Streamer evaporation

Space Science Reviews

Volumn 87, Issue 1-2, 1999, Pages 323-326

  Suess, S T ^a   Wang, A H ^b   Wu, S T ^b   Nerney, S F ^c  

^a NASA MARSHALL SPACE FLIGHT CENTER   (United States)

^b UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^c OHIO UNIVERSITY   (United States)

Author keywords

Corona; Magnetohydrodynamics; Streamers

Indexed keywords

EID: 0042377743     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005149929192     Document Type: Article

References (7)

1. Li, J., et al.: 1998, 'Physical Structure of a Coronal Streamer in the Closed-Field Region as Observer from UVCS/SOHO and SXT/Yohkoh,' Ap. J., 506, 431.
2. Low, B. C.: 1996, 'Solar Activity and the Corona,' Sol. Phys., 167, 217.
3. Pneuman, G.: 1968, 'Some General Properties of Helmeted Coronal Structures,' Sol. Phys., 3, 578.
4. Priest, E. R., et al.: 1998, 'Nature of the Heating Mechanism for the Diffuse Solar Corona,' Nature, 393, 545.
5. Steinolfson, R. S.: 1988, 'Density and White-Light Brightness in Looplike Coronal Mass Ejections: Importance of the Preevent Atmosphere,' J. Geophys. Res., 93, 14261.
6. Steinolfson, R. S., Suess, S. T., and Wu, S. T.: 1982, 'The Steady Global Corona,' Ap. J., 255, 730.
7. Wang, A.-H., Wu, S. T., Suess, S. T., and Poletto, G.: 1998, 'Global Model of the Corona with Heat and Momentum Addition,' J. Geophys. Res., 103, 1913.