دوتنه:Sun in X-Ray.png

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د ويکيپېډيا، وړیا پوهنغونډ له خوا

Sun_in_X-Ray.png ‏(۶۹۰ × ۵۰۰ پېکسل, د دوتنې کچه: ۳۳۸ کيلوبايټ, MIME بڼه: image/png)

دا دوتنه د ويکيمېډيا کامنز لخوا خپرېږې او کېدای شي چې دا په نورو پروژو هم کارېدلې وي. د دوتنې د کارېدنې لا نور مالومات د دوتنې د څرگندنو په مخ کې لاندې ښودل شوی.

لنډيز

څرگندونه 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.
نېټه
سرچينه
  • 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.
ليکوال NASA Goddard Laboratory for Atmospheres and Yohkoh Legacy data Archive
اجازه
(دا دوتنه بيا کارول)		 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].

منښتليک:

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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د دوتنې پېښليک

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نېټه/وختبټنوکډډېکارنتبصره
اوسنی۱۶:۲۲, ۱۱ فبروري ۲۰۰۶د ۱۶:۲۲, ۱۱ فبروري ۲۰۰۶ پورې د بټنوک بڼه۶۹۰ × ۵۰۰ (۳۳۸ کيلوبايټ)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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د نړېوالې دوتنې کارېدنه

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