Three-dimensional MHD simulation for the solar wind structure observed by Ulysses

Chinese Science Bulletin

Volumn 46, Issue 16, 2001, Pages 1352-1355

  Shi, Y ^a   Wei, F ^a   Feng, X ^a   Ye, Z ^a  

^a CENTER FOR SPACE SCIENCE AND APPLIED RESEARCH   (China)

Author keywords

Numerical simulation; Solar wind structure; Ulysses

Indexed keywords

ARTICLE; DENSITY; MAGNETIC FIELD; OBSERVATION; POLARIZATION; SIMULATION; SUN; VELOCITY;

EID: 0034811642     PISSN: 10016538     EISSN: None     Source Type: Journal    
DOI: 10.1007/BF03183386     Document Type: Article

References (11)

1. Ulysses observations from pole-to-pole: An introduction
2. Ulysses observations and discussions of acceleration mechanisms for the solar wind
3. Ulysses solar wind plasma observations from pole to pole
4. Ulysses observations of the radial magnetic field
5. Source of shocks and compressions in the high-latitude solar wind: Ulysses
6. The underlying magnetic field direction in Ulysses observations of the southern polar heliosphere
7. A three-dimensional, time-dependent numerical modeling of super-sonic, super-Alfvenic MHD flow
8. The structure of the heliospheric current sheet: 1978-1982
9. A study of the background corona near solar minimum
10. A global numerical 3-D MHD model of the solar wind
11. Three-dimensional MHD simulation of the Apr. 14, 1994, interplanetary coronal mass ejection and its propagation to the Earth and Ulysess