{"@type": "dcat:Dataset", "accessLevel": "public", "bureauCode": ["026:00"], "contactPoint": {"@type": "vcard:Contact", "fn": "Planetary Data System", "hasEmail": "mailto:pds-operator@jpl.nasa.gov"}, "description": "This data set contains raw and partially processed data from      observations of Magellan radio transmissions while the signal      was passing through the solar corona.  Scintillations on the      signal can be related to structure and motion of the coronal      material [WOO1993]; polarization of the signal can be used to      infer magnetic field within the plasma.      Data were acquired using stations of the NASA Deep Space Network      (DSN).  The Magellan spacecraft transmitted signals that were      100 percent linearly polarized at 13 cm and right-elliptically      polarized at 3.6 cm.  During summer 1992, when Magellan was in      solar superior conjunction, the spacecraft came within 0.6 solar      radii of the Sun's center when viewed from Earth.", "identifier": "urn:nasa:pds:context_pds3:data_set:data_set.mgn-ss-rss-1-odr-openloop-sw-scint-v1.0;urn:nasa:pds:context_pds3:data_set:data_set.mgn-ss-rss-1-odr-openloop-sw-scint-v1.0::99.0", "keyword": ["__"], "license": "https://www.usa.gov/government-works", "modified": "2026-04-06", "programCode": ["026:000"], "publisher": {"@type": "org:Organization", "name": "planetary plasma interactions"}, "theme": ["Planetary Science"], "title": "MAGELLAN SOLAR CORONA                                         AND FARADAY ROTATION V1.0"}