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| Reference : Soft X-ray emissions from planets, moons, and comets |
| Scientific congresses and symposiums : Unpublished conference | |||
| Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics | |||
| http://hdl.handle.net/2268/97475 | |||
| Soft X-ray emissions from planets, moons, and comets | |
| English | |
| Bhardwaj, A. [> > > >] | |
| Gladstone, G. R. [> > > >] | |
| Elsner, R. F. [> > > >] | |
| Waite, J H, Jr [> > > >] | |
Grodent, Denis  [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP) >] | |
| Cravens, T. E. [> > > >] | |
| Howell, R. R. [> > > >] | |
| Metzger, A. E. [> > > >] | |
| Ostgaard, N. [> > > >] | |
| Maurellis, A. N. [> > > >] | |
| Johnson, R. E. [> > > >] | |
| Weisskopf, M. C. [> > > >] | |
| Majeed, T. [> > > >] | |
| Ford, P. G. [> > > >] | |
| Tennant, A. F. [> > > >] | |
| Clarke, J. T. [> > > >] | |
| Lewis, W. S. [> > > >] | |
| Hurley, K. C. [> > > >] | |
| Crary, F. J. [> > > >] | |
| Feigelson, E. D. [> > > >] | |
| Garmire, G. P. [> > > >] | |
| Young, D. T. [> > > >] | |
| Dougherty, M. K. [> > > >] | |
| Espinosa, S. A. [> > > >] | |
| Jahn, J*-M [> > > >] | |
| Battrick, Bruce [> > > >] | |
| Foing, Bernard H [ > > ] | |
| 2002 | |
| No | |
| No | |
| International | |
| Earth-like Planets and Moons | |
| [en] X Rays: Planets ; Moons ; Comets | |
| [en] A wide variety of solar system bodies are now known to radiate in the soft X-ray energy (<5 keV) regime. These include planets (Earth, Jupiter, Venus, Saturn, Mars): bodies having thick atmospheres, with or without intrinsic magnetic field; planetary satellites (Moon, Io, Europa, Ganymede): bodies with thin or no atmospheres; and comets and Io plasma torus: bodies having extended tenuous atmospheres. Several different mechanisms have been proposed to explain the generation of soft X-rays from these objects, whereas in the hard X-ray energy range (>10 keV) X-rays mainly result from the electron bremsstrahlung process. In this paper we present a brief review of the X-ray observations on each of the planetary bodies and discuss their characteristics and proposed source mechanisms. | |
| http://hdl.handle.net/2268/97475 | |
| 514
215-226 |
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