The interplanetary magnetic field - Solar origin and terrestrial effects.
Spacecraft observations relating to interplanetary magnetic field structure, solar origin and terrestrial effects
Engineering topics
Publications and source records attributed to Wilcox, J. M..
Spacecraft observations relating to interplanetary magnetic field structure, solar origin and terrestrial effects
Motion picture report of IMP-1 magnetometer observations of interplanetary magnetic field
Observations related to large-scale structure of interplanetary magnetic field, solar origin, and geomagnetic effects
Solar active region relationship to large scale sector interplanetary field structure
Geomagnetic index response to interplanetary magnetic field
Interplanetary magnetic field sector structure, noting Archimedes spiral directivity and 27 day recurrence period for pattern
Recent observations of solar and interplanetary magnetic fields and plasmas
Mapping interplanetary magnetic field by extrapolating satellite measurements, and sector evolution observations
Interplanetary sector structure observed by IMP-I SATELLITE compared with photospheric magnetic field and plage structure observations
Properties of interplanetary magnetic field observed by IMP-3
Response of geomagnetic activity index to interplanetary magnetic field
Solar magnetograph observation of photospheric brightness, velocity, and magnetic fields
Comparison of satellite interplanetary magnetic field observations with photospheric magnetic field and plage structure
Interplanetary magnetic field and plasma effect on geomagnetic activity during quiet sun conditions
Longitude distribution of solar proton flares as function of recurrence period
Description of movie representing IMP-1 MAGNETOMETER observations of interplanetary magnetic field
Influence of interplanetary magnetic field and plasma on geomagnetic activity during quiet-sun conditions
IMP-1 measurements of interplanetary magnetic field, magnetosphere boundary, and collisionless magnetohydrodynamic shock wave associated with solar wind interaction with geomagnetic field