The generation of magnetic fields in astrophysical bodies. VIII - Dynamical considerations
Milky Way galaxy poloidal magnetic field generation with hydromagnetic dynamos, showing galactic cosmic rays as major driving force
Parker, E. N.↗
Engineering topics
Parker, E. N.
Publications and source records attributed to Parker, E. N..
Recent developments in theory of solar wind
Solar wind theory, discussing thermal conduction and MHD wave energy supply mechanisms of large scale solar corona expansion
Parker, E. N.↗
The generation of magnetic fields in astrophysical bodies. VI - Periodic modes of the galactic field
Galactic dynamo generated magnetic field periodic modes based on mathematical model involving cyclonic turbulence and nonuniform rotation of gaseous disk
Parker, E. N.↗
The generation of magnetic fields in astrophysical bodies. V - Behavior at large dynamo numbers
Astrophysical objects magnetic field generation, examining behavior at large dynamo numbers
Parker, E. N.↗
The generation of magnetic fields in astrophysical bodies. IV - The solar and terrestrial dynamos
Earth and sun magnetic field production models as function of dynamo states, discussing solar field effects on terrestrial space environment
Parker, E. N.↗
Magnetic fields in astrophysics
Terrestrial, solar and galactic magnetic fields, discussing generation by combined nonuniform rotation and cyclonic turbulence based on dynamo equation
Parker, E. N.↗
The generation of magnetic fields in astrophysical bodies. II - The galactic field
Galactic magnetic field generation by dynamo process with nonuniform rotation and turbulence in gaseous disk
Parker, E. N.↗
The generation of magnetic fields in astrophysical bodies. III - Turbulent diffusion of fields and efficient dynamos
Galaxy gaseous disk as low mode dynamo, calculating turbulent diffusion coefficient for passive magnetic fields
Parker, E. N.↗
On the convection, diffusion, and adiabatic deceleration of cosmic rays in the solar wind
Cosmic ray transport in solar wind generalized with anisotropic diffusion approximation
Jokipii, J. R.↗
The origin of solar magnetic fields
Solar magnetic field origin and behavior, discussing hydromagnetic dynamos, cyclonic convection and generation times
Parker, E. N.↗
The origin and dynamical effects of the magnetic fields and cosmic rays in the disk of the Galaxy
Galactic magnetic fields and cosmic ray gas, investigating origin and dynamical effects
Parker, E. N.↗
The occasional reversal of the geomagnetic field
Cyclonic convective cell fluctuation and nonuniform core rotation effects on reversal of geomagnetic field, investigating fossil magnetism
Parker, E. N.↗
Amplification of weak magnetic fields in turbulent flow.
Weak magnetic field amplification in turbulent flow with velocity field as random function of space and time
Parker, E. N.↗
Origin of the magnetic field of the Galaxy.
Galactic magnetic field origin from galactic turbulence, calculating individual Fourier components in random turbulent velocity
Parker, E. N.↗
Physical model of hydrodynamic turbulence.
Model for statistically isotropic homogeneous turbulence in incompressible fluid, representing turbulence as superposition of individual vortex sheets
Parker, E. N.↗
Galactic effects of the cosmic-ray gas
Cosmic ray gas galactic effects, discussing galactic magnetic field, hydromagnetic wave propagation, etc
Parker, E. N.↗
Solar wind interaction with the geomagnetic field.
Solar wind interaction with geomagnetic field, considering bow shock, field confinement in magnetosphere and stretching out of lines of force
Parker, E. N.↗
Theoretical studies of the solar wind phenomenon.
Solar wind phenomenon, discussing angular momentum loss to sun, fluctuations at earth orbit and wind conditions at terminus and regions unvisited by spacecraft
Parker, E. N.↗