On the global structure of the heliospheric magnetic field
- 1 August 2001
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 106 (A8) , 15849-15857
- https://doi.org/10.1029/2000ja000117
Abstract
No abstract availableKeywords
This publication has 28 references indexed in Scilit:
- Nature of the boundary between open and closed magnetic field line regions at the Sun revealed by composition data and numerical modelsJournal of Geophysical Research, 2001
- Acceleration of the fast solar wind by the emergence of new magnetic fluxJournal of Geophysical Research, 1999
- On the Coronal Magnetic Field: Consequences of Large‐Scale MotionsThe Astrophysical Journal, 1999
- Large-scale coronal heating by the small-scale magnetic field of the SunNature, 1998
- Fast and Slow Wind from Solar Coronal HolesThe Astrophysical Journal, 1997
- Motion of the footpoints of heliospheric magnetic field lines at the Sun: Implications for recurrent energetic particle events at high heliographic latitudesJournal of Geophysical Research, 1996
- The underlying magnetic field direction in Ulysses observations of the southern polar heliosphereGeophysical Research Letters, 1995
- Two types of slow solar windThe Astrophysical Journal, 1994
- Corotating particle enhancements out of the ecliptic planeGeophysical Research Letters, 1994
- Understanding the rotation of coronal holesThe Astrophysical Journal, 1993