This dataset consists of edited browse data derived from an original dataset obtained from the Voyager 2 Planetary Radio Astronomy (PRA) instrument in the vicinity of Uranus. Data are provided for 70 instrument channels covering the range from 1.2 kHz to 1326 kHz in uniform 19.2 kHz steps, each 1 kHz wide. Data are included for the period 1986:019:00:00 through 1986:031:23:59. In order to produce this dataset from the original raw PRA data, several steps have been taken:

This data set (VG2-U-PRA-2-RDR-HIGHRATE-60MS-V1.0) contains data acquired by the Voyager-2 Planetary Radio Astronomy (PRA) instrument during the Uranus encounter. Since the PRA instrument is able to observe planetary phenomenon at much larger ranges than other fields and particles experiments, thus the PRA data cover a variable and longer encounter period. PRA lowband data provided here cover the entire Uranus Encounter Phase (1985-10-24 to 1988-07-14).

This dataset consists of edited browse data derived from an original dataset obtained from the Voyager 2 Planetary Radio Astronomy (PRA) instrument in the vicinity of Neptune. Data are provided for 70 instrument channels covering the range from 1.2 kHz to 1326 kHz in uniform 19.2 kHz steps, each 1 kHz wide. Data are included for the period 1989:0:0:0 through 1989:23:59:59.

This data consists of resampled data from the Low Energy Charged Particle (LECP) Experiment on the Voyager 2 Spacecraft for the period when Voyager 2 was in the vicinity of the planet Uranus.

This data set includes data from the Low Field Magnetometer (LFM) in the during the Uranus encounter. The encounter data (1986-01-24T07:00:00 -> 1986-01-25T04:00:00) have been averaged from the 9.6 second averages to a 48 second resampled rate and are provided in the Uranus Longitude (U1) coordinate system. Magnetometer data in the solar wind are given in Heliographic coordinates.

This data set consists of 48-second calibrated, averaged wave electric field intensities from the Voyager 2 Plasma Wave Receiver spectrum analyzer obtained in the vicinity of the Uranian magnetosphere. For each 48-second interval, a geometric average field strength is determined for each of the 16 spectrum analyzer channels whose center frequencies range from 10 Hertz to 56.2 kiloHertz and which are logarithmically spaced in frequency, four channels per decade. The time associated with each set of averages is the beginning of the averaging interval. Averages are stored in units of volt/meter. During data gaps where complete 48-second intervals are missing, no entries exist in the file, that is, the gaps are not zero-filled or tagged in any other way. Additional information about this dataset and the instrument which produced it can be found elsewhere in this catalog. An overview of the data in this data set can be found in Gurnett et al. [1986] and a complete instrument description can be found in Scarf and Gurnett [1977].

This data set consists of edited browse data derived from an original data set obtained from the Voyager 2 Planetary Radio Astronomy (PRA) instrument in the vicinity of Jupiter. Data are provided for 70 instrument channels covering the range from 1.2 kHz to 1326 kHz in uniform 19.2 kHz steps, each 1 kHz wide. Data are included for the period 1979-04-25 00:00:00.000 through 1979-08-04 23:04:00.000.

This data set includes data from the Low Field Magnetometer (LFM) in the during the Uranus encounter. The encounter data (1986-01-24T07:00:00 -> 1986-01-25T04:00:00) have been averaged from the 60ms instrument sample rate to a 1.92 second resampled rate and are provided in the Uranus Longitude (U1) coordinate system. Magnetometer data in the solar wind are given in Heliographic coordinates.

This data set consists of 48-second calibrated, averaged wave electric field intensities from the Voyager 2 Plasma Wave Receiver spectrum analyzer obtained in the vicinity of the Uranian magnetosphere. For each 48-second interval, a geometric average field strength is determined for each of the 16 spectrum analyzer channels whose center frequencie range from 10 Hertz to 56.2 kilo- Hertz and which are logarithmically spaced in frequency, four channels per decade. Th time associated with each set of averages is the beginning of the averaging interval. Averages are stored in units of volt/meter.

This data set includes data from the Low Field Magnetometer (LFM) in the during the Uranus encounter. The encounter data (1986-01-24T07:00:00 -> 1986-01-25T04:00:00) have been averaged from the 1.92 second averaged data to a 9.6 second resampled rate and are provided in the Uranus Longitude (U1) coordinate system. Magnetometer data in the solar wind are given in Heliographic coordinates and are also available in