IUE program SUGSD: Varability time scale of H Ly-alpha from Uranus

Details IUE program SUGSD: Varability time scale of H Ly-alpha from Uranus IUE program SUGSD: Varability time scale of H Ly-alpha from Uranus

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jhu..reptq....d&link_type=abstract

Final Technical Report Johns Hopkins Univ., Baltimore, MD. Center for Astrophysical Sciences.

Astronomy and Astrophysics

Astrophysics

Brightness, Emission Spectra, Lyman Alpha Radiation, Satellite Imagery, Uranus (Planet), Iue, Line Spectra, Raman Spectra, Ultraviolet Spectra

Scientific paper

The scientific motivation for this program was to determine the time scale for the variability of the H Lyman-alpha emission from Uranus. The purpose of this series of observation is to determine its variability on shorter time scales. A series of observations was carried out in coordination with ESA to cover as completely as possible one 24 hour period of the Uranian H Lyman-alpha emission. The observations were obtained on April 23 and 24. Two additional ovservations on April 25 and 26 were obtained to search for longer term trends. A small modulation in the brightness was observed and the results presented.

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