Interrelationship of cosmic-ray anisotropies and the interplanetary magnetic field.
Cosmic ray anisotropy direction during solar proton events compared with concurrent interplanetary magnetic field vector direction, using Pioneer 6 data
Engineering topics
Publications and source records attributed to Ness, N. F..
Cosmic ray anisotropy direction during solar proton events compared with concurrent interplanetary magnetic field vector direction, using Pioneer 6 data
Interplanetary magnetic field perturbations by lunar wake using plasma flow model
Model of interplanetary and solar magnetic field structure above photosphere using Green function solution to Maxwell equations
Interplanetary magnetic field radial gradients between 0.81 and 1.0 AU noting microstructure, mesostructure, macrostructure and directional distribution of discontinuities
Lunar Explorer 35 measurements of solar wind, interplanetary and lunar magnetic fields, cosmic dust, energetic particles, and electromagnetic properties of lunar surface
Explorer 33 and Explorer 35 measurements of perturbed interplanetary magnetic field in lunar wake
Critical review of argument by Fredericks et al concerning ambiguity of IMP 1 data obtained from tilted spinning fluxgate magnetometers
Data from simultaneous measurements of magnetic field and electron component of plasma in near geomagnetic tail during Pioneer 7 passage
Geomagnetics from beginning to current concepts of solar wind and earth shock waves and radiation belts
Motion picture report of IMP-1 magnetometer observations of interplanetary magnetic field
Perturbations of interplanetary magnetic field by lunar wake compared with disturbed solar plasma flow
Solar active region relationship to large scale sector interplanetary field structure
Interplanetary plasma properties, discussing measurement, sector structure, corotation and microstructure
Structure, temporal behavior, shape and length of earth magnetic tail via satellite mapping
Selenocentric orbit magnetic field measurements with Explorer 35 noting negative results on magnetosphere and bow shock wave
Inter relationship of cosmic ray anisotropies and interplanetary magnetic field
Solar wind proton velocity distribution functions obtained by satellite observation
Interplanetary magnetic field sector structure, noting Archimedes spiral directivity and 27 day recurrence period for pattern