Two-fluid model of the solar wind.
Solar wind studied with two fluid model, using proton and electron fluid type heat equations, equation of motion and continuity equation
Engineering topics
Publications and source records attributed to Sturrock, P. A..
Solar wind studied with two fluid model, using proton and electron fluid type heat equations, equation of motion and continuity equation
Stochastic acceleration, diffusion and scattering by weak random electromagnetic fields using Fokker-Planck equation, detailing relativistic particles
Collisionless plasma heating by random magnetic fields using simple betatron model
Evidence for particle acceleration on galactic scale based on radio galaxies observations and radio emission from quasars
Plasma model of quasars and radio galaxies for observations of high energy radiation
Theoretical model for quasars characterizes them as galactic flares, based on study of high energy phenomena associated with solar flares
Two-fluid model of solar wind, assuming spherical symmetric flow without rotation, magnetic fields or viscous stress
Explosive and nonexplosive onsets of instability by nonlinear analysis
Stochastic acceleration of charged particles in randomly time-varying electromagnetic fields
Models that treat events associated with quasi-stellar objects as plasma phenomena
Shock waves in solar wind and magnetic storms, deriving equations governing shock, ambient and driver gas velocities
Coupling of electrostatic waves with electromagnetic waves in plasma leading to radiation from plasma oscillations
Shock waves in solar wind and geomagnetic storms
Local plasma resonances in magnetic field - Alouette Topside Sounder
Dipole resonances of homogeneous plasma in magnetic field