Auroral evidence of a localized magnetic anomaly in Jupiters northern hemisphere
Auroral footprint of Ganymede
Characteristics of Jovian morning bright FUV aurora from Hubble Space Telescope/Space Telescope Imaging Spectrograph imaging and spectral observations
Europas FUV auroral tail on Jupiter
Evolution of the Auroral Signatures of Jupiters Magnetospheric Injections
Jupiters changing auroral location
Jupiters equatorward auroral features: Possible signatures of magnetospheric injections
Magnetosphere-ionosphere coupling in Jupiters middle magnetosphere: Computations including a self-consistent current sheet magnetic field model
Modeling the Jovian magnetic field and its secular variation using all available magnetic field observations
Similarity of the Jovian satellite footprints: Spots multiplicity and dynamics
The far-ultraviolet main auroral emission at Jupiter - Part 1: Dawn-dusk brightness asymmetries
The far-ultraviolet main auroral emission at Jupiter - Part 2: Vertical emission profile
The Infrared Auroral Footprint Tracks of Io, Europa and Ganymede at Jupiter Observed by Juno-JIRAM
The Structure of the Warped Io Plasma Torus Constrained by the Io Footprint
The tails of the satellite auroral footprints at Jupiter
The variation of Ios auroral footprint brightness with the location of Io in the plasma torus
Instrument
ACS, ACS/SBC
Temporal Coverage
2005-01-25T08:54:40Z/2005-05-06T06:46:14Z
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, GRODENT DENIS, 2006, 'Identification of a magnetic anomaly at Jupiter from satellite footprints', 1.0, European Space Agency, https://doi.org/10.5270/esa-8btn8ht