A possible auroral signature of a magnetotail reconnection process on Jupiter
Auroral footprint of Ganymede
Characteristics of Jovian morning bright FUV aurora from Hubble Space Telescope/Space Telescope Imaging Spectrograph imaging and spectral observations
Characteristics of Saturns polar atmosphere and auroral electrons derived from HST/STIS, FUSE and Cassini/UVIS spectra
Discontinuity in Jupiters main auroral oval
Energy-flux relationship in the FUV Jovian aurora deduced from HST-STIS spectral observations
Evolution of the Auroral Signatures of Jupiters Magnetospheric Injections
Ganymedes magnetosphere: Unraveling the Ganymede-Jupiter interaction through combining multi-fluid simulations and observations
Jupiters aurora in ultraviolet and infrared: Simultaneous observations with the Hubble Space Telescope and the NASA Infrared Telescope Facility
Jupiters changing auroral location
Jupiters equatorward auroral features: Possible signatures of magnetospheric injections
Jupiters main auroral oval observed with HST-STIS
Jupiters polar auroral emissions
Jupiter Thermospheric General Circulation Model (JTGCM): Global structure and dynamics driven by auroral and Joule heating
Magnetosphere-ionosphere coupling in Jupiters middle magnetosphere: Computations including a self-consistent current sheet magnetic field model
Magnetospheric Science Objectives of the Juno Mission
Morphology of the ultraviolet Io footprint emission and its control by Ios location
Nightside reconnection at Jupiter: Auroral and magnetic field observations from 26 July 1998
Processes of equatorial thermal structure at Jupiter: An analysis of the Galileo temperature profile with a three-dimensional model
Response of Jupiters UV auroras to interplanetary conditions as observed by the Hubble Space Telescope during the Cassini flyby campaign
Similarity of the Jovian satellite footprints: Spots multiplicity and dynamics
Simultaneous Chandra X ray, Hubble Space Telescope ultraviolet, and Ulysses radio observations of Jupiters aurora
Spectral observations of transient features in the FUV Jovian polar aurora
The Cassini Campaign observations of the Jupiter aurora by the Ultraviolet Imaging Spectrograph and the Space Telescope Imaging Spectrograph
The far-ultraviolet main auroral emission at Jupiter - Part 2: Vertical emission profile
The H Lyman- a emission line from the upper atmosphere of Jupiter: Parametric radiative transfer study and comparison with data
The Infrared Auroral Footprint Tracks of Io, Europa and Ganymede at Jupiter Observed by Juno-JIRAM
The multiple spots of the Ganymede auroral footprint
The tails of the satellite auroral footprints at Jupiter
Ultraviolet emissions from the magnetic footprints of Io, Ganymede and Europa on Jupiter
Variability of Jupiters Main Auroral Emission and Satellite Footprints Observed With HST During the Galileo Era
Instrument
STIS/FUV-MAMA
Temporal Coverage
2000-12-14T10:46:42Z/2001-01-21T23:03:02Z
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, Clarke comma John T., 2002, 'Jovian Auroral Variability Due to the Solar Wind/Magnetosphere Interaction', 1.0, European Space Agency, https://doi.org/10.5270/esa-m7qr9l9
