| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1782592 | Planetary and Space Science | 2007 | 9 Pages |
Abstract
The XMM-Newton observations lend further support to the theory that Jupiter's disk X-ray emission is controlled by the Sun, and may be produced in large part by scattering, elastic and fluorescent, of solar X-rays in the upper atmosphere of the planet.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
G. Branduardi-Raymont, A. Bhardwaj, R.F. Elsner, G.R. Gladstone, G. Ramsay, P. Rodriguez, R. Soria, J.H. Jr., T.E. Cravens,