu S.T., Zhang T.X., and Dryer M. Coronal mass ejection (CME)-induced shock formation, propagation and some temporally and spatially developing shock parameters relevant to particle energization. Astron. Astrophys. 412 (2003) 293-304
23. Wu S.T., Guo W.P., Michels D.J., and Burlaga L.F. MHD description of the dynamical relationships between a flux rope, streamer, coronal mass ejection, and magnetic cloud: an analysis of the January 1997 Sun-Earth connection event. J. Geophys. Res. 104 (1999) 14789-14802
24. Zastenker G.N., Temny V.V., dÚston C., and Bosqued J.M. The form and energy of the shock waves from the solar flares of August 2,4 and 7, 1972. J. Geophys. Res. 83 (1978) 1035-1041