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Fayl:STEREO-A first images.jpg

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Qisqa izoh

Taʼrif Solar Images. A mosaic of the extreme ultraviolet, first, images from STEREO-A's SECCHI/Extreme Ultraviolet Imaging Telescope
Sanasi
Manba NASA, TIF file
Muallif NASA's twin Solar Terrestrial Relations Observatories (STEREO)
Other versions
  • Blue (171 Å)
    Blue (171 Å)
  • Green (195 Å)
    Green (195 Å)
  • Orange (304 Å)
    Orange (304 Å)

Qisqa izoh

English: A mosaic of the extreme ultraviolet, first, images from STEREO-A's SECCHI/Extreme Ultraviolet Imaging Telescope taken on Dec. 4, 2006. These false color images show the sun's atmospheres at a range of different temperatures. Clockwise from top left: 1 million degrees C (171 Å), 1.5 million °C (195 Å), 60,000 - 80,000 °C (304 Å), and 2.5 million °C (286 Å).
Polski: Mozaika pierwszych zdjęć Słońca wykonanych przez sondę STEREO-A 4 grudnia 2006 r. Wykonał je teleskop SECCHI/EUI w zakresie ultrafioletu. Przedstawiają emisję fal elektromagnetycznych różnych długości przez atmosferę Słońca (kolory fałszywe). Zgodnie z ruchem wskazówek zegara, od lewego górnego rogu: 171 Å (odpowiednik temp. 1 mln °C), 195 Å (1,5 mln. °C), 304 Å (60 000 - 80 000 °C), i 286 Å (2,5 mln °C)

Source: NASA archive copy at the Wayback Machine

Litsenziyalash

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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tasvirlangan obyekt

tashkil etilgan

4 dekabr 2006

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Sana/VaqtMiniaturaOʻlchamlariFoydalanuvchiIzoh
joriy17:54, 2009-yil 15-yanvar17:54, 2009-yil 15-yanvar dagi versiya uchun tasvir2 700 × 2 700 (3,85 MB)Sasha Krotovhi-res from .tif file
15:50, 2007-yil 11-yanvar15:50, 2007-yil 11-yanvar dagi versiya uchun tasvir864 × 864 (170 KB)NH2501{{en|A mosaic of the extreme ultraviolet, first, images from STEREO-A's SECCHI/Extreme Ultraviolet Imaging Telescope taken on Dec. 4, 2006. These false color images show the sun's atmospheres at a range of different temperatures. Clockwise from top left:

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