Predicting the heliospheric magnetic field using the current sheet-source surface model

Advances in Space Research

Volumn 16, Issue 9, 1995, Pages 181-184

  Zhao, X ^a   Hoeksema, J T ^a  

^a STANFORD UNIVERSITY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0013286516     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00331-8     Document Type: Article

References (16)

1. The three-dimensional structure of magnetostatic atmospheres. II - Modeling the large-scale corona
2. A model of interplanetary and coronal magnetic fields
3. The solar origin of long-term variations of the interplanetary magnetic field strength
4. Disappearance of the heliospheric sector structure at Ulysses
5. Ulysses at 50° south: constant immersion in the high-speed solar wind
6. Organization of solar wind plasma properties in a tilted, heliomagnetic coordinate system