The solar radial gradient of galactic cosmic rays.
Steady solar radial gradient of galactic cosmic ray intensity in interplanetary region noting convection, diffusion, energy losses and differential streaming
Engineering topics
Publications and source records attributed to Axford, W. I..
Steady solar radial gradient of galactic cosmic ray intensity in interplanetary region noting convection, diffusion, energy losses and differential streaming
Stellar wind model taking into account recombination of ionized hydrogen, noting applications to nonexpanding planetary nebulas
Normal ionizing shock wave structure in argon, integrating shock equation for simple model
Longitudinal plasma oscillations, approximating electric field and distribution function
Extended radio sources confinement through suggested dynamic process permitting intergalactic medium density deduction possibility
Solar wind interaction with magnetosphere, energy dissipation during magnetic storms and magnetic energy conversion in magnetospheric tail
Ionization fronts stability, finding no instabilities for strong D type fronts
Streaming and spatial gradient equations of cosmic ray particles in interplanetary medium model, discussing Fokker-Planck equation and heliocentric field modulation
Head-on collision between stars at high initial relative velocity, considering one-dimensional driven shock motion in inhomogeneous medium
Satellite observations made by two or more satellites simultaneously on interplanetary medium
Closed form solution expressing transonic flow in idealized stellar wind and spherical accretion problems including viscosity and thermoconductivity effects
Electron and ion temperature changes in sporadic E layer based on wind shear theory, using energy equation
Wind shear theory of formation of temperate zone blanketing sporadic E layers, noting motion equation for ions in ionospheric E region
Auroral and polar magnetic substorms related to magnetic field lines reconnection in magnetosphere tail
Shock waves in interplanetary medium caused by sudden expansion of solar corona following flare
Geomagnetic field variations in temperate zone sporadic E layer according to wind-shear theory
Magnetic storm effects associated with tail of magnetosphere
Intensity and spectra of cosmic ray electrons and positrons in determining mean confinement time, density and solar modulation