A numerical simulation on the solar-terrestrial transit time of successive CMEs during November 4-5, 1998

Acta Geophysica Sinica

Volumn 48, Issue 4, 2005, Pages 731-738

  Xiong, Ming ^a   Zheng, Hui Nan ^a   Wang, Yu Ming ^a   Fu, Xiang Rong ^a   Wang, Shui ^a   Dou, Xian Kang ^a  

^a UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

Author keywords

Coronal mass ejection; Magnetohydrodynamics; Numerical simulation; Space weather

Indexed keywords

CORONAL MASS EJECTION;

EID: 28944434851     PISSN: 00015733     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (23)

1. Gosling J T. The solar flare myth. J. Geophys. Res., 1993, 98 (A11): 18,937-18,950
2. Akasofu S I. Energy coupling between the solar wind and the magnetosphere. Space Sci. Rev., 1981, 28: 121-190
3. Gonzalez W D, Gonzalez L C, Tsurutani B T, et al. Solar wind - magnetosphere coupling during intense magnetic storms (1978-1979). J. Geophys. Res., 1989, 94: 8,835-8,851
4. Hakamada K, Akasofu S I. Simulation of three-dimensional solar wind disturbances and resulting geomagnetic storms. Space Sci. Rev., 1982, 31: 3-70
5. Akasofu S I, Fry C D. A first-generation geomagnetic storm prediction scheme. Planetary Space Sci, 1986, 34: 77-92
6. Fry C D, Sun W, Deehr C S, et al. Improvements to the HAF solar wind model for space weather predictions. J. Geophys. Res., 2001, 106(A10): 20,985-21,001
7. Wang C B, Zhao J K, Chen H H, et al. Prediction of the IMF Bz using a 3-D kinematic code. Chinese J. Geophys. (in Chinese), 2002, 45(6): 749-758
8. Groth C P T, De Zeeuw D L, Gombosi T I, et al. Global 3D MHD simulation of a space weather event: CME formation, interplanetary propagation, and interaction with the magnetosphere. J. Geophys. Res., 2000, 105(A11): 25,053-25,078
9. Gopalswamy N, Lara A, Lepping R P, et al. Interplanetary acceleration of coronal mass ejections. Geophys. Res. Lett., 2000, 27: 145-148
10. Gopalswamy N, Lara A, Yashiro S, et al. Predicting the 1-AU arrival times of coronal mass ejections. J. Geophys. Res., 2001, 106(A12): 29,207-29,218
11. Gonzalez-Esparza J A, Lara A, Perez-Tijerina E, et al. A numerical study on the acceleration and transit time of coronal mass ejections in the interplanetary medium. J. Geophys. Res., 2003, 108 (A1): SSH9
12. Burlaga L F, Plunkett S P, st. Cyr O C. Successive CMEs and complex ejecta. J. Geophys. Res., 2002, 107(A10): SSH1
13. Smart D F, Shea M A. A simplified model for timing the arrival of solar-flare-initiated shocks. J. Geophys. Res., 1985, 90: 183-190
14. Smith Z, Dryer M, Ort E, et al. Performance of interplanetary shock prediction models: STOA and ISPM. J. Atmos. Solar-Terr. Phys., 2000, 62: 1265-1274
15. Smith Z, Dryer M. MHD study of temporal and spatial evolution of simulated interplanetary shocks in the ecliptic plane within 1AU. Solar Phys., 1990, 129: 387-405
16. Riley P, Gosling J T. Do coronal mass ejections implode in the solar wind? Geophys. Res. Lett., 1998, 25: 1529-1532
17. Riley P, Gosling J T, Pizzo V J. Investigation of the polytropic relationship between density and temperature within interplanetary coronal mass ejection using numerical simulations. J. Geophys. Res., 2001, 106(A5): 8,291-8,300
18. Dryer M. Interplanetary studies: Propagation of disturbances between the Sun and the magnetosphere. Space Sci. Rev., 1994, 67: 363-419
19. Jeffrey A and Taniuti T. Non-linear Wave Propagation with Applications to Physics and Magnetohydrodynamics. New York: Academic Press, 1964
20. Harten A. High resolution schemes for hyperbolic conservation laws. J. Comput. Phys., 1983, 49: 357-393
21. Parker E N. Interplanetary Dynamical Processes. New York: Wiley-Interscience, 1963
22. Michalek G, Gopalswamy N and Yashiro S. A new method for estimating widths, velocities and source location of halo CMEs. Astrophys. J., 2003, 584: 472-478
23. Vandas M, Fischer S, Dryer M, et al. Simulation of magnetic cloud propagation in the inner heliosphere in two-deimensions 1. A loop perpendicular to the ecliptic plane. J. Geophys. Res., 1995, 100 (A7): 12,285-12,292