A Long-Term Study of Jupiters Equatorial Winds at the Top of the Troposphere
Analysis of the long-term drift rates and oscillations of Jupiters largest vortices
An equatorial thermal wind equation: Applications to Jupiter
A New Dark Vortex on Neptune
A New, Long-lived, Jupiter Mesoscale Wave Observed at Visible Wavelengths
Changes in Jupiters Zonal Wind Profile preceding and during the Juno mission
Constraints on Uranuss haze structure, formation and transport
Dynamics and clouds in planetary atmospheres from telescopic observations
Evolution of Neptune at near-infrared wavelengths from 1994 through 2022
Evolution of the Horizontal Winds in Jupiters Great Red Spot From One Jovian Year of HST/WFC3 Maps
First measurements of Jupiters zonal winds with visible imaging spectroscopy
Formation of a New Great Dark Spot on Neptune in 2018
Giant Planet Atmospheres: Dynamics and Variability from UV to Near-IR Hubble and Adaptive Optics Imaging
High-resolution UV/Optical/IR Imaging of Jupiter in 2016-2019
Historical and Contemporary Trends in the Size, Drift, and Color of Jupiters Great Red Spot
Jovian Vortex Hunter: A Citizen Science Project to Study Jupiters Vortices
Jupiter cloud morphology and zonal winds from ground-based observations before and during Junos first perijove
Jupiters Temperate Belt/Zone Contrasts Revealed at Depth by Juno Microwave Observations
Jupiters Turbulent Power Spectra From Hubble Space Telescope
Lifetimes and Occurrence Rates of Dark Vortices on Neptune from 25 Years of Hubble Space Telescope Images
Longitudinal variability in Jupiters zonal winds derived from multi-wavelength HST observations
Modelling the seasonal cycle of Uranuss colour and magnitude, and comparison with Neptune
Temporal and spatial variations of the absolute reflectivity of Jupiter and Saturn from 0.38 to 1.7 mm with PlanetCam-UPV/EHU
Temporal Variations in Vertical Cloud Structure of Jupiters Great Red Spot, Its Surroundings and Oval BA From HST/WFC3 Imaging
The bolometric Bond albedo and energy balance of Uranus
The Temporal Brightening of Uranus Northern Polar Hood From HST/WFC3 and HST/STIS Observations
UV-dark polar ovals on Jupiter as tracers of magnetosphere-atmosphere connections
Zonal and Regional Jupiter Brightness Trends from the Hubble Outer Planet Atmospheres Legacy Program
Instrument
WFC3/UVIS
Temporal Coverage
2015-09-12T05:04:17Z/2016-10-04T13:17:18Z
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, Simon et al., 2016, 'Hubble 2020: Outer Planet Atmospheres Legacy (OPAL) Program', 1.0, European Space Agency, https://doi.org/10.5270/esa-r1q24k0