tóng-àn:Sun in X-Ray.png

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Sun_in_X-Ray.png ‎（690 × 500 siōng-sò͘ , tóng-àn chiàm-liōng: 338 KB, MIME luī-hêng: image/png）

Khài-iàu

Soat-bêng This image shows the Sun as viewed by the Soft X-Ray Telescope (SXT) onboard the orbiting Yohkoh satellite. The bright, loop-like structures are hot (millions of degrees) plasma confined by magnetic fields rooted in the solar interior. An image of the sun in visible light would show sunspots at the feet of many of these loops. The halo of gas extending well beyond the sun is called the corona. The darker regions at the North and South poles of the Sun are coronal holes, where the magnetic field lines are open to space and allow particles to escape.
Ji̍t-kî
Chhut-chhù
  • NASA Goddard Laboratory for Atmospheres
  • Yohkoh mission of ISAS, Japan. The Yohkoh Soft X-ray telescope was prepared by the Lockheed-Martin Solar and Astrophysics Laboratory, the National Astronomical Observatory of Japan, and the University of Tokyo with the support of NASA and ISAS.
Chok-chiá NASA Goddard Laboratory for Atmospheres and Yohkoh Legacy data Archive
授權允准
(Bô siŏh-huòi sāi ciā ùng-giông)		 The image was apparently prepared from data from the Yohkoh mission, the image here was released by NASA. The underlying data was released into the public domain by the Yohkoh mission team. See [1].

Siū-khoân

Public domain 本作品由NASA創作，屬於公有領域。根據NASA的版權政策：“NASA的創作除非另有聲明否則不受版權保護。”（參見：Template:PD-USGov/zh，NASA版權政策或JPL圖像使用政策）
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hiān-chāi2006-nî 2-goe̍h 11-ji̍t (pài-la̍k) 16:222006-nî 2-goe̍h 11-ji̍t (pài-la̍k) 16:22 bēng-buōng gì sáuk-liŏk-dù690 × 500（338 KB）Arnomane{{Information| |Description = This image shows the Sun as viewed by the Soft X-Ray Telescope (SXT) onboard the orbiting Yohkoh satellite. The bright, loop-like structures are hot (millions of degrees) plasma (electrically charged gas) confined by magnetic

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