A quantitative magnetospheric model derived from spacecraft magnetometer data
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- Type
- article
- Published
- 1975-02-01
- Cited by
- 338
- References
- 35
- OpenAlex
- https://openalex.org/W2039141162
- Semantic Scholar
- https://api.semanticscholar.org/CorpusID:140536256
Keywords
Magnetosphere, Physics, Field line, Solar wind, Geophysics
References
- STRUCTURE OF THE GEOMAGNETIC FIELD AT GREAT DISTANCES FROM THE EARTH.
- Average daily variations in the magnetic field as observed by ATS-5
- A model of the distributed magnetospheric currents
- Motions of charged particles trapped in the Earth's magnetosphere
- Shape of the geomagnetic field solar wind boundary
- Neutral points on the boundary of the closed magnetosphere
- Quiet day magnetic field at ATS 1
- Nightside magnetosphere configuration as obtained from trapped electrons at 1100 kilometers.
- Magnetic field mapping of the inner magnetosphere
- Average and unusual locations of the Earth's magnetopause and bow shock
- A magnetospheric field model incorporating the OGO 3 and 5 magnetic field observations
- Bow shock associated waves observed in the far upstream interplanetary medium
- Quiet time magnetospheric field depression at 2.3–3.6 RE
- Standing waves at low Mach number laminar bow shocks. [earth-solar wind interaction
- A quantitative model of the magnetospheric magnetic field
- Perturbation of the Geomagnetic Field - a Spherical Harmonic Expansion
- The compressed geomagnetic field as a function of dipole tilt
- Average magnetic field configuration of the outer magnetosphere.
- IMP 5 magnetic field measurements in the high latitude outer magnetosphere near the noon meridian
- Adiabatic motion of auroral particles in a model of the electric and magnetic fields surrounding the Earth
Cited by
- Physical Limitations of Empirical Field Models: Force Balance and Plasma Pressure
- Modelling cosmic ray ground levelenhancements
- Investigation of ring current/storm dynamics
- The association between VLF and ELF chorus emissions and electron precipitation.
- Simultaneous polar cap and magnetotail observations of intense polar rain. [precipitation of low-energy electrons
- Modification of the magnetospheric plasma in outside of the noon meridional plane due to ponderomotive forces by ion–cyclotron waves
- Electric field measurements across the harang discontinuity. [of the auroral zone
- Energy Transfer via Solar Wind Driven Ultra Low Frequency Waves in the Earth's Magnetosphere
- Comparison of equatorial plasma mass densities deduced from field line resonances observed at ground for dipole and IGRF models
- An Overview and Discussion of SPENVIS, ESA's Space Environment Information System, and UNILIB, a Fortran Library of Magnetic Field Utilities
- The Importance of Adiabatic Variations in Trapped Particle Distribution Observed by the SCATHA Satellite
- Quantitative models of the magnetospheric magnetic field: Methods and results
- An analytic model of toroidal half‐wave oscillations: Implication on plasma density estimates
- Conditions of excitation of magnetospheric convection by the electric current generated in the bow shock
- Numerical Simulation of the Ring Current: Review
- A model of the cislunar magnetospheric field
- Further evidence for the role of magnetotail current shape in substorm initiation
- Global energy transfer during a magnetospheric field line resonance
- A forecasting model of the magnetosphere driven by an optimal solar wind coupling function
- Global configuration of Saturn's magnetic field derived from observations
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