MHD simulation of two successive interplanetary disturbances driven by cone-model parameters in IPS-based solar wind

Geophysical Research Letters

Volumn 33, Issue 20, 2006, Pages

  Hayashi, Keiji ^a   Zhao, Xue Pu ^a   Liu, Yang ^a  

^a STANFORD UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; EARTH (PLANET); INTERPLANETARY SPACECRAFT; NUMERICAL ANALYSIS;

CORONAL MASS EJECTION; INTERPLANETARY DISTURBANCES; INTERPLANETARY RADIO SCINTILLATION; SOLAR WIND;

SOLAR SYSTEM;

CORONAL MASS EJECTION; INTERPLANETARY DUST; SIMULATION; SOLAR WIND;

EID: 33845602611     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/2006GL027408     Document Type: Article

References (12)

1. Hayashi, K. (2005), MHD simulations of the solar corona and solar wind using a boundary treatment to limit solar wind mass flux, Astrophys. J. Suppl., 161, 480-494, doi:10.1086/491791.
2. Hayashi, K., M. Kojima, M. Tokumaru, and K. Fujiki (2003), MHD tomography using interplanetary scintillation measurement, J. Geophys. Res., 108(A3), 1102, doi:10.1029/2002JA009567.
3. Jackson, V. B., P. L. Hick, M. Kojima, and A. Yokobe (1998), Heliospheric tomography using interplanetary scintillation observations: 1. Combined Nagoya and Cambridge data, J. Geophys. Res., 103, 12,049-12,067.
4. Kojima, M., K. Fujiki, T. Ohmi, M. Tokumaru, A. Yokobe, and K. Hakamada (2001), Latitudinal velocity structures up to the solar poles estimated from interplanetary scintillation tomography analysis, J. Geophys. Res., 106, 15,677-15,686.
5. Linker, J. A., G. van Hoven, and D. D. Schnack (1990), A three-dimensional simulation of a coronal streamer, Geophys. Res. Lett., 17, 2281-2284.
6. Odstrcil, D., and V. J. Pizzo (1999), Distortion of the interplanetary magnetic field by three-dimensional propagation of coronal mass ejections in a structured solar wind, J. Geophys. Res., 104, 28,225-28,239.
7. Odstrcil, D., P. Riley, and X. P. Zhao (2004), Numerical simulation of the 12 May 1997 interplanetary CME event, J. Geophys. Res., 109, A02116, doi: 10.1029/2003JA010135.
8. Schatten, K. H., J. M. Wilcox, and N. F. Ness (1969), A model of interplanetary and coronal magnetic field, Sol. Phys., 6, 442-455.
9. Totten, T. L., J. W. Freeman, and S. Arya (1995), An empirical determination of the polytropic index for the free-streaming solar wind using Helios 1 data, J. Geophys. Res., 100, 13-17.
10. Usmanov, A. V., and M. Dryer (1995), A global 3-D simulation of interplanetary dynamics in June 1991, Sol. Phys., 159, 347-370.
11. Xie, H., L. Ofman, and G. Lawrence (2004), Cone model for halo CMEs: Application to space weather forecasting, J. Geophys. Res., 109, A03109, doi: 10.1029/2003JA010226.
12. Zhao, X. P., S. P. Plunkett, and W. Liu (2002), Determination of geometrical and kinematical properties of halo coronal mass ejections using the cone model, J. Geophys. Res., 107(A8), 1223, doi:10.1029/ 2001JA009143.