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- W2103142384 abstract "Observations of the solar corona and measurements of its rotation are reviewed in order to suggest what rotational characteristics of the solar wind might be observed from the Ulysses mission. Results from 20 years of data from the HAO K-coronameters on Mauna Loa, Hawaii, are described. They show that the corona rotates, on average, rather more rigidly than do any of the usual photospheric or chromospheric tracers on the sun, displaying an average synodic rotation rate of 14.2 degrees per day. The suggestion is made that a similar rotation character will be observed by Ulysses, and some evidence to support that from interplanetary observations is discussed." @default.
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- W2103142384 date "1986-01-01" @default.
- W2103142384 modified "2023-09-25" @default.
- W2103142384 title "The Structure and Rotation of the Solar Corona: Implications for the Heliosphere" @default.
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- W2103142384 doi "https://doi.org/10.1007/978-94-009-4612-5_5" @default.
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