Analysis of the long-term drift rates and oscillations of Jupiters largest vortices
Chromophores from photolyzed ammonia reacting with acetylene: Application to Jupiters Great Red Spot
Coloring Jupiters clouds: Radiolysis of ammonium hydrosulfide (NH4SH)
Composition and structure of fresh ammonia clouds on Jupiter based on quantitative analysis of Galileo/NIMS and New Horizons/LEISA spectra
Dynamics of Jupiters equatorial region at cloud top level from Cassini and HST images
Evolution of the cloud field and wind structure of Jupiters highest speed jet during a huge disturbance
Historical and Contemporary Trends in the Size, Drift, and Color of Jupiters Great Red Spot
Jovian chromophore characteristics from multispectral HST images
On the long-term variability of Jupiters winds and brightness as observed from Hubble
Spectral comparison and stability of red regions on Jupiter
Thermal structure and composition of Jupiters Great Red Spot from high-resolution thermal imaging
The spectrum of Jupiters Great Red Spot: The case for ammonium hydrosulfide (NH4SH)
Instrument
NICMOS/NIC1, NICMOS/NIC2, WFPC2, WFPC2/PC
Temporal Coverage
2008-05-15T06:59:17Z/2008-07-09T07:47:39Z
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., 2008, '2008 Passage of Jupiter's Great Red Spot and Oval BA', 1.0, European Space Agency, https://doi.org/10.5270/esa-5ss62o8