During a total solar eclipse, it is possible to view many wonders, such as the corona. The brightness of the inner corona exceeds that of the full moon, while the brightness of the outer corona is 1/1000th that of the inner corona. Therefore, the significance of recording it lies in its extremely high dynamic brightness range. Images of the corona were recorded based on this feature. After high dynamic range processing, images clearly revealed the structure of the corona including its feathers and flow. In the lower right corner is the solar prominence. It is also possible to see the moon illuminated by the weak reflection of the earth.