ULY JUP SCE DOPPLER HI-RES DATA

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.

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Additional Info

Field Value
Maintainer Thomas Morgan
Last Updated July 17, 2025, 13:59 (UTC)
Created March 31, 2025, 12:44 (UTC)
accessLevel public
accrualPeriodicity irregular
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harvest_source_title DNG Legacy Data
identifier urn:nasa:pds:context_pds3:data_set:data_set.uly-j-sce-3-rdr-doppler-hires-v1.0_2w4c-84xj
issued 2018-06-26
landingPage https://pds.nasa.gov/ds-view/pds/viewDataset.jsp?dsid=ULY-J-SCE-3-RDR-DOPPLER-HIRES-V1.0
modified 2023-01-26
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