Three-dimensional numerical simulation of MHD waves observed by the Extreme Ultraviolet Imaging Telescope

Journal of Geophysical Research: Space Physics

Volumn 106, Issue A11, 2001, Pages 25089-25102

  Wu, S T ^a,i   Zheng, Huinan ^a,i   Wang, S ^a,b,i   Thompson, B J ^c   Plunkett, S P ^d,e   Zhao, X P ^f   Dryer, M ^g,h  

^a University of Alabama in Huntsville ^*  (United States)

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

^c NASA GODDARD SPACE FLIGHT CENTER   (United States)

^d University of Space Research Association   (United States)

^e NAVAL RESEARCH LABORATORY   (United States)

^f STANFORD UNIVERSITY   (United States)

^g NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

^h Exploration Physics International Inc   (United States)

ⁱ UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 39449099867     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2000ja000447     Document Type: Article

References (29)

1. Athay, R. G., and G. E. Moreton, Impulsive phenomena of the solar atmosphere, I, Some optical events associated with flares showing explosive phase, Astrophys. J., 133, 935-950, 1961.
2. Bazer, J., and O. Fleischman, Propagation of weak hydromagnetic discontinuities, Phys. Fluids, 2, 366-373, 1959.
3. Delaboudiniére, J. P., et al., EIT: Extreme-ultraviolet imaging telescope for the SOHO mission, Sol. Phys., 164, 291-312, 1995.
4. ⊙ ≤ 1.50 along the solar equatorial plane, Astrophys. J., 518, 500-507, 1999.
5. Friedrichs, K. O., Non-linear wave motion in magnetohydrodynamics, Rep. 2105, Los Alamos Natl. Lab., Los Alamos, N. M., 1954.
6. Fredrichs, K. O., and H. Kranzer, Nonlinear wave motion in magnetohydrodynamics, Rep. MH-8, Inst. of Math. Sci., New York Univ., New York, 1958.
7. Hoeksema, J. T., Extending the Sun's magnetic field through the three-dimensional heliosphere, Adv. Space Res., 9(4), 141-145, 1989.
8. Hoeksema, J. T., Large-scale solar and heliospheric magnetic fields, Adv. Space Res., 11(1), 15-24, 1991.
9. Hoeksema, J. T., and P. H. Scherrer, An atlas of photospheric magnetic field observations and computed coronal magnetic fields: 1976-1985, Sol. Phys., 105, 205-211, 1985.
10. Hu, Y. Q., and S. T. Wu, A full-implicit-continuous-Eulerian (FICE) scheme for multi-dimensional, transient magnetohydrodynamic (MHD) flows, J. Comput. Phys., 55, 33-64, 1984.
11. Jeffrey, A., and T. Taniuti, Non-linear wave propagation with application to physics and magnetohydrodynamics, chap. 6, p. 219, and Appendix D, Academic, San Diego, Calif., 1964.
12. Low, B. C., Self-similar magnetohydrodynamics, Part four, The physics of coronal transients, Astrophys. J., 281, 392-404, 1984.
13. Meyer, F., Flare-produced coronal waves, in Proc. IAU Sym 35: Structure and Development of Solar Active Regions, edited by K. O. Kiepenheuer, p. 485, D. Reidel, Norwell, Mass., 1968.
14. Moreton, G. E., Hα observations of flare-initiated disturbances with velocities ∼1000 km/sec, Astron. J., 65, 494-501, 1960.
15. Moreton, G. E., Fast-moving disturbances on the Sun, Sky Telescope, 21, 145-146, 1961.
16. Moreton, G. E., Hα shock wave and winking filaments with the flare of 20 September 1963, Astron. J., 69, 145-151, 1964.
17. Nakagawa, Y., Y. Q. Hu, and S. T. Wu, The method of projected characteristics for the evolution of magnetic arches, Astron. Astrophys., 179, 354-370, 1987.
18. Neupert, W. M., Transient coronal extreme ultraviolet emission before and during the impulsive phase of a solar flare, Astrophys. J., 504, 344-353, 1989.
19. Plunkett, S. P., B. J. Thompson, R. A. Howard, D. J. Michels, O. C. St. Cyr, S. J. Tappin, R. Schwenn, and P. L. Lamy, LASCO observations of an Earth-directed coronal mass ejection on May 12, 1997, Geophys. Res. Lett., 25, 2477-2480, 1998.
20. Roache, R. J., Fundamentals of Computational Fluid Dynamics, Hermosa, Albuquerque, N. M., 1999.
21. Sakurai, T., M. Irie, M. Miyashita, K. Yamaguchi, and Y. Shiomi, An X12/3B white-light flare of 1991 June 4 on NOAA Region 6659, in Proceedings of the Second SOLTIP Symposium, Nakaminato, Japan, 13-17 June 1994, STEP GBRSC Special Issue, vol. 5, pp. 33-36, Ibaraki Univ. Press, Mito, Japan, June 1995.
22. Thompson, B. J., S. P. Plunkett, H. B. Gurman, J. S. Newmark, O. C. St. Cyr, and D. J. Michels, SOHO/EIT observations of an Earth-directed coronal mass ejection on May 12, 1997, Geophys. Res. Lett., 25, 2465-2468, 1998.
23. Thompson, B. J., J. B. Gurman, W. M. Neupert, J. S. Newmark, J.-P. Delabourdiniére, O. C. St. Cyr, S. Stezelberger, L. P. Dere, R. A. Howard, and D. J. Michels, SOHO/EIT observations of the 1997 April 7 coronal transient: Possible evidence of coronal Moreton waves, Astrophys. J. Lett., 517, L151-L155, 1999.
24. Uchida, Y., Fast-mode wavefronts and Moreton's wave phenomena, Sol. Phys., 4, 30-44, 1968.
25. Uchida, Y., M. D. Altschuler, and G. Newkirk, Flare-produced coronal MHD-fast-mode wave front and Moreton's wave phenomenon, Sol. Phys., 28, 495-516, 1973.
26. Wang, Y. M., EIT waves and fast-mode propagation in the solar corona, Astrophys. J., 543, L89-L93, 2000.
27. Whang, Y. C., Slow shocks and their transition to fast shocks in the inner solar wind, J. Geophys. Res., 92, 4349-4356, 1987.
28. Wu, S. T., and J. F. Wang, Numerical tests of a modified full implicit continuous Eulerian (FICE) scheme with projected normal characteristic boundary conditions for MHD flows, Comput. Meth. Appl. Mech. Eng., 64, 267-282, 1987.
29. Yanenko, N. N., The Method of Fractional Steps, The Solution of Problems of Mathematical Physics in Several Variables, p. 149, Springer-Verlag, New York, 1971.