Results 1 to 10 of about 27 (27)

Infrared Observations of Ganymede From the Jovian InfraRed Auroral Mapper on Juno

, 2020
The Jovian InfraRed Auroral Mapper (JIRAM) on board the NASA Juno spacecraft is a dual-band imager and spectrometer in the 2–5 μm range with 9-nm spectral sampling, primarily designed to study the Jovian atmosphere and aurorae. In addition to these goals,
Plainaki, C., S. Bolton, MIGLIORINI, Alessandra, G. Filacchione, A. Migliorini, TOSI, Federico, CICCHETTI, ANDREA, ZAMBON, Francesca, R. Sordini, D. Grassi, C. Plainaki, A. Cicchetti, R. Noschese, M. L. Moriconi, GRASSI, Davide, G. Piccioni, Hansen, C. J., C. J. Hansen, F. Zambon, M. Ciarniello, SORDINI, Roberto, PICCIONI, GIUSEPPE, Moriconi, M. L., A. Adriani, ALTIERI, FRANCESCA, NOSCHESE, Raffaella, A. Mura, MURA, Alessandro, F. Tosi, FILACCHIONE, GIANRICO, CIARNIELLO, Mauro, ADRIANI, Alberto, Brooks, S., G. Sindoni, S. Brooks, Bolton, S., F. Altieri, Sindoni, G.   +37 more
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When Moons Create Aurora: The Satellite Footprints on Giant Planets [PDF]

, 2013
Auroral Phenomen Other Planets Geophysical Mon © 2012. American 10.1029/2011GM Satellite footprints are localized auroral emissions in the upper atmosphere of Jupiter (Saturn) near the magnetic field lines linking to satellites, Io, Europa, and Ganymede (Enceladus). They are the auroral signatures of the strong electromagnetic interactions taking place
openaire   +2 more sources

The Magnetodiscs and Aurorae of Giant Planets

, 2016
This volume contains the reports discussed during the Workshop “Giant Planet Magne- todiscs and Aurorae” held 26–30 November 2012, at the International Space Science Insti- tute, organised together with the Europlanet project, supported by FP7 (Grant No.

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Auroras on Saturn, Uranus, and Neptune

, 2000
Aurorae result from the generation of emissions from the high latitudes of a planet due to the precipitation of energetic charged particles from the planet's magnetosphere.
Anil Bhardwaj, Randall Gladstone, G., G. Randall^Gladstone, Bhardwaj, Anil   +3 more
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Small and meso-scale properties of a substorm onset auroral arc

, 2010
International audienceWe present small and meso-scale properties of a substorm onset arc observed simultaneously by the Reimei and THEMIS satellites together with ground-based observations by the THEMIS GBO system.
Whiter, D., J. Weygand, Frey, H.U., H. U. Frey, N. Østgaard, B. Lanchester, Sakanoi, T., Seran, Elena, S. Fu, Frey, H., Ostgaard, N., Asamura, K., Weygand, J., T. Karlsson, Karlsson, T., Amm, O., Chaston, C., Haerendel, G., Seran, E., G. Haerendel, C. C. Chaston, Chaston, C.C., L. Juusola, Nakamura, R., Fu, S., O. Amm, Østgaard, N., Chaston, C. C., M. Hirahara, Lanchester, B., D. Whiter, Juusola, L., T. Sakanoi, E. Séran, Frey, H. U., K. Asamura, Hirahara, M., R. Nakamura, Karlsson, Tomas,   +38 more
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Review of M-I coupling and auroral emissions at the outer planets

, 2012
The bulk morphology of Jupiter's and Saturn's UV aurorae is conveniently divided into three components: 1) the main emission (main oval), 2) the satellites auroral footprints (equatorward of the main emission): Io, Europa and Ganymede for Jupiter and ...
Grodent, Denis
core  

Connecting planets to their moons: The auroral satellite footprints

, 2015
Among the many features of the Giant planets’ aurorae are very special spots which move in a very distinct manner compared with the remaining of the aurora.
Bonfond, Bertrand
core  

SPICAM observations and modeling of Mars aurorae

Icarus, 2016
L Soret, J -C Gérard, Ludivine Libert   +2 more
exaly  

Space Telescope observations of aurorae on the giant planets

Advances in Space Research, 1985
Richard Wagener
exaly  

Magnetospherically driven optical and radio aurorae at the end of the stellar main sequence

Nature, 2015
Gregg Hallinan, S P Littlefair, S Bourke   +2 more
exaly