Distribution and properties of open magnetic flux outside of coronal holes

Journal of Geophysical Research: Space Physics

Volumn 111, Issue 9, 2006, Pages

  Fisk, L A ^a   Zurbuchen, T H ^a  

^a UNIVERSITY OF MICHIGAN   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 33947540572     PISSN: None     EISSN: 21699402     Source Type: Journal    
DOI: 10.1029/2005JA011575     Document Type: Article

References (44)

1. Altschuler, M. D., and G. Newkirk (1969), Magnetic fields and the structure of the solar corona. I: Methods of calculating coronal fields, Sol. Phys., 9, 131.
2. Axford, W. I. (1977), The three-dimensional structure of the interplanetary medium, in Study of Traveling Interplanetary Phenomena, edited by M. A. Shea, D. F. Smart, and S.-T. Wu, p. 145, Springer, New York.
3. Bavassano, B., R. Woo, and R. Bruno (1997), Heliospheric plasma sheet and coronal streamers, Geophys. Res. Lett., 24, 1655.
4. Biskamp, D. (1993), Nonlinear Magnetohydrodynamics, Cambridge Univ. Press, New York.
5. Dulk, G. A., Y. Leblanc, P. A. Robinson, J.-L. Bougeret, and R. P. Lin (1998), Electron beams and radio waves of solar type III bursts, J. Geophys. Res., 103, 17, 223.
6. 6 K temperature regime, Astrophys. J., 522, 1133.
7. Feldman, U., E. Landi, and N. A. Schwadron (2005), On the sources of the fast and slow solar wind, J. Geophys. Res., 110(A7), A07109, doi:10.1029/2004JA010918.
8. Fisk, L. A. (1996), Motion of the footpoints of heliospheric magnetic field lines at the Sun: Implications for recurrent energetic particle events at high heliographic latitudes, J. Geophys. Res., 101, 15, 549.
9. Fisk, L. A. (2005), The open magnetic flux of the Sun 1: Transport by reconnections with coronal loops, Astrophys. J., 626, 563.
10. Fisk, L. A., and N. A. Schwadron (2001), The behavior of the open magnetic field of the Sun, Astrophys. J., 560, 425.
11. Fisk, L. A., T. H. Zurbuchen, and N. A. Schwadron (1999), On the corona magnetic field: Consequences of large-scale motions, Astrophys. J., 521, 868.
12. Handy, B. N., and C. J. Schrijver (2001), On the evolution of the solar photosphere and coronal magnetic field, Astrophys. J., 547, 1100.
13. Geiss, J., et al. (1995), The southern high-speed stream - Results from the SWICS instrument on ULYSSES, Science, 268, 1033.
14. Jokipii, J. R., and E. N. Parker (1969), Random walk of magnetic lines of force in astrophysics, Phys. Rev. Lett., 21, 44.
15. Kahler, S. W., and H. S. Hudson (2001), Origin and development of transient coronal holes, J. Geophys. Res., 106, 29, 239.
16. Kohl, J. L., et al. (1999), EUV spectral line profiles in polar coronal holes from 1.3 to 3.0 R_solar, Astrophys. J., 510, L59.
17. Leighton, R. B. (1964), Transport of magnetic fields on the Sun, Astrophys. J., 140, 1547.
18. Luhmann, J. O., Y. Yi, C. N. Arge, P. R. Gazis, and R. Ulrich (2002), Solar cycle changes in coronal holes and space weather cycles, J. Geophys. Res., 107(A8), 1154, doi: 10.1029/2001JA007550.
19. Miralles, M. P., S. R. Cranmer, A. V. Panasyuk, M. Romoli, and J. L. Kohl (2001), Comparison of empirical models for polar and equatorial coronal holes, Astrophys. J., 549, L257.
20. Mitchell, D. G., E. C. Roelof, and J. H. Wolfe (1981), Latitude dependence of solar wind velocity observed at not less than 1 AU, J. Geophys. Res., 86, 165.
21. Neugebauer, M., and P. C. Liewer (2003), Creation and destruction of transitory coronal holes and their fast solar wind streams, J. Geophys. Res., 108(A1), 1013, doi:10.1029/2002JA009326.
