ALBERT

All Library Books, journals and Electronic Records Telegrafenberg

feed icon rss

Your email was sent successfully. Check your inbox.

An error occurred while sending the email. Please try again.

Proceed reservation?

Export
Filter
  • *Jupiter  (2)
  • American Association for the Advancement of Science (AAAS)  (2)
  • Elsevier
  • Periodicals Archive Online (PAO)
  • 2000-2004  (2)
Collection
Publisher
  • American Association for the Advancement of Science (AAAS)  (2)
  • Elsevier
  • Periodicals Archive Online (PAO)
Years
Year
  • 1
    facet.materialart.
    Unknown
    American Association for the Advancement of Science (AAAS)
    Publication Date: 2000-03-17
    Description: The Galileo orbiter's close pass by Io in 1995 produced evidence for extensive mass loading of the plasma torus through the ionization of SO2. On 11 October 1999, Galileo passed even closer to Io, this time across the upstream side relative to the flow of magnetospheric plasma that corotates with Jupiter. On the first flyby, ion cyclotron waves gave direct evidence for the production of SO2+ ions. On the second flyby, ion cyclotron waves associated with SO+ were stronger and more persistent. Moreover, SO+ emissions were seen closer to Io than SO2+ emissions, suggesting that the exosphere was spatially inhomogeneous. The location of the waves suggests a fan-shaped region of ion pickup extending in the anti-Jupiter direction. Because the wave spectra were different even where the 1995 and 1999 trajectories crossed, we infer that Io's exosphere is temporally variable.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Russell, C T -- Kivelson, M G -- New York, N.Y. -- Science. 2000 Mar 17;287(5460):1998-9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Institute of Geophysics and Planetary Physics, 3845 Slichter Hall, University of California Los Angeles, Los Angeles, CA 90095-1567, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10720321" target="_blank"〉PubMed〈/a〉
    Keywords: Cations ; *Extraterrestrial Environment ; *Jupiter ; Magnetics ; *Oxides ; *Sulfur ; *Sulfur Compounds ; *Sulfur Dioxide
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
  • 2
    Publication Date: 2000-08-26
    Description: On 3 January 2000, the Galileo spacecraft passed close to Europa when it was located far south of Jupiter's magnetic equator in a region where the radial component of the magnetospheric magnetic field points inward toward Jupiter. This pass with a previously unexamined orientation of the external forcing field distinguished between an induced and a permanent magnetic dipole moment model of Europa's internal field. The Galileo magnetometer measured changes in the magnetic field predicted if a current-carrying outer shell, such as a planet-scale liquid ocean, is present beneath the icy surface. The evidence that Europa's field varies temporally strengthens the argument that a liquid ocean exists beneath the present-day surface.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kivelson, M G -- Khurana, K K -- Russell, C T -- Volwerk, M -- Walker, R J -- Zimmer, C -- New York, N.Y. -- Science. 2000 Aug 25;289(5483):1340-3.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90095-1567, USA. mkivelson@igpp.ucla.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10958778" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment ; Ice ; *Jupiter ; Magnetics ; *Water
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Location Call Number Expected Availability
    BibTip Others were also interested in ...
Close ⊗
This website uses cookies and the analysis tool Matomo. More information can be found here...