This Voyager 2 Neptune data set is available on CD-ROM and magnetic tape.

This data set contains all of the Voyager images from Uranus in cleaned, calibrated and geometrically corrected forms. It is derived from data set VG2-N-ISS-2-EDR-V1.0.

This data set contains reformatted records derived from data returned by the Voyager Ultraviolet Spectrometer Subsystem on board Voyager 2 during the Neptune encounter phase of the Voyager mission. Original instrument data were merged with ancillary data from footprint SEDR files provided by the Voyager Project at the Jet Propulsion Laboratory. The final product files are formatted as PDS binary tables.

This data set contains reformatted records derived from data returned by the Voyager Ultraviolet Spectrometer Subsystem on board Voyager 2 during the Neptune encounter phase of the Voyager mission. Original instrument data were merged with ancillary data from footprint SEDR files provided by the Voyager Project at the Jet Propulsion Laboratory. The final product files are formatted as PDS binary tables.

This Voyager 2 Uranus data set is available on CD-ROM and magnetic tape.

This data set consists of 4-second edited, wave electric field intensities from the Voyager 2 Plasma Wave Receiver (PWS) spectrum analyzer obtained in the vicinity of the Neptunian magnetosphere. For each 4-second interval, a 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 intensities (16 channels) is the time of the beginning of the scan. During data gaps where complete 4-second spectra are missing, no entries exist in the file, that is, the gaps are not zero-filled or tagged in any other way. When one or more channels are missing within a scan, the missing measurements are zero-filled. Data are edited but not calibrated. The data numbers in this data set can be plotted in raw form for event searches and simple trend analysis since they are roughly proportional to the log of the electric field strength. Calibration procedures and tables are provided for use with this data set

The data set contains measurements from both the infrared interferometer spectrometer and the broadband reflected solar radiometer and ancillary data. The data set is ordered by time as measured by the Flight Data System Count (FDSC). This represents the data frame number, modulo 60. Also included is pointing and other information on the geometry associated with a given data record.

The data set contains measurements from both the infrared interferometer spectrometer and the broadband reflected solar radiometer and ancillary data. The data set is ordered by time as measured by the Flight Data System Count (FDSC). This represents the data frame number, modulo 60. Also included is pointing and other information on the geometry associated with a given data record.

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. In order to produce this dataset from the original raw PRA data, several steps have been taken:

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 Neptunian 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. [1989] and a complete instrument description can be found in Scarf and Gurnett [1977].