Obtaining potential field solutions with spherical harmonics and finite differences

Astrophysical Journal

Volumn 732, Issue 2, 2011, Pages

  Tóth, Gábor ^a   Van Der Holst, Bart ^a   Huang, Zhenguang ^a  

^a UNIVERSITY OF MICHIGAN   (United States)

Author keywords

magnetic fields; methods: numerical; Sun: corona; Sun: surface magnetism

Indexed keywords

EID: 79955663894     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/732/2/102     Document Type: Article

References (9)

1. Adams, J. & Pneuman, G. W. 1976, Sol. Phys., 46, 185
2. Altschuler, M. D., Levine, R. H., Stix, M., & Harvey, J. 1977, Sol. Phys., 51, 345
3. Clenshaw, C. W. & Curtis, A. R. 1960, Numer. Math., 2, 197
4. Potts, D., Steidl, G., & Tasche, M. 1998, Linear Algebr. Appl., 275, 433
5. Schatten, K. J., Wilcox, J. M., & Ness, N. F. 1969, Sol. Phys., 6, 442
6. Suda, R. & Takami, M. 2001, Math. Comput., 71, 703
7. Tran, T. 2009, Improving the Predictions of Solar Wind Speed and Interplanetary Magnetic Field at the Earth, PhD thesis, UCLA
8. van der Holst, B., Manchester, W. B., IV, Frazin, R. A., Vsquez, A. M., Tóth, G., & Gombosi, T. I. 2010, ApJ, 725, 1373
9. van der Vorst, H. 1992, SIAM J. Sci. Stat. Comput., 13, 631