Prediction of geomagnetic secular change confirmed.
Geomagnetic field model /POGO/ to confirm eccentric dipole westward velocity secular decrease predicted by day length changes
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Geomagnetic field model /POGO/ to confirm eccentric dipole westward velocity secular decrease predicted by day length changes
Venus atmosphere structure determined from Mariner 5 flyby S band radio occultation measurements of ionosphere and atmosphere at illuminated and dark sides
Magnetic dip equator position at E layer and gradient with time and altitude, using geomagnetic field models
Determining entrainment of entrapped liquid as function of air flow, and viscosity
Geomagnetic survey data reduction results by polar orbiters OGO-2 and OGO-4
Observatory calculations of hourly values of equatorial Dst for 1968
Coding techniques for digital communication channels
Hourly values of equatorial storm time variation as function of solar wind pressure on boundary of magnetosphere
Literature survey on geomagnetic modeling from satellite magnetic survey data
S band occultation experiment for Mariner Mars 1971 orbiters, measuring atmospheric density and ionospheric electron density profiles
Proton magnetometer measurements from satellite Cosmos 49, observing residual and broad magnetic anomalies
Inner magnetosphere magnetic field mapping, deriving Pogo model
Solar limb photographic, isodensity and isophotal data for eclipse of 7 March 1970 from coronagraph observations, noting coronal green line and prominence activity
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Evaluating slurry compaction process for fabrication of metal matrix composites
Provisional hourly values of equatorial Dst for 1968
Error correction coding/decoding techniques integration, discussing convolutional and block coding and Viterbi, Sequential and Threshold decoding algorithms
Geomagnetic field models validity from satellite data