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To see a total solar eclipse, one must be within the path of totality on Earth's surface, while observers outside this path witness a partial eclipse. The corona, the Sun's outer atmosphere, is visible during a total solar eclipse.
To see a total solar eclipse, you must be within the shadow of the Moon on Earth's surface, known as the path of totality. This path is usually not more than 50 miles wide. Being in this narrow path allows observers to witness a total eclipse, where the Moon completely covers the Sun.
Observers outside the path of totality will experience a partial eclipse, where only a portion of the Sun is covered by the Moon. The corona, the Sun's outer atmosphere, becomes visible during a total solar eclipse.
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