Non-spherical source-surface model of the heliosphere: A scalar formulation

Annales Geophysicae

Volumn 15, Issue 11, 1997, Pages 1379-1387

  Schulz, M ^a  

^a LOCKHEED MARTIN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0642343438     PISSN: 09927689     EISSN: None     Source Type: Journal    
DOI: 10.1007/s00585-997-1379-1     Document Type: Article

References (22)

1. Altschuler, M. D., and G. Newkirk, Jr., Magnetic fields and the structure of the solar corona, Solar Phys., 9, 131-149, 1969.
2. Hoeksema, J. T., The Solar Magnetic Field - 1985 through 1990, Report CSSA-ASTRO-91-01, Stanford University, Stanford, Calif., 1991.
3. Hoeksema, J. T., and P. H. Scherrer, The Solar Magnetic Field -1976 through 1985, Report UAG-94, World Data Center A for Solar-Terrestrial Physics, Boulder, Colo., 1986.
4. Jackson, J. D., Classical Electrodynamics, pp. 16-17, Wiley, New York, 16-17 1962.
5. Levine, R. H., M. Schulz, and E. N. Frazier, Simulation of the magnetic structure of the inner heliosphere by means of a non-spherical source surface, Solar Phys., 77, 363-392, 1982.
6. Mead, G. D., and D. H. Fairfield, A quantitative magnetospheric model derived from spacecraft magnetometer data, J. Geophys. Res., 80, 523-534, 1975.
7. Mikic, Z., and J. A. Linker, Disruption of coronal magnetic field arcades, Astrophys. J., 430, 898-912, 1994.
8. Pneuman, G. W., and R. A. Kopp, Gas-magnetic field interactions in the solar corona. Solar Phys., 18, 258-270, 1971a.
9. Pneuman, G. W., and R. A. Kopp, Interactions of coronal material with magnetic fields, in Solar Magnetic Fields, ed. R. Howard, pp. 526-533, Reidel, Dordrecht, 1971b.
10. Schatten, K. H., Current sheet magnetic model for the solar corona, in Solar Wind, eds. C. P. Sonett, P. J. Coleman, Jr., and J. M. Wilcox, pp. 44-54, NASA SP-308, Washington, D.C., 1971.
11. Schatten, K. H., J. M. Wilcox, and N. F. Ness, A model of coronal and interplanetary magnetic fields, Solar Phys., 6, 442-455, 1969.
12. Schulz, M., Fourier parameters of heliospheric current sheet and their significance. Space Sci. Rev., 72, 149-152, 1995.
13. Schulz, M., and A. Eviatar, Diffusion of equatorial particles in the outer radiation zone, J. Geophys. Res., 74, 2182-2192, 1969.
14. Schulz, M., E. N. Frazier, and D. J. Boucher, Jr., Coronal magnetic-field model with non-spherical source surface, Solar Phys., 60, 83-104, 1978.
15. Smith, E. J., and A. Balogh, Ulysses observations of the radial magnetic field, Geophys. Res. Lett., 22, 3317-3320, 1995.
16. Smith, E. J., M. Neugebauer, A. Balogh, S. J. Bame, G. Erdös, R. J. Forsyth, B. E. Goldstein, J. L. Phillips, and B. T. Tsurutani, Disappearance of the heliospheric sector structure at Ulysses, Geophys. Res. Lett., 20, 2327-2330, 1993.
17. Stern, D. P., Representation of magnetic fields in space, Rev. Geophys. Space Phys., 14, 199-214, 1976.
18. Stern, D. P., The art of mapping the magnetosphere, J. Geophys. Res., 99, 17169-17198, 1994.
19. Usmanov, A. V., A global numerical 3-D MHD model of the solar wind, Solar Phys., 146, 377-396, 1993.
20. Wang, Y.-M., and N. R. Sheeley, Jr., Solar implications of Ulysses interplanetary field measurements, Astrophys. J., 447, L143-L146, 1995.
21. Wolfram Research, Inc., Mathematica, version 2.1, Wolfram Research, Inc., Champaign, Ill., 1992.
22. Zhao, X.-P., and J. T. Hoeksema, Modeling the out-of-ecliptic interplanetary magnetic field in the declining phase of Sunspot Cycle 22, Space Sci. Rev., 72, 189-192, 1995.