Polarization of 16-mc-s radiation from jupiter
Polarization of 16-mc/s radiation from jupiter
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Polarization of 16-mc/s radiation from jupiter
Polarized radiation from jupiter at decameter wavelengths
Radio and polarization observations of Jupiter, correlation between Jupiter events and solar M-region storms, and observation comparisons with Doppler shifted cyclotron predictions
Combined observations of Jupiter investigating correlation between planet activity and geomagnetic activity, sunspot number, solar radiation and flares
Catalog of radio observations of Jupiter 1961 to 1964
Short duration pulses association with subsidiary B and C sources of Jovian decametric radiation
Continuum bursty emission from Jupiter at 18 MHz observed using interferometer
Jupiter radiation bursts polarization degree and axial ratio, discussing agreement with Doppler shifted cyclotron theory
Nine lunar models for Apollo project for orbit calculations
Lunar surface perturbation effects on Lunar Orbiter Doppler residuals
Summary of radio observatory activities concentrating on polarization and short time resolution burst structure of radiation
Evaluating various lunar gravitational models for Apollo mission control
Light synchronization of deep body temperature rhythms in Macaca nemestrinas, investigating efficiency
Measuring system requiring one blocking oscillator to generate modulated pulse repetition rate is implantable in the bodies of small animals. Device has life of two years and transmission range of about three feet. EKG sensing unit also is used to sense electromyogram or electrooculogram of laboratory animals.
Review of some radio observations of Jupiter made during three recent apparitions using several receivers, each tuned to a slightly different frequency close to 18 MHz. Sequences of oppositely polarized bursts have been observed and also differences in polarization mode between channels 400 kHz apart. Occasionally, isolated bursts of durations of 1 to 2 sec have been found to show real drifts in frequency, as distinct from the apparent drifts shown by changing intensity across a group of features.
An analysis is presented for the propagation of charged cosmic rays away from a source in a relatively smooth galactic magnetic field. The expected intensity of the resulting narrow-angle anisotropy is related to the particle flux produced by the source. The probable number of such anisotropies is derived, based on the lifetime of cosmic rays and the number of sources in the Galaxy. The agreement with experimental evidence and future possibilities of the model are discussed.