The mechanism for reconnection of geomagnetic and interplanetary field lines
Mechanism for reconnection of geomagnetic and interplanetary field lines
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Mechanism for reconnection of geomagnetic and interplanetary field lines
Influence of interplanetary magnetic field and plasma on geomagnetic activity during quiet-sun conditions
History of Mariner space program and discussion of future unmanned vehicles for exploration of interplanetary space
Observations of interplanetary magnetic field by Mariner and Imp spacecraft confirm predictions based on behavior of cosmic rays
Interplanetary dust particles, size distribution, mass density, structure and shape
Comparison of interplanetary magnetic field measurements made by Imp-I satellite and those obtained with solar magnetograph at Mount Wilson
Earth departure plane change, interplanetary mission launches and launch windows
Space probe observations of solar wind, solar magnetic field and interplanetary magnetic field
Interplanetary spacecraft telecommunications system design including block diagrams
Comparison of magnetic and cosmic ray data of Pioneer VI with particle guidance properties of interplanetary magnetic field
Mariner IV observation of 500-kev protons in interplanetary space
Interplanetary plasma stream analysis using bistatic radar transmissions, considering wave propagation in presence of uniform magnetic field, stream velocity, Faraday rotation, etc
Detection and measurement techniques for collisionless MHD shock wave propagation in interplanetary space, using bistatic-radar Earth- to-spacecraft transmissions
Variations in polarity distribution of interplanetary magnetic field from observations by Mariner II and IV and IMP I
Solar flare electron propagation observations in interplanetary space
Correction of magnetic measurements made by Mariner II, noting use of second-order approximation for interplanetary magnetic field
Collision-free hydromagnetic shock observed simultaneously in interplanetary space on October 7, 1962 by Mariner II and Explorer XIV
Collimation of cosmic rays by interplanetary magnetic field based on Pioneer VI measurements during flare event