When the moon eclipses the sun, it unmasks a glorious halo–the glowing gases in the sun’s outer atmosphere, or corona. Six decades ago, observations in visible light revealed that the corona has a temperature greater than 1 million kelvins, making it hundreds of times hotter than the sun’s surface.
Star CN Leonis (arrow). UK SERC/PPARC, AATB, AURA
Contributing to the near-ultraviolet spectra (blue line) of star CN Leonis are emissions (red dashes) from iron ions in the star’s corona and titanium ions in a lower region, just above the star’s surface.
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