Laboratory experiments related to the solar wind and the magnetosphere.
Laboratory models for solar wind and magnetosphere interactions with similarity laws of Vlasov theory as reference system
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Laboratory models for solar wind and magnetosphere interactions with similarity laws of Vlasov theory as reference system
Quantitative magnetic field models of magnetosphere for analyzing field configuration variations and adiabatic particle motion
Dynamics of magnetosphere, discussing auroral oval position, ring currents, plasma density and magnetic field variations in near polar region
Charged particle population dynamics in outer radiation zone of magnetosphere, discussing ring current particles, protons, electrons, alpha particles and electric field
LF wave propagation and emission in magnetosphere, discussing steady noise and discrete emissions
Low energy plasma fluxes in magnetosphere, discussing plasmapause position dependence on geomagnetic activity
Magnetospheric plasma instabilities, discussing pitch angle diffusion instabilities, auroral precipitation boundary location, radial diffusion and maximum dissipation limit
Solar wind induced magnetospheric convection for interpretation of geomagnetic storms, aurora and trapped particle belts, noting electric fields
Magnetosphere model for plasma pressure by solar wind, discussing plasma drift from neutral sheet into geomagnetic tail
Magnetospheric field configuration in midnight meridian, considering cavity boundary surface and trapping region currents and tail sheet current
Time dependent convection electric fields as agents for diffusing trapped magnetospheric radiation inward toward earth, discussing one dimensional diffusion equation
Banded chorus, VLF discrete emissions in magnetosphere in single variable frequency band with frequency depending on equatorial electron gyrofrequency
Low energy solar protons entry into magnetosphere on 26 May 1967 showing diffusion control
Radial diffusion coefficient calculation in presence of magnetic shell splitting in magnetosphere
Venus magnetosphere induced by piling up magnetic field from solar wind due to ionospheric conductivity and collisions with planetary atmospheric particles
High latitude magnetospheric convection patterns determined from ionospheric current distribution using magnetic disturbance plots
Polar upper atmospheric phenomena interpreted as magnetospheric substorm manifestations, discussing role of asymmetric ring current formation
Drift shell splitting in nondipolar distorted magnetosphere tested with data from electron spectrometer on ATS 1 and OGO 3 satellites