A dataset provided by the European Space Agency

Name 6755
Title MORPHOLOGY OF OH IN THE SATURN MAGNETSOPHERE
URL https://hst.esac.esa.int/ehst/#/pages/search;proposal=6755;TAPCLIENT=DOI
DOI https://doi.org/10.5270/esa-38rgixh
Author Shemansky, Donald E.
Description This is a scientific proposal for HST mission. For specific information please visit https://archive.stsci.edu/proposal_search.php?id=6755&mission=hst
Publication
  • A self-consistent model of plasma and neutrals at Saturn: Neutral cloud morphology
  • Icy Saturnian satellites: Disk-integrated UV-IR characteristics and links to exogenic processes
  • Saturn: Search for a missing water source
  • The Bolometric Bond Albedo of Enceladus
  • The Enceladus and OH Tori at Saturn
Instrument FOS/RD
Temporal Coverage 1996-10-04T12:11:59Z/1996-10-13T23:29:26Z
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 1997-10-14T02:55:58Z
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, Shemansky comma Donald E., 1997, 'MORPHOLOGY OF OH IN THE SATURN MAGNETSOPHERE', 1.0, European Space Agency, https://doi.org/10.5270/esa-38rgixh