A dataset provided by the European Space Agency

Name 10083
Title HST UV Images of Saturns Aurora Coordinated with Cassini Solar Wind Measurements
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=10083;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-o3iclpi
Author Clarke, John T.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=10083&mission=hst
Publication
  • An Earth-like correspondence between Saturns auroral features and radio emission
  • A statistical analysis of the location and width of Saturns southern auroras
  • Auroral emissions and electromagnetic interactions between Jupiter and Saturn and their satellites
  • Cassini observations of the Interplanetary Medium Upstream of Saturn and their relation to the Hubble Space Telescope aurora data
  • Dependence of the open-closed field line boundary in Saturns ionosphere on both the IMF and solar wind dynamic pressure: comparison with the UV auroral oval observed by the HST
  • Dependence of the open-closed field line boundary in Saturns ionosphere on the solar wind and its magnetic field derived from the Cassini and HSTdata
  • Energy-flux relationship in the FUV Jovian aurora deduced from HST-STIS spectral observations
  • IMF dependence of the open-closed field line boundary in Saturns ionosphere, and its relation to the UV auroral oval observed by the Hubble Space Telescope
  • Interaction evidence between Enceladus atmosphere and Saturns magnetosphere
  • Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model
  • Morphological differences between Saturns ultraviolet aurorae and those of Earth and Jupiter
  • On the origin of Saturns outer auroral emission
  • Open flux estimates in Saturns magnetosphere during the January 2004 Cassini-HST campaign, and implications for reconnection rates
  • Open flux in Saturns magnetosphere
  • Signature of Saturns auroral cusp: Simultaneous Hubble Space Telescope FUV observations and upstream solar wind monitoring
  • Signatures of field-aligned currents in Saturns nightside magnetosphere
  • Solar wind dynamic pressure and electric field as the main factors controlling Saturns aurorae
  • Survey of Saturn auroral storms observed by the Hubble Space Telescope: Implications for storm time scales
  • Variable morphology of Saturns southern ultraviolet aurora
Instrument STIS/FUV-MAMA
Temporal Coverage 2004-01-08T04:25:59Z/2004-01-30T19:27:16Z
Version 1.0
Mission Description Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
Creator Contact https://support.cosmos.esa.int/esdc/index.php?/Tickets/Submit
Date Published 2004-02-02T13:09:52Z
Keywords Hubble, HST, HLA, HCV, ACS, COS, STIS, WFC3, FOC, FOS, HRS, NICMOS, WFPC, WFPC2
Publisher And Registrant European Space Agency
Credit Guidelines European Space Agency, Clarke comma John T., 2004, 'HST UV Images of Saturn's Aurora Coordinated with Cassini Solar Wind Measurements', 1.0, European Space Agency, https://doi.org/10.5270/esa-o3iclpi