Some observational phenomena are well reproduced by our global MHD while others are not: Remarks on what, why and how

Advances in Space Research

Volumn 28, Issue 12, 2001, Pages 1685-1691

  Janhunen, P ^b   Palmroth, M ^a  

^a FINNISH METEOROLOGICAL INSTITUTE   (Finland)

^b NONE

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETIC FIELDS; MAGNETIC LEAKAGE; MAGNETOHYDRODYNAMICS; MAGNETOSPHERE; NUMERICAL METHODS;

ELLIPTIC SOLVERS; MAGNETOPAUSE;

IONOSPHERE;

MAGNETOSPHERE;

EID: 0035664040     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00533-6     Document Type: Article

References (13)

1. The effect of nonzero ∇ . B on the numerical solution of the magnetohydrodynamic equations
2. GUMICS-3 - A global ionosphere-magnetosphere coupling simulation with high ionospheric resolution
3. The closure of Region-1 field-aligned current in MHD simulation
4. Adaptive mesh in global magnetosphere simulation: Comparison with global convection
5. On the current-voltage relationship in fluid theory
6. A positive conservative method for magnetohydrodynamics based on HLL and Roe methods
7. New model for auroral acceleration: O-shaped potential structure cooperating with waves
8. The connection between transpolar arcs and magnetotail rotation
9. Observations of the electric field fine structure associated with the westward travelling surge and large-scale auroral spirals
10. A solution-adaptive upwind scheme for ideal magnetohydrodynamics
11. A method for enforcing the solenoidal condition on magnetic fields in numerical calculation
12. A new functional form to study the solar wind control of the magnetopause size and shape