Abstract
The transmission of Alfvén waves from Io to the Jovian ionosphere is discussed. Various simplified laws for the variation of plasma density are analyzed and juxtaposed to simulate a realistic density variation along the Io-Jupiter flux line. Apparently the ionosphere is previously only to frequencies in excess of 1 Hz. The ionosphere participates in tilting the flux tube trapped by Io leading to the formation of a neutral point in the vicinity of the satellite.
Original language | English (US) |
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Pages (from-to) | 1417-1429 |
Number of pages | 13 |
Journal | Planetary and Space Science |
Volume | 21 |
Issue number | 8 |
DOIs | |
State | Published - Aug 1973 |
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science