A Comparative Study of Jovian Anticyclone Properties from a Six-Year (1994-2000) Survey
A Comparative Study of Jovian Cyclonic Features from a Six-Year (1994-2000) Survey
Coloring Jupiters clouds: Radiolysis of ammonium hydrosulfide (NH4SH)
Global Context of the Galileo-E6 Observations of Jupiters White Ovals
Historical and Contemporary Trends in the Size, Drift, and Color of Jupiters Great Red Spot
Jupiters Great Red Spot: Fine-scale matches of model vorticity patterns to prevailing cloud patterns
Jupiters Turbulent Power Spectra From Hubble Space Telescope
New Observational Results Concerning Jupiters Great Red Spot
On the long-term variability of Jupiters winds and brightness as observed from Hubble
Simulations of high-latitude spots on Jupiter: Constraints on vortex strength and the deep wind
Temporal variation of the tropospheric cloud and haze in the jovian equatorial zone
The 90-day oscillations of Jupiters Great Red Spot revisited
The dynamics of jovian white ovals from formation to merger
The spectrum of Jupiters Great Red Spot: The case for ammonium hydrosulfide (NH4SH)
Vertical Structure of Jupiters Atmosphere at the Galileo Probe Entry Latitude
Vertical structure of Jupiters Oval BA before and after it reddened: What changed?
Wind variations in Jupiters equatorial atmosphere: A QQO counterpart?
Instrument
WFPC2, WFPC2/PC, WFPC2/WFC
Temporal Coverage
1995-02-13T01:24:16Z/1995-02-18T02:37:17Z
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, Beebe et al., 1996, 'CHARACTERIZATION OF JUPITER'S VERTICAL CLOUD STRUCTURE AND ATMOSPHERIC MOTIONS: CYCLE4 HIGH', 1.0, European Space Agency, https://doi.org/10.5270/esa-wbosf8n