| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10705287 | Planetary and Space Science | 2011 | 17 Pages |
Abstract
⺠So-called Jovian dust streams are strongly affected by the periodic variations of the solar wind. ⺠Dust streams' occurrence, intensity and duration are always linked to the solar wind structure. ⺠In summary, strong enough CIRs and CMEs are keys in the detection of dust streams.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
Alberto Flandes, Harald Krüger, Douglas P. Hamilton, J. Francisco Valdés-Galicia, Linda Spilker, Rogelio Caballero,