File:Jupiter.Aurora.HST.mod.uk.svg

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English: Jupiter's aurorae in November 1998. The image made by HST. The main auroral oval and polar ovals are marked with dash lines. Satellite spots and other features are also shown. (Based on Palier, Laurent (2001). "10.1016/S0032-0633(01)00023-X More about the structure of the high latitude Jovian aurorae". Planetary and Space Sciences 49: 1159–73.)
NASA image of Jupiter aurora in UV, Hubble Space Telescope Bright streaks and dots are caused by magnetic flux tubes connecting Jupiter to its largest moons: * Io: bright streak on the far left * Ganymede: bright dot below center * Europa: dot right of Ganymede dot Image originally from http://apod.gsfc.nasa.gov/apod/ap001219.html Credit: John T. Clarke (U. Michigan), ESA, NASA
English: Jupiter's aurorae in November 1998. The image made by HST. The main auroral oval and polar ovals are marked with dash lines. Satellite spots and other features are also shown. (Based on Palier, Laurent (2001). "10.1016/S0032-0633(01)00023-X More about the structure of the high latitude Jovian aurorae". Planetary and Space Sciences 49: 1159–73.)
Українська: Структура полярних сяйв на Юпітері: показано основне кільце, полярне випромінювання та плями, що виникли як результат взаємодії з природними супутниками Юпітера.
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This is a retouched picture, which means that it has been digitally altered from its original version. Modifications: Ukrainian translation. The original can be viewed here: Jupiter.Aurora.HST.mod.ru.svg: . Modifications made by Jarozwj.

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current06:19, 26 April 2017Thumbnail for version as of 06:19, 26 April 2017752 × 417 (138 KB)Jarozwj (talk | contribs)User created page with UploadWizard

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