ULY JUPITER INTERSTELLAR NEUTRAL-GAS EXPERIMENT SKY MAPS

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not applicable

GALILEO JUPITER RTS MOMENT DATA V1.0

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TBD

GALILEO JUPITER RTS MOMENT DATA V1.0

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TBD

GALILEO ORBITER UVS JUPITER OPERATIONS EDR DATA

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TBD

ULYSSES JUPITER SOLAR CORONA EXPER. RANGING DATA 10 MIN AVG

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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.

GALILEO ORBITER EUV JUPITER OPERATIONS EDR DATA

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TBD

GALILEO ORBITER EUV JUPITER OPERATIONS EDR DATA

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TBD

JUNO JUPITER JUNOCAM 4 RDR L1B V1.0

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NULL

P10 JUPITER HVM B-FIELD INSIDE 7 RJ JG COORDS 1 MIN AVG V1.0

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not applicable

P10 JUPITER HVM B-FIELD INSIDE 7 RJ JG COORDS 1 MIN AVG V1.0

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not applicable