Modeling the radial variation of coronal streamer belts during sunspot ascending phase

Advances in Space Research

Volumn 29, Issue 3, 2002, Pages 411-416

  Zhao, X P ^a   Hoeksema, J T ^a   Rich, N B ^b  

^a STANFORD UNIVERSITY   (United States)

^b NAVAL RESEARCH LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; MAPS; PARAMETER ESTIMATION;

STREAMER BELTS;

SPACE RESEARCH;

PLANETARY ATMOSPHERE;

EID: 0036468713     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00604-4     Document Type: Article

References (5)

1. The large angle spectroscopic coronagraph (LASCO)
2. Global, quasi-steady dynamics of the distant solar wind. 2. Deformation of the heliospheric current sheet
3. Origin and evolution of coronal streamer structure during the 1996 minimum activity phase
4. Prediction of the interplanetary magnetic field strength
5. Modeling magnetic polarity structures of the heliosphere