The true dimensions of interplanetary coronal mass ejections

Advances in Space Research

Volumn 29, Issue 3, 2002, Pages 301-306

  Russell, C T ^a   Mulligan, T ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

GAS DYNAMICS; MAGNETIC FLUX; PLANETS; SPACECRAFT;

MAGNETIC CLOUD;

SPACE RESEARCH;

PLANETARY ATMOSPHERE;

EID: 0036469142     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00588-9     Document Type: Article

References (12)

1. Magnetic loop behind an interplanetary shock: Voyager, Helios, and IMP 8 observations
2. Determining the standoff distance of the bow shock: Mach number dependence and use of models
3. Interplanetary magnetic clouds: Sources, properties, modeling and geomagnetic relationship
4. Magnetic field structure of interplanetary magnetic clouds at 1 AU
5. On the sources of interplanetary shocks at 0.72 AU
6. Relationships between coronal mass ejection speeds from coronagraph images and interplanetary characteristics of associated interplanetary coronal mass ejections
7. Multi-spacecraft modeling of the flux rope structure of interplanetary coronal mass ejections: Cylindrically symmetric versus non-symmetric topologies
8. Intercomparison of NEAR and Wind interplanetary coronal mass ejection observations
9. Inversion studies of magnetic cloud structure of 0.7 AU: Solar cycle variation
10. Hydromagnetic flow around the magnetosphere
11. A three dimensional gas dynamic model for solar wind flow past non axisymmetric magnetospheres: Application to Jupiter and Saturn