Evolution of coronal streamer structure during the rising phase of solar cycle 23

Geophysical Research Letters

Volumn 27, Issue 2, 2000, Pages 149-152

  Wang, Y M ^a   Sheeley, N R ^a   Rich, N B ^b  

^a NAVAL RESEARCH LABORATORY   (United States)

^b INTERFEROMETRICS INC   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

SOLAR CYCLE;

ELECTRON SCATTERING; MAGNETIC FLUX; SUN;

CORONAL STREAMERS; HELIOSPHERIC CURRENT SHEETS; SOLAR CYCLE; THOMSON-SCATTERING ELECTRONS;

SOLAR RADIATION;

EID: 0034353497     PISSN: 00948276     EISSN: None     Source Type: Journal    
DOI: 10.1029/1999GL010698     Document Type: Article

References (12)

1. The large angle spectroscopic coronagraph (LASCO)
2. Quadrupole distortions of the heliospheric current sheet in 1976 and 1977
3. Structure of the heliospheric current sheet in the early portion of sunspot cycle 21
4. Observation of sectored structure in the outer solar corona: Correlation with interplanetary magnetic field
5. The shape of the outer corona during cycle 21
6. Current sheet magnetic model for the solar corona
7. A model of interplanetary and coronal magnetic fields
8. Evolution of the Sun's polar fields during sunspot cycle 21: Poleward surges and long-term behavior
9. On potential field models of the solar corona
10. Origin and evolution of coronal streamer structure during the 1996 minimum activity phase
11. Origin of streamer material in the outer corona