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- c1f85122-1cc1-4aed-a095-df40d7b98c71 definition "The main science objective of the Ulysses Solar Corona Experiment on Ulysses is to derive the plasma parameters of the solar atmosphere using established coronal-sounding techniques. Applying appropriate model assumptions, the 3-D electron density distribution will be determined from dual-frequency ranging and Doppler measurements recorded at the NASA Deep Space Network during the solar conjunctions. Multi-station observations will be used to derive the plasma bulk velocity at solar distances where the solar wind is expected to undergo its greatest acceleration. As a secondary objective profiting from the favorable geometry during Jupiter encounter, radio-sounding measurements will yield a unique cross-scan of the electron density in the Io Plasma Torus. (Abstract from: M.K. Bird et al., Astron. Astrophys. Suppl. Ser. 92, 425-430, 1992)" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 id "1655464" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 path_id 02c354fd-8e2d-4825-b786-aa4b0782d1d6 @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 path_id 5f5e4f2c-61b7-4694-8680-3fc5799f6171 @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 path_id b2140059-b3ca-415c-b0a7-3e142783ffe8 @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 path_label "Instruments" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 path_label "Particle Detectors" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 path_label "Solar/Space Observing Instruments" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 prefLabel "SEC" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 reference "" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 tag "Instruments" @default.