ULY JUP SCE RAW ODR V1.0

공공데이터포털

This data set contains raw Radio Occultation (ROCC) Original Data Records data from the Ulysses (ULY) Solar Corona Experiment (SCE) obtained during the ULY Jupiter flyby. The data target the Io Plasma Torus (IPT) and cover the period 1992-02-03 11:20 to 1992-02-09 20:46.

ULY JUP SCE RAW ARCHIVAL TRACKING DATA FILES V1.0

공공데이터포털

This data set contains raw radio tracking data from the Ulysses (ULY) Solar Corona Experiment (SCE) obtained during the ULY Jupiter flyby. The data target the Io Plasma Torus (IPT) and cover the period 1992-02-04 20:28 to 1992-02-09 15:44.

ULY JUP SCE RAW ARCHIVAL TRACKING DATA FILES V1.0

공공데이터포털

This data set contains raw radio tracking data from the Ulysses (ULY) Solar Corona Experiment (SCE) obtained during the ULY Jupiter flyby. The data target the Io Plasma Torus (IPT) and cover the period 1992-02-04 20:28 to 1992-02-09 15:44.

ULY JUPITER ENCOUNTER EPHEMERIS SYS3/ECL50 COORDS. VER. 1.0

공공데이터포털

This data set contains Ulysses ephemeris data near Jupiter covering the dates 1992-01-25 to 1992-02-18. Two slightly different versions of these data are included. The first (TRJ25_48.TAB), provided by the Ulysses MAG team (Imperial College/JPL), includes position data in Sys 3 spherical, ECL50 spherical, and ECL50 Cartesian coordinates. The Ulysses spin axis position is also provided in ECL50 spherical coordinates. The second version (SPK25_48.TAB), generated at the PDS/PPI node (UCLA), includes Sys 3 spherical trajectory, plus a spacecraft local time. Note that the position values for these two versions differ slightly. This variation is due to differences in the definitions of the Jovian physical constants used to generate them.

ULY JUPITER ENCOUNTER EPHEMERIS SYS3/ECL50 COORDS. VER. 1.0

공공데이터포털

This data set contains Ulysses ephemeris data near Jupiter covering the dates 1992-01-25 to 1992-02-18. Two slightly different versions of these data are included. The first (TRJ25_48.TAB), provided by the Ulysses MAG team (Imperial College/JPL), includes position data in Sys 3 spherical, ECL50 spherical, and ECL50 Cartesian coordinates. The Ulysses spin axis position is also provided in ECL50 spherical coordinates. The second version (SPK25_48.TAB), generated at the PDS/PPI node (UCLA), includes Sys 3 spherical trajectory, plus a spacecraft local time. Note that the position values for these two versions differ slightly. This variation is due to differences in the definitions of the Jovian physical constants used to generate them.

ULY JUP COSPIN HIGH FLUX TELESCOPE HIGH RES. ION FLUX

공공데이터포털

This data set contains ion flux data recorded by the COSPIN High Flux Telescope (HFT) during the Ulysses Jupiter encounter 1992-Jan-25 to 1992-Feb-18

ULY JUP SCE DOPPLER HI-RES DATA

공공데이터포털

The Ulysses spacecraft was occulted by the Io Plasma Torus (IPT) during its Jupiter encounter on 8 February 1992. The Ulysses dual-frequency radio subsystem used by the Ulysses Solar Corona Experiment (SCE) was utilized to measure the electron content (column density) of the IPT [BIRDETAL1992B]. In the nominal mode for radio-sounding observations [BIRDETAL1992A], both downlinks (S-band: f_s = 2.3 GHz X-band: f_x = 8.4 GHz) are phase coherent with the uplink (S-band: f_u = 2.1 GHz). The dual-frequency radio-sounding technique exploits the dispersive nature of ionized media on the propagation of the two downlinks. The tiny Doppler shift due to plasma moving in and out of the ray path is greater at S-band than at the higher frequency X-band.

ULY JUP COSPIN HIGH FLUX TELESCOPE HIGH RES. ION FLUX

공공데이터포털

This data set contains ion flux data recorded by the COSPIN High Flux Telescope (HFT) during the Ulysses Jupiter encounter 1992-Jan-25 to 1992-Feb-18.

ULY JUP SCE DOPPLER HI-RES DATA

공공데이터포털

The Ulysses spacecraft was occulted by the Io Plasma Torus (IPT) during its Jupiter encounter on 8 February 1992. The Ulysses dual-frequency radio subsystem used by the Ulysses Solar Corona Experiment (SCE) was utilized to measure the electron content (column density) of the IPT. In the nominal mode for radio-sounding observations, both downlinks (S-band: f_s = 2.3 GHz X-band: f_x = 8.4 GHz) are phase coherent with the uplink (S-band: f_u = 2.1 GHz). The dual-frequency radio-sounding technique exploits the dispersive nature of ionized media on the propagation of the two downlinks. The tiny Doppler shift due to plasma moving in and out of the ray path is greater at S-band than at the higher frequency X-band.

VG2 J/S/U/N/SS PLASMA WAVE SPECTROMETER RAW WFRM 60MS V1.0

공공데이터포털

This data set consists of electric field waveform samples from the Voyager 2 Plasma Wave Subsystem waveform receiver obtained during the entire mission. Data after 2006-03-07 will be added to the archive on subsequent volumes. The data set encompasses all waveform observations obtained in the cruise mission phases before, between, and after the Jupiter, Saturn, Uranus, and Neptune encounter phases as well as those obtained during the four encounter phases.