The Raman signature of H2 in the uv spectra of Uranus and Neptune: Constraints on the haze optical properties and on the para-H2 fraction fn2 fn2Based on observations made with the NASA⧸ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Science Institute. STScI is operated by the Association of Universities for Research in Astronomy, Inc. under nasa contract nas 5-26555.
1999 ◽
Vol 47
(8-9)
◽
pp. 1077-1100
◽