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#coronalhole • Explore images about coronalhole via Instagram

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Explore aquilesr23's Instagram #Repost @nasa
This elongated coronal hole rotated across the surface of the sun this past week so that it is now streaming solar wind towards Earth. Coronal holes are areas of open magnetic field from which solar wind particles stream into space. The particle stream will likely generate aurora here on Earth. 
In this wavelength of extreme ultraviolet light, the coronal hole appears as a dark area near the center and lower portion of the sun. 
CREDIT: NASA/SDO 
#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430813870620737808_283540624

#repost@nasa This elongated coronal hole rotated across the surface of the sun this past week so that it is now streaming solar wind towards Earth. Coronal holes are areas of open magnetic field from which solar wind particles stream into space. The particle stream will likely generate aurora here on Earth. In this wavelength of extreme ultraviolet light, the coronal hole appears as a dark area near the center and lower portion of the sun. CREDIT: NASA/SDO #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore jimscape's Instagram #Repost @nasa with @repostapp
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Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430719121972268163_353171223

#repost@nasa with @repostapp ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore animals_nature_landscape's Instagram #Repost @nasa with @repostapp Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA
#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430541988545355653_3948332722

#repost@nasa with @repostapp Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore njoyers's Instagram #Repost @nasa with @repostapp
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Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430330868261467955_4188150045

#repost@nasa with @repostapp ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore iamgoutamjha's Instagram regram @nasa
Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430227578350126306_2203977964

regram @nasa Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore fjcruzh's Instagram regram @nasa
Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430184746981399020_4093020252

regram @nasa Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore mamollo's Instagram #inst10 #ReGram @nasa: Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430184444019299196_514588902

#inst10 #regram@nasa: Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore conciencialibreinfinita's Instagram #Repost @nasa with @repostapp
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Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430153394240261256_513528706

#repost@nasa with @repostapp ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore heathercameron_astro's Instagram from @nasa -  Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430151696847675823_2627748568

from @nasa - Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore la_menchito's Instagram #Repost @nasa with @repostapp
・・・
Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430128819696418565_576081396

#repost@nasa with @repostapp ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore liviamfh's Instagram Repost from @nasa @TopRankRepost #TopRankRepost Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430126829616136469_264474664

Repost from @nasa @TopRankRepost #toprankrepostMagnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore ben_haizlip's Instagram #Repost @nasa
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Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1430077600945312104_3115658591

#repost@nasa ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore usembsweden's Instagram #Reposted @nasa : Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429983327066007555_2980414310

#reposted@nasa : Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore davidtsay's Instagram #LooksLikeSciFiButItsRealLife 👽 Definitely my feeling in general lately but this #spacephoto from #NASA is literally that.
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#repost @nasa Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429943959018654539_220900348

#lookslikescifibutitsreallife👽 Definitely my feeling in general lately but this #spacephotofrom #nasais literally that. ・・・ #repost@nasa Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore boba_fett25's Instagram #Repost @nasa
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Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429940240080160702_678750515

#repost@nasa ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore ledfairylights's Instagram Tag your friends ❤️
Credit: @nasa
Follow Us: @ledfairylights #lights #led

Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here.
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429931487080645046_3509296751

Tag your friends ❤️ Credit: @nasa Follow Us: @ledfairylights #lights #led Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore solylunaok's Instagram @Regrann from @nasa -  Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429931160628460422_365519358

@Regrann from @nasa - Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore digitaljegs's Instagram #Repost @nasa with @repostapp
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Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429925010495323998_35134984

#repost@nasa with @repostapp ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore twingo727's Instagram #Repost @nasa with @repostapp
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Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429920644477707337_1339411595

#repost@nasa with @repostapp ・・・ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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Explore stormdots's Instagram New sun, new sight. Hello, Father.

#pagan
 #Repost: @nasa via @renstapp ···
“ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. 
Credit: Solar Dynamics Observatory, NASA"

#nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather 1429896456152474545_2252742911

New sun, new sight. Hello, Father. #pagan #Repost: @nasa via @renstapp ··· “ Magnetic arcs of plasma that spiraled above two active regions held their shape fairly well over 18 hours (Jan. 11-12). The charged plasma is being controlled the magnetic field lines of the active regions. The field lines become clearly visible when viewed in this wavelength of extreme ultraviolet light. Often the arches bend and twist more dynamically than the relatively stable ones seen here. Credit: Solar Dynamics Observatory, NASA" #nasa #space #sun #solar #coronalhole #sdo #observatory #aurora #solarwind#particles #solarsystem #spaceweather

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