فائل:Jupiter.Aurora.HST.UV.jpg

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خلاصہ

تفصیلJupiter.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.
تاریخ	Taken on 26 نومبر 1998
ماخذ	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
مصنف	NASA, ESA & John T. Clarke (Univ. of Michigan)
دوسرے نسخے	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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کسی خاص وقت یا تاریخ میں یہ فائل کیسی نظر آتی تھی، اسے دیکھنے کے لیے اس وقت/تاریخ پر کلک کریں۔

	تاریخ/وقت	ابعاد	صارف	تبصرہ
رائج الوقت	01:14، 16 فروری 2017ء	2,842 × 1,617 (503 کلوبائٹ)	Geagea	from he.wiki --> https://he.wikipedia.org/wiki/%D7%A7%D7%95%D7%91%D7%A5:Satellite_Footprints_Seen_in_Jupiter_Aurora.jpg
	12:21، 16 ستمبر 2008ء	752 × 417 (290 کلوبائٹ)	RupertMillard	Uploading higher quality version from: http://hubblesite.org/newscenter/archive/releases/2000/38/image/a/
	12:17، 16 ستمبر 2008ء	752 × 417 (290 کلوبائٹ)	RupertMillard	{{Information \|Description= \|Source= \|Date= \|Author= \|Permission= \|other_versions= }}
	23:44، 1 جنوری 2007ء	789 × 451 (179 کلوبائٹ)	Wdflake~commonswiki	Removed border and caption, as is the policy on enwiki
	09:41، 11 اگست 2005ء	800 × 514 (33 کلوبائٹ)	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