Datoteka:Coronal Mass Ejection.gif

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Opis
English: Arcs rise above an active region on the surface of the Sun in this series of images taken by the STEREO (Behind) spacecraft. The arcs are plasma, superheated matter made up of moving charged particles (electrons and ions). Just as iron filings arc from one end of a magnet to another, the plasma is sliding in an arc along magnetic field lines. Most coronal mass ejections are more bulbous and wide: this one is quite narrow and contained. Nonetheless, NASA solar scientists agree that its speed and characteristics suggest that it was indeed a non-typical coronal mass ejection.
Datum
Izvor NASA Earth Observatory
Autor Images courtesy of the STEREO Science Center

Licenciranje

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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prikazuje

nastanak

15 februar 2010

vrsta medija na Internetu Serbian (Latin script)

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kontrolna suma Srpski (transliteracija)

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metoda određivanja: SHA-1

veličina podatka Srpski (transliteracija)

1.696.815 Bajt

trajanje

4 sekund

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2.048 piksel

širina

2.048 piksel

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Datum/vrijemeMinijaturaDimenzijeKorisnikKomentar
aktualna13:38, 15 februar 2010Minijatura verzije (13:38, 15 februar 2010)2.048 × 2.048 (1,62 MB)Originalwana{{Information |Description={{en|1=Fiery arcs rise above an active region on the surface of the Sun in this series of images taken by the STEREO (Behind) spacecraft. The arcs are plasma, superheated matter made up of mov

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