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A beaming model of the io-independent jovian decameter radiation based on multipole models of the jovian magnetic field
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Goldstein, M. L. Eviatar, A. Thieman, J. R. |
| Copyright Year | 1978 |
| Description | A geometrical model is presented in which the apparent source locations of the Io-independent decameter radiation are computed. The calculations assume that the radiation is produced by stably trapped electrons radiating near the electron gyrofrequency and that the emission is then beamed onto a conical surface. The maximum occurrence probability of noise storms is associated with regions in the Jovian magnetosphere where the axis of the emission cone is most inclined toward the Jovian equatorial plane. The calculations utilize and compare two of the octupole spherical harmonic expansions of the Jovian magnetic field constructed from data accumulated by the fluxgate and vector helium magnetometers on board Pioneer 11. |
| File Size | 3154753 |
| Page Count | 41 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19780016080 |
| Archival Resource Key | ark:/13960/t8md3qt09 |
| Language | English |
| Publisher Date | 1978-04-01 |
| Access Restriction | Open |
| Subject Keyword | Lunar And Planetary Exploration Planetary Magnetic Fields Trapped Particles Pioneer 11 Space Probe Astronomical Models Noise Storms Decametric Waves Beams Radiation Jupiter Planet Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |
