Atmospheric Dynamics and Vertical Structure of Uranus and Neptunes Weather Layers
Coordinated 1996 HST and IRTF Imaging of Neptune and Triton. II. Implications of Disk-Integrated Photometry
Coordinated 1996 HST and IRTF Imaging of Neptune and Triton. III. Neptunes Atmospheric Circulation and Cloud Structure
Coordinated 1996 HST and IRTF Imaging of Neptune and Triton. I. Observations, Navigation, and Differential Deconvolution
EPIC Simulations of Bright Companions to Neptunes Great Dark Spots
Evolution of Neptune at near-infrared wavelengths from 1994 through 2022
Lifetimes and Occurrence Rates of Dark Vortices on Neptune from 25 Years of Hubble Space Telescope Images
Neptunes cloud and haze variations 1994-2008 from 500 HST-WFPC2 images
Neptunes rotational period suggested by the extraordinary stability of two features
The nature of Neptunes increasing brightness: evidence for a seasonal response *
The Unusual Dynamics of Northern Dark Spots on Neptune
Instrument
WFPC2, WFPC2/PC
Temporal Coverage
1996-08-13T08:33:16Z/1996-08-14T01:09:56Z
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, SROMOVSKY LAWRENCE, 1997, 'ATMOSPHERIC DYNAMICS AND CLOUD STRUCTURE ON NEPTUNE', 1.0, European Space Agency, https://doi.org/10.5270/esa-z294to8