Reference : Simultaneous Chandra X ray, Hubble Space Telescope ultraviolet, and Ulysses radio obs...
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Earth sciences & physical geography
http://hdl.handle.net/2268/4544
Simultaneous Chandra X ray, Hubble Space Telescope ultraviolet, and Ulysses radio observations of Jupiter's aurora
English
Elsner, Ronald F. [NASA Marshall Space Flight Center]
Lugaz, N. [> > > >]
Waite, J. H. [> > > >]
Cravens, T. E. [> > > >]
Gladstone, G. R. [> > > >]
Ford, P. [> > > >]
Grodent, Denis mailto [Université de Liège - ULg > Département d'astrophys., géophysique et océanographie (AGO) > Labo de physique atmosphérique et planétaire (LPAP) >]
Bhardwaj, A. [> > > >]
MacDowall, R. J. [> > > >]
Desch, M. D. [> > > >]
Majeed, T. [> > > >]
14-Jan-2005
Journal of Geophysical Research. Space Physics
American Geophysical Union (AGU)
110
A1
Yes (verified by ORBi)
International
0148-0227
Washington
[en] [1] Observations of Jupiter carried out by the Chandra Advanced CCD Imaging Spectrometer (ACIS-S) instrument over 24 - 26 February 2003 show that the auroral X-ray spectrum consists of line emission consistent with high-charge states of precipitating ions, and not a continuum as might be expected from bremsstrahlung. The part of the spectrum due to oxygen peaks around 650 eV, which indicates a high fraction of fully stripped oxygen in the precipitating ion flux. A combination of the OVIII emission lines at 653 eV and 774 eV, as well as the OVII emission lines at 561 eV and 666 eV, are evident in the measure auroral spectrum. There is also line emission at lower energies in the spectral region extending from 250 to 350 eV, which could be from sulfur and/or carbon. The Jovian auroral X-ray spectra are significantly different from the X-ray spectra of comets. The charge state distribution of the oxygen ions implied by the measured auroral X-ray spectra strongly suggests that independent of the source of the energetic ions, magnetospheric or solar wind, the ions have undergone additional acceleration. This spectral evidence for ion acceleration is also consistent with the relatively high intensities of the X rays compared with the available phase space density of the (unaccelerated) source populations of solar wind or magnetospheric ions at Jupiter, which are orders of magnitude too small to explain the observed emissions. The Chandra X-ray observations were executed simultaneously with observations at ultraviolet wavelengths by the Hubble Space Telescope and at radio wavelengths by the Ulysses spacecraft. These additional data sets suggest that the source of the X rays is magnetospheric in origin and that the precipitating particles are accelerated by strong field-aligned electric fields, which simultaneously create both the several-MeV energetic ion population and the relativistic electrons observed in situ by Ulysses that are correlated with similar to 40 min quasi-periodic radio outbursts.
Researchers ; Professionals ; Students
http://hdl.handle.net/2268/4544
10.1029/2004JA010717

File(s) associated to this reference

Fulltext file(s):

FileCommentaryVersionSizeAccess
Restricted access
elsner_2005.pdfNo commentaryPublisher postprint680.69 kBRequest copy

Bookmark and Share SFX Query

All documents in ORBi are protected by a user license.