ಚಿತ್ರ:Jupiter.Aurora.HST.UV.jpg

ಈ ಮುನ್ನೋಟ ಗಾತ್ರ:೮೦೦ × ೪೫೫ ಪಿಕ್ಸೆಲ್‌ಗಳು. ಇತರ ರೆಸಲ್ಯೂಶನ್ಗಳು: ೩೨೦ × ೧೮೨ ಪಿಕ್ಸೆಲ್‌ಗಳು | ೬೪೦ × ೩೬೪ ಪಿಕ್ಸೆಲ್‌ಗಳು | ೧,೦೨೪ × ೫೮೩ ಪಿಕ್ಸೆಲ್‌ಗಳು | ೧,೨೮೦ × ೭೨೮ ಪಿಕ್ಸೆಲ್‌ಗಳು | ೨,೮೪೨ × ೧,೬೧೭ ಪಿಕ್ಸೆಲ್‌ಗಳು.

ಮೂಲ ಕಡತ ‎(೨,೮೪೨ × ೧,೬೧೭ ಚಿತ್ರಬಿಂದು, ಫೈಲಿನ ಗಾತ್ರ: ೫೦೩ KB, MIME ಪ್ರಕಾರ: image/jpeg)

ಸಾರಾಂಶ

ವಿವರJupiter.Aurora.HST.UV.jpg	Deutsch: Bild von ultraviolettem Polarlicht auf Jupiter, aufgenommen mit dem Space Telescope Imaging Spectrograph (STIS) des Weltraumteleskops Hubble der NASA. • STScI-PRC00-38 Helle Streifen und Tupfen sind verursacht durch magnetischen Flussröhren, die Jupiter mit seinen größten Monden verbindet: Io: heller Streifen ganz links, Ganymed: heller Tupfer unterhalb der Bildmitte, Europa: Tupfer rechts dessen von Ganymed English: This is a spectacular NASA Hubble Space Telescope close-up view of an electric-blue aurora that is eerily glowing one half billion miles away on the giant planet Jupiter. Auroras are curtains of light resulting from high-energy electrons racing along the planet's magnetic field into the upper atmosphere. The electrons excite atmospheric gases, causing them to glow. The image shows the main oval of the aurora, which is centered on the magnetic north pole, plus more diffuse emissions inside the polar cap. Though the aurora resembles the same phenomenon that crowns Earth's polar regions, the Hubble image shows unique emissions from the magnetic "footprints" of three of Jupiter's largest moons. (These points are reached by following Jupiter's magnetic field from each satellite down to the planet). Auroral footprints can be seen in this image from Io (along the left hand limb), Ganymede (near the center), and Europa (just below and to the right of Ganymede's auroral footprint). These emissions, produced by electric currents generated by the satellites, flow along Jupiter's magnetic field, bouncing in and out of the upper atmosphere. They are unlike anything seen on Earth. This ultraviolet image of Jupiter was taken with the Hubble Space Telescope Imaging Spectrograph (STIS) on November 26, 1998. In this ultraviolet view, the aurora stands out clearly, but Jupiter's cloud structure is masked by haze. This image was taken in UV light at 140 nm.
ದಿನಾಂಕ	Taken on ನವೆಂಬರ್ ೨೬, ೧೯೯೮
ಆಕರ	http://hubblesite.org/newscenter/archive/releases/2000/38/image/a/; see also https://www.spacetelescope.org/images/heic0009a/ and http://apod.gsfc.nasa.gov/apod/ap001219.html
ಕರ್ತೃ	NASA, ESA & John T. Clarke (Univ. of Michigan)
ಇತರೆ ಆವೃತ್ತಿಗಳು	Derivative works of this file: Jupiter Aurora HST UV-fr.svg Jupiter.Aurora.HST.mod.ru.svg Jupiter.Aurora.HST.mod.svg Jupiter.Aurora.HST.mod.jpg

This image or video was catalogued by one of the centers of the United States National Aeronautics and Space Administration (NASA) under Photo ID: STScI-2000-38 and Alternate ID: heic0009a.

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ಕಡತದ ಇತಿಹಾಸ

ದಿನ/ಕಾಲ ಒತ್ತಿದರೆ ಆ ಸಮಯದಲ್ಲಿ ಈ ಕಡತದ ವಸ್ತುಸ್ಥಿತಿ ತೋರುತ್ತದೆ.

	ದಿನ/ಕಾಲ	ಆಯಾಮಗಳು	ಬಳಕೆದಾರ	ಟಿಪ್ಪಣಿ
ಪ್ರಸಕ್ತ	೦೬:೪೪, ೧೬ ಫೆಬ್ರವರಿ ೨೦೧೭	೨,೮೪೨ × ೧,೬೧೭ (೫೦೩ KB)	Geagea	from he.wiki --> https://he.wikipedia.org/wiki/%D7%A7%D7%95%D7%91%D7%A5:Satellite_Footprints_Seen_in_Jupiter_Aurora.jpg
	೧೭:೫೧, ೧೬ ಸೆಪ್ಟೆಂಬರ್ ೨೦೦೮	೭೫೨ × ೪೧೭ (೨೯೦ KB)	RupertMillard	Uploading higher quality version from: http://hubblesite.org/newscenter/archive/releases/2000/38/image/a/
	೧೭:೪೭, ೧೬ ಸೆಪ್ಟೆಂಬರ್ ೨೦೦೮	೭೫೨ × ೪೧೭ (೨೯೦ KB)	RupertMillard	{{Information \|Description= \|Source= \|Date= \|Author= \|Permission= \|other_versions= }}
	೦೫:೧೪, ೨ ಜನವರಿ ೨೦೦೭	೭೮೯ × ೪೫೧ (೧೭೯ KB)	Wdflake~commonswiki	Removed border and caption, as is the policy on enwiki
	೧೫:೧೧, ೧೧ ಆಗಸ್ಟ್ ೨೦೦೫	೮೦೦ × ೫೧೪ (೩೩ KB)	Kurgus	''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