वैज्ञानिकों ने सूर्य के ऊपरी वायुमंडल में अधिक तीव्र घूर्णन की खोज की: Although scientists have long studied how different parts of the Sun’s surface rotate at different speeds (called differential rotation) using optical and extreme ultraviolet (EUV) observations, it has been hard to know exactly at what height in the Sun’s atmosphere these measurements are taken. This is because EUV light depends on temperature, which makes the
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