Engineering topics

Parker, E. N.

Publications and source records attributed to Parker, E. N..

At least 181 records · Page 10

All sources NASA NTRS DOE OSTI

NASA NTRS1964

A mechanism for magnetic enhancement of sound- wave generation and the dynamical origin of spicules.

Magnetic enhancement of sound wave generation and application to dynamical origin of spicules

SOLAR MAGNETIC FIELD↗

NASA NTRS1964

Theory of streaming of cosmic rays and the diurnal variation.

Charged particle motion in magnetic field investigated to understand net streaming of cosmic rays through interplanetary space leading to diurnal variation

PARTICLE MOTION↗

NASA NTRS1964

The perturbation of interplanetary dust grains by the solar wind.

Secular perturbation in orbital motion of interplanetary dust grains due to lorentz force exerted by magnetic field carried in solar wind

LORENTZ FORCE↗

NASA NTRS1964

Dynamical properties of stellar coronas and stellar winds. iii. the dynamics of coronal streamers

Filamentary structure of solar corona and effect on dynamics of solar wind

CORONA↗

NASA NTRS1964

Dynamical properties of stellar coronas and stellar winds. iii - the dynamics of coronal streamers.

Solar corona dynamics study indicates that solar wind velocity is not greatly affected by filamentary structure for given coronal temperature distribution

SOLAR WIND↗

NASA NTRS1964

Dynamical Properties of Stellar Coronas and Stellar Winds. 1. Integration of the Momentum Equation

Hydrodynamics of stellar coronas and winds - integration of momentum equation

CORONA↗

NASA NTRS1964

Comments on understanding the solar flare

Nature of solar flares - magnetic field energy source and prediction of flare occurrence

MAGNETIC FIELD↗

NASA NTRS1964

Dynamical properties of stellar coronas and stellar winds. i - integration of the momentum equation.

Stationary hydrodynamic expansion of spherical stellar corona, studied from integrated hydrodynamic momentum and mass conservation equations

CORONA↗

NASA NTRS1963

Dynamical properties of stellar coronas and stellar winds. 11equal integration of the heat-flow equation

Dynamic properties of stellar coronas & stellar winds and integration of heat-flow equation

HEAT FLOW↗

NASA NTRS1963

THE SOLAR FLARE PHENOMENON AND THE THEORY OF RECONNECTION AND ANNIHILATION OF MAGNETIC FIELDS

Solar flare phenomenon and theory of reconnection and annihilation of magnetic fields

SOLAR FLARE↗

NASA NTRS1963

A KINEMATICAL THEORY OF TURBULENT HYDROMAGNETIC FIELDS

Kinematical theory for magnetic fields produced by interaction of turbulent eddies with large-scale weak magnetic field in photosphere

TURBULENCE↗

NASA NTRS1963

THE THEORY OF THE SOLAR WIND

Theory of the solar wind considering the simple case of solar corona composed solely of ionized hydrogen with spherical symmetry about the center of the sun

SOLAR WIND↗

NASA NTRS1963