ମୂଳ ଫାଇଲ(୨,୮୪୨ × ୧,୬୧୭ ପିକସେଲ, ଫାଇଲ ଆକାର: ୫୦୩ KB, ଏମ.ଆଇ.ଏମ.ଇର ପ୍ରକାର: image/jpeg)

ସାରକଥା

ବିବରଣୀ
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.
ତାରିଖ Taken on ୨୬ ନଭେମ୍ବର ୧୯୯୮
ମୂଳାଧାର 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
ଲେଖକ NASA, ESA & John T. Clarke (Univ. of Michigan)
ଅନ୍ୟ ସଂସ୍କରଣ

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୨୬ ନଭେମ୍ବର 1998

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ଫାଇଲ ଇତିହାସ

ଏହା ଫାଇଲଟି ସେତେବେଳେ ଯେମିତି ଦିଶୁଥିଲା ତାହା ଦେଖିବା ପାଇଁ ତାରିଖ/ବେଳା ଉପରେ କ୍ଲିକ କରନ୍ତୁ

ତାରିଖ/ବେଳନଖ ଦେଖଣାଆକାରବ୍ୟବହାରକାରୀମତାମତ
ଏବେକାର୦୬:୪୪, ୧୬ ଫେବୃଆରୀ ୨୦୧୭୦୬:୪୪, ୧୬ ଫେବୃଆରୀ ୨୦୧୭ ପରିକା ସଙ୍କଳନର ନଖଦେଖଣା୨,୮୪୨ × ୧,୬୧୭ (୫୦୩ KB)Geageafrom he.wiki --> https://he.wikipedia.org/wiki/%D7%A7%D7%95%D7%91%D7%A5:Satellite_Footprints_Seen_in_Jupiter_Aurora.jpg
୧୭:୫୧, ୧୬ ସେପ୍ଟେମ୍ବର ୨୦୦୮୧୭:୫୧, ୧୬ ସେପ୍ଟେମ୍ବର ୨୦୦୮ ପରିକା ସଙ୍କଳନର ନଖଦେଖଣା୭୫୨ × ୪୧୭ (୨୯୦ KB)RupertMillardUploading higher quality version from: http://hubblesite.org/newscenter/archive/releases/2000/38/image/a/
୧୭:୪୭, ୧୬ ସେପ୍ଟେମ୍ବର ୨୦୦୮୧୭:୪୭, ୧୬ ସେପ୍ଟେମ୍ବର ୨୦୦୮ ପରିକା ସଙ୍କଳନର ନଖଦେଖଣା୭୫୨ × ୪୧୭ (୨୯୦ KB)RupertMillard{{Information |Description= |Source= |Date= |Author= |Permission= |other_versions= }}
୦୫:୧୪, ୨ ଜାନୁଆରୀ ୨୦୦୭୦୫:୧୪, ୨ ଜାନୁଆରୀ ୨୦୦୭ ପରିକା ସଙ୍କଳନର ନଖଦେଖଣା୭୮୯ × ୪୫୧ (୧୭୯ KB)Wdflake~commonswikiRemoved border and caption, as is the policy on enwiki
୧୫:୧୧, ୧୧ ଅଗଷ୍ଟ ୨୦୦୫୧୫:୧୧, ୧୧ ଅଗଷ୍ଟ ୨୦୦୫ ପରିକା ସଙ୍କଳନର ନଖଦେଖଣା୮୦୦ × ୫୧୪ (୩୩ 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

ଏହି ସବୁପୃଷ୍ଠା ଏହି ଫାଇଲଟିକୁ ଯୋଡ଼ିଥାନ୍ତି:

ଜଗତ ଫାଇଲ ବ୍ୟବହାର

ତଳଲିଖିତ ଉଇକିସବୁ ଏହି ଫାଇଲଟିକୁ ବ୍ୟବହାର କରିଥାନ୍ତି:

ଏହି ଫାଇଲଟିର ଅଧିକ ବିଶ୍ୱବ୍ୟାପୀ ବ୍ୟବହାର ଦେଖନ୍ତୁ ।