Comparison of line-by-line and band models of near-IR methane absorption applied to outer planet atmospheres
Detection of hydrogen sulfide above the clouds in Uranuss atmosphere
Ice Giant Circulation Patterns: Implications for Atmospheric Probes
Latitudinal variation in the abundance of methane (CH4) above the clouds in Neptunes atmosphere from VLT/MUSE Narrow Field Mode Observations
Methane on Uranus: The case for a compact CH 4 cloud layer at low latitudes and a severe CH 4 depletion at high-latitudes based on re-analysis of Voyager occultation measurements and STIS spectroscopy
Modelling the seasonal cycle of Uranuss colour and magnitude, and comparison with Neptune
Probable detection of hydrogen sulphide (H2S) in Neptunes atmosphere
Seasonal change of CH4/H2 ratio in the atmosphere of Uranus
The haze and methane distributions on Neptune from HST-STIS spectroscopy
The haze and methane distributions on Uranus from HST-STIS spectroscopy
The methane distribution and polar brightening on Uranus based on HST/STIS, Keck/NIRC2, and IRTF/SpeX observations through 2015
Instrument
STIS/CCD
Temporal Coverage
2002-08-19T01:39:49Z/2002-08-19T10:57:30Z
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.
European Space Agency, Karkoschka comma Erich, 2007, 'Spatially Resolved Spectroscopy of Uranus and Neptune', 1.0, European Space Agency, https://doi.org/10.5270/esa-s7ha4a0