Add to ORKGThe purpose of this project was to conduct a comprehensive investigation of the radio wave emission observed by the planetary radio astronomy (PRA) instrument on board Voyager 2 as it flew by Neptune. The study has included data analysis, theoretical and numerical calculations, and ray tracing to determine the possible source mechanisms and locations of the radiation, including the narrowband bursty and smooth components of the Neptune radio emission
Abstract Nonthermal radio bursts in the interplanetary medium indicate the far-reaching effect of so...
This grant was for the analysis and interpretation of data obtained by the cosmic ray system (CRS) o...
The Voyager 1 and Voyager 2 Planetary Radio Astronomy Experiments (PRA) have produced the finest set...
Progress under this grant has included identifying certain new radio emission components and determi...
Analysis of nonthermal radio emission data obtained by the Planetary Radio Astronomy (PRA) spectrome...
For more than thirty years the intense decametric radio emissions from Jupiter (DAM) and the corresp...
During the Voyager 2 flyby of Neptune, a series of 16 whistler-like events were detected by the plas...
Smooth broadband radio emission reached a maximum and then cut off as Voyager approached the north m...
This document constitutes the final report for grant NAGW-2442 of the Neptune Data Analysis Program,...
Earth, Jupiter, and Saturn are sources of intense but sporadic bursts of electromagnetic radiation o...
Results are reported from the first low frequency radio receiver to be transported into the Jupiter ...
Section A. Radio Emissions From Jupiter. The thesis begins with a detailed review of the observed ...
Voyager plasma wave wideband frames from the Jovian encounters are analyzed. The 511 frames which we...
Jupiter's low frequency radio emission morphology as observed by the Planetary Radio Astronomy (PRA)...
All magnetized planets are known to produce intense non thermal radio emissions through a mechanism ...
Abstract Nonthermal radio bursts in the interplanetary medium indicate the far-reaching effect of so...
This grant was for the analysis and interpretation of data obtained by the cosmic ray system (CRS) o...
The Voyager 1 and Voyager 2 Planetary Radio Astronomy Experiments (PRA) have produced the finest set...
Progress under this grant has included identifying certain new radio emission components and determi...
Analysis of nonthermal radio emission data obtained by the Planetary Radio Astronomy (PRA) spectrome...
For more than thirty years the intense decametric radio emissions from Jupiter (DAM) and the corresp...
During the Voyager 2 flyby of Neptune, a series of 16 whistler-like events were detected by the plas...
Smooth broadband radio emission reached a maximum and then cut off as Voyager approached the north m...
This document constitutes the final report for grant NAGW-2442 of the Neptune Data Analysis Program,...
Earth, Jupiter, and Saturn are sources of intense but sporadic bursts of electromagnetic radiation o...
Results are reported from the first low frequency radio receiver to be transported into the Jupiter ...
Section A. Radio Emissions From Jupiter. The thesis begins with a detailed review of the observed ...
Voyager plasma wave wideband frames from the Jovian encounters are analyzed. The 511 frames which we...
Jupiter's low frequency radio emission morphology as observed by the Planetary Radio Astronomy (PRA)...
All magnetized planets are known to produce intense non thermal radio emissions through a mechanism ...
Abstract Nonthermal radio bursts in the interplanetary medium indicate the far-reaching effect of so...
This grant was for the analysis and interpretation of data obtained by the cosmic ray system (CRS) o...
The Voyager 1 and Voyager 2 Planetary Radio Astronomy Experiments (PRA) have produced the finest set...