A V-shaped gutter on the nose-cone surface of the heliopause caused by MHD processes

Advances in Space Research

Volumn 27, Issue 3, 2001, Pages 509-515

  Washimi, H ^a   Tanaka, T ^b  

^a SHONAN INSTITUTE OF TECHNOLOGY   (Japan)

^b NATIONAL INSTITUTE OF INFORMATION AND COMMUNICATIONS TECHNOLOGY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; HELIOGRAPHS; NOSE CONES;

SOLAR WIND PLASMAS; V-SHAPED GUTTERS;

MAGNETOHYDRODYNAMICS;

COSMIC RAY;

EID: 0034911496     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00079-5     Document Type: Article

References (10)

1. The interaction of the solar wind with the interstellar medium
2. Interaction between the solar wind and the interstellar medium
3. Heliosphere in the magnetized loal interstellar medium: Results of a three-dimensional MHD simulation
4. Three-dimensional MHD models for the interaction between the solar wind and the interstellar medium
5. Three-dimensional MHD simulation of the solar wind interaction with the ionosphere of Venus: Results of two-component reacting plasma simulation
6. Solar cycle dependence of the heliospheric shape deduced from a global MHD simulation of the interaction process between a nonuniform time-dependent solar wind and the local interstellar medium
7. MHD modeling of the outer heliosphere
8. 3-D magnetic field and current system in the heliosphere