Matches in climatepub4-kg for { <https://climateKG.org/entity/c1f85122-1cc1-4aed-a095-df40d7b98c71> ?p ?o ?g. }
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- c1f85122-1cc1-4aed-a095-df40d7b98c71 ProvidedBy 8894d92c-be32-465b-ae08-e5de755a92fc @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 type Instrument @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 type Location @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 broader 02c354fd-8e2d-4825-b786-aa4b0782d1d6 @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 broader 5f5e4f2c-61b7-4694-8680-3fc5799f6171 @default.
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- c1f85122-1cc1-4aed-a095-df40d7b98c71 definition "The main science objective of the Ulysses Solar Corona Experiment on Ulysses isto derive the plasma parameters of the solar atmosphere using establishedcoronalsounding techniques Applying appropriate model assumptions the 3Delectron density distribution will be determined from dualfrequency rangingand Doppler measurements recorded at the NASA Deep Space Network during thesolar conjunctions Multistation observations will be used to derive theplasma bulk velocity at solar distances where the solar wind is expected toundergo its greatest acceleration As a secondary objective profiting from thefavorable geometry during Jupiter encounter radiosounding measurements willyield a unique crossscan of the electron density in the Io Plasma TorusAbstract from MK Bird et al Astron Astrophys Suppl Ser 92 4254301992" @default.
- c1f85122-1cc1-4aed-a095-df40d7b98c71 prefLabel "SEC" @default.