Fail:Coronal Mass Ejection.gif

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Ringkasan

Keterangan
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.
Tarikh
Sumber NASA Earth Observatory
Pengarang Images courtesy of the STEREO Science Center

Perlesenan

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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tarikh penubuhan

15 Februari 2010

MIME type Inggeris

image/gif

hasil tambah semak

ad07b7cefeddfbeafec5641b97474ca586e5c60b

kaedah penentuan: SHA-1 Inggeris

saiz data

1,696,815 bait

tempoh

4 saat

tinggi

2,048 piksel

lebar

2,048 piksel

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Tarikh/WaktuGambar kenitUkuranPenggunaKomen
semasa11:38, 15 Februari 2010Gambar kenit bagi versi pada 11:38, 15 Februari 20102,048 × 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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