可观的日冕喷发 Coronal Mass Ejection ; CME
伴随著可观的日冕喷发 Coronal Mass Ejection
伴随着可观的日冕喷发 Coronal Mass Ejection ; CME
日冕的变化反映的是太阳内部的变化。
Changes we see in the corona reflect changes deep inside the sun.
“日冕的温度高达两百万度，但是我们不知其原因，”她说。
"The [Sun's] corona has a temperature of 2 million degrees but we don't know why it is so hot," she said.
日冕的形状可以使用基于观测太阳表面活动频繁区域的先进技术准确地预报。
The shape of the corona can be accurately predicted in advance with calculations based on the observed surface magnetic field.
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