urn:nasa:pds:voyager2_rss_uranus_49xr_raw:browse 1.0 1.21.0.0 Product_Collection 2025 This collection contains quick-look plots from radio occultation data acquired during the Voyager 2 Uranus encounter at Parkes Observatory in Australia. The data were collected at X-band (3.6 cm wavelength) in right circular polarization. Quick-look plots from calibration data are also included. 2025-04-12 1.0 Original collection of Voyager 2 Uranus radio occultation browse data from Parkes Observatory. JPEG plots were generated from original binary data, combined with an ASCII summary of observing conditions, and assembled into a JPEG plot with four panels. New PDS4 labels were created. 1986-01-22T18:00:06Z 1986-01-25T02:45:00Z Science Partially Processed Voyager Mission urn:nasa:pds:context:investigation:mission.voyager collection_to_investigation Voyager 2 Host urn:nasa:pds:context:instrument_host:spacecraft.vg2 is_instrument_host Deep Space Network Host urn:nasa:pds:context:facility:observatory.dsn is_facility NASA Deep Space Network Radio Science Instrument urn:nasa:pds:context:instrument:dsn.rss is_instrument Radio Science Subsystem Instrument urn:nasa:pds:context:instrument:vg2.rss is_instrument Parkes 64-m Radio Telescope (as a DSN Antenna) Telescope urn:nasa:pds:context:telescope:parkes.dss49_64m is_telescope Uranus Planet urn:nasa:pds:context:target:planet.uranus collection_to_target Eshleman, V. R., G. L. Tyler, J. D. Anderson, G. Fjeldbo, G. S. Levy, G. E. Wood, and T. A. Croft, Radio Science Investigations with Voyager, Space Science Reviews, 21, 207-232, 1977. The referenced product describes the planned Voyager radio science investigation. Data collection at Parkes Observatory was not part of the original plan. Lindal, G. F.; Lyons, J. R.; Sweetnam, D. N.; Eshleman, V. R.; Hinson, D. P.; Tyler, G. L. The atmosphere of Uranus: results of radio occultation measurements with Voyager 2, Journal of Geophysical Research, 92, A13, 14987-15001, 1987. doi: 10.1029/JA092iA13p14987 Results from the Voyager 2 ingress and egress radio occultations at Uranus. Included are profiles in height of electron density in the ionosphere and gas refractivity, number density, pressure (0.3 mbars to 2.3 bars), temperature, and methane abundance in the troposphere and stratosphere. Gresh, D. L.; Marouf, E. A.; Tyler, G. L.; Rosen, P. A.; Simpson, R. A. Voyager Radio Occultation by Uranus' Rings. 1. Observational Results, Icarus, 78, pp. 131-168, 1989. Uranus' nine previously known rings were observed by radio occultation with optical depth T as large as 6-8 at two azimuths separated by 145°. Rings have rich structural detail that changes significantly with longitude. 28 of 36 ring edges are abrupt with gradients of at least 1 T/km. There is little evidence for differential extinction between the 3.6 and 13 cm wavelengths; but the five rings closest to Uranus differentially retard 13 cm phase more efficiently than the four outer rings. An anomalous scattered signal was observed from the outermost ring that is inconsistent with a Saturn-like scattering model. Browse This collection contains quick-look plots from radio occultation data acquired during the Voyager 2 Uranus encounter at Parkes Observatory (Australia). The data were collected at X-band (3.6 cm wavelength) in right circular polarization. collection_browse.csv 2024-05-14T19:53:00 4592 37985b9eab7daf2d6fbb8d45d1aa3911 0 PDS DSV 1 56 Carriage-Return Line-Feed Comma 2 0 257 Member Status 1 ASCII_String 1 LIDVID_LID 2 ASCII_LIDVID_LID 255 inventory_has_member_product