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Total eclipse sheds light on solar energy phenomena

机译:日全食揭示了太阳能现象

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A perfect total eclipse at Lae, New Guinea, in February, gave information that will help in an understanding of the energies which surge from the sun and create the chromosphere and the sun's corona. The chromosphere is the 1,000-to 10,000-mile band of energy that lies between the sun's visible surface and the region called the corona that extends beyond the chromosphere. It can be seen in full and meaningful view only during a total eclipse. Of particular importance was this rare opportunity to view the lower 600-mile region of the chromosphere, which was seen clearly in this brief glimpse of several seconds' duration.
机译:二月份在新几内亚的莱发生了一次完美的日全食,它提供了有助于理解来自太阳的能量,并产生了色球和太阳日冕的信息。色球层是介于1000到10,000英里的能量带,它位于太阳的可见表面和延伸到色球层之外的称为电晕的区域之间。仅在全食期间才能以完整而有意义的视图看到它。特别重要的是,难得的机会可以看到色球圈的较低600英里区域,这一短暂的持续几秒钟的时间便可以清楚地看到。

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