Modeling the heliosphere: Influence of the interstellar magnetic field in the presence of Lism neutral hydrogen

Advances in Space Research

Volumn 29, Issue 3, 2002, Pages 433-438

  Ratkiewicz, R ^a   Barnes, A ^b   Muller H R ^c   Zank, G P ^c   Webb, G M ^d  

^a Polish Academy of Sciences   (Poland)

^b NASA AMES RESEARCH CENTER   (United States)

^c UNIVERSITY OF DELAWARE   (United States)

^d UNIVERSITY OF ARIZONA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

HYDROGEN; PARAMETER ESTIMATION;

HELIOSPHERE;

MAGNETIC FIELDS;

PLANETARY ATMOSPHERE;

EID: 0036468349     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00608-1     Document Type: Article

References (18)

1. Effect of local interstellar medium hydrogen fractional ionization on the distant solar wind and interface region
2. On the distribution function of H Atoms in the problem of the solar wind interaction with the local interstellar medium
3. Far-ultraviolet echoes from the frontier between the solar wind and the local interstellar cloud
4. Heliosphere in the magnetized local interstellar medium: Results of a three-dimensional MHD simulation
5. Simulation of the heliosphere: Model
6. Interaction of the solar wind with the local interstellar medium
7. Solar wind - Local interstellar medium interaction including charge exchange with neutral hydrogen
8. Interaction of a nonuniform solar wind with the local interstellar medium
9. Interaction of a nonuniform solar wind with the local interstellar medium. 2. A two-fluid model
10. Influence of the interstellar magnetic field direction on the shape of the global heliopause
11. The intrinsic properties of the local interstellar medium
12. Effect of varying strength and orientation of local interstellar magnetic field on configuration of exterior heliosphere: 3D MHD simulations
13. Local interstellar medium and modeling the heliosphere
14. 3-D magnetic field and current system in the heliosphere
15. MHD structure of the outer heliosphere - For the study of the tail-in anisotropy of the cosmic ray
16. The heliospheric hydrogen distribution: A multi-fluid model
17. Interaction of the solar wind with the local interstellar medium: A theoretical perspective
18. Interaction of the solar wind with the local interstellar medium: A multifluid approach