Self-consistent simulation of cylindrical magnetic cloud propagation in the heliosphere with its axis both perpendicular to, and lying within, the ecliptic plane

Advances in Space Research

Volumn 17, Issue 4-5, 1996, Pages 327-330

  Vandas, M ^a   Fischer, S ^a   Dryer, M ^b   Smith, Z ^b   Detman, T ^b  

^a ASTRONOMICAL INSTITUTE   (Czech Republic)

^b NOAA EARTH SYSTEM RESEARCH LABORATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0042037785     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/0273-1177(95)00595-6     Document Type: Article

References (6)

1. Physics of Magnetic Flux Ropes
2. Dynamics of aging magnetic clouds
3. Simulation of a magnetic cloud propagation in the inner heliosphere in two-dimensions: 1. A loop perpendicular to the ecliptic plane
4. Non-planar MHD model for solar flare-generated disturbances in the heliospheric equatorial plane
5. A three-dimensional, time-dependent numerical modeling of supersonic, superalfvenic MHD flow
6. Interplanetary studies: Propagation of disturbances between the Sun and the magnetosphere