22. Neugebauer, M., P. C. Liewer, E. J. Smith, R. M. Skoug, and T. H. Zurbuchen (2002), Sources of the solar wind at solar activity maximum, J. Geophys. Res., 107(A12), 1488, doi:10.1029/2001JA000306.
23. Paesold, G., A. O. Benz, K.-L. Klein, and N. Vilmer (2001), Spatial analysis of solar type III events associated with narrow band spikes at metric wavelengths, Astron. Astrophys., 371, 333.
24. Pan, L.-D., R. P. Lin, and S. R. Kane (1984), Comparison of solar flare X-ray producing'and escaping electrons from about 2 keV to 100 keV, Sol. Phys., 91, 345.
25. Raymond, J. C., R. Suleiman, and J. L. Kohl (1998), Elemental abundance in coronal structures, Space Sci. Rev., 85, 283.
26. Reames, D. V. (1999), Particle acceleration at the Sun and in the heliosphere, Space Sci. Rev., 90, 413.
27. Reames, D. V. (2002), Magnetic topology of impulsive and gradual solar energetic particle events, Astrophys. J., 571, L63.
28. Schatten, K. H., J. M. Wilcox, and N. F. Ness (1969), A model of interplanetary and coronal magnetic fields, Sol. Phys., 6, 442.
29. Schrijver, C. J. (2001), Simulations of the photospheric magnetic activity and outer atmospheric radiative losses of cool stars based on characteristics of the solar magnetic field, Astrophys. J., 547, 475.
30. Schrijver, C. J., and M. L. DeRosa (2003), Photospheric and heliospheric magnetic fields, Sol. Phys., 212, 165.
31. Schrijver, C. J., and A. M. Title (2001), On the formation of polar spots in Sun-like stars, Astrophys. J., 551, 1099.
32. Schrijver, C. J., A. M. Title, A. A. van Ballegooijen, H. J. Hagenaar, and R. A. Shine (1997), Sustaining the quiet photospheric network: The balance of flux emergence, fragmentation, merging and cancellation, Astrophys. J., 487, 424.
33. Schrijver, C. J., A. M. Title, K. L. Harvey, N. R. Sheeley Jr., Y. M. Wang, G. H. J. van den Oord, R. A. D. Shine, T. Tarbell, and N. E. Hurlburt (1998), Large-scale coronal heating by small-scale magnetic field at the Sun, Nature, 394, 152.
34. Schrijver, C. J., M. L. DeRosa, and A. M. Title (2002), What is missing from our understanding of long-term solar and heliospheric activity?, Astrophys J., 577, 1006.
35. Schwerin, R. (1990), Large-scale structure in the interplanetary medium, in Physics of the Inner Heliosphere I, edited by R. Schwenn and E. Marsch, p. 99, Springer, New York.
36. Simon, G. W., A. M. Title, and N. O. Weiss (2001), Sustaining the Sun's magnetic network with emerging bipoles, Astrophys. J., 561, 427.
37. Wang, Y.-M., and N. R. Sheeley Jr. (1991), Magnetic flux transport and the Sun's dipole moment: New twists to the Babcock-Leighton model, Astrophys J., 375, 761.
38. Wang, Y.-M., and N. R. Sheeley (1992), On potential field models of the solar corona, Astrophys. J., 392, 310.
39. Wang, Y.-M., and N. R. Sheeley (1995), Solar implications of ULYSSES interplanetary field measurements, Astrophys. J., 447, L143.
40. Wang, Y.-M., A. G. Nash, and N. R. Sheeley Jr. (1989), Magnetic flux transport on the Sun, Science, 245, 712.
41. Wang, Y.-M., J. Lean, and N. R. Sheeley Jr. (2000a), The long-term variation of the Sun's open magnetic flux, Geophys. Res. Lett., 27, 505.
42. Wang, Y.-M., N. R. Sheeley Jr., and J. Lean (2000b), Understanding the evolution of the Sun's open magnetic flux, Geophys. Res. Lett., 27, 621.
43. Woo, R., and S. R. Habbal (2000), Connecting the Sun and the solar wind: Source regions of the fast solar wind observed in interplanetary space, J. Geophys. Res., 105, 12, 667.
44. Zurbuchen, T. H., S. Hefti, L. A. Fisk, G. Gloeckler, and N. A. Schwadron (2000), Magnetic structure of the slow solar wind: Constraints from composition data, J. Geophys. Res., 105, 18, 327.