The dynamical state of the interstellar gas and field.
Dynamical requirements for existence of interstellar magnetic field in solar neighborhood
Engineering topics
Publications and source records attributed to Parker, E. N..
Dynamical requirements for existence of interstellar magnetic field in solar neighborhood
Nonrelativistic equations of bulk motion of relativistic /cosmic ray/ gas derived by taking moments of collisionless Boltzmann equation
Proton energy density, pressure and compressibility of galactic cosmic ray gas
Properties of nonsymmetric inflation of dipole magnetic field by ionized gas
Adiabatic deceleration effect on cosmic ray spectrum, noting particle momentum and energy change, diffusion coefficient independent of energy, etc
Penetration of interstellar cosmic rays into solar system
Stability of expanding corona against radial compressional waves
Cosmic ray modulation by solar wind fields noting transit time, energy loss and time variations
Dynamical behavior of cosmic ray gases, noting modes of hydromagnetic wave propagation and static equilibrium configurations for thermal interstellar gas and field
General dynamical effects of suprathermal gas particles on hydromagnetic wave propagation in interstellar space
Dynamical properties of solar wind and solar corona atmosphere with extended temperature bound strongly by gravity
Cosmic rays leading to inflation of galactic magnetic fields produce halo of cosmic rays and field around galaxy
Stationary stellar corona energy supplied by thermal conduction from base surrounded by cold vacuum
Interstellar gas-cosmic radiation relationship for inflation of galactic magnetic field and halo production around galaxy
Cosmic ray and energetic solar particle passage through interplanetary space based on idealized examples
Adiabatic deceleration of cosmic rays in quiet-day solar wind and particle momentum and energy loss
Pressure and sound velocity determined for statistically isotropic homogeneous cosmic ray gas