How to address the accuracy of empirical magnetic field models?

Advances in Space Research

Volumn 28, Issue 12, 2001, Pages 1717-1726

  Pulkkinen, T I ^a  

^a FINNISH METEOROLOGICAL INSTITUTE   (Finland)

Author keywords

[No Author keywords available]

Indexed keywords

MAGNETOHYDRODYNAMICS; SPACECRAFT; SUN; WIND;

BEST-FIT FIELDS;

MAGNETIC FIELDS;

MAGNETIC FIELD; MAGNETOSPHERE;

EID: 0035664041     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00537-3     Document Type: Article

References (13)

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2. Topological structure of the magnetotail as a function of interplanetary magnetic field direction
3. Hybrid input algorithm - Possibility to get a realistic event-oriented magnetospheric model
4. Mapping of the ionospheric field-aligned currents to the equatorial magnetosphere
5. Particle scattering and current sheet stability in the geomagnetic tail during the substorm growth phase
6. Two substorm intensifications compared: Onset, expansion, and global consequences
7. Magnetotail currents during the growth phase and local auroral breakup
8. Testing the isotropic boundary algorithm method to evaluate the magnetic field configuration in the tail
9. An observational test of the Tsyganenko (T89a) model of the magnetospheric field
10. Magnetospheric magnetic field model with a warped tail current sheet
11. Quantitative models of the magnetospheric magnetic field: Methods and results
12. Modeling the Earth's magnetospheric magnetic field confined within a realistic magnetopause
13. MHD simulation of the magnetotail during the December 10, 1996 substorm