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ꯃꯔꯨꯑꯣꯏꯕ ꯂꯃꯥꯏ

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ꯅꯨꯃꯤꯠꯁꯤꯒꯤ ꯃꯃꯤ
ꯅꯨꯃꯤꯠꯁꯤꯒꯤ ꯃꯦꯗꯤꯌꯥ
This otherworldly, ever-changing landscape is what the Sun looks like up close. ESA's Solar Orbiter filmed the transition from the Sun's lower atmosphere to the much hotter outer corona. The hair-like structures are made of charged gas (plasma), following magnetic field lines emerging from the Sun's interior. The brightest regions are around one million degrees Celsius, while cooler material looks dark as it absorbs radiation.
 

+/− (mni), +/− (en)

ꯁꯔꯨꯛ ꯌꯥꯔꯤ
ꯊꯤꯔꯤꯔꯥ?
ꯆꯥꯟꯕꯤꯗꯨꯅ ꯂꯃꯥꯢ ꯑꯁꯤꯒꯤ ꯃꯊꯛꯇ ꯂꯩꯕ "ꯊꯤꯅꯕ ꯎꯄꯨ" ꯑꯁꯤ ꯅꯠꯇ꯭ꯔꯒ ꯌꯦꯠꯊꯪꯕꯗ ꯂꯩꯕ "ꯂꯪꯗꯥꯢ" ꯑꯁꯤ ꯁꯤꯖꯤꯟꯅꯕꯤꯌꯨ꯫ ꯑꯩꯈꯣꯢꯒꯤ ꯐꯣꯡꯗꯣꯛꯈꯤꯕ ꯄꯥꯎꯁꯤꯡ ꯑꯁꯤ ꯂꯧꯁꯤꯟꯕꯤꯕ ꯆꯤꯡꯅꯕ ꯂꯩꯕꯤꯒꯅꯨ꯫
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ꯃꯅꯤꯡ ꯇꯝꯕ ꯆꯦ-ꯆꯥꯡ ꯒꯤ ꯑꯆꯪꯕ ꯑꯗꯨ ꯃꯄꯨꯡ ꯐꯥꯅꯅꯕ, ꯆꯥꯟꯕꯤꯗꯨꯅ ꯑꯩꯈꯣꯢꯒꯤ ꯑꯃꯨꯛ ꯍꯟꯅ ꯁꯤꯖꯤꯟꯅꯕ ꯃꯇꯦꯡ ꯑꯁꯤ ꯄꯥꯕꯤꯌꯨ꯫ ꯅꯍꯥꯛꯅ ꯃꯃꯤ ꯑꯃ ꯍꯥꯄꯤꯅꯕ ꯍꯥꯢꯖꯕ ꯑꯁꯤꯁꯨ ꯌꯥꯒꯅꯤ꯫
ꯈꯪꯗꯣꯛꯂꯤꯔꯥ?
ꯊꯤꯕꯤꯌꯨ ꯃꯆꯥꯈꯥꯢꯕ:ꯁꯛꯈꯪꯗꯕ ꯍꯤꯔꯝꯁꯤꯡꯒꯤ ꯈꯨꯠꯊꯥꯡꯗ꯫ ꯀꯔꯤꯒꯨꯝꯕ ꯅꯍꯥꯛꯅ ꯈꯪꯕ ꯉꯝꯕ ꯈꯔ ꯐꯪꯂꯕꯗꯤ, ꯄꯣꯠꯁꯛ ꯑꯗꯨꯒꯤ ꯋꯥꯔꯤ ꯁꯥꯐꯝ ꯂꯃꯥꯢ ꯗ ꯋꯥꯐꯝ ꯈꯔ ꯏꯕ ꯌꯥꯒꯅꯤ ꯫
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ꯑꯗꯨꯒ ꯑꯇꯩ ꯃꯌꯥꯝ!
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ꯑꯩꯈꯣꯢꯒꯤ ꯊꯥ-ꯊꯥꯒꯤ ꯑꯣꯢꯕ ꯍꯤꯔꯝ-ꯍꯤꯔꯝꯒꯤ ꯆꯥꯡꯌꯦꯡ ꯑꯁꯤ ꯊꯦꯡꯅꯕ ꯉꯝꯅꯕ ꯃꯃꯤ ꯈꯔ ꯂꯧꯕꯤꯌꯨ ꯑꯗꯨꯒ ꯊꯥꯒꯠꯄꯤꯌꯨ, ꯄꯨꯛꯅꯤꯡꯗ ꯏꯅꯣꯠ ꯄꯣꯛꯄꯤꯌꯨ ꯑꯗꯨꯒ ꯑꯅꯧꯕ ꯍꯤꯔꯝꯁꯤꯡ ꯌꯦꯡꯕꯤꯌꯨ! ꯆꯥꯡꯌꯦꯡꯁꯤꯡꯒꯤ ꯃꯇꯥꯡꯗ ꯍꯦꯟꯅ ꯈꯪꯕꯤꯌꯨ!
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ꯃꯅꯨꯡꯒꯤ ꯑꯌꯥꯎꯕ