Auroral evidence of radial transport at Jupiter during January 2014
Changes in the Plasma Sheet Conditions at Europas Orbit Retrieved From Lead Angle of the Satellite Auroral Footprints
Characterization of Jupiters secondary auroral oval and its response to hot plasma injections
Dynamics of the flares in the active polar region of Jupiter
Evolution of the Auroral Signatures of Jupiters Magnetospheric Injections
Similarity of the Jovian satellite footprints: Spots multiplicity and dynamics
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 tails of the satellite auroral footprints at Jupiter
Transient internally driven aurora at Jupiter discovered by Hisaki and the Hubble Space Telescope
Variation of Jupiters aurora observed by Hisaki/EXCEED: 1. Observed characteristics of the auroral electron energies compared with observations performed using HST/STIS
Variation of Jupiters aurora observed by Hisaki/EXCEED: 2. Estimations of auroral parameters and magnetospheric dynamics
Weakening of Jupiters main auroral emission during January 2014
Instrument
STIS, STIS/FUV-MAMA
Temporal Coverage
2014-01-01T03:02:53Z/2014-01-16T00:45:41Z
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, Badman et al., 2015, 'A unique opportunity to discover how energy is transported through Jupiter's magnetosphere', 1.0, European Space Agency, https://doi.org/10.5270/esa-bj4karm